Effects of the 17 keV neutrino in supernovae

Details Effects of the 17 keV neutrino in supernovae Effects of the 17 keV neutrino in supernovae

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phlb..269..357m&link_type=abstract

Physics Letters B, Volume 269, Issue 3-4, p. 357-360.

Physics

8

Scientific paper

We discuss the astrophysical implications of the 17 keV neutrino, recently discovered in beta decay experiments. We show that due to their large mixing with the electron neutrinos enhanced by the matter effect, the 17 keV neutrinos are copiously produced in the core of supernovae. This may have substantial effects on the dynamics of the collapse. We consider alternative interpretations of the 17 keV neutrino and give a qualitative discussion on their consequences on the physics of supernovae.

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