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Dark Matter Searches with AMS-02

The Alpha Magnetic Spectrometer (AMS), to be installed on the International Space Station, will provide data on cosmic radiation in a large range of energy from 0.5 GeV to 3 TeV. The main physics goals in the astroparticle domain are the anti-matter and the dark matter searches. Observations indicate that the Universe may include a large amount of unknown Dark Matter. It should be composed of non-baryonic Weakly Interacting Massive Particles (WIMPs), a good WIMP candidate being the lightest supersymmetric particle in R-parity conserving models. AMS offers a unique opportunity to study simultaneously SUSY dark matter in three decay channels from the neutralino annihilation: positrons, antiprotons and gamma rays. The supersymmetric theory frame is considered together with alternative scenarios (extra-dimensions). The expected flux sensitivities in 3 year exposure for the e+/eratio, antiproton and gamma yields as a function of energy are presented.