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N. Agafonova,A. Anokhina,S. Aoki,A. Ariga,T. Ariga,L. Arrabito,D. Autiero,A. Badertscher, A. Bagulya,F. Bersani Greggio,A. Bertolin, M. Besnier,D. Bick, V. Boyarkin,C. Bozza, T. Brugière,R. Brugnera,G. Brunetti,S. Buontempo, E. Carrara, A. Cazes,L. Chaussard, M. Chernyavsky,V. Chiarella, N. Chon-Sen,A. Chukanov,M. Cozzi, G. D’Amato,F. Dal Corso,N. D’Ambrosio,G. De Lellis, Y. Déclais,M. De Serio,F. Di Capua,D. Di Ferdinando,A. Di Giovanni,N. Di Marco,C. Di Troia, S. Dmitrievski, A. Dominjon,M. Dracos,D. Duchesneau,S. Dusini, J. Ebert, O. Egorov, R. Enikeev,A. Ereditato,L. S. Esposito, J. Favier,G. Felici,T. Ferber, R. Fini,D. Frekers,T. Fukuda, C. Fukushima, V. I. Galkin,V. A. Galkin,A. Garfagnini,G. Giacomelli,M. Giorgini, C. Goellnitz, T. Goeltzenlichter,J. Goldberg,D. Golubkov,Y. Gornushkin,G. Grella, F. Grianti, M. Guler,C. Gustavino,C. Hagner,T. Hara,M. Hierholzer,K. Hoshino,M. Ieva,K. Jakovcic, B. Janutta,C. Jollet,F. Juget, M. Kazuyama,S. H. Kim,M. Kimura, B. Klicek, J. Knuesel,K. Kodama,D. Kolev,M. Komatsu,A. Krasnoperov, I. Kreslo,Z. Krumstein, V. A. Kuznetsov, C. Lazzaro, J. Lenkeit,A. Ljubicic,A. Longhin,G. Lutter, A. Malgin, K. Manai,G. Mandrioli,A. Marotta,J. Marteau,V. Matveev,N. Mauri, F. Meisel,A. Meregaglia,P. Migliozzi,P. Monacelli,M. T. Muciaccia,M. Nakamura,T. Nakano, V. Nikitina,K. Niwa, Y. Nonoyama, A. Nozdrin,S. Ogawa, A. Olchevski, G. Orlova, V. Osedlo, D. Ossetski, 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, R. Rescigno,T. Roganova,I. Rostovtseva,A. Russo, A. Schembri,L. Scotto Lavina,H. Shibuya,S. Simone,M. Sioli,L. Stanco,M. Stipcevic, V. Sugonyaev,S. Takahashi, V. Tereschenko,V. Tioukov, S. Tufanli,V. Verguilov,P. Vilain, M. Vladimirov,L. Votano,J. L. Vuilleumier,G. Wilquet, B. Wonsak, V. Yakushev,C. S. Yoon, Y. Zaitsev,A. Zghiche,R. Zimmermann

semanticscholar(2009)

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摘要
The OPERA neutrino detector in the underground Gran Sasso L ab ratory (LNGS) was designed to perform the first detection of neutrino oscil lations in appearance mode through the
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