Warm Inflation
| dc.creator | Berera, Arjun | |
| dc.date | 1995-09-08 | |
| dc.date.accessioned | 2026-07-07T10:34:51Z | |
| dc.date.available | 2026-07-07T10:34:51Z | |
| dc.description | Assuming a first order phase transition during inflation, a model scenario is described which does not require a tiny coupling constant. Thermal equilibrium is closely maintained as inflation commences. No large scale reheating is necessary. Solutions for $N> 70$ are found for any $δρ/ ρ$ in the range $10^{-5} - 10^{-3}$. | |
| dc.description | 11 pages, 2 figures (In press Physical Review Letters 1995) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9509049 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9509049 | |
| dc.identifier | Phys.Rev.Lett.75:3218-3221,1995 | |
| dc.identifier | doi:10.1103/PhysRevLett.75.3218 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/179575 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Warm Inflation | |
| dc.type | text |