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

Gaurav Khanna
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Abstract

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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Gaurav Khanna. 2002-01-21. Evolution of Kerr-Schild type initial data for binary black holes using the horizon penetrating Teukolsky equation. https://doi.org/10.1103/physrevd.65.124018

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