The interplay between the quasi 1-dimensional CuO-chains and the 2-dimensional CuO2 planes of YBa2Cu3O6+x (YBCO) has been in focus for a long time. Although the CuO-chains are known to be important as charge reservoirs that enable superconductivity for a range of oxygen doping levels in YBCO, the understanding of the dynamics of its temperature-driven metal-superconductor transition (MST) remains a challenge. We present a combined study using x-ray absorption spectroscopy and resonant inelastic x-ray scattering (RIXS) revealing how a reconstruction of the apical O(4)-derived interplanar orbitals during the MST of optimally doped YBCO leads to substantial hole-transfer from the chains into the planes, i.e. self-doping. Our ionic model calculations show that localized divalent charge-transfer configurations are expected to be abundant in the chains of YBCO. While these indeed appear in the RIXS spectra from YBCO in the normal, metallic, state, they are largely suppressed in the superconducting state and, instead, signatures of Cu trivalent charge-transfer configurations in the planes become enhanced. In the quest for understanding the fundamental mechanism for high-Tc-superconductivity (HTSC) in perovskite cuprate materials, the observation of such an interplanar self-doping process in YBCO opens a unique novel channel for studying the dynamics of HTSC.
One of the most intriguing problems that remain to be solved in correlated electron physics is finding the mechanism of high Tc-superconductivity (HTSC). The discovery of HTSC was made first for the cuprate perovskites that consist of planes of edge-sharing CuO2 square plaquettes separated by layers containing rare-earth metals and oxygen. A transition to superconductivity below the critical temperature can be detected e.g. by electric conductivity measurements or by the response to an external magnetic field1. Fig. 1A shows the magnetic susceptibility of the optimally-doped compound YBa2Cu3O6.9 as a function of temperature with a transition temperature of Tc = 90.5 K. YBa2Cu3O6+x (YBCO) is a unique case for a superconducting cuprate because the planes of corner-sharing CuO2 plaquettes are linked by additional layers consisting of one dimensional CuO3 chains that are linked by apical oxygen, i.e. O(4) in Fig. 1B. The O(4) 2pz-orbitals hybridize with Cu(1) -orbitals in the chains and with Cu(2,3) -orbitals in the planes. The CuO3 chains of YBCO can be more or less complete depending on the oxygen doping (oxygenation) level (x = [0,1]). Oxygenation leads to transfer of charge carriers (holes) between the chains and planes and thereby tunes the in-plane conductivity via the hole density of the CuO2 planes2. Theoretically, the application of pressure3 increases charge transfer between the planes and the chains. Ab initio local spin density functional calculations have also found a strong coupling between the valence fluctuations of the chain-Cu and the bridging O(4) ions in highly doped YBCO4. This is significant because antiferromagnetic spin fluctuations5, phonons6, and polarons7 are all candidates that may have an influence on the Cooper pairing mechanism in the CuO2 planes. It is also generally recognized that unconventional d-wave symmetry8,9 and charge stripes may be involved. Recently, a pairing model based on magnetic interactions has been scrutinized10 with resonant inelastic x-ray scattering (RIXS) by studying the spin excitation spectrum of YBCO at different doping levels.
Charge-density modulations along the CuO3 chains suggest that the surface CuO chain band develops a short-range charge density wave state as a result of a Peierls instability11,12. Discoveries in the band structure from highly surface sensitive angular resolved photoelectron spectroscopy (ARPES)13,14 have been used to explain the in-plane anisotropy of YBCO12,15 but the technique is less suitable to determine bulk properties. By contrast, x-ray absorption spectroscopy (XAS) is a powerful technique to study the character and density of hole states in the bulk. Early XAS studies of YBCO15,16 have revealed large changes in the hole distribution between the CuO2 planes and the CuO3 chains as a function of oxygen doping. It would be desirable to also gain a detailed understanding of the temperature dependent XAS spectrum across the metal-superconducting transition (MST).
In this work, we present evidence of the dynamic nature of the chain-plane charge transfer as part of the metal-to-superconductor transition of YBCO. It is accompanied by electronic reconstruction of the hybridized Cu(1)-O(4)-Cu(2)-orbitals (Fig. 1B). In effect, the CuO2-planes undergo a self-doping due to a simultaneous configuration interaction between the Cu(1)- and the Cu(2)-sites (Fig. 1C). Thus our study reveals that self-doping is a crucial ingredient for metal-to-superconductor transition and HTSC in YBa2Cu3O6.9.
Figure 2 (left panel) shows Cu L3-XAS data from optimally doped YBCO, measured across the metal-superconducting transition (MST). The XAS and RIXS measurements were performed at the Advanced Resonant Spectroscopies (ADRESS) beamline17 at the Swiss Light Source (SLS), Paul Scherrer Institut, Switzerland, using the Super-Advanced X-ray Emission Spectrometer (SAXES)18. The XAS spectra have been measured in the bulk-sensitive total fluorescence yield (TFY) mode using polarization in-plane (E||ab) or out of plane (E||c), respectively. At the Cu 2p edge, the excitation process creates a 2p core hole at the metal site. While the main peak at 930.7 eV can be assigned to the 3d9→2p53d10 transition, the satellites around 932.4 and 933.4 eV are due to metal-to-ligand charge transfer (MLCT) transitions on the Cu(2)- and Cu(1)-sites of the planes and the chains, respectively19,20.
We find a strong temperature dependence of the spectral weight around the main peak but the most striking observation is that, regardless of the x-ray polarization direction, there are opposing intensity trends in the “chains satellite” and the “planes satellite” upon cooling. This suggests the intriguing possibility that there is a temperature driven redistribution of charge between the planes and the chains of YBCO. The spectral difference in percentages displayed in the figure are derived from the hatched areas relative to the total area (taking into account the atomic step between L3 and L2) under the room temperature spectra. The difference highlights the opposing behavior of the satellites in the MST. Formally, Cu ions in YBa2Cu3O6.9 have a charge state of +2.3. For an intermediate mixed valence system, such as YBCO, one can expect that the ground-state wave function configurations of YBCO can fluctuate4 between different Cu-site configurations and give rise to the transitions listed in Table I, where L+1(L−1) denotes an additional (a missing) electron in the oxygen ligand band and such configurations are the effect of MLCT (see Supplementary Materials).
At the top of the right panel of Fig. 2, we show simulated Cu L3-spectra created by using linear combinations of the pure-configuration spectra at the bottom of the right panel. Since a full theoretical description of the Cu L-XAS spectrum of YBCO has proven to be too complex for state-of-the-art ab initio methods we employ an ionic model approach to project the charge-transfer contributions from essential configurations. Our calculations show that the MLCT transitions 3d9→2p53d9L+1 deriving from formally divalent copper sites must heavily contribute to the spectral weight of the two satellites (reproduced by the double-peaked blue traces in Fig. 2). However, the opposing temperature trends in the satellites suggest the existence of additional contributions besides those from divalent copper sites. Thus the theoretical spectrum belonging to 3d9L+1→2p53d10L+1 and 3d9L−1→2p53d10L−1 (dashed blacked traces in Fig. 2) peaking only at the first satellite, indicates that monovalent and/or trivalent copper sites may contribute to the charge redistribution between the chains and planes. In order to distinguish between contributions from different configurations and to learn more about the nature of the states involved, we have performed incident-energy and -polarization dependent RIXS, in particular to study the transitions belonging to the satellite peaks.
Figure 3 (left panel) shows an overview of the polarization dependent Cu L3 RIXS spectra of optimally doped YBCO measured in the normal state (300 K) and in the superconducting state (15 K), respectively. The RIXS spectra were recorded at a 90°-scattering geometry with a grazing incidence angle of 20° with respect to the sample surface, i.e. for the geometry denoted by E||c there is an angle of 20° between the polarization of the incident x-rays and the crystal c-axis. The RIXS spectra have been normalized to the incident x-ray flux and plotted relative to the incident x-ray energy, i.e. plotted on an energy loss scale. For convenience when comparing spectral shapes, we have applied scaling factors as indicated to spectral pairs of identical geometry.
Excitation close to the L3 resonance (929.8 eV and 930.7 eV) yields spectra dominated by dd-excitations around −1.5 eV that are localized on divalent Cu orbitals. Moreover, magnetic and lattice excitations (here para-magnons and phonons, respectively) at energy losses within a few hundred meV are prominent at this excitation energy10,21. Particularly, out-of-plane polarized components are found to be temperature sensitive (see also Supplemental Materials). Intriguingly, already early on, specific phonon modes have been suggested to be of crucial importance for HTSC of cuprates, e.g. by facilitating interplane pairing. Indeed, the Ag Cu(1)-O(4) stretching vibration has been found to have anomalous strength in infrared reflectivity22 and could be coupled to charge transfer23. Together with structural lattice instabilities in YBCO, the observation of transverse modes sensitive to the MST of YBCO is possible evidence for unconventional, e.g. polaron-mediated, superconductivity. Below, we show that YBCO indeed undergoes a massive out-of-plane electronic reconstruction in the MST as well.
RIXS excitation at the XAS satellite peaks are dominated by MLCT excitations and as such contain unique information about Cu-O bonding properties. Figure 3 (right panel) shows a close-up of the spectra excited at 932.4 eV (planes) and at 933.4 eV (chains). The general structure of the spectra are typical for a transition metal oxide, consisting of a main peak at higher energy loss that reflect states derived from pure O 2p-states and a shoulder at lower energy loss from oxygen states hybridized with the Cu 3d-band. The selfdoping effect across the MST observed in the Cu L3-XAS also manifests itself in RIXS as a swap of sign in the difference spectra (gray traces in Fig. 3, right panel) when the exciation energy is changed from the plane satellite to the chain satellite – consistent to observations made with Cu L3-XAS data. Dramatically, in addition to this, the MLCT excitations of the chain-Cu exhibit sharp, localized states of out-of-plane character that exist above the MST, yet are absent at low temperature. Recently, such structures in the O(4) 2pz-states have been theoretically predicted by first principal calculations24. There also exists good agreement with the expected polarization dependence of the O(4) 2p-DOS. Interestingly, we observe that the RIXS spectra show much greater temperature dependence for out-of-plane polarization (E||c) than in-plane polarization (E||ab), which correlates with the observed decrease of an out-of-plane lattice mode (see above). Thus we observe a reconstruction of orbitals that are aligned perpendicular to the planes and chains and are hybridized with apical oxygen O(4) pz-orbitals. Propensity of these orbitals to reconstruct can also be inferred from a recent study at YBCO/manganite heterostructure interfaces24.
Figure 4 shows a close up of the satellite excited RIXS spectra in comparison to calculations. The spectral shapes are well reproduced using our ligand field model calculations that account for the large contribution for MLCT excitations at energy losses higher than 3 eV, as well as the weaker, lower lying dd-excitations around 1.5 eV energy loss. In order to analyze this orbital reconstruction of the Cu(1)-O(4) bond we performed model calculations using the same ground state configurations as used for the XAS spectra. Particularly, the loss of spectral weight of the localized structures suggests that certain configurations become suppressed by cooling YBCO and it would be elucidating to identify which ones. Even though the raw RIXS spectra result from a superposition of several configurations listed in Table I, we find that the major contribution to the difference spectra (i.e. the electronic reconstruction) can be traced back to a single configuration at each of the incident energies. In Fig. 3 (right panel) we have superimposed calculated spectra (black traces) from configurations that display the best correspondence to the respective experimental temperature dependent difference spectra (gray traces). At the first XAS satellite peak, the RIXS differences correlate closest with those from theoretical spectra of 3d9L−1 configuration, i.e. double hole/ZRS. Correspondingly, for excitation at the second XAS satellite peak, we find that the distinct sharp-peaked structure of the difference can only be reproduced by including a substantial contribution from the d8L+1 configuration. This involves formally divalent Cu ions that have transferred an electron into the ligand band. In other words, the net charge transfer that occurs in the MST is accounted for by the extra holes from the d8L+1 configuration of the chains that are pushed to the planes at low temperature and lead to additional d9L−1 double holes/ZRS (Fig. 2)25. Even though our calculations are based on a quasi localized theoretical approximation for the complex multi-electron state in YBCO, this already can consistently describe the overall intensity increase (reduction) of the corresponding RIXS spectra excited at the first (second) satellite peak (Fig. 2, 932.4 eV and 933.4 eV, respectively) as well as their basic spectral shapes26.
In conclusion, we have studied the temperature-driven MST of YBCO and observed dramatic changes in its electronic structure. We find that the MST is accompanied by self-doping of the superconducting planes via interplanar charge transfer from the chains, possibly mediated by specific phonon modes. While YBCO in its normal, metallic state shows an abundance of quasi-localized Cu 3d8L+1 configurations in the chains they are suppressed below the MST. Concurrently, this reconstruction of the interplanar Cu-O orbitals leads to an increase of the Cu 3d9L−1 configuration in the planes. We expect that the study of charge-transfer excitations by polarization and temperature-dependent RIXS will prove extremely fruitful for gaining insight to the MST of a wide range of cuprate superconductors as well as, strongly correlated materials, in general.
Samples and experiments
Thin films of YBa2Cu3O6+x (YBCO) were grown by pulsed laser deposition on (100) SrTiO3 5 × 5 × 0.5 mm3 single crystal substrates using 25 nm thick CeO2 buffer layers deposited using RF sputtering at a temperature of 780°C. High-resolution XAS and RIXS experiments were performed at the Advanced Resonant Spectroscopies (ADRESS) beamline17 at the Swiss Light Source (SLS), Paul Scherrer Institut, Switzerland, using the Super-Advanced X-ray Emission Spectrometer (SAXES)18. A photon flux of 1013 photons/sec/0.01% bandwidth was focused to a spot size below 5 × 55 μm vertically and horizontally (VxH). The Cu L3 edge XAS measurements were made in the bulk-sensitive total fluorescence yield (TFY) mode with an energy resolution of 100 meV. For the RIXS measurements at the Cu L3 edge (930 eV), the combined energy resolution was 120 meV. The single-impurity Anderson model (SIAM) with full multiplet effects was applied to describe the system (see Supplementary).
We would like to thank the staff at SLS for experimental support. This work was financially supported in part by the Swedish Research Council (VR), the Royal Swedish Academy (KVA) and MyFab-Micro and Nanofabrication infrastructure. This work was performed at the ADRESS beamline of the Swiss Light Source at the Paul Scherrer Institut, Switzerland.
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