Kerr-Schild type initial data for black holes with angular momenta

Details Kerr-Schild type initial data for black holes with angular momenta Kerr-Schild type initial data for black holes with angular momenta

2002-05-15

arxiv.org/abs/gr-qc/0205060v2

Class.Quant.Grav. 19 (2002) 6059-6073

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, 3 figures. Revised version. To appear in Classical and Quantum Gravity

Scientific paper

10.1088/0264-9381/19/23/312

Generalizing previous work we propose how to superpose spinning black holes in a Kerr-Schild initial slice. This superposition satisfies several physically meaningful limits, including the close and the far ones. Further we consider the close limit of two black holes with opposite angular momenta and explicitly solve the constraint equations in this case. Evolving the resulting initial data with a linear code, we compute the radiated energy as a function of the masses and the angular momenta of the black holes.

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