Diem Thi-Xuan Dang*ab,
Hieu Cao Dongab,
Yoshiyuki Kawazoecde,
Jer-Lai Kuof and
Duc Nguyen-Manhg
aCenter for Innovative Materials and Architectures (INOMAR), Ho Chi Minh City 721337, Vietnam. E-mail: dxdiem@inomar.edu.vn; xuandiemdang@gmail.com
bVietnam National University – Ho Chi Minh City, Ho Chi Minh City 721337, Vietnam
cNew Industry Creation Hatchery Center, Tohoku University, Sendai 980-8579, Japan
dDepartment of Physics, Suranaree University of Technology, Nakhon Ratchasima, Thailand
eDepartment of Physics and Nanotechnology, SRM Institute of Science and Technology, Kattankulathur, Tamil Nadu-603203, India
fInstitute of Atomic and Molecular Sciences, Academia Sinica, Taipei 10617, Taiwan
gCCFE, United Kingdom Atomic Energy Authority, Culham Science Centre, UK
First published on 18th September 2020
The crystal symmetries, electronic structures, and magnetic properties of metal–organic VNU-15 frameworks (VNU = Vietnam National University) were investigated using density functional calculations (DFT) with an on-site Coulomb repulsion approximation, Ueff, of 4.30 eV, determined via the linear response method. Two different orientations of dimethylammonium (DMA+) cations in VNU-15 were investigated. Antiferromagnetic configurations were predicted to be the ground states, with Fe ions in high-spin states for both phases. Furthermore, VNU-15 had intrinsic semiconductor electronic behavior with a small band gap of about 1.20 eV. The change in the orientation of DMA+ led to changes in the dispersion of the band structure, the band gap, and the Fe contributions to the valence band and conduction band. A fascinating feature was found involving exchange of oxidation numbers between two adjacent Fe atoms in the two phases. Our results revealed that VNU-15 has strong oxidation activity and predicted the important role of an anisotropic effect on the hole and electron effective masses. The findings presented that the electronic and magnetic properties could be controlled via hydrogen bonds and proved VNU-15 to be a prospective material for photocatalytic applications.
Until now, materials containing mixed-valence Fe atoms, such as Fe3O4, FeIII4[FeII(CN)6]3·xH2O, [NH2(CH3)2][FeIIIFeII(HCOO)6], etc., have shown outstanding performance in several key applications.23–25 Nevertheless, the above MOFs are generally constructed from rod chains of octahedral Fe(II) or Fe(III) SBUs from an ionic bonding point of view and, indeed, MOFs composed of mixed-valence Fe(II)- and Fe(III)-based SBUs are scarcely reported in the literature. Recently, Tu et al. synthesized VNU-15 (VNU stands for Vietnam National University), formulated as Fe4(BDC)2(NDC)(SO4)4(DMA)4, where BDC, NDC, and DMA are benzene-1,4-dicarboxylate, naphthalene-2,6-dicarboxylate, and dimethylammonium, respectively. This material is composed of novel infinite rod SBUs [Fe2(CO2)3(SO4)2(DMA)2]∝ based on both Fe(II) and Fe(III).26 These SBUs connect with two BDC2− and one NDC2− linker to create VNU-15, which is an anionic MOF balanced electrically with DMA cations. VNU-15 was tested as a proton transfer material in fuel cells and the proton conductivity reached 2.90 × 102 S cm−1 at 95 °C and 60% relative humidity. One of the possibilities explaining the high proton conductivity is the formation of a H-bond network between SO42− ions and DMA+ cations through a Grotthuss-type diffusion mechanism.27 Additionally, the proton conductivity of VNU-15 can be maintained for 40 hours without noticeable loss, and it has good heating–cooling stability.
The outstanding properties of infinite rod MOFs combined with the versatility of Fe have been shown in previous works,17,18 motivating us to study VNU-15. Although VNU-15 has been synthesized and its structure has been determined via X-ray diffraction, little is known about its electronic, magnetic, and other physical properties. Obtaining a comprehensive understanding of the many interesting properties of VNU-15 still remains desirable to provide vital fundamental data for its future utilization. Meanwhile, first-principles density functional calculations have been proven to be powerful in predicting the structural, electronic, and magnetic properties and chemical bonding of a wide series of MOFs.28,29 In the present work, density functional theory (DFT) with strong-electron correction was used to accurately describe the structure of VNU-15. The electronic structure and magnetic and chemical bonding properties in the ground state of VNU-15 were predicted. Different orientations of DMA cations in the anionic MOF were found to have significant effects on the electronic and magnetic properties of the material.30 Therefore, in this paper, the influence of the two orientations of DMA cations in VNU-15 on the electronic structures and magnetic properties was also considered.
A cut-off energy of 600 eV was identified to provide effective precision based on a cut-off energy study carried out in the range from 300 eV to 800 eV. The absolute energies were converged to within 10−5 eV per atom. Fully relaxed optimization of the atomic coordinates of VNU-15 was conducted using the standard conjugate gradient algorithm until the forces on all atoms were less than 10−2 eV Å−1. Brillouin-zone integration was performed with a Gaussian broadening of 0.1 eV during all relaxations. In this paper, the PAW treatment of pseudopotentials uses the 3d and 4s electrons for Fe, the 3s and 3p electrons for S, the 2s and 2p electrons for N, C, and O, and the 1 s electron for H. Because of the large primitive cell (approximately 250 atoms per primitive cell), the Γ-point alone was sufficient for sampling the Brillouin zone for all optimization calculations, while a denser 2 × 2 × 3 k-point was utilized for the density of states calculations. To understand the chemical bonding and interactions between constituents in VNU-15, charge density difference and Bader charge analyses37 were performed. The charge density difference was calculated from the subtraction of the electron density of the compound from the electron density of free atoms in the same framework with constant volume. All crystal structures were visualized using the VESTA program.38
As the GGA cannot be used to express well systems containing partially filled d-orbitals, the GGA+U method was used.39 The effective correlation energy, Ueff, for Fe d-orbitals was determined via a linear response approach:
(1) |
(2) |
(3) |
Phase | Atom | Wyckoff position | Site symmetry | x | y | z |
---|---|---|---|---|---|---|
DMA-1 | Fe1 | 16b | 1 | 0.8283 | 0.0894 | 0.5818 |
Fe2 | 0.5373 | 0.2938 | 0.6245 | |||
Fe3 | 0.3264 | 0.5877 | 0.5836 | |||
Fe4 | 0.1219 | 0.8788 | 0.5403 | |||
Fe5 | 0.8312 | 0.5827 | 0.0884 | |||
Fe6 | 0.8751 | 0.6255 | 0.2928 | |||
Fe7 | 0.8329 | 0.5846 | 0.5867 | |||
Fe8 | 0.7897 | 0.5413 | 0.8778 | |||
DMA-2 | Fe1 | 16b | 1 | 0.8307 | 0.0886 | 0.5837 |
Fe2 | 0.5401 | 0.2918 | 0.6251 | |||
Fe3 | 0.3273 | 0.5851 | 0.5869 | |||
Fe4 | 0.1235 | 0.8764 | 0.5424 | |||
Fe5 | 0.8276 | 0.5847 | 0.0876 | |||
Fe6 | 0.8737 | 0.6261 | 0.2908 | |||
Fe7 | 0.8314 | 0.5878 | 0.5841 | |||
Fe8 | 0.7884 | 0.5433 | 0.8754 |
Investigating various spin configurations may be advantageous for achieving an in-depth understanding of electronic behavior.42,43 Starting from the non-spin polarized convergence geometries, spin-polarized structure optimizations were carried out as the next step, where the Fe ions were regarded as magnetic centers and distinctive configurations were studied.44 The Fe cations of VNU-15 interact with each other along the same metal rod, called intra-chain interactions, and between neighboring metal rods (intermediated by linkers), called inter-chain interactions. The directions of these interactions are shown in Fig. 3(a). Eight high-spin Fe ions in the VNU-15 primitive cell can present up and down spins, resulting in 256 (28) spin configuration possibilities. Among the 256 spin configurations that can occur in the primitive cell of VNU-15, we chose the three simplest configurations for consideration. First is the case where all Fe ions are of the same spin value, that is, all with spin up or spin down, as represented in Fig. 3(b). This state is the result of intra- and inter-chain ferromagnetic interactions, and is referred to as FM. The second state is the result of ferromagnetic intra-chain and antiferromagnetic inter-chain interactions, which is named AFM-1. The third occurs with Fe ions showing opposite spin values alternately along the rods, as well as opposite spin values between the adjacent rods of the VNU-15 channel. The latter state, designated as AFM-2, is the result of antiferromagnetic interactions both intra- and inter-chain.
Key crystal structure geometric parameters from the optimized structures of VNU-15 in the different magnetic states are listed in Table 2. The lattice parameters in this work are slightly different from those obtained from X-ray diffraction experiments, but the differences are in a reasonable range (the maximum relative lattice parameter error being smaller than 7.5%). This discrepancy comes from eliminating disorder in the simulated structure and from calculations being done at 0 K, while the experimental structure was obtained at room temperature (298 K). The DMA-2 phase has been found to have a more-negative total energy compared to the DMA-1 phase and, obviously, the DMA-2 phase is more stable than the DMA-1 phase. The lattice parameters of the DMA-1 and DMA-2 phases showed slight discrepancies, and the volume of the DMA-2 phase was smaller by about 0.3% than the DMA-1 phase.
Experiment | Simulation | |||||||
DMA-1 | DMA-2 | |||||||
FM | AFM-1 | AFM-2 | FM | AFM-1 | AFM-2 | |||
IT | 70 | 43 | ||||||
Crystal system | Orthorhombic | |||||||
Space group | Fddd | Fdd2 | ||||||
Number of atoms per unit cell | 1088 | 976 | ||||||
Lattice constant | a (Å) | 16.76 | 16.99 (+1.37%) | 17.01 (+1.49%) | 17.03 (+1.61%) | 17.19 (+2.57%) | 17.18 (+2.51%) | 17.14 (+2.27%) |
b (Å) | 18.83 | 17.80 (−5.49%) | 17.79 (−5.52%) | 17.75 (−5.74%) | 17.42 (−7.49%) | 17.43 (−7.43%) | 17.53 (−6.90%) | |
c (Å) | 39.00 | 39.71 (+1.82%) | 39.73 (+1.87%) | 39.72 (+1.85%) | 40.01 (+2.59%) | 40.00 (+2.56%) | 39.90 (+2.31%) | |
V (Å3) | 12304.49 | 12012.20 (−2.38%) | 12016.08 (−2.34%) | 12006.39 (−2.42%) | 11976.89 (−2.66%) | 11980.13 (−2.64%) | 11990.40 (−2.55%) | |
Bond length (Å) | Fe(1)–Fe(2) | 3.60 | 3.51 | 3.51 | 3.51 | 3.48 | 3.48 | 3.49 |
Fe(1)–Fe(1) | 6.30 | 6.15 | 6.15 | 6.15 | 6.12 | 6.12 | 6.13 | |
Fe(2)–Fe(2) | 7.21 | 7.02 | 7.02 | 7.02 | 6.97 | 6.97 | 6.99 | |
Fe(1)–O(1S) | 2.12 | 2.16 | 2.16 | 2.16 | 2.00 | 2.00 | 1.99 | |
Fe(1)–O(1C) | 2.03 | 2.05 | 2.05 | 2.04 | 2.02 | 2.02 | 2.02 | |
Fe(1)–O(2C) | 2.17 | 2.10 | 2.10 | 2.10 | 2.05 | 2.05 | 2.05 | |
Fe(2)–O(2S) | 2.09 | 1.97 | 1.97 | 1.97 | 2.18 | 2.18 | 2.17 | |
Fe(2)–O(1C) | 2.09 | 1.97 | 1.97 | 1.97 | 2.02 | 2.02 | 2.02 | |
Fe(2)–O(2C) | 2.26 | 2.24 | 2.24 | 2.24 | 2.23–2.34 | 2.24–2.33 | 2.22–2.34 | |
N–H⋯O–S (1) | 1.90–196 | 1.74–1.77 | 1.74 | 1.74 | 1.80–1.83 | 180–1.83 | 1.80–1.82 | |
N–H⋯O–S (2) | — | — | — | — | 1.74 | 1.70–1.74 | 1.71 | |
Angle | Fe1–OC2–Fe2 | 108.89 | 108.14 | 108.09 | 108.20 | 106.83 | 106.98 | 107.26 |
OC2–Fe1–OC2 | 180.00 | 178.01 | 177.92 | 178.08 | 178.67 | 178.70 | 179.12 | |
OC2–Fe2–OC2 | 57.49 | 58.48 | 58.47 | 58.60 | 57.42 | 57.42 | 57.51 | |
Interlayer spacing d (Å) | 3.40 | 3.39 | 3.38 | 3.38 | 3.36 | 3.36 | 3.36 |
Deviations from the experimentally predicted structures have been studied in more detail through analysis of bonding interactions. Fe(1) and Fe(2) octahedra are in 8b (D2h symmetry) and 32 h (C2v symmetry) sites with Fddd symmetry. After optimization, both octahedra were in 16b sites with Fdd2 symmetry. The optimized bonds agreed well with the published crystal structure at a level no worse than that corresponding to a deviation value of 0.20 Å. The different magnetic configurations affected the bond lengths by a tiny amount in the same phase. However, different DMA orientations resulted in different Fe–O(S) bond lengths in each phase. For instance, the Fe(1)–O(1S) bond length in the DMA-2 phase is shorter than that of the DMA-1 phase by 0.16 Å, whereas the Fe(2)–O(2S) length in the DMA-2 phase is longer than that in the DMA-1 phase by 0.21 Å. The Fe(1)–O(1C) bond is stronger than the Fe(1)–O(2C) bond because of its shorter bond length, similar to the Fe(2) case. The dissimilar strengths of the two BDC2− and NDC2− linkers result in the difference in bond length. To further describe the Fe–O chains, the super-exchange Fe(1)–O(2C)–Fe(2) angle and O(2C)–Fe–O(2C) angle were studied. The super-exchange angle of VNU-15 is about 107–108°, larger compared with that of Fe–MOF-74 (105.90°),45 while the distance between two nearest Fe–Fe atoms is equal to 3.60 Å, which is larger than that of Fe–MOF-74 (2.90 Å). The O(2C)–Fe(1)–O(2C) angle is 180°, which leads to an Fe(2)–Fe(2) distance equal to two times that of the Fe(1)–Fe(2) distance. The O(2C)–Fe(2)–O(2C) angle is 57.49°, which leads to an Fe(1)–Fe(1) distance smaller than two times that of the Fe(1)–Fe(2) distance. The calculated super-exchange and O–Fe–O angles were found to be smaller than those from experiments, as shown in Table 2.
Structural analysis revealed that the SBUs were connected via four linker molecules, forming layers parallel to the (001) plane. Dispersion forces are important for capturing long-range interactions, such as the π–π stacking of aromatic rings, which support the framework and are able to permanently sustain pores. Indeed, the distance between two adjacent layers predicted from the present calculations is about 3.37 Å, which is within the vdW interaction distance of 2D conjugated carbon layers, and the closest Fe distance between two layers is 3.50 Å, indicating strong vdW interactions and metal–metal interactions between the two layers, confirming the findings of a previous experimental paper.26
The relative energy per primitive cell can be used to identify the preferred magnetic coupling of VNU-15, as shown in Table 3. It was found that the AFM-1 state has the lowest total energy compared to the others and, thus, the AFM-1 state is the most stable for the DMA-1 phase, while the AFM-2 configuration is the most stable for the DMA-2 phase. It is clear that AFM ordering is the magnetic ground state of VNU-15. Meanwhile, the magnetic ground state of Fe–MOF-74 is FM ordering. This statement is explained based on the distance between adjacent Fe centers affecting the direct exchange interactions between them (dFe−Fe = 2.90 Å in Fe–MOF-74 and dFe−Fe = 3.50 Å in VNU-15). In all cases, there are two local magnetic moments of 3.80 μB and 4.30 μB per Fe ion, reflecting the different oxidation states of Fe(1) and Fe(2). Specifically, Fe(1) and Fe(2) hold values of 3.80 μB and 4.30 μB in the DMA-1 phase, respectively, but the opposite is true in the DMA-2 phase. The magnetic moment of the O atoms has a very small value of 0.10 μB, originating from the interactions of O atoms with neighboring Fe atoms.
Phase | Magnetic model | Exchange energy (eV per primitive cell) | Fe magnetic moment (μB per atom) | Total magnetic moment (μB per primitive cell) | |||
---|---|---|---|---|---|---|---|
DMA-1 | FM | 0.010 | 3.793 | 4.282 | 3.793 | 4.282 | 36.0 |
3.793 | 4.282 | 3.793 | 4.282 | ||||
AFM-1 | 0.000 | −3.793 | −4.282 | −3.793 | −4.282 | 0.0 | |
3.793 | 4.282 | 3.793 | 4.282 | ||||
AFM-2 | 0.020 | 3.776 | −4.282 | 3.777 | −4.282 | 0.0 | |
−3.776 | 4.282 | −3.777 | 4.282 | ||||
DMA-2 | FM | 0.020 | 4.315 | 3.781 | 4.315 | 3.781 | 36.0 |
4.315 | 3.781 | 4.315 | 3.781 | ||||
AFM-1 | 0.018 | −4.315 | −3.781 | −4.315 | −3.781 | 0.0 | |
4.315 | 3.781 | 4.315 | 3.781 | ||||
AFM-2 | 0.000 | 4.311 | −3.773 | 4.311 | −3.773 | 0.0 | |
−4.311 | 3.773 | −4.311 | 3.773 |
The effect of magnetic anisotropy on the electronic structures and magnetic properties was assessed utilizing non-collinear spin calculations. The initial local magnetic moments for each Fe ion were given in different directions. The local magnetic moments of Fe ions are primarily assigned along the z-direction and give rise to small projected values in the x- and y-directions. In addition, the local magnetic moment of each Fe ion, via considering spin–orbit coupling, was found to be only 0.002 μB smaller than the values obtained in the isotropic case. Apparently, spin–orbit coupling was negligible in VNU-15. Consequently, non-collinear and spin–orbit coupling effects were not considered in the rest of the paper as the influence on the atomic magnetic moments is negligible.
In order to check whether long-range magnetic ordering exists in the framework, the spin densities of VNU-15 were calculated and plotted, as shown in Fig. 4. Positive (yellow color) spin densities allocated along each SBU direction were found in the FM state, as shown in Fig. 4(a) and (d). The AFM-1 configuration displayed negative (blue) and positive (yellow) spin densities distributed along each SBU direction, as shown in Fig. 4(b) and (e). Meanwhile, adjacent blue and yellow spin densities distributed along the same chain were presented in the AFM-2 model, as shown in Fig. 4(c) and (f). As can be seen in Fig. 4, the magnetization is utterly localized on the Fe–O chains, resulting in tiny amounts of inter-chain coupling.
To further understand the nature of the band structure, the total DOS of VNU-15 and partial DOS of ions around the Fermi energy EF were examined, as displayed in Fig. 6. The valence and conduction bands of DMA-1 show mainly Fe(1) and Fe(2) 3d-orbital contributions, respectively, whereas the situation is opposite for DMA-2. The low-lying band (below the valence band) is mainly centered on the orbitals of SO42− ions in both phases. The spin-polarized TDOS clearly displays nearly symmetric features in the spin-up and spin-down states of the AFM configurations. The electronic structures were found to be strongly influenced by on-site Coulomb repulsion. This breaks the strong Fe 3d–O 2p hybridization observed in the electronic structure calculated using the GGA (see Fig. S3, ESI†), resulting in the occupied Fe 3d states being shifted to higher energies. In contrast to the GGA, which predicts VNU-15 to be half-metal, GGA+U leads to a charge-transfer-type d–d gap of nearly 1.20 eV. It is reported that the GGA underestimates the band gap because it inadequately describes the strong correlation effect between 3d electrons localized on metal ions.29 Although there is no experimental band gap for reference, the band gap of Fe–MOF-74 was utilized for comparison. Fe–MOF-74 has a band gap of 0.30 eV, with a nearest Fe–Fe distance of 2.90 Å. Therefore, the band gap of VNU-15 may be roughly 1.20 eV with a distance of 3.50 Å. Consequently, the band gap obtained from GGA+U is more reasonable than that obtained via the GGA.17
The LDOS for two adjacent Fe(1) and Fe(2) ions with reverse spins and different ml values are presented in Fig. 7 to clarify the oxidation states. It turns out that the spin-down components relocate to a much higher energy than the spin-up ones. Fe2+ has d6 configuration and four unpaired d electrons, while Fe3+ has d5 configuration and five unpaired d electrons. Fig. 7(a) and (b) show that there are four and five unpaired d electrons from Fe(1) and Fe(2), respectively, in the DMA-1 phase. Fig. 7(c) and (d) show that there are five and four unpaired d electrons for Fe(1) and Fe(2), respectively, in the DMA-2 phase. It was predicted that the oxidation states of Fe(1) and Fe(2) were +2 and +3 in the DMA-1 phase, whereas the oxidation states of Fe(1) and Fe(2) were +3 and +2 in DMA-2. These findings are supported based on the magnetic moments in Table 2 and Bader charges in Table 4. Specifically, the calculated Fe(1) and Fe(2) magnetic moments were 3.80 μB and 4.30 μB for the DMA-1 phase and, reversely, these values were 4.30 μB and 3.80 μB for the DMA-2 phase. The calculated Fe(1) and Fe(2) charges were found to be 1.80|e| and 1.48|e| for the DMA-1 phase, however, these charges were 1.45|e| and 1.86|e| for the DMA-2 phase.
DMA-1 phase | DMA-2 phase | |||||
---|---|---|---|---|---|---|
Atom/state | FM | AFM-1 | AFM-2 | FM | AFM-1 | AFM-2 |
Fe(1) | 1.804 | 1.804 | 1.805 | 1.445 | 1.445 | 1.446 |
Fe(2) | 1.482 | 1.482 | 1.479 | 1.859 | 1.859 | 1.857 |
O(1C) | −1.116 | −1.116 | −1.117 | −1.116 | −1.117 | −1.117 |
O(2C) | −1.139 | −1.139 | −1.136 | −1.147 | −1.146 | −1.143 |
O(1S) | −1.334 | −1.334 | −1.333 | −1.287 | −1.286 | −1.286 |
O(2S) | −1.263 | −1.263 | −1.263 | −1.328 | −1.328 | −1.327 |
O(3S) | −1.315 | −1.316 | −1.315 | −1.319 | −1.320 | −1.319 |
C(1) | 0.353 | 0.353 | 0.356 | 0.344 | 0.344 | 0.343 |
C(2) | 0.215 | 0.215 | 0.213 | 0.227 | 0.226 | 0.228 |
S | 3.712 | 3.713 | 3.711 | 3.733 | 3.734 | 3.733 |
H(linker) | 0.097 | 0.096 | 0.094 | 0.098 | 0.099 | 0.098 |
DMA+ | 0.470 | 0.466 | 0.459 | 0.421 | 0.422 | 0.432 |
SO42− | −1.515 | −1.515 | −1.515 | −1.518 | −1.520 | −1.518 |
From Table 4, the average charges show insignificant variations between the spin configurations in the same phase. O(2C) has similar charges to O(1C) in both phases. The change in the orientation of DMA caused S to increase by 0.02|e| in the DMA-2 phase. In addition, it also changed the charges of O(1S) and O(2S) in the two phases. The charges of O(1S) and O(2S) in DMA-1 were −1.33|e| and −1.26|e|, and these changed to −1.28|e| and −1.33|e| in the DMA-2 phase. The charge of O(3S) underwent a negligible change in the two cases. The charges of the atoms in the linker are very small, indicating the vdW interactions between the linkers. Furthermore, only the charges of O atoms are found to be negative, while the other atom charges are positive, reflecting the ionic bonds between the atoms.
GGA+U calculations of the charge density difference were executed to clarify the nature of chemical bonding in VNU-15, as shown in Fig. 8. For BDC2− and NDC2− linkers, the plot shows that charge is mainly concentrated on the hydrogen atoms, and the charge transfer effect is insignificant. This can be explained by the fact that the stacked layers along the z-direction in the VNU-15 structure are held together by vdW interactions, which in turn is consistent with the analysis in the above discussion. For the SBUs, electrons transferring from O to Fe, C, and S sites indicates that Fe–O, C–O, and S–O bonding is ionic. Moreover, there are remarkable ionic bonds between Fe 3d–O 2p states, which stabilizes the structure. The findings relating to the nature of chemical bonding from GGA+U are similar to those from the GGA.
(4) |
ECB = EVB − Eg, | (5) |
χ is the electronegativity of the semiconductor calculated as the geometric mean of the absolute electronegativities of the constituent atoms, x(A):
(6) |
(7) |
The calculated electronegativity of VNU-15 is 6.79 eV. Therefore, the calculated oxidation and reduction potentials of the VB and CB edges are 2.85 V and 1.72 V, respectively, as shown in Fig. 9. O2 is not reduced to O2•− by the photogenerated electrons in the CB of VNU-15. The VB potential of VNU-15 is more positive than the oxidation potentials of H2O2/H2O (1.77 V), O3/H2O (2.07 V), and •OH/H2O (2.27 V).48 Therefore, the photogenerated holes can oxidize H2O to produce the active species H2O2, O3, and •OH, which can further decompose dye molecules and organic pollutants.
High mobility indicates fast carrier transport speeds from the bulk to the surface. This can diminish the electron–hole recombination probability within a semiconductor and strengthen the photocatalytic activity. The mobility of photogenerated electrons and holes has been investigated in a previous study.49 Based on a nearly free electron approximation, the mobility of photoexcited carriers can be calculated via the following formula:
(8) |
(9) |
In order to achieve good photocatalytic performance, the difference between the electron and hole effective masses should be large, to reduce the rate of recombination. Moreover, the effective hole mass should be smaller than the electron mass in order to move quickly to the surface, because only holes are involved in the photocatalytic process. In the spin-up case, the effective hole mass is lighter than the electron mass along the [100], [010], and [01] directions, whereas the ratio between and along the [01] direction is greater than in the two remaining directions. For the spin-down case, the effective hole mass is lighter than the electron mass along the [001] direction, and the ratio between the electron and hole effective masses is around 5. Therefore, it can be predicted that the photocatalytic activity on the surfaces corresponding to the [01] and [001] directions is efficient in the spin-up and spin-down cases, respectively.
The 3D band structures can qualitatively demonstrate the effective mass in the plane rather than special cases.50 For instance, the 3D band structures for the valence and conduction bands in the ky−kz plane are depicted in Fig. 10, where the chosen k-points are all centered at the S point. Fig. 10(a) and (c) exhibit that the projections of the valence bands are flat ellipses, hence, the effective hole masses are strongly anisotropic. Because of the much longer axis of the flat ellipse, the effective mass of photogenerated holes in the spin-up case is much larger along the [001] direction compared to the [010] direction. Meanwhile, the effective photogenerated hole mass for spin down is larger along the [010] direction compared to the [001] one. Similarly, Fig. 10(b) and (d) show that the projections of the conduction bands are flat ellipses, hence, the effective electron masses show significant differences in different directions. These findings are very supportive of the data shown in Table 5.
Fig. 10 The band structure for AFM-2 of the DMA-2 phase in the ky−kz plane with the (a) valence and (b) conduction bands for spin up, and the (c) valence and (d) conduction bands for spin down. |
The theoretical findings in this paper can be validated by experiments in different ways. Firstly, DMA-2 formation can be detected by electric control of the orientation of H-bonding between the DMA+ molecules and the framework using second-harmonic generation techniques.30,51 The DMA+ band-structure effect could be probed using angular-resolved photoelectron spectroscopy. It is possible to study the effectiveness of VNU-15 in photocatalysis via adding its powder to RhB or TC-H solution. The suspension is stirred for a given time interval in a dark environment to reach adsorption–desorption equilibrium. After infrared light illumination, which is generated using a Xe lamp with a suitable filter, the suspension is collected after a given period of time and separated via centrifugation. This approach was used for mixed-valence FeII/FeIII Fe–MIL-53.52 Secondly, ac impedance measurements can be performed using a pelletized sample of VNU-15 in a magnetic field from low relative humidity to medium humidity at an elevated temperature. This experiment can be used to check how the intrinsic magnetic properties predicted in this work would affect the proton transport properties of VNU-15 with respect to an applied magnetic field.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/d0ra05865c |
This journal is © The Royal Society of Chemistry 2020 |