Counting Black Hole Microstates at Future Null Infinity

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1. Verfasser: Shajiee, Vahid Reza
Format: Preprint
Veröffentlicht: 2025
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author Shajiee, Vahid Reza
author_facet Shajiee, Vahid Reza
contents We propose a black hole microstate counting method based on the canonical quantization of the asymptotic symmetries of a two-dimensional dilaton-gravity system at future null infinity. This dilaton-gravity is obtained from the s-wave reduction of an $N$-dimensional Einstein gravity over a generic asymptotically flat black hole solution. We show that a Cardy-type formula leads to the Bekenstein-Hawking entropy. In this scenario, the quantized bulk degrees of freedom act as a source for the dual field theory operators living at future null infinity that are soft gravitons of the higher dimensional system, up to some gauge fixing.
format Preprint
id arxiv_https___arxiv_org_abs_2503_03297
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Counting Black Hole Microstates at Future Null Infinity
Shajiee, Vahid Reza
High Energy Physics - Theory
General Relativity and Quantum Cosmology
We propose a black hole microstate counting method based on the canonical quantization of the asymptotic symmetries of a two-dimensional dilaton-gravity system at future null infinity. This dilaton-gravity is obtained from the s-wave reduction of an $N$-dimensional Einstein gravity over a generic asymptotically flat black hole solution. We show that a Cardy-type formula leads to the Bekenstein-Hawking entropy. In this scenario, the quantized bulk degrees of freedom act as a source for the dual field theory operators living at future null infinity that are soft gravitons of the higher dimensional system, up to some gauge fixing.
title Counting Black Hole Microstates at Future Null Infinity
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2503.03297