Bulk viscosity impact on the scenario of warm inflation
| dc.creator | Mimoso, Jose Pedro | |
| dc.creator | Nunes, Ana | |
| dc.creator | Pavon, Diego | |
| dc.date | 2006-12-20 | |
| dc.date.accessioned | 2026-07-07T07:36:26Z | |
| dc.date.available | 2026-07-07T07:36:26Z | |
| dc.description | The decay of the inflaton into radiation and particles during the slow-roll suggests that these may interact with each other and that the latter may also decay into subproducts before inflation is completed. As a consequence, the fluid is no longer perfect and a non-negligible bulk viscosity necessarily sets in. We write the corresponding equations as an autonomous system and study the asymptotic behavior, the conditions for the existence of scaling solutions, and show that the late time effect of fluid dissipation alleviates the depletion of matter and increases the duration of inflation. | |
| dc.description | 3 pages, uses World Sci. style; submitted to the Proceedings of Eleventh Marcel Grossmann Meeting | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0612581 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0612581 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/120425 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Bulk viscosity impact on the scenario of warm inflation | |
| dc.type | text |