Electroweak inflation and reheating in the NMSSM

dc.creatorFukuyama, Takeshi
dc.creatorKikuchi, Tatsuru
dc.creatorNaylor, Wade
dc.date2005-11-09
dc.date.accessioned2026-07-07T06:49:55Z
dc.date.available2026-07-07T06:49:55Z
dc.descriptionA 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.description5 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0511105
dc.identifierhttp://arxiv.org/abs/hep-ph/0511105
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/104535
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleElectroweak inflation and reheating in the NMSSM
dc.typetext

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