The intriguing perovskite nickelates family ReNiO3 (with Re=rare-earth)1,2,3,4 have garnered significant research interest in recent years, due to the remarkable properties they exhibit. These include a sharp metal to insulator transition (MIT) tunable with the Re radius2, unusual magnetic order5 and the suggestion of charge order6 in the insulating phase. While ReNiO3 single crystals are very hard to synthesize, causing earlier experiments to be mainly restricted to powder samples, extremely high-quality epitaxial thin films can be now produced. As an additional asset, ReNiO3 in thin film form can exhibit even richer properties compared to bulk, for example, tunability of the metal–insulator transition by strain7,8, thickness9,10,11 or even by ultrafast optical excitation of the substrate lattice degree of freedom12. In addition, there has been a lot of interest in nickelate-based heterostructures, motivated on one hand by theoretical predictions of possible superconductivity13, and on the other hand by recent observations of exchange bias effects14 and modulation of the orbital occupation due to strain and interface effects15,16,17,18.

The origin of the rich physics behind these unique properties is complicated by the usual electron correlation problem of transition metal oxides19. As a consequence, a full understanding of the mechanism driving the MIT in ReNiO3 remains elusive still today. Hampering the discovery of a universally accepted description of the MIT is the more fundamental problem of understanding the ReNiO3 electronic structure and the corresponding Ni 3d orbital occupation.

In Fig. 1, we illustrate in a schematic representation of the single-electron excitation spectra how different electronic configurations can result from the two possible regimes of the effective charge-transfer energy Δ′ (called for simplicity charge-transfer energy throughout the text). Using formal valence rules, it is expected that the Ni atoms exhibit a 3d7 (Ni3+) character, likely in a low spin (S=1/2) configuration. This ground state (GS) is obtained in Fig. 1a for Δ′>0. However, high-valence Ni3+ systems are rare, and although many studies indeed view ReNiO3 as conventional positive charge-transfer compounds yet with the addition of a strong Ni–O covalency and consequently a GS configuration of the type of (where L is an O 2p hole)1,20,21,22,23, mounting evidence suggests that the ground state disobeys conventional rules. Alternatively, a negative charge-transfer situation24,25, where a finite density n of holes Ln is self-doped into the O 2p band and Ni takes on a 3d8 configuration (that is, Ni 3d8Ln), is recently receiving an increasing interest. This scenario is represented in Fig. 1b for Δ′<0. Notably, the negative charge-transfer picture is at the base of recent charge or bond disproportionation model theories where, as first suggested by Mizokawa26, the disproportioned insulating state is characterized by alternating Ni 3d8 (n=0) and Ni 3d8L2 (n=2) sites arranged in a lattice with a breathing-mode distortion27,28,29,30. These models distinctively differ from the more traditional charge-disproportionation ones where the Ni 3d7 lattice moves towards an alternation of Ni 3d6 and 3d8 sites in the insulating phase6,31,32,33,34.

Figure 1: Single-electron excitation spectra in terms of charge removal and charge addition.
figure 1

This sketch introduces conventional parameters used to describe charge dynamics in transition metal oxide (TMO) compounds with formal 3d7 filling: (1) charge-transfer energy Δ: energy cost for transferring an electron/hole from the L band to the Ni 3d band (with respect to the band centre of mass); (2) Hubbard U: energy cost needed to remove an electron from the occupied 3d band and to add it to the unoccupied 3d band; (3) effective charge-transfer energy Δ′: key parameter to distinguish between the two different regimes discussed here. Δ′ is defined by the equation in the figure, starting from Δ. This figure identifies the ground state (GS) and the gap character obtained for two Δ′ regimes: (a) Δ′>0. In conventional positive charge-transfer compounds the lowest energy removal states are ligand based, and the lowest energy addition states are transition metal based, leading to a charge-transfer derived energy gap (O 2p–Ni 3d like) and a 3d7 GS. (b) Δ′<0. In negative charge-transfer compounds, one hole per Ni is doped into the ligand band, giving a density of ligand holes n, Ln. The GS is here Ni 3d8Ln. The red-dashed contour bands are a cartoon-like demonstration of the opening of the gap in the mainly O 2p continuum resulting in the metal to insulator transition. In this case, the lowest energy removal and addition states are both ligand based, leading to an O 2p–O 2p like gap. Under no circumstances can this type of gap result from configuration a, unless active doping is considered. Note that this figure neglects Ni–O hybridization, to provide clear distinction between the regimes.

To get a full understanding of the MIT and of the unique physical properties of the rare-earth nickelates, it is crucial to investigate the ground-state electronic structure in this class of materials. To this purpose, we stress that while both positive and negative charge-transfer interpretations introduced above can be described as highly covalent, there are striking inherent differences between the two. For the former16,20,21,32,34, the GS can be modelled as a Ni 3d7 impurity hybridizing with a full O 2p band. Here the primary low-energy charge fluctuations that couple to the GS in first order are the ones from the O 2p to the Ni 3d7 impurity, mixing in some Ni 3d8L and higher-order character into the wavefunction. However, for the negative charge-transfer case19,25,26,27,28,29,30, all Ni sites assume a 3d8 state with on average n=2 holes in the six oxygens coordinating a central Ni ion. This case is more aptly modelled by a Ni 3d8 impurity hybridizing with a partially filled O 2p band. The electronic structure and consequently the character of the gap are vastly different in the two scenarios: with a O 2p–Ni 3d-like gap or 3d8Ln with a O 2p–O 2p-like gap (refer to Fig. 1a,b, respectively).

Here we combine two X-ray spectroscopies, namely X-ray absorption (XAS) and resonant inelastic X-ray scattering (RIXS) at the Ni L3-edge, to resolve if the electronic structure of ReNiO3 follows a positive or negative charge-transfer picture. While the XAS results are similar to those previously reported, the first ever measurements of high-resolution Ni L3 RIXS on NdNiO3 provide crucial insights into the nature of the excitations present. The unusual coexistence of bound and continuum contributions across the narrow Ni L3 resonance and the specific nature of the orbital excitations, allows us to verify that the electronic ground state contains abundant O 2p holes and that the Ni sites are indeed best described as Ni 3d8Ln, rather than a low spin Ni 3d7, showing that the ReNiO3 are indeed self-doped, negative charge-transfer materials. Further, the RIXS spectra exhibit a clear suppression of the low-energy electron–hole pair continuum in the insulating phase, providing not only a fingerprint of the opening of the insulating gap at T<TMI but also experimental evidence of the dominant O 2p-character for the states across EF, as expected for a negative charge-transfer system.


Bulk-like NdNiO3 thin film

Several high-quality NdNiO3 thin films grown on a variety of substrates were investigated. Epitaxial films were prepared by off-axis radiofrequency magnetron sputtering8,9,35,36 and were fully characterized by X-ray diffraction measurements, atomic force microscopy, transport and soft X-ray scattering measurements. In the following, we will focus on 30 nm thick NdNiO3 film grown on (110)-oriented NdGaO3 substrate under tensile strain conditions (+1.6% of strain) as a representative example of bulk ReNiO3 in general. In this case, coupled metal–insulator and paramagnetic-to-antiferromagnetic transitions have been found at T150 K, consistent with the corresponding bulk compound1.

Bound and continuum excitations across Ni L3 resonance

XAS and RIXS measurements were carried out by exciting at the Ni L3 edge, corresponding to the 2p3/2 to 3d electronic transition at around 852 eV. The XAS spectra have been acquired in the partial fluorescence yield mode, by integrating the RIXS spectra for each incident photon energy in to insure the bulk sensitivity.

Figure 2a–c presents an overview of XAS and RIXS data for the 30 nm thick NdNiO3 film, measured at both 300 K (metallic phase, red colour) and at 15 K (insulating phase, blue colour). The Ni L2,3 XAS shown in Fig. 2a is in good agreement with the previously published data on NdNiO3 (refs 20, 21, 37, 38, 39). At 15 K, the Ni L3 region of the XAS (from 850 to 860 eV), is characterized by two clear structures—a sharp peak at 852.4 eV (A) and a broader peak at 854.3 eV (B)—both of which are present in other ReNiO3 as well1,16,20,24. At 300 K both peaks are still recognizable, however, their separation is less evident.

Figure 2: Overview of XAS and RIXS measurements for a 30 nm NdNiO3 film on NdGdO3.
figure 2

(a) Ni L3,2 XAS measured in partial fluorescence yield mode at 300 K (metallic phase) in red and at 15 K (insulating phase) in blue. Refer to Supplementary Note 2 and Supplementary Fig. 2 for XAS in total electron yield mode. (b,c) RIXS intensity map measured across the Ni L3 edge at 300 K (15 K); intensity scale bar from 0 to 5 (a.u.). The white solid line displays the XAS measured at the same temperature. The letters A, B and C mark the three different incident energies mentioned in the text, while dd, CT and Fl refer to RIXS excitations of different character, also discussed in the text. The grey-dashed line indicates the incident energy giving the most pronounced changes in the RIXS map and in the XAS across the MIT. The red-dotted line provides a guide to the eye for the linearly energy dispersing Fl feature.

A series of high-resolution RIXS spectra have been recorded across the Ni–L3 resonance in steps of 0.1 eV, as shown in the intensity colour maps of Fig. 2b,c. Each spectrum obtained for a specific in measures the intensities of the emitted photons as a function of the energy loss =in-out, where out is the outgoing photon energy. RIXS is able to simultaneously probe excitations of diverse nature, for example, lattice, magnetic, orbital and charge excitations40,41. In addition, one can distinguish with RIXS between localized, bound excitations and delocalized excitations involving continua. For localized electronic excitations, the RIXS signal appears at a fixed while scanning in across a corresponding resonance (Raman-like behaviour). Conversely, for delocalized electronic excitations involving continua, the RIXS signal has a constant out and therefore presents a linearly dispersing energy loss as a function of in (fluorescence-like behaviour)40,41,42,43.

From the RIXS maps of the NdNiO3 thin film in Fig. 2b,c one directly observes a clear, strong Raman-like response at around 1 eV of energy loss when tuning in to the XAS peak A. These atomic-like dd-orbital excitations, which are sensitive to the local ligand field symmetry, behave similarly to those observed in other oxide materials like the prototypical Ni 3d8 system NiO44. A fluorescence-like contribution resonates instead at the XAS peak B, contrary to the Raman-like response dominated by multiplet effects observed in NiO at the corresponding Ni L3 XAS shoulder44. Already by looking at the colour map, this fluorescence-like spectral signature is clearly visible all across the Ni L3-edge and always with a linearly dispersing behaviour, as suggested by the red-dotted line overimposed to the data. Interestingly, the fluorescence intensity distribution in the NdNiO3 RIXS map has also a strong temperature dependence, while at 300 K it merges continuously with the dd-excitations (Fig. 2b), at 15 K a dip in intensity is created corresponding to the incident photon energy C, in=853 eV (see Fig. 2c, dashed grey line).

To gain more insight into the origin of the observed Raman- and fluorescence-like spectral response, we closely examine the individual RIXS spectra and we perform a fitting analysis to extract the general behaviour of the main spectral components. As shown in Fig. 3a, the raw RIXS spectrum is decomposed into three different contributions (see Supplementary Note 1 and Supplementary Fig. 1). Referring to the photon energy in=A, we identify from the corresponding RIXS spectrum localized dd-orbital excitations extending from 1 to 3 eV (black line), a broad background centred around 4 eV (CT, green line), and a residual spectral weight (Fl, magenta line) peaking at 0.7 eV between the elastic line and the dominating dd-profile.

Figure 3: RIXS data analysis across the MIT.
figure 3

(a) RIXS line spectra (grey open-dot line) measured at in=A and in=B at 15 K. The thin solid lines refer to Gaussian fits of dd-excitations (black), the CT excitation (green) and the Fl excitation (magenta). The blue-dashed line refers to the sum of the three fitting contributions, plus the elastic line at 0 eV. (b,c) Integrated intensity of the fit dd-, CT- and Fl-excitations together with the total integrated intensity at 15 K (300 K). The grey arrow marks the incident energy giving the most pronounced changes in the RIXS integrated intensity across the MIT. (d,e) Peak energy dispersion for the CT- and Fl-excitation at 15 K (300 K). The same colour code as in a is used throughout the figure. The error bars of the model parameters are evaluated using the least square fitting routine and expressed in s.e.d. The error bars of the initial RIXS spectra were estimated assuming Poisson statistics.

Remarkably, at this photon energy even the fine multiplet structure of the dd-excitations is in good agreement with that of NiO44, suggesting immediately that NdNiO3 has an unusual Ni 3d8-like S=1 local electronic structure similar to NiO. Figure 4 furthermore endorses this concept, displaying the comparison between the RIXS data and cluster model calculations performed for a Ni 3d7 GS (grey line, model parameters taken from ref. 39) and a crystal field calculation of the dd-excitations for a Ni 3d8 GS (black line, model parameters from NiO45; see also Supplementary Note 3 and Supplementary Table 1). The dd-excitations obtained for the Ni 3d7 case strongly differ from the present NdNiO3 data not only in the peak energy positions displaced to higher energies, but also in the intensity distribution profile, thus ruling out a Ni 3d7 GS scenario. The dd-excitations calculated for the NiO in Ni 3d8 configuration instead present a remarkably good correspondence with the present data, verifying the d8-like character of Ni in this compound: such a finding is the first key result of our study and directly poses the question if NdNiO3 deviates from a conventional positive charge-transfer picture based on a Ni 3d7 GS in favour of a negative charge-transfer scenario based on a Ni 3d8 GS, as illustrated in Fig. 1b. Finally, we note that in the insulating phase an extra dd-peak emerges from the experimental data at 0.75 eV, which is not captured by the Ni 3d8 calculation. We speculate that this contribution could be caused by symmetry-breaking phenomena (related to the presence of different Ni sites in the insulating phase). However, more advanced and detailed calculations have to be developed to reproduce this finding.

Figure 4: Comparison between experimental and calculated dd-excitations.
figure 4

Data: RIXS spectra at T=15 K (blue circles) and at T=300 K (red circles), in=A, σ polarization. Calculation: crystal field RIXS calculation for a Ni 3d8 GS based on NiO parameters45 (black line); cluster calculation for a Ni 3d7 GS using the parameters in ref. 39 (grey line). Please note that the elastic lines have been removed from the calculated spectra to better display the differences at the low energies. The experimental dd-line shape is well reproduced by the Ni 3d8 cluster calculation, supporting the negative charge-transfer scenario for ReNiO3. The good matching between data and calculation shows that: (1) there is no inversion of crystal field in ReNiO3 compared with NiO, in agreement with ref. 25 for dominating Coulomb interaction; (2) being the Ni–O distance shorter in ReNiO3 than in NiO, the negative charge-transfer energy may lead to a reduction of the expected t2g-eg splitting.

Referring now to in=B incident photon energy, the three contributions identified above for in=A—dd, CT and Fl—can be still distinguished in the corresponding RIXS spectrum. However, comparing the two spectra in Fig. 3a, we observe a shift in energy for the CT- and Fl-contributions, contrary to the dd-excitations which are fixed in energy loss, and a strong redistribution of spectral weight between the three spectral components.

To disentangle localized versus delocalized character of the RIXS excitations, we extend in Fig. 3b–e the fitting analysis to all the RIXS spectra between 852 and 858 eV incident photon energies and we track for each contribution the integrated intensity (Fig. 3b,c) and the peak energy dispersion (Fig. 3d,e; see Supplementary Note 1 and Supplementary Fig. 1). While the dd-excitations (black dots) have a Raman-like behaviour throughout the energy range and clearly resonate at in=A, the other two contributions (CT in green and Fl in magenta dots) resonate instead at in=B (see Fig. 3b, 15 K). Interestingly, and contrary to the similarity in their resonant behaviour, the CT- and the Fl-contributions present different peak energy dispersions as a function of the incident photon energy (Fig. 3d). The broad CT-peak (FWHM 6 eV) displays a behaviour characteristic of well-known charge-transfer excitations between the central Ni site and the surrounding oxygens: constant energy loss (4 eV) up to the resonant energy in=B, and a fluorescence-like linear dispersion at higher incident photon energies. The Fl-peak (FWHM 1 eV), instead, linearly disperses versus incident photon energy across the full Ni L3 resonance: as introduced above, this behaviour is a clear fingerprint for a delocalized excitation involving continua. Overall, these findings are common to both low and high temperature data sets. However, in the metallic state (see Fig. 3c,e, 300 K) the intensity of both CT- and Fl-peaks is enhanced at in=C: the resulting extra weight in the integrated RIXS intensity profile (Fig. 3c, blue dots) mimics the filling of the valley observed in the XAS spectrum at 300 K, and explains the absence of a dip in the intensity distribution of the RIXS map (Fig. 2b) at the same incident energy.

In addition, we examine the Fl-excitations more closely in Fig. 5, where we focus on the low energy loss range (<1.5 eV) of the high-statistics RIXS spectra obtained at the Ni L3 pre-peak region, starting 1 eV before peak A. In Fig. 5a, we observe changes in the dd-excitations between 300 and 15 K (across the MIT) likely due in part to local rearrangements of the NiO6 octahedra. Moreover, a sizeable spectral weight continuum around 0.2–0.5 eV (see Fig. 5a, inside the ellipse area) is present only at 300 K in the metallic phase, as better displayed by the RIXS colour maps for 300 and 15 K (see Fig. 5b,c, respectively).

Figure 5: Low-energy electron–hole pair continuum in the RIXS spectra.
figure 5

(a) RIXS line spectra measured for incident energies going from in=A-1 eV up to in=A-0.2 eV in steps of 0.1 eV at 15 K (blue) and 300 K (red). Each spectrum has been acquired for 5 min. The grey ellipse highlights the energy loss region where the electron–hole pair continuum is more prominent. (b,c), Magnification of the low energy loss region (<0.9 eV) of the RIXS map with a logarithmic intensity scale at 300 K (15 K); intensity scale bar from −3 to 1 (a.u.). The spectra have been normalized to the dd-area to have comparable background signal in the low energy loss region. The red ellipses underline the electron–hole pair continuum present at 300 K (b) and the intensity gap in the same energy window at 15 K (c).

Anderson impurity model

To understand the origin of the various RIXS excitations and their link to the electronic structure, one can employ an Anderson impurity model (AIM) interpretation (Supplementary Note 4). While the schematics in Fig. 1a,b show the single-particle removal and addition excitations for different charge-transfer scenarios, RIXS actually measures charge neutral excitations, which are well represented in a configuration interaction-based AIM. These charge neutral excitations are shown schematically in Fig. 6a for the negative charge-transfer case Δ′<0 and the positive charge-transfer case Δ′>0 (NiO like) of a Ni 3d8 impurity. As previously mentioned, for the Δ′>0 case, the only charge fluctuations possible in the AIM are from the full O 2p band to the Ni impurity level. While conserving the total charge, these fluctuations give rise to a Ni 3d9L band corresponding to charge-transfer excitations (shown in green in Fig. 6a for NiO). However, for the Δ′<0 case (recall Fig. 1b), the presence of a self-doped, partially filled O 2p density of states (DOS) extending across the Fermi level opens additional pathways for the neutral charge fluctuations. Electrons can either hop from the O 2p valence band to the O 2p conduction band leaving the Ni impurity occupation unchanged, yielding a characteristic low energy electron-hole pair continuum of m excitations d8vmcm marked in magenta (v is a hole in the valence band and c an electron in the conduction band, as shown in the small O 2p DOS inset of Fig. 6a); or, to and from the Ni impurity level, from the O 2p valence band and toward the O 2p conduction band, respectively, causing the impurity occupation to change by plus or minus one and yielding a charge-transfer like continuum of excitations at higher energy. Eventually these charge-transfer excitations can be dressed by associated electron–hole pair excitations, vmcm, resulting in d9vm+1cm or d7vmcm+1 bands of excitations (green band). We stress that the here introduced low-energy electron–hole pair excitations can be obtained only for the Δ′<0 case, where the O 2p DOS crosses EF.

Figure 6: Anderson impurity model interpretation of the RIXS and XAS spectra.
figure 6

(a) AIM schematic for charge neutral RIXS excitations. The configurations of the AIM are very different for Δ′<0 (NdNiO3) and Δ′>0 (NiO) 3d8 compounds. CT-like excitations are obtained in both cases (green bands), while Fl-like excitations (magenta band) are found only for Δ′<0 and correspond to electron–hole pair excitations as shown in the O 2p DOS inset. (b) Calculated RIXS map for the positive charge-transfer compound NiO, using the AIM. The NdNiO3 CT- and Fl-excitations dispersion curves from Fig. 3d are overlaid for comparison (green and magenta open dots, respectively), as well as the NiO CT-excitation dispersion (green solid line). Horizontal coloured lines make the connection between the RIXS excitations and the assigned interpretation in the AIM schematic of a.

The effects of these two impurity models on RIXS are detailed in Fig. 6b. The case of NiO can be solved numerically including the full correlations within the Ni 3d shell, and we show the calculated RIXS map in Fig. 6b. Comparing this to the schematic NiO configurations in Fig. 6a, we see that there are Raman-like dd-excitations below 4 eV, corresponding to reorganized Ni 3d8 orbital occupations, and a charge-transfer band at distinctively higher energy losses which is Raman-like for lower incident photon energies up to ca. 855 eV, before dispersing like fluorescence for higher photon energies. However, as the schematic in Fig. 6a suggests, the charge-transfer excitations do not extend down to low energy losses for the NiO case (Δ′>0). To gain further insight into the NdNiO3 experimental data, the extracted CT- and Fl-dispersion curves of Fig. 3d are overlaid on the calculated RIXS map in Fig. 6b. Indeed, the NdNiO3 CT-excitations (open green dots) show a similar behaviour as the NiO CT ones (solid green line). The NdNiO3 Fl-excitations, instead, with their distinctive fluorescence-like dispersion differ from any of the NiO excitations. Interestingly, the identified Fl-contribution propagating down to very low energy losses is compatible instead with the electron–hole pair continuum excitations d8vmcm coming from the broad O 2p band: this finding is the second key result of our study and naturally occurs for the negative charge-transfer case (Δ′<0) as represented in the AIM schematic of Fig. 6a (magenta band).


The main findings of the presented data analysis and interpretation are as follows: localized dd-excitations sharply resonate at the XAS peak A with a lineshape consistent with a Ni 3d8 configuration; delocalized Fl-excitations mostly resonate at the XAS peak B and are interpreted as electron–hole pair excitations across the O 2p band cut by EF (Fig. 1b, green contours); spectral weight reduction of the electron–hole pair excitations close to zero energy loss (Fig. 5b,c) suggests the opening of an O–O insulating gap (Fig. 1b, red-dashed contours) at low temperature, in line with previously reported optical conductivity46,47 studies and similarly as in more recent ARPES data48 revealing a spectral weight transfer from near EF to higher binding energies across MIT.

This collection of results clearly identifies NdNiO3 as a negative Δ′ charge-transfer material, with a local Ni 3d8 configuration49, a predominant O 2p character across the Fermi level50 and a consequent GS of mainly Ni 3d8Ln. This picture is compatible with the scenario proposed by Mizokawa26, also discussed as bond disproportionation model in recent theoretical approaches27,28,29,30,51,52, which comprises an expanded 3d8 Ni site (n=0, S=1) and a collapsed 3d8L2 Ni site (n=2, S=0) alternating in the insulating phase with the following spin order ↑0↓0 and a homogeneous Ni 3d8L (n=1) GS in the metallic phase. As underlined in previous works28,29, this model is in agreement with several breakthrough experimental findings: (1/2 0 1/2) antiferromagnetic Bragg peak in the insulating phase5; charge ordering6, which in this model is distributed among both Ni and O sites instead of only Ni sites; absence of orbital order34; evidence of strong Ni–O covalence in the GS4,20,21.

Furthermore, the different resonant behaviour extracted in this study for localized and delocalized RIXS excitations suggests that the two distinct XAS peaks marked at low temperature mostly result from the two different components of the GS, being XAS peak A mostly associated with a Ni 3d8 configuration, and XAS peak B with the delocalized ground-state Ni 3d8L2 configuration. This is in line with the energy dependence of the (1/2 0 1/2) peak resonating at in=A (refs 31, 37), here assigned to the magnetically active S=1 site.

In conclusion, by combining Ni L3 XAS and RIXS measurements we studied the electronic ground-state properties of ReNiO3, to discriminate the electronic structure between a negative and a positive charge-transfer scenario. By analysing the first ever high-resolution Ni L3 RIXS data obtained for ReNiO3, we identified the coexistence of bound, localized excitations and strong continuum excitations in both the XAS and the RIXS spectra, in contrast to earlier absorption studies which assumed primarily charge-transfer multiplet effects in the XAS. Further, we disentangled the continuum features in the RIXS spectra into charge-transfer and fluorescence excitations, showing the latter to arise due to the presence of a ground state containing holes in the oxygen 2p band. Electron–hole pair excitations from oxygen 2p states across the Fermi level have been identified down to zero energy loss, mimicking the opening of a gap for T<TMI. All these experimental observations provide clear indication of an O 2p hole-rich ground state with Ni 3d8Ln electronic configuration as the main component, as expected for a negative charge-transfer system. This GS configuration lends support to the treatment of the ReNiO3 as a S=1 Kondo or Anderson lattice problem with a Ni 3d8Ln (n=1) metallic GS, and realizing the MIT by a bond disproportionation leading to two Ni site environments: Ni 3d8 (n=0, S=1) and Ni 3d8L2 (n=2, S=0), differing in the hybridization with the O 2p hole states yet leaving the charge at the nickel sites almost equal. While this result is vital for the understanding of the rare-earth nickelate family per se, the combined XAS and RIXS approach demonstrated here opens the opportunity to classify the electronic structure for other cases of very small or negative charge-transfer gaps Δ′, which could be common to other materials with unconventionally high formal oxidation states (as for example sulfides, selenides and tellurides).


Experimental details

XAS and high-resolution RIXS measurements have been performed at the ADRESS beamline of the Swiss Light Source53, Paul Scherrer Institute. The sample has been oriented in grazing incidence, with the incoming photon beam impinging at 15° with respect to the sample surface. The scattering plane for the RIXS measurements was coinciding with the crystallographic ac-plane (or bc-plane, equivalently). All the data displayed here have been measured for incoming photons polarized parallel to the a (b) axis (also referred to as σ polarization, perpendicular to the scattering plane). For the RIXS measurements we used the SAXES spectrometer54 prepared with a scattering angle of 130° and a total energy resolution of 110 meV. The spectrometer was set in the high-efficiency configuration, using the 1,500 lines per mm VLS spherical grating. This set-up allowed acquiring around 600–800 photons at the maxima of the prominent spectral structures already in 1 min. The recorded scattered photons were not filtered by the outgoing polarization.

Data availability

The XAS and RIXS data that support the findings of this study are available from the corresponding authors V.B. and T.S. upon request.

Additional information

How to cite this article: Bisogni, V. et al. Ground state oxygen holes and the metal–insulator transition in the negative charge-transfer rare-earth nickelates. Nat. Commun. 7, 13017 doi: 10.1038/ncomms13017 (2016).