Curvaton reheating allows TeV Hubble scale in NO inflation

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dc.creatorSanchez, J. C. Bueno
dc.creatorDimopoulos, K.
dc.date2007-07-26
dc.date.accessioned2026-07-07T11:18:09Z
dc.date.available2026-07-07T11:18:09Z
dc.descriptionCurvaton reheating is studied in non-oscillatory (NO) models of inflation, with the aim to obtain bounds on the parameters of curvaton models and find out whether low scale inflation can be attained. Using a minimal curvaton model, it is found that the allowed parameter space is considerably larger than in the case of the usual oscillatory inflation models. In particular, inflation with Hubble scale as low as 1 TeV is comfortably allowed.
dc.description4 pages, no figures
dc.identifierhttps://arxiv.org/abs/0707.3967
dc.identifierhttp://arxiv.org/abs/0707.3967
dc.identifierJCAP0711:007,2007
dc.identifierdoi:10.1088/1475-7516/2007/11/007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193248
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleCurvaton reheating allows TeV Hubble scale in NO inflation
dc.typetext

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