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首页> 外文期刊>Journal of Crystal Growth >H-dependent magnetic domain structures in La_(0.67)Sr_(0.33)MnO_3 thin films
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H-dependent magnetic domain structures in La_(0.67)Sr_(0.33)MnO_3 thin films

机译:La_(0.67)Sr_(0.33)MnO_3薄膜中H依赖的磁畴结构

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摘要

Maze- and bubble-like magnetic domain structures have been observed under ambient conditions in La_(0.67)Sr_(0.33)MnO_3 (LSMO) films by magnetic force microscopy (MFM) for films grown on a compressive (LaAlO_3) lattice-mismatched substrate. The substrate-induced stress in this soft magnetic material appears to be a necessary but not sufficient condition for the appearance of these structures, i.e. no magnetic structure has been seen for other films grown under similar conditions on the same substrate with similar distortions to the unit cell. In this study, in order to understand the stability of these structures, we have examined two films grown at 750℃ and three films grown at 800℃ by pulsed-laser deposition by scanning tunneling and magnetic force microscopy to obtain microstructure and domain structures as a function of in-plane magnetic field strength. The latter films consisted of pitted coalesced layers with some surface 3D growth. Although the films were nominally grown under the same conditions, there were subtle differences in the domain structure, wall spacing, the latter due in part to differences in film thickness, and response to an applied in-plane magnetic field. As the field was increased, the maze-like structures became stripe domains with reduced out-of-plane magnetization and decreased wall spacing, consistent with parallel rather than antiparallel alignment of in-plane spin polarization. After removal of the field, the stripe domains remained but the wall spacing and z polarization component returned to the original value. For one 800℃ film the field required for changes in and disappearance of the domains paralleled the slope in the field-dependent magnetization. In contrast, the magnetic structure for one film with a thin insulating cap layer was reversible, suggesting that the walls were pinned by the cap.
机译:在La_(0.67)Sr_(0.33)MnO_3(LSMO)膜中,通过磁力显微镜(MFM)在压缩(LaAlO_3)晶格不匹配的基板上生长的膜在环境条件下已观察到迷宫状和气泡状的磁畴结构。对于这些结构的出现,这种软磁性材料中的基板感应应力似乎是必要的但不是充分的条件,即,对于在相同条件下在同一基板上生长且具有与单元相似的变形的其他薄膜,没有看到磁性结构细胞。在这项研究中,为了了解这些结构的稳定性,我们通过扫描隧道和磁力显微镜通过脉冲激光沉积研究了两片在750℃下生长的膜和三片在800℃下生长的膜,从而获得了微结构和畴结构。平面磁场强度的函数。后面的膜由具有一些表面3D生长的凹坑聚结层组成。尽管薄膜是在相同条件下正常生长的,但在畴结构,壁间距方面存在细微的差异,后者的部分原因是薄膜厚度的差异以及对施加的面内磁场的响应。随着磁场的增加,迷宫般的结构变成条带区域,具有减少的面外磁化强度和减小的壁间距,这与面内自旋极化的平行而不是反平行排列一致。在去除场之后,条纹区域保留,但是壁间距和z极化分量返回到原始值。对于一部800℃的胶片,畴的变化和消失所需的场与场相关磁化强度的斜率平行。相比之下,一层带有薄绝缘帽层的薄膜的磁性结构是可逆的,表明壁被帽钉住了。

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