Quantum cross-section of near-extremal black holes

Abstract We explore how to detect the large quantum fluctuations in the throat of a near-extremal black hole, where the dynamics are governed by the Schwarzian theory. To this end, we scatter a low-frequency wave of a massless, minimal scalar off the black hole and calculate the absorption cross-sec...

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Main Author: Roberto Emparan
Format: Article
Language:English
Published: SpringerOpen 2025-04-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP04(2025)122
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author Roberto Emparan
author_facet Roberto Emparan
author_sort Roberto Emparan
collection DOAJ
description Abstract We explore how to detect the large quantum fluctuations in the throat of a near-extremal black hole, where the dynamics are governed by the Schwarzian theory. To this end, we scatter a low-frequency wave of a massless, minimal scalar off the black hole and calculate the absorption cross-section. In the semiclassical regime, where the Schwarzian is weakly coupled, we recover the universal result that the cross-section equals the horizon area. However, in the strongly coupled regime, where quantum fluctuations dominate, we find that the absorption cross-section exceeds the semiclassical prediction. This result may seem counterintuitive, given that the density of black hole states is suppressed in this regime. Nevertheless, two effects outweigh this suppression. First, quantum fluctuations enhance absorption transitions between individual states, with the effect becoming stronger closer to the ground state. Second, these fluctuations significantly reduce stimulated emission. We conclude that a measurement showing an enhanced absorption cross-section serves as a clear signature of the large quantum fluctuations in the geometry.
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spelling doaj-art-b7c18e3ef86d4197a6e218c80810f4d62025-08-20T01:49:33ZengSpringerOpenJournal of High Energy Physics1029-84792025-04-012025411610.1007/JHEP04(2025)122Quantum cross-section of near-extremal black holesRoberto Emparan0Institució Catalana de Recerca i Estudis Avançats (ICREA)Abstract We explore how to detect the large quantum fluctuations in the throat of a near-extremal black hole, where the dynamics are governed by the Schwarzian theory. To this end, we scatter a low-frequency wave of a massless, minimal scalar off the black hole and calculate the absorption cross-section. In the semiclassical regime, where the Schwarzian is weakly coupled, we recover the universal result that the cross-section equals the horizon area. However, in the strongly coupled regime, where quantum fluctuations dominate, we find that the absorption cross-section exceeds the semiclassical prediction. This result may seem counterintuitive, given that the density of black hole states is suppressed in this regime. Nevertheless, two effects outweigh this suppression. First, quantum fluctuations enhance absorption transitions between individual states, with the effect becoming stronger closer to the ground state. Second, these fluctuations significantly reduce stimulated emission. We conclude that a measurement showing an enhanced absorption cross-section serves as a clear signature of the large quantum fluctuations in the geometry.https://doi.org/10.1007/JHEP04(2025)122Black HolesBlack Holes in String Theory2D Gravity
spellingShingle Roberto Emparan
Quantum cross-section of near-extremal black holes
Journal of High Energy Physics
Black Holes
Black Holes in String Theory
2D Gravity
title Quantum cross-section of near-extremal black holes
title_full Quantum cross-section of near-extremal black holes
title_fullStr Quantum cross-section of near-extremal black holes
title_full_unstemmed Quantum cross-section of near-extremal black holes
title_short Quantum cross-section of near-extremal black holes
title_sort quantum cross section of near extremal black holes
topic Black Holes
Black Holes in String Theory
2D Gravity
url https://doi.org/10.1007/JHEP04(2025)122
work_keys_str_mv AT robertoemparan quantumcrosssectionofnearextremalblackholes