https://doi.org/10.1051/epjconf/201713601004
Gamma-ray signatures of Dark Matter
Laboratoire de Physique Théorique et Hautes Energies (LPTHE), UMR 7589 CNRS & UPMC, 4 Place Jussieu, F-75252, Paris, France
a e-mail: marco.cirelli@gmail.com
Published online: 23 March 2017
I review the ways in which Dark Matter can produce gamma-rays (and lower energy photons) and I apply the considerations to three specific examples: the tests of multi-TeV pure-WIMP candidates based on high energy gamma-rays from the Galactic Center or dwarfs, the importance of bremsstrahlung emission for light DM, the updated constraints on DM from all-sky radio surveys of the Milky Way.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
