Schwarzschild black hole levitating in the hyperextreme Kerr field

DOI10.1007/s10714-012-1429-1zbMath1253.83025arXiv0910.0335OpenAlexW2131751082MaRDI QIDQ690997

Eduardo Ruiz, V. S. Man'ko

Publication date: 29 November 2012

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

Full work available at URL: https://arxiv.org/abs/0910.0335

zbMATH Keywords

equilibrium configurationsdouble-Kerr solutionErnst potential

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (1)

Metric for two arbitrary Kerr sources

Cites Work

• Detection of closed timelike curves
• The interaction force between rotating black holes at equilibrium
• The end of black hole uniqueness
• Exact solution of the double-Kerr equilibrium problem
• Extended multi-soliton solutions of the Einstein field equations: II. Two comments on the existence of equilibrium states
• On Gravitational Mass and Angular Momentum of Two Black Holes in Equilibrium
• Covariant Conservation Laws in General Relativity
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• A remark on the mass$ndash$angular$ndash$momentum relation in the double-Kerr solution
• Black holes in higher dimensions

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