Document Type
Article
Publication Date
3-21-2022
Publication Title
The European Physical Journal C
First page number:
1
Last page number:
14
Abstract
We discuss the possibility that accreting black hole systems can be sources for dark matter flux through several different mechanisms. We firstly discuss two types of systems‘: coronal thermal plasmas around supermassive black holes in active galactic nuclei (AGNs), and accretion disks of stellar-mass X-ray black hole binaries (BHBs). We explore how these black hole systems may produce keV light dark matter fluxes and find that the dark fluxes from those sources might be too weak to account for the current XENON1T excess. On the other hand, black holes can be good accelerators to accrete and boost heavy dark matter particles. If considering collisions or dark electromagnetism, those particles can then escape and reach the benchmark speed of 0.1c at the detector. We also extend the black hole mass region to primordial black holes (PBHs) and discuss the possibility of contributing to keV light dark flux via superradiance of PBHs.
Controlled Subject
Black holes (Astronomy);Dark matter (Astronomy);Astronomy
Disciplines
Astrophysics and Astronomy
File Format
File Size
1085 KB
Language
English
Rights
IN COPYRIGHT. For more information about this rights statement, please visit http://rightsstatements.org/vocab/InC/1.0/
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 International License.
Repository Citation
Cai, R.,
Sun, S.,
Zhang, B.,
Zhang, Y.
(2022).
Dark Fluxes From Accreting Black Holes Through Several Mechanisms.
The European Physical Journal C
1-14.
http://dx.doi.org/10.1140/epjc/s10052-022-10173-8