Tachyon warm inflationary universe model in the weak dissipation regimen

Details Tachyon warm inflationary universe model in the weak dissipation regimen Tachyon warm inflationary universe model in the weak dissipation regimen

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.134a2008h&link_type=abstract

Journal of Physics: Conference Series, Volume 134, Issue 1, pp. 012008 (2008).

Physics

2

Scientific paper

Warm inflationary universe model in a tachyon field theory is studied in the weak dissipation regimen. We develop our model for an exponential potential and a dissipation parameter Γ = Γ0 = constant. We describe scalar and tensor perturbations for this scenario. Also, we use recent astronomical observations for constraining the parameters appearing in our model.

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