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Naji, M. |
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Motta, Antonella |
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Aletan, Dirar |
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Mohamed, Tarek |
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Ertürk, Emre |
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Taccardi, Nicola |
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Kononenko, Denys |
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Petrov, R. H. | Madrid |
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Alshaaer, Mazen | Brussels |
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Bih, L. |
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Casati, R. |
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Muller, Hermance |
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Kočí, Jan | Prague |
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Šuljagić, Marija |
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Kalteremidou, Kalliopi-Artemi | Brussels |
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Azam, Siraj |
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Ospanova, Alyiya |
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Blanpain, Bart |
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Ali, M. A. |
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Popa, V. |
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Rančić, M. |
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Ollier, Nadège |
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Azevedo, Nuno Monteiro |
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Landes, Michael |
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Rignanese, Gian-Marco |
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Beattie, Neil
Northumbria University
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (18/18 displayed)
- 2023A structural, optical and electrical comparison between physical vapour deposition and slot-die deposition of Al:ZnO (AZO)
- 2022Elimination of the carbon-rich layer in Cu2ZnSn(S, Se)4 absorbers prepared from nanoparticle inkscitations
- 2022Routes to Increase Performance for Antimony Selenide Solar Cells using Inorganic Hole Transport Layerscitations
- 2022Ex-situ Ge-doping of CZTS Nanocrystals and CZTSSe Solar Absorber Filmscitations
- 2022Exploring the Role of Temperature and Hole Transport Layer on the Ribbon Orientation and Efficiency of Sb2Se3 cells Deposited via Thermal Evaporation
- 2022Recovery mechanisms in aged kesterite solar cellscitations
- 2020Innovative fabrication of low-cost kesterite solar cells for distributed energy applications
- 2019Solution processing route to Na incorporation in CZTSSe nanoparticle ink solar cells on foil substratecitations
- 2018Temperature controlled properties of sub-micron thin SnS filmscitations
- 2018Temperature controlled properties of sub-micron thin SnS filmscitations
- 2018CZTSSe Solar Cells from Nanoparticle Inks
- 2017A combined Na and Cl treatment to promote grain growth in MOCVD grown CdTe thin filmscitations
- 2016Selenization kinetics inCu2ZnSn(S,Se)4 solar cells prepared from nanoparticle inkscitations
- 2016Sodium Induced Microstructural Changes in MOCVD-Grown CdTe Thin Films
- 2016The role of nanoparticle inks in determining the performance of solution processed Cu2ZnSn(S,Se)4thin film solar cellscitations
- 2013Crystallographic properties and elemental migration in two-stage prepared CuIn1−xAlxSe2 thin films for photovoltaic applicationscitations
- 2011Electrical, morphological and structural properties of RF magnetron sputtered Mo thin films for application in thin film photovoltaic solar cellscitations
- 2010Optical properties of thin films of Cu2ZnSnSe4 fabricated by sequential deposition and selenisation
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document
Elimination of the carbon-rich layer in Cu2ZnSn(S, Se)4 absorbers prepared from nanoparticle inks
Abstract
Kesterite Cu2ZnSn(S, Se)4 (CZTSSe) is a promising photovoltaic material attracting significant research interests in recent years. Among the variety of techniques employed for preparation of the absorber thin films, the best results are observed for a hydrazine-based method with efficiency up to 12.6 %. On the other hand, Cu2ZnSnS4 (CZTS) nanoparticle inks annealed in the presence of Se have shown efficiency as high as 9.3 %. Importantly, CZTS nanoparticle inks have the power to be compatible with high volume, high value manufacturing with a variety of substrates including flexible foils, plastics and ultra-thin glass. However, one of the current limitations of the nanoparticle ink technology is the presence of a fine-grain (FG) layer between the CZTSSe large grain (LG) layer and the back contact. The presence of this FG layer is likely to reduce device performance via carrier recombination through traps, interface states and increased grain boundary density. CZTS nanoparticles were synthesized by injection of cold sulphur (25 A^ ∘C) into hot metallic precursors ( (225 A^ ∘C) ). The long carbon chain molecule, oleylamine used in the nanoparticle synthesis step is believed to be the direct reason of the FG layer. Herein, a higher soft-baking temperature of 400 A^ ∘C is studied to evaporate the carbon rich solvent efficiently from the nanoparticle precursor thin films before the selenization process. As a result, the absorber is found to be composed of a single LG CZTSSe layer where the carbon-rich FG layer is eliminated.