Constraints on the parameters of keV-scale mass annihilating Dark Matter obtained with SRG/ART-XC observations

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Hauptverfasser: Zakharov, E. I., Barinov, V. V., Burenin, R. A., Gorbunov, D. S., Krivonos, R. A.
Format: Preprint
Veröffentlicht: 2024
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author Zakharov, E. I.
Barinov, V. V.
Burenin, R. A.
Gorbunov, D. S.
Krivonos, R. A.
author_facet Zakharov, E. I.
Barinov, V. V.
Burenin, R. A.
Gorbunov, D. S.
Krivonos, R. A.
contents In this paper we present new constraints on the velocity-independent cross section of keV-scale mass annihilating Dark Matter particles obtained with SRG/ART-XC after 4 full-sky surveys. These constraints are derived from observations of the Milky Way Halo, 33 Local Group spheroidal dwarf (dSph) galaxies and separately for the dSph galaxy Ursa Major III/UNIONS 1. The constraints from the Milky Way Halo are the strongest among others and among all available in literature for this class of Dark Matter models with particle masses from 4 to 15 keV.
format Preprint
id arxiv_https___arxiv_org_abs_2407_18371
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Constraints on the parameters of keV-scale mass annihilating Dark Matter obtained with SRG/ART-XC observations
Zakharov, E. I.
Barinov, V. V.
Burenin, R. A.
Gorbunov, D. S.
Krivonos, R. A.
High Energy Astrophysical Phenomena
Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
In this paper we present new constraints on the velocity-independent cross section of keV-scale mass annihilating Dark Matter particles obtained with SRG/ART-XC after 4 full-sky surveys. These constraints are derived from observations of the Milky Way Halo, 33 Local Group spheroidal dwarf (dSph) galaxies and separately for the dSph galaxy Ursa Major III/UNIONS 1. The constraints from the Milky Way Halo are the strongest among others and among all available in literature for this class of Dark Matter models with particle masses from 4 to 15 keV.
title Constraints on the parameters of keV-scale mass annihilating Dark Matter obtained with SRG/ART-XC observations
topic High Energy Astrophysical Phenomena
Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2407.18371