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激光尾场加速器粒子模拟中的非物理动力学效应。

Unphysical kinetic effects in particle-in-cell modeling of laser wakefield accelerators.

作者信息

Cormier-Michel Estelle, Shadwick B A, Geddes C G R, Esarey E, Schroeder C B, Leemans W P

机构信息

Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA.

出版信息

Phys Rev E Stat Nonlin Soft Matter Phys. 2008 Jul;78(1 Pt 2):016404. doi: 10.1103/PhysRevE.78.016404. Epub 2008 Jul 23.

Abstract

Unphysical heating and macroparticle trapping that arise in the numerical modeling of laser wakefield accelerators using particle-in-cell codes are investigated. A dark current free laser wakefield accelerator stage, in which no trapping of background plasma electrons into the plasma wave should occur, and a highly nonlinear cavitated wake with self-trapping, are modeled. Numerical errors can lead to errors in the macroparticle orbits in both phase and momentum. These errors grow as a function of distance behind the drive laser and can be large enough to result in unphysical trapping in the plasma wake. The resulting numerical heating in intense short-pulse laser-plasma interactions grows much faster and to a higher level than the known numerical grid heating of an initially warm plasma in an undriven system. The amount of heating, at least in the region immediately behind the laser pulse, can, in general, be decreased by decreasing the grid size, increasing the number of particles per cell, or using smoother interpolation methods. The effect of numerical heating on macroparticle trapping is less severe in a highly nonlinear cavitated wake, since trapping occurs in the first plasma wave period immediately behind the laser pulse.

摘要

研究了在使用粒子模拟代码对激光尾场加速器进行数值模拟时出现的非物理加热和大粒子俘获现象。对一个无暗电流的激光尾场加速器阶段进行了建模,在该阶段不应发生背景等离子体电子被捕获到等离子体波中的情况,还对一个具有自俘获的高度非线性空化尾场进行了建模。数值误差会导致大粒子轨道在相位和动量上出现误差。这些误差会随着驱动激光后面距离的增加而增大,并且可能大到足以导致在等离子体尾场中出现非物理俘获。在强短脉冲激光 - 等离子体相互作用中产生的数值加热,其增长速度比已知的无驱动系统中初始温热等离子体的数值网格加热要快得多,且达到的水平更高。一般来说,至少在激光脉冲后面紧邻的区域,通过减小网格尺寸、增加每个单元格中的粒子数量或使用更平滑的插值方法,可以减少加热量。在高度非线性空化尾场中,数值加热对大粒子俘获的影响不太严重,因为俘获发生在激光脉冲后面紧邻的第一个等离子体波周期内。

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