TY - JOUR
T1 - Stress-induced strain glass to martensite (R) transition in a Ti 50Ni44.5Fe5.5 alloy
AU - Zhang, Jian
AU - Wang, Yu
AU - Ding, Xiangdong
AU - Zhang, Zhen
AU - Zhou, Yumei
AU - Ren, Xiaobing
AU - Otsuka, Kazuhiro
AU - Sun, Jun
AU - Song, Minghui
PY - 2011/5/16
Y1 - 2011/5/16
N2 - Strain glass (STG) in Ni-rich binary Ti-Ni possesses an R-like (rhombohedral) local strain order, but it transforms into B19' martensite under stress. It remains a puzzle why the local strain order in STG yields a different long-range strain order. Here, we systematically investigated a ternary Ti 50Ni44.5Fe5.5 STG, which exhibited the same STG features as the binary STG, and the local strain order is also an R-like one. Different from the binary STG, under stress this ternary STG transforms into a normal R phase rather than B19'. By considering that both systems have bi-instability with respect to both R and B19' martensites in the schematic free-energy landscape, we provide a unified explanation for the different products of the stress-induced STG to martensite (STG-M) transition between a Ti-Ni binary system and the present ternary system. We show that the differences stem from the competing thermodynamic stability between R-phase and B19' martensites.
AB - Strain glass (STG) in Ni-rich binary Ti-Ni possesses an R-like (rhombohedral) local strain order, but it transforms into B19' martensite under stress. It remains a puzzle why the local strain order in STG yields a different long-range strain order. Here, we systematically investigated a ternary Ti 50Ni44.5Fe5.5 STG, which exhibited the same STG features as the binary STG, and the local strain order is also an R-like one. Different from the binary STG, under stress this ternary STG transforms into a normal R phase rather than B19'. By considering that both systems have bi-instability with respect to both R and B19' martensites in the schematic free-energy landscape, we provide a unified explanation for the different products of the stress-induced STG to martensite (STG-M) transition between a Ti-Ni binary system and the present ternary system. We show that the differences stem from the competing thermodynamic stability between R-phase and B19' martensites.
UR - https://www.scopus.com/pages/publications/79961122746
U2 - 10.1103/PhysRevB.83.174204
DO - 10.1103/PhysRevB.83.174204
M3 - 文章
AN - SCOPUS:79961122746
SN - 1098-0121
VL - 83
JO - Physical Review B - Condensed Matter and Materials Physics
JF - Physical Review B - Condensed Matter and Materials Physics
IS - 17
M1 - 174204
ER -