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arXiv 1612.03060cond-mat.str-el
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Sr2RuO4的费米面:自旋轨道和各向异性库仑相互作用效应

The Fermi surface of Sr2RuO4: spin-orbit and anisotropic Coulomb interaction effects

Guoren Zhang, Evgeny Gorelov, Esmaeel Sarvestani, Eva Pavarini

摘要:

在局域密度近似下,考虑自旋轨道相互作用,可以很好地描述Sr 2 RuO 4费米面的拓扑结构,但不能很好地描述其不同层的相对尺寸.通过占多体效应,通过动力学平均场论,我们表明,标准的各向同性库仑相互作用单独的纠正或不纠正这种差异。为了重现实验,必须考虑库仑各向异性。后者是小的,但有很强的影响,它的竞争与库仑增强的自旋轨道耦合和各向同性库仑项在确定费米面的形状。它的影响在其他相关的多轨道系统中可能相当大。此外,我们发现,低能量的自能矩阵-负责费米表面的重塑- sizably不同于静态Hartree-Fock极限。最后,我们发现一个强大的自旋轨道{纠缠},这支持了这样的观点,即传统的描述库珀对通过因式分解的自旋和轨道部分可能不适用于Sr 2 RuO 4。

英文摘要:

The topology of the Fermi surface of Sr2RuO4 is well described by local-density approximation calculations with spin-orbit interaction, but the relative size of its different sheets is not. By accounting for many-body effects via dynamical mean-field theory, we show that the standard isotropic Coulomb interaction alone worsens or does not correct this discrepancy. In order to reproduce experiments, it is essential to account for the Coulomb anisotropy. The latter is small but has strong effects; it competes with the Coulomb-enhanced spin-orbit coupling and the isotropic Coulomb term in determining the Fermi surface shape. Its effects are likely sizable in other correlated multi-orbital systems. In addition, we find that the low-energy self-energy matrix -- responsible for the reshaping of the Fermi surface -- sizably differ from the static Hartree-Fock limit. Finally, we find a strong spin-orbital {entanglement}; this supports the view that the conventional description of Cooper pairs via factorized spin and orbital part might not apply to Sr2RuO4.

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