Spinor fields in an Einstein universe: Finite-temperature effects

Details Spinor fields in an Einstein universe: Finite-temperature effects Spinor fields in an Einstein universe: Finite-temperature effects

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phrvd..18.3557a&link_type=abstract

Physical Review D, vol. 18, Issue 10, pp. 3557-3564

Physics

33

Scientific paper

The finite-temperature corrections to the vacuum energy density of scalar, neutrino, and photon fields in an Einstein universe are calculated by using the statistical-mode-sum technique with the aid of the Poisson summation formula. The theory of relativistic time-temperature Green's functions in static space-time is also considered and used to calculate the temperature correction to the neutrino-field vacuum energy density. Asymptotic limits of low and high temperature are discussed for each case.

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