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Information entropy and the statistical physics of the classical ideal gas

机译:经典理想气体的信息熵与统计物理学

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The link between statistical mechanics and information theory is examined with reference to the classical ideal gas. In particular, Jaynes’ assertion [E. T. Jaynes, Phys. Rev. 106(4), 620 (1957)] that a clear distinction between statistical and physical aspects, the latter consisting of the correct enumeration of the system’s states and their properties, is questioned in relation to the information entropy. Jaynes suggested that statistical mechanics need not be considered a physical theory, as the techniques of statistical inference lead to physically sensible results. However, we show that a physical theory of the statistics of the ideal gas leads to expressions for the information entropy that differ from those found in statistical mechanics because the probability distributions underlying the entropy differ from the canonical distribution. In particular, we show that the distribution of energy states accessible to a classical ideal gas connected to a thermal reservoir is given by the Gamma distribution and in open systems, in which the number of particles fluctuates, by a weighted sum of Gamma distributions. Computer simulations using a hard-sphere model of a classical ideal gas demonstrate the ideas. We compare the Shannon information entropy with the thermodynamic entropy and argue on the basis of the work presented here that information theoretic entropy and thermodynamic entropy, whilst seemingly related, are not necessarily identical.
机译:统计力学和信息论之间的联系是参考经典理想气体来检验的。特别是Jaynes的断言[E. T. Jaynes,物理学Rev. 106(4),620(1957)]认为,统计和物理方面之间存在明显的区别,后者是由系统状态及其属性的正确枚举组成的,这与信息熵有关。杰恩斯(Jaynes)提出,统计力学不必被视为一种物理理论,因为统计推断技术会导致物理上有意义的结果。但是,我们表明,理想气体统计的物理理论导致信息熵的表达式与统计力学中的表达式不同,这是因为熵背后的概率分布不同于规范分布。特别地,我们表明,连接到储热层的经典理想气体可访问的能态分布由Gamma分布给出,而在开放系统中,颗粒数量会波动,由Gamma分布的加权总和给出。使用经典理想气体的硬球模型进行的计算机模拟证明了这些想法。我们将香农信息熵与热力学熵进行了比较,并基于此处介绍的工作认为,信息理论熵和热力学熵虽然看似相关,但不一定相同。

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