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. 2017 Sep 29;3(9):e1701704.
doi: 10.1126/sciadv.1701704. eCollection 2017 Sep.

Entropy-limited topological protection of skyrmions

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Entropy-limited topological protection of skyrmions

Johannes Wild et al. Sci Adv. .

Abstract

Magnetic skyrmions are topologically protected whirls that decay through singular magnetic configurations known as Bloch points. We used Lorentz transmission electron microscopy to infer the energetics associated with the topological decay of magnetic skyrmions far from equilibrium in the chiral magnet Fe1-x Co x Si. We observed that the lifetime τ of the skyrmions depends exponentially on temperature, [Formula: see text]. The prefactor τ0 of this Arrhenius law changes by more than 30 orders of magnitude for small changes of the magnetic field, reflecting a substantial reduction of the lifetime of skyrmions by entropic effects and, thus, an extreme case of enthalpy-entropy compensation. Such compensation effects, being well known across many different scientific disciplines, affect topological transitions and, thus, topological protection on an unprecedented level.

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Figures

Fig. 1
Fig. 1. Magnetic phases and skyrmion decay in Fe1-xCoxSi.
(A) Magnetic phase diagram of Fe1−xCoxSi with x = 0.5 obtained by first cooling the system at a fixed magnetic field, B ≈ 23 mT, and then raising or lowering the field at fixed temperature T. The decrease in the applied field triggers the decay into a helical configuration, whereas either a conical or ferromagnetic state is reached for an increase of the field. (B) Typical LTEM images of helical and skyrmion lattice order, respectively. (C) Schematic image of an early state of the decay of the skyrmion lattice toward a ferromagnetic state. The skyrmion splits by the formation of a pair of Bloch points located at the end of the skyrmion strings, which move toward the surface. (D) Decay of skyrmion lattice order toward the helical state. Neighboring skyrmions merge, and a Bloch point at the merging points moves toward the surface.
Fig. 2
Fig. 2. Key characteristics of the decay of skyrmions into a helical order.
The sample was field-cooled (FC) from above the helical transition temperature (Tc ≈ 38 K) under an applied magnetic field B = 23 mT down to Tm, where the field was reduced to Bm and data recorded as a function of time t. (A to C) Typical LTEM patterns at Tm = 16.7 K after reaching Bm = −2.6 mT for t = 0.1 , 4.8, and 20.2 s, respectively. (D) Evolution of the intensity across the white box marked in (A), (B), and (C) as a function of time (vertical axis). (E) Typical time dependence of the number of skyrmions for Tm = 20.4 K and Bm = −2.6 mT. The blue curve represents an exponential fit.
Fig. 3
Fig. 3. Key characteristics of the decay of skyrmions for increasing magnetic fields.
The sample was field-cooled (FC) from above the helical transition temperature (Tc ≈ 38 K) under an applied magnetic field B = 23 mT down to Tm, where the field was increased to Bm and the data were recorded as a function of time t. (A to C) Typical LTEM patterns at Tm = 18.5 K after reaching Bm = 57 mT, for t = 6.8, 23.6, and 56.0 s, respectively. (D) Evolution of the intensity across the white box marked in (A), (B), and (C) as a function time (vertical axis). (E) Typical time dependence of the number of skyrmions for Tm = 20.4 K and Bm = 57 mT, fitted by an exponential (green line). (F) Time dependence of the intensity within the red dashed circle in (A), (B), and (C). For a small number of skyrmions, a two-step decay via an intermediate state with lower intensity is observed. (G) Statistics of the intermediate-state intensities.
Fig. 4
Fig. 4. Key characteristics of the decay rates of supercooled skyrmions in Fe1−xCoxSi (x = 0.5).
(A) Typical decay times τ after field cooling at B = 23 mT, followed by a decrease/increase to Bm. (B and C) Decay time τ as a function of thermal energy for increasing and decreasing magnetic fields, respectively, and various values of Bm. (D) Attempt time τ0 as a function of energy barrier ΔE inferred from the exponential time dependence of the skyrmion decay. The variation of more than 30 orders of magnitude of τ0 reflects the extreme enthalpy-entropy compensation.

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