Please use this identifier to cite or link to this item: http://dx.doi.org/10.25673/116171
Title: Skyrmion motion in magnetic anisotropy gradients : acceleration caused by deformation
Author(s): De Assis, Ismael Ribeiro
Mertig, IngridLook up in the Integrated Authority File of the German National Library
Göbel, BörgeLook up in the Integrated Authority File of the German National Library
Issue Date: 2023
Type: Article
Language: English
Abstract: Magnetic skyrmions are nano-sized topologically nontrivial spin textures that can be moved by external stimuli such as spin currents and internal stimuli such as spatial gradients of a material parameter. Since the total energy of a skyrmion depends linearly on most of these parameters, like the perpendicular magnetic anisotropy, the exchange constant, or the Dzyaloshinskii-Moriya interaction strength, a skyrmion will move uniformly in a weak parameter gradient. In this paper, we show that the linear behavior changes once the gradients are strong enough so that the magnetic profile of a skyrmion is significantly altered throughout the propagation. In that case, the skyrmion experiences acceleration and moves along a curved trajectory. Furthermore, we show that when spin-orbit torques and material parameter gradients trigger a skyrmion motion, it can move on a straight path along the current or gradient direction. We discuss the significance of suppressing the skyrmion Hall effect for spintronic and neuromorphic applications of skyrmions. Lastly, we extend our discussion and compare it to a gradient generated by the Dzyaloshinskii-Moriya interaction.
URI: https://opendata.uni-halle.de//handle/1981185920/118127
http://dx.doi.org/10.25673/116171
Open Access: Open access publication
License: (CC BY 4.0) Creative Commons Attribution 4.0(CC BY 4.0) Creative Commons Attribution 4.0
Journal Title: Physical review
Publisher: Inst.
Publisher Place: Woodbury, NY
Volume: 108
Issue: 14
Original Publication: 10.1103/physrevb.108.144438
Appears in Collections:Open Access Publikationen der MLU

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