An effect of the solutioning conditions on the aging response (precipitation, age hardening) in a β type titanium alloy, Ti–15V–3Cr–3Sn–3Al, is examined.The aging response is strongly affected by the solutioning conditions and closely related to the concentration of quenched-in vacancies, which is a function of the quenching temperature and the density of vacancy sinks such as β grain boundaries, dislocations, etc. For example, the ω (≤250°C) and the α (300∼350°C) precipitations and the age hardening are greatly accelerated in the specimens in which a large amount of quenched-in vacancies are contained, i.e. the specimens quenched from high temperatures and/or with a small density of vacancy sinks. Furthermore, the α phase precipitates very homogeneously inside the β grains at the aging temperatures between 300 and 500°C. However, the precipitation delays and the denuded zones are sometimes observed in the area in which vacancy sinks exist, e.g. in the vicinity of the β grain boundaries or the isolatedly formed twins, or in the area in which dislocations are introduced due to the weak plastic deformation.In the specimens quenched from lower temperatures in the β region and having a smaller β grain size or a slightly higher density of dislocations, the delay of the aging response is significant and the α phase precipitation is heterogeneous. These phenomena are considered to be caused by a stronger effect of small amount of excessive vacancies, which is due to the relatively high density of the vacancy sinks and the lower quenching temperature, rather than the effect of the β grain boundaries and dislocations as precipitation sites.
Read full abstract