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Anion–π interactions suppress phase impurities in FAPbI3 solar cells

Abstract

Achieving both high efficiency and long-term stability is the key to the commercialization of perovskite solar cells (PSCs)1,2. However, the diversity of perovskite (ABX3) compositions and phases makes it challenging to fabricate high-quality films3,4,5. Perovskite formation relies on the reaction between AX and BX2, whereas most conventional methods for film-growth regulation are based solely on the interaction with the BX2 component. Herein, we demonstrate an alternative approach to modulate reaction kinetics by anion–π interaction between AX and hexafluorobenzene (HFB). Notably, these two approaches are independent but work together to establish ‘dual-site regulation’, which achieves a delicate control over the reaction between AX and BX2 without unwanted intermediates. The resultant formamidinium lead halides (FAPbI3) films exhibit fewer defects, redshifted absorption and high phase purity without detectable nanoscale δ phase. Consequently, we achieved PSCs with power conversion efficiency (PCE) up to 26.07% for a 0.08-cm2 device (25.8% certified) and 24.63% for a 1-cm2 device. The device also kept 94% of its initial PCE after maximum power point (MPP) tracking for 1,258 h under full-spectrum AM 1.5 G sunlight at 50 ± 5 °C. This method expands the range of chemical interactions that occur in perovskite precursors by exploring anion–π interactions and highlights the importance of the AX component as a new and effective working site to improved photovoltaic devices with high quality and phase purity.

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Fig. 1: Schematic illustration and experimental investigation of anion–π interactions.
Fig. 2: Influence of anion–π interactions on film formation.
Fig. 3: Influence of anion–π interactions on final FAPbI3 perovskite films.
Fig. 4: Effect of anion–π interactions on PCE and stability of PSCs.

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All data are available in the main text or the supplementary information.

Code availability

The code used for this study is available from the corresponding authors on reasonable request.

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Acknowledgements

This work was supported by the National Natural Science Foundation of China (grant nos. 52125206, 51972004 and 52202241), the National Key Research and Development Program of China (grant no. 2020YFB1506400) and the Tencent Foundation through the Xplorer Prize. We would like to thank the staff at beamlines BL14B1 and BL11B at the Shanghai Synchrotron Radiation Facility (SSRF) for their help with GIWAXS and EXAFS characterizations, and H. Zhengguan (SSRF) for designing the in situ GIWAXS measurement. We acknowledge Y. Chen (Peking University) for the discussion on DFT calculations, Y. Jiang (Peking University) for the assistance in designing CV measurement and C. Zhu (Beijing Institute of Technology) for the assistance with the material structure analysis. We acknowledge support from T. Yang (Jiangnan University) for the help with the GIWAXS test and L. Xiong and Z. Yan (Jiangnan University) for the help with the QCM-D test.

Author information

Authors and Affiliations

Authors

Contributions

Z.H. and H.Zhou conceived the idea and designed the experiments. Z.H. fabricated and characterized the perovskite films. Z.H. and Y.B. fabricated the solar cell devices. Y.W. ensured device encapsulation and preservation and participates in efficiency certification. Y.B. performed the SIMS mapping test. X.H. and L.W. performed the TEM measurement. J.L. and T.L. performed and helped to analyse the DFT calculations. Y.C. helped with the scheme design. K.L. performed the SEM measurements. X.N. conducted the XPS, EQE and PL mapping measurements. N.L. carried out the FTIR measurements. Y.Z. and H.Zai contributed to the fabrication of high-performance PSCs. H.Zhou, Q.C. and Z.H. wrote and revised the manuscript. All authors were involved in the discussion of data analysis and commented on the manuscript.

Corresponding author

Correspondence to Huanping Zhou.

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Extended data figures and tables

Extended Data Fig. 1 Interaction between FAI and HFB.

a, FTIR spectra of FAI, HFB or mixed FAI and HFB. b, 1H NMR of FAI and FAI with HFB in DMSO-d6. c, CV measurement of iodine ion activity of FAI or FAI with HFB. The electrode oxidation potential \({{\rm{E}}}_{{I}^{-}}\) of FAI (0.2 mg ml−1) in IPA at 293 K is +0.245 V, which dropped to +0.197 V of FAI with the addition of HFB \(({{\rm{E}}}_{{I}^{-}-{\rm{HFB}}})\). The activity of iodide without \(({{\rm{\gamma }}}_{{I}^{-}})\) and with \(({{\rm{\gamma }}}_{{I}^{-}-{\rm{HFB}}})\) HFB could be compared using the Nernst equation \({{\rm{E}}}_{{I}^{-}}-{{\rm{E}}}_{{I}^{-}-{\rm{HFB}}}=RT{\rm{ln}}({{\rm{\gamma }}}_{{I}^{-}}/{{\rm{\gamma }}}_{{I}^{-}-{\rm{HFB}}})/F\). The \({{\rm{\gamma }}}_{{I}^{-}}/{{\rm{\gamma }}}_{{I}^{-}-{\rm{HFB}}}\) ratio is determined to be 2.2, indicating the substantially reduced activity of iodide ions. The decrease in the ion activity ultimately leads to a decrease in the chemical potential of FAI, which retards the reaction between FAI and PbI2.

Extended Data Fig. 2 DFT calculations for the FAIHFBPbI2 three-component system.

DFT-calculated Gibbs energy of three reactions in gas phase (a) and the implicit solvent model (solvent = DMF) (b). According to the implicit solvent model, we observed that the Gibbs energy of reaction 1 (−3.19 kcal mol−1) is still lower than that of reaction 2 (6.00 kcal mol−1) in solvent. Notably, reaction 3 (ΔG = −3.97 kcal mol−1) became more favourable in solvent, which is consistent with the UV–vis absorption spectra of the three-component system (Fig. 1d). This was probably because of the coordination of solvent molecules in the implicit solvent model. But the energy of reaction 3 in solvent is still not enough to cancel out the energy difference between reaction 1 and reaction 2. Therefore, DFT calculations in gas phase as well as in the implicit solvent model (solvent = DMF) yield consistent results, that HFB reacts with FAI to form [FAIHFB] and retards the reaction between FAI and PbI2.

Extended Data Fig. 3 Anion–π interaction between the AX component of perovskite and HFB.

UV–vis absorption spectra for HFB, various salts with different cations and anions FAI (a), MAI (b), CsI (c), MACl (d), MABr (e), MASCN (f) and their mixture. Similar redshift about the absorption edge from 280 nm to more than 320 nm was found after FAI, MAI or CsI solution mixing with HFB, indicating that this polarization appeared regardless of the cation species35. Besides, the absorption edge of HFB at 280 nm shifted to 285 nm and 300 nm after mixing with Br and SCN, respectively. These evidences implied that such polarization also existed between HFB and bromide or even SCN. It should be noted that there is no redshift observed when HFB is mixed with chloride, indicative of no polarization, which is probably because of the small radius of chlorine. However, because anion–π interactions also consisted of the contribution from electrostatic force, the strong electrostatic force between Cl and HFB also leads to anion–π interactions, as reported previously36. These results indicate that the anion–π interaction is widely present between HFB and various types of AX in perovskite.

Extended Data Fig. 4 Effects of other strong electron-deficient molecules.

UV–vis absorption (a) and PL spectra (b) of control perovskite and perovskite fabricated with HFB, 2,4,6-trifluoro-1,3,5-triazine (labelled π-I), s-tetrazine (labelled π-II) and pentafluoropyridine (labelled π-III). PCE (c), FF (d), VOC (e) and JSC (f) of PSCs fabricated with HFB, π-I, π-II and π-III.

Extended Data Table 1 Summarized characteristics of PSCs

Supplementary information

Supplementary Information

This file contains 23 Supplementary Figures and legends for the two Supplementary Videos.

Supplementary Video 1

IPA evaporation rate test. One millilitre of IPA was added dropwise to a watch glass and, after 938 s, IPA volatilized 20% of its initial mass. Video played with 15× acceleration.

Supplementary Video 2

HFB evaporation rate test. One millilitre of HFB was added dropwise to a watch glass (the watch glass specification was the same as that used in Supplementary Video 1) and, after 334 s, the HFB volatilized 20% of its initial mass. This shows that the volatilization rate of HFB is higher than that of IPA under the same conditions. Video played with 15× acceleration.

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Huang, Z., Bai, Y., Huang, X. et al. Anion–π interactions suppress phase impurities in FAPbI3 solar cells. Nature 623, 531–537 (2023). https://doi.org/10.1038/s41586-023-06637-w

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