Abstract
This work revealed the basic mechanism for the stabilization of carbon in ultra-low-carbon (ULC) steels that contain moderate S (0.004 to 0.010 wt pct), adequate Ti (0.060 to 0.080), and low Mn (≤0.20). During cooling through the austenitic region to the ferritic, the initially formed sulfide particles (TiS) undergo an in situ transformation into carbosulfides (H-Ti4C2S2) by absorbing C and Ti. The transformation from TiS to H may be considered as a hybrid of shear and diffusion, i.e., faulted Ti8S9 (9R)+10[Ti]+9[C] → 4 1/2Ti4C2S2 (H). At low temperature (≤930 °C), the stabilization process continues through epitaxial growth of carbides on H phase, i.e., [M]+x[C]+H → epitaxial MC x (on H). This mechanism differs from the traditional view of stabilization, where the carbon is removed from solution by the formation of free-standing or independently nucleated H and/or MCN precipitates. While these two forms of carbon stabilization are now well known, this article presents a method of predicting which mechanism of stabilization will be operative in a given steel based on its bulk composition. Implications bearing upon new ULC steel design, considering the role of S, will be discussed.
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Hua, M., Garcia, C.I. & DeArdo, A.J. Precipitation behavior in ultra-low-carbon steels containing titanium and niobium. Metall Mater Trans A 28, 1769–1780 (1997). https://doi.org/10.1007/s11661-997-0108-4
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DOI: https://doi.org/10.1007/s11661-997-0108-4