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3381
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3382“…For active and sterile neutrinos, we present the globally allowed solutions for two neutrino oscillations. …”
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3383por Zucchelli, Piero“…The evolution of neutrino physics demands new schemes to produce intense, collimated and pure neutrino beams. …”
Publicado 2001
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3384“…We study neutrino oscillations and the level-crossing probability PLZ in power-law potential profiles A(r)\propto r^n. …”
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3385“…In this paper we demonstrate in a string-inspired toy model that such a stringy Z' can indeed guarantee proton longevity and viable phenomenology in the neutrino sector, as well as in the quark and charged lepton sectors.…”
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3386
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3387por Cervera-Villanueva, A, do Couto e Silva, E, Ellis, M, Ferrère, D, Gómez-Cadenas, J J, Gouanère, M, Hernando, J A, Kokkonen, J, Kuznetsov, V E, Linssen, Lucie, Runólfsson, O, Soler, F J P“…This article describes the application of Kalman filter techniques for the tracking and vertexing of particles inside the NOMAD-STAR detector a silicon vertex detector installed in NOMAD, one of the neutrino oscillation experiments at the CERN-SPS. The use of the Kalman filter simplifies computationally the tracking and vertex procedure for NOMAD-STAR. …”
Publicado 2001
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3388
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3389“…Assuming Majorana neutrinos, we infer from oscillation data the expected values of the parameters m_{nu_e} and m_{ee} probed by beta and 0nu2beta-decay experiments. …”
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3390
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3391
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3392
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3393“…In addition to the results obtained from the measurement of the solar neutrino flux, the study of atmospheric neutrinos strongly supports the hypothesis of neutrino oscillation among different flavours. …”
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3394por McDonald, K T, Lü, C, Prebys, E J, Hassenein, A, Kahn, S A, King, B J, Kirk, H G, Ludewig, H, Palmer, R B, Pearson, C E, Samulyak, R V, Simos, N, Stumer, I, Thieberger, P, Weggel, R J, Johnson, C D, Ravn, H L, Hwang, P, Naumovich, G N, Childress, S, Mokhov, N V, Green, M A, Reginato, L L, Zeller, A, Miller, J R, Gabriel, T A, Haines, J R, Spampinato, P T, Fukui, YEnlace del recurso
Publicado 2001
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3395
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3396
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3397
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3398“…Current underground detectors can search for multiple muons from multi-W(Z) production initiated by ultrahigh energy neutrinos from active galactic nuclei. O($\mu$b) cross sections give rise to downward going muon bundles whose features differ from those of atmospheric muon bundles.…”
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3399por Burguet-Castell, J, Gavela-Legazpi, Maria Belen, Gómez-Cadenas, J J, Hernández, Pilar, Mena, O“…Superbeams (SB) and Neutrino Factories (NF) are not alternative facilities for exploring neutrino oscillation physics, but successive steps. …”
Publicado 2002
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3400