Composition dependence of Young's modulus in Ti-V, Ti-Nb, and Ti-V-Sn alloys

The Young's modulus of Ti-V and Ti-V-Sn alloys quenched from the beta-phase region after solution treatment and cold rolling was investigated in relation to alloy compositions, microstructures, and constituent phases. The composition dependence of the Young's modulus for quenched Ti-V binary alloys shows two minima of 69 GPa at Ti-10 mass pet V and 72 GPa at Ti-26 mass pet V. Between the two compositions, athermal omega or stress-induced omega is introduced in retained beta phase and increases Young's modulus. That is, a low Young's modulus is attained unless alloys undergo to omega transformation. In Ti-5 and -8 mass pet V, which undergo alpha' (hcp) martensitic transformation on quenching, the Young's modulus further decreases by cold rolling, which can be reasonably explained by the formation of alpha' rolling texture. Comparing Young's modulus in Ti-V binary alloy with that in Ti-Nb binary alloy, it is found that Young's modulus is remarkably increased by athermal- or stress induced omega phase, and it shows a minimum when both martensitic and to transformation are suppressed during quenching in metastable beta alloys. The Sn addition to Ti-V binary alloy retards or suppresses athermal and stress-induced omega transformation, thereby decreasing Young's modulus. Young's modulus exhibits minimum values of 51 GPa in quenched (Ti-12 pet V)-2 pet Sn and of 57 GPa in cold-rolled (Ti-12 pet V)-6 pet Sn.