Weiwei
Wang
a,
Yang
Zhong
a,
Dahuai
Zheng
b,
Hongde
Liu
*a,
Yongfa
Kong
*ab,
Lixin
Zhang
a,
Rupp
Romano
cd and
Jingjun
Xu
*ab
aMOE Key Laboratory of Weak-Light Nonlinear Photonics and School of Physics, Nankai University, Tianjin 300071, China. E-mail: liuhd97@nankai.edu.cn; kongyf@nankai.edu.cn; jjxu@nankai.edu.cn
bTEDA Institute of Applied Physics, Nankai University, Tianjin 300457, China
cFaculty of Physics, Vienna University, Wien, A-1090, Austria
dDepartment of Complex Matter, Jozef Stefan Institute, Ljubljana, Slovenia
First published on 25th October 2019
Most metal-doped lithium niobates (LiNbO3, LN) exhibit n-type conductivity. The absence of p-type conductive LiNbO3 limits its application. Based on the finding that p-type conductive LiNbO3 can be realized by doping with a non-metallic element N, we investigate the most stable defect configurations and formation energies of LiNbO3 doped with non-metal nitrogen (LN:N) by first-principles calculations. Nitrogen substitution, interstitial and quasi-substitution point defects in different sites and their effects were explored. The results show that N prefers to occupy the oxygen site with only little lattice distortion. Ab initio molecular dynamics (AIMD) simulations confirm the structural stability of an N ion occupying the O site. The charge-state transition level ε(0/−1) slightly above the valence band maximum (VBM) indicates that N point defects would contribute to p-type conductivity of LiNbO3. The analysis of the band structure reveals that the partially filled impurity levels can accommodate electrons that jump from valence bands and result in holes to become the main charge carriers. The calculation not only explains the occurrence of p-type conductivity in LN:N but also provides a simple and efficient way to discover p-type conductive candidates in numerous doped LiNbO3 crystals.
As we know, many efforts have been devoted to the theoretical calculation of LN to explain some experimental phenomena and to provide a predictive guidance for the experiments in the past few years.17–20 Most of these computational studies concentrated on the replacement of Li or Nb cations in doped LN. Xu et al. reported the structures, energies and site preferences of Er defects in LiNbO3.19 And according to the report of Li et al., non-photorefractive ions generally prefer the Li site.18 Despite the cationic dopants being different from each other, all of them resulted in n-type conductivity.18–20 Little attention was paid to the relationship between the conductivity type and dopants. For non-metallic dopants, there is no relevant report to show their site occupation in LN, and the exploration of its impact on the properties of the non-metallic doped LN.
Non-metallic dopants have also played an important role in improving the properties of compounds. For example, graphene doped with nitrogen can open the band gap from zero, change the electronic structure of graphene and improve the free carrier density of graphene.21,22 The N element also plays a role in improving the band structure of titanium dioxide metal compounds.23,24 Due to the distinctive p-type conductivity performance of LN:N it is of importance to explore its p-type conductivity mechanism and its defect structure.
In this paper, employing first-principles calculations, we investigate the formation energies of nitrogen point defects: substitution of anions, N as interstitials and quasi-substitutions. The local atomic relaxations and their effects on the electronic structure of each defect are explored. The charge states of N dopants corresponding to the analysis of the band structure are also examined. The interaction between the dopants and the inherent atoms has also been studied. Finally, we discuss the p-type conductivity mechanism of LN:N through an analysis of the electronic properties.
Defect formation energy (DFE) is related to the difficulty of forming defect clusters, and a lower formation energy corresponds to a more stable defect complex.33 The DFEs of different point defects and defect complexes are calculated to explore the most stable defect complex formed in LN:N. The DFE of defect complex X with charge q is calculated using34,35
![]() | (1) |
![]() | (2) |
![]() | (3) |
![]() | (4) |
Bringing all the stability criteria together, we plotted the thermodynamically stable region of the LN in Fig. 1 according to the method in ref. 36 and 37. As shown in Fig. 1, the purple region CDFG is an area that meets the limitation of the equilibrium equation of lithium oxide, niobium oxide, and LN, and the line DF shows the Nb-rich condition while the line CG represents the Li-rich condition. Since the as-grown crystals and films are Li-deficient compositions, the chemical potentials of Nb and Li are chosen according to the line DF.36,37 The chemical potential of N atoms is assumed to be half of that of N2 (gas). The chemical potentials of Nb, Li, O and N elements are listed in Table 1. Similar results have been reported by other researchers.33,37
Condition | Atom species | Chemical potential (eV) |
---|---|---|
Li-Deficient | Li | −3.63 |
Nb | −18.96 | |
O | −5.59 | |
N | −8.33 |
Due to the total internal energies obtained from DFT calculations corresponding to the Helmholtz free energy at zero temperature, there is a difference between the VASP work environment and real conditions. Therefore, the free energy (F = E − TS) should be taken into account. Strain effects can be considered ignorable in the large supercell, and electronic entropy is negligible due to the large band gap of LiNbO3, too. The free energy is mainly related to the entropy which is related to the configuration contributions of point defects and defect clusters. Boltzmann's entropy can be calculated using17,37,38
S = kB![]() ![]() | (5) |
The ab initio molecular dynamic (AIMD) simulation with a canonical ensemble is performed by using the Nóse algorithm. The temperature of the system is maintained at 300 K.39 The 240-atom supercell with the Γ point is implemented here in the whole AIMD calculation. The time step is 1.0 fs and the total simulation time is 10.0 ps.
As shown in Fig. 2(a), numbers 1–3 present three different O sites that can be substituted by N (marked as NO) corresponding to the three different oxygen octahedron. The DFEs of the three NO point defect models are 5.64, 5.64 and 5.63 eV, respectively, showing a weak difference. This indicates that there is no obvious difference in the position of NO point defects, and the structure of NO point defects is fairly stable. The models for N as an interstitial (named as Ni) are shown in Fig. 2(b). Due to the limitation of the N atomic size, the possible interstitial sites distribute between two different O atoms in the same layer (labeled as 2, 4, 7 in Fig. 2(b)) or different O layers (labeled as 1, 3, 6 in Fig. 2(b)), and N interstitials can also exist at the center of oxygen octahedron, for example, number 5 in Fig. 2(b). The formation energies change significantly: the lowest formation energy is 4.68 eV. The most stable structure corresponds to the model where Ni lies between O atoms and it is close to the O hollow octahedron. The results show that there may be a positional priority for Ni point defects. With N as quasi-substitutions (Nq), N occupies the normal site of the O, while the original O atom becomes an interstitial at the same time. In Fig. 2(c), the different combinations of the N substitution and O interstitial are displayed. The distribution of O interstitials is the same as that of N interstitials. For comparison, the example where an O interstitial is far away from the N substitution is given in Table 2. Fig. 2(c) and Table 2 show that the formation energies of Nq point defects change significantly. The case of N as quasi-substitution usually comes along with strong lattice distortions that will seriously destroy the lattice structure of LiNbO3. Therefore, it is difficult to form N quasi-substitutions in the crystals. As seen from the formation energies, N lying in the specific location as an interstitial point defect has the lowest formation energy, while the distribution of NO is the most stable.
Model | Substitutional | Interstitial | ||||||||
---|---|---|---|---|---|---|---|---|---|---|
① | ② | ③ | ① | ② | ③ | ④ | ⑤ | ⑥ | ⑦ | |
Formation energy (eV) | 5.75 | 5.75 | 5.74 | 5.16 | 5.81 | 7.26 | 5.71 | 7.53 | 4.79 | 10.82 |
Quasi-substitutional | |||||||||
---|---|---|---|---|---|---|---|---|---|
Model | A + ① | A + ② | A + ③ | B + ③ | B + ④ | B + ⑥ | C + ⑤ | C + ⑦ | C + far away |
Formation energy (eV) | 5.16 | 7.52 | 5.20 | 5.16 | 7.68 | 5.21 | 5.24 | 5.20 | 9.71 |
Besides knowing their formation energies, it is also important to know how N point defects influence the crystal lattice. The knowledge of the lattice distortion around point defects greatly contributes to the understanding of their interaction with inherent atoms. The local structures of point defect NO before and after structure relaxation are shown in Fig. 3(a) and (b), respectively. As shown in Fig. 3(b), NO defects cause only a quite slight local distortion of the LN lattice. In detail, the distances from the upper O layer decrease while the distances from the lower O layer increase. The largest distortion is only 1.15% compared to that in the pristine crystals. In addition to the change in the distances of O atoms between different layers, the distances between the same layers of O atoms are increased, which indicates an increase of the O octahedral volume. As a whole, NO point defects are fairly stable. This fact can be ascribed to the similarity between N and O atoms.
Fig. 3(c) and (d), clearly show the lattice relaxation of Ni point defects. In Fig. 3(d), the Ni point defect moves against the z-direction due to the ferroelectric distortion and the distance between Ni and the nearest-neighboring O atoms along the z-direction increases. Due to the Coulomb repulsion of the electrons around N and O atoms, the O plane undergoes serious changes, in which some O atoms get out of the original O plane. Compared with lattice distortions of NO, Ni point defects have a stronger influence. This effect on the lattice structure is mainly reflected in the influence of O atoms, which means the influence on crystal electronic properties. We ignore the situation of Nq because of its strong distortion of the lattice structure.
Based on the above analysis, NO defects are superior to interstitial and quasi-substitution point defects because of their lower and more stable formation energies, and substitutions have the least influence on LN crystals compared with the other two forms of point defects. The charge states of the NO and Ni point defects are studied further to investigate their changes.
AIMD simulations were done to investigate the stability of the NO defect structure. On the basis of first-principles calculations and AIMD simulation, Fig. 4 shows the stability of the NO defect structure at a temperature of 300 K. The oscillation of energy (red line) tends to be stable, and the similarity of the two structures before and after 10 ps AIMD simulation indicates that it is fairly suitable for N ions to substitute O atoms.
![]() | ||
Fig. 4 Total energy fluctuation during AIMD simulations of LN:N at a temperature of 300 K. The structural snapshots of the LN:N crystal at times of 0 and 10 ps during AIMD simulation. |
In general, the formation energy of the point defect NO is lower than that of point defect Ni throughout the whole Fermi energy range. Therefore, the existence of NO is more plausible. Due to the limitation of the doping concentration, the concentration of the Ni point defect can be considered negligible. The transition levels ε(q1/q2) are defined as the points q1 and q2 where the formation energy and Fermi energy become equal.
![]() | (6) |
Clusters | The formation energy (eV per defect) |
---|---|
NbLi4+ + 4VLi− | 2.60 |
NbLi4+ + 3VLi− + 1NO− | 2.95 |
NbLi4+ + 2VLi− + 2NO− | 3.46 |
NbLi4+ + VLi− + 3NO− | 3.94 |
NbLi4+ + 4NO− | 4.35 |
The formation energy of the intrinsic defect cluster NbLi4+ + VLi− is 2.60 eV, remaining to be the most stable defect cluster compared with the defect clusters including the N point defects. With the increase of NO− and the decrease of VLi−, the formation energy becomes higher and higher, indicating a more unstable structure. The results show that it is difficult for N dopants to form a defect cluster with intrinsic defects, and N dopants cannot improve the situation of lithium deficiency.
Corresponding to the defect clusters above, the partial density of states (PDOSs) of the main single atomic states including O 2p, Nb 4d, and N 2p that can reflect the contributions of different atoms in electron density are shown in Fig. 6. Based on the PDOS, we can discriminate whether LN contains only intrinsic defects or also N point defects. The magnified area shows that the introduction of N atoms not only leads to the formation of the new energy level in the band gap, but also causes a strong interaction between N 2p and O 2p electrons. Most N 2p electrons and some O 2p electrons contribute to the defect energy level. With the increase in the number of N point defects, some 4d electrons of Nb ions take part in the formation of defect levels that get closer and closer to the bottom of the conduction band. Although the area of defect levels expands, there is not much overlap between these defect levels as O atoms. This may indicate a preference for isolated N point defects.
Based on the defect formation energies and PDOS analysis, we found that N point defects do not form so easily defect clusters with intrinsic defects or other N point defects. As we know, the formation of defect clusters has a close relationship with the concentration of N atoms, and the results provide an answer to the question why it is difficult to introduce N atoms into LN and why N dopants were experimentally observed to maintain at a relatively low concentration.
The new energy level displays an important role in improving the proprieties of LN. Seen from the PDOS, we can find that the contribution of N 2p electrons and O 2p electrons to the defect level of LN:N is almost the same. The interaction between N 2p and O 2p electrons is obvious. N ions influence the electronic distribution of the valence band, especially the electrons near the VBM, and the electrons of N enhance the activity of valence electrons. The existence of new energy levels is associated with the electronic transition in LN:N. The defect levels are approximately 0.39 eV above the VBM, which provides an opportunity for the O 2p electrons to transfer from the valence band with little energy which can easily be obtained from thermal activation. The result of the valence band electron transition leaves a large number of holes as the main carriers for LN:N. In addition, the occupation of defect energy levels has been explored. The occupation states of the valence band and the conduction band are 2 and 0, thus representing the full occupation state and the empty occupation state, respectively. In the band structure, we can clearly see that there are two energy lines. The occupation of the upper one changes from 0.27 to 1.95, and the other does not also have a fully occupied energy level either. Obviously, the holes in the energy level have a good chance to be thermally activated from the valence band.
Based on the analysis above, we infer that N dopants have a strong influence on the distribution of electrons in LN:N. Therefore, the electronic transformation of NO point defects has been studied. The charge density distributions of an O plane that include N atoms and the electronic charge difference49 between the LN:N and pristine system are given in Fig. 8.
For the NO point defect, N takes the responsibility of the O atom as an electron-withdrawing center. In a sense, NO guarantees the basic charge-transfer in crystals. Fig. 8(a) shows that there is an electron cloud gathering around NO, but it is smaller than the charge density of O atoms. Hence, compared with normal O sites, there is a clear depletion in the O site occupied by N. This is consistent with the conclusion we obtained above that the N point defect shows a −1 charge state. As shown in Fig. 8(b), the yellow ellipsoid around N ions presents the electron depletion compared to the original O site. While the yellow area is surrounded by a blue ellipsoid, it indicates aggregation of electrons between N and O atoms, which enables easy formation of covalent bonds.
In general, the charge density and the electronic charge difference prove the electronic interaction between N and O atoms and confirm that N plays a similar role to O with a negative charge state. Therefore, some of the O 2p electrons have the chance to transit from the valence band to the defect levels, leaving holes in the valence band as the main carriers.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c9cp05019a |
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