Adaptative Mesh Refinement in Numerical Relativity

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dc.creatorMasso, Joan
dc.creatorSeidel, Edward
dc.creatorWalker, Paul
dc.date1994-12-21
dc.date.accessioned2026-07-07T03:30:35Z
dc.date.available2026-07-07T03:30:35Z
dc.descriptionWe discuss the use of Adaptative Mesh Refinement (AMR) techniques in dynamical black hole spacetimes. We compare results between traditional fixed grid methods and a new AMR application for the 1-D Schwarzschild case.
dc.description3 pages, uuencoded gziped ps file including 2 Figs. Also available at http://jean-luc.ncsa.uiuc.edu/Papers/ To appear in the MG7 proceedings
dc.identifierhttps://arxiv.org/abs/gr-qc/9412057
dc.identifierhttp://arxiv.org/abs/gr-qc/9412057
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35576
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAdaptative Mesh Refinement in Numerical Relativity
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