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首页> 外文期刊>Physical review.B.Condensed matter and materials physics >Hippopede curves for modeling radial spin waves in an azimuthally graded magnonic landscape
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Hippopede curves for modeling radial spin waves in an azimuthally graded magnonic landscape

机译:用于在方位级分级级磁景观中建模径向旋转波的河北曲曲线

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摘要

We propose a mathematical model for describing radially propagating spin waves emitted from the core region in a magnetic patch with n vertices in a magnetic vortex state. The azimuthal anisotropic propagation of surface spin waves (SSWs) into the domain, and confined spin waves (or Winter's magnons) in domain walls, increases the complexity of the magnonic landscape. In order to understand the spin wave propagation in these systems, we first use an approach based on geometrical curves called "hippopedes"; however, it provides no insight into the underlying physics. Analytical models rely on generalized expressions from the dispersion relation of SSWs with an arbitrary angle between magnetization M and wave number k. The derived algebraic expression for the azimuthal dispersion is found to be equivalent to that of the hippopede curves. The fitting curves from the model yield a spin wave wavelength for any given azimuthal direction, number of patch vertices, and excitation frequency, showing a connection with fundamental physics of exchange-dominated surface spin waves. Analytical results show good agreement with micromagnetic simulations and can be easily extrapolated to any n-corner patch geometry.
机译:我们提出了一种数学模型,用于描述从磁性膜中的磁贴片中的磁性区域发射的径向传播旋转波,在磁性涡流状态下。表面旋转波(SSW)进入域中的方位角各向异性传播,并限制域壁中的狭窄的旋转波(或冬季摩尔多斯),增加了千兆景观的复杂性。为了了解这些系统中的自旋波传播,我们首先使用一种基于几何曲线的方法,即名为“河马”;但是,它没有对潜在物理学的洞察力。分析模型依赖于来自SSW的色散关系的广义表达式,在磁化M和波数k之间的任意角度。发现方位角分散的衍生代数表达相当于河北曲线的代数表达。来自模型的拟合曲线产生用于任何给定的方位角的自旋波波长,贴片顶点的数量和激发频率,显示与交换主导的表面自旋波的基本物理学的连接。分析结果显示出与微磁模拟的良好一致性,可以很容易地推断到任何N角贴片几何形状。

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  • 来源
    《Physical review.B.Condensed matter and materials physics》 |2020年第10期|104430.1-104430.7|共7页
  • 作者单位

    Department of Physics and Astronomy University of Exeter Exeter EX4 4QL United Kingdom;

    Department of Physics and Astronomy University of Exeter Exeter EX4 4QL United Kingdom;

    Department of Physics and Astronomy University of Exeter Exeter EX4 4QL United Kingdom;

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