Abstract
The warm-inflationary universe model in a tachyon field theory is studied in the weakly dissipative regime. We develop our model for an exponential potential and the dissipation parameter Γ=Γ 0=constant. We describe scalar and tensor perturbations for this scenario.
Original language | English |
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Pages (from-to) | 913-916 |
Number of pages | 4 |
Journal | European Physical Journal C |
Volume | 59 |
Issue number | 4 |
DOIs | |
State | Published - Feb 2009 |