Echoes in the Kerr/CFT correspondence
Ramit Dey, Niayesh Afshordi

TL;DR
This paper explores how quantum modifications near a black hole horizon can be understood through the Kerr/CFT correspondence, predicting observable echoes in gravitational wave signals and relating them to dual CFT parameters.
Contribution
It introduces a dual CFT perspective on near-horizon quantum effects in Kerr-like objects, linking echo delays and reflectivity to CFT modular parameters.
Findings
Quantum effects modify black hole near-horizon structure as finite size/N effects in CFT.
Echo time-delays relate to the CFT circle length and quantum structure position.
Reflectivity of ECO membrane follows a Boltzmann form derived from CFT analysis.
Abstract
The Kerr/CFT correspondence is a possible route to gain insight into the quantum theory of gravity in the near-horizon region of a Kerr black hole via a dual holographic conformal field theory (CFT). Predictions of the black hole entropy, scattering cross-section and the quasi normal modes from the dual holographic CFT corroborate this proposed correspondence. More recently, it has been suggested that quantum gravitational effects in the near-horizon region of a black hole may drastically modify the classical general relativistic description, leading to potential observable consequences. In this paper, we study the absorption cross-section and quasi normal modes of a horizonless Kerr-like exotic compact object (ECO) in the dual CFT picture. Our analysis suggests that the near-horizon quantum modifications of the black hole can be understood as finite size and/or finite effects in…
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