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- W2022846633 abstract "We perform an updated phenomenological analysis of the Mikheyev-Smirnov-Wolfenstein (MSW) solutions of the solar neutrino problem, assuming oscillations between two and three neutrino families. The analysis includes the total rates of the Homestake, SAGE, GALLEX, Kamiokande and Super-Kamiokande experiments, as well as the day-night asymmetry and the 18-bin energy spectrum of Super-Kamiokande. Solutions are found at several values of the ${ensuremath{theta}}_{13}$ mixing angle. Among the most interesting features, we find that solar neutrino data alone put the constraint ${ensuremath{theta}}_{13}ensuremath{lesssim}55ifmmode^circelsetextdegreefi{}--59ifmmode^circelsetextdegreefi{}$ at 95% C.L., and that a fraction of the MSW solutions extends at and beyond maximal $({ensuremath{nu}}_{1},{ensuremath{nu}}_{2})$ mixing $({ensuremath{theta}}_{12}>~ensuremath{pi}/4),$ especially if the neutrino square mass splitting is in its lower range ${(m}_{2}^{2}ensuremath{-}{m}_{1}^{2}ensuremath{sim}{10}^{ensuremath{-}7} {mathrm{eV}}^{2})$ and if ${ensuremath{theta}}_{13}$ is nonzero. In particular, bimaximal (or nearly bimaximal) mixing is possible for atmospheric and MSW solar neutrino oscillations within the stringent reactor bounds on ${ensuremath{theta}}_{13}.$" @default.
- W2022846633 created "2016-06-24" @default.
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- W2022846633 date "2000-05-26" @default.
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- W2022846633 title "Three-flavor MSW solutions of the solar neutrino problem" @default.
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- W2022846633 doi "https://doi.org/10.1103/physrevd.62.013002" @default.
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