Simple excision of a black hole in 3+1 numerical relativity

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dc.creatorAlcubierre, Miguel
dc.creatorBruegmann, Bernd
dc.date2000-08-28
dc.date2001-03-23
dc.date.accessioned2026-07-07T12:01:17Z
dc.date.available2026-07-07T12:01:17Z
dc.descriptionWe describe a simple implementation of black hole excision in 3+1 numerical relativity. We apply this technique to a Schwarzschild black hole with octant symmetry in Eddington-Finkelstein coordinates and show how one can obtain accurate, long-term stable numerical evolutions.
dc.description7 pages, 7 figures, revtex. Incorporates comments made by referee
dc.identifierhttps://arxiv.org/abs/gr-qc/0008067
dc.identifierhttp://arxiv.org/abs/gr-qc/0008067
dc.identifierPhys.Rev.D63:104006,2001
dc.identifierdoi:10.1103/PhysRevD.63.104006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207048
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSimple excision of a black hole in 3+1 numerical relativity
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