The copper-rich precipitates of size 4-8 nm which are found in a PH 15-5 martensitic stainless steel aged at 480°C for 2h are found to have the same twinned 9R structure as copper-rich precipitates of similar size in thermally aged and in electron-irradiated model Fe-Cu and Fe-Cu-Ni alloys. Larger precipitates produced by ageing for the same time at 500°C appear to have transformed to a distorted fcc structure without first untwinning by a mechanism also found in the model alloys, which suggests that the precipitation sequences in the steel and the model alloys are essentially similar.
No takes yet. Share an insight, caveat, or question.
Habibibajguirani et al. (1996) studied this question.
Synapse has enriched 5 related papers. Consider them for comparative context: