  We analyze the rate of detection of minimal supersymmetric neutralino dark
matter in germanium, sapphire and sodium iodide detectors, imposing
cosmological and recent accelerator bounds including those from \bsg\ decay. We
find, in contrast with several other recent analyses, that although the \bsg\
constraint reduces the number of viable models, models still remain where the
counting rate in solid state detectors exceeds 10 kg$^{-1}$ day$^{-1}$.
