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• W2057940597 abstract "We present a detailed analysis of the effect of a large transition magnetic moment of the electron neutrino (i.e., ${ensuremath{mu}}_{{ensuremath{nu}}_{e}}ensuremath{approx}{10}^{ensuremath{-}11}{ensuremath{mu}}_{B}$) on the solar-neutrino flux measured in the chlorine and Kamiokande experiments. For $ensuremath{Delta}{m}_{{ensuremath{nu}}_{ensuremath{mu}}ensuremath{-}{ensuremath{nu}}_{e}}^{2}ensuremath{approx}{10}^{ensuremath{-}8}$ e${mathrm{V}}^{2}$ and ${ensuremath{mu}}_{ensuremath{nu}}ensuremath{approx}{10}^{ensuremath{-}11}{ensuremath{mu}}_{B}$, the combination of matter effects and spin precession enables us to explain the apparent anticorrelation of the neutrino flux with the sun-spot activity in the chlorine experiment, as well as the lack of time variation in the Kamiokande experiment. For this choice of parameters, we predict that the gallium experiment should show strong anticorrelation with the solar activity, with a maximum flux of 80 SNU (solar-neutrino units) during the Sun-spot minimum" @default.
• W2057940597 created "2016-06-24" @default.
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• W2057940597 date "1991-10-15" @default.
• W2057940597 modified "2023-09-23" @default.
• W2057940597 title "Reconciling the time dependence of the chlorine and Kamiokande solar-neutrino data" @default.
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• W2057940597 doi "https://doi.org/10.1103/physrevd.44.2265" @default.
• W2057940597 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/10014108" @default.
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