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Conference Paper

Colliding black holes from a null point of view: the close limit

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Husa,  Sascha
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Campanelli,  Manuela
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Winicour,  Jeffrey
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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3178.pdf
(Preprint), 67KB

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Citation

Husa, S., Campanelli, M., Gomez, R., Winicour, J., & Zlochower, Y. (2001). Colliding black holes from a null point of view: the close limit. In Proceedings of 9th Marcel Grossmann meeting (MG9).


Cite as: https://hdl.handle.net/11858/00-001M-0000-0013-55D8-4
Abstract
We present a characteristic algorithm for computing the perturbations of a Schwarzschild spacetime by means of solving the Teukolsky equations. Our methods and results are expected to have direct bearing on the study of binary black holes presently underway using a fully {em nonlinear} characteristic code cite{Gomez98a}