首页> 外文期刊>Journal of magnetism and magnetic materials >Perpendicular magnetic anisotropy in Mo/Co_2FeAl_(0.5)Si_(0.5)/MgO/Mo multilayers with optimal Mo buffer layer thickness
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Perpendicular magnetic anisotropy in Mo/Co_2FeAl_(0.5)Si_(0.5)/MgO/Mo multilayers with optimal Mo buffer layer thickness

机译:具有最佳Mo缓冲层厚度的Mo / Co_2FeAl_(0.5)Si_(0.5)/ MgO / Mo多层膜的垂直磁各向异性

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摘要

Perpendicular Magnetic Anisotropy (PMA) was realized in as-deposited Mo(10)/Co2FeAl0.5Si0.5(CFAS)(3)/MgO(0.5)/Mo multilayer stacks with large perpendicular magnetic anisotropy energy (Keff). PMA of this multilayer is found to be strongly dependent on the thickness of the individual CFAS (tCFAS), Mo (tMo) and MgO (tMgO) layers and annealing temperatures. The interactions at the Mo/CFAS/MgO interfaces are critical to induce PMA and are tuned by the interfacial oxidation. The major contribution to PMA is due to iron oxide at the CFAS/MgO interface. X-ray diffraction (XRD) and infrared spectroscopic (FT-IR) studies further ascertain this. However, an adequate oxidation of MgO and the formation of (0 2 4) and (0 1 8) planes of α-Fe2O3at the optimal Mo buffer layer thickness is mainly inducing PMA in Mo/CFAS/MgO/Mo stack. Microstructural changes in the films are observed by atomic force microscopy (AFM). X-ray photoelectron spectroscopy (XPS) demonstrates the oxidation of CFAS/MgO interface and the formation of Fe–O bonds confirming that the real origin of PMA in Mo/CFAS/MgO is due to hybridization of Fe (3dz2) and O (2pz) orbitals and the resulted spin-orbit interaction at their interface. The half-metallic nature CFAS with Mo layer exhibiting PMA can be a potential candidate as p-MTJs electrodes for the new generation spintronic devices.
机译:垂直磁各向异性(PMA)在具有较大垂直磁各向异性能(Keff)的Mo(10)/Co2FeAl0.5Si0.5(CFAS)(3)/ MgO(0.5)/ Mo多层堆叠中实现。发现该多层的PMA强烈依赖于各个CFAS(tCFAS),Mo(tMo)和MgO(tMgO)层的厚度以及退火温度。 Mo / CFAS / MgO界面上的相互作用对于诱导PMA至关重要,并通过界面氧化进行调节。对PMA的主要贡献是由于CFAS / MgO界面处的氧化铁。 X射线衍射(XRD)和红外光谱(FT-IR)研究进一步确定了这一点。然而,在最佳Mo缓冲层厚度下,MgO充分氧化并形成(0-2 4)和(0 1 8)平面的α-Fe2O3主要是在Mo / CFAS / MgO / Mo堆中引起PMA。通过原子力显微镜(AFM)观察膜的微观结构变化。 X射线光电子能谱(XPS)证明CFAS / MgO界面的氧化和Fe–O键的形成证实了PMA在Mo / CFAS / MgO中的真正起源是由于Fe(3dz2)和O(2pz )轨道,以及在其界面处产生的自旋轨道相互作用。具有Mo层且呈现PMA的半金属性质CFAS可能是新一代自旋电子器件的p-MTJs电极的潜在候选者。

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