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 find that 10-10pb ≲ σSIp ≲10-8 pb for direct WIMP detection (with details slightly dependent on the assumptions made). We conclude that most of the 95% probability region for the cross section will be explored by future onetonne detectors, that will therefore cover most of the currently favoured region of parameter space.
Prospects for direct dark matter searches in the constrained mssm / Trotta, R.; De Austri, R. R.; Roszkowski, L.. - (2007), pp. 81-86. ((Intervento presentato al convegno 6th International Workshop on the Identification of Dark Matter, IDM 2006 tenutosi a Rhodes, grc nel 2006 [10.1142/9789812770288_0010].
Prospects for direct dark matter searches 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 find that 10-10pb ≲ σSIp ≲10-8 pb for direct WIMP detection (with details slightly dependent on the assumptions made). We conclude that most of the 95% probability region for the cross section will be explored by future onetonne detectors, that will therefore cover most of the currently favoured region of parameter space.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
