Oxygen-octahedral distortion and electronic correlation induced semiconductor gaps in ferrimagnetic double perovskite Ca2MReO6 (M = Cr, Fe)

Sai Gong, San-Dong Guo, Peng Chen and Bang-Gui Liu*
Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China. E-mail: bgliu@iphy.ac.cn

Received 26th May 2015 , Accepted 17th July 2015

First published on 17th July 2015


Abstract

Motivated by experimental nonmetallic features and high magnetic Curie temperatures of 360 and 522 K in double perovskite Ca2CrReO6 and Ca2FeReO6, we systematically investigate the structural, electronic, and magnetic properties of Ca2MReO6 (M = Cr, Fe) by combining the modified Becke–Johnson (mBJ) exchange potential with usual generalized gradient approximation (GGA). Our full optimization leads to stable ground-state structures with monoclinic symmetry (P21/n) consistent with experiment. The mBJ calculation successfully produces ferrimagnetic phase with semiconductor gaps of 0.38 eV and 0.05 eV, respectively, in contrast with wrong metallic phases from GGA calculations. With the spin–orbit coupling (SOC) taken into account, the Ca2MReO6 (M = Cr, Fe) shows high magneto-crystalline anisotropy (MCA) with the magnetic easy axis along the [010] direction. Although reducing to 0.31 and 0.03 eV, the semiconductor gaps remain open in spite of the SOC broadening of the Re t2g bands. Therefore, our DFT investigation has established the correct ferrimagnetic semiconductor ground states for the double perovskite Ca2MReO6 (M = Cr, Fe) materials. Our analysis shows that the semiconductor gaps are due to orbital-selective splitting on Re t2g bands in the minority-spin channel, originated from the O-octahedral distortion and Coulomb correlation effect. This mechanism, different from that in other double perovskite materials such as Sr2CrOsO6, Ca2CrOsO6 and Sr2FeOsO6, can be useful to fully understand chemical and physical properties of double perovskite compounds.


I. Introduction

Because of their rich physics and high technological potential,1 ordered double perovskite A2BB′O6 (A = alkali, alkaline-earth or rare-earth ion; B and B′ = transition metals) have been extensively.2–18 For cubic or tetragonal double perovskite Sr2BB′O6 (B = Cr or Fe, and B = Mo, W, or Re), ferrimagnetic metallic phase is usually formed because the fully occupied high spin state Fe3+ (3d5) or Cr3+ (3d3) is antiferromagnetically coupled with the partially filled 4d and 5d transition-metal cations.18,19 Among them, half-metallic Sr2FeMoO6, Sr2FeReO6, and Sr2CrReO6 have been known as prospective spintronic materials beyond room temperature.3,5,10,18,20 On the other hand, double perovskite Sr2CrOsO6 is a robust ferrimagnetic insulator with the highest magnetic Curie of 725 K, and its semiconductor gap has been shown to originate from spin-exchange splitting of the Os 5d t2g bands.18,21,22 With the same origin of band gap, the recently crystallized Ca2FeOsO6 presents an insulating ferrimagnetic phase below 320 K.23,24 Another compound Sr2FeOsO6 is also revealed to be an insulator in spite of antiferromagnetic arrangement.25,26 Very special are double perovskite Ca2FeReO6 and Ca2CrReO6. It is shown experimentally that they are ferrimagnetic insulators with monoclinic structure and have high magnetic Curie temperatures of 522 and 360 K,9,14,18,20,27,39 but their non-metallic electronic properties have not yet been elucidated although some efforts were made for the Ca2FeReO6 material.40,41 In addition, their structure–property relationship needs to be understood.

Here, we investigate the structural, electronic and magnetic properties of the Ca2CrReO6 and Ca2FeReO6 through density functional theory calculations in order to reveal the origin of their special electronic structures, especially their semiconductor gaps at low temperature. We use Tran and Blahas modified Becke and Johnson (mBJ) approach for the exchange potential28 to investigate their electronic structures because its excellent accuracy has been proved for most of insulators, semiconductors, and transition-metal oxides.28–31 Our calculations reveal that the Ca2CrReO6 and Ca2FeReO6 are both ferrimagnetic semiconductors, even with the spin–orbit effect taken into account. Our further analysis shows that the semiconductor gaps are formed between the full-filled dxz and the empty dyz states around the Fermi level due to the mutual cooperation of O-octahedral distortion and Coulomb correlation. We also explore other properties of the two Ca-based double perovskite compounds in comparison with similar materials. More detailed results will be presented in the following.

The rest of the paper is organized as follows. We shall describe our computational details in the next section. In Sec. III we shall present our optimized ground-state structures for the two compounds. In Sec. IV we shall present our spin-dependent density of states, band structures, and electron density distributions and perform further analyses concerned. In Sec. V we shall present our calculated results with the spin–orbit effect taken into account, including their magneto-crystalline anisotropic energies, spin and orbital moments along the easy axis, and the spin–orbit-effect-modified semiconductor gaps. Finally, we shall give our conclusion in Sec. VI.

II. Computational details

We use the full-potential linear augmented plane wave (FP-LAPW) method within the density functional theory (DFT),32,33 as implemented in the WIEN2k package.34 We take GGA exchange–correlation functional to do structure optimization and preliminary study,35 and then use mBJ exchange potential to do electronic structure calculations. The scalar relativistic approximation is used for valence states, with the spin–orbit coupling (SOC) is taken into account, whereas the radial Dirac equation is self-consistently solved for the core electrons.36–38 The magnetization is chosen to be along all nonequivalent directions for the monoclinic structure when we investigate the magneto-crystalline anisotropy. The muffin-tin radii of the Ca, Cr, Fe, Re, and O atoms are set to be 2.20, 1.96, 2.03, 1.96, and 1.71 bohr, respectively. We make harmonic expansion up to lmax = 10 in the muffin-tin spheres, and set Rmt × Kmax = 8.0. We use 1000 k-points in whole Brillouin zone (234 k-points in the reduced wedge). For testing the accuracy, we also use 2000 k-points in whole Brillouin zone (576 k-points in the reduced wedge) to do the self-consistent calculations. The total energy difference is proved to be less than 1 meV. Therefore, our choice of 1000 k-points is enough for the whole calculation. The self-consistent calculations are considered to be converged only when the integration of absolute charge-density difference per formula unit between the successive loops is less than 0.0001|e|, where e is the electron charge.

III. Structure optimization

The structure of Ca2MReO6 (M = Cr or Fe) has been reported to be monoclinic structure with P21/n symmetry (space group #14) at room temperature,9,18 which is consistent with the prediction of the empirical tolerance factor f.18,39 The monoclinic structure is fairly distorted from cubic double perovskite due to the small size of Ca2+ cation, which forces the MO6 and ReO6 octahedra to tilt and rotate in order to optimize the Ca–O bond lengths. As a representative, we demonstrate the crystal structure of Ca2CrReO6 in Fig. 1. Both P21/n and I4/m structures are presented for the following discussion. In order to investigate the origin of the nonmetallicity in their ground-state phases, we optimize fully their geometric structures and internal atomic positions by combining total energy and force optimizations. We have considered a larger unit cell of 2 f.u. including 20 atoms to relax the structure. The optimized lattice parameters are listed in Table 1, with experimental data included for comparison. Our total energy calculations show that the ground state phase is the P21/n structure for both of the compounds, with lattice constants expanded slightly with respect to experimental ones. This deviation is due to the special property of the GGA functional. However, the tilt angles β of Ca2MReO6 (M = Cr and Fe) decrease by 0.22° and 0.27° with respect to experimental values, respectively, which reflects the large distortion at low temperature.
image file: c5ra09921h-f1.tif
Fig. 1 (a) Crystal structure of double perovskite Ca2CrReO6 with 2 unit cells in P21/n (#14) symmetry, (b) the I4/m (#87) structure is displayed for comparison, (c) and (d) the projected images in the (110) plane for corresponding structures. CrO6 and ReO6 octahedra are denoted with purple and yellow, respectively. The green and black ones are Ca atoms in two different layers.
Table 1 Optimized lattice constants and tilt angle β of Ca2MReO6 (M = Cr, Fe) with space group P21/n (#14), compared with experimental results9
Lattice parameters Ca2CrReO6 Ca2FeReO6
opt. exp. opt. exp.
a (Å) 5.392 5.388 5.417 5.401
b (Å) 5.524 5.460 5.609 5.525
c (Å) 7.680 7.660 7.733 7.684
β (°) 89.74 89.96 89.80 90.07


We present in Table 2 optimized bond lengths and bond angles of Ca2MReO6 (M = Cr, Fe) with P21/n structure. For comparison, we also present the I4/m structure for Ca2CrReO6. It's shown that the three Cr–O bond lengths are slightly larger than Re–O ones in Ca2CrReO6, while the FeO6 octahedra are significantly more expanded than ReO6 octahedra in Ca2FeReO6. This observation is consistent with the ionic size sequence of Re5+ < Cr3+ < Fe3+. The bond angles in ReO6 octahedra all deviate from ideal values of 90°, so do the angles of M–O–Re from 180°. Considering that a large number of double perovskite compounds with half-metallicity are in tetragonal structure with I4/m symmetry (space group #87), and in order to clarify the relationship between the electronic property and lattice structure, we also present the structure parameters of the I4/m structure for Ca2CrReO6 in Table 2. There are actually two nonequivalent kinds of O atoms in I4/m structure. The O1 and O2 atoms are equal to each other and in the same xy-plane. The atom O3 sits along the z-axis with Cr or Re atoms in between. The bond lengths of Cr–O are larger than those of Re–O due to the larger ionic size of Cr3+ versus Re5+. All angles in ReO6 octahedra remain to be 90°, while the Cr–O1,2–Re bond angles reduce significantly from 180°, which makes the Cr–O1,2 and Re–O1,2 lengths much larger than the Cr–O3 and Re–O3 bonds, respectively. Our calculated total energy of Ca2CrReO6 in I4/m structure are higher than that in P21/n structure by 392 meV per formula unit, indicating the P21/n structure is more stable for Ca2CrReO6.

Table 2 Optimized bond lengths and angles of Ca2MReO6 (M = Cr, Fe) with space group P21/n (#14), with those of Ca2CrReO6 with I4/m (#87) structure for comparison. O1 and O2 are equivalent to each other in I4/m structure
  M Cr (#14) Cr (#87) Fe (#14)
Bond length M–O1 1.975 1.984 2.061
M–O2 1.978 1.984 2.046
M–O3 1.971 1.939 2.036
Re–O1 1.974 1.977 1.944
Re–O2 1.968 1.977 1.948
Re–O3 1.964 1.922 1.941
Bond angle O1–Re–O2 90.88 90 90.30
O2–Re–O3 89.43 90 89.28
O1–Re–O3 89.81 90 89.22
M–O1–Re 152.56 154.63 149.34
M–O2–Re 152.85 154.63 150.59
M–O3–Re 153.46 180 150.06


IV. Electronic structures

A. Density of states and energy bands

From now on, we investigate the electronic structures of the optimized Ca2MReO6 (M = Cr, Fe). At first, we use the popular GGA functional to calculate the density of states (DOS). The spin-resolved DOSs are presented in Fig. 2. For the Ca2CrReO6, the electronic energy bands between −8.0 eV and −3.0 eV are dominated by O 2p states. The Fermi energy falls in an energy gap of about 1.0 eV in the majority spin channel, between the fully filled Cr t2g and empty Re t2g bands. As for the Ca2FeReO6, the triplet Fe t2g states in the majority spin channel move to the lower energy between −8.2 eV and −2.2 eV, with a strong mixture of O 2p states. The Fermi energy is in the majority-spin gap of 1.4 eV between Fe eg and Re t2g bands. In contrast, for the minority spin channel, the Fermi level lies in the partially filled t2g bands of hybridized M, Re, and O 2p states in the Ca2MReO6 (M = Cr, Fe). Thus, the GGA calculation produces a half-metallic ferrimagnet. This is contradictory with the reported experimental results9,18 and can be attributed to the false GGA description of Re t2g nature around the Fermi level in the monoclinic structure. For the sake of accurate calculation for Re t2g state, we need to use improved exchange potential to investigate electronic structures of the Ca2MReO6. The modified Becke–Johnson (mBJ) potential is a good choice because it is excellent in describing the hybrid transition-metal ions.29,42
image file: c5ra09921h-f2.tif
Fig. 2 The spin-resolved total (tot) and partial (Cr/Fe, Re, O) density of states (DOSs) of Ca2CrReO6 (a) and Ca2FeReO6 (b) in P21/n structure from GGA calculation.

We present the spin-resolved DOSs and energy bands of the Ca2CrReO6 calculated with mBJ in Fig. 3. It is clear that there is a semiconductor gap open at the Fermi level, which is in good agreement with experimental results.9 Moreover, the occupied Cr t2g and unoccupied Cr eg and Re t2g bands in the majority spin channel are pushed substantially downwards and upwards, respectively, which consequently enhances the majority-spin gap (Gmaj) to 2.5 eV. In the minority spin channel, the triplet Re t2g states around the Fermi level split into a doublet dxy + dxz and a singlet dyz, with two electrons fully occupying the doublet state. This produces a semiconductor gap of 0.38 eV, as shown in Fig. 3(a). The detailed orbital-resolved DOSs around the Fermi level are presented in Fig. 3(b). Both of the unoccupied Cr t2g and eg in the minority spin channel are pushed upwards substantially, with a little overlap between them, which enlarges the spin exchange splitting energy of Cr t2g to 4.7 eV. Fig. 3(c) and (d) show the energy bands of the Ca2CrReO6 in majority-spin and minority-spin channels, respectively. The thicker a line is, the more the Re t2g weight is. There are 72 bands (36 majority spin and 36 minority spin) in the energy window from −7.8 eV to −2.6 eV, because we consider 2 unit cell in our calculation. The energy bands between −2.0 eV and −1.0 eV consist of 6 Cr t2g bands in the majority spin channel. There are 4 occupied bands of Re t2g, including dxy and dxz just below the Fermi level and 2 bands of dyz above the Fermi level. It can be clearly seen that the top of the valence band and the bottom of the conduction band are located in M and Γ points, respectively, resulting in an indirect band gap for the Ca2CrReO6.


image file: c5ra09921h-f3.tif
Fig. 3 Electronic structure of Ca2CrReO6 in P21/n structure calculated with mBJ: spin-resolved total (tot) and partial (Cr, Re, O) DOSs (a); amplified d states split DOSs of Cr and Re around the Fermi level (b); and majority-spin (c) and minority-spin (d) bands.

In Fig. 4 we present the spin-resolved DOSs and energy bands of the optimized Ca2FeReO6 calculated with mBJ. The distinguished feature of the DOSs is that compared to GGA results, the Fe t2g states move to lower energy in the majority spin channel, and the gaps between Fe t2g and eg states almost vanish in both of spin channels. This can be attributed to the enhanced spin exchange effect due to mBJ functional. The semiconductor gap of 0.05 eV is also observed, owing to the same reason as in the Ca2CrReO6. However, the Re t2g splitting in the minority spin channel is much smaller than that in the majority spin channel, in contrast to the Ca2CrReO6. This result is consistent with the fact that the resistivity of the Ca2FeReO6 at low temperature is almost two order of magnitude lower than that of Ca2CrReO6, because the electron inter-band transition takes place easily in the Ca2FeReO6 compound. In the band structures (c) and (d) of the Ca2FeReO6, the Fe t2g bands are pushed down to between −8.0 eV and −3.0 eV in the majority spin channel, in contrast to the minority-spin one. The energy window from −3.0 eV to −2.0 eV consists of 4 bands of Fe eg. The top of valence bands and the bottom of the conduction bands are located in N and Γ points, respectively. This implies that the semiconductor gap of the Ca2FeReO6 is indirect, same as that of the Ca2CrReO6.


image file: c5ra09921h-f4.tif
Fig. 4 Electronic structure of Ca2FeReO6 in P21/n structure calculated with mBJ: spin-resolved total (tot) and partial (Fe, Re, O) DOSs (a); amplified d states split DOSs of Fe and Re around the Fermi level (b); and majority-spin (c) and minority-spin (d) bands.

B. Electron density distributions

The energy-resolved charge and spin density distributions are very important to explore the bonding and magnetic properties. We present in Fig. 5 the valence charge (including up and down) and spin density distributions of the Ca2CrReO6, with all the contribution from −8.0 eV to the Fermi level, calculated with mBJ. The upper three panels are for the (001) plane of the structure shown in Fig. 1, the lower three ones are for the perpendicular plane, being equivalent to the (110) plane, including Cr and Re ions. In the spin-up channel, the charge density distributions at Cr sites look like a quatrefoil, which reflects the fully occupied t2g characteristic between −2 eV to −1 eV, whereas the charge density around Re is fairly small. In the spin-down channel, there is much electron density around Re, in consistence with the partially filled Re t2g state from −1 eV to the Fermi level. The small charge density at Cr sits should result from the hybridization between Re and Cr t2g states. In both of the spin channels, the oxygen atoms with high electron affinities attract the electrons from Cr and Re atoms to form nearly closed O 2p shells with spherically distributed charge densities. It can be seen in the charge density contours that the bonds between Cr and nearest O are almost ionic with respect to the Re–O bonds with covalent characteristic, which is in accordance with the longer bond lengths of Cr–O than Re–O ones, as described in Table 2. The charge distributions also show that there exists no direct interaction between two nearest Cr–Cr or Re–Re pairs. The spin density distribution of the Ca2CrReO6 in Fig. 5(e) and (f) demonstrates that the spin moments of Cr and Re are mainly localized at the ionic sites. The contours, with an increment of 0.013 μB per a.u3, mean that the spin density around Cr varies from −0.5 μB per a.u3 to 0 and that around Re from 0 to 0.5 μB per a.u3. This spin density distribution indicates the antiferromagnetic coupling between the Cr and Re moments in the double perovskite Ca2CrReO6. The some deformed quatrefoils of Cr and Re ions are ascribed to the distortion of O octahedra. It is worth note that different density contours between Re and Cr sites are due to the more closed shells in the inner part of heavier Re ion compared to Cr.
image file: c5ra09921h-f5.tif
Fig. 5 Valence electron charge [up, (a) and (b); dn, (c) and (d)] and spin [(e) and (f)] density distributions, within the energy window from −8.0 eV to the Fermi level, of Ca2CrReO6 projected to the (001) and (110) planes calculated with mBJ. The contours in (a)–(d) are from 0.005 to 0.5e/a.u3 with an increment of 0.025e/a.u3, and those in (e) and (f) from −0.5 to 0 μB per a.u3 for Re sites and 0 to 0.5 μB per a.u3 for Cr sites with an increment of 0.013 μB per a.u3.

As for the Ca2FeReO6, we illustrate the corresponding charge and spin density distributions calculated with mBJ in Fig. 6. It can be seen that charge distributions at the Fe site are nearly spherical because of nearly half-filled Fe 3d orbitals, which is different from the quatrefoils shape of partially occupied Cr 3d orbitals in the Ca2CrReO6. The Fe 3d electrons that are more than half full move to oxygen sites for stabilizing the ground state, leaving the highly ionized Fe atoms, as shown in Fig. 6. The shape of charge density around the Re site is similar to that in the Ca2CrReO6 due to the same valence states of Re5+ ions in the two compounds. Most of the Re 5d electrons with larger orbitals spread out to O 2p states, forming the Re–O covalent bonds. Furthermore, the hybridizations are still along the Fe–O–Re–O–Fe chain, and no direct interaction between Fe–Fe and Re–Re pairs are found. The spin moments of Fe 3d and Re 5d states are mainly localized and coupled antiferromagnetically, as are those of the Cr and Re states in the Ca2CrReO6.


image file: c5ra09921h-f6.tif
Fig. 6 Valence electron charge [up, (a) and (b); dn, (c) and (d)] and spin [(e) and (f)] density distributions, within the energy window from −8.2 eV to the Fermi level, of Ca2FeReO6 projected to the (001) and (110) planes calculated with mBJ. The contours in (a)–(d) are from 0.005 to 0.5e/a.u3 with an increment of 0.025e/a.u3, and those in (e) and (f) from −0.5 to 0 μB per a.u3 for Re sites and 0 to 0.5 μB per a.u3 for Fe sites with an increment of 0.013 μB per a.u3.

C. Further analyses

The spin exchange splitting (Δex) and crystal field splitting (Δcf) of Cr and Fe, the spin exchange splitting Δex of Re ion, and the band gaps across the Fermi level in both majority-spin (Gmaj) and minority-spin (Gmin) channels calculated with GGA and mBJ are summarized in Table 3. Here, the spin exchange splitting energy of Cr (Fe) is defined as the energy difference between the DOS weight centre of the filled Cr-t2g (Fe-3d) spin-up states and that of the empty Cr-t2g (Fe-3d) spin-down ones, and for Re it is similarly defined as the energy difference between the partially filled spin-down 5d states and those empty spin-up ones. Both Δex and Δcf of transition-metals are significantly enhanced by mBJ calculation. As a result, the gaps in the majority spin channel are enlarged by 1.5 eV and 1.9 eV for the Ca2MReO6 (M = Cr, Fe), respectively. The semiconductor gaps are equivalent to 0.38 eV and 0.05 eV, respectively, in contrast to the wrong results from GGA. This implies that electron correlations play an essential role in forming semiconductivity on Ca2MReO6 (M = Cr, Fe) compounds due to the mBJ approach mimics the behavior of orbital-dependent potentials and the correlation effects are treated not only for localized, but also for delocalized electrons. The role of correlations can also be verified by the fact that the Ca2CrWO6 shows insulator behavior,43 while Ca2FeMoO6 exhibits metallic conduction,44 which is attributed to the stronger correlation strength in 5d atoms of W and Re than 4d one of Mo.
Table 3 Spin exchange splitting (Δex) and crystal field splitting (Δcf) of Cr and Fe, spin exchange splitting Δex of Re ion, the band gaps across the Fermi level in the majority-spin channel (Gmaj) and the minority-spin channel (Gmin) of Ca2MReO6 (M = Cr, Fe) calculated with GGA and mBJ
M Scheme Δex (M) Δcf (M) Δex (Re) Gmaj Gmin
Cr GGA (eV) 2.9 3.0 0.8 1.0 0
mBJ (eV) 4.6 6.7 2.0 2.5 0.38
Fe GGA (eV) 3.0 1.0 0.7 1.4 0
mBJ (eV) 6.5 3.0 1.8 3.3 0.05


Besides electron correlations, we also investigate the effect of lattice structure on opening band gaps of Ca2MReO6 (M = Cr, Fe). The DOSs of the Ca2CrReO6 in I4/m structure with both GGA and mBJ functionals are presented in Fig. 7. It's shown that the GGA produces a half-metallicity, which is similar to the GGA result of the Ca2CrReO6 with P21/n symmetry, and however, the metallic property is not changed by using mBJ potential, although the Δex and Δcf of Cr and Re are much enlarged. This comparison indicates that the semiconductor nature of the Ca2MReO6 has intimate relationship with the crystal structure. For discussing the importance of structure in detail, we present in Fig. 8 the band structures near the Fermi level in the minority-spin channel, showing the Re 5d states for the Ca2CrReO6. The corresponding states of the Ca2FeReO6 are similar to those of the Ca2CrReO6. In the I4/m structure, the bond angles of CrO6 and ReO6 octahedra are ideal 90°, as shown in Fig. 1(b), allowing the symmetry operation of rotation 45° and translation along z axis. Therefore, the Re 5d states are preserved in high degeneration. The dxy bands are full-occupied with two electrons and lie below the Fermi level. The remainder two ones half-fill the doublet dxz + dyz states, resulting in the metallicity of the Ca2CrReO6. As for the P21/n structure, the CrO6 and ReO6 octahedra undergo tilting and rotation, making the bond angles deviate from 90°. Meanwhile, the Ca atoms in different layers move oppositely, and then the symmetry along z axis is broken. The symmetry reduction urges the half-filled states to split into full-filled dxz and empty dyz ones, leading to a Peierls-like gap. This fact is consistent with the quatrefoil pattern of the spin density distribution at Re sites, as shown in Fig. 5(e) and (f) and 6(e) and (f). In general, not only the correlation effect, but also octahedral distortion are necessary for the semiconductor nature of the Ca2MReO6 (M = Cr, Fe) compounds.


image file: c5ra09921h-f7.tif
Fig. 7 The spin-resolved total and partial DOSs of Ca2CrReO6 In I4/m structure with GGA (a) and mBJ (b) methods.

image file: c5ra09921h-f8.tif
Fig. 8 The band structures near the Fermi level in the minority-spin channel of Ca2CrReO6 with I4/m (a) and P21/n (b) structures, respectively. The thick dot lines denote the dxz + dyz of Re t2g states for I4/m and the dyz state for P21/n structure. The k-paths of both structures are displayed in (c).

V. Spin–orbit coupling effect

To investigate the effect of spin–orbit coupling on the optimized Ca2MReO6 (M = Cr, Fe), the magnetization is chosen to be approximately along [100], [010], [001], [110], [101], [011] and [111] directions for the P21/n monoclinic structure. The calculated total energies with GGA + SOC method presented in Table 4 indicate high magneto-crystalline anisotropy (MAC) in the Ca2MReO6 compounds. The most stable magnetic orientation are both along [010] direction, equivalent to the b-axis perpendicular to the ac plane in the P21/n structure. These are consistent with experimental results.18
Table 4 Total energies (meV) of Ca2MReO6 (M = Cr, Fe) with different magnetization orientations calculated with GGA + SOC, with the lowest energy set as reference
M [100] [010] [001] [110] [101] [011] [111]
Cr 1.00 0 2.16 1.21 2.08 1.34 1.29
Fe 1.37 0 2.04 2.03 2.62 1.60 1.61


After the magnetic easy axis is fixed, we do further study with SOC along the [010] direction. Our calculated spin and orbital moments for the Ca2MReO6 are summarized in Table 5. When SOC is neglected, the total spin moment is precisely 1 μB and 3 μB per formula unit for the Ca2CrReO6 and Ca2FeReO6, respectively. The results can be elucidated in the ionic model, where the transition-metal ions are in the (MRe)8+ valence state. The M3+ are in the high spin state of S = 3/2 for Cr3+ and S = 5/2 for Fe3+ according to Hund's rule, antiferromagnetically coupled with highly ionized Re5+ with valence spin states of S = 1, resulting the integer moment in Bohr magneton. Note that a large part of the spin moment is delocalized into the interstitial region, and therefore the spin moments of the individual M and Re ions appear small compared to the ionic values.

Table 5 The mBJ results of individual and total spin moments (μs), orbital moments (μo), and net moments (μtot) in μB, and semiconductor gap (Gs, in eV) of Ca2MReO6 (M = Cr, Fe) with P21/n structure with and without SOC
M Scheme μsM μsRe μstot μoM μoRe μtot Gs
Cr mBJ 2.520 −1.264 1.000     1.000 0.38
mBJ + SOC 2.520 −1.239 1.035 −0.018 0.192 1.209 0.31
Fe mBJ 4.090 −1.118 3.000     3.000 0.05
mBJ + SOC 4.090 −1.096 3.033 0.042 0.183 3.258 0.03


When SOC is taken into account, the total spin moments increase by 0.035 μB and 0.033 μB for the Ca2MReO6 (M = Cr, Fe), respectively, due to some increase of Re spin moment. The orbital moments of Cr and Re are both antiparallel to the spin moments, because of the less than half-filled d shell, in accordance with Hund's rule. As for the Ca2FeReO6, the orbital moments of Fe 3d is of the same sign as the spin moment, indicating that the 3d orbital is more than half-filled, consistent with Hund's rule. Our calculated Cr orbital moment of −0.018 μB is much smaller than the Fe one of 0.042 μB, which could be understood as a consequence of stronger ligand field caused by the Cr 3d orbital than by the Fe 3d orbital. For Re ion, the orbital moment is 0.192 μB or 0.183 μB for the Ca2CrReO6 or Ca2FeReO6, due to the strong spin–orbit coupling in 5d orbital. The higher improvement of total magnetic moment, 0.258 μB, in the Ca2FeReO6 than 0.209 μB in the Ca2CrReO6 is due to the positive large orbital moment in Fe ion.

We also present the semiconductor gaps Gs as the true gaps of these compounds in Table 5. When SOC is included, the band gaps remain but become smaller, and is equivalent to 0.31 eV for the Ca2CrReO6 and 0.03 eV for the Ca2FeReO6, respectively. In order to understand in more detail the reason of the smaller gap with SOC, the partial DOS of M and Re projected onto d orbital in the Ca2MReO6 calculated with SOC are plotted in Fig. 9. In the presence of SOC, the bands in both of the spin channels hybridize with each other, in contrast to the pictures in Fig. 3 and 4. The Re t2g states around the Fermi level in one spin channel induce some states in the opposite spin channel, especially in the Ca2FeReO6 compound. Moreover, the Re t2g characteristic states with SOC are broadened compared with those without SOC, which leads to the some reduction of the semiconductor gaps of the Ca2MReO6. It should be pointed out that the noninteger moments in Bohr magneton in the Ca2MReO6 (M = Cr, Fe) with P21/n structure are the consequence of the mixing of spin-up and spin-down states, but the semiconductor gaps are preserved.


image file: c5ra09921h-f9.tif
Fig. 9 The spin-resolved DOSs of Ca2CrReO6 (a) and Ca2FeReO6 (b) calculated with mBJ potential and SOC taken into account.

VI. Conclusion

We have used FP-LAPW method to investigate the structural, electronic, and magnetic properties of double perovskites Ca2MReO6 (M = Cr, Fe). The GGA approach has been used to do geometry optimization, and then the electronic and magnetic properties have been investigated with mBJ exchange potential for improving on description of electronic structures. Our calculated results shows that the ground-state phase assumes the P21/n structure and is a ferrimagnetic semiconductor for both of the Ca2MReO6, being consistent with experiment. In the case of the Ca2CrReO6 (Ca2FeReO6) phase, we have three (five) Cr3+ (Fe3+) 3d electrons and two Re5+ 5d electrons, respectively. The Hund's rule and the crystal field and spin exchange splitting require that three Cr3+ (Fe3+) 3d t2g (t2g + eg) bands below the Fermi level in the majority-spin channel are fully filled and three Re5+ 5d t2g bands astride the Fermi level in the minority-spin channel are filled by two electrons, as the GGA electronic structures shows. Our calculation and comparison shows that the better mBJ exchange potential than GGA and the monoclinic lattice distortion against the I4/m structure are both necessary to obtaining the nonzero semiconductor gaps. This implies that the electron correlations are important in driving the I4/m structure to the monoclinic structure and the resulting cooperation of oxygen-octahedral distortions and electron correlations in the monoclinic phases is necessary to splitting the partially-filled Re 5d triplet bands into the fully-filled doublet bands and the empty singlet bands in the minority-spin channel. In this sense, both electron correlations and O-octahedral distortion are needed for forming the semiconductive nature of the Ca2MReO6. When the spin–orbit coupling is taken into account, the total magnetic moments become noninteger in unit of Bohr magneton due to the mixing of spin-up and spin-down states, and fortunately, the semiconductor gaps (0.31 and 0.03 eV) remain open.

In summary, our calculated results and analyses show that the monoclinic Ca2CrReO6 and Ca2FeReO6 are both ferrimagnetic semiconductors, being consistent with experiment, and their nonzero semiconductor gaps are formed because there exist strong interaction of oxygen-octahedral distortion and electron correlations in them. This mechanism can be useful to fully understand chemical and physical properties of double perovskite compounds.

Acknowledgements

This work is supported by Nature Science Foundation of China (Grant No. 11174359), by Chinese Department of Science and Technology (Grant No. 2012CB932302), and by the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDB07000000).

References

  1. S. A. Wolf, D. D. Awschalom, R. A. Buhrman, J. M. Daughton, S. von Molnár, M. L. Roukes, A. Y. Chtchelkanova and D. M. Treger, Science, 2001, 294, 1488 CrossRef CAS PubMed.
  2. M. T. Anderson, K. B. Greenwood, G. A. Taylor and K. R. Poeppelmeier, Prog. Solid State Chem., 1993, 22, 197 CrossRef CAS.
  3. K. I. Kobayashi, T. Kimura, H. Sawada, K. Terakura and Y. Tokura, Nature, 1998, 395, 677 CrossRef CAS.
  4. W. E. Pickett, Phys. Rev. B: Condens. Matter Mater. Phys., 1998, 57, 10613 CrossRef CAS.
  5. K. I. Kobayashi, T. Kimura, Y. Tomioka, H. Sawada, K. Terakura and Y. Tokura, Phys. Rev. B: Condens. Matter Mater. Phys., 1999, 59, 11159 CrossRef CAS.
  6. A. Arulraj, K. Ramesha, J. Gopalakrishnan and C. N. R. Rao, J. Solid State Chem., 2000, 155, 233 CrossRef CAS.
  7. Y. Moritomo, S. Xu, A. Machida, T. Akimoto, E. Nishibori, M. Takata and M. Sakata, Phys. Rev. B: Condens. Matter Mater. Phys., 2000, 61, R7827 CrossRef CAS.
  8. M. G. Hernández, J. L. Martinez and J. A. Alonso, Phys. Rev. Lett., 2001, 86, 2443 CrossRef.
  9. H. Kato, T. Okuda, Y. Okimoto, Y. Tomioka, K. Oikawa, T. Kamiyama and Y. Tokura, Phys. Rev. B: Condens. Matter Mater. Phys., 2004, 69, 184412 CrossRef.
  10. G. Vaitheeswaran, V. Kanchana and A. Delin, Appl. Phys. Lett., 2005, 86, 032513 CrossRef PubMed.
  11. N. S. Rogado, J. Li, A. W. Sleight and M. A. Subramanian, Adv. Mater., 2005, 17, 2225 CrossRef CAS PubMed.
  12. A. J. Hauser, R. E. A. Williams and F. Yang, Phys. Rev. B: Condens. Matter Mater. Phys., 2011, 83, 014407 CrossRef.
  13. H. P. Wu, Y. Qian and R. F. Lu, Appl. Phys. Lett., 2011, 99, 123116 CrossRef PubMed.
  14. A. Winkler, N. Narayanan, D. Mikhailova, K. G. Bramnik, H. Ehrenberg, H. Fuess, G. Vaitheeswaran, V. Kanchana, F. Wilhelm, A. Rogalev, A. Kolchinskaya and L. Alff, New J. Phys., 2009, 11, 073047 CrossRef.
  15. O. Erten, O. N. Meetei, A. Mukherjee, M. Randeria, N. Trivedi and P. Woodward, Phys. Rev. Lett., 2011, 107, 257201 CrossRef.
  16. A. F. Garcia-Flores, A. F. L. Moreira, U. F. Kaneko, F. M. Ardito, H. Terashita, M. T. D. Orlando, J. Gopalakrishnan, K. Ramesha and E. Granado, Phys. Rev. Lett., 2012, 108, 177202 CrossRef CAS.
  17. C. Du, R. Adur, H. Wang, A. J. Hauser, F. Yang and P. C. Hammel, Phys. Rev. Lett., 2013, 110, 147204 CrossRef.
  18. D. Serrate, J. M. de Teresa and M. R. Ibarra, J. Phys.: Condens. Matter, 2007, 19, 023201 CrossRef.
  19. T. K. Mandal, C. Felser, M. Greenblatt and J. Kübler, Phys. Rev. B: Condens. Matter Mater. Phys., 2008, 78, 134431 CrossRef.
  20. H. Kato, T. Okuda, Y. Okimoto, Y. Tomioka, Y. Takenoya, A. Ohkubo, M. Kawasaki and Y. Tokura, Appl. Phys. Lett., 2002, 81, 328 CrossRef CAS PubMed.
  21. Y. Kronkenberger, K. Mogare, M. Reehuis, M. Tovar, M. Jansen, G. Vaitheeswaran, V. Kanchana, F. Bultmark, A. Delin, F. Wilhelm, A. Winkler and L. Alff, Phys. Rev. B: Condens. Matter Mater. Phys., 2007, 75, 020404(R) CrossRef.
  22. O. N. Meetei, O. Erten, M. Randeria, N. Trivedi and P. Woodward, Phys. Rev. Lett., 2013, 110, 087203 CrossRef.
  23. H. L. Feng, M. Arai, Y. Matsushita, Y. Tsujimoto, Y. Guo, C. I. Sathish, X. Wang, Y. H. Yuan, M. Tanaka and K. Yamaura, J. Am. Chem. Soc., 2014, 136, 3326 CrossRef CAS PubMed.
  24. H. Wang, S. Zhu, X. Ou and H. Wu, Phys. Rev. B: Condens. Matter Mater. Phys., 2014, 90, 054406 CrossRef.
  25. A. K. Pual, M. Jansen, B. Yan, C. Felser, M. Reehuis and P. M. Abdala, Inorg. Chem., 2013, 52, 6713 CrossRef PubMed.
  26. A. K. Paul, M. Reehuis, V. Ksenofontov, B. Yan, A. Hoser, D. M. Többens, P. M. Abdala, P. Adler, M. Jansen and C. Felser, Phys. Rev. Lett., 2013, 111, 167205 CrossRef.
  27. H. Kato, T. Okuda, Y. Okimoto, Y. Tomioka, K. Oikawa, T. Kamiyama and Y. Tokura, Phys. Rev. B: Condens. Matter Mater. Phys., 2002, 65, 144404 CrossRef.
  28. F. Tran and P. Blaha, Phys. Rev. Lett., 2009, 102, 226401 CrossRef.
  29. D. J. Singh, Phys. Rev. B: Condens. Matter Mater. Phys., 2010, 82, 155145 CrossRef.
  30. S. Gong and B. G. Liu, Phys. Lett. A, 2011, 375, 1477 CrossRef CAS PubMed; S. Gong and B. G. Liu, Chin. Phys. B, 2012, 21, 057104 CrossRef.
  31. S. D. Guo and B. G. Liu, Chin. Phys. B, 2012, 21, 017101 CrossRef.
  32. P. Hohenberg and W. Kohn, Phys. Rev., 1964, 136, B864 CrossRef.
  33. W. Kohn and L. J. Sham, Phys. Rev., 1965, 140, A1133 CrossRef.
  34. P. Blaha, K. Schwarz, G. K. H. Madsen, D. Kvasnicka and J. Luitz, WIEN2k An Augmented Plane Wave + Local Orbitals Program for Calculating Crystal Properties, Karlheinz Schwarz Technische Universität Wien, Austria, 2001 Search PubMed.
  35. J. P. Perdew, K. Burke and M. Ernzerhof, Phys. Rev. Lett., 1996, 77, 3865 CrossRef CAS.
  36. A. H. MacDonald, W. E. Pickett and D. D. Koelling, J. Phys. C: Solid State Phys., 1980, 13, 2675 CrossRef CAS PubMed.
  37. J. Kunes, P. Novak, R. Schmid, P. Blaha and K. Schwarz, Phys. Rev. B: Condens. Matter Mater. Phys., 2001, 64, 153102 CrossRef.
  38. D. D. Koelling and B. N. Harmon, J. Phys. C: Solid State Phys., 1977, 10, 3107 CrossRef CAS PubMed.
  39. J. Gopalakrishnan, A. Chattopadhyay, S. B. Ogale, T. Venkatesan, R. L. Greene, A. J. Millis, K. Ramesha, B. Hannoyer and G. Marest, Phys. Rev. B: Condens. Matter Mater. Phys., 2000, 62, 9538 CrossRef CAS.
  40. Z. Szotek, W. M. Temmerman, A. Svane, L. Petit and H. Winter, Phys. Rev. B: Condens. Matter Mater. Phys., 2003, 68, 104411 CrossRef.
  41. H. Iwasawa, T. Saitoh, Y. Yamashita, D. Ishii, H. Kato, N. Hamada, Y. Tokura and D. D. Sarma, Phys. Rev. B: Condens. Matter Mater. Phys., 2005, 71, 075106 CrossRef.
  42. D. Koller, F. Tran and P. Blaha, Phys. Rev. B: Condens. Matter Mater. Phys., 2011, 83, 195134 CrossRef.
  43. J. B. Philipp, P. Majewski, L. Alff, A. Erb, R. Gross, T. Graf, M. S. Brandt, J. Simon, T. Walther, W. Mader, D. Topwal and D. D. Sarma, Phys. Rev. B: Condens. Matter Mater. Phys., 2003, 68, 144431 CrossRef.
  44. J. A. Alonso, M. T. Casais, M. J. Martínez-Lope, J. L. Martínez, P. Velasco, A. Muñoz and M. T. Fernández-Díaz, Chem. Mater., 2000, 12, 161 CrossRef CAS.

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