| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8195064 | Physics Letters B | 2008 | 6 Pages |
Abstract
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 ÎâÏn, with n=0 or nâ 0.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Sergio del Campo, Ramón Herrera,