First events from the CNGS neutrino beam detected in the OPERA experiment

Autor: R Acquafredda, N Agafonova, M Ambrosio, A Anokhina, S Aoki, A Ariga, L Arrabito, D Autiero, A Badertscher, E Baussan, A Bergnoli, F Bersani Greggio, M Besnier, M Beyer, S Bondil-Blin, K Borer, J Boucrot, V Boyarkin, C Bozza, R Brugnera, S Buontempo, Y Caffari, J E Campagne, B Carlus, E Carrara, A Cazes, L Chaussard, M Chernyavsky, V Chiarella, N Chon-Sen, A Chukanov, R Ciesielski, L Consiglio, M Cozzi, F Dal Corso, N D'Ambrosio, J Damet, G De Lellis, Y Déclais, T Descombes, M De Serio, F Di Capua, D Di Ferdinando, A Di Giovanni, N Di Marco, C Di Troia, S Dmitrievski, M Dracos, D Duchesneau, B Dulach, S Dusini, J Ebert, R Enikeev, A Ereditato, L S Esposito, C Fanin, J Favier, G Felici, T Ferber, L Fournier, A Franceschi, D Frekers, T Fukuda, C Fukushima, V I Galkin, V A Galkin, R Gallet, A Garfagnini, G Gaudiot, G Giacomelli, O Giarmana, M Giorgini, L Girard, C Girerd, C Goellnitz, J Goldberg, Y Gornoushkin, G Grella, F Grianti, C Guerin, M Guler, C Gustavino, C Hagner, T Hamane, T Hara, M Hauger, M Hess, K Hoshino, M Ieva, M Incurvati, K Jakovcic, J Janicsko Csathy, B Janutta, C Jollet, F Juget, M Kazuyama, S H Kim, M Kimura, J Knuesel, K Kodama, D Kolev, M Komatsu, U Kose, A Krasnoperov, I Kreslo, Z Krumstein, I Laktineh, C de La Taille, T Le Flour, S Lieunard, A Ljubicic, A Longhin, A Malgin, K Manai, G Mandrioli, U Mantello, A Marotta, J Marteau, G Martin-Chassard, V Matveev, M Messina, L Meyer, S Micanovic, P Migliozzi, S Miyamoto, P Monacelli, I Monteiro, K Morishima, U Moser, M T Muciaccia, P Mugnier, N Naganawa, M Nakamura, T Nakano, T Napolitano, M Natsume, K Niwa, Y Nonoyama, A Nozdrin, S Ogawa, A Olchevski, D Orlandi, D Ossetski, A Paoloni, B D Park, I G Park, A Pastore, L Patrizii, L Pellegrino, H Pessard, V Pilipenko, C Pistillo, N Polukhina, M Pozzato, K Pretzl, P Publichenko, L Raux, J P Repellin, T Roganova, G Romano, G Rosa, A Rubbia, V Ryasny, O Ryazhskaya, D Ryzhikov, A Sadovski, C Sanelli, O Sato, Y Sato, V Saveliev, N Savvinov, G Sazhina, A Schembri, W Schmidt Parzefall, H Schroeder, H U Schütz, L Scotto Lavina, J Sewing, H Shibuya, S Simone, M Sioli, C Sirignano, G Sirri, J S Song, R Spaeti, M Spinetti, L Stanco, N Starkov, M Stipcevic, P Strolin, V Sugonyaev, S Takahashi, V Tereschenko, F Terranova, I Tezuka, V Tioukov, I Tikhomirov, P Tolun, T Toshito, V Tsarev, R Tsenov, U Ugolino, N Ushida, G Van Beek, V Verguilov, P Vilain, L Votano, J L Vuilleumier, T Waelchli, R Waldi, M Weber, G Wilquet, B Wonsak, R Wurth, J Wurtz, V Yakushev, C S Yoon, Y Zaitsev, I Zamboni, R Zimmermann

Publikováno v: New Journal of Physics
New Journal of Physics, Institute of Physics: Open Access Journals, 2006, 8, pp.303. ⟨10.1088/1367-2630/8/12/303⟩

The OPERA neutrino detector at the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in appearance mode, through the study of nu_mu to nu_tau oscillations. The apparatus consists of a lead/e

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::34e6747900d0f1a80abf68b16bc495b3
http://hdl.handle.net/10281/26965