Interaction of an intense relativistic electron beam with a plasma-filled waveguide in a magnetic field

B. Poole, B. Chang, J. F. Camacho
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Abstract

Analytic computations and particle-in-cell (PIC) code simulations for the interaction of an intense relativistic electron beam (REB) and a plasma have been carried out. In the simulations, a fast risetime ( approximately 5 ns) 10-kA REB (1 MeV) was injected into a plasma-filled waveguide immersed in an axial magnetic field. Beam transport and microwave generation by beam-plasma instabilities were investigated in both the infinite- and finite-B-field cases. In the finite-B-field case, both the two-stream and cyclotron instabilities were important. Calculations of charge and current neutralization of the REB were performed in the intense beam regime. These calculations provided the appropriate parameters for the linear dispersion relation of the system, which was solved to determine the nature of the instabilities. For large magnetic fields the linearly unstable waves on the lower branch of the dispersion curve can backscatter off the accumulation of plasma electrons at the beam front produced in the charge neutralization process. These backscattered waves can then mix with the original unstable wave in a three-wave process to produce a wave on the upper branch of the dispersion curve at a higher-frequency. Still higher frequencies can be produced by a cascading of wave-mixing processes.<>
磁场中强相对论电子束与等离子体填充波导的相互作用
本文对强相对论电子束(REB)与等离子体相互作用进行了解析计算和粒子池(PIC)代码模拟。在模拟中,将快速上升时间约为5 ns的10-kA REB (1 MeV)注入浸入轴向磁场中的等离子体填充波导中。在无限和有限b场情况下,研究了束流等离子体不稳定性引起的束流输运和微波产生。在有限b场的情况下,双流和回旋加速器的不稳定性都很重要。计算了强束流条件下REB的电荷和电流中和作用。这些计算为系统的线性色散关系提供了合适的参数,并对其进行求解以确定不稳定性的性质。在大磁场下,色散曲线下支的线性不稳定波可以反向散射电荷中和过程中产生的束前等离子体电子积累。然后,这些反向散射波可以在三波过程中与原始不稳定波混合,在色散曲线的上分支上产生频率更高的波。通过级联的波混合过程还可以产生更高的频率。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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