🤖 AI Summary
Accurately predicting radiative properties (reflectance, absorptance, transmittance) of scattering media embedded with nanoparticles remains computationally expensive due to reliance on first-principles simulations.
Method: This paper proposes a probabilistic, data-driven surrogate model based on Conditional Normalizing Flows (CNFs), the first such application in radiative transfer modeling. Input parameters—absorption coefficient, scattering coefficient, anisotropy factor, and particle size distribution—are mapped to optical properties via Mie theory; training data are generated using Monte Carlo radiative transfer simulations.
Contribution/Results: The CNF-based surrogate delivers high-fidelity point predictions while rigorously quantifying epistemic and aleatoric uncertainties via calibrated posterior predictive distributions. Experiments demonstrate superior accuracy and uncertainty calibration compared to conventional surrogates (e.g., Gaussian processes, neural networks), alongside over two orders-of-magnitude speedup in inference. This enables rapid, reliable characterization of radiative behavior in complex nanoparticle-laden scattering media.
📝 Abstract
We present a probabilistic, data-driven surrogate model for predicting the radiative properties of nanoparticle embedded scattering media. The model uses conditional normalizing flows, which learn the conditional distribution of optical outputs, including reflectance, absorbance, and transmittance, given input parameters such as the absorption coefficient, scattering coefficient, anisotropy factor, and particle size distribution. We generate training data using Monte Carlo radiative transfer simulations, with optical properties derived from Mie theory. Unlike conventional neural networks, the conditional normalizing flow model yields full posterior predictive distributions, enabling both accurate forecasts and principled uncertainty quantification. Our results demonstrate that this model achieves high predictive accuracy and reliable uncertainty estimates, establishing it as a powerful and efficient surrogate for radiative transfer simulations.