Numerical hydrodynamics: SPH vs. AMR
Astrophysics
2007-05-23 v1
Abstract
The 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.
Keywords
Cite
@article{arxiv.astro-ph/0008512,
title = {Numerical hydrodynamics: SPH vs. AMR},
author = {Tomek Plewa},
journal= {arXiv preprint arXiv:astro-ph/0008512},
year = {2007}
}
Comments
4 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