CERN – from Birth to Success
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Spring 1998, Vol
S T A N F O R D L I N E A R A CCELERATOR CENTER Spring 1998, Vol. 28, No.1 A PERIODICAL OF PARTICLE PHYSICS SPRING 1998 VOL. 28, N UMBER 1 Editors RENE DONALDSON, BILL KIRK Contributing Editors MICHAEL RIORDAN, GORDON FRASER JUDY JACKSON, PEDRO WALOSCHEK Editorial Advisory Board GEORGE BROWN, LANCE DIXON JOEL PRIMACK, NATALIE ROE ROBERT SIEMANN, GEORGE TRILLING KARL VAN BIBBER Illustrations TERRY A NDERSON Distribution Lake CRYSTAL TILGHMAN Soudan Superior Duluth The Beam Line is published quarterly by the MN Lake Stanford Linear Accelerator Center WI Michigan PO Box 4349, Stanford, CA 94309. Telephone: (650) 926-2585 Madison INTERNET: [email protected] MI FAX: (650) 926-4500 IA Issues of the Beam Line are accessible electronically on the World Wide Web at http://www.slac.stanford.edu/ Fermilab pubs/beamline IL IN SLAC is operated by Stanford University under contract with the U.S. Department of Energy. The opinions of the authors do not necessarily reflect the policy of the MO Stanford Linear Accelerator Center. Cover:The cover photo was taken in 1917, plus or minus about one year. The photographer is unknown or unre- membered. The young lad shown in the photo with his telescope in the garden of his home in Pretoria, South Africa, is Alan Cousins, at the age of about fourteen (he was born in 1903). Dr. Cousins’ first contribution to the astronomical literature was published in 1924. Seventy-four years have passed since then, but Alan William James Cousins is still at work at his home base, the South African Astronomical Observatory (SAAO), having recently published his latest paper (“Atmospheric Extinc- tion,” The Observatory, April 1998). -
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. -
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. -
I~ Ml 11111111 CM-P00043005
CHS-16 May 1985 CERN LIBRARIES, GENEY A -'°I Cf.l ::i:: u 11111111111111111~111~11111111111'1 ~II I~ I~ ml 11111111 CM-P00043005 STUDIES IN CERN HISTORY From the provisional organization to the permanent CERN May 1952 - September 1954 II. Case studies of some important decisions. John Krige *> GENEVA 1985 The Study of CERN History is a project financed by Institutions in several CERN Member Countries. This report presents preliminary findings, and is intended for incorporation into a more comprehensive study of CERN's history. It is distributed primarily to historians and scientists to provoke discussion, and no part of it should be cited or reproduced without written permission from the Team Leader. Comments are welcome and should be sent to: Study Team for CERN History c/oCERN CH-1211GENEVE23 Switzerland © Copyright Study Team for CERN History, Geneva 1985 CHS-16 May 1985 STUDIES IN CERN HISTORY From the provisional organization to the permanent CERN May 1952 - September 1954 II. Case studies of some important decisions. John Krige*) GENEVA 1985 *) Supported by a grant from the JOINT ESRC/SERC COMMITTEE, United Kingdom. The Study of CERN History is a project financed by Institutions in several CERN Member Countries. This report presents preliminary findings, and is intended for incorporation into a more comprehensive study of CERN's history. It is distributed primarily to historians and scientists to provoke discussion, and no part of it should be cited or reproduced without written permission from the Team Leader. Comments are welcome and should be sent to: Study Team for CERN History c/oCERN CH-1211 GENEVE 23 Switzerland © Copyright Study Team for CERN History, Geneva 1985 CERN - Service d'information scientifique - 300 - juillet 1985 From the provisional organization to the permanent CERN May 1952 - September 1954 II. -
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. -
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. -
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. -
Student Handbook and Programme Syllabus
John Adams Institute for Accelerator Science Education & Training in Accelerator Science Student Handbook and Programme Syllabus 2020-2021 1 The John Adams Institute for Accelerator Science (JAI) The John Adams Institute for Accelerator Science (JAI) is a centre of excellence in the UK for advanced and novel accelerator technology, providing expertise, research, development and training in accelerator techniques, and promoting advanced accelerator applications in science and society. The JAI programme is organised around three pillars: research in accelerator science; training the next generation of accelerator scientists; and science outreach to industry and the public. The JAI is jointly hosted by the physics departments of the University of Oxford, Royal Holloway, University of London and Imperial College London. What the JAI Does The next generation of particle physicists needs the next generation of particle accelerators. The JAI is a UK and world-leading research group dedicated to the research and development of particle accelerators. We are working on the next generation colliders – the Future Circular Collider (FCC), including the Higher-Energy LHC (HE-LHC), and the linear colliders of the Compact Linear Collider (CLIC) and International Linear Collider (ILC) collaborations. These machines may become the next particle accelerators designed to complement the discoveries made at the Large Hadron Collider (LHC) and its high-luminosity upgrade (HL-LHC) at CERN. Modern light sources, synchrotron-based and free electron lasers, are indispensable for scientific and technological development of the modern economy and society. We are working on improving light sources such as Diamond, and working on further ideas. A very challenging, but very promising direction is the creation of compact light sources and accelerators for particle physics based on laser plasma acceleration. -
Uva-DARE (Digital Academic Repository)
UvA-DARE (Digital Academic Repository) Goede humor, slechte smaak: een sociologie van de mop Kuipers, G.M.M. Publication date 2001 Link to publication Citation for published version (APA): Kuipers, G. M. M. (2001). Goede humor, slechte smaak: een sociologie van de mop. Boom. General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:24 Sep 2021 LITERATUUR R Alford,, Finnegan & Richard Alford 19811 A Holo-cultural Study of Humor. Ethos9(2), 149-164. Ambrose,, Anthony 19633 Age of Onset of Ambivalence in Early Childhood: Indications from the Study of Laughter. JournalJournal of Child Psychology and Psychiatry 4, 167-181. Anoniem m 18755 Mijn oom de majoor. In: Almanak van het Leidsche Studentencorps, 111-113. Leiden: P. -
Issue 251 ▸ 20 September 2012 Reportersharing Stories of Imperial’S Community
Issue 251 ▸ 20 September 2012 reporterSharing stories of Imperial’s community Hidden gems Scientists unravel the secrets of proteins in Imperial’s Oxfordshire outpost at Diamond Light Source → centre pages £6 MILLION FEATURE FOCUS “it’s BEEN A LABS OPENED Getting to know PRIVILEGE” Facility to new College Professor explore ways Secretary Kinloch reflects of storing CO2 and Registrar, on his time underground John Neilson as HoD PAGE 3 PAGE 10 PAGE 13 2 >> newsupdate www.imperial.ac.uk/reporter | reporter | 20 September 2012 • issue 251 Imperial physicists help to make accelerator science go faster The John Adams Institute for help accelerator science develop hospitals or research centres. Accelerator Science (JAI) is expand- beyond its current use for research Professor Zulfikar Najmudin, JAI’s EDITOR’S CORNER ing, with a new research base at in fundamental physics, such as deputy director ( Physics), said: “The Imperial joining two existing centres the hunt for new bosons at the JAI now connects the world-leading at Royal Holloway, University of Large Hadron Collider. efforts on laser plasma acceleration Starting London and the University of Oxford. Experts at Imperial will now that were developed in Imperial’s help to develop advanced medical Plasma Physics Group and Oxford’s out Scientists at the Institute are treatments, such as new forms Atomic and Laser Group. It creates researching ways to improve of cancer radiotherapy that avoid new opportunities for developments particle accelerator technology damaging tissue surrounding a of laser plasma acceleration With the glamour and and its applications in science tumour. Future developments applications and new instruments, excitement of the Olympic and medicine.