Abstract
Abstract The indirect detection of particle dark matter (DM) is based on the search for anomalous components in cosmic rays (CRs) due to the annihilation of DM pairs in the galactic halo, on the top of the standard astrophysical production. We revise here the most recent results on the DM searches for γ -rays, antiprotons, antideuterons and positrons in CRs.
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