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Peer-reviewedCC BY-NC-NDThe journal of physical chemistry letters

Electronic Structures of CaSiO3 Glass under Megabar Pressures: Ca L2,3-Edge and O K-Edge X-ray Raman Scattering.

4 affiliations
  1. 1Laboratory of Physics and Chemistry of Earth and Planetary Materials, School of Earth and Environmental Sciences, Seoul National University, Seoul08826, Korea.
  2. 2Research Institute of Basic Sciences, Seoul National University, Seoul08826, Korea.
  3. 3HPCAT, X-ray Science Division, Argonne National Laboratory, Lemont, Illinois60439, United States.
  4. 4Institute of Applied Physics, Seoul National University, Seoul08826, Korea.

Abstract

The extreme densification of silicate glasses above 100 GPa reorganizes chemical bonding around both the oxygen network and the network-modifying cations. These responses, however, have largely been probed separately, leaving their coupling during extreme densification unresolved. Here, we report the first O K-edge and Ca L2,3-edge X-ray Raman scattering measurements of CaSiO3 glass up to 120 GPa, providing element-specific access to the electronic structures under extreme compression. Enhanced oxygen proximity near 100 GPa raises the oxygen electronic states, whereas gradual Ca-O compaction shifts the calcium electronic states to lower energy through increased ligand-field interaction. Pressure-driven structural diversity and network distortion enhance electronic dispersion, broadening the oxygen and calcium density of states at megabar pressures. Comparison with O K-edge results for SiO2 and MgSiO3 glasses reveals that the larger ionic radius of Ca2+ suppresses the pressure-induced shift in electronic states near 100 GPa, highlighting how cation size controls electronic structures to evolve during extreme glass densification. These findings have implications for the stability of Ca-rich melts in planetary interiors and the design of mechanically strengthened glasses.

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BibTeX
@article{yi2026electronic,
  title = {{Electronic Structures of CaSiO3 Glass under Megabar Pressures: Ca L2,3-Edge and O K-Edge X-ray Raman Scattering.}},
  author = {Yoo Soo Yi and Yong-Hyun Kim and Shujia Li and Jae-Hyeon Parq and Jihun Lee and Yuming Xiao and Paul Chow and Guoyin Shen and Sung Keun Lee},
  journal = {The journal of physical chemistry letters},
  year = {2026},
  month = oct,
  doi = {10.1021/acs.jpclett.6c02748},
  url = {https://europepmc.org/article/MED/42917162},
  note = {CC BY-NC-ND},
}
RIS
TY  - JOUR
TI  - Electronic Structures of CaSiO3 Glass under Megabar Pressures: Ca L2,3-Edge and O K-Edge X-ray Raman Scattering.
AU  - Yoo Soo Yi
AU  - Yong-Hyun Kim
AU  - Shujia Li
AU  - Jae-Hyeon Parq
AU  - Jihun Lee
AU  - Yuming Xiao
AU  - Paul Chow
AU  - Guoyin Shen
AU  - Sung Keun Lee
PY  - 2026
DA  - 2026/10/01
JO  - The journal of physical chemistry letters
DO  - 10.1021/acs.jpclett.6c02748
UR  - https://europepmc.org/article/MED/42917162
AB  - The extreme densification of silicate glasses above 100 GPa reorganizes chemical bonding around both the oxygen network and the network-modifying cations. These responses, however, have largely been probed separately, leaving their coupling during extreme densification unresolved. Here, we report the first O K-edge and Ca L2,3-edge X-ray Raman scattering measurements of CaSiO3 glass up to 120 GPa, providing element-specific access to the electronic structures under extreme compression. Enhanced oxygen proximity near 100 GPa raises the oxygen electronic states, whereas gradual Ca-O compaction shifts the calcium electronic states to lower energy through increased ligand-field interaction. Pressure-driven structural diversity and network distortion enhance electronic dispersion, broadening the oxygen and calcium density of states at megabar pressures. Comparison with O K-edge results for SiO2 and MgSiO3 glasses reveals that the larger ionic radius of Ca2+ suppresses the pressure-induced shift in electronic states near 100 GPa, highlighting how cation size controls electronic structures to evolve during extreme glass densification. These findings have implications for the stability of Ca-rich melts in planetary interiors and the design of mechanically strengthened glasses.
SN  - 1948-7185
ER  -