Strong-field tidal distortions of rotating black holes. III. Embeddings in hyperbolic three-space
In previous work, we developed tools for quantifying the tidal distortion of a black hole’s event horizon due to an orbiting companion. These tools use techniques which require large mass ratios (companion mass μ much smaller than black hole mass M), but can be used for arbitrary bound orbits and fo...
| Main Authors: | , , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
American Physical Society
2018
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| Online Access: | http://hdl.handle.net/1721.1/113830 https://orcid.org/0000-0001-6211-1388 https://orcid.org/0000-0003-2492-6505 |