Gravitational Waves on Kerr Black Holes II: Metric Reconstruction with Cosmological Constant

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Berens, Roman, Gravely, Trevor, Lupsasca, Alexandru
Format: Preprint
Publié: 2025
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866914082355937280
author Berens, Roman
Gravely, Trevor
Lupsasca, Alexandru
author_facet Berens, Roman
Gravely, Trevor
Lupsasca, Alexandru
contents In this second paper of our series started with \cite{Berens2024}, we investigate linearized gravitational perturbations of a rotating Kerr black hole in a non-asymptotically flat spacetime with (anti-)de Sitter boundary conditions. Here, we explicitly write down the metric components (in both ingoing and outgoing radiation gauge) of the perturbations that correspond to a given mode of either Weyl scalar. We provide formulas involving Hertz potentials (intermediate quantities with a holographic interpretation) as well as some that involve only the separated radial and angular modes. We expect these analytic results to prove useful in numerical studies of black hole perturbation theory in the context of the holographic correspondence.
format Preprint
id arxiv_https___arxiv_org_abs_2510_07712
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Gravitational Waves on Kerr Black Holes II: Metric Reconstruction with Cosmological Constant
Berens, Roman
Gravely, Trevor
Lupsasca, Alexandru
General Relativity and Quantum Cosmology
In this second paper of our series started with \cite{Berens2024}, we investigate linearized gravitational perturbations of a rotating Kerr black hole in a non-asymptotically flat spacetime with (anti-)de Sitter boundary conditions. Here, we explicitly write down the metric components (in both ingoing and outgoing radiation gauge) of the perturbations that correspond to a given mode of either Weyl scalar. We provide formulas involving Hertz potentials (intermediate quantities with a holographic interpretation) as well as some that involve only the separated radial and angular modes. We expect these analytic results to prove useful in numerical studies of black hole perturbation theory in the context of the holographic correspondence.
title Gravitational Waves on Kerr Black Holes II: Metric Reconstruction with Cosmological Constant
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2510.07712