The certified efficiency of perovskite solar cells with a size of is now 17.8% (Ref. 1) and comes close to the 20.4% efficiency of polycrystalline Si solar cells. Therefore, perovskite solar cells are expected to be one of the important types of solar cells in the next generation printable solar cells. Perovskite solar cells contain (Perov Pb) as the light harvesting layer.220.127.116.11.7.8.–9 The Perov Pb layer is prepared by spin-coating the mixture of (or ) and (MAI) onto a nanoporous layer (scaffold layer); this process is known as a one-step synthesis.3 The Perov Pb can also be prepared with a two-step synthesis, where the layer is fabricated on a porous titania layer (scaffold layer) and the sample is dipped in the MAI solution in dimethylformamide (DMF). The MAI is diffused in the layer to make the perovskite structures.4 It has been reported that the two-step process has the advantage of a higher efficiency over the one-step process.4 In this report, we focus on the two-step process. When the perovskite layer is exposed to light, the perovskite is excited and electrons are injected into the titania layer or are carried by the perovskite itself.5,6,9 The surface of the porous titania affects the electron collection as well as the crystal growth of the perovskite crystals.1011.–12 For example, we have reported that the electron trap density of the perovskite/titania layer is decreased by passivating the surface of the titania.10,12 In addition, the crystal size of the perovskite becomes larger when the titania surface is passivated with amino acid hydroiodic acid (HI) salt.11 The interface between titania and the perovskite crystal is crucial for understanding the photoconversion; however, the interface has not been discussed in detail. Previously, dye adsorption for dye-sensitized solar cells has been discussed using a quartz crystal microbalance (QCM) measurement.13,14 We now discuss the interface structure of the titania/perovskite layer by monitoring the adsorption on the titania layer employing the QCM measurement.
and were prepared in the same way as has been reported in previous works.1011.–12 Figure 1 shows the QCM system (Meywafosus Co. LTD) employed in this experiment. The titania (anatase) compact layer (500 nm) was prepared on a Au QCM sensor by atomic layer deposition (ALD) (Sunable ALD R200 Basic, Picosun) using and water as the precursor. The chamber temperature was kept at 300°C (1000 cycles, 50 nm thickness), followed by annealing the sample at 450°C for 30 min. The titania compact layers had an anatase structure. The titania/Au sensor was placed at position B in Fig. 1. The solution in the DMF (0.2 to 5 mM) was put into container A, and the solution was passed over the titania/QCM sensor B. The flow rate was and the temperature was kept at 25°C. The amount of adsorbed on the titania compact layer was monitored with a frequency shift according to the following Sauerbrey equation:15
The perovskite solar cell was prepared in the same way as in our previous reports.1011.–12 F-doped layered glass (FTO glass, Nippon Sheet Glass Co. Ltd.) was patterned using Zn and a 6 M HCl aqueous solution. On this patterned FTO glass, titanium diisopropoxide bis(acetylacetonate) solution in ethanol was sprayed at 300°C to prepare the compact titania layers. A porous titania layer was fabricated by spin-coating titania paste (PST-18NR, JGC Catalysts and Chemicals Ltd.) in ethanol ( weight ratio), followed by heating the substrate at 550°C for 30 min. The one-step preparation process for perovskite solar cells is as follows: MAI and were mixed in a molar ratio to prepare a 40% solution of perovskite in N,N-dimethylformamide (DMF) and the mixture was spin-coated on the substrate. The substrate was heated at 100°C for 45 min, followed by spin-coating a mixture of 55 mM of tert-butylpyridine, 9 mM of lithium bis(trifluoromethylsyfonyl)imide salt, and 68 mM of 2,2’,7,7’- tetrakis[N,N-di (4-methoxy phenyl) amino]—9,9’- spirobifluorene (spiro). Finally, Ag and Au electrodes were fabricated with a vacuum deposition method (ALS Tech E-299).
The two-step preparation process for perovskite solar cells is as follows: 1 M solution of in N,N’-dimethylformamide (DMF) was spin-coated, followed by baking at 70°C for 30 min. After that, the sample was dipped in a solution of MAI in 2-propanol for 30 s. After rinsing, the sample was heated at 70°C for 30 min. On the sample, spiro and electrode were prepared in the same way as in the one-step preparation. The photovoltaic performance of the cells was evaluated using an AM 1.5G irradiance solar simulator (CEP-2000, Bunkoukeiki Inc.) and a mask on a cell of size .
The thermally stimulated current (TSC) was measured using a TS-FETT apparatus (Rigaku) in the same way as described in our previous reports.16 At a low temperature (), traps were filled with electrons by exposing the substrate to ultraviolet light. As the temperature of the sample increased, these electrons were released from the trap sites. These electrons are detected as a TSC. The TSC at a higher temperature is the result of electrons released from deeper traps and the TSC at a lower temperature is associated with electrons released from shallow traps. The trap depths and trap densities are calculated using the temperature and the current density at that temperature by Eqs. (2) and (3), respectively.16,17
Results and Discussion
Figure 2 shows the relationship between the adsorption time and the adsorption density on a compact titania layer. The solution was introduced to the sensor surface at point A in Fig. 2. The weight of the compact layer increased with time, demonstrating that was adsorbed on the compact titania layer. At point B in Fig. 2, the surface was rinsed by introducing DMF onto the sensor surface. The adsorption curve showed a sharp drop and remained at a constant value after that. The curve was explained as follows. The amount of adsorbed on the compact titania layer increased with time and the uptake speed gradually decreased. Weakly adsorbed was washed away upon rinsing with DMF and strongly adsorbed remained on the titania surface.
The saturated (maximum) adsorption density increased with an increase in the concentration and reached a constant value as shown in Fig. 3, suggesting that was adsorbed on all the adsorption sites. A, B, and C are explained later (Table 1). Supposing that the diameter of is 0.558 to 0.954 nm, the surface area occupied by one molecule is calculated to be 2.45 to . If all surfaces were covered with , the adsorption density of could be calculated to be 107 to . The experimentally determined saturated adsorption density was to as shown in Fig. 3. The experimentally estimated adsorption density was roughly coincident with the calculated value.
Photovoltaic performances for solar cells consisting of CH3NH3PbI3.
|JSC (mA/cm2)||VOC (V)||Fill factor||PCE (%)|
|0.2 mM + One-step (2)||12.14||0.80||0.56||5.47|
|1 mM + One-step (3)||12.87||0.81||0.59||6.12|
|5 mM + One-step (4)||13.84||0.80||0.60||6.64|
The x-ray photoelectron spectroscopy (XPS) of adsorbed on the titania layer is shown in Fig. 4. In Fig. 4(b), the 616 eV peak is assigned to , and both the 135 and 137 eV peaks are assigned to , as estimated from the data base shown in Fig. 4(a). The ratio of Pb:I of adsorbed on the titania layer was estimated from the comparison of the peak intensity of a thin film prepared on a glass substrate and was determined to be . This suggested that is bonded on the titania surface by a Pb-O-Ti linkage as shown in Fig. 5. It is probable that Ti-OH moieties on a titania layer react with Pb-I to form Ti-O-Pb and HI, namely; the negatively charged O of Ti-O attacks the positively charged Pb nucleophilically to form Ti-O-Pb.
The signals of XPS for a Perov Pb bulk layer and a bulk layer were observed at 135.6 and 135.7 eV, respectively, as shown in Fig. 6. After the bulk layer of the Perov Pb layer and the bulk layer of on the titania layer were washed away, the titania surface was analyzed by XPS. The peak assigned to was observed for the rinsed surface at 136.4 eV, which was slightly shifted to a higher bonding energy than that of bulk (135.7 eV). This is consistent with previous reports that the metals of an oxide metal have higher XPS bonding energies than that of the corresponding halides. The rinsed Perov Pb/titania surface also has the same XPS peak (136.4 eV) as the rinsed layer. This suggests that Ti-O-Pb linkages are also formed at the titania/Perov Pb interfaces as well as at the interfaces. Perov Pb crystals may grow from the Pb-O-Ti surfaces.
In order to examine the surface passivation effects on solar cell performance, the surface of the porous titania was treated with dilute solutions with various concentrations, such as 0.2, 1, and 5 mM. The different concentrations correspond to points A, B, and C in Fig. 3, where 150 to 200, 100 to 125, and of were absorbed on the porous titania surface. After the surface treatment of the titania layer with a dilute solution, the mixed solution of and MAI was spin-coated on the porous titania layer to form a perovskite layer (Perov Pb). The photovoltaic performances for these solar cells are summarized in Table 1, in which the performance for a Perov Pb solar cell without any surface pretreatment is also included. It is observed that the photovoltaic performances, namely, and , increased with an increase in the concentration of passivation from 0.2 to 5 mM as shown in A, B, and C in Fig. 3. These results demonstrate that the photovoltaic performances are improved by controlling the titania–perovskite interfaces (passivation effect).
For our experimental conditions, the two-step preparation method showed higher photovoltaic performances (7.33%) than the one-step preparation method (2.91%) as shown in Table 1. In the two-step preparation method, the layer is directly fabricated on the porous titania layer by using a 1 M solution of (a much higher concentration) before MAI is introduced to the layer. Therefore, the interface between the and the porous titania layer was well passivated by the Ti-O-Pb bond formation.
Two possible mechanisms have been proposed for electron collection. One explanation is that electrons are collected through the nanoporous titania, which is a mechanism similar to that of dye-sensitized solar cells.4 The other explanation is that electrons are directly collected by the Perov Pb layers.5 For a Perov Pb solar cell consisting of porous titania, both processes may occur simultaneously. In Perov solar cells consisting of porous titania layer, electrons would be collected by both of porous titania layer and Perob Pb layer.16 Since these traps become charge recombination centers, the trap density must be low.1818.104.22.168.–23 Figure 7 shows the electron trap distribution for the titania porous layer, the layer, and the rinsed with DMF solution. The trap density of porous titania at was and the trap density decreased to and after the porous titania surface was passivated with . Even after the surface was rinsed with the DMF solution, a low trap density was maintained, demonstrating that the titania surface was passivated with Ti-O-Pb linkages by .
The interface structure between titania and a Perov Pb layer was examined by QCM, XPS, and thermally stimulated currents. It was concluded that the interface was made by Ti-O-Pb, which passivates the surface trap of nanoporous titania. The photovoltaic performances were improved after the passivation.
This work was supported by Funding Program for the World–Leading Innovative R&D on Science and Technology (FIRST program headed by Professor Hiroshi Segawa).
Shuzi Hayase graduated from Osaka University in 1978 and received his PhD from Osaka University in 1983. He was with the R&D Center at Toshiba from 1978 to 2000, during which he engaged in the development of ULSI lithography. He was with the polysilane research group of the Robert West group at the University of Wisconsin from 1988 to 1990. He has been a professor at the Kyushu Institute of Technology (National Institute) since 2001. His research interest is printable solar cells and their materials.