  Supersymmetric particles represent the best motivated candidates to fill the
Dark Matter gap, and are actively hunted by a number of competing experiments.
Discriminating experiments are testing for the first time SUSY models
compatible with accelerator constraints. These experiments contradict the 60
GeV WIMP candidate reported by the DAMA experiment. The sensitivities of direct
and indirect detection techniques for both present experiments and future
projects are compared.
