After Sno and Before Kamland: Present and Future of Solar and Reactor Neutrino Physics

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dc.creatorAliani, P.
dc.creatorAntonelli, V.
dc.creatorFerrari, R.
dc.creatorPicariello, M.
dc.creatorTorrente-Lujan, E.
dc.date2002-11-05
dc.date.accessioned2026-07-07T08:11:37Z
dc.date.available2026-07-07T08:11:37Z
dc.descriptionWe present a short review of the existing evidence in favor of neutrino mass and neutrino oscillations which come from different kinds of experiments. We focus our attention in particular on solar neutrinos, presenting a review of some recent analysis of all available neutrino oscillation evidence in Solar experiments including the recent $SNO CC$ and $NC$ data. We present in detail the power of the reactor experiment KamLAND for discriminating existing solutions to the SNP and giving accurate information on neutrino masses and mixing angles.
dc.descriptionExpanded version of the contribution to appear in the Proceedings of ''Third Tropical Workshop on Particle Physics and Cosmology: Neutrinos, Branes and Cosmology (Puerto Rico, August 2002)''
dc.identifierhttps://arxiv.org/abs/hep-ph/0211062
dc.identifierhttp://arxiv.org/abs/hep-ph/0211062
dc.identifierAIP Conf.Proc. 655 (2003) 103-121
dc.identifierdoi:10.1063/1.1543492
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/132180
dc.subjectHigh Energy Physics - Phenomenology
dc.titleAfter Sno and Before Kamland: Present and Future of Solar and Reactor Neutrino Physics
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