arXiv:astro-ph/9509049·v1·Astrophysics
Warm Inflation
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)