Research Article  Open Access
Recep Eryiğit, "First Principles Study of Cerium Monochalcogenides", Advances in Condensed Matter Physics, vol. 2014, Article ID 780245, 8 pages, 2014. https://doi.org/10.1155/2014/780245
First Principles Study of Cerium Monochalcogenides
Abstract
A theoretical investigation of structural, magnetic, electronic, and lattice dynamical properties of cerium monochalcogenides using the generalized gradient approximation (GGA) + U within ultrasoft pseudopotentials and a planewave basis is presented. All the calculated quantities, except the local magnetic moments, are found to be in good agreement with the experimental data. The lattice dynamical results indicate a strong chalcogenide dependence for the anomalous features of the phonon dispersions.
1. Introduction
The single 4f electron of cerium element gives rise to many anomalous and fascinating properties in cerium compounds, such as heavyfermion systems, intermediate valence compounds, Kondo metals, and Kondo insulators. Although the energy of this 4f electron is in the range of 5d and 6s valence electrons, its wave function is spatially localized tighter than semicore 5s and 5p electrons. The competition between cerium 4f electron being itinerant or localized determines the character of many cerium compounds. Cerium monochalcogenides (CeX, X = S, Se, Te) are some of the structurally simplest materials which show interesting electronic and magnetic properties due to the existence of a 4f electron of cerium. CeX compounds crystallize in NaCl structure at ambient conditions and exhibit a type II antiferromagnetic order below , 5.4, and 2.2 K for CeS, CeSe, and CeTe, respectively. The lowestlying multiplet of ion is split into a ground state doublet and an exited state quartet by the cubic crystalline electric field. The saturation magnetic moments are considerably reduced below a value of 0.71 which is expected from ground state [1]. All three compounds undergo structural phase transitions from NaCl to CsCl structure under pressure. Phonon dispersion of CeX also exhibits strong anomalies in the longitudinalacoustic branch, especially near the L point, where it crosses the transverse ones for CeSe [2].
Electronic and lattice dynamical properties of cerium monochalcogenides have been studied theoretically and experimentally by several groups over the years [1–10]. De and Chatterjee [3] used a selfconsistent linear augmented planewave method in the localdensity approximation to study the change in valency with pressure for CeS. Svane et al. [4] investigated the electronic structure of rareearth chalcogenides and pnictides with a selfinteractioncorrected localspindensity approximation within linear muffin tin orbital method along the lines of [3]. Price et al. carried out an LSDA and LDA + study of magnetooptic properties of CeSb and CeTe in full potential linear muffintin orbital scheme and found that the LDA + calculation fails to capture the essential elements of the electronic structure of CeTe, since it failed to obtain a correct magnetic moment [5]. Collins et al. [9] investigated the peculiar magnetic properties of cerium pnictides and chalcogenides by using a model Hamiltonian with LDA derived parameters and LSDA approaches and found that the model was able to reproduce the experimentally observed moment collapse while LSDA and LDA + were not able to predict even the ordering of the magnetic moments of CeS, CeSe, and CeTe. The lattice dynamics of CeSe were investigated by Steiner et al. by using the nonorthogonal tightbinding method of Varma and Weber to explain the longitudinal acoustic phonon softening [2]. Antonov et al. presented a review of experimental and theoretical works on optical and polar Kerr spectra of CeX compounds [10].
To the best of our knowledge, there is no extensive first principles study of electronic and lattice dynamical properties of cerium monochalcogenides. In the present work, we have carried out extensive first principles calculations on lattice, electronical, magnetic, and lattice dynamical properties of cerium monochalcogenides in the framework of density functional and density functional perturbation theory at spin polarized GGA and GGA + levels. The outline of the paper is as follows. The details of the computational method is given in Section 2. The calculated lattice constant, bulk modulus, magnetic moment, electronic band structure, Fermi surface, and phonon dispersion relations are discussed in Section 3. The paper concludes with a brief discussion of the main findings in Section 4.
2. Structure and the Computational Details
All the three chalcogenides, namely, CeS, CeSe, and CeTe, considered in the present work crystallize in the NaCl type structure (B1) with spacegroup symmetry Fm3 m under normal conditions. The cerium atom is positioned at (0, 0, 0) and the chalcogenide atom at (1/2, 1/2, 1/2) reduced coordinates. The antiferromagnetically ordered phase corresponds to a stacking of ferromagnetic (111) planes with the magnetic moments lying along the direction [6]. This AFM type II ordering leads to primitive unit cell with rhombohedral symmetry (space group R3 m, group number 166) [7]. The primitive rhombohedral unit cell contains two Ce located at (0,0,0) and (1/2, 1/2, 1/2) and two X atoms placed at (1/4, 1/4, 1/4) and (3/4, 3/4, 3/4) reduced coordinates.
All the quantities reported here were obtained with the Quantum Espresso suit [11] of programs which implement density functional and density functional perturbation theory. The generalized gradient approximation to the exchange correlation functional of Perdew et al. [12] is used. We used the pseudopotentials Cef1d1pberc1.0.uspp. UPF, S.pbevanak. UPF, Se.pbevan. UPF, and Te.pberrkj. UPF from http://www.quantumespresso.org/. A planewave cutoff of 60 Ry and a MonkhorstPack grid of 8 × 8 × 8 for the Brillouine zone integrations are found to converge all the reported quantities. For the linear response phonon calculations, we use a 8 × 8 × 8 grid to calculate the force constants which are Fourier transformed to obtain the interatomic force constant that are used to obtain the phonon dispersions along high symmetry directions of the first Brillouine zone.
3. Results
3.1. Lattice Structure and Magnetic Properties
First, we consider the equilibrium lattice structure and magnetic moment of CeX compounds and calculate the total static energy for nonmagnetic, ferro and antiferromagnetic configurations at 12 different volumes located symmetrically around the experimental volume of the compound. Although non and ferromagnetic phases can be described by a NaCl type primitive unit cell, we do all calculations in antiferromagnetic rhombohedral cell to avoid possible sampling errors in comparison of total energies. The computed volumeenergy pairs are fitted to a third order Vinet equation of state to determine equilibrium lattice constant, bulk modulus, and pressure derivative of the bulk modulus of each compound and the results are displayed in Table 1 along with calculated magnetic moments and available experimental data as well as some of the findings of previous calculations. The agreement between our calculated lattice constant and the experimental values and the previous calculations is satisfactory; of CeS and CeSe are underestimated ≈ for all magnetic configurations while of nonmagnetic CeTe are underestimated by . Lattice constants for ferro as well as antiferromagnetic structure for all three compounds are found to be slightly higher than those calculated for the nonmagnetic phase. The effect of spin polarization on the bulk modulus is found to be more pronounced; it leads to a softening of the material for all three compounds. While this softening makes the computed bulk modulus closer to the experimental for CeS, bulk modulus of spin polarized CeSe and CeTe is found to be ≈ lower than that of nonmagnetic phase which are already very close to the corresponding experimental values. Available experimental data for the pressure derivative of bulk modulus for CeS (2.2) and CeTe (13.6) are, unusually, low and high, respectively. Our calculated values for these two quantities are in the range 4.44–5.22 which is similar to other theoretical studies and more inline with general values.

All three cerium chalcogenides considered in the present study are known to have antiferromagnetic type II order below , 5.4, and 2.2 K with saturation sublattice moments of 0.31, 0.45, and 0.66 /Ce for CeS, CeSe, and CeTe, respectively [10]. Our calculated magnetic moments for all three compounds, especially for CeS and CeTe, are unsatisfactory. The anomalous magnetic moment reduction and failure of DFT to describe it well might be related to the role of Kondo screening which cannot be accounted for in DFT [13, 14] or the fband hybridization, fband Coulomb exchange, and crystal field interactions which can be better explained with Hamiltonian systems with ab initio determined parameters [9]. To further elucidate the magnetic structure, we include strong correlation effects by repeating the calculations mentioned above in the GGA + framework for eV and display the resulting relative energy and structural and magnetic parameters as function of in Figures 1 and 2, respectively. In Figure 1, we plot , where is the minimum of the total energy among all three considered magnetic structures and is calculated at the equilibrium lattice constant for the given value. From Figure 1, it is obvious that the antiferromagnetic structure has the lowest energy configuration for all considered nonzero corrections. At , the energy difference between the various phases is not resolvable from the plot; we have found that AFM < FM < NM order is also valid at with meV for all three compounds. One should note that this difference is on the order of the systematic errors of DFT.
(a)
(b)
(c)
(a)
(b)
(c)
The dependence of lattice parameters and magnetic moments is displayed in Figures 2(a)–2(c) for CeS, CeSe, and CeTe, respectively. The overall effect including Hubbard correction is found to be an underbinding which is reflected in increasing lattice constant and decreasing bulk modulus with increasing . The reason for the effect is related to the fact that the Hubbard term leads to more localization of the 4f electrons which no longer participate in bonding [15]. Since the lattice parameters are already well reproduced at , inclusion of the Hubbard term leads to a worsening of the agreement between the experimental and the calculated quantities as can be seen from Figure 2, especially for the bulk modulus (middle row of the figure). In an overall consideration, nonmagnetic configuration reproduces the experimental lattice constant and bulk modulus values better than ferro and antiferromagnetic structures.
In Figure 3(a), we display the calculated total electronic charge density of CeTe in the rhombohedral structure as an example of the rearrangement of the electrons in forming cerium monochalcogenides. Figure 3(a) is the threedimensional contour plot of electronic charge density at 0.005 electron/ level. One can discern almost spherical charge density around cerium atom in the center of the figure. Each cerium is bonded to six nearest neighbor tellurium atoms which also have somewhat smaller and near spherical charge density around them. The bonding charge density defined as the difference between the converged charge density of the crystalline structure and the sum of separate atomic charge densities can give an indication of the bonding due to the crystal potential. We display the calculated bonding charge density of CeTe in Figure 3(b) as a threedimensional contour plot at ±0.003 electrons/ levels. The red surface indicates a decrease in the density in forming the crystal and is found around Ce (eight nodal ellipsoids) and Te (almost spherical) atoms in the figure. The blue surface shows the positive bonding charge density which is formed by the charge depleted from the red area. It can be observed from Figure 3 that electrons from 4forbitals of Ce and p orbitals of Te undergo substantial geometrical change to form directional bonds between cerium and tellurium.
(a)
(b)
3.2. Electronic Band Structure
The first Brillouine zone of the rhombohedral structure used in the present calculations is shown in Figure 4. The electronic band structure of CeS, CeSe, and CeTe in the antiferromagnetic phase along the XLT directions of the first Brillouine zone of the rhombohedral lattice is shown along with the total and partial densities of electronic states in Figures 5(a)–5(c). The overall structure for all three compounds is very similar; bands formed by chalcogenide p hybridization with cerium 5d states are located in the approximate range [−6 −4] eV. The exact location of this group of bands moves closer to the Fermi level as one goes from CeS to CeTe by 0.5 eV while the dispersion of the bands in the group remains almost the same. The states around the Fermi level for all three compounds are found to be formed mostly from cerium 4f states with a small contribution from the cerium 5d orbitals as can be observed from the partial densities of states in Figures 5(a)–5(c). The very high density of states just above the Fermi level is due to dispersionless unoccupied flevels of cerium atom.
(a)
(b)
(c)
The band structure and density of electronic states calculations were repeated in an GGA + framework to consider the effect of possible strong correlation effects related with the 4f electrons of cerium. A eV on Ce4f orbitals is used. Its expected effect is to repel the occupied and unoccupied states down and up by . The results are shown in Figures 6(a)–6(c) for CeTe, CeSe, and CeS, respectively. Comparing GGA (Figure 5) and GGA + (Figure 6), the most important effect of + correction is the decrease of density of states at the Fermi level originating from the 4f orbitals. GGA and GGA + band structures of Figures 5 and 6 can be compared with the similar calculations reported for CeS by [10]; while the band structure and the total density of states are very similar for our work and that of [10], the inclusion of + = 6 eV correction was found to move the occupied 4f level 3 eV below the Fermi level by Antonov et al. which is not found in the present work. The discrepancy is probably due to the difference in the implementation of Hubbard correction.
(a)
(b)
(c)
3.3. Fermi Surface
Fermi surfaces of CeS, CeSe, and CeTe are calculated at GGA and GGA + ( = 6 eV) schemes and are displayed in Figures 7(a)–7(c), respectively. GGA + Fermi surface of all three compounds are almost indistinguishable and are formed from two bands. The larger surface is formed from the bands originating from Ce4f orbitals while the red thin cylindrical sector is due to the band formed from Ce5d electron states. The GGA Fermi surfaces (left column in Figure 7) of CeS and CeSe show some similarities.
(a)
(b)
(c)
3.4. Lattice Dynamics
The phonon dispersions of CeS, CeSe, and CeTe are obtained from linear response calculation and are displayed along with total and projected phonon density of states in Figures 8(a)–8(c), respectively. We also display the available experimental data for acoustical branch of the phonons of CeSe [2] in Figure 8(b). The overall agreement between the experimental data and our calculated dispersion is good. While the flatness of the mode dispersions towards the zone boundaries is reproduced well in the computations, the crossing of the longitudinal and transverse acoustic modes near the L point is not reproduced for CeSe. The acoustical branch of the dispersions for all three compounds shows a similar structure; the maximum vibration frequency of the longitudinal acoustic modes reaches ≈ for wave vectors close to the zone boundary. Also, the contribution of chalcogenide atom to the displacement pattern of the acoustical modes decreases with increasing acoustical mode frequency while that of cerium contribution increases. The flatness of the dispersion around X point of the first Brillouine zone is mostly due to the motion of the chalcogenide atom and this flatness is inversely proportional to the mass of the chalcogenide.
(a)
(b)
(c)
On the other hand, the dispersion of the optical branch of the mode displays a richer structure compared to the acoustical ones. The displacement pattern of these modes mostly involves the motion of the chalcogenide atoms. The maximum frequency of the optical branch is around 300, 200, and 150 cm^{−1} for CeS, CeSe, and CeTe, respectively, and is inversely proportional to the square root of the mass of the chalcogenide atom. The optical modes of CeS are found to be almost dispersionless (Figure 8(a)). The width of optical mode dispersion is found to increase with the chalcogenide mass.
4. Conclusion
We have carried out an extensive first principles investigation of lattice, magnetic, electronic, and lattice dynamical properties of cerium monochalcogenides CeS, CeSe, and CeTe by employing density functional and density functional perturbation theory with GGA and Hubbard corrected GGA + exchange correlation functional.
The lattice constant and bulk modulus of all three compounds are found to be well described by GGA functional; adding + correction leads to an underbinding of the crystal which leads to an increase (decrease) in lattice constant (bulk modulus). The magnetic moment is found to be underestimated at the GGA level; GGA predicts ground state of CeS to be nonmagnetic. Inclusion of the correlation effect overestimates the magnetic moments. Both GGA and GGA + are unable to predict the experimentally observed magnetic moments of cerium monochalcogenides investigated in the present study.
We have found that the electronic bands close to the Fermi level have two distinct groups, at the Fermi level, bands are mostly cerium 4f character with a small Ce 5d contribution while bands centered 5 eV below the Fermi level are formed from a hybridization of cerium 5d and chalcogenide p levels. The density of electronic states at the Fermi level is found to be high at GGA level and decreases with the inclusion of strong correlation effects.
The lattice dynamical study indicates that the anomalous acoustical mode dispersion and the width of the dispersion of the optical mode branches strongly depends on the mass of the chalcogenide atom.
Conflict of Interests
The author declares that there is no conflict of interests regarding the publication of this paper.
References
 K. Hiraoka, R. Pittini, and P. Wachter, “Hall effect in Cemonochalcogenides CeX (X = S, Se, Te),” Physica B: Condensed Matter, vol. 230–232, pp. 136–138, 1997. View at: Publisher Site  Google Scholar
 M. M. Steiner, H. Eschrig, and R. Monnier, “Longitudinalacousticphonon softening in YS, LaS, and CeSe,” Physical Review B, vol. 45, no. 13, pp. 7183–7187, 1992. View at: Publisher Site  Google Scholar
 S. K. De and S. Chatterjee, “Electronic and optical properties of CeS under pressure,” Physical Review B, vol. 40, no. 18, pp. 12304–12311, 1989. View at: Publisher Site  Google Scholar
 A. Svane, P. Strange, W. M. Temmerman, Z. Szotek, H. Winter, and L. Petit, “Pressureinduced valence transitions in rare earth chalcogenides and pnictides,” Physica Status Solidi (b), vol. 223, no. 1, pp. 105–116, 2001. View at: Publisher Site  Google Scholar
 D. L. Price, B. R. Cooper, S.P. Lim, and I. Avgin, “Variation of the LDA+U method appropriate to fstate localization: application to magnetooptical properties,” Physical Review B, vol. 61, no. 15, p. 9867, 2000. View at: Publisher Site  Google Scholar
 D. Ravot, P. Burlet, J. RossatMognod, and J. L. Tholence, “Magnetic properties of cerium monotelluride,” Journal de Physique France, vol. 41, no. 10, pp. 1117–1120, 1980. View at: Publisher Site  Google Scholar
 P. SchobingerPapamantellos, P. Fisher, A. Niggli, E. Kaldis, and V. Hildebrandt, “Magnetic ordering of rare earth monochalcogenides. I. Neutron diffraction investigation of CeS, NdS, NdSe, NdTe and TbSe,” Journal of Physics C, vol. 7, p. 2023, 1973. View at: Publisher Site  Google Scholar
 R. Pittini, J. Schoenes, and P. Wachter, “MO Kerr study of the 4f^{1} state,” Physica B: Condensed Matter, vol. 230–232, pp. 538–543, 1997. View at: Publisher Site  Google Scholar
 E. M. Collins, N. Kioussis, S. P. Lim, and B. R. Cooper, “Development of magnetism in strongly correlated cerium systems: nonKondo mechanism for moment collapse,” Physical Review B, vol. 62, Article ID 11533, 2000. View at: Publisher Site  Google Scholar
 V. N. Antonov, L. V. Bekenov, and A. N. Yaresko, “Electronic structure of strongly correlated systems,” Advances in Condensed Matter Physics, vol. 2011, Article ID 298928, 107 pages, 2011. View at: Publisher Site  Google Scholar
 http://www.quantumespresso.org/.
 J. P. Perdew, K. Burke, and M. Ernzerhof, “Generalized gradient approximation made simple,” Physical Review Letters, vol. 77, no. 18, pp. 3865–3868, 1996. View at: Google Scholar
 A. Svane, W. Temmerman, and Z. Szotek, “Theory of pressureinduced phase transitions in cerium chalcogenides,” Physical Review B, vol. 59, no. 12, pp. 7888–7892, 1999. View at: Publisher Site  Google Scholar
 B. Coqblin, “Kondo lattice and magnetic properties in strongly correlated electron systems,” Acta Physica Polonica A, vol. 115, no. 1, pp. 13–18, 2009. View at: Google Scholar
 B. Amadon, F. Jollet, and M. Torrent, “γ and β cerium: LDA+U calculations of groundstate parameters,” Physical Review B, vol. 77, no. 15, Article ID 155104, 2008. View at: Publisher Site  Google Scholar
 Local magnetic moments calculated using the spin polarized GGA minimum structure with GGA + U for U = 6 eV.
 A. Bouhemadou, R. Khenata, M. Sahnoun, H. Baltache, and M. Kharoubi, “Firstprinciples study of structural, elastic and highpressure properties of cerium chalcogenides,” Physica B, vol. 363, no. 1–4, pp. 255–261, 2005. View at: Publisher Site  Google Scholar
 J. M. Leger, “Chalcogenides and pnictides of cerium and uranium under high pressure,” Physica B: Condensed Matter, vol. 190, no. 1, pp. 84–91, 1993. View at: Publisher Site  Google Scholar
 S. P. Lim, D. L. Price, and B. R. Cooper, “Giant magnetooptic rotations: the role of orbital polarization and explicit correlation effects,” IEEE Transactions on Magnetics, vol. 27, no. 4, pp. 3648–3654, 1991. View at: Publisher Site  Google Scholar
 J. M. Léger, R. Epain, J. Loriers, D. Ravot, and J. RossatMignod, “Anomalous behavior of CeTe under high pressures,” Physical Review B, vol. 28, no. 12, pp. 7125–7129, 1983. View at: Publisher Site  Google Scholar
Copyright
Copyright © 2014 Recep Eryiğit. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.