Theoretical studies on the form and effect of N-doping in an ZnGa2O4 photocatalyst

Pan Liab, Xian Zhaoc, Honggang Sun*a, Li Wanga, Bo Songd, Baoyu Gaoe and Weiliu Fan*c
aSchool of Mechanical, Electrical & Information Engineering, Shandong University, Weihai, 264209, China. E-mail: sunhg@sdu.edu.cn; Fax: +86-531-88364864; Tel: +86-531-88366330
bCollege of Physics and Information Engineering, Hebei Normal University, Shijiazhuang, 050024, China
cState Key Laboratory of Crystal Materials, Shandong University, Jinan, 250100, China
dMarine College, Shandong University, Weihai, 264209, China
eSchool of Environmental Science and Engineering, Shandong University, Jinan, 250100, China

Received 14th April 2016 , Accepted 1st August 2016

First published on 1st August 2016


Abstract

In the present work, hybrid density functional theory calculations were employed to analyze the electronic structures of ZnGa2O4 with different N impurity concentrations. The electronic transition energies in N-doped ZnGa2O4 with a molar ratio N/O of ∼3% were 3.35 and 1.43 eV for substituted and interstitial N-doping, respectively, which were much smaller than the value of 4.25 eV of pure ZnGa2O4. In 2N-doped ZnGa2O4 with a molar ratio N/O of ∼6%, three models with different N-doping sites (2Ns, 2Ni, and Ns + Ni) are analyzed. The calculated result indicated that the N impurity atoms preferred to form an N–N dimer rather than two apart N atoms in all three models. The electronic transition energies decreased by about 1.52, 0.91, and 2.51 eV for 2Ns-, 2Ni-, and Ns + Ni-doped ZnGa2O4, respectively, which mainly originated from the N–N π* states in the midgap. The half-filled impurity levels, which originated from the single electron of N-doping, were passivated due to the interaction of the two impurity atoms. The defect formation energies indicated that the oxygen vacancy would promote the introduction of a nitrogen impurity. Urea was recommended as a nitrogen source to easily achieve 2Ns-doping forms. Based on the present calculations, 2Ns-doped ZnGa2O4 was considered as the better photocatalyst due to a smaller band gap for visible light response and a suitable redox couple for overall water splitting. Our work provided a theoretical explanation for the origin of the enhanced visible light photocatalytic activity of N-doped ZnGa2O4.


1. Introduction

One of the promising ways to solve energy and environmental issues is to utilize photocatalytic technology to split water to give H2 and degrade organic pollutants with solar energy. Since Inoue et al. first presented studies about p-block metal oxides of MIn2O4, M2SnO4 and M2Sb2O7 (M = Ca, Sr), demonstrating them as good photocatalysts for water decomposition under UV light,1 semiconductors with a d10 electronic configuration (In3+, Ga3+, Ge4+, and Sn4+ etc.) have been considered as good photocatalysts and showed promising applications.2–8 Among the p-block metal oxide photocatalysts studied, cubic spinel ZnGa2O4 is also a good photocatalyst for water splitting,9–15 organic pollutant degradation,16–21 and CO2 reduction.22–25 However, pure ZnGa2O4 still has a low solar energy utilization due to its wide band gap of about 4.1–4.5 eV.11,14,15 Therefore, broadening the light absorption of the ZnGa2O4 photocatalyst by tuning the band gap energy has become one study aspect.

To reduce the large band gap, some transition metals (TM) have been introduced in ZnGa2O4. Zhang's group synthesized Zn1−xCdxGa2O4 solid solution photocatalysts with better UV light activity for the methylene blue degradation, which exhibited the band gaps between 4.8 and 3.6 eV by different Cd components.26 Xu et al. narrowed the band gaps of ZnGa2O4 from 4.7 to 3.1 eV by introducing Cr to substitute Ga ions (ZnGa2−xCrxO4), presenting a better photocatalytic H2 production activity.27 Irie et al. demonstrated that Rh-doped ZnGa2O4 with a good visible light activity for water splitting had a 600 nm light adsorption onset due to the impurity states in the midgap.28 However, TM-doped materials have some disadvantages for efficient photocatalytic reactions, such as rapid electron–hole recombination and thermal instability. To solve these questions, nonmetal doping gives some promising advantages. Hereinto, the N-doped semiconductor photocatalysts, which displays favorable visible light activity, are the most widely investigated.29–34 N-Doped spinel ZnGa2O4 photocatalysts prepared by Parida et al. through solid–solid reaction method based on different N-precursors, which gave the band gap energy of minimal 2.6 eV.35 Lobo et al. also achieved N-doped ZnGa2O4 photocatalysts by combining sol–gel and nitridation steps, presenting the band gap energy of minimal 2.4 eV.9,15 Interestingly, in Parida's work, a significant band gap change from 3.0 to 2.6 eV was observed corresponding to the nitrogen content change from 0.04% to 0.15%. However, N-doped ZnGa2O4 prepared by nitridation steps gives a slight band gap variation from 2.47 to 2.40 eV when the nitrogen content increases from 0.58% to 2.85%. The result suggests that the different nitrogen sources and contents will influence the effect of N-doping on the band structure of ZnGa2O4. Although the effect of N-doping in the semiconductor photocatalyst was discussed by previous experimental and theoretical work, the form of N-doping and the origin of the improved visible light adsorption were still in debate. For example, the form of N-doping in TiO2 was speculated to be substituted, interstitial, NOx or NHx depending on experimental conditions.30–38 Experiments and theoretical calculations also noted that the forms of N-doping were connected with synthesis conditions.34,39 Lobo's work noted that the band gap narrowing of N-doped ZnGa2O4 should be contributed to the mixing states of N 2p and O 2p above the valence band, inducing by the substituted N-doping. However, Batzill's work and Li's work illustrated the p orbital energy of N was close to that of O, which induced less band gap narrowing.40,41 The fact suggests that the large band gap narrowing of about 2.0 eV of N-doped spinel ZnGa2O4 is still complicated and unclear. Therefore, further studies are necessary to reveal the origin of the experimentally observed large red shift.

Previously, many photocatalysts were prepared and studied with considerable photocatalytic activity. However, the number of visible-light-sensitive photocatalysts with overall water splitting ability is limited due to the strict demand of the band relative positions. That is the conduction band minimum (CBM) must be higher than the hydrogen producing potential and the valence band maximum (VBM) must be lower than the water oxidation potential. Therefore, a great deal of effort has been spent on finding semiconductors with suitable band structures. The potentials of VBM and CBM of ZnGa2O4 are ca. 3.0 and −1.2 V (vs. SHE), respectively, which indicates the ZnGa2O4 has a suitable redox couple for overall water splitting.42 Although some transition metals (TM) and nonmetals have been introduced into ZnGa2O4 to reduce the large band gap of 4.2 eV to response visible light, the influence of impurities on the VBM and CBM relative positions is unclear. Generally, the TM-doping introduces some d impurity states in the gap of semiconductor photocatalysts. Although the d states narrowed the original bandgap and simultaneously retains the potential, others depressed the CBM to suppress the reduction potential for H2 production. The redox ability of photogenerated electron–hole pairs decreases as Cd concentration increases in Zn1−xCdxGa2O4 due to the CB and VB shift to Fermi level.26 Irie's work demonstrates that the introduction of Rh-doping in a regular octahedral coordination (Ga sites) creates fully occupied t62g and empty e0g midgap states due to ligand-field splitting of the octahedrally coordinated Rh3+, and these midgap states had suitable potentials to produce hydrogen/oxygen under visible-light irradiation.28 The nonmetal-doping, such as N, and C introduces p impurity states in the gap of semiconductor photocatalysts. N-Doping induces the VB contraction and stronger oxidation potential in rutile TiO2 and a slight VB extension in anatase TiO2.43 The carbon self-doping in g-C3N4 could shift the potentials of both valence and conduction bands positively, which would increase the photooxidation ability and reduce the photoreduction ability.44 These previous studies indicate that the doping in ZnGa2O4 requires careful design for the visible-light sensitive photocatalyst toward overall water splitting.

Theoretical calculations based on local density functional theory (DFT) are considered as a benefit tool to analyze the properties of semiconductors. However, although the structural parameters are agreement with experiments, the band gaps are severely underestimated by the DFT calculations.45 The band gaps of ZnGa2O4 calculated by local density approximation (LDA) and generalized gradient approximation (GGA) are about 2.6–2.8 eV,46,47 which are much less than the experimental value. Some methods, such as GW, LDA + U, hybrid and screened functionals, were developed and used to correct the gap underestimated problem. The GW approximation48 based on the many-body perturbation theory is to date the top method for calculating quasiparticle band structures. Dixit's work gives the band gap of about 4.6 eV of ZnGa2O4 using the GW approximation, which is in good agreement with experiments.49 However, although the GW approximation shows methodological advances, DFT is still widely used for investigating electronic structure features due to much more computationally demanding by the GW calculations. The LDA + U method,50–53 which includes the on-site Coulomb interaction in the Hamiltonian, has been used to descript the effect of the d-electrons. The band gap of ZnGa2O4 calculated by the LDA + U method was about 3.1 eV,46 which slightly suppressed the error of the LDA calculation. However, the underestimate of band gap is still severe in the LDA + U calculations. Hybrid and screened functionals, which mix a fraction of nonlocal potentials such as Hartree–Fock (HF) exchange potentials or screened nonlocal exchange potentials within Kohn–Sham type approaches, go beyond the local and semi-local approximations of DFT.54 A new class of calculations based on hybrid and screened functionals have been reported to give good band gaps in semiconductors.55,56 These researches suggest that the combination of local DFT and nonlocal functionals will be favorable for accurately calculating the band structure of ZnGa2O4 and its changes induced by N-doping.

In the present paper, theoretical calculations with different local, nonlocal, screened exchange and hybrid functionals are implemented to achieve the accurate band structure of cubic spinel ZnGa2O4. Based on the calculated results, the Perdew–Burke–Ernzerhof (PBE0) hybrid functional is employed to obtain microscopic insight into the effect of N-doping on the electronic properties of ZnGa2O4 correlated with N impurity forms and content. The results provide a solid basis for the rationalization of the experimentally observed red shift and the changes of the VB and CB potentials as a result of N-doping in ZnGa2O4.

2. Computational details and structural aspects

DFT calculations supplied the accurate description of the total energy and equilibrium structure of the crystals. Therefore, to achieve the equilibrium structure of the cubic spinel ZnGa2O4 (56 atoms), the exchange and correlation interactions were dealt with the GGA-PBE functional.57 The norm conserving pseudo-potential was used to deal with the core electrons and the valence atomic configurations were 3d104s2 for Zn, 3d104s24p1 for Ga, 2s22p4 for O, and 2s22p3 for N. The plane wave cut off was set to 800 eV. The k mesh of 4 × 4 × 4 achieved by the Monkhorst–Pack scheme58 was used to achieve accurate structural parameters. The convergence tests of the plane wave cut off and the k points were given in Fig. S1 of the ESI. In the geometrical optimization, all forces on atoms were converged to less than 0.03 eV Å−1, the maximum ionic displacement was within 0.001 Å and the total stress tensor was reduced to the order of 0.05 GPa. The optimized lattice parameters were a = b = c = 8.567 Å, which were in good agreement with the experimental and the other theoretical values.59–62 all calculations were performed using Cambridge Sequential Total Energy Package (CASTEP).

The N-doped models were constructed based on the fully relaxed pure ZnGa2O4. For the substitutional N-doped model, one oxygen atom in the ZnGa2O4 crystal structure was replaced by one nitrogen atom labeled as Ns. For the interstitial N-doped model, one nitrogen atom was set at the interstitial sites of the ZnGa2O4 crystal lattice labeled as Ni. For the higher N impurity concentration, two nitrogen atoms were introduced in the lattice labeled as 2Ns, 2Ni, and Ns + Ni. Different doping positions of two nitrogen atoms were tested, and the relative stability of the doped models was studied to find the most stable structure according to N–N distance. All the electronic structures were calculated on the corresponding optimized models. The local, nonlocal, screened and hybrid functionals are implemented to calculate the band structures of the pure ZnGa2O4 as shown in Fig. S2. The calculated results suggest that the hybrid PBE0 functional63 will be favorable for analyzing the changes of the electronic structures of ZnGa2O4 induced by N-doping.

To examine the thermodynamic stability of the different N-doped models, the formation energies (Ef) were calculated according to the following equation,64–67

Ef = Et(Doping) + nOμOEt(Pure) − nNμN,
where Et(Doping) was the total energy of the structures with the N impurity, and Et(Pure) was the total energy of the ideal cell. nO was the number of O atom being removed from the cell, and nN was the number of N impurity introduced into the lattice. μO and μN were the chemical potentials of N and O, respectively. In the present work, μO was fixed at the energy of half an O2, while μN was calculated based on the different nitrogen sources.

3. Results and discussion

3.1 Ns- and Ni-doped ZnGa2O4

A. Geometrical structures. Cubic spinel ZnGa2O4 has a closed packed face-centered-cubic structure with space group Fd[3 with combining macron]m, in which the Zn atoms are located at tetrahedral sites with the Wyckoff positions 8a (1/8, 1/8, 1/8), while Ga atoms are located at octahedral sites with the 16d (1/2, 1/2, 1/2) and the O atoms at 32e (u, u, u). The lengths of the O–Ga bonds and the O–Zn bonds are 2.030 Å and 2.060 Å, respectively. For the Ns structure as shown in Fig. 1b, the lengths of the optimized Ns–Ga and Ns–Zn bonds are 2.019 and 1.956 Å, respectively, which are slightly shorter than the original O–Ga and O–Zn bonds in the pure ZnGa2O4. For the Ni structure as shown in Fig. 1c, the Ni-doping induces a large local lattice distortion after full structural relaxation. The lattice O atom is pushed away from the original position by the Ni atom, forming a new N–O bond with bond length of about 1.368 Å.
image file: c6ra09655g-f1.tif
Fig. 1 The geometrical structures and electron density of (a) pure, (b) Ns-doped, and (c) Ni-doped ZnGa2O4. The unit of the electron density labeled in the table is e Å−3.

To study the variation of chemical bonding induced by the N-doping for ZnGa2O4, we calculate the total electron density and Mulliken charge population (as shown in Table 1) for the Ns and Ni models. For the pure ZnGa2O4, Fig. 1a shows that the O ions connect with adjacent Ga ions through a common electron cloud, presenting covalent O–Ga bonds. For the Ns-doped ZnGa2O4, Fig. 1b shows more electron cloud between Ns ion and Ga cations (0.672 e Å−3) than that between O ions and Ga cations (0.609 e Å−3), which is consistent with the shorter Ns–Ga and Ns–Zn bonds after geometrical optimization. The charges of −0.87 |e| on the Ns ion are close to −0.84 |e| on the original O ions. The result suggests that N2− ion is localized in the lattice, which will introduce one acceptor level in the ZnGa2O4. For the Ni-doped ZnGa2O4, Fig. 1c shows a covalent interaction between the Ni ion and the adjacent O ion. The charges on the Ni ion and the O ion are −0.48 |e| and −0.50 |e|, respectively. The total charges of −0.98e on the NO species suggests that the NO2− species exist in the lattice.

Table 1 The bond lengths and Mulliken charge populations for pure, Ns-, Ni-, 2Ns-, 2Ni-, Ns + Ni-, and 2Ns + VO-doped ZnGa2O4
Models Bond lengths (Å) Charges (|e|)
O/N–Ga O/N–Zn N–O N–N Ga Zn O N
Pure 2.030 2.060     1.20 0.97 −0.84  
Ns 2.019 1.956     1.21 0.96 −0.84 −0.91
Ni 1.960 1.951 1.368   1.22 0.96 −0.50 −0.48
2Ns 1.994 1.950   1.696 1.20 0.93 −0.84 −0.77
1.987 1.945 −0.77
2Ni   2.084 1.797 1.176 1.22 0.93 −0.75 −0.21
2.014 −0.13
Ns + Ni 1.971 2.160   1.284 1.20 0.97 −0.84 −0.46
1.975 2.131 −0.46
2Ns + VO 1.918/1.945/1.988 1.929     1.21 0.95 −0.84 −1.00
1.932/1.962/1.978 1.996


B. Electronic structures. Fig. 2 gives the band structures, the total density of states (TDOS), and the project density of states (PDOS) of pure, Ns-, and Ni-doped ZnGa2O4. For the pure ZnGa2O4, the calculated band gap is about 4.25 eV using hybrid PBE0 functional, which is in good agreement with the experimental 4.1–4.5 eV.11,14,15 The valance band maximum (VBM) of the pure phase are predominantly contributed by the O 2p states. The conduction band minimum (CBM) basically originates from the Ga 4s states with small O 2p states. The result indicates that the p–s electronic transition is responsible for the optical absorption onset of the pure ZnGa2O4. In the present work, the energy of the VBM of pure ZnGa2O4 is set as the reference (zero energy) to study the changes of the redox ability of N- and 2N-doped models. The redox potentials of water splitting are labeled in all band structures (3.05 eV for H2/H2O and 1.82 eV for H2O/O2).
image file: c6ra09655g-f2.tif
Fig. 2 The band structures, and density of states of (a) pure, (b) Ns-doped, and (c) Ni-doped ZnGa2O4. The dash line presents the Fermi level.

For the Ns-doped ZnGa2O4, as shown in Fig. 2b, the electronic transition energy decreases to about 3.35 eV due to three impurity levels localized at the VBM. The host band gap of 4.35 eV from the host VBM to CBM is slightly larger than 4.25 eV of the pure ZnGa2O4. We contribute the larger band gap to a reduction of the Coulomb repulsion and a contraction of the band, resulting from the removal of one electron when one N atom replaces one O atom in the cell. The PDOS shows that the impurity levels are mainly contributed by the mixing states of N 2p states with little O 2p states. It is clear that the substituted N-doping improve the solar energy utilization of ZnGa2O4 through some continuous states above the VBM, and Ns-doped ZnGa2O4 still shows overall water splitting ability. However, the narrowing of the electronic transition energy is still not enough to response the visible light, which demands the energy of less than 2.8 eV.

For the Ni-doped ZnGa2O4, Fig. 2c shows two isolated impurity levels in the gap. The theoretical gap from the host VBM to the CBM has a slight increasing of about 0.18 eV, which is contributed to the p–p repulsion of the Ni-doping and the VBM. However, the electron excited energy from the top impurity level to the CBM is about 1.43 eV, which is much smaller than 4.25 eV of pure phase. The PDOS indicates that the two midgap levels are mainly originated from the mixing states of N 2p states and O 2p states. The further highest occupied molecular orbital (HOMO) analysis as shown in Fig. 3c shows a remarkable NO π-antibonding character. Therefore, we conclude that the electronic excitations from the NO π* states are one of the reasons of the visible light response in Ni-doped ZnGa2O4. Importantly, the calculated band structure indicates that the overall water splitting ability of ZnGa2O4 has been break due to the deep impurity levels. In addition, the calculated band structures of Ns- and Ni-doped ZnGa2O4 show the top impurity level crossing the Fermi level presents half occupied characteristic, which is agreement with the charge population analysis. However, the partially occupied impurity states go against the photocatalytic activity of semiconductors because these states can act as recombination centers to suppress the photogenerated current and reduce the UV light activity. Thus, the passivated approach is desired to compensate the half occupied impurity states.


image file: c6ra09655g-f3.tif
Fig. 3 The highest occupied molecular orbital (HOMO) of (a) pure, (b) Ns-doped, and (c) Ni-doped ZnGa2O4.

3.2 2Ns-, 2Ni- and Ns + Ni-doped ZnGa2O4

A. Geometrical structures. To achieve the most stable configuration of 2Ns-, 2Ni- and Ns + Ni-doped ZnGa2O4, the different lattice sites are tested for the two N-doping atoms. The relative energies of these models are calculated and shown in Fig. S3–S5. As shown in Fig. 4, all the most stable configurations of the three 2N-doped ZnGa2O4 give a N2 dimer structure formed by the two adjacent N-doping atoms. This result is agreement with the theoretical work of 2N-doped TiO2 and MgTa2O6.39,68 For the 2Ns-doped ZnGa2O4, the two Ns atoms attract each other, which induces one initial N–Ga bond disappearing and forms one Ns–Ns bond with bond length of 1.696 Å. The bonds between Ns-doping ions and adjacent Ga ions are 1.994 and 1.987 Å, which are slightly shorter than that in pure ZnGa2O4. For the 2Ni-doped ZnGa2O4, the two Ni atoms are also bounded together with the bond length of about 1.176 Å, and a large local distortion of lattice is induced by the 2Ni-doping. Meanwhile, the Ni–Ni dimer together with one lattice O atoms forms –Ni–Ni–O– structure, which gives N–O bond length of 1.797 Å. For the Ns + Ni-doped ZnGa2O4, the Ni atom pushes the Ns atom away from the original lattice site to form a new –N2– structure with the Ns–Ni bond length of 1.284 Å. These calculated results note that the N2 dimer is common in N-doped ZnGa2O4, especially for higher nitrogen impurity content.
image file: c6ra09655g-f4.tif
Fig. 4 The geometrical structures and electron density of (a) 2Ns-doped, (b) 2Ni-doped, and (c) Ns + Ni-doped ZnGa2O4. The unit of the electron density labeled in the table is e Å−3.

Fig. 4 shows that the two N-doping ions are bounded together by a common electron cloud, presenting a strong covalent-like characteristic. For 2Ns-doped ZnGa2O4, more electrons are shared by Ns-doping and Ga ions (more than 0.672 e Å−3), which give stronger Ns–Ga covalent bonds. The interaction of the two Ns ions reduces the charges on each Ns ion to −0.77 |e|. For 2Ni-doped ZnGa2O4, the total electron density map indicates that the Ni–O bonds are much weaker than that in Ni-doped ZnGa2O4. This result is consistent with the smaller total charges of −0.34 |e| on the two interstitial N ions, which is contributed to the interaction of the two Ni ions. For Ns + Ni-doped ZnGa2O4, the effect of the N2 dimer is similar to the original O ions. However, the two N–Ga bonds present stronger covalent-like characteristic by capturing more electrons (−0.92 |e|). The present results give strong interaction between the two N-doping for the three 2N-doped models, which will significantly affect the electronic structures of ZnGa2O4.

B. Electronic structures. Fig. 5a for 2Ns-doped ZnGa2O4 shows that two isolated impurity levels localize in the gap, and the other two impurity levels are above the VBM. The electronic transition energy from the highest occupied level to the CBM is about 2.73 eV. The host band gap is about 4.45 eV from the host VBM to CBM. The increase of about 0.20 eV of band gap in 2Ns-doped ZnGa2O4 is larger than that in Ns-doped ZnGa2O4. This phenomenon is contributed to the more reduction of the Coulomb repulsion and the more contraction of the valence band due to the more electronic losing of the two Ns-doping atoms. In addition, the band structure shows that 2Ns-doped ZnGa2O4 still keeps overall water splitting ability. The DOS and PDOS indicate that the two isolated impurity levels are mainly contributed to the N 2p states with a little O 2p states, while the other two impurity levels are dominated by the O 2p states mixing with a little N 2p states. The further HOMO analysis (see Fig. 6a) gives the frontier orbital level of 2Ns-doped ZnGa2O4, presenting a remarkable Ns–Ns π-antibonding character. Especially, no half-filled levels are observed in 2Ns-doped ZnGa2O4, which is contributed to the interaction of the two N-doping. Based on the calculated results, we conclude that the midgap states originated from the N–N π* states are favorable for improving the visible light absorption of ZnGa2O4 and are one of reasons for the observed red shift of the absorption edge in experiments.
image file: c6ra09655g-f5.tif
Fig. 5 The band structures and density of states of (a) 2Ns-doped, (b) 2Ni-doped, and (c) Ns + Ni-doped ZnGa2O4. The dash line presents the Fermi level.

image file: c6ra09655g-f6.tif
Fig. 6 The highest occupied molecular orbital (HOMO) of (a) 2Ns-doped, (b) 2Ni-doped, and (c) Ns + Ni-doped ZnGa2O4.

Fig. 5b gives the band structure of 2Ni-doped ZnGa2O4. Only one isolated level localizes in the gap, which induces the electronic transition energy decrease to 3.34 eV. The host band gap has a slight change of about 0.08 eV, and there are no half-filled levels in the band. The calculated band structure shows a significant difference compared with that of Ni-doped ZnGa2O4, in which two isolated levels, smaller electronic transition energy of 1.43 eV and larger host band gap increasing of 0.18 eV are observed. The DOS and PDOS of 2Ni-doped ZnGa2O4 show that the midgap level is mainly contributed by O 2p states with little N 2p states. The HOMO analysis as shown in Fig. 6b gives an –Ni–Ni–O– mixing characteristic, which consists of Ni–Ni π* and Ni–O σ orbitals. Importantly, some N 2p states localize above the Ga 4s states of the CBM mixing with empty states. Based on the calculated results and combined with charge analysis, we conclude that the unpaired electrons of the Ni-doping are paired, which induce one empty anti-bond molecular orbital moving up and the other occupied anti-bond molecular orbital moving down. The up orbital results in the weakening of the p–p repulsion between the midgap states and the VBM. Thus the broadening of the host band gap is smaller than that in Ni-doped ZnGa2O4. The down orbital increases the electronic transition energy of about 1.91 eV from the impurity states to CBM compared with that in Ni-doped ZnGa2O4. Therefore, although the Ni–Ni impurity induces the electronic transition energy decreasing than pure phase, the interaction of two Ni-doping atoms goes against the further improving of the visible light response of N-doped ZnGa2O4.

The band structure of Ns + Ni-doped ZnGa2O4 as shown in Fig. 5c gives the host band gap of 4.46 eV and no half-filled level localizes in the band structure. One isolated level localizes in the gap, and the electronic transition energy from the level to CBM is 1.74 eV, which is much smaller than 4.25, 3.35, 3.34, and 2.73 eV of pure, Ns-, 2Ni-, and 2Ns-doped ZnGa2O4, and just larger than 1.43 eV of Ni-doped ZnGa2O4. The DOS and PDOS show the N 2p states are responsible for the midgap level. The HOMO analysis presents a remarkable Ns–Ni π anti-bonding character. Therefore, the electronic transition of π*–s is one of reasons that inducing visible light absorption in experiments. The character is agreement with that in 2Ns-doped ZnGa2O4, while is different to that in 2Ni-doped ZnGa2O4. In addition, there are some N 2p impurity states localizing above the Ga 4s states of the CBM. Obviously, this character is similar to that in 2Ni-doped ZnGa2O4, which originates from the charge compensation of the two N-doping. Although the charge compensation may lower the impurity levels to broaden the electronic transition energy as discussed above, two effects play a positive role to narrow the energy in Ns + Ni-doped ZnGa2O4. One is that the Ni-doping introduces more electrons resulting in a strong p–p repulsion of the impurity states and valence bands, the other is that the mixing of the N 2p states and conduction bands as shown in Fig. 5c lowers the CBM. Therefore, based on the calculated results, we conclude that the Ns + Ni-doping units the advantages of substituted and interstitial N-doping, which is favorable for improving the solar energy utilization of ZnGa2O4. However, the redox potentials of the impurity levels indicate that Ns + Ni-doped ZnGa2O4 has no O2 producing ability.

3.3 2Ns + VO-doped ZnGa2O4

In consideration of the fact that the oxygen vacancy (VO) is common in oxide semiconductors, the synergetic effect of N impurity and VO on the geometrical and the electronic structures are calculated and analyzed. The VO will attract the interstitial N impurity to form the substituted N-doping after structural relaxation. Thus, only 2Ns + VO-doped model is considered in the present work. Fig. 7a shows the optimized structure of 2Ns + VO-doped ZnGa2O4, which gives the shortest two N–Ga bonds with 1.918 and 1.932 Å in N-doped models. The result indicates the oxygen vacancy strengths the interaction between N-doping and adjacent cations. The electron density map as shown in Fig. 7b shows that more electrons are common in cloud than that in pure phase and also that in Ns-doped model. Mulliken population listed in Table 2 gives the charges of −1.00 |e| on each N ion, showing more electrons transferring from adjacent cations compared with −0.84 |e| of O ion and −0.91 |e| of Ns ion in Ns-doped ZnGa2O4. Therefore, we conclude that the oxygen vacancy induces the N3− ions formation in the lattice of 2Ns + VO-doped ZnGa2O4 due to the electron transferring between VO donor and Ns acceptor.
image file: c6ra09655g-f7.tif
Fig. 7 (a) The geometrical structure, (b) the electron density, and (c and d) the electronic structures of 2Ns + VO-doped ZnGa2O4. The unit of the electron density labeled in the table is e Å−3. The dash line presents the Fermi level.
Table 2 The electronic transition energies (Etr) and the defect formation energies (Ef) based on the different nitrogen sources of the different N-doped models
Models Etr (eV) Ef (eV)
N2 NH3 N2H4 Urea Hexamine
Pure 4.25          
Ns 3.35 5.28 3.83 4.84 2.47 4.43
Ni 1.43 5.12 3.67 4.68 2.41 4.27
2Ni 2.73 6.80 3.90 5.93 1.39 5.10
2Ns 3.34 9.62 6.62 8.75 4.21 7.92
Ns + Ni 1.74 7.17 4.27 6.30 1.76 5.47
2Ns + VO 3.38 3.25 0.35 2.38 −2.16 1.55


The oxygen vacancy has a significant effect on the band structure of N-doped ZnGa2O4. As shown in Fig. 7c, some impurity levels form a continuous impurity band and extend the width of about 0.8 eV of the VB. The band gap decreases to 3.38 eV and the half-filled level induced by Ns-doping disappears. Obviously, the electron transferring between oxygen vacancy and Ns-doping will be favor of improving the photocatalytic activity. Fig. 7d shows the impurity levels are mainly contributed by the mixing states of N 2p states and O 2p states. The energy of the mixing states is lower, which suggests stronger oxidizing ability of than that in Ns-doped model VB. In addition, the calculated band structure indicates that 2Ns + VO-doped ZnGa2O4 still keep the overall water splitting ability.

3.4 Formation energy

The defect formation energies of N-doped ZnGa2O4 are listed in Table 2. It is clear that the nitrogen impurity atoms are inclined to enter into the interstitial sites in the lattice of ZnGa2O4. This should be contributed to the large interspace of the spinel lattice and the strong interaction between the interstitial N and the lattice O. The Ns-doping is also possible because the Ef of 5.28, 3.83, 4.84, 2.47, and 4.43 eV is close to 5.12, 3.67, 4.68, 2.41, and 4.27 eV of Ni-doping under the different nitrogen sources. The result is agreement with the analysis of N-doped TiO2, which gives the interstitial N first and the substituted N following.34 The formation energies of the 2Ns + VO-doped ZnGa2O4 are much smaller than that of other 2N-doped models. The result indicates the oxygen vacancy will promote the introduction of nitrogen impurity. In most cases, the formations of 2Ns-, 2Ni-, and Ns + Ni-doping are difficult than that of Ns-, and Ni-doping. However, using urea as nitrogen source, the calculated formation energies of 1.39, 2.21, and 1.76 eV for 2Ni-, 2Ns-, and Ns + Ni-doping are smaller than the formation energies of Ns- and Ni-doping, which indicate the N–N dimer could be preferentially formed in a suitable environment. The above calculated electronic structures with the different N-doping forms suggest that the 2Ns-doped ZnGa2O4 has a smaller band gap for absorbing visible light and a suitable redox couple for overall water splitting. Therefore, urea is recommended as nitrogen source to easily achieve the 2Ns-doping from the view of thermodynamics.

4. Conclusions

The geometrical structures and electronic structures of N-doped and 2N-doped ZnGa2O4 are discussed based on the PBE0 calculations. The present work notes that the interstitial N impurity is prior on thermodynamics and induces a larger decrease of the electronic transition energies in N-doped ZnGa2O4 due to the midgap NO π* states. In 2N-doped ZnGa2O4, the two N impurity atoms form N2 dimer structure in the lattice, and the electronic transition energy has a significant decrease, which is contributed to the N–N π* states in the midgap. The oxygen vacancy will promote the introduction of 2Ns-doping in the lattice of ZnGa2O4. Our work provides a theoretical analysis for the visible light photocatalytic activity induced by nitrogen impurity in ZnGa2O4 photocatalyst.

Acknowledgements

This work is supported by the National Natural Science Foundation of China (Grant No. 51402169 and 51502076), the Natural Science Foundation of Shandong Province, China (Grant No. 51402169), and the China Postdoctoral Science Foundation (Grant No. 2013M530322). The numerical calculations in this paper have been done on the supercomputing system in the Supercomputing Center, Shandong University, Weihai.

References

  1. (a) J. Sato, N. Saito, H. Nishiyama and Y. Inoue, J. Phys. Chem., 2001, 105, 6061 CrossRef CAS; (b) J. Sato, N. Saito, H. Nishiyama and Y. Inoue, Chem. Lett., 2001, 9, 868 CrossRef; (c) J. Sato, N. Saito, H. Nishiyama and Y. Inoue, J. Photochem. Photobiol., A, 2002, 148, 85 CrossRef CAS; (d) K. Ikarashi, J. Sato, H. Kobayashi, H. Nishiyama and Y. Inoue, J. Phys. Chem. B, 2002, 106, 9048 CrossRef CAS.
  2. (a) K. R. Reyes-Gil, E. A. Reyes-García and D. Raftery, J. Phys. Chem. C, 2007, 111, 14579 CrossRef CAS; (b) K. R. Reyes-Gil, Y. Sun, E. A. Reyes-García and D. Raftery, J. Phys. Chem. C, 2009, 113, 12558 CrossRef CAS.
  3. Y. D. Hou, X. C. Wang, L. Wu, Z. X. Ding and X. Z. Fu, Environ. Sci. Technol., 2006, 40, 5799 CrossRef CAS PubMed.
  4. (a) Q. Liu, Y. Zhou, J. H. Kou, X. Y. Chen, Z. P. Tian, J. Gao, S. C. Yan and Z. G. Zou, J. Am. Chem. Soc., 2010, 132, 14385 CrossRef CAS PubMed; (b) S. C. Yan, L. J. Wan, Z. S. Li and Z. G. Zou, Chem. Commun., 2011, 47, 5632 RSC.
  5. K. Maeda, T. Takata, M. Hara, N. Saito, Y. Inoue, H. Kobayashi and K. Domen, J. Am. Chem. Soc., 2005, 127, 8286 CrossRef CAS PubMed.
  6. J. Sato, N. Saito, Y. Yamada, K. Maeda, T. Takata, J. N. Kondo, M. Hara, H. Kobayashi, K. Domen and Y. Inoue, J. Am. Chem. Soc., 2005, 127, 4150 CrossRef CAS PubMed.
  7. K. Teramura, D. Lu, T. Takata, N. Saito, Y. Inoue and K. Domen, Nature, 2006, 440, 295 CrossRef PubMed.
  8. K. Maeda and K. Domen, Chem. Mater., 2010, 22, 612 CrossRef CAS.
  9. V. B. R. Boppana, D. J. Doren and R. F. Lobo, ChemSusChem, 2010, 3, 814 CrossRef CAS PubMed.
  10. K. M. Parida, S. Martha, D. P. Das and N. Biswal, J. Mater. Chem., 2010, 20, 7144 RSC.
  11. X. Chen, H. Xue, Z. H. Li, L. Wu, X. X. Wang and X. Z. Fu, J. Phys. Chem. C, 2008, 112, 20393 CAS.
  12. X. N. Zhang, J. H. Huang, K. N. Ding, Y. D. Hou, X. C. Wang and X. Z. Fu, Environ. Sci. Technol., 2009, 43, 5947 CrossRef CAS PubMed.
  13. W. W. Zhang, J. Y. Zhang, X. Lan, Z. Y. Chen and T. M. Wang, Catal. Commun., 2010, 11, 1104 CrossRef CAS.
  14. N. Kumagai, L. Ni and H. Irie, Chem. Commun., 2011, 47, 1884 RSC.
  15. V. B. R. Boppana, D. J. Doren and R. F. Lobo, J. Mater. Chem., 2010, 20, 9787 RSC.
  16. X. Zhang, J. Huang, K. Ding, Y. Hou, X. Wang and X. Fu, Environ. Sci. Technol., 2009, 43, 5947 CrossRef CAS PubMed.
  17. X. Chen, H. Xue, Z. Li, L. Wu, X. Wang and X. Fu, J. Phys. Chem. C, 2008, 112, 20393 CAS.
  18. M. Sun, D. Li, W. Zhang, Z. Chen, H. Huang, W. Li, Y. He and X. Fu, J. Solid State Chem., 2012, 190, 135 CrossRef CAS.
  19. V. B. R. Boppana and R. F. Lobo, ACS Catal., 2011, 1, 923 CrossRef CAS.
  20. X. Li, X. Zhang, X. Zheng, Y. Shao, M. He, P. Wang, X. Fu and D. Li, J. Mater. Chem. A, 2014, 2, 15796 CAS.
  21. Z. Li, B. Li, Z. Liu, D. Li, C. Ge and Y. Fang, RSC Adv., 2014, 4, 48590 RSC.
  22. Z. Wang, K. Teramura, S. Hosokawa and T. Tanaka, J. Mater. Chem. A, 2015, 3, 11313 CAS.
  23. S. C. Yan, S. X. Ouyang, J. Gao, M. Yang, J. Y. Feng, X. X. Fan, L. J. Wan, Z. S. Li, J. H. Ye, Y. Zhou and Z. G. Zou, Angew. Chem., 2010, 122, 6544 CrossRef.
  24. Q. Liu, D. Wu, Y. Zhou, H. Su, R. Wang, C. Zhang, S. Yan, M. Xiao and Z. Zou, ACS Appl. Mater. Interfaces, 2014, 6, 2356 CAS.
  25. S. Yan, J. Wang, H. Gao, N. Wang, H. Yu, Z. Li, Y. Zhou and Z. Zou, Adv. Funct. Mater., 2013, 23, 1839 CrossRef CAS.
  26. W. Zhang, J. Zhang, X. Lan, Z. Chen and T. Wang, Catal. Commun., 2010, 11, 1104 CrossRef CAS.
  27. X. Xu, Y. Xie, S. Ni, A. K. Azad and T. Cao, J. Solid State Chem., 2015, 230, 95 CrossRef CAS.
  28. N. Kumagai, L. Ni and H. Irie, Chem. Commun., 2011, 47, 1884 RSC.
  29. S. Livraghi, M. C. Paganini, E. Giamello, A. Selloni, C. Di Valentin and G. Pacchioni, J. Am. Chem. Soc., 2006, 128, 15666 CrossRef CAS PubMed.
  30. R. Asahi, T. Morikawa, T. Ohwaki, K. Aoki and Y. Taga, Science, 2001, 293, 269 CrossRef CAS PubMed.
  31. C. Di Valentina, E. Finazzia, G. Pacchionia, A. Sellonib, S. Livraghic, M. C. Paganinic and E. Giamelloc, Chem. Phys., 2007, 339, 44 CrossRef.
  32. J. Fang, F. Wang, K. Qian, H. Bao, Z. Jiang and W. Huang, J. Phys. Chem. C, 2008, 112, 18150 CAS.
  33. R. Katoh, A. Furube, K. Yamanaka and T. Morikawa, J. Phys. Chem. Lett., 2010, 1, 3261 CrossRef CAS.
  34. J. Wang, D. N. Tafen, J. P. Lewis, Z. Hong, A. Manivannan, M. Zhi, M. Li and N. Wu, J. Am. Chem. Soc., 2009, 131, 12290 CrossRef CAS PubMed.
  35. K. M. Parida, S. Martha, D. P. Das and N. Biswal, J. Mater. Chem., 2010, 20, 7144 RSC.
  36. H. Irie, Y. Watanabe and K. Hashimoto, J. Phys. Chem. B, 2003, 107, 5483 CrossRef CAS.
  37. K. S. Yang, Y. Dai and B. B. Huang, J. Phys. Chem. C, 2007, 111, 18985 CAS.
  38. S. Sato, Chem. Phys. Lett., 1986, 123, 126 CrossRef CAS.
  39. M. Harb, P. Sautet and P. Raybaud, J. Phys. Chem. C, 2011, 115, 19394 CAS.
  40. M. Batzill, E. H. Morales and U. Diebold, Phys. Rev. Lett., 2006, 96, 026103 CrossRef PubMed.
  41. J. B. Li, S. H. Wei, S. S. Li and J. B. Xia, Phys. Rev. Lett., 2006, 74, 081201 Search PubMed.
  42. S. Lopez, A. H. Romero, P. Rodriguez-Hernandez and A. Munoz, Phys. Rev. B: Condens. Matter Mater. Phys., 2009, 79, 214103 CrossRef.
  43. C. Di Valentin, G. Pacchioni and A. Selloni, Phys. Rev. B: Condens. Matter Mater. Phys., 2004, 70, 085116 CrossRef.
  44. G. Dong, K. Zhao and L. Zhang, Chem. Commun., 2012, 48, 6178 RSC.
  45. W. G. Aulbur, L. Jönsson and J. W. Wilkins, Solid State Phys., 2000, 54, 1 CAS.
  46. S. K. Sampath, D. G. Kanhere and R. Pandey, J. Phys.: Condens. Matter, 1999, 11, 3635 CrossRef CAS.
  47. K. Z. Smagul and R. Ponniah, J. Am. Ceram. Soc., 2010, 93, 3335 CrossRef.
  48. L. Hedin, Phys. Rev., 1965, 139, A796 CrossRef.
  49. H. Dixit, N. Tandon, S. Cottenier, R. Saniz, D. Lamoen, B. Partoens, V. Van Speybroeck and M. Waroquier, New J. Phys., 2011, 13, 063002 CrossRef.
  50. V. I. Anisimov, J. Zaanen and O. K. Andersen, Phys. Rev. B: Condens. Matter Mater. Phys., 1991, 44, 943 CrossRef CAS.
  51. V. I. Anisimov, I. V. Solovyev, M. A. Korotin, M. T. Czyzyk and G. A. Sawatzky, Phys. Rev. B: Condens. Matter Mater. Phys., 1993, 48, 16929 CrossRef CAS.
  52. A. I. Liechtenstein, V. I. Anisimov and J. Zaanen, Phys. Rev. B: Condens. Matter Mater. Phys., 1995, 52, R5467 CrossRef CAS.
  53. V. I. Anisimov, F. Aryasetiawan and A. I. Lichtenstein, J. Phys.: Condens. Matter, 1997, 9, 767 CrossRef CAS.
  54. A. Seidl, A. Görling, P. Vogl, J. A. Majewski and M. Levy, Phys. Rev. B: Condens. Matter Mater. Phys., 1996, 53, 3764 CrossRef CAS.
  55. J. Paier, M. Marsman, K. Hummer, G. Kresse, I. C. Gerber and J. G. Ángyán, J. Chem. Phys., 2006, 124, 154709 CrossRef CAS PubMed.
  56. M. Marsman, J. Paier, A. Stroppa and G. Kresse, J. Phys.: Condens. Matter, 2008, 20, 064201 CrossRef CAS PubMed.
  57. J. P. Perdew, K. Burke and M. Ernzerhof, Phys. Rev. Lett., 1996, 77, 3865 CrossRef CAS PubMed.
  58. H. J. Monkhorst and J. D. Pack, Phys. Rev. B: Condens. Matter Mater. Phys., 1976, 13, 5188 CrossRef.
  59. J. Hornstra and E. Keulen, Philips Res. Rep., 1972, 27, 76 CAS.
  60. L. Pisani, T. Maitra and R. Valentí, Phys. Rev. B: Condens. Matter Mater. Phys., 2006, 73, 205204 CrossRef.
  61. A. Bouhemadou and R. Khenata, Phys. Lett. A, 2006, 360, 339 CrossRef CAS.
  62. S. López, A. H. Romero, P. Rodríguez-Hernández and A. Muñoz, Phys. Rev. B: Condens. Matter Mater. Phys., 2009, 79, 214103 CrossRef.
  63. J. P. Perdew, M. Ernzerhof and K. Burke, J. Chem. Phys., 1996, 105, 9982 CrossRef CAS.
  64. K. Yang, Y. Dai and B. Huang, J. Phys. Chem. C, 2007, 111, 12086 CAS.
  65. R. Long and N. J. English, J. Phys. Chem. C, 2010, 114, 11984 CAS.
  66. M. E. Kurtoglu, T. Longenbach, K. Sohlberg and Y. Gogotsi, Phys. Chem. Chem. Phys., 2011, 13, 1379 RSC.
  67. H. Sun, W. Fan, Y. Li, X. Cheng, P. Li, J. Hao and X. Zhao, J. Phys. Chem. C, 2011, 115, 17392 Search PubMed.
  68. T. Liu, M. Dupuis and C. Li, J. Phys. Chem. C, 2016, 120, 6930 CAS.

Footnote

Electronic supplementary information (ESI) available: The convergence tests, the band structures of the pure ZnGa2O4 calculated by different functionals, the relative energies of 2N-doped ZnGa2O4 with different doping sites. See DOI: 10.1039/c6ra09655g

This journal is © The Royal Society of Chemistry 2016
Click here to see how this site uses Cookies. View our privacy policy here.