4.7 Article

Precipitation of metastable intermetallic phases and nanoindentation behaviors of a Ti-20Zr-9 Nb-4Sn (at%) alloy during aging treatment

Journal

JOURNAL OF ALLOYS AND COMPOUNDS
Volume 933, Issue -, Pages -

Publisher

ELSEVIER SCIENCE SA
DOI: 10.1016/j.jallcom.2022.167762

Keywords

Ti-Zr-Nb-Sn alloy; Aging; Microstructure evolution; Precipitation hardening; Nanoindentation

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This study investigates the microstructure evolution and nanoindentation behavior of a Ti-20Zr-9Nb-4Sn alloy aged at 600 degrees C, demonstrating the potential for precipitation strengthening effect of (Zr,Sn)-rich precipitates. The results show that the hardness of the aged specimens initially increases and then reaches a plateau as aging time prolongs. The (Zr,Sn)-rich precipitates exhibit higher hardness than the alpha precipitate and matrix, indicating their contribution to the overall hardness of the specimen.
In this study, the microstructure evolution and nanoindentation behavior of a Ti-20Zr-9 Nb-4Sn (at%) alloy aged at 600 degrees C for 1-60 h were investigated by field-emission scanning electron microscopy, energy -dis-persive X-ray spectroscopy, Vickers microhardness test and nanoindentation technique to show the po-tential for precipitation strengthening effect of (Zr,Sn)-rich precipitates. The Vickers hardness in the 600 degrees C aged specimens increased from 218 HV to the maximum of 242 HV with increasing the aging time from 1 to 13 h. With further prolonging the aging time to 60 h, the hardness decreased to 219 HV at 45 h aging and then almost keep constant at 45-60 h aging. The metastable intermetallic (Zr,Sn)-rich precipitates were formed in all aged specimens and their composition is highly dependent on the aging time as a result of elemental partitioning during aging. In the specimen aged for 24 h, the nanoindentation hardness (18.6 GPa) of the (Zr,Sn)-rich precipitates (Zr3Sn-type) was much higher than those of the alpha precipitate (9.3 GPa) and matrix (7.6 GPa), which suggests that the hard (Zr,Sn)-rich precipitate should be responsible for the high Vickers hardness in the specimen. These findings show that the precipitation hardening effect in Ti-Zr-Nb-Sn alloys is not just limited to the well-known isothermal omega and/or alpha precipitates and the (Zr,Sn)-rich precipitates also exhibit great potential for precipitation strengthening effect.(c) 2022 Elsevier B.V. All rights reserved.

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