Regulating the Crystallization Process of IntermediatePhase for Wide-Bandgap Perovskite Reduces Open-Circuit Voltage Deficit

Wide-bandgap (WBG) perovskite solar cells with a bandgap exceeding 1.65 eV effectively complement the spectral response of monocrystalline silicon, making them promising candidates for high-performance perovskite–silicon tandem cells. However, achieving WBG perovskites with a bandgap of 1.65 eV typically requires a Br-rich composition, which often results in severe light-induced I–Br phase segregation. In this work, a Cs-rich composition, FA<sub>0.5</sub>Cs<sub>0.5</sub>Pb(I<sub>0.93</sub>Br<sub>0.07</sub>)<sub>3</sub> perovskite with a bandgap of 1.65 eV, was studied and an arylformamidium additive-assisted approach was adopted to regulate the crystallization process of the intermediate phase. The arylformamidium molecules selectively adsorb onto the Cs<sub>2</sub>PbI<sub>2</sub>Cl<sub>2</sub> intermediate grains, inhibiting the interplay between DMSO and Cs<sub>2</sub>PbI<sub>2</sub>Cl<sub>2</sub>, significantly increasing the grain size of intermediate-phase Cs<sub>2</sub>PbI<sub>2</sub>Cl<sub>2</sub> and improving its crystallinity. The highly uniform Cs<sub>2</sub>PbI<sub>2</sub>Cl<sub>2</sub> intermediate grains enhance the nucleation consistency and growth uniformity of the perovskite, ultimately forming a homogeneous perovskite film with large grain sizes and preferential orientation, while reducing the defect state densities. As a result, the 2-thienformamidium iodide (TFAI)-modified WBG perovskite solar cells achieved a power conversion efficiency (PCE) of 21.94%, alongside an impressive open-circuit voltage of 1.27 V. Moreover, the devices retained over 90% of their initial PCE after >1000 h of maximum power point (MPP) tracking degradation testing, and negligible phase segregation was detected after 450 h of AM 1.5G illumination.

Publication Details

Journal
Figshare
Published
2025-02-19
DOI
https://doi.org/10.1021/acsenergylett.4c03219.s001
Primary Topic
Perovskite Materials and Applications
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article
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article

Regulating the Crystallization Process of IntermediatePhase for Wide-Bandgap Perovskite Reduces Open-Circuit Voltage Deficit

Figshare
Perovskite Materials and Applications
article

Regulating the Crystallization Process of IntermediatePhase for Wide-Bandgap Perovskite Reduces Open-Circuit Voltage Deficit

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Abstract

Wide-bandgap (WBG) perovskite solar cells with a bandgap exceeding 1.65 eV effectively complement the spectral response of monocrystalline silicon, making them promising candidates for high-performance perovskite–silicon tandem cells. However, achieving WBG perovskites with a bandgap of 1.65 eV typically requires a Br-rich composition, which often results in severe light-induced I–Br phase segregation. In this work, a Cs-rich composition, FA<sub>0.5</sub>Cs<sub>0.5</sub>Pb(I<sub>0.93</sub>Br<sub>0.07</sub>)<sub>3</sub> perovskite with a bandgap of 1.65 eV, was studied and an arylformamidium additive-assisted approach was adopted to regulate the crystallization process of the intermediate phase. The arylformamidium molecules selectively adsorb onto the Cs<sub>2</sub>PbI<sub>2</sub>Cl<sub>2</sub> intermediate grains, inhibiting the interplay between DMSO and Cs<sub>2</sub>PbI<sub>2</sub>Cl<sub>2</sub>, significantly increasing the grain size of intermediate-phase Cs<sub>2</sub>PbI<sub>2</sub>Cl<sub>2</sub> and improving its crystallinity. The highly uniform Cs<sub>2</sub>PbI<sub>2</sub>Cl<sub>2</sub> intermediate grains enhance the nucleation consistency and growth uniformity of the perovskite, ultimately forming a homogeneous perovskite film with large grain sizes and preferential orientation, while reducing the defect state densities. As a result, the 2-thienformamidium iodide (TFAI)-modified WBG perovskite solar cells achieved a power conversion efficiency (PCE) of 21.94%, alongside an impressive open-circuit voltage of 1.27 V. Moreover, the devices retained over 90% of their initial PCE after >1000 h of maximum power point (MPP) tracking degradation testing, and negligible phase segregation was detected after 450 h of AM 1.5G illumination.

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