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...
Saved in:
| Main Author: | |
|---|---|
| Format: | Artículo |
| Language: | English |
| Published: |
2018
|
| Subjects: | |
| Online Access: | https://doi.org/10.1093/ptep/pty108 https://academic.oup.com/ptep/article/2018/10/103E01/5150479 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
