Cheng Gaoab,
Jiang Liu*b,
Cheng Liaob,
Qinyan Yeb,
Yongzheng Zhangb,
Xulin Heb,
Xiaowei Guo*a,
Jun Meib and
Woonming Laub
aSchool of Optoelectronic Information, University of Electronic Science and Technology, Chengdu, 610054, China. E-mail: guosnu@gmail.com
bChengdu Green Energy and Green Manufacturing Technology R&D Centre, Southwest Airport Economic Development Zone, Shuangliu, Chengdu, 610207, China. E-mail: 546jiang@163.com
First published on 6th March 2015
Organic–inorganic hybrid perovskites were prepared by thermal evaporation from precursor materials PbCl2 and CH3NH3I (MAI). The structures of the perovskite films with various ingredients were characterized by X-ray diffraction (XRD), UV-vis absorption, and scanning electron microscopy (SEM). We found that with the addition of MAI material the evaporated PbCl2 films were initially transformed to PbI2, then to standard a stoichiometric perovskite and finally to the MAPbI3·xMAI phase. The film composition ingredients strongly affect the device performance. An unmatched PbCl2 to MAI ratio in the evaporated films resulted in reduced conversion efficiency and higher moisture sensitivity. The planar perovskite solar cells with organic charge layers showed negligible photocurrent hysteresis and delivered a power conversion efficiency of 10.5%.
Various processing techniques, including thermal evaporation,11,13–15 vapor assisted solution process,16 one-step6,7,10 and two-step solution process,9,12,17 have been used for the preparation of high quality perovskite absorbers. For the solution process, a great deal of effort has been put to control the morphology of the resulting film by adjusting the annealing condition,18,19 using additives20–22 and mixed solvents,8 etc. In contrast, evaporation can offer inherent advantages in obtaining perovskite film with excellent coverage, high material purity and good thickness control. Liu et al.11 first demonstrated vapor-deposited perovskite solar cell with a simple planar device structure. Their findings showed great promise for preparing efficient planar perovskite solar cell by evaporation. Malinkiewicz et al.15 reported an inverted planar perovskite by evaporation, sandwiched between two organic charge transport layers. This inverted structure allows a relative low processing temperature for fabricating perovskite solar cells. In addition, the evaporation process is free of organic solvent, which may erode the underlying charge layer, thus allowing more choice of organic charge materials.23
In this paper, we present a detailed study of the evaporated perovskite film under various evaporation conditions. Based the previously reported results3,24 that the addition of chloride could dramatically increase the photoluminescence lifetime of the photoexcited species and charge diffusion lengths in the absorber, we adopted the PbCl2 and MAI as the precursor materials. The effect of PbCl2 to CH3NH3I (MAI) ratio on structural, optical and electrical properties of evaporated perovskite films was investigated. Using the planar device structure with low-temperature processed organic charge layers, we obtained an optimal device with an efficiency of 10.5% which didn't show obvious hysteresis.
Sample | Evaporation rate ratio yrt | Evaporation rate (Å s−1) | EDX composition | |||
---|---|---|---|---|---|---|
CH3NH3I | PbCl2 | Pb (at%) | I (at%) | Cl (at%) | ||
a The evaporation rate ratio of CH3NH3I to PbCl2 is referred to as yrt, and yrt = 0 means only PbCl2 film was deposited. | ||||||
S1 | 0 | 0 | 2 | 35.55 | 0 | 64.45 |
S2 | 2 | 4 | 2 | 32.18 | 62.10 | 5.72 |
S3 | 3 | 6 | 2 | 25.96 | 73.43 | 0.60 |
S4 | 4 | 8 | 2 | 19.86 | 79.96 | 0.18 |
In order to identify the phase constitution, X-ray diffraction (XRD) analysis was conducted to study the structural evolution of evaporated perovskite films at different deposition conditions. Fig. 1a shows the XRD patterns of four samples listed in Table 1. Much difference can be observed between the samples deposited with different amounts of MAI. When only PbCl2 (yrt = 0) is deposited, the sample exhibits peaks at 19.9°, 23.0°, 25.1° and 32.4°, which is in agreement with PbCl2 XRD data according to JCPDS card 26-1150. For the sample with deposition condition yrt = 2, the peak positions of the X-ray reflection are comparable to the powder-diffraction standard data (JCPDS 07-0235) for PbI2, indicating the formation of PbI2 from the reaction of PbCl2 and MAI. It can be also seen that the PbCl2 peaks disappear entirely although there was a little Cl (5.72 at%) contained in the film, which can be explained by low crystallinity of possible remaining PbCl2 or limited determination precision of XRD used. In this case, no peaks related to perovskite MAPbI3 phase are found from the XRD pattern, indicating the amount of evaporated MAI is not sufficient. As the amount of MAI was further increased (yrt = 3), two strong peaks appear at 14.2° and 28.5°, which correspond to the perovskite CH3NH3PbI3 (110) and (220) crystalline planes, respectively. Compared with the mesostructured perovskite layers in other literatures,17 the evaporated planar perovskite film shows an extremely preferred orientation along (110) plane, perhaps due to lack of the restrictions from oxide scaffolds in the formation of the perovskite layer. For the samples with deposition condition yrt = 4, some extra peaks appeared, which means that the amount of evaporated MAI is too-much. In contrast to the X-ray diffractogram of powdered MAI in Fig. S3,† we found those extra peaks don't originate from the MAI material and may be attributed to the possible compound MAPbI3·xMAI.
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Fig. 1 (a) XRD spectra, (b) UV-vis absorbance and (c–g) photographs of the evaporated films at different deposition conditions. |
In Fig. 1b–g we present UV-vis absorption spectra and photographs of the samples with different deposition rate ratios. The PbCl2 film shows white color and an extremely low absorbance. When the amount of MAI is insufficient, the sample exhibits a yellow color due to the presence of PbI2. When amount of MAI is moderate or excess, the samples after annealing exhibit a dark brown color due to the formation of perovskite phase, and the corresponding absorbance spectra also display an onset of drop at 780 nm, which is in agreement with previously reported results.7 Additional features related to the stability must be also mentioned. The perovskite film with moderate MAI demonstrated good stability, as evidenced by the absorbance spectra change over time (Fig. S4†). In contrast, the perovskite film with excess MAI exhibits rapid degradation in absorbance and the film color varies from dark brown to white (Fig. 1g) after exposing to the air (relative humidity more than 60%) for only 20–30 min. It is noted that the degradation is probably different from the hydrolyzation of perovskite to yellow PbI2. However, the transition is reversible. The brown dark perovskite phase will recover again upon heating. Similar results shown in Fig. S2† were also found for the samples with surface composition gradient. We believe that the excess MAI in the perovskite film affects the morphology and crystalline phase, thus reducing the environmental stability.
To further investigate the morphology of the films, we performed SEM analysis. Fig. 2 shows the SEM micrographs of the evaporated films deposited with different MAI to PbCl2 ratios. It can be seen that all the films have dense microstructures and show a 100% coverage which is hard to realize in solution-processed films. When the film was deposited with either PbCl2 (yrt = 0) or insufficient MAI (yrt = 2), the grain size of the films is within a small range. For the film with yrt = 3, considerable grain growth with smooth surface can be observed. Smooth films could lower the dark current and reduce the density of interface states,26 which is essential for fabricating a high-quality planar solar cell. When yrt was increased to 4, loose porous surface morphology was formed. The significant difference can be contributed to the presence of excess MAI due to its high surface activity and hygroscopic nature.
The above structural and optical results predict that the perovskite film with yrt = 3 should yield good photovoltaic performance. To find the optimal deposition condition, detailed optimizations of evaporation rate ratios around yrt = 3 were carried out. Three perovskite solar cells with FTO/PEDOT:PSS/Perovskite/PCBM/Ag planar structures were prepared. Fig. 3 shows a cross-sectional SEM image of the complete device. The thicknesses of PEDOT:PSS, Perovskite and PCBM layers are about 30 nm, 400 nm and 100 nm, respectively. The average device parameters with the standard deviations are summarized in Table 2. It is observed that three sets of cells demonstrated a low statistical spread in open circuit voltage (Voc), which can be explained by good coverage of the evaporated perovskite films. The main differences in the solar cells performance result from fill factor (FF) and short circuit current density (Jsc). For the solar cells with yrt = 3, the average short circuit current density (Jsc) is only 9.08 mA cm−2, which may be attributed to the non-exactly-matching of MAI to PbCl2 ratio. When the deposition ratio yrt reaches 2.9, the mean power conversion efficiency (PCE) of 7.61% was achieved with increased Jsc and FF. Reducing yrt to 2.8 results in decreased PCE. Therefore, the optimal deposition ratio yrt determined in this work is 2.9.
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Fig. 3 Cross-sectional SEM image of a complete FTO/PEDOT:PSS/CH3NH3PbI3−xClx/PCBM/Ag perovskite device (inset shows a photograph of the perovskite device). |
Evaporation rate ratio yrt | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) |
---|---|---|---|---|
3.0 | 0.87 ± 0.03 | 9.08 ± 1.86 | 0.50 ± 0.05 | 3.87 ± 0.61 |
2.9 | 0.87 ± 0.07 | 14.68 ± 2.52 | 0.59 ± 0.02 | 7.61 ± 1.60 |
2.8 | 0.78 ± 0.08 | 15.89 ± 2.68 | 0.52 ± 0.06 | 6.48 ± 1.18 |
Recently, there has been increasing discussion as to the photocurrent hysteresis in perovskite devices.27,28 To understand the phenomenon of the fabricated perovskite solar cells, the PCE differences were investigated under the forward and reverse scans. 20 devices at the process condition of yrt = 2.9 were prepared. Their performances were characterized under forward (−0.2 V → 1.2 V) and reverse (1.2 V → −0.2 V) scans. The results are shown in Table 3 where detailed photovoltaic parameters are listed in Table S1.† Fig. 4 shows the current–voltage (J–V) curves for the best performing device measured under forward and reverse scans. The champion device (Fig. 4a) exhibited a Jsc of 17.3 mA cm−2, FF of 0.63, Voc of 0.97 V, and PCE of 10.50% under forward scans, and a Jsc of 17.0 mA cm−2, FF of 0.63, Voc of 0.97 V, and PCE of 10.32% under reverse scans. Fig. 4b shows the external quantum efficiency (EQE) curve for one optimized device. The EQE curve starts increasing rapidly at 800 nm, which is related to the optical absorption of the perovskite absorber, reaches a maximum value of 71% at 560 nm, and then drops slowly at about 400 nm. From Fig. 4a, the champion device doesn't show obvious hysteresis of photocurrent. However, the statistics result (see Fig. 5) shows the devices under reverse scans have a 0.66% PCE higher than that under forward scans. The higher efficiency under reverse scans mainly results from a slightly higher Voc by 0.03 V and Jsc by 1.08 mA cm−2. Compared to TiO2-based perovskite planar solar cell in other literatures,8 the difference is rather small, which could be explained by the difference of perovskite preparation process or charge separation interfaces. There is still great room to further increase the conversion efficiency. The best device in this study shows a Voc close to 1 V, and its performance is mainly limited by the relatively low FF and Jsc, which may indicate that the charge transport and collection for the solar cells are not still very efficient. Further understanding and optimization of the device structure, apart from the process control, may help improve the device performance.
Evaporation rate ratio yrt | Scan direction | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) |
---|---|---|---|---|---|
2.9 | Forward | 0.85 ± 0.11 | 13.63 ± 3.29 | 0.58 ± 0.10 | 6.91 ± 2.47 |
Reverse | 0.88 ± 0.09 | 14.71 ± 2.67 | 0.57 ± 0.04 | 7.57 ± 2.06 | |
Best | 0.97 | 17.30 | 0.63 | 10.50 |
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Fig. 4 (a) J–V curves for the best performing perovskite solar cell measured under forward and reverse scans. (b) External quantum efficiency of a perovskite device with deposition ratio yrt = 2.9. |
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c4ra17316c |
This journal is © The Royal Society of Chemistry 2015 |