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  • Search for [nu]^sub [mu]^ [arrow right] [nu]^sub e^ oscillations with the OPERA experiment in the CNGS beam
    Aleksandrov, A; Anokhina, A; Ariga, A; Ariga, T; Autiero, D; Dhahbi, A Ben; Brugnera, R; Brunet, F; Brunetti, G; Chaussard, L; Chiarella, V; Chukanov, A; Consiglio, L; D'ambrosio, N; Del Amo Sanchez, P; Di Ferdinando, D; Di Marco, N; Dmitrievsky, S; Dracos, M; Dusini, S; Ebert, J; Ereditato, A; Fukuda, T; Garfagnini, A; Giacomelli, G; Gornushkin, Y; Grella, G; Grianti, F; Gustavino, C; Hagner, C; Hamada, K; Hara, T; Hierholzer, M; Hollnagel, A; Hosseini, B; Ishida, H; Ishiguro, K; Jakovcic, K; Jollet, C; Juget, F; Kamiscioglu, C; Kamiscioglu, M; Kawada, J; Kimura, M; Klicek, B; Kodama, K; Kose, U; Kreslo, I; Lauria, A; Lenkeit, J; Ljubicic, A; Longhin, A; Malgin, A; Marteau, J; Mauri, N; Medinaceli, E; Meisel, F W; Meregaglia, A; Migliozzi, P; Mikado, S; Montesi, M C; Morishima, K; Nakano, T; Nakatsuka, Y; Niwa, K; Okateva, N; Olchevsky, A; Omura, T; Ozaki, K; Park, I G; Patrizii, L; Pessard, H; Polukhina, N; Pozzato, M; Pretzl, K; Rescigno, R; Rokujo, H; Rostovtseva, I; Rubbia, A; Russo, A; Ryazhskaya, O; Sato, O; Sato, Y; Schchedrina, T; Schembri, A; Sheshukov, A; Shibuya, H; Shiraishi, T; Sioli, M; Spinetti, M; Starkov, N; Stellacci, S M; Tenti, M; Terranova, F; Tufanli, S; Vuilleumier, J-l; Wilquet, G; Yoshida, J; Zaitsev, Y; Zemskova, S

    The journal of high energy physics, 07/2013, Letnik: 2013, Številka: 7
    Journal Article

    (ProQuest: ... denotes formulae and/or non-USASCII text omitted; see image) A first result of the search for nu ^sub mu^ arrow right nu ^sub e^ oscillations in the OPERA experiment, located at the Gran Sasso Underground Laboratory, is presented. The experiment looked for the appearance of nu ^sub e^ in the CNGS neutrino beam using the data collected in 2008 and 2009. Data are compatible with the non-oscillation hypothesis in the three-flavour mixing model. A further analysis of the same data constrains the non-standard oscillation parameters theta ^sub new^ and ... suggested by the LSND and MiniBooNE experiments. For large ... values (>0.1 eV^sup 2^), the OPERA 90% C.L. upper limit on sin^sup 2^(2theta ^sub new^) based on a Bayesian statistical method reaches the value 7.2 × 10^sup -3^.

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