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Weibel Instability Growth Rate in Magnetized Plasmas with Quasi-Relativistic Distribution Function

Weibel Instability Growth Rate in Magnetized Plasmas with Quasi-Relativistic Distribution Function

作     者:Sayed Ahmad Hosseini Mohammad Mahdavi 

作者机构:Physics Department University of Mazandaran 

出 版 物:《Communications in Theoretical Physics》 (理论物理通讯(英文版))

年 卷 期:2016年第65卷第12期

页      面:709-712页

核心收录:

学科分类:080904[工学-电磁场与微波技术] 07[理学] 0809[工学-电子科学与技术(可授工学、理学学位)] 08[工学] 070204[理学-等离子体物理] 0810[工学-信息与通信工程] 081105[工学-导航、制导与控制] 081001[工学-通信与信息系统] 0704[理学-天文学] 081002[工学-信号与信息处理] 0825[工学-航空宇航科学与技术] 0811[工学-控制科学与工程] 0702[理学-物理学] 

主  题:磁化等离子体 Weibel 不稳定性 相对论 增长率 分布函数 电子回旋 碰撞效应 

摘      要:The mechanism of the Weibel instability is investigated for dense magnetized plasmas. As we know, due to the electron velocity distribution, the Coulomb collision effect of electron-ion and the relativistic properties play an important role in such study. In this study an analytical expression for the growth rate and the condition of restricting the Weibel instability are derived for low-frequency limit. These calculations are done for the oscillation frequency dependence on the electron cyclotron frequency. It is shown that, the relativistic properties of the particle lead to increasing the growth rate of the instability. On the other hand the collision effects and background magnetic field try to decrease the growth rate by decreasing the temperature anisotropy and restricting the particles movement.

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