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Hauptverfasser: Corrêa, Mateus Malato, Macedo, Caio F. B., Macedo, Rodrigo Panosso, Oliveira, Leandro A.
Format: Preprint
Veröffentlicht: 2025
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Online-Zugang:https://arxiv.org/abs/2504.00107
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author Corrêa, Mateus Malato
Macedo, Caio F. B.
Macedo, Rodrigo Panosso
Oliveira, Leandro A.
author_facet Corrêa, Mateus Malato
Macedo, Caio F. B.
Macedo, Rodrigo Panosso
Oliveira, Leandro A.
contents Small deviations in the spacetime around black holes can lead to instabilities in the underlying quasinormal mode spectrum, potentially altering the hierarchy of its overtones. A practical way to induce such spectral instability is by introducing small modifications to the effective potential governing the dynamics of fluctuations in the black hole spacetime. While finding a physically meaningful interpretation for such ad hoc modifications in an astrophysical context can be challenging, analogue black hole models provide an alternative framework to explore their effects and study the instabilities. In this work, we consider an analogue black hole modeled by a draining bathtub flow and demonstrate that vorticities in the fluid introduce a small bump in the effective potential of the wave equation. This naturally realizes a physically motivated version of the elephant and the flea configuration. We analyze the spectrum using two complementary approaches: direct mode computation via two distinct frequency-domain methods and time evolution of initial perturbations. As in astrophysical black holes, the vorticities destabilizes the QNM spectrum of the analogue system, possibly yielding time evolution with long-lived ringing effects, akin to those observed for massive fields in curved spacetimes.
format Preprint
id arxiv_https___arxiv_org_abs_2504_00107
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Black hole spectral instabilities in the laboratory: Shallow water analogue
Corrêa, Mateus Malato
Macedo, Caio F. B.
Macedo, Rodrigo Panosso
Oliveira, Leandro A.
General Relativity and Quantum Cosmology
Small deviations in the spacetime around black holes can lead to instabilities in the underlying quasinormal mode spectrum, potentially altering the hierarchy of its overtones. A practical way to induce such spectral instability is by introducing small modifications to the effective potential governing the dynamics of fluctuations in the black hole spacetime. While finding a physically meaningful interpretation for such ad hoc modifications in an astrophysical context can be challenging, analogue black hole models provide an alternative framework to explore their effects and study the instabilities. In this work, we consider an analogue black hole modeled by a draining bathtub flow and demonstrate that vorticities in the fluid introduce a small bump in the effective potential of the wave equation. This naturally realizes a physically motivated version of the elephant and the flea configuration. We analyze the spectrum using two complementary approaches: direct mode computation via two distinct frequency-domain methods and time evolution of initial perturbations. As in astrophysical black holes, the vorticities destabilizes the QNM spectrum of the analogue system, possibly yielding time evolution with long-lived ringing effects, akin to those observed for massive fields in curved spacetimes.
title Black hole spectral instabilities in the laboratory: Shallow water analogue
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2504.00107