Numerical simulation of orbiting black holes

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dc.creatorBruegmann, Bernd
dc.creatorTichy, Wolfgang
dc.creatorJansen, Nina
dc.date2003-12-26
dc.date2004-05-12
dc.date.accessioned2026-07-07T11:57:36Z
dc.date.available2026-07-07T11:57:36Z
dc.descriptionWe present numerical simulations of binary black hole systems which for the first time last for about one orbital period for close but still separate black holes as indicated by the absence of a common apparent horizon. An important part of the method is the construction of comoving coordinates, in which both the angular and radial motion is minimized through a dynamically adjusted shift condition. We use fixed mesh refinement for computational efficiency.
dc.description4 pages, 4 figures; several significant changes to presentation for published version
dc.identifierhttps://arxiv.org/abs/gr-qc/0312112
dc.identifierhttp://arxiv.org/abs/gr-qc/0312112
dc.identifierPhys.Rev.Lett.92:211101,2004
dc.identifierdoi:10.1103/PhysRevLett.92.211101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205933
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNumerical simulation of orbiting black holes
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