Energy dissipation mechanism of G-phase and L-phase metallic glass nanofilms subjected to high-velocity nano-ballistic impact
Abstract
The energy dissipation mechanisms of G-phase and L-phase metallic glass nanofilms subjected to high-velocity nano-particle impact were investigated by molecular dynamics (MD) simulations. We identified the phase transition from G-phase to L-phase in which the locally ordered core structures transform to liquid-like structures due to local mechanical melting and adiabatic heating of the G-phase under high strain rate impact. The appearance of phase transition provides a new channel for energy dissipation, thus the relatively thicker G-phase nanofilm with ordered core structures has a higher specific energy absorption compared with the L-phase film at the same thickness and impact velocity. However, if the thickness decreases below the characteristic length scale of the heterogeneous structure, the broken core structures in the G-phase films act as prefabricated defects that fail prematurely when subjected to impact, resulting in less impact resistance of the G-phase film compared to the L-phase film. This paper provides a useful method for improving the impact resistance of metallic glass films by tailoring the microstructures.
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Acknowledgement
This work was supported by the National Key R&D Program of China (2021YFA0719200), the National Natural Science Foundation of China (12272391 and 12232020), the National Outstanding Youth Science Fund Project of National Natural Science Foundation of China (12125206) and the CAS Project for Young Scientists in Basic Research (YSBR-096).
Contributions
Data Availability
Data will be made available on request.
Supplemental Material
Supplementary material (DOCX)
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Additional details
- Ministry of Science and Technology of the People's Republic of China
- 2021YFA0719200
- National Natural Science Foundation of China
- 12272391
- National Natural Science Foundation of China
- 12232020
- National Natural Science Foundation of China
- 12125206
- Chinese Academy of Sciences
- YSBR-096
- Accepted
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2024-12-13Accepted
- Available
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2024-12-15Available online
- Available
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2024-12-18Version of record
- Publication Status
- Published