NA61/SHINE Facility at the CERN SPS: Beams and Detector System
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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. -
Neutrino Oscillations: T2k and Na61 Experiments, R&D
NEUTRINO OSCILLATIONS: T2K AND NA61 EXPERIMENTS, R&D TOWARDS A FUTURE NEUTRINO PROGRAM 1 Research Plan The field of neutrino physics is certainly one of the most active in particle physics today. It is by now well established that neutrinos have mass and that the three families mix. In the minimal Standard Model, neutrinos are massless; massive neutrinos require either a new ad- hoc conservation law or new phenomena beyond the present framework, with a possible link to the grand unification scale via the see-saw mechanism. A deep field of research is thus open, that could last several decades and culminate with the discovery of leptonic CP violation – a key ingredient in the understanding of the baryon- anti-baryon asymmetry of the universe. Because observation of CP violation in neutrino oscillations requires appearance experiments, accessible at accelerators only, an important investment in accelerator-based neutrino beams and experiments is called for. The CHIPP Roadmap considers neutrino physics as one of the three pillars of particle physics in Switzerland, and so does the 15 years research plan of the DPNC at University of Geneva1. The neutrino group at DPNC has been actively involved in this quest since the nomination of Prof. A. Blondel in early 2000, where participation in the HARP experiment at CERN led us to the K2K experiment in Japan, in which the first observation of neutrino oscillation with a neutrino beam was achieved. The group received an added boost with the nomination of Alessandro Bravar (MER) in 2006. The research program comprises a progression of on- going experiments and far-reaching R&D activity as described in the SNF reports of October 2007 and October 2008. -
Measurements of Hadronic Cross Section for Precise Determination of Neutrino Beam Properties in T2K Oscillation Experiment
University of Warsaw Faculty of Physics Institute of Experimental Physics Measurements of Hadronic Cross Section for Precise Determination of Neutrino Beam Properties in T2K Oscillation Experiment Magdalena Zofia Posiadała Ph.D. thesis written under supervision of prof. dr hab. Danuta Kiełczewska Warsaw, 2011 Abstract Differential cross sections and mean multiplicities in production processes for low momentum charged pion mesons and protons in p+C interactions at 31 GeV/c measured with the large acceptance NA61/SHINE spectrometer at the CERN SPS are presented. A set of data col- lected during the first NA61/SHINE run in 2007 with a thin graphite target was used for the analysis. The results are presented as a function of laboratory momentum in 10 intervals of the laboratory polar angle covering the range from 0 up to 420 mrad. The spectra are compared with predictions of several hadron production models. Measurements for π+ and π− mesons are used by the T2K experiment to tune neutrino beam simulations and reduce uncertainties on charged pion production. Contents List of Figures vii List of Tables xi Acknowledgments xii Introduction 1 1 Neutrinos 4 1.1 Neutrino oscillation mechanism . .5 1.2 The Current Situation in Neutrino Oscillation Physics . .7 2 T2K experiment and its prerequisites for NA61/SHINE measurements 18 2.1 The T2K long baseline neutrino oscillation experiment . 18 2.2 J-PARC facility . 20 2.2.1 J-PARC accelerator . 20 2.2.2 Primary and secondary T2K beamline . 20 2.2.3 Near detector complex . 23 2.3 Overview of the Super-Kamiokande detector . 24 2.4 T2K physical goals . -
Measurement of Hadron-Carbon Interactions for Better Understanding of Air Showers with NA61/SHINE
33RD INTERNATIONAL COSMIC RAY CONFERENCE,RIO DE JANEIRO 2013 THE ASTROPARTICLE PHYSICS CONFERENCE Measurement of hadron-carbon interactions for better understanding of air showers with NA61/SHINE H. P. DEMBINSKI1 FOR THE NA61/SHINE COLLABORATION2. 1 Institut fur¨ Kernphysik, KIT Karlsruhe, Postfach 3640, D - 76021 Karlsruhe 2 Full author list: https: // na61. web. cern. ch/ na61/ pages/ storage/ authors_ list. pdf [email protected] Abstract: The interpretation of air shower measurements requires the detailed simulation of hadronic particle production over a wide range of energies and the forward phase space of secondary particles. In air showers, the bulk of particles is produced at later stages of the shower development and at equivalent beam energies in the sub-TeV range. NA61/SHINE is a fixed target experiment using secondary beams produced at the SPS at 1 CERN. Hadron-hadron interactions have been recorded at beam momenta between 13 and 350 GeVc− with a wide-acceptance spectrometer. In this article we present measurements of the inelastic cross-section and secondary particle yields of pion-carbon interactions, which are essential for modelling air showers. Keywords: hadron interaction, QCD, air shower, pion 1 Hadronic interactions in air showers Cosmic rays initiate extensive air showers (EAS) when they collide with nuclei of the atmosphere. The EAS data recorded by experiments like the Pierre Auger Observa- tory [1], KASCADE [2] or IceTop [3], is used to infer their properties. The interpretation relies on simulations of the shower development during which electromagnetic and hadronic particle interactions are followed from primary 20 9 energies of & 10 eV down to energies of 10 eV. -
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). -
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 -
Arxiv:1109.3262V1 [Hep-Ex] 15 Sep 2011 University of Tokyo, Department of Physics, Bunkyo, Tokyo 113-0033, Japan
Letter of Intent: The Hyper-Kamiokande Experiment | Detector Design and Physics Potential | K. Abe,12, 14 T. Abe,10 H. Aihara,10, 14 Y. Fukuda,5 Y. Hayato,12, 14 K. Huang,4 A. K. Ichikawa,4 M. Ikeda,4 K. Inoue,8, 14 H. Ishino,7 Y. Itow,6 T. Kajita,13, 14 J. Kameda,12, 14 Y. Kishimoto,12, 14 M. Koga,8, 14 Y. Koshio,12, 14 K. P. Lee,13 A. Minamino,4 M. Miura,12, 14 S. Moriyama,12, 14 M. Nakahata,12, 14 K. Nakamura,2, 14 T. Nakaya,4, 14 S. Nakayama,12, 14 K. Nishijima,9 Y. Nishimura,12 Y. Obayashi,12, 14 K. Okumura,13 M. Sakuda,7 H. Sekiya,12, 14 M. Shiozawa,12, 14, ∗ A. T. Suzuki,3 Y. Suzuki,12, 14 A. Takeda,12, 14 Y. Takeuchi,3, 14 H. K. M. Tanaka,11 S. Tasaka,1 T. Tomura,12 M. R. Vagins,14 J. Wang,10 and M. Yokoyama10, 14 (Hyper-Kamiokande working group) 1Gifu University, Department of Physics, Gifu, Gifu 501-1193, Japan 2High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan 3Kobe University, Department of Physics, Kobe, Hyogo 657-8501, Japan 4Kyoto University, Department of Physics, Kyoto, Kyoto 606-8502, Japan 5Miyagi University of Education, Department of Physics, Sendai, Miyagi 980-0845, Japan 6Nagoya University, Solar Terrestrial Environment Laboratory, Nagoya, Aichi 464-8602, Japan 7Okayama University, Department of Physics, Okayama, Okayama 700-8530, Japan 8Tohoku University, Research Center for Neutrino Science, Sendai 980-8578, Japan 9Tokai University, Department of Physics, Hiratsuka, Kanagawa 259-1292, Japan 10 arXiv:1109.3262v1 [hep-ex] 15 Sep 2011 University of Tokyo, Department of Physics, Bunkyo, -
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 NA61/SHINE Experiment: Beams and Detector System
EUROPEAN LABORATORY FOR PARTICLE PHYSICS The NA61/SHINE experiment: beams and detector system By the NA61 Collaboration http://na61.web.cern.ch Abstract NA61/SHINE (SPS Heavy Ion and Neutrino Experiment) is a multi-purpose fixed target experiment to study hadron production in hadron-nucleus and nucleus-nucleus collisions at the CERN Super Proton Synchrotron. It recorded the first physics data with hadron beams in 2009 and with ion beams (secondary 7Be beams) in 2011. NA61/SHINE has greatly profited from the long development of the CERN pro- ton and ion sources and the accelerator chain as well as the H2 beam line of the CERN North Area. The latter has recently been modified to also serve as a fragment separator as needed to produce the Be beams for NA61/SHINE. Numerous compo- nents of the NA61/SHINE set-up were inherited from its predecessors, in particular, the last one, the NA49 experiment. Important new detectors and upgrades of the inherited equipment were introduced the NA61/SHINE Collaboration. This paper describes the NA61/SHINE experimental facility and used beams by the CERN Long Shutdown I, March 2013. June 11, 2013 Contents 1 Introduction 5 2 Beams 6 2.1 The proton acceleration chain . 6 2.2 The ion accelerator chain . 7 2.3 H2 beam line . 9 2.4 Hadron beams . 9 2.5 Primary and secondary ion beams . 10 3 Beam detectors and triggers 13 3.1 Beam counters . 13 3.2 A-detector . 14 3.3 Beam Position Detectors . 14 3.4 Z-detectors . 15 3.5 Trigger system . -
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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