Introduction

Skyrmions were introduced into science by T.H.R. Skyrme who has put forward a non-linear meson model in which baryons, such as protons and neutrons, emerge as topological solitons.1 Importantly, he identified the baryon number with the topological charge of configurations of the meson field. The Skyrme model was applied to describe physical properties of baryons and atomic nuclei,2 as well as creation and annihilation of baryons assisted by monopoles.3 Related topological objects have been discovered in many branches of science, including condensed matter physics.4,5,6,7 The recent observation of magnetic skyrmions,8,9 which are topologically protected nanoscale spin textures, initiated a new rapidly expanding field of research, called skyrmionics. This field is driven by the exploration of new skyrmion materials and novel transport phenomena—quantum manisfestations of the non-trivial skyrmion topology—as well as by the potential of magnetic skyrmions to revolutionize information technologies. The use of skyrmions as information bits holds promise of fast, energy-efficient and high-density magnetic memory devices.10,11,12,13,14

In bulk cubic helimagnets, where magnetic skyrmions were first spotted,8 skyrmion lattices (SkLs) appear spontaneously in a small pocket of the temperature–magnetic field phase diagram, the so-called A-phase, just below the transition temperature TC. Their stability is attributed to the competition between the ferromagnetic exchange, the Dzyaloshinskii–Moriya (DM) and Zeeman interactions in combination with additional small terms,15 such as thermal fluctuations,8,16 dipolar interactions and the softening of the magnetization modulus.17,18 As the free energy imbalance between the skyrmion lattice phase and its main competitor, the conical state, is small, the boundaries of the A-phase can be changed substantially by applying pressure,19 electric fields,13,20,21,22 chemical doping,23 or uniaxial strains.24,25 On the other hand, theoretical models that are based on the Dzyaloshinskii approach26,27 and include magnetic stiffness or anisotropy, predict SkLs to occur in bulk cubic helimagnets over a wide range of magnetic fields and temperatures below TC.15,28,29,30,31,32

Experimental efforts to find anisotropy-stabilized low-temperature SkLs in bulk cubic helimagnets have been largely overshadowed by the search for SkLs and isolated skyrmions in thin films,9,14,33 where the main stabilization mechanism is the chiral surface twists.34,35,36 Nevertheless, the importance of anisotropy in stabilizing states is underscored by the recent discovery of the tilted spiral state in Cu2OSeO337,38 resulting from the competition between the anisotropic exchange and the cubic anisotropy, which is very strong in that material due to the quantum nature of spins of its magnetic building blocks.37,39 Furthermore, similar mechanisms possibly stabilize the low-temperature skyrmion lattice reported in the same material.38

In the following, we present an experimental and theoretical study of skyrmionic states in the chiral magnetic insulator Cu2OSeO3 and discuss the stabilization and nucleation mechanisms thereof. Small angle neutron scattering (SANS) measurements were performed by carefully applying the magnetic field along the three major crystallographic directions, either after zero-field cooling (ZFC) or after fast-field cooling (FFC) through the A-phase.40,41,42,43,44 In this way, extremely robust low-temperature skyrmionic states can be induced for all field directions and over large areas of the phase diagram, stabilized by competing cubic and exchange anisotropies. In particular, when the magnetic field is applied along the cubic axes, triangular arrays of skyrmions are energetically more favorable than both the tilted spiral and conical states near the borderline between modulated and uniform magnetic phases. Our theoretical approach shows that the spatial orientation of the skyrmion lattice is, in low magnetic fields, determined by magnetic anisotropies and not necessarily orthogonal to the applied field. Although emerging and disappearing spiral states near critical magnetic fields act as catalyzers for topological charge changing processes, skyrmions are surprisingly resilient to high magnetic fields: the memory of skyrmionic states persists, possibly in the form of isolated skyrmions or torons, in the field polarized state, even when the skyrmion lattice signal has disappeared. Our findings highlight the paramount role of the strong interplay between the competing magnetic anisotropies resulting from the quantum nature of spin in Cu2OSeO337,39 in stabilizing skyrmionic states, which opens new routes for the manipulation of skyrmions in spintronic devices.

Results

Figure 1 schematically illustrates our measurement protocols as well as the boundaries of the phases generic to cubic helimagnets. For the FFC measurements the sample was cooled to the temperature of interest with an average cooling rate of 10 K/s and under a magnetic field of μ0H = 14 mT. The ZFC measurements were performed by cooling the sample from TTC to the temperature of interest at zero magnetic field following the protocols schematically illustrated in Fig. S6 of the Supplementary Information. The measurements were performed with the magnetic field either perpendicular or parallel to the incident neutron beam wavevector ki. In the following we will focus on the results obtained in the latter configuration, which is the one probing skyrmionic correlations. Representative results for Hki are provided in the Figures S13S15.

Fig. 1
figure 1

Schematic representation of the fast field cooled (FFC) experimental procedure. The sample was (1) first field cooled under a magnetic field of μ0H = 14 mT to the temperature of interest with an average cooling rate of 10 K/s. Subsequently, (2) measurements were performed by stepwise increasing the magnetic field to μ0H = 90 mT, well above the μ0HC2 line. Next, (3) measurements were performed by stepwise decreasing the magnetic field to μ0H = 0 mT. In an additional step, the sample was brought to TTC, (4) field cooled again under μ0H = 14 mT and (5) measurements were performed by stepwise decreasing the field to μ0H = 0 mT. This figure also indicates the boundaries of the helimagnetic phases generic to cubic helimagnets: the Helical phase (H) for μ0H < μ0HC1, the Conical phase (C) for μ0HC1 < μ0H < μ0HC2, the field polarized state (FP) for μ0H > μ0HC2 and the A-phase (A) close to TC

Figure 2 shows a representative set of SANS patterns at T = 3 K after FFC, for H||[111]. A ring of scattering appears at μ0H = 14 mT, which evolves with increasing magnetic field into a weak pattern with the six-fold symmetry characteristic of SkL scattering.8 By further increasing the magnetic field, this scattering weakens and persists up to the μ0HC2 transition line. At higher magnetic fields, the scattering vanishes, implying that the SkLs have dissolved. Surprisingly, when the magnetic field is subsequently decreased from μ0H = 90 to 0 mT, the scattering patterns with six-fold symmetry reappear for 65 mT > μ0H > 7 mT. This is a remarkable result because it implies that a memory of the SkL phase persists at magnetic fields high enough to suppress not only the SkL scattering but also any spiral modulations. Additional measurements indicate that the SkL scattering reappears even after applying a field of 200 mT, i.e. more than twice as large as μ0HC2. Thus, the memory of skyrmionic correlations is extremely robust and can only be erased by (relatively) high magnetic fields. This result is even more remarkable if one considers that these robust skyrmions are metastable, as they were induced by the FFC procedure. Indeed, this scattering disappears once the field has been reduced to zero, and it is not observed by FFC under magnetic fields exceeding the lower and upper boundaries of the A-phase (Fig. S4) or when the sample is field cooled at a much slower cooling rate of 10 K/min, or zero-field cooled (Fig. 2). Skyrmions may survive due to magnetic field inhomogeneities produced by stray fields, in particular near the sample edges, or in the form of magnetic defects such as torons.18,45,46,47

Fig. 2
figure 2

SANS patterns recorded at T = 3 K and with the magnetic field applied along the [111] crystallographic direction. The magnetic field was applied parallel to the incoming neutron beam (H||ki) following the fast field cooled (FFC) and zero field cooled protocols. The arrows and numbers below the SANS patterns indicate the step of the FFC protocol, as defined in Fig. 1, for which the measurements were performed

A similar behavior is found for H||[110], as evidenced by the SANS patterns shown in Fig. 3. After FFC at μ0H = 14 mT, the scattering pattern mainly consists of two helical peaks along the [001] direction—a metastable spiral domain with the wave vector perpendicular to the field. This scattering is superimposed on a very weak additional signal, which evolves to a clear SkL pattern at μ0H = 35 mT, i.e. a field where the helical peaks have almost completely disappeared. With increasing magnetic field, the SkL scattering weakens and finally disappears at μ0H = 85 mT. When the magnetic field is subsequently decreased from μ0H = 90 to 0 mT, the SkL scattering reappears around 50 mT, albeit with a much lower intensity and within a smaller magnetic field interval than for H||[111] (Fig. S3).

Fig. 3
figure 3

SANS patterns recorded at T = 3 K and with the magnetic field applied along the [110] crystallographic direction.The magnetic field was applied parallel to the incoming neutron beam (H||ki) following the fast field cooled (FFC) and zero field cooled protocols. The arrows and numbers below the SANS patterns indicate the step of the FFC protocol, as defined in Fig. 1, for which the measurements were performed

The most intriguing behavior is found for H||[001], the field direction for which the tilted conical phase appears close to μ0HC2.37 After FFC, the SANS pattern at 14 mT, shown in Fig. 4, reveals four Bragg peaks originating from the metastable spiral domains along [001] and [010] that are in the scattering plane. In addition, an intense ring of scattering with radius \(\tau = 2\pi /\ell\) is visible, \(\ell\) being the pitch of a helical modulation. One can distinguish 12 peaks originating from two SkL domains oriented along [001] and [010], as is also the case in the A-phase.48 With increasing magnetic field, the helical peaks fade away, whereas the ring of scattering gains intensity, broadens and its radius decreases considerably. This ring-like scattering is due to skyrmionic correlations because it is concentrated on the plane perpendicular to the field as evidenced by the SANS patterns for Hki shown in Fig. S15. The ring disappears above μ0H ≈ 70 mT and when it reappears by decreasing the magnetic field from 90 to 0 mT, its broadening is even more pronounced. This ring is also seen in the ZFC patterns although the intensity is much lower after ZFC than after FFC (see also Figs. S4 and S5). However, the radius and widths of the rings after FFC and ZFC are the same, which implies that they have the same origin. We thus conclude, that these rings arise from thermodynamically stable skyrmionic correlations which coexist with the conical and tilted spiral phases.

Fig. 4
figure 4

SANS patterns recorded at T = 3 K and with the magnetic field applied along the [001] crystallographic direction. The magnetic field was applied parallel to the incoming neutron beam (H||ki) following the fast field cooled (FFC) and zero field cooled protocols. The arrows and numbers below the SANS patterns indicate the step of the FFC protocol, as defined in Fig. 1, for which the measurements were performed

The experimental results are summarized in Figs. 5 and 6, which show contour plots of the total scattering recorded after FFC (steps (2) and (5) in Fig. 1) and ZFC (steps (2) and (3) in Fig. S6), respectively. The intensity has been obtained by excluding the helical and conical peaks, as explained in the Supplementary Information, and corresponds to the total scattering that can be attributed to skyrmionic correlations. This scattering appears over large areas, the extent of which strongly depends on the specific orientation of the magnetic field with respect to the crystallographic lattice. Remarkably, after FFC the skyrmionic scattering appears around the HC1 line for H||[111] and H||[110], whereas for H||[001] it spreads from below HC1 to above HC2. We note that this metastable skyrmionic scattering is reproducible and does not decay within the time scale of our SANS experiments.

Fig. 5
figure 5

Phase diagrams indicating the extent and intensity of skyrmionic scattering after FFC through the A-phase. Contour plots of the total neutron scattering outside the helical peaks measured following steps 2 and 5 of Fig. 1. The magnetic field was applied parallel to the incoming neutron beam (H||ki) and along the a [111], b [110], and c [001] crystallographic directions and averaged using the masks shown in Fig. S1 of the Supplementary Information. The lower (μ0HC1,(l)) and upper (μ0HC1,(h)) helical-to-conical, conical-to-field polarized (μ0HC2) transition lines, as well as the boundaries of the A-phase just below TC have been derived from susceptibility measurements.37 The letters A, H, C, TS, and FP denote the A-phase, helical, conical, tilted spiral, and field polarized phases, respectively

Fig. 6
figure 6

Phase diagrams indicating the extent and intensity of skyrmionic scattering after zero field cooling (ZFC) for H||ki ||[001]. The measurements were performed upon increasing the magnetic field, step (2) in Fig. S6 (panels a and c) and decreasing the magnetic field, step (3) in Fig. S6 (panels b and d). The contour plots of panels a and b use a logarithmic color scale, whereas those of panels c and d a linear one

The low-temperature skyrmionic scattering seen after ZFC for H||[001] shows a clear hysteretic behavior, appearing around the HC2 line when the magnetic field increases from zero to above HC2 (step (2) in Fig. S6), and around the HC1 line when the magnetic field subsequently decreases from above HC2 to zero (step (3) in Fig. S6). These results provide hints to the underlying skyrmion nucleation and stabilization mechanisms discussed below.

The high quality of our neutron scattering data also provides new insights on the low-temperature skyrmionic correlations observed after ZFC for H||[001]. As revealed by the logarithmic scale of Fig. 6a, b, this low-temperature skyrmionic scattering is not confined to pockets, as previously suggested,38 but extends up to the A-phase. Remarkably, the hysteretic behavior sets in at temperatures just below the A-phase, with one branch following the HC1 line over the whole phase diagram and the other one reaching the HC2 line at low temperatures.

Discussion

In order to understand the large differences between the contour plots shown in Figs. 5 and 6, as well as the underlying skyrmion nucleation and stabilization mechanisms, we consider the Dzyaloshinskii model of cubic non-centrosymmetric ferromagnets.26,27,49 This model includes the ferromagnetic exchange, DM, and Zeeman interaction energies, i.e. the principal interactions essential to stabilize modulated states:

$$w = \left( {{\mathbf{grad}}\,{\mathbf{m}}} \right)^2 + {\mathbf{m}} \cdot {\mathrm{rot}}{\mathbf{m}} - \mu_0M{\mathbf{m}} \cdot {\mathrm{h}}.$$
(1)

Here, distances are measured in units of \({\mathbf{x}} = {\mathbf{r}}/\ell\) and energy is measured in units of D2/A, A and D being the exchange stiffness and Dzyaloshinskii constants, respectively. m is the unit vector in the direction of the magnetization, M = mM, and h = HA/D2.

While for low-symmetry classes, such as Cnv50 and D2d, the DM interaction alone stabilizes SkLs,51 for cubic helimagnets, additional terms are required to lower the energy of the skyrmion lattice with respect to the conical spiral state. We consider anisotropic contributions that include cubic anisotropy with kc > 0 (easy 〈001〉 axes) and exchange anisotropy with bEA < 0 (easy 〈111〉 axes):

$$\begin{array}{*{20}{l}} {w_{\mathrm {a}}} \hfill & = \hfill & {k_{\mathrm {c}}(m_x^2m_y^2 + m_x^2m_z^2 + m_y^2m_z^2)} \hfill \\ {} \hfill & {} \hfill & { + b_{{\mathrm {EA}}}((\partial _xm_x)^2 + (\partial _ym_y)^2 + (\partial _zm_z)^2).} \hfill \end{array}$$
(2)

SkLs that have a lower energy than other modulated states can only be found for H||[001]. This explains why the skyrmionic correlations occur after ZFC only for H||[001] (Fig. 4) and why they are the strongest after FFC (Fig. 5c).

Figure 7a shows the zero-temperature phase diagram in the (kc, h) plane calculated for zero exchange anisotropy, which contains the conical spiral state with the propagation vector q||H||[001] (blue color), the skyrmion lattice phase (pink color) and the field polarized phase (white color). The SkL has the lowest energy for relatively small values of kc 0.04 and is metastable in a much wider region of the phase diagram. The dotted line in Fig. 7a marks the magnetic field at which the energy of the SkL for a given kc becomes equal to the energy of the metastable helical spiral states with the wave vectors along the [100] and [010] directions. One expects that when h becomes higher than this field, metastable spirals rupture forming pairs of merons, each with a topological charge 1/2.52,53 Merons, which may also nucleate at the boundary between the metastable spiral and conical domains, ultimately evolve into skyrmions at higher magnetic fields. Since the SkL phase remains metastable below the dashed line, one expects skyrmionic states to persist for fields lower than h = 0.11, until they undergo an elliptical instability into spiral states,54 which explains the hysteresis effect shown in Fig. 6.

Fig. 7
figure 7

Stable and metastable skyrmion lattice states at zero temperature. a Zero-temperature phase diagrams with the magnetic field applied along [001], where h is the dimensionless field magnitude defined in the text, vs. the cubic anisotropy strength, kc, for zero exchange anisotropy, bEA = 0, (left panel) and vs. bEA, for kc = 0.1 (right panel). b and c Difference between the energy densities of the skyrmion lattice and conical (or helical) spiral states, Δw, plotted as a function of h applied along [111] and [001], respectively, for specific values of the cubic anisotropy. If the magnetic field is applied along [111], Δw is always positive, thus the skyrmion lattice is energetically unfavorable. Δw goes though a minimum, which shifts towards low fields with increasing anisotropy (black dotted line). Moreover, at low fields the helical spiral states have lower energy than the conical phase (solid black line). If the magnetic field is applied along [001], the tendency is quite the opposite and for smaller kc the stability region of the SkL state (Δw < 0) lies within the conical spiral phase. For larger values of kc, this region shifts towards higher fields, and at the upper boundary the SkL undergoes a first-order transition to the field polarized state. The inset shows a sketch of the magnetization rotation in the conical phase in the presence of cubic anisotropy with hard 〈111〉 (red arrows) and easy 〈100〉 (green arrows) axes. d Field dependence of the SkL pitch \(\ell\). The curves, that are in qualitative agreement with the experimental results (Fig. S11), are terminated at the transition to the field polarized state for all considered values of kc. For kc = 0, \(\ell\) diverges at this transition (red line). The upper magnetic field limit for \(\ell\) decreases with increasing kc as lower fields are needed to release isolated skyrmions. The inset shows the three-dimensional polar plot of the conical spiral state energy density as a function of the wave vector direction. The path of the rotating magnetization in the conical phase is imaged by the blue line with blue circles being the minima for the homogeneous state

Above the line separating the SkL from the field polarized state, skyrmions remain stable but the skyrmion lattice disappears because of the repulsion between skyrmions. In this way, it is possible to reconcile the disappearance of the SkL signal upon increasing the field above ~μ0HC2 and its surprising comeback when the field is lowered from a value greatly exceeding μ0HC2. The disappearance of the skyrmion lattice which does not destroy all skyrmions resembles sublimation of a solid. The (meta)stability of isolated skyrmions can be enhanced by stray fields, grain boundaries, and formation of skyrmion bags also considered in the context of chiral liquid crystals.55

Figure 7a shows the effect of exchange anisotropy on the zero temperature phase diagram, which for \(b_{{\mathrm {EA}}} > b_{{\mathrm {EA}}}^ \ast\) transforms the conical spiral state with q||H into the tilted spiral state (dark blue color), in which the wave vector tilts towards one of the nearest four body-diagonal 〈111〉 directions.37 The value of bEA cannot be much larger than \(b_{{\mathrm {EA}}}^ \ast\), because otherwise the tilted spiral state would extend down to zero magnetic field, which is inconsistent with the experimental results. In the b–c–d–e region the tilted spiral state is locally stable but has a higher energy than the SkL phase. We note that neither cubic nor exchange anisotropy stabilizes a square SkL, in agreement with the experimental results.

The SkL is metastable for the [111] and [110] directions explaining the lower FFC scattering intensities and the absence of a ZFC skyrmion signal (Fig. 5a, b). Yet, also for these directions, the SkL scattering is the strongest along the helical-to-conical transition line, which is also the field region where the energy difference between the SkL and spiral states is the smallest (Fig. 7b). In addition, the boundaries between the metastable SkL, helical and conical phases catalyze the appearance of topological charge. Indeed, the nontrivial topology of magnetic skyrmions gives rise to energy barriers hindering their creation and destruction, which makes transitions between topological and non-topological magnetic states different from, e.g. the water–ice transition where both phases are composed of the same building blocks (water molecules).

Furthermore, the intensity of the skyrmion lattice scattering for H||[111] shows a complex temperature dependence: at a constant magnetic field of, e.g. μ0H = 20 mT, the intensity first increases, goes through a maximum at ~30 K, then decreases to a minimum at ~15 K, before increasing again at lower temperatures (see Fig. S7). This complex temperature dependence might be related to different orientations of the metastable skyrmion lattice. Our calculations show that in low magnetic fields the spatial orientation of the metastable skyrmion lattice is determined by magnetic anisotropies and the basis vectors of the skyrmion crystal are not necessarily orthogonal to the applied field. The situation is similar to the temperature dependence of the wave vector of the tilted spiral state: Its deviation from the magnetic field direction decreases with temperature, which can be interpreted as the result of the competition between the temperature-dependent cubic and exchange anisotropies. For dominant cubic anisotropy the skyrmion tubes in the metastable SkL may be normal to the (001) planes, while the relatively large exchange anisotropy may re-orient the tubes along the 〈111〉 directions. The temperature dependence of the SkL intensity along the μ0HC1 line is even more pronounced for H||[110].

In conclusion, extremely robust low-temperature skyrmionic states can be induced for all field directions and over large areas of the phase diagram. These skyrmionic states are stabilized by competing cubic and exchange anisotropies, and are thermodynamically stable when the magnetic field is applied along the [001] axis. The formation and destruction of these skyrmionic states is enhanced by nascent and disappearing spiral states near critical lines which catalyze topological charge changing processes. In particular, at low magnetic fields, the spatial orientation of the skyrmion lattice is determined by magnetic anisotropies and is not necessarily orthogonal to the applied field. On the other hand, these skyrmions are surprisingly resilient to high magnetic fields and their memory persists, possibly in the form of isolated skyrmions or torons, even in the field polarized state. These findings underscore the paramount role of magnetic anisotropies in stabilizing novel skyrmionic states and provide valuable directions to manipulate and tune skyrmions for future applications, possibly with electric fields or strain.

Methods

Cu2OSeO3 has first been synthesized by a reaction of CuO (Alfa Aesar 99.995%) and SeO2 (Alfa Aesar 99.999%) at 300 °C (2 days) and 600 °C (7 days) in evacuated fused silica tubes. Starting from this microcrystalline powder, the 3 × 3 × 4 mm3 Cu2OSeO3 single crystal was grown by a chemical transport reaction in a temperature gradient from 580 °C (source) to 460 °C (sink), and a transport additive concentration of 1 mg/cm3 NH4Cl (23 mg) (Alfa Aesar 99.999%). The sample was the same as the one used in our previous work.37,48 It was glued to an aluminum cylinder with a diameter of 1 mm around which 1 m constantan wire was wound with a total resistance of 30 Ω. The wire was glued with GE low-temperature varnish and was used to generate large heat pulses.

The experiments were performed at the SANS instrument D33 of the Institut Laue-Langevin56 with an incident wavelength of 0.8 nm, a sample-to-detector distance of 12.8 m, and a wave-vector transfer resolution of Δλ/λ = 10%.The sample was placed inside an Oxford Instruments 7 T horizontal-field cryomagnet, the remanent field of which did not exceed some 10−4 T. The constantan heater was connected to an external power supply. Fast cooling was performed by first stabilizing the sample at the temperature of interest. Subsequently, a current of 0.3 A was applied for 1.5 s to the constantan heater, providing sufficiently heat to bring the sample to TTC. Switching off the current resulted in a rapid cooling with an average cooling rate of 10 K/s, as estimated from a comparison of the scattered intensity of the SANS patterns at zero magnetic field (recorded every 0.8 s) with the temperature-dependent evolution of the scattered intensity of the helical Bragg peaks at zero magnetic field. All magnetic fields are corrected for demagnetization effects assuming a demagnetization factor of 1/3. The reader is referred to the Supplementary Information (Figs. S1, S2 and S8S12) for details on the data analysis and treatment.