论文标题

卷曲磁涡旋中卷发模式的时域成像和微磁性研究,探索了核心发出的螺旋旋波的作用

Time-domain imaging of curling modes in a confined magnetic vortex and a micromagnetic study exploring the role of spiral spin waves emitted by the core

论文作者

Ruiz, D. Osuna, Keatley, P. S., Childress, J. R., Katine, J. A., Hicken, R. J., Hibbins, A. P., Ogrin, F. Y.

论文摘要

使用时间分辨扫描KERR显微镜直接对限制在微观盘的铁磁涡流的卷发自旋波模式直接成像。微磁模拟已用于探索旋转涡流核心动力学与在循环内磁化区域中观察到的卷发模式的相互作用。如我们在光谱和测量图像中所观察到的那样,以前已经报道了基本的旋转模式与脱生,最低的方位模式的杂交,方位角模式。模式的卷发性质可以归因于整个圆盘厚度的静态和动态磁化的不对称性,但是在这里我们还提供了证据表明,核心发出的螺旋旋转波可以影响较高频率卷曲模式的空间特征,仅杂交仅以同一含义的旋转含义的杂型模式允许,同一含量具有同一含义的静脉运动。虽然确定在密闭盘中是否真的与模式分散杂交这类模式是一个挑战,但我们的模拟表明,来自核心的螺旋旋转波可以充当核心动力学和方位角模式之间相互作用的介体。在较高的频率下,具有径向特征的模式仅表现出明显的卷发,而是显示出与圆盘边缘产生的自旋波的相互作用的证据。观察到的卷曲模式的测得的时空特性由我们的模拟准确地重现,该模拟揭示了从圆盘的核心和边缘区域发射传播短波长的螺旋波。我们的模拟表明,传播模式不是无关紧要的,但可能在杂交核心模式和面内磁性区域所需的动态重叠中起作用。

The curling spin wave modes of a ferromagnetic vortex confined to a microscale disc have been directly imaged in response to a microwave field excitation using time-resolved scanning Kerr microscopy. Micromagnetic simulations have been used to explore the interaction of gyrotropic vortex core dynamics with the curling modes observed in the region of circulating in-plane magnetization. Hybridization of the fundamental gyrotropic mode with the degenerate, lowest-frequency, azimuthal modes has previously been reported to lead to their splitting and counter propagating motion, as we observe in our spectra and measured images. The curling nature of the modes can be ascribed to asymmetry in the static and dynamic magnetization across the disc thickness, but here we also present evidence that spiral spin waves emitted by the core can influence the spatial character of higher frequency curling modes for which hybridization is only permitted with gyrotropic modes of the same sense of azimuthal motion. While it is challenging to identify if such modes are truly hybridized from the mode dispersion in a confined disc, our simulations reveal that spiral spin waves from the core may act as mediators of the interaction between the core dynamics and azimuthal modes. At higher frequency, modes with radial character only do not exhibit marked curling, but instead show evidence of interaction with spin waves generated at the edge of the disc. The measured spatio-temporal character of the observed curling modes is accurately reproduced by our simulations, which reveal the emission of propagating short-wavelength spiral spin waves from both core and edge regions of the disc. Our simulations suggest that the propagating modes are not inconsequential, but may play a role in the dynamic overlap required for hybridization of modes of the core and in-plane magnetised regions.

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