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相对论、非广延性与扩展幂律分布。

Relativity, nonextensivity, and extended power law distributions.

作者信息

Silva R, Lima J A S

机构信息

Observatório Nacional, Rua Gal. José Cristino 77, 20921-400 Rio de Janeiro, Rio de Janeiro, Brazil and Universidade do Estado do Rio Grande do Norte, 59610-210, Mossoró, RN, Brazil.

出版信息

Phys Rev E Stat Nonlin Soft Matter Phys. 2005 Nov;72(5 Pt 2):057101. doi: 10.1103/PhysRevE.72.057101. Epub 2005 Nov 11.

Abstract

A proof of the relativistic theorem by including nonextensive effects is given. As it happens in the nonrelativistic limit, the molecular chaos hypothesis advanced by Boltzmann does not remain valid, and the second law of thermodynamics combined with a duality transformation implies that the parameter lies on the interval [0,2]. It is also proven that the collisional equilibrium states (null entropy source term) are described by the relativistic power law extension of the exponential Juttner distribution which reduces, in the nonrelativistic domain, to the Tsallis power law function. As a simple illustration of the basic approach, we derive the relativistic nonextensive equilibrium distribution for a dilute charged gas under the action of an electromagnetic field . Such results reduce to the standard ones in the extensive limit, thereby showing that the nonextensive entropic framework can be harmonized with the space-time ideas contained in the special relativity theory.

摘要

给出了一个包含非广延效应的相对论定理的证明。正如在非相对论极限情况下发生的那样,玻尔兹曼提出的分子混沌假设不再成立,并且结合对偶变换的热力学第二定律意味着该参数位于区间[0,2]内。还证明了碰撞平衡态(零熵源项)由指数于特纳分布的相对论幂律扩展来描述,在非相对论域中它简化为 Tsallis 幂律函数。作为基本方法的一个简单示例,我们推导了在电磁场作用下稀薄带电气体的相对论非广延平衡分布。这些结果在广延极限下简化为标准结果,从而表明非广延熵框架可以与狭义相对论中包含的时空观念相协调。

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