Dark Fluxes from Accreting Black Holes and Direct Detections

Understand

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.