论文标题

在W上生长的外延GD膜的磁域结构(110)

Magnetic domain structure of epitaxial Gd films grown on W(110)

论文作者

Härtl, Patrick, Leisegang, Markus, Bode, Matthias

论文摘要

我们提出了一项详细的真实空间自旋扫描隧道显微镜(SP-STM)研究GD(0001)膜在W上外上生根生长(110)的磁结构结构的研究。为了找到最佳的制备条件,研究了沉积过程中底物温度和生长后退火温度的影响。我们的结果表明,对于室温沉积和随后的900 \ k,获得了最低的表面缺陷密度,例如阶梯边缘以及螺钉和边缘位错。 SP-STM数据揭示了在较低退火温度下的小型磁性域,这显然是由于固定晶界和其他晶体缺陷引起的。系统地研究了最佳制备的GD膜的覆盖依赖性磁性域结构。对于低于大约80个原子层(AL)的低覆盖范围,我们观察到$ $ $ M大小的域,这些域被域墙壁隔开,这些域沿着$ [1 {\ bar 1} 0] $方向的定向。在关键膜的​​厚度上方$θ_ {\ text {crit}} \ ail(100 \ pm 20)$ \,al,我们识别条纹域,指示了从平面内到平面外的旋转重新定向过渡。与现有模型一致,覆盖范围超过$θ_ {\ text {crit}} $,覆盖范围的周期性越远。虽然条纹域的方向在$θ_ {\ text {crit}} $上方的大距离上是均匀的,但我们在$θ\ gtrsim 200 $ \ a al和500 \ ef 500 \ a al a al a al and a al和不规则条纹域中找到了一个特征性的zig-zag模式。磁信号的中间最小值和最大值表示分支结构域的成核。根据对总磁能的各种贡献(例如磁结晶,磁静态和磁弹性能密度)讨论结果。

We present a detailed real-space spin-polarized scanning tunneling microscopy (SP-STM) study of the magnetic domain structure of Gd(0001) films epitaxially grown on W(110). To find optimal preparation conditions, the influence of the substrate temperature during deposition and of the post-growth annealing temperature was investigated. Our results show that the lowest density of surface defects, such as step edges as well as screw and edge dislocations, is obtained for room temperature deposition and subsequent annealing at 900\,K. SP-STM data reveal small-sized magnetic domains at lower annealing temperatures, evidently caused by pinning at grain boundaries and other crystalline defects. The coverage-dependent magnetic domain structure of optimally prepared Gd films was systematically investigated. For low coverage up to about 80 atomic layers (AL) we observe $μ$m-sized domains separated by domain walls which are oriented approximately along the $[1{\bar 1}0]$ direction of the underlying W substrate. Above a critical film thicknesses $Θ_{\text{crit}} \approx (100 \pm 20)$\,AL, we identify stripe domains, indicative for a spin reorientation transition from in-plane to out-of-plane. In agreement with existing models, the periodicity of the stripe domains increases the further the coverage exceeds $Θ_{\text{crit}}$. While the orientation of the stripe domains is homogeneous over large distances just above $Θ_{\text{crit}}$, we find a characteristic zig-zag pattern at $Θ\gtrsim 200$\,AL and irregular stripe domains beyond 500\,AL. Intermediate minima and maxima of the magnetic signal indicate the nucleation of branching domains. The results are discussed in terms of various contributions to the total magnetic energy, such as the magneto-crystalline, the magneto-static, and the magneto-elastic energy density.

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