arXiv · hep-ph/9701311
Neutral current induced neutrino oscillations in a supernova
Abstract
Neutral currents induced matter oscillations of electroweak-active (anti-)neutrinos to sterile neutrinos can explain the observed motion of pulsars. In contrast to a recently proposed explanation of the pulsar birth velocities based on the electron to tau (muon) neutrino oscillations [hep-ph/9606428], the heaviest neutrino (either active or sterile) would have to have mass of order several keV.
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Alexander Kusenko, Gino Segre. 1997-01-16. Neutral current induced neutrino oscillations in a supernova. https://doi.org/10.1016/s0370-2693(97)00121-4
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