Cardias R, Szilva A, Bezerra-Neto M M, Ribeiro M S, Bergman A, Kvashnin Y O, Fransson J, Klautau A B, Eriksson O, Nordström L
Faculdade de Física, Universidade Federal do Pará, Belém, PA, Brazil.
Department of Physics and Astronomy, Uppsala University, Box 516, 75120, Uppsala, Sweden.
Sci Rep. 2020 Nov 23;10(1):20339. doi: 10.1038/s41598-020-77219-3.
We have derived an expression of the Dzyaloshinskii-Moriya interaction (DMI), where all the three components of the DMI vector can be calculated independently, for a general, non-collinear magnetic configuration. The formalism is implemented in a real space-linear muffin-tin orbital-atomic sphere approximation (RS-LMTO-ASA) method. We have chosen the Cr triangular trimer on Au(111) and Mn triangular trimers on Ag(111) and Au(111) surfaces as numerical examples. The results show that the DMI (module and direction) is drastically different between collinear and non-collinear states. Based on the relation between the spin and charge currents flowing in the system and their coupling to the non-collinear magnetic configuration of the triangular trimer, we demonstrate that the DMI interaction can be significant, even in the absence of spin-orbit coupling. This is shown to emanate from the non-collinear magnetic structure, that can induce significant spin and charge currents even with spin-orbit coupling is ignored.
我们推导了Dzyaloshinskii-Moriya相互作用(DMI)的表达式,对于一般的非共线磁构型,DMI矢量的所有三个分量都可以独立计算。该形式体系在实空间-线性 muffin-tin轨道-原子球近似(RS-LMTO-ASA)方法中实现。我们选择了Au(111)表面上的Cr三角三聚体以及Ag(111)和Au(111)表面上的Mn三角三聚体作为数值示例。结果表明,共线和非共线状态下的DMI(模和方向)有很大不同。基于系统中流动的自旋电流和电荷电流之间的关系以及它们与三角三聚体的非共线磁构型的耦合,我们证明即使在没有自旋轨道耦合的情况下,DMI相互作用也可能很显著。这表明它源于非共线磁结构,即使忽略自旋轨道耦合,这种结构也能诱导出显著的自旋电流和电荷电流。