Evolution of Kerr-Schild type initial data for binary black holes using the horizon penetrating Teukolsky equation

Details Evolution of Kerr-Schild type initial data for binary black holes using the horizon penetrating Teukolsky equation Evolution of Kerr-Schild type initial data for binary black holes using the horizon penetrating Teukolsky equation

2002-01-16

arxiv.org/abs/gr-qc/0201052v2

Phys.Rev. D65 (2002) 124018

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages, 3 figures; minor error fixed, no changes in conclusions

Scientific paper

10.1103/PhysRevD.65.124018

We use the Kerr-Schild type Teukolsky equation (horizon penetrating) to
evolve binary black hole initial data as proposed by Bishop {\em et al.} in the
close limit. Our results are in agreement with those recently obtained by
Sarbach {\em et al.} from the Zerilli equation evolution of the same initial
data.

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