Numerical Simulations in Cosmology I
天体物理学
2008-02-03 v2
摘要
The purpose of these lectures is to give a short introduction into a very vast field of numerical simulations for cosmological applications. I focus on major features of the simulations: the equations, main numerical techniques, effects of resolution, and methods of halo identification.
引用
@article{arxiv.astro-ph/9605183,
title = {Numerical Simulations in Cosmology I},
author = {A. Klypin},
journal= {arXiv preprint arXiv:astro-ph/9605183},
year = {2008}
}
备注
16 pages TEX. 9 PostScript figures and the text are available at ftp://charon.nmsu.edu/pub/aklypin/LECTURE1 To appear in International School of Physics ``Enrico Fermi'': Dark Matter in the Universe,Varenna 1995, eds. S. Bonometto, J.R. Primack, A. Provenzale. Corrected ftp address