COAGULATION OF DUST PARTICLES IN A PLASMA

被引:116
|
作者
HORANYI, M [1 ]
GOERTZ, CK [1 ]
机构
[1] UNIV IOWA,DEPT PHYS & ASTRON,IOWA CITY,IA 52242
来源
ASTROPHYSICAL JOURNAL | 1990年 / 361卷 / 01期
关键词
Interstellar: grains; Plasmas;
D O I
10.1086/169178
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the electrostatic charge of small dust grains in a plasma in which the temperature varies in time and point out that secondary electron emission might introduce charge separation. If the sign of the charge on small grains is opposite to that on big ones, enhanced coagulation can occur which will affect the size distribution of grains in a plasma. We discuss two scenarios where this process might be relevant: a hot plasma environment with temperature fluctuations and a cold plasma environment with transient heating events. The importance of the enhanced coagulation is uncertain, because the plasma parameters in grain producing environments such as a molecular cloud or a protoplanetary disk are not known. It is possible, however, that this process is the most efficient mechanism for the growth of grains in the size range of 0.1-500 μm.
引用
收藏
页码:155 / 161
页数:7
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