In the Cold Dark Matter scenario, the Dark Matter particle candi-date may be a Weakly Interacting Massive Particle (WIMP). Annihilation of twoWIMPs in local or cosmological structures would result in the production of a num-ber of standard model particles such as photons, leptons and baryons which could beobserved with the presently available or future experiments such as the PAMELA orGLAST satellites or the Cherenkov Telescopes. In this work we review the status-of-the-art of the theoretical and phenomenological studies about the possibility ofindirect detection of signals coming from WIMP annihilation.
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