INSTITUTE OF PHYSICS PUBLISHING SUPERCONDUCTOR SCIENCE AND TECHNOLOGY Supercond. Sci. Technol. 15 (2002) 1–7 PII: S0953-2048(02)27889-6 Lattice fluctuations and inhomogeneous charge states of high Tc superconductors N L Saini1, H Oyanagi2, Ziyu Wu1,3 and A Bianconi1 1 Unitá INFM and Dipartimento di Fisica, Università di Roma ‘La Sapienza’, 00185 Roma, Italy 2 National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba Central 2, 1-1-4 Umezono, Tsukuba, Ibaraki 305, Japan 3 Beijing Synchrotron Radiation Facility, Institute of High Energy Physics, Chinese Academy of Sciences, P O Box 918, Beijing 100039, People’s Republic of China Received 15 August 2001, in final form 7 January 2002 Published March 2002 Online at stacks.iop.org/SUST/15/1 Abstract We have used x-ray absorption spectroscopy as a tool to study instantaneous local lattice distortions of the CuO2 plane in high Tc superconductors and we have investigated the inhomogeneous charge states of these materials. The temperature-dependent Cu K-edge extended x-ray absorption fine structure (EXAFS) has been used to determine the correlated Debye–Waller factor of the Cu–O bonds, measuring local lattice fluctuations. The Debye–Waller factor of the Cu–O bonds shows an order-parameter-like behaviour across the charge stripe ordering temperature. The EXAFS results are supported by a temperature-dependent Cu K-edge x-ray absorption near edge structure (XANES) revealing a particular change in the local lattice displacements at the charge stripe ordering. The experimental Cu K-edge XANES results are well reproduced by full multiple scattering calculations including different distortions of the CuO2 plane showing particular lattice displacements which are consistent with the EXAFS results. The particular distortion mode as a response function to the charge stripe ordering has been discussed with several examples. The results are consistent with an inhomogeneous charge distribution in the high Tc cuprates suggesting an intimate relationship between the charge stripe ordering, local lattice fluctuations and high Tc superconductivity in the cuprates. 1. Introduction Perovskite superconductors are layered materials with CuO2 planes, separated by insulating rock-salt oxide layers. The importance of the CuO2 planes has created major interest in studying the electronic and structural characteristics of this sublattice, since the discovery of high Tc superconductivity in the cuprates. Recently, research in this field has entered a new phase where a collective role of lattice, charge and spin excitations is becoming recognized [1–3]. Indeed recent developments in materials science and advanced experimental tools have allowed us to uncover the fact that the electronic ground state of the cuprates is more complex than previously considered. Indeed the electron–lattice interaction in hightransition temperature superconductors, which has generally been overlooked in the past, plays an important role in describing the basic character of these materials. In fact it 0953-2048/02/000001+07$30.00 is hard to understand the normal and superconducting state properties by simply considering a doped two-dimensional antiferromagnetic CuO2 plane with only spin and charge fluctuations. Even though no consensus has been reached on the pairing ingredients, experiments are converging on the importance of lattice excitations. As an example, a recent photoemission study, probing electron dynamics, velocity and scattering rate in different families of copper oxide superconductors, has shown key features which cannot be explained by any other process than a coupling of the electrons with the lattice displacements involving movement of the oxygen atoms [4]. On the other hand, there are now several experiments to support the emerging view that the electronic ground state of these materials is inhomogeneous with charge stripe ordering; this is one of the main themes of recent debate [1–3]. Several experiments probing different characteristics related with © 2002 IOP Publishing Ltd Printed in the UK 1 N L Saini et al charge, spin and lattice dynamics are found to be consistent with the stripe phases in these materials [4–27]. The stripe phases are now widely observed in closely related structures such as insulating nickelates [28] and manganites [29–33]. Among cuprates, the La2CuO4 family of superconductors has been one of the most popular to study the inhomogeneous charge transport and charge stripe ordering by a variety of experimental techniques [5, 6, 10–13, 16, 19–21, 23, 26, 27]. A popular example is the La1.48Sr0.12Nd0.4CuO4 system [17, 19–21] in which the static charge stripe order has been observed. Recently it has been found that the elastic strain ε [34] due to the lattice mismatch between the bcc CuO2 and the fcc rock-salt sublattices plays a key role in the stripe formation and their dynamics and in the high Tc superconductivity. The superconducting stripes (superstripes) appear to form for a microstrain larger than a critical value (εc) and the superconductivity shows up near this critical value [34]. The La2CuO4 system has a microstrain larger than the critical microstrain εc and the charge stripe order is expected to be comparatively less dynamic. All these experiments have suggested that the inhomogeneous electronic ground state with charge stripe ordering could provide the right key to unlock the puzzle of high Tc superconductivity [1–3]. X-ray absorption spectroscopy (XAS) has been vital to explore the inhomogeneous charge dynamics of high Tc materials, supported by high brilliance and polarized x-ray synchrotron radiation sources allowing us to obtain directional information around a selective site. The technical developments in the field have made it possible to obtain the pair distribution function (PDF) with greater resolution, and have allowed a solution of the local lattice displacements in the CuO2 sublattice of the cuprates. Direct evidence for the Q2-type of distortions in the CuO2 plane has been provided by polarized Cu K-edge extended x-ray absorption fine structure (EXAFS) data [35–37]. The Cu K-edge absorption spectroscopy is a fast (∼10−15 s) and local (∼5–6 Å) tool [38] and is ideally suited to probing local and instantaneous lattice fluctuations in complex systems such as high Tc superconductors. Here we have exploited the Cu K-edge absorption spectroscopy to study the inhomogeneous structure of the CuO2 plane in high Tc cuprates. The temperature-dependent distribution of the local lattice distortions (dynamic and static) are measured by the correlated Debye–Waller factor of the Cu–O bond lengths using EXAFS, revealing an order-parameterlike change across the charge stripe ordering temperature. The x-ray absorption near edge structure (XANES) spectra, measuring instantaneous local geometry, show an abrupt change in the temperature-dependent spectral weight at the charge stripe ordering temperature. The XANES spectra for different distortions have been simulated by full multiple scattering (MS) calculations in order to explore the nature of the geometrical displacements. The temperature-dependent Cu K-edge measurements have been performed on several systems to probe the lattice fluctuations across the charge stripe ordering in these materials. On the basis of the experimental outcome, we argue that the particular local lattice displacement is a response function to the charge stripe ordering in the cuprate superconductors. The results are consistent with an inhomogeneous charge state of the high Tc cuprates. 2 2. Experimental and calculation details Cu K-edge XANES measurements were performed at the beamline BM29 at the European Synchrotron Radiation Facility (ESRF), Grenoble, and the BL13B of the Photon Factory, Tsukuba. At the BM29 the synchrotron radiation emitted by a Bending magnet source at the 6 GeV ESRF storage ring was monochromatized by a double-crystal Si(311) monochromator. For temperature-dependent measurements at the BM29 the samples were mounted in a closed cycle two stage He cryostat. The Cu K α fluorescence yield (FY) off the samples was collected using a 13 element Ge solidstate detector system to measure the absorption signal. At the BL13B the synchrotron radiation emitted by a 27 pole wiggler source at the 2.5 GeV Photon Factory storage ring was monochromatized by a double-crystal Si(111) and sagittally focused on the sample. The samples were mounted in a closed cycle refrigerator placed on a Huber 420 goniometer. The spectra were recorded by detecting the fluorescence photons using a 19 element Ge x-ray detector array. The temperatures were controlled and monitored within an accuracy of ±1 K. The emphasis was given to measuring the spectra with a high signal-to-noise ratio and several scans were collected to limit the noise level to the order of 10−4. Standard procedure was used to extract the EXAFS signal and corrected for the x-ray fluorescence self-absorption before the analysis [38]. Further details on the experiments and data analysis can be found in our earlier publications on cuprates and related systems [6, 30, 35–37]. The calculations were carried out based on the oneelectron full MS theory [39–42]. We have used the Mattheiss prescription [43] to construct the cluster electronic density and the Coulomb part of the potential by superposition of neutral atomic charge densities obtained from the Clementi– Roetti tables [44]. In order to simulate the charge relaxation around the core hole in the photoabsorber of atomic number Z, we have used the screened Z + 1 approximation (final state rule) [45], which consists in taking the orbitals of the Z + 1 atom and in constructing the final state charge density using the excited configuration of the photoabsorber with the core electron promoted to a valence orbital. For the exchange-correlation part of the potential, we have used the energy and position-dependent complex Hedin– Lundquist (H–L) self energy (r, E) as illustrated by Tyson et al [46]. The imaginary part of the H–L potential gives the amplitude attenuation of the excited photoelectronic wave due to extrinsic inelastic losses, and automatically takes into account the photoelectron mean free path in the excited final state. The calculated spectra are further convoluted with a Lorentzian function with a full width tot ∼ 2.5 eV to account for the core hole lifetime [47] and the experimental resolution. We have chosen the muffin-tin radii according to the criterion of Norman [48], allowing a 10% overlap between contiguous spheres to simulate the atomic bond. In our experience, the non-muffin-tin potentials could improve slightly the agreement between experiment and theoretical calculations, however in many cases the muffin-tin approximation gives the same results as the non-muffin-tin approach [49]. The use of overlapping spheres in a highly symmetric system (as in our case) gives a good agreement with 10% overlap. The calculations were Lattice fluctuations and inhomogeneous charge states of high Tc superconductors 0.004 Cu-O 100 20 σ 2CuO (Å2 ) |FT(χ(k)*k2)| 100 Cu-La(Nd,Sr) Cu-O-Cu 20 0.003 0.002 0.001 0 0 2 4 6 R (Å) 8 10 12 Figure 1. Fourier tranform of the EXAFS spectra (multiplied by k2) recorded on the La1.48Nd0.4Sr0.12CuO4 system (raw data). The inset shows an enlargement of the main peaks representing Cu–O, Cu–La (Nd, Sr) and Cu–O–Cu scattering. made for a convergent cluster containing 101 atoms, which covers a radius of ∼7 Å around the photoabsorbing Cu. 3. Results and discussion We have studied several cuprates that are found to show charge stripe ordering in the CuO2 plane. A widely discussed example is La1.48Sr0.12Nd0.4CuO4 (LNS) [20] and hence we start our discussion with this model compound. A well-characterized single crystal of LNS, grown by the travelling solvent floating zone (TFSZ) method was used for the measurements. Fourier transforms (FTs) of the EXAFS spectra (multiplied by k2) recorded in the in-plane geometry of the LNS at representative temperatures is shown in figure 1. The FT represents the global atomic distribution of nearest neighbours around the absorbing Cu atom in the LNS system. The FT in figure 1 represents raw experimental data and shows the standard peaks. The main peaks are shown enlarged in the inset and are denoted by Cu–O, Cu–La(Nd, Sr) and Cu–O–Cu representing respectively the scattering of the ejected photoelectron at the Cu site with the in-plane oxygen atoms (at ∼1.88 Å), La (Nd,Sr) atoms (sitting at ∼3.2 Å and 45◦ from the direction of the photoelectron) and a direct MS with the next Cu atom (at ∼3.8 Å), across the in-plane oxygen. The peaks in the FT do not represent the real atomic distances and the position should be corrected for the photoelectron back-scattering phase shifts to find the quantitative value to the atomic positions with respect to the central Cu. The high signal-to-noise ratio in the data can be judged from the FT (one hardly expects any true signal above ∼9 Å, and above this range the FT amplitude gives an idea of the noise in the data). The FT amplitude of the Cu– La(Nd, Sr) and Cu–O–Cu peaks increases with decreasing temperature (inset). It is clear from the raw data (figure 1) that the amplitude of the Cu–O FT amplitude at 20 K is decreased instead of the expected increase, indicating anomalous local lattice displacements at low temperature. Here we focus our attention on the Debye–Waller factors of the Cu–O pairs, σ 2CuO, that take into account both static and 50 100 150 200 T (K) 250 300 Figure 2. Temperature dependence of the correlated Debye–Waller factors (symbols) of the Cu–O pairs (σ 2CuO). The expected temperature dependence of the Debye–Waller factor for a fully correlated motion of Cu and O, calculated using the Einstein model, is shown by the lower dotted curve. A constant value of 0.001 45 is added to guide the temperature dependence of the experimental Debye–Waller factor (upper dotted curve). dynamic local lattice distortions. The Debye–Waller factors of the Cu–O pairs, σ 2CuO, were obtained by analysis of the EXAFS signal due to the Cu–O bonds, well separated from the higher shells of other neighbouring atoms. Here the Cu–O EXAFS signal is due to single scattering and probes the pair correlation function between Cu and in-plane oxygen. The EXAFS spectra due to Cu–O were simulated by a standard least-squares approach using curved wave theory [38]. The starting parameters were taken from diffraction studies [17]. The temperature dependence of σ 2CuO is shown in figure 2. Before proceeding, it is worth clarifying that σ 2CuO measures the correlated displacements between Cu and O and is not the same as that observed in the diffraction experiments where the Debye–Waller factor accounts for the mean-square deviation of a given atom from its average site in the crystal. σ 2CuO shows an anomalous upturn at ∼60 K. Considering evidence of stripe ordering in LNS appearing at ∼60 K, provided by several experimental techniques [11, 17, 20], we assign the anomalous upturn in σ 2CuO to a charge instability giving charge stripe ordering in this system. Indeed, the appearance of any charge density wave-like instability gives rise to an anomalous change in the Debye–Waller factor, known from studies of density wave systems [50]. This is also consistent with an anomalous upturn in σ 2CuO due to a particular local lattice distortion (the Q2-type of rhombic distortion) in the CuO2 plane that appears at the charge stripe ordering temperature [6, 35, 36]. Therefore the present result provides a clear indication that a particular local lattice distortion, revealed by an anomalous Debye–Waller factor of the Cu–O bonds, appears in the CuO2 plane at the charge stripe ordering in the cuprates. Let us now turn to the XANES results. Figure 3 shows representative Cu K-edge XANES spectra measured on the LNS system in the in-plane (E//ab) and out-of-plane (E//c) polarizations. The XANES spectra show the usual peaks, which are denoted by standard notations [36] in the polarized XANES spectra. The main absorption features are denoted by 3 N L Saini et al 0.68 A2 1.6 B1 B2 0.8 A1 E//ab E//c 0.4 α/α0 R=b1-a1/b1+a1 1.2 0 1.6 A2 0.02 B2 0.01 0.00 0.8 A1 -0.01 0.4 (α/α0) T-(α/α0) 20K B1 1.2 -0.02 absorption (arb. units) 0 B1 A2 B2 A1 8980 8990 9000 9010 Photon Energy (eV) Figure 3. Polarized Cu K-edge XANES of the La1.48Sr0.12Nd0.4CuO4 single crystal measured with E//ab and E//c at 20 K (upper). Different absorption features have been identified by the second derivative of the absorption spectra and denoted as A1 and A2 in the E//c spectrum and by B1 and B2 in the E//ab spectrum. An unpolarized spectrum measured at 20 K on the same system has been shown (middle) along with a difference spectrum between a spectrum measured above the charge stripe ordering. A calculated XANES spectrum for the La2CuO4 (not including the Nd and Sr in the cluster) is also shown (lower panel) to identify the natures of different peaks. The absorption peaks are well reproduced in the calculated spectrum. B1 and B2 in the E//ab spectrum and A1 and A2 in the E//c spectrum. The unpolarized spectrum is shown in the lower panel of figure 3. The unpolarized spectrum contains information on the local and instantaneous displacements in the overall cluster around the central atom. In fact in complex systems, such as the high Tc cuprates, the displacements are anisotropic with doping and temperature and hence the unpolarized spectrum is a useful tool to obtain important information on the local and anisotropic geometrical displacements around the selected site (i.e. Cu). In the lower panel of figure 3, we have shown a difference between a spectrum measured at a temperature (80 K) larger than the charge stripe ordering temperature 4 0.66 0.64 0 50 T (K) 100 150 Figure 4. Temperature evolution of the peak intensity ratio R = (b1 − a1)/(a1 + b1) for the La1.48Sr0.12Nd0.4CuO4. The ratio shows a clear change across the charge stripe ordering temperature. (∼60 K) and a spectrum at the lowest temperature measured in this work (20 K). The absorption features in the polarized Cu K-edge XANES spectrum are due to MS of photoelectrons emitted at the Cu site in the direction of the electric field, and their physical origin is revealed by MS calculations for La2CuO4. The calculated spectrum is also displayed in figure 3. For the La2CuO4 system, a very good agreement is shown for the experimental features in respect to their energy positions and relative intensity. The calculations are also in agreement with those reported by Li et al [51], for La2CuO4. From the calculated spectrum it is easy to find the origin of different features observed in the experimental spectrum. The features A1 and A2 are determined by MS of the ejected photoelectrons off apical oxygen and La, Nd and Sr atoms while the peak B1 corresponds to MS of the in-plane oxygen and Cu in the CuO2 plane. The peak B2 includes a MS contribution, similar to the main peak B1 and also contributed by multi-channel effects. It can be seen that there is a high-energy spectral weight transfer resulting in positive and negative differences with a maximum difference of ∼2% of the normalized absorption (figure 3). On cooling the sample, the spectral weight around the peak A1 (A2) is decreased with an increase around the peak B1 (B2). We have plotted the temperature dependence of the XANES peak intensity ratio R = (b1 − a1)/(b1 + a1) in figure 4. Here, b1 and a1 represent the intensities of the peaks B1 and A1 probing high-energy spectral weight transfer from the core excitations Cu1s → εpz (peak A1) to the Cu1s → εpxy (peak B1). The ratio R shows a clear increase below the charge stripe ordering temperature. We have studied another model system, La1.875Ba0.125CuO4 (LBC125), representing the family of cuprates where clear evidence for the charge stripe ordering is found. The temperature-dependent unpolarized Cu K-edge absorption spectra were used to determine the ratio R = (b1 − a1)/(b1 + a1). The temperature dependence of R for the LBC125 system is shown in figure 5. As for the LNS system, a clear increase of R is observed across the charge stripe ordering temperature (∼60 K) in the LBC125 system, indicating geometrical changes in the CuO2 plane at the charge stripe ordering temperature. This confirms that the ratio R is a good indicator of charge stripe ordering in the cuprates. Lattice fluctuations and inhomogeneous charge states of high Tc superconductors Cu K-edge Absorption (arb. units) La1.875Ba 0.125CuO4 R=b1-a1/b1+a1 0.695 0.69 0 50 100 150 To explore the nature of these local displacements around the Cu atom across the charge stripe ordering, we have made MS calculations and calculated Cu K-edge XANES spectra for different distortions. For this purpose we have taken a simple approach by taking the HgBa2CuO4+δ (Hg1201) system as a model for the calculations, where the Cu–O plane is crystallographically flat due to a small mismatch between the CuO2 planes and the rock-salt oxide layer. In addition the simple structural unit cell with tetragonal crystal structure (a ∼ 3.8755 Å; c ∼ 9.4952 Å) [52] provides the added advantages of simulating different local lattice distortions and investigating the evolution of the XANES spectrum with different geometrical displacements. Figure 6 shows Cu K-edge XANES measured at room temperature on a powder sample of Hg1201 superconductor, along with a calculated spectrum using the MS theory. The real-space MS of the photoelectrons is excited from the Cu 1s states to the cluster of atoms within a radius of ∼7 Å from the central Cu. The features observed in the experimental spectrum could be satisfactorily reproduced not only with respect to the relative intensities, but also in energy separations. The calculations were extended to a distorted CuO2 plane considering a particular rhombic distortion where two oxygen atoms move away and two move closer, as observed in the cuprates [6, 36]. The evolution of the absorption differences with an increasing quantity of the rhombically distorted sites (Q2-type rhombic distortion), with respect to the undistorted CuO2 plane, is shown in figure 6. It is clear from the calculated absorption differences that the Q2-type of rhombic distortion introduces the spectral weight transfer, as observed in the experimental spectra below the charge stripe ordering temperature. Thus the results of the calculations are consistent with the experimental findings, suggesting that the observed weight transfer is due to an octahedral distortion where one of the Cu–O–Cu directions becomes elongated [6], observable only when the amplitude of the lattice fluctuations becomes larger than the amplitude of thermal fluctuations. This rhombic distortion has been previously determined by polarized Cu Kedge EXAFS on the La2CuO4 system [6] and was later found to be common to the CuO2 plane of other high Tc cuprates Experiment A1 MS 0.06 0.003 0.05 0.002 0.04 0.001 0.03 0 0.02 10% Q2 20% Q2 0.01 40% Q2 0 -10 -5 0 5 10 15 Energy (eV) ∆α Figure 5. Temperature evolution of the peak intensity ratio R = (b1 − a1)/(a1 + b1) for the La1.875Ba0.125CuO4. As for La1.48Sr0.12Nd0.4CuO4, the ratio shows a clear change across the charge stripe ordering temperature. α T(K) Hg1201 B1 -0.001 -0.002 20 -0.003 25 Figure 6. Calculated absorption spectrum for Hg1201 is compared with an experimental Cu K-edge XANES measured on the same system (upper). The calculated absorption is plotted along with absorption differences with respect to the calculated spectra considering the variable quantity of distorted sites (Q2-type of rhombic distortion). The rhombic distortion is at the origin of the spectral weight transfer between peaks A1 and B1. [6, 35–37]. Indeed this is the Q2 mode of the Jahn–Teller distortion [53], which appears at the same temperature where the system shows charge stripe ordering. This was demonstrated by combined EXAFS and diffraction experiments [35]. Returning to figures 4 and 5, showing the anomalous change in the ratio R = (b1 − a1)/(b1 + a1), we can state that the Q2-type of rhombic distortions of the CuO2 plane could be considered a suitable response function of the charge stripe ordering parameter in the cuprates. It is worth stating that, even if the temperature-dependent upturn of R at the charge stripe ordering is different, with different magnitude, the change is clear. The differences of R in different systems are due to different strains on the CuO2 plane [1–3] because of different substitutional disorder (rock-salt blocks are different). Figure 7 shows another example, La1.94Sr0.06CuO4, an underdoped superconductor. Again, the ratio R shows an anomalous increase below ∼110 K. Recently, the La1.94Sr0.06CuO4 system was used as a model compound to explore the oxygen isotope effect on the charge stripe ordering temperature [54]. The charge stripe ordering temperature was found to change from 110(±10) K to 170 (±10) K while substituting 18O in place of 16O in La1.94Sr0.06CuO4. The result, showing an isotope shift of ∼60 K, not only suggests a large change in the local structure of the CuO2 plane due to isotope substitution but also provides direct evidence of the important role of local lattice displacements in charge stripe ordering phenomena. 5 N L Saini et al 0.64 R=b1-a1/b1+a 1 La1.94Sr 0.06CuO4 0.63 0.62 0 50 100 150 200 T(K) Figure 7. Temperature evolution of the peak intensity ratio R = (b1 − a1)/(a1 + b1) for La1.94Sr0.06CuO4. The ratio shows an abrupt change below ∼110 K reflecting charge stripe ordering in the system below this temperature. 150 T(K) 100 50 0 Acknowledgments 0.05 0.1 0.15 0.2 0.25 Hole doping Figure 8. Doping dependence of the charge stripe ordering temperature obtained by the jump of the XANES peak intensity ratio R (squares) plotted with that obtained by the wipeout fraction of Cu NQR (circles). The open circles correspond to the data for La2−xSrxCuO4 [11] while the closed circles represent data obtained for the La1.6−xSrxNd0.4CuO4 system [11]. In figure 8 we have plotted the charge stripe ordering temperature (defined by the abrupt local geometrical change as reflected by the anomalous increase of the XANES peak intensity ratio R) as a function of the hole concentration in La-based cuprate superconductors. This temperature has been compared with that obtained by the wipeout fraction of Cu NQR [11, 20]. The temperatures for charge stripe ordering, obtained by the two techniques, agree quite well in the underdoped regime within the experimental uncertainties. The temperature also agrees well with that determined by other techniques [20]. A detailed discussion of the phase diagram of the charge stripe ordering in different cuprates will be presented elsewhere. In summary, we have reported evidence in the local structural fluctuations supporting the inhomogeneous charge 6 distribution in cuprate superconductors. We have used Cu K-edge EXAFS and XANES spectroscopies to explore local lattice fluctuations associated with charge stripe ordering in the cuprates. We find an order-parameter-like change in the instantaneous local lattice fluctuations across the charge stripe ordering temperature, revealed by an anomalous increase in the correlated Debye–Waller factor of the Cu–O pairs. On the other hand, Cu K-edge XANES measurements, measuring geometrical changes, show a particular evolution of temperature-dependent XANES peak intensities with an orderparameter-like change in the anisotropic and instantaneous local displacements around Cu, across the charge stripe ordering. The MS calculations of different distortions suggest that the abrupt change in the spectral weight transfer, reflected by the XANES peak intensities, is due to the appearance of the Q2-type of Jahn–Teller distortions at the charge stripe ordering. On the basis of studying the model systems, we have argued that the Q2-type of displacements across the charge stripe ordering could be considered to be a response function. In addition to providing a new response function, the results construct clear evidence for the importance of electron–lattice interactions in the charge stripe ordering. 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