Black Hole Data via a Kerr-Schild Approach

Details Black Hole Data via a Kerr-Schild Approach Black Hole Data via a Kerr-Schild Approach

1997-11-26

arxiv.org/abs/gr-qc/9711076v1

Phys.Rev. D57 (1998) 6113-6118

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, RevTeX format

Scientific paper

10.1103/PhysRevD.57.6113

We present a new approach for setting initial Cauchy data for multiple black hole spacetimes. The method is based upon adopting an initially Kerr-Schild form of the metric. In the case of non-spinning holes, the constraint equations take a simple hierarchical form which is amenable to direct numerical integration. The feasibility of this approach is demonstrated by solving analytically the problem of initial data in a perturbed Schwarzschild geometry.

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