Abstract
Dark matter particles could self-annihilate or decay producing a flux of antimatter particles, gamma-rays or neutrinos which could be observed as an excess over their expected astrophysical backgrounds, opening the possibility of indirectly detecting dark matter. In this paper, we will review the calculation of the expected fluxes of Standard Model particles produced in the annihilation or the decay of dark matter particles, as well as the limits on the dark matter properties which follow from observations.
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