Effective potential approach to finite temperature quantum cosmology

Details Effective potential approach to finite temperature quantum cosmology Effective potential approach to finite temperature quantum cosmology

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phlb..200...69m&link_type=abstract

Physics Letters B, Volume 200, Issue 1-2, p. 69-74.

Physics

4

Scientific paper

We consider one-loop corrections in finite temperature quantum cosmology in the statis approximation. An exact expression for the effective potential of the Coleman-Weinberg type is given for the scalar field in a closed cosmological model. The role of non-zero temperature and non-zero curvature quantum corrections due to the non-trivial S1×S3 topology is discussed. Quantum topological effects of mass generation of the self-interacting scalar field as well as zero-point fluctuation energy are examined.

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