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

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dc.creatorHusa, Sascha
dc.creatorCampanelli, Manuela
dc.creatorGomez, Roberto
dc.creatorWinicour, Jeffrey
dc.creatorZlochower, Yosef
dc.date2000-12-29
dc.date.accessioned2026-07-07T03:25:33Z
dc.date.available2026-07-07T03:25:33Z
dc.descriptionWe 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}.
dc.description2 pages, contribution to the 9th Marcel Grossmann meeting (MG9), Rome, July 2000
dc.identifierhttps://arxiv.org/abs/gr-qc/0012110
dc.identifierhttp://arxiv.org/abs/gr-qc/0012110
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33754
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleColliding black holes from a null point of view: the close limit
dc.typetext

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