APS March Meeting 2015
Volume 60, Number 1
Monday–Friday, March 2–6, 2015;
San Antonio, Texas
Session D53: Invited Session: Skyrmions in Thin Magnetic Films
2:30 PM–5:30 PM,
Monday, March 2, 2015
Room: Grand Ballroom C3
Sponsoring
Unit:
GMAG
Chair: Axel Hoffmann, Argonne National Laboratory
Abstract ID: BAPS.2015.MAR.D53.5
Abstract: D53.00005 : Dynamics of Skyrmionic Spin Structures
4:54 PM–5:30 PM
Preview Abstract
Abstract
Author:
Christoforos Moutafis
(Paul Scherrer Institute)
Magnetic skyrmions are topologically protected particle-like spin
structures, with a topology characterised by their Skyrmion number. They can
arise due to various interactions, including exchange, dipolar and
anisotropy energy in the case of bubbles (skyrmion bubbles) and an
additional Dzyaloshinskii-Moriya interaction (DMi) in the case of chiral
skyrmions. Numerical predictions suggest that they exhibit rich dynamical
behaviour governed by their topology, such as the basic gyrotropic and
breathing eigenmodes [1,2]. The dynamical experiments are performed on
skyrmion bubbles in nanostructures from symmetric CoB/Pt multilayers,
tailored for high-frequency dynamics. Asymmetric layers were also fabricated
(Co layers in-between 5d-metals) in order to tune the DMi, as expected from
recent experiments [4]. Stabilizing chiral skyrmions confined in such
nanostructures is highly desirable due to their enhanced stability and
smaller size that makes them ideal candidates for integration in recently
proposed novel spintronics devices [3]. By investigating the size of
magnetic domains in magnetic field cycles, and comparing to micromagnetic
simulations, asymmetric multilayers were explored. By performing pump-probe
dynamical X-ray imaging on confined skyrmion bubbles the first observation
of their basic eigenmode dynamics was demonstrated [5]. In particular, we
present picosecond nanoscale imaging data i) of the gyrotropic mode of a
single skyrmion bubble in the GHz regime and ii) the breathing-like
behaviour of a pair of skyrmionic configurations. The observed dynamics is
used to confirm the skyrmion topology and show the existence of an
unexpectedly large inertia that is key for describing skyrmion dynamics
[1,5]. These results demonstrate new ways for observing skyrmion dynamics
and provide a framework for describing their behaviour. The next step is to
achieve chiral skyrmion dynamics on a DMi system.
\\[4pt]
[1] C. Moutafis, S. Komineas, J. A. C. Bland, Phys. Rev. B 79, 224429
(2009).\\[0pt]
[2] N. Nagaosa, Y. Tokura, Nat. Nanotech. 8, 899--911 (2013).\\[0pt]
[3] A. Fert, V. Cros, J. Sampaio, Nat. Nanotech. 8, 152--156 (2013).\\[0pt]
[4] G. Chen, et al. Nat. Comms. \textbf{4}, (2013).\\[0pt]
[5] F. Buettner, C. Moutafis, et al., submitted, Nat. Physics (2014).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2015.MAR.D53.5