4.8 Article

Trochoidal motion and pair generation in skyrmion and antiskyrmion dynamics under spin-orbit torques

Journal

NATURE ELECTRONICS
Volume 1, Issue 8, Pages 451-457

Publisher

NATURE PORTFOLIO
DOI: 10.1038/s41928-018-0114-0

Keywords

-

Funding

  1. European Commission [665095]
  2. Deutscher Akademischer Austauschdienst [57314019]
  3. Deutsche Forschungsgemeinschaft [RI2891/1-1, DU1489/2-1]
  4. Alexander von Humboldt Foundation
  5. Graduate School of Excellence Materials Science in Mainz (MAINZ)
  6. ERC Synergy Grant SC2 [610115]
  7. Transregional Collaborative Research Center (SFB/TRR) [173 SPIN+X]
  8. Grant Agency of the Czech Republic [14-37427G]

Ask authors/readers for more resources

Magnetic skyrmions are swirling magnetic spin structures that could be used to build next-generation memory and logic devices. They can be characterized by a topological charge that describes how the spin winds around the core. The dynamics of skyrmions and antiskyrmions, which have opposite topological charges, are typically described by assuming a rigid core. However, this reduces the set of variables that describe skyrmion motion. Here we theoretically explore the dynamics of skyrmions and antiskyrmions in ultrathin ferromagnetic films and show that current-induced spin-orbit torques can lead to trochoidal motion and skyrmion-antiskyrmion pair generation, which occurs only for either the skyrmion or antiskyrmion, depending on the symmetry of the underlying Dzyaloshinskii-Moriya interaction. Such dynamics are induced by core deformations, leading to a time-dependent helicity that governs the motion of the skyrmion and antiskyrmion core. We compute the dynamical phase diagram through a combination of atomistic spin simulations, reduced-variable modelling and machine learning algorithms. It predicts how spin-orbit torques can control the type of motion and the possibility to generate skyrmion lattices by antiskyrmion seeding.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.8
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available