Radiative Neutrino Mass, Dark Matter and Leptogenesis

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dc.creatorGu, Pei-Hong
dc.creatorSarkar, Utpal
dc.date2007-12-18
dc.date2008-04-22
dc.date.accessioned2026-07-07T11:39:29Z
dc.date.available2026-07-07T11:39:29Z
dc.descriptionWe propose an extension of the standard model, in which neutrinos are Dirac particles and their tiny masses originate from a one-loop radiative diagram. The new fields required by the neutrino mass-generation also accommodate the explanation for the matter-antimatter asymmetry and dark matter in the universe.
dc.description4 pages, 3 figures. Revised version with improved model. Accepted by PRD
dc.identifierhttps://arxiv.org/abs/0712.2933
dc.identifierhttp://arxiv.org/abs/0712.2933
dc.identifierPhys.Rev.D77:105031,2008
dc.identifierdoi:10.1103/PhysRevD.77.105031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199937
dc.subjectHigh Energy Physics - Phenomenology
dc.titleRadiative Neutrino Mass, Dark Matter and Leptogenesis
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