percusyevick结构因素使之简单

R. Botet, Sylvie Kwok, B. Cabane
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引用次数: 5

摘要

通过小角度x射线散射测量粒子色散的结构因子S(q),为研究胶体粒子的空间排列提供了一种独特的方法。然而,由于SAXS信号固有地缺少一些信息,因此不可能从S(q)中找到粒子的确切位置。分析实验结构因子的两种标准方法是将其与从模拟系统计算的结构因子或从近似系统计算的分析结构因子进行比较。对于单分散的硬球液体,后一种方法通过Ornstein-Zernike方程和percusi - yevick闭包方程提供解析结构因子。用这种方法得到的结构因子对于多分散粒子的更常见的分散体来说是不够的。然而,Vrij、Bloom和Stell能够证明,同样的数学框架可以扩展,以产生实验结构因子的精确近似值。尽管如此,由于其数学复杂性,该解决方案仍未得到充分利用。在目前的工作中,我们推导并报告了一般多分散硬球体系的完整percus_yevick解,其形式简洁,易于使用。解的形式很简单,可以给出几种重要的粒子半径分布(舒尔茨分布、截断正态分布和逆高斯分布)的现成解。我们还详细讨论了幂律半径分布的情况,这与最近在高内相比乳剂中实验发现的由球体的阿波罗填料构成的系统有关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Percus–Yevick structure factors made simple
Measuring the structure factor, S(q), of a dispersion of particles by Small-Angle X-ray Scattering provides a unique method to investigate the spatial arrangement of colloidal particles. However, it is impossible to find the exact location of the particles from S(q) because some information is inherently lacking in the SAXS signal. The two standard ways to analyse an experimental structure factor are then to compare it either to structure factors computed from simulated systems, or to analytical structure factors calculated from approximated systems. For liquids of monodisperse hard spheres, the latter method provides analytical structure factors through the Ornstein-Zernike equation used with the Percus-Yevick closure equation. The structure factors obtained in this way were not adequate for the more common dispersions of polydisperse particles. However, Vrij, Bloom and Stell were able to demonstrate that the same mathematical framework could be extended to yield accurate approximations for the experimental structure factor. Still, this solution has remained underused because of its mathematical complexity. In the present work, we derive and report the complete Percus-Yevick solution for general polydisperse hard-spheres systems in a concise form that is straightforward to use. The form of the solution is made simple enough to give ready solutions of several important particle-radius distributions (Schulz, truncated normal and inverse Gaussian). We also discuss in detail the case of the power-law radius distribution, relevant in the case of systems made of an Apollonian packing of spheres, as recently discovered experimentally in high internal-phase-ratio emulsions.
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