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: | XXIII INTERNATIONAL CONFERENCE ON INTEGRABLE SYSTEMS AND QUANTUM SYMMETRIES (ISQS-23) |
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 |