Mirror neutrinos in supernovae

Details Mirror neutrinos in supernovae Mirror neutrinos in supernovae

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phlb..231..439m&link_type=abstract

Physics Letters B, Volume 231, Issue 4, p. 439-443.

Physics

Scientific paper

It is known that in a model containing mirror leptons the magnetic moment of the electron neutrino (μve) may be large enough, μve⋍(10-11-10-10)μB, to explain the deficit of solar neutrinos. We show that such a large μve is consistent with the observations of the supernova SN 1987A. In this model the magnetic transition does not lead to the production of inert neutrinos which would cause a rapid cooling of the star.

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