ENTRY ARTIFICIAL INTELLIGENCE - Department of Mathematics ...
ENTRY ARTIFICIAL INTELLIGENCE - Department of Mathematics ...
ENTRY ARTIFICIAL INTELLIGENCE - Department of Mathematics ...
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<strong>ENTRY</strong> <strong>ARTIFICIAL</strong> <strong>INTELLIGENCE</strong><br />
[<strong>ENTRY</strong> <strong>ARTIFICIAL</strong> <strong>INTELLIGENCE</strong>] Authors: Oliver Knill: March 2000 Literature: Peter Norvig,<br />
Paradigns <strong>of</strong> Artificial Intelligence Programming Daniel Juravsky and James Martin, Speech and Language<br />
Processing<br />
Adaptive Simulated Annealing<br />
[Adaptive Simulated Annealing] A language interface to a neural net simulator.<br />
artificial intelligence<br />
[artificial intelligence] (AI) is a field <strong>of</strong> computer science concerned with the concepts and methods <strong>of</strong> symbolic<br />
knowledge representation. AI attempts to model aspects <strong>of</strong> human thought on computers. Aspectrs <strong>of</strong> AI:<br />
• computer vision<br />
• language processing<br />
• pattern recognition<br />
• expert systems<br />
• problem solving<br />
• roboting<br />
• optical character recognition<br />
• artificial life<br />
• grammars<br />
• game theory<br />
[Babelfish] Online translation system from Systran.<br />
Babelfish<br />
Chomsky<br />
[Chomsky] Noam Chomsky is a pioneer in formal language theory. He is MIT Pr<strong>of</strong>essor <strong>of</strong> Linguistics, Linguistic<br />
Theory, Syntax, Semantics and Philosophy <strong>of</strong> Language.<br />
Eliza<br />
[Eliza] One <strong>of</strong> the first programs to feature English output as well as input. It was developed by Joseph<br />
Weizenbaum at MIT. The paper appears in the January 1966 issue <strong>of</strong> the ”Communications <strong>of</strong> the Association<br />
<strong>of</strong> Computing Machinery”.
Google<br />
[Google] A search engine emerging at the end <strong>of</strong> the 20’th century. It has AI features, allows not only to answer<br />
questions by pointing to relevant webpages but can also do simple tasks like doing arithmetic computations,<br />
convert units, read the news or find pictures with some content.<br />
GPS<br />
[GPS] General Problem Solver. A program developed in 1957 by Alan Newell and Herbert Simon. The aim was<br />
to write a single computer program which could solve any problem. One reason why GPS was destined to fail<br />
is now at the core <strong>of</strong> computer science. There are a large set <strong>of</strong> problems which are NP hard and where finding<br />
a solution becomes exponentially hard in dependence <strong>of</strong> the size <strong>of</strong> the problem. Nonetheless, GPS has been a<br />
useful tool for exploring AI programming.<br />
HAL<br />
[HAL] The HAL 9000 computer was the main character in Stanley Kurbrick’s film 2001: a Space Odyssey. HAL<br />
is an AI agent capable to understand advanced language processing behavior as speaking and understanding<br />
language and even reading lips.<br />
Lisp<br />
[Lisp] Lisp is one <strong>of</strong> the oldest programming languages still in widespread use today. ”Common Lisp” is the most<br />
widely accepted standard. Other dialects like ”Franz Lisp” MacLisp, InterLisp, ZetaLisp or ”Standard Lisp”<br />
are considered obsolete. Lisp is the most popular language for AI programming. Lisp programs are concise and<br />
are uncluttered by low-level detail.<br />
Loebner Prize<br />
[Loebner Prize] A competition attempted to put various computer programs to the Turing test. A consistent<br />
result over the years has been that even the crudest programs can fool some <strong>of</strong> the judges some <strong>of</strong> the time.<br />
MIT ai lab<br />
[MIT ai lab] Massachusetts Institute <strong>of</strong> Technology AI laboratory.
neural network<br />
[neural network] Artificial neural networks try to simulate biological neural networks as found in the brain.<br />
Such a network consists <strong>of</strong> many simple processors called neurons, each possibly having some local memory.<br />
These neurons are connected and evolve depending to their local data and on the inputs they receive via<br />
the connections. A neural network can either be an algorithm, or be realized as actual hardware. Neural<br />
networks typically allow training. They learn by adjusting the weights <strong>of</strong> the connections on the basis <strong>of</strong><br />
presented patterns. The individual neurons are elementary non-linear signal processors. Neural networks are<br />
distinguished from other computing devices by a high degree <strong>of</strong> interconnection allowing parallelism. There is<br />
no idle memory containing data and programs. Each neuron is pre-programmed and continuously active.<br />
pattern recognition<br />
[pattern recognition] A branch <strong>of</strong> artificial intelligence concerned with the classification or description <strong>of</strong> observations.<br />
The classification uses either statistical, syntactic or neural aproches.<br />
[pilot] Programmed Inquiry Learning Or Teaching.<br />
pilot<br />
prolog<br />
[prolog] A popular AI programming language used in Europe and Japan. Prolog shares most <strong>of</strong> Lisp’s advantages<br />
in terms <strong>of</strong> flexibility and conciseness.<br />
regular expression<br />
[regular expression] is a language for specifying text search strings. It is used in UNIX programs like vi, perl,<br />
emacs or grep. It is also used in Micros<strong>of</strong>t word or web search engines.<br />
scheme<br />
[scheme] A dialect <strong>of</strong> Lisp which is gaining popularity, primarily for teaching and experimenting with programming<br />
language design and techniques.<br />
Shrdlu<br />
[Shrdlu] Terry Winograd’s SHRDLU system <strong>of</strong> 1972 simulated a robot embedded in a world <strong>of</strong> toy blocks. The<br />
program was able to accept natural language text commands.
Student<br />
[Student] Student was an early language understanding program written by Daniel Bubrow in 1964. It was<br />
designed to read and solve the kind <strong>of</strong> word problems found in high school algebra books. Unlike Eliza,<br />
”Student” must process and understand a great deal <strong>of</strong> input as well as be able to solve algebraic equations.<br />
toy problem<br />
[toy problem] A deliberately oversimplified case <strong>of</strong> a challenging problem used to investigate, prototype, or test<br />
algorithms for a real problem.<br />
Turing test<br />
[Turing test] A test introduced in 1950 by Alan Turing. There are three participants. Two people and a<br />
computer. One person plays the role <strong>of</strong> an interrogator who has to find out, which <strong>of</strong> the two others is a<br />
machine. This interrogator is connected to the two other participants through teletype. The task <strong>of</strong> the<br />
machine is to fool the interrogator into believing it is a person. The task <strong>of</strong> the other participant is to convince<br />
the interrogator that he is human. Turing predicted that in 2000 a machine with 10 Gig memory would have a<br />
30 percent change <strong>of</strong> fooling a human interrogator after 5 minutes <strong>of</strong> questioning.<br />
Weizenbaum<br />
[Weizenbaum] Joseph Weizenbaum was the principal developer <strong>of</strong> Eliza, one <strong>of</strong> the first programs to feature<br />
English output as well as input.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 22 entries in this file.
Index<br />
Adaptive Simulated Annealing, 1<br />
artificial intelligence, 1<br />
Babelfish, 1<br />
Chomsky, 1<br />
Eliza, 1<br />
Google, 2<br />
GPS, 2<br />
HAL, 2<br />
Lisp, 2<br />
Loebner Prize, 2<br />
MIT ai lab, 2<br />
neural network, 3<br />
pattern recognition, 3<br />
pilot, 3<br />
prolog, 3<br />
regular expression, 3<br />
scheme, 3<br />
Shrdlu, 3<br />
Student, 4<br />
toy problem, 4<br />
Turing test, 4<br />
Weizenbaum, 4<br />
5
<strong>ENTRY</strong> ABSTRACT ALGEBRA<br />
[<strong>ENTRY</strong> ABSTRACT ALGEBRA] Authors: started Oliver Knill: September 2003 Literature: Lecture notes<br />
additive<br />
A function f : G → H from a semigroup G to a semigroup H is [additive] if f(a + b) = f(a) + f(b). A<br />
group-valued function on sets is additive if f(Y ∪ Z) = f(Y ) + f(Z) if Y and Z are disjoint.<br />
algebra<br />
An [algebra] over a field K is a ring with 1 which is also a vector space over K and whose multiplication is<br />
bilinear with respect to K. Examples:<br />
• the complex numbers C is an algebra over the field <strong>of</strong> real numbers K = R.<br />
• The quaternion algebra H is an algebra over the field <strong>of</strong> complex numbers.<br />
• The matrix algebra M(n, R) is an algebra over the field R.<br />
An algebraic number field<br />
[An algebraic number field] is a subfield <strong>of</strong> the complex numbers that arises as a finite degree algebraic extension<br />
field over the field <strong>of</strong> rationals.<br />
alternating group<br />
The [alternating group] G is the subgroup <strong>of</strong> the symmetric group <strong>of</strong> n objects given by the elements which can<br />
be written as a product <strong>of</strong> an even number <strong>of</strong> transpositions.<br />
Artinian module<br />
An [Artinian module] is a module which satisfies the descending chain condition. Every Artinian module is a<br />
Noetherian module but the integers for example are a Noetherian module which is not an Artinian module.<br />
Artinian ring<br />
An [Artinian ring] is a ring which when considered as a R-module is an Artinian module.<br />
Artinian ring<br />
Two elements <strong>of</strong> an integral domain that are unit-multipliers <strong>of</strong> each other are called [associate numbers].
Cayley’s theorem<br />
[Cayley’s theorem] assures that every finite group is isomorphic to a permutation group.<br />
center<br />
The [center] <strong>of</strong> a group (G, ∗) is the set <strong>of</strong> all elements g which satisfy gh = hg for all h in G. The center is a<br />
subgroup <strong>of</strong> G.<br />
commutator<br />
The [commutator] <strong>of</strong> two elements g, h in a group (G, ∗) is defined as [g, h] = g ∗ h ∗ g −1 ∗ h −1 .<br />
commutator subgroup<br />
The [commutator subgroup] <strong>of</strong> a group (G, ∗) is the set <strong>of</strong> all commutators [g, h] in G. It is a subgroup <strong>of</strong> G.<br />
factor group<br />
A [factor group] G/N is defined when N is a normal subgroup <strong>of</strong> the group G. It is the group, where the<br />
elements are equivalent classes gN and operation (gN)(hN) = (gh)N which is defined because N was assumed<br />
to be normal. For example, if G is the group <strong>of</strong> additive integers and N = kN with an integer k, then G/N = Zk<br />
is finite group <strong>of</strong> integers modulo k.<br />
finite group<br />
A group is called a [finite group] if G is a set with finitely many elements. For example, the set <strong>of</strong> all permutations<br />
<strong>of</strong> a finite set form a finite group. The set <strong>of</strong> all operations on the Rubik cube form a finite group.
group<br />
A [group] (X, +, 0) is a set X with a binary operation + and a zero element 0 (also called neutral element or<br />
identity) with the following properties<br />
Examples:<br />
(a + b) + c = a + (b + c) associativity<br />
a + 0 = a zero element<br />
∀a∃ba + b = 0 inverse<br />
• the real numbers form a group under addition 5 + 2.34 = 7.34, 3 − 3 = 0.<br />
• the set GL(n, R) <strong>of</strong> real matrices with nonzero determinant form a group under matrix multiplication<br />
• the nonzero integers form a group under multiplication 4 ∗ 7 = 28.<br />
• all the invertible linear transformations <strong>of</strong> the plane plane form a group under composition. The ”zero<br />
element” is the identity transformation T (x) = x.<br />
• all the continuous functions on the unit interval form a group with addition (f + g)(x) = f(x) + g(x).<br />
• all the permutations on a finite set form a group under composition.<br />
• the set <strong>of</strong> subsets Y <strong>of</strong> a set X with the operation A∆B = (A ∪ B) \ (A ∩ B) form a group. The inverse<br />
<strong>of</strong> A is A itself because A∆A = ∅, the zero element is ∅.<br />
normal subgroup<br />
a [normal subgroup] <strong>of</strong> a group (G, ∗) is a subgroup (H, ∗) <strong>of</strong> (G, ∗) which has the property that for all g in H<br />
and all g in G one has g −1 hg is in H. For an abelian group all subgroups are normal. The subgroup Sl(n, R)<br />
<strong>of</strong> Gl(n, R) is a normal subgroup.<br />
ring<br />
A [ring] (X, +, ∗, 0) is a set X with a binary operation + and a binary operation ∗ such that (X, +, 0) is a<br />
commutative group and (X, ∗) is a semigroup and such that the distributivity laws a ∗ (b + c) = a ∗ b + a ∗ c,<br />
(a + b) ∗ c − a ∗ c + b ∗ c hold. Examples:<br />
• the integers Z form a ring with addition and multiplication<br />
• the set <strong>of</strong> rational numbers Q, the set <strong>of</strong> real numbers R or the complext numbers C form a ring with<br />
addition and multiplication.<br />
• the set <strong>of</strong> 3x3 matrices with real entries form a ring with addition and matrix multiplication.<br />
• the set P <strong>of</strong> polynomials with real coefficients form a ring with addition and multiplication.<br />
• the set <strong>of</strong> subsets Y <strong>of</strong> a set X with addition ∆ and multiplication ∩ forms a ring.<br />
• the set <strong>of</strong> continuous functions on an interval [0, 1] with addition (f +g)(x) = f(x)+g(x) and multiplication<br />
f ∗ g(x) = f(x)g(x).
commutative group<br />
A [commutative group] is a group (X, +, 0) which is commutative: a + b = b + a.<br />
• the set <strong>of</strong> real numbers R forms a commutative group under addition.<br />
• the set <strong>of</strong> permutations S <strong>of</strong> a set X form a noncommutative group under composition.<br />
commutative ring<br />
A [commutative ring] is a ring (X, +, ∗, 0) for which the multiplicative semigroup (X, ∗) is commutative: a ∗ b =<br />
b ∗ a. Examples:<br />
• the integers form a commutative ring.<br />
• the set <strong>of</strong> 2 × 2 matrices form a noncommutative ring<br />
• the set <strong>of</strong> polyomials with real coefficients (x 2 + πx + 2) ∗ (x + 5x) = 6x 3 + 6πx 2 + 12x.<br />
function field<br />
A [function field] is a finite extension <strong>of</strong> the field C(z) <strong>of</strong> rational functions in the variable z.<br />
homomorphism<br />
An [homomorphism] φ between two groups G, H is a map f : G → H which has the property φ(g∗h) = φ(g)∗φ(h)<br />
and φ(0) = 0 for all elements g, h ∈ G. Examples:<br />
• if G is the multiplicative group (R + , ∗) <strong>of</strong> positive real numbers and H is the additive group (R, +) <strong>of</strong> all<br />
positive real numbers then φ(x) = log(x) is a homomorphism:<br />
• if G is the group <strong>of</strong> matrices with nonzero determinant and H is the group <strong>of</strong> nonzero real numbers and<br />
φ(A) = det(A), we have φ(x ∗ y) = φ(x)φ(y).<br />
isomorphism<br />
An [isomorphism] φ between two groups G, H is a homomorphism between groups which is also invertible.
number field<br />
A [number field] is a finite extension <strong>of</strong> Q, the field <strong>of</strong> rational numbers. It is a field extension <strong>of</strong> Q which is also<br />
a vector space <strong>of</strong> finite dimension over Q. Since the elements <strong>of</strong> a number field are algebraic numbers, roots <strong>of</strong><br />
a fixed polyonomial a0 + a1z + ... + z n with integer coefficitients, one calls them also algebraic number fields.<br />
The study <strong>of</strong> algebraic number fields is part <strong>of</strong> algebraic number theory.<br />
Examples:<br />
• quadratic fields: Q( √ d), where d is a rational number. It is in general a field extension <strong>of</strong> degree 2 over<br />
the field <strong>of</strong> rational number.<br />
• cyclotimic fields: Q(ξ), where ξ is a n’th root <strong>of</strong> 1. It is a field extension <strong>of</strong> degree φ(n), where φ(n) is the<br />
Euler function.<br />
octonions<br />
The [octonions] can be written as linear combinations <strong>of</strong> elements e0, e1, e2, ..., e7. The multiplication is determined<br />
by the multiplication table<br />
* 1 e1 e2 e3 e4 e5 e6 e7<br />
1 1 e1 e2 e3 e4 e5 e6 e7<br />
e1 e1 −1 e4 e7 -e2 e6 -e5 -e3<br />
e2 e2 -e4 −1 e5 e1 -e3 e7 -e6<br />
e3 e3 -e7 -e5 −1 e6 e2 -e4 e1<br />
e4 e4 e2 -e1 -e6 −1 e7 e3 -e5<br />
e5 e5 -e6 e3 -e2 -e7 −1 e1 e4<br />
e6 e6 e5 -e7 e4 -e3 -e1 −1 e2<br />
e7 e7 e3 e6 -e1 e5 -e4 -e2 −1<br />
Octonions are also called Cayley numbers. The multiplication <strong>of</strong> octonions is not associative. Octonions have<br />
been discovered by John T. Graves in 1843 and independently by Arthur Cayley.<br />
order<br />
The [order] <strong>of</strong> a finite group is the set <strong>of</strong> elements in the group.<br />
p-group<br />
A [p-group] is a finite group with order p n , where p is a prime integer and n > 0.
quaterions<br />
The [quaterions] can be written as linear combinations <strong>of</strong> elements 1, i, j, k. The multiplication is determined<br />
by the multiplication table<br />
* 1 i j k<br />
1 1 i j k<br />
i i −1 k −j<br />
j j −k −1 i<br />
k k j −i −1<br />
Quaternions are useful to compute rotations in three dimensions.<br />
semigroup<br />
A [semigroup] (X, +) is a set X with a binary operation + which satisfies the associativity law (a + b) + c =<br />
a + (b + c). Examples:<br />
• a group is a semigroup.<br />
• the set <strong>of</strong> finite words in an alphabet with composition form a semigroup word1 + word2 = word1word2<br />
• the natural numbers form a semigroup under addition.<br />
commutative semigroup<br />
A [commutative semigroup] is a semigroup (X, +) which is commutative. a + b = b + a.<br />
• the natural numbers form a commutative semigroup under addition.<br />
• composition <strong>of</strong> words over a finite alphabet form a noncommutative semigroup<br />
kernel<br />
The [kernel] <strong>of</strong> a homomorphism between two groups G, H is the set <strong>of</strong> all elements in G which are maped to<br />
the zero element <strong>of</strong> H. For example, SL(n, R) is the kernel <strong>of</strong> the homomorphism from GL(n, R) to R \ {0}<br />
defined by φ(A) = det(A).<br />
subgroup<br />
A [subgroup] <strong>of</strong> a group G is a subset <strong>of</strong> G which is also a group. Examples:<br />
• the set <strong>of</strong> n × n matrices with determinant 1 is a subgroup <strong>of</strong> the set <strong>of</strong> n × n matrices with nonzero<br />
determinant.<br />
• the trivial subgroup {0} is always a subgroup <strong>of</strong> a group (G, ∗, 0).
Theorem <strong>of</strong> Cauchy<br />
The [Theorem <strong>of</strong> Cauchy] in group theory states that every finite group whose order is divisible by a prime<br />
number p contains a subgroup <strong>of</strong> order p.<br />
sedenions<br />
[sedenions] form a zero Divisor Algebra. By a theorem <strong>of</strong> Frobenius (1877), there are three and only three<br />
associative finite division algebras: the real numbers R, the complex numbers C and the quaternions Q. Similar<br />
algebras in higher dimensions have zero divisors: sedenions are examples.<br />
field<br />
A [field] is a commutative ring (R, +, ∗, 0, 1) such that (R, +, 0) and (R \ 0, ∗, 1) are both commutative groups.<br />
theorem <strong>of</strong> Zorn<br />
By a [theorem <strong>of</strong> Zorn] (1933), every alternative, quadratic, real non-associative algebra without zero divisors<br />
is isomorphic to the 8-dimensional octonions O.<br />
Theorem <strong>of</strong> Hurwitz<br />
[Theorem <strong>of</strong> Hurwitz]: the normed composition algebras with unit are: real numbers, complex numbers, quaternions;<br />
and octonions.<br />
Theorem <strong>of</strong> Kervaire and Milnor<br />
[Theorem <strong>of</strong> Kervaire and Milnor] In 1958, Kervaire and Milnor proved independently <strong>of</strong> each other that the<br />
finite-dimensional real division algebras have dimensions 1, 2, 4, or 8.<br />
Theorem <strong>of</strong> Adams<br />
[Theorem <strong>of</strong> Adams] In 1960, Adams proved that a continuous multiplication in R n+1 with two-sided unit and<br />
with norm product exists only for n + 1 = 1, 2, 4, or 8.
Theorem <strong>of</strong> Hurwitz<br />
[Theorem <strong>of</strong> Hurwitz]: the normed composition algebras with unit are:<br />
• real numbers<br />
• complex numbers<br />
• quaternions<br />
• octonions<br />
Theorems <strong>of</strong> Sylov<br />
[Theorems <strong>of</strong> Sylov] If G is a finite group <strong>of</strong> order |G| = p n q, where p is a prime number, then G has a subgroup<br />
<strong>of</strong> order p n . Such groups are called Sylov groups and all <strong>of</strong> them are isomorphic. Furthermore, the number N<br />
<strong>of</strong> different p-Sylov groups in G satisfies N = 1 mod(p).<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 39 entries in this file.
Index<br />
additive, 1<br />
algebra, 1<br />
alternating group, 1<br />
An algebraic number field, 1<br />
Artinian module, 1<br />
Artinian ring, 1<br />
Cayley’s theorem, 2<br />
center, 2<br />
commutative group, 4<br />
commutative ring, 4<br />
commutative semigroup, 6<br />
commutator, 2<br />
commutator subgroup, 2<br />
factor group, 2<br />
field, 7<br />
finite group, 2<br />
function field, 4<br />
group, 3<br />
homomorphism, 4<br />
isomorphism, 4<br />
kernel, 6<br />
normal subgroup, 3<br />
number field, 5<br />
octonions, 5<br />
order, 5<br />
p-group, 5<br />
quaterions, 6<br />
ring, 3<br />
sedenions, 7<br />
semigroup, 6<br />
subgroup, 6<br />
Theorem <strong>of</strong> Adams, 7<br />
Theorem <strong>of</strong> Cauchy, 7<br />
Theorem <strong>of</strong> Hurwitz, 7, 8<br />
Theorem <strong>of</strong> Kervaire and Milnor, 7<br />
theorem <strong>of</strong> Zorn, 7<br />
Theorems <strong>of</strong> Sylov, 8<br />
9
AMS FIELDS<br />
[AMS FIELDS] Authors: Oliver Knill: September 2003 Literature: AMS Website
[AMS CLASSIFICATION]<br />
AMS CLASSIFICATION<br />
00-xx General<br />
01-xx History and biography<br />
03-xx Mathematical logic and foundations<br />
05-xx Combinatorics<br />
06-xx Order, lattices, ordered algebraic structures<br />
08-xx General algebraic systems<br />
11-xx Number theory<br />
12-xx Field theory and polynomials<br />
13-xx Commutative rings and algebras<br />
14-xx Algebraic geometry<br />
15-xx Linear and multilinear algebra; matrix theory<br />
16-xx Associative rings and algebras<br />
17-xx Nonassociative rings and algebras<br />
18-xx Category theory; homological algebra<br />
19-xx K-theory<br />
20-xx Group theory and generalizations<br />
22-xx Topological groups, Lie groups<br />
26-xx Real functions<br />
28-xx Measure and integration<br />
30-xx Functions <strong>of</strong> a complex variable<br />
31-xx Potential theory<br />
32-xx Several complex variables and analytic spaces<br />
33-xx Special functions<br />
34-xx Ordinary differential equations<br />
35-xx Partial differential equations<br />
37-xx Dynamical systems and ergodic theory<br />
39-xx Difference and functional equations<br />
40-xx Sequences, series, summability<br />
41-xx Approximations and expansions<br />
42-xx Fourier analysis<br />
43-xx Abstract harmonic analysis<br />
44-xx Integral transforms, operational calculus<br />
45-xx Integral equations<br />
46-xx Functional analysis<br />
47-xx Operator theory<br />
49-xx Calculus <strong>of</strong> variations and optimal control; optimization<br />
51-xx Geometry<br />
52-xx Convex and discrete geometry<br />
53-xx Differential geometry<br />
54-xx General topology<br />
55-xx Algebraic topology<br />
57-xx Manifolds and cell complexes<br />
58-xx Global analysis, analysis on manifolds<br />
60-xx Probability theory and stochastic processes<br />
70-xx Mechanics <strong>of</strong> particles and systems<br />
74-xx Mechanics <strong>of</strong> deformable solids<br />
76-xx Fluid mechanics<br />
78-xx Optics, electromagnetic theory<br />
80-xx Classical thermodynamics, heat transfer<br />
81-xx Quantum theory<br />
82-xx Statistical mechanics, structure <strong>of</strong> matter<br />
83-xx Relativity and gravitational theory<br />
85-xx Astronomy and astrophysics<br />
86-xx Geophysics<br />
90-xx Operations research, mathematical programming<br />
91-xx Game theory, economics, social and behavioral sciences<br />
92-xx Biology and other natural sciences<br />
93-xx Systems theory; control<br />
94-xx Information and communication, circuits
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 1 entries in this file.
Index<br />
AMS CLASSIFICATION, 2<br />
4
<strong>ENTRY</strong> MATH CITATIONS<br />
[<strong>ENTRY</strong> MATH CITATIONS] Collected by Oliver Knill: 2000-2002<br />
solution<br />
[solution] Every problem in the calculus <strong>of</strong> variations has a solution, provided the word solution is suitably<br />
understood. – David Hilbert<br />
enhusiast<br />
[enhusiast] The real mathematician is an enthusiast per se. Without enthusiasm no mathematics. – Novalis<br />
[royal] There is no royal road to geometry. – Euclid<br />
royal<br />
computer<br />
[computer] One may be a mathematician <strong>of</strong> the first rank without being able to compute. It is possible to be a<br />
great computer without having the slightest idea <strong>of</strong> mathematics – Novalis<br />
analysis<br />
[analysis] Geometry may sometimes appear to take the lead over analysis, but in fact precedes it only as a<br />
servant goes before his master to clear the path and light him on the way. – James Joseph Sylvester<br />
freedom<br />
[freedom] The essence <strong>of</strong> mathematics lies in its freedom. – Georg Cantor<br />
fantasy<br />
[fantasy] Fantasy, energy, self-confidence and self-criticism are the characteristic endowments <strong>of</strong> the mathematician.<br />
– Sophus Lie<br />
magacian<br />
[magacian] Pure mathematics is the magician’s real wand. – Novalis
axiomatics<br />
[axiomatics] When a mathematician has no more ideas, he pursues axiomatics. – Felix Klein<br />
turbulence<br />
[turbulence] The paper ”On the nature <strong>of</strong> turbulence” with F. Takens was eventually published in a scientific<br />
journal. (Actually, I was an editor <strong>of</strong> the journal, and I accepted the paper by myself for publication. This is<br />
not a recommended procedure in general, but I felt that it was justified in this particular case). – D. Ruelle, in<br />
Chance and Chaos<br />
hairy-ball<br />
[hairy-ball] A good topological theorem to mention any time is the theorem which, in essence, states that<br />
however you try to comb the hair on a hairy ball, you can never do it smoothly - the so-called ’hairy-ball’<br />
theorem. You can make snide comments about the grooming <strong>of</strong> the hosts’ dog or cat in the meantime as you<br />
pick hairs <strong>of</strong>f your trouser leg. – R. Ainsley in Bluff your way in Maths, 1988<br />
large<br />
[large] LARGE NUMBERS: (10 n means that 10 is raised to the n’th power)<br />
104 One ”myriad”. The largest numbers, the Greeks were considering.<br />
105 The largest number considered by the Romans.<br />
10 10 The age <strong>of</strong> our universe in years.<br />
1022 Distance to our neighbor galaxy Andromeda in meters.<br />
1023 Number <strong>of</strong> atoms in two gram Carbon (Avogadro).<br />
1026 Size <strong>of</strong> universe in meters.<br />
1041 Mass <strong>of</strong> our home galaxy ”milky way” in kg.<br />
1051 Archimedes’s estimate <strong>of</strong> number <strong>of</strong> sand grains in universe.<br />
1052 Mass <strong>of</strong> our universe in kg.<br />
1080 The number <strong>of</strong> atoms in our universe.<br />
10100 One ”googol”. (Name coined by 9 year old nephew <strong>of</strong> E. Kasner).<br />
10153 Number mentioned in a myth about Buddha.<br />
10155 Size <strong>of</strong> ninth Fermat number (factored in 1990).<br />
10 (106 ) Size <strong>of</strong> large prime number (Mersenne number, Nov 1996).<br />
10 (107 ) Years, ape needs to write ”hound <strong>of</strong> Baskerville” (random typing).<br />
10 (10( 33)) Inverse is chance that a can <strong>of</strong> beer tips by quantum fluctuation.<br />
10 (10( 42)) Inverse is probability that a mouse survives on sun for a week.<br />
10 (1051)) Inverse is chance to find yourself on Mars (quantum fluctuations)<br />
10 (10100) One ”Gogoolplex”, Decimal expansion can not exist in universe.<br />
– from R.E. Crandall, Scient. Amer., Feb. 1997<br />
analytic<br />
[analytic] The statement sometimes made, that there exist only analytic functions in nature, is in my opinion<br />
absurd. – F. Klein, Lectures on <strong>Mathematics</strong>, 1893
violence<br />
[violence] The introduction <strong>of</strong> numbers as coordinates ... is an act <strong>of</strong> violence... – H. Weyl, Philosophy <strong>of</strong><br />
<strong>Mathematics</strong> and Natural Science 1949<br />
beauty<br />
[beauty] <strong>Mathematics</strong> possesses not only truth but supreme beauty - a beauty cold and austere, like that <strong>of</strong> a<br />
sculpture – Bertrand Russell<br />
geometry<br />
[geometry] Geometry is magic that works... – R. Thom. Stability Structurelle et Morphogenese, 1972<br />
Zermelo<br />
[Zermelo] Ernst Zermelo, who created a system <strong>of</strong> axioms for set theory, was a Privatdozent at Goettingen when<br />
Herr Geheimrat Felix Klein held sway over the fabled mathematics department. As Pauli told it, ”Zermelo taught<br />
a course on mathematical logic and stunned his students by posing the following question: All mathematicians<br />
in Goettingen belong to one <strong>of</strong> two classes. In the first class belong those mathematicians who do what Felix<br />
Klein likes, but what they dislike. In the second class are those mathematicians who do what Felix Klein likes,<br />
but what they dislike. To what class does Felix Klein belong?” Jordan, having listened intently, broke into<br />
roaring laughter. Pauli paused, took a sip <strong>of</strong> wine and said disapprovingly, ”Herr Jordan, you have laughed<br />
too soon”. He continued: ”None <strong>of</strong> the awed students could solve this blasphemous problem. Zermelo then<br />
crowed in his high-pitched voice, ’But, meine Herren, it’s very simple. Felix Klein isn’t a mathematician.’”<br />
Jordan laughed again. Pauli drained his wine glass approvingly and concluded with ”Zermelo was not <strong>of</strong>fered a<br />
pr<strong>of</strong>essorship at Goettingen”. – E.L. Schucking, in ’Jordan, Pauli,Politics, Brecht and a variable gravitational<br />
constant’ Physics Today, Oct. 1999<br />
Conway<br />
[Conway] In the beginning, everything was void, and J.H.W.H.Conway began to create numbers. Conway said,<br />
”Let there be two rules which bring forth all numbers large and small. This shall be the first rule: Every<br />
number corresponds to two sets <strong>of</strong> previously created numbers, such that no member <strong>of</strong> the left set is greater<br />
than or equal to any member <strong>of</strong> the right set. And the second rule shall be this: One number is less than or<br />
equal to another number if and only if no member <strong>of</strong> the first number’s left set is greater than or equal to the<br />
second number, and no member <strong>of</strong> the second number ’s right set is less than or equal to the first number.”<br />
And Conway examined these two rules he had made, and behold! they were very good. And the first number<br />
was created from the void left set and the void right set. Conway called this number ”zero”, and said that it<br />
shall be a sign to separate positive numbers from negative numbers. Conway proved that zero was less than or<br />
equal to zero, and he saw that it was good. And the evening and the morning were the day <strong>of</strong> zero. On the<br />
next day, two more numbers were created, one with zero as its left set and one with zero as its right set. And<br />
Conway called the former number ”one”, and the latter he called ”minus one”. And he proved that minus one<br />
is less than but not equal to zero and zero is less than but not equal to one. And the evening... – D. Knuth,<br />
Surreal numbers, 1979
[obvious] <strong>Mathematics</strong> consists essentially <strong>of</strong> :<br />
a) proving the obvious<br />
b) proving the not so obvious<br />
c) proving the obviously untrue<br />
obvious<br />
For example, it took mathematicians until the 1800’ies to prove that 1+1=2 and not before the late 1970 were<br />
they confident <strong>of</strong> proving that any map requires no more than four colors to make it look nice, a fact known by<br />
cartographers for centuries. There are many not-so-obvious things which can be proved true too. Like the fact<br />
that for any group <strong>of</strong> 23 people, there is an even chance two or more <strong>of</strong> them share birthdays. (With groups<br />
<strong>of</strong> twins this becomes almost certain. Not quite certain as you will <strong>of</strong> course point out: they might all have<br />
been born either side <strong>of</strong> midnight). Mathematicians are also fond <strong>of</strong> proving things which are obviously false,<br />
like all straight lines being curved, and an engaged telephone being just as likely to be free if you ring again<br />
immediately after, as if you wait twenty minutes. – R. Ainsley in Bluff your way in Maths, 1988<br />
infimum<br />
[infimum] There exists a subset <strong>of</strong> the real line such that the infimum <strong>of</strong> the set is greater then the supremum<br />
<strong>of</strong> the set. – Gary L. Wise and Eric B. Hall, Counter examples in probability and real analysis, 1993, First<br />
Example in book<br />
transcendental<br />
[transcendental] Transcendental number : A number which is not the root <strong>of</strong> any polynomial equation, like pi<br />
and e, and which can only be understood after several hours meditation in the lotus position. – R. Ainsley in<br />
Bluff your way in Maths, 1988<br />
illiteracy<br />
[illiteracy] There are great advantages to being a mathematician: a) you do not have to be able to spell b) you<br />
do not have to be able to add up The illiteracy <strong>of</strong> mathematicians is taken for granted. There still persists a<br />
myth that mathematics somehow involves numbers. Many fondly believe that university students spend their<br />
time long dividing by 173 and learning their 39 times table; in fact, the reverse is true. Mathematicians are<br />
renowned for their inability to add up or take away, in much the same way as geographers are always getting<br />
lost, and economists are always borrowing money <strong>of</strong>f you. – R. Ainsley in Bluff your way in Maths, 1988<br />
prime<br />
[prime] In this note we would like to <strong>of</strong>fer an elementary ’topological’ pro<strong>of</strong> <strong>of</strong> the infinitude <strong>of</strong> the prime<br />
numbers. We introduce a topology into the space <strong>of</strong> integers S, by using the arithmetic progressions (from<br />
-infinity to +infinity) as a basis. It is not difficult to verify that this actually yields a topological space. In<br />
fact, under this topology, S may be shown to be normal and hence metrisable. Each arithmetic progression is<br />
closed as well as open, since its complement is the union <strong>of</strong> the other arithmetic progressions (having the same<br />
difference). As a result, the union <strong>of</strong> any finite number <strong>of</strong> arithmetic progressions is closed. Consider now the<br />
set A which is the union <strong>of</strong> A(p), where A(p) consists <strong>of</strong> primes greater or equal to p. The only numbers not<br />
belonging to A are -1 and 1, and since the set -1,1 is clearly not an open set, A cannot be closed. Hence A is<br />
not a finite union <strong>of</strong> closed sets, which proves that there is an infinity <strong>of</strong> primes. – H. Fuerstenberg, On the<br />
infinitude <strong>of</strong> primes, American Mathematical Montly, 62, 1955, p. 353
arber<br />
[barber] The barber in a certain town shaves all the people who don’t shave themselves. Who shaves the barber?<br />
This is meant to be a clever little paradox with no solution but you can annoy the asker intensely by saying it’s<br />
easy and that the barber is a women. You can then ask the following (a version <strong>of</strong> Russell’s Paradox, - point<br />
this out too): in a library there are some books for the catalogue section which is a list <strong>of</strong> all books which don’t<br />
list themselves. Shold he or she include this book in its own list? If so, then it becomes a book which lists<br />
itself, so it shouldn’t be in the list <strong>of</strong> books which don’t and vice versa. This should keep the most determined<br />
assailant at bay while you attack the wine. – R. Ainsley in Bluff your way in Maths, 1988<br />
Hadamard<br />
[Hadamard] Hadamard, trying to find a job in a US university, came to a small university and was received<br />
by the chairman <strong>of</strong> the department <strong>of</strong> mathematics. He explained who he was and gave his curriculum vitae.<br />
The chairman said: ’our means are very limited and I can not promise that we shal take you’. Then Hadamard<br />
noticed that among the portraits on he wall was his own. ’That’s me!’ he said. ’Well, come again in a week,<br />
we shal think about this’. On his next visit, the answer was negative and his portrait had been removed. –<br />
Vladimir Mazya and Tatyana Shaposhnikova, in Jacques Hadamard, a universal Mathematician, AMS History<br />
<strong>of</strong> <strong>Mathematics</strong> Volume 14<br />
Cantor<br />
[Cantor] The appropriate object is known as the Cantor set, because it was discovered by Henry Smith in 1875.<br />
(The founder <strong>of</strong> set theory, Georg Cantor, used Smith’s invention in 1883. Let’s fact it, ’Smith set’ isn’t very<br />
impressive, is it?) – Ian Stewart, in Does God Play Dice, 1989 p. 121<br />
jouissance<br />
[jouissance] ... Thus the erectile organ comes to symbolize the place <strong>of</strong> jouissance, not in itself, or even in the<br />
form <strong>of</strong> an image, but as a part lacking in the desired image: that is why it is equivalent to the (−1) ( 1/2) <strong>of</strong> the<br />
signification produced above, <strong>of</strong> the Jouissance that it restores by the coefficient <strong>of</strong> its statement to the function<br />
<strong>of</strong> lack <strong>of</strong> signifier (−1).<br />
– Lacan, Ecrits, Paris 1966 (cited in ’Fashionable nonsense’ by Alan Sokal and Jean Bricmont)<br />
Mandelbrot<br />
[Mandelbrot] Mandelbrot made quite good computer pictures, which seemed to show a number <strong>of</strong> isolated<br />
”islands” (in the Mandelbrot set M). Therefore, he conjectured that the set M has many distinct connected<br />
components. (The editors <strong>of</strong> the journal thought that his islands were specks <strong>of</strong> dirt, and carefully removed<br />
them from the pictures). – John Milnor, in Dynamics in one complex variable, 1991<br />
sin<br />
[sin] sin, cos, tan, cot, sec, cosec - Formulae derived from the sides <strong>of</strong> triangles but which crop up in completely<br />
unexpected places. Sins are extremely common, but rarely do you encounter secs in mathematics. – R. Ainsley<br />
in Bluff your way in Maths, 1988
Moser<br />
[Moser] This reminds me <strong>of</strong> the Hilbert story, which I learned from my teacher Franz Rellich in Goettingen:<br />
When Hilbert - who was old and retired - was asked at a party by the newly appointed Nazi-minister <strong>of</strong><br />
education: ”Herr Geheimrat, how is mathematics in Goettingen, now that it has been freed <strong>of</strong> the Jewish<br />
influences” he replied: ”<strong>Mathematics</strong> in Goettingen? That does not EXIST anymore”. – Jurgen Moser, in<br />
Dynamical Systems-Past and Present, Doc. Math. J. DMV I p. 381-402, 1998<br />
wine<br />
[wine] There are two glasses <strong>of</strong> wine, one white and one red. A teaspoonful <strong>of</strong> wine is taken from the red and<br />
mixed in with the white. Then a teaspoonful <strong>of</strong> this mixture is taken and mixed in with the red. Which is<br />
bigger, the amount <strong>of</strong> red in the white or the amount <strong>of</strong> white in the red? The answer is that the’re both the<br />
same, because there’s the same volume in each glass, so whatever quantity <strong>of</strong> red is in the white must be equal<br />
to the quantity <strong>of</strong> white in the red. However in practice it is impossible to do this because the white always<br />
runs out first at parties and the red always gets spilt on someone’s white trousers. – R. Ainsley in Bluff your<br />
way in Maths, 1988<br />
Monty-Hall<br />
[Monty-Hall] ”Suppose you’re on a game show and you are given a choice <strong>of</strong> three doors. Behind one door is a<br />
car and behind the others are goats. You pick a door-say No. 1 - and the host, who knows what’s behind the<br />
doors, opens another door-say, No. 3-which has a goat. (In all games, the host opens a door to reveal a goat).<br />
He then says to you, ”Do you want to pick door No. 2?” (In all games he always <strong>of</strong>fers an option to switch). Is<br />
it to your advantage to switch your choice?” – The three doors problem, also known as Monty-Hall Problem<br />
sex<br />
[sex] Pure mathematician - Anyone who prefers set theory to sex. – R. Ainsley in Bluff your way in Maths,<br />
1988<br />
mad<br />
[mad] There was a mad scientist ( a mad ...social... scientist ) who kidnaped three colleagues, an engineer, a<br />
physicist, and a mathematician, and locked each <strong>of</strong> them in separate cells with plenty <strong>of</strong> canned food and water<br />
but no can opener. A month later, returning, the mad scientist went to the engineer’s cell and found it long<br />
empty. The engineer had constructed a can opener from pocket trash, used aluminum shavings and dried sugar<br />
to make an explosive, and escaped. The physicist had worked out the angle necessary to knock the lids <strong>of</strong>f<br />
the tin cans by throwing them against the wall. She was developing a good pitching arm and a new quantum<br />
theory. The mathematician had stacked the unopened cans into a surprising solution to the kissing problem;<br />
his dessicated corpse was propped calmly against a wall, and this was inscribed on the floor in blood:<br />
Theorem: If I can’t open these cans, I’ll die. Pro<strong>of</strong>: assume the opposite...
induction<br />
[induction] Pro<strong>of</strong> by induction - A very important and powerful mathematical tool, because it works by assuming<br />
something is true and then goes on to prove that therefore it is true. Not surprisingly, you can prove almost<br />
everything by induction. So long as the pro<strong>of</strong> includes the following phrases:<br />
a) Assume true for n; then also true for n+1 because.. (followed by some plausible but messy working out in<br />
which n, n+1 appear prominently).<br />
b) But is true for n=0 (a little more messy working out with lots <strong>of</strong> zeros sprayed at random through the pro<strong>of</strong>).<br />
c) So is true for all n. Q.E.D.<br />
– R. Ainsley in Bluff your way in Maths, 1988<br />
horse<br />
[horse] LEMMA: All horses are the same color. Pro<strong>of</strong> (by induction): Case n=1: In a set with only one horse,<br />
it is obvious that all horses in that set are the same color. Case n=k: Suppose you have a set <strong>of</strong> k+1 horses.<br />
Pull one <strong>of</strong> these horses out <strong>of</strong> the set, so that you have k horses. Suppose that all <strong>of</strong> these horses are the same<br />
color. Now put back the horse that you took out, and pull out a different one. Suppose that all <strong>of</strong> the k horses<br />
now in the set are the same color. Then the set <strong>of</strong> k+1 horses are all the same color. We have k true =¿ k+1<br />
true; therefore all horses are the same color.<br />
THEOREM: All horses have an infinite number <strong>of</strong> legs. Pro<strong>of</strong> (by intimidation): Everyone would agree that<br />
all horses have an even number <strong>of</strong> legs. It is also well-known that horses have fore-legs in front and two legs in<br />
back. But 4 + 2 = 6 legs is certainly an odd number <strong>of</strong> legs for a horse to have! Now the only number that is<br />
both even and odd is infinity; therefore all horses have an infinite number <strong>of</strong> legs. However, suppose that there<br />
is a horse somewhere that does not have an infinite number <strong>of</strong> legs. Well, that would be a horse <strong>of</strong> a different<br />
color; and by the Lemma, it doesn’t exist. QED<br />
dean<br />
[dean] Dean, to the physics department. ”Why do I always have to give you guys so much money, for laboratories<br />
and expensive equipment and stuff. Why couldn’t you be like the maths department - all they need is money<br />
for pencils, paper and waste-paper baskets. Or even better, like the philosophy department. All they need are<br />
pencils and paper.”<br />
astronomer<br />
[astronomer] An astronomer, a physicist and a mathematician were holidaying in Scotland. Glancing from a<br />
train window, they observed a black sheep in the middle <strong>of</strong> a field. ”How interesting,” observed the astronomer,<br />
”all Scottish sheep are black!” To which the physicist responded, ”No, no! Some Scottish sheep are black!”<br />
The mathematician gazed heavenward in supplication, and then intoned, ”In Scotland there exists at least one<br />
field, containing at least one sheep, at least one side <strong>of</strong> which is black.” – J. Steward in ’Concepts <strong>of</strong> Modern<br />
<strong>Mathematics</strong>’
c<strong>of</strong>fee<br />
[c<strong>of</strong>fee] An engineer, a chemist and a mathematician are staying in three adjoining cabins at an old motel. First<br />
the engineer’s c<strong>of</strong>fee maker catches fire. He smells the smoke, wakes up, unplugs the c<strong>of</strong>fee maker, throws it out<br />
the window, and goes back to sleep. Later that night the chemist smells smoke too. He wakes up and sees that<br />
a cigarette butt has set the trash can on fire. He says to himself, ”Hmm. How does one put out a fire? One<br />
can reduce the temperature <strong>of</strong> the fuel below the flash point, isolate the burning material from oxygen, or both.<br />
This could be accomplished by applying water.” So he picks up the trash can, puts it in the shower stall, turns<br />
on the water, and, when the fire is out, goes back to sleep. The mathematician, <strong>of</strong> course, has been watching<br />
all this out the window. So later, when he finds that his pipe ashes have set the bed-sheet on fire, he is not in<br />
the least taken aback. He says: ”Aha! A solution exists!” and goes back to sleep.<br />
logs<br />
[logs] Taking logs - Broadly speaking, any equation which looks difficult will look much easier when logs are<br />
taken on both sides. Taking logs on one side only is tempting for many equations, but may be noticed. – R.<br />
Ainsley in Bluff your way in Maths, 1988<br />
cat<br />
[cat] Theorem: A cat has nine tails. Pro<strong>of</strong>: No cat has eight tails. A cat has one tail more than no cat.<br />
Therefore, a cat has nine tails.<br />
chocolate<br />
[chocolate] Prime number - A number with no divisors. Boxes <strong>of</strong> chocolates always contain a prime number so<br />
that, whatever the number <strong>of</strong> people present, somebody has to have that one left over. – R. Ainsley in Bluff<br />
your way in Maths, 1988<br />
aleph<br />
[aleph] Aleph-null bottles <strong>of</strong> beer on the wall, Aleph-null bottles <strong>of</strong> beer, You take one down, and pass it around,<br />
Aleph-null bottles <strong>of</strong> beer on the wall.<br />
qed<br />
[qed] At the end <strong>of</strong> a pro<strong>of</strong> you write Q.E.D, which stands not for Quod Erat Demonstrandum as the books<br />
would have you believe, but for Quite Easily Done. – R. Ainsley in Bluff your way in Maths, 1988<br />
[1+1] 1+1 = 3, for large values <strong>of</strong> 1<br />
1+1
painting<br />
[painting] Group theory - An exceedingly beautiful branch <strong>of</strong> pure mathematics used for showing in how many<br />
ways blocks <strong>of</strong> wood can be painted. – R. Ainsley in Bluff your way in Maths, 1988<br />
engeneer<br />
[engeneer]<br />
Mathematician: 3 is prime,5 is prime,7 is prime, by induction - every odd integer higher than 2 is prime.<br />
Physicist: 3 is prime, 5 is prime, 7 is prime, 9 is an experimental error, 11 is prime,...<br />
Engineer: 3 is prime, 5 is prime, 7 is prime, 9 is prime, 11 is prime,...<br />
Programmer: 3’s prime, 5’s prime, 7’s prime, 7’s prime, 7’s prime,...<br />
Salesperson: 3 is prime, 5 is prime, 7 is prime, 9 – we’ll do for you the best we can,...<br />
S<strong>of</strong>tware seller: 3 is prime, 5 is prime, 7 is prime, 9 will be prime in the next release,...<br />
Biologist: 3 is prime, 5 is prime, 7 is prime, 9 – results have not arrived yet,...<br />
Advertiser: 3 is prime, 5 is prime, 7 is prime, 11 is prime,...<br />
Lawyer: 3 is prime, 5 is prime, 7 is prime, 9 – there is not enough evidence to prove that it is not prime,...<br />
Accountant: 3 is prime, 5 is prime, 7 is prime, 9 is prime, deducing 10 percent tax and 5 percent other obligations.<br />
Statistician: Let’s try several randomly chosen numbers: 17 is prime, 23 is prime, 11 is prime...<br />
Psychologist: 3 is prime, 5 is prime, 7 is prime, 9 is prime but tries to suppress it,...<br />
[pi] PI= 3.14159265358979323846264338327950288419716939937510582097494459230781640628<br />
[e] Euler E= 2.71828182845904523536028747135266249775724709369995957496696762772407663035<br />
pi<br />
e<br />
cancel<br />
[cancel] THEOREM: The limit as n goes to infinity <strong>of</strong> sin x/n is 6. PROOF: cancel the n in the numerator and<br />
denominator.<br />
c<strong>of</strong>fee<br />
[c<strong>of</strong>fee] A mathematician is a device for turning c<strong>of</strong>fee into theorems. – P. Erdos<br />
stupider<br />
[stupider] Finally I am becoming stupider no more. – Epitaph, P. Erdos wrote for himself
Erdoes<br />
[Erdoes]<br />
epsilon child<br />
bosses women<br />
slaves men<br />
captured married<br />
liberated divorced<br />
recaptured remarried<br />
trivial beings nonmathematicians<br />
noise music<br />
poison alcohol<br />
preaching giving a lecture<br />
supreme fascist god<br />
died stopped doing mathematics<br />
preach lecture<br />
Joedom UDSSR<br />
Samland USA<br />
on the long wave length communists on the short wave length fashists – from the vocabulary <strong>of</strong> P. Erdos ’the<br />
man who loved only numbers’<br />
Chebyshev<br />
[Chebyshev] Chebyshev said it, and I say it again There is always a prime between n and 2n – P. Erdos<br />
Outrage<br />
[Outrage] Outrage, disgust, the characterization <strong>of</strong> group theory as a plague or as a dragon to be slain - this is<br />
not an atypical physist’s reaction in the 1930s-50s to the use <strong>of</strong> group theory in physics. – S. Sternberg<br />
digits<br />
[digits] Anyone who considers arithmetical methods <strong>of</strong> producing random digits is, <strong>of</strong> course, in a state <strong>of</strong> sin.<br />
– J. von Neumann<br />
poet<br />
[poet] The mathematician’s patterns, like the painter’s or the poet’s must be beautiful; the ideas, like the colors<br />
or the words, must fit together in a harmonious way. Beauty is the first test: there is no permanent place in<br />
the world for ugly mathematics... It may be very hard to define mathematical beauty, but that is just as true<br />
<strong>of</strong> beauty <strong>of</strong> any kind - we may not know quite what we mean by a beautiful poem, but that does not prevent<br />
us from recognizing one when we read it. – G.H. Hardy<br />
melancholy<br />
[melancholy] It is a melancholy experience for a pr<strong>of</strong>essional mathematician to find himself writing about<br />
mathematics. – G.H. Hardy
Hilbert<br />
[Hilbert] There is a much quoted story about David Hilbert, who one day noticed that a certain student had<br />
stopped attending class. When told that the student had decided to drop mathematics to become a poet,<br />
Hilbert replied, ”Good- he did not have enough imagination to become a mathematician”. – R. Osserman<br />
refreree<br />
[refreree] Referee’s report: This paper contains much that is new and much that is true. Unfortunately, that<br />
which is true is not new and that which is new is not true. – H. Eves ’Return to Mathematical Circles’, 1988.<br />
weapons<br />
[weapons] Structures are the weapons <strong>of</strong> the mathematician. – N. Bourbaki<br />
undogmatic<br />
[undogmatic] <strong>Mathematics</strong> is the only instructional material that can be presented in an entirely undogmatic<br />
way. – M. Dehn<br />
solve<br />
[solve] Each problem that I solved became a rule which served afterwards to solve other problems – R. Decartes<br />
tool<br />
[tool] For a physicist mathematics is not just a tool by means <strong>of</strong> which phenomena can be calculated, it is the<br />
main source <strong>of</strong> concepts and principles by means <strong>of</strong> which new theories can be created. – F. Dyson<br />
sheet<br />
[sheet] If the entire Mandelbrot set were placed on an ordinary sheet <strong>of</strong> paper, the tiny sections <strong>of</strong> boundary<br />
we examine would not fill the width <strong>of</strong> a hydrogen atom. Physicists think about such tiny objects; only<br />
mathematicians have microscopes fine enough to actually observe them. – J. Eving
ecommendation<br />
[recommendation] Sample letter <strong>of</strong> recommendation:<br />
Dear Search Committee Chair, I am writing this letter for Mr. Still Student who has applied for a position<br />
in your department. I should start by saying that I cannot recommend him too highly. In fact, there is no<br />
other student with whom I can adequately compare him, and I am sure that the amount <strong>of</strong> mathematics he<br />
knows will surprise you. His dissertation is the sort <strong>of</strong> work you don’t expect to see these days. It definitely<br />
demonstrates his complete capabilities. In closing, let me say that you will be fortunate if you can get him to<br />
work for you. Sincerely, A. D. Advisor (Pr<strong>of</strong>.) – from MAA Focus Newsletter<br />
cube<br />
[cube] To divide a cube into two other cubes, a fourth power or in general any power whatever into two powers<br />
<strong>of</strong> the same denomination above the second is impossible, and I have assuredly found an admirable pro<strong>of</strong> <strong>of</strong><br />
this, but the margin is too narrow to contain it. – P. de Fermat<br />
reality<br />
[reality] <strong>Mathematics</strong> is not only real, but it is the only reality. That is that entire universe is made <strong>of</strong> matter,<br />
obviously. And matter is made <strong>of</strong> particles. It’s made <strong>of</strong> electrons and neutrons and protons. So the entire<br />
universe is made out <strong>of</strong> particles. Now what are the particles made out <strong>of</strong>? They’re not made out <strong>of</strong> anything.<br />
The only thing you can say about the reality <strong>of</strong> an electron is to cite its mathematical properties. So there’s a<br />
sense in which matter has completely dissolved and what is left is just a mathematical structure. – M. Gardner<br />
[arithmetic] God does arithmetic. – K.F. Gauss<br />
arithmetic<br />
hypothesis<br />
[hypothesis] Don’t just read it; fight it! Ask your own questions, look for your own examples, discover your own<br />
pro<strong>of</strong>s. Is the hypothesis necessary? Is the converse true? What happens in the classical special case? What<br />
about the degenerate cases? Where does the pro<strong>of</strong> use the hypothesis? – P.R. Halmos<br />
dice<br />
[dice] God not only plays dice. He also sometimes throws the dice where they cannot be seen. – S.W. Hawking<br />
wissen<br />
[wissen] ’Wir muessen wissen. Wir werden wissen.’ (We have to know. We will know.) – D. Hilbert (engraved<br />
in tombstone)
physics<br />
[physics] Physics is much too hard for physicists. – D. Hilbert<br />
H<strong>of</strong>stadter<br />
[H<strong>of</strong>stadter] H<strong>of</strong>stadter’s Law: It always takes longer than you expect, even when you take into account H<strong>of</strong>stadter’s<br />
Law. – D.R. H<strong>of</strong>stadter, Goedel-Escher-Bach<br />
experience<br />
[experience] The science <strong>of</strong> mathematics presents the most brilliant example <strong>of</strong> how pure reason may successfully<br />
enlarge its domain without the aid <strong>of</strong> experience. – E. Kant<br />
doughnut<br />
[doughnut] A topologist is one who doesn’t know the difference between a doughnut and a c<strong>of</strong>fee cup. – J.<br />
Kelley<br />
Kovalevsky<br />
[Kovalevsky] Say what you know, do what you must, come what may. – S. Kovalevsky<br />
god<br />
[god] God made the integers, all else is the work <strong>of</strong> man. – L. Kronecker<br />
abstract<br />
[abstract] There is no branch <strong>of</strong> mathematics, however abstract, which may not some day be applied to phenomena<br />
<strong>of</strong> the real world. – N. Lobatchevsky<br />
medicine<br />
[medicine] Medicine makes people ill, mathematics make them sad and theology makes them sinful. – M. Luther
intelligence<br />
[intelligence] The mathematician who pursues his studies without clear views <strong>of</strong> this matter, must <strong>of</strong>ten have<br />
the uncomfortable feeling that his paper and pencil surpass him in intelligence. – E. Mach<br />
flesh<br />
[flesh] I tell them that if they will occupy themselves with the study <strong>of</strong> mathematics they will find in it the best<br />
remedy against the lusts <strong>of</strong> the flesh. – T. Mann<br />
philosophers<br />
[philosophers] Today, it is not only that our kings do not know mathematics, but our philosophers do not know<br />
mathematics and - to go a step further - our mathematicians do not know mathematics. – J.R. Oppenheimer<br />
obvious<br />
[obvious] <strong>Mathematics</strong> consists <strong>of</strong> proving the most obvious thing in the least obvious way. – G. Polya<br />
whispers<br />
[whispers] However successful the theory <strong>of</strong> a four dimensional world may be, it is difficult to ignore a voice<br />
inside us which whispers: ”At the back <strong>of</strong> your mind, you know a fourth dimension is all nonsense”. I fancy<br />
that voice must have had a busy time in the past history <strong>of</strong> physics. What nonsense to say that this solid table<br />
on which I am writing is a collection <strong>of</strong> electrons moving with prodigious speed in empty spaces, which relative<br />
to electronic dimensions are as wide as the spaces between the planets in the solar system! What nonsense to<br />
say that the thin air is trying to cursh my body with a load <strong>of</strong> 14 lbs. to the square inch! What nonsense that<br />
the star cluster which I see through the telescope, obviously there NOW, is a glimpse into a past age 50’000<br />
years ago! Let us not be beguiled by this voice. It is discredited... – Sir Arthur Eddington<br />
decimal<br />
[decimal] The first million decimal places <strong>of</strong> pi are comprised <strong>of</strong>:<br />
99959 0’s<br />
99758 1’s<br />
100026 2’s<br />
100229 3’s<br />
100230<br />
100359<br />
4’s<br />
5’s<br />
–David Blatner, the joy <strong>of</strong> pi<br />
99548 6’s<br />
99800 7’s<br />
99985 8’s<br />
100106 9’s
historians<br />
[historians] Math historians <strong>of</strong>ten state that the Egyptians thought pi = 256/81. In fact, there is no direct<br />
evidence that the Egyptians conceived <strong>of</strong> a constant number pi, much less tried to calculate it. Rather, they<br />
were simply interested in finding the relationship between the circle and the square, probably to accomplish the<br />
task <strong>of</strong> precisely measuring land and buildings. –David Blatner, the joy <strong>of</strong> pi<br />
[pi]<br />
2000 BC Babilonians use pi=25/8, Egyptians use pi=256/81<br />
1100 BC Chinese use pi=3<br />
200 AC Ptolemy uses pi=377/120<br />
450 Tsu Ch’ung-chih uses pi=255/113<br />
530 Aryabhata uses pi=62832/20000<br />
650 Brahmagupta uses pi=sqrt(10)<br />
1593 Romanus finds pi to 15 decimal places<br />
1596 Van Ceulen calculates pi to 32 places<br />
1699 Sharp calculates pi to 72 places<br />
1719 Tantet de Lagny calculates pi to 127 places<br />
1794 Vega calculates pi to 140 decimal places<br />
1855 Richter calculates pi to 500 decimal places<br />
1873 Shanks finds 527 decimal places<br />
1947 Ferguson calculates 808 places<br />
1949 ENIAC computer finds 2037 places<br />
1955 NORC computer computes 3089 places<br />
1959 IBM 704 computer finds 16167 places<br />
1961 Shanks-Wrench (IBM7090) find 100200 places<br />
1966 IBM 7030 computes 250000 places<br />
1967 CDC6600 computes 500000 places<br />
1973 Guilloud-Bouyer (CDC7600) find 1 Mio places<br />
1983 Tamura-Kanada (HITACM-280H) compute 16 Mio places<br />
1988 Kanada (HITAC M-280H) computes 16 Mio digits<br />
1989 Chudnovsky finds 1000 Mio digits<br />
1995 Kanada computes pi to 6000 Mio digits<br />
1996 Chudnovsky computes pi to 8000 Mio digits<br />
1997 Kanada determines pi to 51000 Mio digits<br />
–David Blatner, the joy <strong>of</strong> pi<br />
pi<br />
FBI<br />
[FBI] The following is a transcript <strong>of</strong> an interchange between defence attorney Robert Blasier and FBI Special<br />
Agent Roger Martz on July 26, 1995, in the courtroom <strong>of</strong> the O.J. Simpson trial:<br />
Q: Can you calculate the area <strong>of</strong> a circle with a five-millimeter diameter? A: I mean I could. I don’t...math<br />
I don’t ... I don’t know right now what it is. Q: Well, what is the formula for the area <strong>of</strong> a circle? A: Pi R<br />
Squared Q: What is pi? A: Boy, you ar really testing me. 2.12... 2.17... Judge Ito: How about 3.1214? Q:<br />
Isn’t pi kind <strong>of</strong> essential to being a scientist knowing what it is? A: I haven’t used pi since I guess I was in<br />
high school. Q: Let’s try 3.12. A: Is that what it is? There is an easier way to do... Q: Let’s try 3.14. And<br />
what is the radius? A: It would be half the diameter: 2.5 Q: 2.5 squared, right? A: Right. Q: Your honor, may<br />
we borrow a calculator? [pause] Q: Can you use a calculator? A: Yes, I think. Q: Tell me what pi times 2.5<br />
squared is. A: 19 Q: Do you want to write down 19? Square millimeters, right? The area. What is one tenth<br />
<strong>of</strong> that? A: 1.9 Q: You miscalculated by a factor <strong>of</strong> two, the size, the minimum size <strong>of</strong> a swatch you needed to<br />
detect EDTA didn’t you? A: I don’t know that I did or not. I calculated a little differently. I didn’t use this.<br />
Q: Well, does the area change by the different method <strong>of</strong> calculation? A: Well, this is all estimations based on<br />
my eyeball. I didn’t use any scientific math to determine it. –David Blatner, the joy <strong>of</strong> pi
eauty<br />
[beauty] To those who do not know <strong>Mathematics</strong> it is difficult to get across a real feeling as to the beauty,<br />
the deepest beauty <strong>of</strong> nature. ... If you want to learn about nature, to appreciate nature, it is necessary to<br />
understand the language that she speaks in. – Richard Feynman in ”The Character <strong>of</strong> Physical Law”<br />
Bacon<br />
[Bacon] All science requires <strong>Mathematics</strong>. The knowledge <strong>of</strong> mathematical things is almost innate in us... This<br />
is the easiest <strong>of</strong> sciences, a fact which is obvious in that no one?s brain rejects it; for laymen and people who<br />
are utterly illiterate know how to count and reckon. – Roger Bacon<br />
deductions<br />
[deductions] Pure mathematics consists entirely <strong>of</strong> such asseverations as that, if such and such a proposition is<br />
true <strong>of</strong> anything, then such and such another proposition is true <strong>of</strong> that thing... It’s essential not to discuss<br />
whether the proposition is really true, and not to mention what the anything is <strong>of</strong> which it is supposed to<br />
be true... If our hypothesis is about anything and not about some one or more particular things, then our<br />
deductions constitute mathematics. Thus mathematics may be defined as the subject in which we never know<br />
what we are talking about, nor whether what we are saying is true. – Bertrand Russell<br />
ambitious<br />
[ambitious] The more ambitious plan may have more chances <strong>of</strong> success – G. Polya, How To Solve It<br />
fourteen<br />
[fourteen] THEOREM: Every natural number can be completely and unambiguously identified in fourteen words<br />
or less. PROOF: 1. Suppose there is some natural number which cannot be unambiguously described in fourteen<br />
words or less. 2. Then there must be a smallest such number. Let’s call it n. 3. But now n is ”the smallest<br />
natural number that cannot be unambiguously described in fourteen words or less”. 4. This is a complete<br />
and unambiguous description <strong>of</strong> n in fourteen words, contradicting the fact that n was supposed not to have<br />
such a description! 5. Since the assumption (step 1) <strong>of</strong> the existence <strong>of</strong> a natural number that cannot be<br />
unambiguously described in fourteen words or less led to a contradiction, it must be an incorrect assumption.<br />
6.Therefore, all natural numbers can be unambiguously described in fourteen words or less!<br />
1=2<br />
[1=2] THEOREM: 1=2 PROOF:<br />
1. Let a = b.<br />
2. Then a 2 = ab,<br />
3. a 2 + a 2 = a 2 + ab,<br />
4. 2a 2 = a 2 + ab,<br />
5. 2a 2 − 2ab = a 2 + ab − 2ab,<br />
6. and 2a 2 − 2ab = a 2 − ab<br />
7. Writing this as 2(a 2 − ab) = 1(a 2 − ab),<br />
8. and cancelling the (a 2 − ab) from both sides gives 1 = 2.
primes<br />
[primes] II III V VII XI XIII XVII XIX XXIII XXIX ...<br />
Queen<br />
[Queen] ”Can you do addition?” the White Queen asked. ”What’s one and one and one and one and one and<br />
one and one and one and one and one?” ”I don’t know,” said Alice, ”I lost count.”. – Lewis Carrol alias Charles<br />
Lutwidge Dodgson, Alice’s Adventures in Wonderland<br />
subtraction<br />
[subtraction] ”She can’t do Subtraction”, said the White Queen. ”Can you do Division? Divide a loaf by a knife<br />
– what’s the answer to that?” ”I suppose –” Alice was beginning, but the Red Queen answerd for her. ”Bread<br />
and butter, <strong>of</strong> course ...” – Lewis Carrol alias Charles Lutwidge Dodgson, Alice’s Adventures in Wonderland<br />
subtraction<br />
Theorem: the square root x <strong>of</strong> 2 is irrational. Pro<strong>of</strong>: x=n/m with gcd(n, m) = 1 implies 2 = n 2 /m 2 which is<br />
2m 2 = n 2 so that n must be even and n 2 a multiple <strong>of</strong> 4. Therefore m is even. This contradicts gcd(n,m)=1.<br />
blackboard<br />
[blackboard] It is still an unending source <strong>of</strong> surprise for me to see how a few scribbles on a blackboard or on a<br />
sheet <strong>of</strong> paper could change the course <strong>of</strong> human affairs. – Stanislaw Ulam.<br />
ephermeral<br />
[ephermeral] Of all escapes from reality, mathematics is the most successful ever. It is a fantasy that becomes<br />
all the more addictive because it works back to improve the same reality we are trying to evade. All other<br />
escapes- sex, drugs, hobbies, whatever - are ephemeral by comparison. The mathematician’s feeling <strong>of</strong> triumph,<br />
as he forces the world to obey the laws his imagimation has created, feeds on its own success. The world is<br />
premanently changed by the workings <strong>of</strong> his mind, and the certainty that his creations will endure renews his<br />
confidence as no other pursuit. – Gian-Carlo Rota<br />
[joke] A good mathematical joke is better, and better mathematics than a dozen mediocre papers.<br />
– John Edensor Littlewood<br />
joke
[Leibniz] pi/4 = 1 − 1/3 + 1/5 − 1/7 + 1/9....<br />
– Wilhelm von Leibniz<br />
Leibniz<br />
war<br />
[war] It has been said that the First World War was the chemists’ war because mustard gas and chlorine were<br />
empolyed for the first time, and that the Second World War was the physicists war, because the atom bomb<br />
was detonated. Similarly, it has been argued that the Third World War would be the mathematicians’ war,<br />
because mathematics will have control over the next great weapon <strong>of</strong> war - information. – Simon Singh, in ’The<br />
code book’<br />
clearly<br />
[clearly] Never speak more clearly than you think. – Jeremy Bernstein<br />
Piaget<br />
[Piaget] What, in effect are the conditions for the construction <strong>of</strong> formal thought? The child must not only apply<br />
operations to objects - in other words, mentally execute possible actions on them - he must also ’reflect’ those<br />
operations in the absence <strong>of</strong> the objects which are replaced by pure propositions. Thus ’reflection’ is thought<br />
raised to the second power. Concrete thinking is the representation <strong>of</strong> a possible action, and formal thinking<br />
is the representation <strong>of</strong> a representation <strong>of</strong> possible action... It is not surprising, therefore, that the system <strong>of</strong><br />
concrete operations must be completed during the last years <strong>of</strong> childhood before it can be ’reflected’ by formal<br />
operations. In terms <strong>of</strong> their function, formal operations do not differ from concrete operations except that they<br />
are applied to hypotheses or propositions whose logic is an abstract translation <strong>of</strong> the system <strong>of</strong> ’inference’ that<br />
governs concrete operations. – Jean Piaget<br />
Mersenne<br />
[Mersenne] An integer 2 n − 1 is called a Mersenne number. If it is prime, it is called a Mersenne prime. In<br />
that case, n must be prime. Known examples are n = 2, 3, 5, 7, 13, 17, 19, 31, 61, 89, 107, 127, 521, 607,<br />
1279, 2203, 2281, 3217, 4253, 4423, 9689, 9941, 11213, 19937, 21701, 23209, 44497, 86243, 110503, 132049,<br />
216091, 756839, 859433, 1257787, 1398269, 2976221, 3021377. It is not known whether there are infinitely many<br />
Mersenne primes.<br />
Mersenne<br />
A positive integer n is called a perfect number if it is equal to the sum <strong>of</strong> all <strong>of</strong> its positive divisors, excluding n<br />
itself. Examples are 6=1+2+3, 28=1+2+4+7+14. An integer k is an even perfect number if and only if it has<br />
the form 2 ( n − 1)(2 n − 1) and 2 n − 1 is prime. In that case 2 n − 1 is called a Mersenne prime and n must be<br />
prime. It is unknown whether there exists an odd perfect number.
Wilson<br />
[Wilson] WILSON’S THEOREM: p prime if and only if (p − 1)! == −1 (modp) PROOF. 1, 2, ..., p − 1 are<br />
roots <strong>of</strong> x ( p − 1) == 0 (modp). A congruence has not more roots then its degree, hence x ( p − 1) − 1 ==<br />
(x − 1)(x − 2)...(x − (p − 1)) mod p. For x=0, this gives −1 == (−1) ( p − 1)(p − 1)! == (p − 1)! which is also<br />
true for p=2.<br />
– from P. Ribenboim, ’The new book <strong>of</strong> prime number records’<br />
twin<br />
[twin] There is keen competition to produce the largest pair <strong>of</strong> twin primes. On October 9, 1995, Dubner<br />
discovered the largest known pair <strong>of</strong> twin primes p, p + 2, where p = 570918348 ∗ 10 5120 − 1. It took only one<br />
day with 2 crunchers. The expected time would be 150 times longer! What luck! – from P. Ribenboim, ’The<br />
new book <strong>of</strong> prime number records’<br />
[lion] How to catch a lion:<br />
lion<br />
• THE HILBERT METHOD. Place a locked cage in the desert. Set up the following axiomatic system. (i)<br />
The set <strong>of</strong> lions is non-empty<br />
(ii) If there is a lion in the desert, then there is a lion in the cage.<br />
Theorem. There is a lion in the cage<br />
• THE PEANO METHOD. There is a space-filling curve passing through every point <strong>of</strong> the desert. Such<br />
a curve may be traversed in as short a time as we please. Armed with a spear, traverse the curve faster<br />
than the lion can move his own length.<br />
• THE TOPOLOGICAL METHOD. The lion has a least the connectivity <strong>of</strong> a torus. Transport the desert<br />
into 4-space. It can now be deformed in such a way as to knot the lion. He is now helples.<br />
• THE SURGERGY METHOD. The lion is an orientable 3-manifold with boundary and so may be rendered<br />
contractible by surgery.<br />
• THE UNIVERSAL COVERING METHOD. Cover the lion by his simply-connected covering space. Since<br />
this has no holes, he is trapped.<br />
• THE GAME THEORY METHOD. The lion is a big game, hence certainly a game. There exists an<br />
optimal strategy. Follow it.<br />
• THE SCHROEDINGER METHOD. At any instant there is a non-zero probability that the lion is in the<br />
cage. Wait.<br />
• THE ERASTOSHENIAN METHOD. Enumerate all objects in the desert: examine them one by one;<br />
discard all those that are not lions. A refinement will capture only prime lions.<br />
• THE PROJECTIVE GEOMETRY METHOD. The desert is a plane. Project this to a line, then project<br />
the line to a point inside the cage. The lion goes to the same point.<br />
• THE INVERSION METHOD. Take a cylindrical cage. First case: the lion is in the cage: Trivial. Second<br />
case: the lion is outside the cage. Go inside the cage. Invert at the boundary <strong>of</strong> the cage. The lion is<br />
caught. Caution: Don’t stand in the middle <strong>of</strong> the cage during the inversion!
Euler<br />
[Euler] Euler’s formula: A connected plane graph with n vertices, e edges and f faces satisfies n - e + f = 2<br />
Pro<strong>of</strong>. Let T be the edge set <strong>of</strong> a spanning tree for G. It is a subset <strong>of</strong> the set E <strong>of</strong> edges. A spanning tree is<br />
a minimal subgraph that connects all the vertices <strong>of</strong> G. It contains so no cycle. The dual graph G* <strong>of</strong> G has<br />
a vertex in the interior <strong>of</strong> each face. Two vertices <strong>of</strong> G* are connected by an edge if the correponding faces<br />
have a common boundary edge. G* can have double edges even if the original graph was simple. Consider<br />
the collection T* <strong>of</strong> edges E* in G* that correspond to edges in the complement <strong>of</strong> T in E. The edges <strong>of</strong> T*<br />
connect all the faces because T does not have a cycle. Also T* does not contain a cycle, since otherwise, it<br />
would seperate some vertices <strong>of</strong> G contradicting that T was a spanning subgraph and edges <strong>of</strong> T and T* don’t<br />
intersect. Thus T* is a spanning tree for G*. Clearly e(T)+e(T*)=2. For every tree, the number <strong>of</strong> vertices is<br />
one larger than the number <strong>of</strong> vertices. Applied to the tree T, this yields n = e(T)+1, while for the tree T* it<br />
yields f=e(T*)+1. Adding both equations gives n+f=(e(T)+1)+(e(T*)+1)=e+2. – from M.Aigner, G. Ziegler<br />
”Pro<strong>of</strong>s from THE BOOK”<br />
irrational<br />
[irrational] Theorem: e = sum(k) 1/k! is irrational. Pro<strong>of</strong>. e=a/b with integers a,b would imply N = n! (e<br />
- sum(k¡n+1) 1/k!) is an integer for n¿b because n! e and n!/k! were both integers. However, 0 < N =<br />
�<br />
k>n n!/k! = 1/(n + 1) + 1/(n + 1)(n + 2) + ... < 1/(n + 1) + 1/(n + 1)2 + ... = 1/n (second sum is a geometric<br />
series) for every n is not possible.<br />
– from M.Aigner, G. Ziegler ”Pro<strong>of</strong>s from THE BOOK”<br />
Wiener<br />
[Wiener] After a few years at MIT, the Mathematician Norbert Wiener moved to a larger house. His wife,<br />
knowing his nature, figured that he would forget his new address and be unable to find his way home after<br />
work. So she wrote the address <strong>of</strong> the new home on a piece <strong>of</strong> paper that she made him put in his shirt pocket.<br />
At lunchtime that day, the pr<strong>of</strong>essor had an inspiring idea. He pulled the paper out <strong>of</strong> his pocket and used it<br />
to scribble down some calculations. Finding a flaw, he threw the paper away in disgust. At the end <strong>of</strong> the day<br />
he realized he had thrown away his address, he now had no idea where he lived. Putting his mind to work, he<br />
came up with a plan. He would go to his old house and await rescue. His wife would surely realize that he was<br />
lost and go to his old house to pick him up. Unfortunately, when he arrived at his old house, there was no sign<br />
<strong>of</strong> his wife, only a small girl standing in front <strong>of</strong> the house. ”Excuse me, little girl” he said ”but do you happen<br />
to know where the people who used to live here moved to?” ”It’s okay, Daddy,” said the little girl, ”Mommy<br />
sent me to get you”. Moral 1. Don’t be surprised if the pr<strong>of</strong>essor doesn’t know your name by the end <strong>of</strong> the<br />
semester. Moral 2. Be glad your parents aren’t mathematicians. if your parents are mathematicians, introduce<br />
yourself and get them to help you through the course. - From the introduction <strong>of</strong> ”How to ace calculus” by C.<br />
Adams, A. Thompson and J. Hass<br />
funeral<br />
[funeral] David Hilbert was one <strong>of</strong> the great European mathematicians at the turn <strong>of</strong> the century. One <strong>of</strong> his<br />
students purchased an early automobile and died in one <strong>of</strong> the first car accidents. Hilbert was asked to speak<br />
at the funeral. ”Young Klaus” he said, ”was one <strong>of</strong> my finest students. He had an unusual gift for doing<br />
mathematics. He was insterested in a great variety <strong>of</strong> problems, such as...” There was a short pause, follwed by<br />
”Consider the set <strong>of</strong> differentiable functions on the unit interval and take their closure in the ...” Moral 1. Sit<br />
near the door. Moral 2. Some mathematicians can be a little out <strong>of</strong> touch with reality. If your pr<strong>of</strong>essor falls<br />
in this category, look at the bright side. You will have lots <strong>of</strong> funny stories by the end <strong>of</strong> the semester. - From<br />
the introduction <strong>of</strong> ”How to ace calculus” by C. Adams, A. Thompson and J. Hass
abbit<br />
[rabbit] In a forest a fox bumps into a little rabbit, and says, ”Hi, junior, what are you up to?” ”I’m writing a<br />
dissertation on how rabbits eat foxes,” said the rabbit. ”Come now, friend rabbit, you know that’s impossible!”<br />
”Well, follow me and I’ll show you.” They both go into the rabbit’s dwelling and after a while the rabbit emerges<br />
with a satisfied expression on his face. Along comes a wolf. ”Hello, what are we doing these days?” ”I’m writing<br />
the second chapter <strong>of</strong> my thesis, on how rabbits devour wolves.” ”Are you crazy? Where is your academic<br />
honesty?” ”Come with me and I’ll show you.” ...... As before, the rabbit comes out with a satisfied look on<br />
his face and this time he has a diploma in his paw. The camera pans back and into the rabbit’s cave and, as<br />
everybody should have guessed by now, we see an enormous mean-looking lion sitting next to the bloody and<br />
furry remains <strong>of</strong> the wolf and the fox. The moral <strong>of</strong> this story is: It’s not the contents <strong>of</strong> your thesis that are<br />
important – it’s your PhD advisor that counts. - Unknown Usenet Source<br />
poet<br />
[poet] It is true that a mathematician who is not also something <strong>of</strong> a poet will never be a perfect mathematician.<br />
- K. Weierstrass, Quoted in D MacHale, Comic Sections (Dublin 1993)<br />
equilateral<br />
[equilateral] THEOREM: All triangles are equilateral. PROOF: 1) Given an arbitrary triangle ABC. Construct<br />
the middle orthogonal on AB in D and cut it with the line dividing the angle at C. Call the intersection E.<br />
Form the normal from E to AC in F and from E to BC in G. Draw the lines AE und BE. C * / / *F *G / E*<br />
/ — / — / —D A*———*————*B<br />
2. The angles ECF and ECG are gleich. The angles EFC and EGC are both right angles. Because the triangles<br />
ECF and ECG have also EC common, they must be congruent. Therefore CF=CG and EF=EG.<br />
3. The sides DA and DB are equal. The angle EDA and EDB are both right angles. Because the triangles EDA<br />
and EDB have also ED in common, they have to be congruent and EA=EB.<br />
4. The angle EGB and EFA are both right angle. Also, EF=EG and EA=EB. Therefore both triangles EGB<br />
and EFA are congruent. Therefore FA=GB.<br />
5. Since CF=CG and FA=GB, addition <strong>of</strong> the sides gives also CA=CB.<br />
6. Having proved that two arbitrary sides are equal, all are equal.<br />
widow<br />
[widow] I married a widow, who had an adult stepdaughter. My father, a widow and who <strong>of</strong>ten visited us, fell in<br />
love with my stepdaughter and married her. So, my father became my son-in-law and my stepdaughter became<br />
my stepmother. But my wife became the mother-in-law <strong>of</strong> her father-in-law. My stepmother, stepdaughter<br />
<strong>of</strong> my wife had a son and I therefore a brother, because he is the son <strong>of</strong> my father and my stepmother. But<br />
since he was in the same time the son <strong>of</strong> our stepdaughter, my wife became his grandmother and I became the<br />
grandfather <strong>of</strong> my stepbrother. My wife gave me also a son. My stepmother, the stepsister <strong>of</strong> my son, is in<br />
the same time his grandmother, because he is the son <strong>of</strong> her stepson and my father is the brother-in-law <strong>of</strong> my<br />
child, because his sister is his wife. My wife, who is the mother <strong>of</strong> my stepmother, is therefore my grandmother.<br />
My son, who is the child <strong>of</strong> my grandmother, is the grandchild <strong>of</strong> my father. But I’m the husband <strong>of</strong> my wife<br />
and in the same time the grandson <strong>of</strong> my wife. This means: I’m my own grandfather.<br />
dots<br />
[dots] I never could make out what those damned dots meant. – Lord Randolph Churchill (1849-1895) Brittish<br />
conservative politician, referring to decimal points.
ladder<br />
[ladder] The mathematician has reached the highest rung on the ladder <strong>of</strong> human thought. – Havelock Ellis<br />
ignorant<br />
[ignorant] Let no one ignorant <strong>of</strong> mathematics enter here. – Plato, Inscription written over the entrance to the<br />
academy<br />
god<br />
[god] I knew a mathematician, who said ’I do not know as much as God. But I know as much as God knew at<br />
my age’. – Milton Shulman, Candian writer<br />
english<br />
[english] English pr<strong>of</strong>essor: In English, a double negative makes a positive. In other languages such as Russian,<br />
a double negative is still a negative. There are, however, no languages in which a double positive makes a<br />
negative. Student in back <strong>of</strong> class: ”Yea, right”<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 124 entries in this file.
Index<br />
1+1, 8<br />
1=2, 16<br />
abstract, 13<br />
aleph, 8<br />
ambitious, 16<br />
analysis, 1<br />
analytic, 2<br />
arithmetic, 12<br />
astronomer, 7<br />
axiomatics, 2<br />
Bacon, 16<br />
barber, 5<br />
beauty, 3, 16<br />
blackboard, 17<br />
cancel, 9<br />
Cantor, 5<br />
cat, 8<br />
Chebyshev, 10<br />
chocolate, 8<br />
clearly, 18<br />
c<strong>of</strong>fee, 8, 9<br />
computer, 1<br />
Conway, 3<br />
cube, 12<br />
dean, 7<br />
decimal, 14<br />
deductions, 16<br />
dice, 12<br />
digits, 10<br />
dots, 21<br />
doughnut, 13<br />
e, 9<br />
engeneer, 9<br />
english, 22<br />
enhusiast, 1<br />
ephermeral, 17<br />
equilateral, 21<br />
Erdoes, 10<br />
Euler, 20<br />
experience, 13<br />
fantasy, 1<br />
FBI, 15<br />
flesh, 14<br />
fourteen, 16<br />
freedom, 1<br />
funeral, 20<br />
geometry, 3<br />
god, 13, 22<br />
Hadamard, 5<br />
hairy-ball, 2<br />
Hilbert, 11<br />
historians, 15<br />
H<strong>of</strong>stadter, 13<br />
23<br />
horse, 7<br />
hypothesis, 12<br />
ignorant, 22<br />
illiteracy, 4<br />
induction, 7<br />
infimum, 4<br />
intelligence, 14<br />
irrational, 20<br />
joke, 17<br />
jouissance, 5<br />
Kovalevsky, 13<br />
ladder, 22<br />
large, 2<br />
Leibniz, 18<br />
lion, 19<br />
logs, 8<br />
mad, 6<br />
magacian, 1<br />
Mandelbrot, 5<br />
medicine, 13<br />
melancholy, 10<br />
Mersenne, 18<br />
Monty-Hall, 6<br />
Moser, 6<br />
obvious, 4, 14<br />
Outrage, 10<br />
painting, 9<br />
philosophers, 14<br />
physics, 13<br />
pi, 9, 15<br />
Piaget, 18<br />
poet, 10, 21<br />
prime, 4<br />
primes, 17<br />
qed, 8<br />
Queen, 17<br />
rabbit, 21<br />
reality, 12<br />
recommendation, 12<br />
refreree, 11<br />
royal, 1<br />
sex, 6<br />
sheet, 11<br />
sin, 5<br />
solution, 1<br />
solve, 11<br />
stupider, 9<br />
subtraction, 17<br />
tool, 11<br />
transcendental, 4<br />
turbulence, 2
twin, 19<br />
undogmatic, 11<br />
violence, 3<br />
war, 18<br />
weapons, 11<br />
whispers, 14<br />
widow, 21<br />
Wiener, 20<br />
Wilson, 19<br />
wine, 6<br />
wissen, 12<br />
Zermelo, 3
<strong>ENTRY</strong> COMPUTABILITY<br />
[<strong>ENTRY</strong> COMPUTABILITY] Authors: Oliver Knill: nothing real yet Literature: not yet, some lectures <strong>of</strong><br />
E.Engeler on computation theory<br />
Church’s theses<br />
The generally accepted [Church’s theses] tells that everything which is computable can be computed using a<br />
Turing machine. In that case, the problem to determine, whether a Turing machine will halt, is not computable.<br />
cipher<br />
A [cipher] is a secret mode <strong>of</strong> writing, <strong>of</strong>ten the result <strong>of</strong> subsituting numbers <strong>of</strong> letters and then carrying out<br />
arithmetic operations on the numbers.<br />
Coding theory<br />
[Coding theory] is the theory <strong>of</strong> encryption <strong>of</strong> messages employed for security during the transmission <strong>of</strong> data<br />
or the recovery <strong>of</strong> information from corrupted data.<br />
Cooks hypothesis<br />
[Cooks hypothesis] P = NP . A pro<strong>of</strong> or dispro<strong>of</strong> is one <strong>of</strong> the millenium problems.<br />
Graph isomorphism problem<br />
[Graph isomorphism problem] It is not known whether graph isomorphism can be decided in deterministic<br />
polynomial time. It is an open problem in computational complexity theory.<br />
Inductive structure<br />
[Inductive structure] A set U with a subset A and operations g1, ..., gn define an inductive structure<br />
(U, A, g1, ..., gn) If all elements <strong>of</strong> U can be generated by repeated applications <strong>of</strong> the operations gi on elements<br />
<strong>of</strong> A. Examples:<br />
• (N, A = {0, 1}, g1(a, b) = a + b, g2(a, b) = a ∗ b defines an inductive structure.<br />
• If U = N is the set <strong>of</strong> natural numbers, A = {1, 2, 3} g1(x, y) = 3x − 4, g2(x, y, z) = 7x + 5y − z, then<br />
(U, A, g1, g2) define an inductive structure.
syntactic structure<br />
An inductive structure (U, A, g1, ..., gn) is called a [syntactic structure] if it is uniquely readable that is if<br />
g1(u1, ..., uk) = g2(v1, ..., vl), then g1 = g2, k = l and u1 = v1, ..., uk = vk. Example: if X is the set <strong>of</strong> finite<br />
words in the alphabet {p, q, r, K, N} and A = {p, q, r}. Define g1(x, y) = Kxy and g2(x, y) = Nx and U the<br />
set <strong>of</strong> words generated from A. The structure is the language <strong>of</strong> elementary logic in polnic notation. It is a<br />
syntactic structure. Syntactic structures are in general described by grammers.<br />
grammar<br />
A [grammar] (N, T, G) is given by two sets <strong>of</strong> symbols N, T and a finite set G <strong>of</strong> pairs (ni, ti) which define<br />
transitions ni → ti. For example: N = {S}, T = {K, N, p, q, r}, G = {S → p, S → q, S → r, S → KSS, S →<br />
NS}. Acoording to Chomsky, one classifies grammers with additional conditions like context sensitivity or<br />
regularity.<br />
context sensitive<br />
A grammer (N, T, G) is called [context sensitive] if (n, t) ∈ G then |t| ≥ |n|.<br />
context sensitive<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 10 entries in this file.
Index<br />
Church’s theses, 1<br />
cipher, 1<br />
Coding theory, 1<br />
context sensitive, 2<br />
Cooks hypothesis, 1<br />
grammar, 2<br />
Graph isomorphism problem, 1<br />
Inductive structure, 1<br />
syntactic structure, 2<br />
3
<strong>ENTRY</strong> COMPUTER<br />
[<strong>ENTRY</strong> COMPUTER] Authors: Oliver Knill: May 2001 Literature: for video stuff: http://www.doom9.org,<br />
foldoc<br />
AAC<br />
[AAC] Advanced Audio Coding will be the successor <strong>of</strong> AC3 audio. It is based on AC3 while adding a number<br />
<strong>of</strong> improvements in various areas. Currently player and hardware support for this upcoming audio format is<br />
still very limited.<br />
acrobat<br />
[acrobat] A product from Adobe for manipulating documents stored in the PDF (Portable Document Format).<br />
[amd] Daemon which enables the NFS automount.<br />
[AMD] Advanced Micro Devices, Chip company.<br />
amd<br />
AMD<br />
arpwatch<br />
[arpwatch] Daemon to log and buil a database <strong>of</strong> Ethernet address/IP address pairings it sees on a LAN interface.<br />
ASCII<br />
[ASCII] American Standard Code for Information Interexchange, an industry standard, which assigns letters,<br />
numbers and other characters within the 256 slots available in the 8-bit code.<br />
AC3<br />
[AC3] Initially known as Audio Coding 3 AC3 is a synonym for Dolby Digital these days. Dolby Digital is an<br />
advanced audio compression technology allowing to encode up to 6 separate channels at bitrates up to 448kbit/s.<br />
For more information please check out the Dolby website.
ASF<br />
[ASF] Advanced Streaming Format. Micros<strong>of</strong>t’s answer to Real Media and streaming media in general.<br />
[AT] keyboard The standard keyboard used with the IBM compatible computer.<br />
AT<br />
backdoor<br />
A [backdoor] is a ”mechanism surreptitiously introduced into a computer system to facilitate unauthorized<br />
access to the system”. An example <strong>of</strong> a backdoor is ”bindshell”.<br />
AVI<br />
[AVI] Audio Video Interleave. The video format most commonly used on Windows PC’s. It defines how video<br />
and audio are attached to each other, without specifying a codec.<br />
Bandwidth<br />
[Bandwidth] Bandwidth measures how much information can be carried in a given time period over a<br />
wired or wireless communications link. A typical broadband speed is 1270 Kbps (kilo bit per sec-<br />
Technology Speed mbit/s<br />
56k modem 0.056<br />
DSL varies<br />
cable varies<br />
T1 1.544<br />
Ethernet 10.000<br />
ond) which is 155.6 KBytes/sec T3 44.736 see http://home.cfl.rr.com/cm3/speedtest7.htm<br />
OC-3 155.520<br />
OC-12 622.080<br />
OC-48 2,488.320<br />
OC-96 4,976.640<br />
OC-192 9,953.280<br />
OC-255 13,219.200<br />
http://jetstreamgames.co.nz/speed/ADSLdownload1MB.html http://home.cfl.rr.com/eaa/Bandwidth.htm<br />
BUP file<br />
[BUP file] A bup file is a Back UP file <strong>of</strong> an IFO file. These files are commonly found on DVDs.<br />
Byte<br />
One [Byte] is an information unit <strong>of</strong> a sequence <strong>of</strong> 8 bits.
[CASE]: Computer Aided S<strong>of</strong>tware Engineering.<br />
CASE<br />
Cell (ID)<br />
[Cell (ID)] A cell is the smallest video unit on a DVD. Normally used to contain a chapter it can also be used<br />
to contain a smaller unit in case <strong>of</strong> multiangles or seamless branching titles.<br />
certificate<br />
A [certificate] is a digital identifcation <strong>of</strong> a physical or abstract object, a person, business, computer, program<br />
or document. A digital certificate is much like a passport. It is issued by a certificate authority, which vouches<br />
for its authenticity.<br />
Codec<br />
[Codec] COder/DECoder. A codec is a piece <strong>of</strong> s<strong>of</strong>tware that allows to encode something - usually audio or<br />
video - to a specific format and can decode media encoded in this specific format again. Popular Codecs are<br />
MPEG1, MPEG2, MPEG-4 (=divx=xvid), realvideo, wmv, dv Indeo, etc. MPEG, AVI, ASF, Quicktime is<br />
not a codec but a container format - that can be encoded using different codecs. In avi container files, there’s<br />
mostly mpeg4 video content and mp3 audio content but this is not obligatory. For DVD, the video should be<br />
in mpg2, the audio in mp2 and both <strong>of</strong> these will be in a mpeg-ps (program stream aka ”vob”) container.<br />
Container<br />
[Container] A container is, like the name says, a construct to contain data - in this case video and audio date<br />
and possibly subtitles and navigational information. For instance, you would like to put a soundless video<br />
stream and the audio track together in one file. To do that you need a container format. Examples <strong>of</strong> container<br />
formats are: AVI, ASF, OGM, Quicktime, VOB and MPG. In avi container files, there’s mostly mpeg4 video<br />
content and mp3 audio content but this is not obligatory. For DVD, the video should be in mpg2, the audio<br />
in mp2 and both <strong>of</strong> these will be in a mpeg-ps (program stream aka ”vob”) container. A [cookie] is a block <strong>of</strong><br />
information recorded and stored within the client’s browser.<br />
CSS<br />
[CSS] Cascading Style Sheets is a simple mechanism for adding style (e.g. fonts, colors, spacing) to Web<br />
documents. For example:<br />
body, table font-family: verdana, arial, geneva, sans-serif;
CSS<br />
[CSS] Content Scrambling System. Prioprietary scrambling system for video DVDs. Designed to stop people<br />
from making copies <strong>of</strong> DVDs, most commercial DVDs are encrypted using CSS. During playback, DVDs are<br />
then decrypted on the fly. Only parts <strong>of</strong> the DVD are encrypted (for instance all IFO and BUP files are not<br />
encrypted, and VIDEOTS.VOB <strong>of</strong>ten isn’t encrypted either) and the encryption scheme is rather weak and was<br />
quickly defeated. If you want to know what CSS does, insert a DVD video disc into your PC, start playing the<br />
disc using a s<strong>of</strong>tware DVD player, then close the player. Now copy a 0.99GB VOB file from the disc to your<br />
harddisk and try to play back that VOB file in your s<strong>of</strong>tware DVD player. You’ll see a lot <strong>of</strong> funny colored<br />
blocks all over the picture making the movie unwatchable. But you’ll also see parts <strong>of</strong> the movie (the parts that<br />
are not encrypted).<br />
DAR<br />
[DAR] Display Aspect Ratio. Indicates the dimension <strong>of</strong> a screen. Most PC screens have a DAR <strong>of</strong> 4:3, meaning<br />
that the horizontal size is 4/3 as large as the vertical size. For TVs we have a lot <strong>of</strong> old 4:3 displays and more<br />
and more 16:9 displays. As you can guess from the numbers 16:9 displays are broader than 4:3 displays having<br />
the same diagonal size. 16:9 screens are more suited to display Hollywood movies which are usually shot with<br />
an aspect ratio <strong>of</strong> 1:2.35 or 1:1.85 (meaning that the horizontal size <strong>of</strong> the picture is 1.85 times as wide as the<br />
vertical size).<br />
Deinterlace<br />
[Deinterlace] The process <strong>of</strong> restoring a progressive video stream out <strong>of</strong> an interlaced one is called deinterlacing.<br />
Demultiplexing<br />
[Demultiplexing] The opposite <strong>of</strong> multiplexing. In this process a combined audio/video stream will be separated<br />
into the number <strong>of</strong> streams it consists <strong>of</strong> (a video stream, at least one audio stream and a navigational stream).<br />
Every VOB encoder demultiplexes the VOB files before encoding (FlaskMpeg, mpeg2avi, dvd2mpg, ReMpeg2)<br />
and every DVD player does the same (audio and video are being treated by different circuits, or decoded by<br />
different filters on a PC).<br />
Descrambling<br />
[Descrambling] DVDs are usually CSS scrambled - imagine you decide to give a number to each letter, starting<br />
with 1 for a, etc. A sentence would become a couple <strong>of</strong> digits - that’s what we call scrambled. Of course CSS is<br />
much better than that but it’s still quite easy to crack. Descrambling means reversing the scrambling process,<br />
rendering our digits to a sentence again, or making our movie playable again - you can try to copy a movie to<br />
your hard disk when you’ve authenticated your DVD drive and play it, you’ll get a garbled picture because it’s<br />
still scrambled. Common CSS descramblers either use a pool <strong>of</strong> known descrambling keys (DeCSS or DODSrip<br />
- they contain a large number <strong>of</strong> keys but not all <strong>of</strong> them) or try to derive the key by a cryptographic attack<br />
(VobDec - that’s why it works on most disc since it’s not dependent on a pool <strong>of</strong> discs).
Digital Video<br />
[Digital Video] Digital video is usually compressed. Since standard loss less compression is insufficient for video,<br />
the video codecs have to get rid <strong>of</strong> unimportant information - stuff the human eye won’t see or is unlikely to<br />
see. Since that is still not enough modern compression algorithms use keyframes, I and P frames in order to<br />
save space.<br />
DivX<br />
[DivX] There are 2 flavors <strong>of</strong> DivX today: DivX is the name <strong>of</strong> the hacked Micros<strong>of</strong>t MPEG4 codecs (Windows<br />
Media Video V3). Those codecs were developed by Micros<strong>of</strong>t for use in its proprietary Windows Media architecture<br />
and initially supported encoding AVIs and ASFs but all non-beta versions included an AVI lock, making it<br />
impossible to use them to encode to the AVI format - and only a few tools support ASF today. What the makers<br />
<strong>of</strong> DivX did is remove that AVI lock making it possible to encode to AVI again, and changed the name to DivX<br />
video in order to prevent confusion <strong>of</strong> codecs, since it’s possible to have both the unhacked and hacked codecs<br />
on the same computer if you use the Windows Media Encoder. The latest releases <strong>of</strong> DivX also include a hacked<br />
Windows Media Audio Codec called DivX audio - the hack <strong>of</strong> that codec is not perfect yet and its use is limited<br />
for higher bitrates. This codec is also known as DivX3. The other DivX is a brand-new MPEG-4 video codec<br />
developed by DivXNetworks. It <strong>of</strong>fers much advanced encoding controls and 2 pass encoding. Furthermore the<br />
codec can play the old DivX3 movies. The codec is commonly called DivX4.<br />
DHCPD<br />
[DHCPD] Daemon to service which can dynamically assign IP addresses to its client hosts.<br />
DOM<br />
[DOM] The Document Object Model is a platform- and language-neutral interface that will allow programs and<br />
scripts to dynamically access and update the content, structure and style <strong>of</strong> documents.<br />
DOS<br />
[DOS] is a Disk operating system, based on a command line user interface. MS-DOS 1.0 was released in 1981<br />
for IBM computers. While MS-DOS is not much used by itself today, it still can be accessed from Windows 95,<br />
Windows 98 or Windows ME by clicking Start/Run and typing command or CMD in Windows NT, 2000 or<br />
XP.<br />
DRC<br />
[DRC] Dynamic Range Compression. AC3 Tracks contain a much larger dynamic range that most audio<br />
equipment can handle, therefore most standalone and s<strong>of</strong>tware DVD player will compress the dynamic range<br />
somewhat, according to the actual dynamic range. In layman terms the volume will be augmented dynamically,<br />
e.g. explosions won’t become louder or only a bit louder, whereas in normal dialogues the volume will be<br />
augmented quite a bit. Since your player will do the same this is the way to go to have augmented volume.
[DTML] document template markup language.<br />
[DTP] Desktop publishing.<br />
DTML<br />
DTP<br />
Dynamic HTML<br />
[Dynamic HTML] is a term used by some vendors to describe the combination <strong>of</strong> HTML, style sheets and scripts<br />
that allows documents to be animated.<br />
Elementary Stream (ES)<br />
[Elementary Stream (ES)] An elementary stream is a single (video or audio) stream without container. For<br />
instance a basic MPEG-2 video stream (.m2v or .mpv) is an MPEG-2 ES, and on the audio side we have AC3,<br />
MP2, etc files that are ES. Most DVD authoring program require ES as input.<br />
[EULA] End user licence agreement.<br />
EULA<br />
FAT<br />
[FAT] File allocation table. Filesystem used by Windows. Example: Windows 95 users rely on the FAT 16, In<br />
1996 Micros<strong>of</strong>t introduced the FAT 32 file system, which is still very widely used today besides NTFS on the<br />
windows platform.<br />
FUD<br />
[FUD] stands for Fear, Uncertainty, Doubt. It is a marketing technique used when a competitor launches a<br />
product that is both better than yours and costs less, i.e. your product is no longer competitive. Unable<br />
to respond with hard facts, scare-mongering is used via ’gossip channels’ to cast a shadow <strong>of</strong> doubt over the<br />
competitors <strong>of</strong>ferings and make people think twice before using it.<br />
GUI<br />
[GUI] - Graphical User Interface; A desktop-like interface usually containing icons, menus and windows. Invented<br />
by Xerox, later ”borrowed” by Micros<strong>of</strong>t and Apple.
HTML<br />
[HTML] Hypertext markup language. Will be replaced by XHTML, and XHTML 2.0 in particular.<br />
[HTTP] Hypertext Transfer Protocol.<br />
[HTTPD] Daemon to Apache webserver.<br />
HTTP<br />
HTTPD<br />
Hypertext<br />
[Hypertext] - shortcuts or links between different parts <strong>of</strong> a document, article, website or world wide web.<br />
While early hypertext formats were already Apples Hypercard, it is now common in HTML (Hypertext markup<br />
language).<br />
inetd<br />
[inetd] Daemon which is at the heart <strong>of</strong> providing network services like telnet or ftp.<br />
IFO file<br />
[IFO file] InFOrmation file commonly found on DVDs. Such files contain navigational information for DVD<br />
players.<br />
Interlaced<br />
[Interlaced] Interlaced is a video storage mode. An interlaced video stream doesn’t contain frames but fields<br />
with each field containing either even or odd lines <strong>of</strong> one frame.<br />
IP<br />
[IP] Internet Protocol. Standard which defines the structure <strong>of</strong> a message sent between two computers over the<br />
network.<br />
[IPFW] IP firewall.<br />
IPFW
ICMP<br />
[ICMP] Internet Control Message Protocol. ICMP messages contain information about communication between<br />
two computers.<br />
Java<br />
[Java] is a true compiler-based, low level programming language. [Javascript] is a scripting programming<br />
language. It was developed by Netscape and used to create interactive Web sites. JavaScript is a popular<br />
client-side scripting language because it is supported by virtually all browsers.<br />
KISS<br />
[KISS] - Keep It Simple Stupid. Rule <strong>of</strong> thumb for s<strong>of</strong>tware designers. Keep design small to minimize confusion.<br />
LDAP<br />
[LDAP] Lightweight Directory Access Protocol. A network directory which can substitute DNS and much more.<br />
Not to be confused with a database. A directory is mostly looked up and not written <strong>of</strong>ten into.<br />
LDIF<br />
[LDIF] LDAP interchange Format is a standard text file for storing LDAP configuration information and<br />
directory contents.<br />
MathML<br />
[MathML] is a low-level specification for describing mathematics as a basis for machine to machine communication.<br />
It provides a foundation for the inclusion <strong>of</strong> mathematical expressions in Web pages.<br />
miniDVD<br />
[miniDVD] Basically a DVD on a CD. A miniDVD can contain bitrates up to 10mbit/s (audio and video<br />
combined). Video is MPEG2, preferably VBR and audio can be MPEG1 audio layer 2, raw uncompressed PCM<br />
or AC3. Video quality can be up to an actual DVD level if a limited playtime is accpted.<br />
MPEG<br />
[MPEG] MPEG means Motion Picture Expert Group and it’s the resource for video formats in general. This<br />
group defines standards in digital video, among it the MPEG1 standard (used in Video CDs), the MPEG2<br />
standard (used on DVDs and SVCDs), the MPEG4 standard and several audio standards - among them MP3<br />
and AAC. Files containing MPEG-1 or MPEG-2 video <strong>of</strong>ten use either the .mpg or .mpeg extension.
MPEG4<br />
[MPEG4] Is pretty much a collection <strong>of</strong> standards defined by the MPEG Group, and it should become the next<br />
standard in digital video. MPEG4 allows the use <strong>of</strong> different encoding methods, for instance a keyframe can be<br />
encoded using ICT or Wavelets resulting in different output qualities.<br />
MPG<br />
[MPG] MPG can be either an abbreviation for MPEG or is used as a file extension for MPEG-1 and MPEG-2<br />
video data. It is a container to contain MPEG-1/2 video stream and MPEG1 layer 2 audio (aka mp2 files).<br />
MPG containers are also refered to as program streams (PS).<br />
MM4<br />
[MM4] Multiple MPEG 4: A combination <strong>of</strong> different bitrate encoded files. For instance you could take a<br />
2000kbit/s encode, a 910kbit/s encode and combine the files together, use the lower bitrate file and replace<br />
scenes where the quality gets too bad due to a lot <strong>of</strong> action with the parts taken from the 2000kbit/s one.<br />
NAT<br />
[NAT] Network Address translation. A typical home user with broadband access and router performs Network<br />
Address Translation, or NAT allowing multiple computers to share a single fast Internet connection.<br />
.Net<br />
[.Net] A collection<strong>of</strong> technologies pushed by Micros<strong>of</strong>t. It contains C# programming language (an alternative<br />
to Java). Part <strong>of</strong> the .Net initiative. It builds on standards like XML and SOAP.<br />
Network layers<br />
[Network layers] Application layer: Client and server programs. Transport layer: TCP and UDP protocols,<br />
service ports Network layer: IP packets, IP addresses, ICMP messsages Data link layer: Ethernet frames and<br />
MAC addresses Physical layer: Copper wire, fiberoptic cable, radio<br />
Newbie<br />
[Newbie] - (Also n00b and newb) a newcomer to a certain computer topic or program asking help from experienced<br />
user.<br />
[NFS] Network file system.<br />
NFS
OGM<br />
[OGM] OGM stands for OGg Media which is the name <strong>of</strong> the Ogg container implementation by Tobias Waldvogel.<br />
OGM can be used as an alternative to the AVI container and it can contain Ogg Vorbis, MP3 and AC3<br />
audio, all kinds <strong>of</strong> video formats, chapter information and subtitles.<br />
Perl<br />
[Perl] Perl is a high-level programming language. It derives from the C programming language and to a lesser<br />
extent from sed, awk, the Unix shell, and at least a dozen other tools and languages. Perl’s process, file,<br />
and text manipulation facilities make it particularly well-suited for tasks involving quick prototyping, system<br />
utilities, s<strong>of</strong>tware tools, system management tasks, database access, graphical programming, networking, and<br />
world wide web programming. These strengths make it especially popular with system administrators and CGI<br />
script authors, but mathematicians, geneticists, journalists, and even managers also use Perl.<br />
PHP<br />
[PHP] PHP is a widely-used general-purpose scripting language that is especially suited for Web development<br />
and can be embedded into HTML.<br />
Pocket PC<br />
[Pocket PC] Operating system for handhelds. Usually running Micros<strong>of</strong>t CE or the Palm OS.<br />
PNG<br />
[PNG] is graphics file format for the lossless, portable, well-compressed storage <strong>of</strong> raster images. Indexed-color,<br />
grayscale, and truecolor images are supported, plus an optional alpha channel for transparency. Sample depths<br />
range from 1 to 16 bits per component (up to 48bit images for RGB, or 64bit for RGBA).<br />
Python<br />
[Python] is an interpreted, high-level, object-oriented programming language.<br />
QNX<br />
[QNX] is a realtime, microkernel, preemptive, prioritized, message passing, network distributed, multitasking,<br />
multiuser, fault tolerant operating system.
Qt<br />
[Qt] (”kjut”) Multi platform toolkit and graphics library. Developed by Trolltech. Runs on Windows systems<br />
including XP, all unix derivates with X windows as well as Mac OS X.<br />
PCMCIA<br />
[PCMCIA] Personal Computer Memory Card International Association.<br />
[RDBM] relational data base manager.<br />
RDBM<br />
rff/tff<br />
[rff/tff] RFF means repeat first frame, it’s a technique used to make the necessary 29.97 frames per second<br />
out <strong>of</strong> a 24 frames per second source - the movie like it was recorded with a traditional movie camera used by<br />
Hollywood. The rff flag tells the player to repeat one field <strong>of</strong> the video stream. Tff means top field first and is<br />
also used to perform a telecine to make a 24fps movie into 29.97fps.<br />
Real time operating systems<br />
[Real time operating systems] Operating systems which are used in handhelds, robots, telphone switches. Examples:<br />
QNX, VxWorks (as used in Mars rovers), Windows CE (as used in handhelds), Nucleus RTX. Realtime<br />
systems must function reliably in event <strong>of</strong> failures. It is said that the three most important things in Realtime<br />
system design are timing, timing and timing.<br />
Ripping<br />
[Ripping] Ripping means copying a DVD movie to the hard disk <strong>of</strong> the computer. This includes the authentication<br />
process for the DVD Drive and the actual CSS Descrambling. CSS (Content Scrambling System) is a copy<br />
protection scheme designed to prevent unauthorized copying <strong>of</strong> DVD movies, although many argue that it was<br />
also designed to control where DVD movies can be played since without a CSS license you essentially have to<br />
crack the encryption to play a DVD movie. The term ”ripping” is also <strong>of</strong>ten used to describe the whole process<br />
<strong>of</strong> descrambling a DVD, then convert the audio and video into another format.<br />
RSS<br />
[RSS] is a method <strong>of</strong> distributing links to content in a web site so that others can use use it. It’s a mechanism<br />
to ”syndicate” the content. The original RSS, version 0.90, was designed by Netscape as a format for building<br />
portals <strong>of</strong> headlines to mainstream news sites. RSS is an acronym for Really Simple Syndication.
RTFM<br />
[RTFM] - Read the fucking manual. Common answer to basic and <strong>of</strong>ten repeated questions, that could be<br />
avoided in the first place just by looking at the manual.<br />
RSS<br />
Really Simple Syndication [RSS] is an XML-based format for content distribution. For example, News.com<br />
<strong>of</strong>fers several RSS feeds with headlines, descriptions and links back to News.com for the full story. [ROUTER]<br />
a machine designed to direct packets from their source host to their destination.<br />
RDBMS<br />
[RDBMS] A Relational Database Management System. Stores data related tables. A single database can be<br />
spread across several tables unlike flat-file databases where each database is self-contained in a single table.<br />
SBC<br />
[SBC] Smart Bitrate Control. A new kind <strong>of</strong> DivX encoder called Nandub can modify many internal codec<br />
parameters on the fly during compression, giving you better quality and a lot more control over the encoding<br />
session. More information can be found in the SBC guide in the DivX guides section.<br />
SGML<br />
[SGML] The standard Generalized Markup Language (SGML) is a meta Markup Languages like XML. They are<br />
used for defining markup languages. A markup language defines using SGML or XML has a specific vocabulary.<br />
SMIL<br />
[SMIL] Synchronized Multimedia Integration Language. It enables simple authoring <strong>of</strong> interactive audiovisual<br />
presentations. SMIL is typically used for ”rich media”/multimedia presentations which integrate streaming<br />
audio and video with images, text or any other media type. SMIL is an easy-to-learn HTML-like language, and<br />
many SMIL presentations are written using a simple text-editor.<br />
[SOAP] Simple object access protocol.<br />
[SQL] structured query language.<br />
SOAP<br />
SQL
Sun ONE<br />
[Sun ONE] Sun Open net initiative. Answer to .Net initiative <strong>of</strong> Micros<strong>of</strong>t. Has Java, XML and SOAP as<br />
foundation.<br />
SVG<br />
[SVG] The Scalable Vector Graphics is a language for describing two-dimensional graphics in XML. SVG<br />
allows for three types <strong>of</strong> graphic objects: vector graphic shapes, images and text. Graphical objects can be<br />
grouped, styled, transformed and composited into previously rendered objects. The feature set includes nested<br />
transformations, clipping paths, alpha masks, filter effects and template objects.<br />
TCP<br />
[TCP] Transmission control protocol. An IP message type. Most network services run over TCP. A typical<br />
TCP connection is visiting a remote web site.<br />
TCPA<br />
[TCPA] (Trusted Computing Platform Architecture) belongs to DRM (Digital rights management). TCPA<br />
aims at integrity <strong>of</strong> kernel and system components - to assure you that your system can be trusted. Palladium,<br />
on the other hand, uses similar technology to make sure that the user does not do anything else than what is<br />
allowed by content owners.<br />
TLD<br />
[TLD] Top level domain. The last entry in a webaddress. The TLD <strong>of</strong> www.w3c.org is ”org”. In the 1980s,<br />
seven TLDs (.com, .edu, .gov, .int, .mil, .net, and .org) were created. Later four <strong>of</strong> the new TLDs (.biz, .info,<br />
.name, and .pro) as well as sponsered TLD’s .aero, .coop, and .museum) were created. TLDs with two letters<br />
(such as .de, .mx, and .jp) have been established for over 240 countries and external territories and are referred<br />
to as ”country-code” TLD.<br />
UDP<br />
[UDP] User Datagramm Protocol. Sendes transport-level data between two network-based programs. For<br />
example, internet-time servers are assigned UDP services.<br />
UML<br />
[UML] Unified modelling language is a language for specifying, visualizing, constructing, and documenting<br />
s<strong>of</strong>tware systems, as well as for business modeling and modeling <strong>of</strong> other non-s<strong>of</strong>tware systems.
VCD<br />
[VCD] Video CD, works on many DVD players, there are s<strong>of</strong>tware players on almost every operating systems,<br />
doesn’t need a fast computer but the image is VHS-like. Video is MPEG1 at 1150kbit/s and audio MPEG1<br />
audio layer 2 at 224kbit/s.<br />
[VLDB] Very large data base.<br />
[VML] Vector Markup Language<br />
VLDB<br />
VML<br />
W3C<br />
[W3C] The World Wide Web Consortium (W3C) develops interoperable technologies (specifications, guidelines,<br />
s<strong>of</strong>tware, and tools) to lead the Web to its full potential. W3C is a forum for information, commerce,<br />
communication, and collective understanding.<br />
Wavelets<br />
[Wavelets] Wavelets are an alternative basis space. There are infinitely many wavelet bases (Daubechies, Haar,<br />
Mexican Hat, ”Spline”, Zebra, etc), but their primary feature is that they are localized. Fourier basis functions<br />
span all space (from negative to positive infinity). Wavelets are basically individual pulses <strong>of</strong> waves (at various<br />
positions and scales). Their value in compression stems from factors like the grouping which generally shows<br />
that a good 90filters, with the high-pass filters generally showing very small values that are mostly details. (<strong>of</strong><br />
course, this is not true if the source is noisy in the first place). For images, the greatest value comes from<br />
localization <strong>of</strong> the basis, which means that we can model discontinuities (e.g. edges) VERY well with wavelets.<br />
You will NOT get those weird JPEG halos if you use wavelets.<br />
WebDAV<br />
[WebDAV] Web-based Distributed Authoring and Versioning. A set <strong>of</strong> extensions to the HTTP protocol which<br />
allows users to collaboratively edit and managa files on remote web servers.<br />
Widget<br />
[Widget]- objects that make up interfaces, i.e. mouse, menus, textbox, buttons; basic tools and objects.
Windows Media<br />
[Windows Media] Micros<strong>of</strong>t’s proprietary architecture for audio and video on the PC. It’s based on a collection<br />
<strong>of</strong> codecs which can be used by the WindowsMedia Player to play files encoded in any supported format.<br />
WindowsMedia 7.0 <strong>of</strong>fers a new set <strong>of</strong> codecs, among them a fully ISO compliant MPEG4 codec (called MS<br />
Windows Video V1), an improved MPEG-4 codec called MS Video V7 (although I did not notice any improvement<br />
compared with MS Windows Video V3 on which DivX is based), an encoder that supports Deinterlacing<br />
and Inverse Telecine.<br />
Win FS<br />
[Win FS] Windows Future Storage file system, planned in Windows Longhorn, the successor <strong>of</strong> Windows XP.<br />
WYSIWYG<br />
[WYSIWYG]- What You See Is What You Get. Usually to distinguish document authoring tools. Writing<br />
a Latex file as a text document is not WYSIWYG, while authoring a word document is. Writing a HTML<br />
document with a text editor is not WYSIWYG, while writing it with an authoring tool is.<br />
WORM<br />
[WORM] a program that connects to other machines and replicates itself. Worms have the potential to both<br />
damage infected machines and to interfere with networks and services due to congestion caused by the spread<br />
<strong>of</strong> the worm.<br />
WORM<br />
XHTML 2 is a general purpose markup language designed for representing documents for a wide range <strong>of</strong><br />
purposes across the World Wide Web. To this end it does not attempt to be all things to all people, supplying<br />
every possible markup idiom, but to supply a generally useful set <strong>of</strong> elements. Here is an element <strong>of</strong> a XHTML 2.0<br />
document: ¡?xml version=”1.0” encoding=”UTF-8”?¿ ¡!DOCTYPE html PUBLIC ”-//W3C//DTD XHTML<br />
2.0//EN” ”TBD”¿ ¡html xmlns=”http://www.w3.org/2002/06/xhtml2” xml:lang=”en”¿ ¡head¿ ¡title¿Virtual<br />
Library¡/title¿ ¡/head¿ ¡body¿ ¡p¿Moved to ¡a href=”http://vlib.org/”¿vlib.org¡/a¿.¡/p¿ ¡/body¿ ¡/html¿<br />
XML<br />
[XML] The Extensible textbased Markup Language is a format for structured documents and data on the Web.<br />
It is derived from SGML (ISO 8879). XML is also playing an increasingly important role in the exchange <strong>of</strong> a<br />
wide variety <strong>of</strong> data on the Web.<br />
XviD<br />
[XviD] XviD is a word play, read it the reverse way and you might find a familiar term. XviD is an open source<br />
MPEG-4 codec which depending on whom you’re asking yields even better quality than the best DivX codec.
zombie<br />
[zombie] A unix process that has died but has not yet relinquished its process table slot. The parent process<br />
hasn’t executed a ”wait” for it yet).<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 108 entries in this file.
Index<br />
.Net, 9<br />
AAC, 1<br />
AC3, 1<br />
acrobat, 1<br />
AMD, 1<br />
amd, 1<br />
arpwatch, 1<br />
ASCII, 1<br />
ASF, 2<br />
AT, 2<br />
AVI, 2<br />
backdoor, 2<br />
Bandwidth, 2<br />
BUP file, 2<br />
Byte, 2<br />
CASE, 3<br />
Cell (ID), 3<br />
certificate, 3<br />
Codec, 3<br />
Container, 3<br />
CSS, 3, 4<br />
DAR, 4<br />
Deinterlace, 4<br />
Demultiplexing, 4<br />
Descrambling, 4<br />
DHCPD, 5<br />
Digital Video, 5<br />
DivX, 5<br />
DOM, 5<br />
DOS, 5<br />
DRC, 5<br />
DTML, 6<br />
DTP, 6<br />
Dynamic HTML, 6<br />
Elementary Stream (ES), 6<br />
EULA, 6<br />
FAT, 6<br />
FUD, 6<br />
GUI, 6<br />
HTML, 7<br />
HTTP, 7<br />
HTTPD, 7<br />
Hypertext, 7<br />
ICMP, 8<br />
IFO file, 7<br />
inetd, 7<br />
Interlaced, 7<br />
IP, 7<br />
IPFW, 7<br />
Java, 8<br />
KISS, 8<br />
17<br />
LDAP, 8<br />
LDIF, 8<br />
MathML, 8<br />
miniDVD, 8<br />
MM4, 9<br />
MPEG, 8<br />
MPEG4, 9<br />
MPG, 9<br />
NAT, 9<br />
Network layers, 9<br />
Newbie, 9<br />
NFS, 9<br />
OGM, 10<br />
PCMCIA, 11<br />
Perl, 10<br />
PHP, 10<br />
PNG, 10<br />
Pocket PC, 10<br />
Python, 10<br />
QNX, 10<br />
Qt, 11<br />
RDBM, 11<br />
RDBMS, 12<br />
Real time operating systems, 11<br />
rff/tff, 11<br />
Ripping, 11<br />
RSS, 11, 12<br />
RTFM, 12<br />
SBC, 12<br />
SGML, 12<br />
SMIL, 12<br />
SOAP, 12<br />
SQL, 12<br />
Sun ONE, 13<br />
SVG, 13<br />
TCP, 13<br />
TCPA, 13<br />
TLD, 13<br />
UDP, 13<br />
UML, 13<br />
VCD, 14<br />
VLDB, 14<br />
VML, 14<br />
W3C, 14<br />
Wavelets, 14<br />
WebDAV, 14<br />
Widget, 14<br />
Win FS, 15<br />
Windows Media, 15<br />
WORM, 15<br />
WYSIWYG, 15
XML, 15<br />
XviD, 15<br />
zombie, 16
N[FromContinuedFraction[Table[k,k,0,100]]]<br />
FromContinuedFractionTablek,k,0,100<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 0 entries in this file.
<strong>ENTRY</strong> CONSTANTS<br />
[<strong>ENTRY</strong> CONSTANTS] Authors: Oliver Knill: March 2000 - March 2004 Literature: Some from Mario Livio<br />
”The golden ratio”, www.mathworld.com David Wells: ”The Penguin Dictionary <strong>of</strong> Curious and Interesting<br />
Numbers”.<br />
Archimedes Constant, pi<br />
The [Archimedes Constant, pi] π = 3.14159 is the length <strong>of</strong> a half circle with radius 1. It is the area <strong>of</strong> a disc<br />
<strong>of</strong> radius 1.<br />
Bruns constant<br />
[Bruns constant] is the sum <strong>of</strong> the reciprocals <strong>of</strong> all twin primes. Brun has proven that this sum converges<br />
evenso it is unknown whether there are infinitely many twin primes.<br />
Catalan constant<br />
The [Catalan constant] is defined as the sum (−1) n /(2n + 1) 2 = 0.91596.<br />
Champernown’s number<br />
[Champernown’s number] is 0.12345678910111213... whose digits are those <strong>of</strong> all natural numbers in succession.<br />
Continued fraction constant<br />
[Continued fraction constant] is the number with continued fraction (0, 1, 2, 3, 4, 5, 6, ...) it is about 0.697774658.<br />
Euler Mascheroni constant<br />
[Euler Mascheroni constant] is defined as the limit <strong>of</strong> (1 + 1/2 + 1/3 + ... + 1/n) − log(n) as n goes to infinity.<br />
Aperi constant<br />
[Aperi constant] It is an irrational number ζ(3) = 1.20206, the value <strong>of</strong> the zeta function at 3. [Feigenbaum<br />
constant] When iterating maps f(x) = ax(1 − x) on the unit interval the stable periodic orbits bifurcate when<br />
varing a. If an are the bifurcation values, then δ = lim(an − an−1)/(an+1 − an) is a Feigenbaum constant.
golden ratio<br />
The [golden ratio] is τ = (1 + √ 5)/2 = 0.618... If 1, 1, 2, 3, 5, 8, 13, 21... are the Fibonnachi numbers (the next<br />
number is always the sum <strong>of</strong> the two previous once), then the ratio <strong>of</strong> neighboring entries approaches the<br />
golden mean. 13/21 = 0.61904 is already quite close to the golden mean. The Golden ratio has the continued<br />
fraction expansion [1, 1, 1, 1...] which means that the number can be written as τ = 1 + 1/(1 + 1/(1 + ...)). The<br />
golden mean is an example <strong>of</strong> a Diophantine number, a number which can not be approximated well by rational<br />
numbers. Especially, it is irrational. The golden ratio is also called ”golden mean” or ”divine constant”.<br />
The [golden mean] see golden ratio.<br />
golden mean<br />
Khinchin constant<br />
The [Khinchin constant] is defined as the limit (a1a2...an) 1/n where [a1, a2, ...] is the continued fraction <strong>of</strong> a<br />
random number in the sense that the limit is known to exist for almost all real numbers. It is not known for<br />
example, if π is a typical number in the sense that it produces the Khinchin constant.<br />
natural logarithmic base<br />
The [natural logarithmic base] e = 2.7182818... can be defined as exp(1) = 1 + 1/1! + 1/2! + 1/3! + ... or<br />
limn→∞(1 + 1/n) n .<br />
number <strong>of</strong> the beast<br />
The [number <strong>of</strong> the beast] is the integer 666. The ”beast” is associated with the ”antichrist”. The origin <strong>of</strong><br />
the association is the bible: the book <strong>of</strong> revelations (13:18) reads: ”this calls for wisdom: let anyone with<br />
understanding calculate the number <strong>of</strong> the beast, for it is the number <strong>of</strong> a man. Its number is six hundred and<br />
sixty six.”<br />
Pythagoras constant<br />
The [Pythagoras constant] is the square root <strong>of</strong> 2 x = √ 2 = 1.41421.... It is the length <strong>of</strong> the diagonal <strong>of</strong> the<br />
unit square. It is irrational because x = p/q would imply 2q 2 = x 2 q 2 = p 2 , which is impossible because the<br />
prime factorization on the left contains an odd number <strong>of</strong> 2’s, while it contains an even number <strong>of</strong> 2’s on the<br />
right.<br />
Smith number<br />
[Smith number] Smith numbers are integers n such that the sum <strong>of</strong> its digits in the decimal exapansion <strong>of</strong> n is qual<br />
to the sum <strong>of</strong> the digits <strong>of</strong> its prime factorization, excluding 1. Smith numbers were defined by A. Wilansky. He<br />
called it Smith numbers after his brother in law H. Swmith, whose telephone number 4937775 = 3 ∗ 5 ∗ 5 ∗ 65 ′ 837<br />
is a Smith number. Here are the first Smith numbers: 4, 22, 27, 58, 85, 94, 121, 166, 202, 265....
Wallis constant<br />
The [Wallis constant] is the real solution to the polynomial x 3 −2x+5 which is 2.0945514815.... This equation was<br />
solved by the English mathematicaian John Wallis [1616-1703] to illustrate Newton’s method for the numerical<br />
solution <strong>of</strong> equations. It has since served as a test for many subsequent methods <strong>of</strong> approximation.<br />
Zero<br />
[Zero] The integer zero 0 is the neutral element in the additive group <strong>of</strong> integers n + 0 = n.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 16 entries in this file.
Index<br />
Aperi constant, 1<br />
Archimedes Constant, pi, 1<br />
Bruns constant, 1<br />
Catalan constant, 1<br />
Champernown’s number, 1<br />
Continued fraction constant, 1<br />
Euler Mascheroni constant, 1<br />
golden mean, 2<br />
golden ratio, 2<br />
Khinchin constant, 2<br />
natural logarithmic base, 2<br />
number <strong>of</strong> the beast, 2<br />
Pythagoras constant, 2<br />
Smith number, 2<br />
Wallis constant, 3<br />
Zero, 3<br />
4
<strong>ENTRY</strong> CURVES<br />
[<strong>ENTRY</strong> CURVES] Authors: Oliver Knill, Andrew Chi, 2003 Literature: www.mathworld.com,<br />
www.2dcurves.com<br />
astroid<br />
An [astroid] is the curve t ↦→ (cos 3 (t), a sin 3 (t)) with a > 0. An asteroid is a 4-cusped hypocycloid. It is<br />
sometimes also called a tetracuspid, cubocycloid, or paracycle.<br />
Archimedes spiral<br />
An [Archimedes spiral] is a curve described as the polar graph r(t) = at where a > 0 is a constant. In words:<br />
the distance r(t) to the origin grows linearly with the angle.<br />
bowditch curve<br />
The [bowditch curve] is a special Lissajous curve r(t) = (asin(nt + c), bsin(t)).<br />
brachistochone<br />
A [brachistochone] is a curve along which a particle will slide in the shortest time from one point to an other.<br />
It is a cycloid.<br />
Cassini ovals<br />
[Cassini ovals] are curves described by ((x + a) + y 2 )((x − a) 2 + y 2 ) = k 4 , where k 2 < a 2 are constants. They<br />
are named after the Italian astronomer Goivanni Domenico Cassini (1625-1712). Geometrically Cassini ovals<br />
are the set <strong>of</strong> points whose product to two fixed points P = (−a, 0), Q = (0, 0) in the plane is the constant k 2 .<br />
For k 2 = a 2 , the curve is called a Lemniscate.<br />
cardioid<br />
The [cardioid] is a plane curve belonging to the class <strong>of</strong> epicycloids. The fact that it has the shape <strong>of</strong> a heart<br />
gave it the name. The cardioid is the locus <strong>of</strong> a fixed point P on a circle roling on a fixed circle. In polar<br />
coordinates, the curve given by r(φ) = a(1 + cos(φ)).<br />
catenary<br />
The [catenary] is the plane curve which is the graph y = c cosh(x/c). It was discovered by Jacques Bernoulli.<br />
It has the shape <strong>of</strong> a uniform flexible chain hung from two points.
catenoid<br />
The [catenoid] is the surface obatained by rotating the catenary about the x-axis. The minimal surface bounded<br />
by two coaxial rings can be a catenoid.<br />
circle<br />
A [circle] in the plane is the curve r(t) = (r cos(t), r sin(t)) where the radius r is a constant. It is the set <strong>of</strong><br />
points which have a fixed distance r from the origin. More generally, a circle is the set <strong>of</strong> points in a metric<br />
space which have a fixed distance from a given point.<br />
cissoid<br />
A [cissoid] is a plane curve given in Euclidean coordinates by y 2 (2a − x) = x 3 . In polar coordinates, it satisfies<br />
r(t) = 2a tan(t) sin(t) or in Euclidean coordinates r(t) = (2a sin 2 (t), 2a sin 3 (t)/ cos(t)). The curve has a cusp at<br />
the origin. It was first mentioned by Diocles in 180 B.C.<br />
conic section<br />
A [conic section] is a nondegenerate curve generated by intersecting a plane with one or two nappes <strong>of</strong> a cone.<br />
The three congruence classes <strong>of</strong> conic sections are the ellipse, the parabola, and the hyperbola.<br />
ellipse<br />
An [ellipse] is the locus <strong>of</strong> all points in the plane the sum <strong>of</strong> whose distances from two fixed points is a positive<br />
constant. It is also the conic section which results from a plane which intersects only one nappe <strong>of</strong> the cone.<br />
The general formula for an ellipse up to rotation and translation is x2<br />
a 2 + y2<br />
b 2 = 1.<br />
hyperbola<br />
A [hyperbola] is the set <strong>of</strong> points in the plane for which the difference <strong>of</strong> the distances from two fixed points is<br />
a constant. It is also the conic section which results from a plane intersecting a cone. The general formula for<br />
a hyperbola up to rotation and translation is x2<br />
a 2 − y2<br />
b 2 = 1.<br />
curve<br />
A [curve] is a continuous map from the real line to an the plane or to space. The word ”curve” is <strong>of</strong>ten used to<br />
mean the image <strong>of</strong> this map. Curves can be represented parametrically by r(t) = (x(t), y(t)) or implicitely as<br />
f(x, y) = 0.
Airy function<br />
The [Airy function] is commonly found as a solution to boundary value problems in quantum mechanics and<br />
electromagnetism. It is the solution to the differential equation: y ′′ = xy. The two independent solutions are<br />
(without constants):<br />
Bi(x) =<br />
Ai(x) =<br />
� ∞<br />
0<br />
� ∞<br />
0<br />
� � 3 t<br />
cos + xt dt<br />
3<br />
�<br />
t3 −<br />
e 3 +xt + sin<br />
� t 3<br />
algebraic curve<br />
3<br />
��<br />
+ xt dt<br />
A plane curve is an [algebraic curve] if it is given by g(x, y) = 0 where g is algebraic a polynomial in x and y.<br />
An algebraic curve with degree greater than 2 is called a higher plane curve. The circle g(x, y) = x 2 +y 2 −1 = 0<br />
is an example <strong>of</strong> an algebraic curve, the catenary g(x, y) = y − c cosh(x/c) = 0 is an example <strong>of</strong> a nonalgebraic<br />
curve.<br />
cubic curve<br />
A [cubic curve] is an algebraic curve <strong>of</strong> order three. Newton showed that all cubics can be generated as<br />
projections <strong>of</strong> the five divergent cubic parabolas. Examples include the cissoid <strong>of</strong> Diocles and ellptic curves.<br />
ampersand curve<br />
The [ampersand curve] is a quartic curve with implicit equation (y 2 − x 2 )(x − 1)(2x − 3) = 4(x 2 + y 2 − 2x) 2 .<br />
It looks like an ampersand.<br />
bean curve<br />
The [bean curve] is a quartic curve given by the implicit equation: x 4 + x 2 y 2 + y 4 = x(x 2 + y 2 ). It looks like a<br />
bean.<br />
bicorn<br />
The [bicorn] is the name <strong>of</strong> a collection <strong>of</strong> quartic curves studied by Sylvester in 1864 and Cayley in 1867. It is<br />
given by y 2 (a 2 − x 2 ) = (x 2 + 2ay − a 2 ) 2 .<br />
bicuspid<br />
The [bicuspid] is the quartic curve given by the implicit equation: (x 2 − a 2 )(x − a) 2 + (y 2 − a 2 ) 2 = 0.
ow<br />
The [bow] is a quartic curve with the implicit equation: x 4 = x 2 y − y 3 .<br />
cartesian oval<br />
A [cartesian oval] is a quartic curve consisting <strong>of</strong> two ovals. It is the locus <strong>of</strong> a point P whose distances from<br />
two foci F1 and F2 in two-center bipolar coordinates satisfy<br />
mr ± nr ′ = k<br />
where m and n are positive integers, k is a positive real, and r and r ′ are the distances from F1 and F2. If<br />
m = n, then the oval becomes an ellipse.<br />
Cassini oval<br />
A [Cassini oval] is one <strong>of</strong> a family <strong>of</strong> quartic curves, also called Cassini ellipses, described by a point such that<br />
the product <strong>of</strong> its distances from two fixed points a distance 2a apart is constant b 2 . The shape <strong>of</strong> the curve<br />
depends on b/a. The Cassini ovals are defined in two-center bipolar coordinates by the equation r1r2 = b 2<br />
where b is a positive constant.<br />
cruciform<br />
A [cruciform] is a plane quartic curve also called the cross curve or policeman on point duty curve. It is given<br />
by the implicit equation: x 2 y 2 − b 2 x 2 − a 2 y 2 = 0.<br />
lemniscate<br />
The [lemniscate], also known as the lemniscate <strong>of</strong> Bernoulli, is a polar curve whose most common form is the<br />
locus <strong>of</strong> points the product <strong>of</strong> whose distances from two fixed points a distance 2a away is the constant a 2 . The<br />
usual polar coordinate form is as follows: r 2 = a 2 cos(2θ).<br />
natural equation<br />
A [natural equation] is an equation which specifies a curve independent <strong>of</strong> any choice <strong>of</strong> coordinates or<br />
parametrization. This arose in the solution to the following problem: given two functions <strong>of</strong> one parameter,<br />
find the space curve for which the functions are the curvature and torsion. Often, the natural equation will<br />
be in terms <strong>of</strong> integrals.<br />
polynomial curve<br />
A [polynomial curve] is a curve obtained by fitting polynomials to a sequence <strong>of</strong> points. To fit curves better,<br />
splines like Bezier curve are more suited.
quadrifolium<br />
A [quadrifolium] is a rose curve with n = 2. It has polar equation<br />
r = a sin(2θ).<br />
sextic curve<br />
A [sextic curve] is an algebraic curve <strong>of</strong> degree 6. Examples include the atriphtaloid and the butterfly curve<br />
y 6 = x 2 − x 6 .<br />
atriphtaloid<br />
The [atriphtaloid] is a sextic curve also known as atriphtothlassic curve and given by the equation: x 4 (x 2 +<br />
y 2 ) − (ax 2 − b) 2 = 0.<br />
butterfly curve<br />
The [butterfly curve] is a sextic plane curve given by the implicit equation y 6 = x 2 − x 6 .<br />
trifolium<br />
A [trifolium] is the 3-petalled rose given in polar form as r(t) = a| cos(3t)|.<br />
spiral<br />
A [spiral], in general, is a curve with τ(s)/κ(s) constant for<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 34 entries in this file.
Index<br />
Airy function, 3<br />
algebraic curve, 3<br />
ampersand curve, 3<br />
Archimedes spiral, 1<br />
astroid, 1<br />
atriphtaloid, 5<br />
bean curve, 3<br />
bicorn, 3<br />
bicuspid, 3<br />
bow, 4<br />
bowditch curve, 1<br />
brachistochone, 1<br />
butterfly curve, 5<br />
cardioid, 1<br />
cartesian oval, 4<br />
Cassini oval, 4<br />
Cassini ovals, 1<br />
catenary, 1<br />
catenoid, 2<br />
circle, 2<br />
cissoid, 2<br />
conic section, 2<br />
cruciform, 4<br />
cubic curve, 3<br />
curve, 2<br />
ellipse, 2<br />
hyperbola, 2<br />
lemniscate, 4<br />
natural equation, 4<br />
polynomial curve, 4<br />
quadrifolium, 5<br />
sextic curve, 5<br />
spiral, 5<br />
trifolium, 5<br />
6
<strong>ENTRY</strong> FUNCTIONAL ANALYSIS<br />
[<strong>ENTRY</strong> FUNCTIONAL ANALYSIS] Authors: Oliver Knill: 2002 Literature: various notes<br />
adjoint<br />
The [adjoint] <strong>of</strong> a bounded linear operator A on a Hilbert space is the unique operator B which satisfies<br />
(Ax, y) = (x, By) for all x, y ∈ H. One calls the adjoint A ∗ . An bounded linear operator is selfadjoint, if<br />
A = A ∗ .<br />
Alaoglu’s theorem<br />
[Alaoglu’s theorem] (=Banach-Alaoglu theorem): the closed unit ball in a Banach space is weak-* compact.<br />
angle<br />
The [angle] φ between two vectors v and w <strong>of</strong> a Hilbert space is a solution φ <strong>of</strong> the equation cos(φ)||v||||w|| =<br />
(v, w), usually the smaller <strong>of</strong> the two solutions.<br />
balanced<br />
A subset Y <strong>of</strong> a vector space X is called [balanced] if tx is in Y whenever x is in Y and t < 1.<br />
B*-algebra<br />
A [B*-algebra] is a Banach algebra with a conjugate-linear anti-automorphic involution ∗ satisfying ||xx ∗ || =<br />
||x|| 2 .<br />
Banach algebra<br />
A [Banach algebra] is an algebra X over the real numbers or complex numbers which is also a Banach space<br />
such that ||xy|| ≤ ||x||||y|| for all x, y ∈ X.<br />
Banach limit<br />
A [Banach limit] is a translation-invariant functional f on the Banach space <strong>of</strong> all bounded sequence such that<br />
f(c) = c1 for constant sequences.
A [Banach space] is a complete normed space.<br />
Banach space<br />
barrel<br />
A [barrel] is a closed, convex, absorbing, balanced subset <strong>of</strong> a topological vector space.<br />
basis<br />
A [basis] (= Schauder basis) <strong>of</strong> a separable normed space is a sequence <strong>of</strong> vectors xj such that every vector x<br />
can uniquely be written as y = �<br />
j yjxj.<br />
basis<br />
A [basis] in a vector space is a linearly independent subset that generates the space.<br />
baralled space<br />
A [baralled space] is a topological vector space in which every barrel contains a neighborhood <strong>of</strong> the origin.<br />
biorthogonal<br />
Two sequences an and bn in a Hilbert space are called [biorthogonal] if Anm = (an, bm) is an unitary operator.<br />
Bergman space<br />
The [Bergman � �space]<br />
for an open subset G <strong>of</strong> the complex plane C is the collection <strong>of</strong> all anlytic function f on<br />
G for which G |f(x + iy)|2 dxdy is finite. It is an example <strong>of</strong> a Hilbert space.<br />
Buniakovsky inequality<br />
The [Buniakovsky inequality] (=Cauchy-Schwarz inequality) in a Hilbert space tells that |(a, b)| ≤ ||a|| ||b||.<br />
Cauchy-Schwartz inequality<br />
The [Cauchy-Schwartz inequality] in a Hilbert space H states that |(f, g)| ≤ ||f|| ||g||. It is also called Buniakovsky<br />
inequality or CBS inequality.
compact operator<br />
A [compact operator] is a bounded linear operator A on a Hilbert space, which has the property that the image<br />
A(B) <strong>of</strong> the unit ball B has compact closure in H.<br />
compact operator<br />
A bounded operator A on a separable Hilbert space is called [diagonalizable] if there exists a basis in H such<br />
that Hvi = λivi for every basis vector vi. Compact normal operators are diagonalizable.<br />
dimension<br />
The [dimension] <strong>of</strong> a Hilbert space H is the cardinality <strong>of</strong> a basis <strong>of</strong> H. A Hilbert space is called seperable, if<br />
the cardinality <strong>of</strong> the basis is the cardinality <strong>of</strong> the integers.<br />
Egorov’s theorem<br />
[Egorov’s theorem] Let (X, S, m) be a measure space, where m(S) has finite measure. If a sequence fn <strong>of</strong><br />
measurable functions converges to f almost everywhere, then for every d¿0, there is a set Ed ⊂ X such that<br />
fn → f uniformly on E \ Ed and m(Ed) < d.<br />
finite rank operator<br />
A bounded linear operator A on a Hilbert space H is called a [finite rank operator] if the rank <strong>of</strong> A is finite<br />
dimensional. Finite rank operators are examples <strong>of</strong> compact operators.<br />
Hilbert space<br />
A [Hilbert space] H is a vector space equiped with an inner product (x, y) for which the corresponding metric<br />
d(x, y) = ||x − y|| = (x − y, x − y) makes (H, d) into a complete metric space. Examples:<br />
• l2 (N) is the collection <strong>of</strong> sequences an such that �<br />
n |an| < ∞ is a Hilbert space with inner product<br />
(a, b) = �<br />
n anbn.<br />
• L 2 (G) the space <strong>of</strong> all analytic functions on an open subset <strong>of</strong> the complex plane which are also in L 2 (G, µ),<br />
where µ is the Lebesgue measure on G.<br />
• All vectors <strong>of</strong> a finite dimensional vector space, where the inner product is the usual dot product.<br />
• All square integrable functions L 2 (X, µ) on a measure space (X, S, µ).<br />
idempotent<br />
A bounded linear operator A on a Hilbert space is called [idempotent] if A 2 = A. Projections P are examples<br />
<strong>of</strong> idempotent operators.
Lusin’s theorem<br />
[Lusin’s theorem] If (X, S, m) is a measure space and f is a measureable function on S. For every d > 0, there<br />
is a set Ed with m(Ed) < d and a measurable function g such that g is continuous on Ed.<br />
linear operator<br />
A [linear operator] is a linear map between two Hilbert spaces or two Banach spaces. Important examples are<br />
bounded linear operators, linear operators which also continuous maps. Linear operators are also called linear<br />
transformations.<br />
norm<br />
The [norm] <strong>of</strong> a bounded linear operator A on a Hilbert space H is defined as ||A|| = sup ||x||≤1,x∈H ||Ax||.<br />
normal<br />
A bounded linear operator A is called [normal] if AA ∗ = A ∗ A, where A ∗ is the adjoint <strong>of</strong> A. Examples:<br />
• selfadjoint operators are normal.<br />
• unitary operators are normal<br />
Open mapping theorem<br />
[Open mapping theorem] If a map A from X to Y is a surjective continuous linear operator between two Banach<br />
spaces X and Y , and U is an open set in X, then A(U) is open in Y .<br />
The pro<strong>of</strong> <strong>of</strong> the theorem which is also called the Banach-Schauder theorem uses the Baire category theorem.<br />
implications:<br />
• A bijective continuous linear operator between the Banach spaces X and Y has a continuous inverse.<br />
• Closed graph theorem: if for every sequence xn ∈ X with xn → 0 and Axn → y follows y = 0, then A is<br />
continuous.<br />
Riesz representation theorem<br />
[Riesz representation theorem] If f is a bounded linear functional on a Hilbert space H, then there exists a<br />
vector y ∈ H such that f(x) = (x, y) for all x ∈ H.<br />
Sturm Liouville operator<br />
A [Sturm Liouville operator] L is an unbounded operator on the Hilbert space L 2 [a, b] defined by L(f) =<br />
−f ′′ + gf, where g is a continuous function on [a, b].
unitary<br />
A bounded linear operator A on a Hilbert space is called [unitary] if AA ∗ = A ∗ A = 1 if 1 is the identity operator<br />
1(x) = x.<br />
unit ball<br />
The [unit ball] B in a Hilbert space H is the set <strong>of</strong> all points x ∈ H satisfiying ||x| ≤ 1.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 32 entries in this file.
Index<br />
adjoint, 1<br />
Alaoglu’s theorem, 1<br />
angle, 1<br />
B*-algebra, 1<br />
balanced, 1<br />
Banach algebra, 1<br />
Banach limit, 1<br />
Banach space, 2<br />
baralled space, 2<br />
barrel, 2<br />
basis, 2<br />
Bergman space, 2<br />
biorthogonal, 2<br />
Buniakovsky inequality, 2<br />
Cauchy-Schwartz inequality, 2<br />
compact operator, 3<br />
dimension, 3<br />
Egorov’s theorem, 3<br />
finite rank operator, 3<br />
Hilbert space, 3<br />
idempotent, 3<br />
linear operator, 4<br />
Lusin’s theorem, 4<br />
norm, 4<br />
normal, 4<br />
Open mapping theorem, 4<br />
Riesz representation theorem, 4<br />
Sturm Liouville operator, 4<br />
unit ball, 5<br />
unitary, 5<br />
6
<strong>ENTRY</strong> FUNCTIONS<br />
[<strong>ENTRY</strong> FUNCTIONS] Authors: Oliver Knill: 2003, Literature: no<br />
real-valued function<br />
A [real-valued function] is usually assumed to be map to the reals.<br />
abscissa<br />
[abscissa] The x-coordinate in an (x,y) graph <strong>of</strong> a function. The y-coordinates is called ordinate.<br />
ordinate<br />
[ordinate] The y-coordinate in an (x,y) graph <strong>of</strong> a function. The x-coordinates is called abscissa.<br />
Airy function<br />
The [Airy function] is defined as the solution <strong>of</strong> the differential equation y ′′ − xy = 0.<br />
Briggsian logarithm<br />
The [Briggsian logarithm] also called common logarithm is the logarithm to the base 10.<br />
Bessel function<br />
THe [Bessel function] is a special function. Bessel function <strong>of</strong> the first kind <strong>of</strong> order zero is defined as J0 =<br />
� ∞<br />
k=0 (−1)k (x/2) 2k /(k!) 2 .<br />
Sin<br />
The [Sin] is a trigonometric function. It can be defined by its series sin(x) = x − x 3 /3! + x 5 /5! − ..., where<br />
5! = 54321 is the factorial <strong>of</strong> 5. The sine function can also be defined as the imaginary part <strong>of</strong> exp(ix) =<br />
cos(x) + i sin(x), where i = (−1) ( 1/2) is the imaginary unit. Examples <strong>of</strong> values sin(0) = 0, sin(π/2) =<br />
1, sin(π) = 0, sin(3π/2) = −1.<br />
[Csc] The cosecant is defined as csc(x) = 1/ sin(x).<br />
Csc
Arcsin<br />
[Arcsin] The arcsin is the inverse <strong>of</strong> sin. It is also denoted by sin ( −1)(x) or asin(x). One has the identities<br />
arcsin(sin(x)) = x, or sin(arcsin(x)) = x.<br />
Sinh<br />
[Sinh] The hyperbolic sine can be defined as sinh(x) = (exp(x) − exp(−x))/2. Examples: sinh(0) = 0.<br />
[ArcSinh] The inverse <strong>of</strong> sinh is called arcsinh.<br />
ArcSinh<br />
Cos<br />
The trigonometric function [Cos] can be defined by its series cos(x) = 1 − x 2 /2! + x 4 /4! − x 6 /6! − ..., where<br />
4! = 4321 is the factorial <strong>of</strong> 4. It can also be defined as the real part <strong>of</strong> exp(ix), where i = (−1) 1 /2 is the<br />
imaginary unit, the square root <strong>of</strong> -1. Examples: cos(0) = 1, cos(pi/2) = 0 sin(π) = −1, sin(3π/2) = 0.<br />
Arccos<br />
[Arccos] The inverse <strong>of</strong> the function cos is written arccos(x), also denoted by cos ( −1)(x) or acos(x). We have<br />
the identities arccos(cos(x)) = x, or cos(arccos(x)) = x.<br />
[Sec] The secant is defined as sec(x) = 1/ cos(x).<br />
Sec<br />
Cosh<br />
[Cosh] The hyperbolic cosine can be defined as sinh(x) = (exp(x) + exp(−x))/2. Examples: cosh(0) = 1.<br />
[ArcCosh] The inverse <strong>of</strong> cosh is called arccosh.<br />
ArcCosh<br />
Tan<br />
The [Tan] is a trigonometric function. It can be defined as tan(x) = sin(x)/ cos(x). Examples: tan(0) =<br />
0, tan(π/4) = 1.
Arctan<br />
[Arctan] The inverse <strong>of</strong> tan is the function arctan(x). It is also called tan ( − 1)(x). One has arctan(tan(x)) = x<br />
and tan(arctan(x)) = x. Examples: arctan(1) = π/2.<br />
Cot<br />
[Cot] is a trigonometric function. It can be defined as cot(x) = cos(x)/ sin(x). It can also be defined<br />
geometrically as the relation <strong>of</strong> two sides in a right angle triangle if x is one <strong>of</strong> the angles. Examples:<br />
cot(π/2) = 0, cot(π/4) = 1.<br />
Exp<br />
[Exp] is the exponential function. It can be defined by its series exp(x) = 1 + x + x 2 /2! + x 3 /3! + x 4 /4! + ...<br />
where 4! = 4321 is the factorial <strong>of</strong> 4. Examples: exp(0) = 1, exp(1) = e = 2.712....<br />
Sqr<br />
[Sqr] The square <strong>of</strong> a number is the product <strong>of</strong> the number by itself. For example, the square <strong>of</strong> 4 is 16. The<br />
square <strong>of</strong> a function sin(x) is denoted by sin 2 (x).<br />
Zeta<br />
[Zeta] ζ(s) is the Riemann zeta function. It is defined for complex numbers s which have Re(s) > 1 as<br />
ζ(s) = 1+1/2 s +1/3 s +.... The function can be continued to the entire complex plane except at s = 1, where the<br />
function has a singularity. The zeta function has zeros at −2, −4, −6 and also zeros on the real line Re(s) = 1/2.<br />
The famous Riemann hypothesis claims that all the nontrivial zeros are on this line. This conjecture remains<br />
unproven until today and is considered one <strong>of</strong> the most important open problems in mathematics.<br />
Log<br />
[Log] The logarithm is the inverse to the exponential function: log(exp(x)) = x and exp(log(x)) = x. For<br />
example: log(1) = 0, log(e) = 1. The logarithm function satisfies for example the laws log(xy) = log(x)+log(y),<br />
log(x/y) = log(x) − log(y), log(x y ) = y log(x).<br />
Sqrt<br />
[Sqrt] The square root <strong>of</strong> a number x is the number which<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 24 entries in this file.
Index<br />
abscissa, 1<br />
Airy function, 1<br />
Arccos, 2<br />
ArcCosh, 2<br />
Arcsin, 2<br />
ArcSinh, 2<br />
Arctan, 3<br />
Bessel function, 1<br />
Briggsian logarithm, 1<br />
Cos, 2<br />
Cosh, 2<br />
Cot, 3<br />
Csc, 1<br />
Exp, 3<br />
Log, 3<br />
ordinate, 1<br />
real-valued function, 1<br />
Sec, 2<br />
Sin, 1<br />
Sinh, 2<br />
Sqr, 3<br />
Sqrt, 3<br />
Tan, 2<br />
Zeta, 3<br />
4
<strong>ENTRY</strong> GROUP THEORY<br />
[<strong>ENTRY</strong> GROUP THEORY] Authors: started Mark Lezama: October 2003 Literature: ”Algebra” by Michael<br />
Artin, Mathworld<br />
Group theory<br />
[Group theory] is studies algebraic objects called groups. The German mathematician Karl Friedrich Gauss<br />
(1777-1855) developed but did not publish some <strong>of</strong> the mathematics <strong>of</strong> group theory. The French mathematician<br />
Evariste Galois (1811-1832) is generally credited with being the first to develop the theory, which he did by<br />
developing new techniques to study the solubility <strong>of</strong> equations. Group theory is a powerful method for analyzing<br />
abstract and physical systems in which symmetry –the intrinsic property <strong>of</strong> an object to remain invariant under<br />
certain classes <strong>of</strong> transformations– is present because the mathematical study <strong>of</strong> symmetry is systematized and<br />
formalized in group theory. Consequently, group theory is an important tool in physics particularly in quantum<br />
mechanics.<br />
group<br />
A [group] is an object consisting <strong>of</strong> a set G and a law <strong>of</strong> composition (or binary operation) L on G satisfying:<br />
• L is associative.<br />
• L has an identity in G.<br />
• Every element <strong>of</strong> G has an inverse.<br />
The study <strong>of</strong> groups is known as group theory. If a group G has n elements where n is a positive integer, then<br />
G is a finite group with order n. If a group is not finite it is infinite. Examples:<br />
• Z + , the integers under addition;<br />
• R + = (R, +), the real numbers under addition;<br />
• R × = (R − {0}, ·), the real numbers without zero under multiplication;<br />
• GLn(C), the n × n general linear group under matrix multiplication;<br />
• Sn, the symmetric group on n objects under composition.<br />
law <strong>of</strong> composition<br />
A [law <strong>of</strong> composition] or, binary operation, on a set S is a function from S × S into S. That is, a law <strong>of</strong><br />
composition on S prescribes a rule for combining pairs <strong>of</strong> elements in S to get an element in S. For convenience,<br />
functional notation is not used; that is, if a law <strong>of</strong> composition f sends (a, b) to c, one does not usually write<br />
f(a, b) = c. It is customary to instead use notation that resembles that used for multiplication or addition <strong>of</strong><br />
real numbers, such as ab = c, a · b = c, a ◦ b = c, a + b = c, and so on.<br />
An example <strong>of</strong> a law <strong>of</strong> composition is multiplication on the real numbers, R. If m: R × R → R defines<br />
multiplication on R then m(x, y) = x · y. For example m(2, 5) = 2 · 5 = 10.
inary operation<br />
A [binary operation], or law <strong>of</strong> composition, on a set S is a function from S × S into S. That is, a binary<br />
operation on S prescribes a rule for combining pairs <strong>of</strong> elements in S to get an element in S. For convenience,<br />
functional notation is not used; that is, if a binary operation f sends (a, b) to c, one does not usually write<br />
f(a, b) = c. It is customary to instead use notation that resembles that used for multiplication or addition <strong>of</strong><br />
real numbers, such as ab = c, a · b = c, a ◦ b = c, a + b = c, and so on.<br />
An example <strong>of</strong> a binary operation is multiplication on the real numbers, R. If m: R × R → R defines multiplication<br />
on R then m(x, y) = x · y. For example m(2, 5) = 2 · 5 = 10.<br />
associative<br />
A law <strong>of</strong> composition on a set S is [associative] if for all a, b, c ∈ S, (ab)c = a(bc). The informal intuition<br />
behind associativity (the property <strong>of</strong> being associative) is that if one has an expression in which there are<br />
many parentheses and the only operation performed in this expression is that defined by an associative law <strong>of</strong><br />
composition, then one may ignore the parentheses. For example, if · is an associative law <strong>of</strong> composition on S<br />
and a, b, c, d ∈ S, then ((a · (b · c)) · d = ((a · b) · c) · d = (a · b) · (c · d) and so on; thus one may write a · b · c · d<br />
without being ambiguous.<br />
An example <strong>of</strong> an associative law <strong>of</strong> composition is addition on the integers, Z. That is, for all a, b, c ∈ Z,<br />
(a + b) + c = a + (b + c).<br />
identity<br />
An [identity] for a law <strong>of</strong> composition on a set S is an element e such that, for all a ∈ S, ea = a and ae = a.<br />
Note that a law <strong>of</strong> composition has at most one identity. The symbols e, 0 and 1 are commonly used to denote<br />
the identity element <strong>of</strong> a group. The number 0 is an identity for addition on the real numbers.<br />
identity<br />
Suppose a set S has a law <strong>of</strong> composition with identity 1. For every element a ∈ S, if there exists an element<br />
b ∈ S such that ab = 1 and ba = 1 then b is the [inverse] <strong>of</strong> a. When using multiplicative notation for the law<br />
<strong>of</strong> composition, the inverse <strong>of</strong> a can be written as a −1 . As an example, the inverse <strong>of</strong> any integer n is −n where<br />
the law <strong>of</strong> composition is addition and the identity is 0. As another example, the inverse <strong>of</strong> any nonzero real<br />
, where the law <strong>of</strong> composition is multiplication and the identity is 1.<br />
number x is 1<br />
x<br />
general linear group<br />
The n × n [general linear group] GLn(F ) is the set <strong>of</strong> n × n matrices with entries in the field F and nonzero<br />
determinant, under the law <strong>of</strong> composition <strong>of</strong> matrix multiplication. Thus GLn(F ) is the group <strong>of</strong> n × n<br />
invertible matrices with entries in F . If F is a finite field <strong>of</strong> field order q then sometimes the general linear<br />
group GLn(F ) is denoted by GLn(q). The general linear group <strong>of</strong>ten appears with respect to the real numbers,<br />
R, or the complex numbers, C; that is, the general linear group <strong>of</strong>ten appears as GLn(R) or GLn(C).<br />
The special linear group SLn(F ) is the subgroup <strong>of</strong> GLn(F ) whose elements have determinant equal to 1.
special linear group<br />
The n × n [special linear group] SLn(F ) is the set <strong>of</strong> n × n matrices with entries in the field F and determinant<br />
equal to 1, under the law <strong>of</strong> composition <strong>of</strong> matrix multiplication.<br />
If F is a finite field <strong>of</strong> field order q then sometimes the special linear group SLn(F ) is denoted by SLn(q).<br />
SLn(F ) is a subgroup <strong>of</strong> the general linear group GLn(F ).<br />
trivial<br />
A group is [trivial] if it contains exactly one element. The one element in the group is the identity element. As<br />
all trivial groups are isomorphic, one usually refers to a trivial group as the trivial group. A group that is not<br />
trivial is nontrivial.<br />
trivial<br />
The group containing exactly one element (the identity) is unique up to isomorphism and is therefore called the<br />
[trivial group]. The trivial group is a normal subgroup <strong>of</strong> every group.<br />
A group is [nontrivial] if it is not trivial.<br />
nontrivial<br />
abelian<br />
A group is [abelian] if its law <strong>of</strong> composition is commutative. Examples <strong>of</strong> abelian groups include the following:<br />
• R + = (R, +), the real numbers under addition;<br />
• R × = (R − {0}, ·), the real numbers without zero under multiplication;<br />
• any cyclic group.<br />
Examples <strong>of</strong> nonabelian groups, i.e. groups that are not abelian:<br />
• GLn(C), the general linear group;<br />
• The symmetric group on n objects, where n is a positive integer greater than 2.<br />
commutative<br />
A law <strong>of</strong> composition on a set S is [commutative] if for all a, b ∈ S ab = ba. An example <strong>of</strong> a commutative law<br />
<strong>of</strong> composition is addition on the real numbers: for example, 3.2 + 4 = 7.2 = 4 + 3.2.
cancellation Law<br />
The [cancellation Law] states that if a, b, and c are elements <strong>of</strong> a group and if ab = ac then b = c. Similarly, if<br />
ba = ca then b = c. The Cancellation Law follows from the fact that every element <strong>of</strong> a group has an inverse.<br />
permutation<br />
If S is a set, then a [permutation] <strong>of</strong> S is a bijective map from S into S. The intuition underlying the definition<br />
<strong>of</strong> a permutation is that a permutation determines a reordering <strong>of</strong> the elements in a list or the rearrangement<br />
<strong>of</strong> objects. For example, the permutation σ : {1, 2, 3} → {1, 2, 3} defined by σ(1) = 2, σ(2) = 1, and σ(3) = 3<br />
can be thought to represent the reordering <strong>of</strong> the list 1,2,3 that results in the list 2,1,3. There is an important<br />
kind <strong>of</strong> permutation called a transposition. A transposition <strong>of</strong> a set S is a permutation σ: S → S satisfying the<br />
following: there exist s1, s2 ∈ S such that<br />
• σ(s1) = s2<br />
• σ(s2) = s1<br />
• and for all s ∈ S, if s �= s1 and s �= s2, then σ(s) = s.<br />
Every permutation <strong>of</strong> a finite set can be written as the composition <strong>of</strong> a finite number <strong>of</strong> transpositions <strong>of</strong> that<br />
set. For example, the permutation σ : {1, 2, 3} → {1, 2, 3} defined by σ(1) = 2, σ(2) = 3, and σ(3) = 1 is<br />
equivalent to the composition <strong>of</strong> two transpositions. Define σ1 : {1, 2, 3} → {1, 2, 3} by σ1(1) = 2, σ1(2) = 1,<br />
and σ(3) = 3, and define σ2 : {1, 2, 3} → {1, 2, 3} by σ2(1) = 3, σ1(2) = 2, and σ(3) = 1. Then σ1 and σ2 are<br />
transpositions and σ = σ2 ◦ σ1.<br />
The sign <strong>of</strong> a permutation σ is (−1) n where n is a finite positive integer such that there exist n transpositions<br />
whose composition equals σ. If a permutation has sign 1, then it is called an even permutation. If a permutation<br />
has sign -1 then it is called an odd permutation. Thus the identity permutation is an even permutation (since<br />
it is equal to the composition <strong>of</strong> any transposition with itself), and any transposition is an odd permutation<br />
(since it is equal to one transposition). The sign map encapsulates the notion <strong>of</strong> the sign <strong>of</strong> a permutation <strong>of</strong> a<br />
finite set.<br />
The set <strong>of</strong> permutations on a set forms a group where the law <strong>of</strong> composition is composition <strong>of</strong> functions.<br />
One example <strong>of</strong> a group <strong>of</strong> permutations that appears frequently in group theory is the symmetric group on n<br />
objects, i.e. the group <strong>of</strong> permutations <strong>of</strong> the set {1, 2, . . . , n}.<br />
transposition<br />
A [transposition] <strong>of</strong> a set S is a permutation σ: S → S satisfying the following: there exist s1, s2 ∈ S such that<br />
• σ(s1) = s2<br />
• σ(s2) = s1<br />
• and for all s ∈ S, if s �= s1 and s �= s2, then σ(s) = s.<br />
Every permutation <strong>of</strong> a finite set can be written as the composition <strong>of</strong> a finite number <strong>of</strong> transpositions <strong>of</strong> that<br />
set. For example, the permutation σ : {1, 2, 3} → {1, 2, 3} defined by σ(1) = 2, σ(2) = 3, and σ(3) = 1 is<br />
equivalent to the composition <strong>of</strong> two transpositions. Define σ1 : {1, 2, 3} → {1, 2, 3} by σ1(1) = 2, σ1(2) = 1,<br />
and σ(3) = 3, and define σ2 : {1, 2, 3} → {1, 2, 3} by σ2(1) = 3, σ1(2) = 2, and σ(3) = 1. Then σ1 and σ2 are<br />
transpositions and σ = σ2 ◦ σ1. Every transposition is an odd permutation.
sign<br />
The [sign] <strong>of</strong> a permutation σ is (−1) n where n is a finite positive integer such that there exist n transpositions<br />
whose composition equals σ. If a permutation has sign 1, then it is called an even permutation. If a permutation<br />
has sign -1 then it is called an odd permutation. Thus the identity permutation is an even permutation (since<br />
it is equal to the composition <strong>of</strong> any transposition with itself), and any transposition is an odd permutation<br />
(since it is equal to one transposition).<br />
even permutation<br />
An [even permutation] is a permutation that has sign 1. That is, an even permutation is the composition <strong>of</strong> an<br />
even number <strong>of</strong> transpositions. Thus the identity permutation is an even permutation.<br />
odd permutation<br />
An [odd permutation] is a permutation that has sign -1. That is, an odd permutation is the composition <strong>of</strong> an<br />
odd number <strong>of</strong> transpositions. Thus every tranposition is an odd permutation.<br />
symmetric group<br />
The [symmetric group] on n objects, denoted Sn, is the group <strong>of</strong> permutations <strong>of</strong> the set {1, 2, . . . , n}; the law<br />
<strong>of</strong> composition is composition <strong>of</strong> functions. The order <strong>of</strong> Sn is n! for all positive integers n. For example,<br />
S2 = {e, σ}, where e is the identity permutation, and σ is a transposition. That is, e is the identity element <strong>of</strong><br />
S2 and is defined by e(1) = 1 and e(2) = 2; σ is defined by σ(1) = 2 and σ(2) = 1.<br />
sign map<br />
The [sign map], denoted sign, is a group homomorphism from the symmetric group, Sn, into the group {1, −1}<br />
(under multiplication). The sign map is defined by sign(σ) = (−1) k where σ is equal to the composition <strong>of</strong> k<br />
transpositions. The sign map is well-defined because it is a standard result that if σ is any permutation (<strong>of</strong><br />
any set), and if σ is equal to the composition <strong>of</strong> k transpositions and is also equal to the composition <strong>of</strong> m<br />
transpositions, then (−1) k = (−1) m . The kernel <strong>of</strong> the sign map is the alternating group, An; that is, An is the<br />
group <strong>of</strong> even permutations on n objects.<br />
alternating group<br />
The [alternating group] is the kernel <strong>of</strong> the sign map. In other words, the alternating group on n objects, usually<br />
denoted An, is a normal subgroup <strong>of</strong> the symmetric group on n objects: An = {σ ∈ Sn | sign(σ) = 1}. Thus<br />
An is the group <strong>of</strong> even permutations in Sn. For n ≥ 5, An is a simple group, i.e. a group that has no proper<br />
normal subgroup.
simple group<br />
A group G is a [simple group] if every normal subgroup N <strong>of</strong> G is not a proper subgroup. That is, G is simple<br />
if its only normal subgroups are G and the trivial group. The alternating group An is simple for n ≥ 5. Any<br />
cyclic group <strong>of</strong> prime order is simple. Any cyclic group <strong>of</strong> prime order is simple. In fact, any simple abelian<br />
group is a cyclic group <strong>of</strong> prime order.<br />
subgroup<br />
A subset H <strong>of</strong> a group G is a [subgroup] <strong>of</strong> G if it satisfies the following properties:<br />
• If a ∈ H and b ∈ H, then ab ∈ H.<br />
• 1 ∈ H, where 1 is the identity element <strong>of</strong> G.<br />
• If a ∈ H then the inverse <strong>of</strong> a, a −1 , is also in H.<br />
When it is clear that G is a group, sometimes H ⊆ G is used to denote that H is a subgroup <strong>of</strong> G (as opposed<br />
to merely being a subset <strong>of</strong> G).<br />
Every nontrivial group G has at least two subgroups: the whole group G and the subgroup {1} consisting<br />
exactly <strong>of</strong> the identity element <strong>of</strong> G. If G is trivial then these two subgroups are the same and G has exactly<br />
one subgroup. A subgroup is a proper subgroup if it is neither the whole group nor the trivial group.<br />
As an example, the integers under addition are a subgroup <strong>of</strong> the real numbers under addition.<br />
By Lagrange’s Group Theorem, if H is a subgroup <strong>of</strong> a finite group G, the order <strong>of</strong> H divides the order <strong>of</strong> G.<br />
proper subgroup<br />
A [proper subgroup] <strong>of</strong> a group G is a nontrivial subgroup <strong>of</strong> G that is not equal to G.<br />
order<br />
A finite group G is said to have [order] n if G has n elements. More generally, the order <strong>of</strong> a group G is the<br />
cardinality <strong>of</strong> the set G, both <strong>of</strong> which are <strong>of</strong>ten denoted |G|.<br />
For any given element x <strong>of</strong> a given group, if there exists a positive integer k such that x k = 1, then x is said to<br />
have order m, where m is the least positive integer satisfying x m = 1. If x k �= 1 for all positive integers k, then<br />
x is said to have infinite order.
cyclic group<br />
If G is a group and if x is an element <strong>of</strong> G, the [cyclic group] 〈x〉 generated by x is the set <strong>of</strong> all powers <strong>of</strong> x:<br />
〈x〉 = {. . . , x −2 , x −1 , 1, x, x 2 , . . .}.<br />
Note that 〈x〉 is the smallest subgroup <strong>of</strong> G which contains x. Further note that any cyclic group is abelian. If<br />
x has infinite order then 〈x〉 is said to be infinite cyclic. Note that if 〈x〉 is infinite cyclic then 〈x〉 is isomorphic<br />
to Z + , the integers under addition. As a result, one sometimes refers to any infinite cyclic group as the infinite<br />
cyclic group, denoted Z + .<br />
If x has order n, then 〈x〉 has order n and is called a cyclic group <strong>of</strong> order n:<br />
〈x〉 = {1, x, x 2 , . . . , x n }.<br />
If 〈x〉 is a cyclic group <strong>of</strong> order n, then 〈x〉 is isomorphic to Z/n, where Z/n is the group satisfying the following<br />
properties (we use additive notation as opposed to multiplicative notation for the law <strong>of</strong> composition <strong>of</strong> Z/n):<br />
1. Z/n = {0, 1, 2, . . . , n − 1}. 2. for any x, y ∈ Z/n, x +1 y is the unique element in Z/n which is congruent<br />
modulo n to x + y, where +1 denotes the law <strong>of</strong> composition on Z/n and + denotes conventional integer<br />
addition. Normally + is used to denote the law <strong>of</strong> composition on Z/n, but +1 is used here to distinguish<br />
it from conventional addition. Two integers a and b are congruent modulo n, written a ≡ b(modulo n), if n<br />
divides b − a.<br />
As a result, one sometimes refers to any cyclic group <strong>of</strong> order n as the cyclic group <strong>of</strong> order n, <strong>of</strong>ten denoted<br />
Z/n.<br />
cyclic group<br />
Let G1 and G2 be groups. A map ϕ: G1 → G2 is a group [homomorphism] if ϕ(ab) = ϕ(a)ϕ(b) for all a, b ∈ G1.<br />
Here we use the same multiplicative notation for the laws <strong>of</strong> composition <strong>of</strong> G1 and G2, even though there is<br />
no requirement that their laws <strong>of</strong> composition be the same.<br />
Note that ϕ(1G1 ) = 1G2 and ϕ(a−1 ) = ϕ(a) −1 for all a ∈ G, where 1Gi is the identity <strong>of</strong> Gi.<br />
The kernel <strong>of</strong> ϕ, sometimes denoted ker ϕ, is the set {x ∈ G1 | ϕ(x) = 1G2 }. Note that ker ϕ is a normal<br />
subgroup <strong>of</strong> G2.<br />
Another subgroup <strong>of</strong> G2 determined by ϕ is the image <strong>of</strong> ϕ, sometimes denoted im ϕ. The image <strong>of</strong> ϕ is im<br />
ϕ = {x ∈ G2 | x = ϕ(a) for some a ∈ G1}. Sometimes the image <strong>of</strong> ϕ is denoted ϕ(G1). The following are<br />
examples <strong>of</strong> homomorphisms:<br />
• The inclusion map i: H → G defined by i(a) = a, where H is a subgroup <strong>of</strong> G. ker i = {1G} and im<br />
i = H.<br />
• For a fixed a ∈ G, the map ϕ: Z + → G defined by ϕ(n) = a n , where Z + denotes the integers with addition.<br />
ker ϕ = {n | a n = 1G} and im ϕ = 〈a〉 (the cyclic subgroup generated by a).<br />
• The determinant map det: GLn(R) → R × , where GLn(R) denotes the general linear group and R ×<br />
denotes the real numbers without zero under multiplication. kerdet = SLn(R), the special linear group,<br />
and imdet = R × .<br />
• The sign map on permutations sign: Sn → {1, −1}, where Sn denotes the symmetric group on n objects.<br />
ker sign = An, the alternating group, and im sign = {1, −1}.<br />
Let R1 and R2 be rings. A map ϕ: R1 → R2 is a ring homomorphism if<br />
• ϕ(a + b) = ϕ(a) + ϕ(b),<br />
• ϕ(ab) = ϕ(a)ϕ(b), and<br />
• ϕ(1R1 ) = 1R2 , for all a, b ∈ R1.<br />
Here we use the same additive and multiplicative notation for the laws <strong>of</strong> composition <strong>of</strong> R1 and R2, even<br />
though there is no requirement that their laws <strong>of</strong> composition be the same.
kernel<br />
The [kernel] <strong>of</strong> a group homomorphism ϕ: G1 → G2 is the set ker ϕ = {x ∈ G1 | ϕ(x) = 1G2 }, where 1G2 denotes<br />
the identity <strong>of</strong> G2. The kernel <strong>of</strong> a homomorphism is an important example <strong>of</strong> a normal subgroup. There are<br />
many results involving the kernel <strong>of</strong> a homomorphism.<br />
image<br />
The [image] <strong>of</strong> a map ϕ: G1 → G2 is the set {x ∈ G2 | x = ϕ(a) for some a ∈ G1}. In general, the image <strong>of</strong> ϕ is<br />
<strong>of</strong>ten denoted ϕ(G1). If ϕ is a group homomorphism, then the image <strong>of</strong> ϕ is a subgroup <strong>of</strong> G2 and is sometimes<br />
denoted im ϕ.<br />
isomorphism<br />
A group [isomorphism] is a bijective group homomorphism.<br />
A ring isomorphism is a bijective ring homomorphism.<br />
isomorphic<br />
Two groups G1 and G2 are [isomorphic] if there exists a group isomorphism from G1 into G2. Sometimes<br />
G1 ∼ = G2 is used to denote ‘G1 and G2 are isomorphic.’ Note that ∼ = is an equivalence relation on the set <strong>of</strong><br />
all groups. When one speaks <strong>of</strong> classifying groups, hat is usually referred to is the classification <strong>of</strong> isomorphism<br />
classes. Thus one might say that there are two groups <strong>of</strong> order 6 up to isomorphism, meaning that there are<br />
two isomorphism classes <strong>of</strong> groups <strong>of</strong> order 6.<br />
One sometimes says that ‘G1 is isomorphic to G2’ instead <strong>of</strong> saying ‘G1 and G2 are isomorphic.’<br />
automorphism<br />
An [automorphism] <strong>of</strong> a group G is an isomorphism from G into G. The identity map is a simple example <strong>of</strong> an<br />
automorphism. Conjugation by an element <strong>of</strong> the group is an important example <strong>of</strong> an automorphism. That<br />
is, for a fixed element b ∈ G, conjugation by b is the map ϕ: G → G defined by ϕ(a) = bab −1 . Here we use<br />
multiplicative notation for the group law <strong>of</strong> composition. Note that if G is abelian, then conjugation by any<br />
element is the identity map. However, if G is not abelian, then there exists a nontrivial conjugation (i.e. a<br />
conjugation not equal to the identity map) <strong>of</strong> G.<br />
automorphism<br />
Let G be a group and let b ∈ G. The map ϕ: G → G defined by ϕ(a) = bab −1 is [conjugation] by b. Note that<br />
conjugation is an automorphism <strong>of</strong> G. Further note that if G is abelian, then conjugation by any element is the<br />
identity map. However, if G is not abelian, then there exists a nontrivial conjugation (i.e. a conjugation not<br />
equal to the identity map) <strong>of</strong> G.
conjugation<br />
Let G be a group and let H be a subgroup <strong>of</strong> G. H is a [normal subgroup] <strong>of</strong> G (sometimes written H ⊳ G)<br />
if for all a ∈ H and for all x ∈ G, xax −1 ∈ H. Note that it follows that any subgroup <strong>of</strong> an abelian group is<br />
normal.<br />
Normal subgroups appear <strong>of</strong>ten in group theory. Every group G has at least one normal subgroup, called the<br />
center <strong>of</strong> G, denoted by Z or Z(G). The center <strong>of</strong> G is the set <strong>of</strong> elements that commute with every element <strong>of</strong><br />
G: Z(G) = {z ∈ G | zx = xz for all x ∈ G}. Another important example <strong>of</strong> a normal subgroup is the kernel <strong>of</strong><br />
a group homomorphism.<br />
center<br />
The [center] <strong>of</strong> a group G, denoted by Z or Z(G) is the set <strong>of</strong> elements that commute with every element <strong>of</strong> G:<br />
Z(G) = {z ∈ G | zx = xz for all x ∈ G}. Note that if G is abelian then Z(G) = G.<br />
coset<br />
Given a subgroup H <strong>of</strong> a group G, a [coset] <strong>of</strong> H is a subset H ′ <strong>of</strong> G such that there exists an a ∈ G such that<br />
(1) H ′ = aH = {ah | h ∈ H}, in which case H ′ is said to be a left coset; or (2) H ′ = Ha = {ha | h ∈ H}, in<br />
which case H ′ is said to be a right coset.<br />
Given a ∈ G, aH is not necessarily equal to Ha. However, one can show that the subgroup H <strong>of</strong> G is a normal<br />
subgroup if and only if aH = Ha for every a ∈ G.<br />
In what follows, only left cosets will be discussed, though similar statements may be made about right cosets.<br />
The left cosets <strong>of</strong> H are the equivalence classes <strong>of</strong> the equivalence relation ∼ defined by a ∼ b if there exists<br />
h ∈ H such that a = bh. Since equivalence classes form a partition, the left cosets <strong>of</strong> H partition G.<br />
The cardinality <strong>of</strong> the set <strong>of</strong> left cosets <strong>of</strong> H is called the index <strong>of</strong> H in G and is denoted by [G : H]. Given<br />
a ∈ G, h ↦→ ah defines a bijective map from H into aH. If G is finite, it follows that |G| = |H|[G : H], where<br />
|G| denotes the order <strong>of</strong> G. A very important result follows: if G is finite, then the order <strong>of</strong> H divides the order<br />
<strong>of</strong> G. Moreover, since the order <strong>of</strong> any element <strong>of</strong> G is the order <strong>of</strong> the cyclic subgroup it generates, if G is<br />
finite then the order <strong>of</strong> an element <strong>of</strong> G divides the order <strong>of</strong> G. These results follow from a special case <strong>of</strong> what<br />
is known as Lagrange’s Group Theorem: if G is a group, H is a subgroup <strong>of</strong> G and K is a sugroup <strong>of</strong> H, then<br />
[G : K] = [G : H][H : K], where the products are taken as products <strong>of</strong> cardinals.<br />
An important result that follows from Lagrange’s Theorem is that if the order <strong>of</strong> G is a prime number then<br />
G = 〈a〉 for any a ∈ G such that a is not the identity, where 〈a〉 denotes the cyclic group generated by a.<br />
Note that if ϕ: G → G ′ is a group [homomorphism], then [G : kerϕ] = |imϕ|. Thus another result <strong>of</strong> Langrange’s<br />
Theorem is that |G| = |kerϕ| · |imϕ|.
left coset<br />
Given a subgroup H <strong>of</strong> a group G, a [left coset] <strong>of</strong> H is a subset H ′ <strong>of</strong> G such that there exists an a ∈ G such<br />
that H ′ = aH = {ah | h ∈ H}.<br />
Given a ∈ G, aH is not necessarily equal to Ha. However, one can show that the subgroup H <strong>of</strong> G is a normal<br />
subgroup if and only if aH = Ha for every a ∈ G.<br />
In what follows, only left cosets will be discussed, though similar statements may be made about right cosets.<br />
The left cosets <strong>of</strong> H are the equivalence classes <strong>of</strong> the equivalence relation ∼ defined by a ∼ b if there exists<br />
h ∈ H such that a = bh. Since equivalence classes form a partition, the left cosets <strong>of</strong> H partition G.<br />
The cardinality <strong>of</strong> the set <strong>of</strong> left cosets <strong>of</strong> H is called the index <strong>of</strong> H in G and is denoted by [G : H]. Given<br />
a ∈ G, h ↦→ ah defines a bijective map from H into aH. If G is finite, it follows that |G| = |H|[G : H], where<br />
|G| denotes the order <strong>of</strong> G. A very important result follows: if G is finite, then the order <strong>of</strong> H divides the order<br />
<strong>of</strong> G. Moreover, since the order <strong>of</strong> any element <strong>of</strong> G is the order <strong>of</strong> the cyclic subgroup it generates, if G is<br />
finite then the order <strong>of</strong> an element <strong>of</strong> G divides the order <strong>of</strong> G. These results follow from a special case <strong>of</strong> what<br />
is known as Lagrange’s Group Theorem: if G is a group, H is a subgroup <strong>of</strong> G and K is a sugroup <strong>of</strong> H, then<br />
[G : K] = [G : H][H : K], where the products are taken as products <strong>of</strong> cardinals.<br />
An important result that follows from Lagrange’s Theorem is that if the order <strong>of</strong> G is a prime number then<br />
G = 〈a〉 for any a ∈ G such that a is not the identity, where 〈a〉 denotes the cyclic group generated by a.<br />
Note that if ϕ: G → G ′ is a group [homomorphism], then [G : ker(ϕ)] = |im(ϕ)|. Thus another result <strong>of</strong><br />
Langrange’s Theorem is that |G| = |ker(ϕ)| · |im(ϕ)|.<br />
right coset<br />
Given a subgroup H <strong>of</strong> a group G, a [right coset] <strong>of</strong> H is a subset H ′ <strong>of</strong> G such that there exists an a ∈ G such<br />
that H ′ = Ha = {ha | h ∈ H}.<br />
Given a ∈ G, aH is not necessarily equal to Ha. However, one can show that the subgroup H <strong>of</strong> G is a normal<br />
subgroup if and only if aH = Ha for every a ∈ G.<br />
In what follows, only left cosets will be discussed, though similar statements may be made about right cosets.<br />
The left cosets <strong>of</strong> H are the equivalence classes <strong>of</strong> the equivalence relation ∼ defined by a ∼ b if there exists<br />
h ∈ H such that a = bh. Since equivalence classes form a partition, the left cosets <strong>of</strong> H partition G.<br />
The cardinality <strong>of</strong> the set <strong>of</strong> left cosets <strong>of</strong> H is called the index <strong>of</strong> H in G and is denoted by [G : H]. Given<br />
a ∈ G, h ↦→ ah defines a bijective map from H into aH. If G is finite, it follows that |G| = |H|[G : H], where<br />
|G| denotes the order <strong>of</strong> G. A very important result follows: if G is finite, then the order <strong>of</strong> H divides the order<br />
<strong>of</strong> G. Moreover, since the order <strong>of</strong> any element <strong>of</strong> G is the order <strong>of</strong> the cyclic subgroup it generates, if G is<br />
finite then the order <strong>of</strong> an element <strong>of</strong> G divides the order <strong>of</strong> G. These results follow from a special case <strong>of</strong> what<br />
is known as Lagrange’s Group Theorem: if G is a group, H is a subgroup <strong>of</strong> G and K is a sugroup <strong>of</strong> H, then<br />
[G : K] = [G : H][H : K], where the products are taken as products <strong>of</strong> cardinals.<br />
An important result that follows from Lagrange’s Theorem is that if the order <strong>of</strong> G is a prime number then<br />
G = 〈a〉 for any a ∈ G such that a is not the identity, where 〈a〉 denotes the cyclic group generated by a.<br />
Note that if ϕ: G → G ′ is a group homomorphism, then [G : ke(ϕ)] = |im(ϕ)|. Thus another result <strong>of</strong><br />
Langrange’s Theorem is that |G| = |ker(ϕ)| · |im(ϕ)|.<br />
index<br />
The [index] <strong>of</strong> subgroup H <strong>of</strong> a group G is the cardinality <strong>of</strong> the set <strong>of</strong> left cosets <strong>of</strong> H in G. The index <strong>of</strong> H<br />
in G is denoted [G : H].
quotient group<br />
Given a group G and a normal subgroup N <strong>of</strong> G, the [quotient group] <strong>of</strong> N in G, written G/N and read<br />
“G mod(ulo) N”, is the set <strong>of</strong> cosets <strong>of</strong> N in G, under the law <strong>of</strong> composition that is defined as follows:<br />
(aN)(bN) = abN, where xN = {xn | n ∈ N}. Note that since N is normal, aN = Na for all a ∈ G, so it is not<br />
necessary to define this law <strong>of</strong> composition in terms <strong>of</strong> left cosets instead <strong>of</strong> right cosets.<br />
The order <strong>of</strong> G/N is the index [G : N] <strong>of</strong> N in G.<br />
Quotient groups can be identified by the First Isomorphism Theorem: if ϕ: G → G ′ is a surjective group<br />
homomorphism and if N = ke(ϕ) then ψ: G/N → G ′ is an isomorphism, where ψ is defined by ψ(aN) = ϕ(a).<br />
First Isomorphism Theorem<br />
The [First Isomorphism Theorem]. Suppose ϕ: G → G ′ is a surjective group homomorphism, and let N denote<br />
the kernel <strong>of</strong> ϕ. Then the quotient group G/N is isomorphic to G ′ by the map ψ defined by ψ(aN) = ϕ(a).<br />
The First Isomorphism Theorem is the principle method <strong>of</strong> identifying quotient groups. As an example, consider<br />
the group homomorphism ϕ from C × , the nonzero complex numbers under multiplication, into R × , the nonzero<br />
real numbers under multiplication, defined by ϕ(z) = |z|, where |z| denotes the absolute value <strong>of</strong> z. The kernel<br />
<strong>of</strong> ϕ is the unit circle, U, and the image <strong>of</strong> ϕ is the group <strong>of</strong> positive real numbers. So C × /U is isomorphic to<br />
the multiplicative group <strong>of</strong> positive real numbers.<br />
operation<br />
Given a group G and a set S, an [operation] <strong>of</strong> a G on S is a map from G × S into S - <strong>of</strong>ten written using<br />
multiplicative notation: (g, s) ↦→ gs - satisfying:<br />
• 1s = s for all s ∈ S, where 1 is the identity <strong>of</strong> G; and<br />
• (gg ′ )s = g(g ′ s), for all g, g ′ ∈ G and for all s ∈ S.<br />
There are some terms that are sometimes associated with a group operation: S is <strong>of</strong>ten called a G-set; G is<br />
sometimes called a transformation group; and the group operation is <strong>of</strong>ten also called a group action.<br />
Mathworld: ”Historically, the first group action studied was the action <strong>of</strong> the Galois group on the roots <strong>of</strong><br />
a polynomial. However, there are numerous examples and applications <strong>of</strong> group actions in many branches<br />
<strong>of</strong> mathematics, including algebra, topology, geometry, number theory, and analysis, as well as the sciences,<br />
including chemistry and physics.”<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 44 entries in this file.
Index<br />
abelian, 3<br />
alternating group, 5<br />
associative, 2<br />
automorphism, 8<br />
binary operation, 2<br />
cancellation Law, 4<br />
center, 9<br />
commutative, 3<br />
conjugation, 9<br />
coset, 9<br />
cyclic group, 7<br />
even permutation, 5<br />
First Isomorphism Theorem, 11<br />
general linear group, 2<br />
group, 1<br />
Group theory, 1<br />
identity, 2<br />
image, 8<br />
index, 10<br />
isomorphic, 8<br />
isomorphism, 8<br />
kernel, 8<br />
law <strong>of</strong> composition, 1<br />
left coset, 10<br />
nontrivial, 3<br />
odd permutation, 5<br />
operation, 11<br />
order, 6<br />
permutation, 4<br />
proper subgroup, 6<br />
quotient group, 11<br />
right coset, 10<br />
sign, 5<br />
sign map, 5<br />
simple group, 6<br />
special linear group, 3<br />
subgroup, 6<br />
symmetric group, 5<br />
transposition, 4<br />
trivial, 3<br />
12
<strong>ENTRY</strong> HARVARD<br />
[<strong>ENTRY</strong> HARVARD] Authors: Oliver Knill: 2000, Literature: no<br />
[Harvard]<br />
Harvard<br />
Science center<br />
[Science center] The science center is the Polaroid camera shape building near Harvard square. The actual<br />
building is close to Memorial Hall. I actually live and think in the science center. You can virtually walk into<br />
the science center<br />
president <strong>of</strong> Harvard<br />
[president <strong>of</strong> Harvard] The President <strong>of</strong> Harvard is currently Lawrence H. Summers. To find out more about<br />
him, visit the website<br />
chairman <strong>of</strong> math department<br />
[chairman <strong>of</strong> math department] The chairman <strong>of</strong> the <strong>Mathematics</strong> department is currently Joe Harris.<br />
number people math department<br />
[number people math department] Currently, there are over 190 people at the Math department.<br />
preceptor<br />
[preceptor] Preceptors work alongside other faculty on teaching, developing and supporting sections <strong>of</strong> entry<br />
level courses at the Harvard <strong>Mathematics</strong> department.<br />
ca<br />
[ca] A course assistant (CA) is an undergraduate student who assists the teaching fellow (TF) with grading,<br />
running problem sessions and tutoring in the question center.
tf<br />
[tf] TF stands for teaching fellow. Everybody who is teaching is called a TF. It can be a senior or junior faculty,<br />
a visiting fellow or a graduate student.<br />
concentrator<br />
[concentrator] A (math) concentrator is a sophomore or senior undergraduate student. A math concentrator<br />
would also be called a math major. There are about one hundred math concentrators. Each year, there are<br />
about 30 new concentrators.<br />
head tutor<br />
[head tutor] The head tutor is a pr<strong>of</strong>essor who is the chief undergraduate advisor.<br />
question center<br />
[question center] The question center QC is a place to work on homework problems or exam preparation. Tutors<br />
(both course assistants or teaching fellows) are available for questions.<br />
[qc] see question center<br />
qc<br />
math table<br />
[math table] The math table is a ”dinner seminar” which takes place in one <strong>of</strong> the student houses. A faculty or<br />
student presents a half an hour talk just after a dinner.<br />
grade<br />
[grade] Grades are an important issue for most students. Unfortunately, I have no access to your grades.<br />
where harvard<br />
[where harvard] Harvard University is located in Cambridge, Massachusetts USA. We are on the east cost. One<br />
can see from here Boston. The Campus is quite close to the Charles River. To look up something specific, it is<br />
best to start online with the Harvard search page.
get into Harvard<br />
[get into Harvard] Work hard, have lots <strong>of</strong> interests. You need <strong>of</strong> course some luck.<br />
life at Harvard<br />
[life at Harvard] Fun. Beside a great academic environment, there are a lot <strong>of</strong> things to see. You can spend<br />
weeks at Harvard square and still find new things.<br />
grade inflation<br />
[grade inflation] Grade inflation is when most students get A’s. One <strong>of</strong> the problems with grade inflation is that<br />
grades start losing their purpose.<br />
computer type<br />
[computer type] At the <strong>Mathematics</strong> department, people use all kind <strong>of</strong> operating systems<br />
• Sun work stations running Solaris<br />
• Macintoshs running OSX<br />
• PC’s running Linux<br />
• PC’s running Windows.<br />
s<strong>of</strong>tware<br />
[s<strong>of</strong>tware] Have a look at http://www.math.harvard.edu/computing.<br />
mathematics<br />
[mathematics] <strong>Mathematics</strong> is both a science and an art. It is also a language for other sciences. Quite many<br />
topics in <strong>Mathematics</strong> have turned out to be useful. Examples is the theory <strong>of</strong> operators which provided the<br />
framework for Quantum mechanics. An other example is number theory which provides the foundation for<br />
many encryption algorithms.<br />
afread <strong>of</strong> math<br />
[afread <strong>of</strong> math] You probably had some bad experiences in the past. You should chat more with me!
learn math<br />
[learn math] Just do it! There are hundreds <strong>of</strong> nice books about Math, many resources on the internet. Take a<br />
math class with a good teacher.<br />
physics and math<br />
[physics and math] There are not many differences. Indeed, there are branches <strong>of</strong> <strong>Mathematics</strong> like computational<br />
number theory where people do a lot <strong>of</strong> experiments and there are branches <strong>of</strong> physics, where people do<br />
very abstract theory which presumably never can be tested in laboratories.<br />
[charles river] A great place to row, run bike and relax.<br />
[harvard yard] the center <strong>of</strong> the Harvard campus<br />
charles river<br />
harvard yard<br />
math pr<strong>of</strong>essors<br />
[math pr<strong>of</strong>essors] They are all excellent Mathematicians.<br />
[pi day]<br />
pi day<br />
student number<br />
[student number] There are more than 18’000 degree candidates at Harvard.<br />
Harvard founded<br />
[Harvard founded] Harvard College was established in 1636, already 16 years after the arrival <strong>of</strong> the pilgrims at<br />
Plymouth.
people at harvard<br />
[people at harvard] There are over 14’000 people at Harvard including more than 2’000 faculty. There are also<br />
7,000 faculty appointments in affiliated teaching hospitals.<br />
Nobel Laureates<br />
[Nobel Laureates] Harvard produced nearly 40 Nobel Laureates.<br />
US presidents<br />
[US presidents] Harvard produced seven presidents <strong>of</strong> the United States: John Adams, John Quincy Adams,<br />
Theodore and Franklin Delano Roosevelt, Rutherford B. Hayes, John Fitzgerald Kennedy and George W. Bush.<br />
[Millenium prize problems]<br />
• P versus NP<br />
• Hodge Conjecture<br />
• Poincare Conjecture<br />
• Riemann Hypothesis<br />
• Yang-Mills Existence and Mass Gap<br />
• Navier-Stokes Existence and Smoothness<br />
• Birch-Swinnerton-Dyer Conjecture<br />
Millenium prize problems<br />
Core course<br />
[Core course] In 1978, Harvard adopted a ’core’ <strong>of</strong> courses in fields <strong>of</strong> inquiry that spanned domains, including<br />
historical study, moral reasoning, social analysis, science, music and art, literature and so on. These courses are<br />
designed to introduce ’approaches to knowledge’ rather than specific information and thus legitimized a trend<br />
throughout education toward ways <strong>of</strong> knowing rather than knowledge.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 35 entries in this file.
Index<br />
afread <strong>of</strong> math, 3<br />
ca, 1<br />
chairman <strong>of</strong> math department, 1<br />
charles river, 4<br />
computer type, 3<br />
concentrator, 2<br />
Core course, 5<br />
get into Harvard, 3<br />
grade, 2<br />
grade inflation, 3<br />
Harvard, 1<br />
Harvard founded, 4<br />
harvard yard, 4<br />
head tutor, 2<br />
learn math, 4<br />
life at Harvard, 3<br />
math pr<strong>of</strong>essors, 4<br />
math table, 2<br />
mathematics, 3<br />
Millenium prize problems, 5<br />
Nobel Laureates, 5<br />
number people math department, 1<br />
people at harvard, 5<br />
physics and math, 4<br />
pi day, 4<br />
preceptor, 1<br />
president <strong>of</strong> Harvard, 1<br />
qc, 2<br />
question center, 2<br />
Science center, 1<br />
s<strong>of</strong>tware, 3<br />
student number, 4<br />
tf, 2<br />
US presidents, 5<br />
where harvard, 2<br />
6
<strong>ENTRY</strong> JOKES<br />
[<strong>ENTRY</strong> JOKES] Authors: Oliver Knill: 2002 Literature: not yet<br />
JOKE GARAGE SALE<br />
[JOKE GARAGE SALE] Pride is what you feel when your kids net 143 dollars from a garage sale. Panic is<br />
what you feel when you realize your car is missing.<br />
JOKE DOORBELL<br />
[JOKE DOORBELL] A priest was walking down the street when he saw a little boy jumping up and down to<br />
try to reach a doorbell. So the priest walked over and pressed the button for the youngster. ”And now what,<br />
my little man?” he asked. ”Now.” said the boy, ”run like hell!”<br />
[JOKE FAMOUS LAST WORDS]<br />
JOKE FAMOUS LAST WORDS<br />
postman: ”good doggy, nice doggy”<br />
butcher: ”could you throw me the big knife, please?”<br />
computer: ”are you sure? (yes/no)”<br />
stuntman: ”what? reality TV?”<br />
doorman: ”only over my dead body”<br />
detective” ”clear case: you are the murderer”<br />
muchroom picker: ”I never saw this one”<br />
boss: ”nice present, a lighter which looks like a revolver”<br />
submarine crew: ”I need some fresh air, open the window”<br />
sysadmin: ”I recently had a fresh backup”<br />
student: ”I’m going to eat in the mensa, anybody coming?”<br />
bungee jumper: ”hurrey!”<br />
PC: ”loading windows - please wait”<br />
JOKE PAINT JOB<br />
[JOKE PAINT JOB] There was a college student trying to earn some pocket money by going from house to<br />
house <strong>of</strong>fering to do odd jobs. He explained this to a man who answered one door. ”How much will you charge<br />
to paint my porch?” asked the man. ”Forty dollars.” ”Fine” said the man, and gave the student the paint<br />
and brushes. Three hours later the paint-splattered lad knocked on the door again. ”All done!”, he says, and<br />
collects his money. ”By the way,” the student says, ”That’s not a Porsche, it’s a Ferrari.”<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 4 entries in this file.
Index<br />
JOKE DOORBELL, 1<br />
JOKE FAMOUS LAST WORDS, 1<br />
JOKE GARAGE SALE, 1<br />
JOKE PAINT JOB, 1<br />
2
<strong>ENTRY</strong> K12<br />
[<strong>ENTRY</strong> K12] Authors: Oliver Knill: 2000 Literature: not yet<br />
abacus<br />
An [abacus] is an acient mechanical computing device. It is made <strong>of</strong> beads arranged on a frame.<br />
absolute value<br />
The [absolute value] |n| <strong>of</strong> a real number n is the maximum <strong>of</strong> n and its negative −n. For example, the absolute<br />
value <strong>of</strong> −6 is | − 6| = 6. The absolute value is the distance from 0.<br />
adjacent angles<br />
Two angles that share a ray are called [adjacent angles].<br />
affine cipher<br />
An [affine cipher] uses affine functions to scramble the letters in an alphabet <strong>of</strong> a secret message. For<br />
example, with an alphabet <strong>of</strong> 26 letters, f(x) = bx + a = 5x + 2mod(26) produces a new alphabet <strong>of</strong><br />
the same size if b has no common multiple with 26. The simplest example is the Caesar cipher, where<br />
b = 2. It rotates the letters in an alphabet x ↦→ x + amod(26). For example, for a = 1, we get<br />
a b c d e f g h i j k l m n o p q r s t u v w x y z<br />
This ci-<br />
b c d e f g h i j k l m n o p q r s t u v w x y z a<br />
pher changes the word hello to the word ifmmp. A requently used Caesar cipher is ”rot13” defined by<br />
f(x) = x + 13mod(13). It has the property that encryption and decryption are the same. For example, applying<br />
rot13 on the word ”decryption” produces qrpelcgvba and applying rot13 on that word again gives back<br />
”decryption. More complicated versions <strong>of</strong> affine cyphers can be obtained by writing the to encoded text as a<br />
sequence <strong>of</strong> vectors x and then applying Ax + b on each vector. Affine cyphers are very easy to crack. They are<br />
only used to illustrate the concept like for educational purposes.<br />
algebra<br />
[algebra] is a branch <strong>of</strong> elementary mathematics that generalizes arithmetic by using variables. An example <strong>of</strong><br />
an algebraic identity is x ∗ (y + z) = x ∗ y + x ∗ z.<br />
acute<br />
An angle is called [acute], if is smaller than 90 degrees. An angle which is 90 degrees is called a right angle.
addition<br />
[addition] is a basic operation for numbers. The result is called the sum <strong>of</strong> the two numbers. Examples: 5+3 = 8.<br />
2 3 4 5<br />
+ 9 2 3 5<br />
1 1 5 8 0<br />
More generally, a group operation in a commutative group is <strong>of</strong>ten called addition. Examples <strong>of</strong> groups are<br />
integers, real numbers, vectors or matrices.<br />
alternate exterior angles<br />
[alternate exterior angles] are angles located outside a set <strong>of</strong> two parallel lines and on opposite sides <strong>of</strong> the<br />
transversal line. They are equal.<br />
alternate interior angles<br />
[alternate interior angles] are angles located inside a set <strong>of</strong> parallel lines and on opposite sides <strong>of</strong> the transversal.<br />
angle bisector<br />
A ray that divides an angle into two equal angles is called an [angle bisector]. The bisector can be constructed<br />
with ruler and compass. An angle trisector on the other hand, a ray which splits an angle into three equal parts<br />
can not be constructed by ruler and compass.<br />
apex<br />
The [apex] is the highest vertex in a given orientation <strong>of</strong> a polygon.<br />
Arabic numerals<br />
[Arabic numerals]: symbols 0, 1, 2, 3, 4, 5, 6, 7, 8, 9 that represent successive entries <strong>of</strong> words representing numbers<br />
in the decimal system. For example, 2347 is the number 2000 + 300 + 40 + 7.<br />
area<br />
The [area] <strong>of</strong> a surface is a measure for the number <strong>of</strong> square units needed to cover the surface. For example,<br />
the sphere <strong>of</strong> radius 1 has the surface area 4π.
arithmetic mean<br />
[arithmetic mean] Given two numbers a, b, the arithmetic mean is defined as (a + b)/2. It is sometimes also<br />
called the mean. Other means are the geometric mean √ ab or the harmonic mean 1/(1/a + 1/b).<br />
average<br />
The [average] <strong>of</strong> a few numbers is the sum <strong>of</strong> all the numbers divided by the number <strong>of</strong> numbers. For example,<br />
the average <strong>of</strong> 2, 4, 6 is (2 + 4 + 6)/3 = 4, the average <strong>of</strong> the numbers 1, 5, 8, 4 is (1+5+8+5)/3 = 19/3 The<br />
average is also called the mean. The average <strong>of</strong> two numbers is also called the arithmetic mean.<br />
base<br />
A [base] is the number <strong>of</strong> distinct single-digit numbers in a counting system. Example: the binary system<br />
has base 2. The decimal system has base 10. The base is also called radix. Numbers can be represented<br />
in any base r > 1. Because humans have 10 fingers, the decimal system is the one favoured by this species.<br />
Because computers work with circuits which are based on the principle ”on” or ”<strong>of</strong>f”, they like the base 2. The<br />
hexadecimal system (base 16) or octal system (base 8) are also used a lot by computers. Modern computers<br />
can even work directly with numbers written in base 32 or 64.<br />
bell curve<br />
The [bell curve] is an other term for graph <strong>of</strong> the normal distribution f(x) = 1 √ e π −x2.<br />
It is also called the Gauss<br />
distribution. The bell curve is <strong>of</strong>ten seen in probability distributions. There is a reason for that called the<br />
central limit theorem which assures that if we average independent data with some distribution, we approach<br />
the normal distribution.<br />
billion<br />
A [billion] is one thousand millions in the American or French system, it is a million millions in the English or<br />
German system. In other words<br />
One billion in UK,Germany: 10 12 1’000’000’000’000<br />
One billion in US,France: 10 9 1’000’000’000<br />
binary number<br />
A [binary number] is a number expressed in place-value notation to the base 2. For example: 101101 represents<br />
the decimal number 1 + 0 + 4 + 8 + 0 + 32 = 45.<br />
cipher<br />
[cipher] Ciphers are codes used to encrypt ”secret” messages.
coefficient<br />
The word [coefficient] is used to denote numbers in the front <strong>of</strong> the variables in an algebraic formula. For<br />
example: 4x + 5y = 3 has coefficients 4, 5.<br />
combinatorics<br />
[combinatorics] The science <strong>of</strong> counting things. Combinatorics is an important part <strong>of</strong> probability and statistics.<br />
common factor<br />
A [common factor] <strong>of</strong> two integers n and m is a number which is a factor <strong>of</strong> both. A common factor is also<br />
called a common divisor. Examples: 3 is a common factor <strong>of</strong> 18 and 27. Also, 9 is the greatest common factor<br />
<strong>of</strong> 18 and 27: we write 9 = gcd(18, 27), where gcd stands for the greatest common divisor.<br />
complex numbers<br />
[complex numbers] can be written as a pair <strong>of</strong> real numbers z = x+iy, where i is a symbol which satisfies i 2 = −1.<br />
One can add and subtract complex numbers by adding their coefficients x, y. For example 4+5i+5−7i = 9−2i.<br />
complementary angles<br />
Two angles whose sum is 90 degrees form [complementary angles]. For example, the two non-right angles in a<br />
right triangle form complementary angles.<br />
concave up<br />
A graph <strong>of</strong> a function f is [concave up] if f has the property f((x + y)/2) ≤ (f(x) + f(y))/2. If f is concave<br />
up, then −f is concave down. For example, the graph <strong>of</strong> the function f(x) = x 2 is concave up, the graph <strong>of</strong> the<br />
function f(x) = −x 4 is concave down.<br />
conditional probability<br />
The [conditional probability] is the probability that an event A happens provided a second event B occurs.<br />
One writes P [A|B]. It satisfies P [A|B] = P [A ∩ B]/P [B], where P [B] is the probability <strong>of</strong> the event B and<br />
P [A ∩ B] probability <strong>of</strong> the intersection <strong>of</strong> A and B. For example, if we throw 2 coins and we know one <strong>of</strong><br />
the coins is head H, then the probability that the there is also a coin with tail is 2/3. Pro<strong>of</strong>: The probability<br />
space is X = {HT, T H, T T, HH}. The event that one <strong>of</strong> the coins is head is A = {HT, T H, HH}. The event<br />
B that one <strong>of</strong> the coins shows tail is B = {HT, T H, T T }. The intersection <strong>of</strong> B and A is {T H, HT }. We have<br />
P [B|A] = P [B ∩ A]/P [A] = (1/2)/(3/4) = 2/3.
congruent<br />
Two figures are called [congruent] if one can move one to an other by translation and rotation.<br />
constant<br />
A quantity that does not change in an equation is called a [constant].<br />
constant function<br />
A [constant function] is a function which takes the same value whatever input we enter to it.<br />
coordinate<br />
A [coordinate] is an entry in a collection <strong>of</strong> numbers identifiing the point in coordinate space.<br />
continuous graph<br />
The graph <strong>of</strong> a continuous function is called a [continuous graph]. Roughly speaking, a graph <strong>of</strong> a function<br />
defined on some interval [a, b] is a continuous graph if one can draw the graph using a pencil without having to<br />
the lift the pencil. Examples:<br />
• 1/x is not continuous on [−1, 1].<br />
• x 2 + 1 is continuous on [−1, 1].<br />
• 1/x 2 is not continuous on [−1, 1].<br />
• sin(1/x) is not continuous on [−1, 1].<br />
• x sin(1/x) is continuous on [−1, 1].<br />
• f ′ (x) is not continuous on [−1, 1] if f(x) = |x|.<br />
corresponding angles<br />
[corresponding angles] are two angles in the same relative position on two straight lines when those lines are<br />
intersected by a a transversal straight line.<br />
decimal number<br />
[decimal number] is a fraction, where the denominator is a power <strong>of</strong> 10. It can be expressed using a decimal<br />
point. For example: 0.872 is the decimal equivalent <strong>of</strong> 872/1000.
degrees<br />
An angle is <strong>of</strong>ten measured in [degrees]. The entire circle has 360 degrees, a half a circle is 180 degrees, a quarter<br />
circle is a right angle and has 90 degrees. A more natural unit is the length unit where the entire circle has<br />
angle 2π and the right angle is the angle π/2.<br />
denominator<br />
The [denominator] is the integer q below the fraction in a rational number p/q. The other number p is called<br />
the nominator.<br />
discontinuous graph<br />
A [discontinuous graph] is the graph <strong>of</strong> a function which is not continuous. Discontinuities can occur in different<br />
ways. The function can jump from one value to an other. The function can also be infinite at some point or<br />
the function can oscillate infinitely much at some point. Examples:<br />
• The graph <strong>of</strong> the function f(x) = 1/x on [−1, 1].<br />
• The graph <strong>of</strong> the function f(x) = sin(1/x) on [−1, 1].<br />
• The graph <strong>of</strong> the function f(x) = sign(x), which is 1 for x > 0 equal to 0 for x = 0 and −1 for x = −1.<br />
disjoint events<br />
Two events are called [disjoint events] if they have no common elements.<br />
division<br />
The inverse operation <strong>of</strong> multiplication is called [division].<br />
domain<br />
The [domain] <strong>of</strong> a function f is the set <strong>of</strong> numbers x for which f(x) is defined. For example, the domain <strong>of</strong> the<br />
function f(x) = 1/x is the entire real line except the point 0.<br />
element<br />
An [element] <strong>of</strong> a set is is a member <strong>of</strong> that set. For example table is an element <strong>of</strong> the set {table, chair, floor}.
empty set<br />
The [empty set] ∅ is the set which does not contain any elements.<br />
equally likely<br />
If two events have the same probability they are called [equally likely]. For example, the event <strong>of</strong> throwing an<br />
even number with one dice is equally likely than throwing an odd number.<br />
event<br />
An [event] is a subset <strong>of</strong> the entire probability space. For example, if X = {HH, HT, T H, T T } is the probability<br />
space <strong>of</strong> all throwing <strong>of</strong> two coins, then A = {HH, HT } is the event that in the second throw one had a head.<br />
exponent<br />
The [exponent] <strong>of</strong> an expression a x is part x. One can get the exponent <strong>of</strong> y = a x by the formula x =<br />
log(y)/ log(a).<br />
Fibonacci numbers<br />
[Fibonacci numbers] are numbers obtained in the Fibonacci sequence defined by starting the numbers 0, 1 and<br />
defining the next element as the sum <strong>of</strong> the two previous ones: 0, 1, 1, 2, 3, 5, 8, 13, 21, 34, .... The sequence is<br />
named after Leonardo <strong>of</strong> Pisa, who called himself Fibonacci, short for Filius Bonacci (= Son <strong>of</strong> Bonacci). The<br />
original problem he investigated in 1202 A.D. was the growth <strong>of</strong> rabbits. Explicit expressions for the n’th term<br />
<strong>of</strong> the sequence can be obtained using linear algebra. More generally, one can find explicit formulas for the n’th<br />
term in a linear recursion <strong>of</strong> the form an+1 = � k<br />
j=0 cjan−j.<br />
fractal<br />
A [fractal] is a set which has non-integer dimension. The term was coined by Benoit Mandelbrot in 1975. Many<br />
objects in nature appear to be fractals, like coast lines, trees, mountains. One can mathematically define fractals<br />
using iterative constructions. Examples are the Koch curve, the snow flake, the Menger Sponge, the Shirpinsky<br />
carpet, the Cantor set.<br />
fraction<br />
A [fraction] is a rational number written in the form a/b, where a is called the numerator and b is called the<br />
denominator.
function<br />
A [function] f <strong>of</strong> a variable x is a rule that assigns to each number x in the function’s domain a single number<br />
f(x). For example f(x) = x 2 is a function which assigns to each number its square like f(4) = 16.<br />
geometric sequence<br />
The [geometric sequence] is a sequence where each element is a multiple <strong>of</strong> the previous element. For example:<br />
1, 2, 4, 8, 16, 32, 64, ... is a geometric sequence.<br />
graph <strong>of</strong> the function<br />
The [graph <strong>of</strong> the function] is the set <strong>of</strong> all points (x, f(x)) in the plane, where x in the domain <strong>of</strong> f.<br />
greatest common factor<br />
The [greatest common factor] <strong>of</strong> two numbers n,m is the larest common factor <strong>of</strong> both. One denotes the greatest<br />
common factor with ”gcd”. Examples:<br />
6 is the greatest common factor <strong>of</strong> 12 and 18 6=gcd(12,18)<br />
8 is the greatest common factor <strong>of</strong> 8 and 80. 8=gcd(8,80)<br />
1 is the greatest common factor <strong>of</strong> 7 and 11 1=gcd(7,11)<br />
[greatest common divisor] see greatest common factor.<br />
greatest common divisor<br />
histogram<br />
A [histogram] is a bar graph in which area over each range <strong>of</strong> values is proportional to the relative frequency <strong>of</strong><br />
the data in this interval.<br />
hypotenuse<br />
The [hypotenuse] <strong>of</strong> a right triangle is the opposite side to the right angle.<br />
independent events<br />
Two events A and B are called [independent events] if the probability that both happen is the product <strong>of</strong> the<br />
probabilities that each occurs alone: P [A ∩ B] = P (A)P (B). Using conditional probability one can write this<br />
as P [A|B] = P [A]. Knowing A under the condition B is the same as knowing A without knowing B.
infinity<br />
[infinity] is a ”number” which is larger than any other number. One writes ∞. One should rather treat <strong>of</strong> it as a<br />
symbol evenso some computations can be extended to the real numbers including ∞ like ∞ + x = ∞, ∞ + ∞ =<br />
∞, x ∗ ∞ = ∞ for x > 0, x ∗ ∞ = −∞ for x < 0 or ∞ ∗ ∞ = ∞, (−∞) ∗ ∞ = −∞. One can not define ∞ − ∞<br />
in a consistent way nor can one do that with 0 ∗ ∞. Also the expression 1/0 = ∞ is ill defined because 1/x<br />
takes near x = 0 arbitrary large and arbitrary small values.<br />
integer<br />
An [integer] is a number <strong>of</strong> the form n or −n, where n is a natural number. Examples <strong>of</strong> integers are ... −<br />
3, 2, 1, 0, 1, 2, 3, 4.... The fraction 2/5 is not an integer.<br />
intersection<br />
The [intersection] <strong>of</strong> two or more sets is the set <strong>of</strong> elements which are in both sets. One writes A ∩ B for the<br />
intersection <strong>of</strong> A and B.<br />
isosceles triangle<br />
An [isosceles triangle] is a triangle which has at least two congruent sides. A special case is the isocline triangle<br />
in which all sides are congruent.<br />
least common multiple<br />
The [least common multiple] <strong>of</strong> two numbers n, m is the least common multiple <strong>of</strong> both. One denotes the least<br />
common multiple with ”lcm”. Examples:<br />
18 is the least common multiple <strong>of</strong> 9 and 6 18=lcm(9,6)<br />
77 is the least common multiple <strong>of</strong> 7 and 11 77=gcd(7,11)<br />
limit<br />
The [limit] <strong>of</strong> a sequence <strong>of</strong> numbers is the limiting value the sequence converges to. It needs not to exist. For<br />
example, the sequence an = 1/n converges to 0. One sais that 0 is the limit <strong>of</strong> that sequence. The sequence<br />
an = n has no finite limit. One could assign infinity as a limit. The sequence 1, −1, 1, −1, 1, −1, ... has no limit.<br />
logarithm<br />
The [logarithm] <strong>of</strong> b is the exponent to which one has to rize a base number to get b. For example, 2 is the<br />
logarithm <strong>of</strong> 100 to the base 10 or 10 is the logarithm <strong>of</strong> 1024 to the base 2.
mean<br />
The [mean] <strong>of</strong> a list <strong>of</strong> numbers is their sum divided by the total number <strong>of</strong> members in the list. It is also called<br />
arithmetic mean.<br />
median<br />
The [median] is the ”middle value” <strong>of</strong> a list. If the list has an odd number 2m + 1 elements, the median is the<br />
number in the list such that m scores are smaller or equal and m scores are bigger or equal. If the list has an<br />
even number <strong>of</strong> elements, one usually takes the algebraic average between the middle to elements Examples:<br />
med(1, 1, 2, 2) = 3/2, med(1, 2, 3, 4, 7) = 3, med(1, 2, 3, 4, 5, 6) = 7/2.<br />
multiplication table<br />
[multiplication table] A table <strong>of</strong> products <strong>of</strong> numbers which has to be memorized.<br />
1 2 3 4 5 6 7 8 9 10<br />
1 1 2 3 4 5 6 7 8 9 10<br />
2 2 4 6 8 10 12 14 16 18 20<br />
3 3 6 9 12 15 18 21 24 27 30<br />
4 4 8 12 16 20 24 28 32 36 40<br />
5 5 10 15 20 25 30 35 40 45 50<br />
6 6 12 18 24 30 36 42 48 54 60<br />
7 7 14 21 28 35 42 49 56 63 70<br />
8 8 16 24 32 40 48 56 64 72 80<br />
9 9 18 27 36 45 54 63 72 81 90<br />
10 10 20 30 40 50 60 70 80 90 100<br />
The diagonal contains squares. All numbers between 11 and 99 which do not appear in this table are prime<br />
numbers, numbers only divisible by 1 and itself.<br />
obtuse angle<br />
An angle whose measure is greater than 90 degrees is called an [obtuse angle].<br />
optical illusion<br />
An [optical illusion] is a drawing <strong>of</strong> an object that makes certain things appear which it does not have.<br />
palindrome<br />
A [palindrome] is a word or number that is the same when read backwards. Examples: ”otto”, ”anna”, ”racecar”,<br />
”78777787”.
paradox<br />
A [paradox] is a statement that appears to contradict itself. For example, the statement ”I always lie” is a<br />
paradox. If I tell the truth, then I lie, if I lie, then I tell the truth.<br />
Two lines which do not intersect are called [parallel].<br />
parallel<br />
parallelogram<br />
A [parallelogram] is a quadrilateral that contains two pairs <strong>of</strong> parallel sides.<br />
pattern<br />
A [pattern] is a characteristic observed in one item that may be repeated in other items. For example, the<br />
sequence 3, 4, 5, 4, 3, 4, 5, 4, 3, 4, 5, 4, 3, ... has a pattern which is also visible in a similar way in the sequence<br />
1, 3, 4, 3, 1, 3, 4, 3, 1, 3, 4, 3, 1, ....<br />
percent<br />
A [percent] is one hunderth. The symbol for percent is %. For example 0.1 is 10 percent. 2 is two hundred<br />
percent.<br />
perimeter<br />
The [perimeter] <strong>of</strong> a polygon is the sum <strong>of</strong> the lengths <strong>of</strong> all the sides <strong>of</strong> the polygon.<br />
permutation<br />
A [permutation] is a rearrangement <strong>of</strong> objects in a set. There are for example 6 permutations <strong>of</strong> the set<br />
A = (a, b, c). They are (a, b, c), (a, c, b), (b, a, c), (b, c, a), (c, a, b), (c, b, a).<br />
polygon<br />
A [polygon] is a closed plane figure formed by connecting a finite set <strong>of</strong> points in such a way that they do not<br />
cross each other.
polyhedra<br />
[polyhedra] A solid figure for which the outer surface is composed <strong>of</strong> polygons.<br />
prime number<br />
A [prime number] is a number which is divisible only by 1 and itself. The first prime numbers are<br />
2, 3, 5, 7, 11, 13, 17, 19, 23, 29, 31, 37.... The number 33 for example is no prime number because it is divisible<br />
by 3.<br />
quadrant<br />
A [quadrant] is one <strong>of</strong> the regions in the plane obtained when cutting the plane along the coordinate axes.<br />
• The first quadrant contains all the points with positive x and positive y coordinates.<br />
• The second quadrant contains all the points with negative x and positive y coordinates.<br />
• The third quadrant contains all the points with negative x and negative y coordinates.<br />
• The fourth quadrant contains all the points with positive x and negative y coordinates.<br />
quadratic function<br />
A function <strong>of</strong> the form f(x) = ax 2 + bx + c is called a [quadratic function]. For example f(x) = x 2 + 2 is a<br />
quadratic function. The graph <strong>of</strong> a quadratic function is a parabola if a is not zero. If a is zero it is a linear<br />
function which has as the graph a line.<br />
quotient<br />
The [quotient] <strong>of</strong> two numbers n and m is the largest integer smaller or equal to n/m. for example the quotient<br />
<strong>of</strong> 11 and 4 is 2 with areminder <strong>of</strong> 3.<br />
[smallest common multiple] see least common multiple.<br />
smallest common multiple
subtraction<br />
[subtraction] is a basic operation for numbers. Examples: 5 − 3 = 2.<br />
2 3 5 2<br />
- 1 4 5 6<br />
8 9 6<br />
More generally in any commutative group, the addition <strong>of</strong> the inverse -b <strong>of</strong> an element b to an element a,<br />
denoted by a-b is called a subtraction.<br />
multiplication<br />
[multiplication] is a basic operation for numbers. Example: 4 ∗ 5 = 20.<br />
1 2 4 x 1 2 3 3 4<br />
+ 4 9 3 3 6<br />
+ 2 4 6 6 8<br />
+ 1 2 3 3 4<br />
1 5 2 9 4 1 6<br />
More generally, in any group the group operation is called multiplication. Example: The composition <strong>of</strong> two<br />
transformations in the plane is a multiplication, matrix multiplication is a multiplication.<br />
fraction<br />
[fraction]: The representation <strong>of</strong> a rational number r as p/q, where p and q �= 0 are integers is called a fraction.<br />
Fractions can be added, subtracted, multiplied and one can divide by nonzero fractions.<br />
Addition <strong>of</strong> fractions: 5/3 + 7/5 = 25/15 + 21/15 = 46/15<br />
Subtraction <strong>of</strong> fractions: 5/3 − 7/5 = 25/15 − 21/15 = 4/15<br />
Multiplication <strong>of</strong> fractions: 5/3x7/5 = 35/15<br />
Division <strong>of</strong> fractions: 5/3 : 7/5 = 5/3x5/7 = 25/21<br />
Not all numbers are rational numbers. Non rational numbers are called irrational. For example, sqr(2) can not<br />
be written as p/q because � (2) = p/q would imply 2 = p 2 /q 2 or 2q 2 = p 2 . But by the uniqueness <strong>of</strong> prime<br />
factorisation <strong>of</strong> integers the left hand side has an odd number <strong>of</strong> factors 2, the right hand side an even number.<br />
� (2) is an example <strong>of</strong> an irrational number.<br />
A [hexagon] is a polygon with six sides.<br />
hexagon<br />
parallelogram<br />
A [parallelogram] is a quadrilateral whose opposite sides are parallel and congruent.
polygon<br />
A [polygon] is a closed curve in the plane formed by three or more line segments. One usually assumes that the<br />
segments don’t intersect. Examples:<br />
A [quadrilateral] is a polygon with four sides.<br />
3 sides: triangle<br />
4 sides: quadrilateral, (i.e. rectangle, rhombus, rhombus)<br />
5 sides: pentagon<br />
6 sides: hexagon<br />
7 sides: septagon<br />
8 sides: octogon<br />
quadrilateral<br />
parallel<br />
Two lines in the plane are called [parallel] if they do not intersect. Two parallel lines can be translated into<br />
each other. Two lines in space are called [parallel] if they can be translated into each other. Unlike in the plane,<br />
two lines in space which are not parallel do not need to intersect.<br />
triangle<br />
A [triangle] is a polygon defined by three points in the plane. The three points form the edges <strong>of</strong> the triangles,<br />
the three connections <strong>of</strong> the points form the sides <strong>of</strong> the triangle.<br />
random number generator<br />
A [random number generator] is a device used to produce random numbers. In daily life like for gambling, one<br />
<strong>of</strong>ten uses dice or coin tossing to find random numbers. Computers <strong>of</strong>ten use pseudo random number generators,<br />
which are deterministic sequences which look random. Computers can also access hardware internal staes <strong>of</strong><br />
the computer to improve randomness.<br />
range <strong>of</strong> a function<br />
The [range <strong>of</strong> a function] is the set <strong>of</strong> all values f(x), where x is in the domain <strong>of</strong> f.<br />
ratio<br />
[ratio] A rational number <strong>of</strong> the form a/b where a is called the numerator and b is called the denominator.
ectangle<br />
A [rectangle] is a parallelogram with four right angles. It is a quadrilateral, a polygon with four points in the<br />
plane. All angles have to be right angles. In a rectangle, opposite sides are parallel. A rectangle is therefore a<br />
special parallelogram.<br />
regular polygon<br />
A [regular polygon] is a polygon which has sides <strong>of</strong> equal length and equal angles. Squares, equilateral triangles<br />
or regular hexagons are examples <strong>of</strong> regular polygons.<br />
remainder<br />
The [remainder] <strong>of</strong> a division p/q is the amount left after subtracting the maximal integer multiple <strong>of</strong> q from p.<br />
For example 7/3 has the reminder 1 because 7 − 2 ∗ 3 = 1. −11/5 has the reminder −1.<br />
rhombus<br />
A [rhombus] is a parallelogram with four congruent sides. A special case is the square.<br />
An angle <strong>of</strong> 90 degrees is called a [right angle].<br />
right angle<br />
right triangle<br />
A triangle which has a right angle is also called a [right triangle].<br />
sequence<br />
An ordered list <strong>of</strong> elements is called a [sequence] For example, (1, 3, 2, 1) is a list <strong>of</strong> elements which form a finite<br />
sequence. The list (1, 2, 3, 4, 5, 6, ....) forms an infinite sequence.<br />
set<br />
A [set] is a collection <strong>of</strong> things, without regard to their order.
slope<br />
The [slope] <strong>of</strong> a line y = mx + b is the number m. One <strong>of</strong>ten measures it in percentages. m = 1 means 100<br />
percent. If a street has a slope <strong>of</strong> 10 percent, one climbes for every 10 meters going forwards 1 meter up.<br />
square<br />
A [square] is a polygonal shape in the plane with four sides where each side has the same length and all sides<br />
are perpendicular on each other. A square is also a number <strong>of</strong> the form n*n like 65=8*8. A square with integer<br />
side length has a square number as the area.<br />
subset<br />
A [subset] <strong>of</strong> a set is a set <strong>of</strong> elements which are all contained in that set. For example the set A = {1, 2, 3, 8, 4}<br />
has B = {2, 3} as a subset.<br />
subtraction<br />
[subtraction] is the operation <strong>of</strong> taking the difference between two numbers. For example 7 − 2 = 5.<br />
tessellation<br />
A [tessellation] is a cover <strong>of</strong> the plane using a finite set <strong>of</strong> polygons without leaving gaps or overlaps. Examples<br />
are regular tessellation into triangles or squares or regular hexagons. Semiregular tesselations allow to cover<br />
the plane with different types <strong>of</strong> shapes. Tesselations are also called tilings and can be defined also in higher<br />
dimensions.<br />
trapezoid<br />
A [trapezoid] is a quadrilateral with one pair <strong>of</strong> parallel sides.<br />
union <strong>of</strong> sets<br />
The [union <strong>of</strong> sets] is the set which contains the elements <strong>of</strong> all sets. One writes A ∪ B. For example, if<br />
A = {1, 2, 3, 4} and B = {0, 2, 4, 6}, then A ∪ B = {0, 1, 2, 3, 4, 6}.<br />
Venn Diagram<br />
In a [Venn Diagram] sets are represented as simple geometric shapes. It visualizes intersections and unions <strong>of</strong><br />
sets. For example if A is the set <strong>of</strong> all even numbers between 0 and 10 and B is the set <strong>of</strong> all numbers divisible<br />
by 3 between 0 and 10 one can visualize this with two circles, one <strong>of</strong> which contains 2, 5, 8, 6, the other 3, 6, 9.<br />
The circles intersect in a region which has the single element 6.
whole number<br />
A [whole number] is one <strong>of</strong> the numbers 0, 1, 2, 3, 4, ... A whole number is also called natural number or nonnegative<br />
integer.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 112 entries in this file.
Index<br />
abacus, 1<br />
absolute value, 1<br />
acute, 1<br />
addition, 2<br />
adjacent angles, 1<br />
affine cipher, 1<br />
algebra, 1<br />
alternate exterior angles, 2<br />
alternate interior angles, 2<br />
angle bisector, 2<br />
apex, 2<br />
Arabic numerals, 2<br />
area, 2<br />
arithmetic mean, 3<br />
average, 3<br />
base, 3<br />
bell curve, 3<br />
billion, 3<br />
binary number, 3<br />
cipher, 3<br />
coefficient, 4<br />
combinatorics, 4<br />
common factor, 4<br />
complementary angles, 4<br />
complex numbers, 4<br />
concave up, 4<br />
conditional probability, 4<br />
congruent, 5<br />
constant, 5<br />
constant function, 5<br />
continuous graph, 5<br />
coordinate, 5<br />
corresponding angles, 5<br />
decimal number, 5<br />
degrees, 6<br />
denominator, 6<br />
discontinuous graph, 6<br />
disjoint events, 6<br />
division, 6<br />
domain, 6<br />
element, 6<br />
empty set, 7<br />
equally likely, 7<br />
event, 7<br />
exponent, 7<br />
Fibonacci numbers, 7<br />
fractal, 7<br />
fraction, 7, 13<br />
function, 8<br />
geometric sequence, 8<br />
graph <strong>of</strong> the function, 8<br />
greatest common divisor, 8<br />
greatest common factor, 8<br />
hexagon, 13<br />
18<br />
histogram, 8<br />
hypotenuse, 8<br />
independent events, 8<br />
infinity, 9<br />
integer, 9<br />
intersection, 9<br />
isosceles triangle, 9<br />
least common multiple, 9<br />
limit, 9<br />
logarithm, 9<br />
mean, 10<br />
median, 10<br />
multiplication, 13<br />
multiplication table, 10<br />
obtuse angle, 10<br />
optical illusion, 10<br />
palindrome, 10<br />
paradox, 11<br />
parallel, 11, 14<br />
parallelogram, 11, 13<br />
pattern, 11<br />
percent, 11<br />
perimeter, 11<br />
permutation, 11<br />
polygon, 11, 14<br />
polyhedra, 12<br />
prime number, 12<br />
quadrant, 12<br />
quadratic function, 12<br />
quadrilateral, 14<br />
quotient, 12<br />
random number generator, 14<br />
range <strong>of</strong> a function, 14<br />
ratio, 14<br />
rectangle, 15<br />
regular polygon, 15<br />
remainder, 15<br />
rhombus, 15<br />
right angle, 15<br />
right triangle, 15<br />
sequence, 15<br />
set, 15<br />
slope, 16<br />
smallest common multiple, 12<br />
square, 16<br />
subset, 16<br />
subtraction, 13, 16<br />
tessellation, 16<br />
trapezoid, 16<br />
triangle, 14<br />
union <strong>of</strong> sets, 16
Venn Diagram, 16<br />
whole number, 17
[you sound tired] I worked all night<br />
[This is great] this is fantastic<br />
[ok] not ok<br />
[switzerland] country center europe<br />
[Germany] country in Europe<br />
[Austria] country in Europe<br />
you sound tired<br />
This is great<br />
ok<br />
switzerland<br />
Germany<br />
Austria<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 5 entries in this file.
Index<br />
Austria, 1<br />
Germany, 1<br />
ok, 1<br />
switzerland, 1<br />
This is great, 1<br />
2
Famous Literature<br />
[Famous Literature] List from http://www.literaturepage.com<br />
[A Christmas Carol] Charles Dickens<br />
A Christmas Carol<br />
A Connecticut Yankee in King Arthur’s Court<br />
[A Connecticut Yankee in King Arthur’s Court] Mark Twain<br />
[A Dream Within a Dream] Edgar Allan Poe<br />
[A Midsummer Night’s Dream] William Shakespeare<br />
[A Princess <strong>of</strong> Mars] Edgar Rice Burroughs<br />
[A Room With a View] E. M. Forster<br />
[A Study in Scarlet] Sir Arthur Conan Doyle<br />
[A Tale <strong>of</strong> Two Cities] Charles Dickens<br />
A Dream Within a Dream<br />
A Midsummer Night’s Dream<br />
A Princess <strong>of</strong> Mars<br />
A Room With a View<br />
A Study in Scarlet<br />
A Tale <strong>of</strong> Two Cities
[A Thief in the Night] E. W. Hornung<br />
[A Treatise on Government] Aristotle<br />
[A Woman <strong>of</strong> No Importance] Oscar Wilde<br />
[A Woman <strong>of</strong> Thirty] Honore de Balzac<br />
A Thief in the Night<br />
A Treatise on Government<br />
A Woman <strong>of</strong> No Importance<br />
A Woman <strong>of</strong> Thirty<br />
Adventures <strong>of</strong> Sherlock Holmes<br />
[Adventures <strong>of</strong> Sherlock Holmes] Sir Arthur Conan Doyle<br />
[Aesop’s Fables] Aesop<br />
[Agnes Grey] Anne Bronte<br />
[Alice’s Adventures in Wonderland] Lewis Carroll<br />
[All’s Well That Ends Well] William Shakespeare<br />
Aesop’s Fables<br />
Agnes Grey<br />
Alice’s Adventures in Wonderland<br />
All’s Well That Ends Well
[Allan Quatermain] H. Rider Haggard<br />
[Allan’s Wife] H. Rider Haggard<br />
[An Ideal Husband] Oscar Wilde<br />
[An Occurrence at Owl Creek Bridge] Ambrose Bierce<br />
[Andersen’s Fairy Tales] Hans Christian Andersen<br />
[Anna Karenina] Leo Tolstoy<br />
[Annabel Lee] Edgar Allan Poe<br />
[Anne <strong>of</strong> Green Gables] L. M. Montgomery<br />
[Antony and Cleopatra] William Shakespeare<br />
Allan Quatermain<br />
Allan’s Wife<br />
An Ideal Husband<br />
An Occurrence at Owl Creek Bridge<br />
Andersen’s Fairy Tales<br />
Anna Karenina<br />
Annabel Lee<br />
Anne <strong>of</strong> Green Gables<br />
Antony and Cleopatra
[Apology] Plato<br />
[Around the World in Eighty Days] Jules Verne<br />
[As You Like It] William Shakespeare<br />
[At the Earth’s Core] Edgar Rice Burroughs<br />
[Barnaby Rudge] Charles Dickens<br />
[Berenice] Edgar Allan Poe<br />
[Black Beauty] Anna Sewell<br />
[Bleak House] Charles Dickens<br />
[Buttered Side Down] Edna Ferber<br />
Apology<br />
Around the World in Eighty Days<br />
As You Like It<br />
At the Earth’s Core<br />
Barnaby Rudge<br />
Berenice<br />
Black Beauty<br />
Bleak House<br />
Buttered Side Down
[Cousin Betty] Honore de Balzac<br />
[Crime and Punishment] Fyodor Dostoevsky<br />
[Daisy Miller] Henry James<br />
[David Copperfield] Charles Dickens<br />
[Dead Men Tell No Tales] E. W. Hornung<br />
[Discourse on the Method] Rene Descartes<br />
[Dorothy and the Wizard in Oz] L. Frank Baum<br />
[Dracula] Bram Stoker<br />
[Eight Cousins] Louisa May Alcott<br />
Cousin Betty<br />
Crime and Punishment<br />
Daisy Miller<br />
David Copperfield<br />
Dead Men Tell No Tales<br />
Discourse on the Method<br />
Dorothy and the Wizard in Oz<br />
Dracula<br />
Eight Cousins
[Emma] Jane Austen<br />
[Essays and Lectures] Oscar Wilde<br />
[Essays <strong>of</strong> Francis Bacon] Sir Francis Bacon<br />
[Essays, First Series] Ralph Waldo Emerson<br />
[Essays, Second Series] Ralph Waldo Emerson<br />
[Ethan Frome] Edith Wharton<br />
[Cousin Betty] Honore de Balzac<br />
[Lady Windermere’s Fan] Oscar Wilde<br />
[Lincoln’s First Inaugural Address] Abraham Lincoln<br />
Emma<br />
Essays and Lectures<br />
Essays <strong>of</strong> Francis Bacon<br />
Essays, First Series<br />
Essays, Second Series<br />
Ethan Frome<br />
Cousin Betty<br />
Lady Windermere’s Fan<br />
Lincoln’s First Inaugural Address
[Lincoln’s Second Inaugural Address] Abraham Lincoln<br />
[Little Men] Louisa May Alcott<br />
[Little Women] Louisa May Alcott<br />
[Macbeth] William Shakespeare<br />
[Main Street] Sinclair Lewis<br />
[Mansfield Park] Jane Austen<br />
[Memoirs <strong>of</strong> Sherlock Holmes] Sir Arthur Conan Doyle<br />
[Middlemarch] George Eliot<br />
[Moby Dick] Herman Melville<br />
Lincoln’s Second Inaugural Address<br />
Little Men<br />
Little Women<br />
Macbeth<br />
Main Street<br />
Mansfield Park<br />
Memoirs <strong>of</strong> Sherlock Holmes<br />
Middlemarch<br />
Moby Dick
[Moll Flanders] Daniel Defoe<br />
[Much Ado About Nothing] William Shakespeare<br />
[Night and Day] Virginia Woolf<br />
[Northanger Abbey] Jane Austen<br />
[Nostromo] Joseph Conrad<br />
[O Pioneers!] Willa Cather<br />
[Of Human Bondage] W. Somerset Maugham<br />
[Oliver Twist] Charles Dickens<br />
[On the Decay <strong>of</strong> the Art <strong>of</strong> Lying] Mark Twain<br />
Moll Flanders<br />
Much Ado About Nothing<br />
Night and Day<br />
Northanger Abbey<br />
Nostromo<br />
O Pioneers!<br />
Of Human Bondage<br />
Oliver Twist<br />
On the Decay <strong>of</strong> the Art <strong>of</strong> Lying
On the Duty <strong>of</strong> Civil Disobedience<br />
[On the Duty <strong>of</strong> Civil Disobedience] Henry David Thoreau<br />
[Othello, Moor <strong>of</strong> Venice] William Shakespeare<br />
[Ozma <strong>of</strong> Oz] L. Frank Baum<br />
[Pandora] Henry James<br />
[Paradise Lost] John Milton<br />
[Persuasion] Jane Austen<br />
[Poems <strong>of</strong> Edgar Allan Poe] Edgar Allan Poe<br />
[Pollyanna] Eleanor H. Porter<br />
[Pride and Prejudice] Jane Austen<br />
Othello, Moor <strong>of</strong> Venice<br />
Ozma <strong>of</strong> Oz<br />
Pandora<br />
Paradise Lost<br />
Persuasion<br />
Poems <strong>of</strong> Edgar Allan Poe<br />
Pollyanna<br />
Pride and Prejudice
[Pygmalion] George Bernard Shaw<br />
Pygmalion<br />
Raffles: Further Adventures <strong>of</strong> the Amateur Cracksman<br />
[Raffles: Further Adventures <strong>of</strong> the Amateur Cracksman] E. W. Hornung<br />
[Rebecca Of Sunnybrook Farm] Kate Douglas Wiggin<br />
[Robinson Crusoe] Daniel Defoe<br />
[Romeo and Juliet] William Shakespeare<br />
[Rose in Bloom] Louisa May Alcott<br />
[Sense and Sensibility] Jane Austen<br />
[Silas Marner] George Eliot<br />
[Tarzan <strong>of</strong> the Apes] Edgar Rice Burroughs<br />
Rebecca Of Sunnybrook Farm<br />
Robinson Crusoe<br />
Romeo and Juliet<br />
Rose in Bloom<br />
Sense and Sensibility<br />
Silas Marner<br />
Tarzan <strong>of</strong> the Apes
[Tess <strong>of</strong> the d’Urbervilles] Thomas Hardy<br />
[The Adventures <strong>of</strong> Huckleberry Finn] Mark Twain<br />
[The Adventures <strong>of</strong> Pinocchio] Carlo Collodi<br />
[The Adventures <strong>of</strong> Tom Sawyer] Mark Twain<br />
[The Aeneid] Virgil<br />
[The Age <strong>of</strong> Innocence] Edith Wharton<br />
[The Amateur Cracksman] E. W. Hornung<br />
[The Analysis <strong>of</strong> Mind] Bertrand Russell<br />
[The Ballad <strong>of</strong> Reading Gaol] Oscar Wilde<br />
Tess <strong>of</strong> the d’Urbervilles<br />
The Adventures <strong>of</strong> Huckleberry Finn<br />
The Adventures <strong>of</strong> Pinocchio<br />
The Adventures <strong>of</strong> Tom Sawyer<br />
The Aeneid<br />
The Age <strong>of</strong> Innocence<br />
The Amateur Cracksman<br />
The Analysis <strong>of</strong> Mind<br />
The Ballad <strong>of</strong> Reading Gaol
[The Bells] Edgar Allan Poe<br />
[The Call <strong>of</strong> the Wild] Jack London<br />
[The Cask <strong>of</strong> Amontillado] Edgar Allan Poe<br />
[The Categories] Aristotle<br />
[The Chessmen <strong>of</strong> Mars] Edgar Rice Burroughs<br />
[The Comedy <strong>of</strong> Errors] William Shakespeare<br />
[The Count <strong>of</strong> Monte Cristo] Alexandre Dumas<br />
[The Emerald City <strong>of</strong> Oz] L. Frank Baum<br />
[The Fall <strong>of</strong> the House <strong>of</strong> Usher] Edgar Allan Poe<br />
The Bells<br />
The Call <strong>of</strong> the Wild<br />
The Cask <strong>of</strong> Amontillado<br />
The Categories<br />
The Chessmen <strong>of</strong> Mars<br />
The Comedy <strong>of</strong> Errors<br />
The Count <strong>of</strong> Monte Cristo<br />
The Emerald City <strong>of</strong> Oz<br />
The Fall <strong>of</strong> the House <strong>of</strong> Usher
[The Four Million] O. Henry<br />
[The Gambler] Fyodor Dostoevsky<br />
[The Gettysburg Address] Abraham Lincoln<br />
[The Gods <strong>of</strong> Mars] Edgar Rice Burroughs<br />
[The Happy Prince and Other Tales] Oscar Wilde<br />
The Four Million<br />
The Gambler<br />
The Gettysburg Address<br />
The Gods <strong>of</strong> Mars<br />
The Happy Prince and Other Tales<br />
The History <strong>of</strong> Tom Jones, a foundling<br />
[The History <strong>of</strong> Tom Jones, a foundling] Henry Fielding<br />
The History <strong>of</strong> Troilus and Cressida<br />
[The History <strong>of</strong> Troilus and Cressida] William Shakespeare<br />
The Hound <strong>of</strong> the Baskervilles<br />
[The Hound <strong>of</strong> the Baskervilles] Sir Arthur Conan Doyle<br />
[The Hunchback <strong>of</strong> Notre Dame] Victor Hugo<br />
The Hunchback <strong>of</strong> Notre Dame
[The Hunting <strong>of</strong> the Snark] Lewis Carroll<br />
[The Idiot] Fyodor Dostoevsky<br />
[The Iliad] Homer<br />
[The Importance <strong>of</strong> Being Earnest] Oscar Wilde<br />
[The Innocence <strong>of</strong> Father Brown] G. K. Chesterton<br />
[The Innocents Abroad] Mark Twain<br />
[The Invisible Man] H. G. Wells<br />
[The Island <strong>of</strong> Doctor Moreau] H. G. Wells<br />
[The Jungle Book] Rudyard Kipling<br />
The Hunting <strong>of</strong> the Snark<br />
The Idiot<br />
The Iliad<br />
The Importance <strong>of</strong> Being Earnest<br />
The Innocence <strong>of</strong> Father Brown<br />
The Innocents Abroad<br />
The Invisible Man<br />
The Island <strong>of</strong> Doctor Moreau<br />
The Jungle Book
[The Last Days <strong>of</strong> Pompeii] Edward Bulwer-Lytton<br />
[The Last <strong>of</strong> the Mohicans] James Fenimore Cooper<br />
[The Legend <strong>of</strong> Sleepy Hollow] Washington Irving<br />
The Last Days <strong>of</strong> Pompeii<br />
The Last <strong>of</strong> the Mohicans<br />
The Legend <strong>of</strong> Sleepy Hollow<br />
The Life and Adventures <strong>of</strong> Nicholas Nickleby<br />
[The Life and Adventures <strong>of</strong> Nicholas Nickleby] Charles Dickens<br />
The Life and Death <strong>of</strong> King Richard III<br />
[The Life and Death <strong>of</strong> King Richard III] William Shakespeare<br />
[The Life <strong>of</strong> King Henry V] William Shakespeare<br />
[The Lost Continent] Edgar Rice Burroughs<br />
[The Lost World] Sir Arthur Conan Doyle<br />
[The Man in the Iron Mask] Alexandre Dumas<br />
The Life <strong>of</strong> King Henry V<br />
The Lost Continent<br />
The Lost World<br />
The Man in the Iron Mask
The Man Upstairs and Other Stories<br />
[The Man Upstairs and Other Stories] P. G. Wodehouse<br />
[The Man Who Knew Too Much] G. K. Chesterton<br />
[The Man with Two Left Feet] P. G. Wodehouse<br />
[The Masque <strong>of</strong> the Red Death] Edgar Allan Poe<br />
[The Merchant <strong>of</strong> Venice] William Shakespeare<br />
[The Merry Adventures <strong>of</strong> Robin Hood] Howard Pyle<br />
[The Merry Wives <strong>of</strong> Windsor] William Shakespeare<br />
[The Moon and Sixpence] W. Somerset Maugham<br />
[The Moonstone] Wilkie Collins<br />
The Man Who Knew Too Much<br />
The Man with Two Left Feet<br />
The Masque <strong>of</strong> the Red Death<br />
The Merchant <strong>of</strong> Venice<br />
The Merry Adventures <strong>of</strong> Robin Hood<br />
The Merry Wives <strong>of</strong> Windsor<br />
The Moon and Sixpence<br />
The Moonstone
[The Murders in the Rue Morgue] Edgar Allan Poe<br />
[The Mysterious Affair at Styles] Agatha Christie<br />
[The Mystery <strong>of</strong> Edwin Drood] Charles Dickens<br />
[The Mystery <strong>of</strong> the Yellow Room] Gaston Leroux<br />
[The Odyssey] Homer<br />
The Murders in the Rue Morgue<br />
The Mysterious Affair at Styles<br />
The Mystery <strong>of</strong> Edwin Drood<br />
The Mystery <strong>of</strong> the Yellow Room<br />
The Odyssey<br />
The Origin <strong>of</strong> Species means <strong>of</strong> Natural Selection<br />
[The Origin <strong>of</strong> Species] means <strong>of</strong> Natural Selection] Charles Darwin<br />
[The Phantom <strong>of</strong> the Opera] Gaston Leroux<br />
[The Picture <strong>of</strong> Dorian Gray] Oscar Wilde<br />
[The Pit and the Pendulum] Edgar Allan Poe<br />
The Phantom <strong>of</strong> the Opera<br />
The Picture <strong>of</strong> Dorian Gray<br />
The Pit and the Pendulum
[The Portrait <strong>of</strong> a Lady] Henry James<br />
[The Purloined Letter] Edgar Allan Poe<br />
[The Raven] Edgar Allan Poe<br />
[The Red Badge <strong>of</strong> Courage] Stephen Crane<br />
[The Republic] Plato<br />
The Portrait <strong>of</strong> a Lady<br />
The Purloined Letter<br />
The Raven<br />
The Red Badge <strong>of</strong> Courage<br />
The Republic<br />
The Return <strong>of</strong> Sherlock Holmes<br />
[The Return <strong>of</strong> Sherlock Holmes] Sir Arthur Conan Doyle<br />
The Rime <strong>of</strong> the Ancient Mariner<br />
[The Rime <strong>of</strong> the Ancient Mariner] Samuel Taylor Coleridge<br />
[The Scarecrow <strong>of</strong> Oz] L. Frank Baum<br />
[The Scarlet Letter] Nathaniel Hawthorne<br />
The Scarecrow <strong>of</strong> Oz<br />
The Scarlet Letter
[The Sonnets] William Shakespeare<br />
The Sonnets<br />
The Strange Case <strong>of</strong> Dr. Jekyll and Mr. Hyde<br />
[The Strange Case <strong>of</strong> Dr. Jekyll and Mr. Hyde] Robert Louis Stevenson<br />
[The Taming <strong>of</strong> the Shrew] William Shakespeare<br />
[The Tell-Tale Heart] Edgar Allan Poe<br />
[The Tempest] William Shakespeare<br />
[The Tenant <strong>of</strong> Wildfell Hall] Anne Bronte<br />
[The Three Musketeers] Alexandre Dumas<br />
[The Time Machine] H. G. Wells<br />
[The Tin Woodman <strong>of</strong> Oz] L. Frank Baum<br />
The Taming <strong>of</strong> the Shrew<br />
The Tell-Tale Heart<br />
The Tempest<br />
The Tenant <strong>of</strong> Wildfell Hall<br />
The Three Musketeers<br />
The Time Machine<br />
The Tin Woodman <strong>of</strong> Oz
[The Tragedy <strong>of</strong> Coriolanus] William Shakespeare<br />
[The Tragedy <strong>of</strong> King Lear] William Shakespeare<br />
The Tragedy <strong>of</strong> Coriolanus<br />
The Tragedy <strong>of</strong> King Lear<br />
The Tragedy <strong>of</strong> King Richard the Second<br />
[The Tragedy <strong>of</strong> King Richard the Second] William Shakespeare<br />
[The Voyage Out] Virginia Woolf<br />
[The War in the Air] H. G. Wells<br />
[The War <strong>of</strong> the Worlds] H. G. Wells<br />
[The Wind in the Willows] Kenneth Grahame<br />
[The Wisdom <strong>of</strong> Father Brown] G. K. Chesterton<br />
[The Wonderful Wizard <strong>of</strong> Oz] L. Frank Baum<br />
The Voyage Out<br />
The War in the Air<br />
The War <strong>of</strong> the Worlds<br />
The Wind in the Willows<br />
The Wisdom <strong>of</strong> Father Brown<br />
The Wonderful Wizard <strong>of</strong> Oz
[Three Men in a Boat] Jerome K. Jerome<br />
[Through the Looking Glass] Lewis Carroll<br />
[Thus Spake Zarathustra] Friedrich Nietzsche<br />
[Thuvia, Maid <strong>of</strong> Mars] Edgar Rice Burroughs<br />
[To Helen] Edgar Allan Poe<br />
[Treasure Island] Robert Louis Stevenson<br />
[Twelfth Night] William Shakespeare<br />
Three Men in a Boat<br />
Through the Looking Glass<br />
Thus Spake Zarathustra<br />
Thuvia, Maid <strong>of</strong> Mars<br />
To Helen<br />
Treasure Island<br />
Twelfth Night<br />
Twenty Thousand Leagues Under the Seas<br />
[Twenty Thousand Leagues Under the Seas] Jules Verne<br />
[Twenty Years After] Alexandre Dumas<br />
Twenty Years After
[Typee] Herman Melville<br />
[Ulalume] Edgar Allan Poe<br />
[Uneasy Money] P. G. Wodehouse<br />
Typee<br />
Ulalume<br />
Uneasy Money<br />
Up From Slavery: An Autobiography<br />
[Up From Slavery: An Autobiography] Booker T. Washington<br />
[Vanity Fair] William Makepeace Thackeray<br />
[Walden] Henry David Thoreau<br />
[War and Peace] Leo Tolstoy<br />
[Warlord <strong>of</strong> Mars] Edgar Rice Burroughs<br />
[White Fang] Jack London<br />
Vanity Fair<br />
Walden<br />
War and Peace<br />
Warlord <strong>of</strong> Mars<br />
White Fang
Wuthering Heights<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 198 entries in this file.
Index<br />
A Christmas Carol, 1<br />
A Connecticut Yankee in King Arthur’s Court, 1<br />
A Dream Within a Dream, 1<br />
A Midsummer Night’s Dream, 1<br />
A Princess <strong>of</strong> Mars, 1<br />
A Room With a View, 1<br />
A Study in Scarlet, 1<br />
A Tale <strong>of</strong> Two Cities, 1<br />
A Thief in the Night, 2<br />
A Treatise on Government, 2<br />
A Woman <strong>of</strong> No Importance, 2<br />
A Woman <strong>of</strong> Thirty, 2<br />
Adventures <strong>of</strong> Sherlock Holmes, 2<br />
Aesop’s Fables, 2<br />
Agnes Grey, 2<br />
Alice’s Adventures in Wonderland, 2<br />
All’s Well That Ends Well, 2<br />
Allan Quatermain, 3<br />
Allan’s Wife, 3<br />
An Ideal Husband, 3<br />
An Occurrence at Owl Creek Bridge, 3<br />
Andersen’s Fairy Tales, 3<br />
Anna Karenina, 3<br />
Annabel Lee, 3<br />
Anne <strong>of</strong> Green Gables, 3<br />
Antony and Cleopatra, 3<br />
Apology, 4<br />
Around the World in Eighty Days, 4<br />
As You Like It, 4<br />
At the Earth’s Core, 4<br />
Barnaby Rudge, 4<br />
Berenice, 4<br />
Black Beauty, 4<br />
Bleak House, 4<br />
Buttered Side Down, 4<br />
Cousin Betty, 5, 6<br />
Crime and Punishment, 5<br />
Daisy Miller, 5<br />
David Copperfield, 5<br />
Dead Men Tell No Tales, 5<br />
Discourse on the Method, 5<br />
Dorothy and the Wizard in Oz, 5<br />
Dracula, 5<br />
Eight Cousins, 5<br />
Emma, 6<br />
Essays and Lectures, 6<br />
Essays <strong>of</strong> Francis Bacon, 6<br />
Essays, First Series, 6<br />
Essays, Second Series, 6<br />
Ethan Frome, 6<br />
Lady Windermere’s Fan, 6<br />
Lincoln’s First Inaugural Address, 6<br />
Lincoln’s Second Inaugural Address, 7<br />
Little Men, 7<br />
Little Women, 7<br />
24<br />
Macbeth, 7<br />
Main Street, 7<br />
Mansfield Park, 7<br />
Memoirs <strong>of</strong> Sherlock Holmes, 7<br />
Middlemarch, 7<br />
Moby Dick, 7<br />
Moll Flanders, 8<br />
Much Ado About Nothing, 8<br />
Night and Day, 8<br />
Northanger Abbey, 8<br />
Nostromo, 8<br />
O Pioneers, 8<br />
Of Human Bondage, 8<br />
Oliver Twist, 8<br />
On the Decay <strong>of</strong> the Art <strong>of</strong> Lying, 8<br />
On the Duty <strong>of</strong> Civil Disobedience, 9<br />
Othello, Moor <strong>of</strong> Venice, 9<br />
Ozma <strong>of</strong> Oz, 9<br />
Pandora, 9<br />
Paradise Lost, 9<br />
Persuasion, 9<br />
Poems <strong>of</strong> Edgar Allan Poe, 9<br />
Pollyanna, 9<br />
Pride and Prejudice, 9<br />
Pygmalion, 10<br />
Raffles: Further Adventures <strong>of</strong> the Amateur Cracksman,<br />
10<br />
Rebecca Of Sunnybrook Farm, 10<br />
Robinson Crusoe, 10<br />
Romeo and Juliet, 10<br />
Rose in Bloom, 10<br />
Sense and Sensibility, 10<br />
Silas Marner, 10<br />
Tarzan <strong>of</strong> the Apes, 10<br />
Tess <strong>of</strong> the d’Urbervilles, 11<br />
The Adventures <strong>of</strong> Huckleberry Finn, 11<br />
The Adventures <strong>of</strong> Pinocchio, 11<br />
The Adventures <strong>of</strong> Tom Sawyer, 11<br />
The Aeneid, 11<br />
The Age <strong>of</strong> Innocence, 11<br />
The Amateur Cracksman, 11<br />
The Analysis <strong>of</strong> Mind, 11<br />
The Ballad <strong>of</strong> Reading Gaol, 11<br />
The Bells, 12<br />
The Call <strong>of</strong> the Wild, 12<br />
The Cask <strong>of</strong> Amontillado, 12<br />
The Categories, 12<br />
The Chessmen <strong>of</strong> Mars, 12<br />
The Comedy <strong>of</strong> Errors, 12<br />
The Count <strong>of</strong> Monte Cristo, 12<br />
The Emerald City <strong>of</strong> Oz, 12<br />
The Fall <strong>of</strong> the House <strong>of</strong> Usher, 12<br />
The Four Million, 13<br />
The Gambler, 13<br />
The Gettysburg Address, 13
The Gods <strong>of</strong> Mars, 13<br />
The Happy Prince and Other Tales, 13<br />
The History <strong>of</strong> Tom Jones, a foundling, 13<br />
The History <strong>of</strong> Troilus and Cressida, 13<br />
The Hound <strong>of</strong> the Baskervilles, 13<br />
The Hunchback <strong>of</strong> Notre Dame, 13<br />
The Hunting <strong>of</strong> the Snark, 14<br />
The Idiot, 14<br />
The Iliad, 14<br />
The Importance <strong>of</strong> Being Earnest, 14<br />
The Innocence <strong>of</strong> Father Brown, 14<br />
The Innocents Abroad, 14<br />
The Invisible Man, 14<br />
The Island <strong>of</strong> Doctor Moreau, 14<br />
The Jungle Book, 14<br />
The Last Days <strong>of</strong> Pompeii, 15<br />
The Last <strong>of</strong> the Mohicans, 15<br />
The Legend <strong>of</strong> Sleepy Hollow, 15<br />
The Life and Adventures <strong>of</strong> Nicholas Nickleby, 15<br />
The Life and Death <strong>of</strong> King Richard III, 15<br />
The Life <strong>of</strong> King Henry V, 15<br />
The Lost Continent, 15<br />
The Lost World, 15<br />
The Man in the Iron Mask, 15<br />
The Man Upstairs and Other Stories, 16<br />
The Man Who Knew Too Much, 16<br />
The Man with Two Left Feet, 16<br />
The Masque <strong>of</strong> the Red Death, 16<br />
The Merchant <strong>of</strong> Venice, 16<br />
The Merry Adventures <strong>of</strong> Robin Hood, 16<br />
The Merry Wives <strong>of</strong> Windsor, 16<br />
The Moon and Sixpence, 16<br />
The Moonstone, 16<br />
The Murders in the Rue Morgue, 17<br />
The Mysterious Affair at Styles, 17<br />
The Mystery <strong>of</strong> Edwin Drood, 17<br />
The Mystery <strong>of</strong> the Yellow Room, 17<br />
The Odyssey, 17<br />
The Origin <strong>of</strong> Species means <strong>of</strong> Natural Selection, 17<br />
The Phantom <strong>of</strong> the Opera, 17<br />
The Picture <strong>of</strong> Dorian Gray, 17<br />
The Pit and the Pendulum, 17<br />
The Portrait <strong>of</strong> a Lady, 18<br />
The Purloined Letter, 18<br />
The Raven, 18<br />
The Red Badge <strong>of</strong> Courage, 18<br />
The Republic, 18<br />
The Return <strong>of</strong> Sherlock Holmes, 18<br />
The Rime <strong>of</strong> the Ancient Mariner, 18<br />
The Scarecrow <strong>of</strong> Oz, 18<br />
The Scarlet Letter, 18<br />
The Sonnets, 19<br />
The Strange Case <strong>of</strong> Dr. Jekyll and Mr. Hyde, 19<br />
The Taming <strong>of</strong> the Shrew, 19<br />
The Tell-Tale Heart, 19<br />
The Tempest, 19<br />
The Tenant <strong>of</strong> Wildfell Hall, 19<br />
The Three Musketeers, 19<br />
The Time Machine, 19<br />
The Tin Woodman <strong>of</strong> Oz, 19<br />
The Tragedy <strong>of</strong> Coriolanus, 20<br />
The Tragedy <strong>of</strong> King Lear, 20<br />
The Tragedy <strong>of</strong> King Richard the Second, 20<br />
The Voyage Out, 20<br />
The War in the Air, 20<br />
The War <strong>of</strong> the Worlds, 20<br />
The Wind in the Willows, 20<br />
The Wisdom <strong>of</strong> Father Brown, 20<br />
The Wonderful Wizard <strong>of</strong> Oz, 20<br />
Three Men in a Boat, 21<br />
Through the Looking Glass, 21<br />
Thus Spake Zarathustra, 21<br />
Thuvia, Maid <strong>of</strong> Mars, 21<br />
To Helen, 21<br />
Treasure Island, 21<br />
Twelfth Night, 21<br />
Twenty Thousand Leagues Under the Seas, 21<br />
Twenty Years After, 21<br />
Typee, 22<br />
Ulalume, 22<br />
Uneasy Money, 22<br />
Up From Slavery: An Autobiography, 22<br />
Vanity Fair, 22<br />
Walden, 22<br />
War and Peace, 22<br />
Warlord <strong>of</strong> Mars, 22<br />
White Fang, 22<br />
Wuthering Heights, 23
<strong>ENTRY</strong> SINGLE VARIABLE CALCULUS I<br />
[<strong>ENTRY</strong> SINGLE VARIABLE CALCULUS I] Authors: Oliver Knill: 2001 Literature: not yet<br />
Abel’s partial summation formula<br />
[Abel’s partial summation formula] is a discrete version <strong>of</strong> the partial integration formula: with An = �n k=1 ak<br />
one has �n k=m akbk = �n k=m Ak(bk − bk+1) + Anbn+1 − Am−1bm.<br />
Abel’s test<br />
[Abel’s test]: if an is a bounded monotonic sequence and bn is a convergent series, then the sum �<br />
n anbn<br />
converges.<br />
absolute value<br />
The [absolute value] <strong>of</strong> a real number x is denoted by |x| and defined as the maximum <strong>of</strong> x and −x. We can<br />
also write |x| = + √ x 2 . The absolute value <strong>of</strong> a complex number z = x + iy is defined as � x 2 + y 2 .<br />
accumulation point<br />
An [accumulation point] <strong>of</strong> a sequence an <strong>of</strong> real numbers is a point a which the limit <strong>of</strong> a subsequence ank <strong>of</strong><br />
an. A sequence an converges if and only if there is exactly one accumulation point. Example: The sequence<br />
an = sin(πn) has two accumulation points, a = 1 and a = −1. The sequence an = sin(πn)/n has only the<br />
accumulation point a = 0. It converges.<br />
Achilles paradox<br />
The [Achilles paradox] is one <strong>of</strong> Zenos paradoxon. It argues that motion can not exist: ”set up a race between<br />
Achilles A and tortoise T . At the initial time t0 = 0, A is at the spot s = 0 while T is at position s1 = 1. Lets<br />
assume A runs twice as fast. The reace starts. When A reaches s1 at time t1 = 1, its opponent T has already<br />
advanced to a point s2 = 1 + 1/2. Whenever A reaches a point sk at time tk, where T has been at time tk−1,<br />
T has already advanced further to location sk+1. Because an infinite number <strong>of</strong> timesteps is necessary for A<br />
to reach T , it is impossible that A overcomes T .” The paradox exploits a misunderstanding <strong>of</strong> the concept <strong>of</strong><br />
summation <strong>of</strong> infinite series. At the finite time t = � ∞<br />
n=1 (tn − tn−1) = 2, both A and T will be at the same<br />
spot s = limn→∞ sn = 2.<br />
The [addition formulas] for trigonometric functions are<br />
addition formulas<br />
cos(a + b) = sin(a) cos(b) + cos(a) sin(b)<br />
sin(a + b) = cos(a) cos(b) − sin(a) sin(b)
alternating series<br />
An<br />
�<br />
[alternating series] is a series in which terms are alternatively positive and negative. An example is<br />
∞<br />
n=1 an = �∞ n=1 (−1)n /n = −1 + 1/2 − 1/3 + 1/4 − .... An alternating series with an → 0 converges by<br />
the alternating series test.<br />
alternating series test<br />
Leibniz’s [alternating series test] assures that an alternating series �<br />
n an with |an| → 0 is a convergent series.<br />
acute<br />
An angle is [acute], if it is smaller than a right angle. For example α = π/3 = 60 ◦ is an acute angle. The angle<br />
α = 2π/3 = 120 ◦ is not an acute angle. The right angle α = π/2 = 90 ◦ does not count as an acute angle. The<br />
angle α = −π/6 = −30 ◦ is an acute angle.<br />
antiderivative<br />
The [antiderivative] <strong>of</strong> a function f is a function F (x) such that the derivative <strong>of</strong> F is f that is if d/dxF (x) =<br />
f(x). The antiderivative is not unique. For example, every function F (x) = cos(x) + C is the antiderivative <strong>of</strong><br />
f(x) = sin(x). Every function F (x) = x n+1 /(n + 1) + C is the antiderivative <strong>of</strong> f(x) = x n .<br />
Arithmetic progression<br />
[Arithmetic progression] A sequence <strong>of</strong> numbers an for which bn = an+1 − an is constant, is called an arithmetic<br />
progression. For example, 3, 7, 11, 15, 19, ... is an arithmetic progression. The sequence 0, 1, 2, 4, 5, 6, 7 is not an<br />
arithmetic progression.<br />
arrow paradox<br />
The [arrow paradox] is a classical Zeno paradox with conclusion that motion can not exist: ”an object occupies<br />
at each time a space equal to itself, but something which occupies a space equal to itself can not move. Therefore,<br />
the arrow is always at rest.”<br />
asymptotic<br />
Two real functions are called [asymptotic] at a point a if limx→a f(x)/g(x) = 1. For example, f(x) = sin(x) and<br />
g(x) = x are asymptotic at a = 0. The point a can also be infinite: for example, f(x) = x and g(x) = √ x 2 + 1<br />
are asymptotic at a = ∞.
Bernstein polynomials<br />
The [Bernstein polynomials] <strong>of</strong> a continuous function f on the unit interval 0 ≤ x ≤ 1 are defined as Bn(x) =<br />
� n<br />
k=1 f(k/n)xk (1 − x) n−k n!/(k!(n − k!).<br />
Binomial coefficients<br />
[Binomial coefficients] The coefficients B(n, k) <strong>of</strong> the polynomial (x + 1) n for integer n are called Binomial<br />
coefficients. Explicitly one has B(n, k) = n!/(k!(n − k)!), where k! = k(k − 1)!, 0! = 1 is the factorial <strong>of</strong> k. The<br />
function B(n, k) can be defined for any real numbers n, k by writing n! = Γ(n + 1), where Γ is the Gamma<br />
function. If p is a positive real number and k is an integer, one has one has B(p, k) = p(p − 1)...(p − k + 1)/k!.<br />
For example, B(1/2, 0) = B(1/2, 1) = 1/2, B(1/2, 2) = −1/8. Indeed, (1 + x) 1/2 = 1 + x/2 − x 2 /8 + ....<br />
Binominal theorem<br />
The [Binominal theorem] tells that for a real number |z| < 1 and real number p, one has (1 + z) p =<br />
� ∞<br />
k=0 B(p, k)zk , where B(p, k) is called the Binomial coefficient. If p is a positive integer, then (1 + z) p is<br />
a polynomial. For example:<br />
(1 + z) 4 = 1 + 4z + 6z 2 + 4z 3 + z 4 .<br />
If p is a noninteger or negative, then (1 + z) p is an infinite sum. For example<br />
(1 + z) −1/2 = 1 − x/2 + 3x 2 /8 − 5x 3 /16 + ...<br />
bisector<br />
A [bisector] is a straight line that bisects a given angle or a given line segment. For example, the y-axis x = 0<br />
in the plane bisects the line segment connecting (−1, 0) with (1, 0). The line x = y bisects the angle � (CAB)<br />
where C = (0, 1), A = (0, 0), B = (1, 0) at the point A.<br />
Bolzano’s theorem<br />
[Bolzano’s theorem] also called intermediate value theorem says that a continuous function on an interval (a, b)<br />
takes each value between f(a) and f(b). For example, the function f(x) = sin(x) takes any value between −1<br />
and 1 because f is continuous and f(−π/2) = −1 and f(π/2) = 1.<br />
Fermat principle<br />
The [Fermat principle] tells that if f is a function which is differentiable at z and f(x) > f(z) for all points in<br />
an interval (z − a, z + a) with a > 0, then f ′ (z) = 0.
fundamental theorem <strong>of</strong> calculus<br />
The [fundamental theorem <strong>of</strong> calculus]: if f is a differentiable function on a ≤ x ≤ b where a < b are real<br />
numbers, then f(b) − f(a) = � b<br />
a f ′ (x) dx.<br />
[integration rules]:<br />
• � af(x) dx = a � f(x) dx.<br />
• � f(x) + g(x) dx = � f(x) dx + � g(x) dx.<br />
integration rules<br />
• � fg dx = fG − � f ′ G, where G ′ = g. This is called integration by parts.<br />
intermediate value theorem<br />
The [intermediate value theorem] also called Bolzno theorem assures that a continuous function on an interval<br />
a ≤ z ≤ b takes each each value between f(a) and f(b). For example f(x) = cos(x) + cos(3x) + cos(5x) takes<br />
any value between [−3, 3] on [0, π] because f(0) = 3 and f(π) = −3.<br />
Cauchy’s convergence condition<br />
[Cauchy’s convergence condition]: a sequence an converges, if and only if it is a Cauchy sequence that is if for<br />
every constant c > 0, we can find n, such that for all k > n, m > n one has |am − ak| < c. For example, the<br />
sequence an = 1/ log(n) converges because for all c > 0, and the integer n closest to e 2c + 1 one has for k > n<br />
and m > n |am − ak| ≤ c.<br />
Cauchy’s convergence test<br />
[Cauchy’s convergence test]. Given a series �∞ the series is a convergent series. If r > 1, then the series diverges.<br />
k=1 ak with positive summands ak. If r = limn→∞ a 1/n<br />
n<br />
< 1 then
continuous<br />
A function f is called [continuous] at a point x if for every open interval V around f(x) there exists an open<br />
interval U around x such that f(U) is a subset <strong>of</strong> V . A function f is continuous in a set Y if it is continous at<br />
every point in Y . This definition is equivalent to: for every sequence xn → x, the sequence f(xn) converges to<br />
f(x). Examples:<br />
• Any polynomial like x 5 + 5x 3 + 3x is continuous on the entire line.<br />
• The sum and product <strong>of</strong> continuous functions is continuous.<br />
• the composition <strong>of</strong> two continuous functions is continuous.<br />
Discontinuities can happen in different ways: the function can become infinite like f(x) = 1/x at 0 or tan(x)<br />
at x = π/2, the function can jump like f(x) = sign(x) which is 1 if x > 0, −1 if x < 0 and 0 if x = 0. A<br />
function can also become too oscillatory at a point like f(x) = sin(1/x) at x = 0. Note that f(x) = x sin(1/x)<br />
is continuous on the entire real line. There are functions which are discontinuous at every point. An example<br />
is f(x) = 1 if x is rational and f(x) = −1 if x is irrational.<br />
Note that be restricting the domain <strong>of</strong> a function, one an make it continuous. For example: f(x) = 1/x is<br />
continuous on the positive real axes.<br />
converges<br />
A function f(x) [converges] to a value z at x if the function g which agrees with f away from x and satisfies<br />
g(x) = z is continouous at x. The value z is called the limit <strong>of</strong> f at x. For example the function f(x) =<br />
(1 − x 2 )/(1 − x) has the limit z = 2 at x = 1. The function g(x) which is defined bo be f(x) for x �= 1 and<br />
g(1) = 2 is indeed continuous. One writes z = limy→x f(y). One has<br />
• limx→z(f(x) + g(x)) = limx→z f(x) + limx→z g(x).<br />
• limx→z(f(x)g(x)) = limx→z f(x) + g(x).<br />
• limx→z f(g(x)) = f(limx→z g(x)).<br />
A series an is a [convergent series], if the partial sum sequence bn = � n<br />
k=1 ak converges to a finite limit a.<br />
absolutely convergent series<br />
A series �<br />
n an is called an [absolutely convergent series] if �<br />
n |an| is a convergent series.<br />
series<br />
Summing up a sequence is called a [series]. An important example is the geometric series 1 + 1/2 + 1/4 + 1/8 +<br />
1/16 + ..., which sums up to 2. An other example is the harmonic series 1 + 1/2 + 1/3 + 1/4 + 1/5 + ... which<br />
has no finite limit.<br />
change <strong>of</strong> variables<br />
The [change <strong>of</strong> variables] in integration theory is the formula � f(x)dx = � f(g(u))g ′ (u)du if x = g(u). For<br />
example, � √ 1 − x 2 dx becomes with x = g(u) = sin(u) and dx = g ′ (u)du = cos(u)du the integral � cos 2(u) du.
differentiable<br />
A function f is called [differentiable] at z if there exists a function g which is continuous at z such that<br />
f(x) = f(z) + (x − z)g(x). The derivative <strong>of</strong> f at z is g(z) and also denoted f ′ (x). By solving for g(x) and<br />
letting x → z one can write g(z) = limx→z(f(x) − f(z))/(x − z). The quotient is called the differential quotient.<br />
• The sum <strong>of</strong> two at z differentiable functions is differentiable at z and (f + g) ′ (z) = f ′ (z) + g ′ (z). This is<br />
called the sum rule.<br />
• The prduct <strong>of</strong> two at z differentiable functions is differentiable at z and (fg) ′ = f ′ g + fg ′ . This is called<br />
the product rule.<br />
• The composition <strong>of</strong> two differentiable functions is differentiable and (f ◦ g) ′ = (f ′ ◦ g)g ′ . This is called the<br />
chain rule.<br />
Functions can be continuous without being differentiable. For example f(x) = |x| is continuous at 0 but not<br />
differentiable at 0. There are functions which are continuous everywhere but not differentiable at most points.<br />
An example is the Weierstrass function f(x) = � ∞<br />
k=1 cos(k2 x)/k 2 .<br />
Extended mean value theorem<br />
[Extended mean value theorem]. If f(x) and g(x) are differentiable on the interval (a, b) and are continuous on<br />
the closed interval I = {a ≤ x ≤ b} then there exists a point x ∈ I for which<br />
f ′ (x)/g ′ (x) = (f(b) − f(a))/(g(b) − g(a)) .<br />
Pro<strong>of</strong>. Otherwise one would have one <strong>of</strong> the following two possibilies:<br />
f ′ (x)(g(b) − g(a)) < g ′ (x)(f(b) − f(a)) for all x in (a, b) or<br />
f ′ (x)(g(b) − g(a)) < g ′ (x)(f(b) − f(a)) for all x in (a, b).<br />
Integration <strong>of</strong> these expressions using the fundamental theorem <strong>of</strong> calculus gives<br />
(f(b) − f(a))(g(b) − g(a)) < (g(b) − g(a))(f(b) − f(a)) or<br />
(f(b) − f(a))(g(b) − g(a)) > (g(b) − g(a))(f(b) − f(a)) which both are not possible.<br />
The special case g(x) = x is called the mean value theorem.<br />
factorial<br />
The [factorial] <strong>of</strong> a positive integer n is defined recursively by n! = n(n − 1)! and 0! = 1. For example, 5! = 120.<br />
The factorial function can be extended to the real line and is then called the Γ function: n! = Γ(n + 1), where<br />
Γ(z) =<br />
which is finite everywhere except at z = 0, −1, −2, ....<br />
� ∞<br />
t<br />
0<br />
z−1 e −t dt .<br />
limit<br />
The [limit] <strong>of</strong> a sequence <strong>of</strong> numbers an is a number a such that an converges to a in the following sense: for<br />
every c > 0 there exists an integer m such that |an − a| < c for n > m. Limits can be defined in any metric<br />
space and more generally in any topological space.
maximum-value theorem<br />
The [maximum-value theorem] assures that a continuous function on an interval a < z < b has a maximum on<br />
that interval.<br />
parabola<br />
A [parabola] is the graph <strong>of</strong> the function f(x) = x 2 . More general parabolas can be obtained as graphs <strong>of</strong><br />
f(x) = a(x − b) 2 + c where a, b, c are constants or curves obtained by rotating such a curve in the plane. For<br />
example the set <strong>of</strong> points in the plane satisfying x = y 2 form a parabola. Parabolas are examples <strong>of</strong> conic<br />
sections, intersections <strong>of</strong> a plane with a cone.<br />
L’Hopital rule<br />
The [L’Hopital rule] tells that if f and g are differentiable functions at x and f(x) = g(x) and g ′ (x) �= 0, then<br />
limx→z f(x)/g(x) = limx→z f ′ (x)/g ′ (x).<br />
For example, limx→0 sin(3x)/x = limx→0 3 cos(3x) = 3. The rule essentially tells that one can replace the<br />
functions by their linear approximation near a point to find the limit. The pro<strong>of</strong> follows immediatly from the<br />
definition <strong>of</strong> differentiability: there exist continuous functions F, G such that f(x) = f(z) + (x − z)F (x) and<br />
g(x) = g(z) + (x − z)G(x). Because G(z) �= 0, the function F (x)/G(x) is continuous at z with value F (z)/G(z).<br />
Now: limx→z f(x)/g(x) = limx→z(f(z) + (x − z)F (x))/(g(z) + (x − z)G(x)) == limx→z f(z)/g(z).<br />
[Hopital rule] see L’Hopital rule.<br />
Hopital rule<br />
hyperbola<br />
A [hyperbola] is curve in the plane which can be described as the graph <strong>of</strong> the function f(x) = 1/x. Also<br />
translated, scaled and rotated versions <strong>of</strong> this curve is called a hyperbola. For example, the set <strong>of</strong> points (x, y)<br />
in the plane which satisfy (x − 1) 2 − (y − 2) 2 = 5 is a hyperbola.<br />
Mean value theorem<br />
[Mean value theorem]. If f(x) is a continuous function on an interval I = {a ≤ x ≤ b} which is differentiable<br />
on the open interval (a, b), then there exists a point x ∈ I for which f ′ (x) = C = (f(b) − f(a))/(b − a). Pro<strong>of</strong>.<br />
Otherwise, f ′ (x) < C on (a, b) or f ′ (x) > C on (a, b). Integration gives using the fundamental theorem <strong>of</strong><br />
calculus<br />
especially<br />
f(x) − f(a) = � x<br />
a f ′ (t)dt < C(x − a) or<br />
f(x) − f(a) = � x<br />
a f ′ (t)dt > C(x − a)<br />
f(x) − f(a) = � b<br />
a f ′ (t)dt < C(b − a) or<br />
f(x) − f(a) = � b<br />
a f ′ (t)dt > C(b − a) which is a contradiction<br />
The mean value theorem is a special case <strong>of</strong> the extended mean value theorem.
Rolle’s theorem<br />
[Rolle’s theorem] If f(x) is a continuous function on the interval I = {a ≤ x ≤ b} which is differentiable on the<br />
open interval (a, b) and f(a) = f(b), then there exists a point x ∈ (a, b), for which f ′ (x) = 0.<br />
Pro<strong>of</strong>. f takes both its maximum and minimum on I. If the maximum is equal to the minimum, then f(x) is<br />
constant on I, otherwise, either the minium or the maximum is a point x in (a, b). At that point f ′ (x) = 0.<br />
qed. Rolle’s theorem is a special case <strong>of</strong> the mean value theorem<br />
rule <strong>of</strong> three<br />
The [rule <strong>of</strong> three] ia a rough rule <strong>of</strong> thumb when solving calculus problems or teaching calculus:<br />
Look at a calculus problem graphically, numerically and analytically.<br />
In other words, one should try to understand a calculus problem geometrically, algebraically and computationally.<br />
For example, the notion <strong>of</strong> the derivative <strong>of</strong> a function <strong>of</strong> one variable can be understood geometrically as<br />
a slope, can be understood through algebraic manipulations like (x n ) ′ = nx n−1 or computationally by plugging<br />
in numbers or doing things on a computer.<br />
Weierstrass function<br />
A [Weierstrass function] is an example <strong>of</strong> a function which is continuous but almost nowhere differentiable. An<br />
example is f(x) = � ∞<br />
k=1 cos(k2 x)/k 2 .<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 42 entries in this file.
Index<br />
Abel’s partial summation formula, 1<br />
Abel’s test, 1<br />
absolute value, 1<br />
absolutely convergent series, 5<br />
accumulation point, 1<br />
Achilles paradox, 1<br />
acute, 2<br />
addition formulas, 1<br />
alternating series, 2<br />
alternating series test, 2<br />
antiderivative, 2<br />
Arithmetic progression, 2<br />
arrow paradox, 2<br />
asymptotic, 2<br />
Bernstein polynomials, 3<br />
Binomial coefficients, 3<br />
Binominal theorem, 3<br />
bisector, 3<br />
Bolzano’s theorem, 3<br />
Cauchy’s convergence condition, 4<br />
Cauchy’s convergence test, 4<br />
change <strong>of</strong> variables, 5<br />
continuous, 5<br />
converges, 5<br />
differentiable, 6<br />
Extended mean value theorem, 6<br />
factorial, 6<br />
Fermat principle, 3<br />
fundamental theorem <strong>of</strong> calculus, 4<br />
Hopital rule, 7<br />
hyperbola, 7<br />
integration rules, 4<br />
intermediate value theorem, 4<br />
L’Hopital rule, 7<br />
limit, 6<br />
maximum-value theorem, 7<br />
Mean value theorem, 7<br />
parabola, 7<br />
Rolle’s theorem, 8<br />
rule <strong>of</strong> three, 8<br />
series, 5<br />
Weierstrass function, 8<br />
9
<strong>ENTRY</strong> MULTIVARIABLE CALCULUS<br />
[<strong>ENTRY</strong> MULTIVARIABLE CALCULUS] Author: Oliver Knill: March 2000 -March 2004 Literature: Standard<br />
glossary <strong>of</strong> multivariable calculus course as taught at the Harvard mathematics department.<br />
acceleration<br />
The [acceleration] <strong>of</strong> a parametrized curve r(t) = (x(t), y(t), z(t)) is defined as the vector r ′′ (t). It is the rate <strong>of</strong><br />
change <strong>of</strong> the velocity r ′ (t). It is significant, because Newtons law relates the acceleration r ′′ (t) <strong>of</strong> a mass point<br />
<strong>of</strong> mass m with the force F acting on it: mr ′′ (t) = F (r(t)) . This ordinary differential equation determines<br />
completely the motion <strong>of</strong> the particle.<br />
advection equation<br />
The [advection equation] ut = cux is a linear partial differential equation. Its general solution is u(t,x)=f(x+ct),<br />
where f(x)=u(0,x). The advection equation is also called transport equation. In higher dimensions, it generalizes<br />
to the gradient flow ut = cgrad(u).<br />
Archimedes spiral<br />
The [Archimedes spiral] is the plane curve defined in polar coordinates as r(t) = ct, where c is a constant. In<br />
Euclidean coordinates, it is given by the parametrization r(t) = (ct cos(t), ct sin(t)).<br />
axis <strong>of</strong> rotation<br />
The [axis <strong>of</strong> rotation] <strong>of</strong> a rotation in Euclidean space is the set <strong>of</strong> fixed points <strong>of</strong> that rotation.<br />
Antipodes<br />
Two points on the sphere <strong>of</strong> radius r are called [Antipodes] (=anti-podal points) if their Euclidean distance is<br />
maximal 2r. If the sphere is centered at the origin, the antipodal point to (x, y, z) is the point (−x, −y, −z).
The [boundary] <strong>of</strong> a geometric object. Examples:<br />
boundary<br />
• The boundary <strong>of</strong> an interval I = {a ≤ x ≤ b} is the set with two points {a, b}. For example, {0 ≤ x ≤ 1<br />
the boundary {0, 1}.<br />
• The boundary <strong>of</strong> a region G in the plane is the union <strong>of</strong> curves which bound the region. The unit disc<br />
has as a boundary the unit circle. The entire plane has an empty boundary.<br />
• The boundary <strong>of</strong> a surface S in space is the union <strong>of</strong> curves which bound the surface. For example: A<br />
semisphere has as the boundary the equator. The entire sphere has an empty boundary.<br />
• The boundary <strong>of</strong> a region G in space is the union <strong>of</strong> surfaces which bound the region. For example, the<br />
unit ball has the unit sphere as a boundary. A cube has as a boundary the union <strong>of</strong> 6 faces.<br />
• The boundary <strong>of</strong> a curve r(t), t ∈ [a, b] consists <strong>of</strong> the two points r(a), r(b).<br />
The boundary can be defined also in higher dimensions where surfaces are also called manifolds. The dimension<br />
<strong>of</strong> the boundary is always one less then the dimension <strong>of</strong> the object itself. In cases like the half cone, the tip <strong>of</strong><br />
the cone is not considered a part <strong>of</strong> the boundary. It is a singular point which belongs to the surface. While the<br />
boundary can be defined for far more general objects in a mathematical field called ”topology”, the boundaries<br />
<strong>of</strong> objects occuring in multivariable calculus are assumed to be <strong>of</strong> dimension one less than the object itself.<br />
Burger’s equation<br />
The [Burger’s equation] ut = uut is a nonlinear partial differential equation in one dimension. It is a simple<br />
model for the formation <strong>of</strong> shocks.<br />
Cartesian coordinates<br />
[Cartesian coordinates] in three-dimensional space describe a point P with coordinates x, y and z. Other possible<br />
coordinate systems are cylindrical coordinates and spherical coordinates. Going from one coordinate system to<br />
an other is called a coordinate change.<br />
Cavalieri principle<br />
[Cavalieri principle] tells that if two solids have equal heights and their sections at equal distances have have<br />
areas with a given ratio, then the volumes <strong>of</strong> the solids have the same ratio.<br />
change <strong>of</strong> variables<br />
A [change <strong>of</strong> variables] is defined by a coordinate transformation. Examples are changes between cylindrical<br />
coordinates, spherical coordinates or Cartesian coordinates. Often one uses also rotations, allowing to use a<br />
convenient coordinate system, like for example, when one puts a coordinate system so that a surface <strong>of</strong> revolution<br />
has as the symmetry axes the z-axes.
circle<br />
A [circle] is a curve in the plane whose distance from a given point is constant. The fixed point is called the<br />
center <strong>of</strong> the circle. The distance is the radius <strong>of</strong> the circle. One can parametrize a circle by r(t) = (cos(t),sin(t)<br />
or given as an implicit equation g(x, y) = x 2 +y 2 = 1. The circle is an example <strong>of</strong> a conic section, the intersection<br />
<strong>of</strong> a cone with a plane to which ellipses, hyperbola and parabolas belong to.<br />
cone<br />
A [cone] in space is the set <strong>of</strong> points x 2 + y 2 = z 2 in space. Also translates, scaled and rotated versions <strong>of</strong> this<br />
set are still called a cone. For example 2x 2 + 3y 2 = 7z 2 is an elliptical cone.<br />
conic section<br />
A [conic section] is the intersection <strong>of</strong> a cone with a plane. Hyperbola, ellipses and parabola lines and pairs <strong>of</strong><br />
intersecting lines are examples <strong>of</strong> conic sections.<br />
continuity equation<br />
The [continuity equation] is the partial differential equation ρt + div(ρv) = 0, where ρ is the density <strong>of</strong> the<br />
fluid and v is the velocity <strong>of</strong> the fluid. The continuity equation is the consequence <strong>of</strong> the fact that the negative<br />
change <strong>of</strong> mass in a small ball is equal to the amount <strong>of</strong> mass which leaves the ball. The later is the flux <strong>of</strong> the<br />
current j = vρ through the surface and by the divergence theorem the integral <strong>of</strong> div(j).<br />
cos theorem<br />
The [cos theorem] relates the length <strong>of</strong> the edges a,b,c in a triangle ABC with one <strong>of</strong> the angles α: a 2 =<br />
b 2 + c 2 − 2bc cos(α) Especially, if α = π/2, it becomes the theorem <strong>of</strong> Pythagoras.<br />
critical point<br />
A [critical point] <strong>of</strong> a function f(x, y) is a point (x0, y0), where the gradient ∇f(x0, y0) vanishes. Critical points<br />
are also called stationary points. For functions <strong>of</strong> two variables f(x, y), critical points are typically maxima,<br />
minima or saddle points realized by f(x, y) = −x 2 − y 2 , f(x, y) = x 2 + y 2 or f(x, y) = x 2 − y 2 .<br />
chain rule<br />
The [chain rule] expresses the derivative <strong>of</strong> the composition <strong>of</strong> two functions in terms <strong>of</strong> the derivatives <strong>of</strong> the<br />
functions. It is (fg) ′ (x) = f ′ (g(x))g ′ (x). For example, if r(t) is a curve in space and F a function in three<br />
variables, then (d/dt)f(r(t)) = grad(f)·r ′ (t). Example. If T and S are maps on the plane, then (T S) ′ = T ′ (S)S ′ ,<br />
where T’ is the Jacobean <strong>of</strong> T and S’ is the Jacobean <strong>of</strong> S.
change <strong>of</strong> variables<br />
A [change <strong>of</strong> variables] on a region R in Euclidean space is given by an invertible map T : R → T (R). The change<br />
<strong>of</strong> variables formula �<br />
�<br />
f(x) dx =<br />
T (R) R f(T x)det(T ′ (x)) dx allows to evaluate integrals <strong>of</strong> a function f <strong>of</strong> several<br />
variables on a complicated region by integrating on a simple region R. In one dimensions, the change <strong>of</strong> variable<br />
formula is the formula for substitution. Example: (2D polar coordinates) T (r, φ) = (x cos(θ), y sin(θ). with<br />
det(T’)=r maps the rectangle [0, s] × [0, 2π] into the disc. Example <strong>of</strong> 3D spherical coordinates are T (r, θ, φ) =<br />
(r cos(θ) sin(φ), r sin(θ) sin(φ), r cos(φ)), det(T ′ ) = r2 sin(φ) maps the rectangular region (0, s) × (0, 2π0 × (0, π)<br />
onto a sphere <strong>of</strong> radius s.<br />
curl<br />
The [curl] <strong>of</strong> a vector field F = (P, Q, R) in space is the vector field (Ry − Qz, Pz − Rx, Qx − Py). It measures<br />
the amount <strong>of</strong> circulation = vorticity <strong>of</strong> the vector field. The curl <strong>of</strong> a vector field F=(P,Q) in the plane is the<br />
scalar field (Qx − Py). It measures the vorticity <strong>of</strong> the vector field in the plane.<br />
curvature<br />
The [curvature] <strong>of</strong> a parametrized curve r(t) = (x(t),y(t),z(t)) is defined as k(t) = |r ′ (t) × r ′′ (t)|/|r ′ (t)| 3 .<br />
Examples:<br />
• The curvature <strong>of</strong> a line is zero.<br />
• The curvature <strong>of</strong> a circle <strong>of</strong> radius r is 1/r.<br />
curve<br />
A [curve] in space is the image <strong>of</strong> a map X : t− > r(t) = (x(t), y(t), z(t)), where x(t), y(t), z(t) are three<br />
piecewise smooth functions. For general continuous maps x(t), y(t), z(t), the length or the velocity <strong>of</strong> the curve<br />
would no more be defined.<br />
cross product<br />
The [cross product] <strong>of</strong> two vectors v = (v1, v2, v3) and w = (w1, w2, w3) is the vector (v2w3 − w2v3, v3w1 −<br />
w3v1, v1w2 − w2v1).<br />
curve<br />
A [curve] in three-dimensional space is the image <strong>of</strong> a map r(t) = (x(t), y(t), z(t)), where x(t), y(t), z(t) are<br />
three continuous functions. A curve in two-dimensional space is the image <strong>of</strong> a map r(t) = (x(t), y(t)).
cylinder<br />
A [cylinder] is a surface in three dimensional space such that its defining equation f(x,y,z)=0 does not involve one<br />
<strong>of</strong> the variables. For example, z = 2 sin(y) defines a cylinder. A cylinder usually means the surface x 2 + y 2 = r<br />
or a translated rotated version <strong>of</strong> this surface.<br />
derivative<br />
The [derivative] <strong>of</strong> a function f(x) <strong>of</strong> one variable at a point x is the rate <strong>of</strong> change <strong>of</strong> the function at this<br />
point. Formally, it is defined as limdx→0(f(x + dx) − f(x))/dx. One writes f’(x) for the derivative <strong>of</strong> f. The<br />
derivative measures the slope <strong>of</strong> the graph <strong>of</strong> f(x) at the point. If the derivative exists for all x, the function is<br />
called differentiable. Functions like sin(x) or cos(x) are differentiable. One has for example f ′ (x) = cos(x) if<br />
f(x) = sin(x). An example <strong>of</strong> a function which is not differentiable everywhere is f(x)=—x—. The derivative<br />
at 0 is not defined.<br />
cylindrical coordinates<br />
[cylindrical coordinates] in three dimensional space describe a point P by the coordinates r = (x 2 + y 2 + z 2 ) 1/2 ,<br />
phi=arctan(y/x),z, where P=(x,y,z) are the Cartesian coordinates <strong>of</strong> P. Other coordinate systems are Cartesian<br />
coordinates or spherical coordinates.<br />
The [determinant] <strong>of</strong> a matrix A =<br />
� a b<br />
c d<br />
determinant<br />
⎛<br />
�<br />
is ad − bc. The determinant <strong>of</strong> a matrix A = ⎝<br />
a<br />
d<br />
b<br />
e<br />
c<br />
f<br />
g h i<br />
aei + bfg + cdh − ceg − fha − ibd. The determinant is relevant when changing variables in integration.<br />
directional derivative<br />
The [directional derivative] <strong>of</strong> f(x,y,z) in the direction v is the dot product <strong>of</strong> the gradient <strong>of</strong> f with v. It measures<br />
the rate <strong>of</strong> change <strong>of</strong> f at a point P when moving trough the point (x,y,z) with velocity v.<br />
distance<br />
The [distance] <strong>of</strong> two points P=(a,b,c) and Q=(u,v,w) in three dimensional Euclidean space is the square root<br />
<strong>of</strong> (a − u) 2 + (b − v) 2 + (c − w) 2 . The distance <strong>of</strong> two points P=(a,b) and Q = (u, v) in the plane is the square<br />
root <strong>of</strong> (a − u) 2 + (b − v) 2 .<br />
distance<br />
The [distance] between two nonparallel lines in three dimensional Euclidean space is given by the forumla<br />
d = |(v × w) · u|/|(v × w)|, where v and w are arbitrary nonzero vectors in each line and u is an arbitrary vector<br />
connecting a point on the first line to a point <strong>of</strong> the second line.<br />
⎞<br />
⎠ is
divergence<br />
The [divergence] <strong>of</strong> a vector field F=(P,Q,R) is the scalar field div(F ) = Px +Qy +Rz. The value div(F )(x, y, z)<br />
measures the amount <strong>of</strong> expansion <strong>of</strong> the vector field at the point (x, y, z).<br />
dot product<br />
The [dot product] <strong>of</strong> two vectors v = (v1, v2, v3) and w = (w1, w2, w3) is the scalar v1w1 + v2w2 + v3w3.<br />
ellipse<br />
An [ellipse] is the set <strong>of</strong> points in the plane which satisfy an equation (x − a) 2 /A 2 + (y − b) 2 /B 2 = 1. It is<br />
inscribed in a rectangle <strong>of</strong> length A and width B centered at (a, b). Ellipses can also be defined as the set <strong>of</strong><br />
points in the plance whose sum <strong>of</strong> the distances to two points is constants. The two fixed points are called the<br />
foci <strong>of</strong> the ellipse. The line through the foci <strong>of</strong> a noncircular ellipse is called the focal line, the points where<br />
focal axes and a noncircular ellipse cross, are called vertices <strong>of</strong> the ellipse. The major axis <strong>of</strong> the ellipse is the<br />
line segment connecting the two vertices, the minor axis is the symmetry line <strong>of</strong> the ellipse which mirrors the<br />
two focal points or the two vertices. Ellipses are examples <strong>of</strong> conic sections, the intersection <strong>of</strong> a cone with a<br />
plane.<br />
ellipsoid<br />
An [ellipsoid] is the set <strong>of</strong> points in three dimensional Euclidean space, which satisfy an equation (x − a) 2 /A 2 +<br />
(y − b) 2 /B 2 + (z − c) 2 /C 2 = 1. It is inscribed in a box <strong>of</strong> length, width and height A,B,C centered at (a, b, c).<br />
equation <strong>of</strong> motion<br />
The [equation <strong>of</strong> motion] <strong>of</strong> a fluid is the partial differential equation ρDv/dt = −grad(p) + F , where F<br />
are external forces like gravity rho g, or magnetic force j × B and Dv/dt is the total time derivative Dv/dt =<br />
vt+vgrad(v). The term - grad(p) is the pressure force. Together with an incompressibility assumption div(v)=0,<br />
these equations <strong>of</strong> motion are called Navier Stokes equations.<br />
flux integral<br />
The [flux integral] <strong>of</strong> a vector field F through a surface S=X(R) is defined as the double integral <strong>of</strong> X(F).n over<br />
R, where n = Xu × Xv is the normal vector <strong>of</strong> the surface as defined through the parameterization X(u, v).<br />
[Fubinis theorem] tells that � b � d<br />
a c f(x, y) dxdy = � d<br />
c<br />
Fubinis theorem<br />
� b<br />
f(x, y) dydx.<br />
a
gradient<br />
The [gradient] <strong>of</strong> a function f at a point P=(x,y,z) is the vector (fx(x, y, z), fy(x, y, z), fz(x, y, z)) where fx<br />
denotes the partial derivative <strong>of</strong> f with respect to x.<br />
Hamilton equations<br />
The [Hamilton equations] to a function f(x, y) is the system <strong>of</strong> ordinary differential equations x ′ (t) =<br />
fy(x, y), y ′ (t) = −fx(x, y). which is called Hamilton system. Solution curves <strong>of</strong> this system are located on<br />
level curves f(x, y) = c because by the chain rule one has d/dtf(x(t), y(t)) = fxx ′ + fyy ′ = fxfy − fxfy = 0.<br />
The preservation <strong>of</strong> f is in physics called energy conservation.<br />
heat equation<br />
The [heat equation] is the Partial differential equation ut = mu∆(u), where mu is a constant, and ∆u is the<br />
Laplacian <strong>of</strong> u. The heat equation is also called the diffusion equation.<br />
The [Hessian] is the determinant <strong>of</strong> the Hessian matrix.<br />
Hessian<br />
Hessian matrix<br />
The [Hessian matrix] <strong>of</strong> a function f(x,y,z) at a point (u, v, w) is the 3x3 matrix f ′′ ⎛<br />
⎞<br />
(u, v, w) = H(u, v, w) =<br />
⎝<br />
fxx fxy fxz<br />
fyx fyy fyz<br />
fzx fzy fzz �<br />
fxx fxy<br />
H(u, v, w) =<br />
derivative test.<br />
⎠. The Hessian matrix <strong>of</strong> a function f(x, y) at a point (u,v) is the 2x2 matrix f ′′ =<br />
fyx fyy<br />
�<br />
. The Hessian matrix is useful to classify critical points <strong>of</strong> f(x, y) using the second<br />
hyperbola<br />
A [hyperbola] is a plane curve which can be defined as the level curve g(x, y) = x 2 /a 2 + y 2 /b 2 = 1 or given as<br />
a parametrized curve r(t) = (a cosh(t), b sinh(t)). A hyperbola can geometrically also be defined as the set <strong>of</strong><br />
points whose distances from two fixed points in the plane is constant. The two fixed points are called the focal<br />
points <strong>of</strong> the hyperbola. The line through the focal points <strong>of</strong> a hyperbola is called the focal axis. The points,<br />
where the focal axis and the hyperbola cross are called vertices. A hyperbola is an example <strong>of</strong> a conic section,<br />
the intersection <strong>of</strong> a cone with a plane.
hyperboloid<br />
A [hyperboloid] is the set <strong>of</strong> points in three dimensional Euclidean space, which satisfy an equation (x−u) 2 /a 2 −<br />
(y − v) 2 /b 2 − (z − w) 2 /c 2 = I, where I = 1 or I = −1. For a=b=c=1, the hyperboloid is obtained by rotating<br />
a hyperbola x 2 − y 2 = 1 around the x-axes. It is two-sided for I=-1 (the intersection <strong>of</strong> the plane z=c with the<br />
hyperboloid is then empty) and one-sided for I=1.<br />
incompressible<br />
A vector field F is called [incompressible] if its divergence is zero div(F ) = 0. The notation has its origins from<br />
fluid dynamics, where velocity fields F <strong>of</strong> fluids, gases or plasma <strong>of</strong>ten are assumed to be incompressible. If a<br />
vector field is incompressible and is a velocity field, then the corresponding flow preserves the volume.<br />
continuity equation<br />
The [continuity equation] ρt + div(i) = 0 links density ρ and velocity field i. It is an infinitesimal�description � �<br />
which is equivalent to the preservation <strong>of</strong> mass by the theorem <strong>of</strong> Gauss. The change <strong>of</strong> mass M(t) ρ dV R<br />
inside a region R in space is the minus the flux <strong>of</strong> mass through the boundary S <strong>of</strong> R.<br />
interval<br />
An [interval] is a subset <strong>of</strong> the real line defined by two points a,b. One can write I = {a ≤ x ≤ b} for a closed<br />
interval, I = {a < x < b} for an open interval and I = {a ≤ x < b}, I = {a < x ≤ b} for half open intervals. If<br />
a = −∞ and b = ∞, then the interval is the entire real line. If a = 0, b − ∞, then I = (a, b) is the set <strong>of</strong> positive<br />
real numbers. Intervals can be characterized as the connected sets in the real line.<br />
integral<br />
An [integral] <strong>of</strong> f(x) over an interval I on the line is the limit (1/n) �n i=1 f(i/n) for n → ∞ over the integers<br />
and the sum is taken over all i such that i/n is in I. An integral <strong>of</strong> f(x, y) over a region R in the plane is the<br />
limit (1/n2 ) �<br />
(i/n,j/n)∈R f(i/n, j/n) for n → ∞. Such an integral is also called double integral. Often, double<br />
integrals can be evaluated by iterating two one-dimensional integrals. An integral <strong>of</strong> f(x,y,z) over a domain R<br />
in space is the limit (1/n3 ) �<br />
(i/n,j/n,k/n)∈R f(i/n, j/n, k/n) for n to infinity. Such an integral is also called a<br />
triple integral. Often, triple integrals can be evaluated by iterating three one-dimensional integrals.<br />
intercept<br />
An [intercept] is the intersection <strong>of</strong> a surface with a coordinate axes. Like traces, intercepts are useful for<br />
drawing surfaces by hand. For example, the two sheeted hyperboloid x 2 + y 2 − z 2 = −1 has the intercepts<br />
x 2 − z 2 = −1 and y 2 − z 2 = −1 (hyperbola) and an empty intercept with the z axes.
jerk<br />
The [jerk] <strong>of</strong> a parametrized curve r(t)=(x(t),y(t),z(t)) is defined as r”’(t). It is the rate <strong>of</strong> change <strong>of</strong> the<br />
acceleration. By Newtons law, the jerk measures the rate <strong>of</strong> change <strong>of</strong> the force acting on the body.<br />
Lagrange multiplier<br />
A [Lagrange multiplier] is an additional variable introduced for solving extremal problems under constraints.<br />
To extremize f(x, y, z) on a surface g(x, y, z) = 0 then an extremum satisfies the equations f ′ = Lg ′ , g = 0,<br />
where L is the Lagrange multiplier. These are four equations for four unknowns x,y,z,l. Additionally, one has<br />
to check for solutions <strong>of</strong> g ′ (x, y, z) = 0.<br />
Example. If we want to extremize F (x, y, z) = −x log(x) − y log(y) − z log(z) under the constraint G(x, y, z) =<br />
x + y + z = 1, we solve the equations −1 − log(x) = λ1 −1 − log(y) = λ1 −1 − log(z) = λ1 x + y + z = 1, the<br />
solution <strong>of</strong> which is x = y = z = 1/3.<br />
Lagrange method<br />
The [Lagrange method] to solve extremal problems under constraints:<br />
1) in order that a function f <strong>of</strong> several variables is extremal on a constraint set g = c, we either have ∇g = 0<br />
or the point is a solution to the Lagrange equations ∇f = λ∇g, g = c.<br />
2) in order to extremize a function f <strong>of</strong> several variables under the contraint set g = c, h = d, we have to solve<br />
the Lagrange equations ∇f = λ∇g + µ∇h, g = c, h = d or solve ∇g = ∇h = 0.<br />
Laplacian<br />
The [Laplacian] <strong>of</strong> a function f(x, y, z) is defined as ∆(f) = fxx+fyy+fzz. One can write it as ∆ = divgrad(f).<br />
Functions for which the Laplacian vanish are called harmonic. Laplacian appear <strong>of</strong>ten in PDE’s Examples: the<br />
Laplace equation ∆(f) = 0, the Poisson equation ∆(f) = ρ, the Heat equation ft = µ∆(f) or the wave equation<br />
ftt = c 2 ∆f. The [length] <strong>of</strong> a curve r(t)=(x(t),y(t),z(t)) from t=a to t=b is the integral <strong>of</strong> the speed —r’(t)—<br />
over the interval a,b. Example. the length <strong>of</strong> the curve r(t)=(cos(t),sin(t)) from t=0 to t = π is π because the<br />
speed |r ′ (t)| is 1.<br />
length<br />
The [length] <strong>of</strong> a vector v = (a, b, c) is the square root <strong>of</strong> v · v = a 2 + b 2 + c 2 . An other word for length is norm.<br />
If a vector has length 1, it is called normalized or a unit vector.<br />
level curve<br />
A [level curve] <strong>of</strong> a function f(x, y) <strong>of</strong> two variables is the set <strong>of</strong> points which satisfy the equation f(x, y) = c.<br />
For example, if f(x, y) = x 2 −y 2 , then its level curves are hyperbola. Level curves are orthogonal to the gradient<br />
vector field grad(f).
level surface<br />
A [level surface] <strong>of</strong> a scalar function f(x, y, z) is the set <strong>of</strong> points which satisfy f(x, y, z) = c. For example, if<br />
f(x, y, z) = x 2 + y 2 + 3z 2 , then its level surfaces are ellipsoids. Level surfaces are orthogonal to the gradient<br />
field grad(f).<br />
linear approximation<br />
The [linear approximation] <strong>of</strong> a function f(x,y,z) at a point (u, v, w) is the linear function L(x, y, z) = f(u, v, w)+<br />
∇f(u, v, w) · (x − u, y − v, z − w).<br />
line<br />
A [line] in three-dimensional space is a curve in space given by r(t) = P + tv, where P is a point in space and v<br />
is a vector in space. The representation r(t)=P+tv is called a parameterization <strong>of</strong> the line. Algebraically, a line<br />
can also be given as the intersection <strong>of</strong> two planes: ax+by +cz = d, ux+vy +wz = q. The corresponding vector<br />
v in the line is the cross product <strong>of</strong> (a, b, c) and (u, v, w). A point P = (x, y, z) on the line can be obtained by<br />
fixing one <strong>of</strong> the coordinates, say z=0 and solving the system ax + by = d, ux + vy = q for the unknowns x and<br />
y.<br />
line integral<br />
The [line integral] <strong>of</strong> a vector field F (x, y) along a curve C : r(t) = (x(t), y(t)), t ∈ [a, b] in the plane is defined<br />
as � � b<br />
F · ds = F (r(t)) · r ′ (t) dt ,<br />
C<br />
a<br />
where r ′ (t) = (x ′ (t), y ′ (t)) is the velocity. The definition is similar in three dimensions where F (x, y, z) is a<br />
vector field and C : r(t) = (x(t), y(t), z(t)), t ∈ [a, b] is a curve in space.<br />
Maxwell equations<br />
The [Maxwell equations] are a set <strong>of</strong> partial differential equations which determine the electric field E and<br />
magnetic field B, when the charge density ρ and the current density j are given. There are 4 equations:<br />
div(B) = 0 no magnetic monopoles<br />
curl(E) = −Bt/c Faradays law, change <strong>of</strong> magnetic flux produces voltage<br />
curl(B) = Et/c + (4π/c)j Ampere’s law, current or E change produce magnetism<br />
div(E) = 4πρ Gauss law, electric charges produce an electric field<br />
nabla<br />
[nabla] is a mathematical symbol used when writing the gradient ∇f <strong>of</strong> a function f(x, y, z). Nabla looks like<br />
an upside down ∆. Etymologically, the name has the meaning <strong>of</strong> an Egyption harp.
nabla calculus<br />
The [nabla calculus] introduces the vector ∇ = (∂x, ∂y, ∂z). It satisfies ∇(f) = grad(f), ∇xF = curl(F ),<br />
∇ · F = div(F ). Using basic vector operation rules and differentiation rules like ∇(fg) = (∇f)g + f(∇g) one<br />
can verify identities: like for example<br />
div(curl)F = 0, curl(grad)f = 0, curl(curlF ) = grad(divF ) − ∆(F ), div(E × F ) = F · curl(E) − E · curl(F ).<br />
nonparallel<br />
Two vectors v and w are called [nonparallel] if they are not parallel. Two vectors in space are parallel if and<br />
only if their cross product v × w is nonzero.<br />
normal vector<br />
A [normal vector] to a parametrized surface X(u, v) = (x(u, v), y(u, v), z(u, v)) at a point P=(x,y,z) is the vector<br />
XuxXv. It is orthogonal to the tangent plane spanned by the two tangent vectors Xu and Xv.<br />
normalized<br />
A vector is called [normalized] if its length is equal to 1. For example, the vector (3/5, 4/5) is normalized. The<br />
vector (2, 1) is not normalized.<br />
octant<br />
An [octant] is one <strong>of</strong> the 8 regions when dividing three dimensional space with coordinate planes. It is the<br />
analogue <strong>of</strong> quadrant in two dimensions.<br />
open set<br />
An [open set] R in the plane or in space is a set for which every point P is contained in a small disc U which<br />
is still contained in R. The disc x 2 + y 2 < 1 is an example <strong>of</strong> an open set. The set x 2 + y 2 ≤ 1 is not open<br />
because the point (1, 0) for example has no neighborhood disc contained in R.<br />
open<br />
A set is called [open], if it is an open set. It means that every point in the set is contained in a neighborhood<br />
which still is in the set. The complement <strong>of</strong> open sets are called closed.
ordinary differential equation<br />
An [ordinary differential equation] (ODE) is an equation for a function or curve f(t) which relates derivatives<br />
f,f’,f”.... <strong>of</strong> f. An example is f’=c f which has the solution f(t) = Ce ( ct), where C is a constant. Only<br />
derivatives with respect to one variable may appear in an ODE. In most cases, the variable t is associated with<br />
time. Examples:<br />
f ′ = cf population model c > 0.<br />
f ′ = −cf radioactive decay c > 0<br />
f ′ = cf(1 − f) logistic equation<br />
f ′′ = −cf harmonic oscillator<br />
f ′′ = F (f) general form <strong>of</strong> Newton equations<br />
By increasing the dimension <strong>of</strong> the phase space, every ordinary differential equation can be written as a first<br />
order autonomous system x ′ = F (x). For example, f ′′ = −f can be written with the vector x = (x1, x2) = (f, f ′ )<br />
as (x ′ 1, x ′ 2) = (f ′ , f ′′ ) = (f ′ , f) = (x ′ 2, −x ′ 2). There is a 2 × 2 matrix such that x ′ = Ax.<br />
orthogonal<br />
Two vectors v and w are called [orthogonal] if v · w = 0. An other word for orthogonal is perpendicular. The<br />
zero vector 0 is orthogonal to any other vector.<br />
parabola<br />
A [parabola] is a plane curve. It can be defined as the set <strong>of</strong> points which have the same distance to a line and<br />
a point. The line is called the directrix, the point is called the focus <strong>of</strong> the parabola. One can parametrize a<br />
parabola as r(t) = (t, t 2 ). It is also possible to give a parabola as a level curve g(x, y) = y − x 2 = 0 <strong>of</strong> a function<br />
<strong>of</strong> two variables. A parabola is an example <strong>of</strong> a conic section, to which also circles, ellipses and hyperbola<br />
belong.<br />
parallelogram<br />
A [parallelogram] E can be defined as the image <strong>of</strong> the unit square under a map T (s, t) = sv + tw, where u<br />
and v are vectors in the plane. One says, E is spanned by the vectors v and w. The area <strong>of</strong> a parallelogram is<br />
|v × w|.<br />
parallelepiped<br />
A [parallelepiped] E can be defined as the image <strong>of</strong> the unit cube under a linear map T (r, s, t) = ru+sv+tv, where<br />
u,v,w are vectors in space. One says, E is spanned by the vectors u, v and w. The volume <strong>of</strong> a parallelepiped<br />
is |u · (v × w)|.<br />
perpendicular<br />
Two vectors v and w are called [perpendicular] if v · w = 0. An other word for perpendicular is orthogonal. The<br />
zero vector v = 0 is perpendicular to any other vector.
quadratic approximation<br />
The [quadratic approximation] <strong>of</strong> a function f(x,y,z) at a point (u, v, w) is the quadratic function Q(x, y, z) =<br />
L(x, y, z) + [H(u, v, w)(x − u, y − v, z − w)] · (x − u, y − v, z − w)/2, where H(u, v, w) is the Hessian matrix <strong>of</strong> f<br />
at (u, v, w) and where L(x, y, z) is the linear approximation <strong>of</strong> f(x, y, z) at (u, v, w). For example, the function<br />
f(x, y) = 3 + sin(x + y) + cos(x + 2y) has the linear approximation L(x, y) = 4 + x + y and the quadratic<br />
approximation Q(x, y) = 4 + x + y + (x + 2y) 2 /2.<br />
quadrant<br />
A [quadrant] is one <strong>of</strong> the 4 regions when dividing the two dimensional space using coordinate axes. It is the<br />
analogue <strong>of</strong> octant in three dimensions. For example, the set {x > 0, y > 0} is the open upper right quadrant.<br />
The set {x ≥ 0, y ≥ 0} is the closed upper right quadrant.<br />
parallel<br />
Two vectors v and w are called [parallel] if there exists a real number λ such that v = λw. Two vectors in space<br />
are parallel if and only if their cross product v × w is zero.<br />
A [parametrized surface] is defined by a map<br />
parametrized surface<br />
X(u, v) = (x(u, v), y(u, v), z(u, v))<br />
from a region R in the uv-plane to xyz-space. Examples<br />
• Sphere: X(u, v) = (r cos(u) sin(v), r sin(u) sin(v), r cos(v)) R = [0, 2π) × [0, π], u and v are called Euler<br />
angles.<br />
• Plane X(u, v) = P + uU + vV , where P is a point, U,V are vectors and R is the entire plane.<br />
• Surface <strong>of</strong> revolution is parametrized by X(u, v) = (f(v) cos(u), f(v) sin(u), v) where u is an angle measuring<br />
the rotation round the z axes and f(v) is a nonnegative function giving the distance to the z-axes<br />
at the height v.<br />
• A graph <strong>of</strong> a function f(x, y) is parametrized by X(u, v) = (u, v, f(u, v)).<br />
• A torus is parametrized by X(u, v) = (a + b cos(v)) cos(u), (a + b cos(v)) sin(u), sin(v)) on R = [0, 2π) ×<br />
[0, 2π).
parametrized curve<br />
A [parametrized curve] in space is defined by a map r(t) = (x(t), y(t), z(t)) from an interval I to space. Examples<br />
are<br />
• Circle in the xy-plane r(t) = (cos(t), sin(t), 0) with t ∈ [0, 2π].<br />
• Helix r(t) = (cos(t), sin(t), t) with t ∈ [a, b].<br />
• Line r(t) = P + tV , where V is a vector and P is a point and −∞ < t < ∞.<br />
• A line segment connecting P with Q r(t) = P + t(Q − P ), where t ∈ [0, 1].<br />
partial derivative<br />
The [partial derivative] <strong>of</strong> a function <strong>of</strong> several variables f is the derivative with respect to one variable assuming<br />
the other variables are constants. One writes for example fy(x, y, z) for the partial derivative <strong>of</strong> f(x,y,z) with<br />
respect to y.<br />
partial differential equation<br />
A [partial differential equation] is an equation for a function <strong>of</strong> several variables in which partial derivatives<br />
with respect to different variables appear. Examples:<br />
ut = cux<br />
Advection equation<br />
ut = µ∆(u) Heat equation<br />
utt = c 2 ∆(u) Wave equation<br />
utt = c 2 ∆(u) − m 2 u Klein Gordon equation<br />
∆(u) = 0 Laplace equation<br />
∆(u) = ρ Poisson equation<br />
ut + uxxx + 6uux = 0 KdV equation<br />
ut = uux<br />
Burger equation<br />
div(B) = div(E) = 0 Bt = −ccurl(E) Et = ccurl(B) Maxwell equation (vacuum)<br />
ihut = h2 /2m∆u + V u Schroedinger equation<br />
curl(A) = F Vector potential equation<br />
plane<br />
A [plane] in three dimensional space is the set <strong>of</strong> points (x, y, z) which satisfy an equation ax + by + cz = d. A<br />
parametrization <strong>of</strong> a plane is given by the map (s, t) ↦→ X(u, v) = sv + tw, where v, w are two vectors. If three<br />
points P1, P2, P3 are given in space, then X(s, t) = P1 + s(P2 − P1) + t(P3 − P1) is a parametrisation <strong>of</strong> the<br />
plane which contains all three points.<br />
polar coordinates<br />
[polar coordinates] in the plane describe a point P=(x,y) with the coordinate (r, t) where r = (x 2 + y 2 ) 1/2 is<br />
the distance to the origin and t is the angle between the line OP and the x axes. The angle t = arctan(y/x) ∈<br />
(−π/2, π/2] has to be augmented by π if x < 0 or x = 0, y < 0. The Cartesian coordinates <strong>of</strong> P are obtained<br />
from the Polar coordinates as x = r cos(t), y = r sin(t).
potential<br />
A function U(x, y, z) is called a [potential] to a vector field F (x, y, z) if grad(U) = F at all points. The vector<br />
field F is then called conservative or a potential field. Not every vector field is conservative. If curl(F ) = 0<br />
everywhere in space, then F has a potential.<br />
projection<br />
The [projection] <strong>of</strong> a vector v onto a vector w is the vector w(v · w)/|w| 2 . The scalar projection is the length <strong>of</strong><br />
the projection.<br />
right handed<br />
A coordinate system in space is [right handed] if it can be rotated into the situation such that if the z axes<br />
points to the observer <strong>of</strong> the xy plane, then a 90 degree rotation brings the x axes to the y axes. Otherwise<br />
the coordinate system is called left handed. If u is a vector on the positive x axes, v is a vector on the positive<br />
y axes and w is a vector on the positive z axes, then the coordinate system is right handed if and only if the<br />
triple product u · (v × w) is positive.<br />
second derivative test<br />
The [second derivative test]. If the determinant <strong>of</strong> the Hessian matrix det(f ′′ (x, y)) < 0 then (x, y) is a saddle<br />
point. If f ′′ (x, y) > 0 and and fxx(x, y) < 0 then (x, y) is a local maximum. If det(f ′′ (x, y)) < 0 and<br />
fxx(x, y) > 0 then (x, y) is a local minimum.<br />
Space<br />
[Space] is usually used as an abbreviation for three dimensional Euclidean space. In a wider sense, it can mean<br />
linear space a vector space in which on can add and scale.<br />
speed<br />
The [speed] <strong>of</strong> a curve r(t) = (x(t), y(t), z(t)) at time t is the length <strong>of</strong> the velocity vector r ′ (t) =<br />
(x ′ (t), y ′ (t), z ′ (t)).<br />
sphere<br />
A [sphere] is the set <strong>of</strong> points in space, which have a given distance r from a point P=(a,b,c). It is the set<br />
(x − a) 2 + (y − b) 2 + (z − c) 2 = r 2 . For a=b=c=0,r=1 one obtains the unit sphere: x 2 + y 2 + z 2 = 1. Spheres can<br />
be define in any dimenesions. A sphere in two dimensions is a circle. A sphere in 1 dimension is the union <strong>of</strong> two<br />
points. The unit sphere in 4 dimensions is the set <strong>of</strong> points (x, y, z, w) ∈ R 4 which satisfy x 2 + y 2 + z 2 + w 2 = 1<br />
Spheres can be defined in any space equiped with a distance like d((x, y), (u, v)) = |x − u| + |y − v| in the plane.
superformula<br />
The [superformula] describes a class <strong>of</strong> curves with a few parameters m, n1, n2, n3, a, b. It is the polar graph<br />
r(t) = (| cos(mt/4)| n1 /a + | sin(mt/4)| n2 /b) −1/n3 .<br />
It had been proposed by the Belgian Biologist Johan Gielis in 1997.<br />
superposition<br />
The principle <strong>of</strong> [superposition] tells that the sum <strong>of</strong> two solutions <strong>of</strong> a linear partial differential equation (PDE)<br />
is again a solution <strong>of</strong> the PDE. For example, f(x, y) = sin(x − t) and g(x, y) = e x−t are both solutions to the<br />
transport equation ft(t, x) + fx(t, x) = 0. Therefore also the sum sin(x − t) + e x−t is a solution. For nonlinear<br />
partial differential equations the superposition principle is no more true which is one <strong>of</strong> the reasons for the<br />
difficulty with dealing with nonlinear systems.<br />
surface<br />
A [surface] can either be described as a parametrized surface or implicitely as a level surface g(x, y, z) = 0. In<br />
the first case, the surface is given as the image <strong>of</strong> a map X : (u, v) ↦→ (x(u, v), y(u, v), z(u, v)) where u,v ranges<br />
over a parameter domain R in the plane. In the second case, the surface is determined by a function <strong>of</strong> three<br />
variables. Sometimes, one can describe a surface in both ways like in the following examples:<br />
Sphere: X(u, v) = (r cos(u) sin(v), r sin(u) sin(v), r cos(v)), g(x, y, z) = x 2 + y 2 + z 2 = r 2<br />
Graphs: X(u, v) = (u, v, f(u, v)), g(x, y, z) = z − f(x, y) = 0<br />
Planes: X(u, v) = P + uU + vV , g(x, y, z) = ax + by + cz = d, (a, b, c) = UxV .<br />
Surface <strong>of</strong> revolution: X(u, v) = (f(v) cos(u), f(v) sin(u), v), g(x, y, z) = f((x 2 + y 2 ) ( 1/2)) − z = 0<br />
surface <strong>of</strong> revolution<br />
A [surface <strong>of</strong> revolution] is a surface which is obtained by rotating a curve around a fixed line. If that line<br />
is the z-axes, the surface can be given in cylindrical coordinates as r = f(z). A parametrization is X(t, z) =<br />
(f(z) cos(t), f(z) sin(t), z).<br />
� 2π<br />
0<br />
surface area<br />
� �<br />
The [surface area] <strong>of</strong> surface S = X(R) is defined as the integral <strong>of</strong> R |Xu × Xv(u, v)| dudv. For example,<br />
for X(u, v) = (r cos(u) sin(v), r sin(u) sin(v), r cos(v)) on R = {0 ≤ u ≤ 2π, 0 ≤ v ≤ π}, where S = X(R)<br />
is the sphere <strong>of</strong> radius r, one has Xu × Xv = r sin(v)X and |Xu × Xv| = sin(v)r2 � π<br />
0<br />
. The surface area is<br />
r2 sin(v) dudv = 4πr2 .<br />
surface integral<br />
A [surface integral] <strong>of</strong> a function f(x, y, z) over a surface S = X(R) is defined as the integral <strong>of</strong> f(X(u, v))|Xu ×<br />
Xv(u, v)| over R. In the special case when f(x, y, z) = 1, the surface integral is the surface area <strong>of</strong> the surface<br />
S.
tangent plane<br />
The [tangent plane] to an implicitely defined surface g(x, y, z) = c at the point (x0, y0, z0) is the plane ax + by +<br />
cz = d, where (a, b, c) = ∇f(x0, y0, z0) is the gradient <strong>of</strong> g at (x0, y0, z0) and d = ax0 + by0 + cz0.<br />
tangent line<br />
The [tangent line] to an implicitely defined curve g(x, y) = c at the point (x0, y0) is the line ax + by = d, where<br />
(a, b) is the gradient <strong>of</strong> g(x, y) at the point (x0, y0) and d = ax0 + by0.<br />
theorem <strong>of</strong> Clairot<br />
The [theorem <strong>of</strong> Clairot] assures that one can interchange the order <strong>of</strong> differentiation when taking partial<br />
derivatives. More precicely, if f(x, y) is a function <strong>of</strong> two variables for which both fxy = fyx are continuous,<br />
then fxy = fyx.<br />
theorem <strong>of</strong> Gauss<br />
The [theorem <strong>of</strong> Gauss] states that the flux <strong>of</strong> a vector field F through the boundary S <strong>of</strong> a solid R in threedimensional<br />
space is the integral <strong>of</strong> the divergence div(F) <strong>of</strong> F over the region R:<br />
� � �<br />
� �<br />
div(F ) dV = F · dS .<br />
R<br />
S<br />
theorem <strong>of</strong> Green<br />
The [theorem <strong>of</strong> Green] states that the integral <strong>of</strong> the curl(F ) = Qx − Py <strong>of</strong> a vector field F = (P, Q) over a<br />
region R in the plane is the same as the line integral <strong>of</strong> F along the boundary C <strong>of</strong> R.<br />
� �<br />
�<br />
curl(F ) dA = F ds .<br />
R<br />
The boundary C is traced in such a way that the region is to the left. The boundary has to be piecewise smooth.<br />
The theorem <strong>of</strong> Green can be derived from the theorem <strong>of</strong> Stokes.<br />
[Green’s theorem] see theorem <strong>of</strong> Green.<br />
C<br />
Green’s theorem<br />
Green’s theorem<br />
The determinant <strong>of</strong> the Jacobean matrix is <strong>of</strong>ten called Jacobean or Jacobean determinant.
Jacobean matrix<br />
[Jacobean matrix] If T (u, v) = (f(u, v), g(u, � v)) is a transformation � from a region R to a region S in the plane,<br />
fu(u, v) fv(u, v)<br />
the Jacobean matrix dT is defined as<br />
. It is the linearization <strong>of</strong> T near (u, v). Its<br />
gu(u, v) gv(u, v)<br />
determinant called the Jacobean determiant measures the area change <strong>of</strong> a small area element dA = dudv when<br />
maped by T . For example, if T (r, θ) = (r cos(θ), r sin(θ)) = (x, � y) is the coordinate �transformation<br />
which maps<br />
cos(θ) sin(θ)<br />
R = {r ≥ 0, θ ∈ [0, 2π)} to the plane, then dT is the matrix<br />
which has determinant r.<br />
−r sin(θ) r cos(θ)<br />
theorem <strong>of</strong> Stokes<br />
The [theorem <strong>of</strong> Stokes] states that the flux <strong>of</strong> a vector field F in space through a surface S is equal to the line<br />
integral <strong>of</strong> F along the boundary C <strong>of</strong> S:<br />
� �<br />
�<br />
curl(F ) · dS = F ds .<br />
S<br />
three dimensional space<br />
The [three dimensional space] consists <strong>of</strong> all points (x, y, z) where x, y, z ranges over the set <strong>of</strong> real numbers.<br />
To distinguish it from other three-dimensional spaces, one calls it also Euclidean space.<br />
torus<br />
A [torus] is a surface in space defined as the set <strong>of</strong> points which have a fixed distance from a circle. It can be<br />
parametrized by X(u, v) = (a + b cos(v)) cos(u), (a + b cos(v)) sin(u), sin(v)) on R = [0, 2π) × [0, 2π), where a, b<br />
are positive constants.<br />
trace<br />
The [trace] <strong>of</strong> a surface in three dimensional space is the intersection <strong>of</strong> the surface with one <strong>of</strong> the coordinate<br />
planes x=0 or y=0 or z=0. Traces help to draw a surface when given the task to do so by hand. Other marking<br />
points are intercepts, the intersection <strong>of</strong> the surface with the coordinate axes.<br />
triangle<br />
A [triangle] in the plane or in space is defined by three points P, Q, R. If v = P Q, w = P R, then |v × w|/2 is<br />
the area <strong>of</strong> the triangle.<br />
C<br />
triple product<br />
The [triple product] between three vectors u, v, w in space is defined as the scalar u · (v × w). The absolute<br />
value |u · (v × w)| is the volume <strong>of</strong> the paralelepiped spanned by u, v and w.
[triple dot product] (see triple product).<br />
triple dot product<br />
unit sphere<br />
The [unit sphere] is the sphere x 2 + y 2 + z 2 = 1. It is an example <strong>of</strong> a two-dimensional surface in three<br />
dimensional space.<br />
unit tangent vector<br />
The [unit tangent vector] to a parametrized curve r(t)=(x(t),y(t),z(t)) is the normalized velocity vector T (t) =<br />
r ′ (t)/|r ′ (t)|. Together with the normal vector N(t) = T ′ (t)/|T ′ (t)| and the binormal vector B(t) = T (t)xN(t),<br />
it forms a triple <strong>of</strong> mutually orthogonal vectors.<br />
vector<br />
A [vector] in the plane is defined by two points P, Q. It is the line segment v pointing from P to Q. If P = (a, b)<br />
and Q = (c, d) then the coordinates <strong>of</strong> the vector are v = (c − a, d − b). Points P in the plane can be identified<br />
by vectors pointing from 0 to P. A vector in space is defined by two points P,Q in space. If P = (a, b, c) and<br />
Q = (d, e, f), then the coordinates <strong>of</strong> the vector are v = (d − a, e − b, f − c). Points P in space can be identified<br />
by vectors pointing from 0 to P . Two vectors which can be translated into each other are considered equal.<br />
Remarks.<br />
• One could define vectors more precisely as affine vectors and introduce an equivalence relation among<br />
them: two vectors are equivalent if they can be translated into each other. The equivalence classes are the<br />
vectors one deals with in calculus. Since the concept <strong>of</strong> equivalence relation would unnessesarily confuse<br />
students, the more fuzzy definition above is prefered.<br />
• One should avoid definitions like ”Vectors are objects which have length and direction” given in some<br />
Encyclopedias. The zero vector (0, 0, 0) is an example <strong>of</strong> an object which has length but no direction. It<br />
nevertheless is a vector.<br />
vector field<br />
A [vector field] in the plane is a map F (x, y) = (P (x, y), Q(x, y)) which assigns to each point (x, y) in the<br />
plane a vector F (x, y). An example <strong>of</strong> a vector field in the plane is F (x, y) = (−y, x). An other example is<br />
the gradient field F (x, y) = ∇f(x, y) where f(x, y) is a function. A vector field in space is a map F (x, y, z) =<br />
(P (x, y, z), Q(x, y, z), R(x, y, z)) which assigns to each point (x, y, z) in space a vector F (x, y, z). An example is<br />
the vector field F (x, y, z) = (x 2 , yz, x − y). An other example is the gradient field F (x, y, z) = ∇f(x, y, z) <strong>of</strong> a<br />
function f(x, y, z).<br />
velocity<br />
The [velocity] <strong>of</strong> a parametrized curve r(t)=(x(t),y(t),z(t)) at time t is the vector r ′ (t) = (x ′ (t), y ′ (t), z ′ (t)). It<br />
is tangent to the curve at the point r(t).
volume<br />
The [volume] <strong>of</strong> a body G is defined as the integral <strong>of</strong> the constant function f(x,y,z)=1 over the body G.<br />
wave equation<br />
The [wave equation] is the partial differential equation utt = c 2 ∆(u), where ∆(u) is the Laplacian <strong>of</strong> u.<br />
Light in vacuum satisfies the wave equation. This can be derived from the Maxwell equations: the identity<br />
∆(B) = grad(div(B) − curl(curl(B)) gives together with div(B) = 0 and curl(B) = Et/c the relation<br />
∆(B) = −d/dtcurl(E)/c which leads with the Maxwell equation Bt = −ccurl(E) to the wave equation<br />
∆B = Btt/c 2 . The equation Ett = c 2 ∆E is derived in the same way.<br />
zero vector<br />
The [zero vector] is the vector for which all components are zero. In the plane it is v = (0, 0), in space it is<br />
v = (0, 0, 0). The zero vector is a vector. It has length 0 and no direction. Definitions like ”a vector is a quantity<br />
which has both length and direction” are misleading.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 119 entries in this file.
Index<br />
acceleration, 1<br />
advection equation, 1<br />
Antipodes, 1<br />
Archimedes spiral, 1<br />
axis <strong>of</strong> rotation, 1<br />
boundary, 2<br />
Burger’s equation, 2<br />
Cartesian coordinates, 2<br />
Cavalieri principle, 2<br />
chain rule, 3<br />
change <strong>of</strong> variables, 2, 4<br />
circle, 3<br />
cone, 3<br />
conic section, 3<br />
continuity equation, 3, 8<br />
cos theorem, 3<br />
critical point, 3<br />
cross product, 4<br />
curl, 4<br />
curvature, 4<br />
curve, 4<br />
cylinder, 5<br />
cylindrical coordinates, 5<br />
derivative, 5<br />
determinant, 5<br />
directional derivative, 5<br />
distance, 5<br />
divergence, 6<br />
dot product, 6<br />
ellipse, 6<br />
ellipsoid, 6<br />
equation <strong>of</strong> motion, 6<br />
flux integral, 6<br />
Fubinis theorem, 6<br />
gradient, 7<br />
Green’s theorem, 17<br />
Hamilton equations, 7<br />
heat equation, 7<br />
Hessian, 7<br />
Hessian matrix, 7<br />
hyperbola, 7<br />
hyperboloid, 8<br />
incompressible, 8<br />
integral, 8<br />
intercept, 8<br />
interval, 8<br />
Jacobean matrix, 18<br />
jerk, 9<br />
Lagrange method, 9<br />
Lagrange multiplier, 9<br />
Laplacian, 9<br />
length, 9<br />
21<br />
level curve, 9<br />
level surface, 10<br />
line, 10<br />
line integral, 10<br />
linear approximation, 10<br />
Maxwell equations, 10<br />
nabla, 10<br />
nabla calculus, 11<br />
nonparallel, 11<br />
normal vector, 11<br />
normalized, 11<br />
octant, 11<br />
open, 11<br />
open set, 11<br />
ordinary differential equation, 12<br />
orthogonal, 12<br />
parabola, 12<br />
parallel, 13<br />
parallelepiped, 12<br />
parallelogram, 12<br />
parametrized curve, 14<br />
parametrized surface, 13<br />
partial derivative, 14<br />
partial differential equation, 14<br />
perpendicular, 12<br />
plane, 14<br />
polar coordinates, 14<br />
potential, 15<br />
projection, 15<br />
quadrant, 13<br />
quadratic approximation, 13<br />
right handed, 15<br />
second derivative test, 15<br />
Space, 15<br />
speed, 15<br />
sphere, 15<br />
superformula, 16<br />
superposition, 16<br />
surface, 16<br />
surface area, 16<br />
surface integral, 16<br />
surface <strong>of</strong> revolution, 16<br />
tangent line, 17<br />
tangent plane, 17<br />
theorem <strong>of</strong> Clairot, 17<br />
theorem <strong>of</strong> Gauss, 17<br />
theorem <strong>of</strong> Green, 17<br />
theorem <strong>of</strong> Stokes, 18<br />
three dimensional space, 18<br />
torus, 18<br />
trace, 18<br />
triangle, 18<br />
triple dot product, 19
triple product, 18<br />
unit sphere, 19<br />
unit tangent vector, 19<br />
vector, 19<br />
vector field, 19<br />
velocity, 19<br />
volume, 20<br />
wave equation, 20<br />
zero vector, 20
<strong>ENTRY</strong> LINEAR ALGEBRA<br />
[<strong>ENTRY</strong> LINEAR ALGEBRA] Author: Oliver Knill: Spring 2002-Spring 2004 Literature: Standard glossary<br />
<strong>of</strong> multivariable calculus course as taught at the Harvard mathematics department.<br />
adjacency matrix<br />
The [adjacency matrix] <strong>of</strong> a graph is a matrix Aij, where Aij = 1 whenever there is an edge from node i to<br />
node j in the graph. Otherwise, Aij ⎛ ⎞<br />
= 0. Example: the graph with three nodes with the shape <strong>of</strong> a V has the<br />
0 1 0<br />
adjacency matrix A = ⎝ 1 0 1 ⎠, where node 2 is conneced to both node 1 and 3 and node 1 and 3 are not<br />
0 1 0<br />
connected to each other.<br />
affine transformation<br />
An [affine transformation] is the composition <strong>of</strong> a linear transformation with a shift like for example: T (x, y) =<br />
(2x + y, 3x + 4y) + (2, 3).<br />
Algebra<br />
[Algebra] was originally the art <strong>of</strong> solving equations and systems <strong>of</strong> equations. The word comves from the Arabic<br />
”al-jabr” meaning ”restauration”. The term was used by Mohammed al-Khowarizmi, who worked in Bhagdad.<br />
algebraic multiplicity<br />
The [algebraic multiplicity] <strong>of</strong> a root y <strong>of</strong> a polynomial p is the maximal integer k for which p(x) = (x−y) k q(x).<br />
The algebraic multiplicity is bigger or equal than the geometric multiplicity.<br />
angle<br />
The [angle] between two vectors v and w is arccos((x · y)/(||x||||y||), where x ˙y is the dot product between x and<br />
y and ||x|| = √ x · x is the length <strong>of</strong> x. The inverse <strong>of</strong> cos gives two angles in [0, 2π]. One usually choses the<br />
smaller angle.<br />
argument<br />
The [argument] <strong>of</strong> a complex number z = x + iy is φ if z = re iφ . The argument is determined only up to<br />
addition <strong>of</strong> 2π. It can be determined as φ = arctan(y/x) + A, where A = 0 if x > 0 or x = 0, y > 0 and A = π<br />
if x < 0 or x = 0 and y < 0. For example, arg(i) = π/2 and arg(−i) = 3pi/2. The argument is the imaginary<br />
part <strong>of</strong> log(z) because log(re iphi ) = log(r) + iφ.
associative law<br />
The [associative law] is (AB)C = A(BC). It is an identity which some mathematical operations satisfy. For<br />
example, the matrix multiplication satisfies the associative law. One says also, that the operation is associative.<br />
An example <strong>of</strong> a product which is not associative is the cross product v × w: if i, j, k are the standard basis<br />
vectors, then i × (i × j) = i × k = −j and (i × i) × j = 0 × j = 0.<br />
augmented matrix<br />
The [augmented matrix] <strong>of</strong> a linear equation Ax = b is the n × (n + 1) matrix � A b � . One considers the<br />
augmented matrix when solving a linear system Ax = b. The reduced row echelon form rref � A b � contains<br />
the solution vector x in the last column, if a solution exists. More generally, a matrix which contains a given<br />
matrix as a submatrix is called an augmented matrix.<br />
basis<br />
A [basis] <strong>of</strong> a linear space is a finite set <strong>of</strong> vectors v1, ..., vn, which are linearly independent and which span the<br />
linear space. If the basis contains n vectors, the vector space has dimension n.<br />
basis theorem<br />
The [basis theorem] states that d linearly independent vectors in a vector space <strong>of</strong> dimension d forms a basis.<br />
block matrix<br />
A [block matrix] is a matrix A, where the only non-zero elements are contained in a sequence <strong>of</strong> smaller square<br />
matrices arranged ⎛ along the main ⎞ diagonal <strong>of</strong> A. Such matrices are also called block diagonal matrices. The<br />
1 2 0 0 0<br />
⎜ 3 2 0 0 0 ⎟<br />
matrix A = ⎜ 0 0 5 0 0 ⎟<br />
⎟.<br />
is an example <strong>of</strong> a block-diagonal matrix containing a two 2x2, and a 1x1<br />
⎝ 0 0 0 6 7 ⎠<br />
0 0 0 8 9<br />
matrix in its diagonal.<br />
Cauchy-Schwarz inequality<br />
The [Cauchy-Schwarz inequality] tells that |x · y| is smaller or equal to ||x|| ||y||. Equality holds if and only if x<br />
and y are parallel vectors.<br />
Cayley-Hamilton theorem<br />
The [Cayley-Hamilton theorem] assures that every square matrix A satisfies p(A) = 0, where p(x) = det(A − x)<br />
is the characteristic polynomial <strong>of</strong> A and the right hand side 0 is the zero matrix.
change <strong>of</strong> basis<br />
A [change <strong>of</strong> basis] from an old basis<br />
vj to a new basis<br />
wj is described by an invertible matrix S which relates the coordinates (a1, ..., an) <strong>of</strong> a vector a = �<br />
i aivi<br />
in the old v-basis with the coordinates (b1, ..., bn) <strong>of</strong> the same vector b = �<br />
i biwi in the new w-basis. The<br />
relation <strong>of</strong> the coordinates is b = Sa In that case, one has vj = �<br />
j ST ijwj, where ST is the transpose <strong>of</strong> S.<br />
For example if v1 = (1, 0), v2 = (0, 1), w1 = (3, 4)w2 = (2, �3), then�a = (a1, a2) = (5, 7) in the v-basis has the<br />
3 2<br />
coordinates b = (b1, b2) = (1, 1) in the w-basis. With S =<br />
and S<br />
4 3<br />
T � �<br />
3 4<br />
=<br />
we have b = Sa and<br />
2 3<br />
w1 = 3v1 + 4v2, w2 = 2v1 + 3v2.<br />
characteristic matrix<br />
The [characteristic matrix] <strong>of</strong> a square matrix A is the matrix A(x) = (xI − A) , where I is the identity matrix.<br />
The characteristic matrix is a function <strong>of</strong> the free variable x.<br />
characteristic polynomial<br />
The [characteristic polynomial] <strong>of</strong> a matrix A is the polynomial p(x) = det(xI − A), where I is the identity<br />
matrix. It has the form p(x) = x n − tr(A)x ( n − 1) + ... + (−1) n det(A) where tr(A) is the trace <strong>of</strong> A and det(A)<br />
is the determinant <strong>of</strong> the matrix A. The eigenvalues <strong>of</strong> A are the roots <strong>of</strong> the characteristic polynomial <strong>of</strong> A.<br />
Cholesky factoriztion<br />
The [Cholesky factoriztion] <strong>of</strong> a symmetric and positive definite matrix A is A = R T R, where R is upper<br />
triangular with positive diagonal entries.<br />
circulant matrix<br />
A [circulant matrix] is a square matrix, where the entries in each diagonal are constant. ⎛<br />
0<br />
If S is⎞the shift<br />
1 0<br />
matrix which has 1 in the side diagonal and 0 everywhere else like in the 3x3 case: S = ⎝ 0 0 1 ⎠, then a<br />
1 0 0<br />
circular matrix can be written as A = a0 + a1S + ... + an−1Sn−1 . A general 3x3 circulant matrix has the form<br />
A = a + bS + cS2 ⎛ ⎞<br />
a b c<br />
which is S = ⎝ c a b ⎠.<br />
b c a<br />
classical adjoint<br />
The [classical adjoint] adj(A) <strong>of</strong> a n×n matrix A is the n×n matrix whose entry aij is aij = (−1) ( i+j)det(Aji),<br />
where Aji is a minor <strong>of</strong> A. The classical adjoint plays a role in Cramer’s rule A ( − 1) = adj(A)/det(A). The<br />
name ”adjoint” comes from the fact that we have a change indices like in the adjoint. However, the classical<br />
adjoint has nothing to do with the adjoint.
codomain<br />
The [codomain] <strong>of</strong> a linear transformation T : X → Y is the target space Y . The name has its origin from<br />
naming X the domain <strong>of</strong> A.<br />
c<strong>of</strong>actor<br />
A [c<strong>of</strong>actor] Cij <strong>of</strong> a n × n matrix A is the determinant <strong>of</strong> the (n − 1) × (n − 1) matrix obtained by removing<br />
row i and column j from A and multiplying the result with (−1) i+j .<br />
coefficient<br />
A [coefficient] <strong>of</strong> a matrix A is an entry Aij in the i’th row and the j’th column. For a real matrix, all entries<br />
are real numbers, for a complex matrix, the entries can be complex numbers.<br />
⎜<br />
A [column] <strong>of</strong> a matrix is one <strong>of</strong> the vectors ⎜<br />
⎝<br />
in the image <strong>of</strong> the transformation x ↦→ A(x).<br />
The matrix A defining a linear equation Ax=b or<br />
⎛<br />
A11<br />
A21<br />
A31<br />
. . .<br />
Am1<br />
column<br />
⎞<br />
⎛<br />
⎟<br />
⎠ ,<br />
⎜<br />
⎝<br />
column<br />
A1n<br />
A2n<br />
A3n<br />
. . .<br />
Amn<br />
⎞<br />
A11x1 + . . . A1nxn = b1<br />
. . . = . . .<br />
Am1x1 + . . . Amnxn = bm<br />
⎟ <strong>of</strong> a m × n matrix A. Column vectors are<br />
⎠<br />
is called the [coefficient matrix] <strong>of</strong> the system. The augmented matrix is the m × (n + 1) matrix � A b � ,<br />
where b forms an additional column.<br />
column picture<br />
The [column picture] <strong>of</strong> a linear equation Ax = b is that the vector b becomes a linear combination <strong>of</strong> the<br />
columns <strong>of</strong> A. The linear equation is solvable if the vector b is in the column space <strong>of</strong> A.<br />
column space<br />
The [column space] <strong>of</strong> a matrix A is the linear space spanned by the columns <strong>of</strong> A.
commuting matrices<br />
Two [commuting matrices] A, B satisfy AB = BA. In that case, if A is diagonalizable, then also B is diagonalizable<br />
and both A and B share the same n eigenvectors.<br />
commutative law<br />
The [commutative law] A ∗ B = B ∗ A for some operation ∗ is an identity which holds for certain operations like<br />
the addition <strong>of</strong> matrices. Other operations like the multiplication <strong>of</strong> matrices does not satisfy the commutative<br />
law. One says: matrix multiplication is not commutative.<br />
complex conjugate<br />
The [complex conjugate] <strong>of</strong> a complex number z = x + iy is the complex number x − iy. It has the same length<br />
|z| as z.<br />
Complex numbers<br />
[Complex numbers] form an extension <strong>of</strong> the real numbers. They are obtained by introducing i = (−1) 1/2 and<br />
extending the rules <strong>of</strong> addition (a + ib) + (c + id) = (a + c) + i(b + d) and multiplication (a + ib)(c + id) =<br />
(ac − bd) + i(ad + bc). The absolute value r = |x + iy| is the length <strong>of</strong> the vector (a, b). The argument <strong>of</strong><br />
z, φ = arg(z) is defined as the angle in [0, 2π) between the x axes and the vector (a, b). Using these polar<br />
coordinates one can see the Euler identity z = r exp(iφ) = r cos(φ) + ir sin(φ).<br />
consistent<br />
A system <strong>of</strong> linear equations Ax = b is called [consistent], if there exists for every vector b a solution vector x<br />
to the equation Ax=b. If the system has no solution, the system is called inconsistent.<br />
continuous dynamical system<br />
A [continuous dynamical system] is defined by an ordinary differential equation d/dtu = f(u) where u = u(t) is<br />
a vector valued function and f(u) is a vector field. If f(u) is linear, the equation has the form d/dtu = Au. The<br />
name ”continuous” comes from the fact that the time variable t is taken in the continuum. This distinguishes<br />
the system from discrete dynamical systems u(t+1) = f(u(t)) determined by a map f and where t is an integer.<br />
For linear continuous dynamical systems, the origin 0 is invariant. The origin is called asymptotically stable<br />
if x(t) → 0 for all initial conditions x(0). For continuous dynamical systems ut = Au, this is equivalent with<br />
the requirement that all eigenvalues <strong>of</strong> A have a negative real part. In two dimensions, where the trace and<br />
the determinant determine the eigenvalues, linear stability is characterized by det(A) > 0, tr(A) < 0 (stability<br />
quadrant).
covariance matrix<br />
A [covariance matrix] A <strong>of</strong> two finite dimensional random variables x, y with expectation E[x] = E[y] = 0 is<br />
defined as Aij = E[xiyj], where E[x] = (x1 + ... + xn)/n is the mean or expectation <strong>of</strong> x. The covariance matrix<br />
is always symmetric. If the covariance matrix is diagonal, the random variables x, y are called uncorrelated.<br />
Cramer’s rule<br />
[Cramer’s rule] tells that a solution x <strong>of</strong> a linear equation Ax = b can be obtained as xi = det(Ai)/det(A),<br />
where Ai is the matrix obtained by replacing the column i <strong>of</strong> A with the vector b.<br />
de Moivre formula<br />
The [de Moivre formula] is (cos(x)+i sin(x)) n = cos(nx)+i sin(nx). It is useful to derive trigonometric identities<br />
like cos(x) 3 − 3 sin(x) 2 cos(x) = cos(3x).<br />
determinant<br />
The [determinant] <strong>of</strong> a n × n square matrix A is the sum over all products A[1, π(1)]...A[n, π(n)](−1) π , where<br />
π runs over all permutations <strong>of</strong> {1, 2, ..., n} and (−1) π is the sign <strong>of</strong> the permutation π. Example: ⎛ for a 2 × ⎞2<br />
� �<br />
a b c<br />
a b<br />
matrix A =<br />
the determinant is det(A) = ad − bc. Example: For a 3x3 matrix A = ⎝ d e f ⎠,<br />
c d<br />
g h i<br />
the determinant is det(A) = aei + bfg + cdh − ceg − bfg − cdh. Properties <strong>of</strong> the determinant are det(AB) =<br />
det(A)det(B), det(AT ) = det(A), det(A−1 ) = 1/det(A).<br />
differential equation<br />
A [differential equation] is an equation for a function f in one or several variables which involves derivatives<br />
with respect to these variables. An ordinary differential equation is a differential equation, where derivatives<br />
appear only with respect to one variable. By adding new variables if necessary (for example for t, or derivatives<br />
ut, utt etc, one can write an ordinary differential equation always in the form xt = f(x).<br />
dilation<br />
A [dilation] is a linear transformation x → bx. Dilations scale each vector v by the factor b but leave the<br />
direction <strong>of</strong> v invariant.<br />
dimension<br />
The [dimension] <strong>of</strong> a vector space X is the number <strong>of</strong> basis vectors in a basis <strong>of</strong> X.
distributive law<br />
The [distributive law] is A ∗ (B + C) = A ∗ B + A ∗ C. The set <strong>of</strong> matrices with matrix multiplication * and<br />
addition + is an example where the distributive law applies.<br />
dot product<br />
The [dot product] v · w <strong>of</strong> two vectors v and w is the sum <strong>of</strong> the products viwi <strong>of</strong> their components vi, wi. For<br />
complex vectors, the dot product is defined as �<br />
i viwi. Examples:<br />
• (3, 2, 1) · (1, 2, −1) = 6.<br />
• if v · w = 0, then the vectors are orthogonal.<br />
• the length <strong>of</strong> the vector |v| is the square root <strong>of</strong> v · v.<br />
• v · w = |v||w| cos(α), where α is the angle between v and w.<br />
• if A, B are two n × n matrices, then (AB)ij is the dot product <strong>of</strong> the i’th row <strong>of</strong> A with the j’th column<br />
<strong>of</strong> B<br />
echelon matrix<br />
The [echelon matrix] <strong>of</strong> a matrix A is a matrix rref(A), where the pivot in each row comes after the pivot in<br />
the previous row. The pivot is the first nonzero entry in each row. The echelon matrix is also called a matrix<br />
in reduced row echelon form.<br />
eigenbasis<br />
An [eigenbasis] to a matrix A is a basis which consists <strong>of</strong> eigenvectors <strong>of</strong> A.<br />
eigenvalue<br />
An [eigenvalue] � � λ <strong>of</strong> a matrix A is a number for which there exists a vector v such that Av = λv. Example:<br />
3 2<br />
A =<br />
has the eigenvector v = (0, 1) with eigenvalue x = 4.<br />
0 4<br />
eigenvector<br />
An [eigenvector] � v <strong>of</strong> a� matrix A is a nonzero vector v for which Av = λv with some number λ (called eigenvalue).<br />
−1 1<br />
Example:<br />
has the eigenvector v = (1, 1) with eigenvalue λ = 0.<br />
1 1
Elimination<br />
[Elimination] is a process which reduces a matrix A to its echelon matrix rref(A). See row reduced echelon<br />
form.<br />
ellipsoid<br />
An [ellipsoid] can be written as the set <strong>of</strong> points x which satisfy x ˙ Ax = 1, where A is a positive definit matrix.<br />
The axes vi <strong>of</strong> the ellipse are the eigenvectors <strong>of</strong> A have the length 1/xi , where xi are the eigenvalues <strong>of</strong> A.<br />
entry<br />
An [entry] or coefficient <strong>of</strong> a matrix is the number or the variable A(i, j) <strong>of</strong> a matrix.<br />
expansion factor<br />
The [expansion factor] <strong>of</strong> a linear map is the absolute value <strong>of</strong> the determinant <strong>of</strong> A. It is the volume <strong>of</strong> the<br />
parallelepiped obtained as the image <strong>of</strong> the unit cube under A.<br />
exponential<br />
The [exponential] exp(A) <strong>of</strong> a matrix A is defined as the sum exp(A) = 1 + A + A 2 /2! + A 3 /3! + .... The linear<br />
system <strong>of</strong> differential equations x ′ = Ax for x(t) has the solution x(t) = exp(At)x(0).<br />
factorization<br />
The [factorization] <strong>of</strong> a polynomial p(x) is the representation p(x) = a(λ1 − x)...(λn − x), where lambdai are<br />
the n roots <strong>of</strong> the polynomials whose existence is assured by the fundamental theorem <strong>of</strong> algebra.<br />
Fourier coefficients<br />
The [Fourier coefficients] <strong>of</strong> a 2π periodic function f(x) on [−π, π] is cn = (1/2π) � p<br />
if(x)exp(−inx). One<br />
−pi<br />
has f(x) = �<br />
n cn exp(inx). By writing f(x) = g(x) + h(x), where g(x) = [f(x) + f(−x)]/2 is even and<br />
h(x) = [f(x) − f(−x)]/2 is odd one can obtain real versions: the even function can be written as a cos-series<br />
g(x) = sum∞ n=0an cos(nx), where an = (2/π) � π<br />
0 g(x) cos(nx)dx for n > 0 and a0 = (1/π) � π<br />
g(x) dx. The odd<br />
0<br />
function can be written as the sin-series h(x) = sum∞ n=1bn sin(nx), where bn = (2/π) � π<br />
h(x) sin(nx)dx. The<br />
0<br />
complex Fourier coefficients cn are coordinates <strong>of</strong> f(x) with respect to the orthonormal basis exp(inx). The<br />
real Fourier coefficients are the coordinates <strong>of</strong> f(x) with respect to orthogonal basis 1, cos(nx), sin(nx), n > 0.<br />
The [Fourier series] <strong>of</strong> a function f is f(x) = �∞ n=−∞ cn exp(inx) or f(x) = �<br />
n an cos(nx) for even functions<br />
or f(x) = sum ∞ n=1 bn sin(nx) for odd functions.
fundamental theorem <strong>of</strong> algebra<br />
The [fundamental theorem <strong>of</strong> algebra] states that a polynomial p(x) = x n + ...a1x + a0 <strong>of</strong> degree n has exactly<br />
n roots.<br />
Gauss Jordan elimination<br />
The [Gauss Jordan elimination] is a method for solving linear equations. It was already known by the Chinese<br />
2000 years ago. Gauss called it ”eliminatio vulgaris”. The method does linear combinations <strong>of</strong> the rows <strong>of</strong> a<br />
n × (n + 1) matrix until the system is solved. Example:<br />
2 x + 4y = 2<br />
3 x + y = 12<br />
x + 2y = 1<br />
3 x + y = 13<br />
x + 2y = 1<br />
- 5y = 10<br />
x + 2y = 1<br />
y = -2<br />
x = 5<br />
y = -2<br />
First, the top equation was scaled, then three times the first equation was subtracted from the second equation.<br />
Then the the second equation was scaled. Finally, twice the the second equation was subtracted from the first.<br />
geometric multiplicity<br />
The [geometric multiplicity] <strong>of</strong> an eigenvalue λ is the dimension <strong>of</strong> ker(λ − A). The geometric multiplicity is<br />
smaller or equal to the algebraic multiplicity.<br />
Gibbs phenomenon<br />
The [Gibbs phenomenon] � describes the error when doing a Fourier approximation <strong>of</strong> the discontinuous Heavyside<br />
−1if − π ≤ x ≤ 0<br />
function f(x) =<br />
The Fourier approximation is sn(x) = (4/π)<br />
1if0 < x < π<br />
�n k=1 sin((2k−1)t)/(2k−1).<br />
The derivative d/dxsn can be computed: (differentiate and sum up the geometric series): (2/π) sin(2nx)/ sin(x)<br />
which vanishes at x = ±π/2n. These are the extrema for sn. Now, sn(π/2n) = (4/π) � sin((2k −<br />
1)(π/2n))/((2k−1)(π/2n)) is a Riemann sum approximation for (2/π) � π<br />
0 sin(t)/tdt = π(1−π2 /(3!3)+π4 /(5!5)−<br />
...) = 1.1793... This overshoot is called the Gibbs phenomenon. It was first discoverd by Wilbraham in 1848<br />
then by Gibbs in 1899. The human eye can recognize the Gibbs phenomenon as ”ghosts” on a TV screen, unless<br />
it is corrected for.<br />
Gramm-Schmidt process<br />
The [Gramm-Schmidt process] is an algorithm which constructs from a basis v1, ..., vn an orthonormal basis<br />
w1, ..., wn. The procedure goes by induction: if w1, ..., wk−1 are orthonormal, then the next vector wk is<br />
wk = uk/||uk||, where uk = vk − (w1 · vk)w1 − (w2 · vk)w2 · · · − (wk−1 · v + k)wk−1.
graph<br />
A [graph] is a set <strong>of</strong> n nodes connected by m edges. It is completely defined by its adjacency matrix. In a<br />
directed graph, the nodes are oriented. Examples:<br />
• a complete graph has all nodes connected. There are n(n − 1)/2 edges. Its adjacency matrix is E − I,<br />
where E is the n × n matrix with all entries equal to 1 and I is the identity matrix.<br />
• a tree ⎛has<br />
m = n⎞ − 1 edges and no closed loops. An example is the graph with the adjecency matrix<br />
0 1 0<br />
A = ⎝ 1 0 1 ⎠.<br />
0 1 0<br />
�<br />
0<br />
• The directed graph with two edges 1 → 2 has the adjacency matrix A =<br />
0<br />
1<br />
0<br />
�<br />
.<br />
Hankel matrix<br />
A [Hankel matrix] is a square matrix A, where the entries are constant along the antidiagonal. ⎛ In other ⎞ words,<br />
a b c<br />
each entry Aij depends only on i + j. A general 3 × 3 Hankel matrix is <strong>of</strong> the form A = ⎝ b c d ⎠.<br />
c d e<br />
heat equation<br />
The [heat equation] is the linear partial differential equation ut = µuxx. The heat equation on a finite interval<br />
[0, π] with boundary conditions u(0, t) = 0, u(π, t) = 0 and initial conditions u(x, 0) = f(x) can be solved<br />
with the Fourier series u(x, t) = �<br />
n>0 an sin(nx)e−µn2t , where an = (2/π) � p<br />
if(x) sin(nx) dx are the Fourier<br />
0<br />
coefficients.<br />
Hermitian matrix<br />
A [Hermitian matrix] satisfies A ∗ = A T = A, where A T is the transpose <strong>of</strong> A and A is the complex conjugate<br />
matrix, where all entries are replaced by their complex conjugates.<br />
Hessenberg matrix<br />
A [Hessenberg matrix] A is an upper triangular matrix with only⎛one extra nonzero ⎞ adjacent diagonal below<br />
a b c<br />
the diagonal. Example: a general 3 × 3 Hessenberg matrix is A = ⎝ d e f ⎠.<br />
0 g h
Hilbert matrix<br />
A [Hilbert matrix] is a symmetric square matrix, where Aij = 1/(i + j − 1). It is an example <strong>of</strong> a Hankel matrix<br />
and positive definit. Hilbert matrices are examples <strong>of</strong> matrices which⎛are difficult to invert, ⎞ because their<br />
1 1/2 1/3<br />
determinant is small. For example, for n = 3, the Hilbert matrix A = ⎝ 1/2 1/3 1/4 ⎠ has determinant<br />
1/3 1/4 1/5<br />
1/2160. A [hyperplane] in n-dimensional space V is a (n − 1)-dimensional linear subspace <strong>of</strong> V .<br />
identity matrix<br />
The [identity matrix] is the matrix I which has 1 in the diagonal and zero ⎛ everywhere ⎞ else. The identity matrix<br />
1 0 0<br />
I satisfies IA = A for any matrix A. The 3x3 identity matrix is A = ⎝ 0 1 0 ⎠.<br />
0 0 1<br />
incidence matrix<br />
The [incidence matrix] <strong>of</strong> a directed graph with n nodes and m edges is a m×n matrix which has a row for each<br />
edge connecting nodes i and j with entries −1 and 1 in columns i, j. ⎛Example.<br />
The directed ⎞ graph 1 ⇒ 2 ⇐ 3,<br />
−1 1 0 0<br />
1 → 4 with 3 edges and 4 nodes has the 3 × 4 incidence matrix A = ⎝ 0 1 −1 0 ⎠.<br />
−1 0 0 1<br />
inconsistent<br />
A system <strong>of</strong> linear equations Ax = b is called [inconsistent] if the system has no solutions.<br />
indefinite matrix<br />
An [indefinite matrix] is a matrix, whith eigenvalues <strong>of</strong> different sign. A positive definite matrix is an example<br />
<strong>of</strong> a matrix which is not indefinite.<br />
Independent vectors<br />
[Independent vectors]. If no linear combination a1v1 + ... + anvn is zero unless all ai are zero, then the vectors<br />
v1, ..., vn are called independent. If A is the matrix which contains the vectors vi as columns, then the kernel <strong>of</strong><br />
A is trivial. A basis consists <strong>of</strong> independent vectors.<br />
Independent vectors<br />
The linear transformation corresponding to the identity matrix is called the [identity transformation].
image<br />
The [image] <strong>of</strong> a linear transformation T : X → Y, T (x) = Ax is the subset <strong>of</strong> all vectors y = Ax, xinX in<br />
Y. The image is denoted by im(T ) or im(A) and is a subset <strong>of</strong> the codomain Y <strong>of</strong> T . The image is also<br />
called the range. The dimension <strong>of</strong> the image <strong>of</strong> T is equal to the rank <strong>of</strong> A and the dimension satisfies<br />
dim(ker(A)) + dim(im(A)) = n, where n is the dimension <strong>of</strong> the linear space X.<br />
index<br />
The [index] <strong>of</strong> a linear map T is defined as ind(A) = dim(kerA)−dim(cokerA), where coker(A) is the orthogonal<br />
complement <strong>of</strong> the image <strong>of</strong> A. Examples are:<br />
• The index <strong>of</strong> a n × n matrix A is dim(kerA) − dim(cokerA) = 0.<br />
• The index <strong>of</strong> the differential operator Df = f ′ acting on smooth functions on the real line is 1 − 0 = 1<br />
because D has a one dimensional kernel (the constant functions) and a zero dimensional cokernel (all<br />
functions can be obtained as the image <strong>of</strong> D). The index <strong>of</strong> D n is n.<br />
• The index <strong>of</strong> the differential operator Df = f ′ acting on smooth functions on the circle is 1 − 1 = 0<br />
because D has a one dimensional kernel (the constant functions) and a one-dimensional cokernel (the<br />
constant functions, one can not find a periodic function g such that g’=1).<br />
• The Atiyah-Singer index theorem relates topological properties <strong>of</strong> a surface M with the index <strong>of</strong> a ”Dirac<br />
operator” T on it. The previous two examples exemply that. T = D is a Dirac operator and the topology<br />
<strong>of</strong> the circle or the line are different.<br />
inverse<br />
The [inverse] <strong>of</strong> a square matrix A is a matrix B satisfying � AB � = I and BA = I where I is�the identity� matrix.<br />
a b<br />
d −b<br />
For example, the inverse <strong>of</strong> the transformation A =<br />
is the transformation B =<br />
/(ad −<br />
c d<br />
−c a<br />
bc).<br />
invertible<br />
A square matrix A is [invertible] if there exists a matrix B such that AB = I. A matrix A is invertible if and<br />
only if the determinant <strong>of</strong> A is different from zero.<br />
Jordan normal form<br />
The [Jordan normal form] J = S −1 AS <strong>of</strong> a square matrix A is a block matrix J = diag(J1, ..., Jk), where each<br />
block is <strong>of</strong> the form Jk = xkIk + Nk, where xk is an eigenvalue <strong>of</strong> A, Ik is an identity matrix and Nk is a matrix<br />
with 1 in the first sidediagonal. If all eigenvalues <strong>of</strong> A are different, then the Jordan normal form is a diagonal<br />
matrix.
kernel<br />
The [kernel] <strong>of</strong> a linear transformation T : X → Y , T (x) = Ax is the linear space {xinXsuchthatAx = 0}.<br />
The kernel is denoted by ker(T ) or ker(A) and is a subset <strong>of</strong> the domain X <strong>of</strong> T . The dimension <strong>of</strong> the kernel<br />
dim(ker(A)) and the dimension <strong>of</strong> the image dim(im(A)) are related by dim(ker(A)) + dim(im(A)) = n, where<br />
n is the dimension <strong>of</strong> the linear space X. The kernel <strong>of</strong> a transformation is computed by building rref(A), the<br />
reduced row echelon form <strong>of</strong> A. Echelon = ”series <strong>of</strong> steps”. Every vector in the kernel <strong>of</strong> rref(A) is also in the<br />
kernel <strong>of</strong> A.<br />
Leontief<br />
Wassily [Leontief]. A Russian-born US economist who was working also at Harvard University. Leontief was<br />
a winner <strong>of</strong> the 1973 Economics Nobel prize for the development <strong>of</strong> the input-output method and for its<br />
application to important economic problems. Linear algebra students find the following problem in textbooks:<br />
two industries A and B produce output with value x and y (in millions <strong>of</strong> dollars). Assume that the consumer<br />
demand is a for the product <strong>of</strong> A and b for the product <strong>of</strong> B. Assume also an industry demand: p x is transfered<br />
from A to B, and q y is transfered from B to A. For which x and y are both the industry and conumer demand<br />
satisfied? The problem is equivalent to solving the linear system<br />
x − qy = a<br />
−px + y = b<br />
Laplace equation<br />
The [Laplace equation] in a region G is the linear partial differential equation uxx + uyy = 0. A solution<br />
is determined if u(x, y) is prescribed on the boundary <strong>of</strong> G. On the square [0, π] × [0, π] with boundary<br />
conditions 0 except at the side y = π, where one has u(x, π) = f(x), one can find a solution via Fourier series:<br />
u(x, y) = �<br />
n>0 an sin(nx) sinh(ny)/sinh(nπ), where an = (2/π) � π<br />
f(x) sin(nx) dx. The case with general<br />
0<br />
boundary conditions can be solved by adding corresponding solutions u(x, y), u(y, x), u(x, π − y), u(π − y, x) for<br />
the other 3 sides <strong>of</strong> the square.<br />
Laplace expansion<br />
The [Laplace expansion] is a formula for the determinant <strong>of</strong> A: det(A) = (−1) i+1 ai1det(Ai1) + ... +<br />
(−1) i+n aindet(Ain).<br />
leading one<br />
A [leading one] is an entry <strong>of</strong> a matrix in reduced row echelon form which is contained in a row with this element<br />
as the first nonzero entry.<br />
leading variable<br />
A [leading variable] is a variable which corresponds to a leading one in rref(A).
least-squares solution<br />
A vector x ∈ R n is called a [least-squares solution] <strong>of</strong> the system Ax = b where A is a m × n matrix, if ||b − Ay||<br />
is less or equal then ||b − Ax|| for all y ∈ R n . If x is the least-squares solution <strong>of</strong> Ax = b then Ax is the<br />
orthogonal projection <strong>of</strong> b onto the image im(A). The explicit formula is x = (A T A) ( − 1)A T b and derived from<br />
that A T (Ax − b) = 0 which itself just means that Ax − b is orthogonal to the image <strong>of</strong> A.<br />
length<br />
The [length] <strong>of</strong> a vector v is ||v|| = (v · v) 1/2 = (v 2 1 + ... + v 2 n) ( 1/2). The length <strong>of</strong> a complex number x + iy is<br />
the length <strong>of</strong> (x, y). The length <strong>of</strong> a vector depends on the basis, usually it is understood with respect to the<br />
standard basis.<br />
linear combination<br />
A [linear combination] <strong>of</strong> n vectors v1, ..., vn is a vector a1v1 + ... + anvn.<br />
Linearly dependent vectors<br />
[Linearly dependent vectors]. If there exist a1, ..., an which are not all zero such that a1v1 + ... + anvn = 0, then<br />
the vectors v1, ..., vn are called linearly dependent.<br />
Linearity<br />
[Linearity] is a property <strong>of</strong> maps between linear spaces: it means that lines are maped into lines and the image<br />
<strong>of</strong> the sum <strong>of</strong> two vectors is the same as sum <strong>of</strong> the images. For example: T (x, y, z) = (2x + z, y − x) is linear.<br />
T (x, y) = (x 2 − y, x) is nonlinear.<br />
linear dynamical system<br />
A [linear dynamical system] is defined by a linear map x ↦→ Ax. The orbits <strong>of</strong> the dynamical system are<br />
x, Ax, A 2 x, ....<br />
linear space<br />
A [linear space] is the same as a vector space. It is a set which is closed under addition and multiplication with<br />
real numbers.<br />
linear combination<br />
A sum a1v1 + ... + anvn is called a [linear combination] <strong>of</strong> the vectors v1, ..., vn.
linear subspace<br />
A [linear subspace] <strong>of</strong> a vector space V is a subset <strong>of</strong> V which is also a vector space. In particular, it is closed<br />
under addition, scalar multiplication and contains a neutral element.<br />
linear system <strong>of</strong> equations<br />
A [linear system <strong>of</strong> equations] is an equation <strong>of</strong> the form Ax=b, where A is a m × n matrix, x is a n-vector and<br />
b is a m-vector. There are three possibilities:<br />
• consistent with one solution: no row vector (0...0�1) in rref(A|b). There is exactly one solution if there is<br />
a leading one in each column <strong>of</strong> rref(A).<br />
• consistent with infinitely many solutions: there are columns with no leading one.<br />
• Inconsistent with no solutions: there is a row (0...0�1) in rref(A�b).<br />
logarithm<br />
The [logarithm] log(z) <strong>of</strong> a complex number z = x + iy �= 0 is defined as log |z| + iarg(z), where arg(z) is the<br />
argument <strong>of</strong> z. The imaginary part <strong>of</strong> the logarithm is only defined up to a multiple <strong>of</strong> 2π.<br />
Markov matrix<br />
A [Markov matrix] is a square matrix, where all entries are nonnegative and the sum <strong>of</strong> each column is 1. One<br />
<strong>of</strong> the eigenvalues <strong>of</strong> a Markov matrix is 1 because A T has the eigenvector (1, 1, ..., 1). If all entries <strong>of</strong> a Markov<br />
matrix are positive, then A k v converges to the eigenvector v with eigenvalue 1. This vector is called the ”steady<br />
state” vector.<br />
matrix<br />
A [matrix] is a rectangular ⎛ array <strong>of</strong> numbers. ⎞ The following 3 × 4 matrix for example consists <strong>of</strong> three rows<br />
2 8 4 2<br />
and four columns: A = ⎝ 1 2 1 3 ⎠. The first index addresses the row, the second the column <strong>of</strong> the<br />
2 −1 1 2<br />
matrix. A n × m matrix maps the m-dimensional space to the n-dimensional space.<br />
Matrix multiplication<br />
[Matrix multiplication] is an operation defined between a (n × m) matrix A and a (m × p) matrix B. (AB)ij<br />
is the dot product between the i’th row <strong>of</strong> A with the j’th column <strong>of</strong> B. Example: (n = 2, m = 3, p = 4)<br />
� �<br />
2 1 0<br />
1 0 1<br />
⎛<br />
⎞<br />
2 1 0 0 � �<br />
⎝ 0 0 1 2 ⎠<br />
4 2 1 2<br />
=<br />
.<br />
3 4 1 1<br />
1 3 1 1
minor<br />
A [minor] <strong>of</strong> a matrix A is a matrix A(i, j) which is obtained from A by deleting row i and column j.<br />
nilpotent matrix<br />
A [nilpotent matrix] is a matrix A for which some power Ak ⎛ ⎞<br />
is the zero matrix. A nilpotent matrix has only<br />
0 1 1<br />
zero eigenvalues. he matrix A = ⎝ 0 0 2 ⎠ for example satisfies A<br />
0 0 0<br />
3 = 0 and is therefore nilpotent.<br />
non-leading coefficient<br />
A [non-leading coefficient] is an entry in the row reduced echelon form <strong>of</strong> a matrix A which is nonzero and which<br />
comes after the leading 1. The relevance <strong>of</strong> this definition comes from the fact that the number <strong>of</strong> columns with<br />
non-leading coefficients is the dimension <strong>of</strong> the kernel <strong>of</strong> the map.<br />
normal equation<br />
The [normal equation] to the linear equation Ax=b is the consistent system A T Ax = A T b.<br />
normal matrix<br />
A matrix A is called a [normal matrix], if AA T = A T A. A normal matrix has orthonormal possibly complex<br />
eigenvectors.<br />
null space<br />
The [null space] <strong>of</strong> a matrix A is the same as the kernal <strong>of</strong> A. It is spanned by the solutions Av = 0. The<br />
dimension <strong>of</strong> the null space is n − r, where n is the number <strong>of</strong> columns <strong>of</strong> A and r is the rank <strong>of</strong> A.<br />
ordinary differential equation<br />
An [ordinary differential equation] is a differential equation, where derivatives appear only with respect to one<br />
variable. By adding new variables if necessary (for example for t, or derivatives ut, utt etc. one can write such<br />
an equation always in the form xt = f(x). An ordinary differential equation defines a continuous dynamical<br />
system. The initial condition x(0) determines the trajectories x(t). An ordinary differential equation <strong>of</strong> the<br />
form ut = Au, where A is a matrix is called a linear ordinary differential equation.
orthogonal<br />
Two vectors v,w are [orthogonal] if their dot product v · w vanishes.<br />
orthogonal basis<br />
An [orthogonal basis] is a basis such that all vectors in the basis are orthogonal.<br />
orthonormal basis<br />
An [orthonormal basis] is a basis such that all vectors are orthogonal and normed.<br />
orthonormal complement<br />
The [orthonormal complement] <strong>of</strong> a linear subspace V in R n is the set <strong>of</strong> vectors which are orthogonal to V .<br />
orthogonal projection<br />
The [orthogonal projection] onto a linear space V is proj V (x) = (x · v1)v1 + ... + (x · vn)vn, where the vj form<br />
an orthonormal basis in V . Despite the name, an orthogonal projection is not an orthogonal transformation. It<br />
has a kernel. In an eigenbasis, a projection has the form (x, y) → (x, 0).<br />
Euclidean space<br />
[ Euclidean space ] is the linear space <strong>of</strong> all vectors = 1 × n matrices. R 0 is the space<br />
0. The space R 1 is the real linear space <strong>of</strong> all real numbers, the R 2 is the plane, the R 3 the Euclidean three<br />
dimensional space.<br />
parallel<br />
Two vectors v and w are called [parallel] if v both are nonzero and one is a multiple <strong>of</strong> the other.<br />
parallelepiped<br />
A set in R n is a [parallelepiped] E if it is the linear image A(Q) <strong>of</strong> the unit cube Q. The volume <strong>of</strong> a n-dimensional<br />
parallelepiped E in R n satisfies vol(E) = |det(A)|, in general, vol(E) = (det(A T A)) 1/2 .
partial differential equation<br />
A [partial differential equation] (PDE) is an equation for a multi-variable function which involves partial derivatives.<br />
It is called linear if (u + v) and rv are solutions whenever u and v are solutions. Examples <strong>of</strong> linear<br />
PDEs:<br />
Examples <strong>of</strong> nonlinear PDE:<br />
ut = cux<br />
transport equation<br />
ut = buxx<br />
heat equation<br />
utt = auxx<br />
wave equation<br />
uxx + uyy = 0 Laplace equation<br />
uxx + uyy = f(x, y) Poisson equation<br />
ihut = −uxx + V (x) Schroedinger equation<br />
ut + uux = auxx<br />
ut + uux = −uxxx<br />
Burger equation<br />
Korteweg de Vries equation<br />
utt − uxx = sin(x) Sine Gordon equation<br />
utt − uxx = f(x) Nonlinear wave equation<br />
ihut = −uxx − |x| 2 x Nonlinear Schroedinger equation<br />
ut + ux(x, t) 2 /2 + V (x) = 0 Hamilton Jacobi equation<br />
permutation matrix<br />
A [permutation matrix] A is a square matrix with entries Aij = Iiπ(j) where π is a permutation <strong>of</strong><br />
1, ..., n and where I is the identiy matrix. There are n! permutation ⎛ matrices. ⎞ Example: for n = 3 the<br />
0 1 0<br />
permutation π(1, 2, 3) = (2, 1, 3) defines the permutation matrix A = ⎝ 1 0 0 ⎠.<br />
0 0 1<br />
pivot<br />
A [pivot] d is the first nonzero diagonal entry when a row is used in Gaussian elimination.<br />
pivot column<br />
A column <strong>of</strong> a matrix is called a [pivot column] if the corresponding column <strong>of</strong> rref(A) contains a leading one.<br />
The pivot columns are important because they form a basis for the image <strong>of</strong> A.<br />
polar decomposition<br />
The [polar decomposition] <strong>of</strong> a matrix A is A = OB, where O is orthogonal and where B is positive semidefinit.<br />
positive definite matrix<br />
A [positive definite matrix] is a symmetric matrix which satisfies v · Av > 0, for every nonzero vector v.
power<br />
The n’th [power] <strong>of</strong> a matrix A is defined as An = AA ( n − 1) = AA....A. The eigenvalues <strong>of</strong> An are λn i , where<br />
λi are the eigenvalues <strong>of</strong> A.<br />
QR decomposition<br />
The [QR decomposition] <strong>of</strong> a matrix A is obtained during the Gramm-Schmitt orthogonalization process. It is<br />
A = QR, where Q is an orthogonal matrix and where R is an upper triangular matrix.<br />
rank<br />
The [rank] <strong>of</strong> a linear matrix A is the set <strong>of</strong> leading 1’s in the matrix rref(A).<br />
orientation<br />
The [orientation] <strong>of</strong> n vectors v1, ..., vn in the n-dimensional Euclidean space is defined as the sign <strong>of</strong> det(A),<br />
where A is the matrix with vi in the columns.<br />
orthogonal<br />
A square matrix A is [orthogonal] if it preserves length: ||Av|| = ||v|| for all vectors v.<br />
perpendicular<br />
Two vectors v and w are called [perpendicular] if their dot product vanishes: v · w = 0. A synonym <strong>of</strong><br />
perpendicular is orthogonal.<br />
projection matrix<br />
A [projection matrix] is a matrix P which satisfies P 2 = P = P T . It has eigenvalues 1 or 0. The image is a linear<br />
subspace S. The vectors in S are eigenvectors to the eigenvalues 1. The vectors in the orthogonal complement<br />
<strong>of</strong> S are eigenvectors to the eigenvalue 0. If A is the matrix which contains the basis <strong>of</strong> S as the columns, then<br />
P = A(A T A) −1 A T is the projection onto S.<br />
pseudoinverse<br />
The [pseudoinverse] <strong>of</strong> a (m × n) matrix A is the (n × m) matrix A + that maps the image <strong>of</strong> A to the image <strong>of</strong><br />
A T . The kernel <strong>of</strong> A + is the kernel <strong>of</strong> A T and the rank <strong>of</strong> A + is equal to the rank <strong>of</strong> A. A + A is the projection<br />
on the image <strong>of</strong> A T and AA + is the projection on the image <strong>of</strong> A. Especially, if A is an invertible (n × n)<br />
matrix, then A + is the inverse <strong>of</strong> A. The pseudoinverse is also called Moore-Penrose inverse.
ank<br />
The [rank] <strong>of</strong> a matrix A is the dimension <strong>of</strong> the image <strong>of</strong> A.<br />
Rayleigh quotient<br />
The [Rayleigh quotient] <strong>of</strong> a symmetric matrix A is defined as the function q(v) = (v · Av)/(v · v). The maximal<br />
value <strong>of</strong> q(v) is the maximal eigenvalue <strong>of</strong> A and the minimal value <strong>of</strong> q(v) is the minimal eigenvalue <strong>of</strong> A.<br />
rotation<br />
A [rotation] is a linear transformation which preserves the angle between two vectors as well as their lengths.<br />
A rotation in three dimensional space is determined by the axis <strong>of</strong> rotation as well as the rotation angle.<br />
rotation matrix<br />
A [rotation matrix] is the matrix belonging to a rotation. A rotation matrix is an example <strong>of</strong> an orthogonal<br />
matrix. Example: In two dimensions, a rotation matrix has the form A =<br />
rotation-dilation matrix<br />
� cos(t) sin(t)<br />
− sin(t) cos(t)<br />
�<br />
p<br />
A [rotation-dilation matrix] is a 2x2 matrix <strong>of</strong> the form A =<br />
q<br />
−q<br />
p<br />
�<br />
. It has the eigenvalues p ± iq. The<br />
action <strong>of</strong> A represents the complex multiplication with the complex number p+iq in the complex plane.<br />
A [row] <strong>of</strong> a matrix is formed by horizontal lines A1j, j = 1, ..n <strong>of</strong> a m × n matrix A.<br />
row<br />
shear<br />
A [shear] is a linear transformation in the plane which has in a suitable basis the form T (x, y) = (x, y + ax).<br />
More generally, in n dimensions, one can define as shear along a m-dimensional plane. If a basis is chosen so<br />
that the plane has the from (x, 0) then a shear is T (x, y) = (x, y + ax). Shears have determinant 1 and preserve<br />
therefore volume.<br />
singular<br />
A square matrix A is called [singular] if it has no inverse. A matrix A is singular if and only if det(A) = 0.<br />
�<br />
.
singular value decomposition<br />
The [singular value decomposition] (SVD) <strong>of</strong> a matrix writes a matrix A in the form A = UDV T , where U, V<br />
are orthogonal and D is diagonal. The first r columns <strong>of</strong> U form an orthonormal basis <strong>of</strong> the image <strong>of</strong> A and the<br />
first r columns <strong>of</strong> V form an orthonormal basis <strong>of</strong> the image <strong>of</strong> A T . The last columns <strong>of</strong> U form an orthonormal<br />
basis <strong>of</strong> the kernel <strong>of</strong> A T and the last columns <strong>of</strong> V form a basis <strong>of</strong> the kernel <strong>of</strong> A.<br />
skew symmetric<br />
A matrix A is [skew symmetric] if it is minus its transpose that is if AT = −A. The eigenvalues <strong>of</strong> a skewsymmetric<br />
matrix are purely imaginary. The eigenvectors are orthogonal. If A is skew symmetric, then B =<br />
exp(At) is an orthogonal matrix, because BT � �<br />
0 1<br />
B = exp(−At)exp(At) = 1. For example A =<br />
gives<br />
−1 0<br />
the rotation matrix exp(At).<br />
span<br />
The [span] <strong>of</strong> a set <strong>of</strong> vectors v1, ...vn is the set <strong>of</strong> all linear combinations <strong>of</strong> v1, ..., vn.<br />
spectral theorem<br />
The [spectral theorem] tells that a real symmetric matrix A can be diagonalized A = UDU T , where U is an<br />
orthonormal matrix containing an orthonormal eigenbasis in the columns and where D is a diagonal matrix<br />
D = diag(x1, ..., xn), where xi are the eigenvalues <strong>of</strong> A.<br />
square matrix<br />
A [square matrix] is a matrix which has the same number <strong>of</strong> rows than columns.<br />
asymptotically stable<br />
A linear dynamical system is called [asymptotically stable] if A n x → 0 for all initial values x, where A n is the<br />
n’th power <strong>of</strong> the matrix A. This is equivalent to the fact that all eigenvalues λ <strong>of</strong> A satisfy |λ| < 1.<br />
Stability triangle<br />
[Stability triangle]. A discrete dynamical system in the plane is asymptotically stable if and only if the trace<br />
and determinant are in the stability triangle |tr(A)| − 1 < det(A) < 1. A rotation-dilation A is asymptotically<br />
stable if and only if det(A) < 1.
educed row echelon form<br />
The [reduced row echelon form] rref(A) <strong>of</strong> a m x n matrix A is the end product <strong>of</strong> Gauss-Jordan elimination.<br />
The matrix rref(A) has the following properties:<br />
• if a row has nonzero entries, then the first nonzero entry is 1, called leading 1.<br />
• if a columns contains a leading 1, then all other entries in that column are 0.<br />
• if a row contains a leading 1, then every row above contains a leading 1 further left.<br />
The algorithm to produce rref(A) from A is obtained by putting the cursor to the upper left corner and repeating<br />
the following steps until nothing changes anymore<br />
1. if the cursor entry is zero swap the cursor row with the first row below that has a nonzero entry in that<br />
column<br />
2. divide the cursor row by the cursor entry to make the cursor entry = 1<br />
3. eliminate all other entries in cursor column by subtracting suitable multiples <strong>of</strong> the cursor row from the<br />
other row<br />
4. move the cursor down one row and and to the right one column. If the cursor entry is zero and all entries<br />
below are zero, move the cursor to the next column.<br />
5. repeat 4 if as long as necessary and move then to 1<br />
reflection<br />
A [reflection] is a linear transformation T different from the identity transformation which satisfies T 2 = 1. The<br />
eigenvalues <strong>of</strong> T are −1 or 1. In an eigenbasis, the reflection has the form T (x, y) = (x, −y). The determinant<br />
<strong>of</strong> a reflection is 1 if and only if the dimension � <strong>of</strong> the eigenspace � to -1 is even. For example, a reflection at a<br />
cos(2x) sin(2x)<br />
line in the plane has the matrix A =<br />
which has determinant −1. A reflection at the<br />
sin(2x) −cos(2x)<br />
origin in the plane is −I with determinant 1.<br />
root<br />
A [root] <strong>of</strong> a polynomial p(x) is a complex value z such that p(z) = 0. According to the fundamental theorem<br />
<strong>of</strong> algebra, a polynomial <strong>of</strong> degree n has exactly n roots.<br />
symmetric<br />
A matrix A is [symmetric] if it is equal to its transpose. The spectral theorem for symmetric matrices tells that<br />
they have real eigenvalues and symmetric matrices can always be diagonalized with an orthogonal matrix S.<br />
span<br />
The [span] <strong>of</strong> a finite set <strong>of</strong> vectors v1, ..., vn is the set <strong>of</strong> all possible linear combinations c1v1 + c2v2 + ... + cnvn<br />
where ci are real numbers. For example, if v1 = (1, 0, 0) and v2 = (0, 1, 0), then the span <strong>of</strong> v1, v2 in three<br />
dimensional space is the xy-plane. The span is a linear space.
spectral theorem<br />
The [spectral theorem] for a symmetric matrix A assures that A can be diagonalized: there exists an orthogonal<br />
matrix S such that A ( − 1)AS is diagonal and contains the eigenvalues <strong>of</strong> A in the diagonal.<br />
standard basis<br />
The [standard basis] <strong>of</strong> the n-dimensional Euclidean space consists <strong>of</strong> the columns <strong>of</strong> the identity matrix I.<br />
symmetric<br />
A matrix A is called [symmetric] if A T = A. A symmetric matrix has to be a square matrix. Real symmetric<br />
matrices can be diagonalized.<br />
Toepitz matrix<br />
A [Toepitz matrix] is a square matrix A, where the entries are constant along the diagonal. In other ways Aij<br />
⎛ ⎞<br />
c d e<br />
depends only on j − i. Example: a 3 × 3 Toeplitz matrix is <strong>of</strong> the form A = ⎝ b c d ⎠.<br />
a b c<br />
trace<br />
The [trace] <strong>of</strong> a matrix A is the sum <strong>of</strong> the diagonal entries <strong>of</strong> A. The trace is independent <strong>of</strong> the basis and is<br />
equal to the sum <strong>of</strong> the eigenvalues <strong>of</strong> A.<br />
transpose<br />
The [transpose] A T <strong>of</strong> a matrix A is the matrix with entries Aij if A has the entries Aji. The rank <strong>of</strong> A T is<br />
equal to the rank <strong>of</strong> A. For square matrices, the eigenvalues <strong>of</strong> A T and A agree because A and A T have the<br />
same eigenvalues. Transposition satisfies (A T ) T = A, (AB) T = B T A T and (A ( − 1)) T = (A T ) ( − 1).<br />
triangle inequality<br />
The [triangle inequality] tells that in a linear space, ||v + w|| ≤ ||v|| + ||w||. One has equality if and only if the<br />
vectors v and w are orthogonal.
eigenvalues <strong>of</strong> a two times two matrix<br />
� a b<br />
c d<br />
�<br />
The [eigenvalues <strong>of</strong> a two times two matrix] A =<br />
are λ1 = tr(A)/2 + ((tr(A)/2) 2 − det(A)) 1/2 and<br />
λ2 = tr(A)/2 − ((tr(A)/2) 2 − det(A)) 1/2 � �<br />
� �<br />
λi − d<br />
. The eigenvectors are vi =<br />
if c �= 0 or vi =<br />
if<br />
c<br />
b �= 0. (If b = 0, c = 0, then the standard vectors are eigenvector.)<br />
unit vector<br />
b<br />
λi − a<br />
A [unit vector] is a vector <strong>of</strong> length 1. A given nonzero vector can be made a unit vector by scaling: v/||v|| is<br />
a unit vector.<br />
Vandermonde Matrix<br />
A [Vandermonde Matrix] is a square matrix with entries Aij = x j−1<br />
i , where x1, ..., xn are some real numbers.<br />
The determinant <strong>of</strong> a Vandermonde Matrix is �<br />
j>i (xj − xi). Example: x1 = 2, x2 = 3, x3 = −1 defines the<br />
⎛<br />
⎞<br />
1 2 4<br />
Vandermonde Matrix A = ⎝ 1 3 9 ⎠ which has the determinant det(A) = (3 − 2)(−1 − 2)(−1 − 3) = 12.<br />
1 −1 1<br />
vector<br />
A [vector] is a matrix with one column. The entries <strong>of</strong> the vector are called coefficients.<br />
vector space<br />
A [vector space] X is a set equipped with addition and scalar multiplication. A vector space is also called a<br />
linear space. The addition operation is a group:<br />
The scalar multiplication satisfies:<br />
f + g = g + f Commutativity<br />
(f + g) + h = f + (g + h) Associativity<br />
f + 0 = 0 Existence <strong>of</strong> a neutral element<br />
f + x = 0 Existence <strong>of</strong> a unique inverse<br />
r(f + g) = rf + rg Distributivity<br />
(r + s)f = rf + sf Distributivity<br />
r(sf) = (rs)f Associativity<br />
1f = f One element
wave equation<br />
The [wave equation] is the linear partial differential equation utt = c2uxx where c is a constant. The wave<br />
equation on a finite interval 0 < x < 1 with boundary conditions u(0, t) = 0, u(π, t) = 0 and initial conditions<br />
u(x, 0) = f(x), ut(x, 0) = g(x) can be solved with the Fourier series: u(x, t) = �<br />
n > 0an sin(nx) cos(nct) +<br />
bn sin(nx) sin(nct) where an = (2/π) � π<br />
0 f(x) sin(nx) dx, and bn = (2/π)intπ 0 g(x) sin(nx) dx/(cn) are Fourier<br />
coefficients.<br />
zero matrix<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 157 entries in this file.
Index<br />
Euclidean space , 17<br />
adjacency matrix, 1<br />
affine transformation, 1<br />
Algebra, 1<br />
algebraic multiplicity, 1<br />
angle, 1<br />
argument, 1<br />
associative law, 2<br />
asymptotically stable, 21<br />
augmented matrix, 2<br />
basis, 2<br />
basis theorem, 2<br />
block matrix, 2<br />
Cauchy-Schwarz inequality, 2<br />
Cayley-Hamilton theorem, 2<br />
change <strong>of</strong> basis, 3<br />
characteristic matrix, 3<br />
characteristic polynomial, 3<br />
Cholesky factoriztion, 3<br />
circulant matrix, 3<br />
classical adjoint, 3<br />
codomain, 4<br />
coefficient, 4<br />
c<strong>of</strong>actor, 4<br />
column, 4<br />
column picture, 4<br />
column space, 4<br />
commutative law, 5<br />
commuting matrices, 5<br />
complex conjugate, 5<br />
Complex numbers, 5<br />
consistent, 5<br />
continuous dynamical system, 5<br />
covariance matrix, 6<br />
Cramer’s rule, 6<br />
de Moivre formula, 6<br />
determinant, 6<br />
differential equation, 6<br />
dilation, 6<br />
dimension, 6<br />
distributive law, 7<br />
dot product, 7<br />
echelon matrix, 7<br />
eigenbasis, 7<br />
eigenvalue, 7<br />
eigenvalues <strong>of</strong> a two times two matrix, 24<br />
eigenvector, 7<br />
Elimination, 8<br />
ellipsoid, 8<br />
entry, 8<br />
expansion factor, 8<br />
exponential, 8<br />
factorization, 8<br />
Fourier coefficients, 8<br />
fundamental theorem <strong>of</strong> algebra, 9<br />
26<br />
Gauss Jordan elimination, 9<br />
geometric multiplicity, 9<br />
Gibbs phenomenon, 9<br />
Gramm-Schmidt process, 9<br />
graph, 10<br />
Hankel matrix, 10<br />
heat equation, 10<br />
Hermitian matrix, 10<br />
Hessenberg matrix, 10<br />
Hilbert matrix, 11<br />
identity matrix, 11<br />
image, 12<br />
incidence matrix, 11<br />
inconsistent, 11<br />
indefinite matrix, 11<br />
Independent vectors, 11<br />
index, 12<br />
inverse, 12<br />
invertible, 12<br />
Jordan normal form, 12<br />
kernel, 13<br />
Laplace equation, 13<br />
Laplace expansion, 13<br />
leading one, 13<br />
leading variable, 13<br />
least-squares solution, 14<br />
length, 14<br />
Leontief, 13<br />
linear combination, 14<br />
linear dynamical system, 14<br />
linear space, 14<br />
linear subspace, 15<br />
linear system <strong>of</strong> equations, 15<br />
Linearity, 14<br />
Linearly dependent vectors, 14<br />
logarithm, 15<br />
Markov matrix, 15<br />
matrix, 15<br />
Matrix multiplication, 15<br />
minor, 16<br />
nilpotent matrix, 16<br />
non-leading coefficient, 16<br />
normal equation, 16<br />
normal matrix, 16<br />
null space, 16<br />
ordinary differential equation, 16<br />
orientation, 19<br />
orthogonal, 17, 19<br />
orthogonal basis, 17<br />
orthogonal projection, 17<br />
orthonormal basis, 17<br />
orthonormal complement, 17<br />
parallel, 17
parallelepiped, 17<br />
partial differential equation, 18<br />
permutation matrix, 18<br />
perpendicular, 19<br />
pivot, 18<br />
pivot column, 18<br />
polar decomposition, 18<br />
positive definite matrix, 18<br />
power, 19<br />
projection matrix, 19<br />
pseudoinverse, 19<br />
QR decomposition, 19<br />
rank, 19, 20<br />
Rayleigh quotient, 20<br />
reduced row echelon form, 22<br />
reflection, 22<br />
root, 22<br />
rotation, 20<br />
rotation matrix, 20<br />
rotation-dilation matrix, 20<br />
row, 20<br />
shear, 20<br />
singular, 20<br />
singular value decomposition, 21<br />
skew symmetric, 21<br />
span, 21, 22<br />
spectral theorem, 21, 23<br />
square matrix, 21<br />
Stability triangle, 21<br />
standard basis, 23<br />
symmetric, 22, 23<br />
Toepitz matrix, 23<br />
trace, 23<br />
transpose, 23<br />
triangle inequality, 23<br />
unit vector, 24<br />
Vandermonde Matrix, 24<br />
vector, 24<br />
vector space, 24<br />
wave equation, 25<br />
zero matrix, 25
MATHEMATICIANS<br />
[MATHEMATICIANS] Authors: Oliver Knill: 2000 Literature: Started from a list <strong>of</strong> names with birthdates<br />
grabbed from mactutor in 2000.<br />
[Abbe] Abbe Ernst (1840-1909)<br />
Abbe<br />
Abel<br />
[Abel] Abel Niels Henrik (1802-1829) Norwegian mathematician. Significant contributions to algebra and analysis,<br />
in particular the study <strong>of</strong> groups and series. Famous for proving the insolubility <strong>of</strong> the quintic equation at<br />
the age <strong>of</strong> 19.<br />
[AbrahamMax] Abraham Max (1875-1922)<br />
[Ackermann] Ackermann Wilhelm (1896-1962)<br />
[AdamsFrank] Adams J Frank (1930-1989)<br />
[Adams] Adams John Couch (1819-1892)<br />
[Adelard] Adelard <strong>of</strong> Bath (1075-1160)<br />
[Adler] Adler August (1863-1923)<br />
AbrahamMax<br />
Ackermann<br />
AdamsFrank<br />
Adams<br />
Adelard<br />
Adler
[Adrain] Adrain Robert (1775-1843)<br />
[Aepinus] Aepinus Franz (1724-1802)<br />
[Agnesi] Agnesi Maria (1718-1799)<br />
Adrain<br />
Aepinus<br />
Agnesi<br />
Ahlfors<br />
[Ahlfors] Ahlfors Lars (1907-1996) Finnish mathematician working in complex analysis, was also pr<strong>of</strong>essor at<br />
Harvard from 1946, retiring in 1977. Ahlfors won both the Fields medal in 1936 and the Wolf prize in 1981.<br />
[Ahmes] Ahmes (1680BC-1620BC)<br />
[Aida] Aida Yasuaki (1747-1817)<br />
[Aiken] Aiken Howard (1900-1973)<br />
[Airy] Airy George (1801-1892)<br />
[Aitken] Aitken Alec (1895-1967)<br />
Ahmes<br />
Aida<br />
Aiken<br />
Airy<br />
Aitken
[Ajima] Ajima Naonobu (1732-1798)<br />
[Akhiezer] Akhiezer Naum Ilich (1901-1980)<br />
[Albanese] Albanese Giacomo (1890-1948)<br />
[Albert] Albert <strong>of</strong> Saxony (1316-1390)<br />
[AlbertAbraham] Albert A Adrian (1905-1972)<br />
[Alberti] Alberti Leone (1404-1472)<br />
[Albertus] Albertus Magnus Saint (1200-1280)<br />
[Alcuin] Alcuin <strong>of</strong> York (735-804)<br />
[Alexander] Alexander James (1888-1971)<br />
Ajima<br />
Akhiezer<br />
Albanese<br />
Albert<br />
AlbertAbraham<br />
Alberti<br />
Albertus<br />
Alcuin<br />
Alexander
[AlexanderArchie] Alexander Archie (1888-1958)<br />
[Aleksandrov] Alexandr<strong>of</strong>f Pave (1896-1982)<br />
[AleksandrovAleksandr] Alexandr<strong>of</strong>f Alexander<br />
[Ampere] Ampère André-Marie (1775-1836)<br />
[Amsler] Amsler Jacob (1823-1912)<br />
AlexanderArchie<br />
Aleksandrov<br />
AleksandrovAleksandr<br />
Ampere<br />
Amsler<br />
Anaxagoras<br />
[Anaxagoras] Anaxagoras <strong>of</strong> Clazomenae (499BC-428BC)<br />
[Anderson] Anderson Oskar (1887-1960)<br />
[Andreev] Andreev Konstantin (1848-1921)<br />
[Angeli] Angeli Stephano degli (1623-1697)<br />
Anderson<br />
Andreev<br />
Angeli
[Anstice] Anstice Robert (1813-1853)<br />
[Anthemius] Anthemius <strong>of</strong> Tralles (474-534)<br />
[Antiphon] Antiphon the Sophist (480BC-411BC)<br />
[Apastamba] Apastamba (600BC-540BC)<br />
[Apollonius] Apollonius <strong>of</strong> Perga (262BC-190BC)<br />
[Appell] Appell Paul (1855-1930)<br />
[Arago] Arago Francois (1786-1853)<br />
[Arbogast] Arbogast Louis (1759-1803)<br />
[Arbuthnot] Arbuthnot John (1667-1735)<br />
Anstice<br />
Anthemius<br />
Antiphon<br />
Apastamba<br />
Apollonius<br />
Appell<br />
Arago<br />
Arbogast<br />
Arbuthnot
[Archimedes] Archimedes <strong>of</strong> Syracuse (287BC-212BC)<br />
[Archytas] Archytas <strong>of</strong> Tarentum (428BC-350BC)<br />
[Arf] Arf Cahit (1910-1997)<br />
[Argand] Argand Jean (1768-1822)<br />
[Aristaeus] Aristaeus the Elder (360BC-300BC)<br />
[Aristarchus] Aristarchus <strong>of</strong> Samos (310BC-230BC)<br />
[Aristotle] Aristotle (384BC-322BC)<br />
[Arnauld] Arnauld Antoine (1612-1694)<br />
[Aronhold] Aronhold Siegfried (1819-1884)<br />
Archimedes<br />
Archytas<br />
Arf<br />
Argand<br />
Aristaeus<br />
Aristarchus<br />
Aristotle<br />
Arnauld<br />
Aronhold
[Artin] Artin Emil (1898-1962)<br />
[AryabhataII] Aryabhata II<br />
[AryabhataI] Aryabhata I (476-550)<br />
[Atiyah] Atiyah Michael<br />
[Atwood] Atwood George (1745-1807)<br />
[Auslander] Auslander Maurice (1926-1994)<br />
[Autolycus] Autolycus <strong>of</strong> Pitane (360BC-290BC)<br />
Artin<br />
AryabhataII<br />
AryabhataI<br />
Atiyah<br />
Atwood<br />
Auslander<br />
Autolycus<br />
Bezout<br />
[Bezout] Bézout Etienne (1730-1783) French geometer and analyst.<br />
[Bocher] Bocher Maxime (1867-1918)<br />
Bocher
[Burgi] Bürgi Joost (1552-1632)<br />
[Babbage] Babbage Charles (1791-1871)<br />
[Bachet] Bachet Claude (1581-1638)<br />
[Bachmann] Bachmann Paul (1837-1920)<br />
[Backus] Backus John<br />
[Bacon] Bacon Roger (1219-1292)<br />
[Baer] Baer Reinhold (1902-1979)<br />
[Baire] Baire René-Louis (1874-1932)<br />
[BakerAlan] Baker Alan<br />
Burgi<br />
Babbage<br />
Bachet<br />
Bachmann<br />
Backus<br />
Bacon<br />
Baer<br />
Baire<br />
BakerAlan
[Baker] Baker Henry (1866-1956)<br />
[Ball] Ball Walter W Rouse (1850-1925)<br />
[Balmer] Balmer Johann (1825-1898)<br />
Baker<br />
Ball<br />
Balmer<br />
Banach<br />
[Banach], Stefan, (1892-1945) Polish mathematician who founded functional analysis.<br />
[Banneker] Banneker Benjamin (1731-1806)<br />
[BanuMusaMuhammad] Banu Musa Jafar (810-873)<br />
[BanuMusa] Banu Musa brothers<br />
[BanuMusaal-Hasan] Banu Musa al-Hasan (810-873)<br />
[BanuMusaAhmad] Banu Musa Ahmad (810-873)<br />
Banneker<br />
BanuMusaMuhammad<br />
BanuMusa<br />
BanuMusaal-Hasan<br />
BanuMusaAhmad
[Barbier] Barbier Joseph Emile (1839-1889)<br />
[Bari] Bari Nina (1901-1961)<br />
[Barlow] Barlow Peter (1776-1862)<br />
[Barnes] Barnes Ernest (1874-1953)<br />
[Barocius] Barozzi Francesco (1537-1604)<br />
[Barrow] Barrow Isaac (1630-1677)<br />
[Bartholin] Bartholin Erasmus (1625-1698)<br />
[Batchelor] Batchelor George (1920-2000)<br />
[Bateman] Bateman Harry (1882-1946)<br />
Barbier<br />
Bari<br />
Barlow<br />
Barnes<br />
Barocius<br />
Barrow<br />
Bartholin<br />
Batchelor<br />
Bateman
[Battaglini] Battaglini Guiseppe (1826-1894)<br />
[Al-Battani] Battani Abu al- (850-929)<br />
[Baudhayana] Baudhayana (800BC-740BC)<br />
Battaglini<br />
Al-Battani<br />
Baudhayana<br />
Bayes<br />
[Bayes] Thomas, (1702-1761). English probability theorist and theologian.<br />
[Beaugrand] Beaugrand Jean (1595-1640)<br />
[Bell] Bell Eric Temple (1883-1960)<br />
[Bellavitis] Bellavitis Giusto (1803-1880)<br />
[Beltrami] Beltrami Eugenio (1835-1899)<br />
[Bendixson] Bendixson Ivar Otto (1861-1935)<br />
Beaugrand<br />
Bell<br />
Bellavitis<br />
Beltrami<br />
Bendixson
[Benedetti] Benedetti Giovanni (1530-1590)<br />
[Bergman] Bergman Stefan (1895-1977)<br />
[Berkeley] Berkeley George (1685-1753)<br />
[Bernays] Bernays Paul Isaac (1888-1977)<br />
[BernoulliDaniel] Bernoulli Daniel (1700-1782)<br />
[BernoulliJohann] Bernoulli Johann (1667-1748)<br />
[BernoulliNicolaus] Bernoulli Nicolaus<br />
Benedetti<br />
Bergman<br />
Berkeley<br />
Bernays<br />
BernoulliDaniel<br />
BernoulliJohann<br />
BernoulliNicolaus<br />
BernoulliJacob<br />
[BernoulliJacob] Bernoulli Jakob (1654-1705) Swiss analyst, probability theorist and physicist.<br />
Bernstein<br />
[Bernstein] Sergei Natanovich (1880-1968). Russian analyst.
[BernsteinFelix] Bernstein Felix (1878-1956)<br />
[Bers] Bers Lipa (1914-1993)<br />
[Bertini] Bertini Eugenio (1846-1933)<br />
[Bertrand] Bertrand Joseph (1822-1900)<br />
[Berwald] Berwald Lugwig (1883-1942)<br />
[Berwick] Berwick William (1888-1944)<br />
[Besicovitch] Besicovitch Abram (1891-1970)<br />
BernsteinFelix<br />
Bers<br />
Bertini<br />
Bertrand<br />
Berwald<br />
Berwick<br />
Besicovitch<br />
Bessel<br />
[Bessel] Friedrich Wilhelm, (1784-1846) calculated orbit <strong>of</strong> Halley’s orbit as 20 year old. Made accurate measurements<br />
<strong>of</strong> stellar positions. Pr<strong>of</strong>essor <strong>of</strong> Astronomy at Koenigsberg.<br />
[Betti] Betti Enrico (1823-1892)<br />
Betti
[Beurling] Beurling Arne (1905-1986)<br />
[BhaskaraI] Bhaskara I (600-680)<br />
[BhaskaraII] Bhaskaracharya (1114-1185)<br />
[Bianchi] Bianchi Luigi (1856-1928)<br />
[Bieberbach] Bieberbach Ludwig (1886-1982)<br />
[Bienayme] Bienaymé Iréneé-Jules (1796-1878)<br />
[Binet] Binet Jacques (1786-1856)<br />
[Bing] Bing R (1940-1986)<br />
[Biot] Biot Jean-Baptiste (1774-1862)<br />
Beurling<br />
BhaskaraI<br />
BhaskaraII<br />
Bianchi<br />
Bieberbach<br />
Bienayme<br />
Binet<br />
Bing<br />
Biot
[Birkh<strong>of</strong>f] Birkh<strong>of</strong>f George (1884-1944)<br />
[Birkh<strong>of</strong>fGarrett] Birkh<strong>of</strong>f Garrett (1911-1996)<br />
[Al-Biruni] Biruni Abu al<br />
[BjerknesVilhelm] Bjerknes Vilhelm (1862-1951)<br />
[BjerknesCarl] Bjerknes Carl (1825-1903)<br />
[Black] Black Max (1909-1988)<br />
[Blaschke] Blaschke Wilhelm (1885-1962)<br />
[Blichfeldt] Blichfeldt Hans (1873-1945)<br />
[Bliss] Bliss Gilbert (1876-1951)<br />
Birkh<strong>of</strong>f<br />
Birkh<strong>of</strong>fGarrett<br />
Al-Biruni<br />
BjerknesVilhelm<br />
BjerknesCarl<br />
Black<br />
Blaschke<br />
Blichfeldt<br />
Bliss
[Bloch] Bloch André (1893-1948)<br />
[Bobillier] Bobillier Etienne (1798-1840)<br />
[Bochner] Bochner Salomon (1899-1982)<br />
[Boethius] Boethius Anicus (475-524)<br />
[Boggio] Boggio Tommaso (1877-1963)<br />
[Bohl] Bohl Piers (1865-1921)<br />
[BohrHarald] Bohr Harald (1887-1951)<br />
[BohrNiels] Bohr Niels (1885-1962)<br />
[Boltzmann] Boltzmann Ludwig (1844-1906)<br />
Bloch<br />
Bobillier<br />
Bochner<br />
Boethius<br />
Boggio<br />
Bohl<br />
BohrHarald<br />
BohrNiels<br />
Boltzmann
[BolyaiFarkas] Bolyai Farkas (1775-1856)<br />
[Bolyai] Bolyai Jänos (1802-1860)<br />
BolyaiFarkas<br />
Bolyai<br />
Bolza<br />
[Bolza], Oscar (1857-1943), German-born American analyst.<br />
[Bolzano] Bolzano Bernhard (1781-1848)<br />
[Bombelli] Bombelli Rafael (1526-1573)<br />
[Bombieri] Bombieri Enrico<br />
[Bonferroni] Bonferroni Carlo (1892-1960)<br />
[Bonnet] Bonnet Pierre (1819-1892)<br />
Bolzano<br />
Bombelli<br />
Bombieri<br />
Bonferroni<br />
Bonnet<br />
Boole<br />
[Boole], George (1815-1864), English Logician, who made also contributions to analysis and probability theory.
[Boone] Boone Bill (1920-1983)<br />
[Borchardt] Borchardt Carl (1817-1880)<br />
[Borda] Borda Jean (1733-1799)<br />
Boone<br />
Borchardt<br />
Borda<br />
Borel<br />
[Borel], Felix Edouard Justin Emile, (1871-1956) French measure theorist and probability theorist.<br />
[Borgi] Borgi Piero (1424-1484)<br />
[Born] Born Max (1882-1970)<br />
[Borsuk] Borsuk Karol (1905-1982)<br />
[Bortkiewicz] Bortkiewicz Ladislaus (1868-1931)<br />
[Bortolotti] Bortolotti Ettore (1866-1947)<br />
Borgi<br />
Born<br />
Borsuk<br />
Bortkiewicz<br />
Bortolotti
[Bosanquet] Bosanquet Stephen (1903-1984)<br />
[Boscovich] Boscovich Ruggero (1711-1787)<br />
[Bose] Bose Satyendranath (1894-1974)<br />
[Bossut] Bossut Charles (1730-1814)<br />
[Bouguer] Bouguer Pierre (1698-1758)<br />
[Boulliau] Boulliau Ismael (1605-1694)<br />
[Bouquet] Bouquet Jean Claude (1819-1885)<br />
[Bour] Bour Edmond (1832-1866)<br />
Bosanquet<br />
Boscovich<br />
Bose<br />
Bossut<br />
Bouguer<br />
Boulliau<br />
Bouquet<br />
Bour<br />
Bourbaki<br />
[Bourbaki], Nicolas (1939- ) Collective pseudonym <strong>of</strong> a group <strong>of</strong> mostly French mathematicians.
[Bourgain] Bourgain Jean<br />
[Boutroux] Boutroux Pierre Léon (1880-1922)<br />
[Bowditch] Bowditch Nathaniel (1773-1838)<br />
[Bowen] Bowen Rufus (1947-1978)<br />
[Boyle] Boyle Robert (1627-1691)<br />
[Boys] Boys Charles (1855-1944)<br />
[Bradwardine] Bradwardine Thomas (1290-1349)<br />
[Brahe] Brahe Tycho (1546-1601)<br />
[Brahmadeva] Brahmadeva (1060-1130)<br />
Bourgain<br />
Boutroux<br />
Bowditch<br />
Bowen<br />
Boyle<br />
Boys<br />
Bradwardine<br />
Brahe<br />
Brahmadeva
[Brahmagupta] Brahmagupta (598-670)<br />
[Braikenridge] Braikenridge William (1700-1762)<br />
[Bramer] Bramer Benjamin (1588-1652)<br />
[Brashman] Brashman Nikolai (1796-1866)<br />
[BrauerAlfred] Brauer Alfred (1894-1985)<br />
[Brauer] Brauer Richard (1901-1977)<br />
[Brianchon] Brianchon Charles (1783-1864)<br />
Brahmagupta<br />
Braikenridge<br />
Bramer<br />
Brashman<br />
BrauerAlfred<br />
Brauer<br />
Brianchon<br />
Briggs<br />
[Briggs] Briggs Henry (1561-1630) English mathematician producing tables <strong>of</strong> common logarithms up to 15<br />
digits.<br />
[Brillouin] Brillouin Marcel (1854-1948)<br />
Brillouin
[Bring] Bring Erland (1736-1798)<br />
[Brioschi] Brioschi Francesco (1824-1897)<br />
[Briot] Briot Charlese (1817-1882)<br />
[Brisson] Brisson Barnabé (1777-1828)<br />
[Britton] Britton John (1927-1994)<br />
[Brocard] Brocard Henri (1845-1922)<br />
[Brodetsky] Brodetsky Selig<br />
[Bromwich] Bromwich Thomas (1875-1929)<br />
[Bronowski] Bronowski Jacob (1908-1974)<br />
Bring<br />
Brioschi<br />
Briot<br />
Brisson<br />
Britton<br />
Brocard<br />
Brodetsky<br />
Bromwich<br />
Bronowski
[Brouncker] Brouncker William (1620-1684)<br />
Brouncker<br />
Brouwer<br />
[Brouwer] Brouwer Luitzen Egbertus Jan (1881-1966) Dutch matematician and philosopher.<br />
[Brown] Brown Ernest (1866-1938)<br />
[Browne] Browne Marjorie (1914-1979)<br />
[Bruno] Bruno Giuseppe (1828-1893)<br />
[Bruns] Bruns Heinrich (1848-1919)<br />
[Bryson] Bryson <strong>of</strong> Heraclea (450BC-390BC)<br />
[Buffon] Buffon Georges Comte de (1707-1788)<br />
[Bugaev] Bugaev Nicolay (1837-1903)<br />
Brown<br />
Browne<br />
Bruno<br />
Bruns<br />
Bryson<br />
Buffon<br />
Bugaev
[Bukreev] Bukreev Boris (1859-1962)<br />
[Bunyakovsky] Bunyakovsky Viktor (1804-1889)<br />
[Burchnall] Burchnall Joseph (1892-1975)<br />
[Burkhardt] Burkhardt Heinrich (1861-1914)<br />
[Burkill] Burkill John (1900-1993)<br />
[Burnside] Burnside William (1852-1927)<br />
[Caccioppoli] Caccioppoli Renato (1904-1959)<br />
[Cajori] Cajori Florian (1859-1930)<br />
[Calderon] Calderón Alberto (1920-1998)<br />
Bukreev<br />
Bunyakovsky<br />
Burchnall<br />
Burkhardt<br />
Burkill<br />
Burnside<br />
Caccioppoli<br />
Cajori<br />
Calderon
[Callippus] Callippus (370BC-310BC)<br />
[Campanus] Campanus <strong>of</strong> Novara (1220-1296)<br />
[Campbell] Campbell John (1862-1924)<br />
[Camus] Camus Charles (1699-1768)<br />
[Cannell] Cannell Doris (1913-2000)<br />
[Cantelli] Cantelli Francesco (1875-1966)<br />
[CantorMoritz] Cantor Moritz (1829-1920)<br />
Callippus<br />
Campanus<br />
Campbell<br />
Camus<br />
Cannell<br />
Cantelli<br />
CantorMoritz<br />
Cantor<br />
[Cantor] Cantor Georg (1845-1918) [Cantor] Georg, (1845-1918) German mathematician. Precise definition <strong>of</strong><br />
infinite set.<br />
[Caramuel] Caramuel Juan (1606-1682)<br />
Caramuel
[Caratheodory] Carathéodory Constantin (1873-1950)<br />
Caratheodory<br />
Cardan<br />
[Cardan] Cardano Girolamo (1501-1576) Italian mathematicaian, physician and astrologer. First publication<br />
for the solution <strong>of</strong> the general cubic equation (solution found by Tartaglia).<br />
[Carlitz] Carlitz Leonard (1907-1999)<br />
[Carlyle] Carlyle Thomas (1795-1881)<br />
Carlitz<br />
Carlyle<br />
Carnot<br />
[Carnot] Carnot Lazare (1753-1823) French mathematician and politican best known for his work on the foundations<br />
<strong>of</strong> calculus and modern geometry.<br />
CarnotSadi<br />
[CarnotSadi] Carnot Sadi (1796-1832) French mathematical physisist working on the foundations <strong>of</strong> thermodynamics.<br />
Carnot’s work led directly to the discovery <strong>of</strong> the second law <strong>of</strong> thermodynamics.<br />
[Carslaw] Carslaw Horatio (1870-1954)<br />
[Cartan] Cartan Elie (1869-1951)<br />
[CartanHenri] Cartan Henri<br />
Carslaw<br />
Cartan<br />
CartanHenri
[Cartwright] Cartwright Dame Mary (1900-1998)<br />
[Casorati] Casorati Felice (1835-1890)<br />
[Cassels] Cassels John<br />
[Cassini] Cassini Giovanni (1625-1712)<br />
[Castel] Castel Louis (1688-1757)<br />
[Castelnuovo] Castelnuovo Guido (1865-1952)<br />
[Castigliano] Castigliano Alberto (1847-1884)<br />
[Castillon] Castillon Johann (1704-1791)<br />
[Catalan] Catalan Eugène (1814-1894)<br />
Cartwright<br />
Casorati<br />
Cassels<br />
Cassini<br />
Castel<br />
Castelnuovo<br />
Castigliano<br />
Castillon<br />
Catalan
[Cataldi] Cataldi Pietro (1548-1626)<br />
Cataldi<br />
Cauchy<br />
[Cauchy] Cauchy Augustin-Louis (1789-1857) French mathematician who introduced modern notions <strong>of</strong> continuity<br />
limit, convergence and differentiability, proved Cauchy’s theorem in group theory, contributed to the<br />
calculus <strong>of</strong> variations, probability theory and the study <strong>of</strong> differential equations.<br />
Cavalieri<br />
[Cavalieri] Cavalieri Bonaventura (1598-1647) Italian mathematician. Introduced method <strong>of</strong> indivisibles, a<br />
forerunner <strong>of</strong> integral calculus to determine the area enclosed by certain curves.<br />
Cayley<br />
[Cayley] Cayley Arthur (1821-1895) English mathematician working in the theory <strong>of</strong> matrices, abstract groups<br />
and algebraic geometry.<br />
[Cech] Cech Eduard (1893-1960)<br />
[Cesaro] Cesàro Ernesto (1859-1906)<br />
[CevaGiovanni] Ceva Giovanni (1647-1734)<br />
[CevaTommaso] Ceva Tommaso (1648-1737)<br />
[Chatelet] Chatelet Gabrielle du (1706-1749)<br />
Cech<br />
Cesaro<br />
CevaGiovanni<br />
CevaTommaso<br />
Chatelet
[Chandrasekhar] Chandrasekhar Subrah. (1910-1995)<br />
[Chang] Chang Sun-Yung Alice<br />
[Chaplygin] Chaplygin Sergi (1869-1942)<br />
[Chapman] Chapman Sydney (1888-1970)<br />
[Chasles] Chasles Michel (1793-1880)<br />
[Chebotaryov] Chebotaryov Nikolai (1894-1947)<br />
[Chebyshev] Chebyshev Pafnuty (1821-1894)<br />
[Chern] Chern Shiing-shen<br />
[Chernikov] Chernikov Sergei (1912-1987)<br />
Chandrasekhar<br />
Chang<br />
Chaplygin<br />
Chapman<br />
Chasles<br />
Chebotaryov<br />
Chebyshev<br />
Chern<br />
Chernikov
[Chevalley] Chevalley Claude (1909-1984)<br />
[Ch’in] Chiu-Shao Ch’in (1202-1261)<br />
[Chowla] Chowla Sarvadaman (1907-1995)<br />
[Christ<strong>of</strong>fel] Christ<strong>of</strong>fel Elwin (1829-1900)<br />
[Chrysippus] Chrysippus (280BC-206BC)<br />
[Chrystal] Chrystal George (1851-1911)<br />
[Chuquet] Chuquet Nicolas (1445-1500)<br />
Chevalley<br />
Ch’in<br />
Chowla<br />
Christ<strong>of</strong>fel<br />
Chrysippus<br />
Chrystal<br />
Chuquet<br />
Church<br />
[Church] Church Alonzo (1903-1995) American mathematical logician.<br />
Clairaut<br />
[Clairaut] Clairaut Alexis (1713-1765) French mathematician and physicist who worked on the problem <strong>of</strong><br />
geodesic flows, celestial mechanics and cubic curves.
[Clapeyron] Clapeyron Emile (1799-1864)<br />
[Clarke] Clarke Samuel (1675-1729)<br />
[Clausen] Clausen Thomas (1801-1885)<br />
[Clausius] Clausius Rudolf (1822-1888)<br />
[Clavius] Clavius Christopher (1537-1612)<br />
[Clebsch] Clebsch Alfred (1833-1872)<br />
[Cleomedes] Cleomedes Cleomedes (10AD-70)<br />
[Clifford] Clifford William (1845-1879)<br />
[Coates] Coates John<br />
Clapeyron<br />
Clarke<br />
Clausen<br />
Clausius<br />
Clavius<br />
Clebsch<br />
Cleomedes<br />
Clifford<br />
Coates
[Coble] Coble Arthur (1878-1966)<br />
[Cochran] Cochran William (1909-1980)<br />
[Cocker] Cocker Edward (1631-1675)<br />
[Codazzi] Codazzi Delfino (1824-1873)<br />
Coble<br />
Cochran<br />
Cocker<br />
Codazzi<br />
Cohen<br />
[Cohen] Paul Joseph (1934-) American mathematician who resolved the status <strong>of</strong> the continuum hypothesis.<br />
[Cole] Cole Frank (1861-1926)<br />
[Collingwood] Collingwood Edward (1900-1970)<br />
[Collins] Collins John (1625-1683)<br />
[Condorcet] Condorcet Marie Jean (1743-1794)<br />
Cole<br />
Collingwood<br />
Collins<br />
Condorcet
[Connes] Connes Alain<br />
[Conon] Conon <strong>of</strong> Samos (280BC-220BC)<br />
[ConwayArthur] Conway Arthur (1875-1950)<br />
[Conway] Conway John<br />
[Coolidge] Coolidge Julian (1873-1954)<br />
[Cooper] Cooper Lionel (1915-1977)<br />
[Copernicus] Copernicus Nicolaus (1473-1543)<br />
[Copson] Copson Edward (1901-1980)<br />
[Cosserat] Cosserat Eugène (1866-1931)<br />
Connes<br />
Conon<br />
ConwayArthur<br />
Conway<br />
Coolidge<br />
Cooper<br />
Copernicus<br />
Copson<br />
Cosserat
[Cotes] Cotes Roger (1682-1716)<br />
[Courant] Courant Richard (1888-1972)<br />
[Cournot] Cournot Antoine (1801-1877)<br />
[Couturat] Couturat Louis (1868-1914)<br />
[Cox] Cox Gertrude (1900-1978)<br />
[Coxeter] Coxeter Donald<br />
[Craig] Craig John (1663-1731)<br />
[CramerHarald] Cramér Harald (1893-1985)<br />
[Cramer] Cramer Gabriel (1704-1752)<br />
Cotes<br />
Courant<br />
Cournot<br />
Couturat<br />
Cox<br />
Coxeter<br />
Craig<br />
CramerHarald<br />
Cramer
[Crank] Crank John<br />
[Crelle] Crelle August (1780-1855)<br />
[Cremona] Cremona Luigi (1830-1903)<br />
[Crighton] Crighton David (1942-2000)<br />
[Cunha] Cunha Anastäcio da (1744-1787)<br />
[Cunningham] Cunningham Ebenezer (1881-1977)<br />
[Curry] Curry Haskell (1900-1982)<br />
[Cusa] Cusa Nicholas <strong>of</strong> (1401-1464)<br />
[Durer] Dürer Albrecht (1471-1528)<br />
Crank<br />
Crelle<br />
Cremona<br />
Crighton<br />
Cunha<br />
Cunningham<br />
Curry<br />
Cusa<br />
Durer
[Dandelin] Dandelin Germinal (1794-1847)<br />
[Danti] Danti Egnatio (1536-1586)<br />
[DantzigGeorge] Dantzig George<br />
[Darboux] Darboux Gaston (1842-1917)<br />
[Darwin] Darwin George (1845-1912)<br />
[Dase] Dase Zacharias (1824-1861)<br />
[Davenport] Davenport Harold (1907-1969)<br />
[Davidov] Davidov August (1823-1885)<br />
[Davies] Davies Evan Tom (1904-1973)<br />
Dandelin<br />
Danti<br />
DantzigGeorge<br />
Darboux<br />
Darwin<br />
Dase<br />
Davenport<br />
Davidov<br />
Davies
[Dechales] Dechales Claude (1621-1678)<br />
[Dedekind] Dedekind Richard (1831-1916)<br />
[Dee] Dee John (1527-1608)<br />
[Dehn] Dehn Max (1878-1952)<br />
[Delamain] Delamain Richard (1600-1644)<br />
[Delambre] Delambre Jean Baptiste (1749-1822)<br />
[Delaunay] Delaunay Charles (1816-1872)<br />
[Deligne] Deligne Pierre<br />
[Delone] Delone Boris (1890-1973)<br />
Dechales<br />
Dedekind<br />
Dee<br />
Dehn<br />
Delamain<br />
Delambre<br />
Delaunay<br />
Deligne<br />
Delone
[Delsarte] Delsarte Jean (1903-1968)<br />
[Democritus] Democritus <strong>of</strong> Abdera (460BC-370BC)<br />
[Denjoy] Denjoy Arnaud (1884-1974)<br />
[Deparcieux] Deparcieux Antoine (1703-1768)<br />
[Desargues] Desargues Girard (1591-1661)<br />
[Descartes] Descartes René (1596-1650)<br />
[Dickson] Dickson Leonard (1874-1954)<br />
[Dickstein] Dickstein Samuel (1851-1939)<br />
[Dieudonne] Dieudonné Jean (1906-1992)<br />
Delsarte<br />
Democritus<br />
Denjoy<br />
Deparcieux<br />
Desargues<br />
Descartes<br />
Dickson<br />
Dickstein<br />
Dieudonne
[Digges] Digges Thomas (1546-1595)<br />
[Dilworth] Dilworth Robert<br />
[Dinghas] Dinghas Alexander (1908-1974)<br />
[Dini] Dini Ulisse (1845-1918)<br />
[Dinostratus] Dinostratus (390BC-320BC)<br />
[Diocles] Diocles (240BC-180BC)<br />
[Dionis] Dionis du Séjour A (1734-1794)<br />
[Dionysodorus] Dionysodorus (250BC-190BC)<br />
[Diophantus] Diophantus <strong>of</strong> Alexandria (200-284)<br />
Digges<br />
Dilworth<br />
Dinghas<br />
Dini<br />
Dinostratus<br />
Diocles<br />
Dionis<br />
Dionysodorus<br />
Diophantus
[Dirac] Dirac Paul (1902-1984)<br />
[Dirichlet] Dirichlet Lejeune (1805-1859)<br />
[DixonArthur] Dixon Arthur Lee (1867-1955)<br />
[Dixon] Dixon Alfred (1865-1936)<br />
[Dodgson] Dodgson Charles (1832-1898)<br />
[Doeblin] Doeblin Wolfang (1915-1940)<br />
[Domninus] Domninus <strong>of</strong> Larissa (420-480)<br />
[Donaldson] Donaldson Simon<br />
[Doob] Doob Joseph<br />
Dirac<br />
Dirichlet<br />
DixonArthur<br />
Dixon<br />
Dodgson<br />
Doeblin<br />
Domninus<br />
Donaldson<br />
Doob
[Doppelmayr] Doppelmayr Johann (1671-1750)<br />
[Doppler] Doppler Christian (1803-1853)<br />
[Douglas] Douglas Jesse (1897-1965)<br />
[Dowker] Dowker Clifford (1912-1982)<br />
[Drach] Drach Jules (1871-1941)<br />
[Drinfeld] Drinfeld Vladimir<br />
[Dubreil] Dubreil Paul (1904-1994)<br />
[Dudeney] Dudeney Henry (1857-1931)<br />
[Duhamel] Duhamel Jean-Marie (1797-1872)<br />
Doppelmayr<br />
Doppler<br />
Douglas<br />
Dowker<br />
Drach<br />
Drinfeld<br />
Dubreil<br />
Dudeney<br />
Duhamel
[Duhem] Duhem Pierre (1861-1916)<br />
[Dupin] Dupin Pierre (1784-1873)<br />
[Dupre] Dupré Athanase (1808-1869)<br />
[Dynkin] Dynkin Evgenii<br />
[EckertJohn] Eckert J Presper (1919-1995)<br />
[EckertWallace] Eckert Wallace J (1902-1971)<br />
[Eckmann] Eckmann Beno<br />
[Eddington] Eddington Arthur (1882-1944)<br />
[Edge] Edge William (1904-1997)<br />
Duhem<br />
Dupin<br />
Dupre<br />
Dynkin<br />
EckertJohn<br />
EckertWallace<br />
Eckmann<br />
Eddington<br />
Edge
[Edgeworth] Edgeworth Francis (1845-1926)<br />
[Egorov] Egorov Dimitri (1869-1931)<br />
[Ehrenfest] Ehrenfest Paul (1880-1933)<br />
[Ehresmann] Ehresmann Charles (1905-1979)<br />
[Eilenberg] Eilenberg Samuel (1913-1998)<br />
[Einstein] Einstein Albert (1879-1955)<br />
[Eisenhart] Eisenhart Luther (1876-1965)<br />
[Eisenstein] Eisenstein Gotthold (1823-1852)<br />
[Elliott] Elliott Edwin (1851-1937)<br />
Edgeworth<br />
Egorov<br />
Ehrenfest<br />
Ehresmann<br />
Eilenberg<br />
Einstein<br />
Eisenhart<br />
Eisenstein<br />
Elliott
[Empedocles] Empedocles (492BC-432BC)<br />
[Engel] Engel Friedrich (1861-1941)<br />
[Enriques] Enriques Federigo (1871-1946)<br />
[Enskog] Enskog David (1884-1947)<br />
[Epstein] Epstein Paul (1871-1939)<br />
[Eratosthenes] Eratosthenes <strong>of</strong> Cyrene (276BC-197BC)<br />
[Erdelyi] Erdélyi Arthur (1908-1977)<br />
[Erdos] Erdös Paul (1913-1996)<br />
[Erlang] Erlang Agner (1878-1929)<br />
Empedocles<br />
Engel<br />
Enriques<br />
Enskog<br />
Epstein<br />
Eratosthenes<br />
Erdelyi<br />
Erdos<br />
Erlang
[Escher] Escher Maurits (1898-1972)<br />
[Esclangon] Esclangon Ernest (1876-1954)<br />
[Euclid] Euclid <strong>of</strong> Alexandria (325BC-265BC)<br />
[Eudemus] Eudemus <strong>of</strong> Rhodes (350BC-290BC)<br />
[Eudoxus] Eudoxus <strong>of</strong> Cnidus (408BC-355BC)<br />
Escher<br />
Esclangon<br />
Euclid<br />
Eudemus<br />
Eudoxus<br />
Euler<br />
[Euler] Euler Leonhard (1707-1783) Swiss mathematician, worked on practially all fields <strong>of</strong> mathematics.<br />
[Eutocius] Eutocius <strong>of</strong> Ascalon (480-540)<br />
[Evans] Evans Griffith (1887-1973)<br />
[Ezra] Ezra Rabbi Ben (1092-1167)<br />
Eutocius<br />
Evans<br />
Ezra
[FaadiBruno] Faà di Bruno Francesco (1825-1907)<br />
[Faber] Faber Georg<br />
[Fabri] Fabri Honoré (1607-1688)<br />
[FagnanoGiovanni] Fagnano Giovanni (1715-1797)<br />
[FagnanoGiulio] Fagnano Giulio (1682-1766)<br />
[Faltings] Faltings Gerd<br />
[Fano] Fano Gino (1871-1952)<br />
[Faraday] Faraday Michael (1791-1867)<br />
[Farey] Farey John (1766-1826)<br />
FaadiBruno<br />
Faber<br />
Fabri<br />
FagnanoGiovanni<br />
FagnanoGiulio<br />
Faltings<br />
Fano<br />
Faraday<br />
Farey
[Fatou] Fatou Pierre (1878-1929)<br />
[Faulhaber] Faulhaber Johann (1580-1635)<br />
[Fefferman] Fefferman Charles<br />
[Feigenbaum] Feigenbaum Mitchell<br />
[Feigl] Feigl Georg (1890-1945)<br />
[Fejer] Fejér Lipót (1880-1959)<br />
[Feller] Feller William (1906-1970)<br />
[Fermat] Fermat Pierre de (1601-1665)<br />
[Ferrar] Ferrar Bill (1893-1990)<br />
Fatou<br />
Faulhaber<br />
Fefferman<br />
Feigenbaum<br />
Feigl<br />
Fejer<br />
Feller<br />
Fermat<br />
Ferrar
[Ferrari] Ferrari Lodovico (1522-1565)<br />
[Ferrel] Ferrel William (1817-1891)<br />
[Ferro] Ferro Scipione del (1465-1526)<br />
[Feuerbach] Feuerbach Karl (1800-1834)<br />
[Feynman] Feynman Richard (1918-1988)<br />
[Fields] Fields John (1863-1932)<br />
[Finck] Finck Pierre-Joseph (1797-1870)<br />
[Fincke] Fincke Thomas (1561-1656)<br />
[FineHenry] Fine Henry (1858-1928)<br />
Ferrari<br />
Ferrel<br />
Ferro<br />
Feuerbach<br />
Feynman<br />
Fields<br />
Finck<br />
Fincke<br />
FineHenry
[Fine] Fine Oronce (1494-1555)<br />
[Finsler] Finsler Paul (1894-1970)<br />
[Fischer] Fischer Ernst (1875-1959)<br />
[Fisher] Fisher Sir Ronald (1890-1962)<br />
[Fiske] Fiske Thomas (1865-1944)<br />
[FitzGerald] FitzGerald George (1851-1901)<br />
[Flugge-Lotz] Flügge-Lotz Irmgard (1903-1974)<br />
[Flamsteed] Flamsteed John<br />
[Fomin] Fomin Sergei (1917-1975)<br />
Fine<br />
Finsler<br />
Fischer<br />
Fisher<br />
Fiske<br />
FitzGerald<br />
Flugge-Lotz<br />
Flamsteed<br />
Fomin
FontainedesBertins<br />
[FontainedesBertins] Fontaine des Bertins A (1704-1771)<br />
[Fontenelle] Fontenelle Bernard de (1657-1757)<br />
[Forsyth] Forsyth Andrew (1858-1942)<br />
[Burali-Forti] Forti Cesare Burali- (1861-1931)<br />
[Fourier] Fourier Joseph (1768-1830)<br />
[Fowler] Fowler Ralph (1889-1944)<br />
[Fox] Fox Charles (1897-1977)<br />
[Frechet] Fréchet Maurice (1878-1973)<br />
[Fraenkel] Fraenkel Adolf (1891-1965)<br />
Fontenelle<br />
Forsyth<br />
Burali-Forti<br />
Fourier<br />
Fowler<br />
Fox<br />
Frechet<br />
Fraenkel
[FrancaisJacques] Francais Jacques (1775-1833)<br />
[FrancaisFrancois] Francais Francois (1768-1810)<br />
[Francoeur] Francoeur Louis (1773-1849)<br />
[Frank] Frank Philipp (1884-1966)<br />
[Franklin] Franklin Philip (1898-1965)<br />
[FranklinBenjamin] Franklin Benjamin (1706-1790)<br />
[Frattini] Frattini Giovanni (1852-1925)<br />
[Fredholm] Fredholm Ivar (1866-1927)<br />
[Freedman] Freedman Michael<br />
FrancaisJacques<br />
FrancaisFrancois<br />
Francoeur<br />
Frank<br />
Franklin<br />
FranklinBenjamin<br />
Frattini<br />
Fredholm<br />
Freedman
[Frege] Frege Gottlob (1848-1925)<br />
[Freitag] Freitag Herta (1908-2000)<br />
[Frenet] Frenet Jean (1816-1900)<br />
[FrenicledeBessy] Frenicle de Bessy B (1605-1675)<br />
[Frenkel] Frenkel Jacov (1894-1952)<br />
[Fresnel] Fresnel Augustin (1788-1827)<br />
[Freudenthal] Freudenthal Hans (1905-1990)<br />
[Freundlich] Freundlich Finlay (1885-1964)<br />
[Friedmann] Friedmann Alexander (1888-1925)<br />
Frege<br />
Freitag<br />
Frenet<br />
FrenicledeBessy<br />
Frenkel<br />
Fresnel<br />
Freudenthal<br />
Freundlich<br />
Friedmann
[Friedrichs] Friedrichs Kurt (1901-1982)<br />
[Frisi] Frisi Paolo (1728-1784)<br />
[Frobenius] Frobenius Georg (1849-1917)<br />
[Fubini] Fubini Guido (1879-1943)<br />
[Fuchs] Fuchs Lazarus (1833-1902)<br />
[Fueter] Fueter Rudolph (1880-1950)<br />
[Fuller] Fuller R Buckminster (1895-1983)<br />
[Fuss] Fuss Nicolai (1755-1826)<br />
[Godel] Gödel Kurt (1906-1978)<br />
Friedrichs<br />
Frisi<br />
Frobenius<br />
Fubini<br />
Fuchs<br />
Fueter<br />
Fuller<br />
Fuss<br />
Godel
[Gopel] Göpel Adolph (1812-1847)<br />
[Galerkin] Galerkin Boris (1871-1945)<br />
[Galileo] Galileo Galilei (1564-1642)<br />
[Gallarati] Gallarati Dionisio<br />
[Galois] Galois Evariste (1811-1832)<br />
[Galton] Galton Francis (1822-1911)<br />
[Gassendi] Gassendi Pierre (1592-1655)<br />
[Gauss] Gauss Carl Friedrich (1777-1855)<br />
[Gegenbauer] Gegenbauer Leopold (1849-1903)<br />
Gopel<br />
Galerkin<br />
Galileo<br />
Gallarati<br />
Galois<br />
Galton<br />
Gassendi<br />
Gauss<br />
Gegenbauer
[Geiser] Geiser Karl (1843-1934)<br />
[Gelfand] Gelfand Israil<br />
[Gelfond] Gelfond Aleksandr (1906-1968)<br />
[Gellibrand] Gellibrand Henry (1597-1636)<br />
[Geminus] Geminus (10BC-60AD)<br />
[GemmaFrisius] Gemma Frisius Regnier (1508-1555)<br />
[Genocchi] Genocchi Angelo (1817-1889)<br />
[Gentzen] Gentzen Gerhard (1909-1945)<br />
[Gergonne] Gergonne Joseph (1771-1859)<br />
Geiser<br />
Gelfand<br />
Gelfond<br />
Gellibrand<br />
Geminus<br />
GemmaFrisius<br />
Genocchi<br />
Gentzen<br />
Gergonne
[Germain] Germain Sophie (1776-1831)<br />
[Gherard] Gherard <strong>of</strong> Cremona (1114-1187)<br />
[Ghetaldi] Ghetaldi Marino (1566-1626)<br />
[Gibbs] Gibbs J Willard (1839-1903)<br />
[GirardAlbert] Girard Albert (1595-1632)<br />
[GirardPierre] Girard Pierre Simon (1765-1836)<br />
[Glaisher] Glaisher James (1848-1928)<br />
[Glenie] Glenie James (1750-1817)<br />
[Gohberg] Gohberg Israel<br />
Germain<br />
Gherard<br />
Ghetaldi<br />
Gibbs<br />
GirardAlbert<br />
GirardPierre<br />
Glaisher<br />
Glenie<br />
Gohberg
[Goldbach] Goldbach Christian (1690-1764)<br />
[Goldstein] Goldstein Sydney (1903-1989)<br />
[Gompertz] Gompertz Benjamin (1779-1865)<br />
[Goodstein] Goodstein Reuben (1912-1985)<br />
[Gordan] Gordan Paul (1837-1912)<br />
[Gorenstein] Gorenstein Daniel (1923-1992)<br />
[Gosset] Gosset William (1876-1937)<br />
[Goursat] Goursat Edouard (1858-1936)<br />
[Govindasvami] Govindasvami (800-860)<br />
Goldbach<br />
Goldstein<br />
Gompertz<br />
Goodstein<br />
Gordan<br />
Gorenstein<br />
Gosset<br />
Goursat<br />
Govindasvami
[Graffe] Gräffe Karl (1799-1873)<br />
[Gram] Gram Jorgen (1850-1916)<br />
[Grandi] Grandi Guido (1671-1742)<br />
[Granville] Granville Evelyn<br />
[Grassmann] Grassmann Hermann (1808-1877)<br />
[Grave] Grave Dmitry (1863-1939)<br />
[Green] Green George (1793-1841)<br />
[Greenhill] Greenhill Alfred (1847-1927)<br />
[Gregory] Gregory James (1638-1675)<br />
Graffe<br />
Gram<br />
Grandi<br />
Granville<br />
Grassmann<br />
Grave<br />
Green<br />
Greenhill<br />
Gregory
[GregoryDuncan] Gregory Duncan (1813-1844)<br />
[GregoryDavid] Gregory David (1659-1708)<br />
[DeGroot] Groot Johannes de (1914-1972)<br />
[Grosseteste] Grosseteste Robert (1168-1253)<br />
[Grossmann] Grossmann Marcel (1878-1936)<br />
[Grothendieck] Grothendieck Alexander<br />
[Grunsky] Grunsky Helmut (1904-1986)<br />
[Guarini] Guarini Guarino (1624-1683)<br />
[Guccia] Guccia Giovanni (1855-1914)<br />
GregoryDuncan<br />
GregoryDavid<br />
DeGroot<br />
Grosseteste<br />
Grossmann<br />
Grothendieck<br />
Grunsky<br />
Guarini<br />
Guccia
[Gudermann] Gudermann Christoph (1798-1852)<br />
[Guenther] Guenther Adam (1848-1923)<br />
[Guinand] Guinand Andy (1912-1987)<br />
[Guldin] Guldin Paul (1577-1643)<br />
[Gunter] Gunter Edmund (1581-1626)<br />
[Hajek] Häjek Jaroslav (1926-1974)<br />
[Herigone] Hérigone Pierre (1580-1643)<br />
[Holder] Hölder Otto (1859-1937)<br />
[Hormander] Hörmander Lars<br />
Gudermann<br />
Guenther<br />
Guinand<br />
Guldin<br />
Gunter<br />
Hajek<br />
Herigone<br />
Holder<br />
Hormander
[Haar] Haar Alfréd (1885-1933)<br />
[Hachette] Hachette Jean (1769-1834)<br />
[Hadamard] Hadamard Jacques (1865-1963)<br />
[Hadley] Hadley John (1682-1744)<br />
[Hahn] Hahn Hans (1879-1934)<br />
[Hall] Hall Philip (1904-1982)<br />
[HallMarshall] Hall Marshall Jr. (1910-1990)<br />
[Halley] Halley Edmond (1656-1742)<br />
[Halmos] Halmos Paul<br />
Haar<br />
Hachette<br />
Hadamard<br />
Hadley<br />
Hahn<br />
Hall<br />
HallMarshall<br />
Halley<br />
Halmos
[Halphen] Halphen George (1844-1889)<br />
[Halsted] Halsted George (1853-1922)<br />
[Hamill] Hamill Christine<br />
[Hamilton] Hamilton William R (1805-1865)<br />
[HamiltonWilliam] Hamilton William (1788-1856)<br />
[Hamming] Hamming Richard W (1915-1998)<br />
[Hankel] Hankel Hermann (1839-1873)<br />
[HardyClaude] Hardy Claude (1598-1678)<br />
[Hardy] Hardy G H (1877-1947)<br />
Halphen<br />
Halsted<br />
Hamill<br />
Hamilton<br />
HamiltonWilliam<br />
Hamming<br />
Hankel<br />
HardyClaude<br />
Hardy
[Harish-Chandra] Harish-Chandra (1923-1983)<br />
[Harriot] Harriot Thomas (1560-1621)<br />
[Hartley] Hartley Brian (1939-1994)<br />
[Hartree] Hartree Douglas (1897-1958)<br />
[Hasse] Hasse Helmut (1898-1979)<br />
[Hausdorff] Hausdorff Felix (1869-1942)<br />
[Hawking] Hawking Stephen<br />
[Al-Haytham] Haytham Abu Ali al<br />
[Heath] Heath Thomas (1861-1940)<br />
Harish-Chandra<br />
Harriot<br />
Hartley<br />
Hartree<br />
Hasse<br />
Hausdorff<br />
Hawking<br />
Al-Haytham<br />
Heath
[Heaviside] Heaviside Oliver (1850-1925)<br />
[Heawood] Heawood Percy (1861-1955)<br />
[Hecht] Hecht Daniel (1777-1833)<br />
[Hecke] Hecke Erich (1887-1947)<br />
[Hedrick] Hedrick Earle (1876-1943)<br />
[Heegaard] Heegaard Poul (1871-1948)<br />
[Heilbronn] Heilbronn Hans (1908-1975)<br />
[Heine] Heine Eduard (1821-1881)<br />
[Heisenberg] Heisenberg Werner (1901-1976)<br />
Heaviside<br />
Heawood<br />
Hecht<br />
Hecke<br />
Hedrick<br />
Heegaard<br />
Heilbronn<br />
Heine<br />
Heisenberg
[Hellinger] Hellinger Ernst (1883-1950)<br />
[Helly] Helly Eduard (1884-1943)<br />
[Heng] Heng Zhang (78AD-139)<br />
[Henrici] Henrici Olaus (1840-1918)<br />
[Hensel] Hensel Kurt (1861-1941)<br />
[Heraclides] Heraclides <strong>of</strong> Pontus (387BC-312BC)<br />
[Herbrand] Herbrand Jacques (1908-1931)<br />
[Hermann] Hermann Jakob (1678-1733)<br />
[Hermite] Hermite Charles (1822-1901)<br />
Hellinger<br />
Helly<br />
Heng<br />
Henrici<br />
Hensel<br />
Heraclides<br />
Herbrand<br />
Hermann<br />
Hermite
[Heron] Heron <strong>of</strong> Alexandria (10AD-75)<br />
[HerschelCaroline] Herschel Caroline (1750-1848)<br />
[Herschel] Herschel John (1792-1871)<br />
[Herstein] Herstein Yitz (1923-1988)<br />
[Hesse] Hesse Otto (1811-1874)<br />
[Heyting] Heyting Arend (1898-1980)<br />
[Higman] Higman Graham<br />
[Hilbert] Hilbert David (1862-1943)<br />
[Hill] Hill George (1838-1914)<br />
Heron<br />
HerschelCaroline<br />
Herschel<br />
Herstein<br />
Hesse<br />
Heyting<br />
Higman<br />
Hilbert<br />
Hill
[Hille] Hille Einar (1894-1980)<br />
[Hindenburg] Hindenburg Carl (1741-1808)<br />
[Hipparchus] Hipparchus <strong>of</strong> Rhodes (190BC-120BC)<br />
[Hippias] Hippias <strong>of</strong> Elis (460BC-400BC)<br />
[Hippocrates] Hippocrates <strong>of</strong> Chios (470BC-410BC)<br />
[Hironaka] Hironaka Heisuke<br />
[Hirsch] Hirsch Kurt (1906-1986)<br />
[Hirst] Hirst Thomas (1830-1891)<br />
[Gnedenko] Hniedenko Boris (1912-1995)<br />
Hille<br />
Hindenburg<br />
Hipparchus<br />
Hippias<br />
Hippocrates<br />
Hironaka<br />
Hirsch<br />
Hirst<br />
Gnedenko
[Houel] Hoüel Jules (1823-1886)<br />
[Hobbes] Hobbes Thomas (1588-1679)<br />
[Hobson] Hobson Ernest (1856-1933)<br />
[Hodge] Hodge William (1903-1975)<br />
[Hollerith] Hollerith Herman (1860-1929)<br />
[Holmboe] Holmboe Bernt (1795-1850)<br />
[Honda] Honda Taira (1932-1975)<br />
[Hooke] Hooke Robert (1635-1703)<br />
[HopfEberhard] Hopf Eberhard (1902-1983)<br />
Houel<br />
Hobbes<br />
Hobson<br />
Hodge<br />
Hollerith<br />
Holmboe<br />
Honda<br />
Hooke<br />
HopfEberhard
[Hopf] Hopf Heinz (1894-1971)<br />
[Hopkins] Hopkins William (1793-1866)<br />
[Hopkinson] Hopkinson John (1849-1898)<br />
[Hopper] Hopper Grace (1906-1992)<br />
[Horner] Horner William (1786-1837)<br />
[Householder] Householder Alston (1904-1993)<br />
[Hsu] Hsu Pao-Lu (1910-1970)<br />
[Hubble] Hubble Edwin (1889-1953)<br />
[Hudde] Hudde Johann (1628-1704)<br />
Hopf<br />
Hopkins<br />
Hopkinson<br />
Hopper<br />
Horner<br />
Householder<br />
Hsu<br />
Hubble<br />
Hudde
[HumbertPierre] Humbert Pierre (1891-1953)<br />
[HumbertGeorges] Humbert Georges (1859-1921)<br />
[Huntington] Huntington Edward (1874-1952)<br />
[Hurewicz] Hurewicz Witold (1904-1956)<br />
[Hurwitz] Hurwitz Adolf (1859-1919)<br />
[Hutton] Hutton Charles (1737-1823)<br />
[Huygens] Huygens Christiaan (1629-1695)<br />
[Hypatia] Hypatia <strong>of</strong> Alexandria (370-415)<br />
[Hypsicles] Hypsicles <strong>of</strong> Alexandria (190BC-120BC)<br />
HumbertPierre<br />
HumbertGeorges<br />
Huntington<br />
Hurewicz<br />
Hurwitz<br />
Hutton<br />
Huygens<br />
Hypatia<br />
Hypsicles
[Ibrahim] Ibrahim ibn Sinan (908-946)<br />
[Ingham] Ingham Albert (1900-1967)<br />
[Ito] Ito Kiyosi<br />
[Ivory] Ivory James (1765-1842)<br />
[Iwasawa] Iwasawa Kenkichi (1917-1998)<br />
[Iyanaga] Iyanaga Skokichi<br />
[JabiribnAflah] Jabir ibn Aflah (1100-1160)<br />
[Jacobi] Jacobi Carl (1804-1851)<br />
[Jacobson] Jacobson Nathan (1910-1999)<br />
Ibrahim<br />
Ingham<br />
Ito<br />
Ivory<br />
Iwasawa<br />
Iyanaga<br />
JabiribnAflah<br />
Jacobi<br />
Jacobson
[Jagannatha] Jagannatha Samrat<br />
[James] James Ioan<br />
[Janiszewski] Janiszewski Zygmunt (1888-1920)<br />
[Janovskaja] Janovskaja S<strong>of</strong>’ja (1896-1966)<br />
[Jarnik] Jarnik Vojtech (1897-1970)<br />
[Al-Jawhari] Jawhari al-Abbas al (800-860)<br />
[Al-Jayyani] Jayyani Abu al<br />
[Jeans] Jeans Sir James (1877-1946)<br />
[Jeffrey] Jeffrey George (1891-1957)<br />
Jagannatha<br />
James<br />
Janiszewski<br />
Janovskaja<br />
Jarnik<br />
Al-Jawhari<br />
Al-Jayyani<br />
Jeans<br />
Jeffrey
[Jeffreys] Jeffreys Sir Harold (1891-1989)<br />
[Jensen] Jensen Johan (1859-1925)<br />
[Jerrard] Jerrard George (1804-1863)<br />
[Jevons] Jevons William (1835-1882)<br />
[Joachimsthal] Joachimsthal Ferdinand (1818-1861)<br />
[John] John Fritz<br />
[JohnsonBarry] Johnson Barry<br />
[Johnson] Johnson William (1858-1931)<br />
[JonesBurton] Jones F (1910-1999)<br />
Jeffreys<br />
Jensen<br />
Jerrard<br />
Jevons<br />
Joachimsthal<br />
John<br />
JohnsonBarry<br />
Johnson<br />
JonesBurton
[Jones] Jones William (1675-1749)<br />
[JonesVaughan] Jones Vaughan<br />
[Jonquieres] Jonquières Ernest de (1820-1901)<br />
[Jordan] Jordan Camille (1838-1922)<br />
[Jordanus] Jordanus Nemorarius (1225-1260)<br />
[Jourdain] Jourdain Philip (1879-1921)<br />
[Juel] Juel Christian (1855-1935)<br />
[Julia] Julia Gaston (1893-1978)<br />
[Jungius] Jungius Joachim (1587-1657)<br />
Jones<br />
JonesVaughan<br />
Jonquieres<br />
Jordan<br />
Jordanus<br />
Jourdain<br />
Juel<br />
Julia<br />
Jungius
[Jyesthadeva] Jyesthadeva (1500-1575)<br />
[KonigJulius] König Julius (1849-1913)<br />
[KonigSamuel] König Samuel (1712-1757)<br />
[Konigsberger] Königsberger Leo (1837-1921)<br />
[Kurschak] Kürschäk József (1864-1933)<br />
[Kac] Kac Mark (1914-1984)<br />
[Kaestner] Kaestner Abraham (1719-1800)<br />
[Kagan] Kagan Benjamin (1869-1953)<br />
[Kakutani] Kakutani Shizuo<br />
Jyesthadeva<br />
KonigJulius<br />
KonigSamuel<br />
Konigsberger<br />
Kurschak<br />
Kac<br />
Kaestner<br />
Kagan<br />
Kakutani
[Kalmar] Kalmär Läszló (1905-1976)<br />
[Kaluza] Kaluza Theodor (1885-1945)<br />
[Kaluznin] Kaluznin Lev (1914-1990)<br />
[Al-Farisi] Kamal al-Farisi (1260-1320)<br />
[Kamalakara] Kamalakara (1616-1700)<br />
[AbuKamil] Kamil Abu Shuja (850-930)<br />
[Kantorovich] Kantorovich Leonid (1912-1986)<br />
[Kaplansky] Kaplansky Irving<br />
[Al-Karaji] Karkhi al<br />
Kalmar<br />
Kaluza<br />
Kaluznin<br />
Al-Farisi<br />
Kamalakara<br />
AbuKamil<br />
Kantorovich<br />
Kaplansky<br />
Al-Karaji
[Karp] Karp Carol (1926-1972)<br />
[Al-Kashi] Kashi Ghiyath al (1390-1450)<br />
[Katyayana] Katyayana (200BC-140BC)<br />
[Keill] Keill John (1671-1721)<br />
[Kelland] Kelland Philip (1808-1879)<br />
[Kellogg] Kellogg Oliver (1878-1957)<br />
[Kemeny] Kemeny John (1926-1992)<br />
[Kempe] Kempe Alfred (1849-1922)<br />
[KendallMaurice] Kendall Maurice (1907-1983)<br />
Karp<br />
Al-Kashi<br />
Katyayana<br />
Keill<br />
Kelland<br />
Kellogg<br />
Kemeny<br />
Kempe<br />
KendallMaurice
[Kendall] Kendall David<br />
[Kepler] Kepler Johannes (1571-1630)<br />
[Kerekjarto] Kerékjärtó Béla (1898-1946)<br />
[Keynes] Keynes John Maynard (1883-1946)<br />
[Al-Khalili] Khalili Shams al (1320-1380)<br />
[Al-Khazin] Khazin Abu Jafar al (900-971)<br />
[Khinchin] Khinchin Aleksandr (1894-1959)<br />
[Al-Khujandi] Khujandi Abu al<br />
[Al-Khwarizmi] Khwarizmi Abu al- (790-850)<br />
Kendall<br />
Kepler<br />
Kerekjarto<br />
Keynes<br />
Al-Khalili<br />
Al-Khazin<br />
Khinchin<br />
Al-Khujandi<br />
Al-Khwarizmi
[Killing] Killing Wilhelm (1847-1923)<br />
[Al-Kindi] Kindi Abu al (805-873)<br />
[Kingman] Kingman John<br />
[Kirchh<strong>of</strong>f] Kirchh<strong>of</strong>f Gustav (1824-1887)<br />
[Kirkman] Kirkman Thomas (1806-1895)<br />
[Klugel] Klügel Georg (1739-1812)<br />
[Kleene] Kleene Stephen (1909-1994)<br />
[KleinOskar] Klein Oskar (1894-1977)<br />
[Klein] Klein Felix (1849-1925)<br />
Killing<br />
Al-Kindi<br />
Kingman<br />
Kirchh<strong>of</strong>f<br />
Kirkman<br />
Klugel<br />
Kleene<br />
KleinOskar<br />
Klein
[Klingenberg] Klingenberg Wilhelm<br />
[Kloosterman] Kloosterman Hendrik (1900-1968)<br />
[Kneser] Kneser Adolf (1862-1930)<br />
[KneserHellmuth] Kneser Hellmuth (1898-1973)<br />
[Knopp] Knopp Konrad (1882-1957)<br />
[Kober] Kober Hermann (1888-1973)<br />
[Kochin] Kochin Nikolai (1901-1944)<br />
[Kodaira] Kodaira Kunihiko (1915-1997)<br />
[Koebe] Koebe Paul (1882-1945)<br />
Klingenberg<br />
Kloosterman<br />
Kneser<br />
KneserHellmuth<br />
Knopp<br />
Kober<br />
Kochin<br />
Kodaira<br />
Koebe
[Koenigs] Koenigs Gabriel (1858-1931)<br />
Koenigs<br />
Kolmogorov<br />
[Kolmogorov] Kolmogorov Andrey (1903-1987) Russian probabilist who established in 1933 the mathematical<br />
foundation <strong>of</strong> probability theory and did important work also in other fields like Hamiltonian dynamics (KAM<br />
theorem) or turbulence Kolmogorov scaling.<br />
[Kolosov] Kolosov Gury (1867-1936)<br />
[KonigDenes] Konig Denes (1884-1944)<br />
[Korteweg] Korteweg Diederik (1848-1941)<br />
[Kotelnikov] Kotelnikov Aleksandr (1865-1944)<br />
[Kovalevskaya] Kovalevskaya S<strong>of</strong>ia (1850-1891)<br />
[Kramp] Kramp Christian (1760-1826)<br />
[Krawtchouk] Krawtchouk Mikhail (1892-1942)<br />
Kolosov<br />
KonigDenes<br />
Korteweg<br />
Kotelnikov<br />
Kovalevskaya<br />
Kramp<br />
Krawtchouk
[Krein] Krein Mark (1907-1989)<br />
[Kreisel] Kreisel Georg<br />
[Kronecker] Kronecker Leopold (1823-1891)<br />
[Krull] Krull Wolfgang (1899-1971)<br />
[KrylovAleksei] Krylov Aleksei (1863-1945)<br />
[KrylovNikolai] Krylov Nikolai (1879-1955)<br />
[Kulik] Kulik Yakov (1783-1863)<br />
[Kumano-Go] Kumano-Go Hitoshi (1935-1982)<br />
[Kummer] Kummer Eduard (1810-1893)<br />
Krein<br />
Kreisel<br />
Kronecker<br />
Krull<br />
KrylovAleksei<br />
KrylovNikolai<br />
Kulik<br />
Kumano-Go<br />
Kummer
[Kuratowski] Kuratowski Kazimierz (1896-1980)<br />
[Kurosh] Kurosh Aleksandr (1908-1971)<br />
[Kutta] Kutta Martin (1867-1944)<br />
[Kuttner] Kuttner Brian (1908-1992)<br />
[Leger] Léger Emile (1795-1838)<br />
[LevyPaul] Lévy Paul (1886-1971)<br />
[Lowenheim] Löwenheim Leopold (1878-1957)<br />
[Loewner] Löwner Karl (1893-1968)<br />
[DeL’Hopital] L’Hopital Guillaume de (1661-1704)<br />
Kuratowski<br />
Kurosh<br />
Kutta<br />
Kuttner<br />
Leger<br />
LevyPaul<br />
Lowenheim<br />
Loewner<br />
DeL’Hopital
[LaHire] La Hire Philippe de (1640-1718)<br />
[LaFaille] La Faille Charles de (1597-1652)<br />
[LaCondamine] La Condamine Charles de (1701-1774)<br />
[Lacroix] Lacroix Sylvestre (1765-1843)<br />
[Lagny] Lagny Thomas de (1660-1734)<br />
[Lagrange] Lagrange Joseph-Louis (1736-1813)<br />
[Laguerre] Laguerre Edmond (1834-1886)<br />
[Lakatos] Lakatos Imre (1922-1974)<br />
[Lalla] Lalla (720-790)<br />
LaHire<br />
LaFaille<br />
LaCondamine<br />
Lacroix<br />
Lagny<br />
Lagrange<br />
Laguerre<br />
Lakatos<br />
Lalla
[Lame] Lamé Gabriel (1795-1870)<br />
[Lamb] Lamb Horace (1849-1934)<br />
[Lambert] Lambert Johann (1728-1777)<br />
[Hermann<strong>of</strong>Reichenau] Lame Hermann the (1013-1054)<br />
[Lamy] Lamy Bernard (1640-1715)<br />
[Lanczos] Lanczos Cornelius (1893-1974)<br />
[Landau] Landau Edmund (1877-1938)<br />
[LandauLev] Landau Lev (1908-1968)<br />
[Landen] Landen John (1719-1790)<br />
Lame<br />
Lamb<br />
Lambert<br />
Hermann<strong>of</strong>Reichenau<br />
Lamy<br />
Lanczos<br />
Landau<br />
LandauLev<br />
Landen
[Landsberg] Landsberg Georg (1865-1912)<br />
[Langlands] Langlands Robert<br />
[Laplace] Laplace Pierre-Simon (1749-1827)<br />
[Larmor] Larmor Sir Joseph (1857-1942)<br />
[Lasker] Lasker Emanuel (1868-1941)<br />
[Kramer] Lassar Edna Kramer (1902-1984)<br />
[LaurentHermann] Laurent Hermann (1841-1908)<br />
[LaurentPierre] Laurent Pierre (1813-1854)<br />
[Lavanha] Lavanha Joao Baptista (1550-1624)<br />
Landsberg<br />
Langlands<br />
Laplace<br />
Larmor<br />
Lasker<br />
Kramer<br />
LaurentHermann<br />
LaurentPierre<br />
Lavanha
[Lavrentev] Lavrentev Mikhail (1900-1980)<br />
[Lax] Lax Gaspar (1487-1560)<br />
[LeFevre] Le Fèvre Jean (1652-1706)<br />
[Lebesgue] Lebesgue Henri (1875-1941)<br />
[Ledermann] Ledermann Walter<br />
[Leech] Leech John (1926-1992)<br />
[Lefschetz] Lefschetz Solomon (1884-1972)<br />
[Legendre] Legendre Adrien-Marie (1752-1833)<br />
[Lemoine] Lemoine Emile (1840-1912)<br />
Lavrentev<br />
Lax<br />
LeFevre<br />
Lebesgue<br />
Ledermann<br />
Leech<br />
Lefschetz<br />
Legendre<br />
Lemoine
[Leray] Leray Jean (1906-1998)<br />
[Lerch] Lerch Mathias (1860-1922)<br />
[Leshniewski] Leshniewski Stanislaw (1886-1939)<br />
[Leslie] Leslie John (1766-1832)<br />
[Leucippus] Leucippus (480BC-420BC)<br />
[Levi] Levi ben Gerson (1288-1344)<br />
[Levi-Civita] Levi-Civita Tullio (1873-1941)<br />
[Levinson] Levinson Norman (1912-1975)<br />
[LevyHyman] Levy Hyman (1889-1975)<br />
Leray<br />
Lerch<br />
Leshniewski<br />
Leslie<br />
Leucippus<br />
Levi<br />
Levi-Civita<br />
Levinson<br />
LevyHyman
[Levytsky] Levytsky Volodymyr (1872-1956)<br />
[Lexell] Lexell Anders (1740-1784)<br />
[Lexis] Lexis Wilhelm (1837-1914)<br />
[Lhuilier] Lhuilier Simon (1750-1840)<br />
[Libri] Libri Guglielmo (1803-1869)<br />
[Lie] Lie Sophus (1842-1899)<br />
[Lifshitz] Lifshitz Evgenii (1915-1985)<br />
[Lighthill] Lighthill Sir James (1924-1998)<br />
[Lindel<strong>of</strong>] Lindelöf Ernst (1870-1946)<br />
Levytsky<br />
Lexell<br />
Lexis<br />
Lhuilier<br />
Libri<br />
Lie<br />
Lifshitz<br />
Lighthill<br />
Lindel<strong>of</strong>
[Linnik] Linnik Yuri (1915-1972)<br />
[Lions] Lions Pierre-Louis<br />
[Liouville] Liouville Joseph (1809-1882)<br />
[Lipschitz] Lipschitz Rudolf (1832-1903)<br />
[Lissajous] Lissajous Jules (1822-1880)<br />
[Listing] Listing Johann (1808-1882)<br />
[Littlewood] Littlewood John E (1885-1977)<br />
[LittlewoodDudley] Littlewood Dudley (1903-1979)<br />
[Livsic] Livsic Moshe<br />
Linnik<br />
Lions<br />
Liouville<br />
Lipschitz<br />
Lissajous<br />
Listing<br />
Littlewood<br />
LittlewoodDudley<br />
Livsic
[Llull] Llull Ramon (1235-1316)<br />
[Lobachevsky] Lobachevsky Nikolai (1792-1856)<br />
[Loewy] Loewy Alfred (1873-1935)<br />
[Lopatynsky] Lopatynsky Yaroslav (1906-1981)<br />
[Lorentz] Lorentz Hendrik (1853-1928)<br />
[Love] Love Augustus (1863-1940)<br />
[Lovelace] Lovelace Augusta Ada (1815-1852)<br />
[Loyd] Loyd Samuel (1841-1911)<br />
[Lucas] Lucas F Edouard (1842-1891)<br />
Llull<br />
Lobachevsky<br />
Loewy<br />
Lopatynsky<br />
Lorentz<br />
Love<br />
Lovelace<br />
Loyd<br />
Lucas
[Lueroth] Lueroth Jacob (1844-1910)<br />
[Lukacs] Lukacs Eugene (1906-1987)<br />
[Lukasiewicz] Lukasiewicz Jan (1878-1956)<br />
[Luke] Luke Yudell (1918-1983)<br />
[Luzin] Luzin Nikolai (1883-1950)<br />
[Lyapunov] Lyapunov Aleksandr (1857-1918)<br />
[Lyndon] Lyndon Roger (1917-1988)<br />
[Meray] Méray Charles (1835-1911)<br />
[Mobius] Möbius August (1790-1868)<br />
Lueroth<br />
Lukacs<br />
Lukasiewicz<br />
Luke<br />
Luzin<br />
Lyapunov<br />
Lyndon<br />
Meray<br />
Mobius
[MacCullagh] MacCullagh James (1809-1896)<br />
[MacLane] MacLane Saunders<br />
[MacMahon] MacMahon Percy (1854-1929)<br />
[Macaulay] Macaulay Francis (1862-1937)<br />
[Macdonald] Macdonald Hector (1865-1935)<br />
[Maclaurin] Maclaurin Colin (1698-1746)<br />
[Madhava] Madhava Sangamagramma (1350-1425)<br />
[Al-Maghribi] Maghribi Muhyi al (1220-1280)<br />
[Magnitsky] Magnitsky Leonty (1669-1739)<br />
MacCullagh<br />
MacLane<br />
MacMahon<br />
Macaulay<br />
Macdonald<br />
Maclaurin<br />
Madhava<br />
Al-Maghribi<br />
Magnitsky
[Magnus] Magnus Wilhelm (1907-1990)<br />
[Al-Mahani] Mahani Abu al (820-880)<br />
[Mahavira] Mahavira Mahavira (800-870)<br />
[MahendraSuri] Mahendra Suri (1340-1410)<br />
[Mahler] Mahler Kurt (1903-1988)<br />
[Maior] Maior John (1469-1550)<br />
[Malcev] Malcev Anatoly (1909-1967)<br />
[Malebranche] Malebranche Nicolas (1638-1715)<br />
[Malfatti] Malfatti Francesco (1731-1807)<br />
Magnus<br />
Al-Mahani<br />
Mahavira<br />
MahendraSuri<br />
Mahler<br />
Maior<br />
Malcev<br />
Malebranche<br />
Malfatti
[Malus] Malus Etienne Louis (1775-1812)<br />
[Manava] Manava (750BC-690BC)<br />
[Mandelbrot] Mandelbrot Benoit<br />
[Mannheim] Mannheim Amédée (1831-1906)<br />
[Mansion] Mansion Paul (1844-1919)<br />
[Mansur] Mansur ibn Ali Abu<br />
[Marchenko] Marchenko Vladimir<br />
[Marcinkiewicz] Marcinkiewicz Jozef (1910-1940)<br />
[Marczewski] Marczewski Edward (1907-1976)<br />
Malus<br />
Manava<br />
Mandelbrot<br />
Mannheim<br />
Mansion<br />
Mansur<br />
Marchenko<br />
Marcinkiewicz<br />
Marczewski
[Margulis] Margulis Gregori<br />
[Marinus] Marinus <strong>of</strong> Neapolis (450-500)<br />
[Markov] Markov Andrei (1856-1922)<br />
[Al-Banna] Marrakushi al (1256-1321)<br />
[Mascheroni] Mascheroni Lorenzo (1750-1800)<br />
[Maschke] Maschke Heinrich (1853-1908)<br />
[Maseres] Maseres Francis (1731-1824)<br />
[Maskelyne] Maskelyne Nevil (1732-1811)<br />
[Mason] Mason Max (1877-1961)<br />
Margulis<br />
Marinus<br />
Markov<br />
Al-Banna<br />
Mascheroni<br />
Maschke<br />
Maseres<br />
Maskelyne<br />
Mason
[Mathews] Mathews George (1861-1922)<br />
[MathieuClaude] Mathieu Claude-Louis (1783-1875)<br />
[MathieuEmile] Mathieu Emile (1835-1890)<br />
[Matsushima] Matsushima Yozo (1921-1983)<br />
[Mauchly] Mauchly John (1907-1980)<br />
[Maupertuis] Maupertuis Pierre de (1698-1759)<br />
[Maurolico] Maurolico Francisco (1494-1575)<br />
[Maxwell] Maxwell James Clerk (1831-1879)<br />
[MayerAdolph] Mayer Adolph (1839-1903)<br />
Mathews<br />
MathieuClaude<br />
MathieuEmile<br />
Matsushima<br />
Mauchly<br />
Maupertuis<br />
Maurolico<br />
Maxwell<br />
MayerAdolph
[MayerTobias] Mayer Tobias (1723-1762)<br />
[Mazur] Mazur Stanislaw (1905-1981)<br />
[Mazurkiewicz] Mazurkiewicz Stefan (1888-1945)<br />
[McClintock] McClintock John (1840-1916)<br />
[McDuff] McDuff Margaret<br />
[McShane] McShane Edward (1904-1989)<br />
[Meissel] Meissel Ernst (1826-1895)<br />
[Mellin] Mellin Hjalmar (1854-1933)<br />
[Menabrea] Menabrea Luigi (1809-1896)<br />
MayerTobias<br />
Mazur<br />
Mazurkiewicz<br />
McClintock<br />
McDuff<br />
McShane<br />
Meissel<br />
Mellin<br />
Menabrea
[Menaechmus] Menaechmus (380BC-320BC)<br />
[Menelaus] Menelaus <strong>of</strong> Alexandria (70AD-130)<br />
[Menger] Menger Karl<br />
[Mengoli] Mengoli Pietro (1626-1686)<br />
[Menshov] Menshov Dmitrii (1892-1988)<br />
[MercatorGerardus] Mercator Gerardus (1512-1592)<br />
[MercatorNicolaus] Mercator Nicolaus (1620-1687)<br />
[Mercer] Mercer James (1883-1932)<br />
[Merrifield] Merrifield Charles (1827-1884)<br />
Menaechmus<br />
Menelaus<br />
Menger<br />
Mengoli<br />
Menshov<br />
MercatorGerardus<br />
MercatorNicolaus<br />
Mercer<br />
Merrifield
[Merrill] Merrill Winifred (1862-1951)<br />
[Mersenne] Mersenne Marin (1588-1648)<br />
[Mertens] Mertens Franz (1840-1927)<br />
[Meshchersky] Meshchersky Ivan (1859-1935)<br />
[Meyer] Meyer Wilhelm (1856-1934)<br />
[Miller] Miller George (1863-1951)<br />
[Milne] Milne Edward (1896-1950)<br />
[Milnor] Milnor John<br />
[Minding] Minding Ferdinand (1806-1885)<br />
Merrill<br />
Mersenne<br />
Mertens<br />
Meshchersky<br />
Meyer<br />
Miller<br />
Milne<br />
Milnor<br />
Minding
[Mineur] Mineur Henri (1899-1954)<br />
[Minkowski] Minkowski Hermann (1864-1909)<br />
[Mirsky] Mirsky Leon (1918-1983)<br />
[Mittag-Leffler] Mittag-Leffler Gösta (1846-1927)<br />
[Mohr] Mohr Georg (1640-1697)<br />
[DeMoivre] Moivre Abraham de (1667-1754)<br />
[Molin] Molin Fedor (1861-1941)<br />
[Monge] Monge Gaspard (1746-1818)<br />
[Monte] Monte Guidobaldo del (1545-1607)<br />
Mineur<br />
Minkowski<br />
Mirsky<br />
Mittag-Leffler<br />
Mohr<br />
DeMoivre<br />
Molin<br />
Monge<br />
Monte
[Montel] Montel Paul (1876-1975)<br />
[Montmort] Montmort Pierre Rémond de (1678-1719)<br />
[Montucla] Montucla Jean (1725-1799)<br />
[MooreJonas] Moore Jonas (1627-1679)<br />
[MooreRobert] Moore Robert (1882-1974)<br />
[MooreEliakim] Moore Eliakim (1862-1932)<br />
[Morawetz] Morawetz Cathleen<br />
[Mordell] Mordell Louis (1888-1972)<br />
[DeMorgan] Morgan Augustus De (1806-1871)<br />
Montel<br />
Montmort<br />
Montucla<br />
MooreJonas<br />
MooreRobert<br />
MooreEliakim<br />
Morawetz<br />
Mordell<br />
DeMorgan
[Mori] Mori Shigefumi<br />
[Morin] Morin Arthur (1795-1880)<br />
[MorinJean-Baptiste] Morin Jean-Baptiste<br />
[Morley] Morley Frank (1860-1937)<br />
[Morse] Morse Harald Marston (1892-1977)<br />
[Mostowski] Mostowski Andrzej (1913-1975)<br />
[Motzkin] Motzkin Theodore (1908-1970)<br />
[Moufang] Moufang Ruth (1905-1977)<br />
[Mouton] Mouton Gabriel (1618-1694)<br />
Mori<br />
Morin<br />
MorinJean-Baptiste<br />
Morley<br />
Morse<br />
Mostowski<br />
Motzkin<br />
Moufang<br />
Mouton
[Muir] Muir Thomas (1844-1934)<br />
[Mumford] Mumford David<br />
[Mydorge] Mydorge Claude (1585-1647)<br />
[Mytropolshy] Mytropolshy Yurii<br />
[Naimark] Naimark Mark (1909-1978)<br />
[Napier] Napier John (1550-1617)<br />
[Narayana] Narayana Pandit (1340-1400)<br />
[Al-Nasawi] Nasawi Abu al (1010-1075)<br />
[Nash] Nash John<br />
Muir<br />
Mumford<br />
Mydorge<br />
Mytropolshy<br />
Naimark<br />
Napier<br />
Narayana<br />
Al-Nasawi<br />
Nash
[Navier] Navier Claude (1785-1836)<br />
[Al-Nayrizi] Nayrizi Abu’l al (875-940)<br />
[Neile] Neile William (1637-1670)<br />
[Nekrasov] Nekrasov Aleksandr (1883-1957)<br />
[Netto] Netto Eugen (1848-1919)<br />
[Neuberg] Neuberg Joseph (1840-1926)<br />
[Neugebauer] Neugebauer Otto (1899-1990)<br />
[NeumannHanna] Neumann Hanna (1914-1971)<br />
[NeumannCarl] Neumann Carl Gottfried (1832-1925)<br />
Navier<br />
Al-Nayrizi<br />
Neile<br />
Nekrasov<br />
Netto<br />
Neuberg<br />
Neugebauer<br />
NeumannHanna<br />
NeumannCarl
[NeumannFranz] Neumann Franz Ernst (1798-1895)<br />
[NeumannBernhard] Neumann Bernhard<br />
[Nevanlinna] Nevanlinna Rolf (1895-1980)<br />
[Newcomb] Newcomb Simon (1835-1909)<br />
[Newman] Newman Maxwell (1897-1984)<br />
[Newton] Newton Sir Isaac (1643-1727)<br />
[Neyman] Neyman Jerzy (1894-1981)<br />
[Nicolson] Nicolson Phyllis (1917-1968)<br />
[Nicomachus] Nicomachus <strong>of</strong> Gerasa (60AD-120)<br />
NeumannFranz<br />
NeumannBernhard<br />
Nevanlinna<br />
Newcomb<br />
Newman<br />
Newton<br />
Neyman<br />
Nicolson<br />
Nicomachus
[Nicomedes] Nicomedes (280BC-210BC)<br />
[Nielsen] Nielsen Niels (1865-1931)<br />
[NielsenJakob] Nielsen Jacob<br />
[Nightingale] Nightingale Florence (1820-1910)<br />
[Nilakantha] Nilakantha Somayaji (1444-1544)<br />
[Niven] Niven William (1843-1917)<br />
[NoetherMax] Noether Max (1844-1921)<br />
[NoetherEmmy] Noether Emmy (1882-1935)<br />
[Novikov] Novikov Petr (1901-1975)<br />
Nicomedes<br />
Nielsen<br />
NielsenJakob<br />
Nightingale<br />
Nilakantha<br />
Niven<br />
NoetherMax<br />
NoetherEmmy<br />
Novikov
[NovikovSergi] Novikov Sergi<br />
[Oenopides] Oenopides <strong>of</strong> Chios (490BC-420BC)<br />
[Ohm] Ohm Georg Simon (1789-1854)<br />
[Oka] Oka Kiyoshi (1901-1978)<br />
[Olivier] Olivier Théodore (1793-1853)<br />
[Khayyam] Omar Khayyam (1048-1122)<br />
[Oresme] Oresme Nicole d’ (1323-1382)<br />
[Orlicz] Orlicz Wladyslaw (1903-1990)<br />
[Ortega] Ortega Juan de (1480-1568)<br />
NovikovSergi<br />
Oenopides<br />
Ohm<br />
Oka<br />
Olivier<br />
Khayyam<br />
Oresme<br />
Orlicz<br />
Ortega
[Osgood] Osgood William (1864-1943)<br />
[Osipovsky] Osipovsky Tim<strong>of</strong>ei (1765-1832)<br />
[Ostrogradski] Ostrogradski Mikhail (1801-1862)<br />
[Ostrowski] Ostrowski Alexander (1893-1986)<br />
[Oughtred] Oughtred William (1574-1660)<br />
[D’Ovidio] Ovidio Enrico D’ (1842-1933)<br />
[Ozanam] Ozanam Jacques (1640-1717)<br />
[Peres] Pérès Joseph (1890-1962)<br />
[Peter] Péter Rózsa (1905-1977)<br />
Osgood<br />
Osipovsky<br />
Ostrogradski<br />
Ostrowski<br />
Oughtred<br />
D’Ovidio<br />
Ozanam<br />
Peres<br />
Peter
[Polya] Pólya George (1887-1985)<br />
[Pacioli] Pacioli Luca (1445-1517)<br />
[Pade] Padé Henri (1863-1953)<br />
[Padoa] Padoa Alessandro (1868-1937)<br />
[LePaige] Paige Constantin Le (1852-1929)<br />
[Painleve] Painlevé Paul (1863-1933)<br />
[Paley] Paley Raymond (1907-1933)<br />
[Paman] Paman Roger (1710-1748)<br />
[Panini] Panini (520BC-460BC)<br />
Polya<br />
Pacioli<br />
Pade<br />
Padoa<br />
LePaige<br />
Painleve<br />
Paley<br />
Paman<br />
Panini
[Papin] Papin Denis (1647-1712)<br />
[Pappus] Pappus <strong>of</strong> Alexandria (290-350)<br />
[Pars] Pars Leopold (1896-1985)<br />
[Parseval] Parseval des Chees M-A (1755-1836)<br />
[Pascal] Pascal Blaise (1623-1662)<br />
[PascalEtienne] Pascal Etienne (1588-1640)<br />
[Pasch] Pasch Moritz (1843-1930)<br />
[Patodi] Patodi Vijay (1945-1976)<br />
[Pauli] Pauli Wolfgang (1900-1958)<br />
Papin<br />
Pappus<br />
Pars<br />
Parseval<br />
Pascal<br />
PascalEtienne<br />
Pasch<br />
Patodi<br />
Pauli
[Peacock] Peacock George (1791-1858)<br />
[Peano] Peano Giuseppe (1858-1932)<br />
[Pearson] Pearson Karl (1857-1936)<br />
[PearsonEgon] Pearson Egon (1895-1980)<br />
[PeirceBenjamin] Peirce Benjamin (1809-1880)<br />
[PeirceCharles] Peirce Charles (1839-1914)<br />
[Pell] Pell John (1611-1685)<br />
[Penney] Penney Bill (1909-1991)<br />
[Perron] Perron Oskar (1880-1975)<br />
Peacock<br />
Peano<br />
Pearson<br />
PearsonEgon<br />
PeirceBenjamin<br />
PeirceCharles<br />
Pell<br />
Penney<br />
Perron
[Perseus] Perseus (180BC-120BC)<br />
[Petersen] Petersen Julius (1839-1910)<br />
[Peterson] Peterson Karl (1828-1881)<br />
[Petit] Petit Aléxis (1791-1820)<br />
[Petrovsky] Petrovsky Ivan (1901-1973)<br />
[Petryshyn] Petryshyn Volodymyr<br />
[Petzval] Petzval Józeph (1807-1891)<br />
[Peurbach] Peurbach Georg (1423-1461)<br />
[Pfaff] Pfaff Johann (1765-1825)<br />
Perseus<br />
Petersen<br />
Peterson<br />
Petit<br />
Petrovsky<br />
Petryshyn<br />
Petzval<br />
Peurbach<br />
Pfaff
[Pfeiffer] Pfeiffer Georgii (1872-1946)<br />
[Philon] Philon <strong>of</strong> Byzantium (280BC-220BC)<br />
[PicardEmile] Picard Emile (1856-1941)<br />
[PicardJean] Picard Jean (1620-1682)<br />
[Pieri] Pieri Mario (1860-1913)<br />
[Francesca] Piero della Francesca (1412-1492)<br />
[Pillai] Pillai K C Sreedharan (1920-1980)<br />
[Pincherle] Pincherle Salvatore (1853-1936)<br />
[Fibonacci] Pisano Leonardo Fibonacci (1170-1250)<br />
Pfeiffer<br />
Philon<br />
PicardEmile<br />
PicardJean<br />
Pieri<br />
Francesca<br />
Pillai<br />
Pincherle<br />
Fibonacci
[Pitiscus] Pitiscus Bartholomeo (1561-1613)<br />
[Plucker] Plücker Julius (1801-1868)<br />
[Plana] Plana Giovanni (1781-1864)<br />
[Planck] Planck Max (1858-1947)<br />
[Plateau] Plateau Joseph (1801-1883)<br />
[Plato] Plato (428BC-347BC)<br />
[Playfair] Playfair John (1748-1819)<br />
[Plessner] Plessner Abraham<br />
[Poincare] Poincaré J Henri (1854-1912)<br />
Pitiscus<br />
Plucker<br />
Plana<br />
Planck<br />
Plateau<br />
Plato<br />
Playfair<br />
Plessner<br />
Poincare
[Poinsot] Poinsot Louis (1777-1859)<br />
[Poisson] Poisson Siméon (1781-1840)<br />
[Poleni] Poleni Giovanni (1683-1761)<br />
[Polozii] Polozii Georgii (1914-1968)<br />
[Poncelet] Poncelet Jean-Victor (1788-1867)<br />
[Pontryagin] Pontryagin Lev (1908-1988)<br />
[Poretsky] Poretsky Platon (1846-1907)<br />
[Porphyry] Porphyry <strong>of</strong> Malchus (233-309)<br />
[Porta] Porta Giambattista Della (1535-1615)<br />
Poinsot<br />
Poisson<br />
Poleni<br />
Polozii<br />
Poncelet<br />
Pontryagin<br />
Poretsky<br />
Porphyry<br />
Porta
[Posidonius] Posidonius <strong>of</strong> Rhodes (135BC-51BC)<br />
[Post] Post Emil (1897-1954)<br />
[Potapov] Potapov Vladimir (1914-1980)<br />
[Prufer] Prüfer Heinz (1896-1934)<br />
[Pratt] Pratt John (1809-1871)<br />
[Pringsheim] Pringsheim Alfred (1850-1941)<br />
[Privalov] Privalov Ivan (1891-1941)<br />
Posidonius<br />
Post<br />
Potapov<br />
Prufer<br />
Pratt<br />
Pringsheim<br />
Privalov<br />
PrivatdeMolieres<br />
[PrivatdeMolieres] Privat de Molières Joseph (1677-1742)<br />
[Proclus] Proclus Diadochus (411-485)<br />
Proclus
[DeProny] Prony Gaspard de (1755-1839)<br />
[Prthudakasvami] Prthudakasvami (830-890)<br />
[Ptolemy] Ptolemy (85AD-165)<br />
[Puiseux] Puiseux Victor (1820-1883)<br />
[Puissant] Puissant Louis (1769-1943)<br />
[Pythagoras] Pythagoras <strong>of</strong> Samos (580BC-520BC)<br />
[Al-Qalasadi] Qalasadi Abu’l al (1412-1486)<br />
[Quetelet] Quetelet Adolphe (1796-1874)<br />
[Al-Quhi] Quhi Abu al<br />
DeProny<br />
Prthudakasvami<br />
Ptolemy<br />
Puiseux<br />
Puissant<br />
Pythagoras<br />
Al-Qalasadi<br />
Quetelet<br />
Al-Quhi
[Quillen] Quillen Daniel<br />
[Quine] Quine Willard Van (1908-2000)<br />
[Renyi] Rényi Alfréd (1921-1970)<br />
[Rado] Radó Tibor (1895-1965)<br />
[Rademacher] Rademacher Hans (1892-1969)<br />
[RadoRichard] Rado Richard (1906-1989)<br />
[Radon] Radon Johann (1887-1956)<br />
[Rahn] Rahn Johann (1622-1676)<br />
[Rajagopal] Rajagopal Cadambathur (1903-1978)<br />
Quillen<br />
Quine<br />
Renyi<br />
Rado<br />
Rademacher<br />
RadoRichard<br />
Radon<br />
Rahn<br />
Rajagopal
[Ramanujam] Ramanujam Chidambaram (1938-1974)<br />
[Ramanujan] Ramanujan Srinivasa (1887-1920)<br />
[Ramsden] Ramsden Jesse (1735-1800)<br />
[Ramsey] Ramsey Frank (1903-1930)<br />
[Ramus] Ramus Peter (1515-1572)<br />
[Rankin] Rankin Robert (1915-2001)<br />
[Rankine] Rankine William (1820-1872)<br />
[Raphson] Raphson Joseph (1648-1715)<br />
[Rasiowa] Rasiowa Helena (1917-1994)<br />
Ramanujam<br />
Ramanujan<br />
Ramsden<br />
Ramsey<br />
Ramus<br />
Rankin<br />
Rankine<br />
Raphson<br />
Rasiowa
[Razmadze] Razmadze Andrei (1889-1929)<br />
[Recorde] Recorde Robert (1510-1558)<br />
[Rees] Rees Mina (1902-1997)<br />
[Regiomontanus] Regiomontanus Johann (1436-1476)<br />
[Reichenbach] Reichenbach Hans (1891-1953)<br />
[Reidemeister] Reidemeister Kurt (1893-1971)<br />
[Reiner] Reiner Irving (1924-1986)<br />
[Remak] Remak Robert (1888-1942)<br />
[Remez] Remez Evgeny (1896-1975)<br />
Razmadze<br />
Recorde<br />
Rees<br />
Regiomontanus<br />
Reichenbach<br />
Reidemeister<br />
Reiner<br />
Remak<br />
Remez
[ReyPastor] Rey Pastor Julio (1888-1962)<br />
[Reye] Reye Theodor (1838-1919)<br />
ReyPastor<br />
Reye<br />
DuBois-Reymond<br />
[DuBois-Reymond] Reymond Paul du Bois- (1831-1889)<br />
[Reynaud] Reynaud Antoine-André (1771-1844)<br />
[Reyneau] Reyneau Charles (1656-1728)<br />
[Reynolds] Reynolds Osborne (1842-1912)<br />
[DeRham] Rham Georges de (1903-1990)<br />
[Rheticus] Rheticus Georg Joachim (1514-1574)<br />
[Riccati] Riccati Jacopo (1676-1754)<br />
Reynaud<br />
Reyneau<br />
Reynolds<br />
DeRham<br />
Rheticus<br />
Riccati
[RiccatiVincenzo] Riccati Vincenzo (1707-1775)<br />
[RicciMatteo] Ricci Matteo (1552-1610)<br />
[Ricci] Ricci Michelangelo (1619-1682)<br />
RiccatiVincenzo<br />
RicciMatteo<br />
Ricci<br />
Ricci-Curbastro<br />
[Ricci-Curbastro] Ricci-Curbastro Georgorio (1853-1925)<br />
[RichardLouis] Richard Louis (1795-1849)<br />
[RichardJules] Richard Jules (1862-1956)<br />
[Richardson] Richardson Lewis (1881-1953)<br />
[Richer] Richer Jean (1630-1696)<br />
[Richmond] Richmond Herbert (1863-1948)<br />
RichardLouis<br />
RichardJules<br />
Richardson<br />
Richer<br />
Richmond
[Riemann] Riemann G F Bernhard (1826-1866)<br />
[Ries] Ries Adam (1492-1559)<br />
[RieszMarcel] Riesz Marcel (1886-1969)<br />
[Riesz] Riesz Frigyes (1880-1956)<br />
[Ringrose] Ringrose John<br />
[Roberts] Roberts Samuel (1827-1913)<br />
[Roberval] Roberval Gilles de (1602-1675)<br />
[Robins] Robins Benjamin (1707-1751)<br />
[RobinsonJulia] Robinson Julia Bowman (1919-1985)<br />
Riemann<br />
Ries<br />
RieszMarcel<br />
Riesz<br />
Ringrose<br />
Roberts<br />
Roberval<br />
Robins<br />
RobinsonJulia
[Robinson] Robinson Abraham (1918-1974)<br />
[Rocard] Rocard Yves-André (1903-1992)<br />
[LaRoche] Roche Estienne de La (1470-1530)<br />
[Rogers] Rogers Ambrose<br />
[Rohn] Rohn Karl (1855-1920)<br />
[Rolle] Rolle Michel (1652-1719)<br />
[Rosanes] Rosanes Jakob (1842-1922)<br />
[Rosenhain] Rosenhain Johann (1816-1887)<br />
[Rota] Rota Gian-Carlo (1932-1999)<br />
Robinson<br />
Rocard<br />
LaRoche<br />
Rogers<br />
Rohn<br />
Rolle<br />
Rosanes<br />
Rosenhain<br />
Rota
[Roth] Roth Leonard (1904-1968)<br />
[RothKlaus] Roth Klaus<br />
[Routh] Routh Edward (1831-1907)<br />
[Rudio] Rudio Ferdinand (1856-1929)<br />
[Rudolff] Rudolff Christ<strong>of</strong>f (1499-1545)<br />
[Ruffini] Ruffini Paolo (1765-1822)<br />
[Runge] Runge Carle (1856-1927)<br />
[RussellScott] Russell John (1808-1882)<br />
[Russell] Russell Bertrand (1872-1970)<br />
Roth<br />
RothKlaus<br />
Routh<br />
Rudio<br />
Rudolff<br />
Ruffini<br />
Runge<br />
RussellScott<br />
Russell
[Rutherford] Rutherford Daniel E (1906-1966)<br />
[Rydberg] Rydberg Johannes (1854-1919)<br />
[Saccheri] Saccheri Giovanni (1667-1733)<br />
[Sacrobosco] Sacrobosco Johannes de (1195-1256)<br />
[Saks] Saks Stanislaw (1897-1942)<br />
[Nunez] Salaciense Pedro Nunez (1502-1587)<br />
[Salem] Salem Raphaël (1898-1963)<br />
[Salmon] Salmon George (1819-1904)<br />
[Al-Samarqandi] Samarqandi Shams al (1250-1310)<br />
Rutherford<br />
Rydberg<br />
Saccheri<br />
Sacrobosco<br />
Saks<br />
Nunez<br />
Salem<br />
Salmon<br />
Al-Samarqandi
[Al-Samawal] Samawal Ibn al (1130-1180)<br />
[Samoilenko] Samoilenko Anatoly<br />
[Sang] Sang Edward (1805-1890)<br />
[Sankara] Sankara Narayana (840-900)<br />
[Sasaki] Sasaki Shigeo<br />
[Saurin] Saurin Joseph (1659-1737)<br />
[Savage] Savage Leonard (1917-1971)<br />
[Savart] Savart Felix (1791-1841)<br />
[Savary] Savary Félix (1797-1841)<br />
Al-Samawal<br />
Samoilenko<br />
Sang<br />
Sankara<br />
Sasaki<br />
Saurin<br />
Savage<br />
Savart<br />
Savary
[Abraham] Savasorda (1070-1130)<br />
[Savile] Savile Sir Henry (1549-1622)<br />
[Schonflies] Schönflies Arthur (1853-1928)<br />
[Schatten] Schatten Robert (1911-1977)<br />
[Schauder] Schauder Juliusz (1899-1943)<br />
[Scheffe] Scheffé Henry (1907-1977)<br />
[Scheffers] Scheffers Georg (1866-1945)<br />
[Schickard] Schickard Wilhelm (1592-1635)<br />
[Schlafli] Schläfli Ludwig (1814-1895)<br />
Abraham<br />
Savile<br />
Schonflies<br />
Schatten<br />
Schauder<br />
Scheffe<br />
Scheffers<br />
Schickard<br />
Schlafli
[Schlomilch] Schlömilch Oscar (1823-1901)<br />
[Schmidt] Schmidt Erhard (1876-1959)<br />
[Schoenberg] Schoenberg Isaac (1903-1990)<br />
[Schottky] Schottky Friedrich (1851-1935)<br />
[Schoute] Schoute Pieter (1846-1923)<br />
[Schouten] Schouten Jan (1883-1971)<br />
[Schroder] Schröder Ernst (1841-1902)<br />
[Schrodinger] Schrödinger Erwin (1887-1961)<br />
[Schreier] Schreier Otto (1901-1929)<br />
Schlomilch<br />
Schmidt<br />
Schoenberg<br />
Schottky<br />
Schoute<br />
Schouten<br />
Schroder<br />
Schrodinger<br />
Schreier
[Schroeter] Schroeter Heinrich (1829-1892)<br />
[Schubert] Schubert Hermann (1848-1911)<br />
[Schur] Schur Issai (1875-1941)<br />
[Schwartz] Schwartz Laurent<br />
[SchwarzStefan] Schwarz Stefan (1914-1996)<br />
[Schwarz] Schwarz Herman (1843-1921)<br />
[Schwarzschild] Schwarzschild Karl (1873-1916)<br />
[Schwinger] Schwinger Julian (1918-1994)<br />
[Scott] Scott Charlotte (1858-1931)<br />
Schroeter<br />
Schubert<br />
Schur<br />
Schwartz<br />
SchwarzStefan<br />
Schwarz<br />
Schwarzschild<br />
Schwinger<br />
Scott
[Macintyre] Scott Sheila (1910-1960)<br />
[SegreBeniamino] Segre Beniamino (1903-1977)<br />
[SegreCorrado] Segre Corrado (1863-1924)<br />
[Seifert] Seifert Karl (1907-1996)<br />
[Selberg] Selberg Atle<br />
[Selten] Selten Reinhard<br />
[Semple] Semple Jack (1904-1985)<br />
[Serenus] Serenus (300-360)<br />
[Serre] Serre Jean-Pierre<br />
Macintyre<br />
SegreBeniamino<br />
SegreCorrado<br />
Seifert<br />
Selberg<br />
Selten<br />
Semple<br />
Serenus<br />
Serre
[Serret] Serret Joseph (1819-1885)<br />
[Servois] Servois Francois (1768-1847)<br />
[Severi] Severi Francesco (1879-1961)<br />
[Shanks] Shanks William (1812-1882)<br />
[Shannon] Shannon Claude (1916-2001)<br />
[Sharkovsky] Sharkovsky Oleksandr<br />
[Shatunovsky] Shatunovsky Samuil (1859-1929)<br />
[Shen] Shen Kua (1031-1095)<br />
[Shewhart] Shewhart Walter (1891-1967)<br />
Serret<br />
Servois<br />
Severi<br />
Shanks<br />
Shannon<br />
Sharkovsky<br />
Shatunovsky<br />
Shen<br />
Shewhart
[Shields] Shields Allen (1927-1989)<br />
[Shnirelman] Shnirelman Lev (1905-1938)<br />
[Shoda] Shoda Kenjiro (1902-1977)<br />
[Shtokalo] Shtokalo Josif (1897-1987)<br />
[Siacci] Siacci Francesco (1839-1907)<br />
[Siegel] Siegel Carl (1896-1981)<br />
[Sierpinski] Sierpinski Waclaw (1882-1969)<br />
[Siguenza] Siguenza y Gongora (1645-1700)<br />
[Al-Sijzi] Sijzi Abu al<br />
Shields<br />
Shnirelman<br />
Shoda<br />
Shtokalo<br />
Siacci<br />
Siegel<br />
Sierpinski<br />
Siguenza<br />
Al-Sijzi
[Simplicius] Simplicius Simplicius (490-560)<br />
[Simpson] Simpson Thomas (1710-1761)<br />
[Simson] Simson Robert (1687-1768)<br />
[Avicenna] Sina ibn<br />
[Sinan] Sinan ibn Thabit (880-943)<br />
[Sintsov] Sintsov Dmitrii (1867-1946)<br />
[Sitter] Sitter Willem de (1872-1934)<br />
[Skolem] Skolem Thoralf (1887-1963)<br />
[Slaught] Slaught Herbert (1861-1937)<br />
Simplicius<br />
Simpson<br />
Simson<br />
Avicenna<br />
Sinan<br />
Sintsov<br />
Sitter<br />
Skolem<br />
Slaught
[Sleszynski] Sleszynski Ivan (1854-1931)<br />
[Slutsky] Slutsky Evgeny (1880-1948)<br />
[Sluze] Sluze René de (1622-1685)<br />
[Smale] Smale Stephen<br />
[Smirnov] Smirnov Vladimir (1887-1974)<br />
[Smith] Smith Henry (1826-1883)<br />
[Sneddon] Sneddon Ian (1919-2000)<br />
[Snell] Snell Willebrord (1580-1626)<br />
[Snyder] Snyder Virgil (1869-1950)<br />
Sleszynski<br />
Slutsky<br />
Sluze<br />
Smale<br />
Smirnov<br />
Smith<br />
Sneddon<br />
Snell<br />
Snyder
[Sobolev] Sobolev Sergei (1908-1989)<br />
[Sokhotsky] Sokhotsky Yulian-Karl (1842-1927)<br />
[Sokolov] Sokolov Yurii (1896-1971)<br />
[Somerville] Somerville Mary (1780-1872)<br />
[Sommerfeld] Sommerfeld Arnold (1868-1951)<br />
[Sommerville] Sommerville Duncan (1879-1934)<br />
[Somov] Somov Osip (1815-1876)<br />
[Sonin] Sonin Nikolay (1849-1915)<br />
[Spanier] Spanier Edwin (1921-1996)<br />
Sobolev<br />
Sokhotsky<br />
Sokolov<br />
Somerville<br />
Sommerfeld<br />
Sommerville<br />
Somov<br />
Sonin<br />
Spanier
[Spence] Spence William (1777-1815)<br />
[Sporus] Sporus <strong>of</strong> Nicaea (240-300)<br />
[Spottiswoode] Spottiswoode William (1825-1883)<br />
[Sridhara] Sridhara Sridhara (870-930)<br />
[Sripati] Sripati (1019-1066)<br />
[Stackel] Stäckel Paul (1862-1919)<br />
[Stampioen] Stampioen Jan (1610-1690)<br />
[Steenrod] Steenrod Norman (1910-1971)<br />
[StefanJosef] Stefan Josef (1835-1893)<br />
Spence<br />
Sporus<br />
Spottiswoode<br />
Sridhara<br />
Sripati<br />
Stackel<br />
Stampioen<br />
Steenrod<br />
StefanJosef
[StefanPeter] Stefan Peter (1941-1978)<br />
[Steiner] Steiner Jakob (1796-1863)<br />
[Steinhaus] Steinhaus Hugo (1887-1972)<br />
[Steinitz] Steinitz Ernst (1871-1928)<br />
[Steklov] Steklov Vladimir A (1864-1926)<br />
[Stepanov] Stepanov Vyacheslaw V (1889-1950)<br />
[Stevin] Stevin Simon (1548-1620)<br />
[Stewart] Stewart Matthew (1717-1785)<br />
[Stewartson] Stewartson Keith (1925-1983)<br />
StefanPeter<br />
Steiner<br />
Steinhaus<br />
Steinitz<br />
Steklov<br />
Stepanov<br />
Stevin<br />
Stewart<br />
Stewartson
[Stieltjes] Stieltjes Thomas Jan (1856-1894)<br />
[Stifel] Stifel Michael (1487-1567)<br />
[Stirling] Stirling James (1692-1770)<br />
[Stokes] Stokes George Gabriel (1819-1903)<br />
[Stolz] Stolz Otto (1842-1905)<br />
[Stone] Stone Marshall (1903-1989)<br />
[Stott] Stott Alicia Boole (1860-1940)<br />
[Struik] Struik Dirk (1894-2000)<br />
[Rayleigh] Strutt (1842-1919)<br />
Stieltjes<br />
Stifel<br />
Stirling<br />
Stokes<br />
Stolz<br />
Stone<br />
Stott<br />
Struik<br />
Rayleigh
[Study] Study Eduard (1862-1930)<br />
[Sturm] Sturm J Charles-Francois (1803-1855)<br />
[SturmRudolf] Sturm Rudolf (1841-1919)<br />
[Subbotin] Subbotin Mikhail (1893-1966)<br />
[Suetuna] Suetuna Zyoiti (1898-1970)<br />
[Suter] Suter Heinrich (1848-1922)<br />
[Suvorov] Suvorov Georgii (1919-1984)<br />
[Swain] Swain Lorna (1891-1936)<br />
[Sylow] Sylow Ludwig (1832-1918)<br />
Study<br />
Sturm<br />
SturmRudolf<br />
Subbotin<br />
Suetuna<br />
Suter<br />
Suvorov<br />
Swain<br />
Sylow
[Sylvester] Sylvester James Joseph (1814-1897)<br />
[Synge] Synge John (1897-1995)<br />
[Szasz] Szäsz Otto (1884-1952)<br />
[Szego] Szegö Gäbor (1895-1985)<br />
[Tacquet] Tacquet Andrea (1612-1660)<br />
[Al-Baghdadi] Tahir ibn<br />
[Tait] Tait Peter Guthrie (1831-1901)<br />
[Takagi] Takagi Teiji (1875-1960)<br />
[Seki] Takakazu (1642-1708)<br />
Sylvester<br />
Synge<br />
Szasz<br />
Szego<br />
Tacquet<br />
Al-Baghdadi<br />
Tait<br />
Takagi<br />
Seki
[Talbot] Talbot Henry Fox (1800-1877)<br />
[Taniyama] Taniyama Yutaka (1927-1958)<br />
[TanneryPaul] Tannery Paul (1843-1904)<br />
[TanneryJules] Tannery Jules (1848-1910)<br />
[Tarry] Tarry Gaston (1843-1913)<br />
[Tarski] Tarski Alfred (1902-1983)<br />
[Tartaglia] Tartaglia Niccolo Fontana (1500-1557)<br />
[Tauber] Tauber Alfred (1866-1942)<br />
[Taurinus] Taurinus Franz (1794-1874)<br />
Talbot<br />
Taniyama<br />
TanneryPaul<br />
TanneryJules<br />
Tarry<br />
Tarski<br />
Tartaglia<br />
Tauber<br />
Taurinus
[Taussky-Todd] Taussky-Todd Olga<br />
[TaylorGe<strong>of</strong>frey] Taylor Ge<strong>of</strong>frey (1886-1975)<br />
[Taylor] Taylor Brook (1685-1731)<br />
[Teichmuller] Teichmüller Oswald (1913-1943)<br />
[Temple] Temple George (1901-1992)<br />
[LeTenneur] Tenneur Jacques (1610-1660)<br />
[Tetens] Tetens Johannes (1736-1807)<br />
[Thabit] Thabit ibn Qurra Abu’l (826-901)<br />
[Thales] Thales <strong>of</strong> Miletus (624BC-546BC)<br />
Taussky-Todd<br />
TaylorGe<strong>of</strong>frey<br />
Taylor<br />
Teichmuller<br />
Temple<br />
LeTenneur<br />
Tetens<br />
Thabit<br />
Thales
[Theaetetus] Theaetetus <strong>of</strong> Athens (415BC-369BC)<br />
[Theodorus] Theodorus <strong>of</strong> Cyrene (465BC-398BC)<br />
[Theodosius] Theodosius <strong>of</strong> Bithynia (160BC-90BC)<br />
[Theon<strong>of</strong>Smyrna] Theon <strong>of</strong> Smyrna (70AD-135)<br />
[Theon] Theon <strong>of</strong> Alexandria (335-395)<br />
[Thiele] Thiele Thorvald (1838-1910)<br />
[Thom] Thom René<br />
[Thomae] Thomae Johannes (1840-1921)<br />
[Thomason] Thomason Bob (1952-1995)<br />
Theaetetus<br />
Theodorus<br />
Theodosius<br />
Theon<strong>of</strong>Smyrna<br />
Theon<br />
Thiele<br />
Thom<br />
Thomae<br />
Thomason
[ThompsonJohn] Thompson John<br />
[ThompsonD’Arcy] Thompson D’Arcy W (1860-1948)<br />
[Thomson] Thomson W (1824-1907)<br />
[Thue] Thue Axel (1863-1922)<br />
[Thurston] Thurston Bill<br />
[Thymaridas] Thymaridas (400BC-350BC)<br />
[Tibbon] Tibbon Jacob ben (1236-1312)<br />
[Tietze] Tietze Heinrich (1880-1964)<br />
[Tilly] Tilly Joseph de (1837-1906)<br />
ThompsonJohn<br />
ThompsonD’Arcy<br />
Thomson<br />
Thue<br />
Thurston<br />
Thymaridas<br />
Tibbon<br />
Tietze<br />
Tilly
[Tinbergen] Tinbergen Jan (1903-1994)<br />
[Tinseau] Tinseau Charles (1748-1822)<br />
[Tisserand] Tisserand Félix (1845-1896)<br />
[Titchmarsh] Titchmarsh Edward (1899-1963)<br />
[Todd] Todd John (1908-1994)<br />
[Todhunter] Todhunter Isaac (1820-1884)<br />
[Toeplitz] Toeplitz Otto (1881-1940)<br />
[Torricelli] Torricelli Evangelista (1608-1647)<br />
[Trail] Trail William (1746-1831)<br />
Tinbergen<br />
Tinseau<br />
Tisserand<br />
Titchmarsh<br />
Todd<br />
Todhunter<br />
Toeplitz<br />
Torricelli<br />
Trail
[Tricomi] Tricomi Francesco (1897-1978)<br />
[Troughton] Troughton Edward (1753-1836)<br />
[Tsu] Tsu Ch’ung Chi (430-501)<br />
[Tukey] Tukey John (1915-2000)<br />
[Tunstall] Tunstall Cuthbert (1474-1559)<br />
[Turan] Turän Paul (1910-1976)<br />
[Turing] Turing Alan (1912-1954)<br />
[Turnbull] Turnbull Herbert (1885-1961)<br />
[Turner] Turner Peter (1586-1652)<br />
Tricomi<br />
Troughton<br />
Tsu<br />
Tukey<br />
Tunstall<br />
Turan<br />
Turing<br />
Turnbull<br />
Turner
[Al-TusiSharaf] Tusi Sharaf al (1135-1213)<br />
[Al-TusiNasir] Tusi Nasir al (1201-1274)<br />
[Tikhonov] Tychon<strong>of</strong>f Andrey (1906-1993)<br />
[UhlenbeckKaren] Uhlenbeck Karen<br />
[Uhlenbeck] Uhlenbeck George (1900-1988)<br />
[Ulam] Ulam Stanislaw (1909-1984)<br />
[UlughBeg] Ulugh Beg (1393-1449)<br />
[Al-Umawi] Umawi Abu al (1400-1489)<br />
[Upton] Upton Francis (1852-1921)<br />
Al-TusiSharaf<br />
Al-TusiNasir<br />
Tikhonov<br />
UhlenbeckKaren<br />
Uhlenbeck<br />
Ulam<br />
UlughBeg<br />
Al-Umawi<br />
Upton
[Al-Uqlidisi] Uqlidisi Abu’l al (920-980)<br />
[Urysohn] Urysohn Pavel (1898-1924)<br />
[Vacca] Vacca Giovanni (1872-1953)<br />
[Vailati] Vailati Giovanni (1863-1909)<br />
[DuVal] Val Patrick du (1903-1987)<br />
[Valerio] Valerio Luca (1552-1618)<br />
[ValleePoussin] Vallée Poussin C de (1866-1962)<br />
[Vandermonde] Vandermonde Alexandre (1735-1796)<br />
[Vandiver] Vandiver Harry (1882-1973)<br />
Al-Uqlidisi<br />
Urysohn<br />
Vacca<br />
Vailati<br />
DuVal<br />
Valerio<br />
ValleePoussin<br />
Vandermonde<br />
Vandiver
[Varahamihira] Varahamihira Varahamihira (505-587)<br />
[Varignon] Varignon Pierre (1654-1722)<br />
[Veblen] Veblen Oswald (1880-1960)<br />
[Saint-Venant] Venant Adhémar de St- (1797-1886)<br />
[Venn] Venn John (1834-1923)<br />
[Verhulst] Verhulst Pierre (1804-1849)<br />
[Vernier] Vernier Pierre (1584-1637)<br />
[Veronese] Veronese Giuseppe (1854-1917)<br />
[LeVerrier] Verrier Urbain Le (1811-1877)<br />
Varahamihira<br />
Varignon<br />
Veblen<br />
Saint-Venant<br />
Venn<br />
Verhulst<br />
Vernier<br />
Veronese<br />
LeVerrier
[Vessiot] Vessiot Ernest (1865-1952)<br />
[Viete] Viète Francois (1540-1603)<br />
[Vijayanandi] Vijayanandi<br />
[Saint-Vincent] Vincent Gregorius Saint- (1584-1667)<br />
[Leonardo] Vinci Leonardo da (1452-1519)<br />
[Vinogradov] Vinogradov Ivan (1891-1983)<br />
[Vitali] Vitali Giuseppe (1875-1932)<br />
[Viviani] Viviani Vincenzo (1622-1703)<br />
[Vlacq] Vlacq Adriaan (1600-1667)<br />
Vessiot<br />
Viete<br />
Vijayanandi<br />
Saint-Vincent<br />
Leonardo<br />
Vinogradov<br />
Vitali<br />
Viviani<br />
Vlacq
[VanVleck] Vleck Edward van (1863-1943)<br />
[Volterra] Volterra Vito (1860-1940)<br />
[Voronoy] Voronoy Georgy (1868-1908)<br />
[Vranceanu] Vranceanu Gheorghe (1900-1979)<br />
[VanderWaerden] Waerden Bartel van der (1903-1996)<br />
[Abu’l-Wafa] Wafa al-Buzjani Abu’l (940-998)<br />
[Wald] Wald Abraham (1902-1950)<br />
[WalkerJohn] Walker John (1825-1900)<br />
[WalkerArthur] Walker Ge<strong>of</strong>frey (1909-2001)<br />
VanVleck<br />
Volterra<br />
Voronoy<br />
Vranceanu<br />
VanderWaerden<br />
Abu’l-Wafa<br />
Wald<br />
WalkerJohn<br />
WalkerArthur
[Wall] Wall C Terence<br />
[Wallace] Wallace William (1768-1843)<br />
[Wallis] Wallis John (1616-1703)<br />
[Wang] Wang Hsien Chung (1918-1978)<br />
[Wangerin] Wangerin Albert (1844-1933)<br />
[Wantzel] Wantzel Pierre (1814-1894)<br />
[Waring] Waring Edward (1734-1798)<br />
[Watson] Watson G N (1886-1965)<br />
[WatsonHenry] Watson Henry (1827-1903)<br />
Wall<br />
Wallace<br />
Wallis<br />
Wang<br />
Wangerin<br />
Wantzel<br />
Waring<br />
Watson<br />
WatsonHenry
[Wazewski] Wazewski Tadeusz (1896-1972)<br />
[Weatherburn] Weatherburn Charles (1884-1974)<br />
[Weber] Weber Wilhelm (1804-1891)<br />
[WeberHeinrich] Weber Heinrich Martin (1842-1913)<br />
[Wedderburn] Wedderburn Joseph (1882-1948)<br />
[Weierstrass] Weierstrass Karl (1815-1897)<br />
[Weil] Weil André (1906-1998)<br />
[Weingarten] Weingarten Julius (1836-1910)<br />
[Weinstein] Weinstein Alexander (1897-1979)<br />
Wazewski<br />
Weatherburn<br />
Weber<br />
WeberHeinrich<br />
Wedderburn<br />
Weierstrass<br />
Weil<br />
Weingarten<br />
Weinstein
[Weisbach] Weisbach Julius (1806-1871)<br />
[Weldon] Weldon Raphael (1860-1906)<br />
[Werner] Werner Johann (1468-1522)<br />
[Wessel] Wessel Caspar (1745-1818)<br />
[West] West John (1756-1817)<br />
[Weyl] Weyl Hermann (1885-1955)<br />
[Weyr] Weyr Emil (1848-1894)<br />
[Wheeler] Wheeler Anna J Pell (1883-1966)<br />
[Whiston] Whiston William (1667-1752)<br />
Weisbach<br />
Weldon<br />
Werner<br />
Wessel<br />
West<br />
Weyl<br />
Weyr<br />
Wheeler<br />
Whiston
[White] White Henry (1861-1943)<br />
[Whitehead] Whitehead Alfred N (1861-1947)<br />
[WhiteheadHenry] Whitehead J Henry C (1904-1960)<br />
[Whitney] Whitney Hassler (1907-1989)<br />
[Whittaker] Whittaker Edmund (1873-1956)<br />
[WhittakerJohn] Whittaker John (1905-1984)<br />
[Whyburn] Whyburn Gordon (1904-1969)<br />
[Widman] Widman Johannes (1462-1498)<br />
[Wielandt] Wielandt Helmut (1910-2001)<br />
White<br />
Whitehead<br />
WhiteheadHenry<br />
Whitney<br />
Whittaker<br />
WhittakerJohn<br />
Whyburn<br />
Widman<br />
Wielandt
[Wien] Wien Wilhelm (1864-1928)<br />
[WienerNorbert] Wiener Norbert (1894-1964)<br />
[WienerChristian] Wiener Christian (1826-1896)<br />
[Wigner] Wigner Eugene (1902-1995)<br />
[Wilczynski] Wilczynski Ernest (1876-1932)<br />
[Wiles] Wiles Andrew<br />
[Wilkins] Wilkins John (1614-1672)<br />
[Wilkinson] Wilkinson Jim (1919-1986)<br />
[Wilks] Wilks Samuel (1906-1964)<br />
Wien<br />
WienerNorbert<br />
WienerChristian<br />
Wigner<br />
Wilczynski<br />
Wiles<br />
Wilkins<br />
Wilkinson<br />
Wilks
[Ockham] William <strong>of</strong> Ockham (1285-1349)<br />
[WilsonEdwin] Wilson Edwin (1879-1964)<br />
[WilsonJohn] Wilson John (1741-1793)<br />
[WilsonAlexander] Wilson Alexander (1714-1786)<br />
[Winkler] Winkler Wilhelm (1884-1984)<br />
[Wintner] Wintner Aurel (1903-1958)<br />
[Wirtinger] Wirtinger Wilhelm (1865-1945)<br />
[Wishart] Wishart John (1898-1956)<br />
[DeWitt] Witt Johan de (1625-1672)<br />
Ockham<br />
WilsonEdwin<br />
WilsonJohn<br />
WilsonAlexander<br />
Winkler<br />
Wintner<br />
Wirtinger<br />
Wishart<br />
DeWitt
[Witt] Witt Ernst (1911-1991)<br />
[Witten] Witten Edward<br />
[Wittgenstein] Wittgenstein Ludwig (1889-1951)<br />
[Wolf] Wolf Rudolph (1816-1893)<br />
[Wolfowitz] Wolfowitz Jacob (1910-1981)<br />
[Wolstenholme] Wolstenholme Joseph (1829-1891)<br />
[Woodhouse] Woodhouse Robert (1773-1827)<br />
[Woodward] Woodward Robert (1849-1924)<br />
[Wren] Wren Sir Christopher (1632-1723)<br />
Witt<br />
Witten<br />
Wittgenstein<br />
Wolf<br />
Wolfowitz<br />
Wolstenholme<br />
Woodhouse<br />
Woodward<br />
Wren
[Wronski] Wronski Hoëné (1778-1853)<br />
[Xenocrates] Xenocrates <strong>of</strong> Chalcedon (396BC-314BC)<br />
[Yang] Yang Hui (1238-1298)<br />
[Yates] Yates Frank (1902-1994)<br />
[Yativrsabha] Yativrsabha (500-570)<br />
[Yau] Yau Shing-Tung<br />
[Yavanesvara] Yavanesvara (120-180)<br />
[Yoccoz] Yoccoz Jean-Christophe<br />
[Youden] Youden William (1900-1971)<br />
Wronski<br />
Xenocrates<br />
Yang<br />
Yates<br />
Yativrsabha<br />
Yau<br />
Yavanesvara<br />
Yoccoz<br />
Youden
[Young] Young William (1863-1942)<br />
[YoungAlfred] Young Alfred (1873-1940)<br />
[ChisholmYoung] Young Grace Chisholm (1868-1944)<br />
[Yule] Yule George (1871-1951)<br />
[Yunus] Yunus Abu’l-Hasan ibn<br />
[Yushkevich] Yushkevich Adolph P (1906-1993)<br />
[Ahmed] Yusuf Ahmed ibn (835-912)<br />
[QadiZada] Zada al-Rumi Qadi (1364-1436)<br />
[Vashchenko] Zakharchenko M V- (1825-1912)<br />
Young<br />
YoungAlfred<br />
ChisholmYoung<br />
Yule<br />
Yunus<br />
Yushkevich<br />
Ahmed<br />
QadiZada<br />
Vashchenko
[Zarankiewicz] Zarankiewicz Kazimierz (1902-1959)<br />
[Zaremba] Zaremba Stanislaw (1863-1942)<br />
[Zariski] Zariski Oscar (1899-1986)<br />
[Zassenhaus] Zassenhaus Hans (1912-1991)<br />
[Zeckendorf] Zeckendorf Edouard (1901-1983)<br />
[Zeeman] Zeeman Chris<br />
[Zelmanov] Zelmanov Efim<br />
[Zeno<strong>of</strong>Sidon] Zeno <strong>of</strong> Sidon (150BC-70BC)<br />
[Zeno<strong>of</strong>Elea] Zeno <strong>of</strong> Elea (490BC-430BC)<br />
Zarankiewicz<br />
Zaremba<br />
Zariski<br />
Zassenhaus<br />
Zeckendorf<br />
Zeeman<br />
Zelmanov<br />
Zeno<strong>of</strong>Sidon<br />
Zeno<strong>of</strong>Elea
[Zenodorus] Zenodorus (200BC-140BC)<br />
[Zermelo] Zermelo Ernst (1871-1951)<br />
[Zeuthen] Zeuthen Hieronymous (1839-1920)<br />
[Chu] Zhu Shie-jie (1270-1330)<br />
[Zhukovsky] Zhukovsky Nikolay (1847-1921)<br />
[Zolotarev] Zolotarev Egor (1847-1878)<br />
[Zorn] Zorn Max (1906-1993)<br />
[Zuse] Zuse Konrad (1910-1995)<br />
[Zygmund] Zygmund Antoni (1900-1992)<br />
Zenodorus<br />
Zermelo<br />
Zeuthen<br />
Chu<br />
Zhukovsky<br />
Zolotarev<br />
Zorn<br />
Zuse<br />
Zygmund
[D’Alembert] d’Alembert Jean (1717-1783)<br />
D’Alembert<br />
BudandeBoislaurent<br />
[BudandeBoislaurent] de Boislaurent Budan (1761-1840)<br />
[Coulomb] de Coulomb Charles (1736-1806)<br />
[DeBeaune] de Beaune Florimond (1601-1652)<br />
[Carcavi] de Carcavi Pierre (1600-1684)<br />
[Broglie] de Broglie Louis duc (1892-1987)<br />
[Bougainville] de Bougainville Louis (1729-1811)<br />
[Billy] de Billy Jacques (1602-1679)<br />
[Coriolis] de Coriolis Gustave (1792-1843)<br />
Coulomb<br />
DeBeaune<br />
Carcavi<br />
Broglie<br />
Bougainville<br />
Billy<br />
Coriolis
[Hunayn] ibn Ishaq Hunayn (808-873)<br />
[Lansberge] van Lansberge Philip (1561-1632)<br />
[Roomen] van Roomen Adriaan (1561-1615)<br />
[Schooten] van Schooten Frans (1615-1660)<br />
[Dantzig] van Dantzig David (1900-1959)<br />
[Heuraet] van Heuraet Hendrik (1633-1660)<br />
[VanCeulen] van Ceulen Ludolph (1540-1610)<br />
[Amringe] van Amringe Howard (1835-1915)<br />
[Geiringer] von Mises Hilda Geiringer (1893-1973)<br />
Hunayn<br />
Lansberge<br />
Roomen<br />
Schooten<br />
Dantzig<br />
Heuraet<br />
VanCeulen<br />
Amringe<br />
Geiringer
[Helmholtz] von Helmholtz Hermann (1821-1894)<br />
[Lindemann] von Lindemann Carl (1852-1939)<br />
[Eotvos] von Eötvös Roland (1848-1919)<br />
[Segner] von Segner Johann (1704-1777)<br />
[Seidel] von Seidel Philipp (1821-1896)<br />
[VonNeumann] von Neumann John (1903-1957)<br />
[Vega] von Vega Georg (1754-1802)<br />
[Mises] von Mises Richard (1883-1953)<br />
[VonDyck] von Dyck Walther (1856-1934)<br />
Helmholtz<br />
Lindemann<br />
Eotvos<br />
Segner<br />
Seidel<br />
VonNeumann<br />
Vega<br />
Mises<br />
VonDyck
[Koch] von Koch Helge (1870-1924)<br />
[Tschirnhaus] von Tschirnhaus E (1651-1708)<br />
[Karman] von Kärmän Theodore (1881-1963)<br />
[Leibniz] von Leibniz Gottfried (1646-1719)<br />
[VonStaudt] von Staudt Karl (1798-1867)<br />
[VonBrill] von Brill Alexander (1842-1935)<br />
Koch<br />
Tschirnhaus<br />
Karman<br />
Leibniz<br />
VonStaudt<br />
VonBrill<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 1508 entries in this file.
Index<br />
Abbe, 1<br />
Abel, 1<br />
Abraham, 129<br />
AbrahamMax, 1<br />
Abu’l-Wafa, 153<br />
AbuKamil, 76<br />
Ackermann, 1<br />
Adams, 1<br />
AdamsFrank, 1<br />
Adelard, 1<br />
Adler, 1<br />
Adrain, 2<br />
Aepinus, 2<br />
Agnesi, 2<br />
Ahlfors, 2<br />
Ahmed, 162<br />
Ahmes, 2<br />
Aida, 2<br />
Aiken, 2<br />
Airy, 2<br />
Aitken, 2<br />
Ajima, 3<br />
Akhiezer, 3<br />
Al-Baghdadi, 142<br />
Al-Banna, 96<br />
Al-Battani, 11<br />
Al-Biruni, 15<br />
Al-Farisi, 76<br />
Al-Haytham, 63<br />
Al-Jawhari, 72<br />
Al-Jayyani, 72<br />
Al-Karaji, 76<br />
Al-Kashi, 77<br />
Al-Khalili, 78<br />
Al-Khazin, 78<br />
Al-Khujandi, 78<br />
Al-Khwarizmi, 78<br />
Al-Kindi, 79<br />
Al-Maghribi, 93<br />
Al-Mahani, 94<br />
Al-Nasawi, 104<br />
Al-Nayrizi, 105<br />
Al-Qalasadi, 118<br />
Al-Quhi, 118<br />
Al-Samarqandi, 127<br />
Al-Samawal, 128<br />
Al-Sijzi, 134<br />
Al-TusiNasir, 149<br />
Al-TusiSharaf, 149<br />
Al-Umawi, 149<br />
Al-Uqlidisi, 150<br />
Albanese, 3<br />
Albert, 3<br />
AlbertAbraham, 3<br />
Alberti, 3<br />
Albertus, 3<br />
Alcuin, 3<br />
Aleksandrov, 4<br />
AleksandrovAleksandr, 4<br />
Alexander, 3<br />
169<br />
AlexanderArchie, 4<br />
Ampere, 4<br />
Amringe, 166<br />
Amsler, 4<br />
Anaxagoras, 4<br />
Anderson, 4<br />
Andreev, 4<br />
Angeli, 4<br />
Anstice, 5<br />
Anthemius, 5<br />
Antiphon, 5<br />
Apastamba, 5<br />
Apollonius, 5<br />
Appell, 5<br />
Arago, 5<br />
Arbogast, 5<br />
Arbuthnot, 5<br />
Archimedes, 6<br />
Archytas, 6<br />
Arf, 6<br />
Argand, 6<br />
Aristaeus, 6<br />
Aristarchus, 6<br />
Aristotle, 6<br />
Arnauld, 6<br />
Aronhold, 6<br />
Artin, 7<br />
AryabhataI, 7<br />
AryabhataII, 7<br />
Atiyah, 7<br />
Atwood, 7<br />
Auslander, 7<br />
Autolycus, 7<br />
Avicenna, 135<br />
Babbage, 8<br />
Bachet, 8<br />
Bachmann, 8<br />
Backus, 8<br />
Bacon, 8<br />
Baer, 8<br />
Baire, 8<br />
Baker, 9<br />
BakerAlan, 8<br />
Ball, 9<br />
Balmer, 9<br />
Banach, 9<br />
Banneker, 9<br />
BanuMusa, 9<br />
BanuMusaAhmad, 9<br />
BanuMusaal-Hasan, 9<br />
BanuMusaMuhammad, 9<br />
Barbier, 10<br />
Bari, 10<br />
Barlow, 10<br />
Barnes, 10<br />
Barocius, 10<br />
Barrow, 10<br />
Bartholin, 10<br />
Batchelor, 10
Bateman, 10<br />
Battaglini, 11<br />
Baudhayana, 11<br />
Bayes, 11<br />
Beaugrand, 11<br />
Bell, 11<br />
Bellavitis, 11<br />
Beltrami, 11<br />
Bendixson, 11<br />
Benedetti, 12<br />
Bergman, 12<br />
Berkeley, 12<br />
Bernays, 12<br />
BernoulliDaniel, 12<br />
BernoulliJacob, 12<br />
BernoulliJohann, 12<br />
BernoulliNicolaus, 12<br />
Bernstein, 12<br />
BernsteinFelix, 13<br />
Bers, 13<br />
Bertini, 13<br />
Bertrand, 13<br />
Berwald, 13<br />
Berwick, 13<br />
Besicovitch, 13<br />
Bessel, 13<br />
Betti, 13<br />
Beurling, 14<br />
Bezout, 7<br />
BhaskaraI, 14<br />
BhaskaraII, 14<br />
Bianchi, 14<br />
Bieberbach, 14<br />
Bienayme, 14<br />
Billy, 165<br />
Binet, 14<br />
Bing, 14<br />
Biot, 14<br />
Birkh<strong>of</strong>f, 15<br />
Birkh<strong>of</strong>fGarrett, 15<br />
BjerknesCarl, 15<br />
BjerknesVilhelm, 15<br />
Black, 15<br />
Blaschke, 15<br />
Blichfeldt, 15<br />
Bliss, 15<br />
Bloch, 16<br />
Bobillier, 16<br />
Bocher, 7<br />
Bochner, 16<br />
Boethius, 16<br />
Boggio, 16<br />
Bohl, 16<br />
BohrHarald, 16<br />
BohrNiels, 16<br />
Boltzmann, 16<br />
Bolyai, 17<br />
BolyaiFarkas, 17<br />
Bolza, 17<br />
Bolzano, 17<br />
Bombelli, 17<br />
Bombieri, 17<br />
Bonferroni, 17<br />
Bonnet, 17<br />
Boole, 17<br />
Boone, 18<br />
Borchardt, 18<br />
Borda, 18<br />
Borel, 18<br />
Borgi, 18<br />
Born, 18<br />
Borsuk, 18<br />
Bortkiewicz, 18<br />
Bortolotti, 18<br />
Bosanquet, 19<br />
Boscovich, 19<br />
Bose, 19<br />
Bossut, 19<br />
Bougainville, 165<br />
Bouguer, 19<br />
Boulliau, 19<br />
Bouquet, 19<br />
Bour, 19<br />
Bourbaki, 19<br />
Bourgain, 20<br />
Boutroux, 20<br />
Bowditch, 20<br />
Bowen, 20<br />
Boyle, 20<br />
Boys, 20<br />
Bradwardine, 20<br />
Brahe, 20<br />
Brahmadeva, 20<br />
Brahmagupta, 21<br />
Braikenridge, 21<br />
Bramer, 21<br />
Brashman, 21<br />
Brauer, 21<br />
BrauerAlfred, 21<br />
Brianchon, 21<br />
Briggs, 21<br />
Brillouin, 21<br />
Bring, 22<br />
Brioschi, 22<br />
Briot, 22<br />
Brisson, 22<br />
Britton, 22<br />
Brocard, 22<br />
Brodetsky, 22<br />
Broglie, 165<br />
Bromwich, 22<br />
Bronowski, 22<br />
Brouncker, 23<br />
Brouwer, 23<br />
Brown, 23<br />
Browne, 23<br />
Bruno, 23<br />
Bruns, 23<br />
Bryson, 23<br />
BudandeBoislaurent, 165<br />
Buffon, 23<br />
Bugaev, 23<br />
Bukreev, 24<br />
Bunyakovsky, 24
Burali-Forti, 50<br />
Burchnall, 24<br />
Burgi, 8<br />
Burkhardt, 24<br />
Burkill, 24<br />
Burnside, 24<br />
Caccioppoli, 24<br />
Cajori, 24<br />
Calderon, 24<br />
Callippus, 25<br />
Campanus, 25<br />
Campbell, 25<br />
Camus, 25<br />
Cannell, 25<br />
Cantelli, 25<br />
Cantor, 25<br />
CantorMoritz, 25<br />
Caramuel, 25<br />
Caratheodory, 26<br />
Carcavi, 165<br />
Cardan, 26<br />
Carlitz, 26<br />
Carlyle, 26<br />
Carnot, 26<br />
CarnotSadi, 26<br />
Carslaw, 26<br />
Cartan, 26<br />
CartanHenri, 26<br />
Cartwright, 27<br />
Casorati, 27<br />
Cassels, 27<br />
Cassini, 27<br />
Castel, 27<br />
Castelnuovo, 27<br />
Castigliano, 27<br />
Castillon, 27<br />
Catalan, 27<br />
Cataldi, 28<br />
Cauchy, 28<br />
Cavalieri, 28<br />
Cayley, 28<br />
Cech, 28<br />
Cesaro, 28<br />
CevaGiovanni, 28<br />
CevaTommaso, 28<br />
Ch’in, 30<br />
Chandrasekhar, 29<br />
Chang, 29<br />
Chaplygin, 29<br />
Chapman, 29<br />
Chasles, 29<br />
Chatelet, 28<br />
Chebotaryov, 29<br />
Chebyshev, 29<br />
Chern, 29<br />
Chernikov, 29<br />
Chevalley, 30<br />
ChisholmYoung, 162<br />
Chowla, 30<br />
Christ<strong>of</strong>fel, 30<br />
Chrysippus, 30<br />
Chrystal, 30<br />
Chu, 164<br />
Chuquet, 30<br />
Church, 30<br />
Clairaut, 30<br />
Clapeyron, 31<br />
Clarke, 31<br />
Clausen, 31<br />
Clausius, 31<br />
Clavius, 31<br />
Clebsch, 31<br />
Cleomedes, 31<br />
Clifford, 31<br />
Coates, 31<br />
Coble, 32<br />
Cochran, 32<br />
Cocker, 32<br />
Codazzi, 32<br />
Cohen, 32<br />
Cole, 32<br />
Collingwood, 32<br />
Collins, 32<br />
Condorcet, 32<br />
Connes, 33<br />
Conon, 33<br />
Conway, 33<br />
ConwayArthur, 33<br />
Coolidge, 33<br />
Cooper, 33<br />
Copernicus, 33<br />
Copson, 33<br />
Coriolis, 165<br />
Cosserat, 33<br />
Cotes, 34<br />
Coulomb, 165<br />
Courant, 34<br />
Cournot, 34<br />
Couturat, 34<br />
Cox, 34<br />
Coxeter, 34<br />
Craig, 34<br />
Cramer, 34<br />
CramerHarald, 34<br />
Crank, 35<br />
Crelle, 35<br />
Cremona, 35<br />
Crighton, 35<br />
Cunha, 35<br />
Cunningham, 35<br />
Curry, 35<br />
Cusa, 35<br />
D’Alembert, 165<br />
D’Ovidio, 109<br />
Dandelin, 36<br />
Danti, 36<br />
Dantzig, 166<br />
DantzigGeorge, 36<br />
Darboux, 36<br />
Darwin, 36<br />
Dase, 36<br />
Davenport, 36<br />
Davidov, 36<br />
Davies, 36
DeBeaune, 165<br />
Dechales, 37<br />
Dedekind, 37<br />
Dee, 37<br />
DeGroot, 59<br />
Dehn, 37<br />
DeL’Hopital, 83<br />
Delamain, 37<br />
Delambre, 37<br />
Delaunay, 37<br />
Deligne, 37<br />
Delone, 37<br />
Delsarte, 38<br />
Democritus, 38<br />
DeMoivre, 101<br />
DeMorgan, 102<br />
Denjoy, 38<br />
Deparcieux, 38<br />
DeProny, 118<br />
DeRham, 122<br />
Desargues, 38<br />
Descartes, 38<br />
DeWitt, 159<br />
Dickson, 38<br />
Dickstein, 38<br />
Dieudonne, 38<br />
Digges, 39<br />
Dilworth, 39<br />
Dinghas, 39<br />
Dini, 39<br />
Dinostratus, 39<br />
Diocles, 39<br />
Dionis, 39<br />
Dionysodorus, 39<br />
Diophantus, 39<br />
Dirac, 40<br />
Dirichlet, 40<br />
Dixon, 40<br />
DixonArthur, 40<br />
Dodgson, 40<br />
Doeblin, 40<br />
Domninus, 40<br />
Donaldson, 40<br />
Doob, 40<br />
Doppelmayr, 41<br />
Doppler, 41<br />
Douglas, 41<br />
Dowker, 41<br />
Drach, 41<br />
Drinfeld, 41<br />
DuBois-Reymond, 122<br />
Dubreil, 41<br />
Dudeney, 41<br />
Duhamel, 41<br />
Duhem, 42<br />
Dupin, 42<br />
Dupre, 42<br />
Durer, 35<br />
DuVal, 150<br />
Dynkin, 42<br />
EckertJohn, 42<br />
EckertWallace, 42<br />
Eckmann, 42<br />
Eddington, 42<br />
Edge, 42<br />
Edgeworth, 43<br />
Egorov, 43<br />
Ehrenfest, 43<br />
Ehresmann, 43<br />
Eilenberg, 43<br />
Einstein, 43<br />
Eisenhart, 43<br />
Eisenstein, 43<br />
Elliott, 43<br />
Empedocles, 44<br />
Engel, 44<br />
Enriques, 44<br />
Enskog, 44<br />
Eotvos, 167<br />
Epstein, 44<br />
Eratosthenes, 44<br />
Erdelyi, 44<br />
Erdos, 44<br />
Erlang, 44<br />
Escher, 45<br />
Esclangon, 45<br />
Euclid, 45<br />
Eudemus, 45<br />
Eudoxus, 45<br />
Euler, 45<br />
Eutocius, 45<br />
Evans, 45<br />
Ezra, 45<br />
FaadiBruno, 46<br />
Faber, 46<br />
Fabri, 46<br />
FagnanoGiovanni, 46<br />
FagnanoGiulio, 46<br />
Faltings, 46<br />
Fano, 46<br />
Faraday, 46<br />
Farey, 46<br />
Fatou, 47<br />
Faulhaber, 47<br />
Fefferman, 47<br />
Feigenbaum, 47<br />
Feigl, 47<br />
Fejer, 47<br />
Feller, 47<br />
Fermat, 47<br />
Ferrar, 47<br />
Ferrari, 48<br />
Ferrel, 48<br />
Ferro, 48<br />
Feuerbach, 48<br />
Feynman, 48<br />
Fibonacci, 114<br />
Fields, 48<br />
Finck, 48<br />
Fincke, 48<br />
Fine, 49<br />
FineHenry, 48<br />
Finsler, 49<br />
Fischer, 49
Fisher, 49<br />
Fiske, 49<br />
FitzGerald, 49<br />
Flamsteed, 49<br />
Flugge-Lotz, 49<br />
Fomin, 49<br />
FontainedesBertins, 50<br />
Fontenelle, 50<br />
Forsyth, 50<br />
Fourier, 50<br />
Fowler, 50<br />
Fox, 50<br />
Fraenkel, 50<br />
FrancaisFrancois, 51<br />
FrancaisJacques, 51<br />
Francesca, 114<br />
Francoeur, 51<br />
Frank, 51<br />
Franklin, 51<br />
FranklinBenjamin, 51<br />
Frattini, 51<br />
Frechet, 50<br />
Fredholm, 51<br />
Freedman, 51<br />
Frege, 52<br />
Freitag, 52<br />
Frenet, 52<br />
FrenicledeBessy, 52<br />
Frenkel, 52<br />
Fresnel, 52<br />
Freudenthal, 52<br />
Freundlich, 52<br />
Friedmann, 52<br />
Friedrichs, 53<br />
Frisi, 53<br />
Frobenius, 53<br />
Fubini, 53<br />
Fuchs, 53<br />
Fueter, 53<br />
Fuller, 53<br />
Fuss, 53<br />
Galerkin, 54<br />
Galileo, 54<br />
Gallarati, 54<br />
Galois, 54<br />
Galton, 54<br />
Gassendi, 54<br />
Gauss, 54<br />
Gegenbauer, 54<br />
Geiringer, 166<br />
Geiser, 55<br />
Gelfand, 55<br />
Gelfond, 55<br />
Gellibrand, 55<br />
Geminus, 55<br />
GemmaFrisius, 55<br />
Genocchi, 55<br />
Gentzen, 55<br />
Gergonne, 55<br />
Germain, 56<br />
Gherard, 56<br />
Ghetaldi, 56<br />
Gibbs, 56<br />
GirardAlbert, 56<br />
GirardPierre, 56<br />
Glaisher, 56<br />
Glenie, 56<br />
Gnedenko, 67<br />
Godel, 53<br />
Gohberg, 56<br />
Goldbach, 57<br />
Goldstein, 57<br />
Gompertz, 57<br />
Goodstein, 57<br />
Gopel, 54<br />
Gordan, 57<br />
Gorenstein, 57<br />
Gosset, 57<br />
Goursat, 57<br />
Govindasvami, 57<br />
Graffe, 58<br />
Gram, 58<br />
Grandi, 58<br />
Granville, 58<br />
Grassmann, 58<br />
Grave, 58<br />
Green, 58<br />
Greenhill, 58<br />
Gregory, 58<br />
GregoryDavid, 59<br />
GregoryDuncan, 59<br />
Grosseteste, 59<br />
Grossmann, 59<br />
Grothendieck, 59<br />
Grunsky, 59<br />
Guarini, 59<br />
Guccia, 59<br />
Gudermann, 60<br />
Guenther, 60<br />
Guinand, 60<br />
Guldin, 60<br />
Gunter, 60<br />
Haar, 61<br />
Hachette, 61<br />
Hadamard, 61<br />
Hadley, 61<br />
Hahn, 61<br />
Hajek, 60<br />
Hall, 61<br />
Halley, 61<br />
HallMarshall, 61<br />
Halmos, 61<br />
Halphen, 62<br />
Halsted, 62<br />
Hamill, 62<br />
Hamilton, 62<br />
HamiltonWilliam, 62<br />
Hamming, 62<br />
Hankel, 62<br />
Hardy, 62<br />
HardyClaude, 62<br />
Harish-Chandra, 63<br />
Harriot, 63<br />
Hartley, 63
Hartree, 63<br />
Hasse, 63<br />
Hausdorff, 63<br />
Hawking, 63<br />
Heath, 63<br />
Heaviside, 64<br />
Heawood, 64<br />
Hecht, 64<br />
Hecke, 64<br />
Hedrick, 64<br />
Heegaard, 64<br />
Heilbronn, 64<br />
Heine, 64<br />
Heisenberg, 64<br />
Hellinger, 65<br />
Helly, 65<br />
Helmholtz, 167<br />
Heng, 65<br />
Henrici, 65<br />
Hensel, 65<br />
Heraclides, 65<br />
Herbrand, 65<br />
Herigone, 60<br />
Hermann, 65<br />
Hermann<strong>of</strong>Reichenau, 85<br />
Hermite, 65<br />
Heron, 66<br />
Herschel, 66<br />
HerschelCaroline, 66<br />
Herstein, 66<br />
Hesse, 66<br />
Heuraet, 166<br />
Heyting, 66<br />
Higman, 66<br />
Hilbert, 66<br />
Hill, 66<br />
Hille, 67<br />
Hindenburg, 67<br />
Hipparchus, 67<br />
Hippias, 67<br />
Hippocrates, 67<br />
Hironaka, 67<br />
Hirsch, 67<br />
Hirst, 67<br />
Hobbes, 68<br />
Hobson, 68<br />
Hodge, 68<br />
Holder, 60<br />
Hollerith, 68<br />
Holmboe, 68<br />
Honda, 68<br />
Hooke, 68<br />
Hopf, 69<br />
HopfEberhard, 68<br />
Hopkins, 69<br />
Hopkinson, 69<br />
Hopper, 69<br />
Hormander, 60<br />
Horner, 69<br />
Houel, 68<br />
Householder, 69<br />
Hsu, 69<br />
Hubble, 69<br />
Hudde, 69<br />
HumbertGeorges, 70<br />
HumbertPierre, 70<br />
Hunayn, 166<br />
Huntington, 70<br />
Hurewicz, 70<br />
Hurwitz, 70<br />
Hutton, 70<br />
Huygens, 70<br />
Hypatia, 70<br />
Hypsicles, 70<br />
Ibrahim, 71<br />
Ingham, 71<br />
Ito, 71<br />
Ivory, 71<br />
Iwasawa, 71<br />
Iyanaga, 71<br />
JabiribnAflah, 71<br />
Jacobi, 71<br />
Jacobson, 71<br />
Jagannatha, 72<br />
James, 72<br />
Janiszewski, 72<br />
Janovskaja, 72<br />
Jarnik, 72<br />
Jeans, 72<br />
Jeffrey, 72<br />
Jeffreys, 73<br />
Jensen, 73<br />
Jerrard, 73<br />
Jevons, 73<br />
Joachimsthal, 73<br />
John, 73<br />
Johnson, 73<br />
JohnsonBarry, 73<br />
Jones, 74<br />
JonesBurton, 73<br />
JonesVaughan, 74<br />
Jonquieres, 74<br />
Jordan, 74<br />
Jordanus, 74<br />
Jourdain, 74<br />
Juel, 74<br />
Julia, 74<br />
Jungius, 74<br />
Jyesthadeva, 75<br />
Kac, 75<br />
Kaestner, 75<br />
Kagan, 75<br />
Kakutani, 75<br />
Kalmar, 76<br />
Kaluza, 76<br />
Kaluznin, 76<br />
Kamalakara, 76<br />
Kantorovich, 76<br />
Kaplansky, 76<br />
Karman, 168<br />
Karp, 77<br />
Katyayana, 77
Keill, 77<br />
Kelland, 77<br />
Kellogg, 77<br />
Kemeny, 77<br />
Kempe, 77<br />
Kendall, 78<br />
KendallMaurice, 77<br />
Kepler, 78<br />
Kerekjarto, 78<br />
Keynes, 78<br />
Khayyam, 108<br />
Khinchin, 78<br />
Killing, 79<br />
Kingman, 79<br />
Kirchh<strong>of</strong>f, 79<br />
Kirkman, 79<br />
Kleene, 79<br />
Klein, 79<br />
KleinOskar, 79<br />
Klingenberg, 80<br />
Kloosterman, 80<br />
Klugel, 79<br />
Kneser, 80<br />
KneserHellmuth, 80<br />
Knopp, 80<br />
Kober, 80<br />
Koch, 168<br />
Kochin, 80<br />
Kodaira, 80<br />
Koebe, 80<br />
Koenigs, 81<br />
Kolmogorov, 81<br />
Kolosov, 81<br />
KonigDenes, 81<br />
KonigJulius, 75<br />
KonigSamuel, 75<br />
Konigsberger, 75<br />
Korteweg, 81<br />
Kotelnikov, 81<br />
Kovalevskaya, 81<br />
Kramer, 86<br />
Kramp, 81<br />
Krawtchouk, 81<br />
Krein, 82<br />
Kreisel, 82<br />
Kronecker, 82<br />
Krull, 82<br />
KrylovAleksei, 82<br />
KrylovNikolai, 82<br />
Kulik, 82<br />
Kumano-Go, 82<br />
Kummer, 82<br />
Kuratowski, 83<br />
Kurosh, 83<br />
Kurschak, 75<br />
Kutta, 83<br />
Kuttner, 83<br />
LaCondamine, 84<br />
Lacroix, 84<br />
LaFaille, 84<br />
Lagny, 84<br />
Lagrange, 84<br />
Laguerre, 84<br />
LaHire, 84<br />
Lakatos, 84<br />
Lalla, 84<br />
Lamb, 85<br />
Lambert, 85<br />
Lame, 85<br />
Lamy, 85<br />
Lanczos, 85<br />
Landau, 85<br />
LandauLev, 85<br />
Landen, 85<br />
Landsberg, 86<br />
Langlands, 86<br />
Lansberge, 166<br />
Laplace, 86<br />
Larmor, 86<br />
LaRoche, 125<br />
Lasker, 86<br />
LaurentHermann, 86<br />
LaurentPierre, 86<br />
Lavanha, 86<br />
Lavrentev, 87<br />
Lax, 87<br />
Lebesgue, 87<br />
Ledermann, 87<br />
Leech, 87<br />
LeFevre, 87<br />
Lefschetz, 87<br />
Legendre, 87<br />
Leger, 83<br />
Leibniz, 168<br />
Lemoine, 87<br />
Leonardo, 152<br />
LePaige, 110<br />
Leray, 88<br />
Lerch, 88<br />
Leshniewski, 88<br />
Leslie, 88<br />
LeTenneur, 144<br />
Leucippus, 88<br />
LeVerrier, 151<br />
Levi, 88<br />
Levi-Civita, 88<br />
Levinson, 88<br />
LevyHyman, 88<br />
LevyPaul, 83<br />
Levytsky, 89<br />
Lexell, 89<br />
Lexis, 89<br />
Lhuilier, 89<br />
Libri, 89<br />
Lie, 89<br />
Lifshitz, 89<br />
Lighthill, 89<br />
Lindel<strong>of</strong>, 89<br />
Lindemann, 167<br />
Linnik, 90<br />
Lions, 90<br />
Liouville, 90<br />
Lipschitz, 90<br />
Lissajous, 90
Listing, 90<br />
Littlewood, 90<br />
LittlewoodDudley, 90<br />
Livsic, 90<br />
Llull, 91<br />
Lobachevsky, 91<br />
Loewner, 83<br />
Loewy, 91<br />
Lopatynsky, 91<br />
Lorentz, 91<br />
Love, 91<br />
Lovelace, 91<br />
Lowenheim, 83<br />
Loyd, 91<br />
Lucas, 91<br />
Lueroth, 92<br />
Lukacs, 92<br />
Lukasiewicz, 92<br />
Luke, 92<br />
Luzin, 92<br />
Lyapunov, 92<br />
Lyndon, 92<br />
Macaulay, 93<br />
MacCullagh, 93<br />
Macdonald, 93<br />
Macintyre, 132<br />
MacLane, 93<br />
Maclaurin, 93<br />
MacMahon, 93<br />
Madhava, 93<br />
Magnitsky, 93<br />
Magnus, 94<br />
Mahavira, 94<br />
MahendraSuri, 94<br />
Mahler, 94<br />
Maior, 94<br />
Malcev, 94<br />
Malebranche, 94<br />
Malfatti, 94<br />
Malus, 95<br />
Manava, 95<br />
Mandelbrot, 95<br />
Mannheim, 95<br />
Mansion, 95<br />
Mansur, 95<br />
Marchenko, 95<br />
Marcinkiewicz, 95<br />
Marczewski, 95<br />
Margulis, 96<br />
Marinus, 96<br />
Markov, 96<br />
Mascheroni, 96<br />
Maschke, 96<br />
Maseres, 96<br />
Maskelyne, 96<br />
Mason, 96<br />
Mathews, 97<br />
MathieuClaude, 97<br />
MathieuEmile, 97<br />
Matsushima, 97<br />
Mauchly, 97<br />
Maupertuis, 97<br />
Maurolico, 97<br />
Maxwell, 97<br />
MayerAdolph, 97<br />
MayerTobias, 98<br />
Mazur, 98<br />
Mazurkiewicz, 98<br />
McClintock, 98<br />
McDuff, 98<br />
McShane, 98<br />
Meissel, 98<br />
Mellin, 98<br />
Menabrea, 98<br />
Menaechmus, 99<br />
Menelaus, 99<br />
Menger, 99<br />
Mengoli, 99<br />
Menshov, 99<br />
Meray, 92<br />
MercatorGerardus, 99<br />
MercatorNicolaus, 99<br />
Mercer, 99<br />
Merrifield, 99<br />
Merrill, 100<br />
Mersenne, 100<br />
Mertens, 100<br />
Meshchersky, 100<br />
Meyer, 100<br />
Miller, 100<br />
Milne, 100<br />
Milnor, 100<br />
Minding, 100<br />
Mineur, 101<br />
Minkowski, 101<br />
Mirsky, 101<br />
Mises, 167<br />
Mittag-Leffler, 101<br />
Mobius, 92<br />
Mohr, 101<br />
Molin, 101<br />
Monge, 101<br />
Monte, 101<br />
Montel, 102<br />
Montmort, 102<br />
Montucla, 102<br />
MooreEliakim, 102<br />
MooreJonas, 102<br />
MooreRobert, 102<br />
Morawetz, 102<br />
Mordell, 102<br />
Mori, 103<br />
Morin, 103<br />
MorinJean-Baptiste, 103<br />
Morley, 103<br />
Morse, 103<br />
Mostowski, 103<br />
Motzkin, 103<br />
Moufang, 103<br />
Mouton, 103<br />
Muir, 104<br />
Mumford, 104<br />
Mydorge, 104<br />
Mytropolshy, 104
Naimark, 104<br />
Napier, 104<br />
Narayana, 104<br />
Nash, 104<br />
Navier, 105<br />
Neile, 105<br />
Nekrasov, 105<br />
Netto, 105<br />
Neuberg, 105<br />
Neugebauer, 105<br />
NeumannBernhard, 106<br />
NeumannCarl, 105<br />
NeumannFranz, 106<br />
NeumannHanna, 105<br />
Nevanlinna, 106<br />
Newcomb, 106<br />
Newman, 106<br />
Newton, 106<br />
Neyman, 106<br />
Nicolson, 106<br />
Nicomachus, 106<br />
Nicomedes, 107<br />
Nielsen, 107<br />
NielsenJakob, 107<br />
Nightingale, 107<br />
Nilakantha, 107<br />
Niven, 107<br />
NoetherEmmy, 107<br />
NoetherMax, 107<br />
Novikov, 107<br />
NovikovSergi, 108<br />
Nunez, 127<br />
Ockham, 159<br />
Oenopides, 108<br />
Ohm, 108<br />
Oka, 108<br />
Olivier, 108<br />
Oresme, 108<br />
Orlicz, 108<br />
Ortega, 108<br />
Osgood, 109<br />
Osipovsky, 109<br />
Ostrogradski, 109<br />
Ostrowski, 109<br />
Oughtred, 109<br />
Ozanam, 109<br />
Pacioli, 110<br />
Pade, 110<br />
Padoa, 110<br />
Painleve, 110<br />
Paley, 110<br />
Paman, 110<br />
Panini, 110<br />
Papin, 111<br />
Pappus, 111<br />
Pars, 111<br />
Parseval, 111<br />
Pascal, 111<br />
PascalEtienne, 111<br />
Pasch, 111<br />
Patodi, 111<br />
Pauli, 111<br />
Peacock, 112<br />
Peano, 112<br />
Pearson, 112<br />
PearsonEgon, 112<br />
PeirceBenjamin, 112<br />
PeirceCharles, 112<br />
Pell, 112<br />
Penney, 112<br />
Peres, 109<br />
Perron, 112<br />
Perseus, 113<br />
Peter, 109<br />
Petersen, 113<br />
Peterson, 113<br />
Petit, 113<br />
Petrovsky, 113<br />
Petryshyn, 113<br />
Petzval, 113<br />
Peurbach, 113<br />
Pfaff, 113<br />
Pfeiffer, 114<br />
Philon, 114<br />
PicardEmile, 114<br />
PicardJean, 114<br />
Pieri, 114<br />
Pillai, 114<br />
Pincherle, 114<br />
Pitiscus, 115<br />
Plana, 115<br />
Planck, 115<br />
Plateau, 115<br />
Plato, 115<br />
Playfair, 115<br />
Plessner, 115<br />
Plucker, 115<br />
Poincare, 115<br />
Poinsot, 116<br />
Poisson, 116<br />
Poleni, 116<br />
Polozii, 116<br />
Polya, 110<br />
Poncelet, 116<br />
Pontryagin, 116<br />
Poretsky, 116<br />
Porphyry, 116<br />
Porta, 116<br />
Posidonius, 117<br />
Post, 117<br />
Potapov, 117<br />
Pratt, 117<br />
Pringsheim, 117<br />
Privalov, 117<br />
PrivatdeMolieres, 117<br />
Proclus, 117<br />
Prthudakasvami, 118<br />
Prufer, 117<br />
Ptolemy, 118<br />
Puiseux, 118<br />
Puissant, 118<br />
Pythagoras, 118<br />
QadiZada, 162
Quetelet, 118<br />
Quillen, 119<br />
Quine, 119<br />
Rademacher, 119<br />
Rado, 119<br />
Radon, 119<br />
RadoRichard, 119<br />
Rahn, 119<br />
Rajagopal, 119<br />
Ramanujam, 120<br />
Ramanujan, 120<br />
Ramsden, 120<br />
Ramsey, 120<br />
Ramus, 120<br />
Rankin, 120<br />
Rankine, 120<br />
Raphson, 120<br />
Rasiowa, 120<br />
Rayleigh, 140<br />
Razmadze, 121<br />
Recorde, 121<br />
Rees, 121<br />
Regiomontanus, 121<br />
Reichenbach, 121<br />
Reidemeister, 121<br />
Reiner, 121<br />
Remak, 121<br />
Remez, 121<br />
Renyi, 119<br />
Reye, 122<br />
Reynaud, 122<br />
Reyneau, 122<br />
Reynolds, 122<br />
ReyPastor, 122<br />
Rheticus, 122<br />
Riccati, 122<br />
RiccatiVincenzo, 123<br />
Ricci, 123<br />
Ricci-Curbastro, 123<br />
RicciMatteo, 123<br />
RichardJules, 123<br />
RichardLouis, 123<br />
Richardson, 123<br />
Richer, 123<br />
Richmond, 123<br />
Riemann, 124<br />
Ries, 124<br />
Riesz, 124<br />
RieszMarcel, 124<br />
Ringrose, 124<br />
Roberts, 124<br />
Roberval, 124<br />
Robins, 124<br />
Robinson, 125<br />
RobinsonJulia, 124<br />
Rocard, 125<br />
Rogers, 125<br />
Rohn, 125<br />
Rolle, 125<br />
Roomen, 166<br />
Rosanes, 125<br />
Rosenhain, 125<br />
Rota, 125<br />
Roth, 126<br />
RothKlaus, 126<br />
Routh, 126<br />
Rudio, 126<br />
Rudolff, 126<br />
Ruffini, 126<br />
Runge, 126<br />
Russell, 126<br />
RussellScott, 126<br />
Rutherford, 127<br />
Rydberg, 127<br />
Saccheri, 127<br />
Sacrobosco, 127<br />
Saint-Venant, 151<br />
Saint-Vincent, 152<br />
Saks, 127<br />
Salem, 127<br />
Salmon, 127<br />
Samoilenko, 128<br />
Sang, 128<br />
Sankara, 128<br />
Sasaki, 128<br />
Saurin, 128<br />
Savage, 128<br />
Savart, 128<br />
Savary, 128<br />
Savile, 129<br />
Schatten, 129<br />
Schauder, 129<br />
Scheffe, 129<br />
Scheffers, 129<br />
Schickard, 129<br />
Schlafli, 129<br />
Schlomilch, 130<br />
Schmidt, 130<br />
Schoenberg, 130<br />
Schonflies, 129<br />
Schooten, 166<br />
Schottky, 130<br />
Schoute, 130<br />
Schouten, 130<br />
Schreier, 130<br />
Schroder, 130<br />
Schrodinger, 130<br />
Schroeter, 131<br />
Schubert, 131<br />
Schur, 131<br />
Schwartz, 131<br />
Schwarz, 131<br />
Schwarzschild, 131<br />
SchwarzStefan, 131<br />
Schwinger, 131<br />
Scott, 131<br />
Segner, 167<br />
SegreBeniamino, 132<br />
SegreCorrado, 132<br />
Seidel, 167<br />
Seifert, 132<br />
Seki, 142<br />
Selberg, 132<br />
Selten, 132
Semple, 132<br />
Serenus, 132<br />
Serre, 132<br />
Serret, 133<br />
Servois, 133<br />
Severi, 133<br />
Shanks, 133<br />
Shannon, 133<br />
Sharkovsky, 133<br />
Shatunovsky, 133<br />
Shen, 133<br />
Shewhart, 133<br />
Shields, 134<br />
Shnirelman, 134<br />
Shoda, 134<br />
Shtokalo, 134<br />
Siacci, 134<br />
Siegel, 134<br />
Sierpinski, 134<br />
Siguenza, 134<br />
Simplicius, 135<br />
Simpson, 135<br />
Simson, 135<br />
Sinan, 135<br />
Sintsov, 135<br />
Sitter, 135<br />
Skolem, 135<br />
Slaught, 135<br />
Sleszynski, 136<br />
Slutsky, 136<br />
Sluze, 136<br />
Smale, 136<br />
Smirnov, 136<br />
Smith, 136<br />
Sneddon, 136<br />
Snell, 136<br />
Snyder, 136<br />
Sobolev, 137<br />
Sokhotsky, 137<br />
Sokolov, 137<br />
Somerville, 137<br />
Sommerfeld, 137<br />
Sommerville, 137<br />
Somov, 137<br />
Sonin, 137<br />
Spanier, 137<br />
Spence, 138<br />
Sporus, 138<br />
Spottiswoode, 138<br />
Sridhara, 138<br />
Sripati, 138<br />
Stackel, 138<br />
Stampioen, 138<br />
Steenrod, 138<br />
StefanJosef, 138<br />
StefanPeter, 139<br />
Steiner, 139<br />
Steinhaus, 139<br />
Steinitz, 139<br />
Steklov, 139<br />
Stepanov, 139<br />
Stevin, 139<br />
Stewart, 139<br />
Stewartson, 139<br />
Stieltjes, 140<br />
Stifel, 140<br />
Stirling, 140<br />
Stokes, 140<br />
Stolz, 140<br />
Stone, 140<br />
Stott, 140<br />
Struik, 140<br />
Study, 141<br />
Sturm, 141<br />
SturmRudolf, 141<br />
Subbotin, 141<br />
Suetuna, 141<br />
Suter, 141<br />
Suvorov, 141<br />
Swain, 141<br />
Sylow, 141<br />
Sylvester, 142<br />
Synge, 142<br />
Szasz, 142<br />
Szego, 142<br />
Tacquet, 142<br />
Tait, 142<br />
Takagi, 142<br />
Talbot, 143<br />
Taniyama, 143<br />
TanneryJules, 143<br />
TanneryPaul, 143<br />
Tarry, 143<br />
Tarski, 143<br />
Tartaglia, 143<br />
Tauber, 143<br />
Taurinus, 143<br />
Taussky-Todd, 144<br />
Taylor, 144<br />
TaylorGe<strong>of</strong>frey, 144<br />
Teichmuller, 144<br />
Temple, 144<br />
Tetens, 144<br />
Thabit, 144<br />
Thales, 144<br />
Theaetetus, 145<br />
Theodorus, 145<br />
Theodosius, 145<br />
Theon, 145<br />
Theon<strong>of</strong>Smyrna, 145<br />
Thiele, 145<br />
Thom, 145<br />
Thomae, 145<br />
Thomason, 145<br />
ThompsonD’Arcy, 146<br />
ThompsonJohn, 146<br />
Thomson, 146<br />
Thue, 146<br />
Thurston, 146<br />
Thymaridas, 146<br />
Tibbon, 146<br />
Tietze, 146<br />
Tikhonov, 149<br />
Tilly, 146
Tinbergen, 147<br />
Tinseau, 147<br />
Tisserand, 147<br />
Titchmarsh, 147<br />
Todd, 147<br />
Todhunter, 147<br />
Toeplitz, 147<br />
Torricelli, 147<br />
Trail, 147<br />
Tricomi, 148<br />
Troughton, 148<br />
Tschirnhaus, 168<br />
Tsu, 148<br />
Tukey, 148<br />
Tunstall, 148<br />
Turan, 148<br />
Turing, 148<br />
Turnbull, 148<br />
Turner, 148<br />
Uhlenbeck, 149<br />
UhlenbeckKaren, 149<br />
Ulam, 149<br />
UlughBeg, 149<br />
Upton, 149<br />
Urysohn, 150<br />
Vacca, 150<br />
Vailati, 150<br />
Valerio, 150<br />
ValleePoussin, 150<br />
VanCeulen, 166<br />
Vandermonde, 150<br />
VanderWaerden, 153<br />
Vandiver, 150<br />
VanVleck, 153<br />
Varahamihira, 151<br />
Varignon, 151<br />
Vashchenko, 162<br />
Veblen, 151<br />
Vega, 167<br />
Venn, 151<br />
Verhulst, 151<br />
Vernier, 151<br />
Veronese, 151<br />
Vessiot, 152<br />
Viete, 152<br />
Vijayanandi, 152<br />
Vinogradov, 152<br />
Vitali, 152<br />
Viviani, 152<br />
Vlacq, 152<br />
Volterra, 153<br />
VonBrill, 168<br />
VonDyck, 167<br />
VonNeumann, 167<br />
VonStaudt, 168<br />
Voronoy, 153<br />
Vranceanu, 153<br />
Wald, 153<br />
WalkerArthur, 153<br />
WalkerJohn, 153<br />
Wall, 154<br />
Wallace, 154<br />
Wallis, 154<br />
Wang, 154<br />
Wangerin, 154<br />
Wantzel, 154<br />
Waring, 154<br />
Watson, 154<br />
WatsonHenry, 154<br />
Wazewski, 155<br />
Weatherburn, 155<br />
Weber, 155<br />
WeberHeinrich, 155<br />
Wedderburn, 155<br />
Weierstrass, 155<br />
Weil, 155<br />
Weingarten, 155<br />
Weinstein, 155<br />
Weisbach, 156<br />
Weldon, 156<br />
Werner, 156<br />
Wessel, 156<br />
West, 156<br />
Weyl, 156<br />
Weyr, 156<br />
Wheeler, 156<br />
Whiston, 156<br />
White, 157<br />
Whitehead, 157<br />
WhiteheadHenry, 157<br />
Whitney, 157<br />
Whittaker, 157<br />
WhittakerJohn, 157<br />
Whyburn, 157<br />
Widman, 157<br />
Wielandt, 157<br />
Wien, 158<br />
WienerChristian, 158<br />
WienerNorbert, 158<br />
Wigner, 158<br />
Wilczynski, 158<br />
Wiles, 158<br />
Wilkins, 158<br />
Wilkinson, 158<br />
Wilks, 158<br />
WilsonAlexander, 159<br />
WilsonEdwin, 159<br />
WilsonJohn, 159<br />
Winkler, 159<br />
Wintner, 159<br />
Wirtinger, 159<br />
Wishart, 159<br />
Witt, 160<br />
Witten, 160<br />
Wittgenstein, 160<br />
Wolf, 160<br />
Wolfowitz, 160<br />
Wolstenholme, 160<br />
Woodhouse, 160<br />
Woodward, 160<br />
Wren, 160<br />
Wronski, 161
Xenocrates, 161<br />
Yang, 161<br />
Yates, 161<br />
Yativrsabha, 161<br />
Yau, 161<br />
Yavanesvara, 161<br />
Yoccoz, 161<br />
Youden, 161<br />
Young, 162<br />
YoungAlfred, 162<br />
Yule, 162<br />
Yunus, 162<br />
Yushkevich, 162<br />
Zarankiewicz, 163<br />
Zaremba, 163<br />
Zariski, 163<br />
Zassenhaus, 163<br />
Zeckendorf, 163<br />
Zeeman, 163<br />
Zelmanov, 163<br />
Zenodorus, 164<br />
Zeno<strong>of</strong>Elea, 163<br />
Zeno<strong>of</strong>Sidon, 163<br />
Zermelo, 164<br />
Zeuthen, 164<br />
Zhukovsky, 164<br />
Zolotarev, 164<br />
Zorn, 164<br />
Zuse, 164<br />
Zygmund, 164
<strong>ENTRY</strong> MATH MOVIES<br />
[<strong>ENTRY</strong> MATH MOVIES] Author: Oliver Knill: March 2000 -March 2004 Literature: actual DVD’s and<br />
corresponding movie websites<br />
Enigma<br />
[Enigma] is an espionage thriller set during WW II. Most <strong>of</strong> the story is fictional. The main character Tom<br />
Jericho who serves with the British ”Government Communication Headquarters” at Bletchley Park and played<br />
a significant role in breaking the German ”Enigma” codes using a machine called ”Collossus” to decipher the<br />
Enigma codes. The story is inspired by the lif <strong>of</strong> the mathematician Alan Turing who indeed contributed to<br />
the deciphering <strong>of</strong> Enigma during WW II.<br />
A beautiful mind<br />
The movie [A beautiful mind] describes the life <strong>of</strong> the Mathematician John Nash. Nash is introduced while<br />
entering Princeton as a young graduate student. The movie shows how Nash was struggling writing his PhD<br />
with the title ”Non-cooperative games”, a work which later would give him the Nobel prize. Nash is described<br />
as an impossible college teacher. In a calculus class, he introduces the following problem:<br />
Find a subset X <strong>of</strong> three dimensional space which has the property that if V<br />
is the set <strong>of</strong> vector fields F on the complement <strong>of</strong> X, which satisfy curl(F ) = 0<br />
and W is the set <strong>of</strong> vector fields F which are conservative F = grad(f). Then,<br />
the space V/W should be 8 dimensional.<br />
Good will hunting<br />
The movie [Good will hunting] shows a math prodigy Will Hunting who grew up in a succession <strong>of</strong> orphanages in<br />
South Boston. Working as a janitor at MIT, he has taught himself mathematics. He would anonymously solve<br />
complex math problems which were left overnight on blackboards. From an AMS review: ”The mathematics<br />
referred to later on ranges from basic linear algebra, through simple graph theory, to Parseval’s theorem, Fourier<br />
analysis, and on to what seem to be some deeper graph theoretical results. <strong>Mathematics</strong> is referred to constantly,<br />
but in no scene is it presented coherently.”<br />
Cube<br />
[Cube] Six strangers wake up in a maze <strong>of</strong> cubes equiped with movie traps and have to find their way out. Each<br />
room is equipped with a triple <strong>of</strong> numbers and colored. If all numbers are simultaneously not prime, then the<br />
room is trapped and entering it would kill the person entering it.<br />
Hypercube<br />
[Hypercube] In this horror movie, eight strangers wake up in a bizare cube-shaped room not knowing how they<br />
got there or how to escape. They soon learn that their ”hypercube” operates in the fourth dimension and shifts<br />
into an endless maze <strong>of</strong> danger and in the end everyone dies. The movie is the sequel to the 1999 cult hit cube.<br />
Cube 2 was directed by Andrzej Sekula.
Sneakers<br />
[Sneakers] An espionage thriller with Robert Redford. A hunt for a futuristic device which allows to decrypt<br />
secret messages. The device was built by a ”genious Mathematician” who appears in the movie giving a<br />
pompeous lecture on factorization algorithms. The movie which appeared in 1992 is not totally unrealistic from<br />
the mathematical point <strong>of</strong> view. Shortly after the movie was released, in the year 1993, mathematicians have<br />
shown that in principle, a quantum computer could break the factorization difficulty which is the fundament<br />
for many modern encryption algorithms. An other interpretation for the device would be that a new algorithm<br />
for factoring large integers would be found secretly and be hardwired into a chip.<br />
Pi<br />
[Pi] In the movie Pi, the pursuit <strong>of</strong> the infinite takes on a deeper meaning. Max Cohen is a number theorist<br />
living in New York obsessed with a potentially unsolvable problem. Yet, what the story and the age-old problem<br />
uncovers is the deeper link between the mysteries <strong>of</strong> life and other topics <strong>of</strong> consciousness as seemingly disparate<br />
as the stock market, the Kaballah, technology, the DNA and the stars in the sky.<br />
”11:15 Restate my assumptions:<br />
• <strong>Mathematics</strong> is the language <strong>of</strong> nature.<br />
• Everything around us can be represented and understood through numbers.<br />
• If you graph these numbers, patterns emerge. Therefore: There are patterns<br />
everywhere in nature.”<br />
Max Cohen in Pi<br />
Old School<br />
[Old School] In the college comedy ”old school”, three men, disenchanted with their life try to recapture their<br />
college life and wild youth by opening a frat house. In the movie, some aereal shots <strong>of</strong> Harvard appear evenso<br />
the movie seems have no scenes at all taken in Cambridge. At one point, the fraternaty members have to take<br />
a test in which they are asked about Hariotts method to solve cubics.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 8 entries in this file.
Index<br />
A beautiful mind, 1<br />
Cube, 1<br />
Enigma, 1<br />
Good will hunting, 1<br />
Hypercube, 1<br />
Old School, 2<br />
Pi, 2<br />
Sneakers, 2<br />
3
<strong>ENTRY</strong> MEASURE THEORY<br />
[<strong>ENTRY</strong> MEASURE THEORY] Authors: Oliver Knill: 2003 Literature: measure theory<br />
analytic set<br />
An [analytic set] in a complete seperable metric space is the continuous image <strong>of</strong> a Borel set. Also called A-set.<br />
Any A-set is Lebesgue measurable. Any uncountable A-set topologically contains a perfect Cantor set. Suslins<br />
criterium tells that an analytic set is a Borel set if and only if its complement is also an analytic set.<br />
atom<br />
An [atom] is a measurable set Y <strong>of</strong> positive measure in a measure space such that every subset Z <strong>of</strong> Y has<br />
either zero or the same measure. Often an atom consists <strong>of</strong> only one point. More generally, an atom is minimal,<br />
non-zero element in a Boolean algebra.<br />
atom<br />
A property which holds up to a set <strong>of</strong> measure zero is said to hold [almost everywhere] (= almost surely).<br />
Banach-Tarski theorem<br />
The [Banach-Tarski theorem]: a ball in Euclidean space <strong>of</strong> dimension 3 can be decomposed into finitely many<br />
sets and rearranged by rigid motion to obtain two balls. The<br />
barycentre<br />
The [barycentre] <strong>of</strong> a Lebesgue measurable set S in an Euclidean space is the point �<br />
Boolean algebra<br />
S xdx.<br />
A [Boolean algebra] is a set S with two binary operations + and * which are commutative monoids (S, +, 0),<br />
(S, ∗, 1) and satisfy the two distributive laws (x ∗ (y + z) = x ∗ y + y ∗ z, x + (y ∗ z) = (x + y) ∗ (x + z) as well<br />
as the complementary laws x ∗ x = 1, y + y = 0. A Boolean algebra is especially an algebra. Examples are the<br />
algebra <strong>of</strong> classes, where + is the union and ∗ is the intersection or the algebra <strong>of</strong> propositions, for which + is<br />
and and ∗ is or.<br />
Boolean ring<br />
A [Boolean ring] is a ring in which every member is idempotent.
Borel-Cantelli lemma<br />
The [Borel-Cantelli lemma]: if Yn are events in a probability space and the sum <strong>of</strong> their probabilities is finite,<br />
then the probability that infinitely many events occur is zero. If the events are independent and the sum <strong>of</strong><br />
their probabilities is infinite, then the probability that infinitely many events occur is one.<br />
Borel measure<br />
A [Borel measure] is a measure on the sigma-algebra <strong>of</strong> Borel sets.<br />
Borel set<br />
A [Borel set] (=Borel measurable set) in a topological space is an element in the smallest sigma-algebra which<br />
contains all compact sets. Borel sets are also called B-sets. One can say that a B-set is a set which can be<br />
obtained <strong>of</strong> not more than a countable number <strong>of</strong> operations <strong>of</strong> union and intersection <strong>of</strong> closed open sets in a<br />
topological space. Borel sets are special cases <strong>of</strong> analytic sets.<br />
Borel set<br />
The smallest sigma-algebra A <strong>of</strong> subsets <strong>of</strong> a topological space (X,O) containing O is called a Borel sigmaalgebra.<br />
absolutely continuous<br />
A measure µ is [absolutely continuous] to a measure ν if ν(Y ) = 0 implies µ(Y ) = 0.<br />
centre <strong>of</strong> mass<br />
The [centre <strong>of</strong> mass] (=barycentre) <strong>of</strong> a Borel measure µ in a Euclidean space X is the point x = �<br />
X xµ(x).<br />
For example, if µ is supported on finitely many points xi and mi = µ(xi) then x = �<br />
i mixi. If µ is the mass<br />
distribution <strong>of</strong> a body, then its centre <strong>of</strong> mass is called the centre <strong>of</strong> gravity.<br />
abstract integral<br />
[abstract integral]. Denote by L, L + the set <strong>of</strong> measureable maps from a measure space (X, A, µ) to the real<br />
line (R, B), where B is the Borel sigma-algebra on R, R + . For f ∈ S = {f = �n i=1 αi · 1Ai αi � �<br />
∈ R }, define<br />
f dµ := a∈f(X) a · µ{X = a}. For f ∈ L+ define �<br />
�<br />
g dµ . For f ∈ L finally define<br />
X X f dµ = sup � � � g∈S<br />
+ − + − + f = f − f , where f (x) = max(f(x), 0) and f (x) = −(−f) (x).<br />
X
abstract integral<br />
A sigma-additive function µ : A → [0, ∞] on a measurable space (X,A) is called a [measure]. It is called a finite<br />
measure if µ(X) < ∞.<br />
measure<br />
A map f : X → Y where (X, A), (Y, B) are measurable spaces is called [measurable] if f −1 (B) ∈ A for all<br />
B ∈ B.<br />
The pair (X, A) is called a [measurable space] if<br />
measurable space<br />
measure space<br />
(X, A, µ) is called a [measure space] if (X, A) is a measurable space and µ is a measure on (X, A).<br />
measure space<br />
[sigma-additive: a real-valued function on a set A <strong>of</strong> subsets <strong>of</strong> X is called sigma-additive if for all disjoint<br />
Yn ∈ A, one has µ( �<br />
n Yn) = �<br />
n µ(Yn).<br />
sigma-algebra<br />
A set A <strong>of</strong> subsets <strong>of</strong> a set X is called a [sigma-algebra] if<br />
• X is in A<br />
• Y ∈ A implies Y c ∈ A. (iii) Yn ∈ A, n = 1, 2, 3, ... implies � ∞<br />
n=1 Yn ∈ A.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 20 entries in this file.
Index<br />
absolutely continuous, 2<br />
abstract integral, 2, 3<br />
analytic set, 1<br />
atom, 1<br />
Banach-Tarski theorem, 1<br />
barycentre, 1<br />
Boolean algebra, 1<br />
Boolean ring, 1<br />
Borel measure, 2<br />
Borel set, 2<br />
Borel-Cantelli lemma, 2<br />
centre <strong>of</strong> mass, 2<br />
measurable space, 3<br />
measure, 3<br />
measure space, 3<br />
sigma-algebra, 3<br />
4
<strong>ENTRY</strong> NUMBER THEORY<br />
[<strong>ENTRY</strong> NUMBER THEORY] Authors: Oliver Knill: 2003 Literature: Hua, introduction to number theory<br />
ABC conjecture<br />
[ABC conjecture] If a,b,c are positive integers, let N(a,b,c) be the product <strong>of</strong> the prime divisors <strong>of</strong> a,b,c, with<br />
each divisor counted only once. The conjecture claims that for every ɛ > 0, there is a constant mu¿1 such that<br />
for all coprime a,b and c=a+b, then max(|a|, |b|, |c|) ≤ muN(a, b, c) ( 1 + epsilon).<br />
irreducible polynomial<br />
A root <strong>of</strong> an [irreducible polynomial] with integer coefficients is called an [algebraic number].<br />
amicable<br />
Two integers are called [amicable] if each is the sum <strong>of</strong> the distinct proper factors <strong>of</strong> the other. For example:<br />
220 and 284 are amicable. Amicable numbers are 2-periodic orbits <strong>of</strong> the sigma function σ(n) which is the sum<br />
<strong>of</strong> the divisors <strong>of</strong> n.<br />
Apery’s theorem<br />
[Apery’s theorem]: the value <strong>of</strong> the zeta function at z=3 is rational.<br />
arithmetic function<br />
An [arithmetic function] is a function f(n) whose domain is the set <strong>of</strong> positive integers. An important class <strong>of</strong><br />
arithmetic functions are multiplicative functions f(nm) = f(n)f(m). An example is the Möbius function µ(n)<br />
defined by µ(1) = 1, µ(n) = (−1) r if n is the product <strong>of</strong> r distinct primes and µ(n) = 0 otherwise.<br />
Artinian conjecture<br />
[Artinian conjecture]: a quantitative form <strong>of</strong> the conjecture that every non-square integer is a primitive root <strong>of</strong><br />
infinitely many primes. [Beal’s conjecture] If a x + b y = c z , where a,b,c,x,y,z are positive integers and x, y, z > 2,<br />
then a, b, c must have a common factor. It is known that for every x, y, z, there are only finitely many solutions.<br />
The Beal conjecture is a ageneralization <strong>of</strong> Fermat’s last theorem. The conjecture was announced in December<br />
1997. The prize is now 100’000 Dollars for either a pro<strong>of</strong> or a counterexample. The conjecture was discovered<br />
by the Texan number theory enthusiast and banker Andrew Beal.
Bertrands postulate<br />
[Bertrands postulate] tells that for any integer n greater than 3, there is a prime between n and 2n − 2. The<br />
postulate is a theorem, proven by Tchebychef in 1850.<br />
Bezout’s lemma<br />
[Bezout’s lemma] tells that if f and g are polynomials over a field K and d is the greatest common divisor <strong>of</strong> f<br />
and g, then d = af + bg, where a,b are two other polynomials. This generalizes Euclid’s theorem for integers.<br />
Brun’s constant<br />
The [Brun’s constant] is the sum <strong>of</strong> the reciprocals <strong>of</strong> all the prime twins. It is estimated to be about<br />
1.9021605824. While one does not know, whether infinitely many prime twins exist, the sum <strong>of</strong> their reciprocals<br />
is known to be finite. This has been proven by the Norwegian Mathematician Viggo Brun (1885-1978)<br />
in 1919.<br />
Carmichael numbers<br />
[Carmichael numbers] are natural numbers which are Fermat pseudoprime to any base. Named after R.D.<br />
Carmichael who discoved them in 1909. It is known that there are infinitely many Carmichael numbers. The<br />
Carmichael numbers under 100’000 are 561, 1105, 1729, 2465, 2821, 6601, 8911, 10585, 15841, 29341, 41041,<br />
46657, 52633, 62745, 63973, and 75361.<br />
Chineese reminder problem<br />
The [Chineese reminder problem] tells that if n1, . . . , nk are natural numbers which are pairwise relatively prime<br />
and if a1, . . . , ak are any integers, then there exists an integer x which solves simultaneously the congruences<br />
x == a1(modn1), . . . , x == ak(modnk). All solutions are congruent to a given solution modulo �k j=1 nj. The<br />
theorem was established by Qin Jiushao in 1247.<br />
coprime<br />
Two numbers a,b are called [coprime] if their greatest common divisor is 1.
ElGamal<br />
[ElGamal] The ElGamal cryptosystem is based on the difficulty to solve the discrete logarithm problem modulo<br />
a large number n = p r , where p is a prime and and r is a positive integer: solving g x = bmodn for x is<br />
computationally hard. Suppose you want to send a message encoded as an integer m to Alice. A large integer n<br />
and a base g are chosen and public. Alice who has a secrete integer a has published the integer c = g k mod(n) as<br />
her public key. Everybody knows n, g, c. To send Alice a message m, we chose an integer k at random and send<br />
Alice the pair (A, B) = (g m , kg am ) modulo n. (We can compute g am = (g a ) m = c m using the publically availble<br />
information only.) Alice can recover from this the secret message m = A a /B. However, somebody intercepting<br />
the message is not able to recover m without knowing a. He would have to find the discrete logarithm <strong>of</strong> g m<br />
with base g to do so but this is believed to be a computationally difficult problem.<br />
Farey Sequence<br />
The [Farey Sequence] <strong>of</strong> order n is the finite sequence <strong>of</strong> rational numbers a/b, with 0 ≤ a ≤ b ≤ n such that<br />
a, b have no common divisor different from 1 and which are arranged in increasing order.<br />
[Number]:<br />
F1 = (0/1, 1/1)<br />
F2 = (0/1, 1/2, 1)<br />
F3 = (0/1, 1/3, 1/2, 2/3, 1/1)<br />
F4 = (0/1, 1/4, 1/3, 1/2, 2/3, 3/4)<br />
F5 = (0/1, 1/5, 1/4, 1/3, 2/5, 1/2, 3/5, 2/3, 3/4/4/5)<br />
Number<br />
N: natural numbers e.g. 1, 2, 3, 4, ...<br />
Z: integers e.g. −1, 0, 1, 2, ...<br />
Q: rational numbers e.g. 5/6, 5, −8/10<br />
R: real numbers e.g. 1, π, e, � (2), 5/4<br />
C: complex numbers e.g. i, 2, e + iπ/2, 4π/e<br />
The numbers 1, 2, 3, ... are called the [natural numbers].<br />
natural numbers<br />
Fermats last theorem<br />
[Fermats last theorem]. For any ineger n bigger than 2, the equation x n + y n = z n has no solutions in positive<br />
integers. This theorem was proven in 1995 by Andrew Wiles with the assistance <strong>of</strong> Richard Taylor. The theorem<br />
has a long history: in an annotation <strong>of</strong> his copy ”Diophantus”, Fermat wrote a note: ”On the other hand, it<br />
is impossible to seperate a cube into two cubes, or a biquadrate into two biquadrates, or generally any power<br />
except a squre into two powers with the same exponent. I have discovered a truely marvelous pro<strong>of</strong> <strong>of</strong> this<br />
which however the margin is not large enough to contain.”
Fermat-Catalan Conjecture<br />
[Fermat-Catalan Conjecture] There are only finitely many triples <strong>of</strong> coprime integer powers x q , y q , z r for which<br />
x p + y q = z r with 1/p + 1/q + 1/r < 1.<br />
Fermats little theorem<br />
[Fermats little theorem] If p is prime and a is an integer which is not a multiple <strong>of</strong> p, then a ( p − 1) = 1modp.<br />
Example: 2 4 = 16 = 1 (mod 5). Fermats little theorem is a consequence <strong>of</strong> the Lagrange theorem in algebra,<br />
which says that for finite groups, the order <strong>of</strong> a subgroup divides the order <strong>of</strong> the group. Fermats theorem is the<br />
special case, when the finite group is the cyclic group with p − 1 elements. Fermats little theorem is somtimes<br />
also stated in the form: for every integer a and prime number p, the number a p − a is a multiple <strong>of</strong> p.<br />
Fermat numbers<br />
Numbers Fn = 2 ( 2 n ) + 1 are called [Fermat numbers]. Examples are<br />
F0 = 3 prime<br />
F1 = 5 prime<br />
F2 = 17 prime<br />
F3 = 257 prime<br />
F4 = 65537 prime<br />
F5 = 641 · 6700417 composite<br />
No other prime Fermat number beside the first 5 had been found so far.<br />
fundamental theorem <strong>of</strong> arithmetic<br />
The [fundamental theorem <strong>of</strong> arithmetic] assures that every natural number n has a unique prime factorization.<br />
In other words, there is only one way in which one can write a number as a product <strong>of</strong> prime numbers if the<br />
order <strong>of</strong> the product does not matter. For example, 84 = 2237 is the prime factorization <strong>of</strong> 84.<br />
Goldbach’s conjecture<br />
[Goldbach’s conjecture]: Every even integer n greater than two is the sum <strong>of</strong> two primes. For example: 8 = 5+3<br />
or 20 = 13 + 7. The conjecture has not been proven yet.<br />
greatest common divisor<br />
The [greatest common divisor] <strong>of</strong> two integers n and m is the largest integer d such that d divides n and d divides<br />
m. One writes d = gcd(n, m). For example, gcd(6, 9) = 3. There are few recursive algorithms for gcd: one <strong>of</strong><br />
them is the Euclidean algorithm: gcd(m, n) = {k = m mod n; if (k == 0) return(n); else return(gcd(n, k))}.
prime number or prime<br />
A positive integer n is called a [prime number] or [prime], if it is divisible by 1 and n only. The first prime<br />
numbers are 2, 3, 5, 7, 11, 13, 17. An example <strong>of</strong> a non prime number is 12 because it is divisible by 3. There are<br />
infinitely many primes. Every natural number n can be factorized uniquely into primes: for example 42 = 237.<br />
prime factorization<br />
The [prime factorization] <strong>of</strong> a positive integer n is a sequence <strong>of</strong> primes whose product is n. For example:<br />
18 = 3 · 3 · 2 or 100 = 2 · 2 · 5 · 5 or 17 = 17. Every integer has a unique prime factorization.<br />
Pells equation<br />
Fermat claimed first that [Pells equation] dy 2 + 1 = x 2 , where d is an integer has always integer solutions x<br />
and y. The name ”Pell equation” was given by Euler evenso Pell seems nothing have to do with the equation.<br />
Lagrange was the first to prove the existence <strong>of</strong> solutions. One can find solutions by performing the Continued<br />
fraction expansion <strong>of</strong> the square root <strong>of</strong> d.<br />
Fermat number<br />
A [Fermat number] is an integer <strong>of</strong> the form Fk = 2 ( 2 k ) + 1. The first Fermat numbers are F0 = 3, F1 = 5, F2 =<br />
17, F3 = 257, F4 = 65537. They are all primes and called Fermat primes. Fermat had claimed that all Fk are<br />
primes. Euler disproved that showing that 641 divides F5. The Fermat numbers F5 until F9 are known to be<br />
not prime and also have been factored. Fermat numbers play a role in constructing regular polygons with ruler<br />
and compass. The factorization <strong>of</strong> Fermat numbers serves as a challenge to factorization algorithms.<br />
A [Fermat prime] is a Fermat number which is prime.<br />
Fermat prime<br />
Mersenne number<br />
An integer 2 n − 1 is called a [Mersenne number]. If a Mersenne number is prime, it is called a Mersenne prime.<br />
Mersenne number<br />
If a Mersenne number 2 n − 1 is prime, it is called a [Mersenne prime]. In that case, n must be prime. Known<br />
examples are n = 2, 3, 5, 7, 13, 17, 19, 31, 61, 89, 107, 127, 521, 607, 1279, 2203, 2281, 3217, 4253, 4423, 9689,<br />
9941, 11213, 19937, 21701, 23209, 44497, 86243, 110503, 132049, 216091, 756839, 859433, 1257787, 1398269,<br />
2976221, 3021377. It is not known whether there are infinitely many Mersenne primes.
perfect number<br />
An integer n is called a [perfect number] if it is equal to the sum <strong>of</strong> its proper divisors. For example 6 = 1+2+3<br />
or 28 = 1 + 2 + 4 + 7 + 14 are perfect numbers. Also, if 2 n − 1 is prime then 2 n−1 (2 n − 1) is perfect because<br />
1 + 2 + 4 + ... + 2 ( n − 1) = 2 n − 1. This was known already to Euclid. Every even perfect number is <strong>of</strong> the form<br />
p(p + 1)/2, where p = 2 n − 1 is a Mersenne prime. It is not known whether there is an odd perfect number, nor<br />
whether there are infinitely many Mersenne primes.<br />
partition<br />
The [partition] <strong>of</strong> a number n is a decomposition <strong>of</strong> n into a sum <strong>of</strong> integers. Examples are 5 = 1 + 2 + 2. The<br />
number <strong>of</strong> partitions <strong>of</strong> a number n is denoted by p(n) and plays a role in the theory <strong>of</strong> representations <strong>of</strong> finite<br />
groups. For example: p(4) = 5 because <strong>of</strong> the following partitions 4 = 3+1 = 2+2 = 1+1+2 = 1+1+1+1 Euler<br />
introduced the Power series f(x) = � p(n)x n which is (1−x) −1 (1−x 2 ) −1 .... The algebra <strong>of</strong> formal power series<br />
leads to powerful identites like (1+x) −1 (1+x 2 ) −1 (1+x 3 ) −1 ... = (1+x)(1−x)(1+x 2 )(1−x 2 ).../(1−x)(1−x 2 )... =<br />
(1−x 2 )(1−x 4 ).../(1−x)(1−x 2 )... = (1−x) −1 (1−x 3 ) −1 (1−x 5 ) −1 .... The left hand side is the generating function<br />
for a(n), the number <strong>of</strong> partitions <strong>of</strong> n into distinct numbers. The right hand side is the generating function <strong>of</strong><br />
b(n), the number <strong>of</strong> partitions <strong>of</strong> n into an odd number <strong>of</strong> summands. The algebraic identity has shown that<br />
a(n) = b(n). For example, for n = 5, one has a(5) = 3 decomposition 5 = 5 = 4 + 1 = 3 + 2 into different<br />
summands and also b(5) = 3 decompositions into an odd number <strong>of</strong> summands 5 = 5 = 2+2+1 = 1+1+1+1+1.<br />
prime number<br />
A [prime number] is an positive integer which is divisible only by 1 or itself. For example, 12 is not a prime<br />
number because it is divisible by 3 but the integer 13 is a prime number. The first prime numbers are<br />
2, 3, 5, 7, 11, 13, 17, 23.... There are infinitely many prime numbers because if there were only finitely many,<br />
their product p1p2...pk = n has the property that n + 1 is not divisible by any pi. Therefore, n + 1 would either<br />
be a new prime number <strong>of</strong> be divisible by a new prime number. This contradicts the assumption that there are<br />
only finitely many.<br />
prime twin<br />
[prime twin] Two positive integers p, p + 2 are called prime twins if both p and p + 2 are prime numbers. For<br />
example (3, 5), (11, 13) and 17, 19 are prime twins. It is unknown, whether there are infinitely many prime<br />
twins. One knows that �<br />
i 1/pi, where (pi, pi + 2) are prime times is finite.<br />
Pythagorean triple<br />
Three integers x, y, z form a [Pythagorean triple] if x 2 + y 2 = z 2 . An example is 3 2 + 4 2 = 5 2 . Pythagorean<br />
triples define triangles with a right angle and integer side lengths x, y, z. They were known and useful already<br />
by the Babylonians and used to triangulate rectangular regions. The Pythagorean triples with even x can be<br />
parameterized with p > q and x = 2pq, y = p 2 − q 2 , z = p 2 + q 2 . Each Pythagrean triple corresponds to rational<br />
points on the unit circle: X 2 + Y 2 = 1, where X = x/z, Y = y/z.
elatively prime<br />
Two integers n and m are [relatively prime] if their greatest common divisor gcd(n, m) is 1. In other words, one<br />
does not find a common factor <strong>of</strong> n and m other than 1.<br />
Sieve <strong>of</strong> Eratosthenes<br />
The [Sieve <strong>of</strong> Eratosthenes] allows to construct prime numbers. By sieving away all multiplies <strong>of</strong> 2, 3, ..., N and<br />
listing what is left, one obtains a list <strong>of</strong> all the prime numbers smaller than N 2 . For example:<br />
multiples <strong>of</strong> 2: 4,6,8,10,12,14,16,18,20,22,24,26,...<br />
multiplis <strong>of</strong> 3: 6,9,12,15,18,21,24,...<br />
multiples <strong>of</strong> 5: 10,15,20,25,...<br />
The numbers 2, 3, 5, 7, 11, 13, 17, 19, 23 do not appear in this list and are all the prime numbers smaller or equal<br />
than 5 2 . To list all the prime number up to N 2 , one would have to list all the multiples <strong>of</strong> k for k ≤ N.<br />
quadratic residue<br />
A square modulo m, then n is called a A [quadratic residue] modulo m is an integer n which is a square modulo<br />
m. That is one can find an integer x such that n = x 2 (modm). If m is not a quadratic residue, it is called a<br />
quadratic non-residue modulo n. Examples:<br />
• 2 is a quadratic residue modulo 7 because 3 2 = 2 modulo 7.<br />
• If p is an odd prime, then there are (p − 1)/2 quadratic residues and (p − 1)/2 quadratic nonresidues<br />
modulo p.<br />
Legendre symbol<br />
The [Legendre symbol] encodes, whether n is a quadratic residue modulo a prime number p or not:<br />
Legendre(n, p) = 1 if n is a quadratic residue and Legendre(n, p) = −1 if n is not a quadratic residue. If<br />
p is a prime number, then Legendre(−1, p) = (−1) ( (p − 1)/2) and Legendre(2, p) = (−1) ( (p 2 − 1)/8).<br />
law <strong>of</strong> quadratic reciprocity<br />
The [law <strong>of</strong> quadratic reciprocity] tells that if p, q are distinct odd prime numbers, then Legendre(p, q) ·<br />
Legendre(q, p) = (−1) n , where n = (p − 1)(q − 1)/4. Gauss called this result the ”queen <strong>of</strong> number theory”.<br />
The theorem implies that if p = 3 (mod4) and q = 3 (mod4), then exactly one <strong>of</strong> the two congruences<br />
x 2 = p (modq) or x 2 = q (modp) is solvable. Otherwise, either both or none is solvable.<br />
Jacobi symbol<br />
[Jacobi symbol] If m = p1...pk is the prime factorization <strong>of</strong> m, define Jacobi(n, m) as the product <strong>of</strong><br />
Legendre(n, pi), where Legendre(n, p) denotes the Legendre symbol <strong>of</strong> n and p and m = p1 · · · pk is the prime<br />
factorization <strong>of</strong> m.
Jacobi symbol<br />
A positive integer a which generates the multiplicative group modulo a prime number p is called a [primitive<br />
root <strong>of</strong> p]. Examples:<br />
• a = 2 is a primitive root modulo p = 5, because 1 = a 0 , 2 = a 1 , 4 = a 2 , 3 = a 3 is already the list <strong>of</strong><br />
elements in the multiplicative group <strong>of</strong> 5.<br />
• a = 4 is not a primitive root modulo p − 5 because 4 2 = 1 mod5.<br />
Liouville<br />
An irrational number a is called [Liouville] if there exists for every integer m a sequence pn/qn <strong>of</strong> irreducible<br />
fractions such that limn→∞ q m n |a − pn/qn| = 0. Liouville numbers form a class <strong>of</strong> irrational numbers which can<br />
be approximated well by rational numbers. An example <strong>of</strong> a Liouville number is 0.10100100001000000001...<br />
,where the number <strong>of</strong> zeros between the 1’s grows exponentially.<br />
Möbius function<br />
The [Möbius function] µ is an example <strong>of</strong> multiplicative arithmetic function. It is defined as<br />
⎧<br />
⎨ 1 n = 1<br />
µ(n) =<br />
⎩<br />
(−1) r 0<br />
n = p1 · .. · pr, pi < pi+1<br />
otherwise<br />
.<br />
sigma function<br />
Orbits <strong>of</strong> the [sigma function] σ(n) giving the sum <strong>of</strong> the divisors <strong>of</strong> n is called an [aliquot sequence]. One starts<br />
with a number n and forms σ(n), σ(σ(n)) etc. Example: 12, 16, 15, 9, 4, 3, 1. Perfect numbers are fixed points,<br />
amicable numbers are periodic orbits. Higher periodic orbits are called sociable chains. The Catalan conjecture<br />
states that every aliquot sequence<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 45 entries in this file.
Index<br />
ABC conjecture, 1<br />
amicable, 1<br />
Apery’s theorem, 1<br />
arithmetic function, 1<br />
Artinian conjecture, 1<br />
Bertrands postulate, 2<br />
Bezout’s lemma, 2<br />
Brun’s constant, 2<br />
Carmichael numbers, 2<br />
Chineese reminder problem, 2<br />
coprime, 2<br />
ElGamal, 3<br />
Farey Sequence, 3<br />
Fermat number, 5<br />
Fermat numbers, 4<br />
Fermat prime, 5<br />
Fermat-Catalan Conjecture, 4<br />
Fermats last theorem, 3<br />
Fermats little theorem, 4<br />
fundamental theorem <strong>of</strong> arithmetic, 4<br />
Goldbach’s conjecture, 4<br />
greatest common divisor, 4<br />
irreducible polynomial, 1<br />
Jacobi symbol, 7, 8<br />
law <strong>of</strong> quadratic reciprocity, 7<br />
Legendre symbol, 7<br />
Liouville, 8<br />
Möbius function, 8<br />
Mersenne number, 5<br />
natural numbers, 3<br />
Number, 3<br />
partition, 6<br />
Pells equation, 5<br />
perfect number, 6<br />
prime factorization, 5<br />
prime number, 6<br />
prime number or prime, 5<br />
prime twin, 6<br />
Pythagorean triple, 6<br />
quadratic residue, 7<br />
relatively prime, 7<br />
Sieve <strong>of</strong> Eratosthenes, 7<br />
sigma function, 8<br />
9
<strong>ENTRY</strong> PHYSICS<br />
[<strong>ENTRY</strong> PHYSICS] Authors: Oliver Knill: 2002 Literature: Fundamental formulas in physics (edited by D.H.<br />
Menzel) Kneubuehl, Repetitorium in physics<br />
angular momentum<br />
[angular momentum] If r(t) is the position <strong>of</strong> a mass point <strong>of</strong> mass m, then the vector L = mrxr ′ is called the<br />
angular momentum.<br />
C14 method<br />
[C14 method] Used to estimate the age <strong>of</strong> substances containing carbon. It is useful in the range between 500<br />
and 50’000 years. The C14 method is based on the asumption that the atmosphere has a constant C14 isotope<br />
conentration. The decay <strong>of</strong> C14 is compensated by creation <strong>of</strong> C14 in the stratosphere through cosmic radiation.<br />
A living plant has the same C14 concentration as the atmosphere. When it dies, the exchange <strong>of</strong> air stops and<br />
the C14 concentration in the plant will decay.<br />
Gravity<br />
[Gravity] a fundamental force which is responsible for the attraction <strong>of</strong> different masses like for example the<br />
Sun and the earth.<br />
Keplers laws<br />
[Keplers laws]<br />
1. Law: (1609) Planets move on ellipses around the sun. The sun is in a focal point <strong>of</strong> the ellipse.<br />
2. Law: (1609) The radius vector from the sun to the planet covers equal area in equal time.<br />
3. Law: (1619) The squares <strong>of</strong> the periods <strong>of</strong> the planets are proportional to the cubes <strong>of</strong> the semiaxes <strong>of</strong> the<br />
planets.<br />
Newton laws<br />
[Newton laws] (Newton 1686) established four axioms<br />
1. law) Bodies not subject to forces move along straight lines: r ′′ = 0.<br />
2. law) Force is mass times acceleration F = mr ′′ .<br />
3. law) To every action there is a reation: F12 = −F21.<br />
4. law) Forces add like vectors: two forces F1, F2 acting on a body can be replaced by F1 + F2.
Mass<br />
[Mass] measures amount <strong>of</strong> material in a body. The SI unit is 1 kilogram = 1kg. One liter <strong>of</strong> water at<br />
temperature 4 ◦ C has the mass <strong>of</strong> one kilogram. Typical masses are<br />
• Electron 0.9 · 10 −30 kg<br />
• Hydrogen atom 210 −27 kg<br />
• Virus 610 −19 kg<br />
• Earth 6 · 10 24 kg<br />
• Sun 2 · 10 30 kg<br />
• Milkyway 10 41 kg<br />
• Universe 10 52 kg<br />
Length<br />
[Length] measures the position in space. The SI unit is 1 meter = 1m. The meter was originally defined as 1/40<br />
millionth <strong>of</strong> the meridian <strong>of</strong> the earth but is sine 1960 defined spectroscopically. Typical lengths are<br />
• Diameter <strong>of</strong> an atomic nucleus 3 · 10 −15 m.<br />
• Wave length <strong>of</strong> the visible light 5 · 10 −7 m.<br />
• Diameter <strong>of</strong> the earth 1.3 · 10 7 m<br />
• Diameter <strong>of</strong> the sun 1.4 · 10 9 m<br />
• Distance to alpha centauri 4 · 10 16 m<br />
• Diameter <strong>of</strong> the Milkyway 7 · 10 20 m<br />
• Diameter <strong>of</strong> universe 10 26 m.<br />
Maser<br />
[Maser] Maser stands for Microwave Amplification by Stiumlated Emision <strong>of</strong> Radiation. Masers are oscillators<br />
whose frequency are determined by quantized states <strong>of</strong> atoms or molecules. The frequencies <strong>of</strong> a Maser are in<br />
the microwave range.<br />
[Power] is work per time or force times space. The SI unit is 1 Watt 1W = 1kgm 2 /s 3 .
Time<br />
[Time] measures the position on the time axes. The SI unit is 1 second = 1s. The second was originally defined<br />
as a fraction <strong>of</strong> one tropical year. Since 1967 it is defined as 1s=9’192’631 177 periods <strong>of</strong> a Cesium 133 Maser<br />
oscillation. Typicl times:<br />
• Light passing through kernel 10 −24 s.<br />
• Light passes through atom 10 −19 s.<br />
• Period <strong>of</strong> light 10 −15 s.<br />
• Period <strong>of</strong> sound 10 −3 s.<br />
• One day 10 5 s.<br />
• Life <strong>of</strong> a human 210 9 s.<br />
• Age <strong>of</strong> earth 1.3 · 10 17 s<br />
• Age <strong>of</strong> universe 5 · 10 17 s<br />
Relativitistic addition <strong>of</strong> velocities<br />
[Relativitistic addition <strong>of</strong> velocities] As Poincare has realized first, the Maxwell equations are not invariant<br />
under Galilei transformations but under Lorentz transformations. The Michelson-Morely measurements <strong>of</strong><br />
the speed <strong>of</strong> lights showed that light has a constant speed. The addition <strong>of</strong> velocities has therefore to be<br />
modified to a relativistic addition v = (v1 + v2)/(1 + v1v2/c 2 ). Using a mass which depends on the velocity<br />
m = m0/sqrt1 − v 2 /c 2 the Newton laws hold unmodified.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 10 entries in this file.
Index<br />
angular momentum, 1<br />
C14 method, 1<br />
Gravity, 1<br />
Keplers laws, 1<br />
Length, 2<br />
Maser, 2<br />
Mass, 2<br />
Newton laws, 1<br />
Relativitistic addition <strong>of</strong> velocities, 3<br />
Time, 3<br />
4
<strong>ENTRY</strong> POLYHEDRA<br />
[<strong>ENTRY</strong> POLYHEDRA] Authors: Oliver Knill: December 2000 Source: Translated into this format from data<br />
given in http://netlib.bell-labs.com/netlib<br />
tetrahedron<br />
The [tetrahedron] is a polyhedron with 4 vertices and 4 faces. The dual polyhedron is called tetrahedron.<br />
cube<br />
The [cube] is a polyhedron with 8 vertices and 6 faces. The dual polyhedron is called octahedron.<br />
hexahedron<br />
The [hexahedron] is a polyhedron with 8 vertices and 6 faces. The dual polyhedron is called octahedron.<br />
octahedron<br />
The [octahedron] is a polyhedron with 6 vertices and 8 faces. The dual polyhedron is called cube.<br />
dodecahedron<br />
The [dodecahedron] is a polyhedron with 20 vertices and 12 faces. The dual polyhedron is called icosahedron.<br />
icosahedron<br />
The [icosahedron] is a polyhedron with 12 vertices and 20 faces. The dual polyhedron is called dodecahedron.<br />
small stellated dodecahedron<br />
The [small stellated dodecahedron] is a polyhedron with 12 vertices and 12 faces. The dual polyhedron is called<br />
great dodecahedron.<br />
great dodecahedron<br />
The [great dodecahedron] is a polyhedron with 12 vertices and 12 faces. The dual polyhedron is called small<br />
stellated dodecahedron.
great stellated dodecahedron<br />
The [great stellated dodecahedron] is a polyhedron with 20 vertices and 12 faces. The dual polyhedron is called<br />
great icosahedron.<br />
great icosahedron<br />
The [great icosahedron] is a polyhedron with 12 vertices and 20 faces. The dual polyhedron is called great<br />
stellated dodecahedron.<br />
truncated tetrahedron<br />
The [truncated tetrahedron] is a polyhedron with 12 vertices and 8 faces. The dual polyhedron is called triakis<br />
tetrahedron.<br />
cuboctahedron<br />
The [cuboctahedron] is a polyhedron with 12 vertices and 14 faces. The dual polyhedron is called rhombic<br />
dodecahedron.<br />
truncated cube<br />
The [truncated cube] is a polyhedron with 24 vertices and 14 faces. The dual polyhedron is called triakis<br />
octahedron.<br />
truncated octahedron<br />
The [truncated octahedron] is a polyhedron with 24 vertices and 14 faces. The dual polyhedron is called tetrakis<br />
hexahedron.<br />
rhombicuboctahedron<br />
The [rhombicuboctahedron] is a polyhedron with 24 vertices and 26 faces. The dual polyhedron is called<br />
trapezoidal icositetrahedron.<br />
great rhombicuboctahedron<br />
The [great rhombicuboctahedron] is a polyhedron with 48 vertices and 26 faces. The dual polyhedron is called<br />
hexakis octahedron.
snub cube<br />
The [snub cube] is a polyhedron with 24 vertices and 38 faces. The dual polyhedron is called pentagonal<br />
icositetrahedron.<br />
icosidodecahedron<br />
The [icosidodecahedron] is a polyhedron with 30 vertices and 32 faces. The dual polyhedron is called rhombic<br />
triacontahedron.<br />
truncated dodecahedron<br />
The [truncated dodecahedron] is a polyhedron with 60 vertices and 42 faces. The dual polyhedron is called<br />
triakis icosahedron.<br />
truncated icosahedron<br />
The [truncated icosahedron] is a polyhedron with 60 vertices and 32 faces. The dual polyhedron is called<br />
pentakis dodecahedron.<br />
rhombicosidodecahedron<br />
The [rhombicosidodecahedron] is a polyhedron with 60 vertices and 62 faces. The dual polyhedron is called<br />
trapezoidal hexecontahedron.<br />
great rhombicosidodecahedron<br />
The [great rhombicosidodecahedron] is a polyhedron with 120 vertices and 62 faces. The dual polyhedron is<br />
called hexakis icosahedron.<br />
snub dodecahedron<br />
The [snub dodecahedron] is a polyhedron with 60 vertices and 92 faces. The dual polyhedron is called pentagonal<br />
hexacontahedron.<br />
triangular prism<br />
The [triangular prism] is a polyhedron with 6 vertices and 5 faces.
pentagonal prism<br />
The [pentagonal prism] is a polyhedron with 10 vertices and 7 faces.<br />
hexagonal prism<br />
The [hexagonal prism] is a polyhedron with 12 vertices and 8 faces.<br />
octagonal prism<br />
The [octagonal prism] is a polyhedron with 16 vertices and 10 faces.<br />
decagonal prism<br />
The [decagonal prism] is a polyhedron with 20 vertices and 12 faces.<br />
square antiprism<br />
The [square antiprism] is a polyhedron with 8 vertices and 10 faces.<br />
pentagonal antiprism<br />
The [pentagonal antiprism] is a polyhedron with 10 vertices and 12 faces.<br />
hexagonal antiprism<br />
The [hexagonal antiprism] is a polyhedron with 12 vertices and 13 faces.<br />
octagonal antiprism<br />
The [octagonal antiprism] is a polyhedron with 16 vertices and 18 faces.<br />
decagonal antiprism<br />
The [decagonal antiprism] is a polyhedron with 20 vertices and 22 faces.
triakis tetrahedron<br />
The [triakis tetrahedron] is a polyhedron with 8 vertices and 12 faces. The dual polyhedron is called truncated<br />
tetrahedron.<br />
rhombic dodecahedron<br />
The [rhombic dodecahedron] is a polyhedron with 14 vertices and 12 faces. The dual polyhedron is called<br />
cuboctahedron.<br />
triakis octahedron<br />
The [triakis octahedron] is a polyhedron with 14 vertices and 24 faces. The dual polyhedron is called truncated<br />
cube.<br />
tetrakis hexahedron<br />
The [tetrakis hexahedron] is a polyhedron with 14 vertices and 24 faces. The dual polyhedron is called truncated<br />
octahedron.<br />
trapezoidal icositetrahedron<br />
The [trapezoidal icositetrahedron] is a polyhedron with 26 vertices and 24 faces. The dual polyhedron is called<br />
rhombicuboctahedron.<br />
hexakis octahedron<br />
The [hexakis octahedron] is a polyhedron with 26 vertices and 48 faces. The dual polyhedron is called great<br />
rhombicuboctahedron.<br />
pentagonal icositetrahedron<br />
The [pentagonal icositetrahedron] is a polyhedron with 38 vertices and 24 faces. The dual polyhedron is called<br />
snub cube.<br />
rhombic triacontahedron<br />
The [rhombic triacontahedron] is a polyhedron with 32 vertices and 30 faces. The dual polyhedron is called<br />
icosidodecahedron.
triakis icosahedron<br />
The [triakis icosahedron] is a polyhedron with 32 vertices and 60 faces. The dual polyhedron is called truncated<br />
dodecahedron.<br />
pentakis dodecahedron<br />
The [pentakis dodecahedron] is a polyhedron with 32 vertices and 60 faces. The dual polyhedron is called<br />
truncated icosahedron.<br />
trapezoidal hexecontahedron<br />
The [trapezoidal hexecontahedron] is a polyhedron with 62 vertices and 60 faces. The dual polyhedron is called<br />
rhombicosidodecahedron.<br />
hexakis icosahedron<br />
The [hexakis icosahedron] is a polyhedron with 62 vertices and 120 faces. The dual polyhedron is called great<br />
rhombicosidodecahedron.<br />
pentagonal hexecontahedron<br />
The [pentagonal hexecontahedron] is a polyhedron with 92 vertices and 60 faces. The dual polyhedron is called<br />
snub dodecahedron.<br />
square pyramid<br />
The [square pyramid] is a polyhedron with 5 vertices and 5 faces.<br />
pentagonal pyramid<br />
The [pentagonal pyramid] is a polyhedron with 6 vertices and 6 faces.<br />
triangular cupola<br />
The [triangular cupola] is a polyhedron with 9 vertices and 8 faces.<br />
square cupola<br />
The [square cupola] is a polyhedron with 12 vertices and 10 faces.
pentagonal cupola<br />
The [pentagonal cupola] is a polyhedron with 15 vertices and 12 faces.<br />
pentagonal rotunda<br />
The [pentagonal rotunda] is a polyhedron with 20 vertices and 17 faces.<br />
elongated triangular pyramid<br />
The [elongated triangular pyramid] is a polyhedron with 7 vertices and 7 faces.<br />
elongated square pyramid<br />
The [elongated square pyramid] is a polyhedron with 9 vertices and 9 faces.<br />
elongated pentagonal pyramid<br />
The [elongated pentagonal pyramid] is a polyhedron with 11 vertices and 11 faces.<br />
gyroelongated square pyramid<br />
The [gyroelongated square pyramid] is a polyhedron with 9 vertices and 13 faces.<br />
gyroelongated pentagonal pyramid<br />
The [gyroelongated pentagonal pyramid] is a polyhedron with 11 vertices and 16 faces.<br />
triangular dipyramid<br />
The [triangular dipyramid] is a polyhedron with 5 vertices and 6 faces.<br />
pentagonal dipyramid<br />
The [pentagonal dipyramid] is a polyhedron with 7 vertices and 10 faces.
elongated triangular dipyramid<br />
The [elongated triangular dipyramid] is a polyhedron with 8 vertices and 9 faces.<br />
elongated square dipyramid<br />
The [elongated square dipyramid] is a polyhedron with 10 vertices and 12 faces.<br />
elongated pentagonal dipyramid<br />
The [elongated pentagonal dipyramid] is a polyhedron with 12 vertices and 15 faces.<br />
gyroelongated square dipyramid<br />
The [gyroelongated square dipyramid] is a polyhedron with 10 vertices and 16 faces.<br />
elongated triangular cupola<br />
The [elongated triangular cupola] is a polyhedron with 15 vertices and 14 faces.<br />
elongated square cupola<br />
The [elongated square cupola] is a polyhedron with 20 vertices and 18 faces.<br />
elongated pentagonal cupola<br />
The [elongated pentagonal cupola] is a polyhedron with 25 vertices and 22 faces.<br />
elongated pentagonal rotunds<br />
The [elongated pentagonal rotunds] is a polyhedron with 30 vertices and 27 faces.<br />
gyroelongated triangular cupola<br />
The [gyroelongated triangular cupola] is a polyhedron with 15 vertices and 20 faces.
gyroelongated square cupola<br />
The [gyroelongated square cupola] is a polyhedron with 20 vertices and 26 faces.<br />
gyroelongated pentagonal cupola<br />
The [gyroelongated pentagonal cupola] is a polyhedron with 25 vertices and 32 faces.<br />
gyroelongated pentagonal rotunda<br />
The [gyroelongated pentagonal rotunda] is a polyhedron with 30 vertices and 37 faces.<br />
gyrobifastigium<br />
The [gyrobifastigium] is a polyhedron with 8 vertices and 8 faces.<br />
triangular orthobicupola<br />
The [triangular orthobicupola] is a polyhedron with 12 vertices and 14 faces.<br />
square orthobicupola<br />
The [square orthobicupola] is a polyhedron with 16 vertices and 18 faces.<br />
square gyrobicupola<br />
The [square gyrobicupola] is a polyhedron with 16 vertices and 18 faces.<br />
pentagonal orthobicupola<br />
The [pentagonal orthobicupola] is a polyhedron with 20 vertices and 22 faces.<br />
pentagonal gyrobicupola<br />
The [pentagonal gyrobicupola] is a polyhedron with 20 vertices and 22 faces.
pentagonal orthocupolarontunda<br />
The [pentagonal orthocupolarontunda] is a polyhedron with 25 vertices and 27 faces.<br />
pentagonal gyrocupolarotunda<br />
The [pentagonal gyrocupolarotunda] is a polyhedron with 25 vertices and 27 faces.<br />
pentagonal orthobirotunda<br />
The [pentagonal orthobirotunda] is a polyhedron with 30 vertices and 32 faces.<br />
elongated triangular orthobicupola<br />
The [elongated triangular orthobicupola] is a polyhedron with 18 vertices and 20 faces.<br />
elongated triangular gyrobicupola<br />
The [elongated triangular gyrobicupola] is a polyhedron with 18 vertices and 20 faces.<br />
elongated square gyrobicupola<br />
The [elongated square gyrobicupola] is a polyhedron with 24 vertices and 26 faces.<br />
elongated pentagonal orthobicupola<br />
The [elongated pentagonal orthobicupola] is a polyhedron with 30 vertices and 32 faces.<br />
elongated pentagonal gyrobicupola<br />
The [elongated pentagonal gyrobicupola] is a polyhedron with 30 vertices and 32 faces.<br />
elongated pentagonal orthocupolarotunda<br />
The [elongated pentagonal orthocupolarotunda] is a polyhedron with 35 vertices and 37 faces.
elongated pentagonal gyrocupolarotunda<br />
The [elongated pentagonal gyrocupolarotunda] is a polyhedron with 35 vertices and 37 faces.<br />
elongated pentagonal orthobirotunda<br />
The [elongated pentagonal orthobirotunda] is a polyhedron with 40 vertices and 42 faces.<br />
elongated pentagonal gyrobirotunda<br />
The [elongated pentagonal gyrobirotunda] is a polyhedron with 40 vertices and 42 faces.<br />
gyroelongated triangular bicupola<br />
The [gyroelongated triangular bicupola] is a polyhedron with 18 vertices and 26 faces.<br />
gyroelongated square bicupola<br />
The [gyroelongated square bicupola] is a polyhedron with 24 vertices and 34 faces.<br />
gyroelongated pentagonal bicupola<br />
The [gyroelongated pentagonal bicupola] is a polyhedron with 30 vertices and 42 faces.<br />
gyroelongated pentagonal cupolarotunda<br />
The [gyroelongated pentagonal cupolarotunda] is a polyhedron with 35 vertices and 47 faces.<br />
gyroelongated pentagonal birotunda<br />
The [gyroelongated pentagonal birotunda] is a polyhedron with 40 vertices and 52 faces.<br />
augmented triangular prism<br />
The [augmented triangular prism] is a polyhedron with 7 vertices and 8 faces.
iaugmented triangular prism<br />
The [biaugmented triangular prism] is a polyhedron with 8 vertices and 11 faces.<br />
triaugmented triangular prism<br />
The [triaugmented triangular prism] is a polyhedron with 9 vertices and 14 faces.<br />
augmented pentagonal prism<br />
The [augmented pentagonal prism] is a polyhedron with 11 vertices and 10 faces.<br />
biaugmented pentagonal prism<br />
The [biaugmented pentagonal prism] is a polyhedron with 12 vertices and 13 faces.<br />
augmented hexagonal prism<br />
The [augmented hexagonal prism] is a polyhedron with 13 vertices and 11 faces.<br />
parabiaugmented hexagonal prism<br />
The [parabiaugmented hexagonal prism] is a polyhedron with 14 vertices and 14 faces.<br />
metabiaugmented hexagonal prism<br />
The [metabiaugmented hexagonal prism] is a polyhedron with 14 vertices and 14 faces.<br />
triaugmented hexagonal prism<br />
The [triaugmented hexagonal prism] is a polyhedron with 15 vertices and 17 faces.<br />
augmented dodecahedron<br />
The [augmented dodecahedron] is a polyhedron with 21 vertices and 16 faces.
parabiaugmented dodecahedron<br />
The [parabiaugmented dodecahedron] is a polyhedron with 22 vertices and 20 faces.<br />
metabiaugmented dodecahedron<br />
The [metabiaugmented dodecahedron] is a polyhedron with 22 vertices and 20 faces.<br />
triaugmented dodecahedron<br />
The [triaugmented dodecahedron] is a polyhedron with 23 vertices and 24 faces.<br />
metabidiminished icosahedron<br />
The [metabidiminished icosahedron] is a polyhedron with 10 vertices and 12 faces.<br />
tridiminished icosahedron<br />
The [tridiminished icosahedron] is a polyhedron with 9 vertices and 8 faces.<br />
augmented tridiminished icosahedron<br />
The [augmented tridiminished icosahedron] is a polyhedron with 10 vertices and 10 faces.<br />
augmented truncated tetrahedron<br />
The [augmented truncated tetrahedron] is a polyhedron with 15 vertices and 14 faces.<br />
augmented truncated cube<br />
The [augmented truncated cube] is a polyhedron with 28 vertices and 22 faces.<br />
biaugmented truncated cube<br />
The [biaugmented truncated cube] is a polyhedron with 32 vertices and 30 faces.
augmented truncated dodecahedron<br />
The [augmented truncated dodecahedron] is a polyhedron with 65 vertices and 42 faces.<br />
parabiaugmented truncated dodecahedron<br />
The [parabiaugmented truncated dodecahedron] is a polyhedron with 70 vertices and 52 faces.<br />
metabiaugmented truncated dodecahedron<br />
The [metabiaugmented truncated dodecahedron] is a polyhedron with 70 vertices and 52 faces.<br />
triaugmented truncated dodecahedron<br />
The [triaugmented truncated dodecahedron] is a polyhedron with 75 vertices and 62 faces.<br />
gyrate rhombicosidodecahedron<br />
The [gyrate rhombicosidodecahedron] is a polyhedron with 60 vertices and 62 faces.<br />
parabigyrate rhombicosidodecahedron<br />
The [parabigyrate rhombicosidodecahedron] is a polyhedron with 60 vertices and 62 faces.<br />
metabigyrate rhombicosidodecahedron<br />
The [metabigyrate rhombicosidodecahedron] is a polyhedron with 60 vertices and 62 faces.<br />
trigyrate rhombicosidodecahedron<br />
The [trigyrate rhombicosidodecahedron] is a polyhedron with 60 vertices and 62 faces.<br />
diminished rhombicosidodecahedron<br />
The [diminished rhombicosidodecahedron] is a polyhedron with 55 vertices and 52 faces.
paragyrate diminished rhombicosidodecahedron<br />
The [paragyrate diminished rhombicosidodecahedron] is a polyhedron with 55 vertices and 52 faces.<br />
metagyrate diminished rhombicosidodecahedron<br />
The [metagyrate diminished rhombicosidodecahedron] is a polyhedron with 55 vertices and 52 faces.<br />
bigyrate diminished rhombicosidodecahedron<br />
The [bigyrate diminished rhombicosidodecahedron] is a polyhedron with 55 vertices and 52 faces.<br />
parabidiminished rhombicosidodecahedron<br />
The [parabidiminished rhombicosidodecahedron] is a polyhedron with 50 vertices and 42 faces.<br />
metabidiminished rhombicosidodecahedron<br />
The [metabidiminished rhombicosidodecahedron] is a polyhedron with 50 vertices and 42 faces.<br />
gyrate bidiminished rhombicosidodecahedron<br />
The [gyrate bidiminished rhombicosidodecahedron] is a polyhedron with 50 vertices and 42 faces.<br />
tridiminished rhombicosidodecahedron<br />
The [tridiminished rhombicosidodecahedron] is a polyhedron with 45 vertices and 32 faces.<br />
snub disphenoid<br />
The [snub disphenoid] is a polyhedron with 8 vertices and 12 faces.<br />
snub square antiprism<br />
The [snub square antiprism] is a polyhedron with 16 vertices and 26 faces.
sphenocorona<br />
The [sphenocorona] is a polyhedron with 10 vertices and 14 faces.<br />
augmented sphenocorona<br />
The [augmented sphenocorona] is a polyhedron with 11 vertices and 17 faces.<br />
sphenomegacorona<br />
The [sphenomegacorona] is a polyhedron with 12 vertices and 18 faces.<br />
hebesphenomegacorona<br />
The [hebesphenomegacorona] is a polyhedron with 14 vertices and 21 faces.<br />
disphenocingulum<br />
The [disphenocingulum] is a polyhedron with 16 vertices and 24 faces.<br />
bilunabirotunda<br />
The [bilunabirotunda] is a polyhedron with 14 vertices and 14 faces.<br />
triangular hebesphenorotunda<br />
The [triangular hebesphenorotunda] is a polyhedron with 18 vertices and 20 faces.<br />
tetrahemihexahedron<br />
The [tetrahemihexahedron] is a polyhedron with 7 vertices and 16 faces.<br />
octahemioctahedron<br />
The [octahemioctahedron] is a polyhedron with 13 vertices and 32 faces.
small ditrigonal icosidodecahedron<br />
The [small ditrigonal icosidodecahedron] is a polyhedron with 80 vertices and 72 faces.<br />
dodecadodecahedron<br />
The [dodecadodecahedron] is a polyhedron with 110 vertices and 72 faces.<br />
echidnahedron<br />
The [echidnahedron] is a polyhedron with 92 vertices and 180 faces.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 143 entries in this file.
Index<br />
augmented dodecahedron, 12<br />
augmented hexagonal prism, 12<br />
augmented pentagonal prism, 12<br />
augmented sphenocorona, 16<br />
augmented triangular prism, 11<br />
augmented tridiminished icosahedron, 13<br />
augmented truncated cube, 13<br />
augmented truncated dodecahedron, 14<br />
augmented truncated tetrahedron, 13<br />
biaugmented pentagonal prism, 12<br />
biaugmented triangular prism, 12<br />
biaugmented truncated cube, 13<br />
bigyrate diminished rhombicosidodecahedron, 15<br />
bilunabirotunda, 16<br />
cube, 1<br />
cuboctahedron, 2<br />
decagonal antiprism, 4<br />
decagonal prism, 4<br />
diminished rhombicosidodecahedron, 14<br />
disphenocingulum, 16<br />
dodecadodecahedron, 17<br />
dodecahedron, 1<br />
echidnahedron, 17<br />
elongated pentagonal cupola, 8<br />
elongated pentagonal dipyramid, 8<br />
elongated pentagonal gyrobicupola, 10<br />
elongated pentagonal gyrobirotunda, 11<br />
elongated pentagonal gyrocupolarotunda, 11<br />
elongated pentagonal orthobicupola, 10<br />
elongated pentagonal orthobirotunda, 11<br />
elongated pentagonal orthocupolarotunda, 10<br />
elongated pentagonal pyramid, 7<br />
elongated pentagonal rotunds, 8<br />
elongated square cupola, 8<br />
elongated square dipyramid, 8<br />
elongated square gyrobicupola, 10<br />
elongated square pyramid, 7<br />
elongated triangular cupola, 8<br />
elongated triangular dipyramid, 8<br />
elongated triangular gyrobicupola, 10<br />
elongated triangular orthobicupola, 10<br />
elongated triangular pyramid, 7<br />
great dodecahedron, 1<br />
great icosahedron, 2<br />
great rhombicosidodecahedron, 3<br />
great rhombicuboctahedron, 2<br />
great stellated dodecahedron, 2<br />
gyrate bidiminished rhombicosidodecahedron, 15<br />
gyrate rhombicosidodecahedron, 14<br />
gyrobifastigium, 9<br />
gyroelongated pentagonal bicupola, 11<br />
gyroelongated pentagonal birotunda, 11<br />
gyroelongated pentagonal cupola, 9<br />
gyroelongated pentagonal cupolarotunda, 11<br />
gyroelongated pentagonal pyramid, 7<br />
gyroelongated pentagonal rotunda, 9<br />
18<br />
gyroelongated square bicupola, 11<br />
gyroelongated square cupola, 9<br />
gyroelongated square dipyramid, 8<br />
gyroelongated square pyramid, 7<br />
gyroelongated triangular bicupola, 11<br />
gyroelongated triangular cupola, 8<br />
hebesphenomegacorona, 16<br />
hexagonal antiprism, 4<br />
hexagonal prism, 4<br />
hexahedron, 1<br />
hexakis icosahedron, 6<br />
hexakis octahedron, 5<br />
icosahedron, 1<br />
icosidodecahedron, 3<br />
metabiaugmented dodecahedron, 13<br />
metabiaugmented hexagonal prism, 12<br />
metabiaugmented truncated dodecahedron, 14<br />
metabidiminished icosahedron, 13<br />
metabidiminished rhombicosidodecahedron, 15<br />
metabigyrate rhombicosidodecahedron, 14<br />
metagyrate diminished rhombicosidodecahedron, 15<br />
octagonal antiprism, 4<br />
octagonal prism, 4<br />
octahedron, 1<br />
octahemioctahedron, 16<br />
parabiaugmented dodecahedron, 13<br />
parabiaugmented hexagonal prism, 12<br />
parabiaugmented truncated dodecahedron, 14<br />
parabidiminished rhombicosidodecahedron, 15<br />
parabigyrate rhombicosidodecahedron, 14<br />
paragyrate diminished rhombicosidodecahedron, 15<br />
pentagonal antiprism, 4<br />
pentagonal cupola, 7<br />
pentagonal dipyramid, 7<br />
pentagonal gyrobicupola, 9<br />
pentagonal gyrocupolarotunda, 10<br />
pentagonal hexecontahedron, 6<br />
pentagonal icositetrahedron, 5<br />
pentagonal orthobicupola, 9<br />
pentagonal orthobirotunda, 10<br />
pentagonal orthocupolarontunda, 10<br />
pentagonal prism, 4<br />
pentagonal pyramid, 6<br />
pentagonal rotunda, 7<br />
pentakis dodecahedron, 6<br />
rhombic dodecahedron, 5<br />
rhombic triacontahedron, 5<br />
rhombicosidodecahedron, 3<br />
rhombicuboctahedron, 2<br />
small ditrigonal icosidodecahedron, 17<br />
small stellated dodecahedron, 1<br />
snub cube, 3<br />
snub disphenoid, 15<br />
snub dodecahedron, 3
snub square antiprism, 15<br />
sphenocorona, 16<br />
sphenomegacorona, 16<br />
square antiprism, 4<br />
square cupola, 6<br />
square gyrobicupola, 9<br />
square orthobicupola, 9<br />
square pyramid, 6<br />
tetrahedron, 1<br />
tetrahemihexahedron, 16<br />
tetrakis hexahedron, 5<br />
trapezoidal hexecontahedron, 6<br />
trapezoidal icositetrahedron, 5<br />
triakis icosahedron, 6<br />
triakis octahedron, 5<br />
triakis tetrahedron, 5<br />
triangular cupola, 6<br />
triangular dipyramid, 7<br />
triangular hebesphenorotunda, 16<br />
triangular orthobicupola, 9<br />
triangular prism, 3<br />
triaugmented dodecahedron, 13<br />
triaugmented hexagonal prism, 12<br />
triaugmented triangular prism, 12<br />
triaugmented truncated dodecahedron, 14<br />
tridiminished icosahedron, 13<br />
tridiminished rhombicosidodecahedron, 15<br />
trigyrate rhombicosidodecahedron, 14<br />
truncated cube, 2<br />
truncated dodecahedron, 3<br />
truncated icosahedron, 3<br />
truncated octahedron, 2<br />
truncated tetrahedron, 2
<strong>ENTRY</strong> POTENTIAL THEORY<br />
[<strong>ENTRY</strong> POTENTIAL THEORY] Authors: Oliver Knill: jan 2003 Literature: ”T. Ransford”,”Potential theory<br />
in the complex plane”.<br />
Analytic<br />
[Analytic] Let D ⊂ C be an open set. A continuous function f : D → C is called analytic in D, if for all z ∈ D<br />
the complex partial derivative<br />
∂f 1<br />
:= lim (f(z + h) − f(z))<br />
∂z |h|→0 h<br />
exists and is finite. Analytic functions are also called holomorphic. Properties: the sum and the product <strong>of</strong><br />
analytic functions are analytic. If fn is a sequence <strong>of</strong> analytic maps which converges uniformly on compact<br />
subsets <strong>of</strong> D to a function f, then f is analytic too.<br />
complex partial derivative<br />
Define the [complex partial derivative] <strong>of</strong> a complex function f(z) = f(x + iy) in the complex plane is defined<br />
as ∂f<br />
∂z<br />
= 1<br />
2<br />
( ∂<br />
∂x<br />
− i ∂<br />
∂y )f.<br />
conformal map<br />
A [conformal map] is a differentiable map from the complex plane to the complex plane which preserves angles.<br />
• every conformal map which has continuous partial derivatives is analytic.<br />
• An analytic function f is conformal at every point where its derivative f ′ (z) is different from 0.<br />
Dirichlet problem<br />
Solution <strong>of</strong> the [Dirichlet problem]. If D is a regular domain in the complex plane and f is a continous function<br />
on the boundary <strong>of</strong> D, then there exists a unique harmonic function f on D such that h(z) = f(z) for all<br />
boundary points <strong>of</strong> D.<br />
Dirichlet problem<br />
Let K be a compact subset <strong>of</strong> the complex plane. Let P (K) the set <strong>of</strong> all Borel probability measure on K.<br />
A measure ν maximizing the potential theoretical energy in P (K) is called an [equilibrium measure] <strong>of</strong> K.<br />
Properties:<br />
• every compact K has an equilibrium measure.<br />
• if K is not polar then the equilibrium measure is unique.
fine topology<br />
The [fine topology] on the complex plane is defined as the coarsest topology on the plane which makes all<br />
subharmonic functions continuous.<br />
Frostman’s theorem<br />
[Frostman’s theorem]: If ν is the equilibrium measure on a compact set K, then the potential pν <strong>of</strong> ν is bounded<br />
below by I(ν) everywhere on C. Furthermore, pν = I(ν) everywhere on K except on a Fsigma polar subset E<br />
<strong>of</strong> the boundary <strong>of</strong> K.<br />
Frostman’s theorem<br />
A function h on the complex plane is called harmonic in a region D if it satisfies the mean value property on<br />
every disc contained in D.<br />
harmonic measure<br />
A [harmonic measure] wD on a domain D is a function from D to the set <strong>of</strong> Borel probability measures on<br />
the boundary <strong>of</strong> D. The measure for z is defined as the functional g ↦→ HD(g)(z), where HD(g) is the Perron<br />
function <strong>of</strong> g on D.<br />
• if the boundary <strong>of</strong> D is non-polar, there exists a unique harmonic measure for D.<br />
• if D = Im(z) < 0, then wD(z, a, b) = arg((z − b)/(z − a))/π<br />
Harnack inequality<br />
The [Harnack inequality] assures that for any positive harmonic function h on the disc D(w, R) and for any<br />
r < R and 0 < t < 2P i<br />
h(w)(R − r)/(R + r) ≤ h(w + re it ≤ h(w)(R + r)/(R − r)<br />
extended Liouville theorem<br />
The [extended Liouville theorem]: if f is subharmonic on the complex plane C − E, where E is a closed polar<br />
set and f is bounded above then f is constant.<br />
generalized Laplacian<br />
The [generalized Laplacian] ∆(f) <strong>of</strong> a subharmonic function f on a domain D is the Radon measure µ on D<br />
defined as the linear functional g ↦→ �<br />
u∆g dA. The Laplacian <strong>of</strong> a subharmonic function is also called the<br />
D<br />
Riesz measure. The Laplacian is known to exist and is unique. If pµ is the potential associated to µ, then<br />
∆pµ = µ.
Hadamard’s three circle theorem<br />
[Hadamard’s three circle theorem] assures that for any subharmonic function f on the annulus {r < |z| < R}<br />
the function M(f, r) = sup |z|=rf(z) is an increasing convex function <strong>of</strong> log(r).<br />
Jensen formula<br />
[Jensen formula] If f is holomorphic in the disc D = B(0, R), r < R and a1, ..., an are the zeros <strong>of</strong> f in the closure<br />
<strong>of</strong> D counted with multiplicity, then � 2pi<br />
0<br />
log |f(rexp(it))| dt = log |f(0)| + N log(r) − � n<br />
j=1 log|aj|.<br />
Jensen formula<br />
If f is a subharmonic function in a neighborhood <strong>of</strong> a point z in the complex plane, then the limit<br />
limrto0 M(f, r)/ log(r) exists and is called the [Lelong number] <strong>of</strong> f at z. Here M(f, r) = sup |z|=r f(z).<br />
hyperbolic domain<br />
An open set in the extended complex plane is a [hyperbolic domain] if there is a subharmonic function on G<br />
that is bounded above and not constant on any component <strong>of</strong> G. A domain which is not hyperbolic is called a<br />
parabolic domain. Known facts:<br />
• every bounded region is a hyperbolic domain (take f(z)=Re(z)).<br />
• an open not connected set is hyperbolic.<br />
• the complex plane is not a hyperbolic domain<br />
Perron function<br />
The [Perron function] for a domain D is defined as the functional assigning to a continous function g on the<br />
boundary <strong>of</strong> D the value HD(g), which is the supremum <strong>of</strong> all subharmonic functions u satisfying sup z→w u(z) ≤<br />
g(w).<br />
potential<br />
A subharmonic function f is called a [potential] if f = pµ, where µ = ∆f is the Laplacian <strong>of</strong> f and pmu(z) =<br />
− �<br />
log |z − w|dµ(w)/(2π) is the potential defined by µ.<br />
D
logarithmic capacity<br />
The [logarithmic capacity] <strong>of</strong> a subset E <strong>of</strong> the complex plane is defined as c(E) = sup µ exp(−I(µ)), where I(µ)<br />
is the potential theoretical energy <strong>of</strong> µ and the supremum is taken over all Borel probability measures mu on C<br />
whose support is a compact subset <strong>of</strong> E. Known facts:<br />
• c(E) = 0 if and only if E is polar.<br />
• a disc <strong>of</strong> radius r has capacity r<br />
• a line segment <strong>of</strong> length h has capacity h/4.<br />
• if K has diameter d, then c(K) ≤ d/2.<br />
• if K has area A, then c(A) ≥ (A/π) 1/2 .<br />
mean value property<br />
The [mean value property] tells that if h is a harmonic function in the disc D(w, R) and 0 < r < R, then<br />
h(w) = � 2pi<br />
0 h(w + reit )dt/(2π).<br />
polar set<br />
A subset S <strong>of</strong> the complex plane is called a [polar set] if the potential theoretical energy I(µ) is −∞ for every<br />
finite Borel measure µ with compact support supp(µ) in S. Properties <strong>of</strong> polar sets:<br />
• every countable union <strong>of</strong> polar sets is polar.<br />
• every polar set has Lebesgue measure zero.<br />
Poisson integral formula<br />
The [Poisson integral formula]: if h is harmonic on the disk D(w, R ′ ), then for all 0 < r < R < R ′ and<br />
h(w + Reis )(R2 − r2 )/(R2 − 2Rrcos(s − t) + r2 )ds/(2π)<br />
0 < t < 2π, h(w + re it ) = � 2pi<br />
0<br />
potential theoretical energy<br />
The [potential theoretical energy] I(µ) <strong>of</strong> a finite Borel measure µ <strong>of</strong> compact support on the complex plane is<br />
defined as<br />
� � � �<br />
I(µ) =<br />
log|z − w|dµ(w)dµ(z) .<br />
C<br />
C
potential theoretical energy<br />
A function f on an open subset U <strong>of</strong> the complex plane is called [subharmonic] if it is upper semicontinous and<br />
satisfies the local submean inequality. Examples:<br />
• if g is holomorphic then f = log |g| is subharmonic<br />
• if µ is a Borel measure <strong>of</strong> compact support, then f(z) = � log |z − w| dµ(w) is subharmonic.<br />
• any harmonic function is subharmonic.<br />
• if g is subharmonic, then exp(g) is subharmonic.<br />
regular<br />
A boundary point w <strong>of</strong> a domain D is called [regular] if there exists a barrier at w. A barrier is a subharmonic<br />
function f defined in a neighborhood N <strong>of</strong> w which is negative on D ∩ N and such that limz→w f(z) = 0. It is<br />
known that z is a regular boundary point if and only if the complement <strong>of</strong> D is non-thin at z.<br />
irregular<br />
A boundary point w <strong>of</strong> a domain D is called [irregular] if it is not regular. It is known that if z has a neighborhood<br />
N such that N intersected with the boundary <strong>of</strong> D is polar, then z is irregular.<br />
irregular<br />
A domain D for which every point is regular is called a [regular domain]. For example, a simply connected<br />
domain D such that the complement <strong>of</strong> D in the Riemann sphere contains at least two points, is regular.<br />
Riemann mapping Theorem<br />
The [Riemann mapping Theorem]: if D is a simply connected proper subdomain <strong>of</strong> the complex plane, there<br />
exists a conformal map <strong>of</strong> D onto the unit disc.<br />
Riesz decomposition theorem<br />
The [Riesz decomposition theorem] tells that every subharmonic function f can be written as f = pµ + h, where<br />
µ = ∆f is the Laplacian <strong>of</strong> f, 2πpµ is the potential <strong>of</strong> µ and where h is harmonic.
submean inequality<br />
The local [submean inequality] for a function in the complex plane tells that there exists R > 0 such that for<br />
all 0 < r < R one has<br />
� 2pi<br />
f(w) ≤ f(w + re it ) dt/(2pi) .<br />
0<br />
submean inequality<br />
Let f be a subharmonic function on a domain D. The [maximum principle] says that if f attains a global<br />
maximum in the interior <strong>of</strong> D then f is constant.<br />
thin set<br />
A subset S <strong>of</strong> the complex plane is called a [thin set] if for all w in the closure <strong>of</strong> S − w and all subharmonic<br />
functions f, lim sup z→w f(z) = f(w). Examples:<br />
• every single point in the interiour <strong>of</strong> S is thin.<br />
• Fσ polar sets S are thin at every point.<br />
• connected sets <strong>of</strong> cardinality larger than 1 are non-thin at every point <strong>of</strong> their closure<br />
• A domain S is thin at a point z ∈ S if and only if z is regular.<br />
Wiener criterion<br />
The [Wiener criterion] gives a necessary and sufficient condition for a set S to be thin at a point w. Let S be a<br />
Fσ subset <strong>of</strong> C and let w be in S. Let a < 1 and define Sn = zinS, a n < |z − w| < a ( n − 1) . The criterion says<br />
that S is thin at w if and only if �<br />
n≥1 n/log(2/c(Sn)) < infinity, where<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 33 entries in this file.
Index<br />
Analytic, 1<br />
complex partial derivative, 1<br />
conformal map, 1<br />
Dirichlet problem, 1<br />
extended Liouville theorem, 2<br />
fine topology, 2<br />
Frostman’s theorem, 2<br />
generalized Laplacian, 2<br />
Hadamard’s three circle theorem, 3<br />
harmonic measure, 2<br />
Harnack inequality, 2<br />
hyperbolic domain, 3<br />
irregular, 5<br />
Jensen formula, 3<br />
logarithmic capacity, 4<br />
mean value property, 4<br />
Perron function, 3<br />
Poisson integral formula, 4<br />
polar set, 4<br />
potential, 3<br />
potential theoretical energy, 4, 5<br />
regular, 5<br />
Riemann mapping Theorem, 5<br />
Riesz decomposition theorem, 5<br />
submean inequality, 6<br />
thin set, 6<br />
Wiener criterion, 6<br />
7
Estimation theory<br />
[Estimation theory] part <strong>of</strong> statistics with the goal <strong>of</strong> extracting parameters from noise-corrupted observations.<br />
Applications <strong>of</strong> estimation theory are statistical signal processing or adaptive filter theory or adaptive optics<br />
which allows for example image deblurring.<br />
Parameter estimation problem<br />
[Parameter estimation problem] determine from a set L <strong>of</strong> observations a parameter vector. A paremeter<br />
estimate is a random vector. The estimation error ɛ is the difference between the estimated parameter and the<br />
parameter itself. The mean-squared error is given by the mean squared error matrix E[ɛ T ɛ]. It is a correlation<br />
matrix.<br />
Biased<br />
[Biased] An estimate is said to be biased, if the expected value <strong>of</strong> the estimate is different than the actual value.<br />
Asymptotically unbiased<br />
[Asymptotically unbiased] An estimate in statistics is called asymptotically unbiased, if the estimate becomes<br />
unbiased in the limit when the number <strong>of</strong> data points goes to infinity.<br />
Consistent estimate<br />
[Consistent estimate] An estimate in statistics is called consistent if the mean squared error matrix E[ɛ T ɛ]<br />
converges to the 0 matrix in the limit when the number <strong>of</strong> data points goes to infinity.<br />
Mean squared error matrix<br />
The [Mean squared error matrix] is defined as E[ɛ T ɛ], where ɛ is the difference between the estimated parameter<br />
and the parameter itself.<br />
efficient<br />
An estimator in statistics is called [efficient] if its mean-squared error satisfies the Cramer-Rao bound.<br />
Cramer-Rao bound<br />
[Cramer-Rao bound] The mean-squared error E[ɛ T ɛ] for any estimate <strong>of</strong> a parameter has a lower bound which<br />
is called the Cramer-Rao bound. In the case <strong>of</strong> unbiased estimators, the Cramer-Rao bound gives for each error<br />
ɛi the estimate<br />
E[ɛ 2 i ] ≥ [F −1 ]ii .
Fisher information matrix<br />
The [Fisher information matrix] is defined as the expectation <strong>of</strong> the Hessian F = E[H(− log(p))] =<br />
E[grad(log(p))grad(log(p)) T ] <strong>of</strong> the conditional probability p(r|θ).<br />
maximum likelihood estimate<br />
The [maximum likelihood estimate] is an estimation technique in statistics to estimate nonrandom parameters.<br />
A maximum likelyhood estimate is a maximizer <strong>of</strong> the log likelihood function log(p(r, θ). It is known that<br />
the maximum likelihood estimate is asymptotically unbiased, consistent estimate. Furthermore, the maximum<br />
likelihood estimate is distributed as a Gaussian random variable.<br />
Example. If X is a normal distributed random variable with unknown mean θ and variance 1, the likelyhood<br />
function is p(r, θ) = 1<br />
√ 2π e −(r−θ)2 /2 and the log-likelyhood function is log(p(r, θ)) = −(r − θ) 2 /2 + C. The<br />
maximum likelyhood estimate is r.<br />
The maximum likelihood estimate is difficult to compute in general for non-Gaussian random variables.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 9 entries in this file.
Index<br />
Asymptotically unbiased, 1<br />
Biased, 1<br />
Consistent estimate, 1<br />
Cramer-Rao bound, 1<br />
efficient, 1<br />
Fisher information matrix, 2<br />
maximum likelihood estimate, 2<br />
Mean squared error matrix, 1<br />
Parameter estimation problem, 1<br />
3
<strong>ENTRY</strong> TOPOLOGY<br />
[<strong>ENTRY</strong> TOPOLOGY] Authors: Oliver Knill 2003, John Carlson 2003-2004 Literature: http://at.yorku.ca/cgibin/bell/props.cgi<br />
Alexander compactification<br />
The [Alexander compactification] Y <strong>of</strong> a Hausdorff space (X, O) is the topological space (Y = X ∪ x, P ), where<br />
x is an additional point. The topology P consists <strong>of</strong> the elements in O and the complements <strong>of</strong> closed subsets<br />
as neighborhoods <strong>of</strong> that point. The new topological space Y is compact.<br />
Alexander’s subbase theorem<br />
The [Alexander’s subbase theorem]: if every open cover <strong>of</strong> a topological space X has a finite sub-cover then X<br />
is compact.<br />
arc-connected<br />
A topological space is called [arc-connected] if any two points can be connected by a path, a continuous image<br />
<strong>of</strong> an interval. Path connected is stronger than connected but not equivalent: the subset {(x, sin(1/x)), x ∈<br />
R + } ∪ {(0, y), −1 ≤ y ≤ 1 } <strong>of</strong> the plane with topology induced from the plane is connected but not path<br />
connected. Arc-connected is also called path-connected.<br />
Baire category<br />
[Baire category] is a measure for the size <strong>of</strong> a set in a topological space. Countable unions <strong>of</strong> nowhere dense sets<br />
are called <strong>of</strong> the first categorie or meager, any other set <strong>of</strong> second category. Complements <strong>of</strong> meager sets are<br />
called residual. Baire category is used to quantify certain sets. For example it is known that ”most” numbers<br />
are Liouville numbers in the sense that they form a residual set among all real numbers.<br />
Baire space<br />
A [Baire space] is a topological space with the property that the intersection <strong>of</strong> countable family <strong>of</strong> open dense<br />
subsets is dense.<br />
Baire category theorem<br />
The [Baire category theorem]: a complete metric space is a Baire space.
all<br />
A [ball] in a metric space is a set <strong>of</strong> the form {y | d(x, y) < r }. The closure <strong>of</strong> an open ball is a closed ball. To<br />
make clear that a ball is open, one sometimes calls it also open ball.<br />
barrier function<br />
A [barrier function] for a set S in a topological space (X, O) is a nonnegative continuous function f defined on<br />
X which is zero in S and positive in the complement <strong>of</strong> S. A barrier function is sometimes also called a penalty<br />
function.<br />
basis<br />
A [basis] <strong>of</strong> a topological space (X, T ) is a subset B <strong>of</strong> T such that<br />
• the empty set is in B,<br />
• arbitrary unions <strong>of</strong> sets in B are in B,<br />
• the intersection <strong>of</strong> two sets in B is a union <strong>of</strong> sets in B.<br />
A basis B defines the topology (X, T ). Every A ∈ T is a union <strong>of</strong> elements in B. An example: if (X, d) is a<br />
metric space then the set <strong>of</strong> all balls {y | d(x, y) < 1/k }, where x is taken from a dense set in X and k is a<br />
positive integer form a basis.<br />
bicontinuous<br />
A function is [bicontinuous] if it is continuous invertible and has a continuous inverse. A bicontinuous function<br />
is also called a homeomorphism.<br />
bounded<br />
A subset <strong>of</strong> a metric space is [bounded] if it is contained in some ball <strong>of</strong> finite radius.<br />
boundary<br />
The [boundary] <strong>of</strong> a set A in a topological space (X, T ) is the the set C \ B, where C is the closure <strong>of</strong> A and B<br />
is the interior <strong>of</strong> A. Examples:<br />
• if A is the open unit disc in the plane, then the boundary is the unit circle.<br />
• in a discrete topological space, the boundary <strong>of</strong> any set is empty.<br />
Cantor set<br />
A [Cantor set] is a topological space which is homeomorphic to the Cantor middle set.
Cantor middle set<br />
The [Cantor middle set] is the subset <strong>of</strong> the unit interval which is the complement <strong>of</strong> � ∞<br />
n=1 Yn, where Y1 =<br />
(1/3, 2/3), Y2 = (1/9, 2/9) ∪ (7/9, 8/9) etc. are sucessive middle sets. It is a fractal with Hausdorff dimension<br />
log(2)/ log(3).<br />
Cantor middle set<br />
A topological space homeomorphic to a ball in Euclidean space is called a [cell]. Examples <strong>of</strong> cells are polyhedra<br />
in three dimensional space.<br />
closure<br />
The [closure] <strong>of</strong> a set A in a topological space (X, T ) is the intersection <strong>of</strong> all closed sets in X, which contain<br />
A. One writes Y for the closure <strong>of</strong> Y .<br />
dense<br />
A set A is called [dense] in a topological space (X, T ), if every open set Y ∈ O in X contains at least one point<br />
in A.<br />
finer<br />
A topology (X, T ) is [finer] than a topology (X, S) if S is a subset <strong>of</strong> T . In that case, (X, S) is called a coarser<br />
topology than (X, T ). Examples:<br />
• the discrete topology on X is finer than any other topology on X.<br />
• A set S <strong>of</strong> subsets <strong>of</strong> X defines a topology, the coarsest topology O which contains S.<br />
topological space<br />
A [topological space] is a pair (X,T) where T is a set <strong>of</strong> subsets <strong>of</strong> X satisfying<br />
• ∅ ∈ T ,<br />
• if A, B ∈ T , then A ∩ B ∈ T ,<br />
• an arbitrary union <strong>of</strong> subsets in T is in T.<br />
Elements in T are called open sets. The complement <strong>of</strong> an open set is called a closed set. Examples:<br />
• the discrete topology on X: T is all subsets <strong>of</strong> X<br />
• the indiscrete topology on X: T contains only X and the empty set,<br />
• the c<strong>of</strong>inite topology: T is the set <strong>of</strong> all subsets A such that their complement in X is a finite set.<br />
• (X, d) metric space: T is the set <strong>of</strong> sets A such that for x in A, also a small ball B = {|y − x| < a} is<br />
contained in A.
open set<br />
An [open set] <strong>of</strong> a topological space (X, T ) is an element <strong>of</strong> T .<br />
closed set<br />
A [closed set] is the complement <strong>of</strong> an open set in a topological space (X, T ). A closed set contains all its limit<br />
points.<br />
continuous<br />
A map f between two topological spaces (X, T ) and (Y, S) is called [continuous] if the inverse image <strong>of</strong> any<br />
open set is open: for all A ∈ S one has f ( − 1)(A) ∈ T . Note that f does not need to be invertible: one defines<br />
f −1 (A) = {x ∈ X|f(x) ∈ A}. Examples <strong>of</strong> results known:<br />
• The composition <strong>of</strong> two continuous maps is continuous.<br />
• Every map on the discrete topological space is continuous.<br />
• A map between metric spaces is continuous if and only if it is sequential continuous: for any xn → x, one<br />
has f(xn) → f(x).<br />
• A map between topological spaces is continuous if for every net xt → x, the net f(xt) converges to f(x).<br />
homeomorphism<br />
An invertible map f between two topological spaces (X, T ) and (Y, S) is called a [homeomorphism] if f and the<br />
inverse <strong>of</strong> f are both continuous.<br />
homeomorphic<br />
[homeomorphic] If there exists a homeomorphism between two topological spaces, the topological spaces are<br />
called homeomorphic.<br />
connected<br />
A topological space (X, T ) is called [connected], if there are no two disjoint open sets U, V whose union is X.<br />
For a connected topological space, the empty set ∅ or X are the only sets which are both open and closed. A<br />
subset A <strong>of</strong> a topological space is connected if it is connected with the on A induced topology: there are no<br />
disjoint open sets U, V whose union contains A.
locally connected<br />
A topological space is [locally connected] if every point has arbitrarily small neighborhoods which are connected.<br />
Examples.<br />
• A union <strong>of</strong> disjoint open intervals on the real line is locally connected but not connected.<br />
• The union <strong>of</strong> the graphs <strong>of</strong> f(x) = 2 sin(1/x) and g(x) = 1 and the y-axes all intersected with the set<br />
{y > 1} is connected but not locally connected because small neighborhoods <strong>of</strong> the point (0, 1) are not<br />
connected.<br />
Hausdorff<br />
A topological space (X, T ) is called [Hausdorff] if for every two points x, y ∈ X, there are disjoint open sets<br />
U, V ∈ T such that x ∈ U and y ∈ V . This is refined through seperation axioms, T 0, ..., T 4. Hausdorff is also<br />
called T 2. Any metric space is Hausdorff: if d is the distance betwen x and y, then balls <strong>of</strong> radius d/3 around<br />
x and y seperate the points. The plane X with semimetric d(x, y) = |x1 − y1| is not Hausdorff: the points<br />
x = (0, −1) and y = (0, 1) can not be seperated by open sets.<br />
seperation axioms<br />
[seperation axioms] define classes <strong>of</strong> topological spaces with decreasing seperability properties: T 4 ⇒ T 3 ⇒<br />
T 2 ⇒ T 1 ⇒ T 0.<br />
T0 space:<br />
T1 space:<br />
T2 space:<br />
T3 space:<br />
T4 space:<br />
for two different points x, y in X one <strong>of</strong> the points has an open<br />
neighborhood U not containing the other point.<br />
for two different points x, y in X there exists an open neighborhood<br />
U <strong>of</strong> x and an open neighborhood V <strong>of</strong> y. such that x is not<br />
in V and y is not in U.<br />
also called Hausdorff” two different points x, y can be seperated<br />
with disjoint neighborhoods U, V .<br />
T1 and regular: any point x and any closed set F not containing<br />
x can be seperated by two disjoint neighborhood.<br />
T1 and normal: any two disjoint sets F ,G can be separated by<br />
two disjoint open sets.<br />
It is known that a T4 space with a countable basis is metrizable.<br />
Hausdorff topology<br />
The [Hausdorff topology] is a metric on the set <strong>of</strong> closed bounded subsets <strong>of</strong> a complete metric space. The<br />
distance between two sets A and B is the infimum over all r for which A is contained in a r-neighborhood <strong>of</strong> B<br />
and B is contained in a r-neighborhood <strong>of</strong> A.<br />
Lindeloef<br />
A topological space is called [Lindeloef] if every open cover <strong>of</strong> X contains a countable subcover.
compact<br />
A topological space is called [compact] if every open cover <strong>of</strong> X contains a finite subcover. Examples <strong>of</strong> results<br />
known about compactnes:<br />
• Heine-Borel theorem: a closed interval in the real line is compact.<br />
• If f : X → Y is continuous and onto and X is compact, then Y is compact. As a consequence, a<br />
continouous function on a compact subspace has both a maximum and a minimum.<br />
• In a Hausdorff space, compact sets are closed.<br />
• In a metric space, compact sets are closed and bounded.<br />
• Closed subsets <strong>of</strong> compact spaces are compact.<br />
• Tychon<strong>of</strong> theorem: the product <strong>of</strong> a collection <strong>of</strong> compact spaces is compact.<br />
countably compact<br />
A topological space is called [countably compact] if every countable open cover <strong>of</strong> X contains a finite subcover.<br />
locally compact<br />
A topological space is called [locally compact] if every point has a neighborhood, which has a compact closure.<br />
Examples.<br />
• The real line is compact but not locally compact.<br />
• A compact Hausdorff space is locally compact.<br />
• The n-dimensional Euclidean space R n is lcally compact but not compact.<br />
locally compact<br />
A set U <strong>of</strong> open sets in a topological space (X, O) is called locally finite if every point x ∈ X has a neighborhood<br />
V , such that V has a nonempty intersection with only finitely many elements in U.<br />
paracompact<br />
A topological space (X,O) is called [paracompact] if every open cover has a countable, locally finite subcover.<br />
relatively compact<br />
A subset A <strong>of</strong> a topological space (X, T ) is called [relatively compact] if the closure <strong>of</strong> A is compact.
filter<br />
A [filter] on a nonempty set X is a set <strong>of</strong> subsets F satisfying<br />
• X is in F , but the empty set ∅ is not in F.<br />
• If A and B are in F, then their intersection is in F .<br />
• If A is in F and B is a subset <strong>of</strong> A, then B is in F .<br />
Examples:<br />
• Principal filter for a nonempty subset A consists <strong>of</strong> all subsets <strong>of</strong> X which contain A.<br />
• Frechet filter for an infinite set consists <strong>of</strong> all subsets <strong>of</strong> X such that their complement is finite.<br />
• Neighborhood filter <strong>of</strong> a point x in a topological space (X,T) is the set <strong>of</strong> open neighborhoods <strong>of</strong> x.<br />
• Elementary filter for a sequence xn in X consists <strong>of</strong> all sets A in X such that xn is in A for large enough<br />
n.<br />
converges<br />
A sequence xn in a topological space [converges] to a point x, if for every neighborhood U <strong>of</strong> x, there exists an<br />
integer m, such that for n > m one has xn ∈ U.<br />
Filter convergence<br />
[Filter convergence] A filter F converges to x in a topological space (X, T ) if F contains the neighborhood filter<br />
G <strong>of</strong> x, that is if F contains all neighborhoods <strong>of</strong> x. For example, an elementary filter to a sequence xn converges<br />
to a point x, if and only if xn converges to x.<br />
accumulation point<br />
A point y is called an [accumulation point] <strong>of</strong> a filter F , if there exists a filter G containing F such that G<br />
converges to x.<br />
directed<br />
A set M is called [directed] if there exists a partial order (M,
Koch curve<br />
The [Koch curve] is a fractal in the plane. It has Hausdorff dimension log(4)/ log(3). It is constructed by<br />
building an equilateral triangle on the middle third <strong>of</strong> each side <strong>of</strong> a given equilateral triangle K0 leading to a<br />
curve K1 and recursively build Kn+1 from Kn by replacing each middle third <strong>of</strong> a line segment in Kn with a<br />
triangle. The curve is the limit <strong>of</strong> Kn, when n goes to infinity.<br />
metrizable<br />
A topological space (X, T ) is called [metrizable] if there exists a metric on X such that the topology generated<br />
by the metric is T .<br />
metric space<br />
A [metric space] (X, d) is a set X with a function d from X × X → [0, ∞) satisfying d(x, y) = d(y, x), d(x, y) =<br />
0 ⇔ x = y and d(x, z) ≤ d(x, y) + d(y, z)). The set T = {U ⊂ X | ∀x ∈ X, ∃r > 0, Br(x) = {y | d(x, y) < r} ⊂<br />
U} defines a topological space (X, T ).<br />
metric space<br />
A [metric space] (X, d) is a set X with a nonnegative function d from X×X satisfying d(x, y) = d(y, x),d(x, y) = 0<br />
if and only if x = y and d(x, z) ≤ d(x, y)+d(y, z). A metric space defines a topological space (X,T): the topology<br />
T is the set <strong>of</strong> subsets A <strong>of</strong> X such that for all points x ∈ A, there is a small ball d(y, x) < r which is also<br />
contained in A.<br />
net<br />
A [net] with values in a topological space X is a function f: D -¿ X, where D is a directed set. For example: if<br />
D is the set <strong>of</strong> natural numbers, then a net is a sequence. A net defines a filter F : it is the set <strong>of</strong> all sets A such<br />
that xt is eventually in A. A net xt converges to a point x if and only if the associated filter converges to x.<br />
open cover<br />
[open cover] A subset U <strong>of</strong> O, where (X, O) is a topological space is called an open cover <strong>of</strong> X if the union <strong>of</strong><br />
all elements in U is X. If U and V are open covers and V ⊂ U, then V is called a subcover <strong>of</strong> U.<br />
product space<br />
The [product space] between topological spaces is defined as (X × Y, O × P ), where X × Y is the set <strong>of</strong> all pairs<br />
(x, y), x ∈ X, y ∈ Y and O ×P is the coarsest topological space which contains all products A×B, where A ∈ O<br />
and B ∈ P . For example, if (X, O) = (Y, P ) are both the real line with the topology generated by d(x, y) =<br />
|x−y|, then the product space is homeomorphic to the plane with the metric d(x, y) = � (x1 − x2) 2 + (y1 − y2) 2 .
second countable<br />
A topological space is called [second countable], if it has a countable basis. Example. Every seperable metric<br />
space is second countable. Especially, every finite-dimensional Euclidean space is second countable.<br />
metrizable<br />
A topological space is called [metrizable] if there exists a metric d on the set X that induces the topology <strong>of</strong> X.<br />
Any regular space with a countable basis is metrizable.<br />
homotopic<br />
[homotopic] If f and g are continuous maps from the topological space X to a topological space Y , we say that<br />
f is homotopic to g if there is a continuous map F from X ×I to Y , such that F (x, 0) = f(x) and F (x, 1) = g(x)<br />
for all x. For example, the maps f(x) = x 2 and g(x) = sin(x) on the real line are homotopic, because we can<br />
define F (x, t) = (1 − t)x 2 + t sin(x). The maps f(x) = x and g(x) = sin(2πx) on the circle are not homotopic.<br />
While g is homotopic to the constant function h(x) = 0, the map f(x) can not be deformed to a constant<br />
without breaking continuity.<br />
induced topology<br />
The [induced topology] on a subset A <strong>of</strong> X, where (X, T ) is a topological spoace is the the topological space<br />
(A, {Y ∩ A}Y ∈T ).<br />
path homotopic<br />
[path homotopic] If f and g are and continuous homotopic maps from an interval to a space X, we say f and g<br />
are path homotopic if their images have the same end points. For instance, the maps f(x) = x 2 and g(x) = x 3<br />
are path homotopic on the closed interval from 0 to 1. The maps f(x) = 2x 2 and g(x) = x 3 are homotopic on<br />
the unit interval but not path homotopic.<br />
loop<br />
A [loop] is a path in a topological space that begins and ends at the same point. A loop is also called a closed<br />
curve. Loops play a role in definitions like simply connected: a topological space is simply connected if every<br />
loop is homotopic to a constant loop which is a fancy way telling that every closed path can be collapsed inside<br />
X to a point.<br />
fundamental group<br />
The [fundamental group] <strong>of</strong> a topological space at a point is the set <strong>of</strong> homotopy classes <strong>of</strong> loops based at that<br />
point.
Topologist’s Sine Curve<br />
The [Topologist’s Sine Curve] is the union S <strong>of</strong> the graph <strong>of</strong> the function sin(1/x) on the positive real axes R +<br />
with the y-axes. It an example <strong>of</strong> a topological space which is connected but not path-connected. Pro<strong>of</strong>: if S<br />
were path-connected, there would exist a path r(t) = (x(t), y(t)) connecting the two points (0, 1) and (0, π).<br />
The set {t|r(t) ∈ S} is closed. Let T be the largest t in that set for which r(t) is in the y-axes. Then x(T)=0<br />
and r(t)=(x(t),sin(1/x(t)) for t > T . Because there are times tn > tn−1 > T, tn → T for which y(tn) = (−1) n ,<br />
the function r(t) can not be continuous at t = T .<br />
Urysohn lemma<br />
The [Urysohn lemma] tells that if X is a normal space and A and B are disjoint closed subsets <strong>of</strong> X, then there<br />
exists a continuous map f from X to the unit interval such that f(x) = 0 for all x ∈ A, and f(x) = 1 for all<br />
x ∈ B.<br />
Pro<strong>of</strong>: use the normality <strong>of</strong> X to construct a family Up <strong>of</strong> open sets <strong>of</strong> X indexed by the rational numbers P<br />
in the unit interval so that for p < q, the closure <strong>of</strong> Up is contained in Uq. These sets are simply ordered in the<br />
same way that their subscripts are ordered in the real line. Given some enumeration <strong>of</strong> the rationals, where 1<br />
and 0 are the first two elements <strong>of</strong> the enumeration, define U1 = X \ B. Because A is a closed set contained in<br />
the open set U, there is by normality an open set U0 such that A ⊂ U0 and the closure <strong>of</strong> U0 is a subset <strong>of</strong> U1.<br />
In general, let Pn denote the set consisting <strong>of</strong> the first n rational numbers in the sequence. Suppose that Up is<br />
defined for all rational numbers p in a set Pn, then p < q implies that the closure <strong>of</strong> Up is a subset <strong>of</strong> Uq. If r is<br />
the next rational number in the sequence; we define Ur: the set Pn+1 = Pn ∪ {r} is a finite subset <strong>of</strong> the unit<br />
interval and has a simple ordering induced by the ordering <strong>of</strong> the real line. In a finite simply ordered set, every<br />
element, other than the largest and smallest, has an immediate predecessor and and immediate successor. 0 is<br />
the smallest and 1 is the largest element <strong>of</strong> the simply ordered set Pn+1, and r /∈ {0, 1}. So r has an immediate<br />
predecessor p ∈ Pn+1 and an immediate successor q ∈ Pn+1. The sets Up and Uq are already defined, and the<br />
closure <strong>of</strong> Up is contained in Uq by the induction hypothesis. Because X is normal, we can find an open set<br />
Ur such that the closure <strong>of</strong> Up is contained in Ur and the closure <strong>of</strong> Ur is contained in Uq. Now the induction<br />
condition holds for every pair <strong>of</strong> elements <strong>of</strong> Pn+1.<br />
This file is part <strong>of</strong> the S<strong>of</strong>ia project sponsored by the Provost’s fund for teaching and learning at Harvard<br />
university. There are 58 entries in this file.
Index<br />
accumulation point, 7<br />
Alexander compactification, 1<br />
Alexander’s subbase theorem, 1<br />
arc-connected, 1<br />
Baire category, 1<br />
Baire category theorem, 1<br />
Baire space, 1<br />
ball, 2<br />
barrier function, 2<br />
basis, 2<br />
bicontinuous, 2<br />
boundary, 2<br />
bounded, 2<br />
Cantor middle set, 3<br />
Cantor set, 2<br />
closed set, 4<br />
closure, 3<br />
compact, 6<br />
connected, 4<br />
continuous, 4<br />
converges, 7<br />
countably compact, 6<br />
dense, 3<br />
directed, 7<br />
filter, 7<br />
Filter convergence, 7<br />
finer, 3<br />
fundamental group, 9<br />
Hausdorff, 5<br />
Hausdorff topology, 5<br />
homeomorphic, 4<br />
homeomorphism, 4<br />
homotopic, 9<br />
induced topology, 9<br />
interior, 7<br />
Koch curve, 8<br />
Lindeloef, 5<br />
locally compact, 6<br />
locally connected, 5<br />
loop, 9<br />
metric space, 8<br />
metrizable, 8, 9<br />
net, 8<br />
open cover, 8<br />
open set, 4<br />
paracompact, 6<br />
path homotopic, 9<br />
product space, 8<br />
relatively compact, 6<br />
11<br />
second countable, 9<br />
seperation axioms, 5<br />
topological space, 3<br />
Topologist’s Sine Curve, 10<br />
Urysohn lemma, 10