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The evolution of skyrmions in Ir/Fe/Co/Pt multilayers and their topological Hall signature


The topological Hall effect (THE) is the Hall response to an emergent magnetic field, a manifestation of the skyrmion Berry-phase. As the magnitude of THE in magnetic multilayers is an open question, it is imperative to develop comprehensive understanding of skyrmions and other chiral textures, and their electrical fingerprint. Here, using Hall-transport and magnetic-imaging in a technologically viable multilayer film, we show that topological-Hall resistivity scales with the isolated-skyrmion density over a wide range of temperature and magnetic-field, confirming the impact of the skyrmion Berry-phase on electronic transport. While we establish qualitative agreement between the topological-Hall resistivity and the topological-charge density, our quantitative analysis shows much larger topological-Hall resistivity than the prevailing theory predicts for the observed skyrmion density. Our results are fundamental for the skyrmion-THE in multilayers, where interfacial interactions, multiband transport and non-adiabatic effects play an important role, and for skyrmion applications relying on THE.


Skyrmions are topologically protected, two-dimensional (2D), localized hedgehogs and whorls of spin1. Originally invented as a concept in field theory for nuclear interactions2, skyrmions are central to a wide range of phenomena in condensed matter3,4,5. Their realization at room temperature (RT) in magnetic multilayers6,7,8 has generated considerable interest, fueled by technological prospects and the access granted to fundamental questions. The interaction of skyrmions with charge carriers1,8,9,10,11,12 gives rise to exotic electrodynamics, such as the topological Hall effect (THE)13,14. The topological protection of skyrmions results from the quantization of their topological charge (Qsk), which counts the number of times the magnetization unit-vector n(r) covers the unit-sphere. Qsk is determined by Beff(r), the z-component of the emergent magnetic field that corresponds to the Berry phase accumulated by a spin tracking n(r)1,15,16:

$$Q_{{\mathrm{sk}}} = \frac{1}{{4\pi }}{\int} d^2r{\mathbf{n}} \cdot \partial _x{\mathbf{n}} \times \partial _y{\mathbf{n}} \equiv \frac{1}{{{\mathrm{\Phi }}_0}}{\int} d^2rB_{{\mathrm{eff}}}({\mathbf{r}}) = 0, \pm 1, \pm 2, \ldots .$$

Here Φ0 = h/e is the flux quantum, h is Planck’s constant, −e is the electron charge. THE is the Hall response to Beff(r). When charge carriers flow through a conductor with their spins tracking the skyrmion spin texture, the topological-Hall resistivity (ρTH) is1:

$$\rho _{{\mathrm{TH}}} = PR\prime_{\!\!0} n _{\mathrm{T}}{\mathrm{\Phi }}_0,$$

where nT is the 2D density of total topological charge. Here \(R_0{\!\!\prime} \) is an unknown Hall resistivity representing the effective density of charge contributing to THE. \(R_0^\prime \) is usually taken to be R013,17,18,19, the ordinary Hall coefficient, which is extracted from the high field slope of the Hall resistivity (ρyx), and represents the total density of mobile charge. 0 < P < 1 is the spin-polarization of the charge carriers, and Beff(r) is manifested through Φ0. Assuming skyrmions are the sole carriers of topological charge |Qsk| = 1 implies nT = nsk, the density of isolated skyrmions. Thus, within the adiabatic approximation, one expects a straightforward correlation between ρTH and nsk. From the first observations in B20 systems13,14 to the recent multilayers, THE has been used as an indicator for the presence of skyrmions8,17. However, a clear understanding of the effect is still lacking20, especially in technologically viable multilayer films8,18,19, where disorder and interface effects can play an important role7,21,22. In particular, and as we explain below, the THE features in these multilayers are subtle and call for careful analysis of the transport measurements, as we demonstrate in Supplementary Note 3 and Supplementary Note 4. In contrast, the situation in some B20 systems is straightforward as they show a distinguishable characteristic hump in ρyx as a function of applied magnetic field (H) and temperature (T), corresponding to a skyrmion lattice23,24. However, even in B20 systems such a feature does not appear always25. One of our main goals here is to elucidate the significance of the subtle features that characterize our multilayer and to test their relationship to skyrmions.

Using magnetic force microscopy (MFM) and transport measurements, we present a comprehensive picture of the evolution of magnetic textures and their THE signature in a multilayer film capable of hosting skyrmions from RT down to at least 5 K. We demonstrate the relationship between nsk and |ρTH| over a ≈200 K temperature range. As the applied field H is swept from saturation towards zero, we find that skyrmions aggregate in worm-like magnetic textures, which may carry large topological charge (QW), and manifest as peaks in ρTH. Quantitative modeling of these worm-textures uncovers qualitative agreement between ρTH(H, T) and nT(H, T). Despite this, we find a large quantitative discrepancy indicating that the effect in multilayers is more involved.


Multilayer system

Here we use sputtered [Ir(1)/Fe(0.5)/Co(0.5)/Pt(1)]20 (in parenthesis—thickness in nanometers; subscript denotes the number of repeats) multilayer films, with the composition chosen for exhibiting skyrmions across a large range of T. The RT characterization of the films indicates Dzyaloshinskii–Moriya interaction (DMI) D ≈ 2.0 mJ/m2, and exchange interaction A ≈ 11 pJ/m8. The effective magnetic anisotropy (Keff) varies in the range ≈0.2–0.01 MJ/m3 as we change T from 5 K to 300 K (Supplementary Note 2). As demonstrated here, control over nsk through variation of T is the key for unambiguous identification of the skyrmion THE signature. Without this control, the correspondence between nsk and the subtle THE signal, which we establish by direct imaging, is impossible to uncover. In contrast to the B20 compounds, which host lattices of tubular Bloch-skyrmions26, multilayers sustain skyrmions with tunable properties, and offer smoother integration with existing spintronic technologies. Spin textures in multilayers are influenced by interlayer dipolar and exchange interactions, magnetic frustration27, and granularity7, which can pin, stabilize, and deform the spin textures, and result in coupled pancake-skyrmions with different topologies22,27. This complexity, and associated tunability, provide means for exploring the interplay between disorder, interactions, and topology.

Qualitative agreement between residual Hall signal and the magnetic textures

The magnetoresistance and Hall effect were measured using a lock-in with non-perturbative current densities (≈105 A/m2). The presence of skyrmions is associated with an additional component in the measured ρyx13,14,17. This contribution can be quantified by resolving ρyx into the ordinary (R0H) and anomalous [RSM(H)] Hall components13,17,18,19, and ρTH:

$$\rho _{yx}(H) = R_0H + R_{\mathrm{S}}M(H) + \rho _{{\mathrm{TH}}}(H).$$

We estimate ρTH(H) by Δρyx(H), the residual of the fit of ρyx(H) to \(\rho _{yx}^{fit}(H) = R_0H + R_{\mathrm{S}}M(H)\), which also yields R0 and RS (Supplementary Figure 7). The accuracy of Δρyx is ensured by calibrating field offsets to avoid artifacts resulting from using different measurement setups (Supplementary Note 3 and Supplementary Figure 2). Our conservative estimate for the overall error in Δρyx, including a contribution from data analysis, is ±2 nΩ  cm, corresponding to the non-zero residual signal beyond saturation, where there are no skyrmions. Figure 1a shows Δρyx(H) at 5 K, with the overall features persisting to at least 300 K8.

Fig. 1

Evolution of magnetic textures and THE with H at T = 5 K. a ρyx(H), \(\rho _{yx}^{fit}(H)\), and the residual \({\mathrm{\Delta }}\rho _{yx}(H) = \rho _{yx}(H) - \rho _{yx}^{fit}(H) \approx \rho _{{\mathrm{TH}}}(H)\). The black arrow indicates the field sweep direction for Δρyx and MFM, while ρyx and \(\rho _{yx}^{fit}\) are shown for both sweep directions. bk Selected MFM scans [full sequence in Supplementary Figure 16, scan-height h = 75, 60, 40, 60, 65, 50, 60, 50, 45, 60 nm for each of bk; color bars give the range of Δf, scale bars are 1 μm]. Frames in (i) mark features in focus in Fig. 3b–g

The features of Δρyx(H) in Fig. 1a are subtle. Here, we use MFM to determine the correspondence of these features with the magnetic texture. For this we followed the same field sweep from saturation as we did for Δρyx(H) and magnetization [M(H)]—the images were acquired at field increments as H was swept (Supplementary Note 1). Figure 1b–k shows the result for 5 K. Overall, we observe a similar evolution of the magnetic textures at T = 50, 100, 150, 200 K (Supplementary Figures 17 to 20).

We begin by comparing the magnetic textures to Δρyx(H). Beyond saturation, MFM shows the null signal expected for a polarized ferromagnet [Supplementary Figure 16(a)]. This is accompanied by the suppression of Δρyx (Fig. 1a) as expected for the topologically trivial polarized state. The onset of Δρyx commences at μ0H ≈ −0.3 T with the nucleation of sub-100 nm magnetic domains (Fig. 1b), which we identify as Néel-skyrmions21. By μ0H ≈ −0.25 T (Fig. 1c) the increasing nsk corresponds to a substantial Δρyx as expected from |ρTH| nsk1. Also, as nsk increases, skyrmions aggregate to form worm-like features (Fig. 1c). By μ0H ≈ −0.225 T, images show only worms (Fig. 1d, e). Surprisingly, at this field Δρyx peaks, suggesting a significant contribution from the worms which may have nontrivial topology. Meanwhile, the dense textures at intermediate H (Fig. 1f–h, and Supplementary Figures 17 and 18) correspond to reduced, yet finite, Δρyx. Careful inspection of such scans reveals worm-like features, to which we attribute the finite magnitude of Δρyx (Supplementary Note 7).

As H = 0 is approached, the worms evolve into labyrinthine helical stripes, and proliferate at the expense of the polarized background. This is coincident with the suppression of Δρyx, highlighting the close relationship between Δρyx and the magnetic texture. As H is increased towards positive saturation, the labyrinthine stripes evolve into worms, skyrmions, and eventually a uniformly polarized phase (Fig. 1i–k). For a texture with an opposite topological charge, the sign of Δρyx is reversed when H > 0. However, the MFM contrast does not change, due to the reversal of the tip magnetization near 0.1 T.

The distinct field ranges for isolated skyrmions (near saturation), worms (negative peak in Δρyx), and their coexistence (positive peak in Δρyx) (cf. Supplementary Note 6), offer a unique opportunity to compare the magnetic texture with Δρyx. In particular: (i) Does Δρyx track nsk? (ii) How do worms produce such a large Δρyx ? (iii) Is there quantitative consistency between Δρyx and nT?

To address (i) we exploit nsk(T), which increases by an order-of-magnitude when we increase T from 5 to 200 K (Fig. 2). We attribute this proliferation to the suppression of Keff with temperature8. Interestingly, skyrmion size is only weakly T-dependent and does not change significantly within our resolution, not unlike theoretical predictions28. However, further experiments with similar imaging conditions are required to confirm the size variation. Importantly, we find that Δρyx(T) tracks nsk(T) over the entire range (Fig. 2a), and gives ≈0.6 nΩ  cm per skyrmion/μm2. This correlation between skyrmion nucleation and the emergence of Δρyx strongly points towards the topological origin of the residual signal.

Fig. 2

Temperature dependence of nsk, Δρyx, and R0. The sign of nsk is chosen to match Δρyx. a Δρyx as a function of nsk for different temperatures at μ0H = −0.3T. Labels show the measurement temperature. Error-bars for Δρyx represent a conservative estimate of the systematic error. Errors for nsk are smaller than the symbols. The line is a linear fit (slope 0.6 ± 0.1 nΩ · cm/μm−2, intercept 2.2 ± 0.8 nΩ · cm). b Left axis: magnitude of the THE peaks (H < 0—squares, H > 0—circles). Right axis: the fit parameter R0(T) from Eq. (3) (triangles). cg MFM scans showing isolated skyrmions for nsk(T) in a. [For cg scan-height h = 75, 40, 40, 100, 40 nm, (c) is Fig. 1b, scale bars are 1 μm]

Magnetic worms and their topological charge

Having established the direct correspondence between nsk and Δρyx, we now examine the worms. Though the presence of worms is expected in systems with competing interactions, such as in ferromagnetic films29, their topological role is not obvious. In early MFM work on Bloch skyrmions in a B20 compound26, helical stripe domains resulting from merging skyrmions were described by two half-skyrmions connected by a topologically trivial straight domain26, and hence a topological charge of Qw = ±1. This motivates us to examine whether worms carrying a topological charge given by Qsk = ±1 can describe our results. We therefore plot nsk + nw (nw is the number of worms per unit area) in Fig. 3a, with the sign chosen from the sign of Δρyx. As the plot shows, both nsk(H) and nsk(H) + nw(H) do not track Δρyx(H). This calls for a closer look at the topological nature of the worms.

Fig. 3

Comparison between Δρyx and the signed density of topological charge at 5 K. a Right axis: Δρyx (solid line). Left axis: nsk (squares), nsk + nw (circles), nT (triangles), and Δρyx/(PR0Φ0) (cf. Eq. (2), inverted triangles with dotted line) using P = 0.5643 and R0 from Fig. 2b. For nT, each worm is assigned several skyrmions |QW| by fit, and each isolated skyrmion is counted once. Empty symbols indicate points with a lower confidence, that result from counting worms in a dense background (Supplementary Note 7). Shaded area shows confidence bounds for nT resulting from fit details (Supplementary Note 7). b, e Zooms on areas in Fig. 1i with skyrmions and isolated worms. c, f Results of MEFS fits wherein all skyrmions, including those assigned to worms, are treated as identical. The fit peak height ≈1.15 Hz, full width at half maximum (FWHM) ≈100 nm, and |QW| = 2 in (c) and |QW| = 4 in f. d, g Difference plots between b and c, and between e and f, showing the quality of the fit. Circles give the locations of the skyrmions in the fit. [The scale bars in b and e are 200 nm]

The following analysis of the topological charge of worms is motivated by sequences like Fig. 1b–d [also in Supplementary Figures 17(n)–(o)], which suggest that worms result from skyrmions clustering as nsk increases. The transition of worms into typical stripe domains with |Qw| = 1 requires a complete unwinding of their internal spin structure. The energy barrier for this suggests that the effective topological charge should be at least equal to the total number of skyrmions that form a worm (i.e., |Qw| > 1). While skyrmions are expected to repel each other on very short length-scales because of exchange coupling30, clusters can be stabilized by attraction on an intermediate scale, due to exchange frustration31.

Here our recent work, a magnetic multipole expansion of the field from skyrmions (MEFS)21, provides a direct method to associate an effective Qw with each worm. Figure 3b–g shows two typical examples where we fit the measured signal from worms by trains of skyrmions. Such images, which contain both skyrmions and worms, provide the foundation for this kind of analysis—the isolated skyrmions serve to constrain the fit amplitude per skyrmion, and improve the accuracy (Supplementary Note 7). Meanwhile, the analysis of images containing only worms (Fig. 1d) hinges on skyrmions–skyrmion repulsion on a length scale comparable to their radius30. Therefore, the number of skyrmions clustered in a worm is determined by the total length of the worm, and the typical radius of skyrmions (≈40 nm21). For images with densely packed features (e.g., Fig. 1f–h) identifying and extracting the worms themselves requires additional image processing, for which we employ a deep-learning-model-based algorithm that extracts features relevant for classification from supplied examples (Supplementary Note 7). We note however, that while this analysis provides additional evidence for the correlation between magnetic textures and the Δρyx that we extract, our main conclusion does not rely on it. In all cases, our analysis allows us to compute the total nT(H) from ∑Qw + ∑Qsk, where ∑Qw is the topological charge of a worm after assigning an appropriate number of skyrmions to it, and we assume that all skyrmions (including those in worms) have Qsk = ±1, with the sign chosen to match the sign of Δρyx.

To further verify our assertion of worms as trains of skyrmions, we have performed basic simulations of magnetization and the resulting evolution of magnetic textures in our multilayer stack. Simulations were performed using the MuMax3 package32 at T = 0 K for two different sets of magnetic parameters relevant to the magnetization of the stacks at different temperatures. In the simulations the field is swept incrementally towards saturation from H = 0. The magnetic texture in the simulations starts from labyrinthine stripes and evolves into worms, skyrmions and eventually a fully polarized state, in agreement with our experimental results. A complete set of simulated MFM images is shown in Supplementary Figures 10 and 11.

Figure 4 shows representative simulated maps of nz(r), the corresponding MFM images, and the contribution to Qsk from each individual domain. Dashed domains in Fig. 4c, f mark skyrmion trains which appear as worms in the MFM scans (Fig. 4b, e), clearly indicating |QW| > 1. Here, we point out that while these results are in qualitative agreement with the experimental evolution of magnetic textures and the formation of worms, the simulations do not account for disorder and thermal effects in the multilayers. Addition of such effects and a full theoretical treatment is necessary for a deeper understanding of skyrmion trains and skyrmion–skyrmion interactions.

Fig. 4

Micromagnetic simulations of magnetic textures (Supplementary Note 5) for two sets of magnetic parameters corresponding to 5 and 200 K: ac A = 11 pJ/m, D = 2 mJ/m2, Ms = 1.34 MA/m, Keff = 0.2 MJ/m3, and df A = 11 pJ/m, D = 2 mJ/m2, Ms = 1.16 MA/m, Keff = 0.05 MJ/m3. a, d 2D maps of the out-of-plane magnetization (nz) at 0.230 T. b, e Simulated MFM images at h = 40 nm obtained by integrating the stray field from the micromagnetic simulations and convolving with a model for the tip (Supplementary Note 5). c, f Contribution to the topological charge from each domain, calculated using Eq. (1) (Supplementary Note 5). Dashed lines highlight trains of skyrmions which appear as individual worms in the MFM scans. [The scale bars in a and d are 200 nm]

The qualitative match between nT(H) and Δρyx(H) (Fig. 3a), and the formation of worms from the clustering of skyrmions, as suggested by our micromagnetic simulations, reinforces our modeling of worms as trains of skyrmions. These results provide additional evidence that Δρyx results from skyrmion textures and is thus topological in nature, indicating Δρyx ≈ ρTH. Our observations on the emergence of worms with a potentially high topological number, previously not noticed experimentally, indicate they are distinct from trivial spin spirals, and form an essential part of the phase diagram for multilayer skyrmions33. The presence of worms in a tunable multilayer offers a platform for studying skyrmion–skyrmion interactions over a wide parameter range, as well as applications, such as skyrmion racetracks7.

Quantitative agreement between transport and imaging

Having explored the nontrivial topology of the worms and a qualitative match between ρTH(H, T) and nT(H, T), we examine the quantitative match. As we show in Fig. 3a, the density of topological charge estimated from THE [Δρyx/(PR0Φ0), Eq. (2)] indicates a two-orders-of-magnitude discrepancy. This implies that simply using Eq. (2) with \(R_0^\prime = R_0\) to understand the topological signatures of chiral magnetic textures in multilayer skyrmion-hosts does not yield a comprehensive description of the measured Δρyx.

A possible culprit is the assignment \(R_0^\prime = R_0\) in Eq. (2)34, which is justified for a single band material. This is not the case here: Bulk Fe and Co, the ferromagnetic ingredients of our multilayer stack, have several active electron and hole bands35. In such materials R0 is suppressed because electrons and holes, which experience the same H, compensate each other’s contributions. The cancellation estimated from values reported for bulk Fe35 indicate suppression of R0 by an order of magnitude from the separate contributions of individual bands, partially addressing the discrepancy (Supplementary Note 8). Importantly, the cancellation may not happen in the same way for Beff—the Berry-phase can act differently on charge carriers from different bands23, with an associated sensitivity to occupation36. The fact that the peak value of Δρyx(H) changes by only ≈25% with T despite the sign change of R0(T) (Fig. 2b), probably because of small variations of the occupations of the compensating bands, further confirms that \(R_0^\prime \ne R_0\). In this case, using R0 in Eq. (2) underestimates ρTH18,19, although once \(R_0^\prime \) is determined this fundamental equation may still be used. For this it is essential to account for the electronic band structure of the chiral magnet.

Finally, we comment on the nature of spin transport in multilayers. Here, transport is influenced by various length scales such as the thickness of individual layers, their mean free path (l), charge and spin conductivities, spin diffusion length (ls), and the size of the magnetic textures—including the domain walls and their chirality. In our case, the radius of the skyrmions is ≈40 nm and the domain wall width ≈7–14 nm \(\left( {\sqrt {A/K_{{\mathrm{eff}}}} } \right)\), where, A ≈ 11 pJ/m and ≈0.2–0.05 MJ/m3. These length scales are comparable to the transport length scales reported for single thin layers (lCo ≈ 5 nm and lPt ≈ 13 nm, lsPt ≈1−10 nm)37, indicating their relevance to the relationship between ρTH and nsk. Spin scattering from interfaces and magnetic textures such as domain walls may cause spin-flip scattering, resulting in a non-adiabatic, spin independent transport38,39,40. As a result of the disordered skyrmion configurations, the charge carriers experience an inhomogeneous emergent field, in contrast to charge carriers in bulk systems which experience a systematically varying uniform emergent field due to the ordered arrangement of skyrmion textures. Notably, spin scattering in multilayer systems and its contribution to the anomalous Hall effect is dominated by skew scattering41. Hence, a better understanding of this contribution may help resolve the discrepancy between the observed and the expected THE signal38,39,40,42.


Our complementary imaging and electrical transport studies provide clear evidence for the correlation between Δρyx and the topology of the magnetic texture in technologically viable magnetic multilayers. Furthermore, we elucidate the complexity of the Berry-phase associated with the electrical fingerprint of chiral magnetic textures in those skyrmions hosting platforms. For a comprehensive understanding and in order to utilize THE emerging from magnetic skyrmions, it is imperative to consider (a) the band structure contributing to THE, (b) the possibility of |Qsk| > 127 and skyrmion–skyrmion interactions31, (c) the coupling of skyrmions across layers and complex magnetic textures in buried interfaces22, (d) the contribution from topologically trivial chiral configurations driven by magnetic spin-frustration20, and (e) the validity of the commonly assumed adiabatic approximation20.

Data availability

The authors declare that the data supporting the findings of this study are available within the paper, and its Supplementary Information.

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Journal peer review information: Nature Communications thanks the anonymous reviewers for their contribution to the peer review of this work.

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It is our pleasure to thank A. Petrović for inputs on transport experiments, as well as D. Arovas, A. Auerbach, Shi-Zeng Lin, D. Podolsky, M. Reznikov, and A. Turner for illuminating discussions. We also thank G. Goldman and Y. Schechner for help with image analysis. The work in Singapore was supported by the Ministry of Education (MoE)—Academic Research Fund (Ref. No. MOE2014-T2-1-050), the National Research Foundation—NRF Investigatorship (Reference No. NRF-NRFI2015-04), and the A*STAR Pharos Fund (1527400026). Work at Technion was supported by the Israel Science Foundation (Grant No. 1897/14). We would also like to thank the Micro Nano Fabrication Unit, and to acknowledge support from the Russell Berrie Nano Technology Institute, both at the Technion.

Author information

M.R., A.S., O.M.A. and C.P. designed and initiated the research. M.R. deposited the films and characterized them with A.S. and A.K.C.T. M.R. performed and analyzed magnetization and transport measurements with inputs from A.S., O.M.A. and C.P. A.Y. performed the low temperature MFM experiments with assistance from A.A. and A.Y. and O.M.A. analyzed the low temperature MFM data. F.M. performed micromagnetic simulations and A.Y. analyzed the simulated images. O.M.A. and C.P. coordinated the project. All authors discussed the results and provided inputs to the manuscript.

Competing interests

The authors declare no competing interests.

Correspondence to O. M. Auslaender or C. Panagopoulos.

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