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Communication Dans Un Congrès Année : 2017

Gamma-ray signatures of Dark Matter

Résumé

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.

Dates et versions

hal-01833792 , version 1 (10-07-2018)

Identifiants

Citer

Marco Cirelli. Gamma-ray signatures of Dark Matter. 6th Roma International Workshop on Astroparticle Physics, Jun 2016, Rome, Italy. pp.01004, ⟨10.1051/epjconf/201713601004⟩. ⟨hal-01833792⟩
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