Transition from inspiral to plunge for a compact body in a circular equatorial orbit around a massive, spinning black hole
Author:
Publisher
American Physical Society (APS)
Subject
Nuclear and High Energy Physics
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.62.124022/fulltext
Reference18 articles.
1. Capture of stellar mass compact objects by massive black holes in galactic cusps
2. Estimating the detectable rate of capture of stellar mass black holes by massive central black holes in normal galaxies
3. Gravitational waves from a compact star in a circular, inspiral orbit, in the equatorial plane of a massive, spinning black hole, as observed by LISA
4. Evolution of circular, nonequatorial orbits of Kerr black holes due to gravitational-wave emission
5. Mode sum regularization approach for the self-force in black hole spacetime
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