A multiple time step symplectic algorithm for integrating close encounters

被引:431
作者
Duncan, MJ [1 ]
Levison, HF
Lee, MH
机构
[1] Queens Univ, Dept Phys, Kingston, ON K7L 3N6, Canada
[2] SW Res Inst, Dept Space Sci, Boulder, CO 80302 USA
关键词
celestial mechanics; stellar dynamics; methods : numerical; planetary systems; solar system : general;
D O I
10.1086/300541
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a new symplectic algorithm that has the desirable properties of the sophisticated but highly efficient numerical algorithms known as mixed variable symplectic (MVS) methods and that, in addition, can handle close encounters between objects. This technique is based on a variant of the standard MVS methods, but it handles close encounters by employing a multiple time step technique. When the bodies are well separated, the algorithm has the speed of MVS methods, and whenever two bodies suffer a mutual encounter, the time step for the relevant bodies is recursively subdivided to whatever level is required. We demonstrate the power of this method using several tests of the technique. We believe that this algorithm will be a valuable tool for the study of planetesimal dynamics and planet formation.
引用
收藏
页码:2067 / 2077
页数:11
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