3.1. Structural Properties and Thermodynamic Properties
In the present work, structure relaxations of T, M, and M′-REMO
4 (RE = Y, Dy, Gd, Nd, La; M = Ta, Nb) phases were performed. The crystal structures of M-, M’-RENbO
4, and RETaO
4 phases both belong to the monoclinic crystal structure, and the T phase is the tetragonal crystal.
Table 1 and
Table 2 list the calculated information of the crystal lattice at 0 K and the experimental data [
20,
21]. Our calculated results are consistently consistent with the experimental values. Both the calculations and experiments show that the small rare earth atom in RETaO
4 or RENbO
4 phases have small volumes. Besides, the β angle of the M phase and M’ phase also gradually decrease with the decrease of the atomic radius of RE
3+.
Figure 2a-j show the total energies for T, M, and M′-REMO
4 (RE = Y, Dy, Gd, Nd, La; M = Ta, Nb) phases, which are changed with a function of volume at 0 K. The equation of state (EOS) is used to fit the energy-volume. As we know, there are three crystalline structures in RETaO
4 materials, and they are monoclinic phase (M, space group I2/a), tetragonal phase (T, space group I41/a), and monoclinic-prime phase (M′, space group P2/a). At the high temperature, the stable phase is the T-RETaO
4, and it can transform to the M phase through a displacive transformation of T→M. However, the true equilibrium phase at low temperature is the M’ phase, which only can be obtained by means of synthesizing below the temperature of T→M transformation. Therefore, the M′ phase is the low-temperature phase of the RETaO
4 materials. As shown in
Figure 2a–j, our calculated results show that the M phase and T phase are both less stable than the M’ phase. It implies that the M phase is metastable and the M’ phase is stable at low temperatures. This is consistent with the experimental results [
22]. For RENbO
4 phases, only low-temperature M and high-temperature T phases are existent in the literature. As for comparisons, the M′-RENbO
4 structures are also calculated in this work. In
Figure 2a–j, our calculations exhibit that the total energy of the M-RENbO
4 phase is larger than that of the M′ phase, so the M phase is a true equilibrium phase at low temperature. This is consistent with the experimental results [
22] that M′-RENbO
4 crystalline structures do not exist in the RENbO
4 phases.
Figure 3 presents the relative energies (ΔE
M′→T or M→T) of M′- or M-REMO
4 with respect to that of T-REMO
4 for different rare-earth atoms of Y, Dy, Gd, Nd, and La. It is obvious that the relative energies are inversely proportional to the ionic radius of RE
3+. The Gibbs free energy difference of M′→T or M→T phase transformation ΔG
M′→T or M→T can be expressed as ΔH
M′→T or M→T -ΔS
M′→T or M→T*T. If the differences in the enthalpy ΔH (≈ΔE) and entropy ΔS are assumed to be substantially unchanged 4 [
23] and ΔS is supposed to be similar for the different rare-earth dopants, phase transformation temperature of M′→T or M→T may increase with the decreasing ionic radius of RE
3+ for Y, Dy, Gd, Nd, and La. This is consistent with the measured results using a high-temperature X-ray diffractometer by Stubičan [
24].
Figure 3 presents the comparison of the experimental transformation temperature and our calculated relative energies, which indicates that the relative energies and transformation temperature decrease with the increase of the rare earth ionic radius.
As M′ and M are the stable phases at the low temperature for the RETaO
4 and RENbO
4 structures, respectively, adding the Nb element into the M′-RETaO
4 phase should induce phase transformation of M′→M at the appropriate compositions. Based on the first-principles calculations, phase transformation of M′→M induced by the dopant of Nb is studied in this work.
Figure 4 presents our calculated relative energies (ΔE
M′→M) of M′-RETa
xNb
1−xO
4 (x = 0.25, 0.5, 0.75) with respect to that of M-RETa
xNb
1−xO
4 (x = 0.25, 0.5, 0.75) for different rare-earth atoms of Y, Dy, Gd, Nd, and La. When ΔE
M′→M > 0, this means that M′ is thermodynamically stable. Conversely, when ΔE
M′→M < 0, it implies that M is thermodynamically more stable than M′. In
Figure 4, the M′-RETa
xNb
1−xO
4 phase will transform into the M-RETa
xNb
1−xO
4 phase when the composition of the dopant Nb is about 0.5. It is worth mentioning that our calculated results are related to the phase transformation at 0 K, and transformation composition may decrease at the high temperature.
3.2. Mechanical Properties
The calculated elastic constants are listed in
Table 3,
Table 4 and
Table 5. Because the T-YTaO
4 phase is tetragonal, C
11, C
12, C
13, C
33, C
44, and C
66 can be determined through six deformation modes [
25]. As M′-YTaO
4 and M-YTaO
4 phases are both monoclinic, the thirteen independent elastic constants can be obtained by applying thirteen distortions [
26]. The total energies are varied before and after a set of different strains (±1%, ±2%, ±3%, and ±4%), and the elastic constants were calculated by the quadratic coefficients. For stable structures, the elastic constants need to meet the mechanical stability criterion [
27]. The monoclinic system criteria are C
11 > 0, C
22 > 0, C
33 > 0, C
44 > 0, C
55 > 0, C
66 > 0, C
44C
66 − 2C
46 > 0, C
11 + C
22 + C
33 + 2(C
12 + C
13 + C
23) > 0, C
22 + C
33 − 2C
23 > 0. The tetragonal system criteria are C
11 > 0, C
33 > 0, C
44 > 0, C
66 > 0, C
11-C
12 > 0, C
11 + C
33 − 2C
13 > 0, 2C
11+C
33+2C
12+4C
13 > 0. All RETaO
4 (RE = La, Nd, Gd, Dy) and RENbO
4 (RE = La, Nd, Gd, Dy) materials meet the criterion of mechanical stability, and the structures are stable.
‘The polycrystalline elastic mechanical properties, such as shear modulus (G or μ), bulk modulus (B), Young’s modulus (Y), and Poisson’s ratio (ν) could be obtained through the Voigt and Reuss methods according to the calculated elastic constants. Using energy considerations, Hill [
20] certificated the elastic moduli of the Voigt and Reuss methods are the upper and lower limits of polycrystalline constants. The practical elastic modulus can be estimated by the arithmetic means of these extremes. Generally, the bulk modulus is a measure of resistance to volume change by applied pressure. As seen from
Figure 5 and
Table 6,
Table 7 and
Table 8, the calculated shear modulus and bulk modulus of M-, M′-, T-RETaO
4, and RENbO
4 (RE = Y, Dy, Gd, Nd, La) is decreased with the increase of the rare-earth atoms, which indicate that the resistance to volume change through applied pressure is eventually lowered. Moreover, the calculated bulk modulus of rare-earth tantalate is regularly larger than and rare-earth niobates. The calculated shear modulus shows a similar trend, which means that the resistance to reversible deformations upon shear stress for RETaO
4 and RENbO
4 (RE = Y, Dy, Gd, Nd, La) is decreased with the increase of the rare-earth atoms. The ratio between bulk modulus and shear modulus, proposed by Pugh theory [
28], can be used to empirically predict the brittleness and ductility of materials. A low B/G ratio is associated with brittleness, and a high value indicates its ductile nature. The empirically critical value which distinguishes ductile and brittle materials is around 1.75. In the present work, the calculated B/G of REMO
4 in
Figure 6 is larger than 1.75, which means that all REMO
4 materials are ductile.
Young’s modulus E can be used to estimate the stiffness of materials. The calculations of M-, M′-, T-RETaO
4 or RENbO
4 in
Figure 7 and
Table 6,
Table 7 and
Table 8 suggest that Young’s modulus is decreased with an increase of the rare-earth atoms, which means that M-, M′-, and T-YTaO
4 are the stiffest, and then followed by DyTaO
4, GdTaO
4, NdTaO
4, and LaTaO
4. Moreover, our calculated results indicate that RETaO
4 is stiffer than RENbO
4. Poisson’s ratio (ν) is also related to the brittleness and ductility of materials. A compound is considered brittle if the ν is <0.26 [
29]. The higher value of Poisson’s ratio is, the more ductile the material is. Thus,
Table 6,
Table 7 and
Table 8 show that all REMO
4 materials are ductile. They are in good agreement with the results estimated by the B/G ratio. Besides, the value of Poisson’s ratio suggests that the ductility is inversely proportional to the rare earth atom of REMO
4 materials, and RENbO
4 is more ductile than RETaO
4.
Hardness is a very important mechanical property in applications. Hardness is defined as the resistance of a material to deformation and may be predicted using macroscopic and microscopic models. In this work, we use the semi-empirical equations of hardness proposed by Chen et al. [
30] and Tian et al. [
31] were used to study the hardness of the REMO
4 phases. The equations of these two models are defined as follow:
where k = G/B, G and B are the shear modulus and the bulk, respectively. The obtained hardness of REMO
4 phases are shown in
Figure 8 and
Table 6,
Table 7 and
Table 8 presents a comparison between the calculated and experimental results, which exhibits a good consistency. Besides, our calculations suggest that the Vickers hardness of the T phase decreases, and the single-phase gradually increase with the decrease of the atomic radius.
The anisotropic mechanical properties of the compounds are very important in applications. Based on the G and B values from Reuss and Voigt, Ranganathan et al. [
32] proposed a universal elastic anisotropy index A
U for crystal with any symmetry as shown below:
A
U is equal to zero when the single crystals are locally isotropic. The extent of single-crystal anisotropy can be expressed by the departure from zero indicates. The highly mechanical anisotropic properties exhibit large discrepancies from zero. The calculated elastic anisotropy is shown in
Figure 9. Most values of A
U are lower than 1. The larger the value of A
U is, the stronger the anisotropy of the phase. The M-, M′- and T-REMO
4 are anisotropic, and the elastic anisotropy of M and M′ phases is larger than the tetragonal (T) phase.