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Bibliographic Details
Main Author: Stucker, Thomas
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2407.04612
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author Stucker, Thomas
author_facet Stucker, Thomas
contents We provide a rigorous definition of quasinormal modes for the Kerr black hole. They are obtained as the discrete set of poles of the meromorphically continued cutoff resolvent. The construction combines the method of complex scaling near asymptotically flat infinity with microlocal methods near the black hole horizon. We study the distribution of quasinormal modes in both the high and low energy regimes. We establish the existence of a high energy spectral gap and exclude the accumulation of quasinormal modes at zero energy.
format Preprint
id arxiv_https___arxiv_org_abs_2407_04612
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Quasinormal modes for the Kerr black hole
Stucker, Thomas
Analysis of PDEs
General Relativity and Quantum Cosmology
Spectral Theory
We provide a rigorous definition of quasinormal modes for the Kerr black hole. They are obtained as the discrete set of poles of the meromorphically continued cutoff resolvent. The construction combines the method of complex scaling near asymptotically flat infinity with microlocal methods near the black hole horizon. We study the distribution of quasinormal modes in both the high and low energy regimes. We establish the existence of a high energy spectral gap and exclude the accumulation of quasinormal modes at zero energy.
title Quasinormal modes for the Kerr black hole
topic Analysis of PDEs
General Relativity and Quantum Cosmology
Spectral Theory
url https://arxiv.org/abs/2407.04612