Ion-dust streaming instability with non-Maxwellian ions

被引:20
|
作者
Kaehlert, Hanno [1 ]
机构
[1] Univ Kiel, Inst Theoret Phys & Astrophys, D-24098 Kiel, Germany
关键词
ACOUSTIC INSTABILITY; COMPLEX PLASMAS; WAVES;
D O I
10.1063/1.4926531
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The influence of non-Maxwellian ions on the ion-dust streaming instability in a complex plasma is investigated. The ion susceptibility employed for the calculations self-consistently accounts for the acceleration of the ions by a homogeneous background electric field and their collisions with neutral gas particles via a Bhatnagar-Gross-Krook collision term [e.g., A. V. Ivlev et al., Phys. Rev. E 71, 016405 (2005)], leading to significant deviations from a shifted Maxwellian distribution. The dispersion relation and the properties of the most unstable mode are studied in detail and compared with the Maxwellian case. The largest deviations occur at low to intermediate ion-neutral damping. In particular, the growth rate of the instability for ion streaming below the Bohm speed is found to be lower than in the case of Maxwellian ions, yet remains on a significant level even for fast ion flows above the Bohm speed. (C) 2015 AIP Publishing LLC.
引用
收藏
页数:7
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