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Entropy Terms in Statistical Thermodynamic Analysis Formula for Non-stoichiometric Interstitial Compounds

机译:非化学计量间隙化合物的统计热力学分析公式中的熵项

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A series of statistical thermodynamic analyses were made since 1974 for different types of non-stoichiometric interstitial compounds MXx under simplifying a priori assumption of constant interaction energy E(X-X) between nearest neighbour interstitial atoms X within a homogeneity composition range of MX_(x) at arbitrary temperature T [K]. Mode of distribution of X atoms in interstitial sites in MX_(x) lattice is represented by number θ of available interstitial sites for occupation by X atoms per M atom and the value of θ is determined to fulfil the a priori assumption. Mode of atomic configuration would yield major contribution to entropy term ?S that appears in conventional thermodynamic expression of Gibbs free energy of formation, ?G, in form of T?S. In the statistical thermodynamic formulation, contribution of tightly bound electron appearing in form of RT ln f_(X) where f_(X) refers to atomic partition function of X atom in the MX_(x) lattice and R the universal gas constant. Judging from this mathematical form of the term, R ln f_(X) is considered to represent entropic contribution from tightly bound electron to X atom in MX_(x) lattice. In the published series of works on statistical thermodynamic analysis for non-stoichiometric interstitial compounds, calculated values for R ln f_(X) were reported but they were not reviewed with serious attention because R ln f_(X) was considered merely as a secondary factor compared to principal factor E(X-M) referring to interaction energy between X and M in MX_(x) lattice that represents enthalpy ?H in conventional thermodynamic term. In this review article, consideration is given exclusively to the factor R ln f_(X) evaluated in statistical thermodynamic approach to non-stoichiometric interstitial compounds.
机译:自1974年以来,在简化MX_(x)的同质组成范围内,最邻近的间隙原子X之间的恒定相互作用能E(XX)的先验假设的简化前提下,针对不同类型的非化学计量的间隙化合物MXx进行了一系列统计热力学分析任意温度T [K]。 MX_(x)晶格中间隙位置中X原子的分布方式由每个M原子X个原子占据的可用间隙位置的数目θ表示,确定θ的值以满足先验假设。原子构型的模式将对熵项?S做出主要贡献,该熵项以传统的热力学表达吉布斯形式的自由能?G出现,形式为T?S。在统计热力学公式中,紧密结合的电子以RT ln f_(X)的形式出现,其中f_(X)表示MX_(x)晶格中X原子的原子分配函数,R表示通用气体常数。从该术语的数学形式来看,R ln f_(X)被认为代表了从紧密结合的电子到MX_(x)晶格中X原子的熵贡献。在已发表的关于非化学计量间隙化合物的统计热力学分析的系列工作中,报告了R ln f_(X)的计算值,但由于R ln f_(X)仅被视为次要因素,因此并未受到重视。与主因子E(XM)相比,主因子E(XM)表示MX_(x)晶格中X和M之间的相互作用能,代表常规热力学项中的焓H。在这篇综述文章中,仅考虑了以统计热力学方法对非化学计量间隙化合物进行评估的Rlnf_(X)因子。

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