Abstract
This work examines the feasibility and performance impact of replacing the usual molybdenum back contact with indium-free transparent conductive oxides (TCOs) like fluorine-doped tin oxide (SnO2:F) and aluminum-doped zinc oxide (ZnO:Al) for ultra-thin Cu (In,Ga)Se2 (CIGS) solar cells (250–450 nm). Motivated by indium scarcity and cost reduction, these TCOs are evaluated for their figure of merit, stability under Se atmosphere, Na diffusion permeability, and band alignment with CIGS absorbers. Using simulations, prototype fabrication, and comprehensive characterizations, the compatibility of these TCOs with CIGS absorbers is assessed. Solar cells with thicknesses of 450 and 250 nm are fabricated. Their performance was compared under both rear and front illumination, as well as with the use of reflectors. A record efficiency of 8.6% with front illumination is achieved for a 250-nm CIGS absorber using a gold back reflector with SnO2:F, single-step CIGS deposition, and no heavy alkalines doping. The best rear-illuminated efficiencies are obtained with ZnO:Al back contacts, reaching 6% for a 250-nm CIGS, with only a 9% loss in Jsc compared to front illumination, confirming a lower surface recombination rate at the ZnO:Al/CIGS interface compared to Mo/CIGS or SnO2:F/CIGS interfaces.
| Original language | English |
|---|---|
| Pages (from-to) | 1109-1123 |
| Number of pages | 15 |
| Journal | Progress in Photovoltaics: Research and Applications |
| Volume | 33 |
| Issue number | 10 |
| DOIs | |
| Publication status | Published - 1 Oct 2025 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
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SDG 7 Affordable and Clean Energy
Keywords
- back-contact recombination
- bifacial solar cells
- indium-free transparent conducting back contact
- ultra-thin Cu (In,Ga)Se solar cells
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