Quasi-normal modes and absorption section from regular black holes immersed in perfect fluid dark matter

Fuente: arXiv
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Main Authors: Tovar, L. O. Téllez, Pedraza, Omar, López, L. A., Arceo, R.
Format: Preprint
Published: 2025
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author Tovar, L. O. Téllez
Pedraza, Omar
López, L. A.
Arceo, R.
author_facet Tovar, L. O. Téllez
Pedraza, Omar
López, L. A.
Arceo, R.
contents We study scalar, electromagnetic and gravitational perturbations of three families of regular black holes, Hayward, Bardeen, and Ayon-Beato-García immersed in a Perfect Fluid Dark Matter (PFDM) background. Using both the sixth-order WKB approximation and the Asymptotic Iteration Method (AIM), we determine the corresponding quasi-normal modes and absorption cross sections. By fixing the horizon radius, we analyze the dependence of the parameters of the black holes and the parameter of PFDM. The computed quasi-normal modes confirm the dynamical stability of the black holes under scalar, electromagnetic and gravitational perturbations. Furthermore, both the real and imaginary parts of the quasi-normal modes increase with the multipole number $l$, corresponding to higher oscillation frequencies and faster damping rates. On the other hand, absorption cross sections are compared under similar parametric conditions. The results demonstrate that PFDM influences the dynamical properties of regular black holes.
format Preprint
id arxiv_https___arxiv_org_abs_2507_03627
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Quasi-normal modes and absorption section from regular black holes immersed in perfect fluid dark matter
Tovar, L. O. Téllez
Pedraza, Omar
López, L. A.
Arceo, R.
General Relativity and Quantum Cosmology
We study scalar, electromagnetic and gravitational perturbations of three families of regular black holes, Hayward, Bardeen, and Ayon-Beato-García immersed in a Perfect Fluid Dark Matter (PFDM) background. Using both the sixth-order WKB approximation and the Asymptotic Iteration Method (AIM), we determine the corresponding quasi-normal modes and absorption cross sections. By fixing the horizon radius, we analyze the dependence of the parameters of the black holes and the parameter of PFDM. The computed quasi-normal modes confirm the dynamical stability of the black holes under scalar, electromagnetic and gravitational perturbations. Furthermore, both the real and imaginary parts of the quasi-normal modes increase with the multipole number $l$, corresponding to higher oscillation frequencies and faster damping rates. On the other hand, absorption cross sections are compared under similar parametric conditions. The results demonstrate that PFDM influences the dynamical properties of regular black holes.
title Quasi-normal modes and absorption section from regular black holes immersed in perfect fluid dark matter
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2507.03627