Prospects for direct dark matter detection in the Constrained MSSM

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dc.creatorTrotta, Roberto
dc.creatorde Austri, Roberto Ruiz
dc.creatorRoszkowski, Leszek
dc.date2006-09-05
dc.date.accessioned2026-07-07T11:04:10Z
dc.date.available2026-07-07T11:04:10Z
dc.descriptionWe outline the WIMP dark matter parameter space in the Constrained MSSM by performing a comprehensive statistical analysis that compares with experimental data predicted superpartner masses and other collider observables as well as a cold dark matter abundance. We include uncertainties arising from theoretical approximations as well as from residual experimental errors on relevant Standard Model parameters. We present high-probability regions for neutralino dark matter direct detection cross section, and we find that 10^-10 pb < sigma_p^SI < 10^-8 for direct WIMP detection (with details slightly dependent on the assumptions made). We highlight a complementarity between LHC and WIMP dark matter searches in exploring the CMSSM parameter space. We conclude that most of the 95% probability region for the cross section will be explored by future one-tonne detectors, that will therefore cover most of the currently favoured region of parameter space.
dc.description5 pages, 3 figures. Contribution to the proceedings of the Francesco Melchiorri Memorial conference, Rome, April 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0609126
dc.identifierhttp://arxiv.org/abs/astro-ph/0609126
dc.identifierNewAstron.Rev.51:316-320,2007
dc.identifierdoi:10.1016/j.newar.2006.11.059
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188796
dc.subjectAstrophysics
dc.titleProspects for direct dark matter detection in the Constrained MSSM
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