Finite temperature effective potential for λφ4 theory in Robertson-Walker universes

Details Finite temperature effective potential for λφ4 theory in Robertson-Walker universes Finite temperature effective potential for λφ4 theory in Robertson-Walker universes

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phlb..123..189h&link_type=abstract

Physics Letters B, Volume 123, Issue 3-4, p. 189-196.

Physics

44

Scientific paper

Under the condition that the rate of change of the fluctuation field is much greater than that of the background field and the expansion rate of the universe, a finite temperature field theory can be established in dynamical spacetimes. The one-loop finite temperature effective potential for λφ4 theory in Robertson-Walker universes is computed here by the adiabatic expansion method. It is useful for the study of the symmetry behavior of the GUT and Planck eras in the early universe.

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