Warm-Chaplygin inflationary universe model
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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 $Γ\propto ϕ^n$, with $n=0$ or $n\neq 0$.
17 pages, 4 figures, Accepted for publication in Physics Letters B
17 pages, 4 figures, Accepted for publication in Physics Letters B