Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-11-03
J.Astrophys.Astron. 23 (2002) 185-196
Astronomy and Astrophysics
Astrophysics
published version, significant revisions
Scientific paper
10.1007/BF02702282
We describe the TreePM method for carrying out large N-Body simulations to study formation and evolution of the large scale structure in the Universe. This method is a combination of Barnes and Hut tree code and Particle-Mesh code. It combines the automatic inclusion of periodic boundary conditions of PM simulations with the high resolution of tree codes. This is done by splitting the gravitational force into a short range and a long range component. We describe the splitting of force between these two parts. We outline the key differences between TreePM and some other N-Body methods.
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