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温度和κ的热力学定义以及熵缺陷的介绍。

Thermodynamic Definitions of Temperature and Kappa and Introduction of the Entropy Defect.

作者信息

Livadiotis George, McComas David J

机构信息

Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA.

出版信息

Entropy (Basel). 2021 Dec 15;23(12):1683. doi: 10.3390/e23121683.

DOI:10.3390/e23121683
PMID:34945989
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8700829/
Abstract

This paper develops explicit and consistent definitions of the independent thermodynamic properties of temperature and the kappa index within the framework of nonextensive statistical mechanics and shows their connection with the formalism of kappa distributions. By defining the "entropy defect" in the composition of a system, we show how the nonextensive entropy of systems with correlations differs from the sum of the entropies of their constituents of these systems. A system is composed extensively when its elementary subsystems are independent, interacting with no correlations; this leads to an extensive system entropy, which is simply the sum of the subsystem entropies. In contrast, a system is composed nonextensively when its elementary subsystems are connected through long-range interactions that produce correlations. This leads to an entropy defect that quantifies the missing entropy, analogous to the mass defect that quantifies the mass (energy) associated with assembling subatomic particles. We develop thermodynamic definitions of kappa and temperature that connect with the corresponding kinetic definitions originated from kappa distributions. Finally, we show that the entropy of a system, composed by a number of subsystems with correlations, is determined using both discrete and continuous descriptions, and find: (i) the resulted entropic form expressed in terms of thermodynamic parameters; (ii) an optimal relationship between kappa and temperature; and (iii) the correlation coefficient to be inversely proportional to the temperature logarithm.

摘要

本文在非广延统计力学框架内给出了温度和κ指数这两个独立热力学性质的明确且一致的定义,并展示了它们与κ分布形式体系的联系。通过定义系统组成中的“熵缺陷”,我们说明了具有相关性的系统的非广延熵如何不同于这些系统各组成部分熵的总和。当一个系统的基本子系统相互独立、无关联地相互作用时,该系统是广延组成的;这会导致一个广延的系统熵,它仅仅是子系统熵的总和。相反,当一个系统的基本子系统通过产生相关性的长程相互作用连接时,该系统是非广延组成的。这会导致一个熵缺陷,它量化了缺失的熵,类似于量化与组装亚原子粒子相关的质量(能量)的质量缺陷。我们给出了与源自κ分布的相应动力学定义相关的κ和温度的热力学定义。最后,我们表明,由多个具有相关性的子系统组成的系统的熵,使用离散和连续描述均可确定,并发现:(i)以热力学参数表示的所得熵形式;(ii)κ与温度之间的最优关系;以及(iii)相关系数与温度对数成反比。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/af24004273c4/entropy-23-01683-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/87b5ccec8659/entropy-23-01683-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/3027ee43b1b7/entropy-23-01683-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/886ab5958347/entropy-23-01683-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/af24004273c4/entropy-23-01683-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/87b5ccec8659/entropy-23-01683-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/3027ee43b1b7/entropy-23-01683-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/886ab5958347/entropy-23-01683-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a807/8700829/af24004273c4/entropy-23-01683-g004.jpg

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