PREDICTIONS FOR WIMP DETECTION RATES

Ranges of direct detection cross section are presented for the neutralino in the general MSSM and in the CMSSM. Current experimental sensitivity already allows one to exclude some otherwise allowed points in the MSSM, but it is still at least an order of magnitude away from the most likely values of the direct detection cross section predicted in the CMSSM. A new generation of detectors will be able to explore a large fraction of this range.