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单轴金属间化合物异质结构中的光致自旋动力学

Photoinduced spin dynamics in a uniaxial intermetallic heterostructure .

作者信息

Ovcharenko Sergei, Gaponov Mikhail, Klimov Alexey, Tiercelin Nicolas, Pernod Philippe, Mishina Elena, Sigov Alexandr, Preobrazhensky Vladimir

机构信息

MIREA - Russian Technological University, Moscow, Russia 119454.

Univ. Lille, CNRS, Centrale Lille, Yncréa ISEN, Univ. Polytechnique Hauts-de-France, UMR 8520 - IEMN, 59000 Lille, France.

出版信息

Sci Rep. 2020 Sep 25;10(1):15785. doi: 10.1038/s41598-020-72740-x.

DOI:10.1038/s41598-020-72740-x
PMID:32978474
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7519156/
Abstract

Intermetallic heterostructures of rare-earth and transition metals exhibit physical properties prospective for various applications. These structures combine giant magnetostriction, controllable magnetic anisotropy, magneto-optical activity and allow spin reorientation transitions (SRT) induced by magnetic field at room temperature. Here, we present the results of a study of spin dynamics induced by ultrafast optical excitation in the heterostructure. The time dependence of the light polarization rotation excited by a pump optical pulse with a duration of 35 fs was measured in the total range of the SRT created by external DC magnetic field. We found hysteretic dependence of the polarization rotation on magnetizing field that is specific for spin dynamics near SRT. Enhancement of the rotation is observed in the critical points of the SRT and near the points of magnetization switch from metastable to stable spin states. In the time-domain, two characteristic delays of 20 ps and 200 ps were found, corresponding to the maximum deviation of the light polarization after excitation. The first is explained by the precession motion of spins out of the plane of the structure. The latter is accounted for the spin in-plane deviation from its initial position and thermal relaxation of the anisotropy.

摘要

稀土金属与过渡金属的金属间异质结构展现出适用于各种应用的物理特性。这些结构兼具巨大磁致伸缩、可控磁各向异性、磁光活性,并允许在室温下由磁场诱导自旋重取向转变(SRT)。在此,我们展示了对该异质结构中由超快光激发诱导的自旋动力学的研究结果。在由外部直流磁场产生的SRT的整个范围内,测量了持续时间为35飞秒的泵浦光脉冲激发的光偏振旋转的时间依赖性。我们发现偏振旋转对磁化场具有磁滞依赖性,这是SRT附近自旋动力学的特性。在SRT的临界点以及从亚稳态自旋态到稳定自旋态的磁化切换点附近观察到旋转增强。在时域中,发现了20皮秒和200皮秒的两个特征延迟,对应于激发后光偏振的最大偏差。第一个延迟是由自旋在结构平面外的进动运动所解释。后者则是由于自旋在平面内偏离其初始位置以及各向异性的热弛豫。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/650a/7519156/02cb407afa9e/41598_2020_72740_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/650a/7519156/10eec21b8a74/41598_2020_72740_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/650a/7519156/5730873b061a/41598_2020_72740_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/650a/7519156/02cb407afa9e/41598_2020_72740_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/650a/7519156/10eec21b8a74/41598_2020_72740_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/650a/7519156/5730873b061a/41598_2020_72740_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/650a/7519156/02cb407afa9e/41598_2020_72740_Fig3_HTML.jpg

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