Anatoly Klypin
Published 2000-05-25Version 1
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.
Comments: Lecture at the Summer School "Relativistic Cosmology: Theory and Observations", Italy, Como, May 2000. AASTeX and natbib
Numerical Simulations in Cosmology I
Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
Merger of Massive Black Holes using N-Body Simulations with Post-Newtonian Corrections
