Issue 25, 2023

Ge-alloyed kesterite thin-film solar cells: previous investigations and current status – a comprehensive review

Abstract

The incorporation of Ge into kesterite thin-film absorbers for photovoltaic (PV) applications is thoroughly reviewed. Kesterite materials constitute a promising and critical raw material-free alternative to other inorganic thin-film PV compounds such as Cu(In,Ga)Se2 and CdTe. The interest in Ge alloying is to solve the critical open-circuit voltage (Voc) deficit for kesterite solar cells, which is still unresolved and under strong debate. First, the substitution of Sn with Ge from 0 to 100% in the composition of Cu2Zn(Sn1−x,Gex)(Sy,Se1−y)4 absorbers is largely discussed, with a complete overview on the existing literature. It is concluded that fine composition tuning is essential to ensure the Ge-induced enhancement of morphology and single-phase growth through a modified reaction pathway. In this regard, choosing between vacuum- and non vacuum-based deposition methods also plays a crucial role, since the former allows further up-scaling whereas the latter leads to higher thin-film quality. Second, at the solar cell level, Se-rich devices with less than 40% Ge currently exhibit the lowest Voc and fill factor deficits with the highest efficiencies beyond 13%. This is mainly due to defect and band tail compensation as well as a graded bandgap and enlarged crystalline grains. This study unveils encouraging prospects for Ge-boosted kesterite PV devices.

Graphical abstract: Ge-alloyed kesterite thin-film solar cells: previous investigations and current status – a comprehensive review

Supplementary files

Article information

Article type
Review Article
Submitted
26 Feb 2023
Accepted
08 May 2023
First published
14 Jun 2023
This article is Open Access
Creative Commons BY-NC license

J. Mater. Chem. A, 2023,11, 13174-13194

Ge-alloyed kesterite thin-film solar cells: previous investigations and current status – a comprehensive review

R. Scaffidi, G. Birant, G. Brammertz, J. de Wild, D. Flandre and B. Vermang, J. Mater. Chem. A, 2023, 11, 13174 DOI: 10.1039/D3TA01218B

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