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首页> 外文期刊>Journal of Physics Communications >Collective magnetic skyrmion gyrotropic modes in a dot chain
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Collective magnetic skyrmion gyrotropic modes in a dot chain

机译:点链中的集体磁sky旋回旋模

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We investigate the collective gyrotropic modes in a linear chain of ferromagnetic nanodots in a skyrmion magnetization state. Individual skyrmions in the dots (with thickness about of 1 nm and radius about of 100 nm) are assumed to be stabilized by interplay of isotropic exchange and Dzyaloshinskii-Moriya exchange interactions, magnetic anisotropy and magnetostatic interactions. We consider the dipolar and quadrupolar interactions between moving skyrmions in the dots as prevailing mechanism responsible for dynamic interdot magnetostatic coupling. The frequency dispersion relations of the collective skyrmion gyrotropic excitations are calculated for Bloch and Neel skyrmion configurations and related differences in the frequencies are discussed. The accounting of magnetostatic interactions between the skyrmions removes phase degeneracy of the gyrotropic frequency existing for isolated skyrmions and allows distinguishing the Bloch and Neel skyrmionic configurations by their dynamic response. The interdot magnetostatic coupling and frequency bandwidth are maximal for the large-radius Bloch skyrmions in the relatively thick dots.
机译:我们研究了在Skyrmion磁化状态下铁磁性纳米点线性链中的集体回旋模式。假定各向同性交换和Dzyaloshinskii-Moriya交换相互作用,磁各向异性和静磁相互作用之间相互作用,从而使点中的单个Skyrmion(厚度约为1 nm,半径约为100 nm)稳定。我们将点中移动的天体之间的偶极和四极相互作用视为负责动态点间静磁耦合的主要机制。计算了Bloch和Neel skyrmion构型的集体skyrmion回旋激励的频率色散关系,并讨论了频率的相关差异。对天体离子之间的静磁相互作用的计算消除了孤立天体离子存在的回旋频率的相位简并性,并允许通过它们的动态响应来区分布洛赫和尼尔天体离子构型。点内静磁耦合和频率带宽对于相对较厚的点中的大半径布洛赫天空粒子最大。

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