The Nonlinear Tails in Black Hole Ringdown: the Scattering Perspective

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Hauptverfasser: Ianniccari, A., Bianco, L. Lo, Riotto, A.
Format: Preprint
Veröffentlicht: 2025
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author Ianniccari, A.
Bianco, L. Lo
Riotto, A.
author_facet Ianniccari, A.
Bianco, L. Lo
Riotto, A.
contents Black holes regain their static configuration by emitting ringdown gravitational waves, whose amplitude decays in time following a power law at fixed spatial positions. We show that the nonlinear decay power law may be obtained by simple scattering calculations using the in-in formalism and argue that the nonperturbative law should be $t^{-2\ell-1}$, where $\ell$ is the multipole of the propagating spherical gravitational wave.
format Preprint
id arxiv_https___arxiv_org_abs_2507_17732
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The Nonlinear Tails in Black Hole Ringdown: the Scattering Perspective
Ianniccari, A.
Bianco, L. Lo
Riotto, A.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Black holes regain their static configuration by emitting ringdown gravitational waves, whose amplitude decays in time following a power law at fixed spatial positions. We show that the nonlinear decay power law may be obtained by simple scattering calculations using the in-in formalism and argue that the nonperturbative law should be $t^{-2\ell-1}$, where $\ell$ is the multipole of the propagating spherical gravitational wave.
title The Nonlinear Tails in Black Hole Ringdown: the Scattering Perspective
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2507.17732