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arXiv:astro-ph/9509049·v1·Astrophysics

Warm Inflation

Arjun Berera (Penn State)🇺🇸

PDFarXivINSPIREDOI

Abstract

Assuming a first order phase transition during inflation, a model scenario is described which does not require a tiny coupling constant. Thermal equilibrium is closely maintained as inflation commences. No large scale reheating is necessary. Solutions for are found for any in the range .

Comments: 11 pages, 2 figures (In press Physical Review Letters 1995)

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