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

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

2000-12-03

arxiv.org/abs/hep-ph/0012020v2

Phys.Lett.B512:252-260,2001

Physics

High Energy Physics

High Energy Physics - Phenomenology

Changes in text and figures

Scientific paper

10.1016/S0370-2693(01)00726-2

We 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.

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