High Temperature Solar Technology, Paul Scherrer Institute, CH-5232 Villigen PSI, Switzerland.
J Phys Chem B. 2010 Mar 11;114(9):3219-35. doi: 10.1021/jp906511z.
A decomposition of the Helmholtz free energy of a phase containing a sparse ensemble of heterophase clusters is derived based on classical statistical mechanics and on the general physical characteristics of such systems. It is not assumed that the phase is an ideal gas. The building blocks of this decomposition are the Helmholtz free energies of the constituents (phase and stationary heterophase clusters) and, for every cluster species, a volume V(k)(cm), which is of the magnitude of the thermal fluctuation volume of the center of mass of the stationary cluster containing k monomers. A definition of V(k)(cm) is given in terms of the configuration integrals of the clusters. V(k)(cm) is evaluated for k >> 1, with the result that V(k)(cm) is proportional to k(-1/2) and is a function of temperature, the specific volume, and the isothermal compressibility of the phase in the cluster. A thermodynamically consistent expression for the work to form a stationary cluster, which reads as Delta g(k)/(k(B)T) = -ak + (3/2)bk(2/3) + 3ck(1/3) + d, is derived. The coefficients a, b, c, and d depend on the thermodynamic properties of the homogeneous phases, on the surface tension, and on one additional phenomenological material function of temperature and pressure. The description is general and covers a wide class of materials. It is shown that the heterogeneous system represents the thermodynamic equilibrium and not the pure phase without clusters. The resulting expression for the equilibrium particle number, which is different from the one used in classical nucleation theory, is by a standard procedure input for the calculation of the stationary Becker-Döring nucleation rate and entails a correction factor for the classical nucleation rate. Comparison with experiments is provided for nucleation onset measurements of argon and for measurements of the homogeneous nucleation rate of water. Measurements and theory can be brought to match within the limits of experimental precision in both cases.
基于经典统计力学和此类系统的一般物理特性,推导出了包含稀疏异相团簇的相的亥姆霍兹自由能的分解式。该相不必为理想气体。这种分解的构建块是组成部分(相和稳定异相团簇)的亥姆霍兹自由能,以及对于每个团簇物种,体积 V(k)(cm),其大小与包含 k 个单体的稳定团簇的质心的热涨落体积相当。V(k)(cm) 是根据团簇的构型积分来定义的。对于 k>>1 评估 V(k)(cm),结果表明 V(k)(cm) 与 k(-1/2)成正比,并且是温度、比容和团簇相中等温压缩性的函数。推导出形成稳定团簇的功的热力学一致表达式,其形式为 Delta g(k)/(k(B)T) = -ak + (3/2)bk(2/3) + 3ck(1/3) + d。系数 a、b、c 和 d 取决于均匀相的热力学性质、表面张力以及一个额外的与温度和压力有关的唯象材料函数。描述是通用的,涵盖了广泛的材料类别。结果表明,异相系统代表热力学平衡,而不是没有团簇的纯相。由此得到的平衡粒子数表达式与经典成核理论中使用的表达式不同,它是通过标准程序输入到稳定的 Becker-Döring 成核速率的计算中,并包含经典成核速率的修正因子。对于氩的成核起始测量和水的均匀成核速率测量,提供了与实验的比较。在两种情况下,在实验精度的范围内,测量和理论都可以匹配。