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

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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

Scientific paper

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}.

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