Separating the linearized Einstein equations in the background of a Kerr black hole

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1. Verfasser: Mei, Jianwei
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Veröffentlicht: 2023
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author Mei, Jianwei
author_facet Mei, Jianwei
contents The advancement in gravitational wave detection has made it possible to study the nonlinear effects in black hole perturbations, the modeling of which requires the full knowledge of the linear order perturbation of the metric. For the most interesting Kerr background, the conventional practice is to solve the Teukolsky equations for a Weyl scalar, and then the perturbation of the metric components is obtained using an elaborated metric reconstruction scheme, which, however, comes with unwanted restrictions. So it is desirable to separate the linearized Einstein equations in Kerr directly, i.e., without using metric reconstruction. In this work, I present a method that aims to help achieve this goal.
format Preprint
id arxiv_https___arxiv_org_abs_2311_18409
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Separating the linearized Einstein equations in the background of a Kerr black hole
Mei, Jianwei
General Relativity and Quantum Cosmology
High Energy Physics - Theory
The advancement in gravitational wave detection has made it possible to study the nonlinear effects in black hole perturbations, the modeling of which requires the full knowledge of the linear order perturbation of the metric. For the most interesting Kerr background, the conventional practice is to solve the Teukolsky equations for a Weyl scalar, and then the perturbation of the metric components is obtained using an elaborated metric reconstruction scheme, which, however, comes with unwanted restrictions. So it is desirable to separate the linearized Einstein equations in Kerr directly, i.e., without using metric reconstruction. In this work, I present a method that aims to help achieve this goal.
title Separating the linearized Einstein equations in the background of a Kerr black hole
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2311.18409