Burgos-Parra E, Bukin N, Sani S, Figueroa A I, Beutier G, Dupraz M, Chung S, Dürrenfeld P, Le Q Tuan, Mohseni S M, Houshang A, Cavill S A, Hicken R J, Åkerman J, van der Laan G, Ogrin F Y
College of Engineering, Mathematics and Physical sciences, University of Exeter, EX4 4QL, Exeter, United Kingdom.
Department of Materials and Nanophysics, School of Engineering Sciences, KTH Royal Institute of Technology, 164 40, Kista, Sweden.
Sci Rep. 2018 Aug 1;8(1):11533. doi: 10.1038/s41598-018-29856-y.
A dissipative magnetic soliton, or magnetic droplet, is a structure that has been predicted to exist within a thin magnetic layer when non-linearity is balanced by dispersion, and a driving force counteracts the inherent damping of the spin precession. Such a soliton can be formed beneath a nano-contact (NC) that delivers a large spin-polarized current density into a magnetic layer with perpendicular magnetic anisotropy. Although the existence of droplets has been confirmed from electrical measurements and by micromagnetic simulations, only a few attempts have been made to directly observe the magnetic landscape that sustains these structures, and then only for a restricted set of experimental parameter values. In this work we use and x-ray holography technique HERALDO, to image the magnetic structure of the [Co/Ni]x4 multilayer within a NC orthogonal pseudo spin-valve, for different range of magnetic fields and injected electric currents. The magnetic configuration imaged at -33 mA and 0.3 T for devices with 90 nm NC diameter reveals a structure that is within the range of current where the droplet soliton exist based on our electrical measurements and have it is consistent with the expected size of the droplet (∼100 nm diameter) and its spatial position within the sample. We also report the magnetisation configurations observed at lower DC currents in the presence of fields (0-50 mT), where it is expected to observe regimes of the unstable droplet formation.
耗散磁孤子,即磁滴,是一种在薄磁层中当非线性与色散平衡且驱动力抵消自旋进动的固有阻尼时被预测会存在的结构。这样的孤子可以在纳米接触(NC)下方形成,该纳米接触将大的自旋极化电流密度注入到具有垂直磁各向异性的磁层中。尽管已经通过电学测量和微磁模拟证实了磁滴的存在,但只有少数尝试直接观察维持这些结构的磁景观,而且仅针对有限的一组实验参数值。在这项工作中,我们使用X射线全息技术HERALDO,对NC正交伪自旋阀内的[Co/Ni]x4多层膜的磁结构进行成像,该成像针对不同范围的磁场和注入电流。对于直径为90nm的NC器件,在-33mA和0.3T下成像的磁构型揭示了一种结构,基于我们的电学测量,该结构处于磁滴孤子存在的电流范围内,并且其与预期的磁滴尺寸(直径约100nm)及其在样品中的空间位置一致。我们还报告了在存在磁场(0 - 50mT)的情况下在较低直流电流下观察到的磁化构型,预计在该磁场下会观察到不稳定磁滴形成的状态。