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时间反演对称破缺的量子自旋霍尔效应。

Time-reversal-symmetry-broken quantum spin Hall effect.

机构信息

National Laboratory of Solid State Microstructures, Nanjing University, China.

出版信息

Phys Rev Lett. 2011 Aug 5;107(6):066602. doi: 10.1103/PhysRevLett.107.066602. Epub 2011 Aug 2.

Abstract

The quantum spin Hall (QSH) state of matter is usually considered to be protected by time-reversal (TR) symmetry. We investigate the fate of the QSH effect in the presence of the Rashba spin-orbit coupling and an exchange field, which break both inversion and TR symmetries. It is found that the QSH state characterized by nonzero spin Chern numbers C(±) = ±1 persists when the TR symmetry is broken. A topological phase transition from the TR-symmetry-broken QSH phase to a quantum anomalous Hall phase occurs at a critical exchange field, where the bulk band gap just closes. It is also shown that the transition from the TR-symmetry-broken QSH phase to an ordinary insulator state cannot happen without closing the band gap.

摘要

物质的量子自旋霍尔(QSH)态通常被认为受到时间反演(TR)对称性的保护。我们研究了在拉什巴自旋轨道耦合和外磁场存在下,同时破坏反转和 TR 对称性时,QSH 效应的命运。结果发现,当 TR 对称性被破坏时,具有非零自旋陈数 C(±)=±1 的 QSH 态仍然存在。在一个临界外磁场下,从 TR 对称破坏的 QSH 相到量子反常霍尔相的拓扑相变发生,此时体带隙刚好闭合。还表明,没有闭合带隙,TR 对称破坏的 QSH 相到普通绝缘体态的转变是不可能发生的。

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