Linear stability of charged warm holes
arXiv:2501.03421 · doi:10.1140/epjc/s10052-025-14661-5
Abstract
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 . We have also computed the corresponding quasinormal modes (QNMs) and quasibound states (QBSs).
23 pages, 9 figures. Journal version: Included additional references and expanded discussion in Sec. 1. Added further QBSs calculations in Sec. 10
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