# Applying the Fokker--Planck equation to grating-based x-ray phase and dark-field imaging

## TL;DR

This paper applies the Fokker--Planck equation to model the drift and diffusion of structured illumination in grating-based x-ray phase and dark-field imaging, aiming to understand signal interactions and improve image reconstruction.

## Contribution

It introduces a novel application of the Fokker--Planck equation to describe phase and dark-field signals in x-ray imaging, providing insights into signal cross-talk.

## Key findings

- Fokker--Planck equation models drift and diffusion in structured illumination.
- Enhanced understanding of cross-talk between attenuation, phase, and dark-field signals.
- Potential basis for improved inverse problem solutions in x-ray imaging.

## Abstract

X-ray imaging has conventionally relied upon attenuation to provide contrast. In recent years, two complementary modalities have been added; phase contrast and dark-field x-ray imaging, capturing weakly attenuating and sub-pixel sample structures respectively. These three modalities can be accessed using a crystal analyser, a grating interferometer or by looking at a directly-resolved grid, grating or speckle pattern. Grating and grid-based methods extract a differential phase signal by measuring how far a feature in the illumination has been shifted transversely due to the presence of a sample. The dark-field signal is extracted by measuring how the visibility of the structured illumination is decreased, typically due to the presence of sub-pixel structures in a sample. The strength of the dark-field signal may depend on the grating period, the pixel size and the set-up distances, and additional dark-field signal contributions may be seen as a result of strong phase effects or other factors. In this paper we show that the finite-difference form of the Fokker--Planck Equation can be applied to describe the drift (phase signal) and diffusion (dark-field signal) of the periodic or structured illumination used in phase contrast x-ray imaging with gratings, in order to better understand any cross-talk between attenuation, phase and dark-field x-ray signals. In future work, this mathematical description could be used as a basis for new approaches to the inverse problem of recovering both phase and dark-field information.