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- W2043286053 endingPage "1643" @default.
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- W2043286053 abstract "We explore quantitatively recent suggestions that the solar-neutrino puzzle may be explained by matter enhancement of nonstandard neutral-current scattering of neutrinos on $d$ quarks. These neutral currents introduce two new parameters, relating to flavor-diagonal and off-diagonal $ensuremath{nu}ensuremath{-}d$ scattering, which affect the dynamical mixing of two neutrino flavors in the Sun. We consider this mixing in three alternative scenarios: (a) massless neutrinos, (b) massive neutrinos with off-diagonal but no new diagonal currents, and (c) massive neutrinos with both off-diagonal and new diagonal currents. We determine the regions in parameter space that give consistency between the standard solar model and existing solar-neutrino data from the Homestake and Kamiokande-II experiments, and give the corresponding predictions for future experiments with gallium and superfluid helium detectors. We also discuss the more general situation, with nonstandard neutral-current scattering from $u$ quarks and electrons as well as from $d$ quarks, and consider the effects of transmission through the Earth. Finally, we examine the bounds on nonstandard neutral-current neutrino scattering imposed by other experiments; some particular classes of solution are thereby excluded, but a variety of possibilities remains." @default.
- W2043286053 created "2016-06-24" @default.
- W2043286053 creator A5000465406 @default.
- W2043286053 creator A5061874111 @default.
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- W2043286053 date "1991-09-15" @default.
- W2043286053 modified "2023-09-25" @default.
- W2043286053 title "Solar-neutrino solutions with matter-enhanced flavor-changing neutral-current scattering" @default.
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- W2043286053 doi "https://doi.org/10.1103/physrevd.44.1629" @default.
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