$B_s \to μ^+ μ^-$ and the upward-going muon flux from the WIMP annihilation in the sun or the earth

Details $B_s \to μ^+ μ^-$ and the upward-going muon flux from the WIMP annihilation in the sun or the earth $B_s \to μ^+ μ^-$ and the upward-going muon flux from the WIMP annihilation in the sun or the earth

2005-06-13

arxiv.org/abs/hep-ph/0506115v1

JHEP0511:007,2005

Physics

High Energy Physics

High Energy Physics - Phenomenology

1+13 pages, 5 figures

Scientific paper

10.1088/1126-6708/2005/11/007

We consider the upward-going muon flux due to the WIMP annihilations in the cores of the sun and the earth, including the upper bound on the branching ratio for $B_s \to \mu^+ \mu^-$ decay. We find that the constraint from $B_s \to \mu^+ \mu^-$ is very strong in most parameter space, and exclude the supergravity parameter space regions where the expected upward-going muon fluxes are within the expected reach of AMANDA II.

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