The Evolution of Distorted Rotating Black Holes III: Initial Data

Details The Evolution of Distorted Rotating Black Holes III: Initial Data The Evolution of Distorted Rotating Black Holes III: Initial Data

1996-01-09

arxiv.org/abs/gr-qc/9601010v1

Phys.Rev. D54 (1996) 1403-1416

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages

Scientific paper

10.1103/PhysRevD.54.1403

In this paper we study a new family of black hole initial data sets corresponding to distorted ``Kerr'' black holes with moderate rotation parameters, and distorted Schwarzschild black holes with even- and odd-parity radiation. These data sets build on the earlier rotating black holes of Bowen and York and the distorted Brill wave plus black hole data sets. We describe the construction of this large family of rotating black holes. We present a systematic study of important properties of these data sets, such as the size and shape of their apparent horizons, and the maximum amount of radiation that can leave the system during evolution. These data sets should be a very useful starting point for studying the evolution of highly dynamical black holes and can easily be extended to 3D.

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