Volume 239, 2022

Chemical and electronic structure of the heavily intermixed (Cd,Zn)S:Ga/CuSbS2 interface

Abstract

The interface formation and chemical and electronic structure of the (Cd,Zn)S:Ga/CuSbS2 thin-film solar cell heterojunction were studied using hard X-ray photoelectron spectroscopy (HAXPES) of the bare absorber and a buffer/absorber sample set for which the buffer thickness was varied between 1 and 50 nm. We find a heavily intermixed interface, involving Cu, Zn, and Cd as well as significant Ga and Cu profiles in the buffer. The valence band (VB) offset at the buffer/absorber interface was derived as (−1.3 ± 0.1) eV, which must be considered an upper bound as the Cu diffused into the buffer might form a Cu-derived VB maximum located closer to the Fermi level. The estimated conduction band minimum was ‘cliff’-like; a situation made more severe considering the Cu-deficiency found for the CuSbS2 surface. The complex interface structure’s effect on the performance of (Cd,Zn)S:Ga/CuSbS2-based solar cells and its limitation is discussed together with possible mitigation strategies.

Graphical abstract: Chemical and electronic structure of the heavily intermixed (Cd,Zn)S:Ga/CuSbS2 interface

Associated articles

Supplementary files

Article information

Article type
Paper
Submitted
28 فرؤری 2022
Accepted
11 میٔ 2022
First published
11 میٔ 2022
This article is Open Access
Creative Commons BY license

Faraday Discuss., 2022,239, 130-145

Chemical and electronic structure of the heavily intermixed (Cd,Zn)S:Ga/CuSbS2 interface

C. Hartmann, R. E. Brandt, L. L. Baranowski, L. Köhler, E. Handick, R. Félix, R. G. Wilks, A. Zakutayev, T. Buonassisi and M. Bär, Faraday Discuss., 2022, 239, 130 DOI: 10.1039/D2FD00056C

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