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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| Médium: | Artículo |
| Jazyk: | English |
| Vydáno: |
2018
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| On-line přístup: | https://doi.org/10.1093/ptep/pty108 https://academic.oup.com/ptep/article/2018/10/103E01/5150479 |
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