Quasinormal modes of a static black hole in nonlinear electrodynamics

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Fathi, Mohsen, Guzmán, Ariel, Villanueva, J. R.
Format: Preprint
Published: 2025
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866912752979673088
author Fathi, Mohsen
Guzmán, Ariel
Villanueva, J. R.
author_facet Fathi, Mohsen
Guzmán, Ariel
Villanueva, J. R.
contents We investigate the axial electromagnetic quasinormal modes of a static, asymptotically Anti--de Sitter (AdS) black hole sourced by a nonlinear electrodynamics model of Plebański type. Starting from the master equation governing axial perturbations, we impose ingoing boundary conditions at the event horizon and normalizable (Dirichlet) behavior at the AdS boundary. Following the approach of Jansen, we recast the radial equation into a linear generalized eigenvalue problem by using an ingoing Eddington--Finkelstein formulation, compactifying the radial domain, and regularizing the asymptotic coefficients. The resulting problem is solved using a Chebyshev--Lobatto pseudospectral discretization. We compute the fundamental quasinormal mode frequencies for both the purely electric ($Q_m=0$) and purely magnetic ($Q_e=0$) sectors, emphasizing the role of the nonlinearity parameter $β$ and the effective charge magnitude $Q$. Our results show that increasing either $β$ or $Q$ raises both the oscillation frequency $ω_R$ and the damping rate $-ω_I$, leading to faster but more rapidly decaying ringdown profiles. Nonlinear electrodynamics breaks the isospectrality between electric and magnetic configurations: magnetic modes are systematically less oscillatory and more weakly damped than their electric counterparts. For sufficiently large $β$ and small $Q_m$, the fundamental mode becomes purely imaginary ($ω_R \approx 0$), in agreement with the absence of a trapping potential barrier in this regime. These findings reveal qualitative signatures of nonlinear electromagnetic effects on black hole perturbations and may have implications for high-field or high-charge astrophysical environments.
format Preprint
id arxiv_https___arxiv_org_abs_2512_02714
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Quasinormal modes of a static black hole in nonlinear electrodynamics
Fathi, Mohsen
Guzmán, Ariel
Villanueva, J. R.
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
High Energy Physics - Theory
Mathematical Physics
We investigate the axial electromagnetic quasinormal modes of a static, asymptotically Anti--de Sitter (AdS) black hole sourced by a nonlinear electrodynamics model of Plebański type. Starting from the master equation governing axial perturbations, we impose ingoing boundary conditions at the event horizon and normalizable (Dirichlet) behavior at the AdS boundary. Following the approach of Jansen, we recast the radial equation into a linear generalized eigenvalue problem by using an ingoing Eddington--Finkelstein formulation, compactifying the radial domain, and regularizing the asymptotic coefficients. The resulting problem is solved using a Chebyshev--Lobatto pseudospectral discretization. We compute the fundamental quasinormal mode frequencies for both the purely electric ($Q_m=0$) and purely magnetic ($Q_e=0$) sectors, emphasizing the role of the nonlinearity parameter $β$ and the effective charge magnitude $Q$. Our results show that increasing either $β$ or $Q$ raises both the oscillation frequency $ω_R$ and the damping rate $-ω_I$, leading to faster but more rapidly decaying ringdown profiles. Nonlinear electrodynamics breaks the isospectrality between electric and magnetic configurations: magnetic modes are systematically less oscillatory and more weakly damped than their electric counterparts. For sufficiently large $β$ and small $Q_m$, the fundamental mode becomes purely imaginary ($ω_R \approx 0$), in agreement with the absence of a trapping potential barrier in this regime. These findings reveal qualitative signatures of nonlinear electromagnetic effects on black hole perturbations and may have implications for high-field or high-charge astrophysical environments.
title Quasinormal modes of a static black hole in nonlinear electrodynamics
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
High Energy Physics - Theory
Mathematical Physics
url https://arxiv.org/abs/2512.02714