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Phase diagram of H2O: Thermodynamic functions of the phase transitions of high-pressure ices

机译:H2O的相图:高压冰的相变的热力学函数

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The analysis of the internal structure of the ice satellites of the Solar System's giant planets, Jupiter and Saturn, and the estimation of the composition of other water-containing cosmic bodies require thermodynamic information on the phase transformations in the water-ice system. This work presents experimental and theoretical data on the studies of the phase diagram of water (H^sub 2^O) and the thermodynamic properties of water ices that were generalized, analyzed, and systematized. A brief description of the equations of state for different modifications of high-pressure ices that are most frequently used in thermodynamic calculations is presented. Based on the mathematical treatment of available experimental data for phase equilibria in the water-ice system, the boundaries of the phase transitions between crystal ices I, II, III, V, VI, VII, VIII, and X and liquid water are constructed; in addition, the thermal dependences of the thermodynamic functions (changes in enthalpy, entropy, and volume) of most water-ice phase transitions are obtained.[PUBLICATION ABSTRACT]
机译:对太阳系巨型行星木星和土星的冰卫星内部结构的分析,以及对其他含水宇宙体组成的估算,都需要有关水冰系统中相变的热力学信息。这项工作提供了关于水(H ^ sub 2 ^ O)相图和水冰的热力学性质的研究和理论数据,这些研究已得到概括,分析和系统化。简要介绍了热力学计算中最常使用的高压冰的不同修改状态方程。基于对水冰系统中相平衡可用实验数据的数学处理,构造了冰I,II,III,V,VI,VII,VIII和X与液态水之间的相变边界;此外,还获得了大多数水冰相变的热力学函数(焓,熵和体积的变化)的热依赖性。[出版物摘要]

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