PUBLICATION: CRYSTALS

AUTHORS: Tang, ZG; Zhang, LJ; Su, ZH; Wang, Z; Chen, L; Wang, CY; Xiao, GP; Gao, XY

 

In this article, CsPbI2Br perovskite thin films were spin-coated on FTO, on which CuPc was deposited by thermal evaporation. The electronic structure at the CsPbI2Br/CuPc interface was examined during the CuPc deposition by in situ X-ray photoelectron spectroscopy (XPS) and ultraviolet photoelectron spectroscopy (UPS) measurements. No downward band bending was resolved at the CsPbI2Br side, whereas there is similar to 0.23 eV upward band bending as well as a dipole of similar to 0.08 eV identified at the molecular side. Although the hole injection barrier as indicated by the energy gap from CsPbI2Br valance band maximum (VBM) to CuPc highest occupied molecular orbital (HOMO) was estimated to be similar to 0.26 eV, favoring hole extraction from CsPbI2Br to CuPc, the electron blocking barrier of similar to 0.04 eV as indicated by the offset between CsPbI2Br conduction band minimum (CBM) and CuPc lowest unoccupied molecular orbital (LUMO) is too small to efficiently block electron transfer. Therefore, the present experimental study implies that CuPc may not be a promising hole transport material for high-performance solar cells using CsPbI2Br as active layer.

 

LINKS: http://dx.doi.org/10.3390/cryst11050547