DOI:
10.1039/D3QI01807E
(Research Article)
Inorg. Chem. Front., 2023,
10, 6869-6878
Achieving broadband ultraviolet to mid-infrared transparency in germanate-based nonlinear optical crystals Cs3REGe3O9 (RE = Y, Gd)†
Received
7th September 2023
, Accepted 10th October 2023
First published on 10th October 2023
Abstract
Nonlinear optical (NLO) materials currently attract significant interest and hold paramount importance in the optoelectronic field. Nevertheless, the fabrication of NLO crystals capable of transmitting ultraviolet to mid-infrared wavelengths remains a formidable challenge. Herein, we synthesized two novel NLO crystals, namely Cs3REGe3O9 (RE = Y, Gd), by employing a structural gene strategy that harmoniously merges flexible [YO6] and [GdO6] octahedra with rigid [GeO4] motifs. Remarkably, Cs3REGe3O9 (RE = Y, Gd) crystals exhibit substantial band gaps of 4.92 and 5.3 eV, respectively, while achieving the shortest reported ultraviolet cutoff edges at 210 and 215 nm among the boron-free germanate-based NLO materials. Importantly, these compounds also feature a remarkably broad infrared transparency range exceeding 6.8 μm. Furthermore, both compounds demonstrate a moderate second-harmonic-generation (SHG) response, comparable to that observed in KDP. Additionally, first-principles calculations unveil that the synergistic effect of the [REO6] octahedra and [GeO4] tetrahedra plays a pivotal role in governing the optical properties of Cs3REGe3O9 (RE = Y, Gd). These explored findings offer a novel avenue for leveraging the highly desired NLO materials in the region spanning from ultraviolet to mid-infrared wavelengths.
Introduction
The exploration and fabrication of inorganic oxides exhibiting distinct optoelectronic attributes have garnered considerable recognition over recent decades.1–4 Amongst these materials, those exhibiting acentric structures have assumed paramount significance in academic research and industrial applications due to their diverse functional attributes, including piezoelectricity, ferroelectricity, pyroelectricity, and nonlinear optical (NLO) properties.5–10 The extensively employed NLO oxide compounds, such as borates including KBBF (KBe2BO3F2),11 β-BBO (β-BaB2O4),12 LBO (LiB3O5),13 CLBO(CsLiB6O10) crystals,14 and phosphates including KDP (KH2PO4),15 KTP (KTiOPO4),16 RTP (RbTiOPO4),17etc., have notably demonstrated their application in the spectral range, spanning from deep ultraviolet (UV) to near-infrared (IR). However, the relatively elevated phonon energy inherent in these materials imposes a limitation on their capacity to fabricate NLO devices that operate beyond the wavelength threshold of 4.5 μm.18
In recent years, there has been a notable surge in scientific interest surrounding the pursuit of novel oxide crystals for mid-IR NLO applications. This endeavor involves the incorporation of heavy metal cations that are susceptible to second-order Jahn–Teller (SOJT) effects, and exemplary crystals include BaTeM2O9 (M = Mo, W),19 Li2MTeO6 (M = Zr, Ti, Sn),20,21 LiNbTeO5,22 Cs2Bi2OGe2O7,23 Te2V2O9,24 and Cs4V8O22.25 As anticipated, these crystals exhibit an extended IR transmission cutoff edge beyond 5 μm. Unfortunately, the introduction of transition metal cations such as Bi3+, Ti4+, V5+, Nb5+, Mo6+, W6+, etc., which participate second-order NLO processes, leads to an undesirable red shift of the UV cut-off edge, thereby impeding their suitability for utilization in the UV region. Consequently, the exploration into oxide NLO crystals capable of covering the transmission range from UV to mid-IR wavelengths remains a challenging task.
Based on previous investigations, germanate oxides have emerged as a highly promising and prospective prototype for the exploration of mid-IR NLO crystals, due to their structural diversity, including motifs such as [GeO4], [Ge2O7], and [Ge3O9].26,27 Moreover, the Ge–O bonds in germanate-based compounds possess a favorable low phonon energy, endowing them with an inherent extension of the transmission range in the IR region exceeding 6 μm. Compared with transition metal cations, rare earth cations demonstrate a versatile coordination with oxygen, thus facilitating the creation of acentric coordinated environments. Furthermore, rare earth cations, including Sc3+, Y3+, La3+, Gd3+, and Lu3+, possess closed-shell electronic configurations or half-occupied 4f orbitals, which effectively eliminate d–d or f–f electronic transitions.28 Consequently, this characteristic broadens the UV transparency window. Notable examples are observed in NLO-active rare earth borates such as RECa4O(BO3)3 (RE = Y, Gd),29 K5Mg2La3(BO3)6,30 and K7CdRE2B15O30 (RE = Sc, Y, Gd, Lu).31 Therefore, to widen transmission range, it is speculated that the integration of rare earth cations exhibiting a conspicuous absence of d–d or f–f electron transitions, with germanates characterized by a diminished phonon energy, emerges as a promising avenue. This strategic approach not only preserves the distorted structural environments but also facilitates a favorable extension of the transmission range from UV to IR wavelengths.
Inspired above, we have successfully incorporated rare earth cations Y3+ and Gd3+ into germanates and extracted two novel NLO crystals, Cs3REGe3O9 (RE = Y, Gd) (hereinafter designated as CYGO and CGGO), through spontaneous nucleation. The structure of Cs3GdGe3O9 was initially documented in 2019,32 yet hitherto, the investigation of its NLO properties and the correlation between its structure and properties has remained unexplored. Expectedly, these Cs3REGe3O9 (RE = Y, Gd) crystals display an exceptionally wide transparency range. Notably, their ultraviolet cutoff edges, located at 210 and 215 nm respectively, represent the shortest UV wavelengths reported to date among the NLO boron-free germanates, while their IR cutoff edges extend beyond 6.8 μm. Moreover, these compounds feature good thermal stability and exhibit a moderate SHG activity, comparable to that of KDP. To gain deeper insights into the structure–property relationships of CYGO and CGGO, we performed comprehensive electronic structure analyses using density functional theory (DFT).
Experimental section
Synthesis and powder X-ray diffraction (PXRD)
The raw materials used in the experiments were all untreated: Cs2CO3 (Aladdin, 99.9%), Y2O3 (Aladdin, 99.9%), Gd2O3 (Aladdin, 99.9%), GeO2 (Aladdin, 99.9%). CsF (Aladdin, 99.9%), Bi2O3 (Aladdin, 99.9%), PbO (Aladdin, 99.9%). The polycrystalline of Cs3REGe3O9 (RE = Y, Gd) were synthesized utilizing the conventional high-temperature solid phase method. The raw materials were meticulously weighed according to specific stoichiometric ratios. Subsequently, the mixtures underwent thorough grinding and were preheated in a muffle furnace at 350 °C for a duration of 12 hours. Gradually, the temperature was heated up to 950 °C and sustained for a minimum of 48 hours, with intermittent grinding incorporated throughout the synthetic process. Room temperature PXRD measurements were conducted on the polycrystalline powders of Cs3REGe3O9 (RE = Y, Gd) using a SMartLab9 KW X-ray diffractometer. The measurements utilized a Cu-targeted Kα ray and encompassed a 2θ range spanning from 10–70°, with a set step size of 0.01° and a step time of 2 s.
Thermal properties
Thermogravimetric (TG) and differential scanning calorimetric (DSC) analyses were implemented on polycrystalline powders of the Cs3REGe3O9 (RE = Y, Gd) compounds using a NETZSCH STA 449F5 thermoanalytical instrument. A limited quantity of samples was placed in a closed alumina crucible, which was heated up to 1200 °C at a heating rate of 10 °C min−1 and then cooled to room temperature at the same rate under a nitrogen-protective atmosphere.
Crystal growth
Single crystals of Cs3REGe3O9 (RE = Y, Gd) were extracted by the high temperature solution method. The polycrystalline materials and mixed fluxes CsF–Bi2O3–PbO were placed in platinum crucibles and positioned within resistance furnaces. The temperature was gradually elevated to 900 °C and sustained for a duration of 12 hours to ensure the attainment of a uniform solution. Subsequently, the temperature was systematically reduced to 650 °C at a cooling rate of 3–5 °C per hour, followed by an additional descent to room temperature at a rate of 20 °C per hour. Ultimately, the Cs3REGe3O9 (RE = Y, Gd) crystals were successfully obtained.
Structure determination
The single crystal X-ray diffraction analysis of CYGO and CGGO was executed on a Bruker SMART APEX II 4K CCD diffractometer. The diffraction experiments were carried out by employing Mo Kα radiation at a constant temperature of 297(2) K. The collected data were integrated using the SAINT program,33 and the crystal structure was solved directly using the SHELXTL program,34 which was used to improve the agreement between the calculated structure factors and the actual observations (Shelxt/XL), based on the full-matrix least squares method. The agreement between the calculated structure factors and the actual observations (Shelxt/XL) was used to determine the positions of the atoms in the initial structure, and the PLATON program was used to determine the structural alignment. Elaborated crystal parameters and refined structural data are comprehensively presented in the ESI,† including refined atomic positions, isotropic displacement parameters, bond lengths, and bond angles, documented in Tables S1–4.†
Energy-dispersive spectroscopy (EDS) measurements
The CYGO and CGGO samples were analyzed using a field emission scanning electron microscope equipped with energy dispersive X-ray spectrometry.
Spectroscopy characterizations
The UV-vis-NIR diffuse reflectance spectra of the CYGO and CGGO samples were acquired at ambient temperature using a Hitachi UV-vis-NIR spectrophotometer, operating in the wavelength range of in the range 190–2000 nm, with barium sulfate as the reference sample. The IR spectra of the target samples were recorded employing a Nicolet iS50 FT-IR spectrometer. The recorded spectra encompassed wavelengths within the range of 400–4000 cm−1.
Second harmonic generation (SHG) measurements
According to the method proposed by Kurtz and Perry,35 the powder SHG responses of CYGO and CGGO were investigated by employing a Q-switch laser at the light source 1064 nm. The strength of the SHG response of a compound is contingent upon its particle size dimensions. To elucidate this relationship, the CYGO and CGGO samples were sieved into discrete particle size ranges: 53–75, 75–106, 106–120, 120–150, 150–180, and 180–212 μm. For the purpose of conducting a comparative analysis, KDP was employed as a reference sample within the identical particle size range.
Birefringence measurements
Birefringence, a pivotal characteristic of NLO materials, was assessed via the quartz wedge method, in accordance with the compensatory color principle. Regular crystals were employed in the visible range by using a Nikon Eclipse E200MV polarizing microscope. The experimental birefringence was quantified using the formula R = |Ne − No| × d = Δn × d, where Δn, R, and d represent the experimental birefringence, the optical range difference, and the corresponding thickness of the test crystal, respectively. The thickness of the selected CYGO and CGGO crystals was ascertained using a Bruker SMART APEX III CCD diffractometer. Also, based on the techniques provided by previous literature, we can deduce the color and order of interference exhibited by the crystals.36
Structure–prop-erty relationship
In order to elucidate the electronic structures and optical properties of CYGO and CGGO, we employed the CASTEP package,37 which is grounded in the principles of density functional theory (DFT).38 To achieve this, the crystal structures of CYGO and CGGO were optimized by employing the Perdew–Burke–Ernzerhof (PBE) exchange–correlation functional, bolstered by the generalized gradient approximation (GGA).39 In the calculations, we assigned Cs 5s25p66s1, Y 4d15s2, Gd 5d16s2, Ge 4s24p2, and O 2s22p4 as the valence electrons for the respective atoms in CYGO and CGGO. The theoretical calculations were conducted with the aid of experimental single-crystal structural data for CYGO and CGGO. The kinetic energy cutoff (810 eV) and Monkhorst–Pack k-point meshes (3 × 6 × 3) were employed to ensure the adequate accuracy of the simulated results.
Results and discussion
Synthesis and thermal properties
The polycrystalline samples of CYGO and CGGO were obtained by a high-temperature solid phase reaction process. Fig. 1a and b evidently illustrates that the experimental PXRD patterns of CYGO and CGGO are in good agreement with those observed in theoretical results, thereby attesting to their high purity. Furthermore, DSC thermal analysis conducted over a temperature range of 40–1200 °C revealed a conspicuous absence of absorption peaks in both CYGO and CGGO as presented in Fig. 1c and d. Meanwhile, the corresponding TG curves exhibited negligible weight loss, underscoring the extraordinary thermodynamic stability of CYGO and CGGO, which surpasses 1200 °C. Furthermore, the examinations of CYGO and CGGO were carried out through a variable temperature XRD analysis, spanning a temperature range of 950–1300 °C, as depicted in Fig. 1e and f. Notably, the XRD patterns of both compounds exhibited stability until reaching a temperature threshold of 1250 °C, which further validates the soundness of the thermal analyses. An in-depth analysis of the PXRD spectra of the CYGO and CGGO samples after calcination at 1250 °C (Fig. S1†), thus substantiating that these two target compounds possess a distinctive incongruent melting behavior.
 |
| Fig. 1 (a and b) Experimental and theoretical PXRD patterns of CYGO and CGGO; (c and d) TG-DSC curves of CYGO and CGGO; (e and f) the PXRD patterns evolution of CYGO and CGGO polycrystalline pure phases under elevated temperature conditions. | |
Structural analyses
CYGO and CGGO crystals were cultivated through the high-temperature solution method utilizing mixed fluxes CsF–Bi2O3–PbO. Small crystals of regular shape and high quality are selected for single crystal measurements analysis. The structure of CGGO was initially reported in 2019.32 To investigate the correlation between structure and performance, its crystal structure was reconfirmed. The detailed crystallographic data, along with the corresponding experimental condition are given in Table 1. It was ascertained that CYGO and CGGO are isomorphic, crystallizing in the orthorhombic space group Pna21 (no. 33). The unit cell parameters for these two crystals determined as follows: a = 13.7994(3) Å, b = 7.1087(2) Å, c = 12.7190(3) Å and Z = 4 for CYGO; and a = 13.908(3) Å, b = 7.1769(17) Å, c = 12.8026(5) Å and Z = 4 for CGGO, respectively. Since the structures of these two compounds exhibit isomorphism, the as-synthesized CYGO was selected as the representative to expound upon their structural characteristics. The asymmetric unit of CYGO comprises one crystallographically independent Y site, three Ge sites, three crystallographically distinct Cs sites, and nine oxygen sites. As depicted in Fig. 2a, each Y3+ cation is ligand linked to six oxygen atoms, forming distortive octahedra [YO6], with the Y–O bond lengths varying within the range of 2.241(6)–2.281(6) Å. A Ge4+ cation is coordinated with four oxygen atoms, resulting in the formation of tetrahedra [GeO4], characterized by bond lengths ranging from 1.712(6) to 1.789(6) Å. Notably, the adjacent [GeO4] tetrahedra are interconnected with each other to form [Ge6O19] short zigzag chains, which extend infinitely along the c-axis (Fig. 2b). The separated [YO6] octahedra are evenly distributed throughout the structural space and play a connecting role. As clearly illustrated in Fig. 2c, the neighboring [Ge6O19]∞ zigzag chains are interconnected by the [YO6] octahedra, giving rise to quasi-planar structures. Subsequently, these quasi-planes further interconnect to construct a three-dimensional (3D) framework (Fig. 2d). All the Cs atoms occupy the voids to maintain charge balance.
 |
| Fig. 2 (a) Structural motifs [Ge4], [YO6], [GdO6] of Cs3REGe3O9; (b) [Ge6O19] short-chain unit; (c) quasi-planar structures of Cs3REGe3O9 paralleled to the ac plane, and (d) 3D framework structure of Cs3REGe3O9. | |
Table 1 Crystal data and structure refinements for CYGO and CGGO
R
1 = ∑||Fo| − |Fc||/∑|Fo|; wR2 = [∑w(Fo2 − Fc2)2/∑w(Fo2)2]1/2.
|
Empirical formula |
Cs3YGe3O9 |
Cs3GdGe3O9 |
Formula weight |
849.41 |
917.75 |
Crystal system |
Orthorhombic |
Orthorhombic |
Space group |
Pna21 |
Pna21 |
a (Å) |
13.7994(3) |
13.908(3) |
b (Å) |
7.1087(2) |
7.1769(17) |
c (Å) |
12.7190(3) |
12.826(3) |
Volume (Å3) |
1247.68(5) |
1280.3(5) |
Z
|
4 |
4 |
Density (g cm−3) |
4.522 |
4.761 |
Crystal size (mm3) |
0.074 × 0.050 × 0.038 |
0.19 × 0.07 × 0.06 |
Completeness |
100% |
100% |
R (int) |
0.033 |
0.072 |
GOF on (F2) |
1.065 |
1.112 |
Final R indices [I > 2σ(I)]a |
R
1 = 0.0290, wR2 = 0.0646 |
R
1 = 0.0505, wR2 = 0.1281 |
R indices (all data) |
R
1 = 0.0322, wR2 = 0.0663 |
R
1 = 0.0530, wR2 = 0.1299 |
CCDC number |
2293196
|
2293197
|
To validate the rationality of the structural analysis, the bond valences of various atoms in CYGO and CGGO were calculated. The resulting valence states for the elements Y/Gd, Ge, Cs, and O were determined to be 3.11/3.15, 3.95–4/3.79–4.06, 0.81–1/0.77–1.27, and 1.89–2.06/1.80–2.17, respectively, which agree well with those derived from the structural data. Additionally, the elemental compositions and mapping of these two compounds were analyzed through EDS measurements as presented in Fig. S2 and 3.† The ratios of Cs/Y/Ge/O in CYGO and Cs/Gd/Ge/O in CGGO are found to be 3.3/1/2.8/11.6, and 3.1/1/3.2/12.9, respectively. These observations align remarkably well with the atomic molar ratio of their structures, providing further evidence for the rationality of the proposed structure.
Spectroscopy characterizations
The UV-vis-NIR spectrum of the CYGO and CGGO compounds are deposited in Fig. 3a and b. It's worth noteworthy that both CYGO and CGGO exhibit remarkable UV cut-off edges at 210 nm and 215 nm, respectively, accompanied by wide band gaps of 4.92 and 5.3 eV, as determined through the Kubelka–Munk formula.40 Comparisons made as in Fig. 3e, to the best of our knowledge, these UV cut-off edges represent the shortest reported among boron-free germanate-based NLO crystals. Moreover, the IR spectrum analyses, illustrated in Fig. 3c and d, reveal the absence of conspicuous absorption within a broad range of 3500–731 cm−1 for both CYGO and CGGO. Accordingly, these two crystals demonstrate transparency cover a wide spectral range spanning 3–6.8 μm, as determined by the two-phonon approximation, thereby presenting a favorable prospect for mid-IR NLO applications. The specific vibrational modes of the infrared absorption peaks are shown in Table S5.† Based on the aforementioned observations, it becomes apparent that the transmission range of both crystals almost covers the pivotal solar-blind region, along with the 3–5 μm mid-IR atmospheric transmission window. These findings strongly suggest the potential suitability of these crystals as NLO materials in a wide transmission window from UV to mid-IR wavelengths. A comprehensive comparison of the band gap and UV cut-off of various boron-free germanate-based NLO materials is presented in Table 2.
 |
| Fig. 3 (a and b) UV-vis-NIR diffuse reflectance spectra of the CYGO and CGGO, respectively; (c and d) IR spectrum of the CYGO and CGGO, respectively; (e) comparison of the UV cutoff edge among the boron-free germanate-based NLO crystals (* refers to compounds derived from this work). | |
Table 2 Comparison of the UV cutoff edge among the boron-free germanate-based NLO crystals
Compounds |
Crystal system |
Space group |
Bandgap (eV) |
UV cut-off (nm) |
Structural units |
N/A: not reported or unavailable. |
Rb2ZnGeO6 41 |
Orthorhombic |
C2221 |
3.22 |
370 |
GeO4 + ZnO4 |
K2ZnGeO6 42 |
Orthorhombic |
C2221 |
3.23 |
368 |
GeO4 + ZnO4 |
Cs2Bi2O(Ge2O7) 23 |
Orthorhombic |
Pca21 |
3.15 |
357 |
Bi2O8 + Ge2O7 |
PbTeGeO6 43 |
Trigonal |
P31m |
3.36 |
300 |
Te/GeO6 + PbO6 |
Ba2TiGe2O8 44 |
Orthorhombic |
Cmm2 |
3.14 |
300 |
Ge2O7 + TiO5 |
K3Nb3Ge2O13 45 |
Hexagonal |
P c2 |
3.75 |
287 |
Ge2O7 + Nb3O15 |
Li2K4TiOGe4O12 46 |
Tetragonal |
P4nc |
4.43 |
280 |
TiO5 + GeO4 |
Rb4Li2TiOGe4O12 47 |
Tetragonal |
P4nc |
N/A |
280 |
TiO5 + GeO4 |
Cs3TbGe3O9 39 |
Orthorhombic |
Pna21 |
3.4 |
280 |
GeO4 + TbO6 |
KNbGe3O9 45 |
Hexagonal |
P 2c |
4.59 |
270 |
Ge3O9 + NbO6 |
Pb3TeGa2ZnGe2O14 48 |
Trigonal |
P321 |
4.67 |
265 |
GeO4 + Ga/ZnO4 + TeO6 + PbO8 |
Ca3Ga2Ge4O14 44 |
Trigonal |
P321 |
N/A |
260 |
GeO4 + GeO6 + GaO4 |
Ba3TeZn2Ge3O14 49 |
Trigonal |
P321 |
3.98 |
249 |
GeO4 + ZnO4 + TeO6 + PbO8 |
Li2GeTeO6 50 |
Trigonal |
R3 |
4.65 |
240 |
GeO6 + TeO6 |
La3Ga5GeO14 44 |
Trigonal |
P321 |
N/A |
240 |
GeO4 + LaO8 + GaO6 + GaO4 |
Li3Cs3Ge6O15 51 |
Orthorhombic |
Pca21 |
3.23 |
220 |
GeO4 |
CGGO this work |
Orthorhombic |
Pna21 |
5.1 |
215 |
GeO4 + GdO6 |
CYGO this work |
Orthorhombic |
Pna21 |
4.82 |
210 |
GeO4 + YO6 |
Second-harmonic generation measurement
As CYGO and CGGO crystallize into the non-centrosymmetric (NCS) structure, powder SHG measurements were conducted employing KDP samples as a reference, following the well-established Kurtz–Perry method. As depicted in Fig. 4a and b, the SHG intensities of CYGO and CGGO demonstrate a progressive enhancement as the particle size of the polycrystalline powder increases, ultimately attaining saturation. This phenomenon unequivocally signifies their inherent phase matching behavior. Furthermore, within the particle size range of 180–212 μm, CYGO and CGGO exhibit commendable SHG intensities, approximating that of 0.7 × KDP. Also, the SHG performance of CYGO and CGGO is compared to many other germanate-based oxide crystals, such as Rb2ZnGeO6 and K2ZnGeO6.
 |
| Fig. 4 (a and b) The phase-matched patterns and SHG intensity of CYGO and CGGO with the practical KDP as a reference, respectively. | |
Birefringence properties
The experimental determination of birefringence values for CYGO and CGGO was performed through the utilization of the quartz wedge method. As illustrated in Fig. 5a–f, the thickness of these examined crystals was discerned to be 26.3 and 18.3 μm, respectively. The optical path difference of the Cs3REGe3O9 (RE = Y, Gd) crystals was found to be 489 and 442 nm, respectively, under visible light wavelength. An initial first-order orange hue was ascertained through the control Michal-Levy interferometric chromatogram. Employing the birefringence formula R = |Ne − No| × d = Δn × d, the visible region yielded experimental birefringence values of 0.0186 and 0.0241 for CYGO and CGGO, respectively. These birefringent tendencies exhibited by CYGO and CGGO align favorably with those of other germanate-based crystals, such as Rb2ZnGeO6 (0.019 @ 1 μm), Y2Ge2O7 (0.028 @1064 μm)44 and K2ZnGeO6 (0.017 @1064 μm),42 Li2Ge7O15 (0.018 @1064 μm).
 |
| Fig. 5 (a–c) The original interference color, extinction and thickness of the CYGO crystal, respectively; (d–f) the original interference color, extinction and thickness of the CGGO crystal, respectively. | |
Theoretical calculations
To unravel the underlying optical origin of the target compounds, an analysis of the electronic structure was performed via first-principles calculations. Given the isomorphic nature of the crystal structures of CYGO and CGGO, CYGO was selected as the representative for conducting the theoretical examination. As delineated in Fig. 6a, the apex of the valence band manifests at the X position, while the lowest point of the conduction band emerges at the G position, signifying CYGO to be an indirect band gap compound with a gap width of 4.9 eV. Additionally, as depicted in Fig. 6b, the density of states reveals that the energy range of −5 to 0 eV is largely constituted by Y 4d, Ge 4s 4p, and O 2p orbitals. Likewise, the Cs 5p and O 2p orbitals account for the states spanning −10 to −5 eV, while the energy range of 10–15 eV is predominantly attributable to Ge 4s 4p and O 2s 2p orbitals. Considering that electronic states proximate to the Fermi level wield considerable influence over the optical properties of compounds, it can be concluded that the [YO6] and [GeO4] units play pivotal roles in the NLO and birefringent characteristics of the CYGO crystal.
 |
| Fig. 6 (a) The bandgap structure of CYGO; (b) the TDOS and PDOS of CYGO. | |
Conclusions
In summary, by employing the structural gene engineering, we have cultivated two novel NLO germinate-based crystals, Cs3REGe3O9 (RE = Y, Gd) using a flux method. These compounds exhibit structural isomorphism, forming a 3D framework composed of [YO6]/[GdO6] octahedra and [GeO4] tetrahedra. Notably, Cs3REGe3O9 (RE = Y, Gd) possesses the shortest UV cutoff edges among boron-free germinate-based NLO materials, with values of 210 nm and 215 nm, respectively. Remarkably, IR analyses revealed that these crystals display expansive transmission regions extending beyond 6.8 μm. Moreover, Cs3REGe3O9 (RE = Y, Gd) exhibit a moderate SHG intensity, comparable to that of KDP. Additionally, theoretical analyses have elucidated the pivotal role played by the [YO6]/[GdO6] and [GeO4] units in governing the observed NLO and birefringent properties of Cs3REGe3O9 (RE = Y, Gd). With these favorable attributes, Cs3REGe3O9 (RE = Y, Gd) emerge as prospective contenders for NLO applications spanning the UV to IR region., thereby forging a path toward the exploration of novel NLO crystals endowed with a broad transmission window.
Conflicts of interest
There are no conflicts to declare.
Acknowledgements
This work was financially supported by the National Natural Science Foundation of China (Grant No. 52002273, 61835014 and 51890864), National Key R&D Program of China (2021YFA0717800).
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Footnote |
† Electronic supplementary information (ESI) available: Additional crystallographic data for Cs3REGe3O9 (RE = Y, Gd), selected PXRD spectra and analysis of the vibrational modes of the absorption peaks in the infrared spectra. CCDC 2293196 and 2293197. For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d3qi01807e |
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