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We perform a quantitative analysis of Monte Carlo simulations results ofphase separation in ternary blends upon evaporation of one component.Specifically, we calculate the average domain size and plot it as a function ofsimulation time to compute the exponent of the obtained power-law. We compareand discuss results obtained by two different methods, for three differentmodels: 2D binary-state model (Ising model), 2D ternary-state model with andwithout evaporation. For the ternary-state models, we study additionally thedependence of the domain growth on concentration, temperature and initialcomposition. We reproduce the expected 1/3 exponent for the Ising model, whilefor the ternary-state model without evaporation and for the one withevaporation we obtain lower values of the exponent. It turns out that phaseseparation patterns that can form in this type of systems are complex. Theobtained quantitative results give valuable insights towards devisingcomputable theoretical estimations of size effects on morphologies as theyoccur in the context of organic solar cells.

Quantitative analysis of phase formation and growth in ternary mixtures upon evaporation of one component