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New J. Phys. 11 (2009) 113009
doi:10.1088/1367-2630/11/11/113009

Lattice vibrations in CaV2O5 and their manifestations: a theoretical study based on density functional theory

J Spitaler1,2,5, C Ambrosch-Draxl1,2 and E Ya Sherman3,4

1 Chair of Atomistic Modelling and Design of Materials, University of Leoben, Franz-Josef-Strasse 18, A-8700 Leoben, Austria
2 Institut für Physik, University of Graz, Universitätsplatz 5, A-8010 Graz, Austria
3 Departamento de Química Física, Universidad del País Vasco—Euskal Herriko Unibertsitatea, 48080 Bilbao, Spain
4 IKERBASQUE Basque Foundation for Science, Alameda Urquijo 36-5, 48011, Bilbao, Bizkaia, Spain

5 Author to whom any correspondence should be addressed.

E-mail: juergen.spitaler@unileoben.ac.at

Received 30 July 2009
Published 5 November 2009

Abstract. We present a comprehensive ab initio study of all non fully symmetric Γ point lattice vibrations in CaV2O5. The characteristics of CaV2O5 are a half-filled upper electron band and a ladder-like crystal structure. Adopting the frozen-phonon approach we calculate and analyze in detail the phonon eigenfrequencies and eigenvectors. The corresponding spectra of inelastic light scattering are computed for all Raman-active modes, including their resonance behavior as a function of incoming light. Our results allow for a qualitative and quantitative understanding of the phonon-related features in experimental optical excitation spectra. The theoretical data are employed to discuss available measurements and provide an improved assignment of the observed modes with respect to symmetry and displacement patterns. Electron hopping parameters and spin–spin exchange matrix elements are evaluated from the electronic bands. The changes in these parameters upon atomic displacements along the phonon eigenvectors are analyzed semiquantitatively, yielding the effect of lattice vibrations on charge and spin degrees of freedom. It is discussed how all the obtained results differ from the ones in the quarter-filled NaV2O5 compound due to differences in the electron band structure and in the chemistry.

Contents

1. Introduction

Fascinating physical properties of ladder compounds have been stimulating very active studies in this field over the last 15 years [1], (and references there in [2]). The common feature of these crystals are the pairs of metal ions linked by an oxygen, which form the rungs of the ladder. These rungs are arranged in one dimension in the direction of the ladders' legs. The main electron–electron interactions and electron motion occur within one ladder, while the interactions between neighboring ladders in the same plane are considerably weaker, and ladders in different planes are hardly coupled. In this situation, the coupling of the charge, spin and lattice degrees of freedom causes a rich variety of physical phenomena.

The most intensively studied examples of ladder compounds are formed by copper ions with spin 1/2 per magnetically active site and have half-filled upper bands, such as SrCu2O3 or (Sr, Ca)14Cu24O41. However, there exist also two half-filled V-based ladder compounds, namely CaV2O5 and MgV2O5. In spite of the fact that Ca and Mg have the same valence configuration and both compounds are very similar in their V subsystem, they form crystals with different space groups: Cmnm and Pmmm for MgV2O5 and CaV2O5, respectively. The structural differences have a strong impact on the magnetic properties [3, 4]. While CaV2O5 is best described as a collection of well-isolated single two-leg spin ladders [5, 6], MgV2O5 exhibits an additional strongly frustrated interladder coupling [7, 8]. This leads to a very large gap of 500 K for the triplet excitations in the former compound [5], while in the latter a small gap of only 15 K is observed experimentally [7].

In addition to half-filled systems, V-based ladders show the unique realization of quarter-filling in NaV2O5 [10], which emphasizes the crucial importance of the chemical composition. Since a spin-Peierls transition in this compound was discovered NaV2O5 has become the most intensively investigated vanadium ladder system. It is especially interesting in the context of a comparison with CaV2O5 since both compounds crystallize in the same Pmmn structure with two formula units per unit cell (figure 1) at room temperature.

Figure 1

Figure 1.  The crystal structure of CaV2O5.Note6 

Since the properties of the ladder compounds are expected to be strongly influenced by the interplay of the electron motion, the lattice and the magnetic degrees of freedom, quantitative information about spin–lattice and charge–lattice coupling is strongly desirable, however, so far still lacking. To fill this gap and to gain an understanding of the physics of these compounds, we perform, to the best of our knowledge, the first ab initio investigation of the lattice dynamics of all non fully symmetric phonons in a half-filled ladder system using the example of CaV2O5. We report the theoretical phonon frequencies and eigenvectors for the B1g, B2g and B3g modes, which are visible in Raman measurements, as well as all infrared-active vibrations, seen in light absorption and reflection experiments. A detailed comparison of the theoretical results, including the calculated Raman spectra, to experiment is presented and allows for a better understanding of the inelastic light scattering in this compound. In addition, we study electron– and spin–phonon coupling by mapping the ab initio results on a model band structure and identify the modes showing strong coupling to the electron subsystem. We relate the properties of CaV2O5 to those of NaV2O5 to understand the role of the electron occupancy at the vanadium site, which determines the filling of the upper electron band.

2. Computational methods

All total-energy and band-structure calculations are performed within density functional theory (DFT) using the full-potential augmented plane waves + local orbitals (FP-APW + lo) [11] formalism implemented in the WIEN2k code [12]. Exchange and correlation terms are described within the generalized gradient approximation (GGA) [13]. The atomic sphere radii are chosen as 1.6 au for V, 1.8 au for Ca and 1.4 au for the O atoms. A Kmax value of 4.64 is used in all calculations, corresponding to RMT×Kmax values of 6.5 for O, 7.43 for V and 8.36 for Ca.

The number of k points in the full Brillouin zone (BZ) for the self-consistent field cycles is typically about 600. For the calculation of the dielectric function, which serves as input for the Raman spectra, a number of 3800 k points in the full BZ is used. The Gmax used for charge density and potential is 14. The internal geometry is fully relaxed, taking the experimental atomic positions reported in [14] as starting point. Details about the relaxation can be found in [15].

The phonon eigenfrequencies and eigenvectors are determined in the frozen-phonon approximation, where for each degree of freedom corresponding to the symmetry coordinates four displacements, two in positive and two in negative direction, are considered. The symmetry coordinates for each irreducible representation can be inferred from the degrees of freedom appearing in the corresponding table and figure, respectively.

3. Phonon modes

A factor group analysis yields, after subtraction of three acoustic (B1u + B2u + B3u) and three silent Au modes,

\begin{eqnarray*} \fl\Gamma = 8 A_g (xx,yy,zz)+ 3 B_{1g} (xy) + 8 B_{2g} (xz) + 5 B_{3g} (yz) \nonumber \\ [3pt] \quad +7 B_{1u} ({\bf E} \parallel \hat{z}) +4 B_{2u} ({\bf E} \parallel \hat{y}) + 7 B_{3u} ({\bf E} \parallel \hat{x}), \end{eqnarray*}\noindent

where the letters in parenthesis indicate the polarization of the incoming and outgoing light, respectively. Hence, there are 24 Raman-active Ag and Bng modes and 18 infrared-active Bnu modes (nin{1, 2, 3}). The eigenvectors and frequencies of the Raman-active B1g, B2g and B3g, and all infrared-active phonon modes are presented in table 1, while the fully symmetric Γ point phonons have already been published in [15]. The eigenvectors eαζ (where α denotes the atom and ζ indicates the phonon mode) are normalized with respect to the whole unit cell including two formula units of CaV2O5. For each set of equivalent atoms only the components corresponding to one atom are reported, where this reference atom is highlighted in the respective figures using bold italic characters.

Table 1. Calculated eigenfrequencies in cm–1 and eigenvectors of Γ point phonon modes of CaV2O5. An assignment of the modes in terms of the actual displacement patterns is given in tables 2 and 3, respectively.
ωζ Eigenvector
(cm–1) Vx Vy Vz Cax Cay Caz O1x O1y O1z O2x O2y O2z O3x O3y O3z
B1g                              
593 –0.17 0.47 0.01
253 –0.28 –0.11 0.40
136 0.38 0.14 0.30
B2g                              
842 0.04 –0.25 –0.02 0.03 –0.03 –0.01 –0.05 0.43
652 –0.21 –0.02 –0.01 0.62 –0.07 –0.07 –0.02 –0.04
499 –0.01 0.03 0.02 –0.04 –0.48 0.12 –0.01 –0.02
342 –0.33 0.18 –0.04 –0.12 –0.03 –0.21 0.18 0.15
259 –0.19 –0.23 –0.05 –0.03 0.06 0.29 0.25 –0.07
219 0.28 –0.02 –0.14 0.07 –0.07 –0.16 0.36 –0.02
190 –0.04 –0.28 0.39 –0.06 –0.06 –0.26 0.05 –0.15
135 –0.10 –0.24 –0.38 –0.09 –0.05 –0.20 –0.18 –0.17
B3g                              
605 –0.18 –0.00 –0.01 0.46 0.02
392 –0.16 –0.11 0.59 –0.06 0.19
254 –0.27 0.06 –0.20 –0.12 0.38
195 0.24 –0.51 –0.10 0.08 0.22
113 –0.34 –0.28 –0.07 –0.13 –0.27
B1u                              
903 –0.09 0.23 –0.01 0.03 0.05 –0.01 0.10 –0.42
559 –0.30 –0.02 0.02 –0.00 0.37 –0.10 0.05 0.11
483 –0.15 –0.25 0.00 0.39 –0.05 0.28 0.06 –0.07
348 0.11 0.11 –0.06 0.34 0.07 –0.25 –0.31 –0.00
282 0.17 –0.08 0.04 –0.12 0.27 0.25 –0.24 –0.12
235 –0.30 –0.05 0.13 –0.13 –0.19 –0.02 –0.32 –0.07
195 –0.14 0.14 –0.56 –0.06 –0.04 0.18 –0.11 0.09
B2u                              
550 0.26 0.01 –0.01 –0.43 –0.04
401 –0.16 –0.10 0.58 –0.13 0.19
229 –0.16 0.06 –0.21 –0.13 0.43
196 0.23 –0.56 –0.06 0.11 0.16
B3u                              
845 –0.05 0.24 0.02 –0.01 0.01 –0.00 0.06 –0.43
658 –0.18 –0.07 –0.01 0.63 –0.10 0.01 –0.01 –0.03
479 –0.24 0.03 0.01 0.00 0.41 –0.14 –0.02 0.05
367 0.12 0.24 –0.03 0.06 –0.09 –0.38 –0.10 0.11
229 –0.13 0.08 –0.09 –0.03 –0.09 –0.04 0.44 0.12
174 0.20 –0.02 –0.58 0.07 0.17 0.06 0.00 –0.05
114 –0.07 –0.34 –0.06 –0.07 –0.09 –0.28 0.03 –0.18

3.1. Eigenvectors

Due to the structural similarity to NaV2O5 most of the phonon modes of both compounds are close in frequency [16], and the eigenvectors differ only very little. Figure 2 shows a selection of phonon modes which most strongly differ from their NaV2O5 counterparts.

Figure 2

Figure 2.  Selected Γ point phonon modes of CaV2O5. The arrows show the direction and magnitude of the eigenvectors for each eigenmode, i.e. they are proportional to the displacement times the square root of the mass of the corresponding atom. The reference atoms of table 1 are indicated with bold blue letters.

As in the case of NaV2O5 the eigenvectors of the B1g modes represent a V–O2 stretching, an O3–V–O2 bending, and a vibration where the two legs of one ladder are shifted anti-parallelly along \hat{y} , respectively. The same situation is found for the B2g modes, where the features of the atomic displacements are the same as in the Na compound.

Within the B3g vibrations, two CaV2O5 modes exhibit a particular behavior. The O1–V–O2 B3g mode with 392 cm–1 has some contribution from the Ca atom moving in the {\hat y} -direction, in contrast to Na which hardly participates in the corresponding NaV2O5 mode. For the 195 cm–1 vibration with the same symmetry, where Ca moves out of phase with respect to the ladder and parallel to the {\hat y} -axis, the Ca eigenvector component is twice as large as the corresponding Na component in NaV2O5. Moreover, in CaV2O5 also the in-rung oxygen O1 takes part. Also two of the B1u phonon modes differ from their counterparts in NaV2O5: in CaV2O5, the V–O2–V bending mode (559 cm–1) does not involve a shift of the in-rung oxygen O1, which is present in NaV2O5, and the apex oxygen O3 has a considerable z-component. In the 483 cm–1B1u mode the O3 atom has a larger x-component, while the x-component of the in-leg oxygen O2 is quite small compared to the NaV2O5 mode. Among the phonons with B2u symmetry, the 401 cm–1 vibration shows a noticeable Ca contribution, which makes it differ from the O1–V–O3 bending mode of NaV2O5. The B3u vibration exhibiting the clearest deviation from its NaV2O5 counterpart is the one with 479 cm–1. This mode represents a pure O2–V–O2 bending in the xy plane in CaV2O5, while in NaV2O5 the in-rung oxygen O1 participates considerably.

3.2. Frequencies

Given the close relation between the two compounds in terms of their eigenvectors, it is of special interest to compare the frequencies in CaV2O5 and NaV2O5 (presented in [16]) since they can give a direct information on the bonding and the interaction between the atoms in the two materials. It turns out that the phonon modes can be divided into several groups showing different tendencies in terms of the phonon frequency.

The first group is formed by the V–O3 stretching modes and exhibits a strong frequency decrease compared to NaV2O5. In detail, the changes are –14% for the mode with B2g symmetry (842 cm–1), –7% for the one with B1u symmetry (903 cm–1) and –10% for the B3u V–O3 stretching mode (845 cm–1). A very similar tendency is found for the V–O2 stretching modes, where the frequencies are lowered by 10 and 15% in case of the B1g (593 cm–1) and the B3g vibration (605 cm–1), respectively. In this context the V–O2 stretching mode of the B2u species (550 cm–1) represents an exception, since its frequency is only slightly decreased with respect to NaV2O5. The main reason for the lower energy of the V–O stretching in CaV2O5 is found in the chemical difference between Na and Ca. While Na contributes only one s electron to the system, thus yielding V4.5 +  ions, the extra valence electron in Ca reduces the formal V charge to 4. Correspondingly, a Coulomb picture would imply a frequency decrease by a factor of \sqrt{4/4.5} , i.e. approximately 6%.

A trend to lower frequencies is also found for the group of V–O2–V bending modes with components perpendicular to the xy plane. These vibrations also change the length of the V–O3 bond, such that the same argument as for the stretching modes applies. In case of the B2g vibration with 259 cm–1 and the B3u vibration with 367 cm–1 the decrease is about 10%, while it is more moderate for the 342 cm–1B2g mode with 5%. The B1u483 cm–1 and the B1u348 cm–1 vibrations have very similar frequencies in both CaV2O5 and the NaV2O5.

The situation is different for the V–O2–V bending modes parallel to the xy plane. Here the vibrations in the Ca compound rather exhibit a frequency increase, which is only 1% for the B1u mode with 559 cm–1, but 6% for the 499 cm–1B2g mode and even 8% for the B3u mode with 479 cm–1. This tendency can be related to the stronger ladder–ladder interaction, which shows up in the slightly smaller inter-ladder distance in CaV2O5 (1.98 Å, compared to 2.01 Å in NaV2O5) and in a much larger inter-ladder hopping parameter ti [15]. The latter can be explained by a stronger overlap of orbitals of the V and O2 atoms in neighboring ladders, a consequence of the fact that the z coordinates of these two atoms differ by 0.06 Å less in CaV2O5zV,O2 = 0.42 Å) compared to NaV2O5zV,O2 = 0.48 Å).

The last group is represented by low-energy modes involving Ca. These modes show much higher frequencies compared with their counterparts in NaV2O5. In detail, the increase is 21% in the B2g mode with 190 cm–1, 4% in the B3g mode with 195 cm–1, 24% in the 235 cm–1B1u mode, 27% in the B1u vibration with 195 cm–1, 13% for the B2u mode with 196 cm–1 and 20% in the 174 cm–1B3u vibration. A straightforward explanation of this tendency is delivered by the larger ionicity of Ca2 +  than Na +  ions. This effect alone would imply even larger frequency increases, but it is partly compensated by the larger mass of Ca (40.08 au) compared with Na (22.99 au).

4. Comparison with experiment

4.1. Raman spectra

In order to compute the Raman intensities the atoms are displaced according to the calculated eigenvectors, and the dielectric function for the distorted crystal is calculated. The changes of the dielectric function with respect to such displacements along an eigenvector of mode ζ allow the determination of the corresponding Raman intensity Iij. To this end we first define the operator {\hat{Q}} corresponding to the phonon coordinate via the following relation with the actual displacement coordinate uζα:

Equation (1)

Here, Mα is the mass of ion α and ωζ defines the corresponding frequency. Then, Iij is given by

Equation (2)

where ωR is the Raman shift, the Cartesian indices ij correspond to the polarizations of incident and scattered light, respectively, |1rangle and |0rangle denote the one-phonon and the phonon-less states, respectively, nBζ) = 1/[exp(hslashωζ/T)–1] is the phonon Bose distribution function, ωI is the frequency of the incoming light, and LR, ωζ, Γ) is the Lorentzian shape of the phonon line with a broadening Γ, which is chosen to be 15 cm–1 for all modes. Further information on the applied method can be found in [17].

The results for the B1g, B2g and B3g modes are presented in figure 3. The highest peaks are found at 593 cm–1 for xy polarization, at 135, 259 and 652 cm–1 for xz polarization, and at 254 cm–1 for yz polarization. A specially subtle feature is found for the 219 cm–1B2g peak, which is surrounded by much higher neighbors. The signal of the B3g mode at 195 cm–1 is completely covered by the strongly dominating 254 cm–1 peak.

Figure 3

Figure 3.  Theoretical Raman spectra for the B1g (upper panel), the B2g (central panel) and the B3g modes (lower panel) of CaV2O5, with the polarization of the incoming and outgoing light in parenthesis. All spectra are calculated for an incoming photon energy of 2.54 eV (514 nm).

Figure 4 shows the change of the dielectric function for atomic displacements along the respective eigenvector, i.e. |∂εij/∂Q|2, for selected B1g, B2g and B3g modes, where modes with maximum changes smaller than 0.01 have been omitted. Large values of |∂εij/∂Q|2 at a certain photon energy imply resonances observed with the corresponding laser frequency. Figure 4 shows that some of the modes exhibit a strong dependence on the applied photon energy, among them the B2g mode with 253 cm–1, the B2g mode with 652 cm–1 and the B3g mode with 254 cm–1. Moreover, it is found that the experimentally used 514.5 nm (2.41 eV) line of an Ar +  ion laser [18]–[20] leads to a very small response of the system for all but the 254 cm–1B3g mode. Instead, all modes exhibit resonances for photon energies below 2.0 eV, and many of the modes at photon energies between 2.5 and 3.0 eV.

Figure 4

Figure 4.  Change of the dielectric function with respect to displacements along the eigenvector as a function of the photon energy ωζ for selected phonon modes. Left panel: |∂εxy/∂Q|2 for the B1g modes; upper right panel: |∂εxz/∂Q|2 for the B2g modes; lower right panel: |∂εyz/∂Q|2 for the B3g modes.

In literature one polarized Raman measurement using a polycrystalline sample [18] and two unpolarized ones [19, 20] are reported, but there are no spectra obtained from CaV2O5 single crystals. For this reason no unambiguous experimental evidence for the symmetry of the peaks is found. Table 2 shows a comparison of the measured results with theoretical frequencies.

Table 2. Comparison of theoretical frequencies with experimental results from literature for the Raman-active phonon modes of CaV2O5. Columns marked with * represent an assignment of experimental spectra based on theoretical frequencies and Raman intensities.
  Experiment    
   [18]  [18]*  [20]*  [19]  [19]* Theory Assignment
B1g 638 638 636 636 636 593 V–O2 stretching
  292 292 253 O3–V–O2 bending
  212 137 182 138.6 136 antiparallel leg-shift
B2g 842 V–O3 stretching
    652 V–O1 stretching
  499 O2–V–O1 bending
  310 334 311 342 O2–V–O3 bending
  292 293 311 292 259 O2–V–O3 bending
  212 211 213 213 219 Ca-ladder shear
  182 190 Ca \parallel{\hat{x}} + {\rm chain \ rotation}
  137 138.6 135 chain rotation
B3g 636 605 V–O2 stretching
  369 366 366 392 O1–V–O3 bending
  212 212 280 213 254 rung versus O3 shear
  195 (ladder versus Ca) \parallel{\hat{y}}
  112 112 113 antiparallel ladder shift

Theory reveals that the experimental feature at 638 cm–1 goes back to the highest-frequency B1g mode, which shows up as a very pronounced peak in the theoretical Raman spectra. A B2g mode at almost the same energy is probably covered by the B1g signal in experiment. A measured feature at 138 cm–1, which was interpreted as Ag mode in [19], and not assigned any symmetry in [18], can neatly be traced back to a superposition of the B1g and the B2g peak lowest in energy. A peak measured at about 370 cm–1 is explicitly addressed in [19] and also clearly visible in the crossed-polarized spectra of [18]. This peak is in reasonable agreement with the low theoretical B3g peak at 392 cm–1. The situation is comparable for the modest B2g feature at 342 cm–1, which is resolved in the unpolarized measurements [19, 20] at a slightly lower energy of 311 cm–1. Very good agreement is found for the theoretical B2g peak at 190 cm–1 and the experimental peak at 182 cm–1. A B3g feature at virtually the same energy has very low intensity and is therefore either not visible in experiment or integrated in the stronger B2g peak. Another B3g feature, which is not explicitly addressed in the experiment, but still distinguishable, is found at 113 cm–1, where the position of the experimental and the theoretical peak agree perfectly.

The comparison of ab initio results and measurements is more intriguing for the frequency range between 200 and 300 cm–1: while experiments show two pronounced peaks at 212 and 292 cm–1, theory yields high-intensity peaks at 259 cm–1 in the B2g spectra and at 254 cm–1 in the B3g spectra. Since the peak belonging to the latter is by far the highest, it most probably can be related to the measured feature at 212 cm–1, while the intensity of the former mode is in good qualitative agreement with the experimental peak at 292 cm–1. A third phonon mode with almost the same theoretical frequency is found among the B1g vibrations. However, the intensity of this mode is much smaller, which implies that in the experimental spectra it is probably masked by the Ag peak at 238 cm–1. The tiny calculated B2g peak appearing at 212 cm–1 is most probably integrated in the large experimental feature at 219 cm–1.

For the rest of the Raman peaks no experimental counterpart is found, in perfect accordance with theory yielding very low scattering intensities.

4.2. Infrared active modes

In table 3, the theoretical frequencies for the infrared-active phonon modes are compared to experiment. To the best of our knowledge up to now only one, unpolarized measurement is found in literature [19], where a symmetry assignment was only done by comparison with polarized results for NaV2O5. Thus theory can substantially contribute to a proper symmetry assignment of the peaks. The root mean square deviation between measured and calculated frequencies is less than 5%, with the largest difference (–9 cm–1 = –7.3%) found for the B3u chain-rotation mode with a theoretical frequency of 123 cm–1. As in [16] we have estimated the theoretical intensities of the infrared spectra. To do so, we have calculated the dipole moment P induced by a phonon distortion using a simple model with fixed ion charges (V4.5 + , Ca2 + , O2–), but taking into account the real displacements according to the eigenvectors.

Table 3. Comparison of theoretical frequencies with experimental results from literature for the infrared-active phonon modes of CaV2O5. The column marked with * represents an assignment of experimental spectra based on theoretical frequencies.
  Experiment    
   [19]  [19]* Theory Assignment
B1u 957 957 903 V–O3 stretching
  579 559 V–O2 stretching
  483 O1–V–O2 bending
  348 O1–V–O2 bending  +  O3x
  264 264 282 rung stretching
  244 235 O1–V–O3 bending  +  Ca \parallel{\hat{z}}
  198 198 195 Ca \parallel\hat{z}
B2u 579 515 550 V–O2 stretching
  369 408 401 O1–V–O3 bending
  229 O3 versus ladder shear
  123 198 196 Ca \parallel{\hat{y}}
B3u 892 892 845 V–O3 stretching
  515 658 O1 \parallel\hat{x}
  408 479 O2–V–O1 bending \parallel{\hat{x}}
  369 367 V–O2 bending \parallel{\hat{z}}
  244 229 V–O3 bending
  174 Ca \parallel{\hat{x}}
  123 114 chain rotation

In the experimental infrared spectra, we identify five features as stemming from B1u phonons: in addition to the ones at 957, 282 and 198 cm–1, already identified in [19], the theoretical results show that also the 579 cm–1 and the peak at 198 cm–1 are related to a B1u vibration. In case of the former not only the theoretical frequency but also the rather small induced dipole moment imply that this small experimental peak is associated with the calculated mode at 559 cm–1. The latter turns out to represent a superposition with a B2u mode at the same frequency.

Other B2u modes that can be distinguished in experiment are found at 515 cm–1, where the large phonon-induced dipole moment obtained by theory agrees nicely with experiment, and the feature at 408 cm–1, which just perfectly corresponds to the calculated phonon energy. This is in contrast to the assignment obtained by comparison with NaV2O5, which related these two peaks to B3u modes [19].

The peak at 892 cm–1, which is the second highest in frequency in the infrared spectra, is readily identified as belonging to the B3u species. While the two phonon modes next lower in frequency are not found in the measurement, the peak at 369 cm–1 fits perfectly to the theoretical result of 367 cm–1. The feature with the lowest energy in the measurement, i.e. the one at 123 cm–1, clearly belongs to the B3u species, which means that the assignment based on the comparison with NaV2O5 fails in this case.

5. Model parameters

In order to extract effective model parameters from the Kohn–Sham band structure six bands where mapped onto a tight-binding model, namely the bonding and anti-bonding pair of the V 3 dxy bands at the Fermi level and the two highest lying O 2p bands. We restrict ourselves to the direction {\bf k}\parallel {\hat{y}} and take into account the hopping along the ladder t||, the in-rung hopping t, and the inter-ladder transfer ti. Since the overall features of the electronic structure, except for the Fermi energy, are very similar to the ones in NaV2O5, the same mapping procedure as described [16] is applicable.

The values of the hopping parameters in the undistorted structure, t|| = 0.143, t = 0.321 and ti = 0.244 eV, as well as the vanadium Hubbard parameter U = 2.45 eV have been presented in [15]. With the knowledge of these parameters, one can calculate the spin–spin exchange. Below we consider exchange along the ladder J||, using the expression J|| = t||2/Eg, where Eg is the charge transfer gap between V and O [21]. In order to compare the electron– and spin–phonon coupling parameters for the different phonon modes with each other, the displacements are normalized with respect to the dimensionless phonon coordinate Q defined in equation (1). Since the contribution to Eg which is linear in Q vanishes for all but the fully symmetric phonons, we consider below only the effect of the lattice vibrations on the hopping and spin–spin exchange.

The largest parameters of electron–phonon and spin–phonon coupling for the Raman active B1g, B2g and B3g vibrations and all infrared active phonon modes of CaV2O5t||Q≥0.008 eV), are presented in table 4. Comparing the coupling of t|| to lattice distortions corresponding to the Γ point vibrations, similarly to NaV2O5 , the strongest effect is related to the V–O2 stretching modes. Again, the largest value (δt||Q = 0.040 eV) is found for the B1g mode highest in frequency. This vibration is followed by the B3g V–O2 stretching with 605 cm–1 (figure 5), with a δt||Q of 0.016 eV, where the corresponding parameter is much less significant in the respective mode of NaV2O5. The phonon mode with the next smaller change of t|| coincides with its counterpart in NaV2O5 again, i.e. it is the B1u mode second highest in energy.

Figure 5

Figure 5. Two phonon modes with strong electron phonon coupling.

Table 4. Parameters of electron–phonon (eV) and spin–phonon coupling for selected phonon modes of CaV2O5 (frequency ωζ in cm–1) as obtained from theory. The model parameters for the undistorted system [15] are t|| = 0.143 eV and t = 0.321 eV, respectively.
Symmetry ωζ Assignment \frac{\delta t_\parallel}{\delta Q} \frac{\delta J_\parallel}{J_\parallel \delta Q}
B1g 593 V–O2 stretching 0.040 0.601
B3g 605 V–O2 stretching 0.016 0.210
B3g 254 rung versus O3 shear 0.009 0.139
B3g 113 antipar. ladder shift 0.008 0.134
B1u 903 V–O3 stretch. 0.008 0.104
B1u 559 V–O2 stretch. 0.013 0.155
B1u 483 O1–V–O2 bend. 0.008 0.106

The t show very weak coupling to phonon-distortions for all phonon modes considered here, with all values of δtQ less than 0.007 eV, and are therefore not presented in the table. This means that the Ag vibrations [15] have by far the strongest effect on the hopping matrix element along the rung.

The spin–phonon coupling parameters expressed in terms of relative changes of J|| as induced by phonon distortions are presented in the last column of table 4. In CaV2O5, the highest values for δJ||/(J||δQ) are found for the V–O2 stretching modes with B1g symmetry (0.601), B3g symmetry (0.210), Ag symmetry (0.186) and B1u symmetry (0.155). In fact, the mentioned vibrations are also the ones dominating the electron–phonon coupling of hoppings along the ladder, which seems reasonable due to the interrelation of both quantities. Besides, also in NaV2O5 the V–O2 stretching modes turn out to give the largest respective parameters. All other phonon modes lead to changes of δJ||/J|| per δQ smaller than 0.15. Since t changes very little, all phonon-induced changes of J for the considered phonon modes are very small, too.

6. Conclusions

We have determined the frequencies and eigenvectors of all Raman- and infrared-active low-symmetry Γ point phonons of CaV2O5, a representative example of a half-filled compound with a ladder-like crystal structure. Our results provide detailed information on the lattice dynamics, which is desirable for both, the understanding of experimental data and the development of better models to describe such compounds. Our results provide the first direct symmetry assignment of the phonon modes, thus complementing former assignments based on a mere frequency-based comparison with polarized Raman experiments for NaV2O5 single crystals [19].

We have compared the phonon eigenvectors to the ones of the isostructural NaV2O5, and we have found that, in contrast to the latter, not only the low-frequency vibrations but also the O2–O1–O2 bending modes with B3g symmetry (392 cm–1) and B2u symmetry (401 cm–1) mode exhibit a significant Ca contribution. This shows that the interaction between the in-leg oxygen O1 and the interstitial ion is significantly larger than in NaV2O5, which is also reflected in the smaller distance between them (2.31 Å in CaV2O5, compared with 2.43 Å in NaV2O5).

In terms of frequencies we have distinguished four different groups of vibrations: the first two of them, i.e. the V–O3 stretching modes and the V–O2–V bending modes out of the xy plane, show significantly lower frequencies compared to their NaV2O5 counterparts, which is due to the different chemical situation where Ca provides one more valence electron to the two V sites of one rung, thus increasing its own ionicity and lowering the positive charge on the V sites. In contrast, V–O2–V bending modes within the xy plane show rather higher frequencies compared to NaV2O5, which is due to the stronger overlap of orbitals of the V and O2 atoms in neighboring ladders, a consequence of the fact that the z-coordinates of these atoms differ less in CaV2O5 compared with NaV2O5. The group of low-frequency vibrations involving Ca2 + , finally, exhibits strongly increased phonon frequencies due to the much stronger ionicity compared to Na +  in the sodium ladder compound.

We have calculated the spectra of all Raman active Γ point phonons from first principles, thus providing a sound basis for the analysis of the experimental spectra. This way we can make a direct assignment of the experimental peaks in terms of their symmetry. We have shown that, for example, the experimental peak at 139 cm–1 goes back to a superposition of a B1g and a B2g mode, and that a small feature at 113 cm–1, which is clearly visible but not explicitly addressed in the experimental works, is related to the anti-parallel ladder shift with B3g symmetry. In addition to the Raman spectra, we have determined the dependence of the Raman intensities on the energy of the exciting photons. It turns out that for the photon energy applied in the available experiments the response of the system is rather weak, while strong resonances for all modes are found at energies below 2 eV, and for many phonon modes at the energies between 2.5 and 3.0 eV. Hence, we propose to perform Raman experiments with corresponding laser frequencies, which would allow us to see phonon modes not observed before.

The theoretical eigenmodes of the infrared active phonons, together with an estimate of their induced dipole moment, elucidate experiments as well. We have improved the interpretation of the measured spectra, and shown, e.g. that the experimental feature at 579 cm–1 stems from a B1u mode, while the peak at 198 cm–1 represents a superposition of a B1u and a B3u peak. The measured peak at 123 cm–1, in turn, can be assigned to a B3u vibration.

Finally, we have determined the electron–phonon and spin–phonon coupling parameters by mapping the ab initio eigenvalues for phonon-distorted structures on a 6-band Hamiltonian. We have found that t, and consequently also J, are little affected by the non fully symmetric Γ point phonons. Regarding the hopping along the legs t||, and the corresponding exchange coupling J||, the V–O2 stretching modes show the largest changes, where the B1g593 cm–1 mode reveals the strongest electron- and spin–phonon coupling of all Γ point phonons. In summary, a quantitative description of the interactions that can strongly influence the electron subsystem has been achieved, yielding a profound understanding of this representative half-filled ladder compound.

Acknowledgments

The work was financed by the Austrian Science Fund (FWF), project P15520. We also appreciate support by FWF projects P15834 and P16227 and the EU RTN network EXCITING (contract HCPR-CT-2002-00317).

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Notes

Note1  Crystal structures are produced with XCrySDen [9].

  1. Lattice vibrations in CaV2O5 and their manifestations: a theoretical study based on density functional theory

    J Spitaler et al 2009 New J. Phys. 11 113009

  2. Tracking nanoparticles in an optical microscope using caustics

    Eann A Patterson and Maurice P Whelan 2008 Nanotechnology 19 105502

  3. Operator fidelity approach to the quantum phase transition of the spin-1/2 XX chain with three-spin interaction and the (1/2,1) XXZ mixed-spin chain

    Zhe Sun et al 2009 New J. Phys. 11 113005

  4. Large deviations of the free energy in diluted mean-field spin-glass

    Giorgio Parisi and Tommaso Rizzo 2010 J. Phys. A: Math. Theor. 43 045001

  5. Electron spin relaxation in p-type GaAs quantum wells

    Y Zhou et al 2009 New J. Phys. 11 113039

  6. Hořava–Lifshitz holography

    Tatsuma Nishioka 2009 Class. Quantum Grav. 26 242001

  7. Kondo-effect of substitutional cobalt impurities at copper surfaces

    P Wahl et al 2009 New J. Phys. 11 113015

  8. Low-temperature optical characterization of a near-infrared single-photon emitter in nanodiamonds

    P Siyushev et al 2009 New J. Phys. 11 113029

  9. X-ray polarimetry in astrophysics with the Gas Pixel Detector

    F Muleri et al 2009 JINST 4 P11002

  10. A bosonic Josephson junction

    R Gati and M K Oberthaler 2007 J. Phys. B: At. Mol. Opt. Phys. 40 R61



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