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高无序 Nd₁-xCox 薄膜中通过 EXAFS 测量的 Co 亚网络的大负热膨胀和垂直各向异性。

Large negative thermal expansion of the Co subnetwork measured by EXAFS in highly disordered Nd₁-xCox thin films with perpendicular magnetic anisotropy.

机构信息

Departamento de Física, Facultad de Ciencias, Universidad de Oviedo, Avenida de Calvo Sotelo s/n, Oviedo, E-33007, Spain. Centro de Investigación en Nanomateriales y Nanotecnología (CINN), CSIC-Universidad de Oviedo-Principado de Asturias, E-33428 Llanera, Spain.

出版信息

J Phys Condens Matter. 2013 Oct 23;25(42):426002. doi: 10.1088/0953-8984/25/42/426002. Epub 2013 Sep 25.

DOI:10.1088/0953-8984/25/42/426002
PMID:24067564
Abstract

We have measured a negative thermal expansion (NTE) of the Co subnetwork in amorphous Nd1-xCox (0.78 < x < 0.84) thin films of the order of 1% in volume using linearly polarized EXAFS spectroscopy at RT and 10 K. The expansion, which is anisotropic, is uncorrelated with the perpendicular magnetic anisotropy (PMA) observed in all the films, but correlated with the method used to deposit them. The atomic environments of the Nd atoms resulted in such a strong disorder that Nd-Nd and Nd-Co environments were invisible to EXAFS, and only Co-Co atomic environments were detected. The information on the Nd subnetwork was obtained through its magnetic moment measured by XMCD. These measurements demonstrate an increasing interaction of neodymium atoms with their particular local crystal field as the temperature decreased, suggesting possible structural modifications at their sites. Since the magnetic moment of the cobalt subnetwork remains essentially constant with the temperature, it is proposed that its detected NTE may be caused by the mechanical response of the amorphous network to structural transformations at the Nd sites. These results support that the PMA in RE-TM alloys is localized at the RE sites. The complete absence of EXAFS oscillations in the Nd L3 EXAFS spectra is remarkable: it means that the coherence length of the photoemitted electrons in disordered matter can be strongly reduced from that expected by atomic calculations to the point of being less than first neighbor distances, which is contrary to the common belief that first neighbors are always visible by EXAFS.

摘要

我们使用室温及 10 K 下的线性偏振 EXAFS 光谱测量了非晶态 Nd1-xCox(0.78<x<0.84)薄膜中 Co 子网络的负热膨胀(NTE),其体积膨胀约为 1%。这种各向异性的膨胀与所有薄膜中观察到的垂直磁各向异性(PMA)无关,但与沉积它们的方法有关。Nd 原子的原子环境导致了如此强烈的无序,以至于 Nd-Nd 和 Nd-Co 环境在 EXAFS 中不可见,仅检测到 Co-Co 原子环境。Nd 子网络的信息是通过 XMCD 测量其磁矩获得的。这些测量结果表明,随着温度的降低,Nd 原子与其特定局部晶体场的相互作用增强,表明其位置可能发生结构修饰。由于 Co 子网络的磁矩随温度基本保持不变,因此推测其检测到的 NTE 可能是由非晶网络对 Nd 位结构转变的机械响应引起的。这些结果支持了在 RE-TM 合金中 PMA 定域在 RE 位的观点。Nd L3 EXAFS 光谱中完全没有 EXAFS 振荡这一现象非常显著:这意味着无序物质中光电子的相干长度可以从原子计算所预期的长度大大降低,以至于小于第一近邻距离,这与普遍认为的第一近邻总是可以通过 EXAFS 看到的观点相矛盾。

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