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Abstract: A brief review of the indirect detection signatures of dark matter is given.In particular, detection methods of dark matter particle annihilation toantimatter and gamma-rays are reviewed. With the GLAST satellite soon to belaunched, a crucial window in the energy range of a few GeV up to 300 GeV willopen. The good angular and energy resolution of the instrument means thatstructures predicted by cold dark matter models can be searched for. Large,currently planned ground-based imaging Cherenkov telescope arrays, may furtherimprove the limits, or discover a signal, if the current understanding of halodark matter structure is correct.

Autor: Lars Bergstrom


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