Radiative $b$ Decays and the Detection of Supersymmetric Dark Matter

Details Radiative $b$ Decays and the Detection of Supersymmetric Dark Matter Radiative $b$ Decays and the Detection of Supersymmetric Dark Matter

1995-03-09

arxiv.org/abs/hep-ph/9503283v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

To appear in Proceedings of Beyond the Standard Model IV, Lake Tahoe, California, Dec. 1994. Latex, 6 pages, uses epsf.sty to

Scientific paper

The upper bond on the branching ratio for $b\to s\gamma$ decays implies a stringent lower bound on the mass of the pseudoscalar Higgs boson of the MSSM if sparticles are heavy. This leads to an upper bound on the expected event rate in experiments searching for heavy supersymmetric dark matter. Scenarios with lighter sparticle spectrum and light pseudoscalar Higgs boson are still possible, but only if $\mu < 0$, which again implies a small LSP counting rate.

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