• Open Access

Dzyaloshinskii-Moriya domain walls in magnetic nanotubes

Arseni Goussev, J. M. Robbins, Valeriy Slastikov, and Oleg A. Tretiakov
Phys. Rev. B 93, 054418 – Published 22 February 2016
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Abstract

We present an analytic study of domain-wall statics and dynamics in ferromagnetic nanotubes with spin-orbit-induced Dzyaloshinskii-Moriya interaction (DMI). Even at the level of statics, dramatic effects arise from the interplay of space curvature and DMI: the domains become chirally twisted, leading to more compact domain walls. The dynamics of these chiral structures exhibits several interesting features. Under weak applied currents, they propagate without distortion. The dynamical response is further enriched by the application of an external magnetic field: the domain-wall velocity becomes chirality dependent and can be significantly increased by varying the DMI. These characteristics allow for enhanced control of domain-wall motion in nanotubes with DMI, increasing their potential as information carriers in future logic and storage devices.

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  • Received 8 July 2015
  • Revised 14 January 2016

DOI:https://doi.org/10.1103/PhysRevB.93.054418

This article is available under the terms of the Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

©2016 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Arseni Goussev1, J. M. Robbins2, Valeriy Slastikov2, and Oleg A. Tretiakov3,4,*

  • 1Department of Mathematics and Information Sciences, Northumbria University, Newcastle Upon Tyne, NE1 8ST, United Kingdom
  • 2School of Mathematics, University of Bristol, Bristol BS8 1TW, United Kingdom
  • 3Institute for Materials Research, Tohoku University, Sendai 980-8577, Japan
  • 4School of Natural Sciences, Far Eastern Federal University, Vladivostok 690950, Russia

  • *olegt@imr.tohoku.ac.jp

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Issue

Vol. 93, Iss. 5 — 1 February 2016

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