Marco Cirelli and his collaborators (mostly based at CERN, in Estonia and in Italy) had published back in 2010 a complete set of numerical products for Dark Matter Indirect Detection. This work is increasingly used by the community and it is becoming, for some aspects, the state-of-the-art set of tools for this domain.
Since several decades, cosmological and astrophysical evidence accumulate on the existence of Dark Matter (DM), thanks to its gravitational influence at different scales, showing that it constitutes 80% of the matter in the Universe. On the other hand, an explicit (non- gravitational) manifestation of DM is yet to be identified as its nature is as elusive as ever. One of the most promising approaches to solve this mystery is Indirect Detection, which aims to unravel the possible excess in cosmic rays produced by the annihilations or decay of DM particles in the Galaxy or beyond.
More