Qixian Zhang, Huicong Liu, Weiping Li, Haining Chen. Carbon-Based CsPbI3 Perovskite Solar Cells. Materials Lab 2022, 1, 220029. doi: 10.54227/mlab.20220029
Citation: Qixian Zhang, Huicong Liu, Weiping Li, Haining Chen. Carbon-Based CsPbI3 Perovskite Solar Cells. Materials Lab 2022, 1, 220029. doi: 10.54227/mlab.20220029

Perspective

Carbon-Based CsPbI3 Perovskite Solar Cells

Published as part of the Virtual Special Issue “Beihang University at 70”

More Information
  • Corresponding author: chenhaining@buaa.edu.cn
  • The perovskite solar cells (PSCs) based on carbon electrode (C-PSCs) are expected to address the instability issues faced by conventional PSCs. Recently, inorganic perovskites have been widely used as the light absorber in C-PSCs, which tended to further enhance device stability. Among various inorganic perovskites, CsPbI3 perovskite has been showing the greatest promise due to its suitable band gap (~1.7 eV) and high chemical stability. Benefiting from the progresses on phase stability, crystal quality and surface defect passivation, CsPbI3 C-PSCs have achieved the efficiency of over 15% and exhibited considerable enhancement in device stability. In this perspective, the main advances on CsPbI3 C-PSCs will be highlighted and the future research directions will be proposed.


  • Organic-inorganic hybrid perovskite solar cells (PSCs) have attracted great attention because high power conversion efficiencies (PCE, 25.7%) could be easily achieved by low-cost solution-based processes[1]. The great achievement in PCE is attributed to the advantages of the perovskite absorber: high absorption coefficient, high mobility, long balanced carrier diffusion length and low exciton binding energy[2]. However, the poor stability has seriously limited their practical application.

    For conventional PSCs (e.g., FTO/TiO2/perovskite/organic hole transport material (HTM)/metal electrode, Fig. 1a), the high-performance organic HTM is commonly doped with ions (e.g., Li+), which is humidity-sensitive and is easy to degrade, while the metal electrode tends to be ionized during operation, which would migrate through HTM to react with perovskite layer for inducing device degradation[3-4]. To address these issues, the PSCs based on carbon electrodes (C-PSCs, Fig. 1b) were developed, in which carbon electrode simultaneously replaced organic HTM and metal electrode. Since carbon materials are stable, hydrophobic and inert to ion migration, device stability was well enhanced[5].

    Fig. 1  The device structure of (a) conventional PSCs and (b) PSCs based on carbon electrodes (C-PSCs). (c) Energy band diagrams of CsPbI3-xBrx C-PSCs[10]. Copyright 2021, Elsevier Ltd. (d) Evolution of the reported PCEs of CsPbI3 C-PSCs[13,15,18-23].

    Though C-PSCs exhibited considerably higher stability than conventional PSCs, the organic ions (e.g., CH3NH3+) in the organic-inorganic hybrid perovskites (e.g., CH3NH3PbI3) would be lost under harsh condition (e.g., high temperature and high humidity), which still limits the device stability. To solve this problem, inorganic perovskites (e.g., CsPbBr3, CsPbI3-xBrx and CsPbI3) have been employed in C-PSCs[6]. The inorganic ions (e.g., Cs+) in the inorganic perovskite well enhanced the material and device stability, especially thermal stability.

    In 2016, inorganic CsPbBr3 was for the first time used as the light absorber in C-PSCs. The PCEs of 5%[7] and 6.7%[8] were achieved, which were comparable to the PCEs achieved by the CsPbBr3 PSCs with the conventional architecture. Most importantly, the CsPbBr3 C-PSCs exhibited considerably enhanced thermal stability compared with organic-inorganic hybrid C-PSCs. Soon after, great progresses have been made on CsPbBr3 C-PSCs with the PCE raising up to over 11.08%[9]. Although CsPbBr3 C-PSCs show superior stability and decent PCE was reported, the large Eg (~2.30 eV) of CsPbBr3 means that it could only absorb the visible light below 540 nm and the theoretical PCE is only about 16%[10].

    For achieving higher PCE, it is necessary to find new inorganic perovskite materials with narrower Eg (Fig. 1c). Fortunately, gradually substituting Br with I in CsPbBr3 would reduce the Eg. CsPbIBr2 and CsPbI2Br are the two representative mixed-halide perovskites, whose Eg were calculated to be 2.05 and 1.90 eV, respectively[10]. By employing CsPbI3-xBrx as light absorbers in C-PSCs, the light absorption range was extended and the short-circuit current density (Jsc) was improved. As a result, the champion PCE of 12.05%[11] and 15.24%[12] were achieved by CsPbIBr2 and CsPbI2Br C-PSCs, respectively.

    Compared with mixed-halide CsPbI3-xBrx perovskites, the full-I CsPbI3 perovskite owns the narrowest Eg (~1.7 eV)[13]. However, due to the small size of Cs cations (1.69 Å), the tolerance factor (t) of CsPbI3 perovskite is only 0.81, which is too low to support a stable perovskite structure at low temperature[14]. Consequently, CsPbI3 perovskite phases (α, β and γ) would spontaneously transit to yellow non-perovskite phase (δ, Eg=2.82 eV) at ambient temperature[15-17]. Therefore, it is a great challenge to grow CsPbI3 perovskite for PSCs and only very low performance was obtained for the initial CsPbI3 C-PSCs[18].

    To address the above issues, two effective strategies have been developed in our group. First, excess CsI was introduced into the PbI2/CsI precursor solution, which would lead to the generation of Cs4PbI6 intermediate phase. After immersing the Cs4PbI6 in isopropyl alcohol (IPA), partial CsI would dissolve and the Cs4PbI6 could be converted to stable CsPbI3 perovskite phase[19]. On the other hand, HPbI3 (or DMAPbI3, DMA+= (CH3)2NH2+) was used to replace PbI2 as the precursor to induce the formation of DMAPbI3 and Cs4PbI6 intermediates. After removing DMAI, Cs4PbI6 was converted to stable CsPbI3 perovskite. By applying such CsPbI3 perovskite in C-PSCs, a promising PCE of 9.5% [20] was obtained with high stability.

    Though the phase stability of CsPbI3 has been well improved, the crystal quality was still low, limiting the device performance. To improve crystal quality, elemental doping has been exploited[21]. For B site doping, Sb3+ ions were incorporated into CsPbI3 solution[19]. After deposition, Sb partially replaced the Pb in CsPbI3 lattice. As indicated, crystal quality was improved accompanied with the enhancement in phase stability. In addition to B site doping, A site doping was also implemented and alkali metal ions (Li+, Na+, K+ and Rb+) have been used to partially replace the Cs+ ions in CsPbI3. Interestingly, all these ions well improved the crystal quality of CsPbI3 perovskite and hence elevated the PCE of CsPbI3 C-PSCs to about 11%[22].

    For better passivating the interface and surface defects of CsPbI3 perovskite, a systematic and in-depth study on the growth processes of CsPbI3 crystals was conducted and the solution components were regulated to obtain stable CsPbI3 perovskite and realize the passivation of excess PbI2 on crystal defects[15]. By further treating the CsPbI3 films with medium polarity solvent (e.g., ethanol, IPA), the harmful DMAPbI3 residual could be well converted to PbI2 passivator, which not only eliminated the negative effects of DMAPbI3 but also enhanced the defect passivating effects. As a result, CsPbI3 C-PSCs achieved a PCE of 15.35%[23], a record PCE for inorganic C-PSCs. In addition to PbI2, CsX (X: F, Cl, Br) ethanol solutions were also used to treat the CsPbI3 perovskite. The larger size mismatch between X and I ions would induce the more obvious cation segregation. The moderate size mismatch between I and Cl ions allows a partial substitution of I ions with Cl ions in CsPbI3, and induces the generation of 2D Cs2PbI2Cl2 nanosheets on the surface, which considerably reduced defect density and suppressed carrier recombination. As a result, the CsPbI3 C-PSCs achieved an PCE of 15.23%[13].

    As stated above, much progress has been made on CsPbI3 C-PSCs in recent years (Fig. 1d) and about 15% PCE has been achieved, but the PCE still largely lags behind those achieved by the conventional CsPbI3 PSCs (over 20%)[24-25]. To further improve the PCE of CsPbI3 C-PSCs, higher quality CsPbI3 film should be prepared with enhanced phase stability and reduced defect density. Besides, hole selectivity at the CsPbI3/carbon should be improved to enhance hole transfer, and energy level alignment at the interface needs to be paid more attention.

    This work is financially supported by the National Natural Science Foundation of China (21875013), the Beijing Natural Science Foundation (No. 2182031).

    The authors declare no conflict of interest.

    Qixian Zhang: Investigation, Data Acquisition, Writing-Original Draft; Huicong Liu: Resources, Project Administration; Weiping Li: Conceptualization, Funding Acquisition; Haining Chen: Conceptualization, Methodology, Writing-Review & Editing.

  • Qixian Zhang is a doctoral student of the School of Materials Science and Engineering, Beihang university. He is pursuing a Ph.D. degree under the supervision of Prof. Haining Chen. His current research interest focuses on carbon-based perovskite solar cells.
    Haining Chen is currently an associate professor at the School of Materials Science and Engineering, Beihang University. He obtained his Ph.D. degree from Beihang University in 2013 following which he worked as a postdoctoral fellow at The Hong Kong University of Science and Technology (Prof. Shihe Yang's group). His recent research interests include perovskite solar cells and water splitting.
  • 1. M. Kim, J. Jeong, H. Lu, K. Lee Tae, T. Eickemeyer Felix, Y. Liu, W. Choi In, J. Choi Seung, Y. Jo, H.-B. Kim, S.-I. Mo, Y.-K. Kim, H. Lee, G. An Na, S. Cho, R. Tress Wolfgang, M. Zakeeruddin Shaik, A. Hagfeldt, Y. Kim Jin, M. Grätzel and S. Kim Dong, Science, 2022, 375, 302
    2. X. Luo, Z. Shen, Y. Shen, Z. Su, X. Gao, Y. Wang, Q. Han and L. Han, Adv. Mater., 2022, 34, 2202100
    3. J. Y. Seo, S. Akin, M. Zalibera, M. A. R. Preciado, H. S. Kim, S. M. Zakeeruddin, J. V. Milić and M. Grätzel, Advanced Functional Materials, 2021, 31, 2102124
    4. C. Ding, R. Huang, C. Ahläng, J. Lin, L. Zhang, D. Zhang, Q. Luo, F. Li, R. Österbacka and C.-Q. Ma, Journal of Materials Chemistry A, 2021, 9, 7575
    5. H. Chen and S. Yang, Adv. Mater., 2017, 29, 1603994
    6. H. Chen, S. Xiang, W. Li, H. Liu, L. Zhu and S. Yang, Solar RRL, 2018, 2, 1700188
    7. X. Chang, W. Li, L. Zhu, H. Liu, H. Geng, S. Xiang, J. Liu and H. Chen, ACS Applied Materials & Interfaces, 2016, 8, 33649
    8. J. Liang, C. Wang, Y. Wang, Z. Xu, Z. Lu, Y. Ma, H. Zhu, Y. Hu, C. Xiao, X. Yi, G. Zhu, H. Lv, L. Ma, T. Chen, Z. Tie, Z. Jin and J. Liu, Journal of the American Chemical Society, 2016, 138, 15829
    9. Q. Zhou, J. Duan, J. Du, Q. Guo, Q. Zhang, X. Yang, Y. Duan and Q. Tang, Adv. Sci., 2021, 8, 2101418
    10. C. Dong, B. Xu, D. Liu, E. G. Moloney, F. Tan, G. Yue, R. Liu, D. Zhang, W. Zhang and M. I. Saidaminov, Materials Today, 2021, 50, 239
    11. Q. Guo, J. Duan, J. Zhang, Q. Zhang, Y. Duan, X. Yang, B. He, Y. Zhao and Q. Tang, Adv. Mater., 2022, 34, 2202301
    12. W. Zhu, J. Ma, W. Chai, T. Han, D. Chen, X. Xie, G. Liu, P. Dong, H. Xi, D. Chen, J. Zhang, C. Zhang and Y. Hao, Solar RRL, 2022, 6, 2200020
    13. H. Wang, H. Liu, Z. Dong, T. Song, W. Li, L. Zhu, Y. Bai and H. Chen, Nano Energy, 2021, 89, 106411
    14. X. Fu, W. Li, X. Zeng, C. Yan, X. Peng, Y. Gao, Q. Wang, J. Cao, S. Yang and W. Yang, J. Phys. Chem. Lett., 2022, 13, 2217
    15. H. Wang, H. Liu, Z. Dong, W. Li, L. Zhu and H. Chen, Nano Energy, 2021, 84, 105881
    16. W. Meng, Y. Hou, A. Karl, E. Gu, X. Tang, A. Osvet, K. Zhang, Y. Zhao, X. Du, J. Garcia Cerrillo, N. Li and C. J. Brabec, ACS Energy Letters, 2020, 5, 271
    17. Z. Li, F. Zhou, Q. Wang, L. Ding and Z. Jin, Nano Energy, 2020, 71, 104634
    18. J. Liang, C. Wang, P. Zhao, Z. Lu, Y. Ma, Z. Xu, Y. Wang, H. Zhu, Y. Hu, G. Zhu, L. Ma, T. Chen, Z. Tie, J. Liu and Z. Jin, Nanoscale, 2017, 9, 11841
    19. S. Xiang, W. Li, Y. Wei, J. Liu, H. Liu, L. Zhu and H. Chen, Nanoscale, 2018, 10, 9996
    20. S. Xiang, Z. Fu, W. Li, Y. Wei, J. Liu, H. Liu, L. Zhu, R. Zhang and H. Chen, ACS Energy Letters, 2018, 3, 1824
    21. J. Liang, X. Han, J. H. Yang, B. Zhang, Q. Fang, J. Zhang, Q. Ai, M. M. Ogle, T. Terlier, A. A. Marti and J. Lou, Adv. Mater., 2019, 31, 1903448
    22. S. Xiang, W. Li, Y. Wei, J. Liu, H. Liu, L. Zhu, S. Yang and H. Chen, iScience, 2019, 15, 156
    23. H. Wang, H. Liu, Z. Dong, X. Wei, Y. Song, W. Li, L. Zhu, Y. Bai and H. Chen, Nano Energy, 2022, 94, 106925
    24. S. Tan, B. Yu, Y. Cui, F. Meng, C. Huang, Y. Li, Z. Chen, H. Wu, J. Shi, Y. Luo, D. Li and Q. Meng, Angew. Chem. Int. Ed. Engl., 2022, 61, e202201300
    25. X. Wang, Y. Wang, Y. Chen, X. Liu and Y. Zhao, Adv. Mater., 2021, 33, 2103688
  • This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.

通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Figures(2)

Information

Article Metrics

Article views(2952) PDF downloads(1202) Citation(0)

Other Articles By Authors

Catalog

/

DownLoad:  Full-Size Img  PowerPoint