Supersymmetric Dark Matter in Light of WMAP
| dc.creator | Ellis, J. | |
| dc.creator | Olive, K. A. | |
| dc.creator | Santoso, Y. | |
| dc.creator | Spanos, V. C. | |
| dc.date | 2003-03-05 | |
| dc.date.accessioned | 2026-07-07T10:28:45Z | |
| dc.date.available | 2026-07-07T10:28:45Z | |
| dc.description | We re-examine the parameter space of the constrained minimal supersymmetric extension of the Standard Model (CMSSM), taking account of the restricted range of Ω_{CDM} h^2 consistent with the WMAP data. This provides a significantly reduced upper limit on the mass of the lightest supersymmetric particle LSP: m_χ< 500 GeV for \tan β< 45 and μ> 0, or \tan β< 30 and μ< 0, thereby improving the prospects for measuring supersymmetry at the LHC, and increasing the likelihood that a 1-TeV linear e^+ e^- collider would be able to measure the properties of some supersymmetric particles. | |
| dc.description | 12 pages LaTeX, 7 eps figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0303043 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0303043 | |
| dc.identifier | Phys.Lett.B565:176-182,2003 | |
| dc.identifier | doi:10.1016/S0370-2693(03)00765-2 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/177559 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | Supersymmetric Dark Matter in Light of WMAP | |
| dc.type | text |