Phonon anomalies and lattice dynamics in superconducting oxychlorides Ca{}_{2-x}CuO{}_{2}Cl{}_{2}

Phonon anomalies and lattice dynamics in superconducting oxychlorides CaCuOCl

Matteo d’Astuto matteo.dastuto@impmc.upmc.fr    Ikuya Yamada [    Paola Giura    Lorenzo Paulatto    Andrea Gauzzi Institut de Minéralogie et de Physique des Milieux Condensés (IMPMC), UMR CNRS 7590, Université Pierre et Marie Curie - case 115, 4, place Jussieu, 75252 Paris cedex 05, France    Moritz Hoesch [    Michael Krisch European Synchrotron Radiation Facility, BP 220, F-38043 Grenoble Cedex, France    Masaki Azuma    Mikio Takano Laboratory of Solid State Chemistry, Institute for Chemical Research, Kyoto University, Uji, Kyoto-fu, 611-0011 JAPAN
Abstract

We present a comprehensive study of the phonon dispersion in an underdoped, superconducting CaCuOCl crystal. We interpret the results using lattice dynamical calculations based on a shell model, and we compare the results, to other hole-doped cuprates, in particular to the ones isomorphic to LaSrCuO (LSCO). We found that an anomalous dip in the Cu-O bond stretching dispersion develops in oxychlorides with a simultaneous marked broadening of the mode. The broadening is maximum at that corresponds to the charge-modulations propagation vector. Our analysis also suggests that screening effects in calculations may cause an apparent cosine-shaped bending of the Cu-O bond-stretching dispersion along both the ( 0 0) and ( 0) directions, that is not observed on the data close to optimal doping. This observation suggests that the discrepancy between experimental data and ab-initio calculations on this mode originates from an overestimation of the doping effects on the mode.

Superconductivity, Phonons, Hole-doped Cuprate, Phonon-electron interactions, Phonon dispersion, Inelastic X-ray Scattering
pacs:
74.72.Gh, 63.20.D-, 63.20.kd, 78.70.Ck

Present address: ]Nanoscience and Nanotechnology Research Center (N2RC), Research Institutes for the Twenty-First Century - Osaka Prefecture University 1-2 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8570, Japan

Present address: ]Diamond Light Source, Didcot OX11 0DE, United Kingdom

I Introduction

The discovery of high temperature superconductivity (HTS) in cuprates was originally motivated by the search for superconductors with strong electron-phonon couplingBednorz and Müller (1986). The first HTS compounds, LaBaCuO (LBCO) and LSCO, do indeed display a very large isotopic effect for oxygen, although the doping dependence of this effect turns out to be very anomalousCrawford et al. (1990). Later studies pointed out that electron-phonon coupling may not be the main origin of the Cooper pairingBonn (2006), in particular for optimal doping. But its role across the phase diagram of cuprates is still controversial, in particular in its under-doped region. An important point is that single electron band approximations, such as Density Functional Theory (DFT) find a small electron-phonon coupling Bohnen et al. (2003); Giustino et al. (2008), but they possibly miss many body effects, as it was suggested that large couplings may exist in the presence of strong electron-electron correlations Rösch and Gunnarsson (2004).

An important point stressed in DFT based investigations on electron-phonon coupling in cuprates is that these calculations seem to reproduce well the marked softening with a cosine dispersion, that develops under doping for longitudinal Cu-O bond-stretching mode along the direction ( 0 0) of such bonds (modes with character). At the same time, large discrepancies between those calculations for the same mode, but along the diagonal direction ( 0) (modes with character) are foundFalter et al. (2006); Bohnen et al. (2003). It has been suggested that the physical origin of the anomaly in the dispersion of the Cu-O bond-stretching modes is different for the two directions Bohnen et al. (2003); Giustino et al. (2008).

Underdoped cuprates exhibit a static, or quasi-static, modulation of the charge, characterized by a stripe pattern parallel to the Cu-O bonds, which can give clear diffraction peaks both in the charge Tranquada et al. (1995); Abbamonte et al. (2005) and spin channel, for doping close to with a propagation vector of , i.e. a periodicity of , where is the lattice parameter along the Cu-O bonds. Besides the above mentioned Cu-O bond stretching anomaly with cosine shape, an additional marked dip and a sizable broadening of the line-shape is observed for the same phonon branch, close to the wave stripe vector McQueeney et al. (1999); Pintschovius and Braden (1999); Reznik et al. (2006); d’Astuto et al. (2008); Reznik (2010); it has been established that such feature can not be simulated by DFT Reznik et al. (2008).

Large electron-phonon coupling can drive both phonon softening and broadening as it as been established, for example, in the case of classical superconductors such as, e.g. Nb Butler et al. (1977) and, more recently, in Weber et al. (2012). For cuprates the issue remains controversial. In order to elucidate this aspect, we investigate the lattice dynamics in superconducting, under-doped CaCuOCl, using Inelastic X-ray Scattering (IXS) and compare our results with lattice dynamics calculations based on a shell model.

Doping CaCuOCl oxychloride systems leads to a new family of HTS superconductors with Tc up to 43 KHiroi et al. (2002); Yamada et al. (2005). Their layered structure is similar to the cuprate one, characterized by CuO plane, but without oxygen in the blocks separating these planes (see Fig. 1, left panel). These compounds represent an ideal test bench for the physics governing the high Tc superconductivity that is commonly believed to depend only on the CuO planes, independently from the details of the oxide blocks between them. In particular, oxychlorides have a chlorine ion that replaces the apical oxygen. The apical oxygen is important for the dynamics of the anionic octahedra surrounding the copper cation on most of the hole-doped cuprates. Moreover, oxychlorides are ideal for studying phonon dispersions, particularly the one of the copper-oxygen bond stretching mode by means of IXS spectroscopy, because they are composed only of low Z, thus yielding a higher IXS signal, due to the weaker photoelectric absorption compared to the cuprates, and also thanks to their simple 1-layer structure with small disorder, which reduces the number of modes to be measured and calculated. We note that these characteristics should also facilitate ab-initio calculations. Underdoped oxychlorides show a modulation in the charge density, as their cuprate counterpart. However, this modulation is observed only in real space, using Scanning Tunelling Microscopy (STM) Hanaguri et al. (2004), with a periodicity of as for the stripes, but, up to now, not in diffraction.

Figure 1: (Color on line) DrawingMomma and Izumi (2008) of the Unit cell of CaCuOCl Yamada et al. (2007). The square coordination of copper with its four nearest-neighborhood oxygens ions in the CuO planes is shown. The chlorine ions are located in the apical site above the copper.

In this work, we present a study of the phonon dispersion in superconducting CaCuOCl doped with Ca vacancies. The study is as complete as possible, considering limitation from the crystal mosaic for the particular technique used (IXS), and the limited beam-time available on such highly specialized synchrotron experiment. We interpret the results using lattice dynamical calculations based on a shell model, and we compare our results, to those obtained for other hole-doped cuprates, in particular the ones isomorphic to LSCO (T-structure)Pintschovius and Reichardt (1998); Reznik (2010); Tajima et al. (1991). We found that an anomalous dip in the Cu-O bond stretching dispersion develops also in oxychlorides with a simultaneous marked broadening of the mode. The maximum of the broadening appear at the charge modulation propagation vector of . In addition to this effect, by comparing our results on the longitudinal Cu-O bond-stretching mode in superconducting CaCuOCl to our model, we found that screening effect may lead to a simultaneous bending down of the whole dispersion along both the ( 0 0) and ( 0) directions.

Ii Methods

ii.1 Crystal growth and characteristics

Figure 2: (Color on line) Chartigo () of the magnetization vs temperature across the superconducting transition at 100 Oe for the sample 2b measured by IXS. Inset, front and side view of the crystal, as measured in diffraction and IXS, in a grease film, with the glass fiber holder.

We studied three different crystals of CaCuOCl, selected from several ones, of sizes on the order of 0.5 to 1 mm, from different batches, after a screening of their superconducting and crystalline properties as measured by the Meißner effect in a SQUID magnetometer (Quantum design MPMS©) and the diffraction on a four-circle diffractometer equipped with a Mo K anode, a kappa-type goniometer and a CCD detector (Oxford diffraction Xcalibur©). We selected two of the crystals with nominal Ca vacancies doping x=0.2, grown at high-temperature and high-pressure of C, 5.5 GPaYamada et al. (2007, 2005), and a parent insulating CaCuOCl with stoichiometric composition. The best one, sample 2b, used for all the measurements of in-plane dispersion, of about 0.1 mm volume (see Fig. 2), shows a superconducting transition temperature onset at T=33 K, with a well defined diamagnetic jump on a temperature window 8 K from 10 to 90% of the magnetization, as shown in Fig. 2. This corresponds to an underdoped compounds with a Ca deficiency x0.160.01, slightly lower than the nominal one. The sample was protected from moist by a film of grease (Apizon N©), in order to avoid formation of hydroxides, during all the measurements. The grease film was also used to hold it on the borosilicate glass sample holder for diffraction and Inelastic X-ray Scattering (IXS), as shown in Fig. 2 (inset). The second doped crystal, named 1b, has also a nominal vacancy doping x=0.2, and similar crystalline and superconducting properties.

ii.2 Inelastic X-ray Scattering

The sample 2b was mounted in a vacuum chamber with Kapton© windows, with the scattering plane (,) for measurements along and (,) for measurements along . The angular width of the (200) Bragg reflection rocking curve was FWHM, proving excellent single crystal quality in-plane. The second sample, 1b, was mounted with the direction in the plane of scattering, but it revealed a large mosaic in the c* direction, preventing us from completing the measurements along . This also prevented us for doing measurements on modes with in-plane propagation but out-of-plane polarization as, notably, the oxygen buckling modes. The third, undoped, sample showed a mosaic too large for doing any phonon measurement. Phonons were measured from (1,1,0) to (2.2, 2.2, 0) along and from (2,0,0) to (3,0,0) along in longitudinal geometry, and from (3,0,0) up to (3, 0.5, 0) in transverse one.

The main monochromator was set to the Si (9 9 9) Bragg reflection, with a wave-length of 0.6968 Å(17794 eV) and an energy resolution E = 3.0 0.2 meV (see Ref. Krisch and Sette, 2007; Verbeni et al., 1996, 2008 for details). The back-scattered beam is focused by a platinum-coated toroidal mirror, which provided a focal spot at the sample position of 0.270 (horizontal) and 0.080 (vertical) mm FWHM at the sample position. The IXS spectrometer Masciovecchio et al. (1996) was used with a set-up allowing simultaneous measurements from 5 analyzers. Analyzer slits were open to (60 60) mm, thus integrating over a solid angle of 0.6, amounting to a Q resolution of 0.416 nm corresponding to approximately 0.06 of the Brillouin Zone along .

Fig. 3 shows representative IXS spectra for three different directions, longitudinal along ( 0), with character, longitudinal along the ( 0 0) direction, with character and transverse along the equivalent (0 0) direction, with character, for the same value =0.25. Continuous lines are a model, consisting of Lorentzian function, convoluted with the instrumental function. The model is chosen to fit the data using a minimization procedure James (1998).

Figure 3: (Color online) PlotMat () of the measured IXS intensities as a function of energy on CaCuOCl for the propagation vector corresponding to the middle of the Brillouin Zone along three different symmetry in-plane lines. Left column shows the overall data, while the right column are the respective zoom at the high energy of the Cu-O bond stretching mode. Top panel: Longitudinal at (0.25 0.25 0), with symmetry. Middle panel: Longitudinal at (0.25 0 0), with symmetry. Bottom: Transverse at (0 0.25 0), with symmetry. Red lines are fit to the data described in the text. The contribution from the Cu-O bond stretching mode are singled out as a black line.

In CaCuOCl the contrast between the elastic line and the low energy mode on one side and high energy mode on the other, it is not as strong as in other cuprates. The ratio is determined by the ions number of electrons, as the the IXS scattering yield is proportional to and the photoelectron absorption to , so that the high elements dominate in a system with different atomic species, while the high energy mode come almost exclusively from light element vibrationsd’Astuto and Krisch (2010). In other cuprate systems, measuring the high energy mode dispersion is therefore possible only at few ( 10) Kelvin, where the Bose factor is strongly reduced for modes below 25 meV, compared to the intensity at room temperatured’Astuto et al. (2003a). The measurements presented here are, in turn, all taken at room temperature, so that the contrast in the intensities between high and low energy is largely due to the Bose contributions, still allowing the measurements of all high energy phonon modes.

ii.3 Calculations

Phonon dispersion are simulated using the lattice dynamical calculation package OpenPhononMirone (2001), based on a shell model, further adapted for compilation with python 2.7 Paulatto et al. (2012). In order to be consistent with previous studies on the phonon dispersion in cuprates by INS Pintschovius and Reichardt (1998); Reznik (2010) and IXS d’Astuto et al. (2002, 2008, 2003b) we used a common potential model for cuprates, where the interatomic potentials have been derived from a comparison of the INS results for different HTcS compounds by Chaplot et al. Chaplot et al. (1995). To this model a screening of the Coulomb potential is added, in order to simulate the effect of the free carriers introduced by doping. In the same way as described by Chaplot (see Ref. Chaplot et al., 1995) for metallic and , we replaced the long-range Coulomb potential by , and for the dielectric function we took the semi-classical Thomas-Fermi limit of , where indicates the screening vector. In our calculation, we estimate a screening wave number Å, where is the lattice parameter, which corresponds to a doping of about 10 % according to Ref. Chaplot et al., 1995. For ions and bonds not included in the previous model we used the parameters used by Mittal et al. in Ref. Mittal et al., 2003 for Cl and by Chaplot in Ref. Chaplot, 1988 for Ca as a starting point of our refinement. We used the experimental lattice parameters as reported in Ref. Yamada et al., 2005. The solution is stable with the set of atomic potential found, without adding any additional force constant to equilibrate the fictitious forces originating from anharmonic contribution when using real structural parameters in a quasi-harmonic approximation. A summary of the ions and bonds parameters are given in Table 2 and 2 respectively. In Fig. 4 we show the main atomic displacement pattern as calculated by our model at the zone center , for the in-plane modes we have measured.

(nm)
O -1.56 -3.0 1800
Cl -0.92 -1.0 1800
Cu 1.64 3.0 2000
Ca 1.66 3.0 700
Table 2: Bonds parameters of the lattice dynamical shell model described in the text.
k-k’ (eV) (Å) (ev Å)
Cu-O 4000 0.228
Cu-Cl 4000 0.29
O-O 2000 0.284 100
Ca-O 1600 0.304
Cl-Cl 2000 0.34
Ca-Cl 1600 0.33
Table 1: Ions parameters of the lattice dynamical shell model described in the text.

Note that, from now on, we will use the character of the mode along a particular dispersion line as a label for the line itself (e.g. for the line ( 0 0) in longitudinal geometry) , and the zone center character as a label for the whole mode dispersion (e.g. Eu(1) along for the Cu-O bond stretching mode along the line ( 0 0) in longitudinal geometry).

Iii Results

IXS spectra shows overall well defined phonon modes, in general with resolution-limited energy width, with the notable exception of the Cu-O bond stretching mode (Eu(1)) along . They therefore present no difficulty for the fit procedure, in order to determine the phonon frequencies, width and intensities.

Figure 4: (Color online) DrawingMomma and Izumi (2008) of the atomic displacements of the in-plane modes we have measured at the zone center , as calculated by our lattice dynamical model described in the text. For each mode, we give its character, and the calculated frequency at . We highlight the octahedron formed by the anions, with the two apical chlorines and the four square coordinated oxygens, around the copper, in order to single out the differences and similarities with the analogue displacements in hole-doped cuprates with T structure, as e.g. shown in Ref. Tajima et al., 1991. The calcium cations lies outside the octahedron, on the vertical of the apical chlorine one.
Figure 5: (Color online) ChartMat () of the CaCuOCl phonon dispersion (blue circles) measured by IXS and calculated frequencies using the shell model of lattice dynamics described in the text (red line). We also indicate, on the left panel, the frequencies at the zone center , extrapolated from their positions in the infrared spectra reported in Ref. Zenitani et al., 2005 (empty triangle-right).
Figure 6: (Color online) Calculated (lines) and experimental (symbols) inelastic scattering intensities for phonon modes in CaCuOCl CuO, with character (left panel), (center) and (right panel)Mat (). The intensities units are arbitrary for calculations. Experimental reported areas of peak units are in I/I meV, and are multiplied by a common factor for all modes for a given line in the Brillouin Zone. Mode assignment is based on the closest experimental frequency to a given calculated mode. The only exception is the acoustic and(or) Eu(4) mode at q=(3, 0.5, 0), for which both assignment are proposed (and match) the calculated one. Labels corresponds to the character a the zone center as explained in the text.

The parameters obtained from the fitting of these and several others spectra are plotted in Fig. 5, for the frequency mode dispersions, and Fig. 6, for the mode intensities. In Fig. 5 the experimental frequencies obtained by IXS are compared with the calculated dispersions. We also include experimental zone center modes estimated frequencies, obtained by infrared absorption on heavily underdoped CaNaCuOCl (x=0, 0.3) in Ref. Zenitani et al., 2005. In Fig. 6, the IXS intensities are compared with the dynamical structure factor calculated using the eigenvector simulated in our model. Overall, we observe a good agreement between the measured frequencies and intensities, on one side, and the calculated ones on the other side. This with the notable exception of :

  1. the highest energy optic mode, the Cu-O bond stretching, with symmetry,

  2. a spurious intensity at very low frequency, at about 8 meV, with flat dispersion in-plane,

  3. the dispersion for the Eu(3) mode, the Cu-O bond-bending, along , away from the zone center, and

  4. the acoustic mode close to the zone boundary.

The first anomaly is well known Pintschovius and Reichardt (1998); Reznik (2010); d’Astuto et al. (2002, 2008, 2003b), and widely debated Giustino et al. (2008); Rösch and Gunnarsson (2004), while the other anomalies are rather new. We discuss the details of our observation and possible interpretations in the following section.

In table 2 and 2 we give the ionic and bond parameters used for the model shown in Fig. 5 and 6.

Overall, the agreement between the calculated and measured dispersion is comparable to the one found using similar atomistic modelsPintschovius and Reichardt (1998); Chaplot et al. (1995) or even more advanced ab-initio approaches Reznik (2010); Giustino et al. (2008) . Moreover, we find a satisfying agreement between the calculated intensities, with the experimental ones on the IXS peak with closer frequencies of the calculated dispersion. This, not only supports the assignment we suggest for the phonons branches we have measured, but it is also a proof of the quality of the model, as correct eigenvectors are more delicate to found than frequencies.

Iv Discussion

The lattice dynamical shell model has been refined only with limited tuning of the ionic and bond parameter concerning the chlorine and calcium ions, otherwise imposing the parameters from Ref. Chaplot et al., 1995, confirming that the common potential model is appropriate for the cuprates.

We would like to discuss now in more details our present understanding of the discrepancies between the data and the calculations.

Dispersionless intensity at about 8 meV.

We observe a low energy flat mode (point 2 above), in-plane, mainly along the and , directions. Along the direction the fitting of the central line is improved if we add some intensity in the same frequency region, but it is not well resolved, with perhaps the exception of the zone boundary. The difference is possibly due to the larger intensity of the elastic line in the geometry corresponding to scattering, which is accidental, and therefore, we can not consider this anomalous excitation anisotropic from our data. In the and directions it appears as a rather shallow intensity between the elastic line and the acoustic mode, but with an intensity well above the background. For a few scans only it appears with a well defined maximum. The origin of this mode is not understood at the moment, but also observed in closely related system, for which we are presently running experimental investigationsd’Astuto and Lamago (2012) in order to test different hypotheses of the nature of this additional mode, including defect vibrational states and phonon modes activated by symmetry breaking. We note also that several works using Raman scattering and infrared absorption in underdoped LaSrCuOTassini et al. (2005); Sugai et al. (2006); Caprara et al. (2005); Lucarelli et al. (2003); Venturini et al. (2002) found intensity at similar energy in under-doped sample, which is attributed to modes related to the stripes charge-modulations.

Acoustic mode close to the zone boundary.

The anomaly on the acoustic mode close to the zone boundary concern only one point, while the rest of the dispersion fit quite well with our simulations, both for the frequencies and the intensities. It would be nevertheless interesting to further study this mode, by complementary ab-initio calculation, to verify our findings, as well as with more detailed measurements close to the zone boundary.

Cu-O bond bending mode.

The calculated frequency of the Cu-O bond bending mode at the zone center is very close to the experimental IR position for the corresponding Eu(2) mode, but our calculation shows an upward dispersion, which does not seems to be confirmed in our data along . Indeed, the experimental intensity along between 30 and 40 meV, seems to lie at lower energy with respect to the calculated one. However, the Cu-O bond bending mode has a relatively low yield, along both and comparable to the bond-stretching one, while being at lower energy. They are therefore measured on top of the tails of the much stronger modes at lower energy, as described above, fact that complicates their detection. A further investigation of this dispersion along and would be possible only at low temperature, as discussed above. Note that, on the contrary, for the corresponding Eu(2) mode along the mode is reasonably well resolved, and match very well both the calculated frequency dispersion and the intensity.

Cu-O bond stretching mode.

Concerning the Cu-O bond stretching along the bond direction, (, 0, 0), we calculate a symmetrical dispersion in the extended zone, similarly to other cuprate with T-structure. Frequencies at both zone center =0 and extended zone boundary =2 are the same, and do not change with doping, in the systems where doping dependence is known (see, for example, Ref. Reznik, 2010 and Pintschovius et al., 2006) . For such branch, the mode has a vanishing small dynamical structure factor, so we can not compare directly the dispersion close to zone center and =2. On the other hand, IR data shows well defined phonons mode at the zone center, but only in the insulating phases. We remark that the IR data assigned to the EU(1) mode on heavily underdoped samples, corresponds very well to the frequency we found at the zone boundary for both and Cu-O bond stretching modes. This suggests that the physics for this mode is very similar to the one of LaSrCuOPintschovius et al. (2006); Reznik (2010), despite the present lack of dispersion data in the undoped parent compound, and of mode frequencies an the Zone Center in the doped one.

In Fig. 7, top panels, we shows the detail of the Cu-O bond stretching for the direction with (half-breathing) and (full-breathing) character and compared to our lattice dynamics simulations, with different screening wave number .

Figure 7: (Color on line) Top panels: CaCuOCl Cu-O bond-stretching dispersions (blue circles) measured by IXS and calculated frequencies using a shell model of lattice dynamics. Top, left: along ( 0 0) (). Top, right: along ( 0) (). Black lines corresponds to a model with lower doping and a screening wave number , while red lines corresponds to a model with higher doping, and a screening wave number . The blue dashed line is a cosine function compared to the data of symmetry in order to show the marked anomaly at 0.75. Bottom panel: Blue full circles are the Full Width Half Maximum of the IXS data corresponding to the Cu-O bond-stretching mode along ( 0 0), showing a maximum around 0.75Mat ().

In the same figure, bottom panel, we can follow the corresponding broadening of the mode, which starts at a value of less than 1 meV, once instrumental resolution subtracted, to end up at more than 12 meV. Note that the softening and simultaneous broadening is observed only for the mode with character , propagating along (Fig. 7, left, top and bottom). The same mode propagating along the diagonal (, Fig. 7, left) is dispersing upward, with a line-shape that is resolution limited, as in other cuprates Reznik (2010).

STM experiments in oxychlorides Hanaguri et al. (2004) report a modulation of the Fourier transform of the differential conductance map at wave-vectors of (, 0 0) with integer and 0.25, i.e. for modulations with a periodicity corresponding to 4. This is reminiscent of what happens in cuprates Reznik et al. (2008); Reznik (2010) and other perovskite-like ternary transition metal oxides Weber et al. (2009), with the difference that in oxychlorides, there is no observation of static diffraction by charge density modulation. We can then confirm that the observation of STM has a dynamical precursor at room temperature, as for the stripes in other cuprates. Note that the pattern observed by STM where first labelled as ”checkerboard” Hanaguri et al. (2004), although this was not confirmed by further studiesKohsaka et al. (2007), that maintained, however, a Cu-O-Cu bond-centered electronic pattern without long-range order but with 4-lattice-constant-wide unidirectional electronic domains Kohsaka et al. (2007). Indeed, for a ”checkerboard” pattern, we should have observed the same phonon anomaly along both the and the directions, as it is the case in those transition metal oxides where such a modulation is presentWeber et al. (2009). Here we observe the anomaly only for the mode with character in agreement with other cuprates showing a stripe charge modulation pattern Reznik et al. (2008); Reznik (2010).

Regardless of the exact pattern of the charge modulation, we note that such anomaly can not be accounted for in simple models based on Landau liquid band type as DFT ones Reznik et al. (2008), as the charge modulations themselves can not be simulated in such theoretical framework. We remark also that the propagation vector (0.25, 0 0) of these unidirectional electronic domains, where we observe the ”sharp dip” anomaly (Fig. 7), would corresponds to a nesting vector of the Fermi Surface, as reported for Na-doped CaCuOCl Shen et al. (2005), although the region of the Fermi Surface connected by this vector does not show well defined quasi-particles.

Apart from this peculiar anomaly close to the charge modulation wave-vector ( 0 0), it has been claimed that the overall bending down of the mode with character is well reproduced by DFT calculations Bohnen et al. (2003); Falter et al. (2006); Giustino et al. (2008) that reproduce a smooth cosine function shape. These calculations found that such mode has one of the highest coupling with charge carriers. Nevertheless, the calculated electron-phonon coupling was still too low to account for the strong kink in ARPES dispersion Giustino et al. (2008), and the very high of cuprates Bohnen et al. (2003). Moreover, similar calculations showed a concurrent strong downward bending of the mode, that can lead to discrepancies at the zone boundary X ( 0) between calculated and experimental frequencies in optimal or slightly under-doped compounds up to 10 meV Bohnen et al. (2003); Falter et al. (2006). It was suggested that such a difference originates from unrelated effects over the two directions (, 0, 0) and (, , 0)Bohnen et al. (2003). Note that Giustino and co-workers in Ref. Giustino et al., 2008 use the label half-breathing and full-breathing to distinguish Cu-O bond-stretching modes with different character, as in other worksPintschovius et al. (2006), but the full-breathing label is not consistent throughout literature, as it indicates modes with character in Ref. Pintschovius et al., 2006, while misleadingly label a dispersion along ( 0 0) with character in Ref. Giustino et al., 2008. It is worthwhile to notice that the later dispersion has been found to be flat for all dopings, either experimentally and theoretically. At the same time, the authors of Ref. Giustino et al., 2008 do not show their results along , where a very bad agreement is found in other DFT calculations Bohnen et al. (2003); Falter et al. (2006) and experimental data. We therefore avoid the ”breathing” notation.

Contrary to DFT simulations, our simple lattice dynamical calculation based on a shell model, reproduces well the dispersion of the mode with character, while missing the softening of the one with character, when using a screening wave number of (see Fig. 7). When increasing the doping, and consequently the screening wave number, we observe a modest softening for both bands. The effect is relatively weak in our calculations, as we have kept all other parameters fixed, in order to allow a direct comparison between the two cases. The important point here is that the softening affects exclusively the modes with and character, with a trend that reproduces the experimental one with increasing doping. This suggests that overestimated screening effects can lead to simulations that reproduce the dispersion at much higher doping. If compared to optimal or slightly under-doped compounds, this gives a dispersion which is accidentally similar to the one for the mode with character, while giving a large difference between calculation and experimental dispersion for the mode with character, and accordingly underestimate the electron-phonon coupling. Indeed, the dispersion found in Ref. Bohnen et al., 2003; Giustino et al., 2008 for the Cu-O bond-stretching modes with and character are strikingly similar to the experimental dispersion found only in highly overdoped cuprates LaMCuO (M=Sr,Ba)Pintschovius et al. (2006); d’Astuto et al. (2008). Therefore, a possible unique origin for the softening of modes with both and character in DFT calculation can not be ruled out. This would imply that the phonon simulations by DFT correspond to a much higher doping, that, because of the larger screening, have a lower electron-phonon coupling. To confirm such conclusion also in oxychlorides, it would be important to compare with DFT calculations, and to have data on the un-doped parent compound.

V Conclusions

We presented an extended study of the phonon dispersion in superconducting CaCuOCl, doped with Ca vacancies, close to optimal doping. We interpret the results using lattice dynamical calculations based on a shell model, and we compare them to what obtained for other hole-doped cuprates, in particular with the T-structure. We found an overall agreement between our model and the data, confirming the good choice of parameters of the common interatomic potential for the lattice dynamics of cuprates first proposed in Ref. Chaplot et al., 1995. An anomalous dip in the Cu-O bond stretching dispersion develops also in oxychlorides with a simultaneous marked broadening of the mode. The broadening maximum appears at that corresponds to the charge-modulations propagation vector, observed by means of STM experiments Hanaguri et al. (2004). Our data thus unveil a dynamic precursor state of the above modulations. By comparing our measurements on the longitudinal Cu-O bond-stretching mode in superconducting CaCuOCl with our model, we found that screening effect may bend downwards simultaneously the dispersions along both the ( 0 0) and ( 0) directions, a result that can help explaining the discrepancies between phonon dispersion based on DFT calculationsFalter et al. (2006); Bohnen et al. (2003) and the experimental data in cuprates.

Acknowledgements.
We are very grateful to M. Calandra and F. Mauri for useful discussion. We also thank S. Chaplot and M. Rao for encouraging exchanges and suggestions, and to R. Heid and T. Hanaguri for enlightening discussions and critical reading of the manuscript. We acknowledge D. Gambetti and B. Baptiste for technical help during measurements and A. Shukla for redaction suggestions. This work was supported by ESRF through Experiment No. HS-3461. I.Y. gratefully acknowledges the European Commission for financial support under the contract MIIF-CT-2006-0374.

References

  • Bednorz and Müller (1986) J. G. Bednorz and K. A. Müller, Z. Phys. B 64, 189 (1986).
  • Crawford et al. (1990) M. K. Crawford, W. E. Farneth, E. M. McCarronn, R. L. Harlow,  and A. H. Moudden, Science 250, 1390 (1990)http://www.sciencemag.org/content/250/4986/1390.full.pdf .
  • Bonn (2006) D. A. Bonn, Nature Physics 2, 158 (2006).
  • Bohnen et al. (2003) K.-P. Bohnen, R. Heid,  and M. Krauss, Europhys. Lett. 64, 104 (2003).
  • Giustino et al. (2008) F. Giustino, M. L. Cohen,  and S. G. Louie, Nature 452, 975 (2008).
  • Rösch and Gunnarsson (2004) O. Rösch and O. Gunnarsson, Phys. Rev. Lett. 93, 237001 (2004).
  • Falter et al. (2006) C. Falter, T. Bauer,  and F. Schnetgöke, Phys. Rev. B 73, 224502 (2006).
  • Tranquada et al. (1995) J. M. Tranquada, B. J. Sternlieb, J. D. Axe, Y. Nakamura,  and S. Uchida, Nature 375, 561 (1995).
  • Abbamonte et al. (2005) P. Abbamonte, A. Rusydi, S. Smadici, G. Gu, G. Sawatzky,  and D. Feng, Nat. Phys. 1, 155 (2005).
  • McQueeney et al. (1999) R. J. McQueeney, Y. Petrov, T. Egami, M. Yethiraj, G. Shirane,  and Y. Endoh, Phys. Rev. Lett. 82, 628 (1999).
  • Pintschovius and Braden (1999) L. Pintschovius and M. Braden, Phys. Rev. B 60, R15039 (1999).
  • Reznik et al. (2006) D. Reznik, L. Pitschovius, M. Ito, S. Iikubo, M. Sato, H. Goka, M. Fujita, K. Yamada, G. Gu,  and J. Tranquada, Nature 440, 1170 (2006).
  • d’Astuto et al. (2008) M. d’Astuto, G. Dhalenne, J. Graf, M. Hoesch, P. Giura, M. Krisch, P. Berthet, A. Lanzara,  and A. Shukla, Phys. Rev. B 78, 140511(R) (2008).
  • Reznik (2010) D. Reznik, Advances in Condensed Matter Physics 2010, 523549 (2010).
  • Reznik et al. (2008) D. Reznik, G. Sangiovanni, O. Gunnarsson,  and T. P. Devereaux, Nature 455, E6 (2008).
  • Butler et al. (1977) W. H. Butler, H. G. Smith,  and N. Wakabayashi, Phys. Rev. Lett. 39, 1004 (1977).
  • Weber et al. (2012) F. Weber, S. Rosenkranz, L. Pintschovius, J.-P. Castellan, R. Osborn, W. Reichardt, R. Heid, K.-P. Bohnen, E. A. Goremychkin, A. Kreyssig, K. Hradil,  and D. L. Abernathy, Phys. Rev. Lett. 109, 057001 (2012).
  • Hiroi et al. (2002) Z. Hiroi, N. Kobayashi,  and M. Takano, Nature 371, 139 (2002).
  • Yamada et al. (2005) I. Yamada, A. A. Belik, M. Azuma, S. Harjo, T. Kamiyama, Y. Shimakawa,  and M. Takano, Phys. Rev. B 72, 224503 (2005).
  • Hanaguri et al. (2004) T. Hanaguri, C. Lupien, Y. Kohsaka, D.-H. Lee, M. Azuma, M. Takano, H. Takagi,  and J. C. Davis, Nature 430, 1001 (2004).
  • Momma and Izumi (2008) K. Momma and F. Izumi, J. Appl. Crystallogr. 41, 653 (2008).
  • Yamada et al. (2007) I. Yamada, M. Azuma, Y. Shimakawa,  and M. Takano, Physica C 460-462, 420 (2007).
  • Pintschovius and Reichardt (1998) L. Pintschovius and W. Reichardt, in Physics and Chemistry of Materials with Low-Dimensional Structures, Vol. 20, edited by A. Furrer (Kluwer Academic Publishers, Dordrecht, 1998) p. 165.
  • Tajima et al. (1991) S. Tajima, T. Ido, S. Ishibashi, T. Itoh, H. Eisaki, Y. Mizuo, T. Arima, H. Takagi,  and S. Uchida, Phys. Rev. B 43, 10496 (1991).
  • (25) Data plot and fit obtained using Igor Pro (Wavemetrics, Lake Oswego, OR, USA).
  • Krisch and Sette (2007) M. Krisch and F. Sette, in Light Scattering in Solid IX, Topics in Applied Physics, Vol. 108, edited by M. Cardona and R. Merlin (Springer Berlin / Heidelberg, 2007) pp. 317–370.
  • Verbeni et al. (1996) R. Verbeni, F. Sette, M. Krisch, U. Bergmann, B. Gorges, C. Halcoussis, K. Martel, C. Masciovecchio, J. Ribois, G. Ruocco,  and H. Sinn, J. Synchrotron Radiation 3, 62 (1996).
  • Verbeni et al. (2008) R. Verbeni, M. d’Astuto, M. Krisch, M. Lorenzen, A. Mermet, G. Monaco, H. Requardt,  and F. Sette, Rev. Sci. Instrum.  (2008).
  • Masciovecchio et al. (1996) C. Masciovecchio, U. Bergmann, M. Krisch, G. Ruocco, F. Sette,  and R. Verbeni, Nucl. Instrum. Meth. B 111, 181 (1996).
  • James (1998) F. James, MINUIT Function Minimization and Error Analysis, Computing and Networks Division, CERN, Geneva (1998), (CERN D506 Long Writeup).
  • (31) Graphics obtained using MatplotlibHunter (2007), freely available on http://matplotlib.org/.
  • d’Astuto and Krisch (2010) M. d’Astuto and M. Krisch, JDN 10, 487 (2010).
  • d’Astuto et al. (2003a) M. d’Astuto, P. K. Mang, P. Giura, A. Shukla, A. Mirone, M. Krisch, F. Sette, P. Ghigna, M. Braden,  and M. Greven, International Journal of Modern Physics B 17, 484 (2003a).
  • Mirone (2001) A. Mirone, “OpenPhonon code source,”  (2001).
  • Paulatto et al. (2012) L. Paulatto, A. Mirone,  and M. d’Astuto,  (2012), private communication.
  • d’Astuto et al. (2002) M. d’Astuto, P. K. Mang, P. Giura, A. Shukla, P. Ghigna, A. Mirone, M. Braden, M. Greven, M. Krisch,  and F. Sette, Phys. Rev. Lett. 88, 167002 (2002).
  • d’Astuto et al. (2003b) M. d’Astuto, A. Mirone, P. Giura, D. Colson, A. Forget,  and M. Krisch, Journal of Physics: Condensed Matter 15, 8827 (2003b).
  • Chaplot et al. (1995) S. L. Chaplot, W. Reichardt, L. Pintschovius,  and N. Pyka, Phys. Rev. B 52, 7230 (1995).
  • Mittal et al. (2003) R. Mittal, S. L. Chaplot, A. Sen, S. N. Achary,  and A. K. Tyagi, Phys. Rev. B 67, 134303 (2003).
  • Chaplot (1988) S. L. Chaplot, Phys. Rev. B 37, 7435 (1988).
  • Zenitani et al. (2005) Y. Zenitani, H. Kawashima, T. Suzuki, J. Akimitsu, N. Ogita, T. Kondo,  and M. Udagawa, Journal of the Physical Society of Japan 74, 1877 (2005).
  • d’Astuto and Lamago (2012) M. d’Astuto and D. Lamago,  (2012), private communication.
  • Tassini et al. (2005) L. Tassini, F. Venturini, Q.-M. Zhang, R. Hackl, N. Kikugawa,  and T. Fujita, Phys. Rev. Lett. 95, 117002 (2005).
  • Sugai et al. (2006) S. Sugai, Y. Takayanagi,  and N. Hayamizu, Phys. Rev. Lett. 96, 137003 (2006).
  • Caprara et al. (2005) S. Caprara, C. Di Castro, M. Grilli,  and D. Suppa, Phys. Rev. Lett. 95, 117004 (2005).
  • Lucarelli et al. (2003) A. Lucarelli, S. Lupi, M. Ortolani, P. Calvani, P. Maselli, M. Capizzi, P. Giura, H. Eisaki, N. Kikugawa, T. Fujita, M. Fujita,  and K. Yamada, Phys. Rev. Lett. 90, 037002 (2003).
  • Venturini et al. (2002) F. Venturini, Q.-M. Zhang, R. Hackl, A. Lucarelli, S. Lupi, M. Ortolani, P. Calvani, N. Kikugawa,  and T. Fujita, Phys. Rev. B 66, 060502 (2002).
  • Pintschovius et al. (2006) L. Pintschovius, D. Reznik,  and K. Yamada, Phys. Rev. B 74, 174514 (2006).
  • Weber et al. (2009) F. Weber, N. Aliouane, H. Zheng, J. F. Mitchell, D. N. Argyriou,  and D. Reznik, Nature Mater. 8, 798 (2009).
  • Kohsaka et al. (2007) Y. Kohsaka, C. Taylor, K. Fujita, A. Schmidt, C. Lupien, T. Hanaguri, M. Azuma, M. Takano, H. Eisaki, H. Takagi, S. Uchida,  and J. C. Davis, Science 315, 1380 (2007)http://www.sciencemag.org/content/315/5817/1380.full.pdf .
  • Shen et al. (2005) K. M. Shen, F. Ronning, D. H. Lu, F. Baumberger, N. J. C. Ingle, W. S. Lee, W. Meevasana, Y. Kohsaka, M. Azuma, M. Takano, H. Takagi,  and Z.-X. Shen, Science 307, 901 (2005).
  • Hunter (2007) J. D. Hunter, Computing In Science & Engineering 9, 90 (2007).
Comments 0
Request Comment
You are adding the first comment!
How to quickly get a good reply:
  • Give credit where it’s due by listing out the positive aspects of a paper before getting into which changes should be made.
  • Be specific in your critique, and provide supporting evidence with appropriate references to substantiate general statements.
  • Your comment should inspire ideas to flow and help the author improves the paper.

The better we are at sharing our knowledge with each other, the faster we move forward.
""
The feedback must be of minimum 40 characters and the title a minimum of 5 characters
   
Add comment
Cancel
Loading ...
271795
This is a comment super asjknd jkasnjk adsnkj
Upvote
Downvote
""
The feedback must be of minumum 40 characters
The feedback must be of minumum 40 characters
Submit
Cancel

You are asking your first question!
How to quickly get a good answer:
  • Keep your question short and to the point
  • Check for grammar or spelling errors.
  • Phrase it like a question
Test
Test description