Correspondence between grey-body factors and quasinormal frequencies for rotating black holes

Fuente: arXiv
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Main Authors: Konoplya, R. A., Zhidenko, A.
Format: Preprint
Published: 2024
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author Konoplya, R. A.
Zhidenko, A.
author_facet Konoplya, R. A.
Zhidenko, A.
contents Although the proper oscillation frequencies of black holes (quasinormal modes) and the grey-body factors, which determine the scattering properties of black holes, represent two distinct spectral problems with different boundary conditions, a recent study has revealed an intrinsic connection between these quantities. We have shown that the correspondence between grey-body factors and quasinormal modes, previously established for spherically symmetric and asymptotically flat black holes, also extends to general parametrized axially symmetric black holes. This correspondence is limited to non-superradiant waves.
format Preprint
id arxiv_https___arxiv_org_abs_2408_11162
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Correspondence between grey-body factors and quasinormal frequencies for rotating black holes
Konoplya, R. A.
Zhidenko, A.
General Relativity and Quantum Cosmology
Although the proper oscillation frequencies of black holes (quasinormal modes) and the grey-body factors, which determine the scattering properties of black holes, represent two distinct spectral problems with different boundary conditions, a recent study has revealed an intrinsic connection between these quantities. We have shown that the correspondence between grey-body factors and quasinormal modes, previously established for spherically symmetric and asymptotically flat black holes, also extends to general parametrized axially symmetric black holes. This correspondence is limited to non-superradiant waves.
title Correspondence between grey-body factors and quasinormal frequencies for rotating black holes
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2408.11162