Numerical hydrodynamics: SPH vs. AMR

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dc.creatorPlewa, Tomek
dc.date2000-08-31
dc.date.accessioned2026-07-07T01:55:14Z
dc.date.available2026-07-07T01:55:14Z
dc.descriptionThe advantages and disadvantages of two approaches to astrophysical hydrodynamics, Smoothed Particle Hydrodynamics and Adaptive Mesh Refinement, are briefly discussed together with some current problems of computational hydrodynamics.
dc.description4 pages, LaTeX, requires newpasp.sty. To appear in H. Zinnecker and R.D. Mathieu, eds, Proceedings of the IAU Symposium 200 "The Formation of Binary Stars", held in Potsdam, Germany, April 10-15 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0008512
dc.identifierhttp://arxiv.org/abs/astro-ph/0008512
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1581
dc.subjectAstrophysics
dc.titleNumerical hydrodynamics: SPH vs. AMR
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