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了解压力对CsMnF及其他3d化合物的结构、光学和磁性性质的影响。

Understanding Pressure Effects on Structural, Optical, and Magnetic Properties of CsMnF and Other 3d Compounds.

作者信息

Santamaría Guillermo, Fernández-Ruiz Toraya, García-Lastra Juan María, García-Fernández Pablo, Sánchez-Movellán Inés, Moreno Miguel, Aramburu José Antonio

机构信息

Departamento de Ciencias de la Tierra y Física de la Materia Condensada, Universidad de Cantabria, Avenida de los Castros s/n, 39005 Santander, Spain.

Donostia International Physics Center (DIPC), 20018 Donostia, Euskadi, Spain.

出版信息

Inorg Chem. 2024 Jul 22;63(29):13231-13243. doi: 10.1021/acs.inorgchem.4c00599. Epub 2024 Jul 10.

Abstract

The pressure dependence of structural, optical, and magnetic properties of the layered compound CsMnF are explored through first-principles calculations. The structure at ambient pressure does not arise from a Jahn-Teller effect but from an orthorhombic instability on MnF units in the tetragonal parent phase, while there is a 4/ → 4 structural phase transition at = 40 GPa discarding a spin crossover transition from = 2 to = 1. The present results reasonably explain the evolution of spin-allowed d-d transitions under pressure, showing that the first transition undergoes a red-shift under pressure following the orthorhombic distortion in the layer plane. The energy of such a transition at zero pressure is nearly twice that observed in NaMnF due to the internal electric field and the orthorhombic distortion also involved in KCuF. The reasons for the lack of orthorhombic distortion in KMF (M = Ni, Mn) or CsFeF are also discussed in detail. The present calculations confirm the ferromagnetic ordering of layers in CsMnF at zero pressure and predict a shift to an antiferromagnetic phase for pressures above 15 GPa consistent with the reduction of the orthorhombicity of the MnF units. This study underlines the usefulness of first-principles calculations for a right interpretation of experimental findings.

摘要

通过第一性原理计算,研究了层状化合物CsMnF的结构、光学和磁性性质对压力的依赖性。常压下的结构并非源于 Jahn-Teller 效应,而是源于四方母相中 MnF 单元的正交不稳定性,而在 40 GPa 时存在 4/ → 4 结构相变,排除了从 = 2 到 = 1 的自旋交叉转变。目前的结果合理地解释了压力下自旋允许的 d-d 跃迁的演变,表明第一次跃迁在压力下随着层平面中的正交畸变而发生红移。由于内部电场以及 KCuF 中也存在的正交畸变,这种跃迁在零压力下的能量几乎是在 NaMnF 中观察到的两倍。还详细讨论了 KMF(M = Ni、Mn)或 CsFeF 中缺乏正交畸变的原因。目前的计算证实了 CsMnF 在零压力下各层的铁磁有序性,并预测对于高于 15 GPa 的压力会转变为反铁磁相,这与 MnF 单元正交性的降低一致。这项研究强调了第一性原理计算对于正确解释实验结果的有用性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a9c3/11271007/9cf9027e1e1d/ic4c00599_0001.jpg

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