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

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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}.
2 pages, contribution to the 9th Marcel Grossmann meeting (MG9), Rome, July 2000

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/33754

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0012110
 http://arxiv.org/abs/gr-qc/0012110

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arXiv