Effect of Re on the microstructure and mechanical properties of NbTiZr and TaTiZr equiatomic alloys
Overview & Synopsis
The microstructure, phase composition, and mechanical properties of NbTiZr, TaTiZr, Re$_{0.3}$NbTiZr, and Re$_{0.3}$TaTiZr are reported. The alloys were produced by vacuum arc melting and hot isostatically pressed (HIP’d) at 1400°C for 3 h under 276 MPa hydrostatic pressure of high-purity argon prior to testing. NbTiZr had a single-phase BCC crystal structure, while TaTiZr had a Ti- and Zr-rich BCC matrix phase and Ta-rich nanometer-sized BCC precipitates, at volume fractions of 0.49 and 0.51, respectively. Re$_{0.3}$NbTiZr consisted of a BCC matrix phase and Re-rich precipitates with a FCC crystal structure and the volume fraction of 0.14. The microstructure of Re$_{0.3}$TaTiZr consisted of a Zr-rich BCC matrix phase and coarse, Re and Ta rich, BCC particles, which volume fraction was 0.47. NbTiZr and TaTiZr had a room temperature (RT) yield stress of 920 MPa and 1670 MPa, respectively. While, 10 at.% Re additions increased the RT yield stress to 1220 MPa in Re$_{0.3}$NbTiZr and 1715 MPa in Re0.3TaTiZr. Re also considerably improved the RT ductility of TaTiZr, from about 2.5% to 10% of true strain. The positive strengthening effect from the Re additions was retained at high (800–1200°C) temperatures.
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Document Information
| Document Title | Effect of Re on the microstructure and mechanical properties of NbTiZr and TaTiZr equiatomic alloys |
|---|---|
| Author / Organization | Oleg N Senkov, Stéphane Gorsse, Robert Wheeler, Eric J Payton, Daniel B Miracle |
| Subject & Discipline | Multidisciplinary Academic Open Research |
| Categories | Science & Mathematics |
| Publication Year | 2021 |
| License / Rights | Open Access / Creative Commons |
| Resource Verification | Listed PDF (Verification Pending) |
| Original Host Website |
HAL Open Science
(hal.science)
|
| File Format | application/pdf (Portable Document Format) |
| Language | EN |
| Catalog ID | DOC-63517 |
| Original Source Link | Visit Source Page on hal.science » |