Electroweak phase transition and dark matter abundance

Details Electroweak phase transition and dark matter abundance Electroweak phase transition and dark matter abundance

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phlb..247..601d&link_type=abstract

Physics Letters B, Volume 247, Issue 4, p. 601-606.

Physics

5

Scientific paper

If the critical temperature of the electroweak phase transition is
sufficiently small, it can change the final abundances of heavy dark
matter particles, by keeping them massless for a long time. Recent
experimental bounds on the Higgs mass from LEP imply that this is not
the case in the minimal standard model.

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