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Article

PVP Passivated δ-CsPbI3: Vacancy Induced Visible-Light Absorption and Efficient Photocatalysis

1
College of Physics and Electronic Information Engineering, Key Laboratory of Low-Dimensional Structural Physics and Application, Education Department of Guangxi Zhuang Autonomous Region, Guilin University of Technology, Guilin 541004, China
2
School of Electronic Information and Automation, Guilin University of Aerospace Technology, Guilin 541004, China
*
Author to whom correspondence should be addressed.
Molecules 2024, 29(7), 1670; https://doi.org/10.3390/molecules29071670
Submission received: 12 March 2024 / Revised: 30 March 2024 / Accepted: 1 April 2024 / Published: 8 April 2024
(This article belongs to the Special Issue New Materials and Catalysis in Environmental Protection)

Abstract

:
The aqueous instability of halide perovskite seriously hinders its direct application in water as a potential photocatalyst. Here, we prepared a new type of polyvinylpyrrolidone (PVP) passivated δ-CsPbI3 (δ-CsPbI3@PVP) microcrystal by a facile method. This material can be uniformly dispersed in water and stably maintain its crystal structure for a long time, breaking through the bottleneck of halide perovskite photocatalysis in water. Under visible light, δ-CsPbI3@PVP can almost completely photodegrade organic dyes (including Rhodamine B, methylene blue, and crystal violet) in only 20 min. The efficient photocatalytic activity is attributed to the enhanced visible light absorption arising from PbI2 defects in δ-CsPbI3@PVP and the intrinsic low photoluminescence quantum yield of δ-CsPbI3, which induces efficient light absorption and photocatalytic activity. We highlight δ-CsPbI3@PVP as an effective aqueous photocatalyst, and this study provides new insights into how to exploit the potential of halide perovskite in photocatalytic applications.

1. Introduction

In recent decades, semiconductor-based photocatalysis has attracted much attention, including metal oxides [1,2], metal sulfides [3,4,5], and two-dimensional layered materials [6,7,8,9]. Among metal oxides, TiO2 [10] and ZnO [11] have become the most popular photocatalysts due to their low cost, high activity, and stable chemical properties. However, they possess wide band gaps of 3.2–3.4 eV, which can only absorb UV light, accounting for merely 4% of the sunlight that can be utilized. Among metal sulfides, CdS [12] and ZnS [5] are the most studied. CdS has a band gap of 2.4 eV and can capture visible light, but it is limited by a strong photo corrosion effect. ZnS is inert in corrosive environments, but its band gap of 3.6 eV again leads to poor visible light absorption. Two-dimensional layered materials such as g-C3N4 and MXenes are prospective photocatalysts due to their large specific surface area. However, g-C3N4 fails to cover most visible light [13,14] and MXenes possess low photocatalytic activity [15]. Moreover, all these traditional photocatalysts suffer from the low separation and transfer efficiency of the photogenerated electron–hole pairs. Therefore, in the past two decades, researchers have devoted much effort, including in morphology and size control [16,17], element doping [18], and material compositing [19], to facilitate the separation and transfer of the photogenerated carriers. Nevertheless, the current visible light photocatalytic performances of these materials are still far away from expectations.
As a rising star material, halide perovskite has been widely studied in solar cells [20], light-emitting diodes (LEDs) [21], lasers [22], and photodetectors [23,24] due to its simple synthesis, wide light absorption range, high extinction coefficient, long carrier life and transmission distance, and adjustable band structure [25]. Also, halide perovskite has been successfully used in carbon dioxide reduction [26,27], hydrogen evolution [28,29,30,31,32,33], and organic dye photodegradation [34,35,36,37,38]. However, due to the aqueous instability of halide perovskite, such photocatalytic experiments have to be conducted in organic solvents [35,38,39,40,41,42,43,44,45,46,47,48,49] or after water-resistant-surface passivation [28,29,30,31,32,33,50,51]. Searching for halide perovskite, which can be directly used in water, is important in photocatalysis. In the perovskite family, δ-phase perovskite is well known for its stability in humidity and unsuitability for optoelectronic applications arising from its poor photoluminescence (PL) quantum yield (QY) [52]. Interestingly, the band gap of δ-CsPbI3 is 2.54 eV [53], combined with a high light absorption coefficient and low PLQY, implying that its photo-generated charge carriers are less likely to undergo direct electron–hole recombination and are more likely to effectively participate in photocatalytic reactions. These unique characteristics suggest that δ-CsPbI3 may be a promising photocatalyst.
Here, via a facile method, we synthesized δ-CsPbI3 microcrystals and passivated them by polyvinylpyrrolidone (PVP) to enhance their dispersibility and stability in water. Such δ-CsPbI3@PVP can stably exist in water for at least 30 days without obvious deterioration. It exhibited a striking visible light photodegradation ability for organic dyes, namely, completely photodegrading Rhodamine B (RhB), methylene blue (MB), and crystal violet (CV) in only 20 min. Such a high efficiency was highly related to the enhanced absorption in the visible region induced by the PbI2 vacancy defects in δ-CsPbI3@PVP and its intrinsic low PLQY, since adequate photocarriers can be generated and participate in the photocatalytic process to effectively degrade organic dyes. The δ-CsPbI3@PVP material showed good stability in cyclic tests, indicating its resistance to light corrosion. Our results opened a gate on how to develop the photocatalysis of halide perovskites.

2. Results

Shown in Figure 1a,b are the SEM images of δ-CsPbI3 and δ-CsPbI3@PVP microcrystals. They both are demonstrated as long stripes, with an average length of 22.5 (Figure S1a, δ-CsPbI3) and 20 microns (Figure S1b, δ-CsPbI3@PVP), respectively. Figure 1c shows a typical TEM image of δ-CsPbI3@PVP. It can be clearly seen that, the long-stripe-shaped δ-CsPbI3 was covered by the adherent PVP, which thus enhanced the dispersion and stability of δ-CsPbI3 in water. The inset HRTEM image of δ-CsPbI3@PVP shows a lattice spacing of 0.20 nm, which corresponds to the (414) crystal faces of δ-CsPbI3 microcrystals. The elemental analyses (Figure 1d, δ-CsPbI3@PVP) showed the atomic ratio of Cs/Pb/I = 1:0.65:2.45, basically according with the formula of halide perovskites with some defects.
Figure 2 shows the XRD patterns of δ-CsPbI3 and δ-CsPbI3@PVP microcrystals. One can see that δ-CsPbI3 and δ-CsPbI3@PVP are almost the same, demonstrated as an orthorhombic structure (Pnma space group) and well-matched with the standard PDF card, as found in other studies of the δ-phase CsPbI3[54]. The results indicated that the PVP passivation did not change the crystal structure of δ-CsPbI3. Although a previous study showed that the amide group in PVP may reduce the surface energy to impose an effect on the crystal structure of CsPbI3 [55], here we still deem δ-CsPbI3@PVP as PVP-wrapped orthorhombic δ-phase CsPbI3 crystals. Elemental analyses by EDS of the δ-CsPbI3@PVP crystals showed that the atomic ratio of Cs/Pb/I = 1:0.65:2.45 (Figure 1d), which basically was in accordance with the molecular formula of halide perovskites, however with some defects present.
The aqueous dispersion and stability of photocatalysts are the important factors determining whether they are suitable for photodegrading organic dyes in water. In Figure 3a, it is found that only the newly synthesized δ-CsPbI3 microcrystals could be dispersed in water, and they soon tended to aggregate, so using δ-CsPbI3 microcrystals as water-based photocatalysts was challenging. In contrast, the dispersion of δ-CsPbI3@PVP microcrystals was pretty good without notable aggregation. In Figure 3b, after 30 days, the photoluminescence (PL) spectrum shape and intensity of δ-CsPbI3@PVP barely changed, demonstrating the fantastic water stability of CsPbI3@PVP microcrystals. Obviously, the PVP passivation of perovskite surface improved the dispersion and stability of perovskite in water [36]. The PL center of the δ-CsPbI3@PVP water solution was 530 nm, demonstrating the typical green light due to self-trapped excitons of δ-phase CsPbI3 microcrystals [56]. Its UV-vis absorption spectrum [Figure 3c] also showed typical δ-CsPbI3 behavior, with a broad absorption range in the visible region and a clear band-to-band absorption edge close to 460 nm (2.57 eV), which was consistent with other studies on δ-CsPbI3 [56,57]. Notably, δ-CsPbI3@PVP had a significant absorption shoulder close to 530 nm. We also performed PL measurements on δ-CsPbI3@PVP powder (Figure S2). The δ-CsPbI3@PVP powder demonstrated a broad emission spectrum ranging from 437 to 660 nm, which was in accordance with the previous literature [53,58]. Even so, two peaks also could be clearly distinguished, which were located at about 460 nm and 530 nm, respectively. Similar to its solution counterpart, the former peak was ascribed to band-to-band transition, and the latter was due to the self-trapped excitonic emission. Obviously, the band-to-band emission of δ-CsPbI3@PVP was totally suppressed in water; however, its specific reason remains unclear, and we speculate it is highly related to the aqueous environment. Since the scope of this work is studying the aqueous photocatalysis of δ-CsPbI3, the following discussion is mainly based on the optical properties of the sample water solution.
As known, δ-CsPbI3 is generally the deteriorated product of its perovskite-phase counterpart when exposed to moisture. Water can dissolve some ions and produce vacancy defects in perovskite and eventually result in the δ-phase. Hence, δ-CsPbI3 should be a material rich in vacancies, at least on its crystal surface. The absorption shoulder at ~530 nm (Figure 3) should be highly related to such defects. Therefore, we calculated the changes in optical properties when four common vacancy defects (VCs, VI, VCsI, and V PbI 2 ) were present (Figure 4) [58]. Figure 4a–e respectively depict the structures of pristine and defective δ-CsPbI3 cells. Figure 4f shows that such vacancy defects can all result in the enhancement of the absorption coefficient in the visible range (460–600 nm). Notably, V PbI 2 brings about a prominent absorption shoulder close to 530 nm, similar to our experimental results [Figure 3c]. Combined with the EDS results in Figure 1d, reasonably, we speculate that δ-CsPbI3@PVP crystals contain many vacancy defects, primarily dominated by PbI2 vacancies. It is also noted in Figure 3c that δ-CsPbI3 without a PVP coating showed no prominent absorption shoulder at ~530 nm in water, which may have been due to the further water corrosion of vacancy defects in δ-CsPbI3. Such PbI2 vacancy defects were protected by PVP in δ-CsPbI3@PVP; thus, the absorption characteristics at ~530 nm could be exhibited.
The absorption coefficients of the δ-CsPbI3@PVP water solution were larger than 2 × 102, 0.5 × 102, and 0.2 × 102 L•mol−1•cm−1 in the visible range of 400–460, 460–530, and 530–700 nm, respectively [Figure 3c]. We compared it with two famous photocatalysts, g-C3N4 and TiO2; although, these two are more reasonably deemed suspended rather than soluble in water. As shown in Figure S3, in the visible light region, g-C3N4 had only a band-to-band absorption coefficient of ~0.5 × 102 L•mol−1•cm−1 in the wavelength region of 400–420 nm. When the wavelength exceeded 430 nm, its absorption coefficient soon dropped to less than 0.1 × 102 L•mol−1•cm−1. The star photocatalyst in the UV region was TiO2, of which the absorption coefficient was less than 0.5 × 102 L•mol−1•cm−1, even in the UV region (Figure S3). Undoubtedly, the strong absorption ability of δ-CsPbI3@PVP is important to its visible light photocatalysis. As known, most members in the halide perovskite family have a very high PLQY; that means most photogenerated carriers will directly recombine to emit light, which is obviously not conducive to photocatalytic activity. Fortunately, δ-phase perovskite is notorious for its weak PL intensity [56], which herein would be a merit since plentiful indirectly recombined photocarriers could participate in the photodegradation process. Using quinine sulfate as a reference, we found that the PLQYs of δ-CsPbI3 and δ-CsPbI3@PVP were only 0.17% and 0.43% (see Table 1). Its strong absorption, low PLQY, good dispersion, and stability in water indicated that δ-CsPbI3@PVP has great potential in the photocatalytic field.
Based on the above conjecture, we conducted visible light photodegradation experiments on δ-CsPbI3@PVP microcrystals’ effects on different organic dyes in water. Four representative dyes, 10 mg/L RhB, 20 mg/L MB, 20 mg/L CV, and 5 mg/L methyl orange (MO), were used as degradation references after 30 min in the dark to achieve an equilibrium of absorption–desorption. As shown in Figure 5a–d, small amounts of δ-CsPbI3@PVP (≤50 mg) could photodegrade 99% of RhB, MB, and CV in merely 20 min, but only 25% of MO could be degraded even after increasing the quality of δ-CsPbI3@PVP to 150 mg. The exact reason why δ-CsPbI3@PVP barely photodegraded MO is hard to know; therefore, this thesis focused on the photodegradation of RhB, MB, and CV by δ-CsPbI3@PVP. As expected, the photodegradation ability increased with increasing the mass of the photocatalyst. To avoid any possible deviations on the concentration calibration via absorption spectroscopic measurements of organic dyes, we performed total organic carbon (TOC) experiments and found that all the mineralization of RhB, MB, and CV could exceed 90% after 20 min of photodegradation. After three cycles [Figure 5e], the degradation capacity of δ-CsPbI3@PVP remained stable, and the small decline was attributed to the photo-corrosion of the photocatalyst caused by the prolonged reaction. It was noted that the photo-degradation ability of δ-CsPbI3@PVP was insusceptible to the PH values of the solution; in the PH range of 3–11, δ-CsPbI3@PVP all could degrade 99% of RhB in 20 min (Figure S4).
In order to explore its catalytic process, free radical trapping experiments were carried out. Different trapping agents were added to find the led active species in the catalytic process. P-benzoquinone (BQ), isopropyl alcohol (IPA), potassium iodide (KI), and potassium bromate (KBrO3) were respectively used to scavenge superoxide free radicals (•O2), hydroxyl free radicals (•OH), holes (h+), and electrons (e). As shown in Figure 4f, the photocatalytic performance was significantly reduced after the addition of BQ (71%) and KBrO3 (63%), indicating that •O2 and e were the predominant active species in this photocatalytic process. After the holes were captured, the photodegradation efficiency also had a 30% decrease. Adding IPA had no influence on the photodegradation, which meant that in this process, •OH radicals were hardly produced.
In addition, Table 2 compares the photocatalytic activity of δ-CsPbI3@PVP with that of other perovskite materials. Previously, it has been reported in other studies that to maintain the stability of perovskites, photocatalytic experiments must be conducted solely in organic solvents. In contrast, the δ-CsPbI3@PVP material was capable of direct utilization in water. Furthermore, under visible light, δ-CsPbI3@PVP effectively degraded various organic dyes (such as RhB, MB, and CV) within a mere 20 min timeframe. It can be seen that the photocatalytic activity of the δ-CsPbI3@PVP material was far ahead of those of other reported studies.

3. Discussion

A good photocatalyst is preferred to have a good light absorption ability and good redox ability [59]. A good absorption ability generally requires a narrow band gap, while a good redox ability favors a high conduction and/or low valence band level, which is convenient for the transfer of photogenerated electrons and/or holes, namely, a wide band gap [59]. Obviously, there is a contradiction between these; however, in δ-CsPbI3@PVP, a good compromise was achieved. Its band gap was 2.57 eV [the inset of Figure 3c], which was a wide band gap among the visible light semiconductor photocatalysts. Meanwhile, it also had a strong light absorption ability no matter above or below the band gap [Figure 3c]. Especially, the existence of self-trapping states further enhances the absorption below the band gap. Large amounts of photons were absorbed and turned into transferable, indirectly recombined electrons and holes (PLQY is 0.43%, Table 1), together with its good dispersion and stability in water, which make δ-CsPbI3@PVP become a highly efficient visible light photocatalyst.
Shown in Figure 6 is the schematic diagram of the RhB photodegradation process of δ-CsPbI3@PVP. Using a vacuum level as a reference, the UPS measurements [Figure 6a] could define the valence band maximum (VBM) by EVBM = −[21.22 − (Ecutoff − Eonset)]. For δ-CsPbI3@PVP, the Ecutoff was 16.30 eV and the Eonset was 1.90 eV, so the EVBM was −6.82 eV. Considering the band gap was 2.57 eV, one can know that the conduction band maximum (CBM) was −4.25 eV. The emissive center was located at 530 nm, implying the energy difference between the trap states and VBM was 2.34 eV, namely, the energy level of trap states was −4.48 eV. Conventionally, we expressed the energy levels using a normal hydrogen electrode (NHE) as a reference [E(NHE) = −4.5 − E(vacuum), which represented the relationship between the NHE and vacuum energy levels], and the energy levels of the CBM, trap states, and VBM were −0.25, −0.02, and 2.32 eV, respectively. The photocatalytic mechanism of δ-CsPbI3@PVP could be reasonably inferred according to the experimental results:
δ - CsPbI 3 @ PVP + dyes     * dyes
δ - CsPbI 3 @ PVP + h ν   h + + e
O 2 + e   O 2
O 2 + * dyes   mineralization   products
where *dye denotes the dye molecule activated by δ-CsPbI3@PVP. When δ-CsPbI3@PVP was exposed to visible light, the absorption of photons caused the electrons to be excited from the VB to the CB and trap states, resulting in photogenerated electrons and holes. The electrons were captured by O2 to produce •O2, and then •O2 reacted with the *dye to produce mineralized compounds. If the electrons or •O2 radicals were captured, the photodegradation efficiency would be significantly decreased [Figure 5f]. Moreover, we could not completely neglect the effects of photogenerated holes [Figure 5f] since they also can directly oxidize and degrade dyes [60].

4. Experimental Section

4.1. Materials

CsI (99.9%), PbI2 (99%), polyvinylpyrrolidone (PVP, K29-32), MB, CV, and methyl orange (MO) were purchased from Roan (Olds, AB, Canada). RhB was purchased from the Tianjin Guangfu fine chemical research institute (Tianjin, China). Ethanol (>99.7%, AR) and isopropyl alcohol (IPA, 99.7%, AR) were purchased from Silon Science (Allentown, PA, USA). Potassium iodide (KI, ≥99.0%, AR), potassium bromates (KBrO3, ≥99.8%, AR), P-benzoquinone (BQ, 99%), and hydroiodic acid (HI, 55.5–58.0% with <1.5% H3PO2 stabilizer) were from Aladdin (Shanghai, China). The water was deionized.

4.2. Synthesis of δ-CsPbI3 and δ-CsPbI3@PVP

PbI2 (10 mmol, 4.61 g) was dissolved in hydroiodic acid (8 mL), and then CsI (10 mmol, 2.59 g, dissolved in 3 mL of water) was added dropwise to produce a brown precipitate. The precipitate was filtered, washed twice with ethanol, and dried in a vacuum oven at 60 °C for 12 h. Then, the δ-CsPbI3 microcrystals were obtained.
Adding the above-mentioned brown precipitate with 2 g PVP to 30 mL of ethanol, a suspension was formed after vigorous stirring at room temperature for 30 min. After 15 min of ultrasonication, the precipitation was filtered and then washed with ethanol and water, finally dried in a vacuum oven at 60 °C for 12 h to obtain δ-CsPbI3@PVP microcrystals.

4.3. Characterization

The morphologies of δ-CsPbI3 and δ-CsPbI3@PVP samples were characterized by a transmission electron microscope (TEM, JEM-2100F, JEOL, Akishima, Japan) and a field emission scanning electron microscope (SEM, S-4800, Hitachi, Tokyo, Japan) equipped with an energy dispersive spectrometer (EDS). The crystal structures of δ-CsPbI3 and δ-CsPbI3@PVP were determined by X-ray diffraction (XRD, X ‘Pert PRO, JEOL, Tokyo, Japan). UV photoelectron spectroscopy (UPS) measurements were performed on a photoelectron spectrometer (ESCALAB 250Xi, Thermo Scientific, Waltham, MA, USA) with a He I source of 21.22 eV. A UV spectrophotometer (UV2700, Shimadzu, Kyoto, Japan) and fluorescence spectrometer (Edinburgh FL/FS900 Carry Eclipse, Agilent, Santa Clara, CA, USA) were used to determine the UV-vis absorption spectra, photoluminescence (PL) spectra, and relative quantum yield (QY).
Under the same excitation, the fluorescence spectra of a quinine sulfate solution and sample were tested, and the PLQY was calculated according to the following formula:
Φ x = n x 2 n Q S 2 · A Q S · I x A x · I Q S · Φ Q S
where Φ Q S is the fluorescence quantum yield of the standard reference quinine sulfate solution (54%). AQS, IQS, nQS, and Ax, Ix, nx refer to the absorbance value, integral area, and solution refractive index of the quinine sulfate solution and the sample, respectively.
We used the molar absorption coefficient (ε, L•mol−1•cm−1) to compare the absorption abilities of different solutions. The absorbance (A) was determined by a UV-vis spectrophotometer, and the ε was calculated as follows:
ε = A b c
Among these, c is the concentration (mol/L), and the optical path b was 1 cm. In this work, the concentrations of δ-CsPbI3 and δ-CsPbI3@PVP were both   4.16 × 10 3   mol / L .

4.4. Photocatalytic Activity Measurements

The photocatalytic activity of the δ-CsPbI3@PVP samples was studied by testing the degradation of RhB, MB, MO, and CV dyes under visible light. A xenon lamp (PLS-SXE300, 300 W, λ > 420 nm) was the visible light source. A certain quality of the δ-CsPbI3@PVP sample (15–150 mg) was placed in 50 mL of dye aqueous solution (5–20 mg/L); then, the mixed solution was stirred in the dark for 30 min to achieve an adsorption–desorption equilibrium. Thereafter, every 5 min, the 3 mL solution was taken out to determine the dye concentration by a UV-visible spectrophotometer (UV2700, Shimadzu). The photocatalysts were repeatedly collected by centrifugation and drying and then used for the recycle photodegradation experiments. A total organic carbon (TOC) analyzer (Shimadzu, TOC-L CPN) was also used to determine the photodegradation efficiency of the organic dyes.
The concentration of the organic dyes was determined by a UV-vis spectrophotometer, and the degradation efficiency of the organic dyes was calculated as follows:
degradation   ratio   ( % ) = C 0   C C 0 × 100 = A 0   A A 0 × 100
where C0 and C are the initial and real-time concentrations of the organic dyes, respectively, and A0 and A are the initial and real-time absorbance of RhB at 554 nm (MB at 660 nm, MO at 463 nm, and CV at 583 nm), respectively.

4.5. Computational Details

The calculations in this paper were based on the Vienna Ab initio Simulation Package (VASP), calculated by Density Functional Theory (DFT) [59]. Generalized gradient approximation (GGA) and Perdew–Burke–Ernzerhof (PBE) were used to describe the correlation terms of the computational model. Electron–ion interactions were described using the projection-enhanced wave potential (PAW) [60]. A correction for van der Waals force interactions in the crystal cell model using Grimme’s DFT-D3 approach [61] was performed. The structure of δ-CsPbI3 was orthorhombic, and its lattice constants were a = 10.46 Å, b = 4.80 Å, and c = 17.78 Å, respectively. In this paper, a 1 × 1 × 1 cell model was established, in which there were 20 atoms, including 4 Cs, 4 Pb, and 12 I atoms. The plane-wave cut-off energy was set to 450 eV. An amount of 2 × 2 × 1 K points in the Brillouin zone were sampled using the Gamma method, and non-self-consistent calculations were performed using a 4 × 4 × 1 grid. Then, on the basic structure of the intrinsic perovskite model, the absorption coefficient variation caused by common vacancy defects were calculated. VCs, VI, VCsI, and V PbI 2 referred to the vacancy induced by the removal of a single Cs atom, a single I atom, a Cs atom and an I atom, and a Pb atom and two I atoms in the cell. These vacancy defects are commonly generated during the preparation of halide perovskites. During the optimization process, the convergence energy and force per atom were 10−5 eV and 0.05 eVÅ−1, respectively, and all the atoms of the system (including atomic positions and lattice constants) remained fully relaxed.

5. Conclusions

In summary, we successfully synthesized water-stable δ-CsPbI3@PVP microcrystals to photodegrade various organic dyes in aqueous photocatalytic systems. These δ-CsPbI3@PVP microcrystals exhibited a long stripe shape with an average size of 20 μm and could be well dispersed in water without obvious deterioration for at least one month. Under visible light, δ-CsPbI3@PVP demonstrated an efficient photocatalytic activity, capable of completely degrading a variety of organic dyes, including RhB, MB, and CV, in just 20 min. This high photocatalytic efficiency was attributed to the enhancement of the material’s absorption coefficient in the visible light range arisen from PbI2 defects, as well as its low PLQY, allowing for the effective utilization of photogenerated electrons and holes in the photodegradation process. Therefore, δ-CsPbI3@PVP microcrystals hold significant potential for the rapid photodegradation of typical organic dyes in the field of photocatalysis. This study provides a new idea for the development of efficient photocatalysts and brings new hope for the research and application in the field of environmental protection and wastewater treatment.

Supplementary Materials

The following supporting information can be downloaded at: https://www.mdpi.com/article/10.3390/molecules29071670/s1, Figure S1. The length distributions of (a) δ-CsPbI3 and (b) δ-CsPbI3@PVP microcrystals. Figure S2. The steady-state PL spectra of δ-CsPbI3 and δ-CsPbI3@PVP powders. The excitation wavelength is 390 nm. Figure S3. Absorption coefficients of TiO2, g-C3N4 and δ-CsPbI3@PVP. Figure S4. The visible-light photodegradation of 10 mg/L RhB by δ-CsPbI3@PVP microcrystals in water with different PH values.

Author Contributions

J.W.: conceptualization. X.D.: investigation, data curation, writing—original draft. F.H.: investigation, data curation. Y.G.: investigation. M.L.: supervision. T.T.: funding acquisition, supervision, writing—review and editing. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by Natural Science Foundation of Guangxi Zhuang Autonomous Region of China (2018GXNSFAA050014) and Foundation of Guilin University of Technology (GLUTQD2002023).

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

Data are contained within the article and Supplementary Materials.

Conflicts of Interest

The authors declare no competing financial interests.

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Figure 1. SEM images of (a) δ-CsPbI3 and (b) δ-CsPbI3@PVP microcrystals. The insets are the corresponding high-resolution images. (c) Typical TEM image of a δ-CsPbI3@PVP microcrystal. The inset is the corresponding high-resolution TEM (HRTEM) image. (d) EDS elemental mapping of δ-CsPbI3@PVP microcrystals.
Figure 1. SEM images of (a) δ-CsPbI3 and (b) δ-CsPbI3@PVP microcrystals. The insets are the corresponding high-resolution images. (c) Typical TEM image of a δ-CsPbI3@PVP microcrystal. The inset is the corresponding high-resolution TEM (HRTEM) image. (d) EDS elemental mapping of δ-CsPbI3@PVP microcrystals.
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Figure 2. XRD patterns of δ-CsPbI3 and δ-CsPbI3@PVP microcrystals.
Figure 2. XRD patterns of δ-CsPbI3 and δ-CsPbI3@PVP microcrystals.
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Figure 3. (a) Optical images under sun and UV light of δ-CsPbI3 (left) and δ-CsPbI3@PVP (right) water solutions. (b) Time-dependent PL spectra of δ-CsPbI3 and δ-CsPbI3@PVP aqueous solutions. The excitation wavelength is 390 nm. (c) Absorption coefficients of δ-CsPbI3 and δ-CsPbI3@PVP. The inset is the Tauc plot of δ-CsPbI3@PVP.
Figure 3. (a) Optical images under sun and UV light of δ-CsPbI3 (left) and δ-CsPbI3@PVP (right) water solutions. (b) Time-dependent PL spectra of δ-CsPbI3 and δ-CsPbI3@PVP aqueous solutions. The excitation wavelength is 390 nm. (c) Absorption coefficients of δ-CsPbI3 and δ-CsPbI3@PVP. The inset is the Tauc plot of δ-CsPbI3@PVP.
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Figure 4. (a) δ-CsPbI3 cell model, (b) Cs vacancy cell model, (c) I vacancy cell model, (d) CsI vacancy cell model, (e) PbI2 vacancy cell model, (f) calculated absorption coefficient maps for δ-CsPbI3 and δ-CsPbI3 at four vacancies, VCs, VI, VCsI, and V PbI 2 .
Figure 4. (a) δ-CsPbI3 cell model, (b) Cs vacancy cell model, (c) I vacancy cell model, (d) CsI vacancy cell model, (e) PbI2 vacancy cell model, (f) calculated absorption coefficient maps for δ-CsPbI3 and δ-CsPbI3 at four vacancies, VCs, VI, VCsI, and V PbI 2 .
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Figure 5. Visible light catalytic degradation of δ-CsPbI3@PVP on different organic dyes (50 mL). The concentration variations of (a) 10 mg/L RhB, (b) 20 mg/L MB, (c) 20 mg/L CV, and (d) 5 mg/L MO under photodegradation with different δ-CsPbI3@PVP qualities. C and C0 refer to the current and initial concentration of dyes, respectively. (e) Cyclic photodegradation experiments on different dyes. (f) Effects of different free radical quenchers.
Figure 5. Visible light catalytic degradation of δ-CsPbI3@PVP on different organic dyes (50 mL). The concentration variations of (a) 10 mg/L RhB, (b) 20 mg/L MB, (c) 20 mg/L CV, and (d) 5 mg/L MO under photodegradation with different δ-CsPbI3@PVP qualities. C and C0 refer to the current and initial concentration of dyes, respectively. (e) Cyclic photodegradation experiments on different dyes. (f) Effects of different free radical quenchers.
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Figure 6. (a) UPS spectra of δ-CsPbI3 and δ-CsPbI3@PVP microcrystals. The insets are the corresponding onset and cutoff parts. (b) RhB degradation process of δ-CsPbI3@PVP microcrystals under visible light.
Figure 6. (a) UPS spectra of δ-CsPbI3 and δ-CsPbI3@PVP microcrystals. The insets are the corresponding onset and cutoff parts. (b) RhB degradation process of δ-CsPbI3@PVP microcrystals under visible light.
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Table 1. PLQYs of δ-CsPbI3 and δ-CsPbI3@PVP using quinine sulfate as a reference.
Table 1. PLQYs of δ-CsPbI3 and δ-CsPbI3@PVP using quinine sulfate as a reference.
SampleIntensity (I)Abs. (A)Refractive Index (n)PLQY (Φ)
Quinine sulfate12,728.40.011.330.54
δ-CsPbI3813.20.2021.330.0017
δ-CsPbI3@PVP 2047.40.2021.330.0043
Table 2. Comparison of photocatalytic activity of perovskite photocatalysts for the degradation of organic pollutants.
Table 2. Comparison of photocatalytic activity of perovskite photocatalysts for the degradation of organic pollutants.
PhotocatalystsContaminantsTest ConditionsEfficiencyRef.
δ-CsPbI3@PVPRhB in watervisible99% in 20 minThis work
δ-CsPbI3@PVPMB in watervisible99% in 20 minThis work
δ-CsPbI3@PVPCV in watervisible99% in 20 minThis work
CsPbCl3 QDsMO in ethanolvisible90% in 80 min[35]
CsPbBr3 QDsMO in ethanolvisible82% in 80 min[35]
CsPbBr3 CNCsMB in isopropanolvisible99% in 60 min[36]
CsPbBr3 crystalsRhB in watervisible47.3% in 120 min[44]
CsPb2Br5 crystalsRhB in watervisible53.8% in 120 min[44]
Cs2AgBiBr6RhB in ethanolvisible98% in 120 min[47]
Cs2AgBiBr6Rh110 in ethanolvisible98% in 280 min[47]
Cs2AgBiBr6MR in ethanolvisible98% in 420 min[47]
Cs2AgBiBr6MO in ethanolvisible98% in 300 min[47]
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Wen, J.; Du, X.; Hua, F.; Gu, Y.; Li, M.; Tang, T. PVP Passivated δ-CsPbI3: Vacancy Induced Visible-Light Absorption and Efficient Photocatalysis. Molecules 2024, 29, 1670. https://doi.org/10.3390/molecules29071670

AMA Style

Wen J, Du X, Hua F, Gu Y, Li M, Tang T. PVP Passivated δ-CsPbI3: Vacancy Induced Visible-Light Absorption and Efficient Photocatalysis. Molecules. 2024; 29(7):1670. https://doi.org/10.3390/molecules29071670

Chicago/Turabian Style

Wen, Jianfeng, Xin Du, Feng Hua, Yiting Gu, Ming Li, and Tao Tang. 2024. "PVP Passivated δ-CsPbI3: Vacancy Induced Visible-Light Absorption and Efficient Photocatalysis" Molecules 29, no. 7: 1670. https://doi.org/10.3390/molecules29071670

APA Style

Wen, J., Du, X., Hua, F., Gu, Y., Li, M., & Tang, T. (2024). PVP Passivated δ-CsPbI3: Vacancy Induced Visible-Light Absorption and Efficient Photocatalysis. Molecules, 29(7), 1670. https://doi.org/10.3390/molecules29071670

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