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arXiv · 1806.10818

Extreme binary black holes in a physical representation

I. Cabrera-Munguia
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Abstract

Stationary axisymmetric binary systems of unequal co and counter-rotating extreme Kerr black holes apart by a conical singularity are studied. Both solutions are well identified as two $3$-parametric subfamilies of the Kinnersley-Chitre metric, and fully depicted by Komar parameters: the two masses $M_{1}$ and $M_{2}$, and a coordinate distance $R$, where the angular momenta $J_{1}$ and $J_{2}$ are functions of these parameters. Our physical representation allows us to identify some limits and novel physical properties.

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I. Cabrera-Munguia. 2018-06-28. Extreme binary black holes in a physical representation. https://doi.org/10.1093/ptep%2Fpty108

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