S. Jena, R. Urkude, W.-Y. Choi, K. K. Pandey, S. Karwal, M. Jung, J. Gardner, B. Ghosh, V. R. Singh
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引用次数: 0
摘要
磁性纳米天幕是一种小型复杂的涡旋状拓扑缺陷,主要存在于锰硅等非中心对称晶体中。它们有可能应用于未来的自旋电子器件。本文利用 X 射线衍射、X 射线光发射光谱、共振光发射光谱(RPES)和扩展 X 射线吸收精细结构(EXAFS)研究了面向 c 蓝宝石衬底的多晶锰硅薄膜中锰原子的结构、电子和磁态。价带光谱显示了薄膜的金属性质。共振光发射光谱研究显示,在 EF 附近存在主要的锰 3d 流动态,在 5.3 至 11.3 eV 之间还存在锰 3d 和硅 3s-3p 混合态。EXAFS 光谱没有显示出系统中存在氧空位,而在非化学计量锰硅薄膜中获得的磁矩是部分巡回态和部分局部态 Mn 3d 的组合。
Electronic structures of skyrmionic polycrystalline MnSi thin film studied by resonance photoemission and x-ray near edge spectroscopy
Magnetic nanometric skyrmions are small complex vortex-like topological defects, mainly found in non-centrosymmetric crystals such as MnSi. They have potential applications for future spintronic devices. In this article, the structural, electronic, and magnetic states of the Mn atoms in a polycrystalline MnSi thin film facing a c-sapphire substrate were studied using x-ray diffraction, x-ray photo-emission spectroscopy, resonance photoemission spectroscopy (RPES), and extended x-ray absorption fine structure (EXAFS). The valence band spectra indicate the metallic nature of the film. The RPES study reveals the presence of major itinerant Mn 3d states near EF and also the mixed Mn 3d and Si 3s–3p states from 5.3 to 11.3 eV. The EXAFS spectrum does not show the existence of oxygen vacancies in the system, and the obtained magnetic moment in the non-stoichiometric MnSi thin film is a combination of the partially itinerant and partially localized Mn 3d states.