Dark Matter and Yukawa Unification with Massive Neutrinos

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dc.creatorGomez, M. E.
dc.creatorLola, S.
dc.creatorNaranjo, P.
dc.creatorRodriguez-Quintero, J.
dc.date2009-01-27
dc.date2009-01-27
dc.date.accessioned2026-07-07T13:10:24Z
dc.date.available2026-07-07T13:10:24Z
dc.descriptionWe revisit the WMAP dark matter constraints on Yukawa Unification in the presence of massive neutrinos. The large neutrino mixing indicated by the data modifies the predictions for the bottom quark mass, and enables Yukawa also for large $\tanβ$, and for positive $μ$ that were previously disfavoured. As a result, the allowed parameter space for neutralino dark matter also increases, particularly for areas with resonant enhancement of the neutralino relic density.
dc.descriptionProceedings of 4th International Workshop on the Dark Side of the Universe (DSU 2008), Cairo, June 2008. 7 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/0901.4332
dc.identifierhttp://arxiv.org/abs/0901.4332
dc.identifierAIP Conf.Proc.1115:273-278,2009
dc.identifierdoi:10.1063/1.3131510
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229006
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDark Matter and Yukawa Unification with Massive Neutrinos
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