Photon Rings Around Warped Black Holes
Daniel Kapec, Alexandru Lupsasca, Andrew Strominger

TL;DR
This paper investigates the photon ring structure around warped black holes, demonstrating how classical and quantum resonances relate through holography, and providing an exactly solvable model that links geometric optics, quasinormal modes, and emergent symmetries.
Contribution
It presents an exactly solvable warped AdS3 black hole model that connects photon rings, quasinormal modes, and holographic dualities, revealing the role of symmetries and resonances.
Findings
Geometric optics reproduces the eikonal limit of QNM spectrum.
Emergent conformal symmetry relates to photon ring structure.
Photon ring spectrum matches quantum Ruelle resonances in holographic context.
Abstract
The black hole photon ring is a prime target for upcoming space-based VLBI missions seeking to image the fine structure of astrophysical black holes. The classical Lyapunov exponents of the corresponding nearly bound null geodesics control the quasinormal ringing of a perturbed black hole as it settles back down to equilibrium, and they admit a holographic interpretation in terms of quantum Ruelle resonances of the microstate dual to the Kerr black hole. Recent work has identified a number of emergent symmetries related to the intricate self-similar structure of the photon ring. Here, we explore this web of interrelated phenomena in an exactly soluble example that arises as an approximation to the near-extremal Kerr black hole. The self-dual warped AdS geometry has a photon ring as well as isometries and an exactly calculable quasinormal mode (QNM)…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Black Holes and Theoretical Physics · Pulsars and Gravitational Waves Research
