Black hole horizons must be veiled by photon spheres
Ra\'ul Carballo-Rubio, Astrid Eichhorn

TL;DR
This paper proves that black holes with horizons necessarily have photon spheres, and that observing photon rings is crucial for confirming horizons, with implications for interpreting black hole images.
Contribution
It provides a geometric proof linking horizons to photon spheres and extends the argument to more general spacetimes with modified light propagation.
Findings
Bound photon orbits must exist around horizons in spherically symmetric spacetimes.
Non-observation of photon rings strongly suggests the absence of a horizon.
The proof extends to axisymmetric spacetimes with reflection symmetry.
Abstract
Horizons and bound photon orbits are defining features of black holes that translate into key features of black hole images. We present a purely geometric proof that spherically symmetric, isolated objects with horizons in gravity theories with null-geodesic propagation of light must display bound photon orbits forming a photon sphere. Identifying the key elements of the proof, we articulate a simpler argument that carries over to more general situations with modified light propagation and implies the existence of equatorial spherical photon orbits in axisymmetric spacetimes with reflection symmetry. We conclude that the \emph{non-}observation of photon rings with very-large-baseline interferometry would be a very strong indication against a horizon, irrespective of whether or not the image shows a central brightness depression.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Experimental and Theoretical Physics Studies · Relativity and Gravitational Theory
