Atomistic origins of pressure-induced changes in the O K-edge x-ray Raman scattering features of SiO2 and MgSiO3 polymorphs: Insights from ab initio calculations

Yoo Soo Yi and Sung Keun Lee
Phys. Rev. B 94, 094110 – Published 26 September 2016
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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-z oxides and their corresponding evolution in O K-edge core-electron excitation features under extreme compression has been challenging. Here we calculated the site-resolved partial density of states and O K-edge x-ray Raman scattering (XRS) spectra for two of the important oxide phases in the Earth's lower mantle, MgSiO3 bridgmanite and post-bridgmanite, up to 120 GPa using ab initio calculations, revealing the electronic origins of the O K-edge features for oxides under compression. The absorption threshold (EA) and band gap increase linearly with a decrease in the O-O distance in diverse SiO2 and MgSiO3 high-pressure phases [EA(eV)10.9dO-O(Å)+34.4], providing a predictive relationship between the EA 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 K-edge XRS features of crystalline and amorphous SiO2 and MgSiO3 at high pressures. These results can be applied to studies of the pressure-bonding transitions in a wide range of oxides under extreme compression.

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  • Received 11 July 2016
  • Revised 1 September 2016

DOI:https://doi.org/10.1103/PhysRevB.94.094110

©2016 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Yoo Soo Yi1 and Sung Keun Lee1,2,*

  • 1Laboratory of Physics and Chemistry of Earth Materials, School of Earth and Environmental Sciences, Seoul National University, Korea
  • 2Institute of Applied Physics, Seoul National University, Korea

  • *sungklee@snu.ac.kr

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Issue

Vol. 94, Iss. 9 — 1 September 2016

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