NANOSYSTEMS:
PHYSICS, CHEMISTRY, MATHEMATICS Original article
Shukla R.K., et al. Nanosystems: Phys. Chem. Math., 2024,15 (1), 135-146.
http://nanojournal.ifmo.ru DOI 10.17586/2220-8054-2024-15-1-135-146
Simulation and evaluation of perovskite solar cells utilizing various electron transport layers
R.K. Shukla, Anchal Srivastava, Shikha Rani, Nidhi Singh, Vishnu Kumar Dwivedi, Sharda Pandey, Navina Wadhwani
Physics Department, Lucknow University, Lucknow-226007, India Corresponding author: Navina Wadhwani, [email protected]
Abstract Solar cells that contain perovskite have been a significant object for consideration within the field of solar energy, consistently enhancing their efficiency year by year. In our study, we devised a novel architectural configuration for a tin-based perovskite solar cell, incorporating FTO/ZnO/CH3NH3Snl3/Spiro-OMeTAD/Au. Our investigation into the working of this solar cell involved the utilization of the SCAPS-1D, a versatile tool tailored for the analysis of solar cell behavior. Through this simulation software, we explored different electron-transporting layer (ETL) materials and made adjustments to multiple parameters, including ETL and absorber layer thickness. The outcomes of our research produced promising results, showcasing significant enhancements in different solar cell parameters. These favorable findings underscore the growing allure and potential of perovskite solar cells within the realm of renewable energy. The reported CH3NH3SnI3-based PSCs provide a viable path to the implementation of environmentally benign, low-cost, and high-efficiency PSCs. Keywords solar cells, perovskite, electron transporting material, SCAPS, ZnO
Acknowledgements The authors extend their sincere appreciation to Professor Marc Burgelman of Gent University for graciously supplying the software in this research work.
For citation Shukla R.K., Srivastava A., RaniS., Singh N., DwivediV.K., Pandey S., WadhwaniN. Simulation and evaluation of perovskite solar cells utilizing various electron transport layers. Nanosystems: Phys. Chem. Math., 2024, 15 (1), 135-146.
1. Introduction
The evolution of solar cell technology has passed through distinct phases. The first generation was characterized by the utilization of crystalline and amorphous inorganic materials, exemplified by silicon (Si) and gallium arsenide (GaAs) solar cells. In the second generation, thin-film nanocrystalline solar cells like copper indium gallium selenide and cadmium telluride were introduced. The transition to the third generation marked the emergence of diverse solar cell technologies, encompassing organic, hybrid, nanostructures/quantum dots, and electrochemical (semiconductor/liquid junction) solar cells, including perovskite, plastic, and dye-sensitized solar cells [1-7].
Solar Cells based on perovskite represent a promising alternative to conventional solar cell technologies. Their appeal lies in the cost-effectiveness of their materials and their ability to produce a high number of solar cells using minimal resources, owing to the thin profile of the absorber layer. Significantly, these solar cells are eco-friendly and devoid of lead, positioning them as potential successors to silicon solar cells in the future. This research is dedicated to the investigation of lead-free and environmentally conscious solar cell technologies, employing the SCAPS-1D software for simulations.
Over the years, perovskite solar cells (PSC) have made substantial advancements, with their photoelectric power conversion efficiency (PCE) experiencing significant growth, progressing from 3.80 % in 2003 [8] to an impressive 25.70 % in 2022 [9]. This remarkable progress positions them as frontrunners for the 4th generation of solar cell technologies.
PSCs offer a multitude of advantages when compared with conventional silicon-based solar cells:
i) PSCs demonstrated remarkable PCEs that exceed 25.00 %, bringing them near the power conversion efficiency levels of commercial Si-solar cells [10].
ii) The production of PSCs can be achieved using cost-effective solution-based methods such as spin-coating or printing techniques. This potential reduction in manufacturing costs stands in contrast to the complex and expensive processes required for silicon solar cells [11].
iii) Perovskite materials provide the unique ability to tune their bandgap by adjusting their composition, enabling the absorption of a wider spectrum of solar radiation. This tunability makes PSCs suitable for both single-junction and tandem solar cell configurations [12].
iv) PSCs manufactured on different types of substrates, like flexible and lightweight materials, simplifying their integration into diverse applications such as building-integrated photovoltaics, wearable electronics, and portable devices [13].
© Shukla R.K., Srivastava A., Rani S., Singh N., Dwivedi V.K., Pandey S., Wadhwani N., 2024
PSCs hold significant potential for achieving efficient and profitable solar energy conversion. With ongoing research and development efforts, these cells have the potential to revolutionize the field of photovoltaics and contribute to the widespread adoption of renewable energy sources [14-21].
Several simulation models, including SCAPS, AMPS, GPVDM, and others, are available for simulating solar cells. These models analyze the properties of different layers within solar cells and their respective roles in optimizing overall solar cell performance. SCAPS, is a numerical simulation program operating in one dimension, incorporating seven layers. It was established by a team of researchers specializing in solar cells at the University of Gent. Comprehensive information about the program employed can be found in the literature [22-25].
Choosing to simulate and evaluate perovskite solar cells utilizing various electron transport layers is a strategic decision with several merits. Firstly, perovskite solar cells have emerged as promising candidates for efficient and cost-effective solar energy conversion. By simulating their performance, we gain valuable insights into optimizing their efficiency and stability. The focus on different electron transport layers is particularly relevant because the choice of this layer significantly influences the overall performance of the solar cell. Through simulation, we can systematically assess the impact of various electron transport materials on key parameters like charge transport, recombination rates, and overall device efficiency. Simulating these scenarios provides a cost-effective and time-efficient way to explore a wide range of possibilities, aiding in the identification of optimal electron transport layers for enhanced device performance. This research is crucial for advancing the understanding of perovskite solar cells and contributes to the ongoing efforts to make solar energy more accessible and sustainable. Ultimately, the chosen simulation approach allows for a comprehensive evaluation that can guide experimental efforts toward more efficient and stable perovskite solar cell designs.
2. The elaborate structure of perovskite solar cells
Perovskite is a mineral comprising Calcium, Titanium, and Oxygen with the chemical formula CaTiO3. In a more comprehensive context, the term 'perovskite structure' refers to any compound that possesses the ABX3 composition and shares crystallographic characteristics resembling those of the Perovskite mineral. In this context, 'A' signifies an organic cation, 'B' denotes a larger inorganic cation, and 'X3' indicates a somewhat smaller halogen anion.
The conventional perovskite solar cell adopts an n-i-p type configuration, where 'n' represents the electron-conductive layer, 'i' signifies the absorber layer, and 'p' serves as the hole-conductive layer. For our study, we opted for CH3NH3SnI3 as the absorber layer, and we conducted a systematic evaluation of Electron Transport Layer (ETL) by choosing materials from a range of options, including zinc oxide (ZnO), La-doped BaSnO3 (LBSO), Tin(IV) oxide (SnO2), Ceric oxide (CeO2), Phenyl-C61-butyric acid methyl ester (PCBM), Tungsten trioxide (WO3), Indium Gallium Zinc Oxide (IGZO), Cadmium sulfide (CdS), Copper monoxide (CuO), and Buckminsterfullerene (C60). The hole-conductive layer (HTL) utilized in our design is 2,2',7,7'-Tetrakis(N,N-di-p-methoxyphenylamine)9,9'-spirobifluorene (Spiro-OMeTAD). Fig. 1 provides an illustration of the perovskite solar cell architecture under investigation, and Table 1 offers essential material parameters necessary for conducting the simulation.
Au
Spiro-OMeTAD
CH3NH3S11I3
ETL
(ZnO, LBSO, Sn02, CeOi, PCBM, WOs, IGZO: _CdS, CuO and C6Q)_
FIG. 1. The architecture of the studied PSC
Table 1. Parameters of the materials used in simulation
Parameters FTO ZnO CH3NH3Snl3 Spiro-OMeTAD
t (nm) 250 50 500 50
Eg (eV) 3.2 3.3 1.30 3.2
П (eV) 4.4 3.9 4.2 2.10
er (relative) 9.0 9.0 10 3.0
Nc (cm-3) 2.2-1018 11019 11018 2.5-1018
Nv (cm-3) 1.81019 1019 11018 1.851019
Vnt (cm/s) 1107 1107 1107 1107
Vpt (cm/s) 1107 1107 1107 1107
Pn (cm2/Vs) 20 50 1.6 2-104
Pp (cm2/Vs) 10 0.5 1.6 2-104
Nd (cm-3) 11021 5-1017 — 0
Na (cm-3) 0 0 3.21-1015 11020
Nt (cm-3) 11015 11015 4.5-1016 11014
Reference [26] [27] [28] [29]
3. Results and discussion
SCAPS-1D is specifically designed for the analysis of solar cells, developed by the University of Gent, Belgium. When configuring the input data for the Electron Transport Material (ETM), Table 2 provides a comprehensive listing of all the requisite ETM parameters essential for executing the simulation.
3.1. Effect of the electron transporting layer
In this section, we carried out an evaluation of various ETMs for solar cells, including ZnO, LBSO, SnO2, CeO2, PCBM, WO3, IGZO, CdS, CuO, and C60. Fig. 2 presents a performance comparison, clearly indicating that ZnO outperforms the other materials, exhibiting the highest power conversion efficiency. As a result, ZnO was identified as the optimal electron-transport material. The photovoltaic (PV) parameters for the ZnO layer are as follows: VOC = 0.81 V, Jsc = 29.80 mAcm-2, Fill Factor = 67.29 %, and PCE = 16.26 % at a thickness of 50 nm for the electron transport layer. This choice underscores the effectiveness of ZnO in significantly enhancing the overall performance.
3.2. Impact of electron transport layer thickness on solar cell performance
The primary objective of this simulation is to determine the optimal thickness that results in the most favorable attributes for the PSC. Fig. 3 depicts the simulated parameters of the PSC as the thickness of the perovskite material varies. Specifically, we varied the thickness of the electron transporting layer (ETL) within a range of 10 to 300 nm. The results indicate that the open-circuit voltage (VOC) remains relatively consistent, regardless of the ETL thickness. The value of JSC initially increases up to 30 nm, followed by a subsequent decrease. The FF initially rises as the ETL thickness increases up to 40 nm, after which the value of FF stabilizes. Additionally, the PCE improves as the ETL thickness increases up to 40 nm but starts to decline beyond this point. Based on these findings, we selected an electron transporting layer thickness of 40 nm for further simulations, as it represents a favorable balance of performance characteristics. At this thickness, the solar cell exhibits the solar cell parameters: VOC = 0.81 V, JSC = 29.81 mA cm-2, FF = 67.29 %, and PCE = 16.27 %.
3.3. Influence of electron transport layer donor density (ND) variation
In this simulation, we opted for various ND values to investigate their influence on PSCs functioning. Fig. 4 visually represents the changes in solar cell parameters in relation to the logarithm of ND. All parameter values exhibit fluctuations in response to defect density changes. The VOC initially remains constant, then rises, and finally decreases as the electron transport layer donor density increases from 1 to 1 1022 cm-3. Similarly, the JSC remains constant up to ND equal to
R.K. Shukla, Anchal Srivastava, Shikha Rani, Nidhi Singh, et al. Table 2. Physical parameters of different ETL materials
Material LBSO TiO2 ZnO FTO SnO2 CeO2 PCBM WO3
t (nm) 50 50 50 50 50 50 50 50
Eg (eV) 3.12 3.2 3.3 3.2 3.5 3.5 2 2.6
n (eV) 4.4 4 4 4 4 4.6 3.9 3.8
£r 22 9 9 9 9 9 3.9 4.8
Nc (cm-3) 1.81020 11019 3.7-1018 2.2-1018 4.36-1018 1 1020 2.5 -1021 2.2 -1021
Nv (cm-3) 1.8 -1020 11019 1.81019 1.81019 2.52-1019 2 -1021 2.6 -1021 2.2 -1021
Vnt (cm-s-1) 1107 1107 1107 1107 1107 1107 1 107 1 107
Vpt (cm-s-1) 1107 1107 1107 1107 1107 1 107 1 107 1 107
Mn (cm2V-1s-1) 0.69 0.02 100 20 20 100 0.2 30
Mp (cm2V-1s-1) 0.69 2 25 10 10 25 0.2 30
Nd (cm-3) 2-1021 11012 11018 11019 11018 1 -1021 2.93 -1017 6.35 -1017
Na (cm-3) — — — — — — — —
Nt (cm-3) 11015 11015 11015 11015 1 1015 1 -1015 1 -1015 1 -1015
Reference [30] [31] [27] [26] [31] [36] [31] [32]
Material IGZO CdS CuO C60
t (nm) 50 50 50 50
Eg (eV) 3.05 2.4 1.5 1.7
n (eV) 4.161018 4.18 4.07 3.9
£r 10 10 18.1 4.2
Nc (cm-3) 5-1018 5-1018 2.2-1019 8 1019
Nv (cm-3) 5-1018 5-1018 5.5-1020 8 1019
Vnt (cm-s-1) 1107 1107 1107 1 107
Vpt (cm-s-1) 1107 1107 1107 1 107
Mn (cm2V-1s-1) 15 100 100 8 10-2
Mp (cm2V-1s-1) 0.1 25 0.1 3.5 -10-3
Nd (cm-3) 11018 11015 11015 1 -1017
Na (cm-3) — — — —
Nt (cm-3) 11015 11015 11015 1 1015
Reference [33] [34] [34] [35]
Fig. 2. Performance of PV parameters of different ETL materials
Fig. 3. Effects of ZnO thickness on PSC performance
Fig. 4. Illustrates the influence of ZnO donor density (ND) on PSC functioning
-| o _O 1 O _o
1-10 cm- , then increases as ND increases to 1-10 cm- , followed by a decrease. The fill factor remains constant
1 A _O 1 Q _O
up to Nd value of 10 cm- , then increases as ND increases to 1-10 cm- and finally becomes stable. The power conversion efficiency remains constant at 15.74 % as ND rises to 1-1014 cm-3, then power conversion efficiency rises to 16.27 % as Nd rises to 1-1019 cm-3 but decreases subsequently. Consequently, we identify the optimal value of ND as 4-1017 cm-3 for further calculations.
3.4. Impact of absorber layer thickness on cell functioning
In this section, we explored the influence of varying the thickness of the absorber sheet CH3NH3 SnI3, ranging from 50 to 3000 nm, on the performance of the solar cell. The outcomes revealed intriguing trends in the solar cell's performance metrics. As the absorber film's thickness increased, the VOC exhibited a decline until the absorber film thickness reached 500 nm, at which point VOC stabilized at approximately 0.81 V. The JSC initially rose from 9.86 to 30.15 mA-cm-2, reaching its peak for the absorber film thickness of 1200 nm, but as the absorber film thickness increased further the JSC began to decrease. Concurrently, the FF demonstrated a continuous decrease, spanning from 79.62 to 65.87 % with increasing thickness of the absorber layer. The PCE exhibited an increase from 6.72 to 16.27 % for the 50 to 500 nm thickness of the absorber layer, followed by a slight decline to 16.11 % as the absorber layer thickness increased beyond 500 nm, as depicted in Fig. 5. At a thickness of 500 nm, the PV parameters were as follows: VOC = 0.81 V, JSC = 29.81 mA-cm-2, Fill Factor = 67.27 %, and PCE = 16.27 %. These findings led us to select an absorber thickness of 500 nm for further simulations, as it offered an optimal balance of performance characteristics.
3.5. Influence of varying acceptor density (NA) in the absorber layer on cell performance
The presence of defects has a substantial impact on the optimization of device performance. Higher concentrations of defects in the absorber layer result in increased recombination due to the formation of pinholes, faster degradation of the film, and reduced stability, leading to an overall deterioration in device performance. To ascertain the ideal defect concentration in the absorber layer for optimal parameters, simulations were carried out, varying the defect density from 10 to 1-1022 cm-3.
Figure 6 illustrates that in order to achieve higher efficiency, it is essential to reduce defects in the perovskite to 8-1015 cm-3. At this optimal defect concentration, the solar cell exhibited the following parameters: VOC = 0.83 V, JSC = 29.63 mA-cm-2, Fill Factor = 68.48 %, and PCE = 16.91 %. These findings underscore the importance of minimizing defects in the absorber layer to enhance the total performance of the device.
Fig. 5. Influence of CH3NH3SnI3 thickness on PSC performance
Fig. 6. Illustrates the influence of CH3NH3SnI3 acceptor density (NA) on PSC performance
Fig. 7. Variations in solar cell characteristics with changing temperature
3.6. Influence of temperature on cell performance
Much like other semiconductor devices, solar cells are susceptible to temperature fluctuations, especially when deployed outdoors, where temperatures can surpass 300 K. It is crucial to examine how temperature affects the performance of solar cells. Fig. 7 provides insights into the variations in VOC , JSC , Fill Factor, and PCE at different temperatures. With an increase in temperature from 250 to 500 K, there is a notable decline in PCE, plummeting from 19.04 % to 6.76 %. At 300 K, the solar cell demonstrates the following performance parameters: VOC = 0.83 V, JSC = 29.63 mA-cm-2, Fill Factor = 68.48 %, and PCE = 16.91 %. These findings underscore the significance of considering and optimizing solar cell performance across varying temperature conditions.
3.7. Influence of series resistance on cell performance
The presence of series resistance plays a pivotal role in influencing the behavior of solar cells, stemming from the metal contacts on both the solar cell and layer surfaces. To evaluate the solar cell's efficiency, we systematically adjusted the series resistance within a range of 0 to 12 Ohm-cm2. Fig. 8 provides a visual representation of the outcomes, showing that as the series resistance increases, both JSC and Fill Factor decrease, resulting in higher leakage currents and subsequently leading to reduced PCE. Interestingly, the VOC exhibits relative stability across this spectrum of series resistance values.
3.8. Effect of shunt resistance on cell performance
A solar cell with a low shunt resistance experiences elevated power losses since it permits the light-generated current to deviate along an alternative route. As illustrated in Fig. 9, the fill factor (FF) is the parameter most influenced by this situation, yielding higher values for both VOC and PCE, while the JSC remains relatively unaffected.
3.9. Optimized short-circuit photocurrent density and open-circuit photovoltage curve
After establishing and maintaining the optimized values for both the thickness of the ETL and the absorber layer, along with the defect density, we determined the resulting photovoltaic (PV) parameters: VOC = 0.83 V, JSC of 29.63 mA-cm-2, FF = 68.48 %, and PCE = 16.91 %. Fig. 10 visually depicts the optimized current density versus voltage relationship.
Fig. 8. Illustrates the effect of series resistance on PSC performance
Fig. 9. Illustrates the influence of shunt resistance on PSC performance
Fig. 10. Variations in short-circuit photocurrent density and open-circuit photovoltage of the investigated solar cell at T = 300 K
3.10. Quantum efficiency (QE)
The QE of a PSC measures the current produces when exposed to photons of specific wavelengths. Fig. 11 provides an illustration of the QE curve for a perovskite solar cell, encompassing wavelengths ranging from 300 to 900 nm. Remarkably, the QE values consistently exceed 90 % across most of this spectrum. Upon closer examination of the graph, it becomes apparent that QE increases as the wavelength extends from 300 to 390 nm. QE maintains a consistently high level exceeding 90 % up to wavelengths equal to 400 nm. However, beyond this threshold, QE gradually declines, exhibiting reduced values as the wavelength extends further to wavelengths equal to 900 nm.
300 400 500 600 700 800 900
Wavelength (nm)
Fig. 11. Quantum efficiency curve of studied solar cell
4. Conclusion
We conducted SCAPS-1D simulations to investigate the performance of ETM in lead-free PSCs. We systematically tested various ETL materials to identify the one that offers the best solar cell performance. Subsequently, we identified the optimal ETL material. Furthermore, we independently adjusted the thickness of both the ETL and the absorber layer, along with fine-tuning the working temperature and resistances within the solar cell circuit. The outcomes of these simulations revealed significant results, showcasing the following critical performance metrics for the solar cell: VOC of 0.83 V, Jsc of 29.63 mA ■ cm-2, FF of 68.48 %, and PCE of 16.91 %. Upon thorough analysis, we concluded that the most efficient configuration for the solar cell involves a ZnO (ETL) thickness of 40 nm and a CH3NH3SnI3 (absorber layer) thickness of 500 nm. These precise dimensions resulted in the highest efficiency, offering valuable insights for optimizing future designs of lead-free perovskite solar cells.
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Submitted 31 August 2023; revised 21 December 2023; accepted 8 January 2024
Information about the authors:
R. K. Shukla - Physics Department, Lucknow University, Lucknow-226007, India; ORCID 0000-0001-8505-963; [email protected]
Anchal Srivastava - Physics Department, Lucknow University, Lucknow-226007, India; ORCID 0000-0002-2588-5541; [email protected]
Shikha Rani - Physics Department, Lucknow University, Lucknow-226007, India; ORCID 0009-0003-3326-0706; [email protected]
Nidhi Singh - Physics Department, Lucknow University, Lucknow-226007, India; ORCID 0009-0004-6393-2056; [email protected]
Vishnu Kumar Dwivedi - Physics Department, Lucknow University, Lucknow-226007, India; ORCID 0000-0001-66987598; [email protected]
Sharda Pandey - Physics Department, Lucknow University, Lucknow-226007, India; ORCID 0000-0001-9950-1195; [email protected]
Navina Wadhwani - Physics Department, Lucknow University, Lucknow-226007, India; ORCID 0009-0005-0465-0486; [email protected]
Declaration of Competing Interest: The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Conflict of interest: The authors declare no conflict of interest.