Dressing the inflaton with the Standard Model gauge group

dc.creatorMazumdar, A.
dc.date2007-09-27
dc.date.accessioned2026-07-07T08:32:37Z
dc.date.available2026-07-07T08:32:37Z
dc.descriptionIn this talk we will discuss how inflation can be embedded within a minimal extension of the Standard Model where the inflaton carries the Standard Model charges. There is no need of an ad-hoc scalar field to be introduced in order to explain the temperature anisotropy of the cosmic microwave background radiation, all the ingredients are present within a minimal supersymmetric Standard Model. The model is robust enough to provide a successful exit from inflation with all observed matter in the universe. This is a triumph for an inflationary paradigm which has always begged a simple question: can we identify the inflaton in a laboratory. We will briefly discuss how LHC can shed some insight into the inflaton.
dc.description19 pages, review talk
dc.identifierhttps://arxiv.org/abs/0709.4396
dc.identifierhttp://arxiv.org/abs/0709.4396
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/138846
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDressing the inflaton with the Standard Model gauge group
dc.typetext

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