Unifying inflation and dark matter with neutrino masses

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dc.creatorAllahverdi, Rouzbeh
dc.creatorDutta, Bhaskar
dc.creatorMazumdar, Anupam
dc.date2007-08-29
dc.date.accessioned2026-07-07T11:42:06Z
dc.date.available2026-07-07T11:42:06Z
dc.descriptionWe propose a simple model where a {\it gauge invariant inflaton} is responsible for cosmic inflation and generates the seed for structure formation, while its relic {\it thermal} abundance explains the missing matter of the universe in the form of cold dark matter. The inflaton self-coupling also explains the observed neutrino masses. All the virtues can be attained in a minimal extension of the Standard Model gauge group around the TeV scale. We can also unveil these properties of an inflaton in forthcoming space and ground based experiments.
dc.description4 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/0708.3983
dc.identifierhttp://arxiv.org/abs/0708.3983
dc.identifierPhys.Rev.Lett.99:261301,2007
dc.identifierdoi:10.1103/PhysRevLett.99.261301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200764
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleUnifying inflation and dark matter with neutrino masses
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