Gravitational self-force from radiation-gauge metric perturbations
Calculations of the gravitational self-force (GSF) on a point mass in curved spacetime require as input the metric perturbation in a sufficiently regular gauge. A basic challenge in the program to compute the GSF for orbits around a Kerr black hole is that the standard procedure for reconstructing t...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
2014-01-15.
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| Subjects: | |
| Online Access: | Get fulltext |