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Effect of cooling rate on structures and mechanical behavior of Cu50Zr50 metallic glass: A molecular-dynamics study.
- Source :
-
Physica B . Oct2018, Vol. 547, p48-54. 7p. - Publication Year :
- 2018
-
Abstract
- Abstract In this paper, the molecular dynamics simulations are utilized to study the cooling rate effect and to understand the relationship among the local atomic structure, free volume, and mechanical property in Cu 50 Zr 50 metallic glass. The radial distribution function, bond pair analysis technique, and Voronoi tessellation are performed to characterize the structure evolution and local atomic configurations during the cooling process. The results demonstrate that a faster cooling rate results in a higher glass transition temperature and less amount of icosahedra-like clusters. It has been recognized that the concentration of free volumes presents a strong evidence of upward trends as the cooling rate increases. The analyses for the free volume and Voronoi polyhedron indicate that icosahedral-like clusters show a lower free volumes as compared with the rest clusters, revealing that well-developed icosahedra-like clusters in Cu 50 Zr 50 make the system densely packed and lower free volume structure. In addition, the simulated alloy obtained at a lower cooling rate exhibits a higher yield strength and elastic modulus, all of which may attribute to the structure with more densely icosahedral-like clusters and less free volumes. Highlights • Quantitatively calculate the free volume on the atomic level in Cu 50 Zr 50 metallic glasses. • The free volumes of icosahedral-like, crystal-like, mixed and other type clusters are described quantitatively. • Icosahedral-like cluster is responsible for the densely packed structure and high yield strength. [ABSTRACT FROM AUTHOR]
Details
- Language :
- English
- ISSN :
- 09214526
- Volume :
- 547
- Database :
- Academic Search Index
- Journal :
- Physica B
- Publication Type :
- Academic Journal
- Accession number :
- 131611481
- Full Text :
- https://doi.org/10.1016/j.physb.2018.07.030