Alveena Z. Khan,
Joseph M. Flitcroft
and
Jonathan M. Skelton
*
Department of Chemistry, University of Manchester, Oxford Road, Manchester M13 9PL, UK. E-mail: jonathan.skelton@manchester.ac.uk
First published on 19th August 2025
We present a detailed first-principles study of the electrical and thermal transport, and the thermoelectric figure of merit zT, of the oxide perovskite SrTiO3 in the orthorhombic Pnma, tetragonal I4/mcm and cubic Pmm phases. Analysis of the lattice thermal conductivity shows that the “particle-like” contribution, κp, is highest in the Pm
m phase due to larger phonon group velocities. We also find that all three phases show significant heat transport through glass-like interband tunnelling. On the other hand, we predict the cubic and orthorhombic phases to show superior n-type conductivity, due to significantly stronger polar-optic phonon scattering and shorter electron lifetimes in the tetragonal phase. Due to its superior electrical properties, we predict that the Pm
m phase will attain a 25% larger high-temperature zT than the I4/mcm phase, while we predict the best zT can be obtained for the Pnma phase due to its favourable electrical properties and low κlatt. This work provides new insight into the impact of structure type on the thermoelectric performance of oxide perovskites, and indicates targeting particular structure types, e.g. through chemical doping, could provide a facile route to optimising the zT of SrTiO3 and related systems.
Thermoelectric (TE) power harnesses the Seebeck effect in a TE material to converts heat to electricity and thus recover waste heat as electrical energy. A thermoelectric generator (TEG) combines two TE materials with dominant p-type (hole) and n-type (electron) carriers, connected electrically in series and thermally in parallel, to harvest electrical energy from the temperature gradient between a heat source and sink. TEGs are solid state devices with no moving parts, are maintenance free and easily scalable, and produce no noise or emissions during operation, making them suitable for a wide range of applications. These include, but are not limited to: battery-free power sources for wireless sensors, wearables and medical devices;5–7 heat recovery from automobile powertrains and data centres;8,9 and as a primary geothermal power source.10 The conversion efficiency of a TE material is typically measured by the dimensionless figure of merit zT:
![]() | (1) |
Currently, the most widely used thermoelectric (TE) materials are Bi2Te3 for near-room temperature applications (zT from ∼1–1.5 at 350–450 K)4,14–16 and PbTe for high-temperature power generation (zT up to 2.2 at 915 K),17 due to a combination of a favourable electronic structure and intrinsically low thermal conductivity.18,19 However, Te is scarce and the environmental toxicity of Pb raises potential concerns over end-of-life disposal, which restrict these materials to niche applications.20 Widespread adoption of TEGs thus requires alternative materials that balance high performance with sustainability and cost efficiency.
Oxides are attractive candidate thermoelectric materials due to their low toxicity, low cost, and exceptional chemical stability, the latter of which makes them particularly well suited to high temperature heat recovery in automotive and industrial settings. Oxides often exhibit intrinsically large Seebeck coefficients, but typically also suffer from low electrical conductivity and high lattice thermal conductivity, resulting in overall modest zT values. However, the discovery of high thermoelectric power factors in cobalt oxides in the 1990s led to the identification of several families of prospective oxide TEs. p-type oxides include the layered cobaltites NaxCoO2,21–24 Ca3Co4O9,25–27 and Bi2Sr2Co2Oy.28–30 n-type oxides include ZnO31 and the ABO3 oxide perovskites, in particular SrTiO332–34 (STO) and CaMnO3.35,36
SrTiO3 in particular has emerged as one of the most promising oxide perovskite TEs due to its chemical versatility, high thermal stability, and tunable electronic properties.37 Compared to the related CaTiO3 and BaTiO3, STO has an intrinsically large |S|, reasonable σ, superior PF, and impressive thermal stability at elevated temperature.37–41 Computational modelling has further determined that these advantageous properties are due to STO supporting a significantly higher σ while maintaining comparable |S| to other titanates.42,43
STO is typically prepared and tested in thin-film form, with high-temperature zT competitive with other benchmark thin-film systems, e.g. zT ≈ 0.29 at T = 1000 K in Sr(Ti0.8Nb0.2)O2.7544 vs. zT ≈ 0.3 in Sb2Te3,45 zT ≈ 0.45 in unoptimised SnSe,46 and zT ≈ 0.4 in carbon nanotube films.47 Control of nanostructure can potentially push this much higher, with an unprecedented zT ≈ 1.6 at T = 298 K recently reported for Sr(Ti0.8Nb0.2)O3 through precisely controlled strain and interfacial polarisation.48 This is significantly higher than the zT = 0.02–0.08 obtained for bulk STO at room temperature, where the large κ = 9–12 W m−1 K−1 limits the thermoelectric performance.49
The wide variation in experimental results is in part due to the high structural and chemical flexibility inherent to perovskites, which can adopt multiple crystal phases and can accommodate doping at the A and B cation sites as well as significant levels of oxygen deficiency. Optimising STO and other oxide perovskite thermoelectrics therefore requires a good fundamental understanding of the underlying structure–property relationships. In a previous study, we applied a fully ab initio modelling approach to study the thermoelectric performance of orthorhombic CaTiO3, tetragonal SrTiO3 and rhombohedral BaTiO3.43 Among our key findings was that the crystal structure had a significant impact on the physical properties and in particular the κlatt. In this work, we build on this with a detailed first-principles study of STO in the orthorhombic, tetragonal and cubic phases. We find that the smaller primitive cell of the Pmm phase results in larger phonon group velocities and high κlatt, whereas the I4/mcm phase shows significantly stronger polar-optic phonon carrier scattering and lower electrical conductivity and power factors. As a result, the hypothetical Pnma phase, which combines the lower κlatt of the tetragonal phase and the high PF of the cubic phase, is predicted to show a ∼25% larger zT than the cubic phase and ∼50% larger zT than the tetragonal phase at high temperature. This work therefore demonstrates that materials engineering strategies to stabilise particular structural distortions from the cubic aristotype could be a facile route to optimising the performance of STO and other oxide perovskite thermoelectrics.
In the SM-RTA, the macroscopic κp is obtained as an average over contributions κqj from microscopic phonon modes qj, with wavevector q and band index j:50
![]() | (2) |
![]() | (3) |
![]() | (4) |
![]() | (5) |
![]() | (6) |
The SM-RTA model in eqn (2) only considers phonon depopulation events, whereas in real materials the flow of thermal energy can result in repopulation.51 This additional contribution can be taken into account by full solution of the linearised Boltzmann transport equation (LBTE).51,52
Furthermore, significant overlap between phonon modes, due to small interband frequency spacing and/or to short τqj (broad Γqj) can lead to heat conduction through “wave-like” interband tunnelling characteristic of amorphous materials (glasses).51 This additional contribution κw can be obtained by solving the Wigner transport equation using the approach outlined in ref. 51. The κw can then be combined with either the RTA or LBTE models for the κp to compute the total lattice thermal conductivity as:
κlatt(T) = κp(T) + κw(T) | (7) |
The κp, κw and κlatt are 3 × 3 tensors, with the transport along the three Cartesian directions α = x, y and z given by the diagonal elements καα. As thermoelectric materials typically take the form of consolidated powders or thin films with randomly-oriented crystal grains, we compute a (scalar) average κlatt from:
![]() | (8) |
The spectral conductivity Σ is calculated according to:54
![]() | (9) |
![]() | (10) |
τkj−1(T) = ΓADPkj(T) + ΓPOPkj(T) + ΓIMPkj(T) + ΓPIEkj(T) | (11) |
The Σ is then used to obtain the generalised moments of the transport distribution function, n, from:
![]() | (12) |
![]() | (13) |
Finally, the σ, S and κel are calculated from the n(T) according to:53,54
σ(εF, T) = ![]() | (14) |
![]() | (15) |
![]() | (16) |
The n, and hence the σ, S and κel, depend on the Fermi energy. Under the assumption that dopants do not affect the host band structure, the εF can be adjusted to specify an extrinsic carrier concentration (“doping level”) n to predict the effect of chemical doping. (This is termed the “rigid band approximation” (RBA).)
As for the κlatt, the σ, S and κel are 3 × 3 tensors, and scalar averages σ, S and κel can be obtained in an analogous manner to eqn (8). The power factor S2σ in eqn (1) is also orientation dependent, and the PF along a given Cartesian direction can be calculated from:
(S2σ)α = Sαα2σαα | (17) |
The zT is orientation dependent and the values along the three Cartesian directions can be calculated as:
![]() | (18) |
As noted in Section 2.1.1, heat transport through three different mechanisms can be taken into account when computing the κlatt (particle-like transport with the SM-RTA or LBTE models, and interband tunnelling). We discuss the contributions of these different mechanisms in detail in Section 3.1 below.
Initial structures of SrTiO3 in the tetragonal I4/mcm and cubic Pmm phases were taken from the materials project (MP) database56 (mp-5229, mp-4651), and an orthorhombic Pnma structure was built by substituting the A-site cation in CaTiO3 (mp-1185232). All three structures were then fully optimised to tight tolerances of 10−8 eV on the total energy and 10−3 eV Å−1 on the forces.
Electron exchange and correlation were modelled using the PBEsol generalised gradient approximation (GGA) functional.57 The ion cores were modelled using projector-augmented (PAW) pseudopotentials58,59 with the following valence configurations: Ti – 3d2 4s2; O – 2s2 2p4; Sr – 4s2 4p6 5s2. The valence wavefunctions were described using a plane-wave basis with an 800 eV kinetic-energy cutoff, and the electronic Brillouin zones were sampled using Γ-centred Monkhorst–Pack k-point meshes60 with 6 × 6 × 6, 5 × 5 × 3 and 3 × 2 × 4 subdivisions for the Pmm, I4/mcm and Pnma phases respectively. These parameters were chosen based on explicit testing to converge the absolute total energies to <1 meV atom−1 and the external pressures to <1 kbar (0.1 GPa).
The 3rd-order (anharmonic) force constants were computed in a 3 × 3 × 3 expansion of the Pmm unit cell (135 atoms), a 2 × 2 × 2 expansion of the I4/mcm primitive cell (80 atoms), and a 2 × 1 × 2 expansion of the Pnma unit cell (80 atoms). The “particle-like” lattice thermal conductivities for band transport were calculated using the SM-RTA model by combining the 2nd- and 3rd-order force constants to evaluate the heat capacities Cqj, group velocities νqj and lifetimes τqj on uniform Γ-centred 22 × 22 × 22, 8 × 8 × 8 and 12 × 12 × 12 q-point sampling meshes for the Pm
m, I4/mcm and Pnma phases respectively. These meshes were chosen based on explicit testing to converge the scalar average of the κp tensors (eqn (2) and (8)) to within 5% of the values obtained with larger sampling meshes. We also solved the full linearised phonon BTE to obtain the κp including repopulation effects, and the Wigner transport equation to determine the κw contribution from interband tunnelling.51
AMSET estimates the electronic relaxation times by summing scattering rates from four different processes, viz. acoustic deformation potential (ADP), polar optic phonon (POP), piezoelectric (PIE), and ionised impurity (IMP) scattering, requiring a range of material properties to be calculated. (We note that PIE scattering is negligible in the three systems examined in this work, as they have centrosymmetric space groups and the piezoelectric moduli vanish by symmetry.)
Deformation potentials were computed by performing a series of single-point energy calculations on deformed structures, generated using AMSET, with PBEsol. The high-frequency, ionic and static dielectric constants ε∞, εionic and εs = ε∞ + εionic, together with the Born effective charges Z* and piezoelectric moduli, were determined using DFPT.63 Explicit tests found that 2× (Pmm/Pnma phases) and 3× denser k-point sampling (I4/mcm phase) compared to the “base” meshes used for geometry optimisation were required to converge the ε∞. The Z* were used to determine the infrared (IR) activities of the phonon modes at q = Γ,67,68 evaluated with Phonopy, and to calculate the polar optic phonon (POP) frequency
po. Finally, the elastic constant matrix elements Cij were computed using PBEsol and the finite-differences routines in VASP69 (denser k-point sampling was not required for these calculations).
![]() | ||
Fig. 1 Optimised structures of SrTiO3 in the cubic Pm![]() |
Both the lower-symmetry tetragonal I4/mcm and orthorhombic Pnma phases can be generated from the “parent” Pmm structure by rotations of the TiO6 octahedra.71 The I4/mcm phase is obtained by an anti-phase tilt of successive “layers” of TiO6 octahedra around the z axis, such that the a, b and c lattice vectors of the I4/mcm structure correspond to the (110), (
10) and (002) directions in the cubic phase. The Pnma phase is obtained by a more complex combination of an in-phase tilt around x and anti-phase tilts of the same angle around y and z, and the a, b and c lattice vectors correspond to the (011), (020) and (01
) directions in the Pm
m parent.
The calculated phonon spectra of the three SrTiO3 phases are shown in Fig. 2. The cubic Pmm structure has na = 5 atoms in the primitive cell, resulting in 3na = 15 branches at each phonon wavevector q. In contrast, the I4/mcm and Pnma structures have na = 10 and 20, respectively, and thus considerably more complex phonon spectra with 30 and 60 bands per q. The increase in complexity due to the larger primitive unit cells is further compounded by the lower band degeneracy from the reduced symmetry.
In all three systems, the A-site cation makes the largest contribution to the low-frequency modes, with sharp features in the DoS consistent with some degree of “rattling” behaviour. The mid-frequency optic modes are predominantly due to the motion of the Ti and O atoms, and can be attributed to deformations of the TiO6 octahedra, while all three systems show prominent high-frequency features associated with motion of the O atoms. The calculated phonon spectra of the Pmm and I4/mcm phases agree well with previous calculations.73,74
With the exception of some small interpolation artefacts around q = Γ in the Pnma dispersion, the dispersions of the orthorhombic and tetragonal phases show no imaginary harmonic modes, indicating that both structures are dynamically stable. On the other hand, the dispersion of the Pmm phase shows prominent dynamical instabilities at q = R and M, in agreement with previous calculations.75,76 These off-Γ instabilities are related to the octahedral tilts that generate the lower-symmetry structures.77 We were not able to find reference phonon spectra for the Pnma phase, but the good agreement for the Pm
m and I4/mcm phases compared to previous studies gives us confidence in our calculations on the orthorhombic phase.
The scalar-average “particle-like” conductivity, κp, of the three SrTiO3 phases obtained using the single-mode relaxation-time approximation (SM-RTA) are compared in Fig. 3(a), and values at T = 1000 K are compared in Table 1. At 1000 K, we predict κp = 1.2–1.9 W m−1 K−1, with an ordering of Pmm > I4/mcm > Pnma. Compared to the intermediate I4/mcm phase, which we examined in our previous study,43 the lower-symmetry orthorhombic phase has a 13% lower κp, but the κp is still 26% larger than that of the isostructural CaTiO3 (0.96 W m−1 K−1). On the other hand, the high-symmetry Pm
m phase has a 34% higher κp than the I4/mcm phase. Taken together, this suggests the effects of crystal symmetry and A-site cation mass on the κp are both strong and of similar magnitude. On the other hand, the three phases of STO have very similar density ρ = 5.1–5.12 g cm−3 (Table S1), which in our view cannot explain the significant variation in the κp. This provides further support for crystal symmetry being the key factor in the reduction in κp from the cubic to the orthorhombic phase.
![]() | ||
Fig. 3 “Particle-like” (band transport) contributions κp to the averaged lattice thermal conductivity κlatt of the Pm![]() |
To explore the origin of the differences in the SM-RTA κp, we employ the analysis from our previous studies13 and define a weighted-average phonon lifetime τph such that the κp can be written:
![]() | (19) |
The κp/τph and τph as a function of temperature for the three phases of STO are compared in Fig. 3(b) and (c), respectively, and values at T = 1000 K are listed in Table 1. The calculated κp/τph of the Pnma and I4/mcm phases are similar, differing by only 3.8% at 1000 K, whereas the group velocities of the Pmm phase are around a factor of two larger. Given that the group velocities νqj are the gradient of the phonon dispersion, this difference can be attributed to the impact of the smaller primitive cell of the cubic phase on the phonon dispersion (cf. eqn (4), Fig. 2). On the other hand, the τph fall in the order Pm
m < Pnma < I4/mcm, i.e. the cubic phase has the shortest averaged phonon lifetimes. The τph of the Pnma phase is 17% shorter than the I4/mcm phase at 1000 K, resulting in a lower overall κp, whereas the much larger κp/τph of the Pm
m phase offsets the short τph and results in the largest predicted κlatt among all three phases.
In the SM-RTA, the phonon lifetimes τqj are calculated as the inverse of the linewidths Γqj, which are obtained perturbatively from the imaginary parts of the phonon self-energies.50 The Γqj can be written approximately as:
![]() | (20) |
![]() | (21) |
N2(q, ω, T) = N(1)2(q, ω, T) + N(2)2(q, ω, T) | (22) |
![]() | (23) |
![]() | (24) |
To simplify the comparison between systems, it is useful to average the N2 over q to obtain functions of frequency only, i.e.:
![]() | (25) |
![]() | (26) |
Secondly, we compute weighted-average Ñ2 calculated from the τph and using eqn (20):
![]() | (27) |
The calculated 2 for the Pm
m phase of STO at T = 1000 K is shown in Fig. 4, and equivalent plots for the I4/mcm and Pnma phases are shown in Fig. S1. We find that the scattering phase space of the low-frequency phonon modes is dominated by collision processes, while decay pathways become available from ∼3 THz, are competitive with collisions up to 13 THz, and are the dominant scattering mechanism for the high-frequency modes up to the fmax ≈ 16 THz (cf. Fig. 2).
![]() | ||
Fig. 4 Average scattering phase space function ![]() ![]() ![]() ![]() |
The calculated and the phase space integral and Ñ2 defined in eqn (26) and (27) for all three phases are listed in Table 1. The scaled
and Ñ2 indicate that the three-phonon scattering strengths and phase spaces are similar across all three phases, with
between 5.08–6.09 × 10−7 eV2 and Ñ2 between 5.72–7.95 × 10−2 THz−1. The Ñ2 fall in the order of Pnma ≈ I4/mcm < Pm
m, i.e. the cubic phase has a notably larger scattering phase space. On the other hand, the
fall in the order I4/mcm < Pm
m < Pnma. The short τph of the cubic phase compared to the other two phases is therefore a product of moderate three-phonon interaction strengths and a large scattering phase space, whereas the longer τph of the tetragonal phase is due to comparatively weak three-phonon interactions and a small phase space.
The trend in the κp/τph with crystal symmetry qualitatively mirrors our previous calculations on the Group IV–VI chalcogenides, including the “flagship” thermoelectric materials SnS and SnSe, where low group velocities were found to be characteristic of low-symmetry structures with large primitive cells.13 In absolute terms, however, the κp/τph of all three STO phases are 10–40× larger than chalcogenide phases with comparable symmetry and smaller primitive cells. On the other hand, the τph at T = 300 K range from 0.3–0.5 ps (Table S2), placing them on the same order of magnitude as the shortest averaged lifetimes calculated in ref. 13. The Ñ2 at room temperature are on the same order as the largest values obtained for the chalcogenides, while the averaged three-phonon interaction strengths fall within the mid-to-upper range of . Compared to these other flagship thermoelectric materials, the oxides thus have relatively large three-phonon scattering phase spaces, moderate-to-strong phonon anharmonicity, and, consequently, short τph.
The trends in the group velocity and lifetimes compared to other classes of materials can be partially interpreted in terms of the chemical bonding. The harmonic frequencies and group velocities are both derived from the 2nd-order force constants (FCs), which describe the changes in atomic forces in response to small displacements of the atoms. Strong chemical bonding favours large FCs, high phonon frequencies, and, consequently, high group velocities (cf. eqn (4)). The three-phonon interaction strengths additionally depend on the 3rd-order FCs, which describe the changes in forces in response to pairwise atomic displacements. While we are not aware of any systematic studies to this effect, it is not unreasonable to expect the 2nd- and 3rd-order FCs to be at least loosely correlated, such that stronger bonding results in larger 2nd-order and 3rd-order FCs. From this point of view, the stronger bonding in the oxides results in larger group velocities, but also stronger three-phonon interactions and shorter phonon lifetimes. In these systems, the former dominates the κp.
The generality of our finding that the κlatt depends sensitively on crystal structure is also supported by a recent theoretical study of Zintl compounds.78 In particular, this study found that low group velocities and, in some cases, short lifetimes are favoured by inhomogeneous chemical bonding, for which low crystal symmetry is an indicator, which mirrors the trends for the three phases of SrTiO3 in the present study.
We also compared the κp obtained from the SM-RTA in eqn (2) with that obtained by full solution of the linearised phonon Boltzmann transport equation (LBTE) (Table 2).50,52 The conceptual difference between the two models is that the SM-RTA only considers depopulation events, whereas the LBTE approach also accounts for repopulation. In practice, the full LBTE solution gives similar results to the SM-RTA, with differences between −2.5 and 6.9% in the κp at T = 1000 K.
[W m−1 K−1] | |||||
---|---|---|---|---|---|
κp (SM-RTA) | κp (LBTE) | κw | κlatt (SM-RTA) | κlatt (LBTE) | |
Pm![]() |
1.88 | 2.01 | 1.0 | 2.88 | 3.01 |
I4/mcm | 1.4 | 1.44 | 1.32 | 2.72 | 2.77 |
Pnma | 1.21 | 1.18 | 1.36 | 2.57 | 2.54 |
![]() | ||
Fig. 5 Contribution to the scalar-average lattice thermal conductivity κlatt of the Pm![]() |
In our previous work on the lanthanide cobalates LnCoO379 we found that “wave-like” tunnelling made a significant contribution to the overall κlatt. We find the same for all three phases of SrTiO3, with the κw accounting for 33–35% of the κlatt of the Pmm phase at 1000 K, depending on whether the κp is calculated using the SM-RTA or LBTE model, and a larger 47–49 and 52–54% of the κlatt of the lower-symmetry I4/mcm and Pnma phases (Table 2). The larger κw of the tetragonal and orthorhombic phases can be explained by the more complex phonon dispersions leading to a smaller interband spacing, which more than compensates for the narrower linewidths (longer lifetimes) compared to the cubic phase (cf. Fig. 2 and Table 1). While we only considered the Pnma phases of the LnCoO3, we predicted a similar ∼50% contribution from the κw to the κlatt.79 We have also found that the κw is much more significant in the more structurally-complex “π” phases of the chalcogenides SnS and SnSe than the simpler orthorhombic phases.80 In conjunction with the present results, this suggests that there may be a universal trade-off between high κp in higher-symmetry phases and high κw in lower-symmetry phases.
Taken together, our analysis shows that the κlatt of SrTiO3 is a balance of several competing factors. The “particle-like” conductivity, κp, is largest in the high-symmetry Pmm phase, where the large phonon group velocities compensate for shorter lifetimes. On the other hand, the interband tunnelling contribution, κw, is larger in the lower-symmetry I4/mcm and Pnma phases, where the smaller interband frequency spacing outweighs the narrower linewidths. Overall, however, we predict the Pm
m phase to have a 5–10% larger κlatt than the I4/mcm phase, and a 10–20% larger κlatt than the Pnma phase, at 1000 K, and we therefore conclude that the phonon group velocities are the biggest factor in determining the higher thermal conductivity of the cubic phase. The difference between the tetragonal and orthorhombic phases is more subtle, but the shorter phonon lifetimes of the Pnma phase outweigh the slightly larger group velocities and κw to yield a 5–10% lower κlatt.
More generally, the short phonon lifetimes in comparison to the chalcogenides suggests that the most fruitful approach to optimising the κlatt of the oxide perovskites is likely to be targeting lower group velocities, e.g. through weaker or less homogeneous chemical bonding, the latter through structure types with larger/lower-symmetry unit cells. Our recent set of similar calculations on the LnCoO3 identified lower group velocities, attributed to the weaker ionic bonding, as a key factor in the lower κlatt, which lends support to this hypothesis.79
Finally, we also consider the directional anisotropy in the κlatt. Due to the symmetry of the Pmm, I4/mcm and Pnma structures, the equivalences of the diagonal elements of the κlatt are κxx = κyy = κzz = κlatt, κxx = κyy ≠ κzz and κxx ≠ κyy ≠ κzz. The independent components of the κp, obtained using the SM-RTA and LBTE, the κw and the κlatt at T = 1000 K are compared in Tables S3 and S4. The κp of the I4/mcm phase show modest anisotropy, with the thermal conductivity along the a = b and c directions differing from the scalar average κp in Table 2 by 7.6 and 15% respectively, and with similar % differences obtained for both the SM-RTA and LBTE κp. The anisotropy in the Pnma phase is much smaller, at 2.1–4.4% of the κp. The anisotropy in the κw is also relatively small, with maximum differences of 2.8 and 4.1% in the orthorhombic and tetragonal phases. Notably, differences in the κp and κw combine to minimise the anisotropy in the κlatt, with differences of 2.9–6% and 1.4–4.1%, respectively, for the I4/mcm and Pnma phases. Our calculations therefore predict minimal anisotropy in the κlatt in both non-cubic phases of STO.
As noted in the previous section, the c = z and b = y directions in the I4/mcm and Pnma phases are equivalent to the a = b = c directions in the Pmm phase. For the tetragonal phase, we predict the largest κp along the c direction, and the κlatt along this direction obtained using the SM-RTA and LBTE κp are equal to and 2.7% smaller than, respectively, the κlatt along the three axes in the cubic phase. For the orthorhombic phase, on the other hand, we predict the lowest κp and κw along the b direction, with the result that the κlatt is 14–19% smaller than in the cubic phase. This suggests that the phonon transport along the c direction in the I4/mcm phase remains similar to the parent cubic phase, but is significantly disrupted in the Pnma phase, which again highlights the large impact of the lower crystal symmetry on the κlatt.
Using the HSE06 hybrid functional, we predict bandgaps Eg between 4–4.25 eV for the three phases (Table 3), which are considerably larger than both the direct Eg = 3–3.25 eV and the indirect Eg = 3.75 eV reported in experiments.81,82 However, given the large Eg we would not expect the overestimation of the bandgaps to significantly impact the calculated electronic properties. A measured bandgap for Pnma STO is not available, but our predicted band gap value is consistent with the insulating nature predicted in ref. 83.
Eg,dir [eV] | Eg,indir [eV] | |
---|---|---|
Pm![]() |
4.23 | 4.0 |
I4/mcm | 4.15 | 4.14 |
Pnma | 4.13 | — |
Expt81,82 | 3.75 | 3–3.25 |
Fig. 7 shows the predicted scalar-average electrical conductivity σ, absolute Seebeck coefficient |S|, power factor S2σ (PF) and electronic thermal conductivity κel of the three STO phases with n-type doping as a function of doping level n at a fixed T = 1000 K. A similar plot showing the temperature dependence of the properties at a fixed n = 2 × 1021 cm−3 is provided in Fig. S2.
The relationship between n and σ is given by:
![]() | (28) |
On the other hand, the S is inversely proportional to the n according to:
![]() | (29) |
![]() | (30) |
The opposing behaviour of σ and |S| result in a peak in the S2σ, with the PFs optimised at n ≈ 2 × 1021 cm−3. This is in line with previous studies.43,84 While pristine stoichiometric SrTiO3 can have relatively low n on the order of 1015 cm−3,85 exposure of the material to reducing conditions can produce high concentrations of oxygen vacancies, which act as electron donors, and yield carrier concentrations above 1020 cm−3 without explicit chemical doping.86 It is possible to obtain n > 1021 cm−3 with explicit doping, for example by replacing Sr with La and/or Ti with Nb.86–88 The carrier concentration we predict is required to optimise the PFs should therefore be readily accessible in experiments.
Finally, large n results in “degenerate” semiconducting behaviour with a metallic-like dependence of the conductivity on temperature (Fig. S2). Under these circumstances, the κel is related to the σ through the Wiedemann–Franz law:
κel = LσT | (31) |
We note that we have excluded the temperature dependence of the properties in eqn (28)–(31) for brevity, but the effective masses , τel and L are in general temperature dependent. All four parameters also in general depend on the n.
Table 4 lists the values of the four electrical properties at n = 2 × 1021 cm−3 and T = 1000 K. We predict the Pmm and Pnma phases to show similar electrical properties, with the former having a 10% higher σ and the latter an 11% larger |S|. The net result is that the Pnma phase is predicted to have a 10% larger PF and, due to its lower σ, a 10% lower κel. On the other hand, while all three phases have similar |S|, the I4/mcm phase has notably lower σ, which results in a 32/62% smaller peak PF compared to the Pm
m and Pnma phases, albeit with the benefit of a 40–60% lower κel.
Given the similar band structure and Eg, the lower electrical conductivity of the I4/mcm phase is somewhat surprising. To investigate this further, we followed the procedure in ref. 89 to obtain an estimate of the and
. This entails performing calculations using the constant relaxation-time approximation (CRTA), in which the τkj in eqn (9) are replaced by a constant relaxation time τel. In these calculations, the τel act as a scaling factor for the σ (cf. eqn (28)), and the CRTA conductivity and the σ calculated with per-state scattering rates can thus be used to determine weighted-average τel for comparing between systems in the same way as the τph in eqn (19).
The calculated ,
and τel at n = 2 × 1021 cm−3 and T = 1000 K are included in Table 4. We calculate very similar
and
for the three systems. The 5.9 and 8.6% larger
of the I4/mcm and Pnma phases compared to the cubic phase account for the majority of the 7.7/11.5% larger |S|. On the other hand, the 2.6–5.1% difference in the
of the Pnma and I4/mcm phases compared to the Pm
m phase indicate that the much lower σ of the tetragonal phase is not due to differences in the carrier effective masses. Instead, the calculated τel indicate that the I4/mcm phase has significantly stronger electron scattering compared to the other two phases.
Analysis of the mobility μ as a function of n at T = 1000 K shows that the μ is dominated by polar-optic phonon (POP) scattering (Fig. S3). The associated μPOP are between 1.5–2× larger in the Pnma and Pmm phases, indicating that the shorter τel in the I4/mcm phase is due to stronger POP scattering. The treatment of POP scattering in this work is based on the Frölich model for an electron in a dielectric medium interacting with a dispersionless optic phonon mode with frequency ωpo.90 The scattering matrix elements g are of the form:91
![]() | (32) |
We recently performed a similar analysis for the chalcogenides SnS and SnSe,80 which yielded and
and 0.7–0.81 respectively. The oxides have a larger
, resulting in lower σ that requires roughly an order of magnitude larger n to offset. While the oxides have a 3–4× larger mS, potentially resulting in a larger |S|, this is counterbalanced by the large n required to optimise the PF. Also, while ref. 80 did not calculate τel, similar results to those obtained with per-state τkj were obtained using a typical τel = 10 fs (10−14 s), which suggests a weighted-average relaxation time around an order of magnitude longer than we calculate for STO. The analysis of the κlatt in the previous section suggested that the stronger bonding in the oxides may lead to stronger phonon anharmonicity and shorter phonon lifetimes. Drawing a parallel, analysis of the τel suggests that this also results in stronger electron scattering and shorter electron lifetimes.
Our previous study of the LnCoO3 yielded and
at the n that maximise the PF.79 In terms of optimising the properties, this suggests that, as for the κlatt, exploring alternative perovskite chemistries may be fruitful, although weaker chemical bonding may have the undesirable side effect of increasing the conductivity effective masses. It would be of particular interest to determine whether the much lower σ of the I4/mcm phase is replicated over other perovskite materials, as, if so, it would imply that this phase should ideally be avoided. The results in the present study are however insufficient to confirm, or otherwise, the generality of this finding.
Finally, we again consider the directional anisotropy in the electrical properties. The diagonal σαα, Sαα and κel,αα components of the σ, S and κel tensors, and the corresponding power factors Sαα2σαα, calculated at n = 2 × 1021 cm−3 and T = 1000 K are shown in Table S5. The tetragonal phase shows fairly minimal anisotropy, with up to 5% differences in the directional σ, S and S2σ compared to the scalar averages, and a slightly larger 7.5% variation in the κel. The electrical properties of the orthorhombic phase show more anisotropy, with up to 6–9% variation in the σ, S and κel, and 12.7/10.9% higher/lower S2σ along the crystallographic b and c directions compared to the scalar average, which, for this system, is close to the PF along the a direction. While larger than the anisotropy in the κlatt, we still consider this to be relatively modest.
The I4/mcm structure shows the largest σ and κel but the smallest |S| along the c direction. The |S| is similar to the cubic phase, but the σ and κel are much smaller, as is the S2σ. The equivalent comparison for the Pnma phase shows the smallest σ, largest |S| and intermediate κel along the b direction. The σ and κel are lower than those in the Pmm phase, but more comparable than those in the tetragonal phase, whereas the |S| and, consequently, the PF, are significantly larger. We therefore infer that the distortions in the two lower-symmetry phases have a significant impact on the electrical properties relative to the cubic phase, even when compared along equivalent directions.
Fig. 8 shows the predicted scalar-average zT of the three phases of SrTiO3 as a function of doping level n and temperature T. Given the fall in the κlatt with temperature and the behaviour of the power factor S2σ with n (cf. Fig. 5 and 7), the best performance is obtained at high T and relatively large n ≈ 1021 cm−3.
Table 5 lists the maximum predicted zT, zTmax, at T = 400, 600 and 1000 K, roughly matching the low-, mid- and high-temperature heat-recovery scenarios outlined in ref. 92. We predict zTmax of <0.1, 0.13–0.21 and 0.31–0.47 at the three temperatures, all of which are lower than the typical benchmark zT = 1 but which are consistent at the higher temperature with experimental measurements. With the exception of the cubic and tetragonal phases having similar predicted zTmax at 400 K, we predict that the zT fall in the order of Pnma > Pmm > I4/mcm at all three temperatures. The relatively poor performance of the tetragonal phase is primarily due to its low conductivity, which does not compensate for its larger absolute Seebeck coefficient and results in a low power factor. On the other hand, the superior performance of the Pnma phase compared to the Pm
m phase is primarily due to its 15–30% lower κlatt and correspondingly lower total thermal conductivity, as well as to the combination of slightly lower σ and slightly larger |S| producing a 2–4% larger S2σ.
T [K] | n [cm−3] | ZT | S [μV K−1] | σ [S cm−1] | S2σ (PF) [mW m−1 K−2] | κ [W m−1 K−1] | |||
---|---|---|---|---|---|---|---|---|---|
κel | κlatt | κtot | |||||||
Pm![]() |
400 | 7.5 × 1020 | 0.06 | −109 | 900 | 1.06 | 0.76 | 5.79 | 6.55 |
600 | 7.5 × 1020 | 0.15 | −150 | 581 | 1.31 | 0.7 | 4.29 | 4.99 | |
1000 | 1 × 1021 | 0.39 | −182 | 448 | 1.48 | 0.79 | 3.01 | 3.8 | |
I4/mcm | 400 | 7.5 × 1020 | 0.06 | −128 | 484 | 0.79 | 0.4 | 4.9 | 5.3 |
600 | 1 × 1021 | 0.13 | −148 | 432 | 0.94 | 0.49 | 3.77 | 4.26 | |
1000 | 1 × 1021 | 0.31 | −195 | 261 | 0.99 | 0.45 | 2.77 | 3.22 | |
Pnma | 400 | 5 × 1020 | 0.09 | −148 | 500 | 1.08 | 0.4 | 4.25 | 4.65 |
600 | 7.5 × 1020 | 0.21 | −166 | 487 | 1.34 | 0.58 | 3.33 | 3.91 | |
1000 | 1 × 1021 | 0.47 | −198 | 392 | 1.54 | 0.7 | 2.54 | 3.24 |
Table S6 compares the directional values of the zT, S2σ and κtot under the same conditions as the zTmax in Table 5. The zT of the I4/mcm phase show modest anisotropy, with a 3.2% larger zTmax along the a = b directions and a 6.5% smaller zTmax along the c direction compared to the scalar average at T = 1000 K. This is due primarily to differences in the thermal conductivity. The Pnma phase shows more significant anisotropy, with a 3.9% larger PF and 4.3% smaller κtot along the b direction resulting in an 8.4% higher zTmax compared to the scalar average, and a 7.8% smaller PF and 0.93% higher κtot along the c direction producing a 10% lower zTmax. As for the electrical properties, we find little correspondence between the zT of the cubic phase and the zT along the c direction in the I4/mcm phase and the b direction in the Pnma phase, which indicates that the large impact of the structural distortions on the electrical properties also carries through to the figure of merit.
Experimental values of zT span a range of 0.27–0.37, with σ = 200–303 S cm−1, S = −168 to −233 μV K−1, and κ = 2.6–3.1 W m−1 K−1 at T = 1000 K.93–95 Assuming the Pmm phase, we predict values of between zT = 0.2 (n = 1020 cm−3, σ = 46.1 S cm−1, S = −367 μV K−1, κ = 3.09 W m−1 K−1) and zT = 0.37 (n = 5 × 1020 cm−3, σ = 227 S cm−1, S = −152 μV K−1, κ = 3.41 W m−1 K−1). These predictions, in particular those at the larger n, are reasonably consistent with experimental measurements, confirming the accuracy of our modelling approach. In particular, with reference to Table 2, and as found in our previous work,79 accounting for wave-like tunnelling contributions to the κlatt results in a notably better match to experiments. With this in mind, our predictions suggest that experiments have likely achieved close to the maximum possible for pristine bulk-like cubic STO, but that significant performance enhancements could be possible by targeting chemical modifications (e.g. doping) that stabilise the orthorhombic phase – according to our analysis, doing so would largely retain the favourable electrical properties of the Pm
m phase while significantly reducing the κlatt.
Analysis of the structural dynamics and lattice thermal conductivity shows that the primary impact of structure type is that the smaller primitive cell of the Pmm phase results in larger phonon group velocities and a larger contribution from “particle-like” (band) transport to the κlatt, which more than offsets its shorter phonon lifetimes. More generally, compared to the flagship Group IV–VI chalcogenide thermoelectrics the oxides show relatively strong phonon scattering and short phonon lifetimes, but this is more than compensated by larger group velocities. Based on this, efforts to optimise (i.e. reduce) the κlatt of STO and other oxide perovskites should focus on chemical modifications or alternative perovskite chemistries that favour lower-symmetry crystal structures and/or which have weaker/less homogeneous chemical bonding. A second notable finding from our analysis of the κlatt is the contribution from wave-like transport, which has a large impact on all three phases but is most significant for the lower-symmetry structures. Taken together with our previous work on the lanthanide cobalates, we suggest that accounting for transport through this mechanism is important for an accurate description of the κlatt in oxide perovskites generally, and that the increase in this term in lower-symmetry structures may be universal across different oxide perovskite chemistries.
Analysis of the electrical properties indicates that the I4/mcm phase has significantly lower electrical conductivity due to strong polar-optic phonon scattering, whereas the Pnma phase shows comparable or higher power factors to the cubic Pmm phase due to the combination of a lower σ and larger absolute Seebeck coefficient. Comparing again to the Group IV–VI chalcogenides, we find that the power factors of the oxides are limited by high conductivity effective masses and short electron lifetimes, and that the high carrier concentrations required to offset this effectively nullify the higher |S|. From a fundamental perspective, it is interesting to note that the oxides show both short phonon and electron lifetimes, which could indicate that the electrical properties and κlatt may be coupled in a way which is yet to be explored in detail. We also believe the low predicted σ of the I4/mcm phase warrants further investigation, particularly to determine whether similar behaviour is observed across different perovskite chemistries.
Finally, our predicted zT show that, while STO cannot achieve the benchmark zT ≥ 1 even at a high T = 1000 K, it may be possible to significantly improve upon existing experimental studies by targeting the stabilisation of lower-symmetry structures and in particular the orthorhombic Pnma phase.
We hope that the results presented here will ultimately provide some important insight to support ongoing efforts to obtain high-performance oxide thermoelectrics for sustainable energy recovery.
Raw data from this study will be made available to download free of charge after publication from an online repository at https://doi.org/10.17632/9h4b89b79r. Our analysis code is available on GitHub at https://github.com/skelton-group/ZT-Calc-Workflow.
This journal is © The Royal Society of Chemistry 2025 |