Finite temperature effects in primordial inflation

G. B. Gelmini, D. V. Nanopoulos, K. A. Olive

Research output: Contribution to journalArticlepeer-review

30 Scopus citations


We present a detailed study of a recently proposed model for primordial inflation based on an N=1 locally supersymmetric potential. For a large class of parameters with which all cosmological constraints are satisfied, the temperature corrections can be neglected during the inflation period. At higher temperatures, the minimum is not at the origin, but very close to it.

Original languageEnglish (US)
Pages (from-to)53-58
Number of pages6
JournalPhysics Letters B
Issue number1-3
StatePublished - Nov 10 1983


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