Hair imprints of the gravitational decoupling and hairy black hole spectroscopy

Fuente: arXiv
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Autori principali: Guimarães, V. F., Cavalcanti, R. T., da Rocha, R.
Natura: Preprint
Pubblicazione: 2025
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author Guimarães, V. F.
Cavalcanti, R. T.
da Rocha, R.
author_facet Guimarães, V. F.
Cavalcanti, R. T.
da Rocha, R.
contents Hairy black holes by gravitational decoupling (GD) are probed to derive the gravitational waveform produced by perturbation theory applied to these compact objects. Using the Regge-Wheeler and Zerilli equations governing the metric perturbations and applying a higher-order WKB method, the quasinormal modes (QNMs) are computed and discussed. Compared to the QNMs produced in the ringdown phase of Reissner-Nordström black hole solutions, it yields a clear physical signature of primary hair imprinting the hairy GD black hole gravitational waveforms.
format Preprint
id arxiv_https___arxiv_org_abs_2506_20044
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Hair imprints of the gravitational decoupling and hairy black hole spectroscopy
Guimarães, V. F.
Cavalcanti, R. T.
da Rocha, R.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Hairy black holes by gravitational decoupling (GD) are probed to derive the gravitational waveform produced by perturbation theory applied to these compact objects. Using the Regge-Wheeler and Zerilli equations governing the metric perturbations and applying a higher-order WKB method, the quasinormal modes (QNMs) are computed and discussed. Compared to the QNMs produced in the ringdown phase of Reissner-Nordström black hole solutions, it yields a clear physical signature of primary hair imprinting the hairy GD black hole gravitational waveforms.
title Hair imprints of the gravitational decoupling and hairy black hole spectroscopy
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2506.20044