Gravitational instability of a nonrotating galaxy

被引：0
|
作者：
Chao, AW [1 ]
机构：
[1] Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA
来源：
HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION | 2006年 / 30卷
关键词：
galaxy; gravitational instability; Vlasov eguation; Landau damping;
D O I：
暂无
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
Gravitational instability of the distribution of stars in a galaxy is a well-known phenomenon in astrophysics. This work is a preliminary attempt to analyze this phenomenon using the standard tools developed in accelerator physics. By applying this analysis, it is found that a stable nonrotating galaxy would become unstable if its size exceeds a certain limit that depends on its mass density.
引用
收藏
页码：6 / 10
页数：5
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