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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Virial coefficient ： ウィキペディア英語版 Virial coefficient Virial coefficients $B\_i$ appear as coefficients in the virial expansion of the pressure of a many-particle system in powers of the density, providing systematic corrections to the ideal gas law. They are characteristic of the interaction potential between the particles and in general depend on the temperature. The second virial coefficient $B\_2$ depends only on the pair interaction between the particles, the third ($B\_3$) depends on 2- and non-additive 3-body interactions, and so on. ==Derivation== The first step in obtaining a closed expression for virial coefficients is a cluster expansion of the grand canonical partition function :$\backslash Xi\; =\; \backslash sum\_\}\; =\; e^$ Here $p$ is the pressure, $V$ is the volume of the vessel containing the particles, $k\_B$ is Boltzmann's constant, $T$ is the absolute temperature, $\backslash lambda\; =\backslash exp()$ is the fugacity, with $\backslash mu$ the chemical potential. The quantity $Q\_n$ is the canonical partition function of a subsystem of $n$ particles: :$Q\_n\; =\; \backslash operatorname\; (e^).$ Here $H(1,2,\backslash ldots,n)$ is the Hamiltonian (energy operator) of a subsystem of $n$ particles. The Hamiltonian is a sum of the kinetic energies of the particles and the total $n$-particle potential energy (interaction energy). The latter includes pair interactions and possibly 3-body and higher-body interactions. The grand partition function $\backslash Xi$ can be expanded in a sum of contributions from one-body, two-body, etc. clusters. The virial expansion is obtained from this expansion by observing that $\backslash ln\; \backslash Xi$ equals $p\; V\; /\; (k\_B\; T\; )$. In this manner one derives :$B\_2\; =\; V\; \backslash left(\backslash frac-\backslash frac\backslash right)$ :$B\_3\; =\; V^2\; \backslash left(\backslash frac\backslash Big(\; \backslash frac-1\backslash Big)\; -\backslash frac\backslash Big(\backslash frac-1\backslash Big)$ \right ) . These are quantum-statistical expressions containing kinetic energies. Note that the one-particle partition function $Q\_1$ contains only a kinetic energy term. In the classical limit $\backslash hbar\; =\; 0$ the kinetic energy operators commute with the potential operators and the kinetic energies in numerator and denominator cancel mutually. The trace (tr) becomes an integral over the configuration space. It follows that classical virial coefficients depend on the interactions between the particles only and are given as integrals over the particle coordinates. The derivation of higher than $B\_3$ virial coefficients becomes quickly a complex combinatorial problem. Making the classical approximation and neglecting non-additive interactions (if present), the combinatorics can be handled graphically as first shown by Joseph E. Mayer and Maria Goeppert-Mayer. They introduced what is now known as the Mayer function: :$f(1,2)\; =\; \backslash exp\backslash left(\backslash frac\_2|)\}\backslash right)\; -\; 1$ and wrote the cluster expansion in terms of these functions. Here $u(|\backslash vec\_1-\; \backslash vec\_2|)$ is the interaction potential between particle 1 and 2 (which are assumed to be identical particles). 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Virial coefficient」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.