Xu, Donghua and Lohwongwatana, Boonrat and Duan, Gang and Johnson, W. L. and Garland, Carol (2004) Bulk metallic glass formation in binary Cu-rich alloy series – Cu100−xZrx (x=34, 36, 38.2, 40 at.%) and mechanical properties of bulk Cu64Zr36 glass. Acta Materialia, 52 (9). pp. 2621-2624. ISSN 1359-6454 http://resolver.caltech.edu/CaltechAUTHORS:XUDam04
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The compositional dependence of a glass-forming ability (GFA) was systematically studied in a binary alloy series Cu100−xZrx (x=34, 36, 38.2, 40 at.%) by the copper mold casting method. Our results show the critical casting thickness jumps from below 0.5 mm to above 2 mm when x changes from 34 to 36 while further increase in x reduces the critical casting thickness. The best glass former Cu64Zr36 does not correspond to either the largest undercooled liquid region (ΔT=Tx1−Tg, where Tg is the glass transition temperature, and Tx1 is the onset temperature of the first crystallization event upon heating) or the highest reduced glass transition temperature (Trg=Tg/Tl, where Tl is the liquidus temperature). Properties of bulk amorphous Cu64Zr36 were measured, yielding a Tg ~ 787 K, Trg ~ 0.64, ΔT ~ 46 K, Hv (Vicker's Hardness) ~ 742 kg/mm^2, Young's Modulus ~ 92.3 GPa, compressive fracture strength ~ 2 GPa and compressive strain before failure ~ 2.2%.
|Additional Information:||Published version, Copyright © 2004 Acta Materialia Inc. Received 27 November 2003; received in revised form 5 February 2004; accepted 6 February 2004. Available online 5 March 2004. The authors would like to thank the Defense Advanced Research Projects Agency, Defense Sciences Office, for support under ARO Grant No. DAAD19-01-0525. G. Welsh is also acknowledged for his help with mechanical tests.|
|Subject Keywords:||Metallic glasses; Bulk amorphous materials; Binary; Casting; Compression test; BMG; CuZr; Cu; Zr|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Boonrat Lohwongwatana|
|Deposited On:||17 Aug 2007|
|Last Modified:||26 Dec 2012 09:31|
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