In this equation, the phase fraction for the destination phase tends toward an equilibrium value
, and the rate at which this occurs is characterized by the time constant τs → d. Note here that the equilibrium phase fraction and the time constant are in general both temperature dependent, and that temperature in turn varies with time. At constant temperature, the equation can be integrated analytically, giving
The equilibrium phase fraction can be deduced from an (equilibrium) iron–carbon diagram (Ref. 1) or from dilatometry experiments at a very low temperature rate (or at constant temperature after a rapid temperature drop). If we know this equilibrium phase fraction at a given temperature
t1, we can compute the temperature-dependent time constant from knowing the time it takes to reach a specific phase fraction (isothermally):
the time constant is obtained without knowing the equilibrium phase fraction. Thus, a TTT diagram showing curves of transformation times corresponding to relative phase fractions X can straightforwardly be used to compute the temperature-dependent time constant. In this sense, a TTT diagram is easier to use for phase transformation model calibration than a CCT diagram. This method to the calibration of phase transformation models to TTT diagram data can be used also for the Johnson–Mehl–Avrami–Kolmogorov (JMAK) and Kirkaldy–Venugopalan models. It should be pointed out that given a set of phase transformation model parameters, it is straightforward to
compute both types of diagrams and to adjust the model parameters based on comparisons of the computed diagrams and experimental information. It is sometimes necessary to iterate in this manner to find a sufficiently accurate set of model parameters.