Farhan Yousufa,
Ming-Xun Jianga,
Chen-Fu Lina,
Ming-Hsien Li
b,
Chih-Wei Chu
cd,
Tzung-Fang Guoacdf and
Peter Chen
*adef
aDepartment of Photonics, National Cheng Kung University, Tainan 70101, Taiwan. E-mail: petercyc@ncku.edu.tw
bDepartment of Electro-Optical Engineering, National Formosa University, Yunlin 63201, Taiwan
cResearch Center for Applied Sciences (RCAS), Academia Sinica, Taipei 11529, Taiwan
dResearch Center for Critical Issues (RCCI), Academia Sinica, Tainan, 711010, Taiwan
eHierarchical Green-Energy Materials (Hi-GEM) Research Center, National Cheng Kung University, Tainan 70101, Taiwan
fProgram on Key Materials, Academy of Innovative Semiconductor and Sustainable Manufacturing, National Cheng Kung University, Tainan 70101, Taiwan
First published on 24th July 2025
Perovskite solar cells (PSCs) have made significant advancements, achieving a power conversion efficiency of up to 27%. PSCs are easy to manufacture and cost-effective, making them highly attractive for commercial applications. This study focuses on bifacial transparent PSCs, which utilize transparent electrodes instead of metal electrodes, allowing light absorption from both sides and thereby enhancing energy utilization efficiency. The introduction of buffer layers is aimed at protecting the perovskite absorption layer and organic transport layer from damage during the sputtering process of transparent conductive oxides (TCOs). This research evaluates the effectiveness of three buffer layer preparation methods, soft sputtering deposition, spin coating, and atomic layer deposition (ALD), for bifacial PSCs under various illumination conditions. The results indicated that the bifacial devices with ALD-prepared buffer layers exhibit the best performance under specific albedo conditions, with a front-side illuminated efficiency of 16.2% and a rear-side illuminated efficiency of 15.4% under AM 1.5 G illumination (1 sun), resulting in a bifacial factor of 0.95. A MA-free bifacial PSC with a p-i-n architecture of composition FA0.78Cs0.22Pb(I0.85Br0.15)3 delivers a front-side (glass-side) illuminated efficiency of 19.7% and a rear-side (IZO-side) illuminated efficiency of 18.0% under AM 1.5 G illumination (1 sun). The device exhibited excellent bifacial characteristics, achieving a bifacial factor of 0.91, with a frontside short-circuit current density (Jsc) of 22.8 mA cm−2 and a rear-side Jsc of 20.8 mA cm−2. As the albedo light intensity increases, the bifacial device achieves a significant gain in output power, highlighting the potential of bifacial transparent PSCs in environmental light harvesting scenarios. These results highlight the potential of MA-free perovskite bifacial solar cells as high-efficiency and stable energy conversion candidates, paving the way for further optimization in tandem and large-area photovoltaic applications.
Broader contextThe growing demand for sustainable energy solutions has intensified research into high-performance photovoltaic technologies, particularly bifacial solar cells. Enhancing efficiency and stability while maintaining cost-effectiveness remains a major challenge in the commercialization of these devices. In this work, we investigate the impact of buffer layers on the photovoltaic performance of bifacial perovskite solar cells, comparing MA-free perovskite and triple-cation perovskite materials. Our findings reveal that the MA-free perovskite devices achieved a superior power output of 33 mW cm−2 with a bifacial factor of 90%, while the triple-cation perovskite devices demonstrated bifacial performance with a power output of 29 mW cm−2 with a bifacial factor of 95% under 1 sun illumination intensity from each side. By systematically investigating different buffer layer materials and their impact on charge transport, interface recombination, and optical management, our findings offer valuable insights for advancing the next generation of photovoltaic devices. By improving energy harvesting from both sides, our research contributes to the ongoing pursuit of high-efficiency, cost-effective solar solutions that maximize power output in real-world applications. This study aligns with the global aim for clean energy solutions and contributes to the broader effort of making perovskite photovoltaics commercially viable. |
In this article, we investigated the formation of a transparent window layer for bifacial illuminated PSCs by sputtering transparent conductive electrodes on top of the perovskite. To prevent sputtering damage to the perovskite layer, various methods such as soft-landing sputtering, spin coating, and atomic layer deposition (ALD) were employed to prepare buffer layers. Among these, the ALD buffer layer minimized sputtering damage and maintained a PCE of around 16% for bifacial transparent cells with an anti-reflection coating (ARC). Additionally, bifacial illumination simulations were conducted under different scenarios such as sunny (1 sun), cloudy (0.6 sun), and rainy (0.2 sun) conditions to understand the photovoltaic characteristics of bifacial solar cells under various albedo conditions. Under ample sunlight conditions (1 sun), when the albedo is less than 0.4 sun, only bifacial devices with ALD-deposited films as buffer layers and anti-reflection layers achieve higher power output per unit area than opaque devices. Under simulated cloudy conditions (0.6 sun), bifacial devices with ALD buffer layers require an albedo of less than 0.1 sun (with an ARC) and 0.2 sun (without an ARC) to achieve superior power output compared to opaque devices, while the bifacial devices with spin-coated buffer layers need to increase the albedo to 0.3 sun to surpass the power output of opaque devices. Finally, under simulated indoor conditions (0.2 sun), regardless of the buffer layer preparation method, bifacial devices only need an albedo of 0.2 sun to achieve higher power output than opaque devices. In conclusion, it is indicated that the bifacial illuminated PSCs with proper design can harvest more energy in different scenarios.
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Fig. 2 The J–V curves of the bifacial device where the IZO film is directly deposited on the C60 layer without any buffer layer. |
To reduce the bombardment damage on the surface of C60 during the IZO film deposition, we studied the IZO deposition using a 2-step process. In the first stage, a soft deposition approach was employed with the sputtering power reduced to 10 W, which is the minimum power capable of plasma generation and the Vbias ranging from 70 to 75 V with a working pressure of 7 mTorr. Additionally, a trace amount of oxygen (Ar/O2 = 0.33%) was introduced during the IZO film deposition to enhance the optical properties of the IZO film and decrease the kinetic energy of deposited IZO particles in the first-stage soft deposition.20 The second stage utilized the optimized sputtering parameters (sputtering power = 100 W) to obtain high transparency and good electric conductivity of the IZO film. Bifacial devices prepared using this 2-step deposition process, without a buffer layer between the C60 layer and IZO film, demonstrated a significantly improved diode behavior. The J–V curves of bifacial devices with different deposition times in the first step, under AM 1.5 G illumination, are shown in Fig. 3.
It is clear that the soft-landing deposition process transformed the J–V curves of devices from a linear shape (using 1-step IZO deposition, Fig. 2) to an S-shape (2-step IZO deposition, Fig. 3) characteristic under reduced target power and bias voltage. Specifically, the device under front illumination achieves a peak PCE of 8.2% with a 20-minute soft deposition time in the first stage. The longer soft deposition time results in a thicker soft-deposited IZO film and reduces bombardment damage from subsequent high-power IZO film deposition. Deposition beyond 20 minutes (e.g., 30 minutes) resulted in increased series resistance and degraded transparency, limiting overall efficiency. Thus, 10 and 20 minutes were selected to achieve an optimal trade-off (Fig. S1†). The S-shape J–V behavior under high bias voltage suggested that plasma still damages the C60/IZO interface even under such soft sputtering conditions. This damage induces defects within the C60/IZO interface and may introduce energy barriers, such as Schottky barriers, at the interface.21,22
Thickness of SnO2 | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) |
---|---|---|---|---|
5 nm | 0.43 | 22.2 | 31.7 | 3.0 |
10 nm | 0.88 | 20.0 | 46.1 | 8.1 |
15 nm | 0.86 | 19.7 | 45.0 | 7.7 |
The 5 nm SnO2 buffer layer exhibits lower buffering capability compared to the 10 nm and 15 nm SnO2 buffer layers. Consequently, during subsequent high-power deposition of IZO thin films, greater plasma damage occurs at the C60/SnO2 interface. This results in more severe carrier recombination at the interface, leading to an overall Voc of only 0.43 V and a fill factor (FF) of 31.74% in the bifacial device with the 5 nm SnO2 buffer layer. In contrast, thicker SnO2 layers demonstrate better buffering capabilities. Devices with thicker SnO2 layers achieve Voc values exceeding 0.80 V and FF values above 45%. Among these, the 10 nm thickness shows the optimal performance with a PCE of 8.1%. However, it is indicated that the device performance with the SnO2 buffer layer is slightly lower than that with 2-step IZO deposition due to the Vbias of the sputtering SnO2 layer being approximately 20 V higher than that of the 2-step IZO devices, as mentioned in Section 2.1.
To further reduce bombardment damage during sputtering, the working pressure of SnO2 film deposition was increased to 20 mTorr. As the working pressure increases, the shorter mean free path would lead to more collisions between SnO2 particles and facilitate thermalization of the sputtered species to the mean kinetic energy of the surrounding gas atoms through energy transfer. Another effect under high working pressure is that scattering of the sputtered particles broadens their distribution of incident angles at the substrate, which might decrease the penetration depth or impact on the deposited film. Under the high working pressure condition of 20 mTorr, the bifacial devices with 5 nm, 10 nm, and 15 nm SnO2 buffer layers were fabricated and their device performances were measured. Excessively high pressure can accelerate thermal equilibration among deposited particles. Moreover, the deposited particles may reach the substrate without sufficient kinetic energy, shifting the film microstructure from the bombardment enhanced compact zone T to the porous zone structure. This scenario inhibits the device performance due to poor film quality, which impacts carrier transport and optical properties.24 Therefore, maintaining appropriate working pressure is crucial for ensuring film quality and device performance. It can be observed that the efficiency of bifacial devices under front and rear illumination does not improve under high working pressure, as seen in Fig. 5.
Experimentally, we employ 2-propanol (IPA) to dilute a 37 wt% PEIE solution and compare different mass percentages of PEIE solutions. Here, 0 wt% PEIE denotes devices without a PEIE buffer layer, deposited with a 2-step IZO process for the bifacial cells. The PV parameters of the bifacial cells using various weight percents of PEIE are normalized to that of the device without buffer (0 wt% PEIE). The effect of PEIE concentration on the impact of PV characteristics is illustrated in Fig. 6. Table 2 shows the detailed photovoltaic characteristics of bifacial devices under front illumination for different PEIE concentrations.
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Fig. 6 Normalized PV parameters of bifacial devices with different PEIE concentrations under front-side 1 sun illumination. |
PEIE concentration (wt%) | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) |
---|---|---|---|---|
0 | 0.90 | 18.1 | 51.0 | 8.3 |
0.2 | 0.96 | 18.0 | 64.5 | 11.2 |
0.3 | 0.96 | 18.9 | 69.7 | 12.7 |
0.4 | 0.98 | 19.1 | 71.2 | 13.3 |
0.5 | 0.98 | 18.4 | 66.8 | 12.0 |
In bifacial devices with 2-step IZO film deposition, incorporating PEIE as a buffer layer increased Voc from 0.90 V to 0.96–0.98 V. This indicated that PEIE is effective at reducing the bombardment damage at the PEIE/IZO interface. The photovoltaic parameters of Jsc and FF both increase with increasing PEIE concentration. The optimal device performance was obtained at a PEIE concentration of 0.4 wt%, achieving a PCE of 13.3% under front illumination. The PV performance of the bifacial device with 0.4 wt% PEIE under front and rear illumination is shown in Fig. 7. The front-side and rear-side illuminated efficiency could reach 13.3% and 11.7%, giving a bifacial factor (defined by the ratio of rear-side illuminated efficiency to front-side illuminated efficiency) of 0.88 for the bifacial device. Table 3 shows the detailed photovoltaic characteristics of bifacial devices with 0.4 wt% PEIE under front and rear illumination. Compared to the device without a buffer layer, this represents an efficiency improvement of approximately 50%. However, as the concentration exceeded 0.5 wt%, the device performance began to decline due to the increased series resistance, which reduced the FF with such excessively high PEIE buffer layer concentration.
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Fig. 7 (a) J–V curve and (b) EQE spectra of the bifacial device with 0.4 wt% PEIE under 1 sun illumination from glass and IZO sides. |
Illumination side | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) | Bifacial factor |
---|---|---|---|---|---|
Front side (glass) | 0.98 | 19.1 | 71.8 | 13.3 | 0.88 |
Rear side (IZO) | 0.97 | 17.6 | 68.6 | 11.7 |
To reduce the resistance of the IZO film, 1-step high-power sputtering deposition was further used to achieve the required transparent rear electrode. The results indicate that the devices deposited with a 10 nm SnO2 buffer layer, under front illumination, achieved a Voc of 0.96 V, a Jsc of 20.7 mA cm−2, an FF of 71.2%, and a PCE of 14.4%. When the thickness of the ALD-prepared SnO2 buffer layer increased to 20 nm, it also led to increased resistance, thereby reducing the Jsc and FF of the device and lowering the PCE to 13.1%. Hence, in ALD buffer layer preparation, an appropriate thickness is crucial to effectively mitigate damage during sputtering and maintain effective charge transport. Blindly increasing thickness would elevate device resistance and consequently degrade device performance. To optimize ALD-deposited SnO2 buffer layers, we systematically tested devices with 5 nm, 10 nm, 15 nm, and 20 nm thicknesses. As shown in Fig. S2,† the 10 nm thickness yielded the best performance. The 5 nm layer was too thin to effectively protect the underlying layers, while increasing the thickness to 15 or 20 nm introduced higher series resistance and reduced carrier extraction, leading to lower PCE. Series resistance (Rs) values extracted from J–V fitting further confirm the trade-off between protection and charge transport. As shown in Table S1,† Rs decreased from 84.14 Ω (5 nm) to a minimum of 33.35 Ω (10 nm) and then increased to 50.26 Ω (15 nm) and 112.44 Ω (20 nm), supporting that both under- and over-thick SnO2 layers compromise device performance. Under rear illumination, the efficiency was 12.1%, and the bifacial factor of the bifacial device is 0.84. The J–V curves and EQE spectra of the as-fabricated bifacial device under front and rear illumination are shown in Fig. 8. The corresponding PV parameters are provided in Table 4.
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Fig. 8 (a) J–V curve and (b) EQE spectra of the ALD SnO2 10 nm bifacial device under 1 sun illumination from glass and IZO sides. |
Illumination side | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) | Bifacial factor |
---|---|---|---|---|---|
Front side (glass) | 0.96 | 20.7 | 72.0 | 14.4 | 0.84 |
Rear side (IZO) | 0.95 | 17.1 | 73.7 | 12.1 |
To further enhance device performance under rear illumination, 100 nm of MgF2 was deposited on the IZO by evaporation to serve as an ARC layer.32,33 The J–V curves and EQE spectra of the bifacial-illuminated PSCs under front and rear illumination are presented in Fig. 9(a) and (b), respectively. From the EQE spectra in Fig. 9(b), the deposition of the ARC MgF2 layer significantly improves the device performance, especially increasing the Jsc to 20.2 mA cm−2 under rear illumination. The device efficiency under front illumination reached 16.2%, while under rear illumination, the efficiency was 15.4%. The bifacial factor of the bifacial device increased from 0.84–0.88 to 0.95 (Table 5).
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Fig. 9 (a) J–V curves and (b) EQE spectra of ALD SnO2 bifacial device with an ARC illuminated with 1 sun from glass and IZO sides. |
Illumination side | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) | Bifacial factor |
---|---|---|---|---|---|
Front side (glass) | 1.05 | 21.9 | 70.8 | 16.2 | 0.95 |
Rear side (IZO) | 1.04 | 20.2 | 73.6 | 15.4 |
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Fig. 10 PCE of the opaque device and bifacial devices with different buffer layers under 1 sun illumination from glass and IZO sides. |
Devices | Illumination side | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) | Bifacial factor |
---|---|---|---|---|---|---|
Opaque | Glass | 1.06 | 21.8 | 75.4 | 17.4 | — |
IZO | — | — | — | — | ||
ALD SnO2 with an ARC | Glass | 1.05 | 21.9 | 70.8 | 16.2 | 0.95 |
IZO | 1.04 | 20.2 | 73.6 | 15.4 | ||
ALD SnO2 | Glass | 0.99 | 19.9 | 71.4 | 14.0 | 0.88 |
IZO | 0.97 | 17.6 | 71.3 | 12.4 | ||
PEIE | Glass | 0.95 | 20.5 | 62.6 | 12.2 | 0.79 |
IZO | 0.96 | 15.7 | 65.3 | 9.6 | ||
2-step sputtered IZO | Glass | 0.91 | 17.8 | 51.7 | 8.4 | 0.91 |
IZO | 0.95 | 15.0 | 52.9 | 7.6 | ||
Sputtered SnO2 | Glass | 0.88 | 20.0 | 46.1 | 8.2 | 0.93 |
IZO | 0.89 | 17.7 | 48.5 | 7.6 |
In the bifacial illumination measurement analysis, two solar simulators were used with different light intensities to simultaneously illuminate the bifacial device from both sides, as illustrated in Fig. 11. Three different measurement conditions were set:
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Fig. 11 Schematic measurement of bifacial illumination with simulated scenarios of clear sky, overcast sky, and indoor conditions. |
Condition 1: the front side of the bifacial device was illuminated with a light intensity close to that of a clear sky (1 sun). Under this condition, the back-side illumination intensity was gradually increased from 0.2 sun to 1 sun.
Condition 2: the front side of the bifacial device was illuminated with a light intensity close to that of an overcast sky (0.6 sun). Under this condition, the back-side illumination intensity was gradually increased from 0.2 sun to 1 sun.
Condition 3: the front side of the bifacial device was illuminated with a light intensity close to that of an indoor environment or rainy day (0.2 sun). Under this condition, the back-side illumination intensity was gradually increased from 0.2 sun to 1 sun.
As the buffer layer's resistance to bombardment decreases, the threshold of light intensity for the bifacial cell to outperform the opaque device increases. Spin-coated PEIE bifacial devices achieve higher power output than single-sided opaque devices when rear-side light intensity is approximately 0.7 sun. On the other hand, bifacial devices with 2-step IZO and sputtered SnO2 layers suffer from interface damage during sputtering, resulting in significant defects that impair carrier transport, and hence, their power output remains lower than that of opaque devices (Fig. 12(a)). As a result, the power generation of this bifacial cell will not surpass that generated from the opaque device even at 1 sun of back-side illumination. The major gain in power generation is contributed by the enhanced current density due to back-side illumination, as seen in Fig. 12(b–d). The increase in Jsc with increasing light intensity is linear, and the Voc increase is proportional to the logarithm of incoming light intensity. Moreover, the decrease in the FF is attributed to the higher resistivity of IZO compared to metals, which increases the resistive loss as the total current increases in the device upon additional back-side illumination (Fig. 12(d)).34
To further optimize the bifacial cell performances, we applied a p-i-n structure with FTO/SAM/FA0.78Cs0.22Pb(I0.85Br0.15)3/C60/ALD SnO2/IZO/Ag architecture with an MA free perovskite. The change in the SAM from Me-4PACz to 3PATAT-C3 was driven by its good coverage and better overlap for perovskite. We added the performance comparison between Me-4PACz and 3PATAT-C3 in ESI Fig. S3,† where both SAMs almost showed similar performance, but the device coverage was better in the 3PATAT-C3 SAM. Their J–V and IPCE are illustrated in Fig. 15 with their photovoltaic parameters in Table 7. We further conducted bifacial illumination for this MA free device, where their power output, Jsc, Voc and FF are shown in Fig. 16.
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Fig. 15 (a) J–V curve and (b) EQE spectra of the MA free perovskite (FA0.78Cs0.22Pb(I0.85Br0.15)3) bifacial device under 1 sun illumination from glass and IZO sides. |
Illumination side | Scan | Voc (V) | Jsc (mA cm−2) | FF (%) | PCE (%) | Bi-facial factor |
---|---|---|---|---|---|---|
Glass side | Forward | 1.03 | 22.5 | 83.4 | 19.3 | 91.32 |
Reverse | 1.03 | 22.8 | 84.6 | 19.7 | ||
IZO side | Forward | 1.03 | 20.9 | 82.8 | 17.9 | |
Reverse | 1.03 | 20.8 | 84.2 | 18.0 |
The J–V characteristics in Fig. 15(a) show the photovoltaic behavior under front and rear illumination, where the front-side (glass-side) illumination exhibited a higher current density compared to the rear-side (IZO-side) illumination. The IPCE spectra in Fig. 15(b) further reveal the device's spectral response, demonstrating efficient charge collection across the visible range, with a slightly reduced response at short (350–500 nm) wavelengths for rear-side illumination. Fig. 16 presents the power output, Jsc, Voc, and fill factor (FF) as a function of rear-side light intensity. The power output (Fig. 16(a)) increases with light intensity for both illumination conditions, with the front-side illumination showing slightly higher values. The open-circuit voltage (Voc) (Fig. 16(b)) remains relatively stable, with only minor variations, indicating that charge recombination mechanisms are similar for both illumination conditions. The short-circuit current (Jsc) (Fig. 16(c)) follows a linear trend, reflecting the expected photocurrent generation under varying light intensities. However, the FF (Fig. 16(d)) exhibits a slight reduction with the rear-side illumination, suggesting some resistive or interfacial losses when light is incident from the IZO side.
Under standard front-side illumination (glass side), the device exhibited a short-circuit current density (Jsc) of 22.8 mA cm−2 in forward scan, while under rear-side illumination (IZO side), the Jsc was 20.8 mA cm−2. The bi-faciality factor, which quantifies the efficiency of the rear-side response compared to the front, was calculated to be 91.32%, indicating excellent bifacial performance. The observed minimal Jsc increase in MA-free devices under low IZO-side illumination may be due to the absence of the ARC and increased interfacial recombination. The power output and FF showed a slight decrease under rear illumination, suggesting minor optical and recombination losses. Notably, no anti-reflective coating (ARC) was applied to the IZO side, which could have contributed to the lower Jsc for rear illumination. The addition of an ARC could potentially enhance light absorption at the rear interface, further improving the photocurrent and overall bifacial efficiency of the device.
For high-performance MA-free perovskite bifacial solar cell in a p-i-n architecture with the composition FA0.78Cs0.22Pb(I0.85Br0.15)3, the device exhibited excellent bifacial characteristics, achieving a bifacial factor of 91.32%, with a front-side (glass-side) short-circuit current density (Jsc) of 22.8 mA cm−2 and a rear-side (IZO-side) Jsc of 20.8 mA cm−2. The power output, open-circuit voltage, and fill factor remained stable across different light intensities, indicating good operational reliability under bifacial conditions. The efficiency drop in rear-side illumination was attributed to minor optical and interfacial losses, which could potentially be mitigated by incorporating an anti-reflective coating (ARC) on the IZO layer to enhance light absorption and improve photocurrent generation. These results highlight the potential of MA-free perovskite bifacial solar cells for high-efficiency and stable energy conversion, paving the way for further optimization in tandem and large-area photovoltaic applications.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5el00045a |
This journal is © The Royal Society of Chemistry 2025 |