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Kerr magneto-optic effect in ferromagnetic CrBr3

机译:铁磁CrBr3中的Kerr磁光效应

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摘要

In ferromagnetic CrBr3 the Kerr rotation is a significant effect which is not fully understood. Early investigations suggested that t1u(π)->t*2g and t2u(π)->t*2g and t1u(σ)->e*g and/or t*2g->t*1u were the contributing transitions. Recent investigations have overturned those assignments. Instead, a pair of transitions, t1u(π)->e*g and t2u(π)->e*g, with negative and positive spin-orbit coupling coefficients respectively, were shown to explain the Kerr rotation. A simplistic LCAO calculation on a small cluster, combined with Gaussian fits to data, supports those reassignments. We present results of a similar LCAO calculation and Gaussian fit for CrCl3.
机译:在铁磁CrBr3中,克尔旋转是一个重要的效应,目前尚未完全了解。早期研究表明,t1u(π)-> t * 2g和t2u(π)-> t * 2g和t1u(σ)-> e * g和/或t * 2g-> t * 1u是促成转变。最近的调查推翻了这些任务。取而代之的是,示出了分别具有负和正自旋轨道耦合系数的一对跃迁t1u(π)-> e * g和t2u(π)-> e * g来解释Kerr旋转。在小型群集上进行简单的LCAO计算,再结合对数据的高斯拟合,即可支持这些重新分配。我们提出了类似的LCAO计算结果和CrCl3的高斯拟合结果。

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