Scattering Hawking Radiation

Fuente: arXiv
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Auteur principal: Cheng, Peng
Format: Preprint
Publié: 2025
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author Cheng, Peng
author_facet Cheng, Peng
contents We analyze the physical consequences of scattering Hawking radiation emitted in the vicinity of the horizon of a Schwarzschild black hole. The Hawking radiation from the horizon becomes soft at a large distance away from the horizon due to the gravitational redshift, and the above process is exactly the soft theorem in curved spacetime. For an observer located at infinity, such a scattering process introduces a large gauge transformation, which can be regarded as a memory effect. The large gauge transformation is expected to encode more information about the radiation and might shed light on the black hole information paradox.
format Preprint
id arxiv_https___arxiv_org_abs_2507_17313
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Scattering Hawking Radiation
Cheng, Peng
High Energy Physics - Theory
General Relativity and Quantum Cosmology
We analyze the physical consequences of scattering Hawking radiation emitted in the vicinity of the horizon of a Schwarzschild black hole. The Hawking radiation from the horizon becomes soft at a large distance away from the horizon due to the gravitational redshift, and the above process is exactly the soft theorem in curved spacetime. For an observer located at infinity, such a scattering process introduces a large gauge transformation, which can be regarded as a memory effect. The large gauge transformation is expected to encode more information about the radiation and might shed light on the black hole information paradox.
title Scattering Hawking Radiation
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2507.17313