This study is the first to quantify energy band alignments at a nanostructured TiO2/Au22(SG)18 cluster interface using X-ray photoelectron spectroscopy. The d-band of Au clusters shows band-like character and occupied states at the Fermi level are not detected. The results provide evidence of the existence of a finite optical energy gap in Au22(SG)18 clusters and the molecular-like nature of these clusters. The pinning position of the Fermi energy level at the interface was determined to be 2.8 and 1.3 eV higher than the top of the TiO2 valence band and the highest occupied molecular orbit level of the Au clusters, respectively. A diffuse reflectance and absorption analysis quantified a 3.2 eV bandgap of the TiO2 layer and a 2.2 eV energy gap between the highest occupied molecular orbit (HOMO) and the lowest unoccupied molecular orbit (LUMO) levels of the Au clusters. Thus, a cliff-like offset of 0.5 eV between the LUMO level and the TiO2 conduction band was determined. The cliff-like offset of 0.5 eV provides room for improving the efficiency of metal-cluster-sensitized solar cells (MCSSC) further by lowering the LUMO level through a change in the cluster size. The offset of 0.5 eV between the HOMO level and the 3I-/I-3 redox level yields a remarkable loss-in-potential, which implies the possibility of increasing the open-circuit voltage further by properly replacing the redox couple in the MCSSCs.
|Number of pages||10|
|Publication status||Published - 2021 Jan 7|
Bibliographical noteFunding Information:
This research was supported by the National Research Foundation (NRF) grants (NRF-2020H1D3A2A01111061, NRF-2020R1A4A2002590, NRF-2017R1A2B3006651) funded by the Ministry of Science and ICT, Republic of Korea. This work was partially supported by the Russian Science Foundation under Grant No. 20-69-47124.
© 2021 The Royal Society of Chemistry.
All Science Journal Classification (ASJC) codes
- Materials Science(all)