NA61/SHINE Experiment—Program Beyond 2020
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Il Nostro Mondo
IL NOSTRO MONDO THE DESIGN, CONSTRUCTION AND PERFORMANCE OF THE CERN INTERSECTING STORAGE RINGS (ISR) A RECOLLECTION OF WORLD’S FIRST PROTON-PROTON COLLIDER KURT HÜBNER CERN, Geneva, Switzerland 1 Design which had a beam energy of 160 MeV. The interaction points to increase the collision rate The concept of colliding beams appeared design of these colliders started in 1957. but without special lattice insertions as one first in a German patent by Rolf Widerøe In 1961, the Accelerator Research Group would use these days. registered in 1943 and published in 1952. Division was expanded into the Accelerator Combined-function magnets were chosen However, at that time the intensity of beams Division as experienced manpower had as in the PS, i.e. the main magnets had a was too low for an exploitable collision rate as become available after the running-in of the magnetic dipole field to bend the beam and a beam accumulation had not yet been invented. PS in 1960. At the same time it was decided quadrupole field to focus the beam. This type The first ideas of a realistic design were to construct a small accelerator to test rf of magnet provided space for the elaborate published in 1956 by Gerard O’Neill and by the stacking, a technique to be experimentally pole-face windings foreseen to control the MURA Group lead by Donald Kerst in the USA. proven, as it was essential for the performance magnetic field to a very high precision. It also MURA had come up with beam accumulation and success of the ISR. -
Hagedorn's Hadron Mass Spectrum and the Onset of Deconfinement
Hagedorn’s Hadron Mass Spectrum and the Onset of Deconfinement∗ Marek Gazdzicki´ and Mark I. Gorenstein Abstract A brief history of the observation of the onset of deconfinement - the beginning of the creation of quark gluon plasma in nucleus-nucleus collisions with increasing collision energy - is presented. It starts with the measurement of hadron mass spectrum and the Hagedorn’s hypothesis of the limiting temperature of hadronic matter (the Hagedorn temperature). Then the conjecture that the Hage- dorn temperature is the phase transition temperature was formulated with the crucial Hagedorn participation. It was confirmed by the observation of the onset of decon- finement in lead-lead collisions at the CERN SPS energies. 1 Hadron Mass Spectrum and the Hagedorn Temperature A history of multi-particle production started with discoveries of hadrons, first in cosmic-ray experiments and soon after in experiments using beams of particles produced in accelerators. Naturally, the first hadrons, discovered in collisions of cosmic-ray particles, were the lightest ones, pion, kaon and L. With the rapid ad- vent of particle accelerators new particles were uncovered almost day-by-day. There are about 1000 hadronic states known so far. Their density in mass r(m) increases approximately exponentially as predicted by the Hagedorn’s Statistical Bootstrap Model [1] formulated in 1965: r(m) = const m−a exp(bm) : (1) In the case of point-like hadron states this leads to a single-particle partition func- tion: p ! V Z ¥ Z ¥ k2 + m2 Z(T;V) = dm k2dk exp − r(m) ; (2) arXiv:1502.07684v1 [nucl-th] 26 Feb 2015 2 2p mp 0 T Marek: Goethe-University, Frankfurt, Germany; and Jan Kochanowski University, Kielce, Poland Mark: Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine; and Frankfurt Institute for Advanced Studies, Frankfurt, Germany ∗Chapter in: R. -
Pos(ICRC2019)446
New Results from the Cosmic-Ray Program of the NA61/SHINE facility at the CERN SPS PoS(ICRC2019)446 Michael Unger∗ for the NA61/SHINE Collaborationy Karlsruhe Institute of Technology (KIT), Postfach 3640, D-76021 Karlsruhe, Germany E-mail: [email protected] The NA61/SHINE experiment at the SPS accelerator at CERN is a unique facility for the study of hadronic interactions at fixed target energies. The data collected with NA61/SHINE is relevant for a broad range of topics in cosmic-ray physics including ultrahigh-energy air showers and the production of secondary nuclei and anti-particles in the Galaxy. Here we present an update of the measurement of the momentum spectra of anti-protons produced in p−+C interactions at 158 and 350 GeV=c and discuss their relevance for the understanding of muons in air showers initiated by ultrahigh-energy cosmic rays. Furthermore, we report the first results from a three-day pilot run aimed at investigating the ca- pability of our experiment to measure nuclear fragmentation cross sections for the understanding of the propagation of cosmic rays in the Galaxy. We present a preliminary measurement of the production cross section of Boron in C+p interactions at 13.5 AGeV=c and discuss prospects for future data taking to provide the comprehensive and accurate reaction database of nuclear frag- mentation needed in the era of high-precision measurements of Galactic cosmic rays. 36th International Cosmic Ray Conference -ICRC2019- July 24th - August 1st, 2019 Madison, WI, U.S.A. ∗Speaker. yhttp://shine.web.cern.ch/content/author-list c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). -
NA61/SHINE Facility at the CERN SPS: Beams and Detector System
Preprint typeset in JINST style - HYPER VERSION NA61/SHINE facility at the CERN SPS: beams and detector system N. Abgrall11, O. Andreeva16, A. Aduszkiewicz23, Y. Ali6, T. Anticic26, N. Antoniou1, B. Baatar7, F. Bay27, A. Blondel11, J. Blumer13, M. Bogomilov19, M. Bogusz24, A. Bravar11, J. Brzychczyk6, S. A. Bunyatov7, P. Christakoglou1, T. Czopowicz24, N. Davis1, S. Debieux11, H. Dembinski13, F. Diakonos1, S. Di Luise27, W. Dominik23, T. Drozhzhova20 J. Dumarchez18, K. Dynowski24, R. Engel13, I. Efthymiopoulos10, A. Ereditato4, A. Fabich10, G. A. Feofilov20, Z. Fodor5, A. Fulop5, M. Ga´zdzicki9;15, M. Golubeva16, K. Grebieszkow24, A. Grzeszczuk14, F. Guber16, A. Haesler11, T. Hasegawa21, M. Hierholzer4, R. Idczak25, S. Igolkin20, A. Ivashkin16, D. Jokovic2, K. Kadija26, A. Kapoyannis1, E. Kaptur14, D. Kielczewska23, M. Kirejczyk23, J. Kisiel14, T. Kiss5, S. Kleinfelder12, T. Kobayashi21, V. I. Kolesnikov7, D. Kolev19, V. P. Kondratiev20, A. Korzenev11, P. Koversarski25, S. Kowalski14, A. Krasnoperov7, A. Kurepin16, D. Larsen6, A. Laszlo5, V. V. Lyubushkin7, M. Mackowiak-Pawłowska´ 9, Z. Majka6, B. Maksiak24, A. I. Malakhov7, D. Maletic2, D. Manglunki10, D. Manic2, A. Marchionni27, A. Marcinek6, V. Marin16, K. Marton5, H.-J.Mathes13, T. Matulewicz23, V. Matveev7;16, G. L. Melkumov7, M. Messina4, St. Mrówczynski´ 15, S. Murphy11, T. Nakadaira21, M. Nirkko4, K. Nishikawa21, T. Palczewski22, G. Palla5, A. D. Panagiotou1, T. Paul17, W. Peryt24;∗, O. Petukhov16 C.Pistillo4 R. Płaneta6, J. Pluta24, B. A. Popov7;18, M. Posiadala23, S. Puławski14, J. Puzovic2, W. Rauch8, M. Ravonel11, A. Redij4, R. Renfordt9, E. Richter-Wa¸s6, A. Robert18, D. Röhrich3, E. Rondio22, B. Rossi4, M. Roth13, A. Rubbia27, A. Rustamov9, M. -
FIAS Scientific Report 2012
FIAS Scientific Report 2012 Frankfurt Institute for Advanced Studies Editor: Dr. Joachim Reinhardt Ruth-Moufang-Str. 1 reinhardt@fias.uni-frankfurt.de 60438 Frankfurt am Main Germany Tel.: +49 (0)69 798 47600 Fax: +49 (0)69 798 47611 fias.uni-frankfurt.de Vorstand: Prof. Dr. Volker Lindenstruth, Vorsitzender Regierungspräsidium Darmstadt Prof. Dr. Dirk H. Rischke Az:II21.1–25d04/11–(12)–545 Prof. Dr. Dr. h.c. mult. Wolf Singer Finanzamt Frankfurt Prof. Dr. Dres. h.c. Horst Stöcker Steuernummer: 47 250 4216 1 – XXI/101 Prof. Dr. Jochen Triesch Freistellungsbescheid vom 16.08.2010 Geschäftsführer: Gisbert Jockenhöfer FIAS Scientific Report 2012 Table of Contents Preface..........................................................................5 Research highlights 2012 . 6 1. Partner Research Centers 1.1 HIC for FAIR / EMMI . 9 1.2 Bernstein Focus Neurotechnology . 11 2. Graduate Schools 2.1 HGS-HIRe / HQM . 14 2.2 FIGSS . 16 3. FIAS Scientific Life 3.1 Seminars and Colloquia . 20 3.2 Organized Conferences. .23 3.2 FIAS Forum . 25 4. Research Reports 4.1 Nuclear Physics, Particle Physics, Astrophysics . 26 4.2 Neuroscience. .59 4.3 Biology, Chemistry, Molecules, Nanosystems . 75 4.4 Scientific Computing, Information Technology . .101 5. Talks and Publications 5.1 Conference and Seminar Talks . 117 5.2 Conference Abstracts and Posters . 126 5.3 Cumulative List of Publications . 129 3 4 Preface In the year 2012 FIAS has continued to carry out its mission as an independent research institute performing cutting-edge research in the natural and computer sciences. An account of recent scientific accomplishments can be found in the brief individual research reports collected in Section 4. -
Improving the Slow Extraction Efficiency of the CERN Super
Improving the slow extraction efficiency of the CERN Super Proton Synchrotron Brunner Kristóf Faculty of Science Eötvös Loránd University Supervisors: Barna Dániel, Wigner RCP Christoph Wiesner, CERN May 2018 Contents 1 Introduction4 2 CERN accelerator complex5 2.1 Accelerators..................................... 5 2.2 Experiments..................................... 6 2.2.1 Colliders .................................. 7 2.2.2 Fixed target experiments.......................... 7 2.3 Current and future demands of fixed target experiments.............. 7 3 Introduction to accelerator physics9 3.1 History of linear and circular accelerators ..................... 9 3.2 Design orbit, focusing................................. 11 3.3 Betatron oscillation, the behaviour of single particles ................ 11 3.4 The Twiss-ellipse, the behaviour of the beam ................... 13 3.5 Normalised phase space............................... 15 3.6 Tune and resonances ................................ 16 4 Extraction from a synchrotron 19 4.1 Fast extraction.................................... 19 4.2 Multi-turn extraction ................................ 20 4.3 Sextupole driven slow extraction........................... 21 4.4 Possible enhancements............................... 24 4.4.1 Diffuser................................... 24 4.4.2 Dynamic bump............................... 26 4.4.3 Phase space folding............................. 26 5 Massless septum 28 5.1 Method of phase space folding using a massless septum.............. 29 6 Simulation -
Particle Physics Lecture 4: the Large Hadron Collider and Other Accelerators November 13Th 2009
Subatomic Physics: Particle Physics Lecture 4: The Large Hadron Collider and other accelerators November 13th 2009 • Previous colliders • Accelerating techniques: linacs, cyclotrons and synchrotrons • Synchrotron Radiation • The LHC • LHC energy and luminosity 1 Particle Acceleration Long-lived charged particles can be accelerated to high momenta using electromagnetic fields. • e+, e!, p, p!, µ±(?) and Au, Pb & Cu nuclei have been accelerated so far... Why accelerate particles? • High beam energies ⇒ high ECM ⇒ more energy to create new particles • Higher energies probe shorter physics at shorter distances λ c 197 MeV fm • De-Broglie wavelength: = 2π pc ≈ p [MeV/c] • e.g. 20 GeV/c probes a distance of 0.01 fm. An accelerator complex uses a variety of particle acceleration techniques to reach the final energy. 2 A brief history of colliders • Colliders have driven particle physics forward over the last 40 years. • This required synergy of - hadron - hadron colliders - lepton - hadron colliders & - lepton - lepton colliders • Experiments at colliders discovered W- boson, Z-boson, gluon, tau-lepton, charm, bottom and top-quarks. • Colliders provided full verification of the Standard Model. DESY Fermilab CERN SLAC BNL KEK 3 SppS̅ at CERNNo b&el HERAPrize for atPhy sDESYics 1984 SppS:̅ Proton anti-Proton collider at CERN. • Given to Carlo Rubbia and Simon van der Meer • Ran from 1981 to 1984. Nobel Prize for Physics 1984 • Centre of Mass energy: 400 GeV • “For their decisive • 6.9 km in circumference contributions to large • Two experiments: -
The Search for Charged Massive Supersymmetric Particles at the LHC
The Search for Charged Massive Supersymmetric Particles at the LHC Aleksey Pavlov A Senior Project Presented to Cal Poly June 5, 2012 This material is based upon work supported by The National Science Foundation under grant number 0969966. 1 Contents 1 Abstract 3 2 Introduction 3 3 Supersymmetry: An Extension of the Standard Model 5 4 CHAMPs 8 5 The LHC 9 6 The ALICE Detector 12 7 Analysis 14 8 Results 17 2 1 Abstract Charged Massive Particles (CHAMPs) are predicted in the Supersymmetry (SUSY) extension of the Standard Model though they have never been ob- served. We look for CHAMPs in the ALICE Detector at the Large Hadron Collider at CERN. While the main purpose of ALICE is to study Quark- Gluon Plasma, we take advantage of the tracking and time of flight capabil- ities of several sub-detectors in ALICE to look for signs of CHAMPs. These elusive particles are characterized by their slow velocity, high transverse mo- mentum and therefore heavy mass. Our research found a small handful of candidates among a large sample size but more work is required to confirm their identity and exclude the possibility that they have been misidentified. 2 Introduction The Standard Model of Particle Physics (SM) is the modern theory describ- ing how fundamental particles interact and behave. It was developed in the second half of the 20th Century after physicist Sheldon Glashow found a way to combine, or unify, the electromagnetic and electroweak forces [7]. In 1973 Glashow's electroweak theory was experimentally confirmed at CERN, the European Organization for Nuclear Research in Geneva, Switzerland, when nuetral currents through the weak nuclear force were measured. -
In Experimental Particle Physics
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Bringing the Heavens Down to Earth
International Journal of High-Energy Physics CERN I COURIER Volume 44 Number 3 April 2004 Bringing the heavens down to Earth ACCELERATORS NUCLEAR PHYSICS Ministers endorse NuPECC looks to linear collider p6 the future p22 POWER CONVERTERS Principles : Technologies : • Linear, Switch Node primary or secondary, Current or voltage stabilized • Hani, or résonant» Buck, from % to the sub ppm level • Boost, 4-quadrant operation Limits : Control : * 1A up to 25kA • Local manual and/or computer control * 3V to 50kV • Interfaces: RS232, RS422, RS485, IEEE488/GPIB, •O.lkVAto 3MVA • CANbus, Profibus DP, Interbus S, Ethernet • Adaptation to EPICS • DAC and ADC 16 to 20 bit resolution and linearity Applications : Electromagnets and coils Superconducting magnets or short samples Resistive or capacitive loads Klystrons, lOTs, RF transmitters 60V/350OM!OkW Thyristor controlled (S£M®) I0"4, Profibus 80V/600A,50kW 5Y/30Ô* for supraconducting magnets linear technology < Sppm stability with 10 extra shims mm BROKER BIOSPIN SA • France •m %M W\. WSÊ ¥%, 34 rue de l'industrie * F-67166 Wissembourg Cedex Tél. +33 (0)3 88 73 68 00 • Fax. +33 (0)3 88 73 68 79 lOSPIN power@brukerir CONTENTS Covering current developments in high- energy physics and related fields worldwide CERN Courier is distributed to member-state governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly, except for January and August, in English and French editions. The views expressed are not CERN necessarily those of the CERN management. -
THE PROTON-ANTIPROTON COLLIDER Lecture Delivered at CERN on 25 November 1987 Lyndon Evans
CERN 88-01 11 March 1988 ORGANISATION EUROPÉENNE POUR LA RECHERCHE NUCLÉAIRE CERN EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH CERN ACCELERATOR SCHOOL Third John Adams Memorial Lecture THE PROTON-ANTIPROTON COLLIDER Lecture delivered at CERN on 25 November 1987 Lyndon Evans GENEVA 1988 ABSTRACT The subject of this lecture is the CERN Proton-Antiproton (pp) Collider, in which John Adams was intimately involved at the design, development, and construction stages. Its history is traced from the original proposal in 1966, to the first pp collisions in the Super Proton Synchrotron (SPS) in 1981, and to the present time with drastically improved performance. This project led to the discovery of the intermediate vector boson in 1983 and produced one of the most exciting and productive physics periods in CERN's history. RN —Service d'Information Scientifique-RD/757-3000-Mars 1988 iii CONTENTS Page 1. INTRODUCTION 1 2. BEAM COOLING l 3. HISTORICAL DEVELOPMENT OF THE pp COLLIDER CONCEPT 2 4. THE SPS AS A COLLIDER 4 4.1 Operation 4 4.2 Performance 5 5. IMPACT OF EARLIER CERN DEVELOPMENTS 5 6. PROPHETS OF DOOM 7 7. IMPACT ON THE WORLD SCENE 9 8. CONCLUDING REMARKS: THE FUTURE OF THE pp COLLIDER 9 REFERENCES 10 Plates 11 v 1. INTRODUCTION The subject of this lecture is the CERN Proton-Antiproton (pp) Collider and let me say straightaway that some of you might find that this talk is rather polarized towards the Super Proton Synchrotron (SPS). In fact, the pp project was a CERN-wide collaboration 'par excellence'. However, in addition to John Adams' close involvement with the SPS there is a natural tendency for me to remain within my own domain of competence. -
From the Web to the Grid and Beyond
The Frontiers Collection From the Web to the Grid and Beyond Computing Paradigms Driven by High-Energy Physics Bearbeitet von René Brun, Frederico Carminati, Giuliana Galli-Carminati 1. Auflage 2012. Buch. xx, 360 S. Hardcover ISBN 978 3 642 23156 8 Format (B x L): 15,5 x 23,5 cm Gewicht: 726 g Weitere Fachgebiete > EDV, Informatik > Hardwaretechnische Grundlagen > Grid- Computing & Paralleles Rechnen schnell und portofrei erhältlich bei Die Online-Fachbuchhandlung beck-shop.de ist spezialisiert auf Fachbücher, insbesondere Recht, Steuern und Wirtschaft. Im Sortiment finden Sie alle Medien (Bücher, Zeitschriften, CDs, eBooks, etc.) aller Verlage. Ergänzt wird das Programm durch Services wie Neuerscheinungsdienst oder Zusammenstellungen von Büchern zu Sonderpreisen. Der Shop führt mehr als 8 Millionen Produkte. Preface Modern High Energy Physics (HEP), as a science studying the results of accelerator- driven particle collisions, was born after the Second World War, at the same time as computers. HEP research has been constantly limited by technology, both in the accelerator and detector domains as well as that of computing. At the same time High Energy physicists have greatly contributed to the development of Information Technology. During all these years, the Conseil Europeen´ pour la Recherche Nucleaire´ 1 (CERN [1], located in Geneva, Switzerland) has been a privileged place for the evolution of HEP computing. Several applications conceived for HEP have found applications well beyond it, the World Wide Web (see Chap. 2) being the most notable example. During all these years HEP computing has faced the chal- lenge of software development within distributed communities, and of exploiting geographically distributed computing resources.