Integer lattice dynamics for Vlasov-Poisson

被引:4
|
作者
Mocz, Philip [1 ]
Succi, Sauro [2 ,3 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[2] CNR, Ist Appl Calcolo, Viale Policlin 137, I-00161 Rome, Italy
[3] Harvard Sch Engn & Appl Sci, Inst Appl Computat Sci, Northwest B162,52, Cambridge, MA 02138 USA
基金
美国国家科学基金会;
关键词
gravitation; methods: numerical; stars: kinematics and dynamics; galaxies: kinematics and dynamics; dark matter; COLLISIONLESS; SIMULATION; MESH; CODE;
D O I
10.1093/mnras/stw2928
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We revisit the integer lattice (IL) method to numerically solve the Vlasov-Poisson equations, and show that a slight variant of the method is a very easy, viable, and efficient numerical approach to study the dynamics of self-gravitating, collisionless systems. The distribution function lives in a discretized lattice phase-space, and each time-step in the simulation corresponds to a simple permutation of the lattice sites. Hence, the method is Lagrangian, conservative, and fully time-reversible. IL complements other existing methods, such as N-body/ particle mesh (computationally efficient, but affected by Monte Carlo sampling noise and two-body relaxation) and finite volume (FV) direct integration schemes (expensive, accurate but diffusive). We also present improvements to the FV scheme, using a moving-mesh approach inspired by IL, to reduce numerical diffusion and the time-step criterion. Being a direct integration scheme like FV, IL is memory limited (memory requirement for a full 3D problem scales as N-6, where N is the resolution per linear phase- space dimension). However, we describe a new technique for achieving N-4 scaling. The method offers promise for investigating the full 6D phase- space of collisionless systems of stars and dark matter.
引用
收藏
页码:3154 / 3162
页数:9
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