Liyanage W L N C, Tang Nan, Dally Rebecca L, Quigley Lizabeth J, Buchanan C Charlotte, Shu Guo-Jiun, Butch Nicholas P, Krycka Kathryn, Bleuel Markus, Borchers Julie A, Debeer-Schmitt Lisa, Gilbert Dustin A
Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA.
Materials Science Department, University of Tennessee, Knoxville, TN 37996, USA.
Nanoscale. 2024 Jun 6;16(22):10715-10726. doi: 10.1039/d4nr00858h.
Magnetic skyrmions are topologically protected, nanoscale whirls of the spin configuration that tend to form hexagonally ordered arrays. As a topologically non-trivial structure, the nucleation and annihilation of the skyrmion, as well as the interaction between skyrmions, varies from conventional magnetic systems. Recent works have suggested that the ordering kinetics in these materials occur over millisecond or longer timescales, which is unusually slow for magnetic dynamics. The current work investigates the skyrmion ordering kinetics, particularly during lattice formation and destruction, using time-resolved small angle neutron scattering (TR-SANS). Evaluating the time-resolved structure and intensity of the neutron diffraction pattern reveals the evolving real-space structure of the skyrmion lattice and the timeframe of the formation. Measurements were performed on three prototypical skyrmion materials: MnSi, (Fe,Co)Si, and CuOSeO. To probe lattice formation and destruction kinetics, the systems were prepared in the stable skyrmion state, and then a square-wave magnetic field modulation was applied. The measurements show that the skyrmions quickly form ordered domains, with a significant distribution in lattice parameters, which then converge to the final structure; the results confirm the slow kinetics, with formation times between 10 ms and 99 ms. Comparisons are made between the measured formation times and the fundamental material properties, suggesting the ordering temperature, saturation magnetization and magnetocrystalline anisotropy may be driving the timeframes. Micromagnetic simulations were also performed and support a scaling of the kinetics with sample volume, a behavior which is caused by the reconciling of misaligned domains.
磁斯格明子是自旋构型的拓扑保护纳米级涡旋,倾向于形成六边形有序阵列。作为一种拓扑非平凡结构,斯格明子的成核和湮灭以及斯格明子之间的相互作用与传统磁系统不同。最近的研究表明,这些材料中的有序动力学发生在毫秒或更长的时间尺度上,这对于磁动力学来说异常缓慢。当前的工作使用时间分辨小角中子散射(TR-SANS)研究斯格明子有序动力学,特别是在晶格形成和破坏过程中。评估中子衍射图案的时间分辨结构和强度揭示了斯格明子晶格不断演变的实空间结构以及形成的时间框架。对三种典型的斯格明子材料进行了测量:MnSi、(Fe,Co)Si和CuOSeO。为了探测晶格形成和破坏动力学,将系统制备成稳定的斯格明子状态,然后施加方波磁场调制。测量结果表明,斯格明子迅速形成有序畴,晶格参数存在显著分布,然后收敛到最终结构;结果证实了动力学缓慢,形成时间在10毫秒至99毫秒之间。对测量的形成时间与基本材料特性进行了比较,表明有序温度、饱和磁化强度和磁晶各向异性可能是驱动时间框架的因素。还进行了微磁模拟,支持动力学与样品体积的标度关系,这种行为是由未对准畴的协调引起的。