New Coordinate Systems for Axisymmetric Black Hole Collisions

dc.creatorBrandt, S. R.
dc.creatorWalker, P.
dc.creatorAnninos, P.
dc.date1997-11-06
dc.date.accessioned2026-07-07T03:31:57Z
dc.date.available2026-07-07T03:31:57Z
dc.descriptionWe describe a numerical grid generating procedure to construct new classes of orthogonal coordinate systems that are specially adapted to binary black hole spacetimes. The new coordinates offer an alternative approach to the conventional Čadež coordinates, in addition to providing a potentially more stable and flexible platform to extend previous calculations of binary black hole collisions.
dc.description3 pages, 5 postscript figures, LaTeX, uses mprocl.sty (available at http://shemesh.fiz.huji.ac.il/MG8/submission.html) To appear in the proceedings of the Marcel Grossmann 8 (Jerusalem, 1997)
dc.identifierhttps://arxiv.org/abs/gr-qc/9711018
dc.identifierhttp://arxiv.org/abs/gr-qc/9711018
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36055
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNew Coordinate Systems for Axisymmetric Black Hole Collisions
dc.typetext

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