The Einstein-de Haas Effect in an $\textrm{Fe}_{15}$ Cluster

Tomos Wells, Matthew Foulkes, Andrew Horsfield, Sergei Dudarev
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Abstract

Classical models of spin-lattice coupling are at present unable to accurately reproduce results for numerous properties of ferromagnetic materials, such as heat transport coefficients or the sudden collapse of the magnetic moment in hcp-Fe under pressure. This inability has been attributed to the absence of a proper treatment of effects that are inherently quantum mechanical in nature, notably spin-orbit coupling. This paper introduces a time-dependent, non-collinear tight binding model, complete with spin-orbit coupling and vector Stoner exchange terms, that is capable of simulating the Einstein-de Haas effect in a ferromagnetic $\textrm{Fe}_{15}$ cluster. The tight binding model is used to investigate the adiabaticity timescales that determine the response of the orbital and spin angular momenta to a rotating, externally applied $B$ field, and we show that the qualitative behaviours of our simulations can be extrapolated to realistic timescales by use of the adiabatic theorem. An analysis of the trends in the torque contributions with respect to the field strength demonstrates that SOC is necessary to observe a transfer of angular momentum from the electrons to the nuclei at experimentally realistic $B$ fields. The simulations presented in this paper demonstrate the Einstein-de Haas effect from first principles using a Fe cluster.
$\textrm{Fe}_{15}$簇中的爱因斯坦-德哈斯效应
经典的自旋-晶格耦合模型目前还不能准确地再现铁磁材料的许多特性的结果,如热输运系数或在压力下铁磁磁矩的突然崩溃。这种无能归因于缺乏对本质上固有的量子力学效应的适当处理,特别是自旋轨道耦合。本文介绍了一个具有自旋-轨道耦合和矢量-斯通纳交换项的随时间非共线紧密结合模型,该模型能够模拟铁磁$\textrm{Fe}_{15}$团簇中的爱因斯坦-德哈斯效应。紧密结合模型用于研究确定轨道和自旋角动量对旋转的响应的绝热时间尺度,外部施加的$B$场,我们表明,我们的模拟的定性行为可以通过使用绝热定理外推到现实的时间尺度。转矩对场强的贡献趋势分析表明,在实验实际的$B$场中,为了观察角动量从电子到原子核的转移,SOC是必要的。本文用铁簇从第一原理证明了爱因斯坦-德哈斯效应。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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