Close limit of grazing black hole collisions: non-spinning holes

Details Close limit of grazing black hole collisions: non-spinning holes Close limit of grazing black hole collisions: non-spinning holes

2000-03-02

arxiv.org/abs/gr-qc/0003003v1

New J.Phys.2:3,2000

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

14 Pages, 5 figures, RevTeX, full published version available free (including movies) in NJP web site http://njp.org

Scientific paper

10.1088/1367-2630/2/1/303

Using approximate techniques we study the final moments of the collision of two (individually non-spinnning) black holes which inspiral into each other. The approximation is based on treating the whole space-time as a single distorted black hole. We obtain estimates for the radiated energy, angular momentum and waveforms for the gravitational waves produced in such a collision. The results can be of interest for analyzing the data that will be forthcoming from gravitational wave interferometric detectors, like the LIGO, GEO, LISA, VIRGO and TAMA projects.

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