Paper 13093-202
Characterizing nanoscale thin-film residual stresses for stress mitigation and engineering in next generation X-ray optics
17 June 2024 • 17:30 - 19:00 Japan Standard Time | Room G414/415, North - 4F
Abstract
Reflection gratings are critical components to successful X-ray spectroscopes and represent important priorities for future NASA observatories. As such, significant research efforts have been invested to improve mirror and grating fabrication, resulting in increased collecting area and improved mirror performance. However, residual stresses induced by reflective coatings continue to present challenges, causing mirror deformation, degradation of spectral resolution, and decreased scientific performance. Though macro stresses on thicker layers are more easily calculated, localized stress distributions and the stress response of nanoscale layers (5-30nm) are not well understood and can be difficult to measure. This study demonstrates synchrotron XRD methods using the sin^2ψ technique to better characterize and minimize the stress of single and bi-layered nanoscale reflective layers (5-30 nm) for applications in X-ray optics. Residual stresses are spatially mapped across an optic and analyzed at different deposition conditions and anneal treatments. High-Z materials (Ir, Pt, Au) have been chosen for this study due to their favorable reflectivity over the soft X-ray regime.
Presenter
Taylor Wood
The Pennsylvania State Univ. (United States)
Taylor Wood is a NASA Space Technology Graduate Research Fellow studying Materials Science and Engineering at the Pennsylvania State University. His area of focus lies in X-ray diffractive and curvature methods to characterize thin film residual stresses for use as reflective coatings for astronomical X-ray gratings.