2 research outputs found

    Contorted Hexabenzocoronenes with Extended Heterocyclic Moieties Improve Visible-Light Absorption and Performance in Organic Solar Cells

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    The large band gaps of existing contorted hexabenzocoronene derivatives severely limit visible-light absorption, restricting the photocurrents generated by solar cells utilizing contorted hexabenzocoronene (cHBC). To decrease the band gap and improve the light-harvesting properties, we synthesized cHBC derivatives having extended heterocyclic moieties as peripheral substituents. Tetrabenzofuranyldibenzocoronene (cTBFDBC) and tetrabenzothienodibenzocoronene (cTBTDBC) both exhibit broader absorption of the solar spectrum compared to cHBC, with peak absorbances on the order of 10<sup>5</sup> cm<sup>–1</sup> in the near-ultraviolet and in the visible. Planar-heterojunction organic solar cells comprising cTBFDBC or cTBTDBC as the donor and C<sub>70</sub> as the acceptor surpass those having cHBC in photocurrent generation and power-conversion efficiency. Interestingly, devices containing cTBFDBC/C<sub>70</sub> exhibit the highest photocurrents despite cTBTDBC having the smallest band gap of the three cHBC derivatives. X-ray reflectivity of the active layers indicates a rougher donor–acceptor interface when cTBFDBC is employed instead of the other two donors. Consistent with this observation, internal quantum efficiency spectra suggest improved charge transfer at the donor–acceptor interface when cTBFDBCas opposed to cTBTDBC or cHBCis used as the donor

    Low-Temperature Synthesis of a TiO<sub>2</sub>/Si Heterojunction

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    The classical SiO<sub>2</sub>/Si interface, which is the basis of integrated circuit technology, is prepared by thermal oxidation followed by high temperature (>800 °C) annealing. Here we show that an interface synthesized between titanium dioxide (TiO<sub>2</sub>) and hydrogen-terminated silicon (H:Si) is a highly efficient solar cell heterojunction that can be prepared under typical laboratory conditions from a simple organometallic precursor. A thin film of TiO<sub>2</sub> is grown on the surface of H:Si through a sequence of vapor deposition of titanium tetra­(<i>tert</i>-butoxide) (<b>1</b>) and heating to 100 °C. The TiO<sub>2</sub> film serves as a hole-blocking layer in a TiO<sub>2</sub>/Si heterojunction solar cell. Further heating to 250 °C and then treating with a dilute solution of <b>1</b> yields a hole surface recombination velocity of 16 cm/s, which is comparable to the best values reported for the classical SiO<sub>2</sub>/Si interface. The outstanding performance of this heterojunction is attributed to Si–O–Ti bonding at the TiO<sub>2</sub>/Si interface, which was probed by angle-resolved X-ray photoelectron spectroscopy. Attenuated total reflectance Fourier transform infrared spectroscopy (ATR-FTIR) showed that Si–H bonds remain even after annealing at 250 °C. The ease and scalability of the synthetic route employed and the quality of the interface it provides suggest that this surface chemistry has the potential to enable fundamentally new, efficient silicon solar cell devices
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