Relativistic Stellar Clusters: Equilibrium Models with Anisotropic Momentum Distribution and Dynamic and Thermodynamic Stability of Isotropic Models

被引：0

作者：

Merafina, Marco ^{[1
]}

Bisnovatyi-Kogan, Gennady S. ^{[2
]}

Vaccarelli, Maria Rosaria ^{[1
]}

机构：

[1] Univ Roma La Sapienza, Dept Phys, Piazzale Aldo Moro 2, I-00185 Rome, Italy

[2] IKI, Space Res Inst, Moscow 117997, Russia

来源：

ASTROPHYSICS AND COSMOLOGY AFTER GAMOW | 2009年 / 1206卷

关键词：

Relativity; Stellar Clusters; Anisotropy; Stability; STAR-CLUSTERS; CUTOFF; SYSTEMS; COLLAPSE; ENERGY; PARTICLES; SPHERES;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Models of spherically symmetric relativistic stellar clusters with anisotropic distribution functions in relativistic regime are described by using Maxwellian distribution function with energy cutoff. We consider distributions with different levels of anisotropy and discuss some general characteristics of the models. In addition, we analyze dynamic and thermodynamic stability of isotropic models still described by Maxwellian distribution function with energy cutoff and we find critical values of the onset of instability.

引用

页码：399 / +

页数：2

共 46 条

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