Cold Dark Matter detection in SUSY models at large tan(beta)

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dc.creatorGomez, M. E.
dc.creatorVergados, J. D.
dc.date2000-12-03
dc.date2001-05-09
dc.date.accessioned2026-07-07T10:32:46Z
dc.date.available2026-07-07T10:32:46Z
dc.descriptionWe study the direct detection rate for SUSY cold dark matter (CDM) predicted by the minimal supersymmetric standard model with universal boundary conditions and large values for tan(beta). The relic abundance of the lightest supersymmetric particle (LSP), assumed to be approximately a bino, is obtained by including its coannihilations with the next-to-lightest supersymmetric particle (NLSP), which is the lightest s-tau. The cosmological constraint on this quantity severely limits the allowed SUSY parameter space, especially in the case the CP-even Higgs has mass of around 114 GeV. We find that for large tan(beta) it is possible to find a subsection of the allowed parameter space, which yields detectable rates in the currently planned experiments.
dc.descriptionChanges in text and figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0012020
dc.identifierhttp://arxiv.org/abs/hep-ph/0012020
dc.identifierPhys.Lett.B512:252-260,2001
dc.identifierdoi:10.1016/S0370-2693(01)00726-2
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178871
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCold Dark Matter detection in SUSY models at large tan(beta)
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