论文标题

阳离子和晶格位点选择性磁性深度曲线$ \ mathrm {fe_3o_4} $(001)胶片

Cation- and lattice-site-selective magnetic depth profiles of ultrathin $\mathrm{Fe_3O_4}$(001) films

论文作者

Pohlmann, Tobias, Kuschel, Timo, Rodewald, Jari, Thien, Jannis, Ruwisch, Kevin, Bertram, Florian, Weschke, Eugen, Shafer, Padraic, Wollschläger, Joachim, Kuepper, Karsten

论文摘要

对超薄膜表面特性的详细理解对于正确解释光谱,催化和自旋传输数据至关重要。我们在Ultrathin $ \ Mathrm {Fe_3o_4} $膜上介绍X射线磁圆二色症(XMCD)和X射线谐振磁反射率(XRMR)测量,以获取与不同阳离子物种$ \ Mathrm $ \ Mathrm {fe^fe^^2+{2+{2++{2+{2+{2+{2+{2+{2+{2+{2+{2 $ \ mathrm {fe^{3+} _ {tet}} $和$ \ mathrm {fe^{3+} _ {oct}} $,位于$ \ mathrm {fe_3o_4} $ $ \ mathrm {fe_3o_4} $的八面体和四面体位点上。通过使用多重计算分析$ \ mathrm {Fe_3O_4} $的XMCD光谱,可以隔离每个阳离子物种的共振能。在这三个谐振能量上执行XRMR产生的磁深度曲线,这些磁深度曲线与一个特定的阳离子物种相对应。两种$ \ mathrm {fe^{3+}} $ cations的深度曲线显示出$ \ mathrm {3.9 \ pm 1〜Å} $ - 增强磁化强度的厚表面层,这可能是由于这些离子的过量而造成的,以$ \ \ \ mathrm {fe^^{2+} $} $ {coct} $ {oct} $ {Oct}磁性增强的$ \ mathrm {fe^{3+} _ {tet}} $ layer在$ \ mathrm {3 \ pm 1.5〜Å} $远离$ \ m马理} $远比$ \ mathrm {fe^{3+} _ {3+} _ {oct} _ $ layer上移动。

A detailed understanding of ultrathin film surface properties is crucial for the proper interpretation of spectroscopic, catalytic and spin-transport data. We present x-ray magnetic circular dichroism (XMCD) and x-ray resonant magnetic reflectivity (XRMR) measurements on ultrathin $\mathrm{Fe_3O_4}$ films to obtain magnetic depth profiles for the three resonant energies corresponding to the different cation species $\mathrm{Fe^{2+}_{oct}}$, $\mathrm{Fe^{3+}_{tet}}$ and $\mathrm{Fe^{3+}_{oct}}$ located on octahedral and tetrahedral sites of the inverse spinel structure of $\mathrm{Fe_3O_4}$. By analyzing the XMCD spectrum of $\mathrm{Fe_3O_4}$ using multiplet calculations, the resonance energy of each cation species can be isolated. Performing XRMR on these three resonant energies yields magnetic depth profiles that correspond each to one specific cation species. The depth profiles of both kinds of $\mathrm{Fe^{3+}}$ cations reveal a $\mathrm{3.9 \pm 1~Å}$-thick surface layer of enhanced magnetization, which is likely due to an excess of these ions at the expense of the $\mathrm{Fe^{2+}_{oct}}$ species in the surface region. The magnetically enhanced $\mathrm{Fe^{3+}_{tet}}$ layer is additionally shifted about $\mathrm{3\pm 1.5~Å}$ farther from the surface than the $\mathrm{Fe^{3+}_{oct}}$ layer.

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