The Coleman-Weinberg mechanism in early cosmology

Details The Coleman-Weinberg mechanism in early cosmology The Coleman-Weinberg mechanism in early cosmology

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982nuphb.200..329b&link_type=abstract

Nuclear Physics B, Volume 200, Issue 2, p. 329-344.

Physics

Nuclear Physics

29

Scientific paper

The SU(5) --> SU(3) × SU(2) × U(1) phase transition is examined in the case of zero Higgs bare mass. We find that, depending on assumptions made, two scenarios are most likely to occur. Either the transition is rapidly completed into the SU(3) × SU(2) × U(1) phase, or the Universe supercools down to temperatures where the theory gets strongly coupled. In the latter case non-perturbative effects come into play.

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