  Theories of dark matter that support bound states are an intriguing
possibility for the identity of the missing mass of the Universe. This article
proposes a class of models of supersymmetric composite dark matter where the
interactions with the Standard Model communicate supersymmetry breaking to the
dark sector. In these models supersymmetry breaking can be treated as a
perturbation on the spectrum of bound states. Using a general formalism, the
spectrum with leading supersymmetry effects is computed without specifying the
details of the binding dynamics. The interactions of the composite states with
the Standard Model are computed and several benchmark models are described.
General features of non-relativistic supersymmetric bound states are
emphasized.
