粒子在极强电磁波场中的加速

K. Thielheim
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引用次数: 1

摘要

这篇论文可以在高能宇宙射线粒子起源的研究中看到。基于洛伦兹方程的不含辐射反应的平面波形式,在波幅中等强度的情况下,足以描述粒子动力学。粒子运动在速度空间中是周期性的,因此粒子能量有一个上限。我们已经证明,没有辐射反应的平面波形式也是定义和计算球形波场中粒子动力学重要特征的有力工具。这些特征包括加速边界、等离子体边界和渐近能量定律。在极强的波场中,必须考虑到辐射力的影响。受辐射反应影响的运动在速度空间中不再是周期性的。粒子,至少在原则上,可以获得无限的能量。这可能与宇宙粒子加速到极高能量有关,例如,在与旋转磁化构型相关的宇宙射流中。人们也可以想到由连接天然或人造卫星的激光束组成的人造喷气机。本文的目的是提出和讨论一些结果,这些结果可能对上述背景感兴趣。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Particle acceleration in extremely strong electromagnetic wave fields
The present paper can be seen in the context of work on the origin of high energy cosmic ray particles. The plane-wave formalism without radiation reaction based on the Lorentz equation is adequate for the description of particle dynamics if the wave amplitude is of moderate strength. Particle motion then is periodic in velocity space so that there is an upper limit to particle energy. We have shown that the plane-wave formalism without radiation reaction also is a powerful tool to define and to calculate important features of particle dynamics in spherical wave fields. Among these features are the acceleration boundary, the plasma border and the law of asymptotic energy. In extremely strong wave fields the influence of radiation forces has to be taken into account. Motion under the influence of the radiation reaction is no longer periodic in velocity space. Particles, at least in principle, can achieve unlimited values of energy. This may be relevant for the cosmic particle acceleration to extremely high energies as, for example, in cosmic jets associated with rotating magnetized configurations. One may also think of man made jets constituted of laser beams connecting natural or artificial satellites. It is the intention of this paper to present and to discuss some results, which may be of interest in the above mentioned context.<>
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