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arXiv 2606.04478math.NAcs.NA
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强磁场下带电粒子动力学的一类新型高阶一致精确指数积分器与局部线性扩展

A novel class of high-order uniformly accurate exponential integrators with local linear extension for the charged-particle dynamics under strong magnetic field

School of Mathematics and Statistics, Xi’an Jiaotong University(西安交通大学数学与统计学院);University of Science and Technology Beijing(北京科技大学)

Lina Wang, Bin Wang, Beibei Zhu

AI总结:

针对强磁场下带电粒子动力学中的快速时间振荡问题,提出一类通过引入辅助多项式变量进行局部线性扩展的高阶一致精确指数积分器,无需阶条件即可达到任意高阶,并在最大排序强磁场下证明位置和速度的改进误差估计。

摘要:

本文针对强磁场下的带电粒子动力学,发展了一类新型的高阶一致精确指数积分器。小参数$0<\varepsilon\ll 1$引起快速时间振荡,使得传统数值方法因步长限制严格而计算成本过高。为解决此问题,采用引入辅助多项式变量的线性化技术,将原始带电粒子动力学重新表述为更高维的系统。随后将经典指数积分器应用于这一增强公式,该公式固有地包含更丰富的结构信息,从而产生一族一致精确的指数积分器,无需任何阶条件即可达到任意高阶。对于最大排序标度强磁场,我们通过代数技术严格证明,所提出的具有$k(k\geq 2)$次辅助多项式变量的方案在位置上实现了$\mathcal{O}(\varepsilon h^{k+1})$的改进误差估计,在速度上实现了均匀的$\mathcal{O}(h^{k+1})$误差估计。数值实验验证了方法的优势。最后,将理论和数值研究扩展到具有最大排序标度强磁场的四维框架下的相对论带电粒子动力学。

英文摘要:

In this paper, we develop a novel class of high-order uniformly accurate exponential integrators for charged-particle dynamics under strong magnetic field. The small parameter $0<\varepsilon\ll 1$ induces rapid temporal oscillations, rendering traditional numerical methods prohibitively expensive due to severe step-size restrictions. To address this issue, a linearization technology that introduces auxiliary polynomial variables is employed to recast the original charged-particle dynamics as a higher-dimensional system. Classical exponential integrators are subsequently applied to this augmented formulation, which inherently carries richer structural information, thereby yielding a family of uniformly accurate exponential integrators that can reach arbitrarily high order without requiring any order conditions. For strong magnetic fields under the maximal-ordering scaling, we rigorously establish through algebraic techniques that the schemes with auxiliary polynomial variables of degree $k\geq2$ achieve an improved position error bound of $\mathcal{O}(\min\{\varepsilon^{k+1}h,\varepsilon h^{k+1}\})$ and a uniform velocity error bound of $\mathcal{O}(\min\{\varepsilon^{k}h,h^{k+1}\})$, where $h$ denotes the time-step size. Under the additional condition that the magnetic field gradient vanishes at the origin, these bounds sharpen to $\mathcal{O}(\min\{\varepsilon^{k+2},\varepsilon h^{k+1}\})$ and $\mathcal{O}(\min\{\varepsilon^{k+1},h^{k+1}\})$ for the position and velocity, respectively, for $k\geq1$. The same sharper bounds hold for constant strong magnetic fields. Numerical experiments confirm the advantages of the proposed methods.

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。

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