Implications of Super-Kamiokande atmospheric low-energy data for solar neutrino oscillations

Details Implications of Super-Kamiokande atmospheric low-energy data for solar neutrino oscillations Implications of Super-Kamiokande atmospheric low-energy data for solar neutrino oscillations

1999-02-07

arxiv.org/abs/hep-ph/9902261v2

Physics

High Energy Physics

High Energy Physics - Phenomenology

12 pages including 1 figure, RevTeX

Scientific paper

It is shown that the high-Delta m^2 part of the large mixing angle MSW solution of the solar neutrino problem is disfavored by the Super-Kamiokande data for low-energy upward-going events. A quantitative bound is obtained in the three-neutrino scheme with a negligibly small element U_{e3} of the neutrino mixing matrix, as indicated by the result of the CHOOZ long-baseline antinu_e->antinu_e oscillation experiment.

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