Gamma-ray signatures of Dark Matter

Gamma-ray signatures of Dark Matter

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 emissio...

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Main Author: Cirelli Marco
Format: Article
Language:English
Published: EDP Sciences 2017-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201713601004
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spelling doaj-fe47eb78a5e7452aa437f2deb4a9b0fb2021-08-02T01:19:53ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011360100410.1051/epjconf/201713601004epjconf_ricap2017_01004Gamma-ray signatures of Dark MatterCirelli Marco0Laboratoire de Physique Théorique et Hautes Energies (LPTHE), UMR 7589 CNRS & UPMCI 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.https://doi.org/10.1051/epjconf/201713601004
collection DOAJ
language English
format Article
sources DOAJ
author Cirelli Marco
spellingShingle Cirelli Marco
Gamma-ray signatures of Dark Matter
EPJ Web of Conferences
author_facet Cirelli Marco
author_sort Cirelli Marco
title Gamma-ray signatures of Dark Matter
title_short Gamma-ray signatures of Dark Matter
title_full Gamma-ray signatures of Dark Matter
title_fullStr Gamma-ray signatures of Dark Matter
title_full_unstemmed Gamma-ray signatures of Dark Matter
title_sort gamma-ray signatures of dark matter
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2017-01-01
description 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.
url https://doi.org/10.1051/epjconf/201713601004
work_keys_str_mv AT cirellimarco gammaraysignaturesofdarkmatter
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