Kinetic theory of Jeans instability

被引:0
|
作者
Trigger, SA [1 ]
Ershkovich, AI
van Heijst, GJF
Schram, PPJM
机构
[1] Russian Acad Sci, Joint Inst High Temp, Moscow 127412, Russia
[2] Tel Aviv Univ, IL-69978 Tel Aviv, Israel
[3] Eindhoven Univ Technol, NL-5600 MB Eindhoven, Netherlands
来源
PHYSICAL REVIEW E | 2004年 / 69卷 / 06期
关键词
D O I
暂无
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
Kinetic treatment of the Jeans gravitational instability, with collisions taken into account, is presented. The initial-value problem for the distribution function which obeys the kinetic equation, with the collision integral conserving the number of particles, is solved. Dispersion relation is obtained and analyzed. New modes are found. Collisions are shown not to affect the Jeans instability criterion. Although the instability growth rate diminishes, the collisions they cannot quench the instability. However, the oscillation spectrum is modified significantly: even in the neighborhood of the threshold frequency omega=0 (separating stable and unstable modes) the spectrum of oscillations can strongly depend on the collision frequency. Propagating (rather than aperiodic) modes are also found. These modes, however, are strongly damped.
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页数:6
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