2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/179575Assuming 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 $N> 70$ are found for any $δρ/ ρ$ in the range $10^{-5} - 10^{-3}$.11 pages, 2 figures (In press Physical Review Letters 1995)AstrophysicsHigh Energy Physics - Phenomenologytext