Direct and Indirect Detection of Neutralino Dark Matter In Selected Supersymmetry Breaking Scenarios
arXiv:hep-ph/0309036 · doi:10.1103/PhysRevD.69.035001
Abstract
Various methods of searching for supersymmetric dark matter are sensitive to WIMPs with different properties. One consequence of this is that the phenomenology of dark matter detection can vary dramatically in different supersymmetric breaking scenarios. In this paper, we consider the sensitivities to supersymmetric dark matter of different detection methods and techniques in a wide variety of supersymmetric breaking scenarios. We discuss the ability of various astrophysical experiments, such as direct experiments, gamma-rays satellites, neutrino telescopes and positron and anti-proton cosmic ray experiments, to test various supersymmetry breaking scenarios. We also discuss what information can be revealed about supersymmetry breaking by combining results from complementary experiments. We place an emphasis on the differences between various experimental techniques.
arXiv comment43 pages, 17 figures
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