Modeling of the perovskite nickelate SmNiO3 nucleation from amorphous thin films: A Volmer's thermodynamical approach

IF 8.3 1区 材料科学 Q1 MATERIALS SCIENCE, MULTIDISCIPLINARY Acta Materialia Pub Date : 2024-10-24 DOI:10.1016/j.actamat.2024.120509
Silvère Barrat, Zil Fernández-Gutiérrez, Carlos Calvo-Mola, Pierre-Antoine Tostivint, Stéphanie Bruyère, David Pilloud, Fabien Capon
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Abstract

We present a thermodynamical model based on Volmer's nucleation theory adapted to the case of the perovskite nickelate SmNiO3 crystallization (SNO) from an amorphous (aSNO) thin film. This amorphous phase is synthesized via reactive magnetron sputtering and then subsequently annealed in air at temperatures between 725 and 925 K to crystallize it. This model allows to predict the theoretical nucleation rate of the crystallized perovskite phase according to the annealing temperature, the type of the nucleation (homogeneous and heterogeneous mechanisms) and to estimate some physical and thermodynamical data related to this transformation. A theoretical evaluation of the nucleation rate shows that the optimum temperature for crystallization is close to 800 K for which the nucleation rate can reach 1021 m-3.s-1 if considering both homogeneous and heterogeneous nucleation mechanisms. As the annealing temperature moves away from 800 K, the theoretical nucleation rate drops drastically, as observed experimentally by X-ray Diffraction (XRD) when we annealed 200 nm thick aSNO films. The good agreement between the presented model and the experimental crystallization results allows us to numerically evaluate some physical parameters not yet reported to date in the literature for SNO perovskites such as the surface energy between the amorphous and the crystallized SNO phases, the strain energy when the crystallization occurs and the enthalpy associated with crystallization.

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非晶态薄膜中的包晶镍酸盐 SmNiO3 成核模型:沃尔默热力学方法
我们提出了一个基于沃尔默成核理论的热力学模型,该模型适用于从无定形(aSNO)薄膜结晶出包晶态镍酸盐 SmNiO3(SNO)的情况。这种非晶相是通过反应磁控溅射合成的,随后在 725 至 925 K 的温度下进行空气退火,使其结晶。该模型可根据退火温度、成核类型(均相和异相机制)预测结晶包晶相的理论成核率,并估算与这种转变相关的一些物理和热力学数据。对成核率的理论评估表明,结晶的最佳温度接近 800 K,如果同时考虑均相和异相成核机制,成核率可达 1021 m-3.s-1。当退火温度远离 800 K 时,理论成核率会急剧下降,正如我们在退火 200 nm 厚的 aSNO 薄膜时通过 X 射线衍射 (XRD) 实验观察到的那样。所提出的模型与实验结晶结果之间的良好一致性使我们能够对迄今为止文献中尚未报道的 SNO 包晶体的一些物理参数进行数值评估,如无定形和结晶 SNO 相之间的表面能、发生结晶时的应变能以及与结晶相关的焓。
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来源期刊
Acta Materialia
Acta Materialia 工程技术-材料科学:综合
CiteScore
16.10
自引率
8.50%
发文量
801
审稿时长
53 days
期刊介绍: Acta Materialia serves as a platform for publishing full-length, original papers and commissioned overviews that contribute to a profound understanding of the correlation between the processing, structure, and properties of inorganic materials. The journal seeks papers with high impact potential or those that significantly propel the field forward. The scope includes the atomic and molecular arrangements, chemical and electronic structures, and microstructure of materials, focusing on their mechanical or functional behavior across all length scales, including nanostructures.
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