Abstract
Despite its fundamental importance in condensed matter physics and geophysical implications, establishing the systematic and direct link between the pressure-induced structural changes in crystalline and noncrystalline low- oxides and their corresponding evolution in O -edge core-electron excitation features under extreme compression has been challenging. Here we calculated the site-resolved partial density of states and O -edge x-ray Raman scattering (XRS) spectra for two of the important oxide phases in the Earth's lower mantle, bridgmanite and post-bridgmanite, up to 120 GPa using ab initio calculations, revealing the electronic origins of the O -edge features for oxides under compression. The absorption threshold and band gap increase linearly with a decrease in the O-O distance in diverse and high-pressure phases , providing a predictive relationship between the and the O-O distances in the oxide at high pressure. Despite densification, upon isobaric phase transition from bridgmanite to post-bridgmanite at 120 GPa, a decrease in band gap results in a decrease in edge energy because of an increase in O-O distance. The oxygen proximity is a useful structural proxy of oxide densification upon compression, as it explains the pressure-induced changes in O -edge XRS features of crystalline and amorphous and at high pressures. These results can be applied to studies of the pressure-bonding transitions in a wide range of oxides under extreme compression.
2 More- Received 11 July 2016
- Revised 1 September 2016
DOI:https://doi.org/10.1103/PhysRevB.94.094110
©2016 American Physical Society