Amendola Caterina, Maffeis Giulia, Farina Andrea, Spinelli Lorenzo, Torricelli Alessandro, Pifferi Antonio, Sassaroli Angelo, Fanelli Duccio, Tommasi Federico, Martelli Fabrizio
Opt Express. 2024 Jan 1;32(1):125-150. doi: 10.1364/OE.507646.
Monte Carlo (MC) is a powerful tool to study photon migration in scattering media, yet quite time-consuming to solve inverse problems. To speed up MC-simulations, scaling relations can be applied to an existing initial MC-simulation to generate a new data-set with different optical properties. We named this approach trajectory-based since it uses the knowledge of the detected photon trajectories of the initial MC-simulation, in opposition to the slower photon-based approach, where a novel MC-simulation is rerun with new optical properties. We investigated the convergence and applicability limits of the scaling relations, both related to the likelihood that the sample of trajectories considered is representative also for the new optical properties. For absorption, the scaling relation contains smoothly converging Lambert-Beer factors, whereas for scattering it is the product of two quickly diverging factors, whose ratio, for NIRS cases, can easily reach ten orders of magnitude. We investigated such instability by studying the probability-distribution for the number of scattering events in trajectories of given length. We propose a convergence test of the scattering scaling relation based on the minimum-maximum number of scattering events in recorded trajectories. We also studied the dependence of MC-simulations on optical properties, most critical in inverse problems, finding that scattering derivatives are ascribed to small deviations in the distribution of scattering events from a Poisson distribution. This paper, which can also serve as a tutorial, helps to understand the physics of the scaling relations with the causes of their limitations and devise new strategies to deal with them.
蒙特卡罗(MC)是研究光子在散射介质中迁移的强大工具,但求解逆问题时相当耗时。为了加速MC模拟,可以将缩放关系应用于现有的初始MC模拟,以生成具有不同光学特性的新数据集。我们将这种方法命名为基于轨迹的方法,因为它利用了初始MC模拟中检测到的光子轨迹的知识,这与基于光子的较慢方法相反,在基于光子的方法中,需要使用新的光学特性重新运行新的MC模拟。我们研究了缩放关系的收敛性和适用范围限制,这两者都与所考虑的轨迹样本对于新光学特性也具有代表性的可能性有关。对于吸收,缩放关系包含平滑收敛的朗伯 - 比尔因子,而对于散射,它是两个快速发散因子的乘积,在近红外光谱(NIRS)情况下,其比值很容易达到十个数量级。我们通过研究给定长度轨迹中散射事件数量的概率分布来研究这种不稳定性。我们基于记录轨迹中散射事件的最小 - 最大数量提出了散射缩放关系的收敛性测试。我们还研究了MC模拟对光学特性的依赖性,这在逆问题中最为关键,发现散射导数归因于散射事件分布与泊松分布的小偏差。本文也可作为教程,有助于理解缩放关系的物理原理及其局限性的原因,并设计应对这些局限性的新策略。