Kinetic studies on the massive hydriding of Zr-0.4Nb-XSn (X = 0.5, 0.8, 1.5
, 2.0) and Zr-0.8Sn- YNb (Y = 0.2, 0.4, 0.8, 1.0) ternary alloys are carrie
d out at 400 degrees C under atmospheric pressure by in situ weight gain me
asurements with thermo-gravimetric apparatus (TGA) and transmission electro
n microscope/energy dispersive X-ray spectrometer (TEM/EDX) analysis. It is
confirmed that the hydriding kinetics follow a linear rate law after incub
ation time. It is found that the hydriding reaction rate decreases with inc
reasing Sn content up to 1.5% and then sharply increases in the case of Zr-
0.4Nb-XSn while it steadily increases with Nb content in the case of Zr-0.8
Sn- YNb. The rate does not seem to be affected by the grain size in the XSn
alloys, but is influenced in the YNb alloys. TEM/EDX analysis shows that t
here is no strong relationship between the intermetallic precipitates and t
he kinetic rate in the Zr-XSn-YNb alloy system. It is revealed in this stud
y that the solubility limit of Sn in the Zr-0.4Nb-XSn ternary system become
s higher than that in the Zr-Sn binary system. On the other hand, the Nb so
lubility limit remains unchanged in the Zr-0.8Sn-YNb ternary system. Optimi
zed compositions in the Zr-XSn-YNb ternary alloy are suggested to be about
1.5% Sn and as low Nb as possible in order to minimize hydrogen uptake. (C)
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