Non-minimal supergravity at finite temperatures and cosmological applications

Details Non-minimal supergravity at finite temperatures and cosmological applications Non-minimal supergravity at finite temperatures and cosmological applications

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nuphb.262..556e&link_type=abstract

Nuclear Physics B, Volume 262, Issue 3, p. 556-574.

Physics

Nuclear Physics

7

Scientific paper

We compute thermal one-loop corrections to the scalar potentials of two classes of non-minimal supergravities: the SU(N,1) maximally symmetric supergravity and the generalized SU(N,1) model that allows for cosmological inflation. For completeness, we give the result also for minimal supergravity, including contributions from the D-terms. We discuss the effects of temperature corrections in no-scale GUTs and in primordial maximally symmetric inflation. In particular we show that the latter satisfy trivially the condition for thermal stability.

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