Gamma-ray signatures of Dark Matter

Abstract : 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.
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Communication dans un congrès
6th Roma International Workshop on Astroparticle Physics, Jun 2016, Rome, Italy. EPJ Web Conf., 136, pp.01004, 2017, 〈10.1051/epjconf/201713601004〉
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Soumis le : mardi 10 juillet 2018 - 01:12:52
Dernière modification le : jeudi 12 juillet 2018 - 01:29:59

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Marco Cirelli. Gamma-ray signatures of Dark Matter. 6th Roma International Workshop on Astroparticle Physics, Jun 2016, Rome, Italy. EPJ Web Conf., 136, pp.01004, 2017, 〈10.1051/epjconf/201713601004〉. 〈hal-01833792〉

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