期刊
JOURNAL OF ASTROPHYSICS AND ASTRONOMY
卷 23, 期 3-4, 页码 185-196出版社
INDIAN ACADEMY SCIENCES
DOI: 10.1007/BF02702282
关键词
gravitation; methods : numerical; cosmology : large scale structure of the universe
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 dcodes. 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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