Quantum nature of Skyrmions

Quantum nature of Skyrmions

Oleg Janson,1,2 Ioannis Rousochatzakis,3 Alexander A. Tsirlin,1,2 Marilena Belesi3, Andrei A. Leonov,3 Ulrich K. Rößler,3 Jeroen van den Brink,3,4 and Helge Rosner1 

1Max Planck Institute for Chemical Physics of Solids, D-01087 Dresden, Germany. 2National Institute of Chemical Physics and Biophysics, EE-12618 Tallinn, Estonia. 3Leibniz Institute for Solid State and Materials Research, IFW D-01069 Dresden, Germany. 4Department of Physics, TU Dresden, D-01062 Dresden, Germany

Originally, skyrmions were introduced over half a century ago in the context of dense nuclear matter. However, being at first hand mathematical objects — special types of topological solitons — they can emerge in much broader contexts. Recently skyrmions were observed in metallic helimagnets like MnSi and FeGe, forming nanoscale spin-textures. Extending over length scales much larger than the interatomic spacing, they behave as large, classical objects, yet deep inside they are of quantum nature.  As a large surprise came the recent observation of skyrmions in the strongly correlated spin-½ quantum magnet Cu2OSeO3, which, in contrast to MnSi and FeGe, should exhibit few relevant short-range exchange interactions, only. The key aspects of helimagnetism and skyrmion formation in chiral magnetic systems such as Cu2OSeO3, are shown in Fig. 1.

Penetrating into the microscopic roots of helimagnetism and skyrmion formation requires a multi-scale approach (see Fig. 2), spanning the full quantum to classical domain. For the mentioned metallic systems such an approach is presently intractable due to the strong mixing of delocalized low energy electronic and magnetic degrees of freedom. However, since its band gap enforces a natural separation between electronic and magnetic energy scales, we achieve for the first time a complete multi-scale approach in the skyrmionic Mott insulator Cu2OSeO3. We find that its magnetic building blocks are strongly fluctuating Cu4 tetrahedra, spawning a continuum theory that culminates in 51nm large skyrmions, in striking agreement with experiment.

In our approach, we start at the atomic level with density functional (DFT) band structure calculations to estimate the Heisenberg exchange parameters Jij and Dzyaloshinskii-Moriya (DM) interactions. After deriving a tight-binding model as a first step to analyse the relevant orbitals and couplings, DFT+U calculations include the missing electronic correlations in a static mean-field approximation and yield specific values for the coupling parameters. The resulting Jij's are cross-checked for their accuracy by Quantum Monte Carlo (QMC) simulations. The calculated magnetic ordering temperature TC and the T-dependence of magnetization and magnetic susceptibility are in very good agreement with the measurements (see Fig. 3).

The evaluated parameters define a clear separation of energy scales, leading to an effective model (with renormalized interaction parameters) of weakly interacting Cu4 tetrahedra in a spin-1 triplett state. Interestingly, although Cu2OSeO3 exhibits a much complexer crystal structure, the obtained effective so-called trillium-lattice model is strongly reminiscent to the B20 helimagnets MnSi and FeGe. This effective model can be further extended to a mesoscopic scale by a long wavelength approximation, delivering two basic parameters for the exchange stiffness A and the twisting parameter D which control the skyrmion physics in Cu2OSeO3. Based on these parameters A and D, micromagnetic simulations enable a detailed investigation of the magnetic phase diagram.

In summary, our multi-scale approach successfully models the complex skyrmion formation in Cu2OSeO3 on a basis of weakly coupled, strongly fluctuating Cu4 tetrahedra in surprisingly good agreement with the experiments. 

O. Janson, I. Rousochatzakis, A. A. Tsirlin, M. Belesi, A. A. Leonov, U. K. Rößler, J. van den Brink, H. Rosner, The quantum nature of skyrmions and half-skyrmions in Cu2OSeO3. Nature Commun. 5, 1-11  (2014) http://dx.doi.org/10.1038/ncomms6376

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