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Observation of a first ντ candidate event in the OPERA experiment in the CNGS beam

  • N. Agafonova
  • , A. Aleksandrov
  • , O. Altinok
  • , M. Ambrosio
  • , A. Anokhina
  • , S. Aoki
  • , A. Ariga
  • , T. Ariga
  • , D. Autiero
  • , A. Badertscher
  • , A. Bagulya
  • , A. Bendhabi
  • , A. Bertolin
  • , M. Besnier
  • , D. Bick
  • , V. Boyarkin
  • , C. Bozza
  • , T. Brugière
  • , R. Brugnera
  • , F. Brunet
  • G. Brunetti, S. Buontempo, A. Cazes, L. Chaussard, M. Chernyavsky, V. Chiarella, N. Chon-Sen, A. Chukanov, R. Ciesielski, F. Dal Corso, N. D'Ambrosio, Y. Declais, P. del Amo Sanchez, G. De Lellis, M. De Serio, F. Di Capua, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, A. Di Giovanni, S. Dmitrievsky, 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, V. Galkin, A. Garfagnini, G. Giacomelli, M. Giorgini, J. Goldberg, C. Göllnitz, D. Golubkov, L. Goncharova, Y. Gornushkin, G. Grella, F. Grianti, A. M. Guler, C. Gustavino, C. Hagner, K. Hamada, T. Hara, M. Hierholzer, K. Hoshino, M. Ieva, H. Ishida, K. Ishiguro, K. Jakovcic, C. Jollet, F. Juget, M. Kamiscioglu, J. Kawada, M. 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, G. Lutter, A. Malgin, G. Mandrioli, K. Mannai, A. Marotta, 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, A. Olchevsky, T. Omura, G. Orlova, V. Osedlo, M. Paniccia, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, V. Pilipenko, C. Pistillo, N. Polukhina, M. Pozzato, K. Pretzl, P. Publichenko, F. Pupilli, J. P. Repellin, R. Rescigno, T. Roganova, H. Rokujo, G. Romano, G. Rosa, I. Rostovtseva, A. Rubbia, A. Russo, V. Ryasny, O. Ryazhskaya, Y. Sakatani, O. Sato, Y. Sato, A. Schembri, W. Schmidt-Parzefall, H. Schroeder, L. Scotto Lavina, A. Sheshukov, H. Shibuya, S. Simone, M. Sioli, C. Sirignano, G. Sirri, J. S. Song, M. Spinetti, L. Stanco, N. Starkov, 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
  • P.N. Lebedev Physical Institute of the Russian Academy of Sciences
  • Middle East Technical University (METU)
  • INFN Sezione di Napoli
  • Moscow State University
  • Kobe University
  • University of Bern
  • IGFL, Université de Lyon, Université Lyon 1
  • ETH Zurich
  • Unité de Physique Nucléaire et des Hautes Energies (UPNHE)
  • INFN
  • Université Savoie Mont Blanc
  • Universität Hamburg
  • University of Salerno
  • University of Padova
  • University of Bologna
  • LNF-INFN
  • Université de Strasbourg
  • Joint Institute for Nuclear Research, Dubna
  • Laboratori Nazionali del Gran Sasso
  • University of Naples Federico II
  • INFN Sezione di Bari
  • INFN Sezione di Bologna
  • Università Dell'Aquila
  • Institute for Theoretical and Experimental Physics
  • University of Münster
  • Nagoya University
  • Technion - Israel Institute of Technology
  • University of Urbino Carlo Bo
  • Toho University
  • Ruđer Bošković Institute
  • Gyeongsang National University
  • Aichi University of Education
  • Università degli studi di Bari Aldo Moro
  • Dipartimento di Fisica
  • Utsunomiya University
  • Universität Rostock
  • Université Libre de Bruxelles

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

242 Citations (Scopus)

Résumé

The OPERA neutrino detector in the underground Gran Sasso Laboratory (LNGS) has been designed to perform the first detection of neutrino oscillations in direct appearance mode through the study of the νμ→ντ channel. The hybrid apparatus consists of an emulsion/lead target complemented by electronic detectors and it is placed in the high energy long-baseline CERN to LNGS beam (CNGS) 730 km away from the neutrino source. Runs with CNGS neutrinos were successfully carried out in 2008 and 2009. After a brief description of the beam, the experimental setup and the procedures used for the analysis of the neutrino events, we describe the topology and kinematics of a first candidate ?? charged-current event satisfying the kinematical selection criteria. The background calculations and their cross-check are explained in detail and the significance of the event is assessed.

langue originaleAnglais
Pages (de - à)138-145
Nombre de pages8
journalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume691
Numéro de publication3
Les DOIs
étatPublié - 1 juil. 2010
Modification externeOui

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