The Breton-Manko equatorially antisymmetric binary configuration revisited
arXiv:1302.7110 · doi:10.1088/0264-9381/30/14/145005
Abstract
The Breton-Manko solution for two identical counter-rotating Kerr-Newman charged masses is rewritten in the physical parametrization involving Komar quantities. The new form of the solution turns out to be very convenient for verifying that the black-hole sector of the Bretón-Manko binary configuration saturates a recent geometric inequality for interacting black holes with struts discovered by Gabach Clement.
6 pages, 1 figure; minor improvement of presentation of functions B and G compared to published version
References in corpus (7)
- The double-Reissner-Nordstrom solution and the interaction force between two spherically symmetric charged particles
- Equatorial symmetry/antisymmetry of stationary axisymmetric electrovac spacetimes
- Exact solution for the simplest binary system of Kerr black holes
- Equatorial symmetry/antisymmetry of stationary axisymmetric electrovac spacetimes. II
- Bounds on the force between black holes
- Static charged double-black rings in five dimensions
- On the properties of the Ernst-Manko-Ruiz equatorially antisymmetric solutions
Cited by in corpus (8)
- Geometrical inequalities bounding angular momentum and charges in General Relativity
- Metric for two equal Kerr black holes
- Stationary black diholes
- Thermodynamics of two aligned Kerr-Newman black holes
- Opposite charged two-body system of identical counter-rotating black holes
- Binary system of unequal counterrotating Kerr-Newman sources
- Thermodynamics of two aligned Kerr black holes
- Smarr formula for black holes endowed with both electric and magnetic charges