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由铁磁金钴合金和超细钴颗粒组成的纳米复合薄膜中的磁滞现象。

Magnetic Hysteresis in Nanocomposite Films Consisting of a Ferromagnetic AuCo Alloy and Ultrafine Co Particles.

作者信息

Chinni Federico, Spizzo Federico, Montoncello Federico, Mattarello Valentina, Maurizio Chiara, Mattei Giovanni, Bianco Lucia Del

机构信息

Dipartimento di Fisica e Scienze della Terra and CNISM, Università di Ferrara, I-44122 Ferrara, Italy.

Dipartimento di Fisica e Astronomia and CNISM, Università di Padova, I-35131 Padova, Italy.

出版信息

Materials (Basel). 2017 Jun 28;10(7):717. doi: 10.3390/ma10070717.

DOI:10.3390/ma10070717
PMID:28773075
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5551760/
Abstract

One fundamental requirement in the search for novel magnetic materials is the possibility of predicting and controlling their magnetic anisotropy and hence the overall hysteretic behavior. We have studied the magnetism of Au:Co films (~30 nm thick) with concentration ratios of 2:1, 1:1, and 1:2, grown by magnetron sputtering co-deposition on natively oxidized Si substrates. They consist of a AuCo ferromagnetic alloy in which segregated ultrafine Co particles are dispersed (the fractions of Co in the AuCo alloy and of segregated Co increase with decreasing the Au:Co ratio). We have observed an unexpected hysteretic behavior characterized by in-plane anisotropy and crossed branches in the loops measured along the hard magnetization direction. To elucidate this phenomenon, micromagnetic calculations have been performed for a simplified system composed of two exchange-coupled phases: a AuCo matrix surrounding a Co cluster, which represents an aggregate of particles. The hysteretic features are qualitatively well reproduced provided that the two phases have almost orthogonal anisotropy axes. This requirement can be plausibly fulfilled assuming a dominant magnetoelastic character of the anisotropy in both phases. The achieved conclusions expand the fundamental knowledge on nanocomposite magnetic materials, offering general guidelines for tuning the hysteretic properties of future engineered systems.

摘要

寻找新型磁性材料的一个基本要求是能够预测和控制其磁各向异性,进而控制其整体磁滞行为。我们研究了通过磁控溅射共沉积在原生氧化的硅衬底上生长的浓度比为2:1、1:1和1:2的Au:Co薄膜(厚度约为30 nm)的磁性。它们由一种AuCo铁磁合金组成,其中分散着分离的超细Co颗粒(AuCo合金中Co的分数和分离的Co的分数随着Au:Co比的降低而增加)。我们观察到一种意想不到的磁滞行为,其特征是面内各向异性以及在沿硬磁化方向测量的磁滞回线中出现交叉分支。为了阐明这一现象,我们对一个由两个交换耦合相组成的简化系统进行了微磁学计算:围绕Co团簇的AuCo基体,Co团簇代表颗粒的聚集体。如果两个相具有几乎正交的各向异性轴,磁滞特征就能在定性上得到很好再现。假设两个相中各向异性的主要特征是磁弹性,那么这一要求是合理可实现的。所得结论扩展了关于纳米复合磁性材料的基础知识,为调节未来工程系统的磁滞特性提供了一般指导原则。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/b853e17a8dc1/materials-10-00717-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/356b3e54f45b/materials-10-00717-g010.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/ab9aea20eb97/materials-10-00717-g007.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/b853e17a8dc1/materials-10-00717-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/356b3e54f45b/materials-10-00717-g010.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/8034a54d0c42/materials-10-00717-g011.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/4499afb3afac/materials-10-00717-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/9e68b8cc4aaf/materials-10-00717-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/0eae401979d7/materials-10-00717-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/ab9aea20eb97/materials-10-00717-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/eeb2d0d67561/materials-10-00717-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2511/5551760/b853e17a8dc1/materials-10-00717-g009.jpg

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