# Nucleation and growth of a core-shell composite nucleus by diffusion

**Authors:** Masao Iwamatsu

arXiv: 1704.03369 · 2017-05-24

## TL;DR

This paper investigates the diffusion-driven nucleation process of core-shell structures, defining a kinetic critical radius that explains the formation and growth of such nuclei, aligning with experimental observations.

## Contribution

It introduces the concept of a kinetic critical radius for core-shell nuclei, providing formulas and a theoretical framework that extend classical nucleation theory to these structures.

## Key findings

- Two critical radii exist for core-shell nuclei, corresponding to a single energy barrier.
- The growth follows Ostwald's step rule, consistent with experimental data.
- Formulas similar to classical nucleation theory are derived for the critical radii.

## Abstract

The critical radius of a core-shell-type nucleus grown by diffusion in a phase-separated solution is studied. A {\it kinetic} critical radius rather than the {\it thermodynamic} critical radius of standard classical nucleation theory can be defined from the diffusional growth equations. It is shown that there exist two kinetic critical radii for the core-shell-type nucleus, for which both the inner core radius and the outer shell radius will be stationary. Therefore, these two critical radii correspond to a single critical point of the nucleation path with a single energy barrier even though the nucleation looks like a two-step process. The two radii are given by formulas similar to that of classical nucleation theory if the Ostwald-Freundlich boundary condition is imposed at the surface of the inner nucleus and that of the outer shell. The subsequent growth of a core-shell-type post-critical nucleus follows the classical picture of Ostwald's step rule. Our result is consistent with some of the experimental and numerical results which suggest the core-shell-type critical nucleus.

## Full text

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## Figures

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## References

40 references — full list in the complete paper: https://tomesphere.com/paper/1704.03369/full.md

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Source: https://tomesphere.com/paper/1704.03369