Grassi A, Grech M, Amiranoff F, Pegoraro F, Macchi A, Riconda C
LULI, UPMC Université Paris 06: Sorbonne Universités, CNRS, Ecole Polytechnique, CEA, Université Paris-Saclay, F-75252 Paris Cedex 05, France.
Dipartimento di Fisica Enrico Fermi, Università di Pisa, Largo Bruno Pontecorvo 3, I-56127 Pisa, Italy.
Phys Rev E. 2017 Feb;95(2-1):023203. doi: 10.1103/PhysRevE.95.023203. Epub 2017 Feb 3.
The Weibel instability driven by two symmetric counterstreaming relativistic electron plasmas, also referred to as current-filamentation instability, is studied in a constant and uniform external magnetic field aligned with the plasma flows. Both the linear and nonlinear stages of the instability are investigated using analytical modeling and particle-in-cell simulations. While previous studies have already described the stabilizing effect of the magnetic field, we show here that the saturation stage is only weakly affected. The different mechanisms responsible for the saturation are discussed in detail in the relativistic cold fluid framework considering a single unstable mode. The application of an external field leads to a slight increase of the saturation level for large wavelengths, while it does not affect the small wavelengths. Multimode and temperature effects are then investigated. While at high temperature the saturation level is independent of the external magnetic field, at low but finite temperature the competition between different modes in the presence of an external magnetic field leads to a saturation level lower with respect to the unmagnetized case.
由两个对称的反向流动相对论电子等离子体驱动的韦贝尔不稳定性,也称为电流丝化不稳定性,在与等离子体流对齐的恒定且均匀的外部磁场中进行了研究。使用解析模型和粒子模拟研究了不稳定性的线性和非线性阶段。虽然先前的研究已经描述了磁场的稳定作用,但我们在此表明饱和阶段仅受到微弱影响。在相对论冷流体框架下,考虑单个不稳定模式,详细讨论了导致饱和的不同机制。施加外部磁场会导致大波长的饱和水平略有增加,而对小波长没有影响。然后研究了多模和温度效应。在高温下,饱和水平与外部磁场无关,而在低温但有限温度下,存在外部磁场时不同模式之间的竞争导致饱和水平相对于无磁化情况更低。