Fermion Triplet Dark Matter and Radiative Neutrino Mass

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dc.creatorMa, Ernest
dc.creatorSuematsu, Daijiro
dc.date2008-09-05
dc.date2008-09-16
dc.date.accessioned2026-07-07T13:04:39Z
dc.date.available2026-07-07T13:04:39Z
dc.descriptionThe neutral member of a Majorana fermion triplet (Sigma^+,Sigma^0,Sigma^-) is proposed as a candidate for the dark matter of the Universe. It may also serve as the seesaw anchor for obtaining a radiative neutrino mass.
dc.description11 pages
dc.identifierhttps://arxiv.org/abs/0809.0942
dc.identifierhttp://arxiv.org/abs/0809.0942
dc.identifierMod.Phys.Lett.A24:583-589,2009
dc.identifierdoi:10.1142/S021773230903059X
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/227240
dc.subjectHigh Energy Physics - Phenomenology
dc.titleFermion Triplet Dark Matter and Radiative Neutrino Mass
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