Abstract
The process of ripening has been considered taking into account the noise from different sources, namely the scatter of compositions (supersaturation Δ) in the vicinity of precipitates and scatter of the Gibbs–Thompson term α. The evolution of the particle size distribution (PSD) has been investigated using parameters that characterize the width, sharpness and slope of the peak. Accounting for noise in our model produces a PSD that is closer to the experimental data compared with LSW theory.
Acknowledgements
The authors would like to acknowledge the support of the Civilian Research and Development Foundation (#UE1-2523-CK-09) and the Ministry of Education and Science of Ukraine. They also would like to thank Professor K.N. Tu at the University of California Los Angeles for helpful discussions.