  The DAMA annual modulation signature, interpreted as evidence for a
spin-independent WIMP coupling, seems in conflict with null results from CDMS.
However, in models of ``inelastic dark matter'', the experiments are
compatible. Inelastic dark matter can arise in supersymmetric theories as the
real component of a sneutrino mixed with a singlet scalar. In contrast with
ordinary sneutrino dark matter, such particles can satisfy all experimental
constraints while giving the appropriate relic abundance. We discuss the
modifications to the signal seen at DAMA, in particular noting the strong
suppression of low energy events in both modulated and unmodulated components.
We discuss future experiments, with emphasis on distinguishing inelastic dark
matter from ordinary dark matter, and stressing the significance of experiments
with heavy target nuclei, such as xenon and tungsten.
