arXiv:hep-ph/0303043·v1·High Energy Physics — Phenomenology
Supersymmetric Dark Matter in Light of WMAP
J. Ellis (CERN)🇨🇭 · K.A. Olive (FTPI, U of Minnesota)🇺🇸 · Y. Santoso (FTPI, U of Minnesota)🇺🇸 · V.C. Spanos (FTPI, U of Minnesota)🇺🇸
Abstract
We re-examine the parameter space of the constrained minimal supersymmetric extension of the Standard Model (CMSSM), taking account of the restricted range of \Omega_{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_\chi < 500 GeV for \tan \beta < 45 and \mu > 0, or \tan \beta < 30 and \mu < 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.
Comments: 12 pages LaTeX, 7 eps figures