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- W2030424374 abstract "The spectrum of neutrinos from the Sun contains large fluxes of monoenergetic neutrinos which could be observed in the next generation of solar-neutrino detectors. Such observations directly probe neutrino parameters independent of uncertainties in the standard solar model. Small neutrino mass differences, ${10}^{mathrm{ensuremath{-}}11}$${mathit{m}}_{2}^{2}$-${mathit{m}}_{1}^{2}$${10}^{mathrm{ensuremath{-}}8}$ ${mathrm{eV}}^{2}$, would cause the measured flux of $^{7}mathrm{line}$ neutrinos to oscillate with a period in the range of a week up to a year. A neutrino magnetic moment comparable to the present laboratory bound would produce large distortions in the spectrum of scattered electrons." @default.
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- W2030424374 date "1990-11-12" @default.
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- W2030424374 title "Direct probes of neutrino properties using solar-neutrino lines" @default.
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- W2030424374 doi "https://doi.org/10.1103/physrevlett.65.2479" @default.
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