Kerr-Newman black hole in a Melvin-swirling universe

Fuente: arXiv
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Hauptverfasser: Di Pinto, Andrea, Klemm, Silke, Viganò, Adriano
Format: Preprint
Veröffentlicht: 2025
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author Di Pinto, Andrea
Klemm, Silke
Viganò, Adriano
author_facet Di Pinto, Andrea
Klemm, Silke
Viganò, Adriano
contents We present a new exact solution of Einstein-Maxwell field equations which represents a rotating black hole with both electric and magnetic charges immersed in a universe which itself is also rotating and magnetized, i.e. the dyonic Kerr-Newman black hole in a Melvin-swirling universe. We show that the solution is completely regular and free of any type of singularity; then we analyze its physical properties, such as the ergoregions and the shape of the event horizons. Finally we present the extremal near horizon geometry of the metric and study its entropy via the Kerr/CFT correspondence.
format Preprint
id arxiv_https___arxiv_org_abs_2503_07780
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Kerr-Newman black hole in a Melvin-swirling universe
Di Pinto, Andrea
Klemm, Silke
Viganò, Adriano
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We present a new exact solution of Einstein-Maxwell field equations which represents a rotating black hole with both electric and magnetic charges immersed in a universe which itself is also rotating and magnetized, i.e. the dyonic Kerr-Newman black hole in a Melvin-swirling universe. We show that the solution is completely regular and free of any type of singularity; then we analyze its physical properties, such as the ergoregions and the shape of the event horizons. Finally we present the extremal near horizon geometry of the metric and study its entropy via the Kerr/CFT correspondence.
title Kerr-Newman black hole in a Melvin-swirling universe
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2503.07780