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Search for ν μ→ ν τ oscillation with the OPERA experiment in the CNGS beam

  • N. Agafonova
  • , A. Aleksandrov
  • , O. Altinok
  • , A. Anokhina
  • , S. Aoki
  • , A. Ariga
  • , T. Ariga
  • , D. Autiero
  • , A. Badertscher
  • , A. Bagulya
  • , A. Ben Dhahbi
  • , 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, Y. Déclais, P. Del Amo Sanchez, G. De Lellis, 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. Ishiguro, K. Jakovcic, C. Jollet, F. Juget, M. Kamiscioglu, S. H. Kim, M. Kimura, N. Kitagawa, B. Klicek, J. Knuesel, K. Kodama, K. Kogiso, M. Komatsu, U. Kose, I. Kreslo, 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, Y. Nakatsuka, D. Naumov, V. Nikitina, K. Niwa, Y. Nonoyama, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, O. Palamara, M. Paniccia, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, C. Pistillo, N. Polukhina, M. Pozzato, K. Pretzl, 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, L. Scotto Lavina, A. Sheshukov, H. Shibuya, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, J. S. Song, M. Spinetti, L. Stanco, N. Starkov, M. Stellacci, M. Stipcevic, T. Strauss, P. Strolin, K. Suzuki, 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, J. Yoshida, T. Yoshioka, Y. Zaitsev, S. Zemskova, A. Zghiche, R. Zimmermann
  • Institute for Nuclear Research of the Russian Academy of Sciences
  • INFN Sezione di Napoli
  • Université Libre de Bruxelles
  • Middle East Technical University (METU)
  • Moscow State University
  • Kobe University
  • University of Bern
  • IGFL, Université de Lyon, Université Lyon 1
  • ETH Zurich
  • P.N. Lebedev Physical Institute of the Russian Academy of Sciences
  • Unité de Physique Nucléaire et des Hautes Energies (UPNHE)
  • INFN
  • University of Salerno
  • University of Padova
  • Université Savoie Mont Blanc
  • University of Bologna
  • INFN Sezione di Bologna
  • LNF-INFN
  • Joint Institute for Nuclear Research, Dubna
  • Laboratori Nazionali del Gran Sasso
  • University of Naples Federico II
  • INFN Sezione di Bari
  • Université de Strasbourg
  • Universität Hamburg
  • Institute for Theoretical and Experimental Physics
  • University of Münster
  • Toho University
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Technion - Israel Institute of Technology
  • University of Urbino Carlo Bo
  • Pusan National University
  • Nagoya University
  • Ruđer Bošković Institute
  • Gyeongsang National University
  • Asan Medical Center
  • Aichi University of Education
  • Dipartimento di Fisica
  • Università Dell'Aquila
  • Università degli studi di Bari Aldo Moro
  • Utsunomiya University
  • SUBATECH
  • University of Milano-Bicocca

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

31 Citations (Scopus)

Résumé

The OPERA neutrino experiment in the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in direct appearance mode in the vμ→ v τ channel, the v τ signature being the identification of the τ -lepton created in its charged current interaction. The hybrid apparatus consists of a large mass emulsion film/lead target complemented by electronic detectors. Placed in the LNGS, it is exposed to the high-energy long-baseline CERN Neutrino beam to Gran Sasso (CNGS) 730 km away from the neutrino source. The observation of a first v τ candidate event was reported in 2010. In this paper, we discuss the result of the analysis of the data taken during the first two years of operation (2008-2009) underlining the major improvements brought to the analysis chain and to the Monte Carlo simulations. The statistical significance of the one event observed so far is then evaluated to 95%.

langue originaleAnglais
Numéro d'article33017
journalNew Journal of Physics
Volume14
Les DOIs
étatPublié - 1 mars 2012
Modification externeOui

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