Axis potentials for stationary n-black-hole configurations

DOI10.1088/1361-6382/ABB116zbMath1479.83146arXiv2009.03992OpenAlexW3099620488MaRDI QIDQ5161889

J. D. Hennig

Publication date: 1 November 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2009.03992

zbMATH Keywords

exact solutionssoliton methodsspin-spin repulsionblack hole balance problem

Mathematics Subject Classification ID

Black holes (83C57) Exact solutions to problems in general relativity and gravitational theory (83C15) (n)-body problems (70F10) Motion of the gyroscope (70E05)

Cites Work

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• The inner Cauchy horizon of axisymmetric and stationary black holes with surrounding matter in Einstein-Maxwell theory: study in terms of soliton methods
• Non-existence of stationary two-black-hole configurations: the degenerate case
• Stationary two-black-hole configurations: A non-existence proof
• Non-existence of stationary two-black-hole configurations
• Existence of singularities in two-Kerr black holes
• Constructive proof of the Kerr–Newman black hole uniqueness including the extreme case
• A universal inequality between the angular momentum and horizon area for axisymmetric and stationary black holes with surrounding matter
• On the balance problem for two rotating and charged black holes

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