SUSY spectrum constraints on direct dark matter detection
arXiv:hep-ph/9908427 · doi:10.1103/PhysRevD.62.043524
Abstract
We perform an investigation of the MSSM parameter space at the Fermi scale taking into account available accelerator, non-accelerator and cosmological constraints. Extra assumptions about upper bounds for some of the SUSY particles are also imposed. We show that a non-observation of the SUSY dark matter candidates with a high-accuracy dark matter detector, such as Ge-73, under above-mentioned assumptions can exclude large domains of the MSSM parameter space and, for instance, can make especially desirable collider search for light SUSY charged Higgs boson.
latex, 13 pages, 6 figures, modified version to be published in Phys. Rev. D
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