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Experiments on crystal nucleation are predominantly interpreted theoretically in terms of classical nucleation theory (CNT). This theory relies on thermodynamic concepts developed by Gibbs. Their application implies that the bulk properties of critical clusters governing nucleation are widely identical to those of the newly evolving macroscopic phases. Size effects are incorporated into CNT exclusively by a curvature dependence of the surface tension. This method works well but only down to temperatures near to the maximum of the steady-state nucleation rate. This maximum (at 𝑇 ≅ 𝑇 max ) is correlated with the glass transition temperature, 𝑇 𝑔 , that is, 𝑇 max ≅ 𝑇 𝑔 . For lower temperatures, significant deviations between theoretical predictions and experimental data are observed. We describe here different methods how a curvature dependence of the surface tension can be introduced to describe crystal nucleation correctly in the range 𝑇 ⪆ 𝑇 max ≅ 𝑇 𝑔 . Problems occurring at 𝑇 ⪅ 𝑇 max ≅ 𝑇 𝑔 , denoted sometimes as "breakdown of CNT," are shown to be caused by the glass transition of the liquid. Modifications of CNT are advanced resolving them and giving also the possibility of interpretation of a variety of further experimental data in crystal nucleation (including hysteresis effects in cooling and heating, nucleation flashes in heating) in terms of CNT.
Experiments on crystal nucleation are predominantly interpreted theoretically in terms of classical nucleation theory (CNT). This theory relies on thermodynamic concepts developed by Gibbs. Their application implies that the bulk properties of critical clusters governing nucleation are widely identical to those of the newly evolving macroscopic phases. Size effects are incorporated into CNT exclusively by a curvature dependence of the surface tension. This method works well but only down to temperatures near to the maximum of the steady-state nucleation rate. This maximum (at 𝑇 ≅ 𝑇 max ) is correlated with the glass transition temperature, 𝑇 𝑔 , that is, 𝑇 max ≅ 𝑇 𝑔 . For lower temperatures, significant deviations between theoretical predictions and experimental data are observed. We describe here different methods how a curvature dependence of the surface tension can be introduced to describe crystal nucleation correctly in the range 𝑇 ⪆ 𝑇 max ≅ 𝑇 𝑔 . Problems occurring at 𝑇 ⪅ 𝑇 max ≅ 𝑇 𝑔 , denoted sometimes as "breakdown of CNT," are shown to be caused by the glass transition of the liquid. Modifications of CNT are advanced resolving them and giving also the possibility of interpretation of a variety of further experimental data in crystal nucleation (including hysteresis effects in cooling and heating, nucleation flashes in heating) in terms of CNT.
In the theoretical treatment of crystallization it is commonly assumed that relaxation processes of the liquid proceed fast as compared to crystal nucleation and growth processes. Actually, it is supposed that the liquid is located always in the metastable state corresponding to the current values of pressure and temperature. However, near and below the glass transition temperature, Tg, this condition is commonly not fulfilled. In such cases, in the treatment of crystallization, deviations of the state of the liquid from the respective metastable equilibrium state have to be accounted for in determining the kinetic coefficients governing the crystallization kinetics, the thermodynamic driving force of crystallization, and the surface tension of the aggregates of the newly evolving crystal phase including the surface tension of critical clusters affecting considerably the crystal nucleation rate. These factors may considerably influence the course of the overall crystallization process. A theoretical analysis of the resulting effects is given in the present paper by numerical solutions of the J(ohnson)–M(ehl)–A(vrami)–K(olmogorov)–equation employed as the tool to model the overall crystallization kinetics and by analytical estimates of the crystallization peak temperatures in dependence on cooling and heating rates. The results are shown to be in good agreement with experimental data. Possible extensions of the theory to be explored in future analysis are anticipated.
In the theoretical treatment of crystallization, it is commonly assumed that the relaxation processes of a liquid proceed quickly as compared to crystal nucleation and growth processes. Actually, it is supposed that a liquid is always located in the metastable state corresponding to the current values of pressure and temperature. However, near and below the glass transition temperature, Tg, this condition is commonly not fulfilled. In such cases, in the treatment of crystallization, deviations in the state of the liquid from the respective metastable equilibrium state have to be accounted for when determining the kinetic coefficients governing the crystallization kinetics, the thermodynamic driving force of crystallization, and the surface tension of the aggregates of the newly evolving crystal phase including the surface tension of critical clusters considerably affecting the crystal nucleation rate. These factors may greatly influence the course of the overall crystallization process. A theoretical analysis of the resulting effects is given in the present paper by numerical solutions of the J(ohnson)–M(ehl)–A(vrami)–K(olmogorov) equation employed as the tool to model the overall crystallization kinetics and by analytical estimates of the crystallization peak temperatures in terms of the dependence on cooling and heating rates. The results are shown to be in good agreement with the experimental data. Possible extensions of the theory are anticipated and will be explored in future analysis.
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