Details

Autor(en) / Beteiligte

• Agafonova, N.
• Ariga, A.
• Ariga, T.
• Badertscher, A.
• Dhahbi, A. Ben
• Bozza, C.
• Brunet, F.
• Brunetti, G.
• Buontempo, S.
• Chaussard, L.
• Chiarella, V.
• Chukanov, A.
• Consiglio, L.
• D’Ambrosio, N.
• De Lellis, G.
• del Amo Sanchez, P.
• Di Ferdinando, D.
• Di Marco, N.
• Dmitrievsky, S.
• Dracos, M.
• Dusini, S.
• Ebert, J.
• Ereditato, A.
• Ferber, T.
• Fini, R. A.
• Garfagnini, A.
• Giacomelli, G.
• Goellnitz, C.
• Goldberg, J.
• Grella, G.
• Guler, A. M.
• Gustavino, C.
• Hagner, C.
• Hierholzer, M.
• Hosseini, B.
• Ishida, H.
• Ishiguro, K.
• Juget, F.
• Kamiscioglu, C.
• Kawada, J.
• Kim, J. H.
• Kitagawa, N.
• Kodama, K.
• Komatsu, M.
• Kreslo, I.
• Lauria, A.
• Longhin, A.
• Loverre, P.
• Malgin, A.
• Mancini-Terracciano, C.
• Mandrioli, G.
• Meisel, F. W.
• Meregaglia, A.
• Migliozzi, P.
• Morishima, K.
• Muciaccia, M. T.
• Nakamura, M.
• Nakano, T.
• Nakatsuka, Y.
• Naumov, D.
• Niwa, K.
• Ogawa, S.
• Olchevsky, A.
• Omura, T.
• Paoloni, A.
• Park, B. D.
• Patrizii, L.
• Pennacchio, E.
• Pessard, H.
• Polukhina, N.
• Rescigno, R.
• Roganova, T.
• Rokujo, H.
• Rubbia, A.
• Russo, A.
• Sato, O.
• Sato, Y.
• Schmidt-Parzefall, W.
• Shibuya, H.
• Shiraishi, T.
• Shoziyoev, G.
• Sioli, M.
• Sirignano, C.
• Sirri, G.
• Stanco, L.
• Starkov, N.
• Stellacci, S. M.
• Stipcevic, M.
• Strauss, T.
• Strolin, P.
• Takahashi, S.
• Terranova, F.
• Tioukov, V.
• Tolun, P.
• Vilain, P.
• Votano, L.
• Yoon, C. S.
• Yoshida, J.
• Zaitsev, Y.
• Zemskova, S.

Titel

Search for ν μ → ν e oscillations with the OPERA experiment in the CNGS beam

Ist Teil von

• The journal of high energy physics, 2013-07, Vol.2013 (7), Article 4

Erscheinungsjahr

2013

Quelle

Springer Journals

Beschreibungen/Notizen

• A bstract A first result of the search for ν μ → ν e oscillations in the OPERA experiment, located at the Gran Sasso Underground Laboratory, is presented. The experiment looked for the appearance of ν 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 θ new and $ \varDelta m_{\mathrm{new}}^2 $ suggested by the LSND and MiniBooNE experiments. For large $ \varDelta m_{\mathrm{new}}^2 $ values ( > 0.1 eV 2 ), the OPERA 90% C.L. upper limit on sin 2 (2 θ new ) based on a Bayesian statistical method reaches the value 7 . 2 × 10 −3 .