Abstract
The evolution of precipitates in maraging steel of grade 350 was studied using the complementary techniques of small angle X-ray scattering (SAXS) and transmission electron microscopy (TEM). These investigations revealed that ageing the steel at 703 K involved a rhombohedral distortion of the supersaturated b.c.c. martensite accompanied by the appearance of diffuse ω-like structures. This was followed by the appearance of well-defined ω particles containing chemical order. At the ageing temperature of 783 K, Ni 3(Ti, Mo) precipitates were the first to appear with a growth exponent of 1/3. The values of the Porod exponent obtained from the SAXS profiles indicated that the ω particles, formed below 723 K, had diffuse interfaces up to an ageing time of 48 h. On the other hand, Ni 3(Ti, Mo) precipitates, formed above 723 K, developed sharp interfaces in just about an hour. Also, the steel exhibited scaling in phase separation both at 703 and 783 K, but only during the early stages. Through this study it was established that, at temperatures of ageing less than 723 K, evolution of ω particles takes place through the collapse of the unstable b.c.c. lattice and, at temperatures above 723 K, precipitation of A 3B type of phases through the mechanism of clustering and ordering of atomic species. Sharp interfaces develop rather quickly when the mechanism of precipitation involves development and amplification of a concentration wave alone as in the nucleation of Ni 3(Ti, Mo) at 783 K than when an interplay of both the displacement and concentration waves is required as in the evolution of ω at 703 K. These results indicate towards the possibility of existence of two separate time–temperature–transformation (TTT) curves, one for the evolution of ω-phase and another for nucleation and growth of Ni 3(Ti, Mo).
Published Version
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