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量化双层磁性材料中界面和体相对于自旋轨道扭矩的贡献。

Quantifying interface and bulk contributions to spin-orbit torque in magnetic bilayers.

机构信息

Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA.

Department of Materials Science and Engineering, University of Delaware, Newark, Delaware 19716, USA.

出版信息

Nat Commun. 2014;5:3042. doi: 10.1038/ncomms4042.

Abstract

Spin-orbit interaction-driven phenomena such as the spin Hall and Rashba effect in ferromagnetic/heavy metal bilayers enables efficient manipulation of the magnetization via electric current. However, the underlying mechanism for the spin-orbit interaction-driven phenomena remains unsettled. Here we develop a sensitive spin-orbit torque magnetometer based on the magneto-optic Kerr effect that measures the spin-orbit torque vectors for cobalt iron boron/platinum bilayers over a wide thickness range. We observe that the Slonczewski-like torque inversely scales with the ferromagnet thickness, and the field-like torque has a threshold effect that appears only when the ferromagnetic layer is thinner than 1 nm. Through a thickness-dependence study with an additional copper insertion layer at the interface, we conclude that the dominant mechanism for the spin-orbit interaction-driven phenomena in this system is the spin Hall effect. However, there is also a distinct interface contribution, which may be because of the Rashba effect.

摘要

自旋轨道相互作用驱动的现象,如铁磁体/重金属双层中的自旋霍尔和拉什巴效应,使得通过电流有效地控制磁化成为可能。然而,自旋轨道相互作用驱动现象的基本机制仍未解决。在这里,我们开发了一种基于磁光克尔效应的灵敏自旋轨道扭矩磁强计,该磁强计可测量钴铁硼/铂双层在很宽的厚度范围内的自旋轨道扭矩矢量。我们观察到,类似于斯隆采维奇的扭矩与铁磁体的厚度成反比,而场型扭矩则存在一个阈值效应,只有当铁磁层厚度小于 1nm 时才会出现。通过在界面处添加附加的铜插入层的厚度依赖性研究,我们得出结论,该体系中自旋轨道相互作用驱动现象的主要机制是自旋霍尔效应。然而,也存在明显的界面贡献,这可能是由于拉什巴效应。

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