Non-modal effects in black hole perturbation theory: transient superradiance

Abstract We study the non-modal stability of black hole spacetimes under linear perturbations. We show that large-amplitude growth can occur at finite time, despite asymptotic decay of linear perturbations. In the example presented, the physical mechanism is a transient form of superradiance, and is...

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Main Authors: Javier Carballo, Christiana Pantelidou, Benjamin Withers
Format: Article
Language:English
Published: SpringerOpen 2025-08-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP08(2025)179
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author Javier Carballo
Christiana Pantelidou
Benjamin Withers
author_facet Javier Carballo
Christiana Pantelidou
Benjamin Withers
author_sort Javier Carballo
collection DOAJ
description Abstract We study the non-modal stability of black hole spacetimes under linear perturbations. We show that large-amplitude growth can occur at finite time, despite asymptotic decay of linear perturbations. In the example presented, the physical mechanism is a transient form of superradiance, and is qualitatively similar to the transition to turbulence in Navier-Stokes shear flows. As part of the construction we provide a theorem for the positivity of QNM energies, and introduce a truncated-Hamiltonian approach to black hole pseudospectra which does not suffer from convergence issues.
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institution Kabale University
issn 1029-8479
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spelling doaj-art-70c94f1b8bc84a69927ba55a759a02ed2025-08-24T11:04:50ZengSpringerOpenJournal of High Energy Physics1029-84792025-08-012025812810.1007/JHEP08(2025)179Non-modal effects in black hole perturbation theory: transient superradianceJavier Carballo0Christiana Pantelidou1Benjamin Withers2Mathematical Sciences and STAG Research Centre, University of SouthamptonSchool of Mathematics and Statistics, University College DublinMathematical Sciences and STAG Research Centre, University of SouthamptonAbstract We study the non-modal stability of black hole spacetimes under linear perturbations. We show that large-amplitude growth can occur at finite time, despite asymptotic decay of linear perturbations. In the example presented, the physical mechanism is a transient form of superradiance, and is qualitatively similar to the transition to turbulence in Navier-Stokes shear flows. As part of the construction we provide a theorem for the positivity of QNM energies, and introduce a truncated-Hamiltonian approach to black hole pseudospectra which does not suffer from convergence issues.https://doi.org/10.1007/JHEP08(2025)179Black HolesGauge-Gravity CorrespondenceHolography and Hydrodynamics
spellingShingle Javier Carballo
Christiana Pantelidou
Benjamin Withers
Non-modal effects in black hole perturbation theory: transient superradiance
Journal of High Energy Physics
Black Holes
Gauge-Gravity Correspondence
Holography and Hydrodynamics
title Non-modal effects in black hole perturbation theory: transient superradiance
title_full Non-modal effects in black hole perturbation theory: transient superradiance
title_fullStr Non-modal effects in black hole perturbation theory: transient superradiance
title_full_unstemmed Non-modal effects in black hole perturbation theory: transient superradiance
title_short Non-modal effects in black hole perturbation theory: transient superradiance
title_sort non modal effects in black hole perturbation theory transient superradiance
topic Black Holes
Gauge-Gravity Correspondence
Holography and Hydrodynamics
url https://doi.org/10.1007/JHEP08(2025)179
work_keys_str_mv AT javiercarballo nonmodaleffectsinblackholeperturbationtheorytransientsuperradiance
AT christianapantelidou nonmodaleffectsinblackholeperturbationtheorytransientsuperradiance
AT benjaminwithers nonmodaleffectsinblackholeperturbationtheorytransientsuperradiance