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Event rates for dark matter detectors in neutralino--nucleus scattering arestudied for supergravity unified models, including the constraint arising fromthe $b\rightarrow s\gamma$ experiment. The recent experimental measurement ofthis decay by the CLEO Collaboration leads to strong constraints on the SUSYparticle spectrum,and also significantly affects the event rates in dark matterdetectors. The analysis given here uses the accurate method for the computationof the relic density and leads to a dip in the event rate when the neutralinomass is $\sim M_Z/2$ due to the $Z$-pole, and similar results hold when theneutralino mass is $\sim m_h/2$ due to the Higgs pole . Implication of theseresults for dark matter detectors are discussed.Comment: 9 pages Latex+1page of figs(hard copy available on  request),CERN-TH.7363/94, NUB-TH-3099/94,CTP-TAMU-38/9

physical review letters

Event Rates in Dark Matter Detectors for Neutralinos Including Constraints from<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">b</mml:mi><mml:mi mathvariant="italic" /><mml:mo>→</mml:mo><mml:mi /><mml:mi mathvariant="italic">s</mml:mi><mml:mi>γ</mml:mi></mml:math>Decay

Event Rates in Dark Matter Detectors for Neutralinos Including Constraints fromb→sγDecay