Warm-Chaplygin inflationary universe model

Astronomy and Astrophysics – Astrophysics

Scientific paper

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17 pages, 4 figures, Accepted for publication in Physics Letters B

Scientific paper

10.1016/j.physletb.2008.05.063

Warm inflationary universe models in the context of a Chaplygin gas equation
are studied. General conditions required for these models to be realizable are
derived and discussed. By using a chaotic potential we develop models for a
dissipation coefficient of the form $\Gamma\propto \phi^n$, with $n=0$ or
$n\neq 0$.

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