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On the simplest binary system of rotating black holes

Exact axisymmetric stationary solution of the Einstein equations describing a system of two counter-rotating identical Kerr black holes is worked out in a physical parametrization within the framework of the Ernst formalism and analytically extended double-Kerr solution. The derivation of the limiti...

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Main Authors:	Manko, V. S., Rodchenko, E. D., Sadovnikov, B. I., Ruiz, E.
Format:	Conference Proceeding
Language:	English
Subjects:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY AXIAL SYMMETRY BLACK HOLES COSMOLOGY EINSTEIN FIELD EQUATIONS GENERAL AND MISCELLANEOUS//MATHEMATICS, COMPUTING, AND INFORMATION SCIENCE GENERAL RELATIVITY THEORY KERR METRIC MATHEMATICAL SOLUTIONS QUANTUM FIELD THEORY
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creator	Manko, V. S. Rodchenko, E. D. Sadovnikov, B. I. Ruiz, E.
description	Exact axisymmetric stationary solution of the Einstein equations describing a system of two counter-rotating identical Kerr black holes is worked out in a physical parametrization within the framework of the Ernst formalism and analytically extended double-Kerr solution. The derivation of the limiting case of extreme constituents is also discussed.
doi_str_mv	10.1063/1.3141316
format	conference_proceeding
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identifier	ISSN: 0094-243X
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source	American Institute of Physics:Jisc Collections:Transitional Journals Agreement 2021-23 (Reading list)
subjects	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY AXIAL SYMMETRY BLACK HOLES COSMOLOGY EINSTEIN FIELD EQUATIONS GENERAL AND MISCELLANEOUS//MATHEMATICS, COMPUTING, AND INFORMATION SCIENCE GENERAL RELATIVITY THEORY KERR METRIC MATHEMATICAL SOLUTIONS QUANTUM FIELD THEORY
title	On the simplest binary system of rotating black holes
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