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Critical Temperature and Tunneling Spectroscopy of Superconductor-Ferromagnet Hybrids with Intrinsic Rashba-Dresselhaus Spin-Orbit Coupling

机译:临界温度和隧道谱   具有内在Rashba-Dresselhaus的超导体 - 铁磁体混合物   自旋轨道耦合

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摘要

We investigate theoretically how the proximity effect insuperconductor/ferromagnet hybrid structures with intrinsic spin-orbit couplingmanifests in the density of states and critical temperature. To describe ageneral scenario, we allow for both Rashba and Dresselhaus type spin-orbitcoupling. Our results are obtained via the quasiclassical theory ofsuperconductivity, extended to include spin-orbit coupling in the Usadelequation and Kupriyanov--Lukichev boundary conditions. Unlike previous works,we have derived a Riccati parametrization of the Usadel equation withspin-orbit coupling which allows us to address the full proximity regime.First, we consider the density of states in both SF bilayers and SFS trilayers,where the spectroscopic features in the latter case are sensitive to the phasedifference between the two superconductors. We find that the presence ofspin-orbit coupling leaves clear spectroscopic fingerprints in the density ofstates due to its role in creating spin-triplet Cooper pairs. Unlike SF and SFSstructures without spin-orbit coupling, the density of states in the presentcase depends strongly on the direction of magnetization. We show that thespin-orbit coupling can stabilize singlet superconductivity even in thepresence of a strong exchange field $h \gg \Delta$. This leads to thepossibility of a magnetically tunable minigap: changing the direction of theexchange field opens and closes the minigap. We also determine how the criticaltemperature $T_c$ of an SF bilayer is affected by spin-orbit coupling anddemonstrate that one can achieve a spin-valve effect with a single ferromagnet.We find that $T_c$ displays highly non-monotonic behavior both as a function ofthe magnetization direction and the type and direction of the spin-orbitcoupling, offering a new way to exert control over the superconductivity ofproximity structures.
机译:我们从理论上研究了具有固有自旋-轨道耦合的超导体/铁磁体混合结构在状态密度和临界温度下的邻近效应。为了描述一般情况,我们允许使用Rashba和Dresselhaus类型的自旋-轨道耦合。我们的结果是通过超导的准经典理论获得的,该理论已扩展到包括Usadelequation和Kupriyanov-Lukichev边界条件中的自旋轨道耦合。与以前的工作不同,我们导出了具有自旋-轨道耦合的Usadel方程的Riccati参数化,这使我们能够解决完整的邻近状态。首先,我们考虑了SF双层和SFS三层中的态密度,后一种情况对两个超导体之间的相差敏感。我们发现自旋-轨道耦合的存在由于其在创建自旋三胞胎库珀对中的作用而在状态密度中留下清晰的光谱指纹。与没有自旋轨道耦合的SF和SFS结构不同,目前的状态密度在很大程度上取决于磁化方向。我们证明,即使存在强交换场$ h \ gg \ Delta $,自旋轨道耦合也可以稳定单重态超导。这导致了可磁调谐的小间隙的可能性:改变交换场的方向打开和关闭小间隙。我们还确定了SF双层的临界温度$ T_c $是如何受自旋-轨道耦合影响的,并证明了单个铁磁体可以实现自旋阀效应。我们发现$ T_c $表现出高度非单调性磁化方向,自旋轨道耦合的类型和方向的函数,为控制邻近结构的超导性提供了新的途径。

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