SUSY dark matter: implications for collider searches and direct and indirect DM detection

Abstract

The minimal supergravity model (mSUGRA) has become severely constrained by the WMAP determination of Ω CDM h 2, BF(b → sγ) and (g − 2) μ. We determine the favored remaining regions of model parameter space, and their consequences for future searches for SUSY dark matter (DM) at colliders. We also exhibit regions of parameter space where direct detection of SUSY DM can occur. Finally, we note which regions are open to indirect searches for SUSY DM via neutrino telescope searches, or via observation of γs, e +s or p ¯ s from neutralino annihilation in the galactic core or halo.