DOI:
10.1039/D4QI01781A
(Research Article)
Inorg. Chem. Front., 2024,
11, 7364-7373
Computer-aided screening of bismuth molybdates nonlinear optical crystals γ-Bi2MoO6†
Received
16th July 2024
, Accepted 5th September 2024
First published on 11th September 2024
Abstract
Nonlinear optical (NLO) materials are key components of laser systems that extend their frequency and module laser beam. In this case, d0 transition metals (d0-TMs) and cations with stereochemically active lone pairs (SCALPs) can induce asymmetric coordination environment in crystals owing to second-order Jahn–Teller (SOJT) effects and accordingly are beneficial in enhancing NLO properties. In this work, the first-principles screening method was used to search for NLO materials in a bismuth molybdate system. Finally, γ-Bi2MoO6 and Bi10Mo3O24 were screened and synthesized via high-temperature solid-state synthesis. γ-Bi2MoO6 showed a strong second harmonic generation (SHG) response (9.9 × KDP), large birefringence (0.21 at 1064 nm), and appropriate band gap (2.57 eV). This work presents systematic research on the application of bismuth molybdate systems as nonlinear optical materials and provides a reference for their further development.
Introduction
Nonlinear optical (NLO) crystals, which are the crucial and essential components of laser systems that widely used in laser science, signal processing, and optical communication, have attracted particular research attention.1–3 Since the discovery of the second harmonic generation (SHG) effect, research on nonlinear optical materials has advanced significantly.4,5 The exploration of IR NLO materials in the past decades has been extended from chalcogenides6–9 and pnictides10,11 to halides,12,13 oxyhalides,4,14,15 and transition-metal oxides.16–19 Among them, chalcogenides and phosphides usually have some inherent drawbacks that limit their applications. For instance, the commercially available IR NLO material AgGaS2 has a low laser damage threshold (LDT), while ZnGeP2 suffers from two-photon absorption.20–22 Alternatively, because of their ability to achieve equilibrated performances and grow in an open system, oxides have become promising candidates as mid-infrared NLO materials. Hence, it is urgent to explore new oxide infrared nonlinear optical materials with excellent comprehensive properties.
d0 transition metals (Ti4+, Mo6+, W6+, Nb5+, etc.) and cations with stereochemically active lone pairs (SCALPs) (I5+, Pb2+, Te4+, Bi3+, etc.) exhibiting the second-order Jahn–Teller (SOJT) effect play an important role in the design and synthesis of NLO compounds with significant application value.23–25 Moreover, some studies have indicated that the combination of various NLO-active units in the same compound is a successful strategy for designing promising nonlinear optical materials with enhanced SHG responses, such as K3V2O3F4(IO3)3 (1.3 × KTP at 2050 nm),26 Pb2Bi(SeO3)2Cl3 (13.5 × KDP at 1064 nm),27 CdTeMoO6 (2 × KTP at 1064 nm),28 Cs2TeW3O12 (1.5 × KTP at 1064 nm),29 and BaNbO(IO3)5 (660 × α-SiO2 at 1064 nm).30 Molybdates have rich chemical compositions and crystal structure types, including motifs such as [MoO4], [MoO5] and [MoO6], which have been widely investigated by researchers. In addition, the magnitude of the SOJT distortion of SHG-active d0 cations follows the following order: Mo6+ > V5+ > W6+ > Ti4+ > Nb5+ > Ta5+ > Zr4+.31 It is anticipated that introducing Mo6+ cations into a material will increase the chance of realizing an amplified SHG response. Alternatively, introducing cations with lone pair electrons in materials can enhance their birefringence and SHG performances, such as Pb2(NO3)2(H2O)F2 (12 × KDP at 1064 nm),32 Pb2(BO3)(NO3) (9 × KDP at 1064 nm),33 Sn2PO4X (X = Br and I) (0.336–0.664 at 546 nm),34 Sn9O4Br9X (X = Cl and Br) (0.273–0.258 at 1064 nm),35 and CsSn2(HPO3)2I (0.200 at 546 nm).36 Bi3+ cations with lone pair electrons can generate large polarizability, resulting in enhanced SHG responses, for example, Cs2Bi2OSi2O7 (3.5 × KDP at 1064 nm),37 Cd4BiO(BO3)3 (6 × KDP at 1064 nm),38 Bi32Cd3P10O76 (4 × KDP at 1064 nm),39 and β-Li2RbBi(PO4)2 (5.2 × KDP at 1064 nm).40 Considering this, we focused on bismuth molybdates, in which the d0 transition metal Mo6+ and SCALP cation Bi3+ are combined. Bismuth molybdates are considered of great interest, which possess rich structural diversity and promising functional properties for application in catalysis, optical materials, nanoelectronics and nanophotonics.41–43 For example, α-Bi2Mo3O12, β-Bi2Mo2O9, and γ-Bi2MoO6 are known for their high photo-electrochemical and photo-catalytic activities.44 However, there are only few studies in the nonlinear optical regime, and thus further exploration is needed.
In this work, the first-principles screening method for NLO materials was used to screen bismuth molybdate NLO materials from the Inorganic Crystal Structure Database (ICSD).45 Finally, γ-Bi2MoO6 and Bi10Mo3O24 were synthesized via the traditional high-temperature solid-state method and their nonlinear optical properties reported. The two materials γ-Bi2MoO6 and Bi10Mo3O24 exhibit significant SHG responses, which are 9.9- and 3.7-times that of KDP, respectively. Additionally, they possess appropriate band gaps of 2.57 eV and 3.02 eV, respectively. Here, we provide an in-depth examination of these target compounds, including their synthesis, thermal properties, spectroscopic characteristics, optical birefringence, and structure–property relationships.
Experimental section
Reagents
Bi2O3 (AR, 99.9%) and MoO3 (AR, 99.9%) were commercially purchased and used as received without further purification.
Synthesis
Polycrystalline γ-Bi2MoO6 and Bi10Mo3O24 were synthesized via the traditional high-temperature solid-state method. In the case of γ-Bi2MoO6, commercially available Bi2O3 and MoO3 were completely ground in stoichiometric ratios (1:1) until uniformly mixed. This mixture was placed in a lidded alumina crucible and heated in the air according to the following procedure: heated to 500 °C for 8 h, held at this temperature for 24 h, and cooled to room temperature for 12 h. Then it was ground and pressed into sheets and heated to 600 °C at a rate of 1 °C min−1, kept at this temperature for 6 days, and finally cooled to room temperature in 24 h. A yellow polycrystalline sample was obtained. Using the same procedure, Bi10Mo3O24 was obtained at 750 °C in stoichiometric ratios.
Powder X-ray diffraction
The powder X-ray diffraction (PXRD) data of γ-Bi2MoO6 and Bi10Mo3O24 were measured using a Bruker D8 ADVANCE X-ray diffractometer (Cu Kα, λ = 1.541 Å). The test was performed at room temperature in the 2θ range of 10–70°, with a step of 0.02° and sampling time of 2 s.
Thermal analysis
Thermal gravimetric (TG) analysis and differential scanning calorimetry (DSC) were performed on a NETZSCH STA 449C thermal analyzer instrument. The polycrystalline sample was weighed and placed in an alumina crucible, which was heated in the range of 25 °C to about 1000 °C at a rate of 10 °C min−1 in an air atmosphere.
Fourier transform infrared (FTIR) spectroscopy
A Nicolet IS 10 FTIR spectrometer was used to collect data in the range of 400–4000 cm−1 at room temperature. Using KBr as the background, a mixture of KBr and sample was pressed into a pellet for testing.
UV-vis diffuse reflectance spectroscopy
UV-vis diffuse reflectance spectra were recorded using a Shimadzu UV-3600 spectrometer in the range of 300 to 800 nm at room temperature.
SHG measurement
The powder SHG effect of the γ-Bi2MoO6 and Bi10Mo3O24 crystals were tested using the Kurtz and Perry method46 and an Nd:YAG Q-modulated laser with a wavelength of 1064 nm and a KDP crystal as a reference. The γ-Bi2MoO6 and Bi10Mo3O24 samples and the KDP reference sample were ground into different particle sizes, and then screened, and the powders were sieved into several different particle size ranges of 20–38.5, 38.5–55, 55–88, 88–125, 125–160, 160–200 and 200–250 μm.
Theoretical calculation
The electronic structure of γ-Bi2MoO6 and Bi10Mo3O24 was investigated using first-principle calculations performed using the CASTEP package based on density functional theory (DFT).47 The Perdew–Burke–Ernzerhof (PBE) generalized gradient approximation (GGA) functional for electron exchange-related energies and the norm-conserving pseudopotential to describe electron-nucleus interactions were adopted.48 The γ-Bi2MoO6 and Bi10Mo3O24 structures were used for theoretical calculations and tested for convergence with the plane-wave energy cutoff and interatomic force of 750 eV and 1 × 10−6 eV A−1, respectively. The Monkhorst–Pack method was used for the integration of the Brillouin zone for the selection of k-space grid points, and the final k-points were set to 5 × 2 × 5 and 1 × 4 × 3, respectively.
Results and discussion
We focused on the bismuth molybdate system and 5 asymmetric structures containing Bi, Mo and O elements were searched from the Inorganic Crystal Structure Database (ICSD). Then, the band gap, birefringence, and second-order susceptibility χ(2) of these bismuth molybdates were successfully calculated using the DFT method (Table S1†). Molybdate possesses a wide transmission window in the infrared region, and accordingly can be used as a mid-infrared NLO material. We expected to obtain materials with a large SHG response (χ(2) > 7.8 pm V−1). Finally, the γ-Bi2MoO6 and Bi10Mo3O24 compounds were successfully synthesized.
The structure of γ-Bi2MoO6 was first reported by Van den Elzen and Rieck in 1973.49 In 1986, VK Yanovskii reported that its SHG intensity reached 60 to 80 in units of I2ω of quartz but did not further explore its NLO-related properties.50 Herein, low-temperature phase γ-Bi2MoO6 was synthesized, belonging to the Pca21 (no. 29) space group with cell parameters a = 5.487(2) Å, b = 16.226(6) Å, c = 5.506(2) Å, and Z = 4. Its asymmetric unit contains two Bi atoms, one Mo atom, and six O atoms. In this structure, each Mo atom is coordinated with six O atoms to form an MoO6 octahedron. A significant distortion towards the edge (C2, Δd = 1.64) was observed in the MoO6 octahedron,51 which is highly beneficial in achieving a large local microscopic polarizability and leads to an enhanced SHG response. The MoO6 octahedra are interconnected by co-angled O atoms, which share angles along the a and c directions to form an infinite [MoO4]2− layer (Fig. 1b). The [Bi2O2]2+ layer consists of a square planar network of O2− anions (Fig. 1c), with Bi3+ cations alternating above and below the planes, which can be described as forming a BiO4 square pyramidal cap. Besides, each Bi atoms are connected with two vertex O atoms of MoO6 octahedra to form BiO6 polyhedron with stereochemically active construction. The [Bi2O4]2− and [MoO4]2− layers are alternately stacked along the b-axis by sharing vertex O atoms to form the three-dimensional crystal structure of γ-Bi2MoO6 (Fig. 1a).
|
| Fig. 1 Schematic crystal structure of γ-Bi2MoO6 (a), MoO6 octahedron (b) and [Bi2O2]2+ layer (c). | |
Bi10Mo3O24 crystallizes in the monoclinic crystal system noncentrosymmetric space group C2 (no. 5) with the cell parameters of a = 23.72316(5) Å, b = 5.64745(1) Å, c = 8.68034(2) Å, β = 95.8734(1)°, and Z = 2. The asymmetric unit of Bi10Mo3O24 consists of five Bi, two Mo and thirteen O, which are crystallographically independent atoms. The structure of Bi10Mo3O24, as projected onto the ac plane, is depicted in Fig. S4c.† Its overall structure is composed of an infinite [Bi10O12]n layer (Fig. S4a†), which is oriented parallel to the b direction and repetitively arranged along the c direction. The Bi3+ cations within the [Bi10O12]n layers are coordinated with four, five and six O atoms, forming the BiOn (n = 4, 5, 6) polyhedra with Bi–O bond lengths in the range of 2.023 to 2.692 Å. The {3[MoO4]2−}m tetrahedral groups are situated within the ten-membered ring channels composed of bismuth polyhedra and balance the charge of the structure (Fig. S4b†).
To study the relationship between macroscopic symmetry and microstructure, the local dipole moments of the polyhedra within the crystal structure and the net dipole moment within the unit cell were calculated using the bond-valence method (Tables S2 and S3†). In γ-Bi2MoO6 and Bi10Mo3O24, the Bi–O polyhedra are severely distorted and exhibit significant dipole moments (γ-Bi2MoO6: 15.061–17.406 D; Bi10Mo3O24: 14.861–19.929 D), which may be ascribed to the SCALP of electrons in the Bi3+ cation. Due to the influence of the SOJT effect, the Mo–O polyhedra also undergo varying degrees of distortion. In the case of γ-Bi2MoO6, as a result of its crystal symmetry, the local dipole moments add up and the a and b components of the net dipole moment within the unit cell are canceled, leading to macroscopic polarization along the c-axis. Similarly, Bi10Mo3O24 exhibits a net dipole moment directed along the b-axis. The total dipole moment along the c-axis for γ-Bi2MoO6 is 19.813 D, with a dipole moment density of 0.040 D Å−3. Along the b-axis for Bi10Mo3O24, the total dipole moment is 35.594 D, and the dipole moment density was calculated to be 0.031 D Å−3. The large dipole moments of Bi–O polyhedra indicate strong distortion resulting from SCALP. These two compounds, with their large net dipole moments, are instrumental in achieving optical anisotropy and NLO performance.
The γ-Bi2MoO6 and Bi10Mo3O24 polycrystals were synthesized via the high-temperature solid-phase method. As shown in Fig. 2a and b, the experimental and calculated values in the PXRD plot are consistent, which demonstrates the high purity of γ-Bi2MoO6 and Bi10Mo3O24, respectively. The thermal characteristics were evaluated through TG/DSC examinations. The TG curves of γ-Bi2MoO6 and Bi10Mo3O24 showed no significant weight loss between room temperature and about 1000 °C (Fig. S6a and S6b,† respectively). In the DSC curves (Fig. S6a†), γ-Bi2MoO6 has a phase transition at 641.7 °C.52 Combined with the PXRD patterns of the γ-Bi2MoO6 samples heated at different temperature (Fig. S6c†), the transferred phase is γ′-Bi2MoO6 that crystallized in the space group of P21/c. The new phase melts at 929.2 °C and decomposes at 966.5 °C. As show in Fig. S6c,† some minor impurity peaks were detected at 950 °C and the peaks became obvious at 1000 °C, proving that γ′-Bi2MoO6 will decompose at high temperatures. The DSC profile and PXRD pattern (Fig. S6b and S6d,† respectively) indicate that Bi10Mo3O24 undergoes decomposition at 864.2 °C to form a mixture of Bi38Mo7O78 oxide and unknown high-temperature solid solution,53 and subsequently melted at 946.5 °C. The thermal behaviors of the two crystals suggest that the low temperature flux method is needed to grow single crystals.
|
| Fig. 2 Powder X-ray diffraction patterns of γ-Bi2MoO6 (a) and Bi10Mo3O24 (b). UV-vis diffuse reflectance spectra of γ-Bi2MoO6 (c) and Bi10Mo3O24 (d). FT-IR spectra of γ-Bi2MoO6 (e) and Bi10Mo3O24 (f) samples. | |
The data collected by UV-Vis diffuse reflectance spectroscopy were processed using the Tauc plot method,54 and it was found that γ-Bi2MoO6 shows a band gap of 2.57 eV, which is consistent with the yellow color exhibited by its crystal. Its UV cut-off edge is about 410 nm (Fig. 2c). Furthermore, the UV cut-off edge of Bi10Mo3O24 is 367 nm. The experimental band gap is 3.02 eV (Fig. 2d). The values of these two compounds are comparable to that of molybdates, such as CeClMoO4 (2.91 eV),55 CeBrMoO4 (2.81 eV),55 and MoO2Cl2 (2.88 eV).56
The infrared spectra show absorption bands between 400 and 4000 cm−1, which were employed to elucidate the IR absorption models. In the case of γ-Bi2MoO6 (Fig. 2e), with the absorption peak of the stretching vibration of the Bi–O bond located near 447 cm−1 and the absorption band of the Mo–O–Bi vibration mode near 510 cm−1.57 The absorption peaks at 729 and 842 cm−1 represent the Mo–O stretching vibration.58 In the case of Bi10Mo3O24 (Fig. 2f), the peaks at about 434 and 546 cm−1 can be ascribed to the Bi–O bond vibrations, while the bands at 746 and 802 cm−1 are ascribed to the Mo–O tetrahedral stretching vibration. Using density functional theory calculations, we simulated the infrared vibration modes of γ-Bi2MoO6 (Fig. S7†) and Bi10Mo3O24 (Fig. S8†). The experimental results are consistent with the simulated spectrum. The IR absorption spectra indicate that two compounds have no intrinsic absorption in a broad transmission range.
The SHG responses of the sieved γ-Bi2MoO6 and Bi10Mo3O24 samples with different particle sizes were measured using the Kurtz-Perry method at room temperature with a laser beam with a wavelength of 1064 nm from an Nd:YAG laser. As shown in Fig. 3, the powder SHG intensity of the two samples increased with an increase in their particle size, which indicates that it can achieve phase matching. γ-Bi2MoO6 and Bi10Mo3O24 exhibited SHG responses of 9.9- and 3.7-times that of the KDP samples, respectively, when measured with a particle size in the range of 200–250 μm. To evaluate the performance of γ-Bi2MoO6 and Bi10Mo3O24, the SHG effect of pure molybdate NLO materials were surveyed, as shown in Table 1. It can be seen that γ-Bi2MoO6 has an excellent SHG performance, which indicates that γ-Bi2MoO6 is a promising IR NLO crystal material. Restricted by Kleinman symmetry, three (d15, d24, and d33) and four (d16, d14, d22, and d23) independent nonzero SHG tensors for γ-Bi2MoO6 and Bi10Mo3O24 should be considered, respectively. To get accurate calculation results, we set the scissors operator value as 1.58 eV for γ-Bi2MoO6 and 0.51 eV for Bi10Mo3O24. The calculated SHG coefficients of γ-Bi2MoO6 are d15 = −6.78, d24 = 12.78 and d33 = 5.80 pm V−1, while the SHG coefficients of d16, d14, d22, and d23 for Bi10Mo3O24 are −1.71, 2.54, 1.67, and −0.30 pm V−1, respectively.
|
| Fig. 3 SHG intensities vs. particle sizes with a 1064 nm pump for γ-Bi2MoO6 and Bi10Mo3O24 compared with benchmark KDP with the same particle size. | |
Table 1 Comparison of the SHG effect of typical molybdate NLO materials
No. |
Material |
Space group |
SHG |
Ref. |
This work.
The SHG efficiency at 1064 nm.
The SHG efficiency at around 2090 nm.
|
1 |
Cs2NaBi(MoO4)3 |
R3c |
5 × α-SiO2b |
59
|
2 |
LiNa5Mo9O30 |
Fdd2 |
2 × KDPb |
60
|
3 |
LaBrMoO4 |
Pc
|
0.47 × KDPb |
61
|
4 |
Ba2MoO3F4 |
Cc
|
8 × α-SiO2b |
62
|
5 |
β-BaMo3O10 |
P21 |
1.2 × KDPb |
63
|
6 |
α-BaMoO2F4 |
Pca21 |
0.7 × α-SiO2b |
64
|
7 |
SrMoO2F4 |
Pca21 |
1.1 × α-SiO2b |
64
|
8 |
PbMoO2F4 |
Pca21 |
0.5 × α-SiO2b |
64
|
9 |
KMoO2F3 |
P212121 |
0.4 × α-SiO2b (NPM) |
65
|
10 |
(Ag3MoO3F3)(Ag3MoO4)Cl |
P3m1 |
10 × α-SiO2b |
66
|
11 |
K10(Mo2O4F7)3Cl |
Pmn21 |
0.8 × KDPb (NPM) |
67
|
12 |
K7Ag(MoO4)4 |
P63mc |
2.9 × α-SiO2b |
68
|
13 |
CeClMoO4 |
Pc
|
0.06 × AGSc |
55
|
14 |
CeBrMoO4 |
Pc
|
0.58 × AGSc |
55
|
15 |
MoO2Cl2 |
Fmm2 |
2.1 × KTPc |
56
|
16 |
Bi10Mo3O24a |
C2 |
3.7 × KDPb |
This work |
17 |
γ-Bi2MoO6a |
Pca21 |
9.9 × KDPb |
This work |
The nonlinear optical properties were further investigated by theoretical means to reveal the origin of the SHG response. The calculated electronic band structure indicated that γ-Bi2MoO6 has an indirect band gap of 0.99 eV (Fig. 4a), and Bi10Mo3O24 has a direct band gap of 2.51 eV (Fig. 4b). Due to the discontinuity of the exchange–correlation energy functional, the band gaps are underestimated. Thus, to obtain the accurate band gap of γ-Bi2MoO6, the HSE06 hybrid exchange–correlation functional was used, and its band gap was calculated to be 1.97 eV (Fig. S9†), which is very close to its experimental band gap. The refractive index dispersion curves of the γ-Bi2MoO6 and Bi10Mo3O24 compounds were also calculated. Based on the refractive index curve with the scissors operator, the birefringence at 1064 nm (Δncal) was calculated to be 0.21 and 0.03 (Fig. 4c and d), respectively.
|
| Fig. 4 Calculated band structure and partial densities of states of γ-Bi2MoO6 (a) and Bi10Mo3O24 (b) and refractive index dispersion of γ-Bi2MoO6 (c) and Bi10Mo3O24 (d). | |
According to the calculated partial densities of states (PDOS), it can be seen that γ-Bi2MoO6 and Bi10Mo3O24 exhibit similar electronic structures. The O 2p states and less Bi 6s6p were located in the top of the valence band (TVB) (−5–0 eV), and the bottom of the conduction band (BCB) (0–5 eV) is mainly occupied by the O 2p and Mo 4d states (Fig. 4a and b). Theoretical studies have shown that nonlinear optical properties are directly related to the leap between the states of electrons near the Fermi energy level. Therefore, the optical properties of γ-Bi2MoO6 and Bi10Mo3O24 were determined based on the synergistic effect of the O-2p and Bi 6s6p orbitals in the occupied states, while the Mo-4d and O-2p orbitals in Mo–O polyhedra in the unoccupied states. To further study the stereoactivity of the lone pair electrons on the Bi3+ cations located in different environments, the Bi-related PDOS diagrams and the electron localization function (ELF) were calculated for γ-Bi2MoO6. According to the PDOS diagrams (Fig. 5a), it can be seen that the 6s orbitals of each Bi atom occupy the TVB, contributing to the lone pair electronic configuration and optical properties of the materials. The two individual Bi atoms in γ-Bi2MoO6 exhibit hemispherical isosurfaces (Fig. 5b and c, respectively), confirming the stereoactivity of the Bi3+-6s2 lone pair electrons. The five individual Bi atoms in Bi10Mo3O24 exhibit similar electronic characters to that of γ-Bi2MoO6, as shown in Fig. S10.†
|
| Fig. 5 Partial DOSs of Bi1 and Bi2 atoms from γ-Bi2MoO6 (a). ELF of γ-Bi2MoO6 (b). ELF for two independent Bi atoms in γ-Bi2MoO6 (c). | |
The contributions to the SHG responses were analyzed using the SHG-weighted electron density of the largest tensor. The SHG density was plotted to show the electron orbitals that contribute to SHG in real space. In γ-Bi2MoO6, both the virtual-electron (VE) and virtual-hole (VH) processes contribute equally to the SHG tensor d24. Additionally, the VE process has a larger contribution (91.8%) to the SHG effects in Bi10Mo3O24 than that of the VH process. According to the SHG density diagram of the occupied orbitals in γ-Bi2MoO6, it can be observed that the contribution of the O2 and O3 atoms shared by Bi and Bi are higher than that of the O1 and O6 atoms shared by Bi and Mo, which are higher than that of O4 and O5 atoms shared by Mo and Mo (Fig. S11†). Besides, the lone pair electrons of Bi atom also have slight contributions to SHG. Therefore, the SHG density of γ-Bi2MoO6 in the occupied states mainly accumulates on the BiO6 polyhedra, while the orbitals belonging to MoO6 octahedra are the main source in the unoccupied states (Fig. 6). In the case Bi10Mo3O24 (Fig. S12†), the results indicate that the BiOn (n = 4, 5, 6) polyhedra in the occupied states and MoO4 groups in the unoccupied states dominate the SHG contributions.
|
| Fig. 6 SHG density maps of (a) occupied and (b) unoccupied orbitals of virtual-electron (VE) part as well as (c) occupied and (d) unoccupied orbitals of virtual-hole (VH) part of the largest SHG coefficient d24 for γ-Bi2MoO6. | |
Conclusions
In summary, based on the DFT method, the first-principles screening method was used to search for exceptional non-linear optical (NLO) materials in bismuth molybdates. Finally, two bismuth molybdates, γ-Bi2MoO6 and Bi10Mo3O24, were screened and synthesized via a solid-state reaction. γ-Bi2MoO6 exhibited a strong SHG intensity of 9.9 times that of KDP and a large birefringence of 0.21 at 1064 nm. Bi10Mo3O24 exhibited the SHG effect of about 3.7 × KDP. The theoretical research results indicate that the SHG response of the title compound originates from the BiOn polyhedra in the occupied states, while the MoOn polyhedra in unoccupied states. This report on the two compounds will provide further insights for exploring nonlinear optical crystals of bismuth molybdates and obtaining excellent candidates for the next step of development.
Author contributions
The manuscript was written through the contributions of all authors. All authors have given approval to the final version of the manuscript.
Data availability
The raw data supporting the conclusions of this manuscript will be made available by the authors, without undue reservation, to any qualified researcher.
The authors confirm that the data supporting the findings of this study are available within the article and its ESI.†
Conflicts of interest
There are no conflicts to declare.
Acknowledgements
This work was supported by the National Natural Science Foundation of China (Grant No. 52072109 and 22101069); the Science and Technology Project of Hebei Education Department (Grant No. BJK2023029); the Natural Science Foundation of Hebei Province (Grant No. B2023201068); Key Laboratory of Chemical Biology of Hebei Province (22567635H); the Key Laboratory of Analytical Science and Technology of Hebei Province (No. 22567620H).
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Footnote |
† Electronic supplementary information (ESI) available: Screening results. Calculation of dipole moments in γ-Bi2MoO6 and Bi10Mo3O24. Crystal structure of Bi10Mo3O24. Atomic coordination environment, TG-DSC analysis of γ-Bi2MoO6 and Bi10Mo3O24. The PXRD of γ-Bi2MoO6 and Bi10Mo3O24 samples at different calcination temperatures. The infrared vibration mode of γ-Bi2MoO6 and Bi10Mo3O24. The PDOS, ELF, and SHG density maps of Bi10Mo3O24. See DOI: https://doi.org/10.1039/d4qi01781a |
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