TY - JOUR
T1 - Composition Dependences of Entropy Change and Transformation Temperatures in Ni-rich Ti–Ni System
AU - Niitsu, K.
AU - Kimura, Y.
AU - Xu, X.
AU - Kainuma, R.
N1 - Funding Information:
The authors are grateful to Dr. T. Omori for his useful comments. This study was supported by a Grant-in-Aid for Scientific Research from JSPS and a Grant for Excellent Graduate Schools from MEXT, Japan. K.N. acknowledges the support from a Grant-in-Aid for Scientific Research for JSPS Fellows.
Funding Information:
The authors are grateful to Dr. T. Omori for his useful comments. This study was supported by a Grant-in-Aid for Scientific Research from JSPS and a Grant for Excellent Graduate Schools from MEXT, Japan. K.N. acknowledges the support from a Grant-in-Aid for Scientific Research for JSPS Fellows.
Publisher Copyright:
© 2015, ASM International.
PY - 2015/6/1
Y1 - 2015/6/1
N2 - For Ni-rich Ti–Ni alloys, physical properties such as specific heat and electric resistance were systematically investigated. The B2/B19′ martensitic transformation temperatures ranging from 180 to 373 K were determined for Ni contents of 49.98–51.09 %, and a sudden disappearance of martensitic transformation was confirmed for Ni contents greater than 51.23 %, which has also been well reported in the literatures. The entropy change was also evaluated from differential scanning calorimeter measurement, and it was clarified that the entropy change plotted to T0 temperature shows an S-shaped curve, starting to drastically decrease at about 300 K. Thermodynamic approaches were then carried out attempting to determine the reason for the disappearance of transformation. The entropy change estimated from direct measurements of specific heats for 51.75 Ni (B2) and 50.92 Ni (B19′) was found to be more consistent with the experimental data, rather than the calculated curve based on the Debye model for vibration specific heat. It was proposed that the equilibrium between the parent and martensite phases obeys the Clausius–Clapeyron relationship in the composition–temperature system. Using the constructed composition–temperature diagram, the disappearance of martensitic transformation in the Ti–Ni system can be well understood as being due to the drastic increase of hysteresis at low temperature.
AB - For Ni-rich Ti–Ni alloys, physical properties such as specific heat and electric resistance were systematically investigated. The B2/B19′ martensitic transformation temperatures ranging from 180 to 373 K were determined for Ni contents of 49.98–51.09 %, and a sudden disappearance of martensitic transformation was confirmed for Ni contents greater than 51.23 %, which has also been well reported in the literatures. The entropy change was also evaluated from differential scanning calorimeter measurement, and it was clarified that the entropy change plotted to T0 temperature shows an S-shaped curve, starting to drastically decrease at about 300 K. Thermodynamic approaches were then carried out attempting to determine the reason for the disappearance of transformation. The entropy change estimated from direct measurements of specific heats for 51.75 Ni (B2) and 50.92 Ni (B19′) was found to be more consistent with the experimental data, rather than the calculated curve based on the Debye model for vibration specific heat. It was proposed that the equilibrium between the parent and martensite phases obeys the Clausius–Clapeyron relationship in the composition–temperature system. Using the constructed composition–temperature diagram, the disappearance of martensitic transformation in the Ti–Ni system can be well understood as being due to the drastic increase of hysteresis at low temperature.
KW - Entropy of transformation
KW - Equilibrium temperature
KW - Martensite
KW - NiTi < materials
KW - Phase diagram
KW - Shape memory
KW - Transformation Temperature
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U2 - 10.1007/s40830-015-0023-2
DO - 10.1007/s40830-015-0023-2
M3 - Article
AN - SCOPUS:84978246724
SN - 2199-384X
VL - 1
SP - 124
EP - 131
JO - Shape Memory and Superelasticity
JF - Shape Memory and Superelasticity
IS - 2
ER -