Please use this identifier to cite or link to this item: http://hdl.handle.net/1942/40407
Title: Ge-Alloyed Kesterite Thin-Film Solar Cells: Previous Investigations and Current Status - a Comprehensive Review
Authors: SCAFFIDI, Romain 
BIRANT, Gizem 
DE WILD, Jessica 
VERMANG, Bart 
BRAMMERTZ, Guy 
Flandre, Denis
Issue Date: 2023
Publisher: Royal Society of Chemistry
Source: Journal of Materials Chemistry A, 11(25), p. 13174-13194
Abstract: The incorporation of Ge into kesterite thin-film absorbers for photovoltaics (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 of Ge alloying is to solve the critical open-circuit voltage (Voc) deficit for kesterite solar cells, still unresolved and under strong debate. First, the substitution of Sn by 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 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 graded bandgap and enlarged crystalline grains. This study unveils encouraging prospects for Ge-boosted kesterite PV devices.
Document URI: http://hdl.handle.net/1942/40407
ISSN: 2050-7488
e-ISSN: 2050-7496
DOI: 10.1039/D3TA01218B
ISI #: 001006422300001
Rights: TheRoyalSocietyofChemistry2023 Open Access Article. Published on 14 June 2023. Downloaded on 6/29/2023 12:46:29 PM. This article is licensed under a Creative Commons Attribution-NonCommercial 3.0 Unported Licence
Category: A1
Type: Journal Contribution
Appears in Collections:Research publications

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