Particle-based sampling of N-body simulations

被引:6
|
作者
Faber, N. T. [1 ,2 ,3 ,4 ]
Stibbe, D. [3 ,4 ]
Portegies Zwart, S. [5 ]
McMillan, S. L. W. [6 ]
Boily, C. M. [1 ,2 ]
机构
[1] Univ Strasbourg, Astron Observ, F-67000 Strasbourg, France
[2] CNRS, UMR 7550, F-67000 Strasbourg, France
[3] Univ Amsterdam, Sterrekundig Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[4] Univ Amsterdam, Sect Computat Sci, NL-1098 SJ Amsterdam, Netherlands
[5] Leiden Univ, Sterrewacht Leiden, NL-2300 RA Leiden, Netherlands
[6] Drexel Univ, Dept Phys, Philadelphia, PA 19104 USA
关键词
methods: N-body simulations; methods: numerical; stars: kinematics; STELLAR DYNAMICS; SYSTEMS; EVOLUTION; CLUSTERS;
D O I
10.1111/j.1365-2966.2009.15775.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper introduces a novel approach for sampling the orbits of an N-body simulation. The gist of the method is to exploit individual phase-space coordinates acquired during integration of the equations of motion. This technique, which we dub 'particle-based sampling scheme', is tailor-made for resolving rapid time-variation of coordinates when needed. The PBaSS requires less disk space (by factors of 10 or more) to retrieve orbits at a chosen accuracy than those reconstructed using the classic snapshot approach. Furthermore, the PBaSS also allows a reconstruction of the system at any time-resolution not smaller than the smallest integration time-step in a post-simulation treatment, thus avoiding costly simulation reruns.
引用
收藏
页码:1898 / 1903
页数:6
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