Neutralino Dark Matter in the NMSSM

dc.creatorLopez-Fogliani, D. E.
dc.date2007-03-16
dc.date.accessioned2026-07-07T11:02:52Z
dc.date.available2026-07-07T11:02:52Z
dc.descriptionWe analyze the direct detection of neutralino dark matter in the framework of the Next-to-Minimal Supersymmetric Standard Model. Taking into account all the available constraints from LEPII and Tevatron, including bounds from the muon anomalous magnetic moment and flavor constraint as $b \to s γ$, we compute the neutralino-nucleon cross section and compare the results with the sensitivity of dark matter detectors. We also study the relic abundance of neutralinos, comparing it with WMAP observations. We show that a light singlet-like Higgs can escape accelerator constraints allowing for scenarios with large cross sections, and a very interesting phenomenology.
dc.description6 pages, 6 figures, talk given at IRGAC2006, Barcelona, July 11-15, 2006, to appear in J. Phys. A
dc.identifierhttps://arxiv.org/abs/hep-ph/0703181
dc.identifierhttp://arxiv.org/abs/hep-ph/0703181
dc.identifierJ.Phys.A40:6889-6894,2007
dc.identifierdoi:10.1088/1751-8113/40/25/S35
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188399
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutralino Dark Matter in the NMSSM
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