Shenghao
Wang
,
Luis K.
Ono
,
Matthew R.
Leyden
,
Yuichi
Kato
,
Sonia R.
Raga
,
Michael V.
Lee
and
Yabing
Qi
*
Energy Materials and Surface Sciences Unit (EMSS), Okinawa Institute of Science and Technology Graduate University (OIST), 1919-1 Tancha, Kunigami-gun, Onna-son, Okinawa 904-0495, Japan. E-mail: Yabing.Qi@OIST.jp
First published on 28th May 2015
We provide details on the development of instrumentation and methodology to overcome the common difficulties that the vacuum-related techniques face for fabrication of perovskite thin films and perovskite solar cells (PSCs). Our methodology relies on precisely controlling the flow of methylammonium iodide (CH3NH3I, MAI), which has a high-vapor pressure nature, and the deposition rate of metal halides (PbCl2 or PbI2). This hybrid deposition method allows the growth of perovskite films with smooth surface, good crystallinity, high surface coverage, uniform chemical composition and semi-transparency. We also systematically investigated the effects of the evaporation source materials (PbCl2:
MAI versus PbI2
:
MAI), substrate temperatures, and post-annealing on the properties of perovskite films, as well as device performances based on this method. By employing a thin perovskite film (<200 nm), the power conversion efficiency of PSC can be as high as 11.5%.
Perovskite thin films can be prepared by a range of deposition techniques, such as spin-coating,11,18–20 co-evaporation,14,15,21,22 vapor assisted solution process (VASP),23 hybrid chemical vapor deposition (HCVD),24 vacuum sequential deposition,25,26 and spray-deposition.27 Generally, mesoporous metal oxides (e.g., TiO2 and Al2O3) are used to obtain high PCEs for solution-based methods, in which perovskite is scaffolded by the mesoporous matrices.18,28–32 However, it requires a high-temperature sintering process, limiting the application on flexible substrates.15 Although the planar-type device architecture is particularly attractive due to its simple cell configuration and possible fabrication using a solution process, depositing a homogeneous perovskite film with a thickness comparable to the charge diffusion length has been proven to be difficult.14,33
On the other hand, vacuum evaporation methods offer some unique advantages. (1) Vacuum evaporation methods are desirable to achieve high-purity films, because the films are formed in a vacuum chamber by sublimation of powder materials after extensive outgassing. (2) The initial nominal stoichiometry of methylammonium iodide (CH3NH3I, MAI) and lead halides can be well controlled in both solution and vacuum evaporation methods. However, in solution methods the solubility of reactants in solvents is an additional parameter that needs be considered. For example, it is difficult to dissolve PbCl2 in N,N-dimethylformamide when the MAI:
PbCl2 molar ratio is lower than 3
:
1.32 In this sense vacuum evaporation methods are advantageous because the ratio of the two reactants (i.e. lead halide and MAI) can be tuned and therefore it is not limited by solubility. (3) It is suitable to prepare multi-layered structures of thin films to fine tune the charge collection/injection properties at interfaces among multilayers34,35 or precisely control the electrical properties by doping, a well-established technique in organic solar cells and organic light-emitting diodes.36,37 (4) Perovskite films can be deposited by a vacuum evaporation method on a variety of substrates without concerning solvent compatibilities allowing different device architectures with various contact buffer layers: TiO2,14 NiO/CuSCN,22 poly(3,4-ethyene dioxythiophene):(polystyrene sulfonic acid) (PEDOT:PSS),21 and poly(N,N′-bis(4-butylphenyl)-N,N′-bis(phenyl)benzidine) (poly-TPD).15,21 (5) In addition, vacuum evaporation methods are compatible with conventional processing methods that have been well established for silicon, cadmium telluride (CdTe) and copper indium gallium (di)selenide (CIGS) solar cells. Hybrid tandem junction solar cells obtained by combining PSCs with these first- or second-generation solar cells are very promising to obtain solar cells with even higher efficiencies.
Despite the aforementioned advantages, to date only a handful of studies have utilized vacuum-based deposition to fabricate perovskite layers and solar cells, in sharp contrast to a myriad of solution-based methods and their variants.38–41 Liu et al.14 and Subbiah et al.22 reported uniform deposition of perovskite layers by co-evaporating PbCl2:
MAI. Similarly, Malinkiewicz et al. fabricated PSCs with a PCE as high as 14.8% by using PbI2 and MAI as evaporation materials.15,21 However, difficulties in calibrating the quartz crystal thickness monitor parameters for MAI were mentioned in all these studies as a key challenge to achieve reproducible and controlled film preparation. The evaporation rate of MAI is difficult to be calibrated and controlled because of its relatively high vapor pressure. To solve such a challenge, our group recently developed a new methodology (the hybrid deposition method) to monitor the deposition rate of MAI by orientating the thickness monitor opposite to the evaporation direction of MAI to avoid the cross-talk from the metal halide source.42 Also, a two-step sequential deposition method was recently reported for the fabrication of PSCs.25,26 In this method, a metal halide layer was first deposited on the substrate, and then the MAI layer was subsequently deposited. However, the MAI diffusion depth is limited leaving the bottom metal halide layer unreacted.25 Additionally, similar difficulties faced in the co-evaporation method are also encountered in the sequential deposition method.
In this work, we first present the key challenges of the vacuum-based deposition methods and show how our hybrid deposition method can be used to alleviate these issues. Then we systematically study the effects of evaporation source materials (PbCl2:
MAI versus PbI2
:
MAI), substrate temperatures, and post-annealing on the perovskite film quality (i.e. coverage, uniformity, and crystallinity), as well as device performance. Using optimized conditions, we were able to reliably deposit perovskite films with very smooth surface, good crystallinity, high surface coverage, uniform chemical composition and semi-transparency. PSCs with high performance can be achieved at room temperature. Such a comprehensive study is expected to not only provide a full guide of convenient and reliable fabrication of PSCs by the hybrid deposition method, but also provide insight into the development of a low cost building integrated photovoltaic (BIPV) window.
Considering the challenges to control the individual deposition rates as mentioned above, we developed the hybrid deposition method to precisely control the deposition rates of both materials and the film thickness to obtain a high quality perovskite film. Fig. 1 shows the schematic illustration of the deposition setup. Metal halides (PbCl2 or PbI2) and MAI were used as evaporation source materials. Substrates are placed on a sample holder at a distance of ∼25 cm above the metal halide source. To achieve a high level of film thickness and composition uniformity, two widely open dish-like crucibles are used for evaporating the two source materials. A shield is fixed between the two sources, in order to minimize the thermal “cross-talking” between them, and in particular, to reduce the influence of the metal halide source heating on the MAI source. Such a consideration is often necessary when evaporating two materials with distinctively different evaporation temperatures, e.g., PbI2 typically evaporates at ∼250 °C while MAI evaporates at only ∼70 °C. A shutter with a diameter larger than that of the source crucible is used. It should be emphasised that this shutter is always closed during the evaporation of MAI. The shutter blocks the direct deposition of MAI and avoids the high flux of MAI hitting directly the substrate area, which may cause the non-uniform composition in the film.
There are two sensors in the chamber. The density, z-factor and tooling factor parameters of sensor 1 are set to be 5.85 g cm−3, 0.8 and 7, respectively. For sensor 2, they are nominally set to be 0.2 g cm−3, 0.2, and 3. These optimized parameters enhance the sensitivity of sensor 2 for the rate detection of MAI. The effect of MAI evaporation on sensor 1 is expected to be minimal because MAI has a much smaller density than metal halides. Therefore sensor 1 mainly monitors the rate of metal halides. Sensor 2 is located at the MAI source side and its height is below the height of the shield that separates the two sources. Therefore, it only detects the nominal deposition rate of MAI without the influence of the metal halide source. Further details on the optimization procedure for sensor 2 can be found in the ESI.†
In the hybrid deposition method, after the substrates (multiple substrates can be mounted depending on the substrate size) are transferred into the chamber (base pressure < 4.0 × 10−6 Torr), the metal halide source is heated and the rate is monitored by sensor 1. After reaching a certain rate on sensor 1, we start to heat MAI. As MAI vapor is produced, the pressure inside the chamber increases substantially to ∼10−3 Torr. The evaporation of MAI relies primarily on controlling the vapor and flow of MAI inside the chamber. By optimizing the MAI vapor pressure and flow, a precise control of the deposition rate for MAI can be achieved. The control of pressure is crucial, because if the pressure is too high, it will eventually affect the vapor flow condition and influence the rate of metal halides. To avoid this detrimental effect, a gate valve is used to maintain the pressure constant at a value of ∼3 × 10−3 Torr. The gate valve also allows the control of the MAI vapor pressure inside the chamber (i.e., setting the gate valve to a pre-determined opening position) without being pumped out, resulting in a more efficient use of MAI. An additional pumping line (HiCube80, Pfeiffer) is connected at the top part of the chamber (at the same height as the samples), which provides better vapor flow uniformity across the substrate surface. The uniform vapor flow makes the sensor 2 reading stable and is key to achieve reproducible film deposition. Typical readings of PbI2 and MAI from sensors 1 and 2 are shown in Fig. S2 ESI.† When metal halides and MAI meet on the substrate, the reaction occurs to form perovskite. When the desired thickness is achieved, the heating of the two sources is stopped and the gate valve is immediately opened to quickly pump out the remaining vapor of excess MAI to avoid the formation of a MAI rich layer on the sample surface. Then the samples are transferred to a home-designed nitrogen suit-case immediately after the completion of evaporation that avoids air exposure induced contamination or degradation of perovskite films.
For the co-evaporation method, it is important to precisely control the composition of films by choosing suitable evaporation rates for the two source materials. In the co-evaporation system described by Liu et al., the optimized molar ratio of PbCl2:
MAI = 1
:
4 was used.14 On the other hand, Subbiah et al. reported the optimized molar ratio of PbCl2
:
MAI to be 1
:
5.4,22 substantially different from Liu et al.'s report. This suggests that the optimal rates and ratio between the two source materials are highly dependent on the deposition system, which is another indication of unusual evaporation properties of MAI. To understand the perovskite film formation and to further control the film growth, it is necessary to investigate the properties of the films prepared at different evaporation rate ratios of PbCl2
:
MAI.
First of all, it is necessary to characterize the properties of the pure PbCl2 layer and MAI film, such as XRD features and morphologies. In addition, PbI2 sometimes exists in the perovskite film even though the precursors are PbCl2 and MAI.16 The morphology properties and XRD spectra of PbCl2, PbI2 and MAI films deposited by the hybrid deposition method are shown in Fig. S1 and S3 ESI.†Fig. 2(a) shows the XRD spectra of the films prepared by the hybrid deposition method using different evaporation rate ratios between PbCl2 and MAI. Films 1 to 6 correspond to the samples using the decreasing evaporation rate ratio of PbCl2:
MAI from 0.76 to 0.21. XRD features differ as the evaporation rate ratio varies. When the ratio is 0.76 (film 1), three main diffraction peaks at 15.6°, 31.5° and 48.0° are found, corresponding to the CH3NH3PbCl3 phase.14,16 Phase purity is inferred from the XRD spectrum, because no peaks associated with remaining PbCl2 and other phases of perovskite such as CH3NH3PbI3 are observed. The decrease in the PbCl2
:
MAI ratios (0.61 for film 2 and 0.52 for film 3) induces a mixture of CH3NH3PbCl3 and CH3NH3PbI3 phases, as well as PbI2 indicated by the diffraction peak at 12.6°. When the PbCl2
:
MAI ratio is further decreased to 0.39 (film 4), the XRD spectrum only shows 14.0°, 28.3°, and 43.0° diffraction peaks, corresponding to the (110), (220) and (330) planes of the halide perovskite CH3NH3PbI3 film with an orthorhombic crystal structure.14 If the ratio of PbCl2
:
MAI decreases to 0.30 (film 5), except for the main diffraction peaks of CH3NH3PbI3, a new diffraction peak at 11.4° appears in the XRD patterns. This peak is likely associated with a H2O-incorporated perovskite complex formed during the ex situ XRD measurements due to the excess MAI in the perovskite film.45–47 In addition, the intensity of the perovskite peaks of film 5 becomes lower than that of film 4. With further decrease of the ratio of PbCl2
:
MAI to 0.21 (film 6), the perovskite peaks completely disappear and three distinct peaks at 9.7°, 19.6° and 29.6° dominate the XRD pattern, which corresponds to the formation of a MAI rich film. The diversity of the presented XRD spectra suggests not only the importance of precise control of the ratio between PbCl2 and MAI, but also provides vital information regarding the reaction, which will be discussed in the next section.
The morphological properties of the films with different phases, namely films 1, 3, 4 and 5, were characterized by AFM measurements, as shown in Fig. 2(b). Root mean square (RMS) is used to quantify surface roughness. The films 1, 3 and 4 show uniform and full coverage on the substrates, while film 5 is not uniform. The pure CH3NH3PbCl3 film (film 1) has a very smooth surface (RMS = 2.9 nm) with a grain size of ∼50 nm. When the film consists of a mixture of CH3NH3PbCl3 and CH3NH3PbI3 (film 3), two distinct features with both small and big grains are observed from the AFM image, which may represent the chloride and iodide perovskites, respectively. The pure CH3NH3PbI3 film (film 4, RMS = 11.3 nm) has a much bigger grain size of ∼100 nm. When the excess MAI is contained in the film (film 5), the film shows a substantially rougher surface (RMS = 76.7 nm).
High resolution X-ray photoelectron spectroscopy (XPS) and X-ray fluorescence (XRF) measurements were carried out to determine the chemical composition of the perovskite films. Fig. 3 shows the XPS spectra of the top surface of films 3, 4 and 6. The Cl 2p peak is observed only in film 3 (Fig. 3(a)), which is assigned to the CH3NH3PbCl3 phase. In the case of the absence of CH3NH3PbCl3 for film 4, there is no Cl peak. The XRF results show that the atomic ratio of I/Pb in the bulk of film 4 is around 3.01 (see Fig. S4 of ESI†), suggesting that this perovskite film has well matched stoichiometry. This is also consistent with the pure CH3NH3PbI3 phase as revealed from the XRD result as discussed above. Although XPS is a surface-sensitive technique providing chemical elemental information with a probing depth of a few nanometers, we suppose that a negligible amount of Cl is incorporated into the bulk film. This result is consistent with the report by Yu et al., in which XPS depth profile measurement by sputtering the perovskite films (prepared by the solution method, around 310 nm thick) with an Ar ion gun was performed to investigate the chemical composition from the surface to bulk.43 No signal related to the Cl 2p photoelectrons was found in the bulk perovskite film and only 1% Cl could be detected at the bottom 20 nm of the film.43 Therefore, the chemical formula of “CH3NH3PbI3” is more precise than “CH3NH3PbIxCl3−x” to represent the perovskite in this work. The peak positions of I 3d, Pb 4f, C 1s and N 1s core levels (Fig. 3(b)–(e)) for films 3 and 4 are nearly the same, because the chemical environments for these elements are similar for CH3NH3PbCl3 and CH3NH3PbI3. The C 1s core levels show two distinct peaks, which are assigned to C–N and C–C bonds, respectively.48 For film 6, both C 1s and I 3d core levels shift to higher binding energies, which is attributed to the charging effect by the rich MAI film. Thus, the XPS results presented here corroborate the XRD results. In addition, a minimal oxygen level (Fig. 3(f)) is present in the XPS measurements, confirming the cleanness of the sample.
To investigate the influences of the compositions of the perovskite films on the device performances, PSCs were fabricated employing films 1 and 4. The device structure is FTO/TiO2 (70 nm)/perovskite (50 nm)/spiro-MeOTAD (100 nm)/Au (100 nm), as illustrated in Fig. 4(a). Fig. 4(b) shows the J–V curves of the devices with different compositions in perovskite films. The device with film 1 exhibits very poor photovoltaic properties because of the large bandgap (3.1 eV) of CH3NH3PbCl3,49 which is almost colorless and a poor light absorber. The device employing film 4 shows a reasonable PCE with an open-circuit voltage (Voc) of 1.029 V, a short-circuit current (Jsc) of 13.14 mA cm−2, a fill factor (FF) of 42.67%, and an overall PCE of 5.77% under 1 sun illumination. This is because the absorber layer of film 4 is pure CH3NH3PbI3 perovskite, which has strong light absorption and good charge-transport properties for photo-generated free carriers. We observed that the devices show hysteresis (see Fig. S5 of ESI†), which is commonly observed in planar structured perovskite solar cells.
Interestingly, the XRD features of the perovskite films are different in the cases of PbCl2 and PbI2. The number of diffraction peaks of perovskite films formed from PbI2:
MAI is much larger than that from PbCl2
:
MAI. Fig. 5(b) shows the XRD spectra of perovskite films prepared from PbCl2
:
MAI and PbI2
:
MAI under optimized conditions. The perovskite film prepared from PbCl2
:
MAI is more oriented than that from PbI2
:
MAI. Based on the discussion of the XRD patterns, the following reaction steps are proposed to take place for the perovskite film formation.18
PbCl2 + 2CH3NH3I → 2CH3NH3Cl + PbI2 | (1) |
PbCl2 + CH3NH3Cl → CH3NH3PbCl3 | (2) |
PbCl2 + 3CH3NH3I → CH3NH3PbI3 + 2CH3NH3Cl | (3) |
PbI2 + CH3NH3I → CH3NH3PbI3 | (4) |
In the PbCl2 case, when excess PbCl2 is present, reactions (1) and (2) occur, forming a pure CH3NH3PbCl3 film. As the ratio of PbCl2:
MAI reduces, the formed film consists of CH3NH3PbCl3 and CH3NH3PbI3 and/or PbI2via reactions (1), (2) and (4). This suggests that MACl is generated when MAI is insufficient, because the reaction (1) must occur to form a pure CH3NH3PbCl3 phase. When the PbCl2
:
MAI ratio is further decreased to reach the matched stoichiometry, the pure CH3NH3PbI3 phase forms by reaction (3). This suggests that excess of MAI drives the favorable reaction direction to form pure CH3NH3PbI3 perovskite. On the other hand, only reaction (4) occurs in the case of PbI2. Thus, the remaining PbI2 exists in the film when MAI is not enough, and the H2O-incorporated diffraction peak at 11.4° is observed when excess MAI is present in the film. The stronger preferred orientation along the (110) plane in the case of PbCl2 may be associated with the presence of MACl through the reaction (3), because the introduction of a CH3NH3+ rich environment is critical to slow down the film formation process.43 This finding is also consistent with Zhao et al.'s report,50 in which the incorporation of MACl helps the crystallization of the perovskite film in the one-step solution method. Therefore, the perovskite film shows random orientation in the case of PbI2
:
MAI where no MACl is incorporated in the reactions.
The morphological properties for both cases are similar, as revealed in Fig. 5(c). The RMS roughness values are 24.5 and 26.5 nm for the PbCl2 and PbI2 cases, respectively. From the AFM images, we can see that dense and uniform films completely cover the TiO2/FTO substrates. Taking into account the large substrate roughness of TiO2/FTO (∼20 nm), our AFM analysis showed our perovskite films to be extremely uniform on the length scale of micro-meter (Fig. 5(c)) without clear crystallite domain structures, which is drastically different from the solution processed perovskite films.51 This is in agreement with the observations by Liu et al.14 For the two cases of PbCl2:
MAI and PbI2
:
MAI, we did not find clear difference in device performances.
The results described above suggest that the growth of the perovskite film is highly dependent on the substrate temperature. The drastic changes in the crystal structure and surface morphology as a function of substrate temperature are ascribed to the different sticking coefficients of MAI on the substrate. The sticking coefficient is defined as the fraction of the incident molecules from the source that actually adheres to the substrate, which is dependent on the evaporation source material, substrate temperature, surface properties, and evaporation rate.55,56 The low temperature leads to a high sticking coefficient of MAI to the substrate followed by the poor quality of the perovskite film with partial coverage. The substrate temperature of 20 °C helps the growth of the perovskite film with high crystallinity and complete coverage. At higher temperatures (>80 °C), it is difficult to form pure perovskite films with suitable stoichiometry because of a small sticking coefficient of MAI on the substrate, generating films with excess PbI2 and intermediate phase.
It is hard to make a working device from the perovskite film grown with the substrate temperature held at −50 °C because of the poor morphological properties. The performance of the devices employing the perovskite films prepared at different substrate temperatures is shown in Fig. 6(c). The device with the perovskite film grown at 20 °C exhibits the best performance, with a Voc of 1.010 V, a Jsc of 12.85 mA cm−2, a FF of 66.60%, and an overall PCE of 8.64% under 1 sun illumination. In the case of 80 °C, the decreased PCE is probably ascribed to the presence of PbI2, because PbI2 has a larger bandgap energy (Eg = 2.3 eV),57 resulting in the increase of series resistance and consequently the decrease in FF. In addition, the appearance of the intermediate phase of the perovskite complex at higher substrate temperature may also be responsible for the poor PCE. When further increasing the substrate temperature to 110 °C, Voc and FF become lower, which are ascribed to the poor phase purity and poor morphology of the perovskite film. Therefore, the optimized substrate temperature is 20 °C. Note that the thickness of the perovskite layer for the devices is ∼110 nm, i.e. only one third of the perovskite layer thickness in efficient solution-processed PSCs.4,11,51 When we increase the thickness of the perovskite layer (∼170 nm), the device shows a Voc of 1.098 V, a Jsc of 19.92 mA cm−2, a FF of 52.44%, and an overall PCE of 11.48%. The corresponding J–V curve can be seen in Fig. S6 ESI.†
First, the post-annealing studies were performed on non-stoichiometric perovskite films (see Fig. S7 of ESI†). The results suggest that post-annealing is beneficial on the perovskite films with excess MAI. When the annealing temperature is lower than 110 °C, the influence is negligible. Gentle annealing at 110–120 °C helps to desorb the undesirable H2O-incorporated complex from the perovskite film. High temperature (>130 °C) will decompose CH3NH3PbI3 to PbI2.
The effect of post-annealing on the stoichiometric perovskite films was studied next. Fig. 7 shows the XRD spectra and AFM images of perovskite films with balanced stoichiometry prepared from PbI2:
MAI before and after post-annealing at 120 °C for 1 h. The XRD features before and after annealing are nearly the same, suggesting that the annealing has a negligible effect on the crystallinity of the film. Also the morphology of the perovskite film does not change drastically after the post-annealing, as revealed in Fig. 7(b). The RMS roughnesses before and after annealing is 33.8 and 29.2 nm, respectively. The post-annealing treatment only results in a slight reduction in surface roughness.
The results above suggest that the effect of post-annealing on the crystal structure and morphology of perovskite films with balanced stoichiometry is negligible. Also the device performance was approximately the same with or without post-annealing. This is drastically different from that of solution-processed samples,33,51 where the perovskite film properties and the device performances are strongly dependent on the post-annealing conditions. The results indicate that the hybrid deposition method allows the fabrication of PSCs at lower-temperatures (e.g. room temperature).
In addition, the presence of several hundred nanometer thickness of the spiro-MeOTAD HTL layer (250–600 nm)29,32,33,62 in a solution-based method leads to parasitic absorption loss, reducing further the overall transparency and ultimately limiting its BIPV application.63 However, the thickness of the spiro-MeOTAD HTL layer can be reduced to as thin as 100 nm in our device fabrication, since the perovskite layer prepared by the hybrid deposition method shows a very flat surface and the 100 nm-thick spiro-MeOTAD HTL layer can completely cover the perovskite layer to avoid the direct contact between the top Au layer and the perovskite layer. The transmittance of the 100 nm-thick spiro-MeOTAD HTL layer is shown in Fig. S9 ESI,† which exhibits extremely high transparency in the visible range. Therefore, the spiro-MeOTAD HTL layer does not induce the loss of transparency in the device. Fig. 8 shows a photograph of the PSC with 8.6% PCE prepared under optimized conditions, and the transmittance spectrum of the device without a top Au electrode. Visibly, the PSC also exhibits semi-transparency. Including the glass substrate, the average transmittance of this semi-transparent PSC is 40% in the range of 400–900 nm.
Our PSC can generate significant power while still having good transparency, allowing for the integration of semi-transparent solar cells into windows of buildings. For example, “if 6% efficient window photovoltaics (PVs) were used to cover a building the size of the Willis Tower in Chicago, the glass alone would generate nearly 5.3 gigawatt-hours of energy per year”, as stated by Service.46 The implementation of semi-transparent electrodes, such as Ag grids, Ag nanowires, ITO, graphene and carbon nanotubes64−69 is expected to achieve fully semi-transparent PSCs. Additionally, the perovskite layer thickness dependence results (as summarized in Table S1 of ESI†) indicate the good reproducibility of our hybrid deposition method for fabricating semi-transparent PSCs with high performance.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c5ta03593g |
This journal is © The Royal Society of Chemistry 2015 |