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Updated: May 10, 2025

Methods of Ex Situ and In Situ Investigations of Structural Transformations: The Case of Crystallization of Metallic Glasses
Published on: June 7, 2018
Nanosecond structural evolution in shocked coesite
Xiaokang Feng1,2, Shuning Pan3, Kento Katagiri4,5
1Center for High-Pressure Science and Technology Advanced Research, Beijing 100094, China.
Shocked coesite transforms into novel high-pressure silica phases and back again. These complex phase transitions offer new insights into mineral behavior during meteorite impacts on early Earth, Moon, and Mars.
Area of Science:
- Mineral physics
- Geochemistry
- Materials science
Background:
- Shock-induced phase transitions in minerals are key to understanding impact events.
- Previous studies on shocked silica at 65 GPa suggested complex high-pressure phases.
- Silica's behavior under extreme pressure, especially during superheating before melting, requires further investigation.
Purpose of the Study:
- To investigate the time-dependent response of coesite under laser-driven shock.
- To explore the complex phase evolution pathways of silica under high pressure.
- To provide insights into silica phases found in extraterrestrial impact events.
Main Methods:
- Laser-driven shock experiments.
- Time-resolved X-ray diffraction (XRD) for in-situ analysis.
- Molecular dynamics simulations utilizing a novel machine learning interatomic potential.
Main Results:
- Observed a transient dense supercooled liquid silica.
- Identified crystallization into a semi-disordered d-NiAs-type silica.
- Documented transformations to seifertite or stishovite, pressure-dependent.
- Revealed a back-transformation to coesite upon pressure release, not quartz.
Conclusions:
- Shocked coesite exhibits intricate phase evolution pathways.
- The observed phases and transformations enhance understanding of silica behavior under extreme shock conditions.
- Findings contribute to interpreting high-pressure silica phases in meteorite impact records on terrestrial planets.
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