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Weibel instability oscillation in a dusty plasma with counter-streaming electrons

机译:用反流电子尘埃等离子体中的Weibel不稳定振荡

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摘要

We investigate the Weibel instability (WI) in a dusty plasma which is driven to oscillation by the addition of dust grains in the plasma. Our analysis predicts the existence of three modes in a dusty plasma. There is a high-frequency electromagnetic mode, whose frequency increases with an increase in the relative number density of dust grains and which approaches instability due to the presence of dust grains. The second mode is a damping mode which exists due to dust charge fluctuations in plasma. The third mode is the oscillating WI mode. The dispersion relation and the growth rate of various modes in the dusty plasma are derived using the first-order perturbation theory. The effect of dust grain parameters on frequency and growth rate is also studied and reported.
机译:我们在尘土飞离等离子体中调查Weibel不稳定性(Wi),通过添加等离子体中的灰尘颗粒被驱动到振荡。 我们的分析预测了粉尘等离子体中三种模式的存在。 存在高频电磁模式,其频率随着灰尘颗粒的相对数密度的增加而增加,并且由于粉尘晶粒的存在而接近不稳定性。 第二模式是由于等离子体中的灰尘电荷波动而存在的阻尼模式。 第三种模式是振荡Wi模式。 使用一阶扰动理论来源粉尘等离子体中各种模式的分散关系和生长速率。 还研究了粉尘晶粒参数对频率和生长速率的影响。

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