Resonance of black hole quasinormal modes in coupled systems

Black hole quasinormal modes (QNMs) can exhibit resonant excitations associated with avoided crossings in their complex frequency spectrum. Such resonance phenomena can serve as novel signatures for probing new physics, where additional degrees of freedom are commonly introduced. Motivated by this possibility, we investigate QNMs in systems where multiple degrees of freedom are coupled with each other and introduce a definition of excitation factors suitable for such systems. To demonstrate our formulation, we apply it to a black hole in the Einstein-Maxwell-axion theory, where we find that avoided crossings can appear even between longest-lived modes originating from the fundamental modes of different degrees of freedom, in contrast to the Kerr case in general relativity. We show that the excitation factors are indeed amplified as a manifestation of resonance at parameter values corresponding to the avoided crossings.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-08-11
DOI
https://doi.org/10.1103/59tb-2x9r
Citations
3
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
3.46
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article

Resonance of black hole quasinormal modes in coupled systems

Kazufumi Takahashi, Hayato Motohashi, Takuya Takahashi
3 citations
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
3.46
article

Resonance of black hole quasinormal modes in coupled systems

Kazufumi Takahashi, Hayato Motohashi, Takuya Takahashi
article en
3 citations

Abstract

Black hole quasinormal modes (QNMs) can exhibit resonant excitations associated with avoided crossings in their complex frequency spectrum. Such resonance phenomena can serve as novel signatures for probing new physics, where additional degrees of freedom are commonly introduced. Motivated by this possibility, we investigate QNMs in systems where multiple degrees of freedom are coupled with each other and introduce a definition of excitation factors suitable for such systems. To demonstrate our formulation, we apply it to a black hole in the Einstein-Maxwell-axion theory, where we find that avoided crossings can appear even between longest-lived modes originating from the fundamental modes of different degrees of freedom, in contrast to the Kerr case in general relativity. We show that the excitation factors are indeed amplified as a manifestation of resonance at parameter values corresponding to the avoided crossings.

Physical review. D/Physical review. D.Vol. 112(6)
Nihon University (JP), Kyoto University (JP), Instituto de Física Teórica (ES), Yukawa Institute for Theoretical Physics (JP), Tokyo Metropolitan University (JP), The University of Tokyo (JP)
Openalex Percentile: Top 7%
Pulsars and Gravitational Waves Research
3.46
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Resonance of black hole quasinormal modes in coupled systems — Kazufumi Takahashi, Hayato Motohashi, et al. · Physical review. D/Physical review. D. (2025) | TGRS Research Map | TGRS