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In silico infrared and Raman spectroscopy under pressure: The case of CaSnO3 perovskite

机译:压力下的硅红外和拉曼光谱:钙钛矿型CaSnO3的情况

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The CaSnO3 perovskite is investigated under geochemical pressure, up to 25 GPa, by means of periodic ab initio calculations performed at B3LYP level with local Gaussian-type orbital basis sets. Structural, elastic, and spectroscopic (phonon wave-numbers, infrared and Raman intensities) properties are fully characterized and discussed. The evolution of the Raman spectrum of CaSnO3 under pressure is reported to remarkably agree with a recent experimental determination [J. Kung, Y. J. Lin, and C. M. Lin, J. Chem. Phys. 135, 224507 (2011)] as regards both wave-number shifts and intensity changes. All phonon modes are symmetry-labeled and bands assigned. The single-crystal total spectrum is symmetry-decomposed into the six directional spectra related to the components of the polarizability tensor. The infrared spectrum at increasing pressure is reported for the first time and its main features discussed. All calculations are performed using the CRYSTAL14 program, taking advantage of the new implementation of analytical infrared and Raman intensities for crystalline materials. (C) 2015 AIP Publishing LLC.
机译:CaSnO3钙钛矿在高达25 GPa的地球化学压力下,通过在局部高斯型轨道基组上以B3LYP进行的周期性从头算的方法研究。对结构,弹性和光谱(声子波数,红外和拉曼强度)特性进行了充分表征和讨论。据报道,CaSnO3在压力下的拉曼光谱的演变与最近的实验结果非常吻合[J. Kung,Y.J. Lin,and C.M.Lin,J.Chem。物理135,224507(2011)]。所有声子模式均已对称标记并分配了频段。将单晶总光谱对称地分解为与极化率张量的分量有关的六个方向光谱。首次报道了压力升高时的红外光谱及其主要特征。所有计算均使用CRYSTAL14程序进行,并充分利用了晶体材料的分析红外和拉曼强度的新实现。 (C)2015 AIP Publishing LLC。

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