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 N>70 are found for any δρ/ρ in the range 10-5-10-3. © 1995 The American Physical Society.
CITATION STYLE
Berera, A. (1995). Warm inflation. Physical Review Letters, 75(18), 3218–3221. https://doi.org/10.1103/PhysRevLett.75.3218
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