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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Bibliographic Details
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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Summary: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.
ISSN:0094-243X
1551-7616
DOI:10.1063/1.3141316