Twelve Years at DESY
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Wie Es Zur Gründung Des Instituts Für Hochenergiephysik Kam
HEPHY-PUB-997 24 Nov. 2016 (rev. 19 Sep. 2017) Wie es zur Gründung des Instituts für Hochenergiephysik kam Winfried A. Mitaroff Institut für Hochenergiephysik der ÖAW, Wien ∗ Zusammenfassung Nach dem Beitritt Österreichs zur Europäischen Organisation für Kernforschung (CERN) im Jahr 1959 und bescheidenen Anfängen an der Universität Wien wurde 1966 mit der Gründung des Instituts für Hochenergiephysik (HEPHY) durch die Österreichische Akademie der Wissenschaften (ÖAW) der Grundlagenforschung auf dem Gebiet der experimentellen Teilchenphysik in unserem Land eine solide Entwicklungsmöglichkeit eröffnet. In den seither vergangenen 50 Jahren war das Institut im Rahmen internationaler Kollaborationen an einer Vielzahl von Experimenten an Großforschungsanlagen (vorwiegend, aber nicht ausschließlich, bei CERN) beteiligt – darunter auch an so bedeutenden, welche später zu Physik-Nobelpreisen geführt haben. Hierzu hat es wichtige Beiträge geleistet, insbesondere in den Bereichen Detektorentwicklung, Datenanalyse und Phänomenologie. Die vorliegende Studie zielt auf die Vorgeschichte, welche schließlich zur Institutsgründung führte. Als Quellen dienten Sitzungsprotokolle und Tätigkeitsberichte, Institutsbroschüren, Autobiografien, sowie persönliche Erinnerungen. Dieser Artikel stellt den ersten Teil eines Beitrags zur Monografie “175 Jahre Österreichische Akademie der Wissenschaften” (Wien 2022) dar, welcher die wissenschaftliche Institutsgeschichte bis zur Gegenwart beschreiben wird. 1 Einleitung Die Hochenergiephysik als selbständige Wissenschaftsdisziplin -
Willibald Jentschke –
European organization for nuclear research Willibald Jentschke – Willibald Jentschke founder of DESY and former Director"General of CERN passed away on March + on 18 December 1959. Jentschke became its first director and remained in this position until 1970. Jentschke served as Director-General of CERN Laboratory I – the original Meyrin site – from 1971–75. During the same period, John Adams was Director-General of the neighbouring Laboratory II, where the new SPS pro- ton synchrotron was being construct- ed. Having two Directors-General was an unusual and delicate situation, but to their eternal credit Jentschke and Adams handled it well. Jentschke oversaw the exploitation of important new investments, including an ambi- tious research programme for neutri- no physics. In 1973, this effort enabled physicists to discover the neutral cur- rents of the weak interaction. Faced with a major discovery, CERN was nervous. However, Jentschke ensured that the result went on record as one Born in Vienna, Willibald Jentschke of the Laboratory’s great achieve- obtained his Ph.D. in nuclear physics ments. at the age of 24. He continued working in this field in Vienna for many years. As Director-General of CERN In 1951, he became director of the Jentschke wrote in 1975: "I believe cyclotron laboratory at the University that we must base our future plans on of Illinois. When the University of international collaboration, certainly Hamburg offered him the chair for within Europe, or perhaps, if condi- experimental physics in 1955 he tions eventually permit, within a wider requested funds to create a modern context." This vision is now becoming research facility in Germany. -
After Dinner Speech by Dr
1 After Dinner Speech by Dr. Josef Rembser CERN, Geneva 14 September 2009 Celebration in honour of Professor Herwig Schopper’s 85 th Birthday I. Dear Friends, honourable, dear Professor Schopper! On 28 February of this year, you celebrated your 85th Birthday. This evening we are looking back on this memorable date, wishing you many happy returns of the day. You have been blessed with a life full of harmony and accomplishments, always keeping young physically and intellectually. This is a special blessing granted to a person: Love and family, friendships and encounters, giving and receiving, working and achieving acknowledgements and honours in a fulfilling profession and in challenging missions. Tomorrow, a scientific Colloquium will honour you as researcher and scientific teacher . Today, on the eve of the colloquium, I would like to speak about Herwig Schopper as a research politician and a research manager . My personal remarks and remembrances will focus, dear Herwig Schopper, on the guiding contributions you made in shaping, promoting and advancing science and research and their relevant policies in Germany and in Europe. 2 Professor Heuer, I am grateful for your invitation. It is a pleasure for me to give today's After-Dinner speech in honour of our jubilee. For many years during my service in the German Ministry of Research and Technology (BMFT) in Bonn I had close personal and professional connections with you, dear Professor Schopper, regarding German science and research policy including CERN. II. In 1945, with the end of the 2 nd World War, Germany as guilty party and loser plunged the world and its own country into destruction and suffering, thus experiencing a historical catastrophe. -
Sterns Lebensdaten Und Chronologie Seines Wirkens
Sterns Lebensdaten und Chronologie seines Wirkens Diese Chronologie von Otto Sterns Wirken basiert auf folgenden Quellen: 1. Otto Sterns selbst verfassten Lebensläufen, 2. Sterns Briefen und Sterns Publikationen, 3. Sterns Reisepässen 4. Sterns Züricher Interview 1961 5. Dokumenten der Hochschularchive (17.2.1888 bis 17.8.1969) 1888 Geb. 17.2.1888 als Otto Stern in Sohrau/Oberschlesien In allen Lebensläufen und Dokumenten findet man immer nur den VornamenOt- to. Im polizeilichen Führungszeugnis ausgestellt am 12.7.1912 vom königlichen Polizeipräsidium Abt. IV in Breslau wird bei Stern ebenfalls nur der Vorname Otto erwähnt. Nur im Emeritierungsdokument des Carnegie Institutes of Tech- nology wird ein zweiter Vorname Otto M. Stern erwähnt. Vater: Mühlenbesitzer Oskar Stern (*1850–1919) und Mutter Eugenie Stern geb. Rosenthal (*1863–1907) Nach Angabe von Diana Templeton-Killan, der Enkeltochter von Berta Kamm und somit Großnichte von Otto Stern (E-Mail vom 3.12.2015 an Horst Schmidt- Böcking) war Ottos Großvater Abraham Stern. Abraham hatte 5 Kinder mit seiner ersten Frau Nanni Freund. Nanni starb kurz nach der Geburt des fünften Kindes. Bald danach heiratete Abraham Berta Ben- der, mit der er 6 weitere Kinder hatte. Ottos Vater Oskar war das dritte Kind von Berta. Abraham und Nannis erstes Kind war Heinrich Stern (1833–1908). Heinrich hatte 4 Kinder. Das erste Kind war Richard Stern (1865–1911), der Toni Asch © Springer-Verlag GmbH Deutschland 2018 325 H. Schmidt-Böcking, A. Templeton, W. Trageser (Hrsg.), Otto Sterns gesammelte Briefe – Band 1, https://doi.org/10.1007/978-3-662-55735-8 326 Sterns Lebensdaten und Chronologie seines Wirkens heiratete. -
Asia Pacific Physics Newsletter
Asia Pacific Physics Newsletter March 2016 Volume 5 • Number 1 worldscinet.com/appn Takaaki Kajita 2015 Physics Nobel Laureate published by Institute of Advanced Studies, Nanyang Technological University (IAS@NTU) and South East Asia Theoretical Physics Association (SEATPA) South East Asia Theoretical Physics Association Asia Pacific Physics Newsletter March 2016 • Volume 5 • Number 1 A publication of the IAS@NTU Singapore and SEATPA Asia Pacific Physics Newsletter publishes articles reporting frontier discoveries in EDITORIAL physics, research highlights, and news to facilitate interaction, collaboration and 3 cooperation among physicists in Asia Pacific physics community. PEOPLE Editor-in-Chief 4 “Observing the Distant Supernova” — Interview with Kok Khoo Phua Nobel Laureate Prof Brian Schmidt Associate Editor-in-Chief “Discovering the W and Z Bosons” — Interview with Swee Cheng Lim Nobel Laureate Prof Carlo Rubbia SEATPA Committee Christopher C Bernido Phil Chan Leong Chuan Kwek Choy Heng Lai Swee Cheng Lim Ren Bao Liu Hwee Boon Low Anh Ký Nguyên Choo Hiap Oh OPINION AND COMMENTARY Kok Khoo Phua 10 China’s Great Scientific Leap Forward: Completion of a Roh Suan Tung Preecha Yupapin planned ‘Great Collider’ would transform particle physics Hishamuddin Zainuddin Freddy Zen Editorial Team NEWS Sen Mu 12 CityU’s Institute for Advanced Study will Champion Bold New Han Sun Chi Xiong Research Initiatives Case made for 'Ninth Planet' Graphic Designers Chuan Ming Loo Erin Ong Cover Photo: "Takaaki Kajita 5171- 2015" by Bengt Nyman - Own work. -
Veröffentlichungen Und Vorträge
Veröffentlichungen und Vorträge Veröffentlichungen und Vorträge 287 288 DESY-Kolloquien Festkolloquium für Günter Wolf M. DERRICK (ANL Argonne/USA) The Physics Interplay between Hadron and Electron Facilities. 10 Jahre DESY Zeuthen R. PECCEI (UCLA/USA) Festkolloquium The Deep Inelastic Trail. 3.12.2002 A. WAGNER (DESY Hamburg/D) Begrüßung. DESY Lecture Series in Memory of Prof. Dr. W. Jentschke J. WANKA (Ministerium für Wissenschaft, Forschung und Kultur des Landes Brandenburg) W.K.H. PANOFSKY (Univ. Stanford/USA) Grußwort. The Danger Posed by Nuclear Weapons. 5.12.2002 H. SCHUNCK (BMBF, Berlin/D) Transformation oder Urknall – Physik in Deutschland 10 Jahre danach. V. SOERGEL (Univ. Heidelberg/D) Academic Training 1992 – DESY wird größer: Erinnerung an die Entstehung von DESY Zeuthen. U. GENSCH (DESY Zeuthen/D) P. SCHMÜSER (Univ. Hamburg/D) DESY Zeuthen heute. Basic Elements of Accelerator Physics. 18.–20.02.2002 C. SPIERING (DESY Zeuthen/D) Neutrinoastrophysik – Vom Baikalsee zum Südpol. G. WEIGLEIN (Univ. of Durham/GB) Electroweak Physics: Preparing for TESLA. D. ECKSTEIN (CERN Geneva/CH) 13.–15.05.2002 Struktur des Protons und die starke Kraft. V. MÜLLER (Astrophys. Inst. Potsdam/D) D. PLEITER (DESY Zeuthen/D) Astrophysics and Cosmology. Parallelrechner und Physik auf dem Gitter. 7./8.10.2002 J. ILLANA (Univ. Hamburg/D) Hunting for Precision at High Energies. S. RIEMANN (DESY Zeuthen/D) Vorträge – Physik bei TESLA – Ursprung der Masse. Innerbetriebliche Fortbildung Einführung in die Ausstellung: TESLA – Licht der Zukunft A. WAGNER (DESY Hamburg/D) S. SACK (Hamburg/D) Unternehmensberater – Was tun die eigentlich wirklich? 30.01.2002 16.1.2002 H.-F. GRAF (Hamburg/D) A. -
Polite Debate
4 Nature Vol. 286 3 July 1980 High-energy physics Schopper, would be able to organize and prototype vitrification plant operating at draw on talent throughout CERN, for Windscale by 1990 if the go-ahead for the short and long periods, avoiding the career plant can be given some time this year. LEP leaps ahead problems and inflexibility that would come The decision for British Nuclear Fuels, THE European Centre for Nuclear with a new "LEP division". "We will which runs Windscale, will not be easy, Research (CERN) last week made a firm bring the work to the people", he said. however; it will have to choose between its proposal lo its 12 member states for a new The CERN Council has adopted a own HARVEST process and the French accelerator to be built in the 1980s. The "firm" budget for 1981 of 596 million equivalent (A VM) which has been machine, called LEP, is a 30 km circum Swiss francs (£156 million), but this operating commercially since 1978. ference ring for accelerating, storing and includes no provision for the construction Officials are keen to point out that a colliding very high energy beams of of LEP. Schopper will propose a running decision to opt for A VM would not mean electrons. The proposal already bears the budget which will include LEP in six the end of HAR VEST, which should be mark of CERN's firebrand director months' time: he expects it to be a little kept going to keep later options open. general-designate, German Professor larger than the 198 I budget "but we are The government plans to start producing Herwig Schopper: LEP is now cheaper only talking of a per cent or two". -
Der Mythos Der Deutschen Atombombe
Langsame oder schnelle Neutronen? Der Mythos der deutschen Atombombe Prof. Dr. Manfred Popp Karlsruher Institut für Technologie Ringvorlesung zum Gedächtnis an Lise Meitner Freie Universität Berlin 29. Oktober 2018 In diesem Beitrag geht es zwar um Arbeiten zur Kernphysik in Deutschland während des 2.Weltkrieges, an denen Lise Meitner wegen ihrer Emigration 1938 nicht teilnahm. Es geht aber um das Thema Kernspaltung, zu dessen Verständnis sie wesentliches beigetragen hat, um die Arbeit vieler, gut vertrauter, ehemaliger Kollegen und letztlich um das Schicksal der deutschen Physik unter den Nationalsozialisten, die ihre geistige Heimat gewesen war. Da sie nach dem Abwurf der Bombe auf Hiroshima auch als „Mutter der Atombombe“ diffamiert wurde, ist es ihr gewiss nicht gleichgültig gewesen, wie ihr langjähriger Partner und Freund Otto Hahn und seine Kollegen während des Krieges mit dem Problem der möglichen Atombombe umgegangen sind. 1. Stand der Geschichtsschreibung Die Geschichtsschreibung über das deutsche Uranprojekt 1939-1945 ist eine Domäne amerikanischer und britischer Historiker. Für die deutschen Geschichtsforscher hatte eines der wenigen im Ergebnis harmlosen Kapitel der Geschichte des 3. Reiches keine Priorität. Unter den alliierten Historikern hat sich Mark Walker seit seiner Dissertation1 durchgesetzt. Sein Beitrag zur Geschichte der Kaiser Wilhelm-Gesellschaft im 3. Reich beginnt mit den Worten: „The Kaiser Wilhelm Institute for Physics is best known as the place where Werner Heisenberg worked on nuclear weapons for Hitler.“2 Im Jahr 2016 habe ich zum ersten Mal belegt, dass diese Schlussfolgerung auf Fehlinterpretationen der Dokumente und auf dem Ignorieren physikalischer Fakten beruht.3 Seit Walker gilt: Nicht an fehlenden Kenntnissen sei die deutsche Atombombe gescheitert, sondern nur an den ökonomischen Engpässen der deutschen Kriegswirtschaft: „An eine Bombenentwicklung wäre [...] auch bei voller Unterstützung des Regimes nicht zu denken gewesen. -
The Charm of Theoretical Physics (1958– 1993)?
Eur. Phys. J. H 42, 611{661 (2017) DOI: 10.1140/epjh/e2017-80040-9 THE EUROPEAN PHYSICAL JOURNAL H Oral history interview The Charm of Theoretical Physics (1958{ 1993)? Luciano Maiani1 and Luisa Bonolis2,a 1 Dipartimento di Fisica and INFN, Piazzale A. Moro 5, 00185 Rome, Italy 2 Max Planck Institute for the History of Science, Boltzmannstraße 22, 14195 Berlin, Germany Received 10 July 2017 / Received in final form 7 August 2017 Published online 4 December 2017 c The Author(s) 2017. This article is published with open access at Springerlink.com Abstract. Personal recollections on theoretical particle physics in the years when the Standard Theory was formed. In the background, the remarkable development of Italian theoretical physics in the second part of the last century, with great personalities like Bruno Touschek, Raoul Gatto, Nicola Cabibbo and their schools. 1 Apprenticeship L. B. How did your interest in physics arise? You enrolled in the late 1950s, when the period of post-war reconstruction of physics in Europe was coming to an end, and Italy was entering into a phase of great expansion. Those were very exciting years. It was the beginning of the space era. L. M. The beginning of the space era certainly had a strong influence on many people, absolutely. The landing on the moon in 1969 was for sure unforgettable, but at that time I was already working in Physics and about to get married. My interest in physics started well before. The real beginning was around 1955. Most important for me was astronomy. It is not surprising that astronomy marked for many people the beginning of their interest in science. -
People and Things
People and things such a Subtle effect as the disap provide a good surface-to-volume LEP authorization ratio, and then selectively to observe pearance of bag boundaries. Correla the surface. Weakly interacting tion measurements may be required, The project to build a large elec probes are called for. Most of our such as searches for changes in the tron-positron storage ring, LEP, at considerations must then deal with small mass lepton pair spectra, or in CERN already had the backing of photons, or virtual photons ob the identical particle interference the twelve CERN Member States served as lepton pairs. measurements. (see December 1981 issue, page The emitted photons and leptons, Since we have only rough esti 439), but threç votes remained for example, could be used in an mates of the transition temperature, subject to conditions. At a CERN attempt to observe the phase transi only rather crude notions of 'temper Council meeting in December this tion. The energy of the nuclei is var ature' in collisions, and as yet no 'ad referendum' was lifted by the ied, and the temperature indicated by direct data relevant to the tempera Netherlands, Norway and Sweden. the transverse momentum and mass ture inside nuclear collisions, we can The LEP project thus has the un distribution is determined. The rate not say anything precise about the conditional support of all Member of photon emission is then deter energies necessary to produce tem States. mined as a function of temperature. peratures above the critical tempera Meanwhile the LEP project team As the transition temperature is ture. -
Stanford Linear Accelerator Center
STANFORD LINEAR ACCELERATOR CENTER Winter 1997, Vol. 27, No.4 A PERIODICAL OF PARTICLE PHYSICS Fermilab Media Services Visual WINTER 1997 VOL. 27, NUMBER 4 FOREWORD 2 Burton Richter Editors RENE DONALDSON, BILL KIRK Contributing Editors FEATURES MICHAEL RIORDAN, GORDON FRASER JUDY JACKSON, PEDRO WALOSCHEK 4 INTERNATIONAL COOPERATION: Editorial Advisory Board THE SINE QUA NON FOR THE FUTURE GEORGE BROWN, LANCE DIXON OF HIGH ENERGY PHYSICS JOEL PRIMACK, NATALIE ROE The DOE’s new Associate Director of High ROBERT SIEMANN, GEORGE TRILLING Energy and Nuclear Physics discusses the KARL VAN BIBBER promise and problems of international Illustrations scientific collaboration. TERRY ANDERSON S. Peter Rosen Distribution 12 RETROSPECTIVES ON INTERNATIONAL CRYSTAL TILGHMAN COLLABORATION Four different perspectives on international collaboration in high energy physics are presented. Gordon Fraser The Beam Line is published quarterly by Hirotaka Sugawara the Stanford Linear Accelerator Center, PO Box 4349, Stanford, CA 94309. Alexander N. Skrinsky Telephone: (650) 926-2585 INTERNET: [email protected] Zhou Guang-Zhao FAX: (650) 926-4500 Issues of the Beam Line are accessible electronically on the World Wide Web at http://www.slac.stanford.edu/ 20 U.S. COLLABORATION pubs/beamline. SLAC is operated by Stanford University ON THE LHC PROJECT under contract with the U.S. Department of Energy. The opinions of the authors do not necessarily reflect the A member of the U.S. collaboration, who has policy of the Stanford Linear Accelerator Center. been involved since its beginnings, discusses the history of the Large Hadron Collider and its importance to U.S. particle physics. George Trilling 27 THE ATLAS INNER DETECTOR The U.S. -
A Contribuição De Chien Shiung Wu Para a Teoria Quântica
UNIVERSIDADE FEDERAL DA BAHIA UNIVERSIDADE ESTADUAL DE FEIRA DE SANTANA PROGRAMA DE PÓS-GRADUAÇÃO EM ENSINO, FILOSOFIA E HISTÓRIA DAS CIÊNCIAS ANGEVALDO MENEZES MAIA FILHO PARA UMA HISTÓRIA DAS MULHERES NA CIÊNCIA: A CONTRIBUIÇÃO DE CHIEN SHIUNG WU PARA A TEORIA QUÂNTICA Salvador 2018 ANGEVALDO MENEZES MAIA FILHO PARA UMA HISTÓRIA DAS MULHERES NA CIÊNCIA: A CONTRIBUIÇÃO DE CHIEN SHIUNG WU PARA A TEORIA QUÂNTICA Dissertação apresentada ao Programa de Pós- Graduação em Ensino, Filosofia e História das Ciências, da Universidade Federal da Bahia e da Universidade Estadual de Feira de Santana como requisito parcial para a obtenção do título de Mestre em Ensino, Filosofia e História das Ciências. Orientadora: Profa. Dra. Indianara Lima Silva Salvador 2018 ANGEVALDO MENEZES MAIA FILHO PARA UMA HISTÓRIA DAS MULHERES NA CIÊNCIA: A CONTRIBUIÇÃO DE CHIEN SHIUNG WU PARA A TEORIA QUÂNTICA Dissertação apresentada como requisito parcial para obtenção do grau de mestre em 19 de abril de 2018, Programa de Pós-Graduação em Ensino, Filosofia e História das Ciências, da Universidade Federal da Bahia e da Universidade Estadual de Feira de Santana. 19 de abril de 2018 Banca Examinadora _______________________________________________ Professora Doutora Indianara Lima Silva _______________________________________________ Professora Doutora Maria Margaret Lopes _______________________________________________ Professor Doutor Olival Freire Júnior AGRADECIMENTOS Como não poderia deixar de ser, os agradecimentos revelam o quão importante são as pessoas que nos cercam e o quanto pode ser difícil, no meu caso, absolutamente impossível, realizar um trabalho individualmente. Agradeço a Josenice Assunção Maia e Angevaldo Maia, pessoas que tive a sorte de ter enquanto genitores me apoiando incondicionalmente desde sempre, confiando e acreditando nas minhas escolhas, a maior e inesgotável fonte de amor que pude encontrar na vida.