A new genetic alloy design approach based on thermodynamic and kinetic principles is presented to calculate the optimal composition of MX carbonitrides precipitation strengthened austenitic heat-resistant steels. Taking the coarsening of the MX carbonitrides as the process controlling the life time for steels in high temperature use, the high temperature strength is calculated as a function of steel chemistry, service temperature and time. New steel compositions for different service conditions are found yielding optimal combinations of strength and stability of the strengthening precipitation for specific applications such as fireresistant steels (short-time property guarantee) and creep-resistant steels (longtime property guarantee). Using the same modelling approach, the high temperature strength and lifetime of existing commercial austenitic creep-resistant steels were also calculated and a good qualitative agreement with reported experimental results was obtained. According to the evaluation parameter employed, the newly defined steel compositions may have higher and more stable precipitation strengthening factors than existing high-temperature precipitate-strengthened austenite steels.
IntroductionAustenitic heat-resistant steels are in great demand in power plants, aerospace and other industrial applications operating at elevated temperatures because of their superior creep strength, corrosion and oxidation resistances. The austenite family of temperature-resistant steels predictably contains high amounts of austenite stabilizer, Ni and various alloying elements to strengthen and stabilize the alloys. On top of the solid solution strengthening effect, alloys can be further and more effectively strengthened by different types of precipitates, such as MX carbonitrides (as in high strength low alloy steels [1], creep-resistant steels: 347H, TEMPALOY A-1 and NF 709 [2,3]), Cu particles (as in Super 304H [4]) and Ni 3 Ti (as in A286 [5]). In order to promote the formation of MX carbonitrides, carbonitride-forming elements, such as Ti and Nb, are added in the system. The formation of carbonitrides also prevents the depletion of Cr in the matrix by suppressing the precipitation of Cr-rich M 23 C 6 , and thus helps to sustain a good