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Nr. 40<br />
Juli 2013<br />
SPG MITTEILUNGEN<br />
COMMUNICATIONS DE LA SSP<br />
(a) SF+ (b) SF (c) SF-<br />
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The scientific community celebrates this year the<br />
centennary of the Atomic Mo<strong>de</strong>l of Niels Bohr.<br />
Read more (on p. 52) about the history of this outstanding<br />
event in physics, which is also the topic<br />
of the SCNAT Annual Congress (see p. 60).<br />
3 3<br />
3<br />
What have snowf<strong>la</strong>kes to do with a<br />
hot p<strong>la</strong>sma ? Find out on p. 36.<br />
Four years after its <strong>la</strong>unch the Herschel<br />
space observatory completed<br />
its observations about how stars and<br />
ga<strong>la</strong>xies are formed. The successful<br />
mission is <strong>de</strong>scribed on p. 42.<br />
Joint Annual Meeting of the<br />
Austrian Physical Society and Swiss Physical Society<br />
with<br />
Austrian and Swiss Societies for Astronomy and Astrophysics<br />
September 3 - 6, 2013, JKU Linz<br />
General information: page 10, preliminary program: page 12
SPG Mitteilungen Nr. 40<br />
Inhalt - Contenu - Contents<br />
Gemeinsame Jahrestagung in Linz, 03. - 06. September 2013 - Réunion annuelle commune à Linz, 3 - 6 septembre 2013 3<br />
Vorwort; Preisverleihung, Generalversammlung - Avant-Propos; Cérémonie <strong>de</strong> remise <strong>de</strong>s prix, Assemblée générale 3<br />
Informationen für die Mitglie<strong>de</strong>r - Informations pour les membres 4<br />
Zum Tod von Nobelpreisträger Heinrich Rohrer 9<br />
Allgemeine Tagungsinformationen - Informations générales sur <strong>la</strong> réunion 10<br />
Vorläufige Programmübersicht - Résumé préliminaire du programme 12<br />
Aussteller - Exposants 24<br />
Open Access, where do we stand today? 25<br />
Kurz<strong>mitteilungen</strong> - Short Communications 25, 45<br />
19 th Swiss Physics Olympiad 2013 (SPhO) in Aarau 26<br />
Das Rennen um die Industrieproduktion <strong>de</strong>r Zukunft 27<br />
First result from the AMS experiment 28<br />
Progress in Physics (33): Outreach: Can Physics Cross Boundaries? 30<br />
Progress in Physics (34): On the <strong>de</strong>velopment of physically-based regional climate mo<strong>de</strong>lling 32<br />
Progress in Physics (35): A snowf<strong>la</strong>ke in a million <strong>de</strong>gree p<strong>la</strong>sma 36<br />
Physics Anecdotes (17): IBM Research – Zurich, a Success Story 40<br />
Goodbye Herschel 42<br />
Structural MEMS Testing 44<br />
Physique et <strong>la</strong> Société: Quand <strong>la</strong> Physique rejoint le Sport 46<br />
History of Physics (8): On the Einstein-Grossmann Col<strong>la</strong>boration 100 Years ago 48<br />
Histoire <strong>de</strong> <strong>la</strong> Physique (9): Le modèle atomique <strong>de</strong> Bohr: origines, contexte et postérité (part 1) 52<br />
Buchbesprechung: Geschichte <strong>de</strong>s SIN 56<br />
Lehrerfortbildung: 18 Deutschschweizer Lehrer im Herz von CERN 58<br />
Annual Congress of SCNAT 60<br />
Präsi<strong>de</strong>nt / Prési<strong>de</strong>nt<br />
Dr. Andreas Schopper, CERN, Andreas.Schopper@cern.ch<br />
Vorstandsmitglie<strong>de</strong>r <strong>de</strong>r SPG / Membres du Comité <strong>de</strong> <strong>la</strong> SSP<br />
Physikausbildung und -för<strong>de</strong>rung /<br />
Education et encouragement à <strong>la</strong> physique<br />
Dr. Tibor Gyalog, Uni Basel, tibor.gyalog@unibas.ch<br />
Vize-Präsi<strong>de</strong>nt / Vice-Prési<strong>de</strong>nt<br />
Dr. Christophe Rossel, IBM Rüschlikon, rsl@zurich.ibm.com<br />
Sekretär / Secrétaire<br />
Dr. MER Antoine Pochelon, EPFL-CRPP, antoine.pochelon@epfl.ch<br />
Kassier / Trésorier<br />
Dr. Pascal Ruffieux, EMPA, pascal.ruffieux@empa.ch<br />
Kon<strong>de</strong>nsierte Materie / Matière Con<strong>de</strong>nsée (KOND)<br />
Prof. Christian Rüegg, PSI & Uni Genève, christian.rueegg@psi.ch, christian.rueegg@unige.ch<br />
Angewandte Physik / Physique Appliquée (ANDO)<br />
Dr. Ivo Furno, EPFL-CRPP, ivo.furno@epfl.ch<br />
Astrophysik, Kern- und Teilchenphysik /<br />
Astrophysique, physique nucléaire et corp. (TASK)<br />
Prof. Martin Pohl, Uni Genève, martin.pohl@cern.ch<br />
Theoretische Physik / Physique Théorique (THEO)<br />
Prof. Gian Michele Graf, ETH Zürich, gmgraf@phys.ethz.ch<br />
Physik in <strong>de</strong>r Industrie / Physique dans l‘industrie<br />
Dr. Kai Hencken, ABB Dättwil, kai.hencken@ch.abb.com<br />
Atomphysik und Quantenoptik /<br />
Physique Atomique et Optique Quantique<br />
Prof. Antoine Weis, Uni Fribourg, antoine.weis@unifr.ch<br />
Geschichte <strong>de</strong>r Physik / Histoire <strong>de</strong> <strong>la</strong> Physique<br />
Prof. Jan Lacki, Uni Genève, jan.<strong>la</strong>cki@unige.ch<br />
Physik <strong>de</strong>r Er<strong>de</strong>, Atmosphäre und Umwelt /<br />
Physique du globe et <strong>de</strong> l'environnement<br />
Dr. Stéphane Goyette, Uni Genève, stephane.goyette@unige.ch<br />
SPG Administration / Administration <strong>de</strong> <strong>la</strong> SSP<br />
Allgemeines Sekretariat (Mitglie<strong>de</strong>rverwaltung, Webseite, Druck, Versand, Redaktion Bulletin<br />
& SPG Mitteilungen) /<br />
Secrétariat générale (Service <strong>de</strong>s membres, internet, impression, envoi, rédaction Bulletin<br />
& Communications <strong>de</strong> <strong>la</strong> SSP)<br />
S. Albietz, SPG Sekretariat, Departement Physik,<br />
Klingelbergstrasse 82, CH-4056 Basel<br />
Tel. 061 / 267 36 86, Fax 061 / 267 37 84, sps@unibas.ch<br />
Buchhaltung / Service <strong>de</strong> <strong>la</strong> comptabilité<br />
F. Erkadoo, SPG Sekretariat, Departement Physik,<br />
Klingelbergstrasse 82, CH-4056 Basel<br />
Tel. 061 / 267 37 50, Fax 061 / 267 13 49, francois.erkadoo@unibas.ch<br />
Protokollführerin / Greffière<br />
Susanne Johner, SJO@zurich.ibm.com<br />
Wissenschaftlicher Redakteur/ Rédacteur scientifique<br />
Dr. Bernhard Braunecker, Braunecker Engineering GmbH,<br />
braunecker@bluewin.ch<br />
Impressum:<br />
Die SPG Mitteilungen erscheinen ca. 2-4 mal jährlich und wer<strong>de</strong>n an alle Mitglie<strong>de</strong>r abgegeben.<br />
Abonnement für Nichtmitglie<strong>de</strong>r:<br />
CHF 20.- pro Jahrgang (In<strong>la</strong>nd; Aus<strong>la</strong>nd auf Anfrage), incl. Lieferung <strong>de</strong>r Hefte sofort nach Erscheinen frei Haus. Bestellungen<br />
bzw. Kündigungen jeweils zum Jahresen<strong>de</strong> sen<strong>de</strong>n Sie bitte formlos an folgen<strong>de</strong> Adresse:<br />
Ver<strong>la</strong>g und Redaktion:<br />
<strong>Schweizerische</strong> Physikalische Gesellschaft, Klingelbergstr. 82, CH-4056 Basel, sps@unibas.ch, www.sps.ch<br />
Redaktionelle Beiträge und Inserate sind willkommen, bitte wen<strong>de</strong>n Sie sich an die obige Adresse.<br />
Namentlich gekennzeichnete Beiträge geben grundsätzlich die Meinungen <strong>de</strong>r betreffen<strong>de</strong>n Autoren wie<strong>de</strong>r. Die<br />
SPG übernimmt hierfür keine Verantwortung.<br />
Druck:<br />
Werner Druck & Medien AG, Kanonengasse 32, 4001 Basel<br />
2
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Gemeinsame Jahrestagung in Linz, 03. - 06. September 2013<br />
Réunion annuelle commune à Linz, 3 - 6 septembre 2013<br />
Vorwort<br />
Avant-Propos<br />
Im Zweijahresrhythmus organisiert die SPG ihre Jahrestagung<br />
gemeinsam mit <strong>de</strong>r Österreichischen Physikalischen<br />
Gesellschaft (ÖPG) sowie <strong>de</strong>n <strong>Schweizerische</strong>n und Österreichischen<br />
Gesellschaften für Astronomie und Astrophysik<br />
(SGAA und ÖGAA). Dieser Modus hat sich in <strong>de</strong>n<br />
vergangenen Jahren bei <strong>de</strong>n sehr erfolgreichen Tagungen<br />
in Innsbruck (2009) und Lausanne (2011) bewährt. Die diesjährige<br />
Tagung in Linz soll diese Tradition fortsetzen und<br />
<strong>de</strong>n Dialog zwischen Physikern bei<strong>de</strong>r Län<strong>de</strong>r weiter vertiefen.<br />
Mit rund 400 eingereichten Abstracts in 15 Fachsitzungen,<br />
9 Plenarvorträgen und zwei öffentlichen Abendvorträgen,<br />
einer davon von Serge Haroche (Physiknobelpreisträger<br />
2012), steht ein sehr attraktives Programm zur Verfügung.<br />
Zu<strong>de</strong>m fin<strong>de</strong>t vor <strong>de</strong>r gemeinsamen Jahrestagung noch ein<br />
spezieller Energietag statt, zu <strong>de</strong>m alle Tagungsteilnehmer<br />
herzlich willkommen sind.<br />
Im Folgen<strong>de</strong>n fin<strong>de</strong>n Sie die für die SPG-Mitglie<strong>de</strong>r relevanten<br />
Gesellschaftsnachrichten, die wichtigsten Tagungsinformationen<br />
sowie eine vorläufige Programmübersicht.<br />
Das <strong>de</strong>finitive Programm wird in Kürze auf <strong>de</strong>r SPG-Webseite<br />
verfügbar sein.<br />
Der SPG-Vorstand hofft auf eine rege Teilnahme an <strong>de</strong>r Tagung<br />
und freut sich auf Ihren Besuch.<br />
Tous les <strong>de</strong>ux ans, <strong>la</strong> SSP organise sa réunion annuelle<br />
en col<strong>la</strong>boration avec <strong>la</strong> société autrichienne <strong>de</strong> physique<br />
(ÖPG) et les <strong>de</strong>ux sociétés nationales d'astronomie et<br />
d'astrophysique (SSAA et ÖGAA). Ce modèle a fait ses<br />
preuves au cours <strong>de</strong>s <strong>de</strong>rnières années <strong>de</strong> rencontres très<br />
fructueuses à Innsbruck (2009) et à Lausanne (2011). La<br />
conférence <strong>de</strong> cette année à Linz a comme but <strong>de</strong> poursuivre<br />
cette tradition et d’approfondir le dialogue entre les<br />
physiciens <strong>de</strong> ces <strong>de</strong>ux pays.<br />
Avec environ 400 résumés soumis à 15 séances, 9 conférences<br />
plénières et <strong>de</strong>ux conférences publiques, l'une par<br />
Serge Haroche (Prix Nobel <strong>de</strong> physique 2012), un programme<br />
très attrayant a été mis en p<strong>la</strong>ce. En outre, une<br />
journée spéciale <strong>de</strong> l'énergie aura lieu avant <strong>la</strong> réunion<br />
annuelle commune, à <strong>la</strong>quelle tous les participants <strong>de</strong> <strong>la</strong><br />
conférence sont les bienvenus.<br />
Vous trouverez ci-<strong>de</strong>ssous les nouvelles <strong>de</strong> <strong>la</strong> société d’intérêt<br />
pour les membres, ainsi que les informations les plus<br />
importantes sur <strong>la</strong> conférence et sur le programme provisoire.<br />
La version finale sera accessible sous peu sur le site<br />
<strong>de</strong> <strong>la</strong> SSP.<br />
Le comité <strong>de</strong> <strong>la</strong> SSP comptes donc sur une participation<br />
active et nombreuse à notre réunion annuelle et nous réjouissons<br />
<strong>de</strong> votre visite.<br />
Preisverleihung - Cérémonie <strong>de</strong> remise <strong>de</strong>s prix<br />
Mittwoch 04. September 2013, 11:30h - Mercredi 4 septembre 2013, 11:30h<br />
Johannes Kepler Universität Linz, Keplergebäu<strong>de</strong>, Hörsaal 1<br />
Es wer<strong>de</strong>n alle Preise von SPG und ÖPG in einer gemeinsamen<br />
Zeremonie verliehen.<br />
Tous les prix <strong>de</strong> <strong>la</strong> SSP et l'ÖPG seront remises dans une<br />
cérémonie commune.<br />
Generalversammlung 2013 - Assemblée générale 2013<br />
Donnerstag 05. September 2013, 12:00h - Jeudi 5 septembre 2013, 12:00h<br />
Johannes Kepler Universität Linz, Keplergebäu<strong>de</strong>, Hörsaal 4<br />
Traktan<strong>de</strong>n<br />
Ordre du jour<br />
1. Protokoll <strong>de</strong>r Generalversammlung vom<br />
21. Juni 2012<br />
Procès-verbal <strong>de</strong> l'assemblée générale du<br />
21 juin 2012<br />
2. Kurzer Bericht <strong>de</strong>s Präsi<strong>de</strong>nten Bref rapport du prési<strong>de</strong>nt<br />
3. Rechnung 2012, Revisorenbericht Bi<strong>la</strong>n 2012, rapport <strong>de</strong>s vérificateurs <strong>de</strong>s<br />
comptes<br />
4. Wahlen Elections<br />
5. Projekte Projets<br />
6. Diverses Divers<br />
3
SPG Mitteilungen Nr. 40<br />
Neue Mitglie<strong>de</strong>r 2012 -<br />
Nouveaux membres en 2012<br />
Acremann Yves, Adams Jonathan, Ancu Lucian Stefan,<br />
Andreussi Oliviero, Antognini Aldo, Bachmann Maja, Barhoumi<br />
Rafik, Bernard Laetitia, Bettler Marc-Olivier, Bigler<br />
Matthias, Bonvin Camille, Braun Oliver, Brunner Bernhard,<br />
Casa<strong>de</strong>i Diego, Castiglioni Luca, Cepellotti Andrea, Chandrasekaran<br />
Anand, Cheah Erik, Cholleton Danaël, Cohen<br />
Denis, Crivelli Paolo, Doglioni Caterina, Dragoni Daniele,<br />
Ehtesham Alireza, Fantner Georg, Fernan<strong>de</strong>s Vaz Carlos<br />
Antonio, Gibertini Marco, Goyette Stéphane, Havare Ali Kemal,<br />
Herzog Benedikt, Huppert Martin, Issler Mena, Jaffe<br />
Arthur, Jordan Inga, Knabenhans Mischa, Knopp Gregor,<br />
Kraus Peter, Krauth Felix, Küçükbenli Emine, Kuhn Felix<br />
Arjun, Laine Mikko, Leindl Mario, Locher Reto, Mariotti Nico<strong>la</strong>s,<br />
Marzari Nico<strong>la</strong>, Mathys Christoph, Mermod Philippe,<br />
Miguel Sanchez Javier, Montaruli Teresa, Moutafis Christoforos,<br />
Müller Andreas, Nguyen Ngoc Linh, O'Regan David<br />
Daniel, Pizzi Giovanni, Pozzorini Stefano, Rakotomiaramanana<br />
Barinjaka, Reinle-Schmitt Mathil<strong>de</strong> Léna, Ries Dieter,<br />
Rochman Dimitri, Rønnow Henrik Moodysson, Rückauer<br />
Bodo, Sabatini Ricardo, Salman Zaher, Schwarz Sacha,<br />
Si<strong>la</strong>tani Mahsa, Strassmann Peter, Südmeyer Thomas,<br />
Šulc Miros<strong>la</strong>v, Teh<strong>la</strong>r Andres, Tiwari Rakesh, Tolba Tamer,<br />
Tourneur Stéphane, van Megen Bram, Vaniček Jiří, Vindigni<br />
Alessandro, Walter Manuel, Wyszynski Grzegorz, Zimmermann<br />
Tomáš<br />
Ehrenmitglie<strong>de</strong>r - Membres d'honneur<br />
Prof. Hans Beck (2010)<br />
Dr. J. Georg Bednorz (2011)<br />
Prof. Jean-Pierre B<strong>la</strong>ser (1990)<br />
Prof. Jean-Pierre Borel (2001)<br />
Prof. Jean-Pierre Eckmann (2011)<br />
Prof. Charles P. Enz (2005)<br />
Prof. Øystein Fischer (2010)<br />
Prof. Hans Frauenfel<strong>de</strong>r (2001)<br />
Prof. Jürg Fröhlich (2011)<br />
Prof. Hermann Grun<strong>de</strong>r (2001)<br />
Prof. Hans-Joachim Güntherodt (2010)<br />
Dr. Martin Huber (2011)<br />
Prof. Verena Meyer (2001)<br />
Prof. K. Alex Müller (1991)<br />
Prof. Hans Rudolf Ott (2005)<br />
Prof. T. Maurice Rice (2010)<br />
Dr. Heinrich Rohrer (1990)<br />
Prof. Louis Sch<strong>la</strong>pbach (2010)<br />
Statistik - Statistique<br />
Assoziierte Mitglie<strong>de</strong>r - Membres associés<br />
A) Firmen<br />
• F. Hoffmann-La-Roche AG, 4070 Basel<br />
B) Universitäten, Institute<br />
• Albert-Einstein-Center for Fundamental Physics, Universität<br />
Bern, 3012 Bern<br />
• CERN, 1211 Genève 23<br />
• Département <strong>de</strong> Physique, Université <strong>de</strong> Fribourg,<br />
1700 Fribourg<br />
• Departement Physik, Universität Basel, 4056 Basel<br />
• Departement Physik, ETH Zürich, 8093 Zürich<br />
• EMPA, 8600 Dübendorf<br />
• Lab. <strong>de</strong> Physique <strong>de</strong>s Hautes Energies (LPHE), EPFL,<br />
1015 Lausanne<br />
• Paul Scherrer Institut, 5332 Villigen PSI<br />
• Physik-Institut, Universität Zürich, 8057 Zürich<br />
• Section <strong>de</strong> Physique, Université <strong>de</strong> Genève, 1211 Genève<br />
4<br />
C) Stu<strong>de</strong>ntenfachvereine<br />
• AEP - Association <strong>de</strong>s Etudiant(e)s en Physique, Université<br />
<strong>de</strong> Genève, 1211 Genève 4<br />
• Fachschaft Physik und Astronomie, Universität Bern,<br />
3012 Bern<br />
• Fachschaft Physique, Université <strong>de</strong> Fribourg, 1700 Fribourg<br />
• Fachverein Physik <strong>de</strong>r Universität Zürich (FPU),<br />
8057 Zürich<br />
• FG 14 (Fachgruppe für Physik-, Mathematik- und Versicherungswissenschaft),<br />
Universität Basel, 4056 Basel<br />
• Les Irrotationnels, EPFL, 1015 Lausanne<br />
• Verein <strong>de</strong>r Mathematik- und Physikstudieren<strong>de</strong>n an<br />
<strong>de</strong>r ETH Zürich (VMP), 8092 Zürich<br />
Verteilung <strong>de</strong>r Mitgliedskategorien -<br />
Répartition <strong>de</strong>s catégories <strong>de</strong> membres<br />
(31.12.2012)<br />
Or<strong>de</strong>ntliche Mitglie<strong>de</strong>r 726<br />
Doktoran<strong>de</strong>n 55<br />
Stu<strong>de</strong>nten 80<br />
Doppelmitglie<strong>de</strong>r DPG, ÖPG o<strong>de</strong>r APS 164<br />
Doppelmitglie<strong>de</strong>r PGZ 41<br />
Mitglie<strong>de</strong>r auf Lebenszeit 144<br />
Assoziierte Mitglie<strong>de</strong>r 19<br />
Bibliotheksmitglie<strong>de</strong>r 2<br />
Ehrenmitglie<strong>de</strong>r 18<br />
Beitragsfreie (Korrespon<strong>de</strong>nz) 7<br />
Total 1256<br />
4
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Jahresbericht 2012 <strong>de</strong>s Präsi<strong>de</strong>nten - Rapport annuel 2012 du prési<strong>de</strong>nt<br />
The major event of our society in 2012 was once more the<br />
annual SPS meeting that took p<strong>la</strong>ce from 21-22 June 2012<br />
at the Hönggerberg campus of the ETHZ, jointly organized<br />
with the four National Centres of Competence in Research<br />
(NCCR) MaNEP, MUST, Nano and QSIT as well as with the<br />
Swiss Society for Crystallography. More than 550 persons<br />
atten<strong>de</strong>d the meeting. The scientific program was rather<br />
<strong>de</strong>nse with 6 plenary talks, 237 talks distributed over<br />
14 parallel sessions and 170 posters. Worth mentioning is<br />
the successful session of the new section "Earth, Atmosphere<br />
and Environmental Physics" and a <strong>de</strong>dicated session<br />
to celebrate the birth of crystallography in 1912 "100 Years<br />
of Diffraction". It was very satisfying to observe a <strong>la</strong>rge<br />
participation of young enthusiastic physicists sharing their<br />
research results and their experiences in a lively manner.<br />
The interest by the commercial exhibitors was once more<br />
well <strong>de</strong>monstrated by the attendance of 21 companies. As<br />
every year, the annual meeting was also the occasion to<br />
announce and present the winners of the SPS Awards in<br />
General Physics, Con<strong>de</strong>nsed Matter Physics and Applied<br />
Physics.<br />
It became a tradition that SPS organises in col<strong>la</strong>boration<br />
with the Physikalische Gesellschaft Zürich PGZ a joint symposium<br />
every year. In September 2012, PGZ and SPS celebrated<br />
together the 125 years of PGZ with a meeting in<br />
Zürich on "General re<strong>la</strong>tivity and its applications".<br />
Fostering its international re<strong>la</strong>tions, every other year the<br />
SPS organises its annual meeting together with the Austrian<br />
Physical Society ÖPG that will take p<strong>la</strong>ce in Linz in 2013.<br />
The SPS maintained tight links to the European Physical<br />
Society EPS, participating in its Council and in various activities<br />
of its groups. In 2012 our society also welcomed its<br />
first international Associate Member with domicile in Switzer<strong>la</strong>nd,<br />
namely CERN.<br />
In view of promoting young scientists, the SPS Young<br />
Physicist Forum YPF, that was created in 2010 and that<br />
regroups most of the Swiss physics stu<strong>de</strong>nt associations,<br />
has been accepted as a Commission of SPS in 2012. In the<br />
framework of this very active forum, the young physicists<br />
had organised a SPS sponsored visit to the International<br />
Laboratory for Particle Physics CERN at Geneva. As every<br />
year, our society also sponsored activities of the Swiss<br />
Young Physicists Tournament SYPT as well as of the Swiss<br />
Physics Olympiads SPhO, with two SPS prizes awar<strong>de</strong>d to<br />
the best male and female finalists of SPhO.<br />
Furthermore, our society also supported Swiss stu<strong>de</strong>nts for<br />
attending the 13 th IONS (International OSA Network of Stu<strong>de</strong>nts)<br />
conference, that was jointly organized by PhD stu<strong>de</strong>nts<br />
from EPFL and ETH and that took p<strong>la</strong>ce in Zürich and<br />
Lausanne from 9-12 Jan, 2013.<br />
Three times per year the SPS publishes its "Communications",<br />
which is the most important SPS publication to disseminate<br />
information about on-going activities within the<br />
society and to review scientific progress in various areas.<br />
High-c<strong>la</strong>ss articles have been published in the various,<br />
now well established rubrics. A paper copy is distributed<br />
to all members, whilst open access to this publication is<br />
also granted to the entire Swiss scientific community via<br />
the SPS homepage.<br />
SPS is a member organization of the Swiss Aca<strong>de</strong>my of<br />
Science SCNAT and part of the p<strong>la</strong>tform Mathematics, Astronomy<br />
and Physics MAP. With two SPS representatives<br />
in the organising committee, our society is supporting<br />
the p<strong>la</strong>tform MAP actively in organising the "SCNAT-Jahreskongress<br />
2013" on the occasion of the jubilee of "100<br />
Jahre Bohr'sches Atommo<strong>de</strong>ll".<br />
We are grateful to the organizational and financial support<br />
of SCNAT and acknowledge also support of the Swiss<br />
Aca<strong>de</strong>my of Engineering Science SATW. Thanks to a wellba<strong>la</strong>nced<br />
program the Swiss Physical Society could once<br />
more close its budget with a positive ba<strong>la</strong>nce for 2012.<br />
Andreas Schopper, SPS Presi<strong>de</strong>nt, May 2013<br />
Protokoll <strong>de</strong>r Generalversammlung vom 21. Juni 2012 in Zürich<br />
Protocole <strong>de</strong> l'assemblée générale du 21 juin 2012 à Zürich<br />
Traktan<strong>de</strong>n<br />
1. Protokoll <strong>de</strong>r Generalversammlung vom 16.06.2011<br />
2. Bericht <strong>de</strong>s Präsi<strong>de</strong>nten<br />
3. Rechnung 2011 & Revisorenbericht<br />
4. Anpassung <strong>de</strong>r Statuten<br />
5. Neue Sektion und Kommission<br />
6. Projekte<br />
7. Wahlen<br />
Der Präsi<strong>de</strong>nt, Christophe Rossel, eröffnet die Generalversammlung<br />
um 12:00 Uhr. Anwesend sind 41 Mitglie<strong>de</strong>r.<br />
1. Protokoll <strong>de</strong>r letzten GV vom 16.6.2011 in Lausanne<br />
Herrn Peter Wolff beanstan<strong>de</strong>t <strong>de</strong>n ihn betreffen<strong>de</strong>n ersten<br />
Satz unter Traktandum „6. Diverses“ und verweist auf das<br />
GV-Protokoll 2010 (Basel). Da keine Neuformulierung vorliegt,<br />
wird über die in <strong>de</strong>n SPG-Mitteilungen veröffentlichte<br />
Version abgestimmt und diese mit 35 Stimmen genehmigt,<br />
bei 5 Enthaltungen und 1 Gegenstimme.<br />
(Siehe dazu <strong>de</strong>n NACHTRAG am Schluss dieses Protokolls).<br />
2. Bericht <strong>de</strong>s Präsi<strong>de</strong>nten<br />
Der Jahresbericht 2011 <strong>de</strong>s Präsi<strong>de</strong>nten wur<strong>de</strong> auf Seite 5<br />
<strong>de</strong>r "SPG Mitteilungen Nr. 37" im Mai 2012 veröffentlicht.<br />
Christophe Rossel erläutert kurz einige Punkte:<br />
5
SPG Mitteilungen Nr. 40<br />
• Die gemeinsame Jahrestagung mit <strong>de</strong>r Österreichischen<br />
Physikalischen Gesellschaft (ÖPG) und <strong>de</strong>n<br />
bei<strong>de</strong>n nationalen Gesellschaften für Astronomie und<br />
Astrophysik (SGAA und ÖGAA) vom 15.-17. Juni 2011<br />
in Lausanne war wie<strong>de</strong>rum ein Erfolg mit rund 650 Teilnehmen<strong>de</strong>n,<br />
10 Plenarvorträgen, 470 Beiträgen verteilt<br />
auf 10 Parallel-Sitzungen, dazu zahlreichen Postern<br />
und 22 Ausstellern.<br />
• Die Generalversammlung 2011 ernannte vier neue Ehrenmitglie<strong>de</strong>r:<br />
Dr. J. Georg Bednorz, Prof. Jean-Pierre<br />
Eckmann, Prof. Jürg Fröhlich und Dr. Martin Huber.<br />
• Die Mitglie<strong>de</strong>rzahl ist auf etwa 1'250 gestiegen, was<br />
einer Zunahme von rund 10% gegenüber <strong>de</strong>m Vorjahr<br />
entspricht. Bei <strong>de</strong>n 18 Kollektiv- (neu: assoziierten) Mitglie<strong>de</strong>rn<br />
ist bei <strong>de</strong>n Firmen ein Rückgang zu verzeichnen,<br />
dafür sind mehr Universitäten und Stu<strong>de</strong>ntenorganisationen<br />
vertreten.<br />
3. Rechnung 2011 & Revisorenbericht<br />
Der Kassier, Pierangelo Gröning, präsentiert und erläutert<br />
die Jahresrechnung 2011, die <strong>de</strong>tailliert in <strong>de</strong>n "SPG-Mitteilungen<br />
Nr. 37" auf Seite 7 veröffentlicht wur<strong>de</strong>. Sie schliesst<br />
mit einem Gewinn von CHF 17'200.36 und einem Vereinsvermögen<br />
von CHF 36'606.87.<br />
Der Empfehlung <strong>de</strong>r Revisoren folgend genehmigt die Generalversammlung<br />
die Jahresrechnung 2011 und <strong>de</strong>r Kassier<br />
wird mit bestem Dank für die gute Rechnungsführung<br />
ent<strong>la</strong>stet.<br />
4. Anpassung <strong>de</strong>r Statuten<br />
Die Generalversammlung stimmt <strong>de</strong>r auf Seite 9 <strong>de</strong>r "SPG-<br />
Mitteilungen Nr. 37" veröffentlichten Anpassung <strong>de</strong>r Statuten<br />
einstimmig zu. Somit wird <strong>de</strong>r Begriff "Kollektivmitglie<strong>de</strong>r"<br />
durch "Assoziierte Mitglie<strong>de</strong>r" ersetzt und in Art. 2<br />
die Definition <strong>de</strong>r Gruppe B um "überstaatliche bzw. internationale"<br />
erweitert.<br />
5. Neue Sektion und Kommission<br />
Die Generalversammlung stimmt folgen<strong>de</strong>n Neugründungen<br />
einstimmig zu.<br />
• Neue Sektion:<br />
Physik <strong>de</strong>r Er<strong>de</strong>, Atmosphäre und Umwelt -<br />
Earth, Atmosphere and Environmental Physics -<br />
Physique du Globe et <strong>de</strong> l'Environnement<br />
• Neue Kommission:<br />
Young Physicists Forum<br />
6. Projekte<br />
• Im September 2013 soll die nächste gemeinsame Jahrestagung<br />
mit <strong>de</strong>r ÖPG in Linz stattfin<strong>de</strong>n.<br />
• In Zusammenarbeit mit <strong>de</strong>r PGZ wird am 29.9.2012 das<br />
Symposium „Allgemeine Re<strong>la</strong>tivitätstheorie und ihre<br />
Anwendungen“ an <strong>de</strong>r Universität Zürich, organisiert.<br />
• Das neu als Kommission integrierte „Young Physicists<br />
Forum“ wird Aktivitäten, Betriebsbesichtigungen und<br />
Exkursionen für Stu<strong>de</strong>nten organisieren.<br />
• Die Final-Run<strong>de</strong> <strong>de</strong>r Schweizer Physik-Olympia<strong>de</strong><br />
hat am 21./22. April 2012 in Aarau stattgefun<strong>de</strong>n. Die<br />
Goldmedaillen-Gewinner Thanh Phong Lê und Laura<br />
Gremion wur<strong>de</strong>n zusätzlich mit <strong>de</strong>n bei<strong>de</strong>n SPG-<br />
Nachwuchspreisen ausgezeichnet. Die Internationale<br />
Physik-Olympia<strong>de</strong> fin<strong>de</strong>t im Juli in Est<strong>la</strong>nd statt.<br />
• Ebenfalls im Juli 2012 wird das „International Young<br />
Physicists Tournament“ (IYPT) in Bad Sulgau (D) stattfin<strong>de</strong>n.<br />
• Die SPG könnte sich am Swiss Young Physicists' Tournament<br />
2013 beteiligen. Im Jahr 2016 wird das IYPT<br />
möglicherweise in <strong>de</strong>r Schweiz organisiert.<br />
• Im 2013 wird das Jubiläum "100 Jahre Bohr'sches<br />
Atommo<strong>de</strong>ll" gefeiert.<br />
• 2015 wur<strong>de</strong> zum „Internationalen Jahr <strong>de</strong>s Lichts“ bestimmt.<br />
Dann wird die SCNAT auch ihr 200jähriges Bestehen<br />
feiern.<br />
7. Wahlen<br />
Der Präsi<strong>de</strong>nt dankt <strong>de</strong>n bei<strong>de</strong>n ausschei<strong>de</strong>n<strong>de</strong>n Vorstandsmitglie<strong>de</strong>rn<br />
Urs Staub (Kon<strong>de</strong>nsierte Materie) und<br />
Pierangelo Gröning (Kassier) für Ihren <strong>la</strong>ngjährigen Einsatz.<br />
Und <strong>de</strong>r Vizepräsi<strong>de</strong>nt, Andreas Schopper, dankt <strong>de</strong>m zurücktreten<strong>de</strong>n<br />
Präsi<strong>de</strong>nten, Christophe Rossel, für seine<br />
vierjährige Amtszeit.<br />
In corpore wer<strong>de</strong>n einstimmig gewählt:<br />
• Präsi<strong>de</strong>nt (bisher Vizepräsi<strong>de</strong>nt): Dr. Andreas Schopper,<br />
CERN<br />
• Vize-Präsi<strong>de</strong>nt (bisher Präsi<strong>de</strong>nt): Dr. Christophe Rossel,<br />
IBM Research Zurich<br />
• Kassier (bisher Revisor): Dr. Pascal Ruffieux, EMPA<br />
• Kon<strong>de</strong>nsierte Materie (neu): Dr. Christian Rüegg, PSI<br />
• Theoretische Physik (bisher ad interim): Prof. Gian Michele<br />
Graf, ETH Zürich<br />
• Physik <strong>de</strong>r Er<strong>de</strong>, Atmosphäre und Umwelt (neu): Dr.<br />
Stéphane Goyette, Universität Genf<br />
Die übrigen Vorstandsmitglie<strong>de</strong>r bleiben für ihre restliche<br />
Amtszeit unverän<strong>de</strong>rt.<br />
Der neue Präsi<strong>de</strong>nt dankt <strong>de</strong>n Anwesen<strong>de</strong>n für ihr Erscheinen<br />
sowie <strong>de</strong>n Delegierten und seinen Vorstandskollegen<br />
für ihren Einsatz und die gute Zusammenarbeit.<br />
En<strong>de</strong> <strong>de</strong>r Generalversammlung: 12:45 Uhr.<br />
Zürich, 21. Juni 2012<br />
Die Protokollführerin: Susanne Johner<br />
NACHTRAG zu Punkt 1, Protokoll <strong>de</strong>r letzten GV vom<br />
16.06.2011 in Lausanne<br />
Nach <strong>de</strong>r GV stimmt Herr Peter Wolff folgen<strong>de</strong>r Neuformulierung<br />
zu:<br />
Der erste Satz unter Traktandum "6. Diverses" wird ersetzt<br />
durch:<br />
"Herr Peter Wolff erinnert an sein Anliegen betreffend die<br />
Schwierigkeiten, nicht-englische Artikel in wissenschaftlichen<br />
Zeitschriften zu publizieren, welches er an <strong>de</strong>r GV<br />
2010 in Basel geäussert hatte."<br />
6
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Jahresrechnung 2012 - Bi<strong>la</strong>n annuel 2012<br />
Bi<strong>la</strong>nz per 31.12.2012<br />
Aktiven<br />
Um<strong>la</strong>ufsvermögen<br />
Postscheckkonto 55733,76<br />
Bank - UBS 230-627945.M1U 14378,51<br />
Debitoren - Mitglie<strong>de</strong>r 6450,00<br />
Debitoren - SCNAT/SATW u.a.m. 39180,80<br />
Transitorische Aktiven 2853,81<br />
Passiven<br />
An<strong>la</strong>gevermögen<br />
Beteiligung EP Letters 15840,00<br />
Mobilien 1,00<br />
Fremdkapital<br />
Mobiliar 1,00<br />
Mitglie<strong>de</strong>r Lebenszeit 59824,50<br />
Transitorische Passiven 10729,25<br />
Eigenkapital<br />
Vefügbares Vermögen 36606,87<br />
Total Passiven 134437,88 107161,62<br />
Gewinn 27276,26<br />
Total 134437,88 134437,88<br />
Verfügbares Vermögen per 31.12.12 nach Gewinnzuweisung 63883,13<br />
Erfolgsrechnung per 31.12.2012<br />
Aufwand<br />
Gesellschaftsaufwand<br />
EPS - Membership 14364,81<br />
SCNAT - Membership 8400,00<br />
SATW-Mitglie<strong>de</strong>rbeitrag 1750,00<br />
Ertrag<br />
SCNAT und SATW Zahlungs- und Verpflichtungskredite<br />
SPG-Jahrestagung 18240,86<br />
Schweizer Physik Olympia<strong>de</strong> 4000,00<br />
SPG Young Physicist's Forum 1180,80<br />
SCNAT/SPG Bulletin 9627,00<br />
SCNAT Periodika (SPG-Mitteilungen, Druckkosten) 15720,20<br />
SCNAT Int. Young Phys. Tournament 5500,00<br />
SCNAT Ent<strong>de</strong>ckungen <strong>de</strong>s Jahres 1912 4142,90<br />
SATW Earth Sciences 2350,00<br />
SATW Light and Sound Exhibition 3000,00<br />
Betriebsaufwand<br />
Löhne 11909,76<br />
Sozialleistungen 1806,60<br />
Porti/Telefonspesen/WWW- und PC-Spesen 814,95<br />
Versand (Porti Massensendungen) 7080,30<br />
Unkosten 3395,85<br />
Büromaterial 4492,30<br />
Ausseror<strong>de</strong>ntlicher Aufwand 4536,70<br />
Bankspesen 138,00<br />
Debitorenverluste Mitglie<strong>de</strong>r 1665,00<br />
Debitorenverlust SCNAT/SATW u.a.m. 5319,20<br />
Sekretariatsaufwand extern 12375,00<br />
Ertrag<br />
Mitglie<strong>de</strong>rbeiträge 98826,30<br />
Inserate/Flyerbei<strong>la</strong>gen SPG Mitteilungen 5170,00<br />
Aussteller 12744,94<br />
Zinsertrag 99,80<br />
Ertrag aus EP Letters Beteiligung 2745,45<br />
SCNAT und SATW Zahlungs- und Verpflichtungskredite<br />
SPG-Jahrestagung (SCNAT) 15000,00<br />
Schweizer Physik Olympia<strong>de</strong> 4500,00<br />
SPG Young Physicist's Forum 6000,00<br />
SCNAT Ent<strong>de</strong>ckungen <strong>de</strong>s Jahres 1912 4000,00<br />
SPG Bulletin (SCNAT) 5500,00<br />
Periodika (SPG-Mitteilungen, Druckkosten) (SCNAT) 4000,00<br />
SCNAT Int. Young Phys. Tournament 5500,00<br />
SATW Earth Sciences 2000,00<br />
SATW Light and Sound Exhibition 3000,00<br />
Total Aufwand / Ertrag 141810,23 169086,49<br />
Gewinn 27276,26<br />
Total 169086,49 169086,49<br />
7
SPG Mitteilungen Nr. 40<br />
Revisorenbericht zur Jahresrechnung 2012<br />
Die Jahresrechnung 2012 <strong>de</strong>r SPG wur<strong>de</strong> von <strong>de</strong>n unterzeichneten Revisoren geprüft und<br />
mit <strong>de</strong>n Belegen in Übereinstimmung befun<strong>de</strong>n.<br />
Die Revisoren empfehlen <strong>de</strong>r Generalversammlung <strong>de</strong>r SPG, die Jahresrechnung zu<br />
genehmigen und <strong>de</strong>n Kassier mit bestem Dank für die gute Rechnungsführung zu<br />
ent<strong>la</strong>sten.<br />
Die Revisoren <strong>de</strong>r SPG:<br />
Prof. Dr. Philipp Aebi<br />
Dr. Pierangelo Gröning<br />
Basel, 04. April 2013<br />
F. Erkadoo, SPG Büro, Departement Physik, Klingelbergstrasse 82, CH-4056 Basel<br />
Tel : 061 / 267 37 50, Fax : 061 / 267 13 49, Email : francois.erkadoo@unibas.ch<br />
8
News from SPS committee meetings (February & April)<br />
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Annual Meetings: The SPS meeting in 2014 will be held in Fribourg<br />
beginning of July, together with the National Centres of Competence<br />
in Research (NCCRs). The meeting in 2015 is p<strong>la</strong>nned with<br />
the Austrian Societies in Wien.<br />
Communications: The SPS has two major means of communication,<br />
the "SPG Mitteilungen" ("Communications <strong>de</strong> <strong>la</strong> SSP") and<br />
the SPS homepage (www.sps.ch). To further improve communication,<br />
from now on, we will report about <strong>de</strong>cisions from the executive<br />
committee meetings in the "SPG Mitteilungen". The editorial<br />
board is being en<strong>la</strong>rged, with the entire committee contributing<br />
to articles of the specific rubrics. With the aim of better publicizing<br />
colloquia, talks and seminars of general interest in Swiss<br />
aca<strong>de</strong>mic centres and universities, a list of these events and their<br />
links will be provi<strong>de</strong>d on the SPS website. You are most welcome<br />
to communicate events of interest to the SPS Secretariat<br />
(sps@unibas.ch).<br />
Projects: One of the main emphases of the SPS is to promote<br />
young aca<strong>de</strong>mics through a variety of activities and projects. The<br />
Young Physicists Forum (YPF), a commission of SPS also represented<br />
in the executive committee, organized a 2-day meeting on<br />
"Physics and Sport". (see p. 46 for a <strong>de</strong>tailed report). Another continuous<br />
en<strong>de</strong>avour of the SPS is to improve the contact between<br />
the teachers and the organizers of courses or training for secondary<br />
school teachers. The involvement of teachers varies from<br />
canton to canton, due to very different levels of encouragement<br />
(from the obligation of following paid courses during teaching time<br />
to the encouragement of following only courses at one’s expense<br />
and outsi<strong>de</strong> working time). In view of this year’s discovery of the<br />
Higgs particle, a visit to CERN took p<strong>la</strong>ce in cooperation with H. P.<br />
Beck and www.teilchenphysik.ch , in particu<strong>la</strong>r for teachers from<br />
the Swiss German. For the en<strong>la</strong>rgement of outreach to all domains<br />
of physics, it is felt that simi<strong>la</strong>r activities should <strong>de</strong>velop over the<br />
next years in other fields of physics.<br />
This year the SPS was once more involved in the Swiss Physics<br />
Olympiad (SPhO) by awarding 4 prizes, in the special recipients’<br />
configuration of 2013 including Liechtenstein in the winners. For<br />
the first time, Switzer<strong>la</strong>nd and Liechtenstein will organise the 2016<br />
International Physics Olympiad (typically 400 participants from 95<br />
countries), which will require additional organisational and scientific<br />
forces to be involved.<br />
There exists a <strong>de</strong>mand from secondary schools stu<strong>de</strong>nts to become<br />
members of the Society: as a very first action, we will try<br />
to establish an e-mail list, with the link to the electronic version of<br />
"SPS Communications" to be sent for each new publication.<br />
Contact to Aca<strong>de</strong>mies: The SATW has new structures and commissions<br />
(scientific advisory board, topical p<strong>la</strong>tforms, etc.) in<br />
which now more physicists can take part as experts; SPS will<br />
spread the information to its members. The SCNAT encourages<br />
participation to the "200 years SCNAT" Jubilee in 2015; the SPS<br />
will support the "Pop-up Lab" for this event, a project supported<br />
by AGORA, which is a SNF tool to intensify and fund dialogue<br />
between science and public.<br />
Contact to EPS: SPS has submitted a nomination to the EPS<br />
Physics Education Division Award. A <strong>de</strong>legation has participated<br />
to the Energy Group Meeting. A variety of SPS actions have been<br />
<strong>de</strong>fined to follow-up on the outcome of the EPS council meeting.<br />
Zum Tod von Nobelpreisträger Heinrich Rohrer<br />
Mit grosser Bestürzung und Trauer<br />
musste die SPG vom Tod ihres Ehrenmitglieds<br />
Heinrich Rohrer erfahren, <strong>de</strong>r<br />
am 16. Mai im Alter von 79 Jahren verstarb.<br />
Er war von 1963 bis 1997 am IBM<br />
Forschungszentrum in Rüschlikon tätig<br />
und gilt als einer <strong>de</strong>r massgeben<strong>de</strong>n<br />
Pioniere <strong>de</strong>r Nanowissenschaften, <strong>de</strong>ren<br />
Wer<strong>de</strong>gang aus <strong>de</strong>m Forschungsstadium<br />
heraus zur mittlerweile alle<br />
Bereiche <strong>de</strong>s täglichen Lebens erfassen<strong>de</strong>n<br />
Nanotechnologie er aktiv mitgestalten<br />
konnte. Für seine Erfindung<br />
<strong>de</strong>s Rastertunnelmikroskops wur<strong>de</strong> er<br />
1986 zusammen mit Gerd Binnig mit <strong>de</strong>r<br />
höchsten Auszeichnung in Physik, <strong>de</strong>m<br />
Nobelpreis, geehrt.<br />
Eine <strong>de</strong>r letzten beeindrucken<strong>de</strong>n Anwendungen<br />
seiner Pionierarbeit ist <strong>de</strong>r kurze Film "a Boy<br />
and his Atom" über einen Jungen, <strong>de</strong>r mit einem Atom<br />
spielt, und <strong>de</strong>r als kleinster Film <strong>de</strong>r Welt kürzlich von Wissenschaftlern<br />
am IBM Forschungs<strong>la</strong>bor Alma<strong>de</strong>n / San<br />
Jose (USA) produziert wur<strong>de</strong>. Im gewissen Sinn eine Parabel<br />
über Heini, <strong>de</strong>r gerne seine Begeisterung für die Nanowissenschaft<br />
weltweit an die junge Generation weitergab.<br />
Das mag auch noch folgen<strong>de</strong> kleine Begebenheit illustrieren:<br />
Als eine Gruppe von Leica-Physikern gegen En<strong>de</strong> <strong>de</strong>r<br />
80er Jahre während einer Zugfahrt von Lausanne nach<br />
Image courtesy of IBM Research – Zurich<br />
Heerbrugg unerwartete technische<br />
Schwierigkeiten in einem Gemeinschaftsprojekt<br />
mit <strong>de</strong>r EPFL <strong>la</strong>utstark<br />
bek<strong>la</strong>gte, kam Heini Rohrer aus <strong>de</strong>m<br />
Nebenabteil überraschend zu uns und<br />
meinte schelmisch, dass wir die Beschäftigung<br />
mit Problemen im Submikrometerbereich<br />
doch positiv als Chance<br />
für <strong>de</strong>n Einstieg in <strong>de</strong>n Nanobereich<br />
mit all seinen ungeahnten Möglichkeiten<br />
sehen sollten! Während wir Älteren noch<br />
recht skeptisch blickten, wur<strong>de</strong>n unsere<br />
jüngeren Kollegen durch diese ermuntern<strong>de</strong>n<br />
Worte sichtbar aufgerichtet.<br />
Seine Persönlichkeit und die Be<strong>de</strong>utung<br />
seines Wirkens wer<strong>de</strong>n von IBM unter<br />
folgen<strong>de</strong>m Link http://www.research.<br />
ibm.com/articles/heinrich-rohrer.shtml<br />
eindrücklich geschil<strong>de</strong>rt.<br />
So verlieren wir Physiker einen liebenswerten Freund und<br />
Kollegen, <strong>de</strong>ssen beschei<strong>de</strong>ne Art, sein subtiler Humor,<br />
seine grossartigen wissenschaftlichen Leistungen und vor<br />
allem seine stete Hilfsbereitschaft uns in bester Erinnerung<br />
bleiben wer<strong>de</strong>n.<br />
C. Rossel (IBM Research - Zurich) und B. Braunecker (früher<br />
Leica Geosystems)<br />
9
SPG Mitteilungen Nr. 40<br />
Allgemeine Tagungsinformationen - Informations générales sur <strong>la</strong> réunion<br />
Konferenzwebseite und Anmeldung<br />
Alle Teilnehmeranmeldungen wer<strong>de</strong>n über die Konferenzwebseite<br />
vorgenommen.<br />
www.sps.ch o<strong>de</strong>r www.jku.at/hfp/oepgsps13<br />
Anmel<strong>de</strong>schluß: 1. August 2013<br />
Tagungsort<br />
Johannes Kepler Universität Linz, Keplergebäu<strong>de</strong><br />
Tagungssekretariat<br />
Das Tagungssekretariat befin<strong>de</strong>t sich beim Haupteingang<br />
zur Tagung, vor <strong>de</strong>m Hörsaal 1.<br />
Öffnungszeiten:<br />
Di 03.09. 09:00 - 19:00<br />
Mi - Do 04. - 05.09. 08:00 - 19:00<br />
Fr 06.09. 08:00 - 15:00<br />
Alle Tagungsteilnehmer mel<strong>de</strong>n sich bitte vor <strong>de</strong>m Besuch<br />
<strong>de</strong>r ersten Veranstaltung beim Sekretariat an, wo<br />
Sie ein Namensschild und allfällige weitere Unter<strong>la</strong>gen<br />
erhalten sowie die Tagungsgebühr bezahlen.<br />
Wichtig: Ohne Namensschild ist kein Zutritt zu einer<br />
Veranstaltung möglich.<br />
Wir empfehlen Ihnen, wenn möglich <strong>de</strong>n Dienstag<br />
Nachmittag für die Anmeldung zu nutzen. So können<br />
Sie am Mittwoch direkt ohne Wartezeiten die Vorträge<br />
besuchen.<br />
Achtung: Das Tagungssekretariat gibt kein technisches<br />
o<strong>de</strong>r Büromaterial ab. Je<strong>de</strong>r Teilnehmer ist für seine<br />
Ausrüstung (Mobilrechner, Laserpointer, Adapter, Schere,<br />
Reissnägel, Folien usw.) selber verantwortlich !<br />
Hörsäle<br />
In allen Hörsälen stehen Beamer und Hellraumprojektoren<br />
zur Verfügung. Bitte bringen Sie Ihre eigenen Mobilrechner<br />
und evtl. Adapter und USB Stick/CD mit.<br />
Postersession<br />
Die Postersession fin<strong>de</strong>t am Mittwoch und Donnerstag<br />
Abend sowie am Freitag während <strong>de</strong>r Mittagspause in<br />
<strong>de</strong>r Halle statt. Bitte bringen Sie Befestigungsmaterial<br />
(Reissnägel, Klebestreifen) selbst mit. Die Posterwän<strong>de</strong><br />
sind entsprechend diesem Programm numeriert, sodaß<br />
je<strong>de</strong>r Teilnehmer "seine" Wand leicht fin<strong>de</strong>n sollte. Alle<br />
Poster sollen an allen drei Tagen präsentiert wer<strong>de</strong>n.<br />
Maximale Postergröße: A0 Hochformat<br />
Zahlung<br />
Wir bitten Sie, die Tagungsgebühren im Voraus zu bezahlen.<br />
Sie verkürzen damit die Wartezeiten am Tagungssekretariat,<br />
erleichtern uns die Arbeit und sparen<br />
darüber hinaus noch Geld !<br />
Die Angaben zur Zahlung wer<strong>de</strong>n während <strong>de</strong>r Anmeldung<br />
direkt auf <strong>de</strong>r Webseite angezeigt.<br />
Site web <strong>de</strong> <strong>la</strong> conférence et inscription<br />
L'inscription <strong>de</strong>s participants se fait sur le site web <strong>de</strong><br />
<strong>la</strong> conférence.<br />
www.sps.ch ou www.jku.at/hfp/oepgsps13<br />
Dé<strong>la</strong>i d'inscription: 1 er août 2013<br />
Lieu <strong>de</strong> <strong>la</strong> conférence<br />
Johannes Kepler Universität Linz, Bâtiment "Kepler"<br />
Secrétariat <strong>de</strong> <strong>la</strong> conférence<br />
Le secrétariat <strong>de</strong> <strong>la</strong> réunion se trouve juste à l'entrée,<br />
<strong>de</strong>vant l'auditoire 1.<br />
Heures d'ouverture :<br />
Mar 3.9. 09:00 - 19:00<br />
Mer - Jeu 4. - 5.9. 08:00 - 19:00<br />
Ven 6.9. 08:00 - 15:00<br />
Tous les participants doivent se présenter en premier<br />
lieu au secrétariat <strong>de</strong> <strong>la</strong> conférence afin <strong>de</strong> recevoir leur<br />
badge et les divers documents ainsi que pour le paiement<br />
<strong>de</strong>s frais d'inscription.<br />
Attention: Sans badge, l'accès aux sessions <strong>de</strong> <strong>la</strong> manifestation<br />
sera refusé.<br />
Nous vous recommandons <strong>de</strong> vous inscrire déjà mardi<br />
après-midi afin d'éviter <strong>de</strong>s temps d'attente inutiles<br />
mercredi matin.<br />
Attention: Le secrétariat <strong>de</strong> <strong>la</strong> conférence ne met aucun<br />
matériel technique ni matériel <strong>de</strong> bureau à disposition.<br />
Chaque participant est responsable <strong>de</strong> son équipement<br />
(ordinateur, pointeur <strong>la</strong>ser, adaptateurs, ciseaux, punaises,<br />
...) !<br />
Auditoires<br />
Les auditoires disposent tous d’un projecteur multimédia<br />
(beamer) et d'un projecteur pour transparents.<br />
Veuillez apporter votre ordinateur portable ainsi que<br />
d'éventuels accessoires tels que clé USB ou CD.<br />
Séance posters<br />
Les posters seront présentés dans le hall le mercredi<br />
et jeudi soir et pendant <strong>la</strong> pause <strong>de</strong> midi <strong>de</strong> vendredi.<br />
Veuillez amener vous-même le matériel nécessaire pour<br />
fixer les posters (punaises, ruban adhésif). Les panneaux<br />
<strong>de</strong> posters seront numérotés suivant le numéro<br />
<strong>de</strong> l'abstract indiqué dans le programme. Tous les posters<br />
<strong>de</strong>vraient rester installés pendant les trois jours.<br />
Dimension maximale: A0, format portrait<br />
Paiement<br />
Nous vous prions <strong>de</strong> régler d'avance vos frais d'inscription.<br />
De cette manière vous éviterez <strong>de</strong>s files d'attente<br />
et vous nous facilitez notre travail. En plus vous pourrez<br />
faire <strong>de</strong>s économies !<br />
Les informations pour le paiement sont indiquées directement<br />
sur <strong>la</strong> page web lors <strong>de</strong> l'enregistrement.<br />
10
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Preise gültig bei Zahlung bis 1. August - Prix va<strong>la</strong>ble pour <strong>de</strong>s paiements avant le 1er août<br />
Kategorie - Catégorie<br />
EUR<br />
Mitglie<strong>de</strong>r von SPG, ÖPG, SGAA, ÖGAA - Membres <strong>de</strong> <strong>la</strong> SSP ÖPG, SSAA, ÖGAA 90.-<br />
Doktoran<strong>de</strong>n, die in einer <strong>de</strong>r obigen Gesellschaft Mitglied sind -<br />
70.-<br />
Doctorants qui sont membres d'une <strong>de</strong>s sociétés mentionnées ci-<strong>de</strong>ssus<br />
Doktoran<strong>de</strong>n, die NICHT Mitglied sind - Doctorants qui ne sont PAS membres 90.-<br />
Stu<strong>de</strong>nten VOR Master/Diplom Abschluß - Etudiants AVANT le <strong>de</strong>gré master/diplôme 30.-<br />
Plenar-/Einge<strong>la</strong><strong>de</strong>ne Sprecher, Preisträger - Conférenciers pléniers / invités, <strong>la</strong>uréats 0.-<br />
An<strong>de</strong>re Teilnehmer - Autres participants 120.-<br />
Konferenz Aben<strong>de</strong>ssen - Dîner <strong>de</strong> <strong>la</strong> conférence 70.-<br />
Zusch<strong>la</strong>g für Zahlungen nach <strong>de</strong>m 1. August sowie Barzahler an <strong>de</strong>r Tagung -<br />
20.-<br />
Supplément pour paiements effectués après le 1er août et pour paiements en espèces à <strong>la</strong> conférence<br />
Am Tagungssekretariat kann nur bar bezahlt wer<strong>de</strong>n (in<br />
EUR). Kreditkarten können lei<strong>de</strong>r nicht akzeptiert wer<strong>de</strong>n.<br />
ACHTUNG: Tagungsgebühren können nicht zurückerstattet<br />
wer<strong>de</strong>n.<br />
Kaffeepausen, Mittagessen<br />
Die Kaffeepausen und die zur Postersitzung gehören<strong>de</strong>n<br />
Apéros fin<strong>de</strong>n in <strong>de</strong>r Halle bei Händlerausstellung statt.<br />
Diese Leistungen sind in <strong>de</strong>r Konferenzgebühr enthalten.<br />
Die Mensen auf <strong>de</strong>m Campus sowie umliegen<strong>de</strong> Restaurants<br />
stehen zum Mittagessen zur Verfügung.<br />
Konferenz-Aben<strong>de</strong>ssen<br />
Das Aben<strong>de</strong>ssen fin<strong>de</strong>t am Donnerstag im Anschluß an<br />
die Postersession statt. Der Preis beträgt EUR 70.- pro<br />
Person (beinhaltet Transfer, Menü und Getränke) Bitte<br />
registrieren Sie sich unbedingt im Voraus, damit wir<br />
disponieren können. Eine Anmeldung vor Ort ist nicht<br />
möglich !<br />
Hotels und Anreise<br />
Alle Informationen fin<strong>de</strong>n Sie auf <strong>de</strong>r Konferenzwebseite:<br />
www.jku.at/hfp/oepgsps13<br />
Les paiements lors <strong>de</strong> <strong>la</strong> conférence ne pourront être<br />
effectués qu'en espèces (EUR). Les cartes <strong>de</strong> crédit ne<br />
pourront malheureusement pas être acceptées.<br />
ATTENTION: Les frais d'inscription ne pourront pas être<br />
remboursés.<br />
Pauses café, repas <strong>de</strong> midi<br />
Les pauses café, et les apéros pendant <strong>la</strong> séance posters<br />
se dérouleront dans le hall près <strong>de</strong>s exposants. Ces<br />
prestations sont inclues dans les frais d'inscription.<br />
Les restaurants du campus ainsi que <strong>de</strong>s restaurants<br />
autour <strong>de</strong> l'université sont disponible pour les repas <strong>de</strong><br />
midi.<br />
Dîner <strong>de</strong> <strong>la</strong> conférence<br />
Le dîner se tiendra le jeudi soir après <strong>la</strong> séance posters.<br />
Le prix est <strong>de</strong> EUR 70.- par personne (transfert, repas et<br />
boissons inclus). Veuillez s.v.p. absolument vous enregistrer<br />
d'avance pour <strong>de</strong>s raisons d'organisation. Il n'est<br />
plus possible <strong>de</strong> s'inscrire sur p<strong>la</strong>ce.<br />
Hôtels et Arrivée<br />
Tous les informations se trouvent sur le site web <strong>de</strong> <strong>la</strong><br />
conférence: www.jku.at/hfp/oepgsps13<br />
Neuer MANTIS Kontakt für<br />
die Schweiz und Österreich<br />
Das britische Unternehmen Mantis Deposition Ltd.<br />
ist seit <strong>de</strong>m 1. Oktober 2012 in Deutsch<strong>la</strong>nd mit<br />
einer eigenen Nie<strong>de</strong>r<strong>la</strong>ssung in Mainz vertreten, die<br />
für die Betreuung <strong>de</strong>r Kun<strong>de</strong>n in Deutsch<strong>la</strong>nd,<br />
Österreich und <strong>de</strong>r Schweiz zuständig ist.<br />
Mantis wur<strong>de</strong> im Jahre 2003 in Oxford von<br />
Wissenschaftlern mit Erfahrung in <strong>de</strong>n Bereichen<br />
Nanotechnologie sowie Mess-und<br />
Dünnschichttechnik gegrün<strong>de</strong>t. Ein Team von<br />
erfahrenen und hochqualifizierten Mitarbeitern trägt<br />
in Entwicklung, Produktion, Beratung, Instal<strong>la</strong>tion<br />
und Service zum Erfolg <strong>de</strong>s Unternehmens bei.<br />
Heute steht das Unternehmen für die Herstellung<br />
qualitativ hochwertiger Beschichtungskomponenten<br />
und Vakuumabschei<strong>de</strong>an<strong>la</strong>gen. Die Produkte<br />
wer<strong>de</strong>n sowohl in <strong>de</strong>r innovativen<br />
Materialforschung (Nanobeschichtungen,<br />
Moleku<strong>la</strong>rstrahlexpitaxie, Sputterprozessen uvm.)<br />
als auch in Pilot-Produktionsbeschichtungsan<strong>la</strong>gen<br />
mit Erfolg eingesetzt und stehen an <strong>de</strong>r Spitze <strong>de</strong>r<br />
Dünnschicht-Beschichtungstechnologie. Die Firma hat<br />
in kürzester Zeit mehr als 60 komplette An<strong>la</strong>gen<br />
weltweit verkauft.<br />
Neben universellen Standard Beschichtungssystemen<br />
wer<strong>de</strong>n auch An<strong>la</strong>gen nach Kun<strong>de</strong>nspezifikationen<br />
angeboten. Als beson<strong>de</strong>re Dienstleistung wird ein<br />
Entwicklungsbeschichtungsservice unter Verwendung<br />
<strong>de</strong>r eigenen Nanopartikel- Abscheidungsquelle<br />
angeboten.<br />
Mantis Deposition GmbH<br />
Alte Fahrkartendruckerei<br />
Mombacher Straße 52<br />
55122 Mainz<br />
Deutsch<strong>la</strong>nd<br />
Tel: +49(0)6131-3272520<br />
OfficeDE@mantis<strong>de</strong>position.com<br />
www.mantis<strong>de</strong>position.<strong>de</strong><br />
11
SPG Mitteilungen Nr. 40<br />
Vorläufige Programmübersicht - Résumé préliminaire du programme<br />
Das vollständige Programm wird allen Teilnehmern am Tagungssekretariat<br />
abgegeben sowie auf <strong>de</strong>r SPG-Webseite<br />
publiziert.<br />
Hinweise:<br />
- Je Beitrag wird nur <strong>de</strong>r präsentieren<strong>de</strong> Autor aufgeführt.<br />
- Die Postersitzung ist am Mittwoch und Donnerstag<br />
von 18:30 - ca. 20:00 (mit Apéro) sowie am Freitag von<br />
12:00 - 13:30.<br />
- (p) = Plenarsprecher, (i) = einge<strong>la</strong><strong>de</strong>ner Sprecher<br />
Special: Energy Day 2013<br />
Tuesday, 03.09.2013, HS 1<br />
Le programme final complet sera distribué aux participants<br />
au stand du secrétariat <strong>de</strong> <strong>la</strong> conférence et sera publié sur<br />
le site <strong>de</strong> <strong>la</strong> SSP.<br />
Indication:<br />
- seul le nom <strong>de</strong> l’auteur présentant <strong>la</strong> contribution a été<br />
indiqué.<br />
- <strong>la</strong> session poster a lieu le mercredi et jeudi <strong>de</strong> 18.30 à<br />
env. 20.00 (avec apéro) ainsi que le vendredi <strong>de</strong> 12:00<br />
à 13:30.<br />
- (p) = orateur <strong>de</strong> <strong>la</strong> session plénière, (i) = orateur invité<br />
Special: Thermoelectrics<br />
Tuesday, 03.09.2013, HS 4<br />
Time ID Energy Day<br />
Chair: Werner Spitzl<br />
10:00 21 Energiespeicherung: Das Vorwort zum Energietag<br />
2013<br />
Norbert Pillmayr<br />
10:15 22 Zukünftiges Energiesystem benötigt neue Lösungsansätze<br />
beson<strong>de</strong>rs bei <strong>de</strong>r Speicherung<br />
Horst Steinmüller<br />
10:45 23 Herausfor<strong>de</strong>rungen für <strong>de</strong>n Betrieb <strong>de</strong>s kontinentaleuropäischen<br />
Verbundnetzes<br />
Martin Geidl<br />
11:15 Coffee Break<br />
11:30 24 Smart Grid und das Hauskraftwerk<br />
Michael Zahradnik<br />
12:00 25 Wieviel erneuerbare Energie muss zukünftig gespeichert<br />
wer<strong>de</strong>n? Analyse <strong>de</strong>s zukünftigen<br />
Speicherbedarfs in Österreich mit einem hohen Anteil<br />
an erneuerbarer Energie.<br />
Gerfried Jungmeier<br />
12:30 Diskussion<br />
12:45 Lunch<br />
Chair: Brigitte Pagana-Hammer<br />
13:30 26 Technologische und Ökonomische Aspekte <strong>de</strong>r<br />
Elektrochemischen Energiespeicherung<br />
Stefan Koller<br />
14:00 27 Wasserstoffspeicherung durch Magnesiumhydrid<br />
Iris Bergmair<br />
14:30 28 Superconducting Magnetic Energy Storage<br />
Bartlomiej A. Glowacki<br />
15:00 29 Die Lithium-Ionen Batterie – von <strong>de</strong>r Knopfzelle zur<br />
Traktionsbatterie<br />
Michael Sternad<br />
15:30 Diskussion<br />
15:50 Schlußbemerkungen<br />
Norbert Pillmayr<br />
16:00 END<br />
18:00 RECEPTION<br />
19:00 Official Opening of the Joint Annual Meeting of<br />
ÖPG, SPS, ÖGAA and SSAA<br />
Public Lecture<br />
Chair: Günther Bauer, JKU Linz<br />
19:15 11 Using Nanostructures toward Achieving Energy<br />
Sustainability<br />
Mildred Dresselhaus, MIT (p)<br />
20:30 END<br />
Time ID Thermoelectrics<br />
Chair: Armando Rastelli, JKU Linz<br />
15:15 31 From Superconductivity Towards Thermoelectricity:<br />
Germanium Based Skutterudites<br />
E. Bauer (i)<br />
15:45 32 Half-Heusler compounds for thermoelectricity<br />
Sascha Populoh<br />
16:00 Coffee Break<br />
16:30 33 Seebeck Effect in the Kondo Insu<strong>la</strong>tor CeRu 4<br />
Sn 6<br />
un<strong>de</strong>r<br />
Magnetic Field<br />
Valentina Martelli<br />
16:45 34 Seebeck-effect in organic semiconductors<br />
Kristin Wil<strong>la</strong><br />
17:00 35 Crucial role of surface-segregation-driven intermixing<br />
on the thermal transport through p<strong>la</strong>nar Ge/Si<br />
super<strong>la</strong>ttices<br />
Peixuan Chen<br />
17:15 36 X-ray characterization of Si/Ge thermoelectric<br />
structures<br />
Tanja Etzelstorfer<br />
17:30 37 Intermetallic transition metal c<strong>la</strong>thrates<br />
Andrey Prokofiev<br />
17:45 END<br />
ID<br />
Thermoelectrics Poster<br />
41 Influence of process variables of ball milling and hot pressing<br />
on the thermoelectric performance of type I c<strong>la</strong>thrates<br />
Xinlin Yan<br />
42 Development of a Measuring P<strong>la</strong>tform for Thermoelectric<br />
Properties of Nanowires<br />
Günther Lientschnig<br />
43 Thermoelectric properties of melt-spun SPS sintered type-<br />
VIII Ba 8<br />
Ga 16<br />
Sn 30-x<br />
Ge x<br />
c<strong>la</strong>thrates<br />
Petr Tomes<br />
44 Experimental setup and sample processing for direct measurements<br />
of the cross-p<strong>la</strong>ne Seebeck coefficient of nanostructured<br />
Si/Ge materials<br />
Lukas Nausner<br />
45 Melt spinning of CoSb 3<br />
: e ect<br />
of microstructure on phonon<br />
thermal conductivity<br />
Matthias Ikeda<br />
46 Thermoelectric properties of the anisotropic Kondo insu<strong>la</strong>tor<br />
CeRu 4<br />
Sn 6<br />
Jonathan Haenel<br />
47 Resonant scattering induced thermopower peak in one dimensional<br />
disor<strong>de</strong>red systems<br />
Daniel Müller<br />
12
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Special: Photovoltaics<br />
Tuesday, 03.09.2013, HS 5<br />
Time ID Photovoltaics<br />
Chair: Markus C<strong>la</strong>rk Scharber, JKU Linz<br />
14:45 51 Theory of light-harvesting in photosynthesis: From<br />
structure to function<br />
Thomas Renger<br />
15:15 52 Artificial Photosynthesis for the Storage of Chemical<br />
Energy<br />
Kerstin Oppelt<br />
15:30 53 Ultrathin, lightweight, and flexible organic so<strong>la</strong>r<br />
cells<br />
Matthew White<br />
15:45 54 Colloidal Quantum dot photovoltaics: Tuning optoelectronic<br />
properties<br />
Philipp Stadler<br />
16:00 Coffee Break<br />
16:30 55 Organic nanocrystals from <strong>la</strong>tent pigments for environmentally-friendly<br />
and biocompatible electronics<br />
Mykhailo Sytnyk<br />
16:45 56 Metal sulfi<strong>de</strong> nanoparticle/polymer hybrid so<strong>la</strong>r<br />
cells<br />
Gregor Trimmel<br />
17:00 57 Flexible Monograin Membrane Photovoltaic Membranes<br />
Axel Neisser<br />
17:15 58 15 years of research on organic so<strong>la</strong>r cells: lessons<br />
learned from 1 % to 10 % efficiency<br />
Christoph J. Brabec (i)<br />
18:00 END<br />
Plenary Session<br />
Wednesday, 04.09.2013, HS 1<br />
Time ID Plenary Session I<br />
Chair: NN<br />
08:55 Welcome note<br />
09:00 1 P<strong>la</strong>smons, forces and currents in atomic and molecu<strong>la</strong>r<br />
contacts<br />
Richard Berndt, Uni Kiel (p)<br />
09:40 2 Quantum simu<strong>la</strong>tion with Atoms, Ions and Molecules<br />
Peter Zoller, Uni Innsbruck (p)<br />
10:20 Coffee Break<br />
Chair: NN<br />
10:50 3 The Quantum Way of Doing Computations<br />
Rainer B<strong>la</strong>tt, Uni Innsbruck (p)<br />
11:30 Award Ceremony<br />
12:30 Lunch<br />
13:30 Topical Sessions<br />
18:30 Postersession and Apéro<br />
Public Lecture<br />
Chair: Rainer B<strong>la</strong>tt, Uni Innsbruck<br />
20:00 12 Manipu<strong>la</strong>tion of single quantum systems<br />
Serge Haroche, Collège <strong>de</strong> France (p)<br />
21:15 END<br />
Thursday, 05.09.2013, HS 1<br />
Time ID Plenary Session II<br />
Chair: NN<br />
09:00 4 100 years Bohr's Atomic Mo<strong>de</strong>l: Its birth and its importance<br />
in the rise of QM<br />
Jan Lacki, Uni Genève (p)<br />
09:40 5 Exop<strong>la</strong>nets and their atmospheres<br />
Lisa Kaltenegger, MPI Hei<strong>de</strong>lberg (p)<br />
10:20 Coffee Break<br />
Chair: NN<br />
10:50 6 GEO: Using Earth observation for Integrated Water<br />
Resources Management<br />
Doug<strong>la</strong>s Cripe, GEOSS Genève (p)<br />
11:30 16 Winner of the ÖPG Boltzmann Award<br />
12:00 General Assemblies<br />
12:30 Lunch<br />
13:30 Topical Sessions<br />
18:30 Postersession (continued)<br />
20:00 Conference Dinner<br />
Friday, 06.09.2013, HS 1<br />
Time ID Plenary Session III<br />
Chair: NN<br />
09:00 7 LHC - The first three years<br />
Rainer Wallny, ETH Zürich (p)<br />
09:40 8 Quantum phase transitions in con<strong>de</strong>nsed matter<br />
Silke Bühler-Paschen, TU Wien (p)<br />
10:20 Coffee Break<br />
Chair: Georg Pabst, Uni Graz<br />
10:50 9 Theoretical Insights into Structure of Animal Tissues<br />
Primoz Ziherl, Uni Ljubljana (p)<br />
11:30 17 Winner of the SPS ABB Award<br />
12:00 Best Poster Awards<br />
12:15 Postersession (continued), Lunch<br />
13:30 Topical Sessions<br />
15:30 END<br />
Careers for Physicists<br />
Thursday, 05.09.2013, K001A<br />
Time ID Careers for Physicists<br />
Chair: Kai Hencken, ABB Ba<strong>de</strong>n<br />
14:00 71 "Advanced Manufacturing", ein interessantes Feld<br />
für Physikerinnen und Physiker?<br />
Bernhard Braunecker (i)<br />
14:30 72 What does a physicist do at ETH Zürich if he is not<br />
in research?<br />
Bernd Rinn (i)<br />
15:00 73 On the Cutting Edge: Publication Dynamics and the<br />
Society of Scientific Journals<br />
Istvan Daruka<br />
15:30 Coffee Break<br />
13
SPG Mitteilungen Nr. 40<br />
16:00 74 A new generation of Physicists<br />
Stefano Verginelli (i)<br />
16:30 75 Workshop: Wie? Mit Physik Karriere machen?<br />
Josef Siess (i)<br />
17:00 END<br />
18:30 Postersession and Apéro<br />
20:00 Conference Dinner<br />
Physik und Schule<br />
Wednesday, 04.09.2013, K269D<br />
Time ID Physik und Schule<br />
Chair: Engelbert Stütz, JKU Linz<br />
13:15 81 Sexl-Preisträger: Preisvortrag 1<br />
13:35 82 Sexl-Preisträger: Preisvortrag 2<br />
14:00 83 Hat Aristoteles doch recht?<br />
Siegfried Bauer (i)<br />
Prämierte Fachbereichsarbeiten<br />
Chair: Leopold Mathelitsch, Uni Graz<br />
15:00 84 Introduction to Rutherford Backscattering Spectrometry<br />
(RBS)<br />
Maximilian Heinz Ruep<br />
15:15 85 Schwerelosigkeit und Mikrogravitation<br />
Bianca Neureiter<br />
15:30 Coffee Break<br />
16:00 86 Stringtheorie; Grundgedanken und ihr Einfluss auf<br />
Teilchenphysik und Kosmologie<br />
Stefan Purkhart<br />
16:15 87 Bildsensorik. Physikalische und technische Grund<strong>la</strong>gen<br />
am Beispiel <strong>de</strong>s CCD<br />
Stefan Janisch<br />
Chair: Engelbert Stütz, JKU Linz<br />
16:30 88 Präsentation <strong>de</strong>s österreichischen Teams <strong>de</strong>s IYPT<br />
2013<br />
16:50 89 Präsentation <strong>de</strong>s österreichischen Teams <strong>de</strong>r IPhO<br />
2013<br />
17:10 Sitzung <strong>de</strong>s FA Physik und Schule<br />
18:00 ENDE<br />
18:30 Postersession and Apéro<br />
ID<br />
Physik und Schule Poster<br />
91 Construction, <strong>de</strong>velopment and tests of a cost-effective<br />
force p<strong>la</strong>tform<br />
Florian Rie<strong>de</strong>r<br />
92 Schülervorstellungen zum Thema Strahlung<br />
Martin Hopf<br />
93 Astrobiology as an Interdisciplinary Starting Point to Natural<br />
Sciences<br />
Johannes Leitner<br />
94 Let`s P<strong>la</strong>y Physics! Making physics education physically - A<br />
project on the transit of the venus<br />
Christina Rothenhäusler<br />
95 Nanophysik am Beispiel eines Rastertunnelmikroskops in<br />
<strong>de</strong>r Schule<br />
Thomas Möst<br />
96 Professionswissen Physiklehramtsstudieren<strong>de</strong>r in Österreich<br />
Ingrid Krumphals<br />
KOND<br />
Wednesday, 04.09.2013, HS 5<br />
Time ID Magnetism, Superconductivity<br />
and Quantum Criticality<br />
Chair: Silke Bühler-Paschen, TU Wien<br />
13:30 101 Superconductivity in Materials without Inversion<br />
Symmetry<br />
Ernst Bauer (i)<br />
14:00 102 Quantum criticality of the heavy-fermion compound<br />
CeCoGe 2.2<br />
Si 0.8<br />
Julio Larrea<br />
14:15 103 Strong Pressure Depen<strong>de</strong>nce of the Magnetic<br />
Penetration Depth in Single Crystals of the Heavy-<br />
Fermion Superconductor CeCoIn 5<br />
Studied by Muon<br />
Spin Rotation<br />
Ludovic Howald<br />
14:30 104 Electric and magnetic coupling of quantum-critical<br />
materials to a microwave cop<strong>la</strong>nar wavegui<strong>de</strong> resonator<br />
at milli-Kelvin temperatures<br />
Diana Geiger<br />
14:45 105 Superconductivity and Quantum Criticality<br />
Johan Chang (i)<br />
15:15 106 About the origin of frustration in the magnetismdriven<br />
multiferroic YBaCuFeO 5<br />
Marisa Medar<strong>de</strong><br />
15:30 Coffee Break<br />
Neutrons and Synchrotron Radiation<br />
for Con<strong>de</strong>nsed Matter<br />
Chair: Oskar Paris, Uni Leoben<br />
16:00 111 X-ray absorption spectroscopy for element selective<br />
investigations of structure, valence and magnetism<br />
in doped oxi<strong>de</strong>s<br />
Andreas Ney (i)<br />
16:30 112 Growing semiconductor nitri<strong>de</strong>s into spintronic and<br />
magnetooptic materials<br />
Alberta Bonanni<br />
16:45 113 X-ray strain microscopy of inhomogoenously<br />
strained Ge micro-bridges<br />
Tanja Etzelstorfer<br />
17:00 114 A New Crystalline Phase of Gallium Phosphi<strong>de</strong>:<br />
Wurtzite Nanowires Investigated by X-ray Diffraction<br />
Dominik Kriegner<br />
17:15 115 In-situ synchrotron SAXS studies on Colloidal Nanocrystal<br />
Formation<br />
Rainer T. Lechner<br />
17:30 116 In-situ and ex-situ study of mesostructured silica<br />
synthesized in the gas phase<br />
Barbara Sartori<br />
17:45 117 Humidity Driven Pore-Lattice Deformation in Or<strong>de</strong>red<br />
Mesoporous Thin Films<br />
Parvin Sharifi<br />
18:00 118 Radiation assisted material synthesis and processing<br />
by <strong>de</strong>ep X-ray lithography<br />
Bene<strong>de</strong>tta Marmiroli<br />
18:15 119 Novel insights into photoemission from solids: Surface<br />
RABBITT yields absolute <strong>de</strong><strong>la</strong>ys and reveals<br />
temporal structure beyond transport phenomena.<br />
Luca Castiglioni<br />
18:30 Postersession and Apéro<br />
20:00 Public Lecture<br />
14
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Thursday, 05.09.2013, HS 5<br />
Friday, 06.09.2013, HS 5<br />
Time ID Soft Matter and Other Systems I<br />
(Shared with the Biophysics session)<br />
Chair: Georg Pabst, Uni Graz<br />
13:30 121 Equilibrium and flow of cluster-forming complex<br />
fluids<br />
Christos N. Likos (i)<br />
14:00 122 Optimized Fourier Monte Carlo Simu<strong>la</strong>tion of Solid<br />
and Hexatic Membranes<br />
Andreas Troester<br />
14:15 123 Biomimetic folding particle chains<br />
Peter Oostrum<br />
Soft Matter and Other Systems II<br />
Chair: Oskar Paris, Uni Leoben<br />
14:30 124 Small Angle Scattering Study of the self-assembly<br />
of an amphiphilic <strong>de</strong>signer pepti<strong>de</strong> from the monomer<br />
to a helical superstructure<br />
Heinz Amenitsch<br />
14:45 125 Liquid Structure and the Noncoinci<strong>de</strong>nce Effect of<br />
Liquid Dimethyl Sulfoxi<strong>de</strong> Revisited<br />
Maurizio Musso<br />
15:00 126 Generation of multiply twinned Ag clusters (n
SPG Mitteilungen Nr. 40<br />
Surfaces, Interfaces and Thin Films<br />
Wednesday, 04.09.2013, HS 1<br />
Time ID Surfaces + organic thin films<br />
Chair: Christian Teichert, Uni Leoben<br />
13:30 201 Iso<strong>la</strong>ted Pd Sites on PdGa Mo<strong>de</strong>l Catalyst Surfaces<br />
Jan Prinz<br />
13:45 202 Metal clusters and simple adsorbates on ultra-thin<br />
ZrO 2<br />
/Pt 3<br />
Zr<br />
Joong Il J. Choi<br />
14:00 203 Mechanics of single molecules<br />
Ernst Meyer (i)<br />
14:30 204 Initial steps of indigo film growth on silicon dioxi<strong>de</strong><br />
Boris Scherwitzl<br />
14:45 205 Tuning the 1D-self-assembly of dicyano-functionalized<br />
helicene building-blocks<br />
Aneliia Shchyrba<br />
15:00 206 Using po<strong>la</strong>rized light in PEEM<br />
Thorsten Wagner<br />
15:15 207 Substrate enhanced intermolecu<strong>la</strong>r dispersion:<br />
Pentacene on Cu(110)<br />
Thomas Ules<br />
15:30 Coffee Break<br />
Theory + clusters<br />
Chair: Ernst Meyer, Uni Basel<br />
16:00 211 Ohmic contacts for resistance measurements of<br />
ultra-thin metal-on-silicon <strong>la</strong>yers<br />
Bernhard Lutzer<br />
16:15 212 Electrical and Physical Characterization of Interfacial<br />
Germanates in Ge-based MOS <strong>de</strong>vices<br />
Ole Bethge<br />
16:30 213 Numerical Simu<strong>la</strong>tions of a Capil<strong>la</strong>rity Driven Morphological<br />
Transition on the Nanoscale<br />
Istvan Daruka<br />
16:45 214 Reflectance Anisotropy spectrum of water covered<br />
Cu(110) surface studied from first principles<br />
Amirreza Baghbanpourasl<br />
17:00 215 Organic Semiconductors Interfaces Explored With<br />
Ab-initio Electronic Structure Methods<br />
Peter Puschnig (i)<br />
17:30 216 Solid-solid interfaces in metal oxi<strong>de</strong> nanoparticle<br />
ensembles<br />
Oliver Diwald<br />
17:45 217 Single gold nanoparticles as nanoscopic pH-sensors<br />
Cynthia Vidal<br />
18:00 218 Efficient random <strong>la</strong>sing from star-shaped nanoparticles<br />
Johannes Ziegler<br />
18:15 219 Growth of in-p<strong>la</strong>ne SiGe nanowires<br />
Hannes Watzinger<br />
18:30 Postersession and Apéro<br />
20:00 Public Lecture<br />
Thursday, 05.09.2013, HS 1<br />
Time ID Metho<strong>de</strong>s<br />
Chair: Peter Zeppenfeld, Uni Linz<br />
13:30 221 On-surface magnetochemistry: controlling spins in<br />
adsorbed molecules by a chemical switch<br />
Christian Wäckerlin (i)<br />
14:00 222 Electronic and Magnetic Properties of Surface-<br />
Supported Hydrocarbon Radicals Studied by Low-<br />
Temperature Scanning Tunneling Microscopy<br />
Stefan Müllegger<br />
14:15 223 Using AFM nanoin<strong>de</strong>ntation to investigate mechanical<br />
properties of cellulose fibers in controlled humidities<br />
Christian Ganser<br />
14:30 224 Helium Atom Scattering Measurements of the<br />
Sb(111) Surface<br />
Markus Po<strong>la</strong>nz<br />
14:45 225 Formation of HCN + in Heterogeneous Reactions of<br />
N 2+ and N + with Surface Hydrocarbons<br />
Martina Harnisch<br />
15:00 226 Hydrogen Induced Buckling of Gold Films<br />
Baran Eren<br />
15:15 ÖPG-OGD Division Meeting<br />
15:30 Coffee Break<br />
Oxi<strong>de</strong>s<br />
Chair: Ulrike Diebold, TU Wien<br />
16:00 231 Growth and Morphology of Epitaxial MgO Films on<br />
GaAs(001)<br />
Anirban Sarkar<br />
16:15 232 Compositional and structural study of homoepitaxial-STO<br />
based oxi<strong>de</strong>s heterostructures<br />
Mathil<strong>de</strong> L. Reinle-Schmitt<br />
16:30 233 Single Metal Adatoms on Fe 3<br />
O 4<br />
(001)-(√2x√2)R45°<br />
Gareth Parkinson (i)<br />
17:00 234 Water Gas Shift Chemistry at the Fe 3<br />
O 4<br />
(001) Surface<br />
Oscar Gamba<br />
17:15 235 STM and photoemission study of vacancies and hydroxyls<br />
at the SrTiO 3<br />
(110)-(4×1) surface<br />
Stefan Gerhold<br />
17:30 236 Interface Fermi states of LaAlO 3<br />
/SrTiO 3<br />
and re<strong>la</strong>ted<br />
heterostructures<br />
C<strong>la</strong>udia Cancellieri (i)<br />
18:00 237 Combined Spectroscopic Study of the Evolution<br />
from the Metallic Surface State on SrTiO 3<br />
to the Interface<br />
of LaAlO 3<br />
/SrTiO 3<br />
Nicho<strong>la</strong>s Plumb<br />
18:15 238 Field-induced migration of oxygen vacancies towards<br />
the surface of TiO 2<br />
anatase(101)<br />
Martin Setvin<br />
18:30 Postersession and Apéro<br />
20:00 Conference Dinner<br />
Friday, 06.09.2013, HS 1<br />
Time ID Graphene + flexible electronics<br />
Chair: Adolf Winkler, TU Graz<br />
13:30 241 Observing Graphene grow: In-situ metrology for<br />
controlled growth of graphene and carbon nanotubes<br />
Bernhard Bayer<br />
13:45 242 Optical characterization of atomically precise<br />
graphene nanoribbons<br />
Richard Denk<br />
14:00 243 Electronic Structure of Atomically Precise Graphene<br />
Nanoribbons<br />
Pascal Ruffieux<br />
14:15 244 Modification of exfoliated graphene: a case study<br />
Markus Kratzer (i)<br />
16
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
14:45 245 In-situ thin film transistor fabrication: Electrical and<br />
surface analytical characterization<br />
Roman Lassnig<br />
15:00 246 Valve metal anodic oxi<strong>de</strong>s for flexible electronics<br />
Andrei Ionut Mardare<br />
15:15 247 Direct writing of high-k metal oxi<strong>de</strong> dielectrics for<br />
flexible <strong>la</strong>rge area electronics<br />
Christian M. Siket<br />
15:30 END<br />
ID Surfaces, Interfaces and Thin Films Poster<br />
251 Stabilization mechanisms at po<strong>la</strong>r ZnO surfaces in i<strong>de</strong>al<br />
vacuum conditions: a SCC-DFTB study<br />
Stefan Huber<br />
252 Shockley Surface States Revisited: A Comprehensive Density<br />
Functional Study<br />
Bernd Kollmann<br />
253 Molecule-Substrate Hybridization Revealed by Angle-Resolved<br />
Photoemission Spectroscopy<br />
Dario Knebl<br />
254 Initial growth of quinacridone on Ag(111)<br />
Thorsten Wagner<br />
255 Adsorption of quinacridone on Cu(110) and Cu(110)-(2x1)O<br />
surfaces<br />
Harald Zaglmayr<br />
256 Attachment-limited nucleation and growth of organic films:<br />
Pentacene on sputter modified mica (001)<br />
Levent Tümbek<br />
257 Interfacial structure and <strong>de</strong>vice efficiency of an organic bi<strong>la</strong>yer<br />
heterojunction so<strong>la</strong>r cell<br />
Michael Zawodzki<br />
258 Adsorption of pentacene and perfluoro-pentacene on<br />
Cu(110) studied by reflectance difference spectroscopy<br />
Johannes Gall<br />
259 Influences of rippled titania surfaces on to the growth morphologies<br />
of 6P thin films<br />
Reinhold Wartbichler<br />
260 Hydrogen adsorption on TiO 2<br />
anatase(101)<br />
Benjamin Daniel<br />
261 Optical properties of metal doped ZnO thin films on g<strong>la</strong>ss<br />
and polymer substrates<br />
Meirzhan Dosmailov<br />
262 Negative muonium as a local probe for the <strong>de</strong>tection of the<br />
photo-induced inversion of a Ge surface <strong>la</strong>yer<br />
Thomas Prokscha<br />
263 Short-Term Metastable Effects in Amorphous Silicon So<strong>la</strong>r<br />
Modules<br />
Ankit Mittal<br />
264 Oxi<strong>de</strong> diffusion barriers on GaAs(001)<br />
Shibo Wang<br />
265 Formation of Tungsten Oxi<strong>de</strong> Nano<strong>la</strong>yers by (WO 3<br />
) 3<br />
Cluster<br />
Con<strong>de</strong>nsation on Ag(100)<br />
Thomas Obermüller<br />
266 Influence of the Ni content in AlCu alloy using the combinatorial<br />
approach.<br />
Martina Hafner<br />
267 Susceptibility measurements of Ni clusters embed<strong>de</strong>d in<br />
organic matrices<br />
Mariel<strong>la</strong> Denk<br />
268 Investigation of Single Ni Adatoms on the Magnetite (001)<br />
Surface<br />
Ro<strong>la</strong>nd Bliem<br />
269 Investigation of Exchange Coupled Composites with Scanning<br />
Transmission X-ray Microscopy<br />
Phillip Wohlhüter<br />
270 Spin resolved photoemission spectroscopy of Fe 3<br />
O 4<br />
: The<br />
effect of surface structure<br />
Jiri Pavelec<br />
271 Charge behavior on insu<strong>la</strong>ting monocrystallic surfaces by<br />
Kelvin probe force microscopy<br />
Monika Mirkowska<br />
272 Stabilization of explosive compounds on metallic surfaces<br />
Stefan Ralser<br />
273 Characterizations of HOPG and Graphene Treated with Low<br />
Temperature Hydrogen P<strong>la</strong>sma<br />
Baran Eren<br />
274 Characterization of thin two-element compound material<br />
films by time-of-flight Low Energy Ion Scattering<br />
Dietmar Roth<br />
275 Indication of phonon-assisted electron-hole re<strong>la</strong>xations on<br />
Sb(111) and Bi(111) in iHAS measurements<br />
Patrick Kraus<br />
276 Determination of atmospheric corrosion of coated steel<br />
surfaces by in situ infrared reflection absorption spectroscopy<br />
(IRRAS)<br />
Maurizio Musso<br />
277 Al-Si thin films for hydrogen reference materials<br />
Cezarina Ce<strong>la</strong> Mardare<br />
Nuclear, Particle- and Astroparticle Physics<br />
Wednesday, 04.09.2013, HS 6<br />
Time ID I: LHC Physics I<br />
Chair: Martin Pohl, Uni Genève<br />
13:30 301 Search for a Higgs-like Boson <strong>de</strong>caying into bottom<br />
quarks<br />
Philipp Eller<br />
13:45 302 Search for long lived charged and massive particles<br />
at LHCb <strong>de</strong>tector<br />
Thi Viet Nga La<br />
14:00 303 Measurement of differential iso<strong>la</strong>ted diphoton production<br />
cross section at CMS<br />
Marco Peruzzi<br />
14:15 304 Search for Higgs boson production in supersymmetric<br />
casca<strong>de</strong>s using fully hadronic final states<br />
Mario Masciovecchio<br />
14:30 305 Search for supersymmetry in hadronic final states<br />
with MT2 at CMS<br />
Hannsjörg Weber<br />
14:45 306 Search for supersymmetry in events with two opposite-sign<br />
same-f<strong>la</strong>vor leptons, jets and missing<br />
energy<br />
Marco - Andrea Buchmann<br />
15:00 307 Application of CMS and ATLAS Simplified Mo<strong>de</strong>ls<br />
Results to Theories Beyond the Standard Mo<strong>de</strong>l<br />
(BSM)<br />
Ursu<strong>la</strong> Laa<br />
15:15 308 Measurement of quarkonium po<strong>la</strong>rization at CMS<br />
Valentin Knünz<br />
15:30 Coffee Break<br />
II: Astroparticle and Non-accelerator Physics<br />
Chair: Eberhard Widmann, ÖAW Wien<br />
16:00 311 Neutron Capture Measurements on 62 Ni, 63 Ni and<br />
197<br />
Au and their Relevance for Stel<strong>la</strong>r Nucleosynthesis<br />
C<strong>la</strong>udia Le<strong>de</strong>rer (i)<br />
17
SPG Mitteilungen Nr. 40<br />
16:30 312 Latest Results of Searches for Point and Exten<strong>de</strong>d<br />
Sources with Time In<strong>de</strong>pen<strong>de</strong>nt and Time Depen<strong>de</strong>nt<br />
emissions of Neutrinos with the IceCube Neutrino<br />
Observatory<br />
Asen Christov (i)<br />
17:00 313 High resolution 3D-simu<strong>la</strong>tions of ga<strong>la</strong>ctic cosmic<br />
ray propagation using GALPROP<br />
Michael Werner<br />
17:15 314 The cosmological constant puzzle: Vacuum energies<br />
from QCD to dark energy<br />
Steven Bass<br />
17:30 315 Numerical 3D-hydrodynamic mo<strong>de</strong>lling of colliding<br />
winds in massive star binaries: particle acceleration<br />
and gamma-ray emission<br />
K<strong>la</strong>us Reitberger<br />
17:45 316 High precision tests of the Pauli Exclusion Principle<br />
for Electrons at LNGS<br />
Johann Marton<br />
18:00 317 Search of neutrinoless double beta <strong>de</strong>cay with the<br />
GERDA experiment<br />
Giovanni Benato<br />
18:15 318 qBounce: A quantized frequency reference with<br />
gravity-resonance-spectroscopy<br />
Gunther Cronenberg<br />
18:30 Postersession and Apéro<br />
20:00 Public Lecture<br />
Thursday, 05.09.2013, HS 6<br />
Time ID III: Protons and Neutrons<br />
Chair: Johann Marton, ÖAW Wien<br />
13:30 321 Spectroscopy apparatus for the measurement of<br />
the hyperfine structure of antihydrogen<br />
Chloe Malbrunot (i)<br />
14:00 322 A progress report on <strong>de</strong>tector and analysis <strong>de</strong>velopment<br />
for the Hbar-HFS experiment within the<br />
ASACUSA col<strong>la</strong>boration<br />
Clemens Sauerzopf<br />
14:15 323 Beamline Simu<strong>la</strong>tions for cold Antihydrogens<br />
Berna<strong>de</strong>tte Kolbinger<br />
14:30 324 Gravitational interaction of antihydrogen: the AEgIS<br />
experiment at CERN<br />
Michael Doser<br />
14:45 325 Design of the downstream interface in the AEgIS<br />
beamline<br />
Sebastian Lehner<br />
15:00 326 Ultracold neutrons for fundamental physics experiments<br />
at the Paul Scherrer Institute<br />
Bernhard Lauss (i)<br />
15:30 Coffee Break<br />
IV: Protons and Neutrons, F<strong>la</strong>vor Physics<br />
Chair: Christoph Schwanda, ÖAW Wien<br />
16:00 331 Comparison of the Larmor precession frequencies<br />
of 199 Hg and ultracold neutrons in the nEDM experiment<br />
at PSI<br />
Beatrice Franke<br />
16:15 332 Vector Cesium Magnetometer for the nEDM Experiment<br />
Samer Afach<br />
16:30 333 The future neutron beta <strong>de</strong>cay facility PERC<br />
Jacqueline Erhart<br />
16:45 334 Tailoring of po<strong>la</strong>rised neutron beams by means of<br />
spatial magnetic spin resonance<br />
Erwin Jericha<br />
17:00 335<br />
PMNS<br />
F<strong>la</strong>vour GUT mo<strong>de</strong>ls with u 13<br />
= u C<br />
/ 2<br />
Constantin Sluka<br />
17:15 336 Angu<strong>la</strong>r analysis of B d<br />
" K*µ + µ - with the ATLAS <strong>de</strong>tector<br />
Emmerich Kneringer<br />
17:30 337 Measurement of B (B 0 " J/cf), B s (B0 " J/cf' (1525))<br />
s 2<br />
and B (B 0 " s J/cK+ K - ) and a <strong>de</strong>termination of the<br />
B 0 " J/cf po<strong>la</strong>rization at the Belle experiment<br />
s<br />
Felicitas Thorne<br />
17:45 338 Measurement of |V cb<br />
| through exclusive semileptonic<br />
B -> D l n <strong>de</strong>cays with a tagged fully reconstructed<br />
B meson at the Belle experiment<br />
Robin G<strong>la</strong>ttauer<br />
18:00 339 Monte Carlo simu<strong>la</strong>tion for Kaonic <strong>de</strong>uterium studies<br />
Carolina Berucci<br />
18:15<br />
18:30 Postersession and Apéro<br />
20:00 Conference Dinner<br />
Friday, 06.09.2013, HS 6<br />
Time ID V: LHC Physics II and Detectors<br />
Chair: Rainer Wallny, ETH Zürich<br />
13:30 341 Measurement of Charged Particle Multiplicities<br />
with the ATLAS <strong>de</strong>tector at the LHC<br />
Wolfgang Lukas<br />
13:45 342 Jet production in association with a Z boson at CMS<br />
Andrea Carlo Marini<br />
14:00 343 The Readout System of the Belle II Silicon Vertex<br />
Detector<br />
Richard Thalmeier<br />
14:15 344 Interstrip capacitance of double si<strong>de</strong>d silicon strip<br />
<strong>de</strong>tectors<br />
Bernhard Leitl<br />
14:30 345 Over Saturation Behaviour of SiPMs at High Photon<br />
Exposure<br />
Lukas Gruber<br />
14:45 346 FLUKA studies of hadron-irradiated scintil<strong>la</strong>ting<br />
crystals for calorimetry at the High-Luminosity LHC<br />
Milena Quittnat<br />
15:00 347 Studies of radiation hardness of diamond strip<br />
trackers.<br />
Felix Bachmair<br />
15:15 348 Irradiation Studies with the New Digital Readout<br />
Chip for the Phase I Upgra<strong>de</strong> of the CMS Pixel Detector<br />
Jan Hoss<br />
15:30 END<br />
ID Nuclear, Particle- and Astrophysics Poster<br />
351 Measurement of the thermal neutron flux at the source for<br />
ultracold neutrons at the Paul Scherrer Institute<br />
Dieter Ries<br />
352 An uncompensated magnetic field drifts in a search for an<br />
electric dipole moment of the neutron (nEDM) carrying out<br />
at Paul Scherrer Institute (PSI).<br />
N Prashanth Pataguppi<br />
353 High-volume production of Silicon strip <strong>de</strong>tectors for particle<br />
physics experiments<br />
Thomas Bergauer<br />
354 Bethe–Salpeter Description of Light Pseudosca<strong>la</strong>r Mesons<br />
Wolfgang Lucha<br />
355 Lock-in based <strong>de</strong>tection scheme for a hydrogen beam<br />
Michael Wolf<br />
356 Spin po<strong>la</strong>rized atomic hydrogen beam source<br />
Martin Diermaier<br />
18
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
357 A neutron interferometric measurement and calcu<strong>la</strong>tion of<br />
a phase shift induced by Laue transmission<br />
Thomas Potocar<br />
358 Development of a novel muon beam line for next generation<br />
precision experiments<br />
Kim Siang Khaw<br />
359 Measurements and simu<strong>la</strong>tions of magnetic field insi<strong>de</strong> the<br />
ASACUSA Antihydrogen spin-flip cavity<br />
Nazli Di<strong>la</strong>ver<br />
360 Neutron Reflectometry as Matura project - Verifying the<br />
Wave-Particle Dualism at the NARZISS Instrument at the<br />
Paul Scherrer Institut.<br />
Car<strong>la</strong> Kreis<br />
Theoretical Physics<br />
Wednesday, 04.09.2013, K034D<br />
Time ID Theoretical Physics I<br />
Chair: Jakob Yngvason, Uni Wien<br />
14:00 401 Lattice effects on vortex dynamics in strongly corre<strong>la</strong>ted<br />
electron systems<br />
Sebastian Huber (i)<br />
14:30 402 Strongly Interacting Dipo<strong>la</strong>r Quantum Gases<br />
Robert Zillich (i)<br />
15:00 403 On currents, anomalies and the RG-behaviour of<br />
supersymmetric gauge theories.<br />
Jean-Pierre Derendiger (i)<br />
15:30 Coffee Break<br />
16:00 404 Maximally entangled sets<br />
Barbara Kraus (i)<br />
16:30 405 Geometry as a Semic<strong>la</strong>ssical Effect in a Quantum<br />
World - Emergent gravity from matrix mo<strong>de</strong>ls<br />
Daniel B<strong>la</strong>schke<br />
16:45 406 Electrostatic Interactions with Dielectric Samples<br />
in Scanning Probe Microscopies<br />
Alexis Baratoff<br />
17:00<br />
18:30 Postersession and Apéro<br />
20:00 Public Lecture<br />
Thursday, 05.09.2013, K034D<br />
Time ID Theoretical Physics II<br />
Chair: Gian Michele Graf, ETH Zürich<br />
13:30 411 Exterior Navier-Stokes problems in two dimensions:<br />
results and open questions<br />
Peter Wittwer (i)<br />
14:00 412 Quantum many-body effects in transport through<br />
quantum dots: renormalization-group approaches<br />
Sabine An<strong>de</strong>rgassen (i)<br />
14:30 413 Atomic clocks: A mathematical physics perspective<br />
Martin Fraas (i)<br />
15:00 414 Non-local perturbations of hyperbolic PDEs and<br />
QFT mo<strong>de</strong>ls on non-commutative spacetimes<br />
Gandalf Lechner (i)<br />
15:30 Coffee Break; END<br />
Applied, P<strong>la</strong>sma and Geophysics<br />
Wednesday, 04.09.2013, K153C<br />
Time ID Applied Physics<br />
Chair: Ivo Furno, CRPP-EPFL<br />
13:30 451 Analysis of the Microscopic Fluid Flow of State-ofthe-art<br />
Absorption Heat Pump Working Pairs un<strong>de</strong>r<br />
Operational Conditions<br />
Johann Emhofer<br />
13:45 452 Entwicklung eines Kon<strong>de</strong>nsationswindkanals zur<br />
Untersuchung <strong>de</strong>s Wärme- und Massetransports<br />
an Wärmeüberträgern<br />
Sanda Seichter<br />
14:00 453 Precision Metrology with a Dio<strong>de</strong>-Pumped Solid-<br />
State Laser Optical Frequency Comb<br />
Stephane Schilt<br />
14:15 454 I<strong>de</strong>ntifying Photoreaction Products in Cinnamatebased<br />
Photoalignment Materials<br />
Daniele Passerone<br />
14:30 455 Experimental and simu<strong>la</strong>ted results on adsorption<br />
of molecules on fullerenes.<br />
Alexan<strong>de</strong>r Kaiser<br />
14:45 456 Dual-Comb Spectroscopy based on Mid-IR Quantum-Casca<strong>de</strong>-Lasers<br />
Frequency-combs<br />
Gustavo Vil<strong>la</strong>res<br />
15:00 457 Coinci<strong>de</strong>nce Time Resolution(CTR) of PMT and<br />
SiPM and readout components<br />
Albulena Berisha Shabani<br />
15:15<br />
15:30 Coffee Break<br />
Geohysics and Applied Physics<br />
Chair: Stéphane Goyette, Uni Genève<br />
16:00 461 Towards an integrated Observation System of the<br />
B<strong>la</strong>ck Sea catchment<br />
Nico<strong>la</strong>s Ray (i)<br />
16:30 462 Cs-137 in Wildpilzen in Österreich: Verteilung und<br />
zeitliche Trends<br />
Herbert Lettner<br />
16:45 463 Simu<strong>la</strong>tion of microwave propagation and absorption<br />
in heterogeneous rocks<br />
Ronald Meisels<br />
17:00 464 Calcu<strong>la</strong>tion of atom evaporation rates using entropy<br />
production maximisation<br />
Frank Kassubek<br />
P<strong>la</strong>sma Physics<br />
Chair: Ivo Furno, CRPP-EPFL<br />
17:15 465 Zeitaufgelöste schnelle Messungen von Wachstumsrate<br />
und Teilchentransport in HIPIMS-P<strong>la</strong>smen<br />
Christian Maszl<br />
17:30 466 P<strong>la</strong>sma fluctuations study in the new closed fluxsurfaces<br />
configuration of the TORPEX experiment<br />
Fabio Avino<br />
17:45 467 Simu<strong>la</strong>ting the effect of fine radial structures resulting<br />
from non-adiabatic passing electrons on turbulent<br />
transport in the ITG and TEM regimes<br />
J. Dominski<br />
18:00 468 Characterization of rf discharges in non-thermal atmospheric<br />
pressure p<strong>la</strong>sma jets using helium<br />
Johann Laimer<br />
18:15 END<br />
18:30 Postersession and Apéro<br />
20:00 Public Lecture<br />
19
SPG Mitteilungen Nr. 40<br />
ID<br />
Applied, P<strong>la</strong>sma and Geophysics Poster<br />
481 Simu<strong>la</strong>ted insertion loss of noise barriers using the boundary<br />
element method<br />
Holger Waubke<br />
482 In-line measurements of chlorine containing polymers in an<br />
industrial waste sorting p<strong>la</strong>nt by <strong>la</strong>ser-induced breakdown<br />
spectroscopy<br />
Norbert Huber<br />
483 Element analysis of complex materials by calibration-free<br />
<strong>la</strong>ser-induced breakdown spectroscopy<br />
Johannes D. Pedarnig<br />
484 Variable Capacitance Energy Harvesting<br />
Robert Pichler<br />
485 Photoluminescence enhancement of Double-Walled Carbon<br />
Nanotubes filled with linear carbon chains<br />
Philip Rohringer<br />
486 Inter-atomic Coulombic Decay (ICD) of clusters upon electron<br />
impact<br />
Elias Jabbour Al Maalouf<br />
487 The Inner Structure of Jupiter’s Moon Europa – Estimations<br />
on the Physical Conditions at the Sea Floor of its Potential<br />
Subsurface Ocean<br />
Susanne Pol<strong>la</strong>ck-Drs<br />
488 The evolution of hotspots on Earth and Venus<br />
Elisabeth Fahrngruber<br />
489 Comparing Characteristics of Polygonal Impact Craters on<br />
Mercury and Venus<br />
Gerhard Weihs<br />
490 Mo<strong>de</strong>ling the evolution and fate of early Mars' hypothesized<br />
ocean<br />
Gabor Imre Kiss<br />
Atomic Physics and Quantum Optics<br />
Wednesday, 04.09.2013, HS 4<br />
Time ID Atomic Physics and Quantum Optics I<br />
Chair: NN<br />
13:30 501 Measuring higher-or<strong>de</strong>r interferences with a fivepath<br />
interferometer<br />
Thomas Kauten<br />
13:45 502 Extraction of Ionic Cores From Charged Helium Nanodroplets<br />
Michael Renzler<br />
14:00 503 Probing Non-Equilibrium Dynamics of Iso<strong>la</strong>ted<br />
Quantum Many-Body Systems<br />
Bernhard Rauer<br />
14:15 504 Buffer gas cooling of atoms and molecules<br />
Sarah Skoff<br />
14:30 505 Spectroscopic and Theoretical Studies of Chromium<br />
Doped Helium Nanodroplets<br />
Andreas Kautsch<br />
14:45 506 A graph state formalism for mutually unbiased bases<br />
Christoph Spengler<br />
15:00 507 Strong coupling between single atoms and nontransversal<br />
photons<br />
Christian Junge<br />
15:15 508 Interactions of He – in doped He droplets<br />
Michael Neustetter<br />
15:30 Coffee Break<br />
Time ID Atomic Physics and Quantum Optics II<br />
Chair: NN<br />
16:00 511 Decoration of anionic and cationic fullerenes with<br />
po<strong>la</strong>r and apo<strong>la</strong>r molecules.<br />
Niko<strong>la</strong>us Weinberger<br />
16:15 512 Nonequilibrium dynamics, Optimal Control and Nanofibers<br />
on an Atom Chip<br />
Dominik Fischer<br />
16:30 513 A Spin Po<strong>la</strong>rised Temperature Controlled Atomic<br />
Hydrogen Beamline<br />
Peter Caradonna<br />
16:45 514 Theoretical Investigation of Excited States of the<br />
Diatomic Molecule LiCa<br />
Johann Pototschnig<br />
17:00 515 Single atom cavity quantum electrodynamics with<br />
non-transversally po<strong>la</strong>rized light fields<br />
Michael Scheucher<br />
17:15 516 Mapping Magnetic Nanostructures Using Radical<br />
Pair Reactions<br />
Jofre Espigule Pons<br />
17:30 517 Merging two immiscible BECs of Rb and Cs for optimized<br />
production of RbCs ground-state molecules<br />
Lukas Reichsöllner<br />
17:45 518 Cavity cooling of free silicon nanoparticles in high<br />
vacuum<br />
Peter Asenbaum<br />
18:00 519 Integrated Mach-Zehn<strong>de</strong>r interferometer for Bose-<br />
Einstein con<strong>de</strong>nsates<br />
T. Berrada<br />
18:15 520 Entanglement Swapping over a 143 km free-space<br />
link<br />
Thomas Herbst<br />
18:30 Postersession and Apéro<br />
20:00 Public Lecture<br />
Thursday, 05.09.2013, HS 4<br />
Time ID Atomic Physics and Quantum Optics III<br />
Chair: NN<br />
13:30 521 Tenfold reduction of Brownian noise in high-reflectivity<br />
optical coatings<br />
Garrett D. Cole<br />
13:45 522 Doublon stability and <strong>de</strong>cay mechanisms<br />
M. J. Mark<br />
14:00 523 Cavity cooling of an optically levitated nanoparticle<br />
Niko<strong>la</strong>i Kiesel<br />
14:15 524 Entanglement properties of locally maximally entangleable<br />
states<br />
Martí Cuquet<br />
14:30 525 Decrease in query complexity for quantum computers<br />
with superposition of circuits<br />
M. Araujo<br />
14:45 526 Optimal state reconstruction for cavity-optomechanical<br />
systems via Kalman filtering<br />
Jason Hoelscher-Obermaier<br />
15:00 527 Quantum Entanglement of High Angu<strong>la</strong>r Momenta<br />
Robert Fickler<br />
15:15 528 Cooling-by-measurement and mechanical state tomography<br />
via pulsed optomechanics<br />
M. R. Vanner<br />
15:30 Coffee Break<br />
20
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Time ID Atomic Physics and Quantum Optics IV<br />
Chair: NN<br />
16:00 531 Einstein-Podolsky-Rosen corre<strong>la</strong>tions from colliding<br />
Bose-Einstein con<strong>de</strong>nsates<br />
M. Ebner<br />
16:15 532 Real-Time Imaging of Quantum Entanglement<br />
Robert Fickler<br />
16:30 533 Creation of nitrogen-vacancy centres for cavity<br />
QED<br />
Kathrin Buczak<br />
16:45 534 Studies of Quantum Entanglement in 100 Dimensions<br />
Mario Krenn<br />
17:00 END<br />
18:30 Postersession and Apéro<br />
20:00 Conference Dinner<br />
ID Atomic Physics and Quantum Optics Poster<br />
541 Coupling Spins and Diamond Color Centers to<br />
Superconducting Cavities<br />
Stefan Putz<br />
542 Dipole-dipole influenced Ramsey interferometry<br />
Laurin Ostermann<br />
543 Ultracold atoms on a superconducting Atomchip<br />
Stefan Minniberger<br />
544 Coherent manipu<strong>la</strong>tion of cold cesium atoms in a nanofiberbased<br />
two-color dipole trap<br />
Daniel Reitz<br />
545 Coherence properties of cold cesium atomic spins in a<br />
nanofiber-based dipole trap<br />
Rudolf Mitsch<br />
546 see talk 516<br />
547 Photonic p<strong>la</strong>tform for experiments in higher dimensional<br />
quantum systems<br />
Christoph Schaeff<br />
548 Loophole- free Einstein Podolsky Rosen Experiment via<br />
Quantum Steering<br />
Bernhard Wittmann<br />
549 Quantum communication with satellites, its preparatory<br />
terrestrial free-space <strong>de</strong>monstrations and future missions<br />
Thomas Scheidl<br />
550 Laser <strong>de</strong>sorption/vaporization/ionization techniques for<br />
matter-wave interferometry<br />
Ugur Sezer<br />
Infrared Optical Nanostructures<br />
Wednesday, 04.09.2013, HS 3<br />
Time ID I: Quantum Casca<strong>de</strong> Lasers<br />
Chair: Karl Unterrainer, TU Wien<br />
13:30 601 Quantum casca<strong>de</strong> <strong>la</strong>ser frequency combs: spectroscopy<br />
and novel <strong>de</strong>velopments<br />
Jerome Faist (i)<br />
14:00 602 Bi-functional Quantum Casca<strong>de</strong> Laser/Detectors<br />
for Integrated Photonics<br />
Gottfried Strasser (i)<br />
14:30 603 Broadband external cavity tuning of a quantum casca<strong>de</strong><br />
<strong>la</strong>ser in the 3 - 4 µm window<br />
Sabine Riedi<br />
14:45 604 Terahertz spectroscopy of coupled cavity quantum<br />
casca<strong>de</strong> <strong>la</strong>sers<br />
Dominic Bachmann<br />
15:00 605 Terahertz Photonic Crystal Quantum Casca<strong>de</strong> Laser<br />
Coupled to a Second Or<strong>de</strong>r Bragg Vertical Extractor<br />
Christopher Bonzon<br />
15:15 606 From photonic crystal to micropil<strong>la</strong>r terahertz quantum<br />
casca<strong>de</strong> <strong>la</strong>sers and recent progress towards<br />
nanowire-based <strong>de</strong>vices<br />
Michael Krall<br />
15:30 Coffee Break<br />
II: Nanocrystals<br />
Chair: Gunther Springholz, JKU Linz<br />
16:00 611 Ultra strained Si and Ge for <strong>de</strong>vice applications<br />
Hans Sigg (i)<br />
16:30 612 Nanowires for so<strong>la</strong>r cell applications<br />
Knut Deppert (i)<br />
17:00 613 On polytypism in III-V nanowires<br />
Friedhelm Bechstedt (i)<br />
17:30 614 PbS nanocrystal photo<strong>de</strong>tectors with inorganic ligands<br />
Wolfgang Heiss (i)<br />
18:00 615 X-ray analysis of nanowires<br />
Julian Stangl<br />
18:15 616 Towards group IV direct gap semiconductors<br />
Martin G<strong>la</strong>ser<br />
18:30 Postersession and Apéro<br />
20:00 Public Lecture<br />
Thursday, 05.09.2013, HS 3<br />
Time ID III: Quantum Nanostructures<br />
Chair: Jérôme Faist, ETH Zürich<br />
13:30 621 Superconducting Split Ring Resonators for Ultrastrong<br />
Coupling<br />
Curdin Maissen<br />
13:45 622 Terahertz-induced nonlinear intersubband dynamics.<br />
Daniel Dietze<br />
14:00 623 Symmetric farfield, short-wavelength ( = 4.53 µm)<br />
MOPA quantum casca<strong>de</strong> <strong>la</strong>sers with Watt-level optical<br />
outpout power<br />
Boris<strong>la</strong>v Hinkov<br />
14:15 624 Optically pumped QD VECSEL for the Mid-Infrared<br />
Amir Khiar<br />
14:30 625 Intersublevel transition study of InAs/AlInAs quantum<br />
dashes by absorption, electroluminescence<br />
and magneto-tunneling spectroscopy<br />
Gian Lorenzo Paravicini Bagliani<br />
14:45 626 Erasing the exciton fine structure splitting in semiconductor<br />
quantum dots<br />
Rinaldo Trotta<br />
15:00 627 Grating-<strong>de</strong>sign based po<strong>la</strong>rization modifications of<br />
ring cavity quantum casca<strong>de</strong> <strong>la</strong>sers<br />
Rolf Szed<strong>la</strong>k<br />
15:15 628 Active control of THz-waves by coupling <strong>la</strong>rge-area<br />
CVD-graphene to a THz-Metamaterial<br />
Fe<strong>de</strong>rico Valmorra<br />
15:30 Coffee Break; END<br />
18:30 Postersession and Apéro<br />
20:00 Conference Dinner<br />
21
SPG Mitteilungen Nr. 40<br />
ID<br />
Infrared Optical Nanostructures Poster<br />
631 Enhancement of light extraction from aligned SiGe-based<br />
photonic crystal s<strong>la</strong>bs<br />
Magdalena Schatzl<br />
632 Optically driven current turnstile based on self-assembled<br />
semiconductor quantum dots<br />
Giancarlo Cerulo<br />
633 PbS quantum dots - silicon on insu<strong>la</strong>tor hybrid photonics<br />
Markus Humer<br />
634 Electronic and optical properties of strained and unstrained<br />
group-IV semiconductor Germanium alloys<br />
Kerstin Hummer<br />
635 Enhanced photoluminescence efficiency of SiGe is<strong>la</strong>nds integrated<br />
into <strong>la</strong>rge area photonic crystals<br />
Elisabeth Lausecker<br />
636 Tuning the emission properties of single semiconductor<br />
quantum dots via electro-e<strong>la</strong>stic fields<br />
Johannes Wildmann<br />
637 High power terahertz quantum casca<strong>de</strong> <strong>la</strong>ser for 63 μm<br />
Dana Turcinkova<br />
638 Quaternary Barrier InGaAs/AlInGaAs Terahertz Quantum<br />
Casca<strong>de</strong> Laser<br />
Keita Ohtani<br />
639 Distributed-Feedback Quantum Casca<strong>de</strong> Laser at 3.2 µm<br />
Johanna Wolf<br />
640 Tuning of resonances in photonic crystal photo<strong>de</strong>tectors<br />
Andreas Harrer<br />
641 Frequency noise in mid-infrared quantum casca<strong>de</strong> <strong>la</strong>sers<br />
Lionel Tombez<br />
642 Observation of THz Photo-luminescence from Multi<strong>la</strong>yer SiC<br />
Epitaxial Graphene Pumped by a Mid-infrared Quantum Casca<strong>de</strong><br />
Laser<br />
Peter Qiang Liu<br />
15:15 703 Innovating nanosensing technique to <strong>de</strong>tect living<br />
bacteria and reveal resistance to antibiotics<br />
Justin Notz<br />
15:30 Coffee Break<br />
Biophysics/Medical Physics<br />
Chair: Giovanni Dietler, EPF Lausanne<br />
Georg Pabst, Uni Graz<br />
16:00 711 Cell mechanics measured with Atomic force microscopy<br />
Jose Luis Toca- Herrera<br />
16:15 712 Measuring the stability of lipid membrane domains<br />
with nanometer resolution.<br />
Georg Fantner<br />
16:30 713 Protein partitioning in liquid-or<strong>de</strong>red (Lo) / liquiddisor<strong>de</strong>red<br />
(Ld) domains<br />
Benjamin Kollmitzer<br />
16:45 714 Filter gate closure inhibits ion but not water transport<br />
through potassium channels<br />
Peter Pohl<br />
17:00 715 Core-shell nanoparticles and their assembly<br />
Erik Reimhult<br />
17:15 716 Characterization of augmented bone structures<br />
with µ-computed tomography and Raman spectroscopy<br />
Johann Charwat-Pessler<br />
17:30 717 Raman spectroscopic investigation of urinary calculi<br />
and salivary stones<br />
Matthias E<strong>de</strong>r<br />
17:45 718 Saving Joint with Aerosolphysics<br />
Karoline Mühlbacher<br />
18:00 719 Probing metabolism in vivo in real time via hyperpo<strong>la</strong>rized<br />
NMR<br />
Arnaud Comment (i)<br />
18:30 END; Postersession and Apéro<br />
20:00 Conference Dinner<br />
Biophysics and Medical Physics<br />
Thursday, 05.09.2013, K153C<br />
Time ID Soft Matter<br />
(Shared with the Con<strong>de</strong>nsed Matter session)<br />
Go to HS 5<br />
Chair: Georg Pabst, Uni Graz<br />
13:30 121 Equilibrium and flow of cluster-forming complex<br />
fluids<br />
Christos N. Likos (i)<br />
14:00 122 Optimized Fourier Monte Carlo Simu<strong>la</strong>tion of Solid<br />
and Hexatic Membranes<br />
Andreas Troester<br />
14:15 123 Biomimetic folding particle chains<br />
Peter Oostrum<br />
14:30 Go back to K153C<br />
Biophysics<br />
Chair: Georg Pabst, Uni Graz<br />
14:30 701 Fluorescence and atomic force microscopy to<br />
visualize the interaction of HDL particles with lipid<br />
membranes<br />
Gerhard J. Schütz (i)<br />
15:00 702 Characterization of Curli A Production on Living<br />
Bacterial Surfaces by Scanning Probe Microscopy<br />
Yoojin Oh<br />
ID<br />
Biophysics and Medical Physics Poster<br />
721 Photomodification and Nanopatterning of Polystyrene for<br />
Bioapplications<br />
R. A. Barb<br />
722 Fractal characterization of tissue with the new Pyramid<br />
Method<br />
Michael Mayrhofer-Reinhartshuber<br />
723 The open pore of SecYEG does not show physiologically relevant<br />
ion selectivity<br />
Denis Knyazev<br />
724 Advancing high resolution structural analysis of lipid membranes<br />
using a generic algorithm<br />
Peter Heftberger<br />
725 Studies on the Cherenkov effect for improved TOF-PET<br />
Stefan Brunner<br />
726 Progress in the Structure-based Simu<strong>la</strong>tion of P<strong>la</strong>nt Light-<br />
Harvesting Complexes<br />
Frank Müh<br />
727 The <strong>de</strong>nsity and distribution of sacrificial bonds in polymer<br />
chains <strong>de</strong>termines the amount of dissipated energy<br />
S. Soran Nabavi<br />
728 STED-lithography nano-anchors with single protein capacity<br />
Richard Wollhofen<br />
729 These IgGs are ma<strong>de</strong> for walkin’: Random antibody movement<br />
on bacterial and viral surfaces<br />
Johannes Preiner<br />
730 Chemically tagged DNA tetrahedra as linker for single molecule<br />
force spectroscopy<br />
Michael Leitner<br />
22
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
731 Long and short lipid molecules experience the same interleaflet<br />
drag in lipid bi<strong>la</strong>yers<br />
Andreas Horner<br />
732 Bachelor thesis: Hyper Spectral Imaging with Two-Photon<br />
Microscopy<br />
Harald Razum<br />
733 Investigation of the pH stability of avidins and newly <strong>de</strong>veloped<br />
avidin mutants with atomic force microscopy based on<br />
single molecule sensors<br />
Me<strong>la</strong>nie Köhler<br />
734 Electrokinetic Trap<br />
Metin Kayci<br />
735 Towards a Non-Perturbative Theory of Optical Spectra of<br />
Pigment Protein Complexes: Application to the Water Soluble<br />
Chlorophyll Protein.<br />
Thanh-Chung Dinh<br />
17:15 820 Dynamical atmospheres of earth-like protop<strong>la</strong>nets<br />
Ernst Dorfi<br />
17:30 821 Constraining stel<strong>la</strong>r wind properties in habitable<br />
zones<br />
Colin Johnstone<br />
17:45 822 The analysis of young so<strong>la</strong>r-like stars and their stel<strong>la</strong>r<br />
winds observed with the EVLA to <strong>de</strong>fine mass<br />
loss rates<br />
Bibiana Fichtinger<br />
18:00 823 Stel<strong>la</strong>r magnetic fields and their potential influence<br />
on p<strong>la</strong>netary surroundings<br />
Theresa Lüftinger<br />
18:15 824 Photometry of different Minor Bodies and comparisons<br />
Mattia Galiazzo<br />
18:30 END; Postersession and Apéro<br />
20:00 Conference Dinner<br />
Astronomy and Astrophysics<br />
Thursday, 05.09.2013, K269D<br />
Time ID Astronomy and Astrophysics<br />
11:00 General Assembly ÖGAA<br />
12:30 Lunch<br />
13:30 801 Talk 1<br />
NN<br />
13:45 802 Talk 2<br />
NN<br />
14:00 803 Talk 3<br />
NN<br />
14:15 804 Talk 4<br />
NN<br />
Selected ÖGAA Talks<br />
Chair: NN<br />
Habitable Worlds:<br />
From Detection to Characterization<br />
Chair: NN<br />
14:30 811 Observing Exop<strong>la</strong>net Atmospheres: Recent Results<br />
from ESO and National Facilities<br />
Monika Lendl<br />
14:45 812 A massive stars' view on carbon-to-oxygen abundance<br />
ratios in exop<strong>la</strong>net host stars<br />
Norbert Przybil<strong>la</strong><br />
15:00 813 Composition of extraso<strong>la</strong>r p<strong>la</strong>nets<br />
Amaury Thiabaud<br />
15:15 814 The effect of metallicity in the envelope of protop<strong>la</strong>nets<br />
Julia Venturini<br />
15:30 Coffee Break<br />
16:00 815 Pathways to Habitability (PatH): An Austrian National<br />
Research Network<br />
Manuel Gü<strong>de</strong>l<br />
16:15 816 Long term evolution of protop<strong>la</strong>netary disks<br />
Alexan<strong>de</strong>r Stökl<br />
16:30 817 Formation of Chondrules in radiative shock waves<br />
Helmut Joham<br />
16:45 818 Formation of terrestrial p<strong>la</strong>nets in binary stel<strong>la</strong>r systems<br />
Zsolt Sándor<br />
17:00 819 A possible mo<strong>de</strong>l of water <strong>de</strong>livery by collisions in<br />
early p<strong>la</strong>netary systems<br />
Thomas I. Maindl<br />
ID<br />
Astronomy and Astrophysics Poster<br />
831 BRITE-Constel<strong>la</strong>tion and the chances for <strong>de</strong>tecting exop<strong>la</strong>nets<br />
Werner Weiss<br />
832 Simu<strong>la</strong>tions of Prebiotic Chemistry un<strong>de</strong>r Post-Impact Conditions<br />
on Titan<br />
Johannes Leitner<br />
833 On the Internal Structure of Ence<strong>la</strong>dus<br />
Ruth-Sophie Taubner<br />
834 Kepler-62 e and Kepler-62 f: The Potential Internal Structure<br />
of these habitable worlds<br />
Ruth-Sophie Taubner<br />
835 Theoretical mo<strong>de</strong>ls of p<strong>la</strong>netary system formation<br />
David Swoboda<br />
History of Physics<br />
Thursday, 05.09.2013, K012D<br />
Time ID History of Physics<br />
Chair: Heinz Krenn, Uni Graz<br />
13:30 901 Die Untersuchung p<strong>la</strong>netarer und interp<strong>la</strong>netarer<br />
Magnetfel<strong>de</strong>r: von <strong>de</strong>n ersten Satellitenmissionen<br />
bis zur Landung auf Asteroi<strong>de</strong>n und Kometen<br />
Konrad Schwingenschuh<br />
14:00 902 Die Novara-Weltumsegelung (1857-1859): Wen<strong>de</strong>punkt<br />
für Geophysik / Meteorologie / Ozeanographie<br />
in Österreich<br />
Bruno Besser<br />
14:15 903 Eine frühe Anwendung radioaktiver Tracer<br />
Heinrich Mitter<br />
14:30 904 G. E. Rosenthal, a follower of Deluc in northern Germany<br />
Jean-François Lou<strong>de</strong><br />
14:45 905 Die steinernen Schattenlinien <strong>de</strong>r Sonne: Die Sonnenuhren<br />
<strong>de</strong>s Andreas Pleninger<br />
Reinhard Folk<br />
15:00 906 The Incosistencies of the Lorentz transformations<br />
first formu<strong>la</strong>ted by Wol<strong>de</strong>mar Voigt in 1887<br />
Hartwig Thim<br />
15:15 Discussion<br />
15:30 Coffee Break<br />
23
SPG Mitteilungen Nr. 40<br />
Time ID Chair: Reinhard Folk, Uni Linz<br />
16:00 911 Physics in magnetic fields from Faraday to Pierre<br />
Weiss and his contemporaries<br />
Jean-François Lou<strong>de</strong><br />
16:30 912 Zur Erfindung <strong>de</strong>s Magnetinduktions-Zeigertelegraphen<br />
durch Charles Wheatstone<br />
Franz Pichler<br />
16:45 913 The Effective Mass Concept<br />
Gerhard Brunthaler<br />
17:00 914 Das Elektrotechnische Institut <strong>de</strong>r Universität Innsbruck,<br />
1907 – 1946. Ein 'vergessenes' Institut<br />
Armin Denoth<br />
17:15 915 Die Kommentare in Le Seurs und Jacquiers Ausgabe<br />
von Newtons Principia<br />
Harald Iro<br />
17:30 916 Viktor von Lang und Ernst Lecher – die Säulen <strong>de</strong>s<br />
I. Physikalischen Institutes<br />
Franz Sachslehner<br />
17:45 917 Das wissenschaftliche Exil in Großbritannien<br />
Wolfgang L. Reiter<br />
18:00 918 The *Squinting* in the Doppler-effect and the Hid<strong>de</strong>n<br />
Ether-drifts<br />
Karl Mocnik<br />
18:15 END<br />
18:30 Postersession and Apéro<br />
20:00 Conference Dinner<br />
Aussteller - Exposants<br />
Agilent Technologies, Vacuum Products Division,<br />
DE-60528 Frankfurt<br />
www.agilent.com<br />
Anton Paar GmbH, 8054 Graz;<br />
www.anton-paar.com/<br />
attocube systems AG, DE-80539 München<br />
www.attocube.com<br />
CryoVac GmbH & Co. KG, DE-53842 Troisdorf<br />
www.cryovac.<strong>de</strong><br />
Dr. Eberl MBE-Komponenten GmbH, DE-71263 Weil <strong>de</strong>r Stadt<br />
www.mbe-komponenten.<strong>de</strong><br />
EPL-IOP, UK-Bristol<br />
www.iop.org<br />
Finetech GmbH & Co. KG, DE-12681 Berlin<br />
www.finetech.<strong>de</strong><br />
Goodfellow GmbH, DE-61213 Bad Nauheim<br />
www.goodfellow.com<br />
Hositrad Deutsch<strong>la</strong>nd Vacuum Technology,<br />
DE-93047 Regensburg<br />
www.hositrad.com<br />
Mad City Labs GmbH, CH-8302 Kloten<br />
www.madcity<strong>la</strong>bs.eu<br />
Mantis Deposition GmbH, DE-55122 Mainz<br />
www.mantis<strong>de</strong>position.com<br />
MaTecK GmbH, DE-52428 Jülich<br />
www.mateck.<strong>de</strong><br />
Nanosurf AG, CH-4410 Liestal<br />
www.nanosurf.com<br />
Pfeiffer Vacuum Austria GmbH, AT-1150 Wien<br />
www.pfeiffer-vacuum.com<br />
Physik Instrumente (PI) GmbH & Co.KG, DE-76228 Karlsruhe<br />
www.pi.ws<br />
SPECS Surface Nano Analysis GmbH, DE-13355 Berlin<br />
www.specs.com<br />
VAQTEC - Scientific, DE-13189 Berlin<br />
www.vactec-scientific.com<br />
VAT – Deutsch<strong>la</strong>nd GmbH, DE-85630 Grasbrunn bei München<br />
www.vatvalve.com/<strong>de</strong>/contacts/vat-<strong>de</strong>utsch<strong>la</strong>nd<br />
VIDEKO GmbH, AT-2512 Oeynhausen<br />
www.vacuumtechnology.at<br />
Zurich Instruments, CH-8005 Zürich<br />
www.zhinst.com<br />
24
Open Access, where do we stand today?<br />
Your opinion interests us.<br />
Christophe Rossel, SPS Vice-Presi<strong>de</strong>nt<br />
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
With the <strong>de</strong>velopment of Open Access (OA) where the research<br />
papers become freely accessible by the rea<strong>de</strong>rs, the<br />
aca<strong>de</strong>mic publishing scheme is changing rapidly all over<br />
the world. The general consensus is that the results of research<br />
should be accessible in the public domain so that<br />
they will bring benefits for public services and economic<br />
growth. They need nevertheless to un<strong>de</strong>rgo some quality<br />
control for relevance and reliability reasons and for avoiding<br />
misleading statements and erroneous conclusions. Open<br />
Access is not strictly speaking free access because somewhere<br />
time and money must be found to make it functioning.<br />
Any new business mo<strong>de</strong>l, different from the conventional<br />
subscription-based mo<strong>de</strong>l must then be robust and<br />
sustainable.<br />
In 2009 the European Physical Society (EPS) published a<br />
position paper, <strong>de</strong>c<strong>la</strong>ring its support, like other organizations,<br />
to the 2003 Berlin Dec<strong>la</strong>ration on Open Access to<br />
Knowledge in the Sciences and Humanities (http://oa.mpg.<br />
<strong>de</strong>/openaccess-berlin/berlin<strong>de</strong>c<strong>la</strong>ration.html).<br />
The ongoing discussions are based on several critical issues.<br />
Whereas most researchers are essentially concerned<br />
about publishing their results in the journal of their choice<br />
without concerns about any business mo<strong>de</strong>ls, librarians<br />
who are facing <strong>de</strong>creasing budgets and increasing journal<br />
prices are ready for alternatives to the subscription-based<br />
mo<strong>de</strong>l. But how to meet publication costs if the subscription<br />
income is removed?<br />
Part of the <strong>de</strong>bate is to <strong>de</strong>ci<strong>de</strong> whether the Gold OA mo<strong>de</strong>l<br />
where publishers get their revenues from authors rather<br />
than from rea<strong>de</strong>rs is preferable to the Green OA mo<strong>de</strong>l<br />
where the final refereed article is p<strong>la</strong>ced temporarily in their<br />
institutional repository, in a central repository, or on some<br />
other OA archive like arXiv for physics. Critical voices c<strong>la</strong>im<br />
that some <strong>de</strong>trimental embargo time of 6–12 months or<br />
longer might be associated with the Green OA mo<strong>de</strong>l, as<br />
done already by some non-OA journals.<br />
Funding is therefore a critical issue for research agencies<br />
and aca<strong>de</strong>mic institutions, which will have to subsidize not<br />
only the work of editors but also support charges re<strong>la</strong>ted to<br />
Gold OA. This leads to another concern, namely the aca<strong>de</strong>mic<br />
freedom. Critics c<strong>la</strong>im in<strong>de</strong>ed that full Open Access<br />
mo<strong>de</strong>l will see universities, not rea<strong>de</strong>rs, pay for articles to<br />
be published in journals, meaning the <strong>de</strong>cision on how to<br />
publish new research will rest with university and funding<br />
agencies administrators and not aca<strong>de</strong>mics themselves.<br />
Science Europe (www.scienceeurope.org), an umbrel<strong>la</strong><br />
organization of the most important research and funding<br />
institutions in Europe, has published in April 2013 a <strong>de</strong>c<strong>la</strong>ration<br />
entitled Principles for the Transition to Open Access<br />
to Research Publications. It <strong>de</strong>scribes the benefits of OA<br />
and proposes a set of common principles agreed by all its<br />
members to support the transition to full OA. It is stated<br />
that each organization will have to implement policies according<br />
to their own needs but in agreement with the proposed<br />
principles, viewed as a contribution to a global dialogues<br />
and cooperation with other stakehol<strong>de</strong>rs in Europe<br />
and worldwi<strong>de</strong>.<br />
Funding organizations, including the Swiss National Science<br />
Foundation, endorse both publications in openaccess<br />
journals and second publications on document<br />
servers. However, they are explicitly against supporting<br />
so-called hybrid publication mo<strong>de</strong>ls offered by most <strong>la</strong>rge<br />
commercial publishers. In<strong>de</strong>ed in the case of hybrid journals,<br />
the authors can, in exchange for a fee, p<strong>la</strong>ce the<br />
article with publishers on OA. This mo<strong>de</strong>l might result in<br />
double charges since on one si<strong>de</strong> libraries still pay for the<br />
journal subscriptions and licenses and, on the other, for the<br />
OA publication fees of the authors<br />
The OA policies of all participating institutions, including<br />
those in Switzer<strong>la</strong>nd, are published in the Registry of Open<br />
Access Repository Mandatory Archiving Policies (ROAR-<br />
MAP) and can be found un<strong>de</strong>r http://roarmap.eprints.org/.<br />
Since the active <strong>de</strong>bate on the economics and reliability<br />
of OA continues among researchers, librarians, universities<br />
and funding agencies administrators, government officials,<br />
and commercial publishers, the SPS Board would<br />
be very interested in collecting comments by its members<br />
in or<strong>de</strong>r to evaluate the general opinions prevailing in the<br />
Swiss scientific community. Please send your comments to<br />
sps@unibas.ch.<br />
Kurz<strong>mitteilungen</strong> - Short Announcements<br />
Initiative for Science in Europe<br />
The Initiative for Science in Europe is an in<strong>de</strong>pen<strong>de</strong>nt p<strong>la</strong>tform<br />
of European learned societies and scientific organizations<br />
whose aim is to promote mechanisms to support all<br />
fields of science at a European level, involve scientists in<br />
the <strong>de</strong>sign and implementation of European science policies,<br />
and to advocate strong in<strong>de</strong>pen<strong>de</strong>nt scientific advice<br />
in European policy making. In Winter 2012/13, ISE has coordinated<br />
the campaign "No-Cuts-On-Research.EU".<br />
More Info: http://www.initiative-science-europe.org/<br />
25
SPG Mitteilungen Nr. 40<br />
2013 PSI Summer School on Con<strong>de</strong>nsed Matter Research:<br />
Materials - structure and magnetism<br />
August 17-23, 2013, Lyceum Alpinum, Zuoz, Switzer<strong>la</strong>nd<br />
The 12 th edition of the PSI summer school on con<strong>de</strong>nsed<br />
matter physics is open for registration. This year the school<br />
will be <strong>de</strong>dicated to some of the main topics addressed at<br />
<strong>la</strong>rge scale user facilities such as neutron and muon sources<br />
or synchrotron photon sources: Materials - structure<br />
and magnetism.<br />
International experts and PSI staff members will introduce<br />
and <strong>de</strong>epen your knowledge not only about these scientific<br />
topics but also about the main methods applied to un<strong>de</strong>rstand<br />
the phenomena, which are presently at the forefront<br />
of mo<strong>de</strong>rn solid state physics and chemistry.<br />
The school is fully open to the national and non-national<br />
public and the <strong>la</strong>nguage of the school is English.<br />
Following the school a practical training is offered at PSI. It<br />
will allow a limited number of participants to get hands-on<br />
experience with state-of-the-art instrumentation using photons,<br />
neutrons, and muons.<br />
More information, the school’s programme and online registration<br />
is avai<strong>la</strong>ble from the school’s webpage:<br />
http://www.psi.ch/summerschool<br />
19 th Swiss Physics Olympiad 2013 (SPhO) in Aarau<br />
The final round of the Swiss Physics Olympiad took p<strong>la</strong>ce<br />
on March 23/24 in Aarau at the Neue Kantonsschule. The<br />
competition was held between twenty-four stu<strong>de</strong>nts from<br />
Switzer<strong>la</strong>nd and two from Liechtenstein.<br />
The selection process began in January with a preliminary<br />
round with a record participation of over 100 stu<strong>de</strong>nts, a<br />
success with 50% more participation than in earlier years.<br />
The stu<strong>de</strong>nts, aged between 16 and 20, had the chance to<br />
prepare for the final round at a three day training<br />
session at EPFL. The final round consisted of two<br />
challenging days, totalling no less than six and a<br />
half hours of theoretical and experimental exams,<br />
something like a Marathon! The top five participants<br />
– gold medals - will have the unique opportunity<br />
to travel to Denmark to represent Switzer<strong>la</strong>nd<br />
at the International Physics Olympiad in July.<br />
The award ceremony was a <strong>de</strong>dicated moment with talks<br />
and piano pieces, where one could feel the mood of the<br />
accomplished effort. After an excellent pedagogical talk by<br />
Gabriel Pa<strong>la</strong>cios on Fraunhofer lines, presi<strong>de</strong>nt of SPhO, it<br />
was the tour of the Swiss Physical Society – who is sponsoring<br />
the event – to present the mission and vision of the<br />
Society, and to proceed to the awards distribution.<br />
Antoine Pochelon, SPS Secretary<br />
The absolute best was Lukas Lang, from Liechtenstein.<br />
Followed just next by Sven Pfeiffer, from Münsingen (BE)<br />
and Rafael Winkler, from Mettauertal (AG). The SPS was<br />
happy to <strong>de</strong>liver the woman award to Viviane Kehl, from<br />
Küsnacht (ZH) who already illustrated herself in the preliminary<br />
round as 4 th and at the time best of the present Swiss<br />
winner group.<br />
Such an event is the opportunity to strengthen<br />
contact with offspring and teachers in a nice and<br />
stimu<strong>la</strong>ting climate. As summarized by Markus<br />
Meier, the local organizer: I hope and believe that<br />
this event (with SPS presentation and award giving)<br />
is the first and also successful contact of the<br />
SPS to future physicists. And truly, at this occasion<br />
young people of 15 or 16 were asking how to become<br />
member of the SPS and how they could be better<br />
informed about courses, seminars, ateliers … : a hint for the<br />
SPS to be well present for the young leaves.<br />
PS: Let us note that in Switzer<strong>la</strong>nd such Olympiads - in addition<br />
to Physics (www.swi<strong>ssp</strong>ho.ch) - are also organized in<br />
Biology, Chemistry, Informatics, Mathematics, Philosophy<br />
(www.olympiads.ch).<br />
The four recipients of the SPS awards: Sven Pfeiffer (first Swiss), Rafael Winkler (second Swiss), Viviane Kehl (first woman) and Lukas<br />
Lang (first Liechtensteiner and absolut best)<br />
26
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Das Rennen um die Industrieproduktion <strong>de</strong>r Zukunft<br />
Rolf Hügli, SATW Generalsekretär<br />
Die Schweiz gehört bekanntlich zu <strong>de</strong>n innovativsten Län<strong>de</strong>rn<br />
<strong>de</strong>r Welt. Die Ausgaben für die Forschung sind hoch<br />
und auf Jahre hinaus gesichert. Wenn die Schweiz aber<br />
eine be<strong>de</strong>uten<strong>de</strong> Industrienation bleiben will, muss auch<br />
<strong>de</strong>r Produktionsstandort Schweiz eine Zukunft haben. Produktions-Knowhow<br />
gehört zu <strong>de</strong>n Schlüsselkompetenzen<br />
für die "alten Industrienationen", die nicht auf billige Arbeitskräfte<br />
setzen können.<br />
In <strong>de</strong>n letzten 5 Jahren hat die EU 10% ihrer Industrieproduktion<br />
und 3 Millionen Jobs verloren. Zumin<strong>de</strong>st vor<strong>de</strong>rhand<br />
hat sich die Schweiz gut behaupten können, weil<br />
ihre Industriegüter hochspezialisiert sind. Diese Produkte<br />
sind weniger preissensitiv und ihre Herstellung ist sehr anspruchsvoll.<br />
Ob dies in Zukunft hilft, ist ungewiss. Die Währungssituation<br />
ist nach wie vor angespannt und Län<strong>de</strong>r wie<br />
China und Indien sind im Begriff, immer komplexere Eigenprodukte<br />
zu entwickeln und herzustellen.<br />
Hinzu kommt, dass sich be<strong>de</strong>uten<strong>de</strong> Neuerungen bei <strong>de</strong>n<br />
Herstellungsverfahren abzeichnen. Die massgeblichen Treiber<br />
dafür sind:<br />
• weitgehen<strong>de</strong> Digitalisierung <strong>de</strong>r Wertschöpfungskette<br />
(Herstellungsdaten wer<strong>de</strong>n verschickt, nicht physische<br />
Produkte)<br />
• präzisere Verfahren bei <strong>de</strong>r automatischen maschinellen<br />
Bearbeitung (schnelle, hochwirksame Korrekturalgorithmen<br />
verbessern die automatisierte mechanische<br />
Bearbeitung)<br />
• völlig neue, additive Herstellungsverfahren (z.B. 3D<br />
Printing).<br />
Dadurch wird eine kostengünstige Produktion anspruchsvoller<br />
Komponenten an einem beliebigen Ort <strong>de</strong>r Welt<br />
<strong>de</strong>nkbar. Auch die rentable Produktion von Kleinstserien<br />
o<strong>de</strong>r Einzelstücken könnte damit gelingen.<br />
Während diese Entwicklung für qualifizierte Facharbeiter<br />
eine Gefahr darstellen könnte, bietet sie <strong>de</strong>n westlichen Industrienationen<br />
die Möglichkeit, dank kostengünstiger Produktion<br />
einen Teil <strong>de</strong>s verlorenen Marktes zurückzuerobern.<br />
Welcher Aspekt dominieren wird, ist völlig unk<strong>la</strong>r. Für <strong>de</strong>n<br />
Werkp<strong>la</strong>tz Schweiz ist es von grosser Be<strong>de</strong>utung, diese<br />
Trends zu verstehen und richtig darauf zu reagieren.<br />
Die SATW hat kürzlich ein Forum unter <strong>de</strong>m Titel "advanced<br />
manufacturing" veranstaltet. Unter <strong>de</strong>n Teilnehmern waren<br />
Produktions- und Materialexperten, Wissenschaftler und<br />
Repräsentanten von Verwaltung und Industrieverbän<strong>de</strong>n.<br />
Auch unter <strong>de</strong>n Anwesen<strong>de</strong>n herrschte keine Einigkeit, in<br />
welche Richtung sich die Dinge entwickeln wer<strong>de</strong>n. K<strong>la</strong>r<br />
herausgeschält haben sich jedoch zwei Dinge:<br />
• Die neuen Verfahren bestehen aus einzelnen Komponenten<br />
und Arbeitsschritten, die aufeinan<strong>de</strong>r abgestimmt<br />
sein müssen. Es ist daher empfehlenswert,<br />
diese Verfahren „vertikal integriert“, d.h. in Konsortien<br />
zu entwickeln, welche die ganze Wertschöpfungskette<br />
ab<strong>de</strong>cken.<br />
• C. M. C<strong>la</strong>yton hat <strong>de</strong>n Begriff <strong>de</strong>r "disruptiven" Innovation<br />
geprägt. Gemeint sind damit Verän<strong>de</strong>rungen,<br />
die auf (vom Markt) unerwarteten, neuen Prinzipien<br />
beruhen und die die Spielregeln einer ganzen Branche<br />
verän<strong>de</strong>rn können. Die erwähnten neuen Herstellungsmetho<strong>de</strong>n<br />
haben das Potential dazu. Allerdings<br />
ist unk<strong>la</strong>r, welche Verfahren sich wo durchsetzen wer<strong>de</strong>n.<br />
Damit entstehen grosse Investitionsrisiken. Da<br />
nicht gewartet wer<strong>de</strong>n kann, bis völlige K<strong>la</strong>rheit darüber<br />
herrscht, ist zu prüfen ob eine finanzielle För<strong>de</strong>rung<br />
von Pilotprojekten durch Bun<strong>de</strong>smittel (evtl. im<br />
Rahmen KTI o<strong>de</strong>r SNF) im Sinne eines Schwerpunktprogrammes<br />
angezeigt wäre.<br />
Die SATW wird dieses Thema weiter bearbeiten. Im Verbund<br />
<strong>de</strong>r europäischen technischen Aka<strong>de</strong>mien (Euro-CASE) ist<br />
sie an einem Diskussionspapier für die EU-Kommission beteiligt.<br />
Sie verfolgt zu<strong>de</strong>m <strong>de</strong>n Jahreskongress <strong>de</strong>r Canadian<br />
Aca<strong>de</strong>my of Engineering (CAE), an <strong>de</strong>m ähnliche Fragen<br />
diskutiert wer<strong>de</strong>n. Die SATW p<strong>la</strong>nt ausser<strong>de</strong>m im Herbst ein<br />
Folgemeeting mit einzelnen Teilnehmern <strong>de</strong>s Forums, um<br />
praktische Handlungsoptionen zu bestimmen. Zusätzlich<br />
möchte die SATW ihr Netzwerk mit Produktionsexperten<br />
aus <strong>de</strong>r Industrie verstärken. Gerne nimmt sie auch Beiträge<br />
o<strong>de</strong>r Anregungen von Mitglie<strong>de</strong>rn <strong>de</strong>r SPG entgegen.<br />
"Advanced Manufacturing’", ein interessantes Feld<br />
für Physikerinnen und Physiker?<br />
Mo<strong>de</strong>rne Produktionsmetho<strong>de</strong>n beruhen auf <strong>de</strong>r durchgängigen<br />
Digitalisierung nahezu aller Prozessschritte,<br />
vom Design über die eigentliche Fertigung bis zur Auslieferung.<br />
Dabei umfasst <strong>de</strong>r Begriff Digitalisierung sowohl<br />
computergesteuerte Datenerfassung, numerische<br />
Mo<strong>de</strong>llierung wie Echtzeit-Kommunikation. Weist das<br />
zu fertigen<strong>de</strong> Gerät ab einer gewissen Fertigungsstufe<br />
einen bestimmten Grad an interner Digitalisierung auf,<br />
kann es -ab dann- selber mit <strong>de</strong>n Produktionswerkzeugen<br />
kommunizieren, was zu Genauigkeitssteigerungen<br />
und Durch<strong>la</strong>ufzeitverkürzungen führt. Im gleichen Sinne<br />
kann die interne Digitalisierung später im Einsatz beim<br />
Kun<strong>de</strong>n die Kommunikation mit <strong>de</strong>r Herstellfirma o<strong>de</strong>r<br />
einem Provi<strong>de</strong>r ermöglichen, um die Dienstleistung <strong>de</strong>s<br />
Gerätes nur dann und dort abzurufen, wann und wo es<br />
vom Kun<strong>de</strong>n benötigt wird. Für <strong>de</strong>n Kun<strong>de</strong>n be<strong>de</strong>utet<br />
das eine <strong>de</strong>utliche Effizienzsteigerung seiner Arbeit und<br />
eine Senkung <strong>de</strong>r Betriebskosten.<br />
Im Mittelpunkt all dieser Ansätze steht die Erfassung <strong>de</strong>r<br />
realen Fertigungsabläufe und <strong>de</strong>ren mathematische Mo<strong>de</strong>llierung<br />
('Virtuelle Fabrik'). Das erfor<strong>de</strong>rt ein profun<strong>de</strong>s<br />
physikalisches Verständnis, wenn man an die technischen<br />
Machbarkeitsgrenzen gehen will. Für Industriephysiker<br />
öffnen sich attraktive Betätigungsfel<strong>de</strong>r<br />
B. Braunecker<br />
27
SPG Mitteilungen Nr. 40<br />
First result from the AMS experiment<br />
Martin Pohl, Center for Astroparticle Physics, CAP Genève<br />
Beginning of April 2013, the Alpha Magnetic Spectrometer<br />
(AMS) Col<strong>la</strong>boration published its first physics result in<br />
Physical Review Letters 1 . The AMS experiment is a powerful<br />
and sensitive particle physics spectrometer. As seen in<br />
Figure 1, AMS is located on the exterior of the International<br />
Space Station (ISS). Since its instal<strong>la</strong>tion on 19 May 2011 it<br />
has measured over 30 billion cosmic rays in the GeV to TeV<br />
energy range. Its permanent magnet and array of precision<br />
particle <strong>de</strong>tectors collect and i<strong>de</strong>ntify charged cosmic rays<br />
passing through. Over its long duration mission on the ISS,<br />
AMS will record signals from 16 billion cosmic rays every<br />
year and transmit them to Earth for analysis by the AMS<br />
Col<strong>la</strong>boration. This is the first of many physics results to be<br />
reported.<br />
onboard the final mission of space shuttle En<strong>de</strong>avour (STS-<br />
134) on 16 May 2011. Once installed on 19 May 2011, AMS<br />
was powered up and immediately began collecting data<br />
from primary sources in space and these were transmitted<br />
to the AMS Payload Operations Control Center located at<br />
CERN, Geneva, Switzer<strong>la</strong>nd.<br />
Once AMS became operational, the first task for the AMS<br />
Col<strong>la</strong>boration was to ensure that all instruments and systems<br />
performed as <strong>de</strong>signed and as tested on the ground.<br />
The AMS <strong>de</strong>tector, with its multiple redundancies, has proven<br />
to perform f<strong>la</strong>wlessly in space. Over the <strong>la</strong>st 22 months in<br />
flight, AMS col<strong>la</strong>borators have gained invaluable operational<br />
experience in running a precision spectrometer in space<br />
and mitigating the hazardous conditions to which AMS is<br />
exposed as it orbits the Earth every 90 minutes. Conditions<br />
like this are not encountered by ground-based accelerator<br />
experiments or satellite-based experiments and require<br />
constant vigi<strong>la</strong>nce in or<strong>de</strong>r to avoid irreparable damage.<br />
They inclu<strong>de</strong> the extreme thermal variations caused by so<strong>la</strong>r<br />
effects and the re-positioning of ISS onboard radiators<br />
and so<strong>la</strong>r arrays. In addition, the AMS operators regu<strong>la</strong>rly<br />
transmit software updates from the AMS POCC at CERN to<br />
the AMS computers in space in or<strong>de</strong>r to match the regu<strong>la</strong>r<br />
upgra<strong>de</strong>s of the ISS software and hardware.<br />
Figure 1: From its vantage point about 400 km above the Earth, the<br />
Alpha Magnetic Spectrometer (AMS) collects data from primordial<br />
cosmic rays that traverse the <strong>de</strong>tector.<br />
The first publication from the AMS Experiment is a major<br />
milestone for the AMS international col<strong>la</strong>boration. Hundreds<br />
of scientists, engineers, technicians and stu<strong>de</strong>nts from all<br />
over the world have worked together for over 18 years to<br />
make AMS a reality. The col<strong>la</strong>boration represents 16 countries<br />
from Europe, Asia and North America (Fin<strong>la</strong>nd, France,<br />
Germany, Italy, the Nether<strong>la</strong>nds, Portugal, Spain, Switzer<strong>la</strong>nd,<br />
Romania, Russia, Turkey, China, Korea, Taiwan, Mexico<br />
and the United States) un<strong>de</strong>r the lea<strong>de</strong>rship of Nobel<br />
Laureate Samuel Ting of M.I.T. The col<strong>la</strong>boration continues<br />
to work closely with the NASA AMS Project Management<br />
team from Johnson Space Center as it has throughout the<br />
entire process. Many countries have ma<strong>de</strong> important contributions<br />
to the AMS <strong>de</strong>tector construction and presently<br />
to the data analysis. These inclu<strong>de</strong> two groups from Switzer<strong>la</strong>nd,<br />
University of Geneva and ETHZ, supported by fe<strong>de</strong>ral<br />
and cantonal authorities as well as the SNF.<br />
AMS was constructed at universities and research institutes<br />
around the world and assembled at the European Organization<br />
for Nuclear Research, CERN, Geneva, Switzer<strong>la</strong>nd.<br />
It was <strong>la</strong>unched by NASA to the ISS as the primary payload<br />
1 AMS Col<strong>la</strong>boration, M. Agui<strong>la</strong>r et al., First Result from the Alpha<br />
Magnetic Spectrometer on the International Space Station: Precision<br />
Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350<br />
GeV, Phys. Rev. Lett. 110, 141102 (2013)<br />
28<br />
Positron fraction measurement<br />
In the initial 18 months period of space operations, from<br />
19 May 2011 to 10 December 2012, AMS analyzed 25 billion<br />
primary cosmic ray events. Of these, an unprece<strong>de</strong>nted<br />
number, 6.8 million, were unambiguously i<strong>de</strong>ntified as<br />
electrons and their antimatter counterpart, positrons. The<br />
6.8 million particles observed in the energy range 0.5 to<br />
350 GeV are the subject of the precision study reported in<br />
this first paper.<br />
Electrons and positrons are i<strong>de</strong>ntified by the accurate and<br />
redundant measurements provi<strong>de</strong>d by the various AMS instruments<br />
against a <strong>la</strong>rge background of protons. Positrons<br />
are clearly distinguished from this background through the<br />
robust rejection power of AMS of more than one in one million.<br />
Currently, the total number of positrons i<strong>de</strong>ntified by AMS,<br />
in excess of 400,000, is the <strong>la</strong>rgest number of energetic<br />
antimatter particles directly measured and analyzed from<br />
space. The first paper can be summarized as follows:<br />
AMS has measured the positron fraction (ratio of the positron<br />
flux to the combined flux of positrons and electrons)<br />
in the energy range 0.5 to 350 GeV. We have observed that<br />
from 0.5 to 10 GeV, the fraction <strong>de</strong>creases with increasing<br />
energy. The fraction then increases steadily between 10<br />
GeV to ~250 GeV. Yet the slope (rate of growth) of the positron<br />
fraction <strong>de</strong>creases by an or<strong>de</strong>r of magnitu<strong>de</strong> from 20 to<br />
250 GeV. At energies above 250 GeV, the spectrum appears<br />
to f<strong>la</strong>tten but to study the behavior above 250 GeV requires<br />
more statistics – the data reported represents ~10% of the
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
total expected. The positron fraction spectrum exhibits neither<br />
structure nor time <strong>de</strong>pen<strong>de</strong>nce. The positron to electron<br />
ratio shows no anisotropy indicating the energetic positrons<br />
are not coming from a preferred direction in space.<br />
Together, these features show evi<strong>de</strong>nce of a new physics<br />
phenomena. Figure 2 illustrates the AMS data presented in<br />
the first publication.<br />
statistics avai<strong>la</strong>ble distinguish the reported positron fraction<br />
spectrum from earlier experiments 3 , by extending the<br />
energy range and improving the precision by an or<strong>de</strong>r of<br />
magnitu<strong>de</strong>.<br />
Outlook<br />
AMS is a magnetic spectrometer with the ability to explore<br />
new physics because of its precision, statistics, energy<br />
range, capability to i<strong>de</strong>ntify different particles and nuclei and<br />
its long duration in space. It is expected that hundreds of<br />
billions of cosmic rays will be measured by AMS throughout<br />
the lifetime of the Space Station. The volume of raw data<br />
requires a massive analysis effort. The parameters of each<br />
signal collected are meticulously reconstructed, characterized<br />
and archived before they un<strong>de</strong>rgo analysis by multiple<br />
in<strong>de</strong>pen<strong>de</strong>nt groups of AMS physicists thus ensuring the<br />
accuracy of the physics results.<br />
Figure 2: The positron fraction measured by AMS <strong>de</strong>monstrates<br />
excellent agreement with the mo<strong>de</strong>l <strong>de</strong>scribed below. Even with<br />
the high statistics, 6.8 million events, and accuracy of AMS, the<br />
fraction shows no fine structure.<br />
The exact shape of the spectrum, as shown in Figure 2, exten<strong>de</strong>d<br />
to higher energies, will ultimately <strong>de</strong>termine whether<br />
this spectrum originates from the collision of dark matter<br />
particles or from pulsars in the ga<strong>la</strong>xy. The high level of accuracy<br />
of this data indicates that AMS may soon resolve<br />
this issue.<br />
Over the <strong>la</strong>st few <strong>de</strong>ca<strong>de</strong>s there has been much interest on<br />
the positron fraction from primary cosmic rays by both particle<br />
physicists and astrophysicists. The un<strong>de</strong>rlying reason<br />
is that by measuring the ratio between positrons and electrons<br />
and by studying the behavior of any excess across<br />
the energy spectrum, a better un<strong>de</strong>rstanding of the origin<br />
of dark matter and other physics phenomena may be obtained.<br />
The first AMS result has been analyzed using several phenomenological<br />
mo<strong>de</strong>ls, one of which is <strong>de</strong>scribed in the<br />
paper and inclu<strong>de</strong>d in Figure 2. This generic mo<strong>de</strong>l, with<br />
diffuse electron and positron components and a common<br />
source component, fits the AMS data surprisingly well. This<br />
agreement indicates that the positron fraction spectrum is<br />
consistent with electron positron fluxes each of which is the<br />
sum of its diffuse spectrum and a single energetic common<br />
source. In other words, a significant portion of the highenergy<br />
electrons and positrons originate from a common<br />
source. More specific mo<strong>de</strong>ls 2 based on dark matter self<br />
annihi<strong>la</strong>tion and/or pulsar sources in the Milky Way have<br />
been published immediately after the release of the AMS<br />
data.<br />
As shown in Figure 3, the accuracy of AMS and the high<br />
2 See e.g.: Andrea De Simone, Antonio Riotto, Wei Xuec, CERN-<br />
PH-TH/2013-054 (April 3, 2013). Tim Lin<strong>de</strong>n and Stefano Profumo,<br />
arXiv:1304.1791v1 [astro-ph.HE], (April 5, 2013). Peng-Fei Yin, Zhao-Huan<br />
Yu, Qiang Yuan and Xiao-Jun Bi, arXiv:1304.4128v1 [astro-ph.HE] (April<br />
15, 2013)<br />
Figure 3: A comparison of AMS results with recent published measurements.<br />
With the wealth of data emitted by primary cosmic rays<br />
passing through AMS, the Col<strong>la</strong>boration will also explore<br />
other topics such as the precision measurements of the boron<br />
to carbon ratio, nuclei and antimatter nuclei, and antiprotons,<br />
precision measurements of the helium flux, proton<br />
flux and photons, as well as the search for new physics and<br />
astrophysics phenomena such as strangelets.<br />
The AMS Col<strong>la</strong>boration will provi<strong>de</strong> new, accurate information<br />
over the lifetime of the Space Station as the AMS<br />
<strong>de</strong>tector continues its mission to explore new physics phenomena<br />
in the cosmos.<br />
(This article is based on http://press.web.cern.ch/tags/ams.)<br />
3 TS93: R. Gol<strong>de</strong>n et al., Astrophys. J. 457 (1996) L103. Wizard/<br />
CAPRICE: M. Boezio et al., Adv. Sp. Res. 27-4 (2001) 669. HEAT: J. J.<br />
Beatty et al., Phys. Rev. Lett. 93 (2004) 241102; M. A. DuVernois et al.,<br />
Astrophys. J. 559 (2001) 296. AMS-01: M. Agui<strong>la</strong>r et al., Phys. Lett. B 646<br />
(2007) 145. PAMELA: P. Picozza, Proc. of the 4 th International Conference<br />
on Particle and Fundamental Physics in Space, Geneva, 5-7 Nov. 2012,<br />
to be published. O. Adriani et al., Astropart. Phys. 34 (2010) 1; O. Adriani<br />
et al., Nature 458 (2009) 607. Fermi-LAT: M. Ackermann et al., Phys. Rev.<br />
Lett. 108 (2012) 011103.<br />
29
SPG Mitteilungen Nr. 40<br />
Progress in Physics (33)<br />
Outreach: Can Physics Cross Boundaries?<br />
Jean-Pierre Eckmann, Département <strong>de</strong> Physique Théorique et Section <strong>de</strong> Mathématiques, Université <strong>de</strong> Genève<br />
Recently, physical thinking has been making progress in<br />
domains at which it did not aim originally. In this contribution,<br />
I want to sketch some examples of what can be done.<br />
The method consists of finding systems which originate in<br />
complex or complicated structure or dynamics, and which<br />
can profit from questions physicists ask. The examples I<br />
want to present comprise biology, <strong>la</strong>nguage and the Worldwi<strong>de</strong>-web<br />
(WWW).<br />
I find it fascinating that re<strong>la</strong>tively simple methods, questions,<br />
and techniques from the exact sciences seem to be<br />
able to shed new light, and also new insight, into structures<br />
which are mostly self-generated. I want to suggest<br />
and illustrate that questions outsi<strong>de</strong> physics proper can be<br />
<strong>de</strong>veloped fruitfully by physicists. My story is neither totally<br />
new (see, e.g., [14]) nor as revolutionary as it may seem. I<br />
just want to convey my interest and pleasure in addressing<br />
"esoteric" questions with the tools of mathematics and<br />
physics.<br />
The discussion will be in the subject of "network theory,"<br />
and I first summarize some of its literature [1, 12] : With the<br />
advent of powerful computers on every scientist’s <strong>de</strong>sk, it<br />
has become easy to analyze <strong>la</strong>rge data sets. These data<br />
sets come often, and quite naturally, in the form of <strong>la</strong>rge<br />
networks (graphs, directed or undirected), where the no<strong>de</strong>s<br />
of the graph are certain objects, and the edges are certain<br />
binary re<strong>la</strong>tions between them. For example, the no<strong>de</strong>s<br />
could be individual researchers, and the links could signify<br />
that they either co-author a paper, or cite each other.<br />
Other examples are pages and links in the WWW, which<br />
connect two pages; airports and connections provi<strong>de</strong>d by<br />
commercial airlines; words and links between these words<br />
and their <strong>de</strong>finition in a dictionary. I will call such graphs<br />
real-life graphs 1 . Experimental automation, and the avai<strong>la</strong>bility<br />
of <strong>la</strong>rge databases through the internet provi<strong>de</strong> many<br />
interesting networks for analysis. The most useful ones are<br />
obtained in col<strong>la</strong>boration with experimental scientists.<br />
Continuing a long tradition in statistical physics, the studies<br />
of <strong>la</strong>rge networks often concentrate on their statistical<br />
properties. Erdős and Rényi <strong>de</strong>scribed a set of random<br />
graphs which are built as follows [3]: Take N no<strong>de</strong>s (N very<br />
<strong>la</strong>rge) and assume that the mean <strong>de</strong>gree (number of links<br />
coming out of a no<strong>de</strong>) is k > 0, in<strong>de</strong>pen<strong>de</strong>ntly of N. Then,<br />
paraphrasing Erdős and Rényi, one can make two statements:<br />
1. Such a graph looks locally like a tree (i.e., it has very<br />
few loops, and these loops are all very long) [4].<br />
2. The expected number of triangles is k 3 /6, (i.e., this<br />
number does not grow with N). (Longer loops are also<br />
rare 2 .)<br />
1 One may legitimately ask why only binary re<strong>la</strong>tions seem important, but<br />
I will argue <strong>la</strong>ter that triangles in these graphs p<strong>la</strong>y the role of three-bodyinteractions<br />
and are the main indicators of semantic contexts.<br />
2 It is actually quite easy to prove these statements, although, at first,<br />
they certainly seem totally anti-intuitive.<br />
3 also called "rich get richer"<br />
30<br />
The first surprise was the discovery that real-life graphs are<br />
not random in the above sense. In contrast to general results<br />
on random graphs, the graphs of "affinities" or "connections"<br />
between "authors," "entities" have very specific<br />
general properties, namely power <strong>la</strong>w behavior over several<br />
<strong>de</strong>ca<strong>de</strong>s [1]. By this, one means the statistics of the number<br />
N^ j h of no<strong>de</strong>s which are attached to exactly j others (the<br />
-c<br />
<strong>de</strong>gree of the no<strong>de</strong>). In formu<strong>la</strong>s, N^ j h . const.<br />
j for <strong>la</strong>rge<br />
j. The point here is that the <strong>de</strong>cay is a power <strong>la</strong>w, and not<br />
an exponential, pointing to the important feature of no<strong>de</strong>s<br />
in the graph with very many connections, many more than<br />
a Gaussian, or Poisson distribution would allow for. In many<br />
real-life graphs g takes a value between 2 and 3.<br />
What this means is that there are a few no<strong>de</strong>s which have<br />
a really high <strong>de</strong>gree. For example, in studying the connections<br />
in Twitter, one finds that there are a few no<strong>de</strong>s with<br />
over 100’000 "friends" (these are usually politicians, perhaps<br />
also singers), the interesting question here is whether<br />
they are friends (the singers) or whether they think they<br />
have friends (the politicians...).<br />
Many studies then concentrate on the dynamics of how<br />
such networks come into being. This is usually called the<br />
"preferential attachment" 3 problem [2], namely the i<strong>de</strong>a<br />
that the networks build up in time, and that people have a<br />
ten<strong>de</strong>ncy to connect to well-known other people (or services).<br />
These mo<strong>de</strong>ls have successfully exp<strong>la</strong>ined how longrange<br />
(scale-free) properties of graphs come about.<br />
Another important aspect of network studies is summarized<br />
un<strong>de</strong>r the term of "clustering coefficient" [18]. In contrast to<br />
the power <strong>la</strong>ws <strong>de</strong>scribed above, this is a local property of<br />
any graph. In mathematical terms, if a no<strong>de</strong> n has j neighbors,<br />
then you count the number t of triangles which have<br />
the no<strong>de</strong> n as a corner. Obviously, there cannot be more<br />
than T^<br />
j h = j^j - 1h / 2 such triangles, and the clustering<br />
coefficient is <strong>de</strong>fined as t/<br />
T^ j h, which is a number between<br />
0 and 1. A high clustering coefficient means that many of<br />
the possible triangles are actually realized.<br />
When I started to study real-life graphs [7], I was puzzled by<br />
the abundance of triangles, which appear or<strong>de</strong>rs of magnitu<strong>de</strong><br />
above (k 3 ) predicted by Erdős and Rényi. What<br />
does this mean? It soon turned out that triangles p<strong>la</strong>y a<br />
strong semantic role. In other words, in all studies of this<br />
type, one can attach meaning to this abundance.<br />
The first case where we discovered this phenomenon was<br />
the set of links in the WWW [7]. While there are many links<br />
which seem irrelevant, we found that those links which form<br />
triangles re<strong>la</strong>te to common interests of the owners of the<br />
pages involved. Carrying this i<strong>de</strong>a further, we found that<br />
triangles of connections among neurons of C. Elegans (a little<br />
worm with 302 neurons) organize their function. Another<br />
example is provi<strong>de</strong>d by triangles of e-mail messages sent<br />
between people, and this <strong>de</strong>termines their social grouping<br />
[8].
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
The neurons of C. Elegans and their connections: Height is clustering<br />
coefficient, color co<strong>de</strong>s function (motor, sensory,...)<br />
My final example is the appearance of loops in the <strong>de</strong>finitions<br />
of words in a dictionary [10]. Here, the graph is formed<br />
by arrows pointing from each word (actually nouns) to the<br />
words in their <strong>de</strong>finition. One finds not only triangles, but<br />
also bi-angles, back-and-forth, (which are synonyms) and<br />
also longer loops. When the loops are too long, there might<br />
be a jump in interpretation, such as at the broken arrow in<br />
railcar & rails & bar & weapon & instrument &<br />
skill Z train & railcar.<br />
But the surprising fact is that the medium size loops are<br />
semantically coherent, and their words form the core of the<br />
<strong>la</strong>nguage. (We checked that by comparing the core-words<br />
to those of [13].) And furthermore, as a bonus, one can<br />
show that they are re<strong>la</strong>ted to the historical appearance of<br />
new concepts in <strong>la</strong>nguage [9].<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
What fascinates me in all this is that questions and methods<br />
from physics can shed new light on several systems<br />
with complex dynamics or structure. The most accessible<br />
among such systems are those where sub-units are assembled<br />
without a master building p<strong>la</strong>n.<br />
The common structure which appears in such studies is<br />
that the more "interesting dynamics" (biochemistry, feedback)<br />
[16], the "meaning" (<strong>la</strong>nguage) [5] or "mechanisms"<br />
(emergent life) are all revealed by <strong>de</strong>viations from the natural<br />
statistical structures of random assemblies. In general, the<br />
connected objects have some "<strong>de</strong>eper" i<strong>de</strong>ntity (meaning,<br />
semantics) that curves the pathways back to some originating<br />
no<strong>de</strong>, in contrast to the "rich get richer" scenario.<br />
So far, these methods have allowed to give some insight<br />
into realms outsi<strong>de</strong> of physics proper. I am convinced that<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
The structuring of words in a dictionary.<br />
<br />
<br />
<br />
<br />
<br />
this outreach has an interesting future, and will penetrate<br />
further new domains.<br />
Where does all this lead? The studies I have presented all<br />
use only the topology of the network, but never the metrics,<br />
namely the way some real-life networks are embed<strong>de</strong>d in<br />
the space in which we live. Adding this component opens<br />
new possibilities, especially in studying aspects of life. This<br />
is so because many aspects of life are about spatial connections,<br />
organisms are a linked set of individual units that<br />
have to interact well and "intelligently" in or<strong>de</strong>r to function.<br />
It is too early to make strong methodological statements<br />
about how mathematics and physics can p<strong>la</strong>y a role in<br />
studying such problems, but certainly, a few studies on<br />
neuronal networks [6, 17], or the interaction of ants in colonies<br />
[11, 15] seem to me promising beginnings in <strong>de</strong>veloping<br />
a methodology for studies in living systems.<br />
References<br />
[1] R. Albert and A.-L. Barabási. Statistical mechanics of complex<br />
networks. Rev. Mo<strong>de</strong>rn Phys. 74 (2002), 47–97.<br />
[2] A.-L. Barabási and R. Albert. Emergence of scaling in random<br />
networks. Science 286 (1999), 509–512.<br />
[3] B. Bollobás. Random graphs, volume 73 of Cambridge Studies<br />
in Advanced Mathematics (Cambridge: Cambridge University<br />
Press, 2001), second edition.<br />
[4] A. Dembo and A. Montanari. Ising mo<strong>de</strong>ls on locally tree-like<br />
graphs. Ann. Appl. Probab. 20 (2010), 565–592.<br />
[5] B. Dorow, D. Widdows, K. Ling, J.-P. Eckmann, D. Sergi, and<br />
E. Moses. Using curvature and Markov clustering in graphs for<br />
lexical acquisition and word sense discrimination. In: MEAN-<br />
ING-2005, 2nd Workshop organized by the MEANING Project,<br />
February 3rd-4th 2005, Trento, Italy. (2005).<br />
[6] J.-P. Eckmann, O. Feinermann, L. Gruendlinger, E. Moses,<br />
J. Soriano, and T. Tlusty. The physics of living neural networks.<br />
Physics Reports 449 (2007), 54–76.<br />
[7] J.-P. Eckmann and E. Moses. Curvature of co-links uncovers<br />
hid<strong>de</strong>n thematic <strong>la</strong>yers in the World Wi<strong>de</strong> Web. Proc. Natl. Acad.<br />
Sci. USA 99 (2002), 5825–5829 (electronic).<br />
[8] J.-P. Eckmann, E. Moses, and D. Sergi. Entropy of dialogues<br />
creates coherent structures in e-mail traffic. Proc. Natl. Acad. Sci.<br />
USA 101 (2004), 14333–14337 (electronic).<br />
[9] D. Harper. Online Etymology Dictionary. (2010).<br />
[10] D. Levary, J.-P. Eckmann, E. Moses, and T. Tlusty. Loops and<br />
self-reference in the construction of dictionaries. Phys. Rev. X 2<br />
(2012), 031018.<br />
[11] D. P. Mersch, A. Crespi, and L. Keller. Tracking individuals<br />
shows spatial fi<strong>de</strong>lity is a key regu<strong>la</strong>tor of ant social organization.<br />
Science 340.<br />
[12] M. Newman, A.-L. Barabási, and D. J. Watts, eds. The structure<br />
and dynamics of networks. Princeton Studies in Complexity<br />
(Princeton, NJ: Princeton University Press, 2006).<br />
[13] C. Og<strong>de</strong>n. Basic English: a general introduction with rules and<br />
grammar (Kegan Paul, London, 1930).<br />
[14] L. Onsager. Nobel lecture, The motion of ions: Principles and<br />
concepts. In: Nobel Lectures (December 11, 1968).<br />
[15] N. Razin, J.-P. Eckmann, and O. Feinerman. Desert ants<br />
achieve reliable recruitment across noisy interactions. J. Royal<br />
Soc. Interface 10 (2013) 20130079.<br />
[16] S. Shen-Orr, R. Milo, S. Mangan, and U. Alon. Network motifs<br />
in the transcriptional regu<strong>la</strong>tion network of Escherichia coli. Nature<br />
Genetics 31 (2002), 64–68.<br />
[17] T. Tlusty and J.-P. Eckmann. Remarks on bootstrap perco<strong>la</strong>tion<br />
in metric networks. J. Phys. A 42 (2009), 205004, 11.<br />
[18] D. Watts and S. Strogatz. Collective dynamics of 'small-world'<br />
networks. Nature 393 (1998), 409–410.<br />
31
SPG Mitteilungen Nr. 40<br />
Progress in Physics (34)<br />
On the <strong>de</strong>velopment of physically-based regional climate mo<strong>de</strong>lling<br />
Stéphane Goyette<br />
Institute for Environmental Sciences, University of Geneva, 7 route <strong>de</strong> Drize, Geneva<br />
There are huge scientific and technical challenges in research<br />
directed towards un<strong>de</strong>rstanding climate and climate<br />
change. No clear picture of how the weather and climate<br />
system works emerged prior to the 20 th century because<br />
of the <strong>la</strong>ck of connection between atmospheric variables.<br />
In fact, there was still some doubt about <strong>de</strong>riving a theory<br />
about how to interpret daily weather patterns, general circu<strong>la</strong>tion<br />
of the atmosphere, and the global climate. Atmospheric<br />
physics reached a <strong>la</strong>ndmark in the early 20 th century<br />
when empirical climatology, theoretical meteorology and<br />
forecasting were about to converge into a conceptualisation<br />
of this "vast machine" (Edwards, 2010). The problem of<br />
un<strong>de</strong>rstanding the causes of weather, climate and climate<br />
change is not one to be solved quickly or easily, but contributing<br />
to its solution is particu<strong>la</strong>rly worthwhile. In fact, the<br />
status of the climate results from the complex interactions<br />
between the atmosphere with the physical and biological<br />
systems which bound it - the <strong>la</strong>kes and oceans, ice sheets,<br />
<strong>la</strong>nd and vegetation through a spectrum of temporal and<br />
spatial scales. These elements all <strong>de</strong>termine the state and<br />
the evolution of the Earth’s weather and climate, owing to<br />
a particu<strong>la</strong>r influence of the general circu<strong>la</strong>tion of the atmosphere<br />
which redistributes energy, along with the ocean<br />
currents, from the Tropics to the Poles. This highly-coupled<br />
system presents a genuine challenge for mo<strong>de</strong>llers, and<br />
this has led to a body of literature which <strong>de</strong>tails the range<br />
and hierarchy of numerical climate mo<strong>de</strong>ls (e.g. Trenberth,<br />
1996, Schlesinger, 1988).<br />
Back in 1904, Vilhelm Bjerknes recognised that a physically-based<br />
weather forecast is a fundamental initial-value<br />
problem in the mathematical sense; this was <strong>la</strong>ter c<strong>la</strong>ssified<br />
as predictability of the first kind according to Lorenz (1975).<br />
The foundation of what became a framework of studying<br />
the geophysical fluid motions in or<strong>de</strong>r to predict the state<br />
of the atmosphere was shaping up. The <strong>de</strong>rivation of the<br />
equations of motion began in the 17 th century with Newton’s<br />
Laws of Motion, which were <strong>la</strong>ter applied for fluid flow<br />
purposes by Euler and Bernoulli in the 18 th century. The<br />
mo<strong>de</strong>rn conservation of momentum formu<strong>la</strong>tion consists<br />
of a form of the Navier–Stokes equations, an extension of<br />
Euler’s (but for viscous flow), that <strong>de</strong>scribe hydrodynamical<br />
flow. A continuity equation, also accredited to Euler, represents<br />
the conservation of mass. Hadley in 1735, and Ferrel,<br />
around 1850, showed that the <strong>de</strong>flection of rising warm air<br />
is due to the Coriolis effect, a force that began to be used in<br />
connection with meteorology in the early 20 th century. The<br />
first <strong>la</strong>w of thermodynamics, a version of the <strong>la</strong>w of conservation<br />
of energy, was codified near the end of the 19 th century<br />
by a number of scientists, but the first full statements<br />
of the <strong>la</strong>w came earlier from C<strong>la</strong>usius and Rankine. This led<br />
to the thermal energy equation re<strong>la</strong>ting the overall temperature<br />
of the system to heat sources and sinks. The gas state<br />
variables were re<strong>la</strong>ted in 1834 when, C<strong>la</strong>peyron combined<br />
Boyle’s Law and Charles’ <strong>la</strong>w into the first statement of the<br />
i<strong>de</strong>al Gas Law. The basic ingredients employed to approximate<br />
atmospheric flow were then gathered to progress<br />
from concepts to operational computer forecasting, thus<br />
aiming at representing weather by numbers (Harper, 2008).<br />
The partitioning of the atmospheric fluid into a dry and water<br />
vapour mixture, according to the Dalton’s <strong>la</strong>w, was <strong>la</strong>ter<br />
inclu<strong>de</strong>d in numerical mo<strong>de</strong>ls; this premise led to a genuine<br />
improvement when the water cycle and its associated energy<br />
exchange was introduced as an extra equation, <strong>de</strong>scribing<br />
the transport of water vapour handling the effects of<br />
changes of water phases for calcu<strong>la</strong>ting precipitation. All of<br />
the above form the basic equations used today for weather<br />
forecasting and climate prediction. The conservation equations<br />
are partial differential equations. For a unit mass, with<br />
a frame of reference attached to the Earth and the origin at<br />
its centre, these equations may be written as follows (e.g.<br />
Washington and Parkinson, 1986, Hen<strong>de</strong>rson-Sellers and<br />
McGuffie, 1987, Jacobson, 1998, Coiffier, 2011):<br />
dV<br />
=-2X<br />
# V -<br />
1<br />
dp<br />
- dU<br />
+ F momentum equation (1)<br />
dt<br />
t<br />
dT dp<br />
=<br />
1<br />
c + Q m<br />
dt c p dt<br />
thermodynamic equation (2)<br />
dt<br />
=- td $ V<br />
dt<br />
continuity equation (3)<br />
dq<br />
dt<br />
p<br />
= M<br />
water vapour equation (4)<br />
= tRT<br />
equation of state (5)<br />
which gives us a set of seven equations with seven unknowns,<br />
where V represents the three-dimensional wind<br />
velocity, T is the air temperature, p is the pressure, q is<br />
the specific humidity, and t is the air <strong>de</strong>nsity, all varying in<br />
space and in time. The other quantities are: X is the angu<strong>la</strong>r<br />
of rotation of the Earth, is the geopotential <strong>de</strong>fined as<br />
the product of geometric height above the surface z by the<br />
acceleration due to gravity g, (the <strong>la</strong>tter including the Newtonian<br />
gravity and the centrifugal acceleration), R and c p<br />
are<br />
the specific gas constant and the specific heat at constant<br />
pressure, and t is the time. F, Q and M represent the sources<br />
and sinks of momentum (e.g. frictional forces), heat (e.g.<br />
so<strong>la</strong>r and infrared radiation, and <strong>la</strong>tent heat release) and<br />
moisture (e.g. evaporation and con<strong>de</strong>nsation), respectively,<br />
and their expression <strong>de</strong>pends on the scale of the atmospheric<br />
motion the mo<strong>de</strong>l aims to <strong>de</strong>scribe, and they represent<br />
subgrid-scale processes commonly expressed in<br />
terms of resolved quantities. In the prognostic equations<br />
(1-4), the <strong>de</strong>rivative of any sca<strong>la</strong>r quantities } with respect<br />
to time taken following the fluid is expressed as<br />
d} 2}<br />
= + V $ d}<br />
(6)<br />
dt 2t<br />
where the first term on the right is a local partial <strong>de</strong>riva-<br />
32
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
tive at a fixed point in the chosen frame of reference and<br />
the second the advection of the same quantity. Advection<br />
that induces non-linear effects is a transport mechanism of<br />
a quantity by a fluid due to its bulk motion. Simplification<br />
and transformation are required in or<strong>de</strong>r to resolve for some<br />
analytical solutions or the numerical methods used to seek<br />
numerical solutions. The discretization of these continuous<br />
equations would ren<strong>de</strong>r them amenable, using appropriate<br />
algorithms, to a numerical solution of the continuous behaviour<br />
of the circu<strong>la</strong>ting atmosphere.<br />
Around 1920, Richardson, who may be consi<strong>de</strong>red as the<br />
father of today’s mo<strong>de</strong>ls for weather and climate, tried to<br />
solve a simplified set of equations using numerical methods<br />
"by hand and step-by-step". However, his 6-hour<br />
"retrospective forecast" proved unrealistic. Computational<br />
instability and imba<strong>la</strong>nce in the initial data set were <strong>la</strong>ter<br />
found to be the cause of this "setback". However, in 1928,<br />
Courant, Friedrichs, and Lewy showed that a time step<br />
must be less than a certain value in explicit time-marching<br />
schemes to warrant stable numerical solutions using the<br />
method of finite differences. Then, Richardson realised that<br />
64’000 computers [human automata] would be nee<strong>de</strong>d to<br />
race the weather for the whole globe, but by the time he<br />
published "Weather Prediction by Numerical Process" in<br />
1922, fast computers were unavai<strong>la</strong>ble. The <strong>de</strong>velopment<br />
of complex mo<strong>de</strong>ls remained dormant until the <strong>de</strong>velopment<br />
of electronic computers handling self-programmed<br />
sequences of instructions. In 1950, Charney, Ragnar Fjörtoft,<br />
and von Neumann ma<strong>de</strong> the first numerical weather<br />
prediction (NWP) using "simplified" equations to represent<br />
<strong>la</strong>rge-scale eddy motion. This accomplishment then fostered<br />
the <strong>de</strong>velopment of more complex prediction mo<strong>de</strong>ls<br />
of even greater spatial resolution, allowing small scales of<br />
motion to be resolved. In 1956, Phillips <strong>de</strong>veloped a mo<strong>de</strong>l<br />
which could realistically <strong>de</strong>pict monthly and seasonal patterns<br />
in the troposphere, which became the first successful<br />
climate mo<strong>de</strong>l. Following Phillips’ work, several groups<br />
began working out General Circu<strong>la</strong>tion Mo<strong>de</strong>ls (GCMs) of<br />
the atmosphere of increasing complexities, including the<br />
effects of sub-systems such as these induced by oceans.<br />
The challenge of numerical mo<strong>de</strong>ls is to run forward in time<br />
much faster than the real atmosphere and oceans with<br />
avai<strong>la</strong>ble electronic computers. To do this, they must make<br />
a <strong>la</strong>rge number of simplifying assumptions. Although there<br />
have been great advances ma<strong>de</strong> in the discipline of climate<br />
mo<strong>de</strong>lling over the <strong>la</strong>st fifty years, the most sophisticated<br />
mo<strong>de</strong>ls remain very much simpler than that of the full climate<br />
system (McGuffie and Hen<strong>de</strong>rson-Sellers, 2001).<br />
The first atmospheric general circu<strong>la</strong>tion mo<strong>de</strong>l applied<br />
for long-term integrations, were <strong>de</strong>rived directly from numerical<br />
mo<strong>de</strong>ls <strong>de</strong>signed for short-term numerical weather<br />
forecasting, which did not have a global coverage at this<br />
time. Then, the advance of computing technologies, along<br />
with the requirements of weather predictions needing hemispheric<br />
or even global computational domains, the longer<br />
integration periods became a matter of avai<strong>la</strong>bility of computer<br />
resources. The early climate mo<strong>de</strong>l grid spacing was<br />
very coarse in the horizontal and vertical dimensions. The<br />
evolution towards greater resolution and increased complexity<br />
has been the rule since. This has been facilitated<br />
by the avai<strong>la</strong>bility of <strong>la</strong>rge computing technologies and<br />
by new algorithms and numerical methods thus allowing<br />
longer numerical time-stepping (Mote and O’Neil, 2000). To<br />
this day, climate mo<strong>de</strong>lling and weather forecasting groups<br />
co-exist, but the needs and focus of the two disciplines<br />
differ. For climate mo<strong>de</strong>lling, long-term mass, energy and<br />
moisture conservation is an important issue. This may thus<br />
be consi<strong>de</strong>red as a fundamental boundary-value problem<br />
in the mathematical sense, c<strong>la</strong>ssified as predictability of<br />
the second kind according to Lorenz (1975). Not all climate<br />
mo<strong>de</strong>ls originated from weather forecast mo<strong>de</strong>ls, however.<br />
Simpler mo<strong>de</strong>ls based on global energy conservation are<br />
collectively called Energy Ba<strong>la</strong>nce Mo<strong>de</strong>ls, or EBMs (Hen<strong>de</strong>rson-Sellers<br />
and McGuffie, 1987). They take into account<br />
the different forms of energy driving the climate system and<br />
look for a steady state solution for the surface temperature.<br />
Their main advantage is that they can be extensively used<br />
to do sensitivity studies of the role of external forcing on the<br />
surface temperature (that of the greenhouse gases, of the<br />
Earth’s orbital parameters in the very long term, the impacts<br />
of volcanic eruptions, etc.), which can thus be investigated<br />
at a low computational cost. However, the atmospheric circu<strong>la</strong>tion<br />
is not explicitly resolved so they cannot be used<br />
neither to forecast daily conditions nor the general circu<strong>la</strong>tion<br />
of the atmosphere.<br />
During the early days of weather forecasting, the computational<br />
domains were restricted to an area of interest. These<br />
Limited Area Mo<strong>de</strong>ls (LAMs) were <strong>de</strong>veloped to enable<br />
short range predictions to be ma<strong>de</strong> over a <strong>la</strong>rge domain.<br />
Their major drawback is that flow field values have to be<br />
specified at the area boundary for each time step. Later on,<br />
to overcome this problem, these field values were interpo<strong>la</strong>ted<br />
from those obtained from a global <strong>la</strong>rger-scale mo<strong>de</strong>l.<br />
This technique has led to "nested mo<strong>de</strong>ls" that are the basis<br />
of operational prediction systems in most meteorological<br />
services. Following the pioneering work in the U.S. in<br />
the 1980s (e.g. Giorgi et al., 1989), the approach, consisting<br />
of driving a high resolution LAM <strong>la</strong>teral boundaries with<br />
low-resolution GCM flow fields, entered the scene (Laprise,<br />
2008). In practice, one or<strong>de</strong>r of magnitu<strong>de</strong> in resolution can<br />
be gained with this approach, so the small-scale structures<br />
of atmospheric circu<strong>la</strong>tion can be reproduced. One advantage<br />
of such a LAM is that it can also be driven by atmospheric<br />
reanalyses (data <strong>de</strong>rived from global observations<br />
using data assimi<strong>la</strong>tion schemes and mo<strong>de</strong>ls), rather than<br />
by GCM outputs; this feature is very convenient for <strong>de</strong>velopment<br />
and validation purposes. When LAMs are applied<br />
to long time scales, they are referred to as Regional Climate<br />
Mo<strong>de</strong>ls (RCMs). They are now exploited in a number of research<br />
centres around the world and used in a wi<strong>de</strong> range of<br />
climate applications, from pa<strong>la</strong>eoclimate to anthropogenic<br />
climate change studies (IPCC, 2007). The <strong>de</strong>velopment and<br />
application of such numerical tools has been motivated by<br />
the needs of assessing what the impact of global climate<br />
will be in different regions. This downscaling approach is<br />
very versatile since RCMs are locatable in any part of the<br />
world. Moreover, simu<strong>la</strong>ting climate and climate change at<br />
the regional and national levels is of paramount importance<br />
for policymaking. Any regional climate mo<strong>de</strong>lling approach<br />
affords focusing over an area of the globe with a regional<br />
grid-point spacing of a few tens of kms in the horizontal, for<br />
operational use on climate timescales. Furthermore, even<br />
when the increase of computing power will permit the operational<br />
use of GCMs at a resolution of a few tens of km,<br />
33
SPG Mitteilungen Nr. 40<br />
Global reanalysis (~ 2.5° x 2.5°) or GCM simu<strong>la</strong>ted outputs<br />
20-km RCM<br />
2-km<br />
RCM<br />
Figure 1. Regional climate mo<strong>de</strong>ls self-nesting methodology<br />
indicating two computational domains onto<br />
which simu<strong>la</strong>tions are performed. Starting with low<br />
resolution GCM outputs or global reanalysis, the finegrain<br />
<strong>de</strong>tails of the flow fields are downscaled in a<br />
step-wise manner to 2 km grid-spacing. The intermediate<br />
5-km RCM domain has been omitted for better<br />
c<strong>la</strong>rity. The re<strong>la</strong>tive humidity, represented in colour<br />
sha<strong>de</strong>s, is meant to show how the increase in the horizontal<br />
resolution impacts on the reproduction of these<br />
small scale <strong>de</strong>tails.<br />
the RCM approach could still be useful, allowing reaching<br />
resolution of a few kms for a simi<strong>la</strong>r computational load. In<br />
principle, specific physical parameterizations for the sources<br />
and sinks of momentum, heat and moisture, respectively<br />
F, Q and M as <strong>de</strong>picted in Eqs (1) - (2), and (4) are scale<br />
<strong>de</strong>pen<strong>de</strong>nt. In the historical <strong>de</strong>velopment of RCMs, these<br />
parameterisations often benefited from packages coming<br />
from either NWPs or from GCMs. Improvements to existing<br />
schemes and also new <strong>de</strong>velopments were nevertheless<br />
<strong>de</strong>emed necessary. This enables RCMs to be applied<br />
to a <strong>la</strong>rge range of atmospheric flows. This downscaling<br />
technique can be further exten<strong>de</strong>d to finer <strong>de</strong>tail with the<br />
casca<strong>de</strong> self-nesting capability as shown in Fig 1 (Goyette<br />
et al., 2001). The enhancement of horizontal resolution,<br />
also prompted for on the specification of surface boundary<br />
conditions as a sizeable portion of the performance of<br />
RCMs relies on the surface forcing not captured by GCMs.<br />
Their success <strong>de</strong>pends on their ability to respond to these<br />
forcing factors in a realistic manner in space and time. An<br />
important surface forcing not captured by GCMs (Fig 2.)<br />
which has received much attention <strong>la</strong>tely is the regional influence<br />
of in<strong>la</strong>nd water bodies (Goyette et al., 2000). Also,<br />
much attention is being paid to the capability of RCMs to<br />
reproduce extreme events. Wind gusts are fundamental<br />
characteristics of the variability of wind climate; physicallybased<br />
parameterization to simu<strong>la</strong>te gusts has been <strong>de</strong>veloped<br />
to better capture the effects of extremes associated<br />
with these features (Goyette et al., 2003).<br />
There is also a need for future climate projection at local and<br />
regional scales. In addition, climate mo<strong>de</strong>ls, either global or<br />
regional, are constantly improved so as to inclu<strong>de</strong> stateof-the-art<br />
numerical schemes, physical parameterizations,<br />
new scenarios for greenhouse gas forcing, etc. to warrant<br />
realistic simu<strong>la</strong>tions at an ever-increasing spatial resolution.<br />
For example, the European project "PRUDENCE" was<br />
34
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
20-km RCM<br />
2-km<br />
RCM<br />
Figure 2. Surface topography prescribed as a lower boundary<br />
condition in a 20- and a 2-km RCM. Local weather and climate<br />
are significantly influenced by local topographical features such as<br />
mountains. Small-scale topographical features are not resolved by<br />
GCMs neither by low resolution RCMs (e.g. 20-km RCM) due to<br />
the coarse resolution of their computational grids.<br />
aimed at quantifying confi<strong>de</strong>nce and uncertainties in predictions<br />
of future European climate and its impacts using a<br />
suite of high resolution RCMs driven by a coarser resolution<br />
GCM (Christensen et al., 2002).<br />
Ultra-high climate simu<strong>la</strong>tions, i.e. 30 years or more with an<br />
horizontal grid spacing on the or<strong>de</strong>r of one kilometre, is not<br />
foreseen in the near future due to as yet ina<strong>de</strong>quate computational<br />
resources. Some specific case studies using RCMs<br />
with 2 and even 1 km grid spacing have been carried out<br />
for short term integrations to test the downscaling ability of<br />
such an approach (Goyette, 2001). The analysis has shown<br />
that the mo<strong>de</strong>l cannot overcome the massive increase in<br />
resolution from coarse resolution GCM or reanalysis data<br />
down to these fine scales without introducing intermediate<br />
steps (Fig 1). The casca<strong>de</strong> self-nesting method requires, for<br />
long-term simu<strong>la</strong>tions, that the ratio between successive<br />
grid meshes should range between 3 and 5 to avoid numerical<br />
inconsistencies. However, 2.2-km numerical weather<br />
predictions do exist and this mo<strong>de</strong>l is particu<strong>la</strong>rly aimed at<br />
assisting in short-term local forecasting, showing skill for<br />
a 24-h forecast (COSMO 1 ). Much research remains to be<br />
done, <strong>de</strong>spite all the post World War II achievements. There<br />
are still many scientific and technical challenges in weather<br />
and climate research, and contributing to these innovations<br />
and findings is in<strong>de</strong>ed worthwhile.<br />
1 www.meteosuisse.admin.ch/web/fr/meteo/previsions_numeriques/<br />
cosmo.html<br />
References<br />
Coiffier, J.: Fundamentals of numerical weather prediction. Cambridge<br />
University Press, Cambridge 2011, 340 pp.<br />
Charney, J., R. Fjørtoft, J. von Neumann, 1950: Numerical Integration<br />
of the Barotropic Vorticity Equation. Tellus, 2, 237-254.<br />
Christensen, J. H., T. Carter, F. Giorgi, 2002: PRUDENCE Employs<br />
New Methods to Assess European Climate Change, EOS, 83,<br />
147.<br />
Courant, R., Friedrichs, K., Lewy, H., 1928: "Über die partiellen<br />
Differenzengleichungen <strong>de</strong>r mathematischen Physik", Mathematische<br />
Annalen, 100 (1), 32–74.<br />
Edwards, P.: A vast machine: Computer mo<strong>de</strong>ls, climate data, and<br />
the politics of global warming. MIT Press, Cambridge, 2010,<br />
518 pp.<br />
Giorgi. F, and G.T. Bates, 1989: The climatological skill of a regional<br />
mo<strong>de</strong>l over complex terrain, Mon. Weather Rev. 11,<br />
2325–2347.<br />
Goyette, S, O. Brasseur, and M. Beniston, 2003: Application of<br />
a new wind gust parameterisation. Multi-scale case studies<br />
performed with the Canadian RCM. J. of Geophys. Res., 108,<br />
4374-4390.<br />
Goyette, S., M. Beniston, D. Caya, J. P. R. Laprise, and P. Jungo,<br />
2001: Numerical investigation of an extreme storm with the<br />
Canadian Regional Climate Mo<strong>de</strong>l: The case study of windstorm<br />
VIVIAN, Switzer<strong>la</strong>nd, February 27, 1990. Clim. Dyn., 18,<br />
145 - 178.<br />
Goyette, S., N. A. McFar<strong>la</strong>ne, and G. M. F<strong>la</strong>to, 2000: Application<br />
of the Canadian Regional Climate Mo<strong>de</strong>l to the Laurentian<br />
Great Lakes region: Implementation of a <strong>la</strong>ke mo<strong>de</strong>l. Atmos.-<br />
Ocean, 38, 481 - 503.<br />
Harper, K. J.: Weather by the numbers: The genesis of mo<strong>de</strong>rn<br />
meteorology. MIT Press 2008, 308 pp.<br />
Hen<strong>de</strong>rson-Sellers, A, and K. McGuffie: A climate mo<strong>de</strong>lling primer.<br />
Wiley, Chichester, 2006, 296 pp.<br />
IPCC 2007, Solomon, S., D. Qin, M. Manning, Z. Chen, M. Marquis,<br />
K. B. Averyt, M. Tignor and H. L. Miller (eds.). Contribution<br />
of Working Group I to the Fourth Assessment Report of<br />
the Intergovernmental Panel on Climate Change. Cambridge<br />
University Press, Cambridge, United Kingdom and New York,<br />
NY, USA, 996 pp.<br />
Jacobson, M. Z.: Fundamentals of atmospheric mo<strong>de</strong>lling. Cambridge<br />
University Press, Cambridge 1998, 828 pp.<br />
Laprise, R, 2008: Regional climate mo<strong>de</strong>lling. J. Comput. Phys,<br />
227, 3641-3666.<br />
Lorenz, E. N.: Climate predictability. In: The Physical Basis of Climate<br />
and Climate Mo<strong>de</strong>lling, WMO GARP Publ. Ser. No. 16,<br />
1975, 265 pp.<br />
McGuffie, K, and A. Hen<strong>de</strong>rson-Sellers, 2001: Forty years of numerical<br />
climate mo<strong>de</strong>lling. Int. J Climatol., 12, 1067 - 1109.<br />
Mote, P., and A. O’Neill, Numerical Mo<strong>de</strong>ling of the Global Atmosphere<br />
in the Climate System. Kluwer Aca<strong>de</strong>mic Publishers<br />
2000, Boston, Massachusetts, 517 pp.<br />
Phillips, N. A., 1956: The general circu<strong>la</strong>tion of the atmosphere:<br />
a numerical experiment. Quart. J. Roy. Meteor. Soc. 82, 123–<br />
154.<br />
Richardson, L. F.: Weather prediction by numerical processes.<br />
Cambridge University Press (reprinted by Dover Publications,<br />
1966), 236 pp.<br />
Schlesinger, M (ed.): Physically-based mo<strong>de</strong>lling and simu<strong>la</strong>tion of<br />
climate and climatic change - Part 1 and 2, Nato ASI Series C,<br />
No 243,Kluwer Aca<strong>de</strong>mic Publisher, Dordrecht 1988, 1084 pp.<br />
Washington, W., and C. Parkinson: An introduction to three-dimensional<br />
climate mo<strong>de</strong>ling. University Science books, 1986,<br />
Mill Valley, CA, 322 pp.<br />
WMO, The World Meteorological Organisation: The physical basis<br />
of climate and climate mo<strong>de</strong>lling. Garp Publication series No<br />
16, WMO/ICSU, Geneva 1975, 265 pp.<br />
35
SPG Mitteilungen Nr. 40<br />
Progress in Physics (35)<br />
A snowf<strong>la</strong>ke in a million <strong>de</strong>gree p<strong>la</strong>sma<br />
Y. Martin, B. Labit, H. Reimer<strong>de</strong>s, W. Vijvers<br />
CRPP, EPFL, Association EURATOM – Confédération Suisse, CH-1015 Lausanne<br />
Introduction<br />
Fusion is the energy that powers the stars. Harnessing fusion<br />
on Earth would offer the world almost inexhaustible,<br />
environmentally clean and safe energy, see box 1. Research<br />
and <strong>de</strong>velopment performed during a few <strong>de</strong>ca<strong>de</strong>s already<br />
brought significant results. In the domain of magnetic confinement,<br />
for instance, 16MW of fusion power have been<br />
produced in the JET tokamak [1] in 1997. Since then an<br />
international col<strong>la</strong>boration was set to build the next step<br />
<strong>de</strong>vice, ITER 1 , the first fusion reactor that would <strong>de</strong>liver<br />
500 MW of fusion power, 10 times the power injected into<br />
the <strong>de</strong>vice, see box 2. Recently, the European fusion scientists,<br />
un<strong>de</strong>r the banner of European Fusion Development<br />
Agreement 2 (EFDA), <strong>de</strong>veloped and published a roadmap 3<br />
that <strong>de</strong>scribes the steps and the challenges to achieve the<br />
production of electricity from fusion before 2050, see box<br />
3. The steps consist in completing the construction of ITER,<br />
operating ITER, <strong>de</strong>signing, building and operating DEMO, a<br />
prototype reactor that would provi<strong>de</strong> the electrical network<br />
1 ITER: www.iter.org<br />
2 EFDA: www.efda.org<br />
3 Fusion roadmap: http://www.efda.org/efda/activities/the-road-tofusion-electricity/<br />
with several hundreds of MW. The roadmap is divi<strong>de</strong>d into<br />
8 missions, including the 'heat exhaust' issue: if one extrapo<strong>la</strong>tes<br />
from the present <strong>de</strong>vices to a reactor gra<strong>de</strong> <strong>de</strong>vice,<br />
the heat flux <strong>de</strong>nsity produced by particles escaping<br />
from the p<strong>la</strong>sma would reach levels that may exceed the<br />
material capabilities. To mitigate the heat flux impact several<br />
strategies are proposed. One of these strategies aims<br />
at the exploration of the so-called snowf<strong>la</strong>ke configuration.<br />
The scientists of the CRPP-EPFL were the first to realise a<br />
snowf<strong>la</strong>ke configuration in a tokamak, thanks to the high<br />
shaping capability of the TCV tokamak but especially to<br />
the hard work of these <strong>de</strong>dicated scientists. It should be<br />
emphasized that this work was subsequently awar<strong>de</strong>d the<br />
R&D100 prize in 2012 4 . This paper presents the achieved<br />
snowf<strong>la</strong>ke configuration and its advantages with respect to<br />
heat exhaust.<br />
P<strong>la</strong>sma configuration<br />
The TCV tokamak is equipped with 16 in<strong>de</strong>pen<strong>de</strong>ntly driven<br />
poloidal field coils that are used for shaping the p<strong>la</strong>sma.<br />
Depending on the combination of coil currents, the p<strong>la</strong>s-<br />
4 R&D magazine: http://www.rdmag.com/award-winners/2012/08/highperformance-tokamak-exhaust<br />
Fusion<br />
The fusion of hydrogen isotopes, <strong>de</strong>uterium and tritium,<br />
is the easiest reaction that could be implemented<br />
on Earth, because of its higher cross section at a lower<br />
temperature than other possible reactions.<br />
Temperatures of about 100 MºC must be achieved<br />
so that fusion power becomes exploitable. Before<br />
reaching these temperatures, a gas turns to p<strong>la</strong>sma<br />
wherein particles are ionised.<br />
Magnetic fields then provi<strong>de</strong> a good way to gui<strong>de</strong> the<br />
ionised particles.<br />
The most attractive magnetic confinement <strong>de</strong>vice so<br />
far is the tokamak, a toroidal <strong>de</strong>vice wherein a poloidal<br />
field, induced by a toroidal current, is superimposed to<br />
a toroidal magnetic field to form the magnetic structure<br />
that gui<strong>de</strong>s and maintains the p<strong>la</strong>sma away from the<br />
vacuum vessel walls. In addition poloidal field coils are<br />
used to shape the p<strong>la</strong>sma.<br />
To reach the required temperatures, the p<strong>la</strong>sma is heated<br />
by either energetic neutral particles or by microwaves<br />
<strong>de</strong>livering their power in the p<strong>la</strong>sma through<br />
different possible resonant schemes.<br />
The CRPP-EPFL tokamak, called TCV 1 for 'Tokamak<br />
à Configuration Variable' has a high shaping capability<br />
and an Electron Cyclotron Heating (ECH) system of 4.5<br />
MW.<br />
Figure: The CRPP-EPFL Tokamak à Configuration Variable (TCV).<br />
Cyan: vacuum vessel; green: main toroidal field coils; orange:<br />
poloidal field coils (for p<strong>la</strong>sma current induction and p<strong>la</strong>sma shaping);<br />
yellow: microwave <strong>la</strong>unchers; pink: p<strong>la</strong>sma. TCV diameter:<br />
3.3m<br />
1 http://crpp.epfl.ch/research_TCV<br />
36
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
ma either lies against the carbon tile covered wall of the<br />
vacuum vessel, the so-called limited configuration, or is<br />
fully <strong>de</strong>tached from the wall thanks to the presence of a null<br />
point in the poloidal field (X-point) and the resulting separatrix<br />
that <strong>de</strong>limits the p<strong>la</strong>sma as shown in Fig. 1. In the<br />
<strong>la</strong>tter configuration, the so-called divertor configuration, the<br />
p<strong>la</strong>sma is not in immediate contact with the wall. Particles<br />
that escape from the p<strong>la</strong>sma are diverted towards the vessel<br />
wall, along the 'separatrix legs', towards a more remote<br />
position than in the limited configuration. In addition, the<br />
journey of particles escaping from a diverted p<strong>la</strong>sma is particu<strong>la</strong>rly<br />
long because the low value of the poloidal field in<br />
the vicinity of the X-point leads to almost entirely toroidal<br />
trajectories. For these reasons, higher performances can<br />
be achieved in diverted p<strong>la</strong>smas, making this configuration<br />
most suitable for fusion reactors.<br />
However, those escaping particles may damage the surface<br />
of the divertor because they <strong>de</strong>posit their significant<br />
energy on a re<strong>la</strong>tively small area leading to unacceptably<br />
high heat flux <strong>de</strong>nsities. The snowf<strong>la</strong>ke configuration has<br />
been proposed as a potential solution to mitigate the strong<br />
heat flux in the divertor.<br />
and SF-, reflecting the excess or <strong>la</strong>ck of current flowing in<br />
the conductors, respectively. The distance between the two<br />
X-points, indicated by the green crosses, normalized by the<br />
minor radius of the p<strong>la</strong>sma torus, is used as the measure,<br />
<strong>de</strong>noted s, of the proximity to the perfect snowf<strong>la</strong>ke.<br />
SF+ SF SF-<br />
I d1<br />
I p<br />
(a) ( b ) ( c)<br />
Figure 2: Schematic representation of a perfect snowf<strong>la</strong>ke configuration<br />
(b). Upper lobe represents the p<strong>la</strong>sma while the lower lobes<br />
encompass the current conductors. A small vertical disp<strong>la</strong>cement<br />
of the p<strong>la</strong>sma would generate the (a) or (c) configurations <strong>de</strong>pending<br />
of the direction of the disp<strong>la</strong>cement.<br />
I d2<br />
(a) SF+ (b) SF (c) SF-<br />
1<br />
1<br />
1<br />
#19421 t=2.2s<br />
#24239 t=0.37s<br />
2<br />
4<br />
2<br />
4<br />
2<br />
4<br />
Figure 1: Comparison of p<strong>la</strong>sma cross-sections in the limited (left,<br />
19421) and diverted (right, 24239) configurations. Also shown are<br />
the vessel and p<strong>la</strong>sma shaping coils cross-sections.<br />
Snowf<strong>la</strong>ke configuration<br />
A snowf<strong>la</strong>ke configuration is obtained when not only the<br />
poloidal field vanishes, as in the diverted configuration, but<br />
also its first <strong>de</strong>rivatives. This second or<strong>de</strong>r null implies that<br />
six separatrix sprout from the X-point instead of four for the<br />
diverted configuration, as shown in sketch (b) of Fig. 2. The<br />
name 'snowf<strong>la</strong>ke' comes from this 6-fold geometry. In the<br />
sketch, the upper lobe represents the p<strong>la</strong>sma enclosed in<br />
its separatrix while the lower lobes encompass two poloidal<br />
field coils. The vacuum vessel then cuts both lower lobes<br />
resulting in four separatrix legs instead of two. It directly<br />
reveals the advantage of such a configuration: the heat flux<br />
power may be diverted towards four sections of the vacuum<br />
vessel walls, thereby reducing the heat flux <strong>de</strong>nsities<br />
onto the divertor p<strong>la</strong>tes. If the configuration slightly <strong>de</strong>viates<br />
from the perfect snowf<strong>la</strong>ke shown in Fig. 2b, it produces the<br />
other configurations shown in Fig. 2. These variants of the<br />
snowf<strong>la</strong>ke configuration are <strong>la</strong>belled SF+ (snowf<strong>la</strong>ke plus)<br />
37<br />
1<br />
2<br />
3<br />
4<br />
1<br />
2<br />
3<br />
3 3<br />
3<br />
Figure 3: Equilibrium reconstruction and tangential views of the<br />
p<strong>la</strong>sma obtained with a CCD camera at three different times during<br />
a p<strong>la</strong>sma discharge in which the p<strong>la</strong>sma was vertically disp<strong>la</strong>ced<br />
to go through the variant configurations shown in Fig. 2.<br />
4<br />
1<br />
2<br />
3<br />
4
SPG Mitteilungen Nr. 40<br />
The snowf<strong>la</strong>ke configuration was proposed by Ryutov et al<br />
[2,3]. It was experimentally realised for the first time in the<br />
TCV tokamak at the CPPP-EPFL [4] and then reproduced in<br />
the NSTX spherical tokamak at the Princeton P<strong>la</strong>sma Physics<br />
Laboratory [5] and more recently in the DIII-D tokamak<br />
at General Atomics [6].<br />
Fig. 3 shows an example of a TCV discharge wherein the<br />
p<strong>la</strong>sma was vertically shifted to reveal the different snowf<strong>la</strong>ke<br />
configurations <strong>de</strong>scribed in the schematic representation<br />
(Fig. 2). The p<strong>la</strong>sma equilibrium reconstructions, based<br />
on magnetic measurements, are shown in the first row. The<br />
numbering 1-4 helps to i<strong>de</strong>ntify the regions where the separatrix<br />
legs reach the vacuum vessel walls. Locations 1 & 4<br />
are called primary locations since they correspond to the<br />
divertor legs of the traditional divertor configuration (field<br />
lines surrounding the p<strong>la</strong>sma hit the wall at the primary location).<br />
In opposition locations 2 & 3 are called secondary<br />
regions due to the absence of direct connection with the<br />
vicinity of the p<strong>la</strong>sma.<br />
The second row exhibits tangential views of the p<strong>la</strong>sma<br />
obtained with a CCD camera. Since most line radiation<br />
originates from re<strong>la</strong>tively "cold" p<strong>la</strong>sma, the measurement<br />
of the emitted visible light provi<strong>de</strong>s an excellent mean to<br />
locate the edge of the p<strong>la</strong>sma as well as the separatrix legs.<br />
This series of measurements shows a clear agreement between<br />
both information sources.<br />
In all three cases shown in Fig. 3, the emitted light clearly<br />
reveals that all separatrix become active. This suggests<br />
that the low poloidal field in the vicinity of the null point enhances<br />
the cross-field transport. If this transport were sufficiently<br />
<strong>la</strong>rge it could not only distribute the heat among four<br />
divertor legs instead of two, but also wi<strong>de</strong>n the power flux<br />
ITER<br />
ITER, currently un<strong>de</strong>r construction in the south of France,<br />
aims to <strong>de</strong>monstrate that fusion is an energy source of<br />
the future. ITER is a col<strong>la</strong>boration between European Union,<br />
including Switzer<strong>la</strong>nd, Japan, South Korea, China,<br />
India, Russia and United States.<br />
Main goals<br />
• Ratio of fusion power to input power <strong>la</strong>rger than 10<br />
(Q>10)<br />
• Fusion power up to 500 MW<br />
• Test of key technologies such as divertor materials<br />
and b<strong>la</strong>nket modules wherein neutrons will <strong>de</strong>liver<br />
their energy and breed tritium<br />
Main parameters<br />
• P<strong>la</strong>sma major & minor radii: 6.2 m & 2 m<br />
• Toroidal field: 5.3T<br />
• P<strong>la</strong>sma current: 15 MA<br />
• P<strong>la</strong>sma duration: 500 s<br />
Figure: ITER. Orange: divertor; dark blue: b<strong>la</strong>nket modules. ITER diameter: 28.6m<br />
38
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
channel at each leg and thereby further reduce the power<br />
flux <strong>de</strong>nsity onto material surfaces. Dedicated measurements<br />
were done in the most promising scenario for ITER:<br />
the H-mo<strong>de</strong>.<br />
H-mo<strong>de</strong> and snowf<strong>la</strong>kes<br />
In the early 1980's, tokamak experiments performed in<br />
diverted configuration revealed the existence of an operational<br />
regime wherein the confinement of particles and<br />
energy sud<strong>de</strong>nly increases by a factor of two [7]. It was<br />
called H-mo<strong>de</strong> regime (H for 'high') and has since been obtained<br />
in most tokamaks. By comparing results obtained<br />
in several <strong>de</strong>vices it was shown that the additional heating<br />
power should exceed a threshold that <strong>de</strong>pends on the<br />
p<strong>la</strong>sma <strong>de</strong>nsity, the p<strong>la</strong>sma size and the main toroidal field<br />
[8]. The improvement in the p<strong>la</strong>sma confinement properties<br />
observed in this H-mo<strong>de</strong> regime makes it the selected<br />
operational mo<strong>de</strong> for the ITER baseline scenario. Unfortunately,<br />
H-mo<strong>de</strong>s are generally accompanied with p<strong>la</strong>sma<br />
edge instabilities (ELM) that repeatedly release particles towards<br />
the divertor in sharp bursts that threaten the divertor<br />
material.<br />
H-mo<strong>de</strong>s are also regu<strong>la</strong>rly obtained and investigated in<br />
TCV diverted p<strong>la</strong>smas. Soon after the realisation of the<br />
first snowf<strong>la</strong>ke in TCV, efforts have been <strong>de</strong>dicated to the<br />
search for H-mo<strong>de</strong>s in snowf<strong>la</strong>ke configuration and results<br />
came soon: the access to the H-mo<strong>de</strong> regime occurs at approximately<br />
the same power as in the quadrupole diverted<br />
configuration. The confinement improvement is simi<strong>la</strong>r or<br />
even slightly better.<br />
Regarding the heat flux to the divertor, <strong>de</strong>dicated measurements<br />
were performed. The high pressure observed near<br />
Fusion electricity – EFDA roadmap<br />
European scientists established the necessary steps<br />
and challenges that should be solved in or<strong>de</strong>r to realise<br />
a fusion reactor that would provi<strong>de</strong> the electrical<br />
network with electricity before 2050.<br />
Steps<br />
• 2012-2020: Construction of ITER<br />
• 2020-2030: Exploitation of ITER<br />
• 2030-2050: Construction and exploitation of<br />
DEMO<br />
Challenges<br />
• P<strong>la</strong>sma regimes of operation<br />
• Heat exhaust<br />
• Neutron resistant materials<br />
• Tritium self-sufficiency<br />
• Integration of intrinsic safety features<br />
• Integrated DEMO <strong>de</strong>sign<br />
• Competitive cost of electricity<br />
• Stel<strong>la</strong>rator<br />
The roadmap to fusion electricity can be downloa<strong>de</strong>d<br />
from: http://www.efda.org/efda/activities/the-road-tofusion-electricity/<br />
the second or<strong>de</strong>r null even increased the cross-field transport<br />
re<strong>la</strong>tive to the conventional configuration. This resulted<br />
in an efficient distribution of the power on the secondary<br />
divertor regions as shown in Fig. 4. The power <strong>de</strong>posited<br />
onto the divertor tiles, measured in regions <strong>la</strong>belled 1 and<br />
3 in Fig. 3, shows a strong reduction in the primary divertor<br />
region while the secondary zone receives a significantly<br />
<strong>la</strong>rger fraction. [9].<br />
Fraction of ELM energy loss (%)<br />
100<br />
80<br />
60<br />
40<br />
20<br />
Snowf<strong>la</strong>ke<br />
Primary region<br />
Second. region<br />
Traditional<br />
divertor<br />
0<br />
0 0.5 1 1.5<br />
σ<br />
Figure 4: Fraction of the ELM energy loss reaching two of the divertor<br />
p<strong>la</strong>tes as a function of s, the measure of the proximity to the<br />
perfect snowf<strong>la</strong>ke (perfect at s=0). When the snowf<strong>la</strong>ke is formed<br />
by <strong>de</strong>creasing s below 0.75, up to 20% of the power (red curve)<br />
reaches the divertor at the additional location (<strong>la</strong>bel 3 in Fig. 3)<br />
while the power <strong>de</strong>creases (blue curve) at the primary location (<strong>la</strong>bel<br />
1 in Fig. 3).<br />
Conclusions<br />
CRPP-EPFL scientists have <strong>de</strong>monstrated the feasibility<br />
of the snowf<strong>la</strong>ke configuration and shown the advantage<br />
of the corresponding increase of the number of separatrix<br />
legs, in the form of a significant reduction of the heat flow<br />
onto the divertor p<strong>la</strong>tes. While snowf<strong>la</strong>kes will not likely be<br />
achievable in ITER, <strong>de</strong>sign studies for the subsequent <strong>de</strong>vice,<br />
DEMO, are evaluating the snowf<strong>la</strong>ke configuration as<br />
a potential divertor solution.<br />
[1] M. Keilhacker et al., Nucl. Fus. 39 (1999) 209.<br />
[2] D. D. Ryutov et al., Phys. P<strong>la</strong>smas 14 (2007) 064502.<br />
[3] D. D. Ryutov et al., Phys. P<strong>la</strong>smas 15 (2008) 092501.<br />
[4] F. Piras et al., P<strong>la</strong>sma Phys. Control. Fusion 51 (2009) 055009.<br />
[5] V. A. Soukhanovskii et al., Phys. P<strong>la</strong>smas 19 (2012) 082504.<br />
[6] S. L. Allen et al., 24th IAEA FEC Conf. 2012, PD/1-2.<br />
[7] F. Wagner et al., Phys. Rev. Lett. 49 (1982) 1408.<br />
[8] Y. Martin et al., Jou. Phys. Conf. Ser. 123 (2008) 012033.<br />
[9] W. Vijvers et al., IAEA FEC Conf. 2012, San Diego, US.<br />
39
SPG Mitteilungen Nr. 40<br />
An Industrial Lab Grows in Switzer<strong>la</strong>nd<br />
As the Zurich Lab recognizes its 50 th year in the leafy Zurich<br />
suburb of Rüschlikon, a closer look inspects the <strong>de</strong>tails of<br />
how this <strong>la</strong>b became the home of four Nobel Prize <strong>la</strong>ureates<br />
and countless innovations spanning material sciences,<br />
<strong>communications</strong>, analytics and Big Data.<br />
There are several reasons why IBM was consi<strong>de</strong>ring a research<br />
<strong>la</strong>b outsi<strong>de</strong> of the United States in the 1950s. At this<br />
time IBM was in its heyday. The company was financially<br />
strong, and the success of the recently opened San Jose<br />
<strong>la</strong>b ma<strong>de</strong> the management realize the benefits of having research<br />
conducted with the support of headquarters in New<br />
York, but without the local stress and peer pressure.<br />
Physics Anecdotes (17)<br />
IBM Research – Zurich, a Success Story<br />
Chris Sciacca and Christophe Rossel<br />
Switzer<strong>la</strong>nd wasn’t IBM’s first option for a European research<br />
<strong>la</strong>b; London and Amsterdam were also on the short<br />
list, and in 1955 an IBM electrical engineer named Arthur<br />
Samuel was tasked with scouting the three cities.<br />
Fig. 1. The building of IBM Research in Adliswil in 1956. Inset: Ambros<br />
Speiser, first <strong>la</strong>b director, in discussion with Thomas Watson<br />
Jr., CEO of IBM<br />
While officials in Eng<strong>la</strong>nd were receptive to the i<strong>de</strong>a, the<br />
proposed location was in the suburbs of London that he <strong>de</strong>scribed<br />
as, "the most dismal p<strong>la</strong>ces that I have ever seen."<br />
And shortly after, Samuel passed on Eng<strong>la</strong>nd and travelled<br />
to Switzer<strong>la</strong>nd, to a completely different experience - he<br />
never ma<strong>de</strong> it on to Amsterdam.<br />
Simultaneously, as Samuel was visiting Switzer<strong>la</strong>nd, Ambros<br />
Speiser, a young Swiss electrical engineer from ETH<br />
Zurich, had applied for positions at Remington Rand and<br />
IBM. He never got a response from Rand, but by that summer<br />
Speiser became an IBMer.<br />
How to Build a Research Lab<br />
Now that Speiser was on board he was tasked with building<br />
a new <strong>la</strong>boratory, and the challenges he faced were<br />
immense.<br />
As he tells it in the IEEE Annals of the History of Computing<br />
[1], "There was no established pattern to follow - an industrial<br />
<strong>la</strong>boratory, separate from production facilities, did not<br />
exist in Switzer<strong>la</strong>nd."<br />
But Speiser knew he nee<strong>de</strong>d to be close to Zurich, its universities<br />
and within reach of public transport. After viewing<br />
a number of locations, he <strong>de</strong>ci<strong>de</strong>d to rent the wing of a<br />
Swiss stationary company in Adliswil, which was at the end<br />
of a tram line and only a few kilometers from the city.<br />
Having the building for the new <strong>la</strong>b, Speiser nee<strong>de</strong>d brilliant<br />
scientists and engineers. Leveraging his acquaintances,<br />
professional societies and contacts at ETH, he began a<br />
recruiting campaign and quickly amassed a team from all<br />
parts of Europe.<br />
The goal set by IBM management was to build new and<br />
better computer hardware. At the time everyone knew that<br />
vacuum tubes would be rep<strong>la</strong>ced by solid-state circuits,<br />
40<br />
so it was obvious that IBM should begin <strong>de</strong>veloping transistors<br />
and magnetic <strong>de</strong>vices, but this was never formalized.<br />
This <strong>la</strong>ck of direction weighed heavily on Speiser’s mind because<br />
he knew that simi<strong>la</strong>r research was being conducted<br />
insi<strong>de</strong> and outsi<strong>de</strong> of IBM and that they would never achieve<br />
the global recognition he so <strong>de</strong>sired by doing the same<br />
science as everyone else.<br />
After building a stronger rapport with Research’s new management<br />
team in 1958, Speiser was given new direction<br />
for the Zurich Lab to change from electronics to physics,<br />
with a focus on solid-state as the basis for electronic <strong>de</strong>vices<br />
of the future.<br />
Once again Speiser went on recruiting missions across Europe<br />
to find young, creative physicists. Little did he know<br />
at the time that he was also <strong>la</strong>ying the groundwork for what<br />
would become a renowned team for <strong>de</strong>ca<strong>de</strong>s to come.<br />
Fig. 2. Hans Peter Louis one of the earlier research staff members<br />
in the 50’s, in front of a prototype technology called the phototron,<br />
which was never finished.
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Moving to Rüschlikon<br />
In addition to electrical engineering and physics, Speiser<br />
soon ad<strong>de</strong>d a mathematics <strong>de</strong>partment, and quickly the <strong>la</strong>b<br />
was outgrowing its mo<strong>de</strong>st space in Adliswil. Knowing that<br />
the growth would continue and to establish a more stable<br />
reputation, he requested approval from Thomas Watson Jr.,<br />
IBM’s CEO at the time and son of the foun<strong>de</strong>r, to look for<br />
a new location where the <strong>la</strong>b would have its own facilities.<br />
Again, Speiser knew the new <strong>la</strong>b had to be close to the city,<br />
the airport, but most importantly to ETH Zurich, and after<br />
some <strong>de</strong>bate a 10-acre site was purchased in Rüschlikon<br />
for $400,000.<br />
As for the actual <strong>de</strong>sign of the <strong>la</strong>b, Speiser’s main tenant<br />
was that it created spaces for personal interaction, which<br />
he referred to as "a vital process for a research <strong>la</strong>boratory".<br />
To assure this i<strong>de</strong>a, instead of building up, he wanted<br />
the <strong>la</strong>b to be horizontal with long corridors to encourage<br />
chance meetings, simi<strong>la</strong>r to the <strong>de</strong>sign of Bell Laboratories<br />
in New Jersey. It was also important for the <strong>la</strong>b to have a<br />
proper cafeteria for informal discussion and an auditorium<br />
for guest lectures. While initially this was met with some<br />
skepticism because of its costs, he eventually got his wish<br />
and construction started in 1961. The <strong>la</strong>b was officially inaugurated<br />
in front of several hundred guests on 23 May<br />
1963, that is, 50 years ago.<br />
Fig. 3. Introduced in 1956, the IBM 305 RAMAC (Random Access<br />
Memory Accounting System) was an electronic general purpose<br />
data-processing machine that maintained business records on a<br />
real-time basis. The 305 RAMAC was one of the <strong>la</strong>st vacuum tube<br />
systems <strong>de</strong>signed by IBM, and more than 1000 of them were built<br />
before production en<strong>de</strong>d in 1961.<br />
Impacting the Future of the Lab<br />
In the coming <strong>de</strong>ca<strong>de</strong>, the groundwork of Speiser and his<br />
successor began to bear fruit. The i<strong>de</strong>a to start a physics<br />
<strong>de</strong>partment resulted in the hiring of Heinrich Rohrer and<br />
Karl Alex Müller, who through their research and subsequent<br />
publications began to cement a strong reputation for<br />
the Zurich Lab, which reached its apex in the mid-80s when<br />
these two scientists and their colleagues Gerd Binnig and<br />
Georg Bednorz were recognized with the Nobel Prize for<br />
Physics in 1986 and 1987.<br />
This period also saw the addition of a new line of research<br />
in <strong>communications</strong>. Once again the <strong>la</strong>b succee<strong>de</strong>d with the<br />
<strong>de</strong>velopment of the token ring and trellis-co<strong>de</strong>d modu<strong>la</strong>tion,<br />
each p<strong>la</strong>ying a critical role in making the Internet what<br />
it is today.<br />
By 1987 the <strong>la</strong>b also had its own manufacturing line for<br />
semiconductor <strong>la</strong>sers which were used by telecommunication<br />
equipment manufacturers. The research became<br />
so successful that the Uniphase Corporation acquired the<br />
technology and the people from IBM for $45 million, a huge<br />
sum for the future tele<strong>communications</strong> giant with only 500<br />
people at the time.<br />
The Crash and Recovery<br />
With the end of the 80s, towards the mid-90s, IBM found<br />
itself in a dire position. IBM’s near-<strong>de</strong>ath experience was<br />
caused by its failure to recognize that the 40-year-old mainframe<br />
computing mo<strong>de</strong>l was out of touch with the needs of<br />
clients, and other firms like Sun Microsystems pounced on<br />
the opportunity.<br />
This experience also impacted IBM Research. Throughout<br />
the 1970s IBM Research was corporate fun<strong>de</strong>d, it had its<br />
own research agenda and occasionally it did some technology<br />
transfer, but it was not done in a very coordinated<br />
manner because the funding kept coming every year and<br />
the profit margins were strong. This affor<strong>de</strong>d the scientists<br />
the freedom they nee<strong>de</strong>d.<br />
By the 1980s IBM began doing more applied research, and<br />
management took a more active role in influencing the direction<br />
in which the <strong>de</strong>velopments had to go. For example,<br />
IBM started joint programs between Research and the<br />
product divisions with a shared agenda that both parties,<br />
Research and Development, had to agree upon. IBM also<br />
created col<strong>la</strong>borative teams to accelerate the transfer of<br />
research results which went into products spanning from<br />
storage to personal computers. It’s strange to look back at<br />
this now, as today this seems so obvious.<br />
In the 1990s change truly came. To preserve Research, scientists<br />
in Zurich tried to become more proactive in working<br />
on actual customer problems. At the time this was unheard<br />
of at IBM and a <strong>la</strong>rge reason why the company stumbled.<br />
The i<strong>de</strong>a was to interact with clients, gain insights into their<br />
challenges, and find solutions. The concept was a great<br />
success, and in 2000 the Zurich Lab opened up a <strong>de</strong>dicated<br />
facility called the Industry Solutions Lab (ISL), with the<br />
goal of hosting and interacting with clients on a daily basis.<br />
Today, there are simi<strong>la</strong>r facilities around the world hosting<br />
hundreds of clients every month and working directly with<br />
clients. This is a fundamental strategy across all twelve IBM<br />
Research <strong>la</strong>bs on the six continents. "The world is now our<br />
<strong>la</strong>b," as says Dr. John E. Kelly III, IBM senior vice presi<strong>de</strong>nt<br />
and director of Research.<br />
IBM Research in Zurich Today<br />
Un<strong>de</strong>r the direction of seven successive <strong>la</strong>b directors, the<br />
expansion in Zurich continued well into 2000s. Today, there<br />
are five <strong>de</strong>partments, namely, storage, computer science<br />
and systems in addition to physics (science and technology)<br />
and mathematics (mathematics and computational<br />
sciences).<br />
41
SPG Mitteilungen Nr. 40<br />
In addition, the <strong>la</strong>b has a new cutting-edge facility called<br />
the Binnig and Rohrer Nanotechnology Center, named for<br />
the two Nobel Laureates. When the current <strong>la</strong>b director requested<br />
the funding to upgra<strong>de</strong> the existing clean rooms on<br />
the campus he was greeted with a pleasant surprise: "I was<br />
told to make it much bigger and to find a partner. ETH Zurich<br />
was an obvious and logical choice," says Dr. Matthias<br />
Kaiserswerth, the current director of IBM Research - Zurich.<br />
No one could have predicted it, but Speiser’s intuition to<br />
keep the <strong>la</strong>b close to ETH Zurich was a fortuitous <strong>de</strong>cision.<br />
Nobel Laureates K. Alex Müller, Georg Bednorz and Heinrich<br />
Rohrer all came from ETH. And now nearly 60 years<br />
<strong>la</strong>ter, the partners built a $90 million facility, which features<br />
a <strong>la</strong>rge clean room and in particu<strong>la</strong>r six Noise Free Labs<br />
unlike any in the world.<br />
Outsi<strong>de</strong> of the nano world, IBM scientists are working on<br />
some of the greatest challenges of our society today.<br />
On Earth Day 2013, scientists in Zurich announced that<br />
they will be building an affordable photovoltaic system<br />
capable of concentrating so<strong>la</strong>r radiation 2,000 times and<br />
converting 80 percent of the incoming radiation into useful<br />
energy. The system can also provi<strong>de</strong> <strong>de</strong>salinated water and<br />
cool air in sunny, remote locations where both are often in<br />
short supply.<br />
Another team is col<strong>la</strong>borating with a consortium of scientists<br />
in the Nether<strong>la</strong>nds and South Africa on extremely fast,<br />
but low-power exascale computer systems aimed at <strong>de</strong>veloping<br />
advanced technologies for handling the Big Data<br />
that will be produced by the Square Kilometer Array (SKA),<br />
the world’s <strong>la</strong>rgest and most sensitive radio telescope that<br />
consortium will build.<br />
And to improve the much-strained energy grid, IBM scientists<br />
are col<strong>la</strong>borating with utility companies in Denmark,<br />
Austria and Switzer<strong>la</strong>nd to improve to ba<strong>la</strong>nce between <strong>de</strong>mand<br />
and the supply of renewable energy.<br />
While much has changed at IBM Research – Zurich, the<br />
essence of col<strong>la</strong>boration and the spirit of innovation and<br />
excellence that Speiser envisioned remains true to this day.<br />
Fig. 4. The newly built Binnig and Rohrer Nanotechnology Center<br />
and as inset an example of the complete atomic structure of a<br />
pentacene molecule resolved by AFM [2]. The extreme resolution<br />
of the C, H atoms and chemical bonds is achieved by the CO molecule<br />
attached to the tip.<br />
[1] A. P. Speiser, IEEE Annals of the History of Computing 20(1), 15<br />
(Jan.-March 1998).<br />
[2] L. Gross, F. Mohn, N. Moll, P. Liljeroth, G. Meyer, Science 325,<br />
1110 (2009).<br />
On April 29 this year the Herschel space observatory exhausted<br />
its supply of helium that cooled the sensors in the<br />
far-infrared and submillimeter range, wavelengths that cannot<br />
be observed from the ground. Herschel was put into the<br />
Lagrange position L2 in the Sun-Earth system, 1.5 million<br />
kilometres from us. Four years after its <strong>la</strong>unch by the European<br />
Space Agency (ESA), the mission completed its novel<br />
observations about how stars and thus ga<strong>la</strong>xies form and<br />
evolve throughout the universe. The Herschel observatory<br />
was sent to space with 2,300 litres of superfluid helium. The<br />
helium was pumped around the spacecraft in such a way as<br />
to cool the three observing instruments and gradually evaporated<br />
in the process. Herschel cannot observe without<br />
cooling below 1 K in the most critical components, but the<br />
amount was limited and chosen to out<strong>la</strong>st the expected lifetime<br />
of the cutting-edge, but new-to-space electronics.<br />
Herschel excee<strong>de</strong>d expectations both in technology and<br />
science. The technical <strong>de</strong>velopments required by the unusual<br />
observing wavelengths <strong>de</strong><strong>la</strong>yed the start by more than<br />
two years. Swiss industry provi<strong>de</strong>d the <strong>la</strong>rge cryostat and<br />
Goodbye Herschel<br />
Arnold Benz, ETH Zürich<br />
42<br />
the optical assemblies for the HIFI instrument; the low-noise<br />
low-power indium phosphi<strong>de</strong> amplifiers for HIFI (Heterodyne<br />
Instrument for the Far Infrared) were <strong>de</strong>veloped at<br />
ETH Zürich, software for HIFI at the Fachhochschule FHNW<br />
in Windisch. After four years in space all three instruments<br />
on board were still fully operational.<br />
Herschel's observations have revealed the cosmos in unprece<strong>de</strong>nted<br />
<strong>de</strong>tail at these wavelengths. This raised interest<br />
in the astronomical community and resulted in 160<br />
"first results papers" within the first four months of scientific<br />
data taking. However, most results emerged and still do<br />
so after careful data analysis, mo<strong>de</strong>lling and interpretation.<br />
Some highlights of my personal selection are <strong>de</strong>scribed below.<br />
Herschel observations allowed studying ga<strong>la</strong>xies in the<br />
early universe that form stars at prodigious rates and apparently<br />
also in the absence of mergers. Other processes<br />
like inflowing interga<strong>la</strong>ctic streams of cold gas may thus<br />
be equally effective. In nearby active ga<strong>la</strong>xies, on the other
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
The region of ionized molecules in the inner parts of star<br />
and p<strong>la</strong>net forming regions is certainly a field of future research.<br />
On the other hand, O 2<br />
, also not observable from the<br />
ground, was much har<strong>de</strong>r to <strong>de</strong>tect than predicted. Free<br />
oxygen, not bound to carbon monoxi<strong>de</strong>, doesn’t seem to<br />
be in molecu<strong>la</strong>r gas form, but might hi<strong>de</strong> in silicates of the<br />
interstel<strong>la</strong>r dust.<br />
The Herschel image is a composite of observations at 70 (blue),<br />
160 (green), and 250 – 500 μm (red) wavelengths indicating hot,<br />
warm and cold regions, respectively. The image size is 2×2 <strong>de</strong>gree<br />
in the constel<strong>la</strong>tion of the Southern Cross. Note cloud cores (white<br />
dots) located on fi<strong>la</strong>ments (Credit: ESA and the SPIRE & PACS<br />
consortia).<br />
intensity<br />
hand, Herschel found for the first time vast amounts of outflowing<br />
molecu<strong>la</strong>r gas that may <strong>de</strong>plete a ga<strong>la</strong>xy's supply<br />
to form new stars.<br />
In observations of our own ga<strong>la</strong>xy, Herschel i<strong>de</strong>ntified the<br />
presence of a fi<strong>la</strong>mentary network in the gas of molecu<strong>la</strong>r<br />
clouds, fi<strong>la</strong>ments which contain cloud cores that will col<strong>la</strong>pse<br />
un<strong>de</strong>r their own weight to form stars. Herschel <strong>de</strong>monstrated<br />
that fi<strong>la</strong>ments are nearly everywhere in clouds<br />
and that they are a key to star formation. It is not clear how<br />
fi<strong>la</strong>ments originate; intersecting shock waves and magnetic<br />
fields are proposed.<br />
A chief goal of Herschel is the study of the chemical composition<br />
of cosmic objects through high-resolution spectroscopy,<br />
and in particu<strong>la</strong>r the search for water in the gas<br />
state, which cannot be observed from the ground. Of special<br />
interest at ETH Zürich were the chemical network of water<br />
in star formation and the evolution of protostel<strong>la</strong>r disks.<br />
Herschel found gaseous water already in a cold pre-stel<strong>la</strong>r<br />
core before the start of star formation. It amounts to a few<br />
million times the amount of water in the Earth's oceans. The<br />
10 million year old disc surrounding nearby star TW Hydrae<br />
still contains a water supply equivalent to several thousand<br />
times Earth's oceans. Disks ol<strong>de</strong>r than some 60 million years<br />
were observed to contain not enough gas to form new<br />
p<strong>la</strong>nets. These findings suggest that water p<strong>la</strong>yed an important<br />
role throughout the formation of the so<strong>la</strong>r system.<br />
Several molecules were discovered in interstel<strong>la</strong>r clouds for<br />
the first time. We mo<strong>de</strong>lled the chemistry in regions of star<br />
formation in an attempt to predict which molecules – especially<br />
ionised ones – exist there and could be used to<br />
infer the physical conditions. In particu<strong>la</strong>r, ultraviolet and<br />
X-ray irradiation change the chemistry and heat the col<strong>la</strong>psing<br />
envelope and its walls to the outflows. The surprise:<br />
new molecules in interstel<strong>la</strong>r space, like SH + , OH + , and<br />
H 2<br />
O + were discovered to be more abundant than expected.<br />
frequency<br />
The Herschel space observatory has discovered ionized water,<br />
H 2<br />
O + , in absorption at a location where a massive star is forming<br />
in the W3 molecu<strong>la</strong>r cloud. The star- forming region in the Perseus<br />
spiral arm of the Milky Way ga<strong>la</strong>xy is completely opaque in visual<br />
light shown as background in colour (Diameter of image: 500 light<br />
years; credit: ESA/ETH Zürich/Sierra Remote Observatories, Don<br />
Goldman, CA, USA).<br />
The water profile in the atmospheres of Mars is studied at<br />
the University of Bern. For the first time the water vapour<br />
was <strong>de</strong>termined from a global perspective yielding a view<br />
on overall seasonal changes. The group was also part of<br />
the team that discovered O 2<br />
in the Mars atmosphere.<br />
Two weeks after the end of the helium the Herschel observatory<br />
was moved away from the Lagrange point and the<br />
communication was terminated. The loss of pointing control<br />
ends the direct contact with Herschel. The observatory<br />
will slowly drift away from Earth and orbit in<strong>de</strong>finitely the<br />
Sun like a small p<strong>la</strong>net.<br />
Herschel has observed more than we expected, but the<br />
project is not over yet. More than 35,000 scientific observations<br />
were executed with Herschel, and more than 50.000<br />
lines have been <strong>de</strong>tected with the HIFI instrument alone.<br />
They will eventually be i<strong>de</strong>ntified, analyzed in more <strong>de</strong>tail,<br />
and mo<strong>de</strong>lled. Only limited parts of the data are fully exploited.<br />
It will probably be a long time before the next opportunity<br />
to gather this kind of data in space. Due to the breadth<br />
and completeness throughout the entire wavelength range,<br />
the Herschel data are bound to be unparalleled for many<br />
years to come. In a year, all the data will become a public<br />
legacy. Most important will be their combination with<br />
observations at other wavelengths, such as the millimetre/<br />
submillimetre telescope ALMA in Chile. ESA has just announced<br />
a Herschel data analysis course for beginners.<br />
43
SPG Mitteilungen Nr. 40<br />
Structural MEMS Testing<br />
Alex Dommann and Antonia Neels*<br />
EMPA, Lerchenfeldstrasse 5, 9014 St. Gallen, alex.dommann@empa.ch<br />
*CSEM, Microsystems Technology Division, 2002 Neuchâtel<br />
In single crystal silicon (SCSi) based <strong>de</strong>vices, stress and<br />
loading in operation introduces <strong>de</strong>fects during the Micro-<br />
ElectroMechanical Systems (MEMS) life time and increases<br />
the risk of failure. Reliability studies on potential<br />
failure sources have an impact on MEMS <strong>de</strong>sign and are<br />
essential to assure the long term functioning of the <strong>de</strong>vice.<br />
Defects introduced by Deep Reactive-Ion Etching (DRIE),<br />
thermal annealing, dicing and bonding and also the <strong>de</strong>vice<br />
environment (radiations, temperature) influence the crystalline<br />
perfection and have a direct impact on the mechanical<br />
properties of MEMS and their aging behavior. Defects and<br />
<strong>de</strong>formations are analyzed using High Resolution X-ray Diffraction<br />
Methods (HRXRD) such as Reciprocal Space Maps<br />
(RSM). Micro systems technology can be highly reliable,<br />
but can be different from those of solid-state electronics.<br />
Therefore testing techniques must be <strong>de</strong>veloped to accelerate<br />
MEMS-specific failures [1 - 4].<br />
which is <strong>de</strong>tected via the broa<strong>de</strong>ning of the X-ray peak<br />
in a "rocking-curve" (RC) measurement. Analysis is performed<br />
with high resolution X-ray diffraction. The set-up is<br />
composed by curved multi<strong>la</strong>yer x-ray mirrors named after<br />
Herbert Göbel (Göbel mirror) in front of the X-ray tube, followed<br />
by a monochromator for monochromatization and<br />
collimation of X-ray beams by using a 4-Crystal monochromator<br />
with two channel-cut Ge [220] called Bartels monochromator<br />
(Fig. 2). Two configurations are possible for the<br />
diffracted beam si<strong>de</strong>, <strong>de</strong>pending on the methods applied:<br />
Rocking curve (RC) or Reciprocal space map (RSM). Both<br />
methods allow measuring strain and <strong>de</strong>fects concentration<br />
in a crystal. The instrument used for HRXRD is shown (Figure<br />
1).<br />
New MEMS fabrication processes and packaging concepts<br />
find applications in areas where a high reliability is nee<strong>de</strong>d<br />
such as in aerospace, automotive or watch industry. This<br />
creates a strong <strong>de</strong>mand in quality control and failure analysis<br />
and also brings new challenges, particu<strong>la</strong>rly in the fields<br />
of testing and qualification. Non-<strong>de</strong>structive HRXRD methods<br />
are applied to monitor the mobility of <strong>de</strong>fects and strain<br />
Figure 1: Diffractometer used for HRXRD applications.<br />
HRXRD allows measuring the strain of a crystal with high<br />
resolution (Fig. 1). We use HRXRD to assess the strain in<br />
DRIE etched processed silicon beams. Strain <strong>de</strong>forms the<br />
silicon beam leading to an appreciable sample curvature<br />
A rocking curve (RC) is obtained as angu<strong>la</strong>r distribution<br />
of the reflected X-ray beam, when the <strong>de</strong>tector is<br />
set at a specific Bragg angle and when the sample is<br />
rotated about small angles normal to the Bragg p<strong>la</strong>ne<br />
axis. The rocking curve is broa<strong>de</strong>ned by disruptions of<br />
the p<strong>la</strong>ne parallelity and by crystal <strong>de</strong>fects like those<br />
introduced by mechanical stress. Reciprocal space<br />
mapping (RSM) adds, by the restriction of the angu<strong>la</strong>r<br />
acceptance of the <strong>de</strong>tector, another dimension to<br />
the information avai<strong>la</strong>ble from the HRXRD experiment.<br />
Strain and tilt elements being present in a sample are<br />
i<strong>de</strong>ntified separately. An excellent introduction to both<br />
analytical methods can be found at http://prism.mit.<br />
edu/xray/tutorials.htm. See 'Basics of High Resolution<br />
X-Ray Diffraction for Studying Epitaxial Thin Films'.<br />
Fig 2: Diffractometer setup for RSM’s (<strong>de</strong>tector position 1) and RC’s (<strong>de</strong>tector position 2)<br />
44
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
As the Q-factor is not only <strong>de</strong>pen<strong>de</strong>nt on the vacuum level<br />
of the MEMS cavity but also on the strain state of the <strong>de</strong>vice,<br />
the simultaneous data collection for the Q factor <strong>de</strong>termination<br />
and the strain state is evi<strong>de</strong>nt. The packaging<br />
induced strain created at the important interfaces such as<br />
the interfaces close to the bonding material and more importantly<br />
to the <strong>de</strong>vice <strong>la</strong>yer has been analyzed by means<br />
of X-ray Rocking Curves (Fig. 3). The stress profile can be<br />
<strong>de</strong>termined. Especially the strain close to the functional <strong>de</strong>vice<br />
is important as the strain state influences the application<br />
relevant physical parameters such as the resonance<br />
frequency and the Q factor in resonator.<br />
The combination of functional testing with state-of-the-art<br />
X-ray methods for the evaluation of <strong>de</strong>fect and strain gradients<br />
will serve as a useful tool for setting up a fundamental<br />
un<strong>de</strong>rstanding of the reliability and also aging problems of<br />
MEMS.<br />
References<br />
Figure 3: Schematic HRXRD measurement setup and silicon crystal<br />
orientation (top) and measured rocking curves RC’s from the<br />
bonding interface 1 of the <strong>de</strong>vice <strong>la</strong>yer to the bonding interface 2<br />
(bottom) resulting in a stress profiling.<br />
and along the MEMS fabrication and packaging processes.<br />
RSM is a powerful tool for evaluating the strain state of<br />
the entire structure. Due to the much more limited vertical<br />
divergence and the very small horizontal divergence of<br />
the RSM settings, it is possible to get a 'g-function like'<br />
reciprocal-space probe which is almost invariant over the<br />
Ewald sphere. Figure 2 shows a setup used for measuring<br />
such RSMs.<br />
HRXRD is a very sensitive and non-<strong>de</strong>structive technique<br />
for <strong>de</strong>termining the strain in MEMS <strong>de</strong>vices.<br />
An example of such a test structure is a silicon based piezoelectric<br />
resonator (Fig. 3), <strong>de</strong>veloped at CSEM, targeting<br />
vacuum hermetic wafer-level packaging technology [5]. The<br />
monitoring of quality factors (Q) for the resonators permits<br />
to evaluate the pressure level (hermeticity) of the <strong>de</strong>vice<br />
cavity and the leakage rate.<br />
[1] A. Dommann, A. Neels, “Reliability of MEMS” (2011), Proceedings<br />
of SPIE - The International Society for Optical Engineering,<br />
7928, art. no. 79280B.<br />
[2] A. Neels, A. Dommann, A. Schifferle, O. Papes, E. Mazza, Reliability<br />
and Failure in Single Crystal Silicon MEMS Devices, Microelectronics<br />
Reliability, 48, 1245-1247, 2008.<br />
[3] Herbert R. Shea ; Reliability of MEMS for space applications,<br />
Proc. SPIE Int. Soc. Opt. Eng. 6111, 61110A (2006).<br />
[4] Schweitz, J.-Å; Mechanical Characterization of Thin Films by<br />
Micromechanical Techniques, MRS Bulletin, XVII, 7, 1992, pp.34-<br />
45.<br />
[5] J. Baborowski, et al. "Wafer level packaging technology for<br />
silicon resonators", Procedia Chemistry 1, 1535-1538 (July 2009).<br />
Alex Dommann's research concentrates on the<br />
structuring, coating and characterization of thin films,<br />
MEMS and interfaces. In July 2013 he was appointed<br />
Head of Departement "Materials meet Life" at Empa,<br />
Swiss Fe<strong>de</strong>ral Laboratories for Materials Science and<br />
Technology. He is member of different national and international<br />
committees.<br />
Antonia Neels is heading the XRD Application Lab of<br />
CSEM’s Microsystems Technology Division. She has a<br />
broad experience in the application of X-ray diffraction<br />
methods for microsystems (MEMS) and thin films with<br />
respect to quality control and failure mo<strong>de</strong> analysis.<br />
Kurz<strong>mitteilungen</strong> (Fortsetzung)<br />
Felicitas Pauss und Karl Ga<strong>de</strong>mann neu im Vorstand SCNAT<br />
Die Physikerin Felicitas Pauss und <strong>de</strong>r Chemiker Karl Ga<strong>de</strong>mann<br />
sind an <strong>de</strong>r Delegiertenversammlung <strong>de</strong>r Aka<strong>de</strong>mie<br />
<strong>de</strong>r Naturwissenschaften Schweiz (SCNAT) am 24. Mai<br />
2013 in Bern neu in <strong>de</strong>n Vorstand gewählt wor<strong>de</strong>n. Zu<strong>de</strong>m<br />
wur<strong>de</strong> <strong>de</strong>r Verein <strong>Schweizerische</strong>r Naturwissenschaftslehrerinnen<br />
und -lehrer in die Aka<strong>de</strong>mie aufgenommen. Die<br />
Professorin für Experimentelle Teilchenphysik, Felicitas<br />
Pauss, forscht an <strong>de</strong>r ETH Zürich und am CERN in Genf,<br />
wo sie die «Internationalen Beziehungen» führt. Karl Ga<strong>de</strong>mann<br />
ist Professor für organische Chemie an <strong>de</strong>r Universität<br />
Basel und aktueller Präsi<strong>de</strong>nt <strong>de</strong>r P<strong>la</strong>tform Chemistry<br />
<strong>de</strong>r SCNAT. 2012 wur<strong>de</strong> er mit <strong>de</strong>m renommierten Latsis-<br />
Preis ausgezeichnet. Felicitas Pauss nimmt ab Juni 2013<br />
Einsitz im Vorstand, Karl Ga<strong>de</strong>mann ab Januar 2014. In <strong>de</strong>n<br />
Vorstand wie<strong>de</strong>rgewählt wur<strong>de</strong> Helmut Weissert von <strong>de</strong>r<br />
ETH Zürich.<br />
Quelle: SCNAT Newsletter Juni 2013<br />
45
SPG Mitteilungen Nr. 40<br />
Paul Scherrer Institute: User facilities - calls for proposals<br />
The Paul Scherrer Institute (PSI) in Villigen operates four<br />
major user <strong>la</strong>boratories: a third generation X-ray synchrotron<br />
source (SLS), the only continuous spal<strong>la</strong>tion neutron<br />
source worldwi<strong>de</strong> (SINQ), the world’s most powerful continuous-beam<br />
μSR facility (SμS) and a meson factory for<br />
fundamental nuclear and elementary particle physics (LTP).<br />
In fact, PSI is the only p<strong>la</strong>ce worldwi<strong>de</strong> to offer the three<br />
major probes for con<strong>de</strong>nsed matter research (synchrotron<br />
X-rays, neutrons and muons) on one campus.<br />
The instal<strong>la</strong>tions are all open access user facilities and offer<br />
regu<strong>la</strong>r calls for proposals.<br />
More information is avai<strong>la</strong>ble here:<br />
http://www.psi.ch/useroffice/proposal-<strong>de</strong>adlines<br />
Contact address:<br />
Paul Scherrer Institute phone: +41-56-310-4666<br />
User Office<br />
email: useroffice@psi.ch<br />
5232 Villigen PSI<br />
User facility<br />
Proposal submission<br />
<strong>de</strong>adline<br />
SLS<br />
all beamlines, except PX-I,-II,-III Mar 15, Sep 15<br />
PX beamlines Feb 15, Jun 15, Oct 15<br />
SINQ<br />
all beamlines May 15, Nov 15<br />
SμS<br />
DOLLY, GPD, GPS, LEM and LTF Dec 10<br />
GPD, GPS and LTF June 11<br />
PARTICLE PHYSICS<br />
all Dec 10<br />
Physique et <strong>la</strong> Société<br />
Quand <strong>la</strong> Physique rejoint le Sport<br />
Christophe Rossel<br />
Une quarantaine d’étudiants et étudiantes en physique <strong>de</strong>s<br />
universités suisses se sont réunis les 17 et 18 mai 2013 à<br />
Macolin pour un atelier <strong>de</strong> travail sur le thème Physique<br />
et Sport. Organisée dans le cadre du Forum <strong>de</strong>s Jeunes<br />
Physiciens (YPF) en col<strong>la</strong>boration avec <strong>la</strong> Société Suisse<br />
<strong>de</strong> Physique (SSP) et l’office fédéral du sport (OFSPO) cette<br />
réunion a permis à ces jeunes <strong>de</strong> se rencontrer dans une<br />
atmosphère amicale.<br />
L’YPF a été créé en 2009 à l’instigation <strong>de</strong> <strong>la</strong> SSP, grâce au<br />
soutien financier <strong>de</strong> l’Académie suisse <strong>de</strong>s sciences naturelles<br />
(SCNAT) et <strong>de</strong> sa p<strong>la</strong>teforme MAP. Les buts du Forum<br />
sont d’encourager <strong>la</strong> communication entre les sociétés<br />
d’étudiants en physique entre elles, avec les physiciens<br />
professionnels membres <strong>de</strong> <strong>la</strong> SSP ainsi que <strong>de</strong> créer une<br />
p<strong>la</strong>teforme pour discuter <strong>de</strong>s sujets d’intérêts communs et<br />
organiser <strong>de</strong>s évènements divers tels que visites ou séminaires.<br />
C’est dans ce contexte qu’a eu lieu ce premier workshop<br />
sur le splendi<strong>de</strong> site <strong>de</strong> <strong>la</strong> Haute école fédérale <strong>de</strong> sport<br />
(HEFS) <strong>de</strong> Macolin. Arrivés le vendredi soir les étudiants<br />
ont été reçus officiellement par le recteur <strong>de</strong> cette école,<br />
Walter Mengisen, qui leur a décrit <strong>la</strong> fonction et les activités<br />
<strong>de</strong> l’OFSPO qui est un centre <strong>de</strong> prestations, <strong>de</strong> formation<br />
et d’entraînement au service du sport d’élite, du sport <strong>de</strong><br />
compétition et du sport popu<strong>la</strong>ire.<br />
Après une soirée conviviale <strong>de</strong> discussion et <strong>de</strong> jeux au bar<br />
et <strong>la</strong> nuit passée au Grand Hôtel, les participants se sont<br />
retrouvés le samedi matin pour <strong>la</strong> série <strong>de</strong> conférences prévues<br />
au programme. Après une introduction générale sur le<br />
thème et l’organisation du workshop par Christophe Rossel,<br />
le premier conférencier, Didier Stau<strong>de</strong>nman du département<br />
<strong>de</strong> mé<strong>de</strong>cine <strong>de</strong> l’université <strong>de</strong> Fribourg a présenté<br />
le sujet <strong>de</strong> <strong>la</strong> biomécanique et <strong>de</strong> l’activation muscu<strong>la</strong>ire<br />
à une audience attentive. En particulier, il a décrit <strong>la</strong> tech-<br />
Une partie <strong>de</strong>s participants réunis <strong>de</strong>vant le Grand Hôtel <strong>de</strong> Macolin avec une vue imprenable sur les alpes<br />
46
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
nique d'électromyographie (EMG) qui permet d'enregister<br />
et analyser les signaux électriques produits par les variations<br />
physiologiques <strong>de</strong>s fibres muscu<strong>la</strong>ires.<br />
Dans une secon<strong>de</strong> présentation Pierre Cornu, avocat et<br />
conseiller juridique pour les affaires d’intégrité et <strong>de</strong> régu<strong>la</strong>tions<br />
à l’UEFA ainsi qu’au Centre international d’étu<strong>de</strong> du<br />
sport (CIES) <strong>de</strong> Neuchâtel a développé le sujet <strong>de</strong>s manipu<strong>la</strong>tions<br />
dans les compétitions sportives et <strong>la</strong> bonne gouvernance.<br />
De manière captivante avec maints exemples il<br />
a évoqué les paris illégaux, les manipu<strong>la</strong>tions en football,<br />
le dopage et ses effets pervers ainsi que les métho<strong>de</strong>s <strong>de</strong><br />
contrôle et <strong>de</strong> sanctions disciplinaires.<br />
Pascal Arnold, doctorant à l’Institut <strong>de</strong>s systèmes mécaniques<br />
<strong>de</strong> le l’ETHZ nous a ensuite expliqué les défis humains<br />
et technologiques dans le bobsleigh <strong>de</strong> compétition.<br />
De manière remarquable il nous a décrit toutes les étapes<br />
techniques dans <strong>la</strong> construction d’un bob professionnel<br />
qu’il a développé dans le cadre <strong>de</strong> sa thèse <strong>de</strong> doctorat.<br />
Par chance un exemp<strong>la</strong>ire d’un tel bob a été exposé en<br />
présence du pilote professionnel Rico Peter <strong>de</strong> l’équipe Suisse.<br />
II qui a aussi répondu aux nombreuses questions.<br />
Démonstration d’agilité sur <strong>la</strong> s<strong>la</strong>ckline<br />
Changement <strong>de</strong> décors l’après-midi où l’occasion a été<br />
donnée <strong>de</strong> passer <strong>de</strong> <strong>la</strong> théorie à <strong>la</strong> pratique grâce au soutien<br />
organisationnel <strong>de</strong> Bruno Tschanz. Sous un soleil radieux<br />
et en tenue sportive les participants se sont rendus à <strong>la</strong><br />
salle et au sta<strong>de</strong> <strong>de</strong> <strong>la</strong> Fin du Mon<strong>de</strong> pour tester différentes<br />
instal<strong>la</strong>tions. Par exemple ils ont pu se mesurer aux professionnels<br />
<strong>de</strong> l’équipe <strong>de</strong> bob du Lichtenstein à <strong>la</strong> poussée<br />
d’engins d’entrainement simi<strong>la</strong>ires sur roues ou encore<br />
tester leur habileté d’équilibristes en s<strong>la</strong>ckline, ou littéralement<br />
cor<strong>de</strong> souple. Dans ce sport créé dans les années 80,<br />
l’objectif est <strong>de</strong> se dép<strong>la</strong>cer ou <strong>de</strong> faire <strong>de</strong>s figures sur une<br />
sangle légèrement é<strong>la</strong>stique et ceci sans aucun accessoire.<br />
Un autre clou <strong>de</strong>s activités sportives a été sans conteste<br />
le football joué avec analyse <strong>de</strong>s performances <strong>de</strong> chaque<br />
joueur, visionné sur petit écran après <strong>la</strong> partie. Enfin chacun<br />
a aussi pu tester les signaux induits par le mouvement <strong>de</strong><br />
leur biceps grâce à un système <strong>de</strong> mesure électriques avec<br />
électro<strong>de</strong>s multiples et en comprendre les principes avec<br />
les explications <strong>de</strong> Didier Stau<strong>de</strong>nman.<br />
Pascal Arnold présentant les caractéristiques techniques du bob<br />
Suisse II en présence <strong>de</strong> son pilote Rico Peter<br />
Tous les secrets <strong>de</strong> <strong>la</strong> mesure <strong>de</strong> position en sport nous ont<br />
été révélés par Martin Rumo <strong>de</strong> <strong>la</strong> Haute école fédérale <strong>de</strong><br />
sport <strong>de</strong> Macolin. Il a expliqué les développements récents<br />
dans les instruments d’analyse <strong>de</strong> performance dans les<br />
sports d’élite et en particulier les métho<strong>de</strong>s <strong>de</strong> mesures locales<br />
<strong>de</strong> <strong>la</strong> position <strong>de</strong>s joueurs <strong>de</strong> football et du ballon. En<br />
effet les données 3D obtenues en temps réel permettent un<br />
entraînement précis, une observation exacte et une analyse<br />
<strong>de</strong> chaque joueur et <strong>de</strong> l’équipe.<br />
Finalement le <strong>de</strong>rnier conférencier, Benedikt Fasel du Laboratoire<br />
<strong>de</strong> mesure et d'analyse <strong>de</strong>s mouvements <strong>de</strong> l’EPFL<br />
s’est exprimé sur les métho<strong>de</strong>s d’analyse du mouvement et<br />
en particulier sur <strong>la</strong> prévention <strong>de</strong>s acci<strong>de</strong>nts dans les compétitions<br />
<strong>de</strong> ski alpin. Il a expliqué l’utilisation <strong>de</strong> senseurs<br />
inertiels p<strong>la</strong>cées sur le skieur, <strong>de</strong> caméras 3D ou du GPS<br />
pour mesurer <strong>la</strong> trajectoires, les forces et <strong>la</strong> dynamique du<br />
corps pendant <strong>la</strong> <strong>de</strong>scente et comment utiliser les données<br />
pour optimaliser <strong>la</strong> géométrie <strong>de</strong>s skis.<br />
Un bel exercice sportif, <strong>la</strong> poussée du bob à <strong>de</strong>ux<br />
C’est enthousiastes et presque à regret que les participants<br />
ont quitté le site en fin d’après-midi pour retourner chez<br />
eux après une journée riche en information scientifique et<br />
technique et en activités sportives.<br />
47
SPG Mitteilungen Nr. 40<br />
Introduction<br />
History of Physics (8)<br />
On the Einstein-Grossmann Col<strong>la</strong>boration 100 Years ago<br />
Norbert Straumann, Institute for Theoretical Physics, Uni Zürich<br />
Einstein’s path to general re<strong>la</strong>tivity (GR) mean<strong>de</strong>red steeply,<br />
encountered confusing forks, and also inclu<strong>de</strong>d a big U-<br />
turn. In this brief account I discuss in some <strong>de</strong>tail Einstein's<br />
remarkable progress beginning in August 1912, after his<br />
second return to Zürich, until Spring 1913. Before we come<br />
to this, some indications of what he had already achieved<br />
until this period are necessary.<br />
In 1907, while writing a review article on special re<strong>la</strong>tivity<br />
(SR), Einstein specu<strong>la</strong>ted – attempting to un<strong>de</strong>rstand the<br />
empirical equality of inertial and gravitational mass – on the<br />
possibility of extending the principle of re<strong>la</strong>tivity to accelerated<br />
motion, and ad<strong>de</strong>d an important section on gravitation<br />
in his review [2] 1 . With this "basic i<strong>de</strong>a", which he referred<br />
to as principle of equivalence, he went beyond the framework<br />
of SR. His (special formu<strong>la</strong>tion) of the equivalence<br />
principle – "the most fortunate thought of my life" – became<br />
the guiding thread in his search for a re<strong>la</strong>tivistic theory of<br />
gravitation. Until 1911 Einstein worked apparently mainly<br />
on the quantum puzzles and did not publish anything about<br />
gravitation, but continued to think about the problem. In<br />
[3] he writes: "Between 1909-1912 while I had to teach<br />
theoretical physics at the Zürich and Prague Universities I<br />
pon<strong>de</strong>red ceaselessly on the problem". When Einstein realized<br />
in 1911 that gravitational light <strong>de</strong>flection should be<br />
experimentally observable [4], he took up the problem of<br />
gravitation again and began to "work like a horse" in <strong>de</strong>veloping<br />
a coherent theory of the static gravitational fields.<br />
Since he had found that the velocity of light <strong>de</strong>pends on the<br />
gravitational potential, he conclu<strong>de</strong>d that the speed of light<br />
p<strong>la</strong>ys the role of the gravitational potential, and proposed a<br />
non-linear field equation, in which the gravitational energy<br />
<strong>de</strong>nsity itself acts as a source of the gravitational potential.<br />
Therefore, the field equation implied that the principle of<br />
equivalence is valid only for infinitely small spatial regions.<br />
In the second of his Prague papers on "gravito-statics" [5]<br />
he also showed how the equations of electrodynamics and<br />
thermodynamics are modified in the presence of a static<br />
gravitational field. At this point he began to investigate the<br />
dynamical gravitational field.<br />
Einstein gains Marcel Grossmann as a col<strong>la</strong>borator<br />
When Einstein arrived in Zürich in early August, he was<br />
convinced that a metric field of spacetime, generalizing<br />
the Minkowski metric to a pseudo-Riemannian dynamical<br />
metric, was the right re<strong>la</strong>tivistic generalization of Newton’s<br />
potential. The main question was to find the basic equation<br />
for this field. But how to achieve this was in the dark<br />
and he looked for mathematical help. Fortunately, Marcel<br />
Grossmann, his old friend since his stu<strong>de</strong>nt time, was now<br />
also professor at the ETH and Einstein succee<strong>de</strong>d in gain-<br />
1 References to papers that have appeared in the Collected Papers of<br />
Albert Einstein (CPAE) [1] are always cited by volume and document of<br />
CPAE.<br />
48<br />
ing him as a col<strong>la</strong>borator in his search for the gravitational<br />
field equation. In a 1955 reminiscence, shortly before his<br />
<strong>de</strong>ath, Einstein wrote [3]:<br />
I was ma<strong>de</strong> aware of these [works by Ricci and Levi-Civita]<br />
by my friend Grossmann in Zürich, when I put the<br />
problem to investigate generally covariant tensors, whose<br />
components <strong>de</strong>pend only on the <strong>de</strong>rivatives of the coefficients<br />
of the quadratic fundamental invariant.<br />
He at once caught fire, although as a mathematician he<br />
had a somewhat sceptical stance towards physics. (...)<br />
He went through the literature and soon discovered that<br />
the indicated mathematical problem had already been<br />
solved, in particu<strong>la</strong>r by Riemann, Ricci and Levi-Civita.<br />
This entire <strong>de</strong>velopment was connected to the Gaussian<br />
theory of curved surfaces, in which for the first time systematic<br />
use was ma<strong>de</strong> of generalized coordinates.<br />
Louis Kollros, another stu<strong>de</strong>nt friend of Einstein, who was<br />
also mathematics professor at the ETH during this time, remembered<br />
also in 1955 [6]:<br />
[Einstein] spoke to Grossmann about his troubles and<br />
said one day: "Grossmann, you must help me, otherwise<br />
I’ll go crazy ! ".<br />
The fruitful col<strong>la</strong>boration of<br />
Einstein and Grossmann<br />
led to the famous joint article<br />
with the mo<strong>de</strong>st title<br />
"Outline of a Generalized<br />
Theory of Re<strong>la</strong>tivity and a<br />
Theory of Gravitation" [7],<br />
one of the most important<br />
physics papers in the<br />
twentieth century. A lot of<br />
additional insight can be<br />
gained from Einstein’s <strong>de</strong>tailed<br />
'Zürich Notebook'<br />
[8]. It is really fascinating<br />
Figure 1: Marcel Grossmann.<br />
to study these research<br />
notes, because one can see Einstein at work, and theoretical<br />
physics at its best: A <strong>de</strong>licate interp<strong>la</strong>y between physical<br />
reasoning, based on an intuitive estimate of the most<br />
relevant empirical facts, and – equally important – mathematical<br />
structural aspects and requirements. We shall see<br />
that already <strong>la</strong>te in 1912 Einstein came very close to his<br />
final theory, but physical and conceptual arguments, that<br />
will be discussed <strong>la</strong>ter, convinced him for a long time that –<br />
with "heavy heart" – he had to abandon the general covariance<br />
of the gravitational field equation. In a letter to Lorentz<br />
[9] he called this the "ugly dark spot" of the theory. With<br />
this <strong>de</strong>cision, based on erroneous judgement, Einstein lost<br />
almost three years until physics and mathematics came<br />
into harmony in his beautiful general theory of re<strong>la</strong>tivity.<br />
The Einstein-Grossmann theory, published almost exactly<br />
hundred years ago, contains, however, virtually all essential<br />
elements of Einstein’s <strong>de</strong>finite gravitation theory.
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
The corresponding Euler-Lagrange equation is the geo<strong>de</strong>sic<br />
equation of motion for a point particle. Consi<strong>de</strong>ring<br />
an incoherent dust distribution as an ensemble of particles,<br />
Einstein guesses that the energy-momentum conservation<br />
<strong>la</strong>w of special re<strong>la</strong>tivity, n<br />
T mn = f m , with the energy-stress<br />
tensor T mn = 0<br />
u m u n ( 0<br />
= rest-mass matter <strong>de</strong>nsity, u m = fourvelocity<br />
field) and an external force <strong>de</strong>nsity f m , should be<br />
rep<strong>la</strong>ced by<br />
1<br />
mo<br />
( g g T )<br />
1<br />
ab<br />
2o<br />
- nm - 2ngabT<br />
= 0 (2)<br />
-g<br />
2<br />
(g := <strong>de</strong>t(g mn<br />
). The <strong>de</strong>tails of Einstein’s consi<strong>de</strong>rations are<br />
<strong>de</strong>scribed in his Part I, Sect. 4 of the "Entwurf" paper by<br />
Einstein and Grossmann [7]. This is just an explicit form of<br />
the equation n<br />
T mn<br />
= 0, as stated by Grossmann in his Part II<br />
of [7]. Later in Sect. 6 of [7] Einstein generalizes Maxwell’s<br />
equations in generally covariant form. This part has survived<br />
in GR. The coupling of electromagnetic fields to external<br />
gravitational fields is not yet formalized to the " $ " rule,<br />
as a mathematically precise expression of a local version of<br />
the equivalence principle.<br />
In search of the gravitational field equation<br />
Figure 2: Cover sheet of the Einstein-Grossmann "Entwurf" paper.<br />
Requirements to be satisfied by the future theory<br />
The following mixture of physical and mathematical properties<br />
of a re<strong>la</strong>tivistic theory of gravitation are among Einstein’s<br />
main guiding principles:<br />
• The theory reduces to the Newtonian limit for weak<br />
fields and slowly moving matter.<br />
• Conservation <strong>la</strong>ws for energy and momentum must<br />
hold.<br />
• The equivalence principle must be embodied.<br />
• The theory respects a generalized principle of re<strong>la</strong>tivity<br />
to accelerating frames, taking into account that gravitation<br />
and inertia are <strong>de</strong>scribed by one and the same<br />
metric field g mn<br />
. Einstein expressed this by the requirement<br />
of general covariance of the basic equations (to<br />
become a much <strong>de</strong>bated subject).<br />
Non-gravitational <strong>la</strong>ws in external gravitational fields<br />
The easier part of the new theory was to <strong>de</strong>scribe the coupling<br />
of external gravitational fields to matter and electromagnetic<br />
fields. In one of the Prague papers Einstein had<br />
<strong>de</strong>rived the equation of motion for a point particle in a static<br />
field from a variational principle, which is now generalized<br />
in an natural manner to<br />
2<br />
n o<br />
d # ds = 0, ds = g no dx dx .<br />
(1)<br />
Soon, Einstein begins to look for candidate field equations.<br />
The pages before 27 of the Zürich Notebook show that he<br />
was not yet acquainted with the absolute calculus of Ricci<br />
and Levi-Civita. On p. 27, referring to Grossmann, Einstein<br />
writes down the expression for the fully covariant Riemann<br />
curvature tensor R abg<br />
. Next, he forms by contraction the<br />
Ricci tensor R mn<br />
. The resulting terms involving second<br />
<strong>de</strong>rivatives consist, besi<strong>de</strong> g ab a<br />
b<br />
g mn<br />
, of three additional<br />
terms. Einstein writes below their sum: "should vanish"<br />
["sollte verschwin<strong>de</strong>n"]. The reason is that he was looking<br />
for a field equation of the following general form:<br />
with<br />
no<br />
no<br />
C 6 g@ = lT<br />
,<br />
(3)<br />
no<br />
ab no<br />
C 6 g@ = 2a( g 2bg<br />
) + terms that vanish in linear<br />
approximation. (4)<br />
After long complicated calcu<strong>la</strong>tions, Einstein discovers that<br />
the Ricci tensor is of the <strong>de</strong>sired form, when the coordinates<br />
are assumed to be harmonic. (Rea<strong>de</strong>rs who are not familiar<br />
with this may regard this as a kind of gauge condition,<br />
analogous to the Lorentz condition in electrodynamics.)<br />
This seems to look good, and Einstein begins to analyse<br />
the linear weak field approximation of the field equation 2<br />
R<br />
= lT<br />
.<br />
no no (5)<br />
(Rea<strong>de</strong>rs, familiar with GR, know that Einstein has to run<br />
into problems, because of the contracted Bianchi i<strong>de</strong>ntity.)<br />
2 Never before had Einstein used in his work such advanced and complex<br />
mathematics. This is expressed in a letter to Arnold Sommerfeld on 29<br />
October 1912 (CPAE, Vol. 5, Doc. 421): “But one thing is certain: never<br />
before in my life have I toiled any where near as much, and I have gained<br />
enormous respect for mathematics, whose more subtle parts I consi<strong>de</strong>red<br />
until now, in my ignorance, as pure luxury. Compared with this problem,<br />
the original theory of re<strong>la</strong>tivity is child’s p<strong>la</strong>y.”<br />
49
SPG Mitteilungen Nr. 40<br />
The weak field approximation<br />
The linearized harmonic coordinate condition becomes for<br />
h no: = g no - hno ( hno : Minkowski metric)<br />
na<br />
( h<br />
1 na<br />
2n<br />
- h h)<br />
= 0<br />
(6)<br />
2<br />
(h := h μ , indices are now raised and lowered by means of<br />
μ<br />
the Minkowski metric). This is nowadays usually called the<br />
Hilbert condition, but Einstein imposed it already in 1912.<br />
The field equation becomes an inhomogeneous wave<br />
equation:<br />
Xh<br />
=-2lT<br />
no no (7)<br />
Einstein takes for T mn<br />
his earlier expression for dust.<br />
But now he runs into a serious problem:<br />
From n T mn<br />
= 0 in the weak field limit, it follows that<br />
o<br />
X( 2 h no ) = 0 hence the harmonic coordinate condition requires<br />
X( 2 o h)<br />
= 0 , and therefore the trace of the the field<br />
equation implies Xh =- 2lT = const., T:<br />
= T<br />
n n . For dust<br />
this requires that T = -r 0<br />
= const. This is, of course, unacceptable.<br />
One would not even be able to <strong>de</strong>scribe a star,<br />
with a smooth distribution of matter localized in a finite region<br />
of space.<br />
Einstein’s modified linearized field equation<br />
Now, something very interesting happens. Einstein avoids<br />
this problem by modifying the field equation (7) to<br />
X( h -<br />
1<br />
h h)<br />
=-2lT<br />
2<br />
no no no (8)<br />
Then the harmonic coordinate condition (6) is compatible<br />
with n<br />
T mn = 0 . Remarkably, (8) is the linearized equation<br />
of the final theory (in harmonic coordinates). One won<strong>de</strong>rs<br />
why Einstein did not try at this point the analogous substitution<br />
R no $ R no - 2 g no R or Tno $ Tno - 2 g no T in the full<br />
1<br />
1<br />
non-linear equation (5), which would have led to the final<br />
field equation of GR. One probable reason for this is connected<br />
with the Newtonian limit.<br />
The problem with the Newtonian limit<br />
The problem with the Newtonian limit was, it appears, one<br />
of the main reasons why Einstein abandoned the general<br />
covariance of the field equation. Apparently, (8) did<br />
not reduce to the correct limit. That it leads to the Poisson<br />
equation for g 00<br />
(x) is fine, but because of the harmonic<br />
coordinate condition the metric can not be spatially f<strong>la</strong>t.<br />
(The almost Newtonian approximation of (6) and (8) is <strong>de</strong>rived<br />
in textbooks on GR; see, e.g., [11], Sect. 4.2.) Einstein<br />
found this unacceptable. He was convinced that for<br />
(weak) static gravitational fields the metric must be of the<br />
form (g mn<br />
) = diag(g 00<br />
(x), 1, 1, 1), as he already noted on p. 1<br />
of his research notes. I won<strong>de</strong>r why he did not remember<br />
his cautious remark in one of his Prague papers [12] on<br />
static gravitational fields, in which – while assuming spatial<br />
f<strong>la</strong>tness – he warned that this may very well turn out to be<br />
wrong, and says that actually it does not hold on a rotating<br />
disk. Since a non-f<strong>la</strong>tness would not affect the geo<strong>de</strong>sic<br />
equation in the Newtonian limit, there is actually, as we<br />
all know, no problem. But Einstein realized this only three<br />
years <strong>la</strong>ter 3 . Well(!): "If wise men did not err, fools should<br />
<strong>de</strong>spair" (Wolfgang Goethe).<br />
At the time, Einstein arrived at the conviction that there<br />
were other difficulties implied by generally covariant field<br />
equations. One was connnected with energy-momentum<br />
conservation (see [10].)<br />
The 'hole' argument against general covariance<br />
At the time when he finished the paper with Grossmann,<br />
Einstein wrote to Ehrenfest on May 28, 1913: "The conviction<br />
to which I have slowly struggled through is that there<br />
are no preferred coordinate systems of any kind. However,<br />
I have only partially succee<strong>de</strong>d, even formally, in reaching<br />
this standpoint." (CPAE, Vol. 5, Doc. 441.) In a lecture given<br />
to the Annual Meeting of the Swiss Naturforschen<strong>de</strong> Gesellschaft<br />
in September 1913, Einstein stated: "It is possible<br />
to <strong>de</strong>monstrate by a general argument that equations<br />
that completely <strong>de</strong>termine the gravitational field cannot be<br />
generally covariant with respect to arbitrary substitutions."<br />
(CPAE, Vol. 4, Doc. 16.) He repeated this statement shortly<br />
afterwards in his Vienna lecture [13] of September 23, 1913.<br />
The so-called "hole" ("Loch") argument runs as follows<br />
(instead of coordinate transformations, I use a more mo<strong>de</strong>rn<br />
<strong>la</strong>nguage): Imagine a finite region D of spacetime – the<br />
'hole' – in which the stress-energy tensor vanishes. Assume<br />
that a metric field g is a solution of a generally covariant<br />
field equation. Apply now a diffeomorphism on g,<br />
Figure 3: A typical page in Einstein's 'Zürich Notebook', CPAE,<br />
Vol. 4, Doc. 10, p.262.<br />
50<br />
3 In his calcu<strong>la</strong>tion of the perihelion motion (on the basis of the vacuum<br />
equations R mn<br />
= 0) it became clear to him that spatial f<strong>la</strong>tness did not hold<br />
even for weak static fields.
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
producing *g (push-forward), and choose the diffeomorphism<br />
such that it leaves the spacetime region outsi<strong>de</strong> D<br />
pointwise fixed. Clearly, g and *g are different solutions<br />
of the field equation that agree outsi<strong>de</strong> D. In other words,<br />
generally covariant field equations allow huge families of<br />
solutions for one and the same matter distribution (outsi<strong>de</strong><br />
the hole). At the time, Einstein found this unacceptable, because<br />
this was in his opinion a dramatic failure of what he<br />
called the <strong>la</strong>w of causality (now usually called <strong>de</strong>terminism).<br />
He then thought that the energy-momentum tensor should<br />
(for appropriate boundary or initial conditions) <strong>de</strong>termine<br />
the metric uniquely.<br />
It took a long time until Einstein un<strong>de</strong>rstood that this nonuniqueness<br />
is an expression of what we now call gauge<br />
invariance, analogous to the local invariance of our gauge<br />
theories in elementary particle physics. On January 3, 1916<br />
he wrote to Besso: "Everything in the hole argument was<br />
correct up to the final conclusion."<br />
The role of diffeomorphism invariance of GR, especially for<br />
the Cauchy problem, was first un<strong>de</strong>rstood by Hilbert.<br />
Final remarks<br />
When Einstein was finishing his work on GR un<strong>de</strong>r great<br />
stress and was suspending all correspon<strong>de</strong>nce with colleagues,<br />
he still found time to communicate with Michele<br />
Besso. On November 17, 1915 he mailed a postcard from<br />
Berlin, that contains the great news:<br />
I have worked with great success during these months. General<br />
covariant gravitational equations. Motions of the perihelion<br />
quantitatively exp<strong>la</strong>ined. (...). You will be amazed. I<br />
worked horribly strenuously [schau<strong>de</strong>rhaft angestrengt], [it<br />
is] strange that one can endure that. (...) (CPAE, Vol. 8, Part<br />
A, Doc. 147).<br />
Besso passed this card on to Zangger: "I enclose the historical<br />
card of Einstein, reporting the setting of the capstone<br />
of an epoch that began with Newton’s 'apple'."<br />
The discovery of the general theory of re<strong>la</strong>tivity has often<br />
been justly praised as one of the greatest intellectual<br />
achievements of a human being. At the ceremonial presentation<br />
of Hubacher’s bust of A. Einstein in Zürich, W. Pauli<br />
said:<br />
The general theory of re<strong>la</strong>tivity then completed and - in<br />
contrast to the special theory - worked out by Einstein<br />
alone without simultaneous contributions by other researchers,<br />
will forever remain the c<strong>la</strong>ssic example of a<br />
theory of perfect beauty in its mathematical structure.<br />
Auszug aus einem Interview von Res Jost mit Otto<br />
Stern, <strong>de</strong>r mit Einstein von Prag nach Zürich kam<br />
und zwei Jahre später an <strong>de</strong>r ETH (mit einem Gutachten<br />
von Einstein) habilitierte:<br />
In Zürich war's natürlich sehr schön (...) und beson<strong>de</strong>rs<br />
<strong>de</strong>swegen interessant, weil Laue an <strong>de</strong>r Universität<br />
war. Ausser<strong>de</strong>m waren Ehrenfest und Tatjana (...)<br />
min<strong>de</strong>stens ein Vierteljahr, vielleicht auch etwas länger<br />
zu Besuch (...). Das gab natürlich immer herrliche Diskussionen<br />
im Kolloquium (...). Wir waren auch ein paar<br />
jüngere Leute, die ganz eifrig waren. Ehrenfest nannte<br />
uns immer <strong>de</strong>n 'Dreistern'. Das waren <strong>de</strong>r Herzfeld<br />
und <strong>de</strong>r Kern (und ich). (Kern hatte <strong>de</strong>n Doktor bei Debye<br />
gemacht.) Debye war ja <strong>de</strong>r Vorgänger von Laue<br />
an <strong>de</strong>r Universität (...). Nur <strong>de</strong>r Weiss (...), Pierre Weiss<br />
war damals Experimentalphysiker und Institutsdirektor,<br />
<strong>de</strong>r kam nie ins Kolloquium. Er verbot auch das<br />
Rauchen, das war furchtbar (...). Dem Einstein konnte<br />
man das aber nicht verbieten. Infolge<strong>de</strong>ssen, wenn<br />
es eben zu schlimm war, dann bin ich einfach ins<br />
Einstein'sche Zimmer gegangen (...) und konnte mich<br />
mit ihm unterhalten (...). Das gab dann immer lebhafte<br />
Diskussionen (...) über damals völlig ungelöste Rätsel<br />
<strong>de</strong>r Quantentheorie. Das einzige, was man über<br />
Quantentheorie wirklich wusste, war die P<strong>la</strong>nck'sche<br />
Formel, Schluss (...). Ich bin auch ins Kolleg zu Einstein<br />
gegangen (...), das war (...) auch sehr schön,<br />
aber nicht für Anfänger. Einstein hat sich ja nie richtig<br />
vorbereitet auf die Vorlesung, aber er war eben doch<br />
Einstein (...), wenn er da so herumgemorkst hat, war<br />
es doch sehr interessant (...), immer sehr raffiniert gemacht<br />
und sehr physikalisch vor allen Dingen (...).<br />
References<br />
[1] CPAE, The collected papers of Albert Einstein, Edited by J.<br />
Stachel et al., Vols. 1-12. Princeton: Princeton University Press,<br />
1987–2010.<br />
[2] A. Einstein, On the Re<strong>la</strong>tivity Principle and the Conclusions<br />
Drawn from It, CPAE, Vol. 2, Doc. 47.<br />
[3] A. Einstein, Erinnerungen-Souveniers, <strong>Schweizerische</strong> Hochschulzeitung<br />
28 (Son<strong>de</strong>rheft) (1955), pp. 145-153; reprinted as<br />
"Autobiographische Skizze", in Carl Seelig, ed., Helle Zeit-Dunkle<br />
Zeit. In Memoriam Albert Einstein, Zürich, Europa Ver<strong>la</strong>g, 1955,<br />
pp. 9-17.<br />
[4] A. Einstein, On the Influence of Gravitation on the Propagation<br />
of Light, CPAE, Vol. 3, Doc. 23.<br />
[5] A. Einstein, On the Theory of the Static Gravitational Field,<br />
CPAE, Vol. 4, Doc. 4.<br />
[6] L. Kollros, Erinnerungen-Souveniers, <strong>Schweizerische</strong> Hochschulzeitung<br />
28 (Son<strong>de</strong>rheft) (1955), pp. 169-173; reprinted as<br />
"Erinnerungen eines Kommilitonen", in Carl Seelig, ed., Helle Zeit-<br />
Dunkle Zeit. In Memoriam Albert Einstein, Zürich, Europa Ver<strong>la</strong>g,<br />
1955, pp. 17-31.<br />
[7] A. Einstein and M. Grossmann, Outline of a Generalized Theory<br />
of Re<strong>la</strong>tivity and a Theory of Gravitation, CPAE, Vol. 4, Doc.<br />
13. Entwurf einer verallgemeinerten Re<strong>la</strong>tivitätstheorie und einer<br />
Theorie <strong>de</strong>r Gravitation, Zeitschrift für Mathematik und Physik, 62,<br />
225-259 (1914).<br />
[8] A. Einstein, Research Notes on a Generalized Theory of Gravitation,<br />
August 1912, CPAE, Vol. 4, Doc. 10.<br />
[9] A. Einstein, Letter to H.A. Lorentz, CPAE, Vol. 5, Doc. 470.<br />
[10] N. Straumann, Einstein’s Zürich Notebook and his Journey<br />
to General Re<strong>la</strong>tivity, Ann. Phys. (Berlin) 523, 488 (2011); [arXiv:1106.0900].<br />
[11] N. Straumann, General Re<strong>la</strong>tivity, Graduate Texts in Physics,<br />
Springer Berlin, 2013.<br />
[12] A. Einstein, The Speed of Light and the Statics of the Gravitational<br />
Field, CPAE, Vol. 4, Doc. 3.<br />
[13] A. Einstein, On the Present State of the Problem of Gravitation,<br />
CPAE, Vol. 4, Doc. 17.<br />
51
SPG Mitteilungen Nr. 40<br />
Histoire <strong>de</strong> <strong>la</strong> Physique (9)<br />
Le modèle atomique <strong>de</strong> Bohr: origines, contexte et postérité (part 1)<br />
Jan Lacki, Uni Genève<br />
Nous célébrons cette année le centième anniversaire du<br />
modèle atomique <strong>de</strong> Niels Bohr. Pour le physicien, il est le<br />
commencement <strong>de</strong> <strong>la</strong> route qui al<strong>la</strong>it mener à <strong>la</strong> formu<strong>la</strong>tion<br />
<strong>de</strong> <strong>la</strong> mécanique quantique; pour l'homme <strong>de</strong> <strong>la</strong> rue,<br />
il symbolise à lui tout seul <strong>la</strong> nature quantique du mon<strong>de</strong><br />
atomique. Nombre <strong>de</strong> ses particu<strong>la</strong>rités sont <strong>de</strong>puis passées<br />
dans les esprits et se sont banalisées: c'est oublier<br />
combien ce modèle a été révolutionnaire à son époque et<br />
combien il reste encore aujourd'hui paradoxal, mais <strong>de</strong> ces<br />
paradoxes profonds et fructueux qui ont pavé <strong>la</strong> voie <strong>de</strong><br />
<strong>la</strong> physique contemporaine. L'atome <strong>de</strong> Bohr appartient<br />
ainsi à cette c<strong>la</strong>sse restreinte <strong>de</strong> gran<strong>de</strong>s idées qui ont fait<br />
basculer le cours <strong>de</strong> <strong>la</strong> science. Malgré cette importance,<br />
peu <strong>de</strong> personnes, y compris les physiciens, connaissent le<br />
contexte précis <strong>de</strong> <strong>la</strong> découverte <strong>de</strong> Bohr et <strong>la</strong> formu<strong>la</strong>tion<br />
qu'il donna à ses idées. Son article, tout comme, pour donner<br />
un autre exemple notable, celui d'Einstein initiant <strong>la</strong> re<strong>la</strong>tivité<br />
en 1905, est aujourd'hui peu connu et encore moins<br />
lu. Le centennaire du modèle <strong>de</strong> Bohr offre une excellente<br />
occasion <strong>de</strong> revenir sur cet épiso<strong>de</strong> capital <strong>de</strong> l'histoire <strong>de</strong><br />
<strong>la</strong> physique quantique.<br />
1 Une courte histoire <strong>de</strong> <strong>la</strong> spectroscopie<br />
Quand Bohr entre en scène, l'étu<strong>de</strong> <strong>de</strong>s spectres est vieille<br />
<strong>de</strong> plus d'un <strong>de</strong>mi-siècle, et ses racines remontent encore<br />
plus loin 1 . L'histoire commence avec l'observation du<br />
spectre so<strong>la</strong>ire par le britannique William H. Wol<strong>la</strong>ston, qui<br />
relève en 1802 l'existence <strong>de</strong>s raies sombres; elles intrigueront<br />
ensuite fortement Joseph v. Fraunhofer qui en comptera<br />
476 entre 1814 et 1815. Fraunhofer introduira aussi dans<br />
le champ <strong>de</strong> <strong>la</strong> spectroscopie l'usage <strong>de</strong>s réseaux et obtiendra<br />
ainsi <strong>de</strong>s résultats remarquables sur <strong>la</strong> re<strong>la</strong>tion entre<br />
l'angle d'observation et <strong>la</strong> longueur d'on<strong>de</strong> <strong>de</strong>s raies. Il se<br />
livrera également à l'étu<strong>de</strong> <strong>de</strong>s spectres d'émission provenant<br />
<strong>de</strong> f<strong>la</strong>mmes colorées ou encore d'étincelles produites<br />
par décharge <strong>de</strong>s machines électrostatiques. L'étu<strong>de</strong> <strong>de</strong>s<br />
spectres électriques se poursuivra et se systématisera avec<br />
l'utilisation <strong>de</strong>s bobines d'induction et, dans les années<br />
1845-1850, <strong>de</strong> <strong>la</strong> bobine <strong>de</strong> Ruhmkorff.<br />
Il reviendra à Gustav Kirchhoff (1859) d'apporter <strong>de</strong>s arguments<br />
décisifs en faveur <strong>de</strong> l'interprétation <strong>de</strong>s raies<br />
sombres du soleil comme <strong>de</strong>s raies d'absorption. Observons<br />
que c'est dans le contexte <strong>de</strong> ces travaux que Kirchhoff<br />
parviendra à une découverte capitale pour le développement<br />
ultérieur <strong>de</strong> <strong>la</strong> physique. Réfléchissant sur le<br />
rapport entre les pouvoirs d'émission et d'absorption d'un<br />
corps à une longueur d'on<strong>de</strong> et température données, Kirchhoff<br />
obtient son fameux résultat affirmant son universalité<br />
pour tout corps. C'est le début <strong>de</strong> <strong>la</strong> problématique du<br />
rayonnement du corps noir qui amènera à <strong>la</strong> toute fin du<br />
siècle à <strong>la</strong> loi du rayonnement <strong>de</strong> P<strong>la</strong>nck et <strong>la</strong> découverte<br />
<strong>de</strong>s quanta.<br />
A défaut d'une correspondance stable entre les éléments et<br />
leurs spectres (on a réalisé dans les années 1870 qu'un élément<br />
peut produire plusieurs spectres selon les conditions<br />
physiques ce qui met fin à l'espoir d'une spectrochimie), on<br />
observe tout <strong>de</strong> même d'autres régu<strong>la</strong>rités. On remarque<br />
<strong>de</strong>s analogies entre les spectres d'éléments aux mêmes<br />
propriétés chimiques et on relève <strong>de</strong>s rapports numériques<br />
entre raies d'un même élément (Mascart 1869, Lecoq <strong>de</strong><br />
Boisbaudrant 1869, Cornu 1885). L'observation <strong>de</strong>s doublets<br />
et triplets suggère que l'on a affaire à <strong>de</strong>s harmoniques.<br />
Les tentatives d'expliquer les spectres sur <strong>la</strong> base<br />
d'une mécanique <strong>de</strong> vibrations en analogie avec les phénomènes<br />
sonores s'en trouvent renforcées. Les spectres<br />
à raies correspondraient aux vibrations internes <strong>de</strong>s molécules<br />
alors que leur interaction dans les liqui<strong>de</strong>s et les soli<strong>de</strong>s<br />
conduirait aux spectres continus (Clifton 1866, Stoney<br />
1868, 1871). L'hypothèse d'harmoniques perd cependant<br />
<strong>de</strong> son attrait à partir <strong>de</strong>s années 1880: certaines raies seraient<br />
associées à <strong>de</strong>s harmoniques d'ordre trop élevé par<br />
rapport à ce qui est physiquement p<strong>la</strong>usible. Alors que l'on<br />
ne croit plus à une explication aussi simple <strong>de</strong>s spectres,<br />
<strong>la</strong> conviction <strong>de</strong> l'existence <strong>de</strong> lois bien définies régissant<br />
les fréquences spectrales et susceptibles <strong>de</strong> renseigner sur<br />
les mécanismes internes à l'atome va cependant croissant.<br />
L'histoire <strong>de</strong> <strong>la</strong> spectroscopie franchit une étape capitale<br />
avec l'obtention <strong>de</strong> premières lois empiriques pour les longueurs<br />
d'on<strong>de</strong> <strong>de</strong>s raies. La formule <strong>de</strong> Balmer (1885) pour<br />
les raies d'Ångström <strong>de</strong> l'hydrogène (1868), d'une précision<br />
remarquable, donne une impulsion forte à <strong>la</strong> recherche<br />
<strong>de</strong> formules empiriques <strong>de</strong> plus en plus générales. Cellesci<br />
culminent avec les contributions <strong>de</strong> Rydberg (1890) et<br />
bien sûr <strong>de</strong> Ritz avec son principe <strong>de</strong> combinaisons (1908).<br />
Ces travaux s'appuient <strong>de</strong> manière fondamentale sur <strong>la</strong> découverte<br />
récente, pour <strong>de</strong>s éléments chimiquement semb<strong>la</strong>bles,<br />
<strong>de</strong> l'existence <strong>de</strong> séries homologues aux propriétés<br />
communes comme celles <strong>de</strong> présenter un point d'accumu<strong>la</strong>tion<br />
vers les hautes fréquences avec <strong>de</strong>s intensités <strong>de</strong><br />
raies al<strong>la</strong>nt décroissant.<br />
2 La spectroscopie et <strong>la</strong> structure <strong>de</strong> l'atome: questions<br />
et enjeux au tournant du siècle<br />
1 Pour <strong>de</strong>s étu<strong>de</strong>s détaillées <strong>de</strong> l'histoire <strong>de</strong> <strong>la</strong> spectroscopie, on<br />
consultera H. Dingle, A Hundred Years of Spectroscopy, British Journal<br />
of History of Science, vol. 1 (1963), 199-216 ; M.C. Lawrence, The Role of<br />
Spectroscopy in the Acceptance of an Internally Structured Atom (1860-<br />
1920), thèse <strong>de</strong> doctorat, University of Wisconsin, 1964 ; W. McGucken,<br />
Nineteenth-Century Spectroscopy : <strong>de</strong>velopment of the un<strong>de</strong>rstanding of<br />
spectra, 1802-1897, Johns Hopkins Press, 1969 ; J. C. D. Brand, Lines<br />
of Light: The Sources of Dispersive Spectroscopy, 1800-1930, Gordon<br />
& Breach Science Pub., 1995 ou encore M. Sail<strong>la</strong>rd, Histoire <strong>de</strong> <strong>la</strong><br />
spectroscopie, Cahiers d'histoire et <strong>de</strong> philosophie <strong>de</strong>s sciences, no 26<br />
(1988).<br />
52<br />
L'obtention <strong>de</strong> formules empiriques pour les fréquences<br />
<strong>de</strong> séries <strong>de</strong> raies ne pouvait qu'aviver les tentatives pour<br />
concevoir un modèle <strong>de</strong> l'atome. Des modèles dynamiques<br />
avaient été proposés bien avant l'avènement <strong>de</strong> <strong>la</strong> théorie<br />
<strong>de</strong>s quanta et <strong>la</strong> découverte <strong>de</strong> l'électron. La conception <strong>de</strong><br />
<strong>la</strong> lumière comme ondu<strong>la</strong>tion d'un éther é<strong>la</strong>stique suggérait<br />
que les spectres résultaient <strong>de</strong> vibrations molécu<strong>la</strong>ires<br />
transmises mécaniquement à l'éther (Stokes 1852, Stoney<br />
1868). La question <strong>de</strong> <strong>la</strong> structure atomique qui permettait
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
ces vibrations ne pouvait donner lieu qu'à <strong>de</strong>s spécu<strong>la</strong>tions.<br />
Suivant les travaux <strong>de</strong> Helmholtz sur l'hydrodynamique<br />
<strong>de</strong>s vortex dans un flui<strong>de</strong> idéal (1858), William Thomson<br />
(Lord Kelvin) proposait déjà en 1867 un modèle <strong>de</strong> l'atome<br />
comme un vortex <strong>de</strong> l'éther. Plus que les résultats <strong>de</strong> <strong>la</strong><br />
spectroscopie, <strong>la</strong> découverte <strong>de</strong> l'électron (1896) rendit<br />
obsolètes ces premières tentatives. Avec l'idée d'électrons<br />
comme corpuscules fondamentaux <strong>de</strong> <strong>la</strong> matière, et<br />
donc <strong>de</strong> l'atome, on disposait d'un nouveau principe <strong>de</strong><br />
sa construction en prenant en compte l'émission <strong>de</strong> rayonnement<br />
électromagnétique par <strong>de</strong>s charges en accélération.<br />
Le mécanisme d'excitation mécanique <strong>de</strong> l'éther était<br />
remp<strong>la</strong>cé par celui <strong>de</strong> l'excitation électromagnétique par le<br />
mouvement <strong>de</strong> l'électron <strong>de</strong>venu oscil<strong>la</strong>teur hertzien (Larmor<br />
1897, pressenti par Stoney 1889). La difficulté principale<br />
consistait alors à concilier les conditions assurant les<br />
stabilités mécanique et radiative <strong>de</strong> l'atome. En effet, on<br />
savait <strong>de</strong>puis longtemps (Earnshaw 1831) qu'un système<br />
<strong>de</strong> corpuscules sous l'effet mutuel <strong>de</strong>s forces en inverse du<br />
carré <strong>de</strong> <strong>la</strong> distance ne pouvait donner lieu à <strong>de</strong>s configurations<br />
statiques stables: il fal<strong>la</strong>it donc que les électrons <strong>de</strong><br />
l'atome soient en mouvement. Ce<strong>la</strong> impliquait à son tour<br />
que ces électrons <strong>de</strong>vaient, pour rester confinés et assurer<br />
<strong>la</strong> permanence <strong>de</strong> l'atome, subir nécessairement <strong>de</strong>s accélérations<br />
et donc rayonner <strong>de</strong> l'énergie électromagnétique,<br />
ce qui hypothéquait <strong>de</strong> nouveau <strong>la</strong> stabilité <strong>de</strong> l'atome par<br />
perte <strong>de</strong> son énergie.<br />
Larmor montrait cependant en 1897 que les déperditions<br />
d'énergie pour un système <strong>de</strong> charges accélérées pouvaient<br />
être limitées, voire nulles, si <strong>la</strong> somme vectorielle <strong>de</strong>s<br />
accélérations était nulle. On le voit, <strong>la</strong> satisfaction simultanée<br />
<strong>de</strong> conditions assurant <strong>la</strong> stabilité constituait déjà en<br />
soi un problème formidable mais il fal<strong>la</strong>it encore que les solutions<br />
<strong>de</strong> ce problème soient en nombre suffisant pour expliquer<br />
<strong>la</strong> variété d'éléments chimiques connus. Comme si<br />
ces défis ne suffisaient pas, tout modèle stable <strong>de</strong> l'atome<br />
<strong>de</strong>vait <strong>de</strong> surcroît rendre compte <strong>de</strong>s raies spectrales en<br />
accord avec les formules empiriques <strong>de</strong> Rydberg et Ritz.<br />
Au vu <strong>de</strong> ces multiples exigences, souvent contradictoires,<br />
il n'est pas étonnant que peu <strong>de</strong> modèles atomiques réussissaient<br />
à les satisfaire toutes et encore, ils ne le faisaient<br />
qu'au prix d'hypothèses au caractère ad hoc marqué 2 . En<br />
1901, James H. Jeans proposait pour chaque électron <strong>de</strong><br />
l'atome l'existence d'un partenaire positif <strong>de</strong> même masse.<br />
Dans l'état normal <strong>de</strong> l'atome, <strong>la</strong> configuration d'ensemble<br />
pouvait être stable grâce à l'hypothèse d'une force compensant<br />
l'interaction électrostatique ; le spectre résultait<br />
<strong>de</strong>s oscil<strong>la</strong>tions électroniques autour <strong>de</strong>s positions d'équilibre.<br />
Avec ses "dynami<strong>de</strong>s", Philipp Lenard concevait au<br />
contraire <strong>de</strong>s paires <strong>de</strong> charges où le partenaire <strong>de</strong> l'électron<br />
avait une masse sensiblement plus gran<strong>de</strong> (1903).<br />
Nous nous souvenons mieux aujourd'hui <strong>de</strong>s conceptions<br />
<strong>de</strong> Jean Perrin qui, en 1901, suggérait un atome p<strong>la</strong>nétaire<br />
avec une charge positive retenant les charges négatives en<br />
orbite. Le Japonais Hantaro Nagaoka 1904 s'inspirait pour<br />
sa part <strong>de</strong>s réflexions <strong>de</strong> jeune Maxwell sur <strong>la</strong> stabilité gravitationnelle<br />
<strong>de</strong>s anneaux <strong>de</strong> Saturne (1860) pour proposer<br />
un modèle saturnien où <strong>de</strong>s anneaux <strong>de</strong> charges négatives<br />
en orbite présentent <strong>de</strong>s oscil<strong>la</strong>tions responsables <strong>de</strong>s<br />
2 Pour une étu<strong>de</strong> <strong>de</strong>s modèles atomiques proposés dans le cadre <strong>de</strong><br />
<strong>la</strong> physique c<strong>la</strong>ssique, voir Bruno Carazza et Nadia Robotti, Exp<strong>la</strong>ining<br />
Atomic Spectra within C<strong>la</strong>ssical Physics: 1897-1913, Annals of Science,<br />
vol. 59 (2002), 299-320.<br />
raies. Comme il s'avéra rapi<strong>de</strong>ment, le modèle <strong>de</strong> Nagaoka,<br />
basé sur les forces électrostatiques et non gravitationnelles,<br />
présentait en fait <strong>de</strong>s problèmes <strong>de</strong> stabilité mécanique,<br />
un handicap plus sérieux que celui <strong>de</strong> <strong>la</strong> déperdition<br />
d'énergie par rayonnement qui pouvait être résolu selon les<br />
lignes suggérées par Larmor.<br />
Dès 1903, J. J. Thomson concevait à son tour un modèle<br />
qui marqua pendant quelques années les esprits. Selon sa<br />
conception, <strong>la</strong> charge positive <strong>de</strong> l'atome était distribuée<br />
<strong>de</strong> manière uniforme dans tout le volume <strong>de</strong> l'atome. Les<br />
électrons, distribués en anneaux, tournaient à l'intérieur.<br />
S'appuyant sur les observations <strong>de</strong> Larmor, Thomson mettait<br />
beaucoup d'espoir dans le fait que ses configurations<br />
électroniques, pourvu qu'un nombre suffisant d'électrons<br />
soit considéré, présentaient un moment dipo<strong>la</strong>ire total nul,<br />
ce qui assurait, à cet ordre, l'absence <strong>de</strong> rayonnement<br />
électromagnétique. Peu <strong>de</strong> temps après le même Thomson<br />
montrait cependant que le nombre d'électrons dans l'atome<br />
<strong>de</strong>vait être <strong>de</strong> même ordre <strong>de</strong> gran<strong>de</strong>ur que le nombre atomique<br />
(1906). Ce<strong>la</strong> mettait fin à <strong>de</strong> nombreux modèles qui<br />
multipliaient le nombre <strong>de</strong>s électrons à outrance, à commencer<br />
par le sien.<br />
La contrainte sur le nombre d'électrons présents dans<br />
l'atome permit à l'époque <strong>de</strong> trancher aussi l'importante<br />
question <strong>de</strong> savoir si l'ensemble <strong>de</strong> raies du spectre pouvait<br />
être imputé à une seule source, un atome dans une<br />
seule configuration, ou si <strong>de</strong>s configurations différentes<br />
d'un même atome, voire <strong>de</strong>s variétés atomiques différentes,<br />
<strong>de</strong>vaient être envisagées pour chaque raie. Comme<br />
les solutions à une seule source pour l'ensemble du spectre<br />
impliquaient un nombre prohibitif d'électrons 3 , on finit par<br />
pencher en faveur <strong>de</strong> configurations atomiques différentes<br />
pour chaque raie.<br />
Une étu<strong>de</strong> <strong>de</strong>s modèles atomiques ne <strong>de</strong>vrait pas à ce<br />
sta<strong>de</strong> omettre les conceptions du suisse Walter Ritz et <strong>de</strong><br />
son compatriote Arthur Schidlof. Comme j'eus déja l'occasion<br />
<strong>de</strong> traiter du parcours scientifique <strong>de</strong> ces <strong>de</strong>ux pionniers<br />
<strong>de</strong> <strong>la</strong> physique théorique suisse dans les Communications<br />
4 je terminerai juste sur une remarque. Les modèles<br />
<strong>de</strong> Ritz étaient caractéristiques <strong>de</strong> leur temps. Tout comme<br />
ceux <strong>de</strong> ses contemporains, ils étaient a posteriori handicapés<br />
par <strong>la</strong> conjonction d'une physique c<strong>la</strong>ssique et d'hypothèses<br />
ad hoc. Schidlof, en prenant en compte l'existence<br />
du quantum d'action (1911), apparaît au contraire se mettre<br />
résolument du côté d'une physique nouvelle 5 . Sa pensée<br />
est pourtant encore insuffisamment affranchie <strong>de</strong> <strong>la</strong> tradition<br />
c<strong>la</strong>ssique: elle ne visait pas tant l'obtention d'un modèle<br />
quantique <strong>de</strong> l'atome qu'une explication <strong>de</strong> l'existence<br />
et <strong>de</strong> <strong>la</strong> valeur du quantum d'action <strong>de</strong> P<strong>la</strong>nck. Ce sera tout<br />
le contraire avec <strong>la</strong> contribution <strong>de</strong> Bohr.<br />
3 L'avancée <strong>de</strong> Niels Bohr<br />
Quand Bohr propose son modèle, les quanta viennent à<br />
peine d'être acceptés comme une réalité physique incon-<br />
3 Voir Carazza et Robotti, op. cit., pp. 313-315.<br />
4 J. Lacki, Arthur Schidlof, un pionnier <strong>de</strong> <strong>la</strong> physique théorique suisse,<br />
Communications <strong>de</strong> <strong>la</strong> SSP, no 34, mai 2011, 48-51; Walter Ritz (1878-<br />
1909), the revolutionary c<strong>la</strong>ssical physicist, Communications <strong>de</strong> <strong>la</strong> SSP,<br />
no 35, septembre 2011, 26-29.<br />
5 A. Schidlof, Zur Aufklärung <strong>de</strong>r universellen elektrodynamischen<br />
Be<strong>de</strong>utung <strong>de</strong>r P<strong>la</strong>nckschen Strahlungskonstanten h, Annalen <strong>de</strong>r Physik,<br />
vol. 340 (1911), 90-100.<br />
53
SPG Mitteilungen Nr. 40<br />
tournable. Autant on salue en 1900 <strong>la</strong> loi du rayonnement<br />
du corps noir <strong>de</strong> P<strong>la</strong>nck comme une gran<strong>de</strong> réussite, autant<br />
on fait peu <strong>de</strong> cas, pour ne pas dire qu'on rejette, l'explication<br />
("désespérée" comme l'avait qualifiée lui-même<br />
P<strong>la</strong>nck) <strong>de</strong> cette loi en termes <strong>de</strong> discontinuités dans les<br />
échanges énergétiques entre matière et rayonnement. Des<br />
années après <strong>la</strong> découverte <strong>de</strong> P<strong>la</strong>nck on en cherchera encore<br />
une justification "c<strong>la</strong>ssique". Il y a pourtant <strong>de</strong>s esprits<br />
qui prennent les quanta d'emblée au sérieux, ainsi le jeune<br />
Einstein qui contribuera pour beaucoup à leur donner une<br />
respectabilité. Dans l'un <strong>de</strong>s articles <strong>de</strong> sa "merveilleuse<br />
année" 1905 Einstein montre que dans le régime <strong>de</strong> Wien<br />
(gran<strong>de</strong>s fréquences/petites températures) les propriétés<br />
thermodynamiques d'un volume d'énergie électromagnétique<br />
monochromatique <strong>de</strong> fréquence n sont thermodynamiquement<br />
semb<strong>la</strong>bles à celles d'un gaz <strong>de</strong> corpuscules<br />
d'énergie individuelle hn 6 . Ces "grains" d'énergie, dont<br />
Einstein se gar<strong>de</strong> encore bien d'affirmer l'existence physique<br />
autonome, signalent un aspect corpuscu<strong>la</strong>ire <strong>de</strong> <strong>la</strong><br />
lumière: plus tard Einstein montrera, toujours dans le cadre<br />
d'une analyse <strong>de</strong> propriétés énergétiques, que cet aspect<br />
cohabite avec celui, c<strong>la</strong>ssique et familier, <strong>de</strong>s phénomènes<br />
ondu<strong>la</strong>toires 7 . C'est l'application <strong>de</strong> <strong>la</strong> nature "granu<strong>la</strong>ire"<br />
<strong>de</strong> l'énergie électromagnétique à l'explication <strong>de</strong> l'effet photoélectrique,<br />
plutôt que <strong>la</strong> re<strong>la</strong>tivité, qui apportera à Einstein<br />
son prix Nobel 8 . En 1907 Einstein récidive sur le chemin <strong>de</strong><br />
l'exploration <strong>de</strong>s conséquences "quantiques" <strong>de</strong> <strong>la</strong> loi <strong>de</strong><br />
P<strong>la</strong>nck: si on comprend cette <strong>de</strong>rnière comme remp<strong>la</strong>cant<br />
l'énergie moyenne c<strong>la</strong>ssique d'un oscil<strong>la</strong>teur unidimensionnel,<br />
kT, par l'expression:<br />
kT "<br />
ho<br />
ho<br />
e kT - 1<br />
alors pourquoi ne pas opérer cette substitution pour les oscil<strong>la</strong>teurs<br />
matériels modélisant <strong>la</strong> matière dans les soli<strong>de</strong>s ?<br />
9<br />
Le résultat permet d'expliquer immédiatement <strong>la</strong> décroissance<br />
<strong>de</strong>s chaleurs spécifiques à basse température, l'une<br />
<strong>de</strong>s énigmes qui, vers <strong>la</strong> fin du XIX e siècle, constituait un<br />
argument puissant contre <strong>la</strong> théorie cinétique <strong>de</strong>s gaz et<br />
contre toute reconstruction <strong>de</strong> <strong>la</strong> thermodynamique sur <strong>la</strong><br />
base d'une mécanique <strong>de</strong>s constituants atomiques: grâce<br />
à Einstein, on comprend que ce n'était pas tant cette approche<br />
qui était fautive, mais les lois mécaniques sur les-<br />
6 Über einen die Erzeugung und Verwandlung <strong>de</strong>s Lichtes betreffen<strong>de</strong>n<br />
heuristischen Gesichtspunkt, Annalen <strong>de</strong>r Physik, vol. 17 (1905), pp. 132-<br />
148<br />
7 Entwicklung unserer Anschauungen über das Wesen und die<br />
Konstitution <strong>de</strong>r Strahlung, Physikalische Zeitschrift, vol. 10 (1909),<br />
817-825, conférence donnée lors du 81 e congrès <strong>de</strong> <strong>la</strong> Gesellschaft<br />
Deutscher Naturforscher à Salzburg. Einstein y argumente aussi en faveur<br />
d'un quantum <strong>de</strong> lumière aux propriétés résolument corpuscu<strong>la</strong>ires. Il<br />
faudra cependant encore <strong>de</strong>s années avant que l'idée ne s'impose: les<br />
expériences <strong>de</strong> <strong>la</strong> diffusion <strong>de</strong> Compton (1923) jouèrent ici un rôle décisif.<br />
Il est intéressant d'observer que Niels Bohr lui-même rejettera intialement<br />
<strong>la</strong> réalité <strong>de</strong>s corpuscules <strong>de</strong> lumière préférant dans un premier temps<br />
voir dans les aspects corpuscu<strong>la</strong>ires une manifestation <strong>de</strong> l'insuffisance,<br />
à l'échelle atomique, <strong>de</strong>s <strong>de</strong>scriptions spatio-temporelles, voir par<br />
exemple Dugald Murdoch, Niels Bohr's philosophy of physics, Cambridge<br />
University Press, 1989.<br />
8 On connaît bien les hésitations du comité du Nobel <strong>de</strong> physique à<br />
récompenser Einstein pour <strong>la</strong> re<strong>la</strong>tivité, voir R. M. Friedman, The Politics<br />
of Excellence: Behind the Nobel Prize in Science, W. H. Freeman Books,<br />
2001.<br />
9 Die P<strong>la</strong>ncksche Theorie <strong>de</strong>r Strahlung und die Theorie <strong>de</strong>r spezifischen<br />
Wärme, Annalen <strong>de</strong>r Physik, vol. 22 (1907),180-190.<br />
54<br />
quelles elle s'appuyait 10 .<br />
Ces <strong>de</strong>ux succès, où le génie d'Einstein se révèle autant<br />
que dans son article sur l'électrodynamique <strong>de</strong>s corps en<br />
mouvement, contribuent plus que tout autre, à convaincre<br />
<strong>la</strong> communauté <strong>de</strong> l'intérêt <strong>de</strong> l'hypothèse quantique et,<br />
progressivement, <strong>de</strong> l'existence réelle <strong>de</strong>s quanta. La première<br />
conférence Solvay en 1911 dont nous connaissons<br />
<strong>la</strong> photographie emblématique est consacrée à "La théorie<br />
du rayonnement et les quanta": on peut dire que ses travaux<br />
officialisent les quanta comme partie intégrante <strong>de</strong> <strong>la</strong><br />
physique 11 . Cependant, nous sommes encore loin d'une<br />
modification que les quanta opéreraient sur les lois <strong>de</strong>s<br />
systèmes individuels: dans ses <strong>de</strong>ux travaux Einstein tire<br />
les conséquences <strong>de</strong> l'existence <strong>de</strong>s quanta à partir d'un<br />
travail d'analyse <strong>de</strong>s lois phénoménologiques obtenues par<br />
ses prédécesseurs (Wien, P<strong>la</strong>nck, etc.) mais il ne les dérive<br />
pas d'une modification postulée <strong>de</strong>s lois <strong>de</strong> base <strong>de</strong> <strong>la</strong> mécanique<br />
ou <strong>de</strong> l'électrodynamique affectant les constituants<br />
élementaires 12 . Bohr se confrontera en revanche frontalement<br />
à ces lois c<strong>la</strong>ssiques et c'est précisément pour cette<br />
raison que sa contribution est une étape capitale sur le chemin<br />
<strong>de</strong> <strong>la</strong> mécanique quantique.<br />
A l'époque <strong>de</strong> <strong>la</strong> formu<strong>la</strong>tion <strong>de</strong> son modèle Niels Bohr est<br />
<strong>de</strong>puis mars 1912 col<strong>la</strong>borateur au <strong>la</strong>boratoire <strong>de</strong> Rutherford<br />
à Manchester. Il vient à peine <strong>de</strong> défendre sa thèse<br />
à Copenhague sur "<strong>la</strong> théorie électronique <strong>de</strong>s métaux"<br />
(1911). Après un séjour décevant chez J. J. Thomson à<br />
Cambridge qui voit les <strong>de</strong>ux hommes s'affronter à propos<br />
du... modèle atomique <strong>de</strong> Thomson, Bohr se tourne<br />
vers Rutherford 13 . Celui-ci vient à l'époque d'apporter <strong>de</strong>s<br />
arguments décisifs contre <strong>la</strong> conception <strong>de</strong> Thomson en<br />
montrant que les expériences <strong>de</strong> <strong>la</strong> diffusion à <strong>la</strong>rge angle<br />
<strong>de</strong>s particules alpha concluent aux effets d'une déflection<br />
unique sur <strong>de</strong>s centres <strong>de</strong> diffusion intraatomiques: le<br />
noyau atomique est découvert 14 . L'accueil que Bohr reçoit<br />
<strong>de</strong> <strong>la</strong> part du Néo-zé<strong>la</strong>ndais est d'emblée meilleur que celui<br />
que lui a reservé Thomson. Rutherford est convaincu <strong>de</strong><br />
l'importance <strong>de</strong>s idées <strong>de</strong> P<strong>la</strong>nck et encourage les efforts<br />
<strong>de</strong> son jeune collègue. Dans son <strong>la</strong>boratoire Bohr travaille<br />
sur l'absorption <strong>de</strong>s particules alpha par <strong>la</strong> matière et c'est<br />
pour lui l'occasion <strong>de</strong> se rapprocher encore plus <strong>de</strong> <strong>la</strong> pro-<br />
10 Pour les critiques <strong>de</strong> <strong>la</strong> théorie cinétique au XIXe siècle, voir S. Brush,<br />
The kind of motion we call heat. A History of the Kinetic Theory of Gases in<br />
the Nineteenth Century, North Hol<strong>la</strong>nd, 1986.<br />
11 C'est Walter Nernst, impressionné par les travaux d'Einstein, qui<br />
persua<strong>de</strong> le riche industriel Ernest Solvay <strong>de</strong> financer une conférence<br />
solennelle consacrée à <strong>la</strong> physique quantique, voir D. Kormos Barkan,<br />
The Witches' Sabbath: The First International Solvay Congress in Physics,<br />
Science in Context, vol. 6 (1993), 59-82. aussi M.-C. Bustamante, Paul<br />
Langevin et le Conseil Solvay <strong>de</strong> 1911, Images <strong>de</strong> <strong>la</strong> physique, 2011, 3-9.<br />
12 Ce<strong>la</strong> permet <strong>de</strong> comprendre comment Einstein est dans ces<br />
années indiscutablement un père fondateur <strong>de</strong> <strong>la</strong> théorie quantique alors<br />
qu'il <strong>de</strong>viendra, un dizaine d'années plus tard, un féroce critique <strong>de</strong> <strong>la</strong><br />
mécanique quantique. L'existence <strong>de</strong>s quanta n'entrait à ce moment pas<br />
en conflit avec les convictions profon<strong>de</strong>s d'Einstein sur <strong>la</strong> réalité et sur<br />
<strong>la</strong> manière dont nous <strong>de</strong>vrions <strong>la</strong> décrire: les thèmes d'indéterminisme,<br />
<strong>de</strong> l'inexistence <strong>de</strong> propriétés objectives <strong>de</strong>s systèmes, contre lesquels<br />
Einstein se battra jusqu'à <strong>la</strong> fin, n'étaient pas (encore) affleurants à<br />
<strong>la</strong> surface <strong>de</strong> <strong>la</strong> nouvelle physique quantique. Tout changera avec <strong>la</strong><br />
mécanique quantique et surtout l'interprétation qu'en prônera Bohr.<br />
13 Dans son survol "60 years of quantum mechanics", E. U. Condon<br />
rapporte que Bohr, suite à son désaccord avec Thomson, avait été<br />
"poliment invité" à aller voir ailleurs, voir Physics Today, vol. 15 (1962), 45.<br />
14 The scattering of alpha and beta particles by matter and the structure<br />
of the atom, Philosophical Magazine, vol. 21 (1911), 669-688.
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
blématique <strong>de</strong> l'atome 15 . Le modèle nucléaire <strong>de</strong> l'atome<br />
suggéré par Rutherford offre un cadre prometteur mais entraîne<br />
aussi son lot <strong>de</strong> problèmes. En particulier, Bohr réalise<br />
que les lois dynamiques c<strong>la</strong>ssiques sont impuissantes<br />
à fixer seules une échelle pour sa taille. En termes d'analyse<br />
dimensionnelle, il manque un ingrédient: le modèle <strong>de</strong><br />
Rutherford faisant intervenir les masses et les charges <strong>de</strong>s<br />
électrons, on peut se convaincre qu'il est impossible <strong>de</strong><br />
construire à partir <strong>de</strong> là une constante ayant <strong>la</strong> dimension<br />
d'une longueur. Tout change cependant si l'on introduit<br />
<strong>la</strong> constante <strong>de</strong> P<strong>la</strong>nck: on peut alors former l'expression<br />
h 2 /me 2 qui a non seulement <strong>la</strong> bonne dimension mais aussi<br />
le bon ordre <strong>de</strong> gran<strong>de</strong>ur atomique (h 2 /me 2 2·10 -10 m). La<br />
stratégie <strong>de</strong> Bohr al<strong>la</strong>it dès lors différer considérablement<br />
<strong>de</strong> celle <strong>de</strong> ses pré<strong>de</strong>cesseurs comme Schidlof. Alors que<br />
ce <strong>de</strong>rnier espérait, comme on l'a vu, justifier <strong>la</strong> valeur <strong>de</strong><br />
<strong>la</strong> constante h sur <strong>la</strong> base d'un mécanisme atomique décrit<br />
en termes c<strong>la</strong>ssiques, Bohr renverse <strong>la</strong> perspective en<br />
prenant acte <strong>de</strong> l'existence du quantum d'action et <strong>de</strong> sa<br />
valeur h pour rendre compte <strong>de</strong> <strong>la</strong> structure <strong>de</strong> l'atome et<br />
dériver les propriétés <strong>de</strong> son spectre. Il fal<strong>la</strong>it encore qu'il<br />
comprenne comment lier <strong>la</strong> constante <strong>de</strong> P<strong>la</strong>nck au champ<br />
<strong>de</strong> ses recherches. De retour à Copenhague dès septembre<br />
1912, Bohr ne prenait pas encore en considération ce que<br />
les données spectroscopiques pouvaient lui enseigner mais<br />
dès qu'il eut compris l'importance <strong>de</strong>s formules établies<br />
par Balmer, Rydberg et Ritz, les pièces du puzzle commencèrent<br />
à s'assembler: "dès que je pris connaissance <strong>de</strong> <strong>la</strong><br />
formule <strong>de</strong> Balmer, toute cette affaire <strong>de</strong>vint c<strong>la</strong>ire" 16 .<br />
Nous pouvons maintenant examiner les idées fortes du<br />
modèle <strong>de</strong> Bohr, non pas tant pour les découvrir (elles sont<br />
passées <strong>la</strong>rgement dans notre culture), mais pour examiner<br />
comment Bohr les exposa à l'origine dans sa publication 17 .<br />
Pour un atome constitué d'une charge positive E autour <strong>de</strong><br />
<strong>la</strong>quelle orbite une charge égale mais <strong>de</strong> signe opposé e,<br />
l'énergie totale est:<br />
W T V<br />
1 2<br />
= + = mv +<br />
Ee<br />
2<br />
2 r<br />
La condition <strong>de</strong> stabilité pour une orbite circu<strong>la</strong>ire <strong>de</strong> rayon<br />
r et fréquence n donne<br />
mv<br />
r<br />
2<br />
Ee<br />
2<br />
=- m r<br />
Ee<br />
2<br />
, ~ =-<br />
2<br />
,<br />
r<br />
r<br />
et, pour l'atome d'hydrogène (E = -e),<br />
2<br />
2<br />
2<br />
m r<br />
e<br />
2 e<br />
2<br />
~ =<br />
2<br />
( ~ =<br />
3<br />
= ( 2ro)<br />
.<br />
r<br />
mr<br />
2<br />
Ainsi W =-<br />
e<br />
, alors que o<br />
2r<br />
2<br />
3<br />
=-<br />
8W<br />
2 4<br />
.<br />
4r<br />
e m<br />
15 On the theory of the <strong>de</strong>crease of velocity of moving electrified particles<br />
on passing through matter, Philosophical Magazine, vol. 25 (1913), 10-31.<br />
16 "As soon as I saw Balmer's formu<strong>la</strong>, the whole thing was immediately<br />
clear to me", cité par Max Jammer, The conceptual <strong>de</strong>velopement of<br />
quantum mechanics, McGraw Hill, 1966, p. 77.<br />
17 On the constitution of atoms and molecules, Philosophical Magazine,<br />
vol. 26 (1913), 1-25, 476-502, 857-875.<br />
La donnée <strong>de</strong> l'energie détermine donc entièrement l'orbite<br />
circu<strong>la</strong>ire correspondante 18 .<br />
Mais comment faire entrer l'hypothèse <strong>de</strong>s quanta, et <strong>la</strong> dimension<br />
<strong>de</strong> h, dans le problème <strong>de</strong> <strong>la</strong> structure <strong>de</strong> l'atome ?<br />
Certes, <strong>la</strong> quantification <strong>de</strong>s échanges énergétiques entre<br />
<strong>la</strong> matière et le rayonnement doit avoir une conséquence<br />
au niveau <strong>de</strong> <strong>la</strong> structure atomique, mais comment faire le<br />
lien ? Bohr propose <strong>de</strong> considérer le processus <strong>de</strong> <strong>la</strong> formation<br />
<strong>de</strong> l'atome par <strong>la</strong> capture d'un électron par le noyau.<br />
Infiniment loin du noyau l'électron est libre, W = 0. Supposons<br />
qu'il soit capturé sur une orbite d'énergie W négative<br />
(état lié !). Par <strong>la</strong> conservation <strong>de</strong> l'énergie, une quantité<br />
d'énergie positive, -W, doit être libérée dans le processus:<br />
Bohr, suivant l'hypothèse quantique, suppose que c'est<br />
sous <strong>la</strong> forme d'un rayonnement d'un certain nombre t (entier<br />
!) <strong>de</strong> quanta d'énergie. Il pose:<br />
- W = xhol / xh o , (1) 2<br />
avec <strong>la</strong> fréquence du quantum rayonné n' posée égale à<br />
<strong>la</strong> moitié (!) <strong>de</strong> <strong>la</strong> fréquence <strong>de</strong> révolution mécanique <strong>de</strong><br />
l'orbite <strong>de</strong> capture. L'hypothèse <strong>de</strong> Bohr fixe, parmi le<br />
continuum <strong>de</strong>s énergies un nombre infini, mais néanmoins<br />
discret, d'entre elles :<br />
2 4<br />
- W =<br />
2r<br />
e m 1<br />
2 2<br />
. (2)<br />
h x<br />
La différence <strong>de</strong>s énergies, pour <strong>de</strong>ux nombres t 1<br />
et t 2<br />
donnés est alors :<br />
2 4<br />
D W =-<br />
2r<br />
e m 1 1<br />
2 c 2<br />
-<br />
2 m ;<br />
h x2<br />
x1<br />
Si <strong>de</strong> tels processus <strong>de</strong> changement <strong>de</strong> niveau énergétique<br />
surviennent dans l'atome, on doit supposer, avec Bohr,<br />
qu'ils donnent lieu à une émission/absorption <strong>de</strong> quanta<br />
d'énergie <strong>de</strong> rayonnement électromagnétique <strong>de</strong> frequence<br />
n' donnée par <strong>la</strong> formule<br />
2 4<br />
hol =- DW<br />
=<br />
2r<br />
e m 1 1<br />
2 c 2<br />
-<br />
2 m .<br />
h x2<br />
x1<br />
En posant t 2<br />
= 2, et t 1<br />
= 3; 4; 5; ... <strong>la</strong> formule ci-<strong>de</strong>ssus<br />
reproduit les valeurs <strong>de</strong>s fréquences <strong>de</strong>s raies spectrales<br />
<strong>de</strong> <strong>la</strong> série <strong>de</strong> Balmer (1885) exprimée, dans <strong>la</strong> formule <strong>de</strong><br />
Rydberg (1890), par:<br />
ol = Rcc 1 1<br />
2<br />
-<br />
2 m .<br />
x2<br />
x1<br />
Bohr avait donc réussi à obtenir <strong>la</strong> valeur <strong>de</strong> <strong>la</strong> constante <strong>de</strong><br />
Rydberg R à partir <strong>de</strong> constantes élémentaires,<br />
2 4<br />
R =<br />
2r<br />
e m<br />
3<br />
.<br />
ch<br />
18 En fait on peut montrer que le résultat s'applique aussi aux orbites<br />
elliptiques: leur grand axe 2r et <strong>la</strong> fréquence <strong>de</strong> rotation <strong>de</strong> l'électron n sont<br />
déterminés par <strong>la</strong> donnée <strong>de</strong> l'énergie <strong>de</strong> l'orbite et ne <strong>de</strong>pen<strong>de</strong>nt pas <strong>de</strong><br />
<strong>la</strong> valeur <strong>de</strong> l'excentricité.<br />
Pour <strong>de</strong>s raisons éditoriales, <strong>la</strong> suite <strong>de</strong> cet article apparaîtra dans les prochaines Communications <strong>de</strong> <strong>la</strong> SSP, no. 41.<br />
55
SPG Mitteilungen Nr. 40<br />
Geschichte <strong>de</strong>s SIN<br />
Buchbesprechung von Andreas Pritzker<br />
Im Hinblick auf Scherrers Emeritierung 1960 wählte <strong>de</strong>r<br />
Bun<strong>de</strong>srat 1959 Jean-Pierre B<strong>la</strong>ser zu <strong>de</strong>ssen Nachfolger<br />
an <strong>de</strong>r ETH. B<strong>la</strong>ser "erbte" die Zyklotronp<strong>la</strong>nungsgruppe.<br />
Unter <strong>de</strong>m Eindruck <strong>de</strong>r weltweiten Entwicklung strebte<br />
B<strong>la</strong>ser allerdings anstelle eines Zyklotrons für die Kernphysik<br />
eine Maschine an, die <strong>de</strong>n Einstieg in die Hochenergiephysik<br />
ermöglichte. Er wur<strong>de</strong> dabei unterstützt durch <strong>de</strong>n<br />
Theoretiker Res Jost, <strong>de</strong>r die Hochenergiephysik als fruchtbares<br />
künftiges Arbeitsgebiet betrachtete.<br />
B<strong>la</strong>ser, <strong>de</strong>r En<strong>de</strong> Februar 2013 seinen 90. Geburtstag feiern<br />
konnte, verfolgte dabei die I<strong>de</strong>e eines grossen Teilchenbeschleunigers,<br />
<strong>de</strong>n die ETH für sämtliche schweizerischen<br />
Universitäten betreiben sollte. In <strong>de</strong>n 1950er Jahren waren<br />
weltweit mehrere Maschinen im Bereich um 500 MeV gebaut<br />
wor<strong>de</strong>n. Sie ermöglichten es, Mesonen künstlich zu<br />
erzeugen und vorerst als solche zu studieren. Der nächste<br />
Schritt war die I<strong>de</strong>e, Mesonen als Werkzeuge einzusetzen.<br />
Die Mesonen wur<strong>de</strong>n mit Protonenbeschleunigern erzeugt.<br />
Für die sogenannten Mesonenfabriken waren hohe Protonenströme<br />
- man sprach von 100 Mikroamp - notwendig.<br />
Andreas Pritzker: Geschichte <strong>de</strong>s SIN. 188 Seiten,<br />
ISBN 978-3-905993-10-3, munda-Ver<strong>la</strong>g.<br />
Das Buch erzählt die Geschichte <strong>de</strong>s <strong>Schweizerische</strong>n Instituts<br />
für Nuklearforschung (SIN). Das Institut wur<strong>de</strong> 1968<br />
gegrün<strong>de</strong>t und ging 1988 ins Paul Scherrer Institut (PSI)<br />
über. Die Gründung <strong>de</strong>s SIN erfolgte in einer Zeit, als die<br />
Physik als Schlüsseldisziplin für die technologische und<br />
gesellschaftliche Entwicklung galt. Der Schritt war für ein<br />
kleines Land wie die Schweiz ungewöhnlich und zeugte<br />
von Mut und Weitsicht. Ungewöhnlich waren in <strong>de</strong>r Folge<br />
die Leistungen <strong>de</strong>s SIN im weltweiten Vergleich sowie sein<br />
Einfluss auf die schweizerische, teils auf die internationale<br />
Wissenschaftspolitik.<br />
Die Ausgangs<strong>la</strong>ge war günstig. Die ETH Zürich war bereits<br />
in <strong>de</strong>n 1930er Jahren führend im Gebiet <strong>de</strong>r Kernphysik.<br />
Zu<strong>de</strong>m wur<strong>de</strong> in <strong>de</strong>n 1950er Jahren das CERN in Genf gegrün<strong>de</strong>t.<br />
An bei<strong>de</strong>m war Paul Scherrer, Leiter <strong>de</strong>s Physikalischen<br />
Instituts <strong>de</strong>r ETH, massgeblich beteiligt. Er sorgte<br />
früh dafür, dass an <strong>de</strong>r ETH Teilchenbeschleuniger als Forschungsinstrumente<br />
eingesetzt wur<strong>de</strong>n. Eines davon war<br />
das berühmte ETH-Zyklotron. Als sich <strong>de</strong>ssen Nutzungsmöglichkeiten<br />
in <strong>de</strong>n 1950er Jahren allmählich erschöpften,<br />
grün<strong>de</strong>te Scherrer die Zyklotronp<strong>la</strong>nungsgruppe, welche<br />
<strong>de</strong>n Bau einer leistungsfähigeren Maschine für die Kernphysik<br />
zum Ziel hatte. Bereits diese hätte <strong>de</strong>n Rahmen<br />
eines einzelnen Hochschulinstituts gesprengt. In <strong>de</strong>r P<strong>la</strong>nungsgruppe<br />
waren <strong>de</strong>nn auch die Universitäten von Basel<br />
und Zürich vertreten.<br />
56<br />
Der Ringbeschleuniger <strong>de</strong>s SIN mit seinen Erbauern im September<br />
1973<br />
Hans Wil<strong>la</strong>x, <strong>de</strong>n bereits Scherrer als Physiker angestellt<br />
hatte, entwarf das zweistufige Zyklotron-Konzept, das später<br />
unter seiner Leitung verwirklicht wur<strong>de</strong>. Obschon <strong>de</strong>m<br />
Projekt, wie bei solchen Vorhaben üblich, Opposition aus<br />
Hochschulkreisen erwuchs, waren Bun<strong>de</strong>srat Tschudi und<br />
ETH-Präsi<strong>de</strong>nt Pallmann entschlossen, es zu verwirklichen,<br />
weil sie sich starke Impulse für <strong>de</strong>n Forschungsstandort<br />
Schweiz versprachen. Die Eidgenössischen Räte bewilligten<br />
1965 (im Rahmen einer Baubotschaft, welche auch die<br />
ersten Bauten <strong>de</strong>r ETH-Hönggerberg umfasste) einen Baukredit<br />
von beinahe 100 Millionen Franken. Und auf Anfang<br />
1968 wur<strong>de</strong> das SIN als Annexanstalt <strong>de</strong>r ETH gegrün<strong>de</strong>t.<br />
Von 1966 an entwickelten zumeist junge, begabte Physiker<br />
unter <strong>de</strong>r Leitung von B<strong>la</strong>ser und Wil<strong>la</strong>x an <strong>de</strong>r ETH, dann<br />
bei <strong>de</strong>r Maschinenfabrik Oerlikon das SIN-Zyklotron, und<br />
ab 1968 wur<strong>de</strong> das Institut auf <strong>de</strong>r grünen Wiese in Villigen,<br />
gegenüber <strong>de</strong>m ebenfalls zur ETH gehören<strong>de</strong>n Eidgenössischen<br />
Institut für Reaktorforschung (EIR) erbaut. Im Februar<br />
1974 war es dann soweit: das SIN produzierte die<br />
ersten Pionen.
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Gute Stimmung im Kontrollraum <strong>de</strong>s SIN am 24. Februar 1974, als<br />
die ersten Pionen produziert wur<strong>de</strong>n.<br />
Die Beschleunigeran<strong>la</strong>ge erfüllte sämtliche Erwartungen.<br />
Sie wur<strong>de</strong> in <strong>de</strong>n folgen<strong>de</strong>n Jahrzehnten <strong>la</strong>ufend ausgebaut<br />
und erreichte in ihrem Einsatzbereich die Weltspitze. Ihre<br />
Qualität <strong>la</strong>g aber darin, dass sie, als die Teilchenphysik an<br />
Aktualität verlor, zusätzlich für viele weitere Forschungsprogramme<br />
in Medizin und Materialwissenschaften eingesetzt<br />
wor<strong>de</strong>n konnte. Sie ist heute noch ein Standbein <strong>de</strong>s PSI.<br />
Dass diese Geschichte nun in allgemein verständlicher<br />
Form vorliegt, ist das Verdienst einiger von Anfang an am<br />
Projekt beteiligter Physiker, welche die Initiative dazu ergriffen,<br />
so<strong>la</strong>nge noch Zeitzeugen befragt wer<strong>de</strong>n konnten.<br />
Wie immer zeigen die offiziellen Dokumente nur einen Ausschnitt<br />
<strong>de</strong>r Wirklichkeit. Will man <strong>de</strong>n Menschen, die ihren<br />
Beitrag zum Gelingen leisteten, nahe kommen, braucht es<br />
persönliche Erinnerungen. Der Text stützt sich auf bei<strong>de</strong>s.<br />
Er hält zu<strong>de</strong>m die Geschehnisse in zahlreichen (schwarzweiss)<br />
Bil<strong>de</strong>rn fest.<br />
Wi<strong>de</strong>rstand gegen das SIN-Projekt<br />
Das Projekt <strong>de</strong>r Mesonenfabrik traf teilweise bei <strong>de</strong>n Physikern<br />
auf Wi<strong>de</strong>rstand. Beson<strong>de</strong>rs die Kernphysiker hätten<br />
lieber eine Maschine gehabt, wie sie von <strong>de</strong>r ursprünglichen<br />
Zyklotron-P<strong>la</strong>nungsgruppe ETH-Uni Zürich-Uni Basel gep<strong>la</strong>nt<br />
gewesen war. Die Projektleiter <strong>de</strong>r Mesonenfabrik gingen<br />
daher einen Kompromiss ein, in<strong>de</strong>m sie als Injektor für<br />
<strong>de</strong>n Ringbeschleuniger das Philips-Zyklotron wählten. Da<br />
dieses nicht geeignet war für <strong>de</strong>n späteren Hochstromausbau,<br />
entwickelte das SIN schon bald <strong>de</strong>n Injektor II nach<br />
<strong>de</strong>mselben Prinzip wie für <strong>de</strong>n Ringbeschleuniger.<br />
Im Hinblick auf <strong>de</strong>n SIN-Baukredit in <strong>de</strong>r ETH-Baubotschaft<br />
1965 wandte sich eine Gruppe von Physikern an Bun<strong>de</strong>srat<br />
Tschudi, um das Projekt zu verhin<strong>de</strong>rn. Tschudi und<br />
ETH-Präsi<strong>de</strong>nt Pallmann liessen sich nicht beirren. Tschudi<br />
meinte B<strong>la</strong>ser gegenüber, dass ein Projekt, das <strong>de</strong>rmassen<br />
auf Opposition stosse, gut sein müsse; er solle weiterfahren<br />
damit.<br />
Der Autor arbeitete in <strong>de</strong>n 1980er Jahren selbst am<br />
SIN, später beim ETH-Rat und schliesslich in <strong>de</strong>r Direktion<br />
<strong>de</strong>s PSI.<br />
Die Opposition f<strong>la</strong>mmte in <strong>de</strong>n Eidgenössischen Räten<br />
nochmals beim teuerungsbedingten Zusatzkredit in <strong>de</strong>r<br />
ETH-Baubotschaft 1972 auf. Sprecher <strong>de</strong>r Opposition war<br />
<strong>de</strong>r Basler Stan<strong>de</strong>sherr Wenk, <strong>de</strong>r sich wohl auf eine Intervention<br />
von Basler Physikern stützte. Das veran<strong>la</strong>sste Bun<strong>de</strong>srat<br />
Tschudi zur Erklärung:<br />
"Die Finanzverwaltung ist in <strong>de</strong>r Lage, dieses Kreditbegehren<br />
zu beurteilen, weil die Direktion <strong>de</strong>r Finanzverwaltung<br />
in <strong>de</strong>r Baukommission für das <strong>Schweizerische</strong> Institut für<br />
Nuklearforschung mitwirkt. Ich muss - Herr Wenk hat das<br />
schon gesagt - unterstreichen: die Finanzverwaltung ist <strong>de</strong>r<br />
Meinung, dass hier ein beson<strong>de</strong>rs mustergültiger Bau erstellt<br />
wird, <strong>de</strong>r in bezug auf P<strong>la</strong>nung <strong>de</strong>s Baus, auf sparsame<br />
Bauausführung an<strong>de</strong>rn als Mo<strong>de</strong>ll dienen kann, dass also in<br />
Bezug auf die Sparsamkeit und die gute Bauorganisation,<br />
die gute P<strong>la</strong>nung <strong>de</strong>s Baues <strong>de</strong>r Baukommission, die unter<br />
Leitung <strong>de</strong>s früheren Direktors <strong>de</strong>r Brown Boveri, Herrn Dr.<br />
Seippel, steht, das beste Zeugnis ausgestellt wer<strong>de</strong>n kann."<br />
Andreas Pritzker hat mit Unterstützung von Kollegen<br />
aus <strong>de</strong>m ehemaligen <strong>Schweizerische</strong>n Institut<br />
für Nuklearforschung (SIN) die Vorgeschichte, Gründung<br />
und Forschungsaktivitäten <strong>de</strong>s SIN nachgezeichnet.<br />
Es wird lebendig, mit zahlreichen Anekdoten<br />
umrahmt beschrieben, wie die erste Schweizer<br />
Grossforschungsan<strong>la</strong>ge, eine "Mesonenfabrik", mit<br />
<strong>de</strong>m von Hans Wil<strong>la</strong>x entworfenen zweistufigen Protonenbeschleuniger<br />
mit Injektor- und Ringzyklotron,<br />
in Zusammenarbeit mit <strong>de</strong>r Industrie realisiert wur<strong>de</strong>.<br />
Eng verbun<strong>de</strong>n mit <strong>de</strong>r Geschichte <strong>de</strong>s SIN ist<br />
das Wirken von Prof. Dr. Jean-Pierre B<strong>la</strong>ser. Er war<br />
Initiant dieser strategischen Forschungsinitiative, die<br />
<strong>de</strong>n Aufbau eines nationalen Forschungs<strong>la</strong>bors für<br />
universitäre Forschungsbedürfnisse auch ausserhalb<br />
<strong>de</strong>r Grund<strong>la</strong>genphysik zum Ziel hatte. Er war Grün<strong>de</strong>r<br />
und Direktor <strong>de</strong>s SIN während <strong>de</strong>n 20 Jahren seines<br />
Bestehens. Und er war auch einer <strong>de</strong>r Hauptinitianten<br />
für die Zusammenführung <strong>de</strong>s SIN mit <strong>de</strong>m Eidgenössischen<br />
Institut für Reaktorforschung (EIR) zum Paul<br />
Scherrer Institut (PSI) im Jahre 1988. Andreas Pritzker<br />
zeigt in <strong>de</strong>r Nachzeichnung <strong>de</strong>r SIN-Geschichte wie<br />
die breiten naturwissenschaftlichen Interessen von<br />
Jean-Pierre B<strong>la</strong>ser über die Physik hinaus zur Realisierung<br />
und För<strong>de</strong>rung von einzigartigen Projekten im<br />
Bereich <strong>de</strong>r Medizin (Krebstherapie und -diagnostik),<br />
<strong>de</strong>r Material- und Festkörperforschung (Spal<strong>la</strong>tionsneutronenquelle,<br />
Supraleitung) und <strong>de</strong>r Energieforschung<br />
(Kernfusion) führten. Das Buch über das SIN<br />
gibt einen guten Einblick in <strong>de</strong>n Forschungsbetrieb einer<br />
Institution, die grosse Forschungsan<strong>la</strong>gen kreiert<br />
und betreibt und diese auch externen Forschen<strong>de</strong>n<br />
zur Verfügung stellt. Das Buch ist sehr lesenswert.<br />
Es ist auch eine Hommage an Jean-Pierre B<strong>la</strong>ser, <strong>de</strong>r<br />
dieses Jahr bei guter Gesundheit seinen 90. Geburtstag<br />
feiern konnte.<br />
Martin Jermann, Paul Scherrer Institut<br />
57
SPG Mitteilungen Nr. 40<br />
Lehrerfortbildung:<br />
18 Deutschschweizer Lehrer im Herz von CERN<br />
Christine P<strong>la</strong>ss (Text und Bil<strong>de</strong>r)<br />
Im Rahmen <strong>de</strong>r Nachwuchsför<strong>de</strong>rung setzt sich die SPG<br />
für die Lehrerfortbildung im Gebiet <strong>de</strong>r Physik ein. Im Frühjahr<br />
wur<strong>de</strong> aus aktuellem An<strong>la</strong>ss, im Zusammenhang mit<br />
<strong>de</strong>r Higgs-Ent<strong>de</strong>ckung am CERN, eine Lehrerfortbildung<br />
mit Schwerpunkt Teilchenphysik zusammen mit teilchenphysik.ch<br />
durchgeführt. Anfang Juni 2013 reisten 18 Lehrerinnen<br />
und Lehrer aus <strong>de</strong>r Deutschschweiz nach Genf. Der<br />
Weiterbildungstag am CERN vermittelte ihnen Anschauungsmaterial<br />
und Experimente, um Hochenergiephysik zu<br />
unterrichten.<br />
"Das ist eine einmalige Gelegenheit, <strong>de</strong>n Detektor zu besichtigen!",<br />
erkannten acht Physiklehrer <strong>de</strong>r Kantonschule<br />
Zug, als ihr Kollege Markus Schmidinger ihnen von seiner<br />
Ein<strong>la</strong>dung ans CERN erzählte. Schmidinger hatte an einer<br />
Fortbildung zu Teilchenphysik in Bern teilgenommen und<br />
war zur Folgeveranstaltung ans CERN nach Genf einge<strong>la</strong><strong>de</strong>n<br />
wor<strong>de</strong>n. Höflich fragte er an, ob seine Kollegen wohl<br />
mitkommen dürften? Initiator Hans Peter Beck, Physiker<br />
am CERN und Dozent <strong>de</strong>r Uni Bern, überlegte nicht <strong>la</strong>nge.<br />
Er konzipierte sein Programm so um, dass es auch ohne<br />
Vorbildung verständlich war. Insgesamt nahmen18 Lehrerinnen<br />
und Lehrer aus <strong>de</strong>r Kantonsschule Ausserschwyz,<br />
<strong>de</strong>m Gymnasium Oberaargau, <strong>de</strong>m Gymnasium Rämibühl<br />
in Zürich und <strong>de</strong>m Gymnasium Biel die Chance wahr, das<br />
CERN von innen kennen zu lernen. Um trotz längerer Anreise<br />
einen vollen Tag am CERN zu erleben, waren sie bereits<br />
am Tag zuvor angereist und konnten kostenlos im CERN-<br />
Hostel übernachten.<br />
Es gehört zum Verständnis <strong>de</strong>s Conseil Européen pour<br />
<strong>la</strong> Recherche Nucléaire (kurz CERN) die Schulbildung zu<br />
unterstützen. "Wir möchten, dass mo<strong>de</strong>rne Physik in die<br />
Schulen Einzug fin<strong>de</strong>t und <strong>de</strong>r Unterricht nicht bei <strong>de</strong>r<br />
schiefen Ebene aufhört", erklärt Hans Peter Beck. Aus aller<br />
Welt kommen Lehrkräfte ans CERN um sich dort tage- und<br />
wochen<strong>la</strong>ng fortzubil<strong>de</strong>n o<strong>de</strong>r gemeinsam mit ihren Schülern<br />
eines <strong>de</strong>r faszinierendsten Forschungszentren <strong>de</strong>r Welt<br />
kennen zu lernen.<br />
Im Herz von CERN, <strong>de</strong>r Protonenquelle. Am Mo<strong>de</strong>ll erklärt Mick<br />
Storr, wie <strong>de</strong>m Wasserstoffgas hier die Protonen entzogen wer<strong>de</strong>n,<br />
die dann im Large Hadron Colli<strong>de</strong>r (LHC) miteinan<strong>de</strong>r kollidieren.<br />
Nach <strong>de</strong>r kurzen Einführung durch Hans Peter Beck geht<br />
es direkt ins Herz von CERN, <strong>de</strong>n LINAC2. Hier wer<strong>de</strong>n die<br />
Protonen bereitgestellt, die sie im Large Hadron Colli<strong>de</strong>r<br />
aufeinan<strong>de</strong>r schiessen. "Welcome to the Startrek Enterprise",<br />
scherzt Mick Storr, als wir <strong>de</strong>n Vorraum zur Protonenquelle<br />
betreten. Er erstrahlt im Design <strong>de</strong>r 70er Jahre, und<br />
das ist kein Retro, son<strong>de</strong>rn Original. Fehlt nur noch, dass<br />
Captain Kirk um die Ecke kommt. Mick Storr weiss, wie<br />
er seinen Besuchern die Scheu vor <strong>de</strong>r High-End-Physik<br />
nehmen kann. Doch was vielleicht noch viel wichtiger ist,<br />
er schätzt sehr, was die Lehrer in <strong>de</strong>n Schulen leisten: "Die<br />
physikalischen Grund<strong>la</strong>gen, die Sie an Ihren Schulen vermitteln,<br />
sind die Grund<strong>la</strong>ge von allem, was hier im CERN<br />
passiert", sagt Mick Storr und lädt seine Zuhörer ein, das,<br />
was sie heute sehen, auch einmal mit ihren Schülern zu besichtigen.<br />
Hans Peter Beck erklärt das CERN und wie Lehrer ihre Schüler mit<br />
einfachen Mo<strong>de</strong>llen und Experimenten an Teilchenphysik heranführen<br />
können.<br />
58<br />
Original-Kontrollraum <strong>de</strong>r Protonenquelle.
Communications <strong>de</strong> <strong>la</strong> SSP No. 40<br />
Mit <strong>de</strong>m Bus geht es zur nächsten Station, <strong>de</strong>m LHCb-<br />
Experiment. "Sie haben ein Riesenglück, dass Sie direkt<br />
in <strong>de</strong>n Detektor reingehen können! Das hab ich selbst<br />
seit zehn Jahren nicht mehr gemacht", begrüsst Andreas<br />
Schopper seine Besucher. Der Physiker am CERN hat<br />
das LHCb Experiment mit aufgebaut und ist Präsi<strong>de</strong>nt <strong>de</strong>r<br />
<strong>Schweizerische</strong>n Physikalischen Gesellschaft (SPG). Sie<br />
hat die Reisekosten für die Lehrer ans CERN übernommen.<br />
Bevor ein Fahrstuhl die Reisegruppe 100 Meter ins<br />
Erdinnere beför<strong>de</strong>rt, erklärt Schopper an einem Mo<strong>de</strong>ll,<br />
was das Beson<strong>de</strong>re am LHCb ist. 700 Wissenschaftler aus<br />
61 Institutionen und 16 Län<strong>de</strong>rn forschen dort nach <strong>de</strong>n<br />
Unterschie<strong>de</strong>n zwischen Materie und Antimaterie. Aus <strong>de</strong>r<br />
Schweiz sind die ETH Lausanne und die Universität Zürich<br />
am Experiment beteiligt. So untersuchten die Forscher<br />
erstmals <strong>de</strong>n Zerfall eines weiteren Teilchens, <strong>de</strong>ssen Messung<br />
abermals beweist, dass Materie und Antimaterie nicht<br />
exakt symmetrisch sind.<br />
Nach einer zügigen Fahrt in 100 Meter Tiefe wartet die<br />
nächste Schleuse. Radioaktivität, vor <strong>de</strong>r auf <strong>de</strong>r Tür gewarnt<br />
wird, herrscht zur Zeit <strong>de</strong>s Shutdowns hier unten<br />
zwar nicht. Trotz<strong>de</strong>m hat Schopper ein Dosimeter dabei,<br />
da es sich um eine kontrollierte Zone han<strong>de</strong>lt, für die bestimmte<br />
Sicherheitsvorkehrungen gelten. Langweilig wird<br />
es <strong>de</strong>n Physikern während <strong>de</strong>s Shutdowns übrigens trotz<strong>de</strong>m<br />
nicht, <strong>de</strong>nn es gibt noch riesige Datenmengen, die auf<br />
ihre Auswertung warten, wie Markus Joos erklärt. Der Informatiker<br />
arbeitet an <strong>de</strong>r Software, die die Messergebnisse<br />
aufzeichnet, filtert und speichert. 100 Petabyte Rohdaten<br />
sind auf 40.000 Festp<strong>la</strong>tten und 40.000 Bandkassetten gespeichert.<br />
Bandkassetten? Tatsächlich setzten die Informatiker<br />
am CERN auf diese vermeintlich veralteten Speichermedien,<br />
da sie die Daten 100 Mal sicherer aufbewahren als<br />
eine Festp<strong>la</strong>tte.<br />
durch <strong>de</strong>n LHC hindurch. Gäbe es keine Supraleitungen<br />
müsste <strong>de</strong>r LHC <strong>de</strong>n Umfang <strong>de</strong>s Äquators haben.<br />
Unsere vorletzte Station ist <strong>de</strong>r Kontrollraum <strong>de</strong>s Alpha<br />
Magnetic Spectrometer (AMS2). Der schüttelsichere Detektor<br />
wur<strong>de</strong> 16 Jahre <strong>la</strong>ng gebaut und getestet, mit <strong>de</strong>m<br />
letzten Spaceshuttle zur Internationalen Raumstation (ISS)<br />
geschossen und von NASA Astronauten auf <strong>de</strong>r ISS installiert.<br />
Dort jagt er nach Antimaterie. Wenigstens ein einziges<br />
Anti-Helium. Noch besser zwei. Zehn, um ein Paper zu<br />
veröffentlichen. Die Wissenschaftler gehen nämlich davon<br />
aus, dass beim Urknall riesige Mengen von Materie und<br />
Anti-Materie freigesetzt wur<strong>de</strong>n, um sich sogleich wie<strong>de</strong>r<br />
gegenseitig zu zerstören. Nach dieser Theorie dürfte es<br />
keine stabile Antimaterie in unserem Universum geben –<br />
es sei <strong>de</strong>nn, AMS2 lieferte <strong>de</strong>n Gegenbeweis. Bis<strong>la</strong>ng hat<br />
AMS2 noch keine Antimaterie dingfest gemacht. Dafür fan<strong>de</strong>n<br />
Wissenschaftler signifikante Hinweise auf unbekannte<br />
Quellen kosmischer Strahlung, die beantworten könnten,<br />
was es mit <strong>de</strong>r dunklen Materie auf sich hat.<br />
Doch man braucht gar nicht ins All o<strong>de</strong>r ans CERN reisen,<br />
um Teilchen zu sehen. Wie sie ihren Schülern Elektronen<br />
und Alphateilchen in einem Experiment zeigen können, erfahren<br />
die Lehrer am Nachmittag beim Bau einer Nebelkammer.<br />
Rasch ist k<strong>la</strong>r, hier sind Profis am Werk. In Win<strong>de</strong>seile<br />
haben sie die Nebelkammern fachgerecht aufgebaut und<br />
die Gardinen zugezogen. Dann <strong>la</strong>uern sie auf Teilchen, die<br />
sich im Licht <strong>de</strong>r Taschen<strong>la</strong>mpe zeigen. "Joh, jetzt seh' ich<br />
eins", ruft einer. "Was für ein dicker Brummer!", stellt ein<br />
an<strong>de</strong>rer fest. Kleine wurmförmige Partikel bewegen sich<br />
horizontal und vertikal durch <strong>de</strong>n Lichtstrahl. Das einfache<br />
wie eindrückliche Experiment lässt sich sogar mit P<strong>la</strong>stikbecher<br />
und Alu-Aschenbecher durchführen. Trockeneis ist<br />
allerdings unentbehrlich.<br />
Die Lehrer sind von ihrem abwechslungsreichen Tag am<br />
CERN sichtlich begeistert. Als "sehr eindrücklich", beurteilt<br />
Markus Schmidinger <strong>de</strong>n Tag am CERN: "Es ist etwas an<strong>de</strong>res,<br />
wenn man das Experiment vor Ort sieht und Zutritt<br />
zu einer Welt erhält, die einem sonst verborgen bleibt". Er<br />
nimmt viele Anregungen mit nach Hause, die er gleich umsetzen<br />
will: "Zum Beispiel bei <strong>de</strong>r Lorentzkraft im Unterricht<br />
zeigen, dass es keine blosse Theorie ist, son<strong>de</strong>rn Ingenieure<br />
am CERN damit arbeiten."<br />
Gerfried Wiener von <strong>de</strong>r Uni Wien erklärt, warum Supraleitungen<br />
im LHC zum Einsatz kamen. Alle dürfen mal testen, wie schwer<br />
konventionelle Kupferkabel sind, die in <strong>de</strong>r Lage wären, 13000<br />
Ampère zu leiten, ohne zu schmelzen.<br />
Danach geht es weiter zur Magnettesthalle. Anhand einiger<br />
Mo<strong>de</strong>lle erklärt Gerfried Wiener von <strong>de</strong>r Universität Wien,<br />
wie <strong>de</strong>r LHC gebaut wur<strong>de</strong> und welche Hür<strong>de</strong>n dabei zu<br />
bewältigen waren. Allein die Kabel! 13000 Ampère <strong>la</strong>ufen<br />
Das von PD Dr. Hans Peter Beck (Universität Bern/<br />
CERN) initiierte 1. Deutschschweizer Lehrerprogramm<br />
am CERN wur<strong>de</strong>, in Zusammenarbeit mit www.teilchenphysik.ch,<br />
durch die fachliche und finanzielle<br />
Unterstützung von CERN und <strong>de</strong>r <strong>Schweizerische</strong>n<br />
Physikalischen Gesellschaft (SPG) ermöglicht. In regelmässigen<br />
Abstän<strong>de</strong>n wer<strong>de</strong>n weitere Programme<br />
für Schweizer Lehrer/innen folgen. Anmeldungen zu<br />
einer weiteren Fortbildung am 8./9. November zu diesem<br />
Thema, inklusive CERN Besuch, wer<strong>de</strong>n schon<br />
jetzt unter indico.cern.ch/event/swissteachers entgegengenommen.<br />
59
Annual Congress 2013 of the Swiss Aca<strong>de</strong>my of Sciences (SCNAT)<br />
The Quantum Atom at 100 –<br />
Niels Bohr’s Legacy<br />
Fotos: shutterstock.com | PSI<br />
November 21-22, 2013 | Winterthur<br />
The congress will celebrate the 100 th anniversary of Niels Bohr’s publication<br />
„On the Constitution of Atoms and Molecules“ and offer an overview on subsequent<br />
<strong>de</strong>velopments, leading to the mo<strong>de</strong>rn version of quantum mechanics and its implications<br />
and to the current un<strong>de</strong>rstanding of the constitution of matter.<br />
The Zurich University of Applied Science in Winterthur will host this year’s congress.<br />
• Aspects of Bohr’s 1913 Atomic Theory: Helge Kragh, University of Aarhus, Denmark<br />
• From Bohr’s Atom to Quantum Mechanics: Olivier Darrigol, CRNS, Paris<br />
• Ultrahigh-Resolution Spectroscopy of the Hydrogen Atom: Thomas U<strong>de</strong>m, MPI Quantum Optics, Garching<br />
• Muonic Hydrogen: Atomic Physics for Nuclear Structure: Randolf Pohl, MPI Quantum Optics, Garching<br />
• Antihydrogen: Past, Present, Future: Michael Doser, CERN, Geneva<br />
• Hydrogen, the Most Abundant Element in the Universe: Ruth Durrer, University of Geneva<br />
• Defining and Measuring Time: From Cesium to Atomic Clocks: Jacques Vanier, University of Montreal,<br />
Canada<br />
• Rydberg States of Atoms and Molecules: Frédéric Merkt, ETH Zurich<br />
• Manipu<strong>la</strong>ting trapped Photons and raising Schrödinger Cats of Light: Serge Haroche, Nobel Laureate<br />
2012, ENS and Collège <strong>de</strong> France, Paris<br />
• At the End of the Periodic Table: Yuri Oganessian, JINR, FLNR, Dubna, Russia<br />
• Insights and Puzzles in Particle Physics: Heinrich Leutwyler, University of Bern<br />
• Quantum Mechanics and Photosynthesis: Rienk van Gron<strong>de</strong>lle, VU Amsterdam, The Nether<strong>la</strong>nds<br />
Public Evening Lecture: Reinhard Werner, Leibniz Universität Hannover:<br />
Die Bohr-Einstein-Debatte zur Quantenmechanik<br />
There is no conference fee for registered participants. Registration Deadline: November 1 st , 2013<br />
More information and registration: http://congress13.scnat.ch