Fang
Lin
a,
Guicheng
Yu
a,
Shuchen
Weng
a,
Chao
Zhou
ab,
Yonglei
Han
ab,
Wei
Liu
c,
Kang
Zhou
a,
Yongfei
Wang
b and
Haoran
Lin
*a
aHoffmann Institute of Advanced Materials, Shenzhen Polytechnic, 7098 Liuxian Blvd, Nanshan District, Shenzhen, 518055, China. E-mail: hlin@szpt.edu.cn
bSchool of Materials and Metallurgy, University of Science and Technology Liaoning, 185 Qianshan Zhong Road, Anshan, 114051, China
cSchool of Chemical Engineering and Technology, Sun Yat-Sen University, Zhuhai, 519000, China
First published on 8th November 2022
Low-dimensional organic–inorganic metal halide hybrids exhibit promising optical properties for light emitting applications. However, developing lead-free blue-light emitters with high photoluminescence quantum efficiency (PLQE) remains an ongoing challenge. In our work, a novel zero-dimensional (0D) indium hybrid compound (MA)4InCl7 (MA = CH3NH3+) was developed which exhibited broadband blue emission with a PLQE of 11.2% when excited by ultraviolet (UV) light. More interestingly, upon Cs+ or Mn2+ doping, the emission of the 0D compound further blue-shifted and became narrower, while the PLQE was significantly enhanced to 18.8% (Cs+) or 20.7% (Mn2+). More prominent PLQE enhancement to 74.7% was observed after Sb3+ doping, which also altered the emission spectrum to the orange region. According to experimental characterization and theoretical calculations, we attribute the PLQE enhancement upon Cs+ and Mn2+ doping to defect passivation and the orange emission upon Sb3+ doping to altered emission centers. We have demonstrated that multiple metal ions possess the ability to improve the light emitting properties of 0D organic–inorganic metal halides, and (MA)4InCl7 could be utilized as a Sb3+ heavy metal ion sensor with high selectivity and sensitivity.
Zero-dimensional (0D) OIMHs comprising isolated inorganic polyhedrons and organic cations possess high structural versatility, color tunability and high photoluminescence quantum efficiency (PLQE) due to their quantum-confined structures, making them promising materials for luminescence applications.11 For example, a series of 0D hybrid materials, such as (C5H14N3)2MnBr4,12 (C10H16N)2MnBr4,13 (TMA)2SbCl5·DMF,14 (MePPh3)2SbCl5,15 (C12H28N)2SbCl5,16 and (C4N2H14Br)4SnBr6,17 were developed with various emission colors and near-unity PLQEs. To achieve the three primary colors, blue-emissive 0D OIMHs were also reported, mostly lead-containing compounds such as (BAPrEDA)PbCl6·(H2O)2,18 (C13H19N4)2PbBr4,19 and (C9NH20)7(PbCl4)Pb3Cl11.20 However, the toxicity of lead limits their development and applications. Lead-free blue emitters were developed using all-inorganic materials in which alkali copper(I) halides such as Cs3Cu2X5,21–23 Rb2CuX3,24 and K2CuX325 have shown extraordinary PLQYs of up to 100%. On the other hand, lead-free 0D OIMHs have also been massively investigated in recent years.26,27 Several reports suggest that the substitution of lead by indium is an effective strategy to develop lead-free blue emitters. For example, the PLQE of blue-emissive (C7H8N6)InCl9 with a long lifetime of 1.2 s can be enhanced from 25.2% to 42.8% upon illumination.28 BAPP4+-associated blue emission in BAPPIn2Cl10 endows it with intriguing afterglow properties.29 TpyInClx (x = 3 or 5) emitters were tuned to be blue-emissive and with an increased PLQE of up to 47.66% by regulating the polarity of the solvent.30 [H2EP]2InCl6·Cl·H2O·C3H6O and [H3AEP]InCl6·H2O peaking at 430 nm displayed a PLQY of 13.44% and 4.12%, respectively.31 (C14H22N)InBr4, isolated tetrahedral [InBr4]− separated by organic ligands, showed a visibly bright blue emission with a PLQE of 16.36%.32 Despite the recent advances of 0D indium OIMH blue emitters, their poor stability and relatively low PLQEs still remain problematic.
For low-dimensional OIMHs, metal ion doping is considered as an attractive and effective strategy to optimize their photoluminescence properties and enhance their stability. There are also several cases of doping Sb3+ in 0D indium OIMHs to simultaneously manipulate the emission spectrum and enhance the PLQE. Upon rational control of the Sb amount, both near-unity PLQEs and a bright white-light emission were achieved in (C7H8N6)InCl9,28 BAPPIn2Cl10,29 (C8NH12)6InBr9·H2O33 and InCl7(C4H10SN4).34 However, as far as we know, there are no reports on using metal ions other than Sb3+ to dope 0D indium OIMHs. The light-emitting mechanism upon ion doping is less explored. Also, exploration of the applications of metal ion doped 0D indium compounds is limited besides Kuang's29 and Chen's34 recent works which suggest that antimony doped indium compounds could be used as anti-counterfeiting materials and solvent sensors.
Here, we have synthesized a lead-free 0D indium-based OIMH (MA)4InCl7 (MA = CH3NH3+), which exhibits a bright broadband blue emission peaked at 455 nm with a PLQE of 11.2%. The metal ion doping strategy was applied to this material and a series of compounds including (MA)4InCl7:Cs+, (MA)4InCl7:Mn2+ and (MA)4InCl7:Sb3+ were obtained. Reduced full width at half maxima (FWHM) and increased PLQE (from 11.2% to 20.7%) have been achieved through introducing Cs+ or Mn2+ into the pristine material. Upon Sb3+ doping, (MA)4InCl7:Sb3+ exhibits significantly shifted orange STE emission and a greatly enhanced PLQE of up to 74.7%, which makes it a perfect sensor for Sb3+ ion sensing.
The calculated extent of distortion (λoct1 = 7.21 × 10−6, λoct2 = 6.82 × 10−7; σ2oct1 = 0.271, σ2oct2 = 0.264) is much smaller than those of the reported Sn2+-, Bi3+-, and Sb3+-based OIMHs because of the strongly antibonding nature of the ns orbitals of the later ones.36,37 In addition, the lattice parameters (Table S1, ESI†) and the extent of distortion of InCl63− for all doped compounds (Table S4, ESI†) are similar to those of the pristine compound, which indicate that a small amount of metal doping do not alter the crystal structure significantly. It is worth mentioning that Cs+ is observable in the experimental crystal structure of (MA)4InCl7:Cs+ in which Cs+ ions have substituted a small amount of MA+ (8% occupancy in each MA+), which improves the crystal symmetry leading to different space groups compared to the pristine compound. Nevertheless, the two crystals are still almost the same with similar atom positions, distances, compositions, etc., which is evidenced by the similarity of the area in the red dash line and unit cell of (MA)4InCl7:Cs+ in Fig. S2 (ESI†). Mn2+ and Sb3+ ions were not observed in the crystal structures of (MA)4InCl7:Mn2+ and (MA)4InCl7:Sb3+, probably due to the small doping ratio of Mn2+ and similar sizes between Sb3+ and In3+. The experimentally measured powder X-ray diffraction (PXRD) patterns of the pristine and doped compounds display high similarity to their simulated patterns as shown in Fig. S3 (ESI†), not only suggesting the reliability of the crystal structures, but also further evidencing the unchanged crystal structures upon metal ion doping.
To determine the actual atom ratios of the doped compounds, inductively coupled plasma optical emission spectrometry (ICP-OES) was utilized and the experimental ratios are summarized in Table S5 (ESI†). The amount of Sb3+ is close to the actual experimental amount (∼10%), while the experimental ratios of Cs+ or Mn2+ (∼2.5% and ∼0.2% respectively) are much less than the feeding ratios (∼5.8% and ∼3.0% respectively), indicating that Sb3+ can be more efficiently incorporated into the crystal with a homogeneous distribution than the other dopants (Cs+ and Mn2+). Effective doping was also confirmed by X-ray photoelectron spectroscopy (XPS). As shown in Fig. 2a and Fig. S4 (ESI†), In 3d3/2 and In 3d5/2 peaks (at 452.43 and 444.88 eV) in pristine (MA)4InCl7 are shifted to higher binding energy by 0.50, 0.40 and 0.45 eV upon Cs+, Mn2+ and Sb3+ doping, respectively. Accordingly, the peaks of Cs 3d3/2 and Cs 3d5/2 (738.1 and 724.2 eV), Mn 2p1/2 and Mn 2p3/2 (653.5 and 641.6 eV) and Sb 3d3/2 (539.9 eV) are observed in (MA)4InCl7:Cs+, (MA)4InCl7:Mn2+ and (MA)4InCl7:Sb3+ respectively, verifying the presence of doped ions in the crystals (Fig. 2b–d).
The PL properties of all compounds were characterized by steady state and time-resolved emission spectroscopy, which are summarized in Table 1. We compare the photophysical properties of (MA)4InCl7 with (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+ first. (MA)4InCl7 exhibits a broadband blue emission peaked at 455 nm with a PLQE of 11.2% when excited by 365 nm UV light as shown in Fig. 3a. The large Stokes shift and broadband emission suggest a self-trapped exciton mechanism, in which the generated excitons go through exciton–phonon interactions into self-trapped states (STE) with lower energy as commonly observed in other 0D OIMHs.38–41 Cs+ and Mn2+ doping slightly blue-shifts and narrows the blue emission peak. This phenomenon could have possibly originated from either the less extent of exciton–phonon coupling strength or more homogenous crystal structure. Given that the experimental crystal structures remain almost unchanged upon doping, the latter reason is more likely. Interestingly, the PLQE is significantly enhanced to 18.8% and 20.7% for Cs+ doping and Mn2+ doping, respectively, which is not reported for other 0D indium OIMHs before.
Materials | Optical bandgap (eV) | λ exc (nm) | λ em (nm) | FWHM (nm) | PLQE (%) | τ (ns) |
---|---|---|---|---|---|---|
(MA)4InCl7 | 3.34 | 273, 366 | 455 | 152 | 11.2 | 6.72 |
(MA)4InCl7:Cs+ | 3.36 | 298, 359 | 445 | 139 | 18.8 | 6.53 |
(MA)4InCl7:Mn2+ | 3.00 | 278, 363 | 445 | 114 | 20.7 | 7.94 |
(MA)4InCl7:Sb3+ | 3.23 | 283, 323 | 611 | 164 | 74.7 | 5420 |
Fig. 3 (a) Excitation and emission spectra of (MA)4InCl7, (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+. (b) Time-resolved PL decays of (MA)4InCl7, (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+. |
Furthermore, the PL decay dynamics of (MA)4InCl7, (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+ are characterized by time-resolved PL (TRPL) spectroscopy at room temperature (Fig. 3b). The PL decay curves can be well fitted using a bi-exponential fitting function as follows:
As shown in Table S6 (ESI†), the short lifetime τ1 and the long lifetime τ2 for all three compounds lie in the range of 2–3 ns (81–84%) and 11–12 ns (19–16%) respectively, resulting in an average PL decay lifetime of 6–7 ns. We attribute the fast decay and the slow decay components to the non-radiative and radiative recombination processes of the excitons, respectively. The faster decay through the non-radiative channel with a larger weighted amplitude could well explain the relatively low PLQE of the three compounds. Also, the radiative recombination rate an a nanosecond scale implies that the emission may be classified as fluorescence originating from singlet excitons. Together with the possible STE emission mechanism, the blue emission of (MA)4InCl7, (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+ could be attributed to the 1STE to 1S0 transition of In3+ (Fig. 4e), which could be confirmed from the density functional theory (DFT) calculations in the following section.
When it comes to the Sb3+ doped compound (MA)4InCl7:Sb3+, the emission mechanism is a totally different story. Upon Sb3+ doping, partial substitution of InCl63− to SbCl63− was anticipated, due to the similar size and chemical reactivity of the two elements. Compared with that of the pristine (MA)4InCl7, the emission peak of (MA)4InCl7:Sb3+ significantly red-shifted to 611 nm, with the PLQE greatly enhanced to 74.7%. This orange emission is likely to originate from the STE emission from the SbCl63− moiety suggested by previously reported 0D antimony OIMHs and antimony doped 0D indium OIMHs.15,42,43 To prove that, the excitation wavelength–dependent PL spectra of (MA)4InCl7:Sb3+ were first collected at room temperature. There is not much variation in the PL spectra excited at different wavelengths (from 250 to 360 nm) at room temperature, which confirms that the orange emission stems from the same excited states (Fig. S5, ESI†). The large Stokes shift of 170 nm and the broadband emission are typical characteristics of STE emissions.
Temperature-dependent PL spectra were further obtained to confirm the photoluminescence mechanism by monitoring the electron dynamics of the excited states. As shown in Fig. 4a, there emerges another emission peak located at 436 nm when the temperature was lowered to 77 K (excited by 280 nm UV light), which is not observed at room temperature. According to previous studies, the first excited state of OIMHs with 5s2Sb3+ could split into a singlet state (1P1) and triplet states (3Pn, n = 0, 1, and 2) and then go through lattice distortion to form self-trapped excitons.44,45 The 1STE to 3STE transition of Sb3+ was suspended when the temperature was lowered to 77 K due to the energy barrier between the two states, resulting in dual emission at 77 K. The lifetimes of 4.65 ns for the 436 nm emission peak and 6.11 μs for the 578 nm emission peak clearly evidence the fast and slow transitions of 1STE → 1S0 and 3STE → 1S0 respectively (Fig. 4b and c). Therefore, the orange emission of (MA)4InCl7:Sb3+ has originated from the 3STE of SbCl63+ as a result of metal ion substitution and fast 1STE to 3STE transition at room temperature (Fig. 4f). In addition, the absence of emission from InCl63− in (MA)4InCl7:Sb3+ implies efficient energy transfer from excited InCl63− to SbCl63−.
A negative thermal quenching effect was observed for the 578 nm peak of (MA)4InCl7:Sb3+ in the temperature-dependent PL spectra. As shown in Fig. 4d, the peak intensity first increases and then decreases when the temperature increases from 77 K to 297 K. This can be explained by the existence of shallow traps (STs) in 0D OIMHs as suggested by Sun et al.46 The excitons in the shallow traps could be thermally activated to detrap into the STE of (MA)4InCl7:Sb3+ to increase the emission intensity (Fig. 4f). It's intriguing that the negative thermal quenching effect was not observed for (MA)4InCl7, (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+. This may imply that they possess deeper traps that excitons could not detrap at room temperature. The shallow/deep traps in these 0D indium OIMHs could explain the dramatic enhancement of PLQE when (MA)4InCl7 was doped with Sb3+.
We found a big difference in the crystal morphologies between the pristine and doped ones using a UV-microscope. The photographs of the four compounds under ambient and UV light are shown in Fig. 5a–h. We observed that the doped crystals are more regular-shaped and transparent with fewer bulk defects compared with the parental (MA)4InCl7. This indicates that metal ion doping can improve the crystal quality and reduce bulk defects. The defect passivation effect introduced by metal ion doping may be an imperative reason for the PLQE enhancement in these 0D OIMHs due to the reduced trap-assisted non-radiative recombination centers. Better crystal quality also results in a more homogenous crystal structure, which is supported by the UV absorption spectra of the four compounds. As shown in Fig. S6 (ESI†), (MA)4InCl7, (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+ exhibit various degrees of Urbach tails which indicate that there are a certain number of sub-band-gap states underneath the conduction band of each structure upon photoexcitation, which could be the result of defects, structural disorders or inhomogeneity of crystals.47–51 When passivated by Cs+ and Mn2+, the sub-band-gap states of (MA)4InCl7 should partially diminished, explaining the reduced FWHM and increased PLQE. A very small Urbach tail was observed for (MA)4InCl7:Sb3+, suggesting minimized sub-band-gap states and homogenous crystals with less defects. Less defect-mediated degradation may explain the high stability of (MA)4InCl7:Sb3+, which maintained a high PLQE when stored under ambient or under continuous UV irradiation for 4 days (Fig. S7, ESI†).
To validate the origin of the emission from the four compounds, we calculated the electronic band structure and partial density of states (PDOS) of (MA)4InCl7, (MA)4InCl7:Cs+, (MA)4InCl7:Mn2+ and (MA)4InCl7:Sb3+ using density functional theory as shown in Fig. 6. Models of (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+ for DFT calculations were built by partially replacing MA+ by Cs+ and Mn2+ (two MA+ were replaced by one Mn2+ for charge balance) respectively, which could be regarded as the doped Cs+ and Mn2+ occupying the defect sites of MA+ vacancy. The model of (MA)4InCl7:Sb3+ for DFT calculations was based on partial substitution of In3+ by Sb3+. The single crystal structures of these models are listed in Fig. S8 (ESI†) and the calculated band structures of these four compounds are shown in Fig. S9 (ESI†). The calculated band gaps of (MA)4InCl7 and (MA)4InCl7:Cs+ are consistent with their experimental values, while the calculated band gaps of (MA)4InCl7:Mn2+ and (MA)4InCl7:Sb3+ are expected to be underestimated due to the well-known PBE band gap error. Nevertheless, the decreased band gaps upon Mn2+ and Sb3+ doping follow the trend of the calculation results. (MA)4InCl7 exhibits a slightly indirect bandgap of 3.36 eV. The flat conduction band and valence band indicate large effective mass of charges and localized electronic states commonly observed in other 0D OIMHs. The calculated partial density of states suggest that the valence band maximum (VBM) is comprised mostly of Cl 3p, while the conduction band minimum (CBM) is the hybrid of In 5s and Cl 3p orbitals. The contribution of MA+ organic moieties to the band structure is negligible. Therefore, the excitation of (MA)4InCl7 should lead to a self-trapped exciton localized on the InCl63− inorganic moiety, which in turn distorts its structural conformation. The band structure of (MA)4InCl7:Cs+ is almost identical to that of (MA)4InCl7, suggesting that Cs+ was not involved in the electron transition of the blue emission. In contrast, Mn2+ doping introduced mid-gap states, lowering the theoretical bandgap to 2.07 eV. It was reported that doped Mn2+could exhibit red emission arising from the d–d electron transition,12,52–55 which could be the origin of the PL intensity increase at ∼650 nm in Fig. 3a and the absorption increase at 330 nm in Fig. S6 (ESI†). However, these changes of photoluminescent properties upon Mn2+ doping are limited due to the small doping ratio of Mn2+. The blue emission of (MA)4InCl7:Mn2+ should have the same origin as (MA)4InCl7 and the dramatic PLQE enhancement upon Mn2+ doping should come from defect passivation and better crystal quality as analyzed above. Combined with the TRPL results, we conclude that (MA)4InCl7, (MA)4InCl7:Cs+ and (MA)4InCl7:Mn2+ share the same light-emitting mechanism, in which the broadband blue emission with large Stokes shift is the manifestation of the radiative recombination of the singlet excitons from the self-trapped excited states of In3+ (Fig. 4e). On the other hand, Sb3+ doping also introduced mid-gap states which lowers the bandgap to 2.31 eV. Evidenced by the PL properties and negative thermal quenching effect, the high PLQE of (MA)4InCl7:Sb3+ could be attributed to the highly efficient radiative recombination of 3STE on SbCl63− and the absence of deep trap states (Fig. 4f).
Fig. 6 Partial density of states of (a) (MA)4InCl7, (b) (MA)4InCl7:Cs+, (c) (MA)4InCl7:Mn2+ and (d) (MA)4InCl7:Sb3+. |
As mentioned above, the pristine (MA)4InCl7 exhibits intense blue emission but quickly turned to orange after the reaction with Sb3+, which makes it a promising antimony ion sensor. To prove this concept, a demo sensor was simply made by mixing (MA)4InCl7 powder with ethanol which do not dissolve the compound. As shown in Fig. 7a, when a small amount of dilute Sb3+ ethanol solution was added to the sensor, the emission under UV rapidly switched to orange accompanied by the PL intensity increase. The working curve of the sensor was measured by correlating the PL intensity of the 610 nm emission with the concentration of Sb3+, which shows a near-linear relationship beneficial for the quantitative analysis. This sensor also exhibits an ultra-low detection limit of 0.1 mM (22.8 ppm) for antimony metal ions, and a fast responsive time of up to 15 s in the working region. We also tested its selectivity by adding solution of other metal ions (Pb2+ and Bi3+), which introduces little changes to its PL spectrum as shown in Fig. S11 (ESI†), suggesting that the sensor is highly selective for Sb3+ among other heavy metal ions.
Fig. 7 (a) The sensor demo and the PL change after adding Sb3+ ethanol solution (excited by 365 nm UV light). (b) Working curve of the Sb3+ sensor. |
Footnote |
† Electronic supplementary information (ESI) available: Experimental section, crystallographic data, PXRD patterns, TGA data, UV-vis absorption spectra and PL spectra. CCDC 2195355–2195358. For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d2qm00866a |
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