Interactions between dust grains in a dusty plasma

被引:281
|
作者
Lampe, M [1 ]
Joyce, G
Ganguli, G
Gavrishchaka, V
机构
[1] USN, Res Lab, Div Plasma Phys, Washington, DC 20375 USA
[2] Sci Applicat Int Corp, Mclean, VA 22102 USA
关键词
D O I
10.1063/1.1288910
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
Dust grains in plasma acquire a large negative charge, and can constitute a strongly coupled system. If the plasma is stationary, the plasma-mediated electrostatic potential around a single grain can be calculated by orbital-motion-limited (OML) theory, including ion absorption at the grain surface. This potential is repulsive at all ranges, and falls off as r(-2) at long range. Nonlinear modifications occur when there are several grains, but the interaction is still repulsive. If the plasma is streaming by the grains, each grain generates a wake field potential which can be calculated via linear response theory, and which attracts other grains to stationary points behind the grain. There is in addition an attractive force between grains, due to ion-impact momentum deposition. In certain parameter regimes, this "shadowing" force can yield a weak net attraction at long range. Trapped-ion effects are significant at high plasma density, but have not yet been calculated. (C) 2000 American Institute of Physics. [S1070-664X(00)01310-0].
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页码:3851 / 3861
页数:11
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