Solving the solar neutrino problem with kamLAND and BOREXINO

Details Solving the solar neutrino problem with kamLAND and BOREXINO Solving the solar neutrino problem with kamLAND and BOREXINO

2002-05-07

arxiv.org/abs/hep-ph/0205061v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, 5 figures, Talk given at 37th Rencontres de Moriond on Electroweak Interactions and Unified Theories, Les Arcs, Franc

Scientific paper

We 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 \chi^2 analysis, we obtain a LMA solution with a g.o.f. of 84.38%.

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