Critical temperature and primordial neutrino abundances

Details Critical temperature and primordial neutrino abundances Critical temperature and primordial neutrino abundances

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phlb..240..170e&link_type=abstract

Physics Letters B, Volume 240, Issue 1-2, p. 170-174.

Physics

Scientific paper

We consider the effects of the electroweak phase transition on the relic neutrino abundances in the standard big bang cosmology. We show that when the critical temperature Tc is less than the mass of the neutrino, the relic density will be strongly suppressed. The Lee-Weinberg bound, however, will be affected only if Tc

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