Analysis of microroughness evolution in X-ray astronomical multilayer mirrors by surface topography with the MPES program and by X-ray scattering
R. Canestrari, D. Spiga, G. Pareschi

TL;DR
This paper investigates the evolution of microroughness in X-ray multilayer mirrors using surface topography analysis and X-ray scattering, employing a kinetic model to predict optical performance for future telescopes.
Contribution
It introduces the MPES program implementing a kinetic model to analyze roughness growth and predict X-ray scattering effects in multilayer coatings.
Findings
Roughness evolution correlates with deposition techniques.
Model predictions match experimental XRS measurements.
Insights into surface roughness impact on imaging quality.
Abstract
Future hard X-ray telescopes (e.g. SIMBOL-X and Constellation-X) will make use of hard X-ray optics with multilayer coatings, with angular resolutions comparable to the achieved ones in the soft X-rays. One of the crucial points in X-ray optics, indeed, is multilayer interfacial microroughness that causes effective area reduction and X-Ray Scattering (XRS). The latter, in particular, is responsible for image quality degradation. Interfacial smoothness deterioration in multilayer deposition processes is commonly observed as a result of substrate profile replication and intrinsic random deposition noise. For this reason, roughness growth should be carefully investigated by surface topographic analysis, X-ray reflectivity and XRS measurements. It is convenient to express the roughness evolution in terms of interface Power Spectral Densities (PSD), that are directly related to XRS and, in…
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