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来自混浊平板的偏振光前向散射:理论与蒙特卡罗模拟

Forward scattering of polarized light from a turbid slab: theory and Monte Carlo simulations.

作者信息

Otsuki Soichi

出版信息

Appl Opt. 2016 Dec 20;55(36):10276-10282. doi: 10.1364/AO.55.010276.

Abstract

It is proved that if reciprocity and mirror symmetry hold for single scattering by a particle, they also hold for multiple scattering in turbid slab media. Monte Carlo simulations generate a reduced effective Mueller matrix for forward scattering, which satisfies reciprocity and mirror symmetry, but satisfies only reciprocity if the medium contains chiral components. The scattering matrix was factorized by using the Lu-Chipman polar decomposition, which affords the polarization parameters as a function of the radial distance from the center. The depolarization coefficients decrease with increasing distance, whereas the scattering-induced linear diattenuation and retardance become larger in the middle-distance range. The optical rotation for a chiral medium increases with increasing distance.

摘要

事实证明,如果粒子的单次散射满足互易性和镜面对称性,那么在浑浊平板介质中的多次散射也同样满足。蒙特卡罗模拟生成了一个用于前向散射的简化有效穆勒矩阵,该矩阵满足互易性和镜面对称性,但如果介质包含手性成分,则仅满足互易性。通过使用陆 - 奇普曼极分解对散射矩阵进行因式分解,该分解给出了作为距中心径向距离函数的偏振参数。退偏系数随距离增加而减小,而在中距离范围内,散射引起的线性双衰减和相位延迟变得更大。手性介质的旋光性随距离增加而增大。

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