On new regular charged black hole solutions: Limiting Curvature Condition, Quasinormal modes and Shadows

Fuente: arXiv
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Auteurs principaux: Balart, Leonardo, Panotopoulos, Grigoris, Rincon, Angel
Format: Preprint
Publié: 2024
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author Balart, Leonardo
Panotopoulos, Grigoris
Rincon, Angel
author_facet Balart, Leonardo
Panotopoulos, Grigoris
Rincon, Angel
contents We introduce two new static, spherically symmetric regular black hole solutions that can be obtained from non-linear electrodynamics models. For each solution, we investigate the dynamic stability with respect to arbitrary linear fluctuations of the metric and electromagnetic field, and also examine the energy conditions that those black holes satisfy. Moreover, based on those solutions, we present two additional ones that satisfy the Limiting Curvature Condition. Finally, we make a comparison between the two solutions exploring their null geodesics and circular photon orbits.
format Preprint
id arxiv_https___arxiv_org_abs_2412_00550
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle On new regular charged black hole solutions: Limiting Curvature Condition, Quasinormal modes and Shadows
Balart, Leonardo
Panotopoulos, Grigoris
Rincon, Angel
General Relativity and Quantum Cosmology
We introduce two new static, spherically symmetric regular black hole solutions that can be obtained from non-linear electrodynamics models. For each solution, we investigate the dynamic stability with respect to arbitrary linear fluctuations of the metric and electromagnetic field, and also examine the energy conditions that those black holes satisfy. Moreover, based on those solutions, we present two additional ones that satisfy the Limiting Curvature Condition. Finally, we make a comparison between the two solutions exploring their null geodesics and circular photon orbits.
title On new regular charged black hole solutions: Limiting Curvature Condition, Quasinormal modes and Shadows
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2412.00550