Department of Chemical Engineering, Carnegie Mellon University , 5000 Forbes Ave., Pittsburgh, Pennsylvania 15213, United States.
Department of Materials Science and Engineering, Carnegie Mellon University , 5000 Forbes Ave., Pittsburgh, Pennsylvania 15213, United States.
ACS Appl Mater Interfaces. 2017 Feb 1;9(4):4106-4118. doi: 10.1021/acsami.6b11791. Epub 2017 Jan 17.
Metastable polymorphs, many of which have never been fabricated, have been predicted to exhibit interesting and technologically relevant properties. Epitaxial synthesis is a powerful structure-directing method that can produce metastable polymorphs but is typically done in a trial and error fashion. Unfortunately, the relevant thermodynamic terms governing epitaxial synthesis of new materials are unknown. Accurate calculation of the relevant thermodynamic terms and their incorporation into predictive models would accelerate the synthesis of metastable polymorphs by identifying thermodynamically favorable paths. Using density functional theory with three different functionals, we computed several relevant terms for TiO anatase (A) and rutile (R) film growth on low-index surfaces of SrTiO (STO) and BaTiO (BTO) cubic perovskites. After identifying potential coherent epitaxial interfaces based on experimental observations, the volumetric formation, volumetric strain, and areal substrate-film interface energies were calculated for (001)∥(001), (102)∥(011), (100)∥(111), and (112)∥(111) coherent interfaces. These terms were integrated into a standard model of epitaxial nucleation, and the results yielded reasonable agreement between experimental observations and DFT predictions of the preferred epitaxial polymorph. Predicted trends in epitaxial stability were essentially independent of the three functionals used in the calculations. These results are discussed in light of their promise that DFT-informed epitaxial film growth can accelerate fabrication of new polymorphs. These results also validate the recently proposed 20 kJ/mol stability window for predicting which polymorphs could be epitaxially stabilized.
亚稳多晶型物,其中许多从未被制造出来,被预测具有有趣和技术相关的性质。外延合成是一种强大的结构导向方法,可以产生亚稳多晶型物,但通常是通过试错的方式进行。不幸的是,控制新材料外延合成的相关热力学条件未知。准确计算相关热力学条件并将其纳入预测模型将通过确定热力学有利的路径来加速亚稳多晶型物的合成。我们使用三种不同的函数分别使用密度泛函理论计算了 TiO 锐钛矿(A)和金红石(R)在 SrTiO(STO)和 BaTiO(BTO)立方钙钛矿低指数表面上的薄膜生长的几个相关项。在基于实验观察确定潜在的相干外延界面后,计算了(001)∥(001)、(102)∥(011)、(100)∥(111)和(112)∥(111)相干界面的体积形成能、体积应变和面积衬底-薄膜界面能。这些项被整合到一个标准的外延成核模型中,结果与实验观察和 DFT 对首选外延多晶型物的预测之间产生了合理的一致性。预测的外延稳定性趋势基本上与计算中使用的三种函数无关。这些结果根据它们的承诺进行了讨论,即 DFT 启发的外延薄膜生长可以加速新多晶型物的制造。这些结果还验证了最近提出的 20 kJ/mol 稳定性窗口,用于预测哪些多晶型物可以外延稳定。