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= 0.8896) and demonstrated high predictability. SHAP enhanced the interpretability and trustworthiness of the model by providing accurate predictions and interpretable insights into the relevance of molecular descriptors. Various investigations, such as UV-visible spectroscopy, hole-electron transport, frontier molecular orbital (FMO), density of states (DOS) and transition density matrix (TDM) analyses, were conducted on the entitled chromophores. The HOMO/LUMO energy gaps of BNPD1-BNPD5 were found to be within the range of 4.050-2.683 eV, with the absorption maxima observed in the UV region (434.179-393.826 nm). According to the DOS and TDM analyses, good charge transfer occurred from the terminal donors to the central acceptor in all the derivatives. All the investigated chromophores exhibited relatively low exciton binding energies, following a decreasing trend (in eV): BNPD4 (0.648) > BNPD5 (0.621) > BNPR (0.611) > BNPD2 (0.340) > BNPD3 (0.335) > BNPD1 (0.069). A benchmark study using Spiro-OMeTAD (a reference HTM) illustrated close agreement, which also suggested that these materials can act as reasonable HTMs for perovskite solar cells.
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Shafiq et al. (2026) studied this question.
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