ALBA Synchrotron Light Source , Cerdanyola del Vallès, E-08290 Barcelona , Catalonia , Spain.
Institut de Ciència de Materials de Barcelona (ICMAB-CSIC) , Campus UAB , 08193 Bellaterra , Catalonia , Spain.
ACS Appl Mater Interfaces. 2018 Apr 11;10(14):12031-12041. doi: 10.1021/acsami.8b00384. Epub 2018 Mar 30.
Pure spin currents have potential for use in energy-friendly spintronics. They can be generated by a flow of charge along a nonmagnetic metal with large spin-orbit coupling. This produces a spin accumulation at the surfaces, controllable by the magnetization of an adjacent ferromagnetic layer. Paramagnetic metals typically used are close to ferromagnetic instability and thus magnetic proximity effects can contribute to the observed angular-dependent magnetoresistance (ADMR). As interface phenomena govern the spin conductance across the metal/ferromagnetic-insulator heterostructures, unraveling these distinct contributions is pivotal for a full understanding of spin current conductance. Here, we report X-ray absorption and magnetic circular dichroism (XMCD) at Pt M and (Co, Fe) L absorption edges and atomically resolved energy electron loss spectroscopy (EELS) data of Pt/CoFeO bilayers, where CoFeO layers have been capped by Pt grown at different temperatures. It was found that the ADMR differs dramatically, dominated either by spin Hall magnetoresistance (SMR) associated with the spin Hall effect or by anisotropic magnetoresistance. The XMCD and EELS data indicate that the Pt layer grown at room temperature does not display any magnetic moment, whereas when grown at a higher temperature, it becomes magnetic due to interfacial Pt-(Co, Fe) alloying. These results enable differentiation of spin accumulation from interfacial chemical reconstructions and tailoring of the angular-dependent magnetoresistance.
纯自旋流在节能型自旋电子学中有应用潜力。它们可以通过在具有大自旋轨道耦合的非磁性金属中沿电荷流动产生。这会在表面产生自旋积累,可通过相邻铁磁层的磁化来控制。通常使用的顺磁金属接近铁磁不稳定性,因此磁近邻效应可能有助于观察到的角度相关磁电阻(ADMR)。由于界面现象控制着金属/铁磁绝缘体异质结构中的自旋电导,因此解开这些不同的贡献对于全面理解自旋电流电导至关重要。在这里,我们报告了 Pt M 和(Co,Fe)L 吸收边缘的 X 射线吸收和磁圆二色性(XMCD)以及 Pt/CoFeO 双层的原子分辨能量电子损失光谱(EELS)数据,其中 CoFeO 层被在不同温度下生长的 Pt 覆盖。结果发现,ADMR 差异很大,主要由与自旋霍尔效应相关的自旋霍尔磁电阻(SMR)或各向异性磁电阻主导。XMCD 和 EELS 数据表明,在室温下生长的 Pt 层不显示任何磁矩,而当在较高温度下生长时,由于界面处的 Pt-(Co, Fe) 合金化,它会变得具有磁性。这些结果使我们能够区分自旋积累和界面化学重构,并调整角度相关的磁电阻。