The propagation of light in a scattering medium is described as the motion of a special kind of a Brownian particle on which the fluctuating forces act only perpendicular to its velocity. This enforces strictly and dynamically the constraint of constant speed of the photon in the medium. A Fokker-Planck equation is derived for the probability distribution in the phase space assuming the transverse fluctuating force to be a white noise. Analytic expressions for the moments of the displacement $<x^{n}>$ along with an approximate expression for the marginal probability distribution function $P(x,t)$ are obtained. Exact numerical solutions for the phase space probability distribution for various geometries are presented. The results show that the velocity distribution randomizes in a time of about eight times the mean free time ($8t^*$) only after which the diffusion approximation becomes valid. This factor of eight is a well known experimental fact. A persistence exponent of $0.435 \pm 0.005$ is calculated for this process in two dimensions by studying the survival probability of the particle in a semi-infinite medium. The case of a stochastic amplifying medium is also discussed.
翻译:在散射介质中,光在散射介质中的传播被描述为一种特殊的布朗粒子的动作, 其波动力只对它的速度产生直角。 这严格和动态地强制施加介质中光子的恒定速度的制约。 Fokker- Planck 方程式的产物是相位空间的概率分布, 假设反向波动力是白色噪音。 迁移时间的分析性表达式$<x ⁇ n ⁇ $, 以及边际概率分布函数的近似表达式 $P(x, t) 。 提供了各种地貌的相位空间概率分布的精确数字解决方案。 结果显示, 速度分布在平均自由时间大约八倍( 8美元 美元 ) 之后, 扩散近似有效 。 8 系数是一个众所周知的实验事实 。 通过在半精度介质介质中研究粒子的生存概率, 计算出这一过程的两个维度为 0. 435\ pm 0.005$。