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1361por Kachelriess, Michael“…Different approximations for the survival probability of supernova neutrinos are compared. Results of a combined likelihood analysis of the observed SN1987A neutrino signal and of the latest solar neutrino data including the recent SNO CC measurement are presented.…”
Publicado 2001
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1362“…We discuss the possibility to observe matter effects in atmospheric neutrino oscillations. The main conclusion is that an impact on the nu_mu survival probability requires the action of the MSW resonance, which becomes visible for baselines above ~7000 km. …”
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1363“…We present an updated analysis of all the data available about solar neutrinos, including the charged current SNO results. …”
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1364por Gruber, P“…Ionisation cooling is one of the main ingredients of a Neutrino Factory -- a high-intensity, high-energy neutrino machine. …”
Publicado 2001
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1365por Suzuki, Y, Ieiri, M, Kato, Y, Kusano, E, Minakawa, M, Noumi, H, Takasaki, M, Tanaka, K H, Yamanoi, YEnlace del recurso
Publicado 1999
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1366
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1367
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1368por Ambrosio, M, Antolini, R, Aramo, C, Auriemma, G, Baldini, A, Barbarino, G C, Barish, B C, Battistoni, G, Bellotti, R, Bemporad, C, Bernardini, E, Bernardini, P, Bilokon, H, Bisi, V, Bloise, C, Bower, C, Brigida, M, Bussino, S, Cafagna, F, Calicchio, M, Campana, D, Carboni, M, Cecchini, S, Cei, F, Chiarella, V, Choudhary, B C, Coutu, S, De Cataldo, G, Dekhissi, H, De Marzo, C, De Mitri, I, Derkaoui, J E, De Vincenzi, M, Di Credico, A, Erriquez, O, Favuzzi, C, Forti, C, Fusco, P, Giacomelli, G, Giannini, G, Giglietto, N, Giorgini, M, Grassi, M, Gray, L, Grillo, A, Guarino, F, Gustavino, C, Habig, A, Hanson, K, Heinz, R, Huang, Y, Iarocci, Enzo, Katsavounidis, E, Katsavounidis, I, Kearns, E T, Kim, H, Kyriazopoulou, S, Lammanna, E, Lane, C, Lari, T, Levins, D S, Lipari, P, Longley, N P, Longo, M J, Loparco, F, Maaroufi, F, Mancarella, G, Mandrioli, G, Margiotta, A, Marini, A, Martello, D, Marzari-Chiesa, A, Mazziotta, M N, Michael, D G, Mikheyev, S P, Miller, L, Monacelli, P, Montaruli, T, Monteno, M, Mufson, S L, Musser, J, Nicolò, D, Nolty, R, Orth, C, Osteria, G, Ouchrif, M, Palamara, O, Patera, V, Patrizii, L, Pazzi, R, Peck, C W, Perrone, L, Petrera, S, Pistilli, P, Popa, VR, Rainó, A, Rastelli, A, Reynoldson, J, Ronga, F, Rubizzo, U, Satriano, C, Satta, L, Scapparone, E, Scholberg, K, Sciubba, A, Serra, P, Severi, M, Sioli, M, Sitta, M, Spinelli, P, Spinetti, M, Spurio, M, Steinberg, R, Stone, J L, Sulak, Lawrence R, Surdo, A, Tarle, G, Togo, V, Ugolotti, D, Vakili, M, Walter, C W, Webb, REnlace del recurso
Publicado 1999
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1369“…We review theoretical ideas, problems and implications of different models for neutrino masses and mixing angles. We give a general discussion of schemes with three or more light neutrinos. …”
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1370“…We review some astrophysical and cosmological properties and implications of neutrino masses and mixing angles. These include: constraints based on the relic density of neutrinos, limits on their masses and lifetimes, BBN limits on mass parameters, neutrinos and supernovae, and neutrinos and high energy cosmic rays.…”
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1371
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1372“…The 3-dimensional (3-D) calculation of the atmospheric neutrino flux by means of the FLUKA Monte Carlo model is here described in all details, starting from the latest data on primary cosmic ray spectra. …”
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1373
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1374
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1375
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1376
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1377“…It is shown how, in a class of models, the sign of the baryon number of the universe can be related to CP violation in neutrino oscillation experiments.…”
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1378
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1379por Kokkonen, J“…In order to demonstrate the feasibility of conducting future muon neutrino - tau neutrino oscillation searches using a high-resolution, large-area silicon microstrip detector, the Silicon TARget (STAR) detector was built. …”
Publicado 2002
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1380por Duchesneau, D.“…This paper reviews the current experimental program envisaged with the future CERN neutrino beam called CNGS. Two detectors, OPERA and ICARUS, are under preparation and should investigate the neutrino properties coming from the CNGS to shed light on neutrino oscillation physics.…”
Publicado 2002
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