Prediction of bulk metallic glass formation in Cu–Zr–Ag–Hf system by thermodynamic and topological modeling

Vincent, S. ; Murty, B. S. ; Bhatt, Jatin (2012) Prediction of bulk metallic glass formation in Cu–Zr–Ag–Hf system by thermodynamic and topological modeling Transactions of the Indian Institute of Metals, 65 (6). pp. 827-831. ISSN 0972-2815

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Official URL: https://link.springer.com/article/10.1007/s12666-0...

Related URL: http://dx.doi.org/10.1007/s12666-012-0209-7

Abstract

Cu based Bulk Metallic Glasses (BMGs) are widely studied because of their high Glass Forming Ability (GFA) and interesting combination of properties such as high strength coupled with good ductility and low cost. With these attributes, Cu based BMGs are being projected as promising materials for practical applications. The process of glass formation in metallic systems is a challenging task and alloys should be cooled from the liquid state at rates faster than a critical cooling rate (Rc) to resist crystallization. Interestingly, composition plays an important role in achieving easy glass formation, which is usually measured in terms of Rc. In the present work, attempt has been made to identify the composition for easy glass formation in Cu based quaternary system by theoretical approach. A GFA parameter PHS, which is a product of enthalpy of chemical mixing (ΔHchem) and mismatch entropy normalized with Boltzmann’s constant (ΔSσ/kB) is used to identify the best glass forming composition in Cu–Zr–Ag–Hf system. Further, a new parameter PHSS, which is a product of PHS and configurational entropy (ΔSconfig/R) is found to illustrate strong correlation with GFA. An attempt has also been made to correlate PHSS parameter with critical diameters and Rc using reported data in Cu–Zr–Ag–Hf system.

Item Type:Article
Source:Copyright of this article belongs to Springer-Verlag.
Keywords:Glass Forming Ability; Critical Cooling Rate; Enthalpy Of Chemical Mixing; Mismatch Entropy; Configurational Entropy
ID Code:110899
Deposited On:06 Dec 2017 11:03
Last Modified:06 Dec 2017 11:03

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