Solar cells using ABX3-type perovskite semiconductors are attracting attention due to their high photoelectric conversion efficiency. However, since most of them use lead (Pb), there is a need to develop Pb-free perovskite solar cells from the viewpoint of environmental impact. Perovskites using tin (Sn) have shown promise as an alternative material for Pb-based perovskites, but many challenges remain in achieving high performance because Sn2+ is more susceptible to oxidation than Pb2+. We have previously improved the quality of Sn-based perovskite films by scavenging the Sn4+ ions1 and applying different surface passivation methods.2,3 Most of the materials used for surface passivation have ammonium groups that can bind to the A-site of the perovskite lattice, or thiocyanate or carboxyl groups that can bind to the X-site. In this work, we present a novel modification method using halometallylene, a highly reactive chemical species that is expected to replace the metal at the B-site of the perovskite structure. For this purpose, we designed a series of halostannylenes, (Trp)XSn: (Trp = 9-triptycyl group, X = F, Cl, Br, and I). These compounds can be added to the precursor solution or applied to the surface of the perovskite layer.The reaction of 9-triptycyl lithium, which was generated by a lithiation of 9-bromotriptycene with n-BuLi, with SnX2 (X = Cl, Br) gave thermally stable yellow crystals of the product (Figure 1a). The crystals were determined to have a novel five-membered ring structure, {(Trp)XSn}5 (Figure 1b). In a coordinating solvent (dimethyl sulfoxide (DMSO) or pyridine), the compounds transformed into monomeric halostannylene complexes. From cyclic voltammetry (CV) measurements of (Trp)XSn: in DMSO solutions, the shift of the oxidation potential below any tin halide (SnX2, X = F, Cl, Br, and I) confirms that reaction active Sn2+ species, which can reduce Sn4+, were obtained. When (Trp)ClSn: was added to the solution of SnI4 in DMSO-d 6, in the 119Sn NMR spectra, a peak at –2030 ppm corresponding to SnI4 disappeared, and a new peak at –685 ppm was observed corresponding to SnI2. From these results, it’s expected that the compound will function as a reductant for Sn4+ generated in the perovskite precursor solution. In the presentation, we will further discuss the characteristics of (Trp)XSn: and its application to tin perovskite solar cells.1) T. Nakamura, A. Wakamiya et al, Nat. Commun. 2020, 11, 3008. 2) T. Nakamura, A. Wakamiya et al., ACS Appl. Mater. Interfaces 2022, 14, 56290. 3) S. Hu, A. Wakamiya et al., Adv. Mater. 2023, 35, 2208320. Figure 1
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