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Colliding black holes from a null point of view: the close limit
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Colliding black holes from a null point of view: the close limit
classification
gr-qc
keywords
blackcharacteristicholesalgorithmbearingbinaryciteclose
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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}.
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