Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-06-03
Phys.Lett.B665:100-105,2008
Astronomy and Astrophysics
Astrophysics
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
$n\neq 0$.
del Campo Sergio
Herrera Ramon
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