New Directions in the Search for Dark Matter
  The identification of the nature of dark matter is one of the most important
problems confronting particle physics. Current observational constraints permit
the mass of the dark matter to range from $10^{-22}$ eV - $10^{48}$ GeV. Given
the weak nature of these bounds and the ease with which dark matter models can
be constructed, it is clear that the problem can only be solved experimentally.
In these lectures, I discuss methods to experimentally probe a wide range of
dark matter candidates.
