Radial orbit instability as a dissipation-induced phenomenon

被引：11

作者：

Marechal, L. ^{[1
]}

Perez, J. ^{[1
]}

机构：

[1] ENSTA, Lab Math Appl, Paris, France

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2010年 / 405卷 / 04期

关键词：

gravitation; instabilities; methods: analytical; stars: kinematics and dynamics; SPHERICAL STELLAR-SYSTEMS; STAR-CLUSTERS; STABILITY; UNIVERSAL; COLLAPSE; HALOS;

D O I：

10.1111/j.1365-2966.2010.16663.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper is devoted to radial orbit instability in the context of self-gravitating dynamical systems. We present this instability in the new frame of dissipation-induced instability theory. This allows us to obtain a rather simple proof based on energetics arguments and to clarify the associated physical mechanism.

引用

页码：2785 / 2790

页数：6

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