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- W2144151582 abstract "We study type II supernova signatures of neutrino mass generation via symmetry breaking at a scale in the range from keV to MeV. The scalar responsible for symmetry breaking is thermalized in the supernova core and restores the symmetry. The neutrinos from scalar decays have about half the average energy of thermal neutrinos. The Bose-Einstein distribution of the scalars can be established with a megaton water ifmmode check{C}else v{C}fi{}erenkov detector. The discovery of the bimodal neutrino flux is, however, well within the reach of the Super-Kamiokande detector, without a detailed knowledge of the supernova parameters." @default.
- W2144151582 created "2016-06-24" @default.
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- W2144151582 date "2005-11-02" @default.
- W2144151582 modified "2023-10-16" @default.
- W2144151582 title "Probing the Origins of Neutrino Mass with Supernova Data" @default.
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- W2144151582 doi "https://doi.org/10.1103/physrevlett.95.191302" @default.
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