Gravitational Waves from binary black holes in the extreme mass ratio regime: Self-force calculations
arXiv:astro-ph/0501238 · doi:10.1088/0264-9381/22/10/031
Abstract
We present a report on the progress made in the development of computational techniques to evaluate the gravitational radiation generated by a particle orbiting a massive black hole to second pertrubative order.
7 pages. Contribution to 5th LISA Symposium
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- A Finite Element Computation of the Gravitational Radiation emitted by a Point-like object orbiting a Non-rotating Black Hole
- A Toy Model for Testing Finite Element Methods to Simulate Extreme-Mass-Ratio Binary Systems
- Analytic toy-model for the ISCO shift
- Self-gravitating ring of matter in orbit around a black hole: The innermost stable circular orbit
- The gravitational two-body problem in the vicinity of the light ring: Insights from the black-hole-ring toy model
- Marginally bound circular orbits in the composed black-hole-ring system