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Neutral current induced neutrino oscillations in a supernova

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arxiv hep-ph/9701311 v1 pith:FPWX3OTA submitted 1997-01-16 hep-ph astro-ph

Neutral current induced neutrino oscillations in a supernova

classification hep-ph astro-ph
keywords neutrinooscillationsinducedneutralneutrinossterileactiveanti-
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Sterile Neutrino as an Asymmetric Dark Matter

    hep-ph 2026-02 reject novelty 4.0

    A model for asymmetric freeze-in production of Dirac sterile neutrino dark matter is proposed, but the relic density calculation ignores the symmetric component and assumes an equilibrium mediator abundance.