Desy Marks 50 Years of Accelerator Research
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From God's Particle to Dark Matter
SAE./No.65/October 2016 Studies in Applied Economics FROM GOD'S PARTICLE TO DARK MATTER Joachim Mnich Johns Hopkins Institute for Applied Economics, Global Health, and Study of Business Enterprise From God’s Particle to Dark Matter Investigating the Universe: Getting the Big Picture by Colliding Small Particles1 by Joachim Mnich Copyright 2016 by the author. About the Series The Studies in Applied Economics series is under the general direction of Prof. Steve H. Hanke, Co-Director of The Johns Hopkins Institute for Applied Economics, Global Health, and the Study of Business Enterprise ([email protected]). About the Author Joachim Mnich is the Director for Particle and Astroparticle Physics at the Deutsches Elektronen-Synchrotron (DESY) and Professor of Physics at the University of Hamburg. He is currently Chair of the International Committee for Future Accelerators (ICFA), a panel working under the auspice of the International Union of Pure and Applied Physics (IUPAP) to promote international collaboration in all phases of the construction and exploitation of high energy accelerators. He is also a member of numerous national and international strategy and advisory boards. Prof. Joachim Mnich has a graduate degree in electrical engineering and obtained a PhD in particle physics, both from Aachen University. In the past, he has worked on large particle physics experiments at DESY and CERN. His interest is experimental particle physics, particularly precision tests of the electroweak interaction, and the design, development, and construction of modern tracking detectors. Since 2000, he has been a member of the CMS experiment at the Large Hadron Collider at CERN and contributed to the construction of the silicon-based central tracking detector as well as to studies to test the Standard Model of particle physics. -
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. -
Recent Changes to the E- / E+ Injector (Linac II) at DESY
Proceedings of LINAC08, Victoria, BC, Canada TUP008 RECENT CHANGES TO THE e+ /e- INJECTOR (LINAC II) AT DESY M. Hüning#, M. Schmitz, DESY, Hamburg, Germany Abstract required together with the high revolution frequency of The Linac II at DESY consists of a 6A/150kV DC PIA a reduction of beam pulse duration. electron gun, a 400 MeV primary electron linac, an Today DESY II with its injector Linac II provides 800 MW positron converter, and a 450 MeV secondary electrons and positrons for the synchrotron radiation electron/positron linac. facility DORIS, the synchrotron radiation facility under The Positron Intensity Accumulator (PIA) is also construction PETRA III, and for test beam targets inside considered part of the injector complex accumulating and DESY II. The injection into HERA via PETRA II is shut damping the 50 Hz beam pulses from the linac and off, but there is an option to inject directly into HERA if transferring them with a rate of 6.25 Hz or 3.125 Hz into there is the requirement by future projects. the Synchrotron DESY II. The typical positrons rates are 6⋅1010/s. LINAC OVERVIEW DESY II and Linac II will serve as injectors for the two synchrotron light facilities PETRA III and DORIS. Since Injection System PETRA III will operate in top-up mode, Linac availability The primary electron beam is produced by a 120 kV of 98-99% is required. DORIS requires positrons for pulsed DC diode gun. Beam pulses of up to 6 A and 4 μs operation. Therefore during top-up mode positrons are duration are produced. -
European XFEL Status of Technical Developments Massimo Altarelli
European XFEL Status of Technical Developments Massimo Altarelli On behalf also of Serguei Molodtsov, Andreas Schwarz, Thomas Tschentscher and Karl Witte European XFEL - Status of Technical Developments The European XFEL – “Start-up” Version 2 Some specifications Photon energy 0.8–12.4 keV beam transport & instruments ~1000 m Pulse duration <100 fs Pulse energy few mJ undulator ~200 m super-conducting accelerator 10 Hz/4.5 MHz (27 000 b/s) accelerator ~1700 m 3 beamlines/6 instruments ¾ extension to TDR version with 5 BLs and 10 instruments possible Various other extensions possible SASE 2 tunable, planar e- ¾ variable polarization ID’s ~0.15 – 0.4 nm ¾ electrons shorter wavelengths 17.5 GeV ¾ possibly CW operation SASE 1 - e planar SASE 3 Experiments First beam 2014 0.1 nm tunable, planar 0.4 – 1.6 nm Start of user operation 2015 1.2 – 4.9 nm (10 GeV) Fourth European XFEL Users' Meeting, Hamburg, 27-29.01.2010 Massimo Altarelli, European XFEL European XFEL - Status of Technical Developments Scientific instruments 3 Ultrafast Coherent Diffraction Imaging of Single Particles, Clusters, and Biomolecules (SPB) Structure determination of single particles: atomic clusters, bio-molecules, virus particles, cells. Materials Imaging & Dynamics (MID) Structure determination of nano- devices and dynamics at the nanoscale. Femtosecond Diffraction Experiments (FDE) Time-resolved investigations of the dynamics of Hard x-rays solids, liquids, gases High Energy Density Matter (HED) Investigation of matter under extreme conditions using hard -
Collider Physics at HERA
ANL-HEP-PR-08-23 Collider Physics at HERA M. Klein1, R. Yoshida2 1University of Liverpool, Physics Department, L69 7ZE, Liverpool, United Kingdom 2Argonne National Laboratory, HEP Division, 9700 South Cass Avenue, Argonne, Illinois, 60439, USA May 21, 2008 Abstract From 1992 to 2007, HERA, the first electron-proton collider, operated at cms energies of about 320 GeV and allowed the investigation of deep-inelastic and photoproduction processes at the highest energy scales accessed thus far. This review is an introduction to, and a summary of, the main results obtained at HERA during its operation. To be published in Progress in Particle and Nuclear Physics arXiv:0805.3334v1 [hep-ex] 21 May 2008 1 Contents 1 Introduction 4 2 Accelerator and Detectors 5 2.1 Introduction.................................... ...... 5 2.2 Accelerator ..................................... ..... 6 2.3 Deep Inelastic Scattering Kinematics . ............. 9 2.4 Detectors ....................................... .... 12 3 Proton Structure Functions 15 3.1 Introduction.................................... ...... 15 3.2 Structure Functions and Parton Distributions . ............... 16 3.3 Measurement Techniques . ........ 18 3.4 Low Q2 and x Results .................................... 19 2 3.4.1 The Discovery of the Rise of F2(x, Q )....................... 19 3.4.2 Remarks on Low x Physics.............................. 20 3.4.3 The Longitudinal Structure Function . .......... 22 3.5 High Q2 Results ....................................... 23 4 QCD Fits 25 4.1 Introduction.................................... ...... 25 4.2 Determinations ofParton Distributions . .............. 26 4.2.1 TheZEUSApproach ............................... .. 27 4.2.2 TheH1Approach................................. .. 28 4.3 Measurements of αs inInclusiveDIS ............................ 29 5 Jet Measurements 32 5.1 TheoreticalConsiderations . ........... 32 5.2 Jet Cross-Section Measurements . ........... 34 5.3 Tests of pQCD and Determination of αs ......................... -
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. -
DESY) DESY Is One of the World's Leading Accelerator Centres and a Member of the Helmholtz Association
Deutsches Elektronen- Synchrotron Deutsches Elektronen-Synchrotron (DESY) DESY is one of the world's leading accelerator centres and a member of the Helmholtz Association. DESY develops, builds and operates large particle accelerators used to investigate the structure of matter. DESY offers a broad research spectrum of international standing focusing on three main areas: accelerator development, construction and operation; photon science; particle and astroparticle physics. Facts and figures Established in Hamburg on 18 December 1959 • Locations: Hamburg and Zeuthen (Brandenburg) • Budget: 192 Mio.€ (Hamburg 173/Zeuthen 19 Mio.€ ) , Financing: 90% on the national level (German Federal Ministry of Education and Research); 10% on the state level (City of Hamburg and Federal State of Brandenburg) • Employees: approx. 2000, including 650 scientists working in the fields of accelerator operation, research and development • Guest scientists: more than 3000 from over 40 countries p.a. • Training: more than 100 young people in commercial and technical vocations • Young scientists: more than 700 diploma students, doctoral candidates and postdocs Year DESY activities 2009 Start with XFEL 2010 Start with PETRA III 2010 „Go“ for CSSB building 2011 Start of FLASH Extension: FLASH II 2012 Completion of CFEL building 2012 DORIS III shutdown 2013 Start of construction PETRA III Ext. North , East International and national cooperations: HSE Organisation CFEL, CSSB, PIER, LHC, Ice Cube, CTA etc. The classical Safety, Fire protection and Environmental Group and Radiation Protection Group are administrative departments. Personnel safety and experimental safety is under the administration of the different work departments. In total there are 12 engineers, 10 technicians and 5 administrative assistants to support DESY employees and guests in safety, health and environmental interests. -
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 European X-Ray Free-Electron Laser Technical Design Report
XFEL X-Ray Free-Electron Laser The European X-Ray Free-Electron Laser Technical design report Editors: Massimo Altarelli, Reinhard Brinkmann, Majed Chergui, Winfried Decking, Barry Dobson, Stefan Düsterer, Gerhard Grübel, Walter Graeff, Heinz Graafsma, Janos Hajdu, Jonathan Marangos, Joachim Pflüger, Harald Redlin, David Riley, Ian Robinson, Jörg Rossbach, Andreas Schwarz, Kai Tiedtke, Thomas Tschentscher, Ivan Vartaniants, Hubertus Wabnitz, Hans Weise, Riko Wichmann, Karl Witte, Andreas Wolf, Michael Wulff, Mikhail Yurkov DESY 2006-097 July 2007 Publisher: DESY XFEL Project Group European XFEL Project Team Deutsches Elektronen-Synchrotron Member of the Helmholtz Association Notkestrasse 85, 22607 Hamburg Germany http://www.xfel.net E-Mail: [email protected] Reproduction including extracts is permitted subject to crediting the source. ISBN 978-3-935702-17-1 Contents Contents Authors ...................................................................................................................... vii Foreword .................................................................................................................. xiii Executive summary .....................................................................................................1 1 Introduction ..........................................................................................................11 1.1 Accelerator-based light sources..................................................................11 1.2 Free-electron lasers ....................................................................................13 -
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.