Photon rings of spherically symmetric black holes and robust tests of non-Kerr metrics
Maciek Wielgus

TL;DR
This paper analyzes photon ring structures around spherically symmetric black holes to explore how these features can enable more robust, less model-dependent tests of General Relativity and the Kerr hypothesis.
Contribution
The study compares photon ring structures across various spherically symmetric black hole spacetimes, highlighting their potential for testing spacetime metrics independently of astrophysical source models.
Findings
Photon rings depend mainly on spacetime geometry, not source structure.
Photon ring diameters can be used to probe black hole metrics.
Comparison with Kerr black holes shows potential for testing GR.
Abstract
Under very general assumptions on the accretion flow geometry, images of a black hole illuminated by electromagnetic radiation display a sequence of photon rings (demagnified and rotated copies of the direct image) which asymptotically approach a purely theoretical critical curve - the outline of the black hole photon shell. To a distant observer, these images appear dominated by the direct emission, which forms a ring whose diameter is primarily determined by the effective radius of the emitting region. For that reason, connecting the image diameter seen by a distant observer to the properties of the underlying spacetime crucially relies on a calibration that necessarily depends on the assumed astrophysical source model. On the other hand, the diameter of the photon rings depends more on the detailed geometry of the spacetime than on the source structure. As such, a photon ring…
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.
