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瑞利-德拜-甘斯理论在分形聚集体光学中的有效性范围。

Range of validity of the Rayleigh-Debye-Gans theory for optics of fractal aggregates.

作者信息

Farias T L, Köylü U Ö, Carvalho M G

出版信息

Appl Opt. 1996 Nov 20;35(33):6560-7. doi: 10.1364/AO.35.006560.

DOI:10.1364/AO.35.006560
PMID:21127680
Abstract

The range of validity of the Rayleigh-Debye-Gans approximation for the optical cross sections of fractal aggregates (RDG-FA) that are formed by uniform small particles was evaluated in comparison with the integral equation formulation for scattering (IEFS), which accounts for the effects of multiple scattering and self-interaction. Numerical simulations were performed to create aggregates that exhibit mass fractallike characteristics with a wide range of particle and aggregate sizes and morphologies, including x(p) = 0.01-1.0, ‖m - 1‖ = 0.1-2.0, N = 16-256, and D(f) = 1.0-3.0. The percent differences between both scattering theories were presented as error contour charts in the ‖m - 1‖x(p) domains for various size aggregates, emphasizing fractal properties representative of diffusion-limited cluster-cluster aggregation. These charts conveniently identified the regions in which the differences were less than 10%, between 10% and 30%, and more than 30% for easy to use general guidelines for suitability of the RDG-FA theory in any scattering applications of interest, such as laser-based particulate diagnostics. Various types of aggregate geometry ranging from straight chains (D(f) ≈ 1.0) to compact clusters (D(f) ≈ 3.0) were also considered for generalization of the findings. For the present computational conditions, the RDG-FA theory yielded accurate predictions to within 10% for ‖m - 1‖ to approximately 1 or more as long as the primary particles in aggregates were within the Rayleigh scattering limit (x(p) ≤ 0.3). Additionally, the effect of fractal dimension on the performance of the RDG-FA was generally found to be insignificant. The results suggested that the RDG-FA theory is a reasonable approximation for optics of a wide range of fractal aggregates, considerably extending its domain of applicability.

摘要

通过与考虑多次散射和自相互作用影响的散射积分方程公式(IEFS)相比较,评估了由均匀小颗粒形成的分形聚集体(RDG - FA)光学截面的瑞利 - 德拜 - 甘斯近似的有效性范围。进行了数值模拟,以创建具有质量分形特征的聚集体,这些聚集体具有广泛的颗粒和聚集体尺寸及形态,包括x(p) = 0.01 - 1.0、‖m - 1‖ = 0.1 - 2.0、N = 16 - 256以及D(f) = 1.0 - 3.0。两种散射理论之间的百分比差异在‖m - 1‖x(p)域中以误差等高线图的形式呈现,用于各种尺寸的聚集体,强调了代表扩散限制簇 - 簇聚集的分形特性。这些图表方便地确定了差异小于10%、在10%至30%之间以及大于30%的区域,以便为RDG - FA理论在任何感兴趣的散射应用(如基于激光的颗粒诊断)中的适用性提供易于使用的一般指导原则。还考虑了从直链(D(f)≈1.0)到紧密簇(D(f)≈3.0)的各种类型的聚集体几何形状,以推广研究结果。对于当前的计算条件,只要聚集体中的初级颗粒处于瑞利散射极限内(x(p)≤0.3),RDG - FA理论对于‖m - 1‖约为1或更大时能给出准确至10%以内的预测。此外,一般发现分形维数对RDG - FA性能的影响不显著。结果表明,RDG - FA理论对于广泛的分形聚集体光学是一种合理的近似,大大扩展了其适用范围。

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