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自引力系统的热力学

Thermodynamics of self-gravitating systems.

作者信息

Chavanis Pierre-Henri, Rosier Carole, Sire Clément

机构信息

Laboratoire de Physique Quantique-UMR CNRS 5626, Université Paul Sabatier, 118, route de Narbonne, 31062 Toulouse, France.

出版信息

Phys Rev E Stat Nonlin Soft Matter Phys. 2002 Sep;66(3 Pt 2A):036105. doi: 10.1103/PhysRevE.66.036105. Epub 2002 Sep 10.

DOI:10.1103/PhysRevE.66.036105
PMID:12366182
Abstract

We study the thermodynamics and the collapse of a self-gravitating gas of Brownian particles. We consider a high-friction limit in order to simplify the problem. This results in the Smoluchowski-Poisson system. Below a critical energy or below a critical temperature, there is no equilibrium state and the system develops a self-similar collapse leading to a finite time singularity. In the microcanonical ensemble, this corresponds to a "gravothermal catastrophe" and in the canonical ensemble to an "isothermal collapse." Self-similar solutions are investigated analytically and numerically.

摘要

我们研究了布朗粒子自引力气体的热力学和坍缩。为了简化问题,我们考虑了高摩擦极限。这导致了斯莫卢霍夫斯基 - 泊松系统。在临界能量以下或临界温度以下,不存在平衡态,系统会发生自相似坍缩,导致有限时间奇点。在微正则系综中,这对应于“引力热灾变”,在正则系综中对应于“等温坍缩”。我们对自相似解进行了解析和数值研究。

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