On the simplest binary system of rotating black holes

Journal Article · Fri May 01 00:00:00 EDT 2009 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.3141316· OSTI ID:21304818

Manko, V S ^[1]; Rodchenko, E D; Sadovnikov, B I ^[2]; Ruiz, E ^[3]

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1. Departamento de Fisica, Centro de Investigacion y de Estudios Avanzados del IPN, A.P. 14-740, 07000 Mexico D.F. (Mexico)
2. Department of Quantum Statistics and Field Theory, Lomonosov Moscow State University, Moscow 119899 (Russian Federation)
3. Instituto Universitario de Fisica Fundamental y Matematicas, Universidad de Salamanca, 37008 Salamanca (Spain)

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.

• OSTI ID: 21304818
• Journal Information: AIP Conference Proceedings, Vol. 1122, Issue 1; Conference: Spanish relativity meeting 2008, Salamanca (Spain), 15-19 Sep 2008; Other Information: DOI: 10.1063/1.3141316; (c) 2009 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
99 GENERAL AND MISCELLANEOUS//MATHEMATICS, COMPUTING, AND INFORMATION SCIENCE
AXIAL SYMMETRY
BLACK HOLES
COSMOLOGY
EINSTEIN FIELD EQUATIONS
GENERAL RELATIVITY THEORY
KERR METRIC
MATHEMATICAL SOLUTIONS
QUANTUM FIELD THEORY