  Expected event rates for a number of dark matter nuclear targets were
calculated in the effective low-energy minimal supersymmetric standard model,
provided the lightest neutralino is the dark matter Weakly Interacting Massive
Particle (WIMP). These calculations allow direct comparison of sensitivities of
different dark matter detectors to intermediate mass WIMPs expected from the
measurements of the DArk MAtter (DAMA) experiment.
