论文标题

量化由块状磁不对称引起的dzyaloshinskii-moriya相互作用

Quantifying the Dzyaloshinskii-Moriya Interaction Induced by the Bulk Magnetic Asymmetry

论文作者

Zhang, Qihan, Liang, Jinghua, Bi, Kaiqi, Zhao, Le, Bai, He, Cui, Qirui, Zhou, Heng-An, Bai, Hao, Feng, Hongmei, Song, Wenjie, Chai, Guozhi, Gladii, O., Schultheiss, H., Zhu, Tao, Zhang, Junwei, Peng, Yong, Yang, Hongxin, Jiang, Wanjun

论文摘要

通常认为,超薄铁磁性/重金属(FM/HM)双层中的破碎界面反演对称性通常被认为是容纳Dzyaloshinskii-Moriya相互作用(DMI)和稳定手性旋转质地的先决条件。在这些双层中,随着FM层的厚度的增加和消失,DMI的强度会衰减。在本研究中,通过合成相对较厚的组合物或fept,CoCu或Fecu,FeGD和Feni的合成膜,从组成梯度诱导的体积磁不对称(BMA)和自旋孔偶联(SOC)对DMI的贡献进行了系统的检查。在实验研究的情况下,使用Brillouin光散射光谱,在具有可控制的方向和强度的膜中,在SOC的存在和不存在的情况下,DMI的符号和幅度均已进行了实验研究。特别是,我们表明,可以在COPT或具有BMA和强SOC的Fept膜中实现相当大的DMI(0.15 MJ/M^2),而在其他具有BMA的厚膜中可以观察到可忽略的DMI强度,但没有明显的SOC。基于三个位点Fert-levy模型和第一原理计算,进一步研究了BMA和SOC的关键作用。可以预期,我们的发现可能有助于进一步了解手性磁性的起源并设计新颖的非连线性旋转纹理。

A broken interfacial inversion symmetry in ultrathin ferromagnet/heavy metal (FM/HM) bilayers is generally believed to be a prerequisite for accommodating the Dzyaloshinskii-Moriya interaction (DMI) and for stabilizing chiral spin textures. In these bilayers, the strength of the DMI decays as the thickness of the FM layer increases and vanishes around a few nanometers. In the present study, through synthesizing relatively thick films of compositions CoPt or FePt, CoCu or FeCu, FeGd and FeNi, contributions to DMI from the composition gradient induced bulk magnetic asymmetry (BMA) and spin-orbit coupling (SOC) are systematically examined. Using Brillouin light scattering spectroscopy, both the sign and amplitude of DMI in films with controllable direction and strength of BMA, in the presence and absence of SOC are experimentally studied. In particular, we show that a sizable amplitude of DMI (0.15 mJ/m^2) can be realized in CoPt or FePt films with BMA and strong SOC, whereas negligible DMI strengths are observed in other thick films with BMA but without significant SOC. The pivotal roles of BMA and SOC are further examined based on the three-site Fert-Levy model and first-principles calculations. It is expected that our findings may help to further understand the origin of chiral magnetism and to design novel non-collinear spin textures.

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