Electroweak inflation and reheating in the NMSSM
| dc.creator | Fukuyama, Takeshi | |
| dc.creator | Kikuchi, Tatsuru | |
| dc.creator | Naylor, Wade | |
| dc.date | 2005-11-09 | |
| dc.date.accessioned | 2026-07-07T06:49:55Z | |
| dc.date.available | 2026-07-07T06:49:55Z | |
| dc.description | A low reheating temperature is now well motivated by the recently reconsidered gravitino problem, if we incorporate supergravity. In this article, we propose a model which naturally realizes a low reheating temperature. The model is based on the next to minimal supersymmetric standard model (NMSSM) by identifying a singlet scalar field as the inflaton. This entertains the possibility that the inflaton may be detected at future colliders, such as the LHC. | |
| dc.description | 5 pages, 2 figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0511105 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0511105 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/104535 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Electroweak inflation and reheating in the NMSSM | |
| dc.type | text |