Finite temperature energy density and effective quasi-potential in anisotropic universes

Details Finite temperature energy density and effective quasi-potential in anisotropic universes Finite temperature energy density and effective quasi-potential in anisotropic universes

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phlb..160...36c&link_type=abstract

Physics Letters B, Volume 160, Issue 1-3, p. 36-42.

Physics

21

Scientific paper

By means of the adiabatic expansion method we derive the finite temperature energy density and the finite temperature effective quasi-potential of a massive λ∅4 scalar field arbitrarily coupled to a Bianchi type I universe with small anisotropy. These results and higher-dimensional generalizations thereof are useful for the study of thermal and quantum back-reaction effects inBianchi and Kaluza-Klein cosmologies.
One of us (LFC) wishes to thank members of the Theoretical General Relativity Group for hospitality and the Center for Theoretical Physics for partial support during his visit to the University of Maryland.

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