Particle Production and Inflaton Decay
| dc.creator | Yoshimura, M. | |
| dc.date | 1996-02-10 | |
| dc.date.accessioned | 2026-07-07T03:58:51Z | |
| dc.date.available | 2026-07-07T03:58:51Z | |
| dc.description | A new theory of thermal history after inflation is outlined by taking into account the effect of parametric resonance caused by inflaton oscillation. A typical outcome is existence of a high temperature phase, that makes possible GUT baryogenesis consistently with low enough gravitino abundance. | |
| dc.description | 9 pages | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9602268 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9602268 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/45985 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Particle Production and Inflaton Decay | |
| dc.type | text |