Gravitational Waves from binary black holes in the extreme mass ratio regime: Self-force calculations

Details Gravitational Waves from binary black holes in the extreme mass ratio regime: Self-force calculations Gravitational Waves from binary black holes in the extreme mass ratio regime: Self-force calculations

2005-01-13

arxiv.org/abs/astro-ph/0501238v1

Class.Quant.Grav. 22 (2005) S369-374

Astronomy and Astrophysics

Astrophysics

7 pages. Contribution to 5th LISA Symposium

Scientific paper

10.1088/0264-9381/22/10/031

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.

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