Limits on direct detection of neutralino dark matter from b -> s gamma decays

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dc.creatorBergstrom, L.
dc.creatorGondolo, P.
dc.date1995-10-09
dc.date.accessioned2026-07-07T10:35:13Z
dc.date.available2026-07-07T10:35:13Z
dc.descriptionWe 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$^{-1}$.
dc.descriptionuuencoded, gzipped postscript (17 pages), figures available at http://vanosf.physto.se/lbe/bg_figs.uu
dc.identifierhttps://arxiv.org/abs/hep-ph/9510252
dc.identifierhttp://arxiv.org/abs/hep-ph/9510252
dc.identifierAstropart.Phys.5:263-278,1996
dc.identifierdoi:10.1016/0927-6505(96)00027-8
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179686
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleLimits on direct detection of neutralino dark matter from b -> s gamma decays
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