Wenxuan
Li
a,
Guoying
Yao
ab,
Yilan
Zhang
a,
Lingjiao
Zhang
c,
Sujuan
Hu
c,
Chuan
Liu
c,
Baiquan
Liu
c,
Tao
Zeng
b and
Zhenyu
Yang
*ad
aMOE Laboratory of Bioinorganic and Synthetic Chemistry, Lehn Institute of Functional Materials, School of Chemistry, IGCME, Sun Yat-sen University, Guangzhou, Guangdong 510275, China. E-mail: yangzhy63@mail.sysu.edu.cn
bDepartment of Chemistry, York University, Toronto, ON, Canada M3J 1P3
cState Key Laboratory of Optoelectronic Materials and Technologies, School of Electronics and Information Technology, Sun Yat-sen University, Guangzhou, 510275, China
dNanchang Research Institute, Sun Yat-sen University, Nanchang, Jiangxi 330096, China
First published on 2nd October 2023
Reduced-dimensional (RD) metal halide perovskites (MHPs) have received much attention from scientific researchers for their highly tunable optoelectronic properties and solution processability. To date, the large cation candidates for constructing RD MHPs have mostly been selected from the organoamine/organoammonium salt family which is commercially available. We previously reported a straightforward approach for preparing new types of RD perovskites based on the organothiol redox or condensation reactions on the organic cations (Yuan et al., CCS Chem., 2022, 3, 1276–1284). Here, we further apply the synthetic strategy to prepare two new series of Dion–Jacobson (DJ) type RD MHPs with dithioketal-containing intercalating cations. The single-crystal X-ray crystallography and spectroscopic results indicate the evolution of the distortion of the RD structures and the photophysical behaviors following the increase in the inorganic components. The materials are solution processable for near-infrared light-emitting diode application, and the best device emitting at 746 nm achieved an EQE of 2%.
Conventional hybrid MHPs consist of a three-dimensional (3D) framework and share a general chemical formula ABX3, where A is a monovalent cation such as methylammonium (CH3NH3+, MA), formamidinium (CH(NH2)2+), or Cs+, B is a divalent metal cation (e.g., Pb2+ or Sn2+), and X represents a halide group such as Cl−, Br−, and I−. When small A-site cations are fully or partially substituted by large organic cations (e.g., long-chain aliphatic or aromatic organoammonium cations), the original 3D framework is cleaved into a reduced-dimensional (RD) structure with layered, localized two-dimensional (2D) frameworks intercalated between two 3D MHP components. The intercalating organic cations between MHP layers introduce quantitatively appreciable van der Waals (vdW) interactions, which in turn increase the formation energy of MHPs, thus improving the material and device stability.8–10 The formation of octahedral-layer-based quantum wells promotes radiative recombination, thus enabling the efficient luminescence of RD MHPs.11,12
The dimensionality of RD MHPs can be continuously tuned by mixing stoichiometric quantities of precursors such as lead iodide (PbI2), MAI, and organoammonium iodide (RI, where R = large organic cation) to yield compounds with different numbers of layers (n) in the series Rx(MA)n−1PbnI3n+1. In this structure, n indicates the thickness of (PbI42−) octahedral sites, and thus, n = 1 corresponds to a 2D structure, and the compounds with n > 1 correspond to RD MHPs; x corresponds to the number of large organic cations inserted in the unit cell, which is dependent on the type of RD MHP. Dion–Jacobson (DJ) type MHP is a relatively new member of the RD MHP family. In DJ MHPs, the quantum wells are constructed based on the intercalation of divalent organic cations (e.g., organodiammonium cations) between two adjacent inorganic frameworks. Because there is only a single layer of organic cations that serve as the organic ligands, DJ type MHPs have thinner walls between two quantum wells, which are believed to have better charge transport function along the reduced dimension compared to other types of RD MHPs.
To date, the cations for constructing DJ type MHPs have been limited13–15 as most of the reported DJ MHPs with well-defined structures are prepared based on co-crystallization approaches using metal halides and diammonium salts as the precursors.16,17 However, the number of commercially available organic diammonium salts is limited, and the synthesis of the target cations is somewhat challenging. A general approach to preparing diammonium salts for constructing new types of DJ MHPs is highly desired.
The recently introduced post-synthetic crystal conversion method via organothiol-based chemistry is a promising approach to explore new RD MHP structures.1,18,19 The crystal formation and conversion are driven by the highly reactive thiol end groups on the intercalating cations, which can effectively convert to disulfide and dithioketal structures when interacting with oxidative reagents and ketones, respectively. In recent years, compared with traditional 3D perovskite, the operational stability of reduced dimensional (RD) perovskite and its optoelectronic devices has dramatically improved, attracting research interest worldwide.9,20 In this study, we take a step forward to explore new RD MHPs with well-defined single-crystal structures based on two types of dithioketal-containing cations: 2,2′-(methylenebis(sulfanediyl))bis(ethan-1-aminium) (MSBA) and 2,2′-(propane-2,2-diylbis(sulfanediyl))bis(ethan-1-aminium) (PDSBA) cations. Single-crystal analyses indicate that the concentration of the intercalating cations within the RD MHP lattice regulates the degrees of distortion and the stacking modes of the inorganic components. Combined computational and photophysical studies further confirm the highly tunable electronic structures following the increase in thickness of the inorganic layers. Like other RD structures, these two series of DJ MHPs can be processed using solution-based processes to prepare uniform thin films for LED applications. The best device exhibits EQE peak values of up to 2.0%.
Both series of DJ type MHPs crystallize in similar layered structures with a corner-sharing (PbI6)4− octahedral network. However, the degree of distortion of the inorganic layers varies depending on both the type of the cation and the n value. To better visualize the distortion of octahedral sites, we classify the Pb–I–Pb angles into two types, the axial (i.e., along the longest unit cell axis) and the equatorial (i.e., along the inorganic plane) angles (Fig. 2a). The increased thickness of the inorganic layers results in an increase in equatorial Pb–I–Pb angles in both series of RD MHPs from 153.2° ((MSBA)PbI4) and 147.6° ((PDSBA)PbI4) to 156.9° ((MSBA)(MA)2Pb3I10) and 155.1° ((PDSBA)(MA)2Pb3I10), which gradually converge to the bulk MHP crystals (i.e., 160° for MAPbI3, Fig. 2b). Consistent with other reported DJ MHP structures,21–25 the distortion of the inorganic layer gradually decreases for both series of DJ type MHPs following the increase in the n value (Fig. 2c). The axial Pb–I–Pb angles are always close to the bulk phase value of 180°; the linearity of the axial Pb–I–Pb alignment is maintained, regardless of the thickness of the 2D framework.
We next investigated the interaction between the diammonium cations and the inorganic layers, which is primarily due to the strong electrostatic interaction between the ammonium end groups and two types of I atoms on the boundary of the inorganic layer, i.e., the terminal I and the bridging I atoms (Fig. 2d). The distances between the H atom on the NH3+ groups and the adjacent I atoms are shown in Fig. 2e (ranging from 2.69 Å to 3.05 Å), which are shorter than the summation of the van der Waals radii of H and I atoms (ca. 3.1 Å) and thus can be attributed to the formation of hydrogen bonds. Following the increase in the n value, the distance between the H atom and the terminal I atom increases (from 2.75 Å to 2.97 Å for the MSBA series and from 2.83 Å to 3.03 Å for the PDSBA series). We ascribe this to the gradual reduction of in-plane distortion of the inorganic layer, which is in good agreement with the equatorial Pb–I–Pb angles mentioned above. The distortion allows more flexibility in the interface configuration and hence allows stronger hydrogen bonds between the surface I and the ammonium end groups.
The optical band gaps of the single crystals are shown in Fig. 3c. Similar to other reported RD structures,12,22,26 the increase in the n value results in the reduced bandgap of both types of DJ structures (MSBA: n = 1, 2.20 eV; n = 2, 2.02 eV; n = 3, 1.81 eV and PDSBA: n = 1, 2.29 eV; n = 2, 2.04 eV; n = 3: 1.83 eV). The bandgaps of (PDSBA)PbI4 are slightly larger than those of (MSBA)PbI4. This is expected because the distances between the inorganic layers of the MSBA series (from 5.93 to 5.64 Å) are significantly larger than those of the PDSBA series (from 7.36 to 7.04 Å), see Fig. 3d. Larger distances reduce the interlayer interaction, which is mediated by the organic cations, and hence reduce the widths of the valence band and the conduction band. Consequently, the band gap is enhanced.
To gain insight into the electronic structures of RD MHPs, we turned to density functional theory (DFT) calculations. The calculated density of states (DOS) and atomic projected density of states (pDOS) are shown in Fig. 4. The calculated band gaps (MSBA: n = 1, 2.10 eV; n = 2, 1.88 eV; n = 3, 1.88 eV and PDSBA: n = 1, 2.20 eV; n = 2, 2.07 eV; n = 3, 1.90 eV) are in good agreement with the aforementioned optical bandgaps and the literature, where the band gaps of the MSBA series are systematically smaller than those of the PDSBA series. The bandgap of ∼1.88 eV for n = 2, 3 of the MSBA series shall not bother us. Despite the identical gaps, the DOS at the conduction band minimum is undoubtedly more pronounced for the n = 3 structure, indicating the trend of band gap reduction. It is important to note that both the CBM and valence band maximum (VBM) are dominated by lead and iodide atoms in the inorganic layer of both types of MHPs regardless of the n value, suggesting that the I and Pb atoms are primarily responsible for conducting holes and electrons in both series of DJ structures. Similar to the RD MHPs,26 the VB and CB DOS are increasingly dominated by the pDOS of I and Pb atoms following the increase in the n value in both series of MHPs, suggesting that the inorganic components (i.e., the PbnI3n+1 layers) serve as the main charge transport media.
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Fig. 4 Electronic properties of PDSBA-based and MSBA-based MHPs. DOS and pDOS plots of (a) (MSBA)(MA)n−1PbnI3n+1 and (b) (PDSBA)(MA)n−1PbnI3n+1, where n = 1–3. |
To further understand the distribution of organic and inorganic components in the layered structures, we prepared a series of MHP polycrystalline films via a spin-cast process (see the Experimental section for more details). The powder X-ray diffraction (PXRD) results show distinct patterns of (h00), (0k0), and (00l) orientations for MSBA-based and PDSBA-based films with 〈n〉 values below 3, respectively (Fig. 5a and d), indicating that the inorganic components are oriented parallel to the substrate.10,27,28 Overall, the growth orientation of the layered structures with low 〈n〉 values is similar to the commonly reported RD MHPs,26 suggesting that these MHPs undergo a similar kinetic process during the polycrystalline film formation. As for the polycrystalline films with 〈n〉 values above 3, the PXRD results show the emergence of multiple signals that cannot be assigned to any specific RD phase, indicating the coexistence of layered inorganic components with different thicknesses and random growth orientations. Two intense signals at 14.2° and 28.5° can be found from the MHP films with 〈n〉 = 2, 3, and 5, which can be assigned to the (110) and (220) lattice planes of the bulk-like inorganic layers.29 These features indicate the presence of perpendicular-standing inorganic components, which are believed to benefit the charge transport of the MHP thin films for photovoltaic and light-emitting applications.30
To experimentally confirm the photophysical properties of the DJ type polycrystalline film, we measured the absorption and photoluminescence (PL) spectra of the MHP thin films. A red-shift of the absorption edge is observed for both MSBA-based and PDSBA-based MHPs following the increase in the 〈n〉 value (MSBA: from 539 nm (〈n〉 = 1) to 721 nm (〈n〉 = 5) and PDSBA: from 531 nm (〈n〉 = 1) to 739 nm (〈n〉 = 5), Fig. 5b and e). These results are expected due to the increase in the thickness of the inorganic layers and are consistent with the trend of the calculated electronic band gaps. Small absorption features at 565 nm and 555 nm, found from the spectra of the samples with 〈n〉 = 3 and 5, can be assigned to the distinctive (MSBA)(MA)Pb2I7 and (PDSBA)(MA)Pb2I7, respectively. These absorption features confirm the coexistence of layered structures with different thicknesses. The absorption edges are shifted to 721 nm and 739 nm for (MSBA)(MA)4Pb5I16 and (PDSBA)(MA)4Pb5I16, respectively, which are dominated by the bulk-like absorption feature at 760–780 nm,26 consistent with RD MHPs with other large organic cations.22
Comparison of the absorption and PL spectra clearly shows a regular Stokes shift in the emission of (MSBA)PbI4 and (PDSBA)PbI4 thin films, consistent with other reported DJ type MHP structures.22 As for (MSBA)PbI4, two emission maxima are present in the PL results. The dual emission maxima may result from self-trapped excitons (STEs) which are dependent on lattice deformation, involving interactions between inorganic skeletons and organic cations to consequently affect electron–phonon coupling.31,32 Due to the decrease in the bandgap, an evident red-shift of the PL maxima can be clearly seen from those thin films following the increase in the 〈n〉 value (MSBA: from 529 nm to 737 nm and PDSBA: from 522 nm to 755 nm, Fig. 5c and f). The corresponding PL spectra also show the compositional evolution of the assembly of the inorganic components with various thicknesses of the inorganic layer. Specifically, a more rapid red-shift of the PL signals was observed from the thin film samples of the PDSBA series following the increase in the 〈n〉 value compared to their MSBA-based counterparts (Fig. 5c and f). This may be because of the difference in the population distribution of quantum well thicknesses within those thin films.11,12 It is therefore reasonable to speculate that the PDSBA cations assist in the formation of multicrystalline thin films containing RD MHP domains with a narrower distribution of n values.28
The evolution of the emission patterns of the DJ type MHPs with relatively large 〈n〉 values (e.g., 〈n〉 = 3 and 5) drove us to further investigate the corresponding electroluminescence (EL) of those MHPs in the near-infrared region. We constructed LEDs with the architecture shown in Fig. 6a.33 ZnO nanoparticles (NPs) and poly-(9,9-dioctylfluorenyl-2,7-diyl)-alt-(4,4′-(N-(4-butylphenyl))) (TFB) were used as the electron transport layer (ETL) and hole transport layer (HTL), respectively. Cross-sectional scanning electron microscopy (SEM) imaging revealed that the thicknesses of the layers of ZnO NPs, MHP films, and TFB are around 30 nm, 175 nm, and 35 nm, respectively (Fig. S6†).
We next investigated the performance of the corresponding devices. The EL maxima of all devices were around 671 nm and 746 nm (Fig. 6b), an approximately 0–38 nm blue-shift with respect to the corresponding PL spectra.34 We obtained the champion device based on 〈n〉 = 5 PDSBA-based MHP devices with a relatively low turn-on voltage of 1.5 V (Fig. 6d). The EQE maximum of the corresponding device was 2.0% at 2.0 V with a current density of ∼140 mA cm−2 (Fig. 6c), and a radiance value of 25 W sr−1 cm−2 (corresponding radiant flux: 6.3 × 10−4 W) was achieved at 2.4 V.
Footnote |
† Electronic supplementary information (ESI) available. CCDC 2249121, 2249140–2249143. For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d3qi01512b |
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