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Broken spin-Hall accumulation symmetry by magnetic field and coexisted Rashba and Dresselhaus interactions

机译:磁场破坏了自旋霍尔累积对称性,并存在Rashba和Dresselhaus相互作用

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The spin-Hall effect in the two-dimensional electron gas (2DEG) generates symmetric out-of-plane spin S_z accumulation about the current axis in the absence of external magnetic field. Here we employ the real space Landauer-Keldysh formalism [B. K. Nikolic et al., Phys. Rev. Lett. 95, 046601 (2005); Phys. Rev. B 73, 075303 (2006)] by considering a four-terminal setup to investigate the circumstances in which this symmetry is broken. For the absence of Dresselhaus interaction, starting from the applied out-of-plane B corresponding to Zeeman splitting energy Δ=0-0.5 times the Rashba hopping energy t_(SO)~R, the breaking process is clearly seen. The influence of the Rashba interaction on the magnetization of the 2DEG is studied herein. For coexisted Rashba t_(SO)~R and Dresselhaus t_(SO)~D spin-orbit couplings in the absence of B, interchanging t_(SO)~R and t_(SO)~D reverses the entire accumulation pattern.
机译:在没有外部磁场的情况下,二维电子气(2DEG)中的自旋霍尔效应产生围绕电流轴的对称平面外自旋S_z累积。在这里,我们采用了真正的空间Landauer-Keldysh形式主义[B. K. Nikolic et al。,Phys。牧师95,046601(2005);物理Rev. B 73,075303(2006)]通过考虑四端设置来研究这种对称性被破坏的情况。对于不存在Dresselhaus相互作用的情况,从对应于塞曼分裂能Δ= 0-0.5倍于Rashba跳跃能t_(SO)〜R的施加的平面外B开始,可以清楚地看到破坏过程。本文研究了Rashba相互作用对2DEG磁化强度的影响。对于在没有B的情况下共存的Rashba t_(SO)〜R和Dresselhaus t_(SO)〜D自旋轨道耦合,交换t_(SO)〜R和t_(SO)〜D会反转整个累积模式。

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