Extreme binary black holes in a physical representation

Stationary axisymmetric binary systems of unequal co- and counter-rotating extreme Kerr black holes separated by a conical singularity are studied. Both solutions are identified as two three- parametric subfamilies of the Kinnersley–Chitre metric, and fully depicted by Komar parameters: the two mass...

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Bibliographic Details
Main Author: Cabrera Munguia, Ivan
Format: Artículo
Published: 2018
Online Access:https://doi.org/10.1093/ptep/pty108
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