Abstract
Perovskite‐on‐silicon tandem solar cells have emerged as a leading technology enabling high power conversion efficiencies (PCE) over 30%. Despite current progress, the intrinsic multilayer device design presents vast challenges in complexity, which can be a drawback in future mass production. Multifunctional nanolayer materials that simplify large‐scale production are therefore highly desirable. Herein, a TiOx layer (∼3–5 nm) grown by atomic layer deposition (ALD) enables a series interconnection of a perovskite n‐i‐p top cell with a silicon wafer directly. The TiOx layer serves as an all‐in‐one interconnect, fulfilling the functions of silicon surface passivation, hole extraction from silicon, and recombination junction at the top/bottom cell interface. As a result, a proof‐of‐concept 22.4%‐efficient tandem device is demonstrated. Furthermore, an improved PCE of 26.5% is achieved by capping the TiOx with a thin ALD‐TiNy layer (∼4 nm). This represents a performance as high as the reference tandem device (PCE = 25.5%) that uses amorphous silicon passivating selective contacts and an indium‐tin‐oxide interlayer. Such a TiOx multifunctional nanolayer can reduce the number of deposition tools and eliminate the need of an indium‐based interconnection. It offers a potential for low‐cost, scalable, and sustainable tandem solar cell manufacturing.
Keywords: passivating contact, perovskite/silicon tandem solar cell, recombination junction, titanium nitride, titanium oxide
TiOx nanolayer enables a series interconnection of a perovskite top cell with a silicon wafer directly in perovskite/silicon tandem solar cells. The TiOx serves as an all‐in‐one interconnect, providing surface passivation, hole transport, and recombination junction. A TiNy capping layer boosts performance to a level comparable to that of conventional tandem devices employing amorphous silicon and indium oxide layers.

1. Introduction
Crystalline Si solar cells, which account for over 95% of the global market today,[ 1 ] require innovative breakthroughs to further enhance efficiency while maintaining cost‐effectiveness and sustainable manufacturing processes, enabling multi‐terawatt scale production.[ 2 ] The power conversion efficiency (PCE) of the state‐of‐the‐art Si solar cells (∼27%)[ 3 ] is approaching its theoretical limit of 29.4%,[ 4 ] making it impossible to achieve higher PCEs with Si alone. Recently, a perovskite/Si tandem solar cell architecture has gathered attention to surpass the limitations of Si. Small‐area laboratory devices (∼1 cm2) have been reported with PCEs over 33%,[ 5 , 6 ] which is well above the PCEs of Si and perovskite single‐junction devices.
From an industrial perspective, however, the trend toward increasing the number of layers stacked to attain higher tandem cell efficiency poses critical challenges in scalability and deployment. The most prevalent Si bottom cell used in perovskite/Si tandem devices is the silicon heterojunction (SHJ) architecture,[ 5 , 6 , 7 , 8 , 9 , 10 , 11 , 12 , 13 ] which uses hydrogenated amorphous Si (a‐Si:H) thin layers at the front and rear of the Si wafer. Despite their broad use, the global market share of SHJ technology is still below 10%[ 1 ] due to the higher capital expenditure and material cost (indium and silver) compared to the Si homojunction architecture, including passivated emitter rear cell (PERC)[ 14 , 15 ] and tunnel oxide passivated contact (TOPCon).[ 16 , 17 ] Furthermore, the recombination junction (RJ) (p/n inverse junction), which is key to interconnect the perovskite top cell and Si bottom cell, is mostly formed using indium‐based oxides such as an indium‐tin oxide (ITO) made by physical vapor deposition. This leads to a higher consumption of indium which is a critical and scarce metal.[ 18 ]
We have recently developed a titanium oxide (TiOx or TiO2) nanolayer grown by atomic layer deposition (ALD) that uniquely acts as a hole‐selective passivating contact in Si solar cells.[ 19 , 20 ] We further demonstrated that the carrier selectivity of the TiOx can be tailored by the ALD process[ 21 ] and/or the choice of Ti precursors.[ 22 ] The hole selective function in TiOx is in contrast to the generally understood behavior of TiOx. TiOx is typically considered an electron selective material with respect to various solar cell absorbers including Si,[ 23 , 24 ] III‐V materials such as InP[ 25 ] and perovskite.[ 26 , 27 ] Using our TiOx nanolayer (∼5 nm) as a hole contact at the front or rear of both n‐ and p‐type Si, PCEs of >20% have been demonstrated without using any buffer layer between the Si absorber and TiOx contact layer.[ 19 , 20 ] This unique function of the TiOx is particularly suited for its application to homojunction solar cells because it offers the potential to replace the dielectric insulator layers (such as Al2O3 and Si3N4) with the semiconducting TiOx passivating contact. It also facilitates 1D charge carrier transport from the Si absorber to the contacts, without resulting in unpassivated Si‐metal local interfaces. We now take this material to the next level by demonstrating that this technology can be applied as an interconnection between Si and perovskite solar cells in a tandem architecture.
In this work, we apply our hole‐selective TiOx passivating contact in perovskite/Si tandem solar cells. While ALD‐TiOx has been previously used to form an RJ in perovskite/Si tandem solar cells,[ 28 ] our new TiOx concept reported in this work not only forms an RJ with the charge transport layer of the top cell, but also performs the surface passivation and the hole transport layer of the Si bottom cell. Furthermore, we show that the TiOx layer deposition followed by an ALD‐TiNy capping can boost the tandem cell efficiency to be comparable with the tandem devices that use standard SHJ bottom cells and ITO interlayers. This multifunctionality of our TiOx allows us to reduce the number of deposition processes, simplifying the tandem structure without using indium‐based interconnection materials. Finally, we propose that this TiOx technology enables the potential of integrating industrial homojunction solar cells (like PERC and TOPCon) into a tandem architecture.
2. Results and Discussion
Figure 1a,b shows the schematic diagrams of perovskite/Si tandem devices fabricated in this study. The device in Figure 1a is based on a standard SHJ bottom cell architecture used as a reference, while that shown in Figure 1b features TiOx layer deposited on the front side of n‐Si wafer. For both devices, front‐planar and rear‐textured n‐Si wafers were used, and the rear side was made with an electron contact composed of an i‐n a‐Si:H/ITO/Ag layer stack. These tandem devices have a perovskite top cell made entirely by solution process (spin coating) in an n‐i‐p deposition sequence. The perovskite top cell consists of SnO2 (∼40 nm) as electron transport layer (ETL), perovskite absorber (∼530 nm) with a bandgap of 1.63 eV, and doped 2,2′,7,7′‐Tetrakis[N,N‐di(4‐methoxyphenyl)amino]‐9,9′‐spirobifluorene (Spiro‐MeOTAD) (∼200 nm) as hole transport layer (HTL). An ITO front electrode was formed by sputtering followed by Ag‐grid deposition by either sputtering or thermal evaporation, and an MgF2 antireflection layer was formed by thermal evaporation. The tandem cell shown in Figure 1a has an ITO interlayer to form an RJ at the interface between top and bottom cells. On the other hand, for the device shown in Figure 1b, the hole‐selective TiOx layer (emitter) was deposited directly on an n‐Si wafer by thermal ALD,[ 19 , 22 ] which is interconnected by the ETL of the top cell. Hereafter, we term these devices “reference tandem” and “TiOx tandem”, respectively. A cross‐sectional transmission electron microscopy (TEM) image of the TiOx tandem is shown in Figure 1c, where the thicknesses of the perovskite top‐cell component layers can be identified. A photo of tandem device fabricated on a 25 mm × 25 mm Si substrate is shown in Figure 1d. With a black shadow mask (not shown), the illumination area is designated to 1.0 cm2. The current density‐voltage (J‐V) curves of the reference tandem and the TiOx tandem are presented in Figure 1e. It has been reported that, without an ITO interlayer in the reference tandem, the J‐V results in an S‐shape curve due to a non‐ideal Schottky barrier developed between the top and bottom cells.[ 29 ] This is a well‐known difficulty in contacting the carrier selective contact of the Si bottom cell to the charge transport layer of the perovskite top cell. Nevertheless, the TiOx tandem exhibits a diode J‐V curve without using such an additional interlayer, as shown in Figure 1e (blue lines).
Figure 1.

Tandem device architecture and performance. a,b) Schematic illustrations of solar cells fabricated in this work ((a) reference tandem and (b) TiOx tandem). c) Cross‐sectional high‐annular angle dark‐field scanning transmission electron microscopy (HAADF‐STEM) image of the perovskite top cell (TiOx tandem). d) A photo of the tandem solar cell fabricated on a 25 mm × 25 mm Si substrate. e) J‐V curves of the reference tandem (black lines) and the TiOx tandem (blue lines). The full and dashed lines represent the J‐V curves measured in forward and backward scans, respectively. The J‐V curves of the corresponding Si single‐junction solar cells are also shown (black: rear contact/n‐Si/i‐a‐Si:H/p‐a‐Si:H/ITO/Ag‐grid (SHJ), blue: rear contact/n‐Si/TiOx/ITO/Ag‐grid (TiOx‐Si cell). The detailed information of these single‐junction solar cells is given in Figures S1 and S2, Supporting Information).
Despite such a simple device structure, the TiOx tandem exhibits a PCE of 22.4% (short‐circuit current density (JSC) = 16.8 mA cm−2, open‐circuit voltage (VOC) = 1.704 V, fill factor (FF) = 0.784) (blue dashed line in Figure 1e). The VOC of this device is well above the VOC of the Si (∼0.7 V) and perovskite (∼1.15–1.2 V) single‐junction solar cells. More detailed information about the device structures and properties of these single‐junction solar cells is provided in Figures S1 and S2 (Supporting Information). To the best of our knowledge, this is the first demonstration of a perovskite/Si tandem device whose subcells are interconnected through a non‐Si passivation contact of the bottom cell. The experimental result of the TiOx tandem demonstrates that a 5‐nm‐thick TiOx nanolayer provides all‐in‐one functionality: Si surface passivation, hole extraction from Si, and RJ at the top/bottom cell interface. However, the reference tandem that comprises three layers (i.e., i‐a‐Si:H/p‐a‐Si:H/ITO) for fulfilling each function shows a higher PCE of 23.8% (JSC = 17.3 mA cm−2, VOC = 1.837 V, FF = 0.748) (black dashed line in Figure 1e). The VOC of this device is nearly equivalent to the sum of the VOC of each subcell. The lower VOC of the TiOx tandem can be attributed in part to the lower VOC of the Si bottom cell (Figure 1e). However, the VOC of these single‐junction devices differs only by 20 mV, which cannot fully account for the VOC loss of ∼>150 mV observed in the tandem devices. The mechanism behind this VOC loss and a way of mitigating it will be provided in the following sections. Meanwhile, the slightly lower JSC of the TiOx tandem compared to that of the reference tandem (Figure 1e) is caused by the batch‐to‐batch variation of thicknesses of component layers (mainly the HTL thickness) that results in the different current matching conditions. The difference in JSC of single‐junction devices originates from the lower parasitic absorption loss in the short wavelengths for TiOx compared to a‐Si:H layers (Figures S1, Supporting Information). However, this effect is not reflected in tandem cells because the short wavelength light is completely absorbed by the top cell.
Figure 2a shows the bright‐field transmission electron microscope (BF‐TEM) image taken at the cross‐section of the top/bottom cell interface of the TiOx tandem. The elemental map and its line profiles measured by energy dispersive x‐ray (EDX) analysis are shown in Figure 2b,c, respectively. Both TEM image and EDX map show atomically sharp Si/TiOx and TiOx/SnO2 interfaces. Similar to previous studies,[ 22 , 30 ] a ∼1 nm‐thick SiOz (SiO2) interlayer that contains a slight amount of Ti is spontaneously created at the Si/TiOx interface. The ∼5‐nm‐thick TiOx layer exhibits a predominantly amorphous microstructure since no lattice fringe pattern is identified in the TEM image. This amorphous nature differs strikingly from the ALD‐TiOx layer previously used in the perovskite/Si tandem solar cells.[ 28 ] In addition, this amorphous structure of the TiOx layer contrasts with the nanocrystalline structure observed in the spin‐coated SnO2 layer, where lattice fringe patterns with <10 nm diameter are visible. Interestingly, the EDX line profiles indicate that the elements of the perovskite absorber layer (such as Pb, I, and Br) penetrate into the SnO2 layer. The migration of halide atoms into SnO2 and even underlying ITO layer has been reported in single‐junction devices and it is responsible for the performance degradation.[ 31 ] In Figure 2c, however, there is a sudden drop off in the Pb and halide signal at the interface with TiOx, indicating that Pb and halide species cannot penetrate the TiOx layer probably due to its denser amorphous nature. Thus, we highlight that the TiOx layer provides an additional function of protecting Si bottom cell from chemical reactions arising from the in‐diffusion of lead and highly reactive halide species.
Figure 2.

Top/bottom interface structure. a) Cross‐sectional bright‐field transmission electron microscope (BF‐TEM) image at the top/bottom cell interface of the TiOx tandem, and its b) EDX elemental map and c) line profiles.
We next investigate the electrical contact properties of the TiOx layer with a focus on its role as an RJ in the tandem device. We prepared specific test samples consisting of the same layers as used in the tandem devices and measured the dark J‐V characteristics, as shown in Figure 3a. Note that p‐Si was used instead of n‐Si to study the degree of recombination of majority carriers injected from Si (holes) and SnO2 (electrons) at the RJ. Al was chosen to have a good electrical contact with the SnO2 layer. As shown in Figure 3b, the dark J‐V curves exhibit a rectifying behavior, while the threshold voltage is largely influenced by the presence of the TiOx layer. When the TiOx layer is present between the p‐Si and the SnO2 layer, high current flows even when a very low reverse voltage is applied (J = 20 mA cm−2 at V ∼ 0.05 V). The similar level of contact resistivity was measured for the p‐Si/TiOx interface.[ 22 ] However, the test sample without a TiOx layer requires a higher voltage (V ∼ 0.5 V) to achieve the same current density. In the forward‐biased regime, much lower current flows particularly for the sample without the TiOx layer. To explain these results, device simulations were carried out for the same sample structures using the SCAPS_1D finite element device simulator.[ 32 ] The band diagrams obtained by the simulation with and without the TiOx layer are shown in Figure 3c,d, respectively. Here, we assume a presence of fixed negative charges at the p‐Si/TiOx interface in the order of 1013 cm−2, based on the band bending measurement for the n‐Si/TiOx interface.[ 22 ] The detailed parameters assumed in the simulation are given in Table S1 (Supporting Information). In Figure 3c, hole accumulation occurs at the p‐Si/TiOx interface due to the presence of a high concentration of fixed negative charge. In an actual tandem device, a hole inversion layer is induced in n‐Si near the n‐Si/TiOx interface.[ 22 ] This facilitates the transport of holes in the Si wafer to the SnO2 layer through the trap‐assisted tunneling mechanism, within the bandgap of the TiOx layer, allowing the current flow by the exchange of majority carriers.[ 33 ] The lesser voltage dependence observed in the forward bias regime indicates tunneling of electrons in the valence band of p‐Si to SnO2, which is similar to the J‐V behavior of a metal‐insulator‐semiconductor tunnel diode when the semiconductor is in accumulation mode.[ 34 , 35 ] In contrast, the band diagram without the TiOx layer (Figure 3d) indicates the depletion of holes in the p‐Si near the p‐Si/SnO2 interface due to the work function difference between these two materials. This situation hinders the majority carrier recombination and thus the current flow without applying a large bias voltage equivalent to the conduction band offset at the p‐Si/SnO2 interface (∼0.5 eV), in agreement with the experimental J‐V curves. These simulation results account for the significantly different dark J‐V behaviors depending on the presence of the TiOx layer between the Si and the ETL (SnO2) of the top cell.
Figure 3.

Current flow mechanism at the recombination junction. a) Test structure for contact resistivity measurement and b) the corresponding dark J‐V characteristics with and without a TiOx layer between the Si wafer and the SnO2 layer. Six identical Al pads were fabricated on a substrate and measured with both forward and backward voltage scans. Note that p‐Si was used as substrate instead of n‐Si to characterize the hole injection from Si to TiOx/SnO2 recombination junction. c,d) Band diagrams of the test structures c) with TiOx and d) without TiOx layer obtained by a SCAPS finite element device simulation. E C and E V denote energy levels of conduction band and valence band, respectively. E F is the Fermi level.
Although the TiOx monolayer can provide multiple functions, one major issue in replacing the conventional thin multilayers with the TiOx monolayer is a non‐negligible VOC loss of ∼>150 mV (Figure 1e). We confirmed that this VOC loss is markedly larger than that of the Si single‐junction solar cells (∼20 mV). To address this issue, we have introduced an ALD‐TiNy capping layer on top of the TiOx layer. TiNy was chosen because of its relatively high work function (4.40–4.53 eV),[ 37 ] since the passivation and carrier selectivity of the TiOx layer depend on the work function of the capping material.[ 20 , 21 , 22 , 36 ] In addition, TiNy is known to exhibit relatively high electrical conductivity arising from its ease of partial crystallization (Figure S3, Supporting Information). The TiNy layer was deposited by thermal ALD using tetrakis(dimethylamido)titanium (TDMAT) as the Ti precursor and NH₃ as the reactant gas. Because the particular ALD system used for TiOx deposition did not support NH₃ gas, the TiNy layer was deposited in a separate ALD system. However, in principle, the TiNy layer can also be deposited in the same ALD chamber immediately after the TiOx layer deposition and the following hydrogen plasma treatment.[ 19 ] This enables the integration of a TiOx/TiNy stack using a single deposition tool.
Figure 4a,b shows the schematic diagram of the TiOx tandem with a TiNy capping layer and the corresponding cross‐sectional BF‐TEM image taken at the top/bottom interface, respectively. The TEM image is similar to that in Figure 2a except for the additional TiNy layer between the TiOx and SnO2 layers. Although their phase boundary is not clearly visible, dashed lines are marked for the TiOx (3.6 nm) and TiNy (4.3 nm) layers, separating them from their slightly different image contrast. This image contrast originates from the presence of the crystalline phase in the TiNy layer, which can be identified in the high‐resolution TEM included in Figure S3 (Supporting Information). To investigate the elemental depth profile, we applied an electron energy loss spectroscopy (EELS) measurement instead of EDX due to the difficulty in separating the overlapping x‐ray signals of N and Ti atoms in the EDX measurement. Figure 4c shows the EELS profiles at different depths (∼0.75nm step) in the whole region of the Si/TiOx/TiNy/SnO2 stack. A weak but clear N K‐edge signal is identified in the TiNy layer. In contrast, the much clearer peak due to O K‐edge appears in this layer, indicating that a significant incorporation of O atoms occurs. This is caused by the post‐deposition processes that include annealing in a low vacuum, SnO2 spin‐coating, and the subsequent hotplate annealing in air. Despite the O incorporation, we name this layer TiNy for simplicity, as the material was deposited without any oxygen‐containing precursor during the ALD process.
Figure 4.

ALD‐TiNy capping layer improves tandem solar cell performance. a) Schematic device structure of the TiOx tandem with a TiNy capping layer. b) Cross‐sectional BF‐TEM image taken at the top/bottom cell interface of the TiOx tandem with a TiNy capping layer. c) EELS spectra measured at different positions near the top/bottom cell interface. Signals due to Ti L edge, O K‐edge, N K‐edge are shown. A broad signal appearing at ∼530 eV originates from Sn. Each line was averaged over the three EELS lines. d) Solar cell parameters of TiOx tandem solar cells with different TiNy thicknesses. Two to seven cells fabricated under identical conditions were measured. Each cell was tested twice under both forward and backward scans. e) PL image of the TiOx tandem with different TiNy capping layer thicknesses before top cell deposition (upper) and after finishing the whole deposition processes (lower).
Figure 4d shows the solar cell parameters of the TiOx tandem as a function of the thickness of the TiNy layer (t TiNy). An adverse effect due to the TiNy layer is seen in JSC when t TiNy is greater than 2 nm. We confirmed the presence of broadband light absorption in the 6‐nm‐thick TiNy layer (Figure S4, Supporting Information), accounting for the large JSC drop of 1 mA cm−2. However, when t TiNy ∼ 4 nm, almost no optical absorption is identified similar to the TiOx layer. This implies that the abrupt increase in optical absorption for t TiNy ∼ 6 nm can be associated with the increased nucleation density and the following crystalline growth of TiNy. We further confirmed that t TiNy ∼ 4 nm is a critical thickness below which no Jsc loss is identified in our optimized tandem solar cells (Table S2 and Figure S5, Supporting Information). On the other hand, VOC and FF show a clear increase with increasing t TiNy up to 4 nm. As a result, an overall PCE gain of ≈1% absolute is obtained by applying the ∼4 nm‐thick TiNy capping layer. It should be added that the insertion of the TiNy layer at the TiOx/SnO2 interface does not alter the electrical contact properties, as confirmed by the dark J‐V measurements on the test structure shown in Figure 3a (Figure S6, Supporting Information). Furthermore, it does not alter the Si single‐junction solar cell performance either (Figure S7, Supporting Information).
To gain insight into the role of the TiNy layer in the TiOx tandem, the impact of t TiNy on the Si bottom cell performance was investigated by photoluminescence (PL) imaging. Here, carrier injection into the Si bottom cell took place in the tandem structure by illuminating the Si with an infrared laser (850 nm) through the perovskite top cell. Figure 4e shows the PL images of the TiOx tandem with various t TiNy before the perovskite n‐i‐p top cell deposition and after completing the device fabrication including front ITO/Ag‐grid sputtering. Here, the PL intensity reflects the magnitude of radiative recombination of photogenerated electron‐hole pairs in Si bottom cell, and it decreases when the rate of the non‐radiative recombination via surface defects increases. It is evident from Figure 4e that the finished device without a TiNy layer exhibits the darkest PL image, indicating that the surface recombination rate of photogenerated carriers increases in the Si bottom cell after depositing the top cell component layers. We confirmed that the PL darkening does not occur after SnO2 deposition on the TiOx layer, but after depositing the perovskite layer. SCAPS‐1D simulation indicates that the hole inversion near the n‐Si/TiOx interface is not affected by the presence of the perovskite layer over the SnO2 ETL (Figure S8, Supporting Information). Thus, the band bending lowering in the n‐Si by the perovskite overlayer is unlikely. We further confirmed that the PL darkening does not occur in the reference tandems. Based on these facts, we hypothesize that the migrating ionic species of the perovskite (such as Pb, I, and Br) to the TiOx through the porous SnO2, which is evidenced by the EDX measurements (Figure 2c), causes a chemical reaction with the TiOx layer and/or the electrostatic influence on the charge distribution near the n‐Si/TiOx interface. Thus, the TiNy layer is likely to work as a barrier to prevent such species from contacting the TiOx layer. Further investigation is necessary to elucidate the detailed mechanism.
Along with fine‐tuning the TiOx and TiNy deposition processes, we have optimized the tandem cell fabrication process. Notably, changing the Ag‐grid formation method from DC sputtering to thermal evaporation results in improved performance (particularly VOC and FF) and reproducibility, likely due to the mitigation of sputter‐induced damage. This leads to a performance improvement in both TiOx and reference tandems. The J‐V curves and the external quantum efficiency (EQE) spectra of the best‐performing TiOx tandem with a TiNy capping layer are shown in Figure 5a (blue lines) and Figure 5b, respectively. The PCE of this device under forward scan is 26.5% (JSC = 17.3 mA cm−2, VOC = 1.875 V, FF = 0.817). A sister device fabricated in an earlier batch under the same condition showed a PCE of 24.0% (JSC = 16.8 mA cm−2, VOC = 1.778 V, FF = 0.809) in in‐house measurements, and a PCE of 24.80% (JSC = 17.4 mA cm−2, VOC = 1.784 V, FF = 0.798) with a steady‐state PCE of 24.82% via independently‐confirmed measurements (Figure S9, Supporting Information). In Figure 5a, the TiOx tandem exhibits a higher PCE (26.5%) in comparison with the improved reference tandem (25.5%) due to its higher JSC. The higher JSC of the TiOx tandem comes from the batch‐to‐batch variation in the thickness of the top cell component layers (mainly the HTL thickness). On the other hand, the VOC achieved in the TiOx tandem is 1.875 V which is comparable to that in the reference tandem (1.887 V). This manifests that the TiOx/TiNy bilayer provides comparable Si passivation, hole extraction, and RJ functions to those achieved with the a‐Si:H passivating contact layers and an ITO interlayer.
Figure 5.

The best performing tandem solar cells. a) J‐V curves of a best‐performing TiOx tandem with a TiNy layer between the TiOx and SnO2 layers (blue lines). The J‐V curves of a best‐performing reference tandem (black lines) after the process optimization, which are superior to those in Figure 1e, are also shown for comparison. Solid and dashed lines represent the forward (FW) and backward (BW) scans, respectively. b) EQE spectra of the top and bottom cells of the corresponding TiOx tandem. The summed EQE spectrum is shown in dashed line. Absorption spectrum (1‐ reflectance (R)) measured by spectrometer is included (solid black line).
Previously, it has been reported that the ITO interlayer can be replaced by an n‐type hydrogenated nanocrystalline Si (nc‐Si:H) layer.[ 29 ] Replacing ITO with nc‐Si:H provides a PCE of 24.4% in the same device design but without applying the latest process optimization such as Ag‐grid formation by evaporation (Figure S10, Supporting Information). The nc‐Si:H also offers an indium‐free interconnection although it still requires the use of an SHJ bottom cell architecture.
Although recent tandem cell development focuses more on an inverted p‐i‐n configuration, we discuss our tandem cell results in comparison with the state‐of‐the‐art tandem devices with an n‐i‐p configuration. Among the n‐i‐p tandem solar cells reported so far,[ 38 , 39 , 40 , 41 , 42 ] our device performance is lower by ∼1–3% absolute. This mainly stems from the following reasons: First, our perovskite top cell was made without any interface passivation. The performance of our perovskite single‐junction solar cell using the same recipe as for the top cell is about PCE ∼ 17–18% (Figure S2, Supporting Information). The 27%‐efficient tandem device in the literature has a perovskite top cell with higher performance (PCE > 20% single‐junction efficiency).[ 38 ] Second, the band gap of the perovskite absorber (1.63 eV) is not optimized for tandem solar cells (∼1.7 eV). Third, the performance of our TiOx tandem is limited by the low JSC (∼17 mA cm−2) due to the larger optical reflection (Figure 5b), compared to the JSC (∼20 mA cm−2) of the state‐of‐the‐art tandem cells.[ 38 , 40 , 41 , 42 ] The replacement of thick spiro‐MeOTAD (∼200 nm) with similar derivatives such as evaporated 2,2′,7,7′‐tetra(N,N‐di‐p‐tolyl)amino‐9,9‐spirobifluorene (spiro‐TTB) with much lower thickness (∼25 nm) would improve the JSC and PCE of our devices. In addition, the introduction of a nanoscale texture that allows uniform top cell formation by the solution process should also increase JSC.[ 6 , 43 , 44 ]
The aim of this study is to extend the developed TiOx technology to commercial homojunction bottom cells such as PERC and TOPCon. In both cell architectures, the TiOx proposed here can interconnect the hole‐collecting side of the Si bottom cell (e.g., p‐Si absorber of PERC and boron‐doped Si in TOPCon) with the perovskite top cell deposited in an n‐i‐p sequence. In the case of TOPCon based on n‐Si absorber, TiOx can be used as an emitter without creating a boron doped emitter. This offers the opportunity to combine low‐cost industrial Si solar cells with perovskite solar cells via the TiOx transparent passivating contact, without the need for indium‐oxide‐based interlayers. This has crucial implications for the design of terawatt‐scale sustainable tandem devices.
3. Conclusion
We have demonstrated that an ALD‐TiOx nanolayer enables direct interconnection between an n‐i‐p perovskite top cell and an n‐Si wafer, achieving a PCE of 22.4% despite the significantly simplified tandem device structure. We show that the TiOx layers are multifunctional, fulfilling the requirements in Si surface passivation, hole extraction from Si, and RJ at the top/bottom cell interface. The introduction of a partially‐crystallized ALD‐TiNy capping layer on top of the TiOx layer improves the n‐Si/TiOx interface passivation, achieving a PCE up to 26.5% which is comparable with the performance of the tandem cells that use a conventional SHJ bottom cell with an ITO interlayer (PCE = 25.5%). This result offers the potential for lowering the manufacturing cost of perovskite/Si tandem solar cells as well as the application of industrial Si solar cells (such as PERC and TOPCon) in tandem solar cell designs.
4. Experimental Section
ALD Processes for TiOx and TiNy Layers
TiOx layers were deposited by a custom‐made ALD chamber equipped with an inductively‐coupled plasma source and a load‐lock chamber (Eiko Corporation). TiOx layers were grown by thermal ALD at a substrate heater temperature of 300 °C using titanium tetraisopropoxide (TTIP) and H2O vapor as a Ti precursor and an oxidant, respectively. TTIP source temperature was kept at 60 °C in a constant temperature bath and it was delivered to the chamber by an Ar bubbler system. TTIP dose time was 1.2 s. The H2O dose was controlled by the valve opening time (1.2 s) and the number of H2O pulses (3 times) in an ALD cycle. By repeating ALD cycle for 128 times, ∼5 nm‐thick TiOx layer was deposited. Then, the TiOx layer underwent a hydrogen plasma treatment (HPT) in the same ALD chamber under a pressure of 10 Pa, a H2 flow rate of 100 SCCM, and an rf plasma power of 600 W.
As mentioned in the main text, the TiNy layers were deposited in a different ALD system (FlexAL, Oxford Instruments) from the above‐mentioned ALD system for the TiOx layer deposition due to the lack of access to the NH3 gas. The TiNy layers were grown at a substrate heater temperature of 300 °C using TDMAT and NH3 as a Ti precursor and a reactant gas, respectively. In similar to TTIP, TDMAT source temperature was kept at 60 °C and it was delivered to the chamber by an Ar bubbler system. The dose times for TDMAT and NH3 were 1.2 and 6 s, respectively. By repeating ALD cycle for 50 times, ∼4 nm‐thick TiNy layer was deposited.
Solar Cell Fabrication
Planar monocrystalline Si wafers (phosphorous‐doped n‐type float zone Si, 2–3 Ωcm, (100) orientation, 280 µm thick) were used in this study. The front‐planar and rear‐textured structure was prepared by the following process step. First, a SiNx layer was deposited on the single side of the Si wafer by plasma‐enhanced chemical vapor deposition (PECVD). This SiNx served as a protection layer during the following etching process. Then, Si wafers were subjected to wet‐chemical etching in a KOH‐based solution (Hayashi Pure Chemical, Pure Etch TP101) to form random pyramidal textures on the uncoated side. Finally, the SiNx film was stripped by immersing the wafers in a diluted HF solution.
The wafers were cleaned using H2SO4, H2O2, HCl, and HF.[ 45 ] Then, an intrinsic and phosphorous‐doped (n‐type) a‐Si:H layer stack was deposited as an electron‐selective passivating contact on the textured side of the Si wafers by means of PECVD operated at 13.56 MHz using SiH4, PH3, and H2 as source gases.[ 45 ] After HF‐dip, TiOx layer was deposited by ALD as a hole‐selective passivating contact on the planar side of the Si wafers. After HPT, some of the samples were capped with a TiNy layer. As a reference, a standard SHJ solar cell was prepared by depositing an intrinsic and boron‐doped (p‐type) a‐Si:H layers, instead of the TiOx layer. A 5‐nm‐thick ITO layer was deposited on a p‐a‐Si:H layer as an interlayer through a shadow mask whose aperture area was designed to have a slightly larger area than the front‐side ITO layer. As for the textured rear side, ITO (70 nm) and Ag (500 nm) layers were formed by magnetron sputtering for the entire area of the samples without patterning. Then, these Si bottom cells were thermally annealed at 180 °C in a low vacuum oven (∼10 Pa of air).
Prior to spin‐coting of the SnO2 layer, the front surface of bottom cells was treated using two different methods. For the TiOx tandem, the surface of the TiOx or TiNy layer was exposed to the same HPT in the ALD system as used for treating the TiOx surface. However, the plasma power was 300 W. For the reference tandem, the front surface of the SHJ bottom cells was treated with UV‐ozone (SAMCO, UV‐1). UV ozone was not used for the TiOx tandem to avoid UV‐induced passivation degradation.[ 19 ] For SnO2 spin coating, an SnO2 nanoparticle colloidal solution (Taki Chemical) was diluted with deionized water with a volume ratio of 1:0.5, and then 300 µL of the solution was spin‐coated (2000 rpm for 30 s) followed by hotplate annealing at 100 °C on a hot plate in dry air for 1 h. This results in a ∼40‐nm‐thick SnO2 layer. For perovskite layer, Rb0.05(FA0.83MA0.17)0.95Pb(I0.83Br0.17)3 perovskite[ 29 , 46 ] was prepared by dissolving 1.4 m PbI2, 0.25 m PbBr2, 0.09 m RbI, 0.25 m methylammonium bromide (MABr), and 1.26 m formamidinium iodide (FAI) in a 4:1 (V:V) mixture of dimethylformamide (DMF) and dimethylsulfoxide (DMSO). A 10% molar excess of methylammonium chloride (MACl) was added to the solution. The solution was mixed overnight at room temperature and used the next day. An amount of 60 µL of the solution was pipetted onto the substrate and spin‐coated in a two‐step program: 1300 rpm for 5 s with 200 rpm s−1 ramp and then 5000 rpm for 30 s with 2000 rpm s−1 ramp. Ten seconds before the end of the second step, 300 µL of anhydrous anisole was pipetted onto the rotating substrate. The substrates were then annealed at 110 °C for 15 min. The HTL was prepared by dissolving 72 mg of spiro‐MeOTAD (Nippon Fine Chemical) in 1 mL of chlorobenzene. The spiro‐MeOTAD solution was doped by adding 17.5 µL of Li‐TFSI (520 mg mL−1 in acetonitrile) and 28.5 µL of 4‐tertbutylpyridine to the spiro‐MeOTAD solution. The solution was shaken at room temperature for 3 h prior to use. An amount of 50 µL of the doped spiro‐MeOTAD solution was pipetted onto the substrate and spun at 4000 rpm for 30 s. Devices were then placed in dry air (<1% relative humidity) over night. Next, a ∼100‐nm‐thick ITO (In2O3/SnO2 96.5/3.5 wt.% in target) was sputtered through a shadow mask in an Ar−O2 (O2: 0.5%) gas mixture using a long‐throw magnetron rf‐sputtering system (CANON‐ANELVA, E‐400S). Here, no buffer layer was used between HTL and ITO layer. To mitigate the sputter‐induced damage, a long target‐substate distance of 250 mm was used. The Ag finger and busbar were formed either in the same sputtering system or in a different thermal evaporation system. The Ag was capped with an ITO (20 nm) thin layer to protect underlying Ag from corrosion during storage. The resulting device area was ∼1 cm2. The tandem devices were coated with a ∼100 nm‐thick MgF2 AR layer using a vacuum evaporator (Moorfield, MiniLab 090). Finally, the devices were then placed in a N2 ‐purged oven at 50 °C for 1 h.
Characterization
The effective minority carrier lifetime and the implied VOC (iVOC) of the Si solar cell precursors (before metallization) were measured with a transient photoconductance measurement setup (Sinton Instruments, WCT‐120). For the finished tandem cells, the J‐V characteristics were evaluated at 25 °C using a dual‐light source class AAA sun simulator (Wacom, WXS‐50S‐L2 or Sanei‐Denki, XHS‐80S1) with an air mass 1.5 global (AM1.5 g) irradiance spectrum at 100 mW cm−2. For perovskite single‐junction solar cells, a Xe lamp sun simulator (AM1.5 g, 100 mW cm−2) was used (Bunkou‐Keiki, OtentoSun). The light intensity of sun simulator was calibrated using calibrated reference Si solar cells (the one used for perovskite single‐junction cell has an IR cut filter). The illumination area of 1.0 cm2 was designated by using a black shadow mask whose aperture area was designed to be slightly smaller than the area of the front ITO electrode. The J‐V parameters of solar cells were recorded using a source meter (Keithley 2400 or 2401) in the voltage range from −0.1 to 1.9 V without any voltage soaking or light soaking. The scan rate used was 0.125 V s−1. All devices were tested in air at room temperature (25 °C). The EQE spectrum was measured in alternating current (AC) mode using a monochromatic light (Bunkou‐Keiki, CEP‐25BXS). The step size was 10 nm. When measuring perovskite top cells, light bias (λ>750 nm) was applied via a blue‐cut filter to saturate the bottom‐cell current; when measuring Si bottom cells, the tandem devices were light‐biased via a red‐cut filter (λ<450 nm) to saturate the top‐cell current. In addition to the light bias, a forward bias voltage (Vbias), which is equivalent to the VOC of the saturated (untested) subcell, was applied (for top cell: Vbias = 0.7 V, for bottom cell: Vbias = 1.2 V). When measuring bottom cell EQE, a small signal arising from the perovskite top cell (EQE<0.05) appears for wavelength of 400–800 nm, particularly for the TiOx tandems. Such an artifact was corrected after the measurements.
Dark J‐V test structures were fabricated on planar 280‐µm‐thick 3 Ωcm p‐type FZ Si wafers. To form an ohmic contact at the rear side of the wafer, a 25‐nm‐thick p‐a‐Si:H layer (same doping type with the wafer) and a sputtered Ag (600 nm) were deposited. The TiOx and SnO2 layers stack under investigation was deposited on the front side of the Si wafer, and then capped with six pads of evaporated Al layers (500 nm) with an area of 0.25 cm2. Two‐terminal J‐V measurements were performed using a Keithley 6430 source meter.
The PL measurement was carried out in an ITES PVX1000 + POPLI‐Λ system. The samples were homogeneously illuminated by an excitation laser with a wavelength of 850 nm through a beam expander and a PL signal was recorded in a Si‐CCD camera with a cut‐on wavelength of 990 nm.
TEM, EDX, and EELS measurements were carried out at JFE Techno‐Research Corporation, Japan. Cross‐sections of the samples were observed by HAADF‐STEM or bright‐field TEM imaging combined with EDX spectroscopy at an acceleration voltage of 80 kV (JEOL JEM‐ARM200F). To avoid the electron‐beam induced degradation of the samples, the EDX scanning was carried out under the minimum irradiation condition.
Conflict of Interest
The authors declare no conflict of interest.
Author Contributions
T.M. supervised the project, designed the experiments, performed the ALD processes, thin‐film coatings, and measurements at AIST, and analyzed the experimental data. C.M. and M.A. performed perovskite single‐junction solar cell development and characterizations. H.S. constructed the baseline processes and characterizations for crystalline Si solar cells at AIST. J.M. and R.S.B. carried out device simulations. T.M. wrote the manuscript. The manuscript was corrected by R.S.B., C.M., A.M., and H.S. All authors discussed the results and provided comments on the manuscript.
Supporting information
Supporting Information
Supplemental Table
Acknowledgements
The authors are grateful to T. Oku, Y. Sato, Y. Muto, and M. Tanabe for the technical assistance in wafer preparation, cell fabrication, and characterization. The authors particularly acknowledge to M. Yamazaki for assisting with part of the ALD processes which were conducted at the AIST Nano‐Processing Facility, supported by “Nanotechnology Platform Program” of the Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan. This work was supported by the New Energy and Industrial Technology Development Organization (NEDO), Japan, project code JPNP20005. R.S.B was supported by the Royal Academy of Engineering under the Research Fellowship scheme (RF/201819/18/38), the UK Engineering and Physical Sciences Research Council grant number EP/V038605/1 and EP/X037169/1, and the John Fell Fund at University of Oxford.
Matsui T., McDonald C., Mirzehmet A., McQueen J., Bonilla R. S., Sai H., Monolithic Perovskite/Silicon Tandem Solar Cells Enabled by Multifunctional TiOx Interconnects. Small 2025, 21, 2500969. 10.1002/smll.202500969
Data Availability Statement
The data that support the findings of this study are available from the corresponding author upon reasonable request.
References
- 1. International Technology Roadmap for Photovoltaic (ITRPV), 15th ed., 2024.
- 2. Haegel N. M., Verlinden P., Victoria M., Altermatt P., Atwater H., Barnes T., Breyer C., Case C., De Wolf S., Deline C., Dharmrin M., Dimmler B., Gloeckler M., Goldschmidt J. C., Hallam B., Haussener S., Holder B., Jaeger U., Jaeger‐Waldau A., Kaizuka I., Kikusato H., Kroposki B., Kurtz S., Matsubara K., Nowak S., Ogimoto K., Peter C., Peters I. M., Philipps S., Powalla M., et al., Science 2023, 380, 39. [DOI] [PubMed] [Google Scholar]
- 3. Lin H., Yang M., Ru X., Wang G., Yin S., Peng F., Hong C., Qu M., Lu J., Fang L., Han C., Procel P., Isabella O., Gao P., Li Z., Xu X., Nat. Energy 2023, 8, 789. [Google Scholar]
- 4. Richter A., Hermle M., Glunz S. W., IEEE J. Photovoltaics 2013, 3, 1184. [Google Scholar]
- 5. Ugur E., Said A. A., Dally P., Zhang S., Petoukhoff C. E., Rosas‐Villalva D., Zhumagali S., Yildirim B. K., Razzaq A., Sarwade S., Yazmaciyan A., Baran D., Laquai F., Deger C., Yavuz I., Allen T. G., Aydin E., De Wolf S., Science 2024, 385, 533. [DOI] [PubMed] [Google Scholar]
- 6. Liu J., He Y., Ding L., Zhang H., Li Q., Jia L., Yu J., Lau T. W., Li M., Qin Y., Gu X., Zhang F., Li Q., Yang Y., Zhao S., Wu X., Liu J., Liu T., Gao Y., Wang Y., Dong X., Chen H., Li P., Zhou T., Yang M., Ru X., Peng F., Yin S., Qu M., Zhao D., et al., Nature 2024, 635, 596. [DOI] [PubMed] [Google Scholar]
- 7. Albrecht S., Saliba M., Correa Baena J. P., Lang F., Kegelmann L., Mews M., Steier L., Abate A., Rappich J., Korte L., Schlatmann R., Nazeeruddin M. K., Hagfeldt A., Grätzel M., Rech B., Energy Environ. Sci. 2015, 8, 81. [Google Scholar]
- 8. Bush K. A., Palmstrom A. F., Yu Z. J., Boccard M., Cheacharoen R., Mailoa J. P., McMeekin D. P., Hoye R. L. Z., Bailie C. D., Leijtens T., Peters I. M., Minichetti M. C., Rolston N., Prasanna R., Sofia S., Harwood D., Ma W., Moghadam F., Snaith H. J., Buonassisi T., Holman Z. C., Bent S. F., McGehee M. D., Nat. Energy 2017, 2, 17009. [Google Scholar]
- 9. Sahli F., Kamino B. A., Werner J., Bräuninger M., Paviet‐Salomon B., Barraud L., Monnard R., Seif J. P., Tomasi A., Jeangros Q., Hessler‐Wyser A., De Wolf S., Despeisse M., Nicolay S., Niesen B., Ballif C., Adv. Energy Mater. 2018, 8, 1701609. [Google Scholar]
- 10. Al‐Ashouri A., Köhnen E., Li B., Magomedov A., Hempel H., Caprioglio P., Márquez J. A., Vilches A. B. M., Kasparavicius E., Smith J. A., Phung N., Menzel D., Grischek M., Kegelmann L., Skroblin D., Gollwitzer C., Malinauskas T., Jošt M., Matič G., Rech B., Schlatmann R., Topič M., Korte L., Abate A., Stannowski B., Neher D., Stolterfoht M., Unold T., Getautis V., Albrecht S., Science 2020, 370, 1300. [DOI] [PubMed] [Google Scholar]
- 11. Chin X. Y., Turkay D., Steele J. A., Tabean S., Eswara S., Mensi M., Fiala P., Wolff C. M., Paracchino A., Artuk K., Jacobs D., Guesnay Q., Sahli F., Andreatta G., Boccard M., Jeangros Q., Ballif C., Science 2023, 381, 59. [DOI] [PubMed] [Google Scholar]
- 12. Wang G., Zheng J., Duan W., Yang J., Mahmud M. A., Lian Q., Tang S., Liao C., Bing J., Yi J., Leung T. L., Cui X., Chen H., Jiang F., Huang Y., Lambertz A., Jankovec M., Topič M., Bremner S., Zhang Y.‐Z., Cheng C., Ding K., Ho‐Baillie A. W. Y., Joule 2023, 7, 2583. [Google Scholar]
- 13. Wright M., Vicari Stefani B., Jones T. W., Hallam B., Soeriyadi A., Wang L., Altermatt P., Snaith H. J., Wilson G. J., Bonilla R. S., Energy Environ. Sci. 2023, 16, 1721. [Google Scholar]
- 14. Green M. A., Blakers A. W., Zhao J., Milne A. M., Wang A., Dai X., IEEE Trans. Electron Dev. 1990, 37, 331. [Google Scholar]
- 15. Dullweber T., Schmidt J., IEEE J. Photovolt. 2016, 6, 1366. [Google Scholar]
- 16. Feldmann F., Bivour M., Reichel C., Hermle M., Glunz S. W., Sol. Energy Mater. Sol. Cells 2014, 120, 270. [Google Scholar]
- 17. Richter A., Müller R., Benick J., Feldmann F., Steinhauser B., Reichel C., Fell A., Bivour M., Hermle M., Glunz S. W., Nat. Energy 2021, 6, 429. [Google Scholar]
- 18. Wang L., Zhang Y., Kim M., Wright M., Underwood R., Bonilla R. S., Hallam B., Prog. Photovolt. Res. Appl. 2023, 31, 1442. [Google Scholar]
- 19. Matsui T., Bivour M., Hermle M., Sai H., ACS Appl. Mater. Interfaces 2020, 12, 49777. [DOI] [PubMed] [Google Scholar]
- 20. Matsui T., McNab S., Bonilla R. S., Sai H., ACS Appl. Energy Mater. 2022, 5, 12782. [Google Scholar]
- 21. Matsui T., Bivour M., Ndione P. F., Bonilla R. S., Hermle M., Sol. Energy Mater. Sol. Cells 2020, 209, 110461. [Google Scholar]
- 22. Matsui T., Fukaya S., McNab S., McQueen J., Gotoh K., Sai H., Usami N., Bonilla R. S., Adv. Sci. 2025, 12, 2410179. [DOI] [PMC free article] [PubMed] [Google Scholar]
- 23. Yang X., Bi Q., Ali H., Davis K., Schoenfeld W. V., Weber K., Adv. Mater. 2016, 28, 5891. [DOI] [PubMed] [Google Scholar]
- 24. Bullock J., Wan Y., Hettick M., Xu Z., Phang S. P., Yan D., Wang H., Ji W., Samundsett C., Hameiri Z., Macdonald D., Cuevas A., Javey A., Adv. Energy Mater. 2019, 9, 1803367. [Google Scholar]
- 25. Yin X., Battaglia C., Lin Y., Chen K., Hettick M., Zheng M., Chen C.‐Y., Kiriya D., Javey A., ACS Photonics 2014, 1, 1245. [DOI] [PMC free article] [PubMed] [Google Scholar]
- 26. Burschka N. P., Moon S.‐J., Humphry‐Baker R., Gao P., Nazeeruddin M. K., Gratzel M., Nature 2013, 499, 316. [DOI] [PubMed] [Google Scholar]
- 27. Lee M., Teuscher J., Miyasaka T., Murakami T. N., Snaith H. J., Science 2013, 338, 643. [DOI] [PubMed] [Google Scholar]
- 28. Shen H., Omelchenko S. T., Jacobs D. A., Yalamanchili S., Wan Y., Yan D., Phang P., Duong T., Wu Y., Yin Y., Samundsett C., Peng J., Wu N., White T. P., Andersson G. G., Lewis N. S., Catchpole K. R., Sci. Adv. 2018, 4, aau9711. [DOI] [PMC free article] [PubMed] [Google Scholar]
- 29. McDonald C., Sai H., Svrcek V., Kogo A., Miyadera T., Murakami T. N., Chikamatsu M., Yoshida Y., Matsui T., ACS Appl. Mater. Interfaces 2022, 14, 33505. [DOI] [PubMed] [Google Scholar]
- 30. Dwivedi N., Yeo R. J., Tan H. R., Stangl R., Aberle A. G., Bhatia C. S., Aaron D., Liao B., Adv. Funct. Mater. 2018, 28, 1707018. [Google Scholar]
- 31. Gao F., Luo C., Wang X., Zhan C., Li Y., Li Y., Meng Q., Yang M., Su K., Yuan D., Zhu R., Zhao Q., Adv. Funct. Mater. 2023, 33, 2211900. [Google Scholar]
- 32. SCAPS, Ghent University , scaps.elis.ugent.be.
- 33. De Bastiani M., Subbiah A. S., Aydin E., Isikgor F. H., Allen T. G., De Wolf S., Mater. Horiz. 2020, 7, 2791. [Google Scholar]
- 34. Green M. A., King F. D., Shewchun J., Solid‐State Electron. 1974, 17, 551. [Google Scholar]
- 35. Shewchun J., Green M. A., King F. D., Solid‐State Electron. 1974, 17, 563. [Google Scholar]
- 36. Allen T. G., Bullock J., Jeangros Q., Samundsett C., Wan Y., Cui J., Hessler‐Wyser A., De Wolf S., Javey A., Cuevas A., Adv. Energy Mater. 2017, 7, 1602606. [Google Scholar]
- 37. Zhuang Y., Liu Y., Xia H., Li Y., Li X., Li T., AIP Adv. 2022, 12, 125222. [Google Scholar]
- 38. Aydin E., Liu J., Ugur E., Azmi R., Harrison G. T., Hou Y., Chen B., Zhumagali S., De Bastiani M., Wang M., Raja W., Allen T. G., Rehman A. U., Subbiah A. S., Babics M., Babayigit A., Isikgor F. H., Wang K., Van Kerschaver E., Tsetseris L., Sargent E. H., Laquai F., De Wolf S., Energy Environ. Sci. 2021, 14, 4377. [Google Scholar]
- 39. Wang L., Song Q., Pei F., Chen Y., Dou J., Wang H., Shi C., Zhang X., Fan R., Zhou W., Qiu Z., Kang J., Wang X., Lambertz A., Sun M., Niu X., Ma Y., Zhu C., Zhou H., Hong J., Bai Y., Duan W., Ding K., Chen Q., Adv. Mater. 2022, 34, 2201315. [DOI] [PubMed] [Google Scholar]
- 40. Gao C., Zhang H., Ma S., Su H., Huang H., He L., Zhang D., Du D., Liu H., Shen W., Nano Energy 2024, 129, 110066. [Google Scholar]
- 41. Duan L., Phang S. P., Yan D., Stuckelberger J., Walter D., Hou Y., Wang W., Chang N., Bui A. D., Mayon A. O., Chang L., Kang D., Duong T., Basnet R., Nguyen H., White T., Bullock J., Weber K., MacDonald D., Catchpole K., Shen H., J. Mater. Chem. A. 2024, 12, 20006. [Google Scholar]
- 42. Zhang M., Ying Z., Li X., Li S., Chen L., Guo X., Liu L., Sun Y., Wu J., Zeng Y., Xiao C., Wu J., Yang X., Ye J., Adv. Mater. 2025, 37, 2416530. [DOI] [PubMed] [Google Scholar]
- 43. Harter A., Mariotti S., Korte L., Schlatmann R., Albrecht S., Stannowski B., Prog. Photovolt. Res. Appl. 2023, 31, 813. [Google Scholar]
- 44. Li Y., Sai H., McDonald C., Xu Z., Kurokawa Y., Usami N., Matsui T., Adv. Mater. Interfaces 2023, 10, 2300504. [Google Scholar]
- 45. Sai H., Oku T., Sato Y., Tanabe M., Matsui T., Matsubara K., Prog. Photovolt. Res. Appl. 2019, 27, 1061. [Google Scholar]
- 46. Saliba M., Matsui T., Domanski K., Seo J. Y., Ummadisingu A., Zakeeruddin S. M., Correa‐Baena J. P., Tress W. R., Abate A., Hagfeldt A., Grätzel M., Science 2016, 354, 206. [DOI] [PubMed] [Google Scholar]
Associated Data
This section collects any data citations, data availability statements, or supplementary materials included in this article.
Supplementary Materials
Supporting Information
Supplemental Table
Data Availability Statement
The data that support the findings of this study are available from the corresponding author upon reasonable request.
