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长尺度近似下自旋1/2粒子的相对论动力学方程。

Relativistic kinetic equation for spin-1/2 particles in the long-scale-length approximation.

作者信息

Ekman R, Asenjo F A, Zamanian J

机构信息

Department of Physics, Umeå University, SE-901 87 Umeå, Sweden.

Facultad de Ingeniería y Ciencias, Universidad Adolfo Ibáñez, Santiago 7941169, Chile.

出版信息

Phys Rev E. 2017 Aug;96(2-1):023207. doi: 10.1103/PhysRevE.96.023207. Epub 2017 Aug 22.

Abstract

In this paper, we derive a fully relativistic kinetic theory for spin-1/2 particles and its coupling to Maxwell's equations, valid in the long-scale-length limit, where the fields vary on a scale much longer than the localization of the particles; we work to first order in ℏ. Our starting point is a Foldy-Wouthuysen (FW) transformation, applicable to this regime, of the Dirac Hamiltonian. We derive the corresponding evolution equation for the Wigner quasidistribution in an external electromagnetic field. Using a Lagrangian method we find expressions for the charge and current densities, expressed as free and bound parts. It is furthermore found that the velocity is nontrivially related to the momentum variable, with the difference depending on the spin and the external electromagnetic fields. This fact that has previously been discussed as "hidden momentum" and is due to that the FW transformation maps pointlike particles to particle clouds for which the prescription of minimal coupling is incorrect, as they have multipole moments. We express energy and momentum conservation for the system of particles and the electromagnetic field, and discuss our results in the context of the Abraham-Minkowski dilemma.

摘要

在本文中,我们推导了一种适用于自旋为1/2粒子的完全相对论性动力学理论及其与麦克斯韦方程组的耦合,该理论在长尺度极限下有效,即场的变化尺度远长于粒子的局域化尺度;我们在ħ的一阶近似下进行研究。我们的出发点是适用于此情形的狄拉克哈密顿量的福尔德 - 乌斯怀森(FW)变换。我们推导了外电磁场中维格纳准分布的相应演化方程。使用拉格朗日方法,我们找到了电荷和电流密度的表达式,它们表示为自由部分和束缚部分。此外,我们发现速度与动量变量有非平凡的关系,其差异取决于自旋和外电磁场。这一事实此前被讨论为“隐藏动量”,其原因在于FW变换将点状粒子映射为粒子云,对于粒子云而言,最小耦合的规定是不正确的,因为它们具有多极矩。我们阐述了粒子与电磁场系统的能量和动量守恒,并在亚伯拉罕 - 闵可夫斯基困境的背景下讨论了我们的结果。

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