Linear stability of charged warm holes

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Gannouji, Radouane, Antonucci, Alejandro Guzmán
Format: Preprint
Published: 2025
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866918135891755008
author Gannouji, Radouane
Antonucci, Alejandro Guzmán
author_facet Gannouji, Radouane
Antonucci, Alejandro Guzmán
contents Charged black holes are known to suffer from an interior instability associated with the presence of the Cauchy horizon. Recently, a hairy charged black hole was proposed that avoids the formation of a Cauchy horizon. It is natural to question whether this instability might manifest in the exterior solution. In this paper, we have analyzed the stability of this black hole. Our results show that vector perturbations are stable, along with the scalar sector for $l=0$. We have also computed the corresponding quasinormal modes (QNMs) and quasibound states (QBSs).
format Preprint
id arxiv_https___arxiv_org_abs_2501_03421
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Linear stability of charged warm holes
Gannouji, Radouane
Antonucci, Alejandro Guzmán
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Charged black holes are known to suffer from an interior instability associated with the presence of the Cauchy horizon. Recently, a hairy charged black hole was proposed that avoids the formation of a Cauchy horizon. It is natural to question whether this instability might manifest in the exterior solution. In this paper, we have analyzed the stability of this black hole. Our results show that vector perturbations are stable, along with the scalar sector for $l=0$. We have also computed the corresponding quasinormal modes (QNMs) and quasibound states (QBSs).
title Linear stability of charged warm holes
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2501.03421