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We perform an indirect search for Weakly Interacting Massive Particles(WIMPs) using the MACRO detector to look for neutrino-induced upward-goingmuons resulting from the annihilation of WIMPs trapped in the Sun and Earth.The search is conducted in various angular cones centered on the Sun and Earthto accommodate a range of WIMP masses. No significant excess over thebackground from atmospheric neutrinos is seen and limits are placed on theupward-going muon fluxes from Sun and Earth. These limits are used to constrainneutralino particle parameters from supersymmetric theory, including thosesuggested by recent results from DAMA/NaI.Comment: 14 pages, 7 figures, submitted to Phys. Rev.

Limits on dark matter WIMPs using upward-going muons in the MACRO detector