Numerical stability of the AA evolution system compared to the ADM and BSSN systems

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dc.creatorJansen, Nina
dc.creatorBruegmann, Bernd
dc.creatorTichy, Wolfgang
dc.date2003-10-20
dc.date.accessioned2026-07-07T12:01:20Z
dc.date.available2026-07-07T12:01:20Z
dc.descriptionWe explore the numerical stability properties of an evolution system suggested by Alekseenko and Arnold. We examine its behavior on a set of standardized testbeds, and we evolve a single black hole with different gauges. Based on a comparison with two other evolution systems with well-known properties, we discuss some of the strengths and limitations of such simple tests in predicting numerical stability in general.
dc.description16 pages, 12 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0310100
dc.identifierhttp://arxiv.org/abs/gr-qc/0310100
dc.identifierPhys.Rev.D74:084022,2006
dc.identifierdoi:10.1103/PhysRevD.74.084022
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207065
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNumerical stability of the AA evolution system compared to the ADM and BSSN systems
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