Binary black-hole evolutions of excision and puncture data

dc.creatorSperhake, Ulrich
dc.date2006-06-19
dc.date2007-10-16
dc.date.accessioned2026-07-07T11:04:27Z
dc.date.available2026-07-07T11:04:27Z
dc.descriptionWe present a new numerical code developed for the evolution of binary black-hole spacetimes using different initial data and evolution techniques. The code is demonstrated to produce state-of-the-art simulations of orbiting and inspiralling black-hole binaries with convergent waveforms. We also present the first detailed study of the dependence of gravitational waveforms resulting from three-dimensional evolutions of different types of initial data. For this purpose we compare the waveforms generated by head-on collisions of superposed Kerr-Schild, Misner and Brill-Lindquist data over a wide range of initial separations.
dc.description21 pages, 13 figures, final version accepted for publication in PRD
dc.identifierhttps://arxiv.org/abs/gr-qc/0606079
dc.identifierhttp://arxiv.org/abs/gr-qc/0606079
dc.identifierPhys.Rev.D76:104015,2007
dc.identifierdoi:10.1103/PhysRevD.76.104015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188896
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBinary black-hole evolutions of excision and puncture data
dc.typetext

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