Supersymmetric dark matter and neutralino-nucleon cross section
| dc.creator | Cerdeno, D. G. | |
| dc.creator | Khalil, S. | |
| dc.creator | Munoz, C. | |
| dc.date | 2001-05-17 | |
| dc.date | 2001-08-09 | |
| dc.date.accessioned | 2026-07-07T03:44:33Z | |
| dc.date.available | 2026-07-07T03:44:33Z | |
| dc.description | We review the direct detection of supersymmetric dark matter in the light of recent experimental results. In particular, we show that regions in the parameter space of several supergravity scenarios with a neutralino-nucleon cross section of order of $10^{-6}$ pb, i.e., where current dark matter detectors are sensitive, can be obtained. These are scenarios with large $\tan β$, with non-universal soft supersymmetry-breaking terms, with multi-TeV masses for scalar superpartners known as `focus point' supersymmetry, and finally scenarios with intermediate unification scale which appear naturally in some superstring constructions. | |
| dc.description | Extension of a talk given at Cairo International Conference on High Energy Physics (CICHEP 2001), January 9-14, 22 pages, 10 figures. Conventions clarified, figures improved, references added | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0105180 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0105180 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/40604 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Supersymmetric dark matter and neutralino-nucleon cross section | |
| dc.type | text |