Quantum induced superradiance

Superradiance, the phenomenon enabling energy extraction through radiation amplification, is not universal to all black holes. We show that semiclassical backreaction can induce superradiance, even when absent at the classical level. Specifically, we compute the quasinormal modes of a massless scalar field probing a family of rotating “quantum” black holes in three-dimensional anti-de Sitter space, accounting for all orders of backreaction due to quantum conformal matter. A subset of these modes is identified as superradiant, leading to the formation of quantum black hole “bombs.” Further, we find all thermally unstable black holes exhibit modal linear instabilities, though the converse does not hold generally. Our findings thus suggest a semiclassical version of the Hollands-Wald conjecture on black hole stability. This motivates us to propose a stability criterion for quantum black holes.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-08-26
DOI
https://doi.org/10.1103/dhsc-9kk9
Citations
2
Primary Topic
Quantum Electrodynamics and Casimir Effect
Type
article
Field-Weighted Citation Impact
2.49

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article

Quantum induced superradiance

Juan F. Pedraza, Casey Cartwright, Umut Gürsoy, Andrew Svesko
2 citations
Physical review. D/Physical review. D.
Quantum Electrodynamics and Casimir Effect
2.49
article

Quantum induced superradiance

Juan F. Pedraza, Casey Cartwright, Umut Gürsoy, Andrew Svesko
article en
2 citations

Abstract

Superradiance, the phenomenon enabling energy extraction through radiation amplification, is not universal to all black holes. We show that semiclassical backreaction can induce superradiance, even when absent at the classical level. Specifically, we compute the quasinormal modes of a massless scalar field probing a family of rotating “quantum” black holes in three-dimensional anti-de Sitter space, accounting for all orders of backreaction due to quantum conformal matter. A subset of these modes is identified as superradiant, leading to the formation of quantum black hole “bombs.” Further, we find all thermally unstable black holes exhibit modal linear instabilities, though the converse does not hold generally. Our findings thus suggest a semiclassical version of the Hollands-Wald conjecture on black hole stability. This motivates us to propose a stability criterion for quantum black holes.

Physical review. D/Physical review. D.Vol. 112(4)
King's College London (GB), Utrecht University (NL)
Royal Society, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Ministerio de Ciencia e Innovación, Science and Technology Facilities Council, European Regional Development Fund, Agencia Estatal de Investigación
Openalex Percentile: Top 10%
Quantum Electrodynamics and Casimir Effect
2.49
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