RelSIM: A Relativistic Semi-implicit Method for Particle-in-cell Simulations

被引:5
作者
Bacchini, Fabio [1 ,2 ]
机构
[1] Katholieke Univ Leuven, Ctr Math Plasma Astrophys, Dept Math, Celestijnenlaan 200B, B-3001 Leuven, Belgium
[2] Solar Terr Ctr Excellence, Royal Belgian Inst Space Aeron, Ringlaan 3, B-1180 Uccle, Belgium
基金
美国国家科学基金会;
关键词
CHARGE CONSERVATION; MAGNETIC RECONNECTION; PLASMA SIMULATION; FULLY IMPLICIT; ENERGY; ACCELERATION; ELECTRON; SHOCKS; CODE; LAW;
D O I
10.3847/1538-4365/acefba
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a novel Relativistic Semi-Implicit Method (RelSIM) for particle-in-cell (PIC) simulations of astrophysical plasmas, implemented in a code framework ready for production runs. While explicit PIC methods have gained widespread recognition in the astrophysical community as a reliable tool to simulate plasma phenomena, implicit methods have been seldom explored. This is partly due to the lack of a reliable relativistic implicit PIC formulation that is applicable to state-of-the-art simulations. We propose the RelSIM to fill this gap: our new method is relatively simple, being free of nonlinear iterations and only requiring a global linear solve of the field equations. With a set of one- and two-dimensional tests, we demonstrate that the RelSIM produces more accurate results with much smaller numerical errors in the total energy than standard explicit PIC, in particular when characteristic plasma scales (skin depth and plasma frequency) are heavily underresolved on the numerical grid. By construction, the RelSIM also performs much better than the relativistic implicit-moment method, originally proposed for semi-implicit PIC simulations in the relativistic regime. Our results are promising to conduct large-scale (in terms of duration and domain size) PIC simulations of astrophysical plasmas, potentially reaching physical regimes inaccessible by standard explicit PIC codes.
引用
收藏
页数:16
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