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Molecular Dynamics Study of Dynamic Responses of Glassy Silica under Shock Impact

Luming Shen1

School of Civil Engineering, University of Sydney, NSW 2006 Australia; Email: Luming.Shen@sydney.edu.au

Computers, Materials & Continua 2010, 15(3), 241-260. https://doi.org/10.3970/cmc.2010.015.241

Abstract

In this study, molecular dynamics (MD) simulations are performed to form glassy silica from meltedb-cristobalite using cooling rates of 2, 20 and 200 K/ps. The resulting glassy silica samples are then shocked at particle velocities ranging from 0.3 to 11 km/s in the MD simulations. The effect of the cooling rate on the shock wave velocity is observed for particle velocities below 2 km/s. Moreover, the simulated pressure and density of the shocked glassy silica increase as the cooling rate increases. As compared with the experimental data, the MD simulation can approximately identify the initiation of densification and predict the shock wave velocity within the reasonable accuracy. The simulated pressure and density of the shocked silica match the experimental and EOS analysis data well when the shock pressure is below 500 GPa. However, the proposed MD simulations under-estimate the density when the glass is shocked at pressures above 500 GPa, which indicates that a better interatomic potential model is required for modeling silica under ultrahigh pressures.

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Cite This Article

APA Style
Shen, L. (2010). Molecular dynamics study of dynamic responses of glassy silica under shock impact. Computers, Materials & Continua, 15(3), 241-260. https://doi.org/10.3970/cmc.2010.015.241
Vancouver Style
Shen L. Molecular dynamics study of dynamic responses of glassy silica under shock impact. Comput Mater Contin. 2010;15(3):241-260 https://doi.org/10.3970/cmc.2010.015.241
IEEE Style
L. Shen, “Molecular Dynamics Study of Dynamic Responses of Glassy Silica under Shock Impact,” Comput. Mater. Contin., vol. 15, no. 3, pp. 241-260, 2010. https://doi.org/10.3970/cmc.2010.015.241



cc Copyright © 2010 The Author(s). Published by Tech Science Press.
This work is licensed under a Creative Commons Attribution 4.0 International License , which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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