It was proposed that the zone formation due to a miscibility gap is a hardening mechanism in the age-hardening of Fe–Ni–Mn martensitic alloys, and the propriety of this mechanism was confirmed by thermodynamic considerations. The results obtained may be summarized as follows :
(1) The nose temperature of the hardening rate on the reciprocal temperature-time diagram (C-curve), was raised as the Ni and Mn contents were increased. This result showed the existence of a solubility limit surface in the
bcc phase of the ternary Fe–Ni–Mn system.
(2) Possible combinations of the energy parameters of Fe–Ni, Fe–Mn and Ni–Mn binary systems were deduced from the extent of the miscibility gap island by application of Meijering’s treatment. This explained result (1).
(3) From the equilibrium phase diagrams of Fe–Ni, Fe–Mn and Ni–Nn systems, energy parameters for interaction between different atoms in
bcc phase were estimated. The energy parameters of Fe–Ni and Fe–Mn systems were nearly equal, and that of Ni–Mn system was shown to have larger value of negative number than either of them. This result satisfies the condition of (2).
(4) Because the energy parameter of Ni–Mn system had a large negative value, the zone rich in Ni and Mn should be ordered. It was pointed out that both shearing of the ordered zone by dislocations and the strain caused by the zone formation contributed to the hardening of the alloy.
(5) The intense hardening response observed in the 10∼12% Ni, 5∼6% Mn alloy was interpreted in terms of the relation between the solubility line and the martensitic region.
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