Unique probe of dark matter in the core of M87 with the Event Horizon Telescope
Thomas Lacroix, Mansour Karami, Avery E. Broderick, Joseph Silk, and, Celine Boehm

TL;DR
This paper demonstrates that the Event Horizon Telescope can image and constrain dark matter profiles near supermassive black holes, revealing potential dark matter spikes and providing new insights into dark matter properties through high-resolution observations.
Contribution
The study introduces the first model of dark matter annihilation-induced synchrotron emission near a supermassive black hole, accounting for gravitational lensing and matching EHT data.
Findings
EHT can resolve dark matter spikes if present.
Dark matter emission fits existing EHT data.
Current observations constrain dark matter annihilation cross sections.
Abstract
We demonstrate the unprecedented capabilities of the Event Horizon Telescope (EHT) to image the innermost dark matter profile in the vicinity of the supermassive black hole at the center of the M87 radio galaxy. We present the first model of the synchrotron emission induced by dark matter annihilations from a spiky profile in the close vicinity of a supermassive black hole, accounting for strong gravitational lensing effects. Our results show that the EHT should readily resolve dark matter spikes if present. Moreover, the photon ring surrounding the silhouette of the black hole is clearly visible in the spike emission, which introduces observable small-scale structure into the signal. We find that the dark matter-induced emission provides an adequate fit to the existing EHT data, implying that in addition to the jet, a dark matter spike may account for a sizable portion of the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
