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

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dc.creatorGiunti, C.
dc.creatorKim, C. W.
dc.creatorLee, U. W.
dc.creatorNaumov, V. A.
dc.date1999-02-07
dc.date1999-02-11
dc.date.accessioned2026-07-07T04:06:22Z
dc.date.available2026-07-07T04:06:22Z
dc.descriptionIt 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.
dc.description12 pages including 1 figure, RevTeX
dc.identifierhttps://arxiv.org/abs/hep-ph/9902261
dc.identifierhttp://arxiv.org/abs/hep-ph/9902261
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/48742
dc.subjectHigh Energy Physics - Phenomenology
dc.titleImplications of Super-Kamiokande atmospheric low-energy data for solar neutrino oscillations
dc.typetext

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