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- W1991701404 startingPage "2146" @default.
- W1991701404 abstract "Neutron stars formed in supernovae are very intense sources of neutrinos of all species and masses ensuremath{le} 100 MeV. If such neutrinos decayed via ${ensuremath{nu}}_{H}ensuremath{rightarrow}{ensuremath{nu}}_{e}+{e}^{ensuremath{-}}+{e}^{ensuremath{-}}$ inside the Galaxy, annihilation of the trapped positrons would yield a 511-keV line exceeding the experimental bounds by many orders of magnitude. This allows us to exclude decay lifetimes in the range ${10}^{4}$-${10}^{15}$ sec for neutrinos of mass 1-100 MeV. Our result corroborates and extends earlier astrophysical bounds." @default.
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- W1991701404 date "1987-05-18" @default.
- W1991701404 modified "2023-09-24" @default.
- W1991701404 title "Can Supernovae Exclude Neutrinos More Massive than 30 eV?" @default.
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- W1991701404 doi "https://doi.org/10.1103/physrevlett.58.2146" @default.
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