The occurrence of martensitic stabilization shows a strong positive dependence on Ms temperature in Cu-Zn-Al alloys. Compared with Cu-Zn-Al alloys, Cu-Al-Ni alloys have a more excellent resistance to martensitic stabilization. However, whether the occurrence of martensitic stabilization is dependent on Ms temperature in Cu-Al-Ni alloys is still unknown. To clarify this question, we investigated the relationship between SME and Ms temperature in directly-quenched Cu-Al-Ni alloys. Results showed that the positive dependence of martensitic stabilization on Ms temperature indeed existed in directly-quenched Cu-Al-Ni alloys. The Cu-Al-Ni alloys with Ms≤488 K possess a good resistance to martensitic stabilization. For the directly-quenched Cu-Al-Ni alloys with remarkably higher than 488 K, they cannot obtain SME due to the occurrence of martensitic stabilization after recovery heating at <25 K/s. The original number of vacancies at martensite boundaries (Nvmb) rising with the increment in Ms temperature was responsible for the remarkable lowering in resistance to martensitic stabilization during the process of slow heating. To adjust the original Nvmb in alloys with remarkably high Ms temperature, we changed the Ms temperature through precipitating α phase. The precipitation of α phase can enrich the matrix with Al and Ni elements and thus decrease the Ms temperature. The reduction in Ms temperature to below ∼500 K significantly decreased the original Nvmb and improved the resistance to martensitic stabilization during the slow heating process.
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