In the modelling of the kinetics of first order phase transformations, classical theory of nucleation (CTN) and cluster dynamics (CD) rely both on the same physical basis: clusters (i.e. heterophase fluctuations or precipitates of the growing phase) exchange diffusing solute atoms, nucleate and grow in the matrix above a critical size. Both have to solve a set of kinetic master equations. [1][2][3][4] Their bond is given in the Martin talk of this conference. The CD approach is a numerical solving of the master equations which allow determining the time evolution of the cluster size distribution function and from it all physical quantities like cluster number density, mean cluster size, solute within the cluster and in solid solution _.The method is first applied to the precipitation of the ordered L1 2 Al 3 Zr(Sc) phase in binary AlZr and AlSc alloys, [4] and extended to ternary Al(ZrSc) alloys. It is shown that CD gives for multicomponent alloys new insights in the composition path of the precipitates which can be at departure of the classical concepts.
Master Equations and Kinetics Coefficients
Binary AlloysThe time evolution of the cluster size distribution function C n (t) containing n solute atoms must satisfy n differential equations:The absorption coefficient b n is controlled by the solute long range diffusion in series with its impingement rate on the cluster interface. The emission coefficient is deduced from the absorption one by application of a constraint equilibrium condition to the cluster gas b n S n R n DC 1 (for the purely diffusive mode),where S n , R n are the surface area, size of a n cluster and D is the solute diffusion coefficient. C n , the equilibrium distribution function of the cluster gas in a slightly supersaturated COMMUNICATIONS ADVANCED ENGINEERING MATERIALS 2006, 8, No. 12