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.
@article{arxiv.gr-qc/0201052,
title = {Evolution of Kerr-Schild type initial data for binary black holes using the horizon penetrating Teukolsky equation},
author = {Gaurav Khanna},
journal= {arXiv preprint arXiv:gr-qc/0201052},
year = {2009}
}
Comments
6 pages, 3 figures; minor error fixed, no changes in conclusions