Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter

Fuente: arXiv
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Main Author: Lütfüoğlu, Bekir Can
Format: Preprint
Published: 2026
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author Lütfüoğlu, Bekir Can
author_facet Lütfüoğlu, Bekir Can
contents We study massless scalar, electromagnetic, and Dirac perturbations of the exact asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld scalar. Using the Padé-improved WKB method, with a time-domain Prony check for the scalar fundamental mode, we compute representative quasinormal frequencies and find that larger regularity shifts the spectrum toward smaller oscillation frequencies and damping rates, whereas the quality factor changes only weakly. The spectral shifts remain well above the estimated numerical uncertainty, demonstrating that the DBI regularity scale leaves a robust spin-dependent imprint on ringdown.
format Preprint
id arxiv_https___arxiv_org_abs_2604_24349
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter
Lütfüoğlu, Bekir Can
General Relativity and Quantum Cosmology
We study massless scalar, electromagnetic, and Dirac perturbations of the exact asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld scalar. Using the Padé-improved WKB method, with a time-domain Prony check for the scalar fundamental mode, we compute representative quasinormal frequencies and find that larger regularity shifts the spectrum toward smaller oscillation frequencies and damping rates, whereas the quality factor changes only weakly. The spectral shifts remain well above the estimated numerical uncertainty, demonstrating that the DBI regularity scale leaves a robust spin-dependent imprint on ringdown.
title Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2604.24349