arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 1602.09062math.NAcs.NAphysics.comp-ph
收藏

相对论维拉尔-麦克斯韦方程组在经典极限下的渐近保持方案

An asymptotic preserving scheme for the relativistic Vlasov--Maxwell equations in the classical limit

INRIA(法国国家信息与自动化研究所);IRMAR(雷恩数学与应用数学研究中心);University of Innsbruck(因斯布鲁克大学);ENS Cachan(巴黎高等师范学院卡昂分校)

Nicolas Crouseilles, Lukas Einkemmer, Erwan Faou

AI总结:

本文提出一种渐近保持数值方案,用于处理相对论维拉尔-麦克斯韦方程组在光速趋于无穷大的经典极限下的收敛问题,通过时间分裂方法和隐式时间积分器抑制高频振荡,并通过数值模拟验证了方案在相对论和经典极限下的性能。

摘要:

我们考虑相对论维拉尔-麦克斯韦(RVM)方程组在光速 $c$ 趋向于无穷大的极限情况下的行为。在此极限下,RVM系统收敛到维拉尔-泊松系统,本文的目标是构造一种渐近保持的数值方案,以鲁棒地处理这一极限。我们的方法采用时间分裂方法处理RVM系统,利用隐式时间积分器对麦克斯韦方程组进行求解,以抑制数值解中逐渐增大的高频振荡。进行了若干数值模拟以研究所提出的数值方案在相对论和经典极限下的性能。此外,我们还推导了连续和离散问题中Weibel不稳定性 dispersion relation。

英文摘要:

We consider the relativistic Vlasov--Maxwell (RVM) equations in the limit when the light velocity $c$ goes to infinity. In this regime, the RVM system converges towards the Vlasov--Poisson system and the aim of this paper is to construct asymptotic preserving numerical schemes that are robust with respect to this limit. Our approach relies on a time splitting approach for the RVM system employing an implicit time integrator for Maxwell's equations in order to damp the higher and higher frequencies present in the numerical solution. A number of numerical simulations are conducted in order to investigate the performances of our numerical scheme both in the relativistic as well as in the classical limit regime. In addition, we derive the dispersion relation of the Weibel instability for the continuous and the discretized problem.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑