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

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

1995-10-09

arxiv.org/abs/hep-ph/9510252v1

Astropart.Phys.5:263-278,1996

Physics

High Energy Physics

High Energy Physics - Phenomenology

uuencoded, gzipped postscript (17 pages), figures available at http://vanosf.physto.se/lbe/bg_figs.uu

Scientific paper

10.1016/0927-6505(96)00027-8

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$^{-1}$.

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