Search

Laser-light sails are a spacecraft concept wherein lightweight "sails" are propelled to high speeds by lasers with high intensities. The sails must comprise materials with low optical loss, to minimize the risk of laser damage. Stoichiometric silicon nitride (Si$_3$N$_4$) is a candidate material with low loss in the near infrared, but the precise absorption coefficient has not been characterized in the membrane form-factor needed for sails. We use photothermal common-path interferometry (PCI), a sensitive pump-probe technique, to measure the absorption coefficient of stoichiometric and nonstoichiometric silicon nitride. To calibrate PCI measurements of membranes, we developed a self-referencing technique where a measurement is performed twice: once on a bare membrane, and a second time with a monolayer of graphene deposited on the membrane. The absorption of the sample with graphene can be measured by both PCI and more-conventional spectroscopic techniques, enabling the calibration of the PCI measurement. We find that with an absorption coefficient of (2.09 $\pm$ 0.76) $\times$ 10$^{-2}$ cm$^{-1}$ at 1064 nm, Si$_3$N$_4$ is a suitable laser-sail material for laser intensities as high as ~10 GW/m$^{2}$, which have been proposed for some laser-sail missions, while silicon-rich SiN$_x$ (x~1), with an absorption coefficient of 7.94 $\pm$ 0.50 cm$^{-1}$, is unlikely to survive such high laser intensities., Comment: Main text + supplementary

We report the results of Brillouin-Mandelstam spectroscopy and Mueller matrix spectroscopic ellipsometry of the nanoscale "pillar with the hat" periodic silicon structures, revealing intriguing phononic and photonic properties. It has been theoretically shown that periodic structures with properly tuned dimensions can act simultaneously as phononic and photonic - phoxonic - crystals, strongly affecting the light-matter interactions. Acoustic phonon states can be tuned by external boundaries, either as a result of phonon confinement effects in individual nanostructures, or as a result of artificially induced external periodicity, as in the phononic crystals. The shape of the nanoscale pillar array was engineered to ensure the interplay of both effects. The Brillouin-Mandelstam spectroscopy data indicated strong flattening of the acoustic phonon dispersion in the frequency range from 2 GHz to 20 GHz and the phonon wave vector extending to the higher-order Brillouin zones. The specifics of the phonon dispersion dependence on the pillar arrays orientation suggest the presence of both periodic modulation and spatial localization effects for the acoustic phonons. The ellipsometry data reveal a distinct scatter pattern of four-fold symmetry due to nanoscale periodicity of the pillar arrays. Our results confirm the dual functionality of the nanostructured shape-engineered structure and indicate a possible new direction for fine-tuning the light-matter interaction in the next generation of photonic, optoelectronic, and phononic devices., Comment: 25 pages, 7 figures

There is strong interest in being able to accurately and sensitively monitor materials degradation in both ground-based and space-based environments. Two optical techniques for sensitive degradation monitoring are reviewed: spectroscopic ellipsometry and photothermal spectroscopy. These techniques complement each other in that ellipsometry is sensitive to atomically thin surface and subsurface changes, and photothermal spectroscopy is sensitive to local defects, pin-holes, subsurface defects, and delamination. Progress in applying these spectroscopies (both ex situ and in situ) to atomic oxygen degradation of space materials is reviewed.