Johansen Øyvind, Linder Jacob
Department of Physics, NTNU, Norwegian University of Science and Technology, N-7491 Trondheim, Norway.
Sci Rep. 2016 Sep 22;6:33845. doi: 10.1038/srep33845.
We consider theoretically the impact of Rashba spin-orbit coupling on spin torque oscillators (STOs) in synthetic ferromagnets and antiferromagnets that have either a bulk multilayer or a thin film structure. The synthetic magnets consist of a fixed polarizing layer and two free magnetic layers that interact through the Ruderman-Kittel-Kasuya-Yosida interaction. We determine analytically which collinear states along the easy axis that are stable, and establish numerically the phase diagram for when the system is in the STO mode and when collinear configurations are stable, respectively. It is found that the Rashba spin-orbit coupling can induce anti-damping in the vicinity of the collinear states, which assists the spin transfer torque in generating self-sustained oscillations, and that it can substantially increase the STO part of the phase diagram. Moreover, we find that the STO phase can extend deep into the antiferromagnetic regime in the presence of spin-orbit torques.
我们从理论上考虑了 Rashba 自旋轨道耦合对具有体多层或薄膜结构的合成铁磁体和反铁磁体中自旋扭矩振荡器(STO)的影响。合成磁体由一个固定的极化层和两个通过 Ruderman-Kittel-Kasuya-Yosida 相互作用相互作用的自由磁层组成。我们通过解析确定了沿易轴哪些共线状态是稳定的,并分别通过数值方法建立了系统处于 STO 模式和共线配置稳定时的相图。结果发现,Rashba 自旋轨道耦合可以在共线状态附近诱导反阻尼,这有助于自旋转移扭矩产生自持振荡,并且它可以显著增加相图中的 STO 部分。此外,我们发现,在存在自旋轨道扭矩的情况下,STO 相可以深入延伸到反铁磁区域。