Measurement of Hadron-Carbon Interactions for Better Understanding of Air Showers with NA61/SHINE

Total Page:16

File Type:pdf, Size:1020Kb

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. The penetrating muon component of an EAS is particu- larly important for the interpretation of data from ground detectors. Myons that reach ground typically originate from mesons produced in low energy interactions in the late stages of an air shower. Depending on the primary energy and detection distance, the relevant interaction energies are between 10 and 1000 GeV and the modeling of the corre- sponding low energy interactions contributes at least 10% Figure 1: Schematic layout of the NA61/SHINE experi- to the overall uncertainty of the predicted muon number at ment. ground (see e.g. Refs. [4–7]). Comprehensive and precise particle production measure- properties of the onset of de-confinement and a search for ments in this energy range are of great value. Unfortunately, the critical point of strongly interacting matter (see e.g. direct measurements are sparse, even for the most numer- Ref. [10]). ous projectile in air showers, the p-meson. Thus new data The layout of the NA61/SHINE detector is sketched in 1 with pion beams at 158 and 350 GeVc− on a thin car- Fig. 1. A set of scintillation and Cherenkov counters as bon target (as a proxy for nitrogen) were collected by the well as beam position detectors upstream of the spectrom- NA61/SHINE experiment at the CERN SPS and prelimi- eter provide timing reference, identification and position nary results from this data set are presented here. measurements of the incoming beam particles. Large time- projection-chambers (TPCs) inherited from the NA49 exper- iment [11] are used to measure the charge and momentum of 2 The NA61/SHINE experiment particles. The momentum resolution, s(1=p) = s(p)=p2, 4 1 NA61/SHINE (SHINE = SPS Heavy Ion and Neutrino Ex- is about 10− GeV− c at full magnetic field and the track- periment) [8] is a multi-purpose fixed target experiment to ing efficiency is better than 95%. Particle identification is study hadron production in hadron-nucleus and nucleus- achieved by measuring the energy loss along the tracks in nucleus collisions at the CERN Super Proton Synchrotron the TPCs and by determining their velocity from the time (SPS). Among its physics goals are precise hadron pro- of flight provided by large scintillator walls placed down- duction measurements for improving calculations of the stream of the TPCs. neutrino beam flux in the T2K neutrino oscillation experi- The centrality of nucleus-nucleus collisions can be esti- ment [9] as well as for more reliable simulations of hadronic mated using the measurement of the energy of projectile interactions in air showers. Moreover, p+p, p+Pb and nu- spectators with a calorimeter [12] located behind the time cleus+nucleus collisions are measured for a study of the of flight detectors. For nucleon-nucleus collisions, the cen- Hadron-carbon interactions measured with NA61/SHINE 33RD INTERNATIONAL COSMIC RAY CONFERENCE,RIO DE JANEIRO 2013 1 0 1 0 10− 10 10− 10 103 103 102 102 2 c 2 10 10 − 1 1 1 1 / mb GeV 10− 10− T p d σ 2 2 2 lab d 10− 10− p d 3 1 + 1 3 10− h− at 158 GeV c− h at 158 GeV c− 10− NA61/SHINE preliminary NA61/SHINE preliminary 4 4 10− 10− 103 103 102 102 2 c 2 10 10 − 1 1 1 1 / mb GeV 10− 10− T p d σ 2 2 2 lab d 10− 10− p d 3 1 + 1 3 10− h− at 350 GeV c− h at 350 GeV c− 10− NA61/SHINE preliminary NA61/SHINE preliminary 4 4 10− 10− 1 0 1 0 10− 10 10− 10 1 1 pT/GeV c− pT/GeV c− 1 Figure 2: Inclusive pT-spectra of charged hadrons produced in p−+C interactions at 158 and 350 GeVc− . In each figure, 1 1 the particle momentum p ranges from 0.58 to 145 GeVc− in steps of log10(plab=GeVc− ) = 0:08 from top to bottom. The 1 markers alternate between circle and square for each step in log10(plab=GeVc− ) to guide the eye. Hadron-carbon interactions measured with NA61/SHINE 33RD INTERNATIONAL COSMIC RAY CONFERENCE,RIO DE JANEIRO 2013 ] 10 2 0.5 NA61/SHINE preliminary simulation 1 0.4 1 1 − [mb/(GeV/c) T 0.3 σ 2 d -1 dp 10 /GeV c 10 1 0.2 data T − p QGSJetII-3 lepton fraction EPOS1.99 0.1 10-2 Sibyll2.1 NA61/SHINE preliminary 2 10− 0.0 0.5 1 1.5 2 2.5 0 1 2 p [GeV/c] 10 10 10 T 1 plab/GeV c− Figure 3: Transverse momentum spectrum of negatively Figure 4: Predicted fraction of negative leptons in charged 1 charged hadrons produced in p−+C interactions at particles produced in p−+C interactions at 158 GeVc− 1 1 158 GeVc beam momentum at plab =10.4 GeVc . beam momentum (average of VENUS and EPOS). − h i − trality is determined by counting low momentum particles are displayed in Fig. 3. The uncertainties shown are the from the target (so called ’gray protons’) with a small TPC total uncertainties including the statistical uncertainty and around the target. systematics from model correction, normalization, trigger NA61/SHINE started data taking in 2007. During the last bias, calibration and track topology. four years, a wealth of data has been recorded by the exper- These preliminary measurements are already useful to 1 iment at beam momenta ranging from 13 to 350 GeVc− judge the quality of event generators used in air-shower with various beam particles and targets. simulations. An example of the pT distribution of negatively charged hadrons produced in p−+C interactions at a beam 1 momentum of 158 GeVc− is shown in Fig. 3 for particle 1 3 NA61/SHINE results for the momenta with plab =10.4 GeVc and compared to h i − interpretation of cosmic ray air showers predictions by QGSJETII-03 [19], SIBYLL2.1 [20] and EPOS1.99 [21]. As can be seen, none of these hadronic 6 The analysis presented here is based on 4:7 10 inelastic interaction models which are used to simulate air showers · 1 events collected with pion beams at 158 and 350 GeVc− on can reproduce that data and especially SIBYLL2.1 predicts a thin carbon target. We present the production cross-section a too steep spectrum at high transverse momenta. The and momentum spectra of produced charged hadrons [13]. underestimation of charged hadron production at large The production cross-section in p−+C interactions was transverse momenta is present at all momenta for EPOS1.99 determined in a similar manner as described in Ref. [14]. and SIBYLL2.1. Of all the models studied QGSJETII-03 The experimental interaction cross-section is corrected for describes our data best with only a small deficit of tracks residual contributions from elastic and quasi-elastic scat- with high pT at large particle momentum but slightly too tering as well as for the inelastic contribution to which the many particles at low traverse momenta. Comparisons with NA61/SHINE interaction trigger is not sensitive. The uncer- the latest models will be shown at the conference. tainties of the measurement are currently dominated by the A shortcoming of the present analysis is the model de- model-dependence of this correction. Preliminary values pendent correction of the charged hadron spectra for lep- : : are sprod = 172 2(stat ) 4(syst.) and 178 2(stat ) ton contamination (almost entirely e±). The contamination ± ± 1 ± ± 1 1 4(syst.) at 158 and 350 GeVc− respectively [15]. This exceeds 20 % at plab < 10GeVc− and pT < 0:1GeVc− measurement is compatible with previous results [16,17] as indicated in Fig. 4 and data in this range are not shown and already gives the most precise value of the production because of the associated large systematic uncertainty. 1 cross section at around 160 GeVc− . Currently work is ongoing to use the measured en- The momentum spectra of charged hadrons produced ergy loss along the tracks in the TPCs to identify the in these interactions are presented in Fig.
Recommended publications
  • 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.
    [Show full text]
  • 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 .
    [Show full text]
  • 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.
    [Show full text]
  • 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,
    [Show full text]
  • US-NA61 Collaboration
    Hadron Production Measurements for Fermilab Neutrino Beams US participation in the NA61/SHINE experiment at CERN Letter of Intent May 2, 2012 Abstract This is a Letter of Intent to develop a limited-scope collaboration with the NA61/SHINE experiment at CERN to exploit its unique capabilities for particle production measurements. This effort would allow the US group to collect dedicated and optimized high-precision hadron production data needed for improved neutrino beams modeling nec- essary for ongoing and future experiments at Fermilab. The ultimate goal of this effort is to expose thin targets and replicas of targets used at Fermilab to the NA61 hadron beam to accumulate a suitably large sample of events to provide a data set which would be essential for future neutrino beams. An initial phase of this program, to be supported by existing funds, will be a two- day pilot run during the start-up of the 2012 run of NA61/SHINE. The pilot run will use a 120 GeV/c proton beam on a thin graphite target. It could provide valuable data for the MINERvA experiment, and would allow the US group to gain better practical under- standing of the capabilities of the NA61/SHINE experiment so that a broader collaborative program can be fully developed for later years. We envision this program to serve many future accelerator-based neutrino experiments at Fermilab and elsewhere. 1 The US NA61 Collaboration S. R. Johnson, A. Marino, E. D. Zimmerman University of Colorado, Boulder, Colorado 80302, USA D. Harris, A. Marchionni, D. Schmitz∗ Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA E.
    [Show full text]
  • Fixed-Target Hadron Production Experiments
    EPJ Web of Conferences 99, 02002 (2015) DOI: 10.1051/epjconf/20159902002 c Owned by the authors, published by EDP Sciences, 2015 Fixed-target hadron production experiments Boris A. Popov1,2,a 1 Laboratoire de Physique Nucleaire´ et de Hautes Energies, 4 place Jussieu, 75005 Paris, France 2 Joint Institute for Nuclear Research, Joliot-Curie 6, 141980 Dubna, Russia Abstract. Results from fixed-target hadroproduction experiments (HARP, MIPP, NA49 and NA61/SHINE) as well as their implications for cosmic ray and neutrino physics are reviewed. HARP measurements have been used for predictions of neutrino beams in K2K and MiniBooNE/SciBooNE experiments and are also being used to improve predictions of the muon yields in EAS and of the atmospheric neutrino fluxes as well as to help in the optimization of neutrino factory and super-beam designs. Recent measurements released by the NA61/SHINE experiment are of significant importance for a precise prediction of the J-PARC neutrino beam used for the T2K experiment and for interpretation of EAS data. These hadroproduction experiments provide also a large amount of input for validation and tuning of hadron production models in Monte-Carlo generators. 1. Introduction in order to illustrate some common features of modern hadron production experiments. The interpretation of extensive air shower (EAS) data – as for instance recorded by the Pierre Auger Observatory [1], To provide a large angular and momentum coverage KASCADE [2] or IceTop [3] – relies to a large extent on of the produced charged particles, the HARP experiment the correct modeling of hadron-air interactions that occur makes use of a large-acceptance spectrometer consisting during the shower development.
    [Show full text]
  • Particle and High-Energy Heavy-Ion Physics
    PARTICLE AND HIGH-ENERGY HEAVY-ION PHYSICS The Standard Model of the weak, electromagnetic and strong interactions is one of the most successful theoretical schemes ever developed in particle physics. The Standard Model explains to a high accuracy almost all relevant experimental observations. Nevertheless, it is not a fundamental theory, but a low-energy limit of some underlying theory which probably originates from the very high-energy scales like the Planck scale (of the order of 1019 GeV). There are some experimental results which can be treated as arguments for new physics beyond the Standard Model: The neutrino oscillations and perhaps neutrinoless nuclear double-beta decay data show that neutrinos have mass, neutrinos have mixing, neutrino properties are a mystery; There is missing mass in the Universe and there is acceleration of the Universe (dark matter and dark energy); LEP and Tevatron experiments have given strong indications to new physics at the TeV scale; There are too many external parameters and unsolved problems in the Standard Model; in particular, the gravity is not included, the electroweak symmetry breaking is not clear, there are hierarchy problems (Higgs mass diverges), etc. The main problems beyond the Standard Model very generally and very shortly can be grouped into three large classes with labels of Mass, Unification and Flavor. In more details they can be cast into the following basic questions: What is the origin of the particle masses, are they indeed due to the Higgs boson? What is the nature of
    [Show full text]
  • Curriculum Vitae
    Curriculum Vitae Alain BLONDEL Born 26 march1953 in Neuilly (92000 FRANCE), French citizen Personal address: 590 rte d'Ornex, 01280 Prévessin, France. Tel. +33 (0)4 50 40 46 51 Prefessional address: Université de Genève Département de Physique Nucléaire et Corpusculaire Quai Ernest-Ansermet 24 CH-1205 Genève 4 Tel. [41](22) 379 6227 [email protected] University grades and prizes : Engineer Ecole Polytechnique Paris (X1972) DEA in Nuclear Physics, University of Orsay (1975) 3d cycle Thesis, University of Orsay (1976) PhD in physics University of Orsay (1979) Bronze Medal CNRS (1979) (given yearly to the best PhD thesis in Particle/Nuclear physics) Prize of the Thibaud Foundation, Académie des Sciences, Arts et Belles Lettres de Lyon (1991) Silver Medal CNRS (1995) (given yearly for the best achievement in the field) Paul Langevin Prize from the French Academy of Sciences (1996) Manne Siegbahn Medal from the Royal Academy of Science in Sweden (1997) Prize from the foundation Jean Ricard by the French Physical Society (2004) (given yearly for best achievement in Physics) Professional curriculum : 1975 Stagiaire Ecole Polytechnique (Palaiseau, France) (PhD student grant) 1977 Attaché de Recherche au CNRS (Permanent position as junior researcher) 1980 Chargé de Recherche au CNRS (Permanent position as senior researcher) 1983-1985 Boursier CERN (CERN fellow) 1985-1989 Membre du Personnel CERN (CERN staff) 1989 → Directeur de Recherches au CNRS (Director of research group) 1991 → 2000 Maître de Conférences à l'Ecole Polytechnique (Junior professor) 1995 Attaché scientifique CERN (CERN scientific associate) 2000 Professeur ordinaire à l'Université de Genève (Full professor) Scientific activities • Began research in 1974 in the Gargamelle neutrino experiment with the study of background to the Neutral Current search.
    [Show full text]
  • Organisation Europeenne Pour La Recherche Nucleaire Larecherche Pour Europeenne Organisation
    DRAFT CERN/DG/Research Board 2012-425 Minutes-198 12 January 2012 ORGANISATION EUROPEENNE POUR LA RECHERCHE NUCLEAIRE CERN EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH _______________________________________________________________ CERN RESEARCH BOARD MINUTES OF THE 198th MEETING OF THE RESEARCH BOARD HELD ON WEDNESDAY 30 NOVEMBER 2011 Present I. Antoniadis, S. Bertolucci, P. Bloch, H. Breuker, P. Butler, P. Collier, E. Elsen, M. Ferro-Luzzi, R. Forty (Secretary), R. Heuer (Chair), P. Janot, M. Kowalska, S. Myers, E. Rondio, R. Saban, E. Tsesmelis, C. Vallée Apologies F. Hemmer Items 1. Procedure 2. Accelerator schedules for 2012 3. Report from the LHCC meeting of 21-22 September 2011 4. Report from the SPSC meeting of 25-26 October 2011 5. Report from the INTC meeting of 3-4 November 2011 CERN-DG-RB-2012-425 / M-198 09/03/2012 6. Any other business DRAFT CERN/DG/Research Board 2012-425 2 DRAFT CERN/DG/Research Board 2012-425 1. PROCEDURE 1.1 The minutes of the last meeting [1] were approved without modification. 2. ACCELERATOR SCHEDULES FOR 2012 2.1 P. Collier presented the accelerator schedules for 2012 [2]. This will be the final year of the current LHC running period, before the long shutdown for consolidation work to allow the machine to approach its design energy. For this year the physics running is planned to start in April, most likely with an energy of 4 TeV per beam, and 50 ns bunch spacing, although the final decision will be taken following discussion at the Chamonix workshop at the beginning of February. The physics run will end with a month dedicated to ions in November, most likely in p-A configuration.
    [Show full text]
  • Shine Xenlsprio:Pormevzoifraiu Msc
    Eötvös Loránd University Faculty of Informatics Department of Computer Algebra Shine - The new software framework for the NA61 Experiment MSc. Thesis CERN-THESIS-2012-432 Supervisor: Author: Dr. Ágnes Fülöp Roland Sipos External supervisor: Programtervez˝oInformatikus MSc. Dr. András László Budapest, 2012 Contents 1 Introduction 3 1.1 Experimental physics . .3 1.2 The CERN NA61/SHINE Experiment . .4 1.3 Thesis objectives . .7 2 Legacy software 9 2.1 Software environment . .9 2.2 Software architecture . 10 3 Software upgrade 20 3.1 Lessons learned from legacy . 20 3.2 Proposal . 23 4 The Shine Offline Framework 28 4.1 Core of the framework . 28 4.2 Modules . 41 4.3 SHOE . 46 4.4 Utilities . 50 4.5 Support . 56 5 Integration of legacy software 58 5.1 Porting technique . 58 5.2 Dependencies . 63 ii CONTENTS iii 5.3 Problems . 64 5.4 Validation . 67 6 Results 68 7 Acknowledgments 71 Chapter 1 Introduction This diploma thesis is a study on the CERN NA61 software upgrade, especially to follow the advancement of the Shine Offline Software Framework. In this chapter a description is found about the topics which are related to the development, including detector setup and software systems as parts of the experiment. The most important fields concerning the software upgrade are summarized, starting with experimental physics, which is discussed in section 1.1, followed by an overview of NA61/SHINE in section 1.2. 1.1 Experimental physics In the field of physics research we need to distinguish two main branch in the ap- proach how theories become justified.
    [Show full text]
  • Neutrino Oscillations with the MINOS, MINOS+, T2K, and Nova Experiments
    New J. Phys. 18 (2016) 015009 doi:10.1088/1367-2630/18/1/015009 PAPER Neutrino oscillations with the MINOS, MINOS+, T2K, and NOvA OPEN ACCESS experiments RECEIVED 4 August 2015 Tsuyoshi Nakaya1 and Robert K Plunkett2,3 REVISED 1 Kyoto University, Department of Physics, Kyoto 606-8502, Japan 23 November 2015 2 Fermi National Accelerator Laboratory, Batavia, IL 60510, USA ACCEPTED FOR PUBLICATION 3 Author to whom any correspondence should be addressed. 24 November 2015 PUBLISHED E-mail: [email protected] and [email protected] 18 January 2016 Keywords: neutrino, particle physics, oscillations Content from this work may be used under the terms of the Creative Abstract Commons Attribution 3.0 licence. This paper discusses recent results and near-term prospects of the long-baseline neutrino experiments Any further distribution of MINOS, MINOS+, T2K and NOvA. The non-zero value of the third neutrino mixing angle θ13 allows this work must maintain attribution to the experimental analysis in a manner which explicitly exhibits appearance and disappearance dependencies author(s) and the title of on additional parameters associated with mass-hierarchy, CP violation, and any non-maximal θ .These the work, journal citation 23 and DOI. Article funded current and near-future experiments begin the era of precision accelerator long-baseline measurements 3 by SCOAP . and lay the framework within which future experimental results will be interpreted. 1. Introduction to long-baseline accelerator experiments 1.1. Motivation and three-flavor model Beginning with the successful operation of the K2K experiment [1], the physics community has seen a profound expansion of our knowledge of the mixing of neutrinos, driven by long-baseline accelerator experiments [2–6], experiments studying atmospheric neutrinos [7–9], solar neutrinos [10], and, most recently, high-precision experiments with reactor neutrinos [11].
    [Show full text]
  • The T2K Off-Axis Near Detector: Recent Physics Results
    Available online at www.sciencedirect.com Nuclear and Particle Physics Proceedings 273–275 (2016) 2696–2698 www.elsevier.com/locate/nppp The T2K off-axis near detector: recent physics results Le¨ıla Haegel, on behalf of the T2K collaboration University of Geneva, Switzerland Abstract The T2K near detector complex, ND280, is located at the J-PARC accelerator facility in Tokai, Japan, 280 meters downstream from the target. This proceeding will summarize recent physics results from ND280. Keywords: long baseline experiment, neutrino cross sections, neutrino oscillations 1. Introduction: the T2K experiment The T2K experiment is a long baseline experiment probing neutrino oscillation parameters via νe appeare- ance and νμ disappeareance [1]. The neutrino flux is generated by the J-PARC super beam and sent towards Super-Kamiokande (SK), the 50 kton water Cherenkov far detector located 295 km away and 2.5◦ off the beam axis. The near detector complex is located 280 m from the beam target and contains the on-axis INGRID de- tector which measures the beam intensity and direction, while the off-axis ND280 detector is used to constrain the event rates on SK. ND280 is a complex of detectors which are used to constrain the off-axis flux and neutrino interaction model. Charged current (CC) interactions are measured ff in the tracker, which is made of two fine grained de- Figure 1: ND280, the T2K o -axis near detector. tectors (FGDs) placed between three time projection chambers (TPCs). The FGDs provide target mass and the old UA1 magnet to recontruct the particles momenta good vertex and tracking resolution, alongside a full car- from their curvatures in the magnetic field.
    [Show full text]