The nature of ferromagnetism in the chiral helimagnet Cr1/3NbS2


The chiral helimagnet Cr1/3NbS2 hosts exotic spin textures, whose influence on the magneto-transport properties make this material an ideal candidate for future spintronic applications. To date, the interplay between macroscopic magnetic and transport degrees of freedom is believed to result from a reduction in carrier scattering following spin order. Here, we present electronic structure measurements across the helimagnetic transition temperature TC that challenges this view. We show that the Fermi surface is comprised of strongly hybridized Nb- and Cr-derived electronic states, and that spectral weight close to the Fermi level increases anomalously as the temperature is lowered below TC. These findings are rationalized on the basis of first principle density functional theory calculations, which reveal a large nearest-neighbor exchange energy, suggesting the interaction between local spin moments and hybridized Nb- and Cr-derived itinerant states to go beyond the perturbative interaction of Ruderman-Kittel-Kasuya-Yosida, suggesting instead a mechanism rooted in a Hund’s exchange interaction.


The development of next-generation electronic devices relies on the ability to precisely control other intrinsic degrees of freedom (DOF) beyond that of charge. In this endeavor, chiral helimagnets (CHMs) have emerged as promising materials to be used for spintronic and other information technology applications, where the intent is to actively manipulate either the individual or average spin angular momentum of itinerant carriers1. In CHMs the chiral framework of the crystal structure allows for the arrangement of spins into incommensurate periodic spirals, or helices, resulting from an anti-symmetric spin interaction known as the Dzyaloshinskii–Moriya interaction2,3,4,5,6. Such an interaction, which originates from relativistic spin–orbit coupling, not only underlies the helical ground state of CHMs but also unusual spin textures like the two-dimensional spin vortex known as a skyrmion as well7,8. Skyrmions are of particular technological interest owing to the fact that they can be manipulated at the nanoscale level by externally applied magnetic fields8 and spin polarized currents9,10, and are found to have a profound influence on electronic transport11,12,13.

Given these important functionalities, there has been a great incentive for the discovery of new CHM materials relevant to the design and fabrication of future spintronic devices14. One such material is Cr1/3NbS215, which has been shown to host a unique one-dimensional solitonic excitation known as a chiral soliton lattice (CSL)16. Much like skyrmions the CSL can be manipulated by external magnetic field16, but unlike other CHMs, Cr1/3NbS2 crystallizes in a more anisotropic, Nb3CoS6 (hp20), layered structure consisting of ferromagnetic (FM) planes of intercalated Cr atoms ordering in a (√3 × √3)R(30°) superstructure within the ab plane. Each Cr atom occupies a trigonally distorted octahedral (Oh) sites in the van der Waals gaps of 2H-NbS2 (Fig. 1a)17 and hosts a local spin moment (LSM) of ~3μB Cr−1 that order below a Curie temperature, TC = 116–132 K15,16,17. Due to such high anisotropy and the fact that inversion symmetry breaks only along the non-centrosymmetric c-axis, where the long-range (~48 nm) helimagnetic ordering develops, Cr1/3NbS2 has been recognized as an ideal system for studying spin textures in magnetic thin films, devices fabricated on a substrate, and spin–orbit coupling effects in magnetic multilayers18,19.

Fig. 1: Crystal and electronic structures of Cr1/3NbS2 in the helimagnetic state.

Cr1/3NbS2 a unit cell, b magnetic susceptibility, c Fermi surface, and d electronic band dispersion along the ΓK direction for temperatures below the helimagnetic transition temperature, TC. The unit cell, defined by lattice constants a = b = 5.741 Å and c = 12.101 Å, contains 20 atoms, with 12 S atoms occupying the general site, and six Nb atoms having two inequivalent positions. Helimagnetic order is verified by the presence of a prominent kink in the magnetic susceptibility at 131 K as measured within a 100 Oe external magnetic field. The NbS2-derived hole pockets at Γ and K are shown in black, while additional bands arising from Cr intercalation are shown in green. The three dispersive bands, labeled α, β1, and β2, found near the zone center are the focus of this experimental work.

More generally, Cr1/3NbS2 belongs to a class of transition metal dichalcogenides (TMDs) intercalated by magnetic, 3d elements. According to a conventional description of the electronic structure for these materials, Curie–Weiss spin moments localized on the Cr site do not alter the Fermi surface (FS) or band topology of the host NbS2 compound, aside from raising the chemical potential following a donation of charge to Nb-derived bands20,21. Due to the large separation distance between Cr neighbors (√3a), long-range magnetic order is believed to be mediated by Nb conduction electrons through a Ruderman–Kittel–Kasuya–Yosida (RKKY) exchange interaction22,23,24,25. Under such an exchange mechanism, the raise in chemical potential that accompanies intercalation serves to alter the nesting condition in the FS, and in turn change the periodicity and range of interaction for the oscillatory exchange coupling between screened, LSMs26. In this regard, the identity of the intercalant atom has little impact on the resultant order or ordering temperature so long as each species possesses the same oxidation state and spacing in the lattice. Hence, both the drop in resistivity and negative magnetoresistance (MR) observed throughout this class of materials are argued to result from a reduction in spin scattering due entirely to magnetic ordering27,28. However, recent experimental and theoretical findings for Cr1/3NbS2 not only propose an alternative exchange mechanism beyond a conventional RKKY29 but also show abrupt, anisotropic changes in the magneto-transport that suggest that Cr-derived states play a more active role in the interplay between LSMs and itinerant electrons30.

The importance of these findings is underscored by a major technological appeal of Cr1/3NbS2, which lies in the interplay between transport and magnetic DOF. Namely, inter-layer magneto-transport measurements have revealed a direct correlation between the transverse, negative MR and the soliton lattice density, which is attributed to Bragg scattering of conduction electrons by the magnetic superlattice potential of the CSL27,28. However, recent in-plane transport, MR, and magnetic anisotropy measurements both in proximity to TC and at the CHM to CSL transition show abrupt changes29,31 that depend sensitively on the direction of applied magnetic field relative to the ab plane30. This includes a drop in the in-plane resistivity by more than an order of magnitude as T < TC as well as a decrease in the intra-layer MR by 6% at the CSL transition29. Such results cannot be readily explained by spin ordering arguments alone, as it is not obvious how a modulation of the CSL state along the crystallographic c-axis could have such a strong impact on the in-plane transport properties. Rather, Ghimire et al.29 and Bornstein et al.30 argue on the basis of first-principle calculations that details of the electronic structure must play a more central role in shaping magneto-transport in Cr1/3NbS2. Thus, there exists an experimental need to better elucidate the microscopic mechanisms underlying such a close interplay between in-plane transport and magnetic DOF in this material.

In this article, we provide experimental evidence showing the electronic structure to play a non-trivial role in the description of in-plane magneto-transport in Cr1/3NbS2. Through the use of resonant photoemission spectroscopy (ResPES), we find the FS of this material to be comprised of strongly hybridized Cr- and Nb-derived electronic states, while angle-resolved photoemission spectroscopy (ARPES) reveals an anomalous increase of spectral weight in proximity to the Fermi level (EF) as temperature is lowered below TC. Such behavior is inconsistent with that of a conventional itinerant ferromagnet, and can be rationalized on the basis of first-principle density functional theory (DFT) calculations to result from a strong exchange (Hund’s) interaction between itinerant electrons and LSMs on the Cr sites.


Overview of electronic structure

Previous work focusing on how the electronic structure of NbS2 is modified with Cr intercalation for temperatures below the helimagnetic transition temperature (Fig. 1b) is reported by Sirica et al.32. To summarize these results, Fig. 1c, d shows a schematic diagram of both the FS and band dispersion along the high-symmetry ΓK-axis, where crossing points α, β1,2, γ, and δ follow the same labeling convention as used in this previous study32. As expected, Cr intercalation injects electronic charge into the NbS2 layers, resulting in a sinking of the bonding, bilayer split NbS2 band (S) below EF, while the remaining NbS2-derived, anti-bonding band has crossing points α and γ consistent with a raise in chemical potential. However, the electronic charge introduced by the Cr intercalant not only changes the total number of carriers but also causes a significant modification to the electronic structure of NbS2 through the addition of two additional bands at Γ1, β2), and one additional band at Κ (δ). Since these bands cannot be rationalized on the basis of a rigid band picture, it is natural to inquire about their origin. Here, we focus on the temperature dependence of the α and β1,2 bands in proximity to Γ, as the bands at Κ are found to exhibit no significant change with temperature across TC.

Temperature-dependent angle-resolved photoemission

Temperature-dependent ARPES is used to map the dispersion of the α and β1,2 bands in proximity to EF as the temperature is tuned across TC (Fig. 2). For T < 131 K, three dispersive bands can be identified at Γ, while only two bands are present as temperature is raised above TC. From Fig. 2, it is evident that the outermost β2 band shifts towards Γ with increasing temperature until the two β-bands can no longer be distinguished. Such behavior is more clearly demonstrated in Fig. 3, which gives the temperature dependence of the band crossing points (kF) along the two high-symmetry directions ΓM (Fig. 3a) and ΓK (Fig. 3b). Here, momentum distribution curves (MDCs) illustrating the distributions of spectral weight at a fixed energy E = EF along these two high-symmetry directions reveals a monotonic shift in kF for the β2 band to be accompanied by a progressive decrease in spectral weight for 50 K < T < 120 K. The fact that this behavior is observed along both the ΓM and ΓK directions suggests it to be isotropic about Γ. Moreover, given the close proximity to TC, the relative shift of β2 towards β1 implies the β1,2 bands arise from magnetic exchange splitting. While dedicated spin-resolved ARPES measurements are required to establish unambiguously the spin polarization of these bands, such a finding is consistent with the notion that the β1,2 bands result from intercalation of a magnetic element (Cr) into NbS2, and suggest the presence of Cr-derived states at EF. Indeed, this finding has been confirmed with ResPES, a methodology that allows photoemission spectra of the valence band (VB) to acquire elemental sensitivity33,34.

Fig. 2: Temperature-dependent angle-resolved photoemission.

Temperature-dependent angle-resolved photoemission spectra obtained along the ΓΜ direction at a 10 K, b 50 K, c 90 K, d 120 K, e 131 K, f 140 K, g 170 K, and h 220 K using π-polarized photons having an energy,  = 48 eV. Here, band crossing points are denoted by white arrows in a, while the dashed line in a, e denotes the presence and absence of a β2 band crossing as temperature is raised above the helimagnetic transition temperature.

Fig. 3: Temperature dependence of band crossing points.

Momentum distribution curves extracted at the Fermi level from spectra measured along a ΓM and b ΓK using photons of energy  = 48eV. Note the emergence of a split β1,2 band for temperatures below 120 K, and a loss of spectral weight along both high-symmetry axes for temperatures below the helimagnetic transition temperature.

Resonant photoemission

By tuning the incident photon energy across the Cr L3-edge, it is possible to identify Cr 3d states in the VB within 3 eV of EF (Fig. 4a, b). The increase in signal intensity at resonance, that is, with the photon energy tuned on the maximum of the Cr absorption edge, reveals that the structures at ≈2.5 eV and within ≈1 eV from EF are states possessing Cr 3d character.

Fig. 4: Identifying Nb- and Cr-derived states in the valence band.

Resonant photoemission spectra measured across the a, b Cr L3 and c, d Nb M5 absorption edges using linear horizontal photon polarization. Intensity maps (a, c) and selected photoemission spectra generated across the b Cr and d Nb x-ray absorption edge (XAS) shown in the inset. Spectra denoted 1–4 in a, c are taken through the Cr and Nb resonance, respectively. Hatched area in b, d denotes the difference between spectra taken on resonance (1–4) and off resonance (0).

The states at Γ have been shown by polarization-dependent ARPES to exhibit predominantly out-of-plane orbital character32. Therefore, in contrast to our previous ResPES measurements32, whose purpose was to identify non-dispersive Cr states remaining on the surface following sample cleave, the photon polarization used in this report was chosen to emphasize those bulk states having an out-of-plane character through ensuring a component of the photon polarization to lie perpendicular to the sample plane. In doing so, a direct comparison of ResPES spectra taken with photon energies tuned across the Cr L-edge (Fig. 4a, b) and Nb M-edge (Fig. 4c, d) reveals a clear resonance over the Nb “dz2 sub-band”21 (EB ≈0.6 eV < E < EF), indicating the presence of hybridization between Cr- and Nb-derived states in the VB. This is made possible by noting spectra taken across the Cr L3-edge to be sensitive, in these experimental conditions, to the projection of Cr 3d orbitals, whose splitting is dictated by a trigonally distorted octahedral environment22,23. Hence, our ResPES data clarify that the VB states at Γ originate from a linear combination of Nb dz2 and mixed Cr 3d orbitals (\(\sqrt 2\)dxz − dx2 − y2 and \(\sqrt 2\)dyz + dxy), having an overall out-of-plane orbital character.

In addition to taking ResPES measurements across the Cr L3 ionization edge for T > TC (Fig. 4a, b), ARPES spectra were collected at T < TC along the ΓΚ-axis using photon energies that have likewise been tuned across the Cr resonance (Fig. 5a–c). In doing so, the α band, belonging to the host NbS2 compound, and two β1,2 bands, arising from Cr intercalation, are well separated, allowing for the elemental sensitivity of ResPES to benefit from an added momentum resolution. Here, a comparison of the integrated energy distribution curves (EDCs) shown in Figs. 4b and  5d reveal a resonant enhancement of Cr 3d states occurring near EF that is independent of temperature. However, MDCs extracted from Fig. 5a–c at EF as a function of photon energy show an initial resonance of the β1,2 bands (k ~0.5 Å−1) occurring at the onset of absorption (Fig. 5e). This finding not only provides evidence for a Cr-derived elemental character of these bands but also reveals a lack of hybridization with the Nb-derived α band that is consistent with its anti-bonding orbital character32. Given the large separation distance between Cr neighbors, the formation of dispersive β1,2 bands following Cr intercalation can only occur through hybridization with Nb. This is made clear from our ResPES results, but is also indicated by the higher degree of kz dispersion exhibited by the β1,2 bands as compared to α32. Thus, by measuring ARPES across the Cr absorption edge, a band resolved picture of Cr-derived d states in the VB is obtained.

Fig. 5: Angle-resolved photoemission across the Cr resonance.

Angle-resolved photoemission spectra measured below the helimagnetic transition temperature (110 K) using a photon energy tuned a off the Cr L3 resonance (hν = 570 eV), b at the onset of Cr absorption ( = 574eV) and c at the maximum of Cr absorption ( = 576 eV), where the contribution due to photon momentum is taken into account. An angle of 60° is made between the polarization vector of the incoming light and the crystal surface plane, resulting in a dominant component perpendicular to the sample surface. d Integrated energy-dispersive curves taken over a momentum range, Δk = ±0.5 Å−1 with respect to Γ, encompassing the α and two β1,2, bands. e Resonant momentum distribution curves obtained by integrating ±50 meV about the Fermi level. For the resonance tuned on the maximum of Cr absorption, a featureless MDC is observed, indicating various scattering channels have opened across the Fermi surface.

Change in spectral weight in proximity to T C

By revealing the presence of Cr-derived d states at EF, our data show that a clear separation of magnetic and itinerant DOF does not occur in Cr1/3NbS2, as the same states forming LSMs are also participating in the formation of the FS. The consequences of this finding are illustrated in the temperature dependence of the EDCs integrated over a broad momentum range (kΓΜ = 0.24–0.8 Å−1) encompassing both crossing points of the β1,2 bands (Fig. 6a). Here, as T >50 K, the spectral weight in proximity to EF begins to drop and is transferred towards higher binding energies until T >120 K, whereupon there is no longer any change. Similarly, the temperature dependence of the α band appears to be less pronounced as compared to that of the β band, but still reveals a monotonic drop of spectral weight at EF, as well as a slight reduction in the separation between peaks at 100 and 400 meV as T > TC (Fig. 6b). In both cases, the spectral weight at EF changes in close proximity to TC (T = 130–90 K), allowing for thermal broadening effects to be excluded, suggesting instead a microscopic mechanism that links electron itinerancy to the onset of ferromagnetism.

Fig. 6: Changes in spectral weight near the Fermi level across the helimagnetic transition.

a Energy distribution curves normalized to photon flux and integrated from kΓM = 0.24–0.8 Å−1. b Energy distribution curves extracted at the Fermi crossing of the α band as a function of temperature from a separate temperature-dependent angle-resolved photoemission study used to confirm the findings in a. Note the monotonic suppression of spectral weight as the temperature is increased above the helimagnetic transition temperature. This behavior is more clearly highlighted by the inset in b showing a change in spectral weight occurring within 150 meV from the Fermi level.


For ferromagnetism being mediated by an indirect RKKY exchange interaction, as is the case for rare-earth metals like Gd, the electronic states forming the FS are distinct from those hosting LSMs35, where the interaction between local moments and itinerant electrons is treated as a weak perturbation resulting from a FS instability26. Under an RKKY exchange interaction, the VB states are exchange split by the local moment. Temperature controls the ordering of the LSMs, and affects the exchange splitting of the VB according to a behavior that is intermediate between two extreme limits. In one instance, there is no change in exchange splitting with temperature. This occurs when VB states have wavefunctions that are incoherent over the magnetic correlation length of the local moment. Such behavior is exhibited by band states that are either localized, or in systems consisting of a few magnetic impurities embedded in metals. In the opposite limit, the exchange splitting of the valence states continuously decreases with increasing temperature until vanishing all together when magnetic order is lost. This Stoner-like behavior occurs when band states are delocalized so as to remain coherent over a distance that is large compared to the magnetic correlation length of the local moment35. In a prototypical system described by an RKKY exchange, like Gd, VB states with different degrees of localization/delocalization exhibit behavior that spans these two extremes36.

As this pertains to Cr1/3NbS2, despite the merging of β1,2 bands as temperature is raised above TC, the transfer of spectral weight away from EF as T > TC runs counter to our initial first-principle, DFT calculations, showing the Stoner criterion to be well satisfied29. By revisiting these calculations using the same experimental structure as used by Ghimire et al.29 with internal coordinates optimized, we focus on an underappreciated aspect of Cr1/3NbS2, which is how a material having such a large in-plane, Cr–Cr nearest-neighbor distances (5.75 Å) can exhibit an ordering temperature as high as 131 K. While evident that such a large Cr–Cr distance discounts the possibility of a direct exchange interaction, more conventional indirect exchange interactions are expected to be weak and will therefore play a role only at considerably lower energy scales. Our calculations find an energy difference between the FM and nearest-neighbor excited anti-FM state to be in excess of 30 meV Cr−1, implying a TC ≈116 K under a mean-field approximation alone. Such a large energy scale for the exchange energetics is expected to dominate over any higher-order corrections, like the magnetic anisotropy30, that arise from spin–orbit coupling in this material. While an RKKY interaction has been experimentally established as the fundamental exchange interaction in 3d-intercalated TMDs23,25, including Cr1/3NbS237, such a significant exchange energy implies the interaction between LSMs and hybridized Nb- and Cr-derived itinerant states may go beyond this perturbative interaction, originating instead from a microscopic interaction between itinerant electrons and LSMs.

The data presented here show a clear separation of magnetic and itinerant DOF does not occur, leading to the motion of itinerant electrons influencing LSMs reciprocally, and in a self-consistent fashion, as is found for other itinerant, 3d magnetic systems38,39. In such a case, a strong Hund’s coupling establishes a connection between the onset of ferromagnetism and metallicity, as it enforces electron itinerancy on Cr sites when the spin of the majority carrier is parallel to the LSM. In this way, an on-site Hund’s correlation shapes the interaction between itinerant electrons and LSM’s in such a way that a synergistic and regenerative character is acquired. That is, FM order fosters electron itinerancy by a reduction of electron scattering from thermal fluctuations of the LSMs, while electron itinerancy promotes a decrease of the electron kinetic energy and FM order, overall resulting in a minimization of energy for the entire system. Hence, electron itinerancy acquires a fundamental role in the attainment of FM order, and the FM transition in Cr1/3NbS2 is viewed as a cooperative phenomenon driven by the mutual interaction of itinerant electrons and LSMs enforced by Hund’s coupling. The concomitant increase of electron itinerancy and alignment of the LSMs provide a route for the minimization of the total energy of the system, offering a microscopic means by which important aspects of the in-plane transport can be rationalized. This includes a natural explanation for the pronounced drop of the in-plane resistivity occurring at TC, along with the negative in-plane MR28,29. In this way, the magneto-transport properties of Cr1/3NbS2 are in some respect reminiscent of the colossal magnetoresistive manganites. Both systems exhibit the same correlation between the ordering of LSMs and the onset of metallicity, and both exhibit a negative MR, albeit quite different in order of magnitude.

In Cr1/3NbS2, elucidating the mechanisms that underlies both inter- and intra-layer magneto-transport acquires particular importance in light of the possible technological relevance that this material has for future spintronic applications. Our results suggest that arguments based entirely on magnetic scattering due to spin ordering in the CSL state may not fully capture the magneto-transport properties observed in this material. As our high-resolution photoemission results are sensitive to only the first few atomic layers, our findings are directly relevant to a microscopic description of the in-plane, magneto-transport properties. Nevertheless, it is unlikely that the microscopic interaction between itinerant electrons and LSMs evidenced by our data would be entirely irrelevant for the inter-layer magneto-transport properties as well. In fact, any mechanism proposed to explain the inter-layer MR must be rooted in a Hamiltonian that takes into account the interaction of itinerant electrons with the LSMs. Thus, despite the long length scales of the CSL, our results highlight the relevance of the electronic structure in a description of the magneto-transport properties in Cr1/3NbS2, as underscored by the strong Hund’s coupling between itinerant electrons and LSMs. For this reason, we hope this work encourages future investigations into other 3d-intercalated TMDs, where the interaction between LSMs and itinerant electrons extends beyond a rigid band interpretation and will be relevant for shaping anisotropic functionalities in this class of materials.

In conclusion, electronic structure measurements of Cr1/3NbS2, taken above and below the helimagnetic transition temperature, reveal a clear separation of magnetic DOF, and itinerant DOF does not occur, as the same states forming LSMs are also participating in the formation of the FS. An anomalous increase of spectral weight in proximity to the Fermi level (EF) as temperature is lowered below TC marks a behavior that is inconsistent with conventional itinerant ferromagnets, and is rationalized on the basis of first-principle DFT calculations to result from a strong exchange (Hund’s) interaction between itinerant electrons and LSMs on the Cr sites. Our results suggest that arguments based entirely on magnetic scattering due to spin ordering in the CSL state may not fully capture the magneto-transport properties observed in this material, as the electronic structure is clearly shown to play a non-trivial role as temperature is tuned across TC.


Crystal growth

Polycrystalline Cr1/3NbS2 samples were grown by heating stoichiometric ratios of Cr, Nb, and S to 950 °C for 1 week. Single crystal growth was carried out under chemical vapor transport using 0.5 g iodine transport agent per 3 g Cr1/3NbS2. The 5 mm × 5 mm plate-like crystals oriented along (0 0 1) formed across a 100 °C (950–850 °C) temperature gradient of the transport tube. Due to the deleterious effect that Cr disorder has on the appearance of helimagnetic ordering in this material40, x-ray and low-energy electron diffraction measurements were used to confirm a P6322 space group showing (√3 × √3) Cr ordering29,32. Sample quality was further verified with superconducting quantum interference device magnetometry (Fig. 1b), which reveals a prominent kink at TC = 131 K, indicating helimagnetic ordering in this sample batch.

Photoemission spectroscopy

Temperature-dependent ARPES experiments were carried out on Cr1/3NbS2 single crystals cleaved in situ on Beamline 10.0.1 of the Advanced Light Source (ALS) and the Advanced Photoelectric Effect beamline at the Elettra Synchrotron Facility. The total instrumental energy resolution ranged from 15 to 30 meV, while an angular resolution of ±0.5° gives a momentum resolution of <0.06 Å−1 for the photon energies used in these experiments ( = 40 and 48 eV). ResPES and ResARPES experiments were performed above and below TC on the Beamline for Advanced diCHroism at Elettra with a total instrumental energy resolution being better than 300 meV.

Ab initio calculations

First-principles DFT calculations were carried out using the linearized augmented plane-wave DFT code WIEN2K41 in the generalized gradient approximation of Perdew et al.42. The respective sphere radii of 2.01, 2.33, and 2.37 Bohr were used for S, Cr, and Nb, with a value for the product of the smallest sphere radius (S) and the largest plane-wave expansion vector being set to RKmax = 8.0. Calculations of the magnetic properties, performed with and without spin–orbit coupling, were carried out under the internal coordinates of the structure being relaxed in the FM state. A minimum of 800 k points in the full Brillouin zone were used for the FM calculations, while this number was proportionally reduced for the 2 × 2 × 1 supercell of the planar anti-FM state.

A comparison of DFT energetics with and without spin–orbit coupling is made between a FM and two possible anti-FM states denoted as AFM1 and AFM2. These states represent either anti-aligned Cr–Cr pairs along the c-axis (AFM1), or four of six anti-aligned Cr–Cr neighboring pairs in the ab plane (AFM2). From our calculation, we find an energy difference in meV/Cr for AFM1 and AFM2 relative to the FM state that shows DFT can describe the normal (i.e., non-Dzyaloshinskii–Moriya) exchange interaction without the need to consider spin–orbit coupling (Table 1). This <1 meV/Cr difference is fully consistent with the high (131 K) magnetic ordering temperature found in this material.

Table 1 Comparison of first-principle calculations with and without spin–orbit coupling.

Data availability

All data presented in this manuscript can be made available upon reasonable request to corresponding authors, N.S. and N.M.

Change history

  • 07 May 2020

    An amendment to this paper has been published and can be accessed via a link at the top of the paper.


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This work was supported by the National Science Foundation, Division of Material Research, Grant No. DMR-1151687 (N.M.). This work was performed, in part, at the ALS, a DOE Office of Science User Facility under contract no. DE-AC02-05CH11231. N.S. acknowledges support from the Center for Integrated Nanotechnologies at Los Alamos National Laboratory (LANL), a US Department of Energy, Office of Basic Energy Science user facility. DSP was supported by the US Department of Energy (DOE), Office of Science, Basic Energy Sciences, Materials Science and Engineering Division. Partial funding for open access to this research was provided by University of Tennessee’s Open Publishing Support Fund.

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Samples were provided by L.L., D.S., and D.G.M. Temperature-dependent ARPES experiments were performed by N.S. and N.M. with the help of S.-K.M., A.V.F., P.K.D., I.V., and J.F. ResPES and ResARPES experiments were carried out by N.S. with the help of F.B., I.P., and S.N. N.S. and P.V. analyzed the data, with input from N.M. and D.S.P., who provided ab initio calculations. N.S., P.V., and N.M. wrote the manuscript with input from all authors.

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Correspondence to N. Sirica or N. Mannella.

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Sirica, N., Vilmercati, P., Bondino, F. et al. The nature of ferromagnetism in the chiral helimagnet Cr1/3NbS2. Commun Phys 3, 65 (2020).

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