Warm Inflation

Details Warm Inflation Warm Inflation

1995-09-08

arxiv.org/abs/astro-ph/9509049v1

Phys.Rev.Lett.75:3218-3221,1995

Astronomy and Astrophysics

Astrophysics

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

Scientific paper

10.1103/PhysRevLett.75.3218

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 $\delta \rho / \rho$ in the
range $10^{-5} - 10^{-3}$.

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