In addition to the oxides with the delafossite structure, wide band gap chalcogenide semiconductors have also been employed as p-type TCMs most recently.22–24 Due to the delocalized S-3p orbital, the valence band of sulfur-based TCMs (e.g. CuAlS2) exhibits more pronounced dispersion than their oxide-based counterparts (e.g. CuAlO2), leading to a low hole effective mass and high hole mobility.25–27 Additionally, the atomic energy level value of the S-3p orbital is higher than that of the O-2p orbital. Consequently, sulfur-based TCMs typically possess higher valence band positions relative to oxide-based TCMs, which makes them more favorable for p-type doping.26 Therefore, the wide band gap chalcogenide semiconductors such as BaCu2S2,28–30 CuAlS2,31,32 LaCuOS,33,34 and Cu3TaS4,35,36etc. have been investigated as p-type TCMs. Certain chalcogenide semiconductors have emerged as promising candidates for optoelectronic device applications, primarily attributed to their distinctive wide band gaps and inherent p-type conductivity. Zhang et al.37 successfully fabricated a transparent p–n junction with n-type AZO by exploiting the good electrical and optical properties of p-type LaCuOS. This device exhibited a high rectifying ratio of 300, demonstrating its potential applications in next-generation invisible electronics and optoelectronic devices. Yang et al.38 synthesized a transparent p-type conductive CuAl0.90Zn0.10S2 thin film using the pulsed plasma deposition technique and further fabricated a transparent p-CuAlS2:Zn/n-In2O3:W heterojunction diode. Similarly, Cu3TaS4 also has promising application prospects in transparent electronic devices due to its high optical transmittance and potential p-type conductivity.35
In this study, the electronic structure, optical properties, defect properties and p-type conductivity of Cu3TaS4 are investigated based on first-principles calculations. The wide electronic band gap and high optical transparency make it a viable candidate for TCMs. The calculated defect properties revealed that the intrinsic Cu3TaS4 exhibits p-type conductivity due to the low defect formation energy of VCu under Cu-poor conditions. Based on the defect properties, both pristine and p-type doping Cu3TaS4 exhibit poor p-type conductivity, primarily due to the strong compensation effect by the n-type defect Cui. The existence of the empty “channel” along the (100) direction in the Cu3TaS4 crystal allows the introduction of Cui into the crystal, whose n-type characteristics induce a strong compensation effect on p-type conductivity. Because of the strong compensation effect by Cui, it is difficult to achieve high hole concentration and excellent p-type conductivity for Cu3TaS4.
3.3.1 Intrinsic defect properties of Cu3TaS4.
Before the calculation of the intrinsic defect properties of Cu3TaS4, the relative chemical potentials should be evaluated. In general, the sum of the relative chemical potentials of the elements composed of Cu3TaS4 (i.e. ΔμCu, ΔμTa, and ΔμS) should be equal to the formation enthalpy of Cu3TaS4 under the thermodynamic equilibrium conditions:64 | 3ΔμCu + ΔμTa+ 4ΔμS = ΔH(Cu3TaS4) = −5.97 eV. | (2) |
In addition, to avoid the formation of element solids and binary or ternary competing phases, ΔμCu, ΔμTa, and ΔμS should be satisfied as the following:
| ΔμCu ≤ 0, ΔμTa ≤ 0, ΔμS ≤ 0. | (3) |
| 2ΔμCu + ΔμS ≤ ΔH(Cu2S) = −0.80 eV; | (4) |
| 2ΔμCu + 3ΔμS ≤ ΔH(Cu2S3) = −1.08 eV; | (5) |
| 7ΔμCu + 4ΔμS ≤ ΔH(Cu7S4) = −2.99 eV; | (6) |
| ΔμCu + ΔμS ≤ ΔH(CuS) = −0.50 eV; | (7) |
| ΔμCu + ΔμTa + 2ΔμS ≤ ΔH(CuTaS2) = −3.73 eV; | (8) |
| ΔμCu + ΔμTa + 3ΔμS ≤ ΔH(CuTaS3) = −4.35 eV; | (9) |
| 3ΔμTa + 2ΔμS ≤ ΔH(Ta3S2) = −4.51 eV; | (10) |
| ΔμTa + 2ΔμS ≤ ΔH(TaS2) = −3.53 eV; | (11) |
| ΔμTa + 3ΔμS ≤ ΔH(TaS3) = −3.56 eV; | (12) |
| 2ΔμTa + ΔμS ≤ ΔH(Ta2S) = −2.21 eV; | (13) |
| 6ΔμTa + ΔμS ≤ ΔH(Ta6S) = −2.56 eV; | (14) |
Based on the constraints mentioned above, the shadow area, as depicted in Fig. 4(a), is the allowed range of relative chemical potentials for stable Cu3TaS4. The intrinsic defect formation energies with the charge state q in different chemical environments (i.e. point A to point G) are calculated based on the supercell model. The calculation method is based on the following eqn:65
|  | (15) |
where
Edefect represents the total energy of the supercell containing defects with the charge state
q,
Eperfect is the total energy of the perfect supercell, and
ni is the number of the atom. Here, if an atom is added into the supercell,
n = −1, while
n = 1 represents that an atom is removed from the supercell.
μi is the chemical potential of element
i in the solid state, and Δ
μi is the relative chemical potential of corresponding element
i.
εVBM is the VBM of pure Cu
3TaS
4.
EF is the Fermi level in the range of 0 to 2.97 eV. Δ
V represents the electrostatic potential correction term between the defect and perfect systems, which is calculated by aligning the energy level position based on the average potential of the atom far away from the dopant.
66,67 Furthermore, the image charge correction term
Ecorr for charged defects is also considered,
68 which is calculated by the finite-corrections proposed by Lany and Zunger. The defect formation energies of intrinsic defects with the charge state
q under seven different chemical environments are calculated based on the above mentioned. Here, four intrinsic donors [
i.e. Ta interstitial (Ta
i), Ta substituted at the Cu site (Ta
Cu), the S vacancy (V
S), and Cu
i], four intrinsic acceptors [
i.e. vacancy Ta (V
Ta), S interstitial (S
i), Cu substituted at the Ta site (Cu
Ta), and V
Cu] and the defect complex of V
Cu + Cu
i are considered in the calculations on defect formation energies. To investigate the effect of defect separation (V
Cu and Cu
i), adjacent/distant configurations were calculated. The defect separations for adjacent and distant configurations are 3.95 Å and 10.45 Å, with total energies of −461.31 eV and −461.21 eV, respectively. The 0.1 eV energy difference between the two configurations negligibly impacts the computational results. As shown in
Fig. 4(b)–(h), Cu
i exhibits the lowest formation energy among donor defects, while V
Cu shows the minimum among acceptor defects. To evaluate the influence of chemical environments on the conductivity behaviour, the Cu-rich and Cu-poor conditions are considered, respectively. The Fermi level is pinned in the middle of the band gap in
Fig. 4(b), indicating that intrinsic Cu
3TaS
4 is an insulator under Cu-rich conditions (
i.e. point A). In contrast, the Fermi level is pinned at 0.62 eV above the VBM under Cu-poor conditions (
i.e. point D), demonstrating that the intrinsic Cu
3TaS
4 is more inclined to be doped as p-type under Cu-poor conditions. Based on the calculated results, the p-type defect V
Cu exhibits the lowest defect formation energy under Cu-poor conditions, indicating that the p-type conductivity of intrinsic Cu
3TaS
4 is associated with the p-type defect V
Cu under Cu-poor conditions. Therefore, our calculation results align well with the experimental studies.
42,43 Additionally, we also calculate the electronic structures of Cu
3TaS
4 with V
Cu, Cu
i, and the defect complex V
Cu + Cu
i, as presented in Fig. S2–S4 (ESI
†). It is observed that the Fermi level crosses the VBM in Cu
3TaS
4 with V
Cu, indicating the p-type conductivity, as shown in Fig. S2 (ESI
†). For the electronic structure of Cu
3TaS
4 with Cu
i, the Fermi level crosses the CBM, demonstrating the n-type conductivity. In addition, the electronic band gap of Cu
3TaS
4 with Cu
i is reduced to 2.87 eV and its CBM exhibits the antibonding states from the Ta_d and S_p states, as shown in Fig. S3 (ESI
†). In the case of Cu
3TaS
4 with the defect complex V
Cu + Cu
i, one can see that it is only affected the electronic band gap of Cu
3TaS
4, as shown in Fig. S4 (ESI
†). Accordingly, based on the band structures of Cu
3TaS
4 with V
Cu, Cu
i, and the defect complex V
Cu + Cu
i, the p-type conductivity of Cu
3TaS
4 should originate from the V
Cu, which is in line with the calculated intrinsic defect properties. Besides, it is also found that the donor defect Cu
i shows a strong compensation for the p-type conductivity under both Cu-rich and Cu-poor conditions, which negatively affects the increase of hole concentration. The reason could be attributed to the empty “channel” in the Cu
3TaS
4 crystal [
Fig. 1(b)], which make it easy to introduce Cu
i into the Cu
3TaS
4 crystal [
Fig. 1(d)]. In order to quantitatively study the facile introduction of the Cu
i, the lattice parameters and volume changes after the introduction of Cu
i are discussed. One can note that the fully optimized lattice constant (11.13 Å) and the supercell volume (1382.88 Å
3) are slightly decreased compared with those of the unoptimized supercell (the lattice constant and supercell volume are 11.17 Å and 1394.26 Å
3, respectively) after the introduction of Cu
i. In addition, the total energy of the fully optimized supercell with the Cu
i (−464.75 eV) is also slightly lower than that of the unoptimized supercell (−464.45 eV), which indicates that Cu
i produces only 0.30 eV of lattice deformation energy and then has a low formation energy. Combined with the slight reductions of the lattice parameter and the supercell volume, as well as the small lattice deformation energy, the Cu atom can be easily introduced into the empty “channel” of the supercell of Cu
3TaS
4.
 |
| Fig. 4 The allowed range of relative chemical potentials for stable Cu3TaS4 (a). The defect formation energies of Cu3TaS4 as a function of the Fermi level under seven extreme chemical potential environments [(point A to point G) (b)–(h)]. The black vertical dotted lines represent the Fermi level at 300 K. | |
In order to clearly characterize the p-type conductivity of intrinsic Cu3TaS4, the hole concentrations under Cu-rich and Cu-poor conditions are calculated based on the obtained defect properties. While Cu3TaS4 has been experimentally synthesized, the adopted preparation methods correspond to thermodynamic equilibrium growth processes.36,49 Recently, the non-equilibrium growth process has been utilized in both theoretical and experimental studies.69–72 The non-equilibrium growth process involves high-temperature synthesis of the sample followed by rapid quenching to room temperature. Samples fabricated via this method retain the defect density established during high-temperature growth, thereby resulting in enhanced electrical conductivity. Here, the model associated with the high-temperature growth and subsequent quenching processes is applied in our calculations, and the relevant details are presented in the ESI.†Fig. 5(a) and (b) depict the hole concentrations as a function of growth temperature. One can note that the hole concentration is rapidly increased to 1 × 1016 cm−3 after increasing the growth temperature to 1200 K under Cu-rich conditions (point A), as shown in Fig. 5(a). Generally, high temperature is widely used to prepare a defective sample and after sample preparation it is utilized at room temperature. After quenching to room temperature, the Fermi level is pinned in the middle of the band gap and therefore the hole concentration is reduced to 1 × 1012 cm−3, which is mainly ascribed to the compensation of the n-type defect Cui. In the case of the Cu-poor conditions (point D), the hole concentration reaches 5 × 1018 cm−3 when the growth temperature is increased to 1200 K, as shown in Fig. 5(b). However, after quenching to room temperature, the hole concentration is reduced near 1 × 1015 cm−3, which is significantly lower than that of commercialized n-type TCMs. The low hole concentration under Cu-poor conditions is mainly caused by the compensation of the donor defect Cui. To further assess the p-type conductivity of the intrinsic Cu3TaS4, the carrier mobility and the bipolar Seebeck coefficient are also calculated. It is worth noting that the carrier concentration should be given after using the AMSET code. Based on the calculated results, the hole concentration of intrinsic Cu3TaS4 under Cu-poor conditions was estimated to 1.00 × 1015 cm−3. However, the electron concentration of the intrinsic Cu3TaS4 could not be determined due to its p-type conductivity. We therefore estimated the electron concentration of intrinsic Cu3TaS4 based on the detailed balanced theory. The details of electron concentration calculations are presented in the ESI.† The calculated carrier mobility and the bipolar Seebeck coefficient are listed in Table S1 (ESI†). From Table S1 (ESI†), one can conclude that the intrinsic Cu3TaS4 with p-type conductivity has high hole mobility comparing with that of n-type. The calculated hole mobility is lower than that of the previous theoretical study41 using the deformation theory. This discrepancy is attributed to the distinct scattering mechanisms considered in our work. One can note that the Seebeck coefficient of n-type is slightly higher than that of the p-type as shown in Table S1 (ESI†), which is attributed to the inverse relationship between the Seebeck coefficient and carrier concentration. Although the n-type conductivity exhibits a large Seebeck coefficient, the hole concentration exceeding the electron concentration guarantees the p-type conductivity of intrinsic Cu3TaS4. Furthermore, both experimental studies35,36 and our calculation results confirm the p-type conductivity of Cu3TaS4. This is attributed to its suitable hole mobility and lowest defect formation energy of VCu under Cu-poor conditions. In addition, since the growth temperature is increased to 1200 K, it is essential to evaluate the stability of the sample under high temperature. We therefore employ the AIMD simulation to calculate the thermal stabilities at 300 K and 1200 K, respectively. The calculated results are depicted in Fig. S5 (ESI†). It is found that huge energy variations are hardly observed at both 300 K and 1200 K from 0 ps to 10 ps, indicating the thermal stabilities of the sample.
 |
| Fig. 5 The hole concentration of intrinsic Cu3TaS4 as a function of growth temperature under Cu-rich (a) and Cu-poor conditions (b), respectively. | |