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2081
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2082por Wu, Qun“…The NOMAD (Neutrino Oscillation MAgnetic Detector) experiment, using the SPS (Super Proton Syncrotron) neutrino beam (1 GeV < E [nu] < 200 GeV) at CERN (European Organization for Nuclear Research), has collected more than 1.7 million neutrino induced charged and neutral current (CC and NC) events. …”
Publicado 2006
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2083
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2084por Shapshak, Paul“…A bilateral approach, using neutrino and electromagnetic (EM) radiation technologies, can be used to simultaneously characterize star types that generally have exoplanets and exomoons. …”
Publicado 2023
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2085por Agafonova, N., Alexandrov, A., Anokhina, A., Aoki, S., Ariga, A., Ariga, T., Bertolin, A., Bozza, C., Brugnera, R., Buonaura, A., Buontempo, S., Chernyavskiy, M., Chukanov, A., Consiglio, L., D’Ambrosio, N., De Lellis, G., De Serio, M., del Amo Sanchez, P., Di Crescenzo, A., Di Ferdinando, D., Di Marco, N., Dmitrievsky, S., Dracos, M., Duchesneau, D., Dusini, S., Dzhatdoev, T., Ebert, J., Ereditato, A., Fini, R. A., Fornari, F., Fukuda, T., Galati, G., Garfagnini, A., Gentile, V., Goldberg, J., Gorbunov, S., Gornushkin, Y., Grella, G., Guler, A. M., Gustavino, C., Hagner, C., Hara, T., Hayakawa, T., Hollnagel, A., Ishiguro, K., Iuliano, A., Jakovčić, K., Jollet, C., Kamiscioglu, C., Kamiscioglu, M., Kim, S. H., Kitagawa, N., Kliček, B., Kodama, K., Komatsu, M., Kose, U., Kreslo, I., Laudisio, F., Lauria, A., Lavasa, A., Longhin, A., Loverre, P., Malgin, A., Mandrioli, G., Matsuo, T., Matveev, V., Mauri, N., Medinaceli, E., Meregaglia, A., Mikado, S., Miyanishi, M., Mizutani, F., Monacelli, P., Montesi, M. C., Morishima, K., Muciaccia, M. T., Naganawa, N., Naka, T., Nakamura, M., Nakano, T., Niwa, K., Ogawa, S., Okateva, N., Ozaki, K., Paoloni, A., Park, B. D., Pasqualini, L., Pastore, A., Patrizii, L., Pessard, H., Podgrudkov, D., Polukhina, N., Pozzato, M., Pupilli, F., Roda, M., Roganova, T., Rokujo, H., Rosa, G., Ryazhskaya, O., Sato, O., Shakirianova, I., Schembri, A., Shchedrina, T., Shibayama, E., Shibuya, H., Shiraishi, T., Šimko, T., Simone, S., Sirignano, C., Sirri, G., Sotnikov, A., Spinetti, M., Stanco, L., Starkov, N., Stellacci, S. M., Stipčević, M., Strolin, P., Takahashi, S., Tenti, M., Terranova, F., Tioukov, V., Tsanaktsidis, I., Tufanli, S., Ustyuzhanin, A., Vasina, S., Vidal García, M., Vilain, P., Voevodina, E., Votano, L., Vuilleumier, J. L., Wilquet, G., Yoon, C. S.“…The OPERA experiment was designed to discover the v(τ) appearance in a v(μ) beam, due to neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of a nuclear photographic emulsion/lead target with a mass of about 1.25 kt, complemented by electronic detectors. …”
Publicado 2021
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2086por Baussan, E., Dracos, M., Ekelof, T., Martinez, E.Fernandez, Ohman, H., Vassilopoulos, N.“…Results are presented of preliminary calculations of the sensitivity to neutrino CP violation and the mass hierarchy as a function of the neutrino baseline. …”
Publicado 2012
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2087
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2088“…We consider a general symmetric $(3\times 3)$ mass matrix for three generations of neutrinos. Imposing the constraints, from the atmospheric neutrino and solar neutrino anomalies as well as from the CHOOZ experiment, on the mass squared differences and on the mixing angles, we identify the ranges of allowed inputs for the 6 matrix elements. …”
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2089
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2090por Field, J H“…The definition of `lepton flavour eigenstates' introduced in a recent paper hep-ph/0302045 is in disagreement with the Standard Model prediction for the structure of the leptonic charged current and implies the absence of neutrino oscillations following pion decay, in contradiction to experimental data…”
Publicado 2003
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2091
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2092
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2093por Abe, T, Aihara, H, Andreopoulos, C, Ankowski, A, Badertscher, A, Battistoni, G, Blondel, A, Bouchez, J, Bross, A, Bueno, A, Camilleri, L, Campagne, J E, Cazes, A, Cervera-Villanueva, A, DeLellis, G, DiCapua, F, Ellis, M, Ereditato, A, Esposito, L S, Fukushima, C, Gschwendtner, E, Gómez-Cadenas, J J, Iwasaki, M, Kaneyuki, K, Karadzhov, Y, Kashikhin, V, Kawai, Y, Komatsu, M, Kozlovskaya, E, Kudenko, Y, Kusaka, A, Kyushima, H, Laing, A, Long, K, Longhin, A, Marchionni, A, Marotta, A, McGrew, C, Menary, S, Meregaglia, A, Mezzeto, M, Migliozzi, P, Mondal, N K, Montanari, C, Nakadaira, T, Nakamura, M, Nakumo, H, Nakayama, H, Nelson, J, Nowak, J, Ogawa, S, Peltoniemi, J, Pla-Dalmau, A, Ragazzi, S, Rubbia, A, Sanchez, F, Sarkamo, J, Sato, O, Selvi, M, Shibuya, H, Shozawa, M, Sobczyk, J, Soler, F J P, Strolin, P, Suyama, M, Tanaka, M, Terranova, F, Tsenov, R, Uchida, Y, Weber, A, Zlobin, AEnlace del recurso
Publicado 2009
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2094por Steele, D M“…A search is performed for single, isolated photons from X 0 decay, where X 0 represents either a neutrino excited state or an unknown, neutral, massive particle produced in a rare pi+ decay along the neutrino beam line as hypothesized by the KARMEN Collaboration[1] as a possible solution to their anomalous time spectra for pi+ -> u+ + vu. …”
Publicado 1996
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2095
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2096
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2097“…Results in the alternative case of quasi-degenerate in mass heavy Majorana neutrinos, are also derived. The minimal supersymmetric extension of the standard theory with right-handed Majorana neutrinos and see-saw mechanism of neutrino mass generation is discussed as well. …”
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2098
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2099
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2100por Gschwendtner, E“…The CNGS, CERN Neutrinos to Gran Sasso project, aims at directly detecting muon-neutrino to tau-neutrino oscillations. …”
Publicado 2006
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