Parametrized quasinormal mode framework for modified Teukolsky equations

Modifications to general relativity lead to effects in the spectrum of quasinormal modes of black holes. In this paper, we develop a parametrized formalism to describe deviations from general relativity in the Teukolsky equation, which governs linear perturbations of spinning black holes. We do this by introducing a correction to the effective potential of the Teukolsky equation in the form of a $1/r$ expansion controlled by free parameters. The method assumes that a small deviation in the effective potential induces a small modification in the spectrum of modes and in the angular separation constants. We isolate and compute the universal linear contribution to the quasinormal mode frequencies and separation constants in a set of coefficients and test them against known examples in the literature (massive scalar field, Dudley-Finley equation and higher-derivative gravity). We make the coefficients publicly available for relevant overtone, angular momentum, and azimuthal numbers of modes and different values of the black hole spin.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-11-05
DOI
https://doi.org/10.1103/physrevd.110.104007
Citations
17
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
5.64

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article

Parametrized quasinormal mode framework for modified Teukolsky equations

Pablo A. Cano, S. Maenaut, Sebastian H. Völkel, Lodovico Capuano et al.
17 citations
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
5.64
article

Parametrized quasinormal mode framework for modified Teukolsky equations

Pablo A. Cano, S. Maenaut, Sebastian H. Völkel, Lodovico Capuano, Nicola Franchini
article en
17 citations

Abstract

Modifications to general relativity lead to effects in the spectrum of quasinormal modes of black holes. In this paper, we develop a parametrized formalism to describe deviations from general relativity in the Teukolsky equation, which governs linear perturbations of spinning black holes. We do this by introducing a correction to the effective potential of the Teukolsky equation in the form of a $1/r$ expansion controlled by free parameters. The method assumes that a small deviation in the effective potential induces a small modification in the spectrum of modes and in the angular separation constants. We isolate and compute the universal linear contribution to the quasinormal mode frequencies and separation constants in a set of coefficients and test them against known examples in the literature (massive scalar field, Dudley-Finley equation and higher-derivative gravity). We make the coefficients publicly available for relevant overtone, angular momentum, and azimuthal numbers of modes and different values of the black hole spin.

Physical review. D/Physical review. D.Vol. 110(10)
Scuola Internazionale Superiore di Studi Avanzati (IT), University of Trieste (IT), Université Paris Cité (FR), Institut Català de Ciències del Clima (ES), Max Planck Institute for Gravitational Physics (DE), Istituto Nazionale di Fisica Nucleare, Sezione di Trieste (IT), Institute for Fundamental Physics of the Universe (IT), Universitat de Barcelona (ES), KU Leuven (BE)
“la Caixa” Foundation, European Commission, Deutsche Forschungsgemeinschaft, Vlaamse Interuniversitaire Raad, Fundación Bancaria Caixa d'Estalvis i Pensions de Barcelona, Horizon 2020 Framework Programme, H2020 European Research Council, H2020 Marie Skłodowska-Curie Actions
Openalex Percentile: Top 4%
Pulsars and Gravitational Waves Research
5.64
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