  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.
