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Target-skyrmions and skyrmion clusters in nanowires of chiral magnets

机译:手性磁体纳米线中的目标天体离子和天体离子簇

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In bulk non-centrosymmetric magnets the chiral Dzyaloshinskii-Moriya exchange stabilizes tubular skyrmions with a reversed magnetization in their centers. While the double-twist is favorable in the center of a skyrmion, it gives rise to an excess of the energy density at the outskirt. Therefore, magnetic anisotropies are required to make skyrmions more favorable than the conical spiral in bulk materials. Using Monte Carlo simulations, we show that in magnetic nanowires unusual skyrmions with a doubly twisted core and a number of concentric helicoidal undulations (target-skyrmions) are thermodynamically stable even in absence of single-ion anisotropies. Such skyrmions are free of magnetic charges and carry a non-integer skyrmion charge s. This state competes with clusters of s = 1 skyrmions. For very small radii, the target-skyrmion transforms into a skyrmion with s < 1, that resembles the vortex-like state stabilized by surface-induced anisotropies.
机译:在块状非中心对称磁体中,手性Dzyaloshinskii-Moriya交换可稳定管状的天空形粒子,并在其中心具有反向磁化强度。尽管双绞线在天窗的中央比较有利,但会导致郊区的能量密度过大。因此,在散装材料中需要磁各向异性来使天体比圆锥形螺旋更有利。使用蒙特卡洛模拟,我们显示出在磁性纳米线中,即使没有单离子各向异性,具有双绞芯和许多同心螺旋波状起伏的非寻常的Skyrmion在热力学上也是稳定的。这样的天体离子没有磁性电荷并且携带非整数的天体离子电荷s。该状态与s = 1天文离子的簇竞争。对于很小的半径,目标单峰转换为s <1的单峰,类似于表面诱导的各向异性稳定的涡状状态。

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