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arXiv 1504.04451cond-mat.mes-hall
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自旋霍尔效应的规范物理

Gauge Physics of Spin Hall Effect

Seng Ghee Tan, Mansoor B. A. Jalil, Congson Ho, Zhuobin Siu, Shuichi Murakami

摘要:

自旋霍尔效应(SHE)已经在Kubo公式,几何物理,自旋轨道力和许多半经典处理的背景下进行了讨论。如果不同的图片对SHE有部分或重叠的贡献,可能会令人困惑。在这篇文章中,我们提出了规范理论,时间动量的说明,它提供了一个通用的SHE运动方程,统一在一个理论框架下,所有的贡献SHE电导率由于动力学,自旋轨道力(杨米尔斯),和几何(村上藤田)的影响。我们的工作提出了正确的模糊性周围以前部分治疗涉及久保,半经典,贝里曲率,或自旋轨道力。完全处理显示Rashba 2DEG SHE电导率为+e/8π而不是-e/8π,Rashba重空穴为+9e/8π而不是-9e/8π。

英文摘要:

Spin Hall effect (SHE) has been discussed in the context of Kubo formulation, geometric physics, spin orbit force, and numerous semi-classical treatments. It can be confusing if the different pictures have partial or overlapping claims of contribution to the SHE. In this article, we present a gauge-theoretic, time-momentum elucidation, which provides a general SHE equation of motion, that unifies under one theoretical framework, all contributions of SHE conductivity due to the kinetic, the spin orbit force (Yang-Mills), and the geometric (Murakami-Fujita) effects. Our work puts right an ambiguity surrounding previously partial treatments involving the Kubo, semiclassical, Berry curvatures, or the spin orbit force. The full treatment shows the Rashba 2DEG SHE conductivity to be +e/8π instead of -e/8π , and Rashba heavy hole +9e/8π instead of -9e/8π .

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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