Introduction

5d transition-metal oxides exhibit various exotic physical properties arising from the strong spin-orbit coupling (SOC) that competes with Hund’s coupling and Jahn-Teller effect and strongly influences the exchange interaction1,2,3. Particularly attractive have been the Mott-insulating Ir4+ (5d5) compounds with effective angular momentum Jeff = 1/2 and the Kitaev quantum-spin-liquid candidate of Ru3+ (4d5) honeycomb lattices. Especially exotic are localized 5d2 electrons in a cubic crystal field. A d2 ion coordinated by ligand atoms in the octahedral (Oh) environment is expected to be Jahn-Teller active, but many cubic crystals with 5d2 ions remain undistorted, probably due to the strong SOC of the 5d electrons4. Such a 5d2 ion in the Oh-symmetry crystal field has a non-Kramers doublet ground state that supports either an electric quadrupole or a magnetic octupole5,6,7,8,9. This is contrasted with 5d1 systems, where the 5d ion has an electric quadrupole and Jahn-Teller distortion is induced1,2,4,7,10. As a staggered octupolar order has been predicted theoretically for quarter-filled manganites11, one may conceive disordered octupoles or a quantum octupole liquid under particular conditions in manganites or other materials.

The B-site-ordered double perovskite Ba2AOsO6, where A is an alkali-earth metal, is one of such 5d2 (Os6+) systems. The face-centered cubic (fcc) lattice formed by the Os ions may induce geometrical frustrations between the multipoles, and may lead to intriguing quantum magnetism predicted theoretically5,6,7,8,9. For example, Ba2CaOsO6 shows a cusp-like anomaly in the magnetic susceptibility at T* ~ 50 K, signaling a magnetic transition, and muon-spin rotation (μ-SR) has revealed a small magnetic moment of ~0.2 μB12 or ~0.05 μB per Os ion13 whereas neutron scattering has detected no magnetic Bragg peaks below T*12. (According to ref. 13, the small magnetic moment may be induced by impurities and may not be intrinsic.) According to X-ray diffraction, the crystal remains cubic down to the lowest temperatures14. This precludes static electric quadrupolar order, which should distort the cubic lattice10, but is consistent with magnetic octupolar order as the origin of the ‘hidden order’ in Ba2AOsO6. Theoretically, exchange coupling between neighboring Os ions favors ferro-octupolar order in the fcc lattice6.

In an Oh-symmetry crystal field, the one-electron Os 5d level is split into the t2g and eg levels separated by ΔLF [Fig. 1a]. The strong SOC splits the t2g level into the \({j}_{{\rm{eff}}}=\frac{1}{2}\) and \({j}_{{\rm{eff}}}=\frac{3}{2}\) sublevels, and the latter is occupied by the two electrons of the Os6+ ion. In the two-electron energy diagram [Fig. 1b], the ground state has the total effective angular momentum of Jeff = 2. Under the Oh symmetry, the ‘residual’ cubic crystal-field splits the Jeff = 2 quintet into the ground-state Eg doublet and the triply-degenerate T2g excited states with a separation Δc14,15. The Eg ground state is a non-Kramers doublet consisting of \(| {\psi }_{g,\uparrow }\left.\right\rangle \equiv | {J}_{{\rm{eff}}}^{z}=0\left.\right\rangle\) and \(| {\psi }_{g,\downarrow }\left.\right\rangle \equiv \frac{1}{\sqrt{2}}(| {J}_{{\rm{eff}}}^{z}=2\left.\right\rangle +| {J}_{{\rm{eff}}}^{z}=-2\left.\right\rangle )\), whereas the T2g excited states consist of \(| {\psi }_{e,\pm }\left.\right\rangle \equiv | {J}_{{\rm{eff}}}^{z}=\pm 1\left.\right\rangle\) and \(| {\psi }_{e,0}\left.\right\rangle \equiv \frac{1}{\sqrt{2}}(| {J}_{{\rm{eff}}}^{z}=2\left.\right\rangle -| {J}_{{\rm{eff}}}^{z}=-2\left.\right\rangle )\). In the ferro-octupole-ordered state, all the Os ions are in one of the two eigenstates, \(| {\psi }_{g,\pm }\left.\right\rangle \equiv \frac{1}{\sqrt{2}}(| {\psi }_{g,\uparrow }\left.\right\rangle \pm i| {\psi }_{g,\downarrow }\left.\right\rangle )\), of the octupole operator \({T}_{xyz}\propto \overline{{J}^{x}{J}^{y}{J}^{z}}\), where the overline denotes symmetrization.

Fig. 1: Energy diagrams of the Os6+ (5d2) ion in the cubic (Oh) crystal field.
figure 1

a One-electron energy diagram. ΔLF is the t2g-eg splitting. Spin-orbit coupling (SOC) further splits the t2g level into \({j}_{{\rm{eff}}}=\frac{1}{2}\) and \({j}_{{\rm{eff}}}=\frac{3}{2}\) levels separated by \(\frac{3}{2}\zeta\), and the \({j}_{{\rm{eff}}}=\frac{3}{2}\) level is occupied by two electrons. b Two-electron energy diagram. The \({t}_{2g}^{2}\) part of the d2 multiplet is shown whereas the t2geg part is located at higher energies separated by ~ ΔLF. Due to the ligand field (LF) of cubic symmetry, the Jeff = 2 ground state is split by a ‘residual’ cubic splitting Δc into the non-Kramers Eg doublet and the T2g triplet. The first Jeff = 0 excited state appears ΔE ~ 0.4 eV above the ground state, and the first Jeff = 1 excited state ~ 0.065 eV above it.

While the magnetic properties of Ba2AOsO6 double perovskites have been widely studied and microscopic models to explain the observed anomalies have been proposed, their electronic structure remains unexplored experimentally. The present paper aims to fill this gap. In particular, we studied Ba2CaOsO6 by X-ray absorption spectroscopy (XAS) and resonant inelastic X-ray scattering (RIXS) at the O K edge. RIXS studies of 5d transition-metal oxides have so far been performed mainly at the transition-metal L2,3 edge since one can directly study the spin and orbital excitation of the 5d states16,17,18,19. However, owing to the strong SOC of the 5d electrons, RIXS at the O K edge can also be used to study spin excitations [Fig. 1b]20,21,22,23,24. O K-edge RIXS has the advantage of having higher energy resolution than transition-metal L2,3-edge RIXS, allowing us to study low-energy electronic excitation and electron-phonon interaction. We have also utilized Raman scattering to detect possible local lattice distortion that induces low-symmetry crystal fields. None of the above measurements have indeed shown evidence for the lowering of the cubic symmetry, favoring the scenario that the Os ions have dominantly octupolar moments in Ba2CaOsO6.

Results and analyses

We performed O K-edge RIXS on high-quality polycrystalline samples with the energy resolution of ~30 meV using π polarized X-rays and 90° scattering angle (see Methods). The O K-edge XAS spectrum is shown in Fig. 2a. Figure 2b shows the RIXS intensity map in the Ein-Eloss plane, where Ein is the energy of incident X-ray and Eloss is the energy loss of scattered X-rays. The same data are plotted in the Ein-Eem plane in Fig. 2c, where Eem is the energy of emitted X-ray. RIXS spectra are plotted in Fig. 2d. In the figure, above Ein ~ 529 eV, some spectral features start to shift to higher Eloss with increasing Ein, indicating a cross-over from Raman-like to fluorescence-like.

Fig. 2: X-ray absorption spectroscopy (XAS) and resonant inelastic X-ray scattering (RIXS) spectra of Ba2CaOsO6 at the oxygen K edge recorded at 25 K.
figure 2

a XAS spectra. Top: XAS spectrum measured using the total fluorescence-yield method. The broad absorption band at 532–536 eV consists of transitions to the empty eg states (blue dashed curve) as well as to the Ba 5d- and Ca 3d-derived conduction-band states. The blue dashed curve is the partial fluorescence-yield spectrum measured at Eem = 528 eV. Bottom: Spectrum calculated using ligand-field (LF) multiplet theory. See Methods. b, c Colored intensity maps of scattered X-rays: b as a function of incident X-ray energy Ein and energy loss Eloss. Solid lines mark the positions of constant Eloss. Dashed lines indicate those of constant Eem, c Scattered X-ray intensity map plotted against Ein and emission energy Eem. Dashed lines indicate constant Eem’s, corresponding to fluorescence from occupied states to the O 1s core level. d RIXS spectra measured for various Ein’s indicated by vertical bars at the top spectrum of (a). The shaded parts mark transitions from O 2p → Os 5d charge-transfer (CT) excitation. e LF multiplet calculation to simulate the RIXS spectra. The red curves show spectra arising from d-d excitation for a series of Ein’s indicated by vertical bars in the calculated O K-edge XAS spectrum shown at the bottom of (a). The dashed blue curves show O 2p → Os 5d CT excitation simulated by 5d2 → 5d3 multiplet calculation. The black curve is the measured RIXS spectrum for Ein = 528.5 eV [spectrum d in panel (d)].

Splitting due to ligand field and spin-orbit coupling

In O K-edge RIXS, the excitation of the O 1s core electron into empty states followed by the electron transition from the non-bonding O 2p band to the O 1s core level leaves a hole in the non-bonding O 2p band and an electron in the empty states. The resulting final state is equivalent to that of the O 2p → Os 5d charge-transfer (CT) excitation, which measures the unoccupied part of the O 2p partial density of states (PDOS). Because the energy position of the non-bonding O 2p band is located near the top of the O 2p band, we assumed it located ~ 2 eV below the Fermi level (EF), based on the occupied O 2p PDOS deduced from fluorescence spectra as discussed below. Thus one finds the eg band 4-6 eV above EF, the \({j}_{{\rm{eff}}}=\frac{1}{2}\) band ~ 1 eV above EF, the empty and occupied parts of the \({j}_{{\rm{eff}}}=\frac{3}{2}\) band just above and below EF, respectively.

The occupied part of the O 2p PDOS can be measured by the fluorescence component of the O K-edge RIXS. We have taken spectrum k in Fig. 2d as the representative fluorescence spectrum. The EF position for the fluorescence spectrum has been fixed under the assumption that Eem = 528.2 eV is the excitation threshold of the O K-edge XAS [photon energy c in Fig. 2a]. The combined occupied and unoccupied parts of the O 2p PDOS thus derived are plotted in Fig. 3a.

Fig. 3: O 2p partial density of states (PDOS) derived from experiment and theory.
figure 3

a Experimental O 2p PDOS. The empty part is derived from the O 2p → Os 5d CT excitation in the RIXS spectrum [Ein = 528.2 eV, c in Fig. 2d], and the occupied part from the fluorescence component of the RIXS spectrum [Ein = 534.6 eV, k in Fig. 2d]. The shaded part marked by “dd” arises from \({t}_{2g}^{2}\to {t}_{2g}{e}_{g}\) transition, and is unrelated to the O 2p PDOS. b PDOS of the nonmagnetic state obtained by the GGA+U+SOC calculation with UJH = 2.5 eV.

The obtained O 2p PDOS is compared with the DOS calculated by DFT (see Methods) in Fig. 3b. One can see good one-to-one correspondence between the experimental and calculated structures in the O 2p PDOS. In particular, the assumed non-bonding O 2p-band position well agrees with the peak position of the calculated non-bonding O 2p band. Nevertheless, the conclusion of the present paper will not be altered by the magnitude of the band gap unless it collapses and the system becomes metallic.

Low-energy multiplet and phonon satellites

In order to examine the effect of electron-phonon coupling and possible low-symmetry crystal field, an enlarged plot of the RIXS spectra in the low-energy region is shown in Fig. 4a. The “elastic” peak at Eloss = 0 eV is a superposition of the genuine elastic scattering (which should be very weak for the present π scattering geometry) and low-energy (0–20 meV) elastic and quasi-elastic scattering between the nearly degenerate five components of the Jeff = 2 ground state [see Fig. 1b]. The sharp peak at Eloss ~ 0.4 eV is due to excitation from the Jeff = 2 ground state to the Jeff = 0 and 1 excited states. The latter excitation is also observed by Raman scattering as described below. The weak peak at Eloss ~ 0.8 eV is an excited state of the \({t}_{2g}^{2}\) multiplet having the quantum number Jeff = 2 [Fig. 1b]. Unfortunately, the residual cubic splitting Δc of the Jeff = 2 state [Fig. 1b] is too small to be resolved in the RIXS spectra. Each of the quasi-elastic, Eloss ~ 0.4 eV, and ~ 0.8 eV peaks are accompanied by sub-peaks with ~ 80 meV intervals on the higher-energy side. These sub-peaks are attributed to phonon replicas, as described below.

Fig. 4: Low-energy excitations measured by O K-edge RIXS.
figure 4

Δc is the ‘residual’ cubic splitting of the Jeff = 2 ground state defined in Fig. 1b. a RIXS spectra in the low energy-loss region at different temperatures across the magnetic transition at T* ~ 50 K for the incident photon energy of 528.5 eV. The d-d excitation shown in Fig. 1b is seen. The energy-loss peaks as well as the quasi-elastic peaks are accompanied by multiple phonon satellites. The splitting Δc ~ 20 meV is not resolved in the spectra. Details of the line-shape analysis are given in Supplementary Note 1 with Supplementary Fig. 1 and Supplementary Table 1. b Energies of low-lying excited states of the Os6+ (5d2) ion as functions of the low-symmetry D4h LF parameter 6Cp26, the splitting of the t2g level. The Oh LF parameter ΔLF is set to 4.1 eV. 6Cp 0.15 reproduces the low-energy excitation in the O-K RIXS spectra of the 5d1 double perovskites22,23.

Analyses using ligand-field multiplet theory

The magnitude of the SOC of the Os 5d states can be estimated from the O K-edge XAS [Fig. 2a]. X-ray absorption into the empty t2g state observed at 528–530 eV is split into double peaks separated by \(\frac{3}{2}\zeta \sim\) 0.7 eV. Note that for the effective angular momentum operator leff, the SOC constant \({\zeta }^{{\prime} }\), defined through the SOC energy \({\zeta }^{{\prime} }{{\bf{l}}}_{{\rm{eff}}}\cdot {\bf{s}}\), is given by \({\zeta }^{{\prime} }\equiv -\zeta\) because leff ≡ − l for the t2g electrons25, where l is the bare angular momentum operator. The cubic ligand-field (LF) splitting ΔLF of the Os 5d level into t2g and eg [Fig. 1a] can also be estimated from the O K-edge XAS. From the broad absorption feature at 532–536 eV, the eg component could be isolated by monitoring the RIXS intensity of the Jeff = 2 (\({t}_{2g}^{2}\)) → t2geg energy-loss feature at Eloss ~ 5 eV [marked by a solid line in Fig. 2b] as a function of Ein: Thus obtained intensity plotted by the blue dashed curve at the bottom of Fig. 2a gives the eg component, allowing us to obtain ΔLF 4 eV.

To interpret the RIXS spectra quantitatively, LF multiplet calculations were performed and their results are shown in Fig. 2e. (For details, see Methods.) The calculated d2 multiplet (red curves) reproduces the observed loss peaks at Eloss ~ 0.4 and 0.8 eV (\({t}_{2g}^{2}\) part), and those at Eloss ~ 4 eV (t2geg part). The RIXS spectra in the blue shaded parts, Eloss 2–4 and 6–7 eV, cannot be reproduced by the d2 multiplet. We attribute these features to O 2p → empty Os 5d CT excitation, and simulate the CT excitation spectrum by d2d3 multiplet calculation of inverse-photoemission leaving a hole in the non-bonding O 2p band. By assuming that the non-bonding O 2p band is located ~ 2 eV below EF, as indicated by the DFT calculation, and by ignoring the p-band width, we could reproduce the CT spectrum from the Jeff = 2 ground state and plotted it by dashed blue curves in Fig. 2e. The Eloss 2–4 eV region arises from O 2pt2g excitation and the Eloss 6–7 eV region arises from O 2peg CT excitation.

Note that there are no features in the RIXS spectra that indicate the lowering of the cubic symmetry: If the LF symmetry were lower than the cubic one, the Jeff = 2 ground state, which is split into the doublet Eg and the triplet T2g [Fig. 1b], would be further split into multiple states as shown in Fig. 4b for cubic (Oh)-to-tetragonal (D4h) symmetry lowering, and the low-energy part of the RIXS spectra would be significantly different from the experimental ones in Fig. 4a. If the tetragonal distortion were comparable to that of the 5d1 double perovskites Ba2NaOsO622 and Ba2MgReO623, which show peak at Eloss ~ 0.1 eV in the O K-edge RIXS spectra, the tetragonal crystal field 6Cp, which is equal to the tetragonal splitting of the t2g level26 should be as large as ± 0.15 eV, and the quasi-elastic Jeff = 2 → Jeff = 2 peak would be split into a few peaks over an energy range of ~ 0.1 eV in addition to the phonon satellites. The absence of temperature dependence in the spectral line shapes across the magnetic transition at T* ~ 50 K suggests that the magnetic transition does not involve any appreciable structural change. Furthermore, there are no spectral features that can be attributed to magnons nor bi-magnons, consistent with the absence of spin order in Ba2CaOsO6.

The octupolar nature of the ground state of the Os6+ ion in the Oh field can be demonstrated by LF multiplet calculation with a weak magnetic field in the (1,1,1) direction as a time-reversal symmetry-breaking perturbation that splits the non-Kramers Eg doublet into \(| {\psi }_{g,+}\left.\right\rangle\) and \(| {\psi }_{g,-}\left.\right\rangle\). For B = 10 T, we obtained octupolar moment \({T}_{xyz}\equiv \langle \overline{{J}^{x}{J}^{y}{J}^{z}}\rangle \simeq\) 1.2 with a tiny dipole magnetic moment of ~ 8 × 10−3μB induced along the (1,1,1) direction on top of the octupolar ground state. For a smaller field of B = 1 T, the induced dipolar moment was as small as ~ 7 × 10−4μB. Generally, for a small field B Δc/μB, the induced magnetic dipole moment along the direction of B (~μBB/Δc) is proportional to B. While ordering with the finite magnetic octupolar or electric quadrupolar moment can occur within the Eg ground state, the appearance of a finite magnetic dipolar moment requires hybridization between the Eg and T2g states. Thus, to obtain a stable magnetic dipole order by the exchange interaction, a molecular field of μBB > Δc at least is required.

Phonon Raman scattering

To further confirm the absence of low-symmetry crystal field, we employed Raman scattering spectroscopy, a sensitive probe of lattice symmetry. Figure 5a shows one-phonon Raman spectra of a Ba2CaOsO6 polycrystal taken at 80 K with two polarization geometries ( and ; for technical details, see Methods). There must be phonons of A1g + Eg + T1g + 2T2g + 5T1u + T2u symmetries at the Brillouin-zone center in case of cubic \({\rm{Fm}}\bar{3}{\rm{m}}\) structure, out of which four (A1g, Eg, and 2T2g) phonons are Raman-active.

Fig. 5: Raman spectra in two scattering symmetries.
figure 5

(red) and (black) are presented. a Frequency range with one-phonon excitation. b Extended frequency range where the high-order phonon processes (blue arrows show features originating from the A1g branch, black - another weak two-phonon features) and electronic excitation are seen. The latter seen in the range from 3000 to 5000 cm−1, as shown in the inset, most probably due to the Jeff = 2 ground state to the Jeff = 1, 0 excited states seen by RIXS (Fig. 4).

To obtain information about the symmetry of the observed excitation, polarization measurements were performed in two geometries - with parallel () and with mutually perpendicular () polarizations of the incident and scattered light. We utilized the rules that in isotropic or cubic systems the depolarization ratio ρ = I/I does not exceed 0.75 for totally symmetric modes, while it is close to 0.75 for non-totally symmetric ones27. One can see that the line at ~ 796.5 cm−1 obviously dominates in the spectrum and can be assigned to the A1g mode, while the phonons at frequencies 102.5, 375, and 495 cm−1 are observed in both polarized and depolarized spectra and are assigned to T2g, T2g, and Eg modes, respectively, with the help of the non-magnetic DFT calculation of phonon modes as described in Supplementary Note 2 with Supplementary Fig. 2. The broad peak at 720 cm−1 has a fairly low depolarization ratio (~0.2), which suggests its A1g symmetry. While its origin is not clear, the symmetry lowering cannot split the A1g mode without the increase of the unit cell. (Note also that the second intensive T2g mode remains unsplit.) The appearance of this low intensity A1g peak can be, e.g., due to imperfections of the crystal structure (e.g. there are indications of anti-phase boundary defects with disorder at the B sites and other types of defects28,29,30,31) or a two-phonon repetition of 375 cm−1 vibration. Thus, our Raman experiments do not detect any direct evidence of the symmetry lowering in the cubic Ba2CaOsO6.

To examine the possible lattice distortions across T* ~ 50 K, we measured spectra at 10 K with better resolution and found only minor changes in the spectrum, such as further hardening and narrowing of the A1g mode at ~ 796.5 cm−1. Interestingly, the frequency and unique line width of the low-frequency T2g mode did not change in the whole temperature range of 10–300 K.

The higher frequency range from 800 to 3000 cm−1 presented in Fig. 5b shows several peaks dominating in the geometry and hence of the A1g symmetry. The weak peaks at 870 and 1055 cm−1 indicated by black arrows are probably two-phonon features. The peaks at 1450, 1540 and 2310 cm−1 shown by blue arrows can be associated with double and triple phonon scattering from the A1g phonon branch. At higher frequencies (>3000 cm−1), two broad peaks are observed. They are clearly seen in both polarization geometries ( and ), as well as upon excitation by both used laser lines (532 and 633 nm, see Methods), which indicates Raman scattering by electron excitations of T2g or Eg symmetry. Their energies agree well with the Jeff = 2 → Jeff = 0, 1 RIXS peaks (Fig. 4).

Typically, in the case of 5d2 double perovskites, the effect of tetragonal distortions on the ground state is considered due to their stronger coupling with electronic structure32. Interestingly, Rayyan et al.33 included the trigonal distortions in their analysis and demonstrated that, while these distortions are unable to split the Eg doublet due to symmetry constraints, they can lift the degeneracy of the higher-lying T2g triplet. Under trigonal distortions, some of these T2g states go to a lower energy. However, as shown in ref. 33 there is a rather wide range of trigonal distortion under which the non-Kramers Eg doublet remains the ground state. This doublet may, therefore, survive as the ground state under a small lattice distortion. It is also possible that distortion is substantially reduced due to dynamical Jahn-Teller effect. Whether the Eg doublet hosts an electric quadrupole or a magnetic octupole or both depends on the type of broken symmetry (spatial symmetry or time-reversal symmetry) and the strength of the mean field from neighboring Os ions.

Electron-phonon coupling effects on RIXS

In the low-energy RIXS spectra shown in Fig. 4, the quasi-elastic peak and the peak at Eloss 0.4 eV are accompanied by sub-peaks separated by ~80, 160, and 240 meV with decreasing intensities. We attribute the sub-peaks to phonon replicas created by the simultaneous excitation of optical phonons. The one-phonon energy of ~80 meV is somewhat lower but in a similar range as the Raman A1g mode energies 720 cm−1 = 88 meV and 796.5 cm−1 = 99 meV. The replica energies are close to those observed in the RIXS spectra of Ba2NaOsO622. From the replica intensities, the dimensionless electron-phonon coupling constant is estimated to be M/ω0 1, where M is the average electron-phonon coupling matrix element and ω0 is the phonon energy34. In spite of the moderately strong coupling, Jahn-Teller distortion is suppressed in Ba2CaOsO6 due to the strong SOC and dynamical Jahn-Teller effect, suggesting that Os-Os exchange interaction is strong enough to stabilize the magnetic octupole over the electric quadrupole. Here, it should be noted that sub-peaks similar to the phonon replicas may appear in the RIXS spectra if dynamical Jahn-Teller effect35 exists, as reported for the 5d1 system Ba2CaReO618,19. Whether such an effect also exists in 5d2 systems or not is an interesting question to be pursued in future studies. Considering the different time scales of RIXS (on the order of 0.01 fs) and Raman scattering (>10 fs), it is possible that dynamical Jahn-Teller effect was seen in RIXS as the “phonon replicas” but not in Raman scattering.

Discussion

We have investigated the electronic structure of Ba2CaOsO6 by XAS, RIXS, and Raman scattering experiment as well as DFT calculation, focusing on extracting reliable parameters characterizing the systems, as summarized in Table 1, and on the confirmation of the local cubic symmetry of the Os ions that favors the octupolar state as the origin of its ‘hidden order’. We have also confirmed the octupolar nature of the non-Kramers Eg doublet ground state (Sz = 0 and Lz = 0 under an infinitesimally small magnetic field) by LF multiplet calculation.

Table 1 Parameter values for the Os 5d electrons hybridized with O 2p orbitals in Ba2CaOsO6 derived in the present XAS and RIXS spectra

Owing to the hybridization between the O 2p and Os 5d orbitals, electronic excitation within the 5d2 multiplet and charge-transfer excitation from the occupied O 2p to the empty Os 5d states could be identified by the O K-edge RIXS. From comparison of the XAS and RIXS line shapes with the LF multiplet calculation, the absence of splitting of low-energy RIXS peaks as well as the lack of additional lines in Raman scattering spectra, we conclude that no crystal field lower than the cubic one can be identified, consistent with the small (~20 meV) residual cubic splitting of the Jeff = 2 ground state. The present results obtained by different types of X-ray and optical spectroscopy, which are typically very sensitive to a local environment of transition metals, substantially strengthen previous findings, in particular diffraction data demonstrating the absence of non-cubic distortions14.

There are two possible mechanisms working hand-in-hand in suppressing the Jahn-Teller distortion expected for the Os6+ ion with the d2 configuration. In both mechanisms, the strong SOC is involved. One is an on-site effect related to the stabilization of electrons not at cubic harmonics as the crystal field (i.e. Jahn-Teller effect) would prefer, but rather on entangled spin-orbitals4,36. Our RIXS measurements clearly resolved phonon replicas of the Jeff = 2 → 1, 0, 2 excitation peaks. This allowed us to estimate the electron-phonon coupling strength, which turns out to be moderately strong, M/ω0 1 and, therefore, may not be sufficiently strong to recover the Jahn-Teller distortion but might induce dynamical Jahn-Teller effect. On the other hand, there is also inter-site effect – the energy gain due to exchange interaction between the octupoles, which are formed by SOC. Further spectroscopic and theoretical studies are necessary to identify the octupolar order and its microscopic origin.

Methods

Materials preparation

Polycrystalline Ba2CaOsO6 was synthesized through a solid-state reaction using fine powders of BaO2 (99% purity, Kojundo Chemical Laboratory Co., Ltd.), CaO2 (prepared in the laboratory37), and Os (99.95% purity, Nanjing Dongrui Platinum Co. Ltd.) in a ratio of 2:1:1. Approximately 200 mg of the mixed materials were placed into an alumina crucible. The mixture was then heated in air to 1000 °C for 7 hours, followed by a 1-h dwell time, and subsequent cooling to room temperature over a span of 7 h. After re-mixing and pressing, the sample was annealed at 1000 °C for 24 h. The resulting product is a gray sintered pellet, possessing sufficient solidity to be manipulated with tweezers. Powder X-ray diffraction analysis was performed using Cu Kα radiation within the 5° ≤ 2θ ≤ 65° range at 293 K. The measurements were conducted with a MiniFlex600 diffractometer (Rigaku, Tokyo, Japan). The acquired data, shown in Supplementary Fig. 3, exhibited good agreement with simulations based on the crystallographic data of Ba2CaOsO612, confirming the single-phase nature of the product.

Resonant inelastic X-ray scattering

All resonant inelastic X-ray scattering (RIXS) and X-ray absorption spectroscopy (XAS) measurements at the O K edge were performed using the AGM-AGS spectrometer of beamline 41A at Taiwan Photon Source of National Synchrotron Radiation Research Center (NSRRC)38. This beamline is based on the energy compensation principle of grating dispersion39. The energy bandwidth of incident X-ray was 0.2 eV (0.1 eV for XAS measurement) while keeping the total energy resolution of RIXS as 30 meV at the incident photon energy of 528.5 eV. The sample surface was cleaned by scraping with a diamond file in the Ar glove box before the measurement and was transferred into the measurement chamber without exposure to the air. The base pressure of the measurement chamber was ≤1 × 10−8 Torr. The sample was cooled down to 25 K with liquid helium during the measurements. Both RIXS and XAS measurements were carried out using linear horizontally (π) polarized X-rays. The XAS spectra were measured with a normal-incident X-ray in the total fluorescence yield mode. For the RIXS measurement, the incidence angle was fixed at 20°, and the scattering angle was fixed at 90°. The combination of the π-polarized X-rays and the 90° scattering angle makes the RIXS signals purely magnetic. The same geometry also allowed us to reduce the elastic peak and to study low-energy excitation effectively.

Ligand-field multiplet calculation

Ligand-field multiplet (LF) calculations were performed by using the XTLS 8.5 package40. In the calculation of the O K-edge RIXS spectra, we assumed that the excited states of the 5d2 multiplet can be reached by O K-edge RIXS through the strong Os 5d-O 2p hybridization and could be simulated by the calculation of Os L2,3-edge RIXS by setting the 2p-5d Slater integrals and the Os 2p core-level SOC to zero. While this simulation would give the energy positions of RIXS features correctly, it would not give correct intensities because relevant transition-matrix elements are not used. The O K-edge XAS [Fig. 2a] was also simulated by the Os L2,3-edge XAS in the same manner.

In general, the Slater integrals F’s and G’s (anisotropy of Coulomb interaction) and the SOC coupling constant ζ in solids are smaller than those of isolated atoms, because the wavefunctions are more spatially extended due to hybridization. In order to model this effect, the atomic Slater integrals and ζ, deduced from Hartree-Fock calculations41,42, were multiplied by constant factors RSlater and RSOC (0 ≤ RSlater < 1, 0 ≤ RSOC < 1), respectively. These factors RSlater and RSOC and the cubic LF splitting ΔLF were treated as adjustable parameters. For O K-edge RIXS, ζ = 0.50 eV and ΔLF = 4.1 eV were used, and the Slater integrals between the Os 5d orbitals were reduced to 35% of the atomic Hartree–Fock values. Hund’s coupling JH between two d electrons (Table 1) is related to Slater integrals through \({J}_{{\rm{H}}}=\frac{3}{49}{F}^{2}+\frac{20}{441}{F}^{4}\)43. The value JH = 0.27 eV in the table is smaller than JH = 0.5 eV used for the DFT+U+SOC calculation because the former is for the Os 5d-O 2p anti-bonding orbitals while the latter for the Os 5d atomic orbitals. The reduction of JH from 0.5 eV to 0.27 eV suggests that the atomic orbitals consisting of the antibonding t2g band have the weight Os 5d: O 2p ~70%: 30%.

In the calculation of the RIXS spectra, the same geometry as the experiment was adopted: The incident and scattered X-rays were set parallel to the cubic [001] and [100] directions, respectively. Taking the [001], [100], and [010] directions as the z, x, y axes, respectively, the linear polarizations of the incident and scattered X-rays were set to be (x, y) and (x, z), and the spectra for these two polarization sets were averaged.

The calculated spectra were broadened by a Voigt function, which is the convolution of a Lorentz function and a Gauss function. The widths (half width at half maximum, HWHM) of the Lorentz functions were determined from the natural lifetime of the core holes: 0.05 eV for the O K-edge RIXS44. The widths (standard deviation) of the Gauss functions were assumed to be 0.01 eV. The XAS and RIXS spectra were calculated for the five lowest states [the lowest Jeff = 2 state in Fig. 1b] as the initial state and were summed up according to the Boltzmann distribution of the initial states.

Raman spectroscopy

Raman measurements in the 10–300 K range were performed in backscattering geometry from the polycrystalline sample using an RM1000 Renishaw microspectrometer equipped with a 532 nm solid-state laser and 633 helium-neon laser. Very low power (up to 1 mW) was used to avoid local heating of the sample. A pair of notch filters with a cut-off at 60 cm−1 were used to suppress light from the 633 nm laser line. To reach as close to the zero frequency as possible, we used a set of three volume Bragg gratings (VBG) at 532 nm excitation to analyze the scattered light. The resolution of our Raman spectrometer was estimated to be 2–3 cm−1.

The temperature dependence of the two narrow lines in the spectrum [Fig. 5a] turned out to be opposite. The fully symmetric line softened from 797.5 to 788.5 cm−1 with an increase in the temperature range from 10 to 300 K, and its width increased from 6.5 to 12 cm−1, which can be explained by anharmonicity effects. In contrast to this behavior, the energy and width of the low-frequency T2g phonon line remains constant within the measurement error (ω ~ 102.5 cm−1 and Γ ~ 1.5 cm−1) when heated from 10 to 300 K. Unfortunately, the temperature behavior of the two broad lines - T2g at 375 cm−1 (Γ ~ 20 cm−1) and Eg at 495 cm−1 (Γ ~ 60 cm−1) - is difficult to study due to their weak intensity. However, despite the large width of the lines, we did not find any signs of their splitting.

Density-functional-theory calculation

The generalized gradient approximation (GGA) in the form proposed by Perdew, Burke, and Ernzerhof45 as realized in VASP code46 was used for the density functional theory calculations. Phonon spectra shown in Supplementary Fig. 2 were calculated by the frozen phonon method47 with 5 × 5 × 5 mesh of the Brillouin zone of the 2 × 2 × 2 supercell in non-magnetic GGA. Planewave cut-off was set up to 500 eV. The structure was relaxed until convergence in energy of 10−6 eV in electronic subsystem and 10−5 eV in ionic one was achieved.