Single-step synthesis of Cs3Bi2I9 nanocrystals for scalable direct X-ray detectors
ACS Energy Letters American Chemical Society 10:12 (2025) 6092-6103
Abstract:
Lead-free perovskite-inspired materials have emerged as promising candidates for direct X-ray detection. However, in the early exploration of emerging materials, the focus was on large single crystals. Herein, we report a facile, scalable, single-step synthesis of high-quality Cs3Bi2I9 nanocrystals (NCs) directly from their precursor powders through an ultrasonication approach. The large-scale synthesis of the NCs allowed for the production of 0.78 cm2 pellets used in the fabrication of X-ray detection devices, which exhibit a high bulk resistivity of 1 × 1011 Ω cm and a low dark current density of 3.3 nA cm–2 under an applied bias of 50 V (357 V cm–1 electric field). These devices achieve a limit detection of 108 nGyair s–1, an order of magnitude improvement over the a-Se used in commercial medical imaging, along with stable current under continuous X-ray exposure with a peak energy of 35 keVp. Finally, we demonstrate the scale-up of these detectors by producing thick films 9 cm2 in area, achieving a performance comparable to that of the detectors based on pellets.Evaluating the potential of CsBiSCl 2 as a solar absorber
EES Solar Royal Society of Chemistry (2025)
Abstract:
Efforts to develop lead-free and stable alternatives to halide perovskites have thus far mostly yielded materials with power conversion efficiencies (PCEs) well below 10% in solar cells. Recently, photovoltaics based on CsBiSCl2 were reported to achieve 10.38% PCE. Still, the crystal structure is unknown, and it is unclear whether the reported thin film synthesis method could realize thin films with the desired phase and stoichiometry. Herein, we use ab initio Random Structure Searching (AiRSS) with a bespoke machine learned interatomic potential to explore the potential energy surface of CsBiSCl2, finding the previously-proposed cubic perovskite structure to be implausible. The lowest-energy structure we find is a four formula unit orthorhombic structure (Pnma space group) that lies 2.4 meV per atom above the convex hull. There is strong competition in the Cs–Bi–S–Cl family, which can lead to phase impurities. By examining the reported solution synthesis method, we find that it is challenging to obtain the dimethylammonium bismuth sulfide intermediate product, and that Bi2S3 with dimethylammonium iodide on the surface likely forms instead. The significant I-containing residues in this intermediate results in Cs3Bi2I9 being preferentially formed in thin films instead of CsBiSCl2. Solid state synthesis without I present leads to phase impurities, consistent with the lowest-energy CsBiSCl2 phase being metastable. Taking these experimental and computational results together, it is unlikely that >10%-efficient CsBiSCl2 solar cells have been achieved.Evaluating the potential of CsBiSCl2 as a solar absorber
University of Oxford (2025)
Abstract:
Raw data for all the figures in the main text and SI for this paperSingle-step synthesis of Cs3Bi2I9 nanocrystals for scalable direct X-ray detectors
University of Oxford (2025)
Abstract:
Raw data for all the figures in the main text and SI for this paperElectrospinning nonspinnable sols to ceramic fibers and springs
ACS Nano American Chemical Society 18:21 (2024) 13538-13550