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261por Dighe, Amol S.“…We analyze the neutrino conversions inside a supernova in the 3$\nu$ mixing scheme, and their effects on the neutrino spectra observed at the earth. …”
Publicado 1999
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262“…We show that the neutrino mixing pattern with the large mixing required forthe atmospheric neutrino problem and the small mixing angle MSW solution forthe solar neutrino problem can be naturally generated through radiativemagnification, even though all the mixing angles at the seesaw scale may besmall. …”
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263
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265“…The article contains information about the construction and parameters of the 'IHEP-JINR neutrino detector', the largest experimental set-up at the U-70 accelerator (IHEP, Protvino). …”
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266por Pupilli, Fabio, Ballerini, G, Berra, A, Boanta, R, Bonesini, M, Brizzolari, C, Brunetti, G, Calviani, M, Carturan, S, Catanesi, M G, Cecchini, S, Cindolo, F, Coffani, A, Collazuol, G, Conti, E, Dal Corso, F, De Rosa, G, Gola, A, Intonti, R A, Jollet, C, Kudenko, Y, Laveder, M, Longhin, A, Loverre, P F, Ludovici, L, Magaletti, L, Mandrioli, G, Margotti, A, Mascagna, V, Mauri, N, Meregaglia, A, Mezzetto, M, Nessi, M, Paoloni, A, Pari, M, Paternoster, G, Patrizii, L, Piemonte, C, Pozzato, M, Prest, M, Radicioni, E, Riccio, C, Ruggieri, A C, Soldani, M, Sirri, G, Tenti, M, Terranova, F, Vallazza, E, Vesco, M, Votano, L, Wildner, E“…This contribution will report the results achieved in the first year of activities. The expected neutrino fluxes at an hypothetical far detector have been estimated. …”
Publicado 2018
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267
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268por Giacomelli, G.“…The CERN to Gran Sasso Neutrino beam (CNGS) was commissioned at CERN in early August 2006 and was first sent at low intensity to Gran Sasso on August 17, 2006. …”
Publicado 2007
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269
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270
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274
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275“…This book explains the physics and phenomenology of massive neutrinos. The authors argue that neutrino mass is not unlikely and consider briefly the search for evidence of this mass in decay processes before they examine the physics and phenomenology of neutrino oscillation. …”
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278“…We present a model for neutrino-nucleus scattering in the energy region relevant for present and forthcoming neutrino-oscillation experiments. …”
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