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Dark matter particles could be the major component of the haloes of galaxies.Their mutual annihilations or decays would produce an indirect signature underthe form of high-energy cosmic-rays. The focus of this presentation is onantimatter species, a component so rare that any excess over the backgroundshould be easily detected. After a recap on Galactic propagation, I willdiscuss positrons, antiprotons and anti-nuclei. For each of these species,anomalies have been reported. The antiproton excess, for instance, is currentlya hot topic. Alas, it does not resist a correct treatment of theoretical anddata errors.

What charged cosmic rays tell us on dark matter