Tachyon warm inflationary universe model in the weak dissipation regimen
Abstract
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. © 2008 IOP Publishing Ltd.
Más información
| Título según SCOPUS: | Tachyon warm inflationary universe model in the weak dissipation regimen |
| Título de la Revista: | 4TH EUROPEAN SYMPOSIUM ON FIRE SAFETY SCIENCE |
| Volumen: | 134 |
| Editorial: | IOP PUBLISHING LTD |
| Fecha de publicación: | 2008 |
| Idioma: | eng |
| URL: | http://www.scopus.com/inward/record.url?eid=2-s2.0-65249100153&partnerID=q2rCbXpz |
| DOI: |
10.1088/1742-6596/134/1/012008 |
| Notas: | SCOPUS |