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Energy spectra for quantum wires and two-dimensional electron gases in magnetic fields with Rashba and Dresselhaus spin-orbit interactions

机译:具有Rashba和Dresselhaus自旋轨道相互作用的磁场中的量子线和二维电子气的能谱

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We introduce an analytical approximation scheme to diagonalize parabolically confined two-dimensional (2D) electron systems with both the Rashba and Dresselhaus spin-orbit interactions. The starting point of our perturbative expansion is a zeroth-order Hamiltonian for an electron confined in a quantum wire with an effective spin-orbit induced magnetic field along the wire, obtained by properly rotating the usual spin-orbit Hamiltonian. We find that the spin-orbit-related transverse coupling terms can be recast into two parts W and V, which couple crossing and noncrossing adjacent transverse modes, respectively. Interestingly, the zeroth-order Hamiltonian together with W can be solved exactly, as it maps onto the Jaynes-Cummings model of quantum optics. We treat the V coupling by performing a Schrieffer-Wolff transformation. This allows us to obtain an effective Hamiltonian to third order in the coupling strength k_Re of V, which can be straightforwardly diagonalized via an additional unitary transformation. We also apply our approach to other types of effective parabolic confinement, e.g., 2D electrons in a perpendicular magnetic field. To demonstrate the usefulness of our approximate eigensolutions, we obtain analytical expressions for the nth Landau-level g_n factors in the presence of both Rashba and Dresselhaus couplings. For small values of the bulk g factors, we find that spin-orbit effects cancel out entirely for particular values of the spin-orbit couplings. By solving simple transcendental equations we also obtain the band minima of a Rashba-coupled quantum wire as a function of an external magnetic field. These can be used to describe Shubnikov-de Haas oscillations. This procedure makes it easier to extract the strength of the spin-orbit interaction in these systems via proper fitting of the data.
机译:我们引入了一种解析近似方案,以使具有Rashba和Dresselhaus自旋轨道相互作用的抛物线受限二维(2D)电子系统对角化。我们的扰动展开的起点是零电子哈密顿量,该电子是被限制在量子线中的电子,沿着该线具有有效的自旋轨道感应磁场,是通过适当旋转通常的自旋轨道哈密顿量获得的。我们发现,与自旋轨道有关的横向耦合项可以重塑为W和V两部分,分别耦合相交和不相交的相邻横向模式。有趣的是,零阶哈密顿量和W可以精确求解,因为它映射到量子光学的Jaynes-Cummings模型上。我们通过执行Schrieffer-Wolff变换来处理V耦合。这使我们能够在V的耦合强度k_Re上获得有效的哈密顿量至三阶,可以通过附加的unit变换直接将其对角线化。我们还将我们的方法应用于其他类型的有效抛物线约束,例如垂直磁场中的2D电子。为了证明我们近似本征解的有效性,我们在存在Rashba和Dresselhaus耦合的情况下,获得了第n个Landau级g_n因子的解析表达式。对于总g因子的较小值,我们发现自旋轨道效应完全抵消了自旋轨道耦合的特定值。通过求解简单的超越方程,我们还获得了Rashba耦合量子线的能带最小值,它是外部磁场的函数。这些可以用来描述Shubnikov-de Haas振荡。通过适当拟合数据,此过程使提取这些系统中自旋轨道相互作用的强度变得更加容易。

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