Numerical Simulations in Cosmology I: Methods
arXiv:astro-ph/0005502
Abstract
This lecture gives a short introduction to different methods used in cosmology. The focus is on major features of N-body simulations: equations, main numerical techniques, effects of resolution, and methods of halo identification.
Lecture at the Summer School "Relativistic Cosmology: Theory and Observations", Italy, Como, May 2000. AASTeX and natbib