We 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≲ σpSI ≲ 10-8 pb 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. © 2006 Elsevier B.V. All rights reserved.
Prospects for direct dark matter detection in the constrained MSSM / Trotta, R.; de Austri, R. R.; Roszkowski, L.. - In: NEW ASTRONOMY REVIEWS. - ISSN 1387-6473. - 51:3-4(2007), pp. 316-320. [10.1016/j.newar.2006.11.059]
Prospects for direct dark matter detection in the constrained MSSM
Trotta R.;
2007-01-01
Abstract
We 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≲ σpSI ≲ 10-8 pb 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. © 2006 Elsevier B.V. All rights reserved.File | Dimensione | Formato | |
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