Sub-GeV dark matter and X-rays

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URI: https://hdl.handle.net/10902/31501
ISSN: 1824-8039
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Autoría
Cirelli, Marco; Fornengo, Nicolao; Kavanagh, Bradley James; Pinettia, Elena
Fecha
2022
Derechos
Attribution-NonCommercial-NoDerivatives 4.0 International © Los autores
Publicado en
PoS - Proceedings of Science, 2022, 406, 096
Editorial
Sissa Medialab
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Resumen/Abstract
We present bounds on Dark Matter (DM) in the MeV to GeV mass range, obtained by using X-ray measurements from the Integral telescope. A crucial element, that allows us to derived bounds competitive or stronger than existing ones from other techniques, resides in the inclusion of the contribution from inverse Compton scattering on galactic radiation fields and on the CMB. This contribution is based on [1], to which we refer for additional details
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Attribution-NonCommercial-NoDerivatives 4.0 International © Los autoresExcepto si se señala otra cosa, la licencia del ítem se describe como Attribution-NonCommercial-NoDerivatives 4.0 International © Los autores