Universal properties of distorted Kerr-Newman black holes

DOI10.1007/s10714-010-1136-8zbMath1215.83003arXiv1005.3128OpenAlexW2002366250MaRDI QIDQ540530

Marcus Ansorg, Carla Cederbaum, J. D. Hennig

Publication date: 3 June 2011

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1005.3128

zbMATH Keywords

black holesEinstein-Maxwell spacetimes

Mathematics Subject Classification ID

Black holes (83C57) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Einstein-Maxwell equations (83C22)

Related Items (9)

Quantum correction to the entropy of noncommutative BTZ black hole ⋮ Quantum-corrected two-dimensional Horava-Lifshitz black hole entropy ⋮ Generalized second law and universal relations of cosmological black hole ⋮ More on the entropy product and dual CFTs ⋮ Entropy bound of horizons for accelerating, rotating and charged Plebanski-Demianski black hole ⋮ Geometric inequalities for black holes ⋮ Angular momentum -- area -- proportionality of extremal charged black holes in odd dimensions ⋮ Quantization of area for event and Cauchy horizons of the Kerr-Newman black hole ⋮ A note on entropy relations of black hole horizons

Cites Work

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• On space-times with U(1)\(\times U(1)\) symmetric compact Cauchy surfaces
• Non-existence of stationary two-black-hole configurations
• A universal inequality between the angular momentum and horizon area for axisymmetric and stationary black holes with surrounding matter
• The inner Cauchy horizon of axisymmetric and stationary black holes with surrounding matter
• Regularity of Cauchy horizons in S ² × S ¹ Gowdy spacetimes
• A universal constraint between charge and rotation rate for degenerate black holes surrounded by matter

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