Search for anomalies in the [nu]^sub e^ appearance from a [nu]^sub [mu]^ beam

We report an updated result from the ICARUS experiment on the search for ν ^sub [mu]^[arrow right]ν ^sub e^ anomalies with the CNGS beam, produced at CERN with an average energy of 20 GeV and traveling 730 km to the Gran Sasso Laboratory. The present analysis is based on a total sample of 1995 event...

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Veröffentlicht in:The European physical journal. C, Particles and fields Particles and fields, 2013-10, Vol.73 (10), p.1
Hauptverfasser: Antonello, M, Baibussinov, B, Benetti, P, Boffelli, F, Bubak, A, Calligarich, E, Canci, N, Centro, S, Cesana, A, Cielik, K, Cline, D B, Cocco, A G, Dabrowska, A, Dequal, D, Dermenev, A, Dolfini, R, Falcone, A, Farnese, C, Fava, A, Ferrari, A, Fiorillo, G, Gibin, D, Gninenko, S, Guglielmi, A, Haranczyk, M, Holeczek, J, Kirsanow, M, Kisiel, J, Kochanek, I, Lagoda, J, Mania, S, Menegolli, A, Meng, G, Montanari, C, Otwinowski, S, Picchi, P, Pietropaolo, F, Plonski, P, Rappoldi, A, Raselli, G L, Rossella, M, Rubbia, C, Sala, P, Scaramelli, A, Segreto, E, Sergiampietri, F, Stefan, D, Sulej, R, Szarska, M, Terrani, M, Torti, M, Varanini, F, Ventura, S, Vignoli, C, Wang, H G, Yang, X, Zalewska, A, Zani, A, Zaremba, K
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Sprache:eng
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Zusammenfassung:We report an updated result from the ICARUS experiment on the search for ν ^sub [mu]^[arrow right]ν ^sub e^ anomalies with the CNGS beam, produced at CERN with an average energy of 20 GeV and traveling 730 km to the Gran Sasso Laboratory. The present analysis is based on a total sample of 1995 events of CNGS neutrino interactions, which corresponds to an almost doubled sample with respect to the previously published result. Four clear ν ^sub e^ events have been visually identified over the full sample, compared with an expectation of 6.4±0.9 events from conventional sources. The result is compatible with the absence of additional anomalous contributions. At 90 % and 99 % confidence levels, the limits to possible oscillated events are 3.7 and 8.3 respectively. The corresponding limit to oscillation probability becomes consequently 3.4×10^sup -3^ and 7.6×10^sup -3^, respectively. The present result confirms, with an improved sensitivity, the early result already published by the ICARUS Collaboration.
ISSN:1434-6044
1434-6052
DOI:10.1140/epjc/s10052-013-2599-z