Spin-orbit torque driven domain wall motion in the absence of Dzyaloshinskii-Moriya interactions

A. Thiaville, J. Miltat
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Abstract

The fine structure and dynamics of magnetic domain walls in ultrathin films with perpendicular magnetization, in presence of a secondary anisotropy, is analysed owing to micro-magnetics. Two cases are considered, a cubic anisotropy typical for (111) oriented garnet epitaxial films, and an orthorhombic anisotropy as found in e.g. Co/W(110) films. The statics is solved first, showing that, in general, domain walls are not of the pure Bloch type. The dynamics under the spin Hall effect induced by a current flowing in an adjacent layer is then monitored. Finite and non-negligible domain wall velocities are predicted in both cases, in the absence of Dzyaloshinskii-Moriya interactions, with distinct behaviours regarding the current density and its orientation with respect to the secondary anisotropy axes. The relevance of these results to recent reports of current driven domain wall dynamics in insulating ultrathin garnet films, capped with platinum, is discussed.
在没有 Dzyaloshinskii-Moriya 相互作用的情况下,自旋轨道力矩驱动的畴壁运动
本研究利用微磁学分析了垂直磁化超薄薄膜中磁畴壁的结构和动态,其中存在二次各向异性。研究考虑了两种情况,一种是 (111) 取向石榴石外延薄膜的典型立方各向异性,另一种是 Co/W(110) 薄膜的正交各向异性。首先求解的是静力学,结果表明,一般来说,畴壁不是纯布洛赫类型的。然后,在相邻层中流动的电流诱导下,对自旋霍尔效应下的动力学进行了监测。在这两种情况下,在没有 Dzyaloshinskii-Moriya 相互作用的情况下,都预测出了有限且不可忽略的畴壁速度,电流密度及其相对于次级各向异性轴的取向具有不同的行为。本文讨论了这些结果与最近关于绝缘超薄石榴石薄膜中电流驱动的畴壁动力学的相关性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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