The Lazarus project: Plunge waveforms from inspiralling black holes

Details The Lazarus project: Plunge waveforms from inspiralling black holes The Lazarus project: Plunge waveforms from inspiralling black holes

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..746b&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 746-750 (2001).

Physics

Black Holes, Mathematical Procedures And Computer Techniques, Relativity And Gravitation, Binary And Multiple Stars, Physics Of Black Holes

Scientific paper

We study the coalescence of binary black holes from the innermost stable circular orbit down to the final single rotating black hole. We use a technique that combines the full numerical approach to solve Einstein equations, applied in the truly nonlinear regime, and linearized perturbation theory around the final distorted single black hole at later times. We thus produce an estimate for the plunge radiation with a non negligible signal lasting for over t~100M, and we obtain estimates of the total gravitational radiated energy and angular momentum during this process, plunging time, and waveforms. .

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