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 a...
Main Authors: | , , |
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Other Authors: | , |
Format: | Article |
Language: | English |
Published: |
American Physical Society,
2018-02-20T15:40:25Z.
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Subjects: | |
Online Access: | Get fulltext |