| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8182375 | Nuclear and Particle Physics Proceedings | 2017 | 5 Pages |
Abstract
Detection of gamma rays and cosmic rays from the annihilation or decay of dark matter particles is a promising method for identifying dark matter, understanding its intrinsic properties, and mapping its distribution in the universe. I will review recent results from the Fermi Gamma-ray Space Telescope and other space-based experiments, and highlight the constraints these currently place on particle dark matter models. I will also discuss the prospects for indirect searches to robustly identify or exclude a dark matter signal using upcoming experiments at energies below Fermi (ASTROGAM) and above Fermi, Magic and H.E.S.S. (CTA, LHAASO).
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Aldo Morselli,