Solving the solar neutrino problem with kamLAND and BOREXINO

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dc.creatorAliani, P.
dc.creatorAntonelli, V.
dc.creatorFerrari, R.
dc.creatorPicariello, M.
dc.creatorTorrente-Lujan, E.
dc.date2002-05-07
dc.date.accessioned2026-07-07T03:46:56Z
dc.date.available2026-07-07T03:46:56Z
dc.descriptionWe analyze the expected signals of two future neutrino experiments, kamLAND and BOREXINO. We show that with just these experiments, we will hopefully be able to determine which of the existing solutions to the solar neutrino problem is the real solution. We also analyze existing solar neutrino data and determine the best-fit points in the oscillation-parameter space finding that with the inclusion of SNO-charged current, the global-rates analysis gives a favored LMA solution with a goodness of fit (g.o.f) of just 32.63%, whereas the g.o.f of the SMA solution is 9.83%. Nonetheless, maximal and quasi-maximal mixing is not favored. If we include the Superkamiokande spectrum in our χ^2 analysis, we obtain a LMA solution with a g.o.f. of 84.38%.
dc.description4 pages, 5 figures, Talk given at 37th Rencontres de Moriond on Electroweak Interactions and Unified Theories, Les Arcs, France, 9-16 Mar 2002
dc.identifierhttps://arxiv.org/abs/hep-ph/0205061
dc.identifierhttp://arxiv.org/abs/hep-ph/0205061
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41477
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSolving the solar neutrino problem with kamLAND and BOREXINO
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