高压气体中的相对论电子束输运:鼻物理的热流体处理

R. Roubaud, P. Maggi-Videlaine
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引用次数: 0

摘要

在超相对论性电子束穿过初始中性致密气体的束头处,径向离焦静电力几乎被自磁挤压力抵消。因此,波束头几乎是力费的,并以由波束发射率决定的速率遭受诺德西克膨胀。在下游,由于次级等离子体中驱动的轴向感应电场,束流电子失去能量并向外扩散。这种欧姆侵蚀与诺德斯克的侵蚀结合在一起。作者对该梁进行了数值研究。鼻子物理的热流体处理允许光束具有其轮廓扭曲,同时比粒子代码消耗更少的时间。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Relativistic electron beam transport in high pressure gases: a warm fluid treatment of nose physics
At the beam head of an ultrarelativistic electron beam propagating through an initially neutral dense gas, the radial defocusing electrostatic force is nearly cancelled by the self-magnetic pinching force. The beam head is thus almost force fee and suffers Nordsieck expansion at a rate governed by the beam emittance. Downstream, owing to the axial inductive electric field driven in the secondary plasma, beam electrons lose energy and spread out. This ohmic erosion combines with that of Nordsieck. The authors have carried out a numerical study of the beam. The warm fluid treatment of the nose physics allows the beam to have its profile distorted while being less time consuming than a particle code.<>
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