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Study of neutrino interactions with the electronic detectors of the OPERA experiment

  • N. Agafonova
  • , A. Aleksandrov
  • , O. Altinok
  • , A. Anokhina
  • , S. Aoki
  • , A. Ariga
  • , T. Ariga
  • , D. Autiero
  • , A. Badertscher
  • , A. Bagulya
  • , A. Bendhahbi
  • , A. Bertolin
  • , C. Bozza
  • , T. Brugière
  • , R. Brugnera
  • , F. Brunet
  • , G. Brunetti
  • , S. Buontempo
  • , A. Cazes
  • , L. Chaussard
  • M. Chernyavskiy, V. Chiarella, A. Chukanov, N. D'Ambrosio, F. Dal Corso, G. De Lellis, P. Del Amo Sanchez, Y. Déclais, M. De Serio, F. Di Capua, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, O. Egorov, R. Enikeev, A. Ereditato, L. S. Esposito, J. Favier, T. Ferber, R. A. Fini, D. Frekers, T. Fukuda, A. Garfagnini, G. Giacomelli, M. Giorgini, C. Göllnitz, J. Goldberg, D. Golubkov, L. Goncharova, Y. Gornushkin, G. Grella, F. Grianti, A. M. Guler, C. Gustavino, C. Hagner, K. Hamada, T. Hara, M. Hierholzer, A. Hollnagel, K. Hoshino, M. Ieva, H. Ishida, K. Jakovcic, C. Jollet, F. Juget, M. Kamiscioglu, K. Kazuyama, S. H. Kim, M. Kimura, N. Kitagawa, B. Klicek, J. Knuesel, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, H. Kubota, C. Lazzaro, J. Lenkeit, I. Lippi, A. Ljubicic, A. Longhin, P. Loverre, G. Lutter, A. Malgin, G. Mandrioli, K. Mannai, J. Marteau, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, F. Meisel, A. Meregaglia, P. Migliozzi, S. Mikado, S. Miyamoto, P. Monacelli, K. Morishima, U. Moser, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, D. Naumov, V. Nikitina, K. Niwa, Y. Nonoyama, S. Ogawa, N. Okateva, A. Olchevskiy, M. Paniccia, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, K. Pretzl, V. Pilipenko, C. Pistillo, N. Polukhina, M. Pozzato, F. Pupilli, R. Rescigno, T. Roganova, H. Rokujo, G. Romano, G. Rosa, I. Rostovtseva, A. Rubbia, A. Russo, V. Ryasny, O. Ryazhskaya, O. Sato, Y. Sato, A. Schembri, W. Schmidt-Parzefall, H. Schroeder, L. Scotto Lavina, A. Sheshukov, H. Shibuya, G. Shoziyeov, S. Simone, M. Sioli, C. Sirignano, G. Sirri, J. S. Song, M. Spinetti, L. Stanco, N. Starkov, M. Stipcevic, T. Strauss, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, I. Tezuka, V. Tioukov, P. Tolun, A. Trabelsi, T. Tran, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, V. Yakushev, C. S. Yoon, T. Yoshioka, J. Yoshida, Y. Zaitsev, S. Zemskova, A. Zghiche, R. Zimmermann
  • Institute for Nuclear Research of the Russian Academy of Sciences
  • INFN Sezione di Napoli
  • Middle East Technical University (METU)
  • SINP MSU-Skobeltsyn Institute of Nuclear Physics
  • Moscow State University
  • Kobe University
  • Centre for Research and Education in Fundamental Physics
  • University of Bern
  • IGFL, Université de Lyon, Université Lyon 1
  • ETH Zurich
  • ETH Zurich
  • P.N. Lebedev Physical Institute of the Russian Academy of Sciences
  • Unité de Physique Nucléaire et des Hautes Energies (UPNHE)
  • INFN
  • Sezione di Roma
  • Dipartimento di Fisica
  • University of Padova
  • Université Savoie Mont Blanc
  • Dipartimento di Fisica
  • INFN Sezione di Bologna
  • LNF-INFN
  • Joint Institute for Nuclear Research, Dubna
  • Laboratori Nazionali del Gran Sasso
  • Dipartimento di Scienze Fisiche
  • INFN Sezione di Bari
  • Université de Strasbourg
  • Universität Hamburg
  • Institute for Theoretical and Experimental Physics
  • University of Münster
  • Nagoya University
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Department of Physics
  • Technion - Israel Institute of Technology
  • University of Urbino Carlo Bo
  • Toho University
  • Ruđer Bošković Institute
  • Gyeongsang National University
  • Pusan National University
  • Aichi University of Education
  • Dipartimento di Fisica
  • Asan Medical Center
  • Utsunomiya University
  • Fachbereich Physik
  • Universität Rostock
  • SUBATECH
  • Université Libre de Bruxelles

Research output: Contribution to journal › Article › peer-review

57 Citations (Scopus)

Abstract

The OPERA experiment is based on a hybrid technology combining electronic detectors (EDs) and nuclear emulsions. OPERA collected muon-neutrino interactions during the 2008 and 2009 physics runs of the CNGS neutrino beam, produced at CERN with an energy range of about 5-35 GeV. A total of 5.3 × 1019 protons on target equivalent luminosity have been analysed with the OPERA EDs: scintillator strips target trackers and magnetic muon spectrometers equipped with resistive plate gas chambers and drift tubes, allowing a detailed reconstruction of muon-neutrino interactions. Charged current (CC) and neutral current (NC) interactions are identified, using the measurements in the EDs, and the NC/CC ratio is computed. The momentum distribution and the charge of the muon tracks produced in CC interactions are analysed. Calorimetric measurements of the visible energy are performed for both the CC and NC samples. For CC events, the Bjorken-y distribution and the hadronic shower profile are computed. The results are compared with a detailed Monte Carlo simulation of the response of EDs.

Original languageEnglish
Article number053051
JournalNew Journal of Physics
Volume13
DOIs
Publication statusPublished - 1 May 2011
Externally publishedYes

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