Dust-induced instability with dust charge fluctuations in a rotating dusty plasma

被引：3

作者：

Yang, Xiao-Song ^{[1
]}

Wang, Bing ^{[1
,2
]}

Chen, Hui ^{[1
]}

Chen, Xiao-Chang ^{[1
,2
]}

Liu, San-Qiu ^{[1
]}

机构：

[1] Nanchang Univ, Dept Phys, Nanchang 330031, Jiangxi, Peoples R China

[2] Nanchang Univ, Expt Ctr Basic Phys, Sch Sci, Nanchang 330031, Jiangxi, Peoples R China

来源：

EUROPEAN PHYSICAL JOURNAL D | 2020年 / 74卷 / 06期

基金：

中国国家自然科学基金;

关键词：

Plasma Physics; ACOUSTIC-WAVES; TRANSPORT; IMPURITIES; TURBULENCE;

D O I：

10.1140/epjd/e2020-10229-x

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

The dust-induced instability involving charge fluctuations is studied in rotating dusty plasma. Due to dust charging dynamics, the dust-induced instability mode which was first put forward by Mikhailovskii et al. [A.B. Mikhailovskii, S.V. Vladimirov, J.G. Lominadze, V.S. Tsypin, A.P. Churikov, N.N. Erokhin, R.M.O. Galvao, Phys. Plasmas15, 014504 (2008)] will be replaced by dust-charging-rotational instability (DCRI) mode. Comparing to the dust-induced instability, the new instability mode also exists in an increasing rotation frequency profile, but always with a greater growth rate. The analysis indicates that the rotational instability mode induced by dust charge is always unstable. The present results may be used to investigate the rotating dusty plasma experiments and observations.

引用

页数：5

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