Nanosecond structural evolution in shocked coesite

The phase transitions in minerals under shock are crucial for understanding meteorite impact history. Recent time-resolved x-ray diffraction (XRD) studies on silica shocked to 65 GPa proposed the formation of different high-pressure phases between fused silica and quartz. Furthermore, the dynamics of silica behavior under higher pressure need to be investigated, particularly during nonequilibrium superheating before melting. This study examines the time-dependent response of coesite, using laser-driven shock coupled with fast XRD and molecular dynamics simulations with our recently developed machine learning interatomic potential. Our results reveal a transient dense supercooled liquid crystallizes into a semi-disordered d-NiAs-type silica, followed by transforming into either seifertite or stishovite, depending on the pressure. Instead of thermodynamically stable quartz, a back-transformation to coesite phase is identified after release. The complicated phase evolution pathways in shocked coesite provide deeper insights into the high-pressure silica phases observed in the meteorite bombardments on the early Moon, Mars, and Earth.

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Publication Details

Journal
Science Advances
Published
2025-04-25
DOI
https://doi.org/10.1126/sciadv.ads3139
Citations
4
Primary Topic
High-pressure geophysics and materials
Type
article
Field-Weighted Citation Impact
7.47
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article

Nanosecond structural evolution in shocked coesite

Pinwen Zhu, Takuo Okuchi, Xiaokang Feng, Liang Sun et al.
4 citations
Science Advances
High-pressure geophysics and materials
7.47
article

Nanosecond structural evolution in shocked coesite

Pinwen Zhu, Takuo Okuchi, Xiaokang Feng, Liang Sun, Keiichi Sueda, Cong Liu, T. Yabuuchi, Takayoshi Sano, Jia Qu, Norimasa Ozaki, Yoichiro Hironaka, Yuichi Inubushi, Keita Nonaka, Wenge Yang, Hirotaka Nakamura, Toshimori Sekine, Kento Katagiri, Y. Umeda, Yusuke Seto, Tadashi Togashi, Makina Yabashi, Kohei Miyanishi, Shuning Pan, Jian Sun, Jiuyang Shi
article en
4 citations

Abstract

The phase transitions in minerals under shock are crucial for understanding meteorite impact history. Recent time-resolved x-ray diffraction (XRD) studies on silica shocked to 65 GPa proposed the formation of different high-pressure phases between fused silica and quartz. Furthermore, the dynamics of silica behavior under higher pressure need to be investigated, particularly during nonequilibrium superheating before melting. This study examines the time-dependent response of coesite, using laser-driven shock coupled with fast XRD and molecular dynamics simulations with our recently developed machine learning interatomic potential. Our results reveal a transient dense supercooled liquid crystallizes into a semi-disordered d-NiAs-type silica, followed by transforming into either seifertite or stishovite, depending on the pressure. Instead of thermodynamically stable quartz, a back-transformation to coesite phase is identified after release. The complicated phase evolution pathways in shocked coesite provide deeper insights into the high-pressure silica phases observed in the meteorite bombardments on the early Moon, Mars, and Earth.

Science AdvancesVol. 11(17)
Jilin University (CN), Carnegie Institution for Science (US), Kyoto University (JP), Chinese Academy of Engineering (CN), SPring-8 (JP), Japan Synchrotron Radiation Research Institute (JP), Shanghai Advanced Research Institute (CN), Collaborative Innovation Center of Advanced Microstructures (CN), Center for High Pressure Science and Technology Advanced Research (CN), State Key Laboratory of High Pressure and Superhard Materials (CN), Kobe University (JP), Nanjing University (CN), The University of Osaka (JP)
Openalex Percentile: Top 3%
High-pressure geophysics and materials
7.47
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