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Extension of temperature anisotropy Weibel instability to non-Maxwellian plasmas by 2D PIC simulation

机译:2D PIC模拟将温度各向异性的延伸到非千年人等离子体的不稳定性

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The Weibel instability driven by temperature anisotropy is investigated in a two-dimensional (2D) particle-in-cell simulation in non-extensive statistics in the relativistic regime. In order to begin the simulation, we introduced a new 2D anisotropic distribution function in the context of non-extensive statistics. The heavy ions considered to be immobile and form the neutralizing background. The numerical results show that non-extensive parameter q plays an important role on the magnetic field saturation time, the time of reduction temperature anisotropy, evolution time to the quasi-stationary state, and the peak energy density of magnetic field. We observe that the instability saturation time increases by increasing the non-extensive parameter q. It is shown that structures with superthermal electrons (q 1) could generate strong magnetic fields during plasma thermalization. The simulation results agree with the previous simulations for an anisotropic Maxwellian plasma (q = 1).
机译:在相对论制度的非广泛统计中,在二维(2D)粒子内模拟中研究了由温度各向异性驱动的Weibel不稳定性。 为了开始模拟,我们在非广泛统计的背景下介绍了一个新的2D各向异性分布函数。 沉重的离子被认为是不动的,形成中和背景。 数值结果表明,非广泛的参数Q在磁场饱和时间,减少温度各向异性,演化时间到准静止状态的时间和磁场的峰值能量密度。 我们观察到不稳定饱和时间通过增加非广泛参数Q来增加。 结果表明,具有超高热电子(Q& 1)的结构可以在等离子体热化期间产生强磁场。 仿真结果与先前的各向异性Maxwell血浆(Q = 1)的模拟一致。

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