1. IntroductionHybrid organic–inorganic perovskite, the chemical general formula ABX3 (A = CH3NH3, HC(NH2)2, Cs; B = Pb, Sn; X = Cl, Br, I) perovskite family, is a well-known material with excellent absorption coefficient,[1,2] long carrier diffusion length,[3–5] high mobility,[6,7] and a tunable bandgap.[8–10] These properties can be tuned by changing the A, B, and X atoms. Nowadays, the certified efficiency of a hybrid organic–inorganic perovskite solar cell (PSC) has already reached up to 22.1%,[11] which proves that the hybrid organic–inorganic perovskite is a viable candidate for crystalline silicon solar cells and copper indium gallium selenide (CIGS) commercial photovoltaic (PV) devices, owing to its low-cost and facile solution-based fabrication process.
The perovskite film is at the core of PSC, whose quality greatly determines the photovoltaic performance. Many photo-physical properties, such as light harvesting, charge carrier transport and diffusion length, can be dramatically affected by the crystallization of the perovskite.[12–14] The defects and the crystal grain boundaries of the perovskite crystallites act as the traps of carriers, which aggravate the charge recombination. The current density–voltage (J–V) hysteresis effect, which causes inaccuracy in evaluating cell efficiency, is also believed to be related to the crystallinity and interfaces of the perovskite.[15,16] Thus, the performance of perovskite solar cell strongly depends on the morphology and composition.[17–22] So far, many methods have been exploited to prepare perovskite films with excellent photon and electron properties through tuning nucleation growth and the resulting micro-morphology of perovskite films.[23] Compared with the one-step method, the two-step method offers the good controlling of morphology, and it is much more economical and convenient than the vapor deposition method. For the two-step method, an inorganic halide (e.g., lead (II) iodide, PbI2) layer is first deposited, whereupon organic ions (e.g., methyl ammonium iodide, MAI) are intercalated between the layers of edge sharing PbI6 octahedra and form the perovskite. Burschka et al. used this two-step method to fabricate a perovskite solar cell in 2013,[24] wherein the spin-coated and dried PbI2 layer was dipped in an appropriate 2-propanol solution with MAI. The process for PbI2 deposition in the sequential deposition was found to be crucial to the final MAPbI3 morphology and photovoltaic performance.[25] As a perovskite inorganic framework, the morphology of the original PbI2 may affect the reproducibility of the photovoltaic performance because high-quality perovskite thin film depends on the morphology of the PbI2 layer, dipping time, concentration and temperature of the MAI solution. In addition, the MAI penetration is a serious issue due to the volume expansion when the MAI is inserted into the PbI2 crystal lattice.[25,26] This will lead to incomplete transformation of PbI2 to perovskite on account of the fact that the initially formed MAPbI3 compact layer blocks the MAI from being diffused and inserted into the PbI2 layer. Moreover, the residual PbI2 has detrimental effects on the carrier separation and transportation. In the present work, we fabricate the materials with different surface morphologies (mainly surface coverage and different roughness) by adjusting the drying process of the PbI2 layer.[26] Then the influences of synthesis conditions on the microstructures of perovskite films and the optical-electrical performances of the cells are investigated.
2. Solar cell fabricationPatterned fluorine-doped tin oxide (FTO) substrates were cleaned in the solvents of detergent solution, acetone, ethanol and deionized water sequentially. Then the cleaned substrates were treated by UV-O3 for 15 min to make them well hydrophilic. After that, 50-nm thick compact TiO2 (c-TiO2) was formed on the cleaned FTO glass by spin-coating 0.15-M solution of titanium diisopropoxide bis (acetylacetonate) (75 wt% in isopropanol, Aldrich) in 1-butanol (99.8%, Aldrich) at 3000 r.p.m for 30 s, which was dried at 125 °C for 5 min, then the process was repeated once again. A mesoporous TiO2 (m-TiO2) layer composed of 20 nm-sized particles was deposited by spin-coating at 3000 r.p.m for 30 s by using a commercial TiO2 paste (18-NRT, Dyesol) diluted in ethanol (2:7, weight ratio). After drying at 125 °C for 10 min, the substrate was annealed at 500 °C for 30 min.
2.1. PbI2 layer fabricationPbI2 (99.99%, Sigma-Aldrich) was dissolved in several kinds of polar solvents (N, N-dimethylformamide, DMF,
, Sigma-Aldrich; N, N-dimethylsulfoxide, DMSO, 99.5%, Sigma-Aldrich) under stirring at 70 °C until its complete dissolution. The PbI2 precursor solution was spin-coated on the substrates (FTO/c- TiO2/m-TiO2) at 3000 r.p.m for 30 s within an N2 filled glovebox (deposition spinning details can be seen in Fig. 1). Also, different solutions used were simplified with A, B, C, and D, respectively, and then PbI2 films with different solutions would be prepared after the coating process. The precursor solution of 1-M PbI2 in DMSO and DMF/DMSO (92/8 v/v) mixture, which are marked with PbI2-DMSO and PbI2-DMF & DMSO, respectively. The preparation details of the PbI2 precursor film with 1-M final concentration are shown in Table 1.
Table 1.
Table 1.
Table 1.
The PbI2 precursor films prepared with different processes.
.
|
Method |
Precursor solution |
PbI2/g |
PbI2 film formation process |
I |
A |
DMF & DMSO (92:8, v/v) |
0.462 |
PbI2 solution was deposited by spin coating at 3000 r.p.m for 30 s under an N2 atmosphere within a glovebox, followed by immediately heating on a hot plate at 80 °C for 15 min. |
B |
DMF & DMSO (92:8, v/v) |
0.462 |
After the solution of PbI2 was spin-coated, the wet film was kept in a covered Petri dish at room-temperature within a glovebox for 10 min and then heated on a hot plate at 80 °C for 5 min. |
II |
C |
DMSO |
0.462 |
Before a spin coating procedure the substrates were preheated at 80 °C, and the PbI2 solution was deposited by repeating step a. |
D |
DMSO |
0.462 |
Repeating step a. |
| Table 1.
The PbI2 precursor films prepared with different processes.
. |
2.2. MAPbI3 layer fabricationTo convert the PbI2 layer into MAPbI3, after cooling the substrates to room temperature, PbI2 films were dipped into a solution of CH3NH3I (MAI,
, Xi’an Polymer Light Technology Corp.) in 2-propanol (10 mg/ml) for 10 min, rinsed with 2-propanol and dried at 100 °C for 10 min. The 60-
hole transport material (HTM) solution which consists of 72.3-mg Spiro-MeOTAD (2, 2′, 7, 7′-tetrakis-(N,N-di-4-methoxyphenylamino)-9, 9′-spirobifluorene,
, Merck),
of 4-tert-butyl pyridine and
of lithium bis (trifl uoromethanesulfonyl) imide (Li-TFSI,
, Sigma-Aldrich) solution (520-mg Li-TSFI in 1-ml acetonitrile (99.8 %, Sigma-Aldrich)) in 1 ml of chlorobenzen, was spin-coated on the perovskite layer at 3000 r.p.m for 30 s. Finally, an Ag electrode was deposited by thermal evaporator at a constant evaporation rate of 5 Å/s.
2.3. CharacterizationThe x-ray diffraction measurements were performed on the D8 DISCOVER diffractometer (Bruker D8D, Germany) in grazing incidence x-ray diffraction (GIXRD) mode. The XRD patterns in a range from 10° to 60° were recorded at room temperature by using Cu Kα radiation under the following measurement conditions: a tube voltage of 40 kV, tube current of 40 mA, step size of 0.04°, and 20 s per step. The value of the grazing incidence angle was 0.05°. The absorption spectra of perovskite films were characterized by a UV-Vis-NIR spectrophotometer (SHIMADZU, UV3600) with an integrating sphere in the interval of 600 nm–900 nm. The photoluminescence (PL) spectra were measured by using an integrated Raman system (Horiba Jobin Yvon LabRam HR-800) with an Olympus 10X lens (
). A 532-nm Nd-Yag laser (Laser Quantum, Torus 50 mW) was used as an excitation source and the wavelength scale was from 600 nm to 900 nm. The morphologies of perovskite films were observed by scanning electron microscopy (SEM, FEI Nova Nano 450). The current–voltage (J–V) characteristics of solar cells were measured with a fixed active area of 0.09 cm2 by using a xenon (USHIO, UXL-150SO) based solar simulator lamp (Newport Oriel Sol 1A) and a Keithley 2420 source meter under 1-Sun illumination (AM 1.5G 1000 W/m2) in air. All samples for characterization were prepared on the substrates FTO/c-TiO2/m-TiO2 with the same preparation procedure of thin films used in solar cells, unless otherwise stated.
3. Results and discussionThe PbI2 morphology-related reaction kinetics in the two-step method is assigned to heterogeneous nucleation, which leads to the formation of PbI2 nuclei on the m-TiO2 stack layers. The liquid nature of the film, augmented by the presence of a large amount of solvent, leads to subsequent crystal growth, where the extent of growth is controlled by adjusting the nucleation density and growth condition. Figure 2 shows the top views of PbI2 precursor films processed under different deposition conditions, each of which is composed of platelet-shaped PbI2 crystals that are between 100 nm and 400 nm in diameter. It is clear that there is a big difference in surface morphology, which is due to their different fabrication processes. As seen clearly from Figs. 2(a) and 2(b), the slow crystallization process prefers to generate polyporous crystals because of the slow solvent evaporation. The drying process of PbI2 film also helps to create larger pores and voids in the PbI2 crystals which penetrate through the whole film. This porous morphology is probably related to the controlled slow solvent evaporation in the sealed box. These loose cavities can enhance the penetration of MAI in the PbI2 layer during dipping, leading to the formation of perovskite. Thus, it can be seen that the morphology of the PbI2 film is likely to be influenced by the low-temperature drying process. Compared with the nanoparticles in mixed solvent, the nanoparticles in pure DMSO solvent have sizes of 250 nm–400 nm and stack with a PbI2 layer on the m-TiO2 film as shown in Figs. 2(c) and 2(d). The majority of voids are formed within the PbI2 layer, which is probably attributed to the high viscosity DMSO solvent and low nucleation density during the spin-coating process. Especially, the particulate network of PbI2 is very much sparser in appearance (Fig. 2(d)), and the surface coverage on the TiO2 film is smaller than that in the case of PbI2 formed by using the substrate-preheating technique. The coverage seems to be related to competition between the solvent evaporation rate and the PbI2 nucleation rate, that is, the PbI2 nucleation rate becomes higher than the solvent evaporation rate because the substrate pre-heating process increases the nucleation sites. In the case of PbI2 fabricated through process D, too much of a large gap forms in the grain and it is speculated that the MAPbI3 films could not cover the substrates completely during the following deposition process, which will be discussed later in this work.
The DMSO acts as both a solvent and a coordination reagent in the formation of a complex of PbI2·DMSO, while DMF behaves only as a solvent with a higher evaporation rate than DMSO (vapor pressure data are listed in Table 2). Because of the relatively low evaporation rate and high viscosity of pure DMSO, the coverage of the substrates is very poor, which is unfavorable for the formation of perovskite in the second dipping step. Meanwhile, the coverage of PbI2 film decreases if no pre-heating process is employed, which might be attributed to the hydrophobicity and large viscosity of DMSO. For mixed solvents, DMF solvent possesses a lower vapor pressure at room temperature which affects the morphology of the obtained PbI2 film via the slow crystallization process.
Table 2.
Table 2.
Table 2.
Typical physical parameters for DMF and DMSO solvents used for PbI2 precursor.
.
Solvent |
Density/(g/mL) |
Boiling Point/°C |
Viscosity/mPa·s |
Vapor pressure/(mmHg, 20 °C) |
DMF |
0.948 |
152–154 |
0.92 |
2.7 |
DMSO |
1.100 |
189 |
2.0 |
0.42 |
| Table 2.
Typical physical parameters for DMF and DMSO solvents used for PbI2 precursor.
. |
A series of MAPbI3 films is prepared from different PbI2 precursor films. For comparison, these perovskite thin films are denoted as PSC-a, PSC-b, PSC-c, PSC-d, respectively. Figure 3 shows the SEM images of the MAPbI3 films prepared. It can be seen that the grain sizes and coverage rates of the resulting perovskite films change significantly. All the samples exhibit similar cuboid crystals. However, PSC-a and PSC-b overlayer have better quality than PSC-c and PSC-d in the aspect of smoothness and compactness, especially PSC-b is nearly pinhole-free and has a relatively uniform surface (size distribution is shown in Fig. 3(f)). The PSC-a appears to be composed of small sized perovskite crystals (
), and its surface is covered with few uneven large cubic grain. The formation of coarse perovskite crystal usually appears during the Ostwald ripening process because of the dissolution-re-crystallization process (i.e., smaller perovskite crystals dissolve and re-deposit onto larger perovskite crystals). Obviously, the existence of slow crystallization at room temperature, with the same dipping time, is favorable for the large nanoparticles (cubic shape) on the surface MAPbI3 film, an observation that is assistant and supports that the dense PbI2 morphology impedes the penetration of MAI, so a portion of the formed small perovskites nanoparticles most likely continue to evolve by the above proposed mechanism.
In brief, the drying process at room temperature enhances the formation of larger pores in the PbI2 film and larger MAPbI3 particles, indicating the complete transformation of PbI2 into MAPbI3. In the case of pure DMSO used (PSC-c and PSC-d), the MAPbI3 films are mainly composed of large crystals (
) filled with
-nm small crystals, indicating the uneven coverage of the perovskite film. Without the preheating deposition, the gaps in perovskite film are formed (Fig. 3(k)) because localized nucleation gives rise to leakage current and direct contact between electron-and hole-transporting layers, resulting in serious charge recombination and deterioration of light absorption. These results reveal that the preheating of substrate has an important effect on PbI2 spin coating through ameliorating the surface morphology and improving the quality of the resulting MAPbI3 films.
Taking it into consideration that the reaction between PbI2 and MAI is a solid–liquid reaction, we believe that the reaction rate is determined by three major factors: (i) property of PbI2 film, such as preferential orientations of crystal, crystallinity and morphology of PbI2 precursor film; (ii) concentration of MAI/IPA solution; (iii) temperature of the reaction system. In our study, the latter two factors have been carefully controlled. So we believe that the great difference among PbI2 films in the preparation of perovskite comes from the morphology difference as shown in Fig. 2. Thus, controlling the morphology of PbI2 may adjust the number of nuclei of the perovskite, and then affect the morphology of perovskite and grain size. We control the morphology of PbI2 by adjusting the solvent polarity and drying process. Mainly, two main factors contribute to the faster conversion of nanoporous PbI2 into perovskite rather than compact PbI2: firstly, the interpenetrating nanoporous morphology enables the occurrence of reaction in the entire film simultaneously; secondly, the crystallite size is lower in the nanoporous PbI2 than those in the compact PbI2, shortening the diffusion length for MAI. In a word, the reaction is limited by the interface of PbI2(s)–MAI (l) and fresh MAPbI3, so the morphology of PbI2 film is affected indeed in the two-step method because a large volume expansion occurs when PbI2 converts into MAPbI3 (about 74.8 cm3–149.0 cm3) due to the density difference between originally edge-sharing octahedral PbI2 (6.16 g/cm3) and the corner-sharing octahedral perovskite (4.29 g/cm3).
In general, GIXRD is an effective tool to determine the surface crystallinity by changing the incident angle of x-ray. The samples are kept in a carefully controlled measurement condition, so the diffraction peak intensity is mainly determined by the crystallization, densification and components of the sample. The GIXRD patterns of the MAPbI3 films obtained from PbI2 are shown in Fig. 4. All film samples consisting of a cubic crystal phase possess similar patterns but with different diffraction intensities. The strong diffraction peaks at 14.21°, 20.68°, 24.57°, 28.52°, 31.90°, 35.04°, 40.62°, and 43.19° could be ascribed to (002), (022), (222), (004), (042), (422), (044), and (006) planes of the MAPbI3 perovskite, respectively. Apart from the cubic character of an obvious perovskite phase with the space group of F23, a small number of PbI2 phases exist in the PSC-d sample (the rose red curve in Fig. 4), and the peak at 12.73° corresponds to the (001) lattice plane of PbI2, which indicates incomplete conversion of PbI2. In combination with the SEM result, we speculate that the rough and nonuniform stacking nature of PbI2 crystal retards the diffusion of MAI and therefore results in the subsequent incomplete conversion of PbI2.
The higher intensity in the PSC-b film should be attributed to the slight thickness of the sample, or uniformly distributed nanocrystals and complete crystallization of the sample. Furthermore, the slight differences in lattice constant and full widths at half maximum (FWHMs) for different films imply that the PbI2 precursor film only influences the perovskite film coverage and morphology without causing significant changes in the crystalline structure of the material.
Table 3 shows the lattice constants and FWHMs of the diffraction peak at
. The average grain size D of the MAPbI3 nanocrystals can be estimated from the (002) peak at 14.2° by using the Scherrer equation:
, where k is the Scherrer constant (equal to 0.89), λ is the x-ray wavelength (equal to 0.154 nm), θ is the Bragg diffraction angle, and β is the FWHM of the (002) diffraction peak. The FWHMs of the (002) diffraction peaks are 0.350, 0.381, 0.423, and 0.377, which correspond to average grain sizes of 22.6, 20.8, 18.7, and 21.0 nm for the PSC-a, PSC-b, PSC-c, and PSC-d sample, respectively.
Table 3.
Table 3.
Table 3.
Lattice constants of MAPbI3 films.
.
Sample |
a/Å |
Vol/Å3
|
FWHM |
Grain size |
PSC-a |
12.560 |
1981.385 |
0.350 |
22.6 |
PSC-b |
12.578 |
1989.916 |
0.381 |
20.8 |
PSC-c |
12.618 |
2008.961 |
0.423 |
18.7 |
PSC-d |
12.582 |
1991.815 |
0.377 |
21.0 |
| Table 3.
Lattice constants of MAPbI3 films.
. |
Figure 5 shows the absorption spectra and PL spectra of the corresponding PSC films. Their absorptions cover a wide range of light wavelengths from visible to the near-infrared region. All of these films exhibit the same absorption shoulders near 750 nm, which is typical nature for the MAPbI3 phase. As a result of the poor coverage of the substrate by film when MAPbI3 is prepared with pure DMSO solvent, their absorptions are lower than those of the MAPbI3 fabricated with mixed solvents, which is more prominent in the short wavelength region (350 nm–550 nm). The PSC-b shows the most enhanced absorption, which is related to the improved morphology and coverage rate. In addition, it can be seen that MAPbI3 films prepared with DMF/DMSO mixed polar solvent have strong absorptions, indicating that more PbI2 nanoparticles are converted into MAPbI3 nanoparticles. The increase in absorption supports that the loose structure assembled from PbI2 nanoparticles allows MAI to reach the interior of PbI2 very easily and facilitates the complete transformation of PbI2. The characteristic absorption shoulder near 750 nm for PSC-c film increases slightly, which reflects the stronger light-scattering effect associated with abnormally large grains. This result reveals that good surface morphology of the MAPbI3 film is important for the light absorption of the perovskite solar cell. Figure 5(b) shows the steady-state PL spectra of perovskite films excited at 532 nm. The PL quenches at around 776 nm, which is consistent with the behavior of the optical gap from the absorption spectra. These results suggest that the controlled growth of PbI2 scaffolds could be a useful new route to manipulating the morphology of the perovskite active layer, opening new possibilities for enhancing device performance.
The photovoltaic performances of the fabricated PSCs based on FTO/c-TiO2/m-TiO2/MAPbI3/HTM/Ag architecture are examined and the current–voltage (J–V) characteristics are measured in the reverse bias condition (
) under standard AM 1.5G illumination, with an effective area of 0.09 cm2. All the performance parameters such as short-circuit current density (
), open circuit voltage (
), fill factor (FF) and power conversion efficiency (PCE) are summarized in Table 4, which are achieved by a reverse bias scan. The solar cell with the PSC-b perovskite film exhibits a highest PCE performance of 11.59% with
of 21.86 mA/cm2,
of 0.882 V and
of 60.73 as expected. Meanwhile, the PCE of PCS-b keeps a high level of more than 93% of the initial efficiency (from 11.59% to 10.87%) after 43-day storage in air (Fig. 6(b)).
Table 4.
Table 4.
| Table 4.
Photovoltaic parameters of devices with different fabrication methods.
. |
For mixed solvents, the higher PCE of PSC of the material prepared by method B is attributed to the PbI2 scaffold with mesoporous structure, which promotes the conversion process of and less damage to perovskite. In addition, many studies have shown that a larger perovskite grain size can reduce the interfacial area, which can hinder charges from being collected. Larger grains also possess less bulk defects and higher mobilities, so the photo-generated carriers could be collected more easily.[27,28] We note that Yi et al.[29] reported solar cells based on bilayer porous lead halide (PbX2, containing PbI2 and PbBr2) films prepared by using PbX2 solutions of DMF/DMSO mixed-solvent. The MAI solution can easily diffuse through the PbI2 film and react with PbI2 more completely because of the continuous mesoporous structure. At the same time, these pores also provide the space needed to accommodate the large volume expansion and the insertion of the organic cations into the PbI2 lattice. The interpenetrating nanoporous morphology enables fast penetration of the MAI solution during the conversion step, and perovskite grains can grow freely and form a compact MAPbI3 film. For pure DMSO solvent, PCE of 3.92% is achieved without pre-heating and increases to 5.22% when the substrate is heated to 80 °C. The pre-heating treatment can lead to the increase of photocurrent and voltage. By contrast, the PbI2-DMSO based device suffers relatively low
and FF, which is attributed to the poor coverage with high leak current and low light-harvesting. The coverage of PbI2 film on the m-TiO2 layer decreases when only DMSO is used as solvent, because the hydrophobicity and high viscosity of DMSO make it difficult to spread on the substrate surface. In addition, since the substrate surface can provide nucleation sites for the nucleation of crystals, pre-heated substrate is likely to play a positive role in nucleating. And a higher coverage of perovskite layer is beneficial for the light absorption, leading to higher photocurrent and voltage.