2016
DOI: 10.1016/j.solmat.2015.12.016
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Selenization kinetics in Cu2ZnSn(S,Se)4 solar cells prepared from nanoparticle inks

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Cited by 50 publications
(33 citation statements)
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“…In order to produce ecient absorbing layers, CZTS precursor thin lms were then selenised to introduce grain growth, resulting in CZTSSe absorbers with lm thickness ∼ 1 µm. This process has been described in greater detail in our previous work (Qu et al, 2016b). The crystal structure of both types of lm is kesterite in nature determined from X-ray diraction (XRD).…”
Section: Methodsmentioning
confidence: 99%
“…In order to produce ecient absorbing layers, CZTS precursor thin lms were then selenised to introduce grain growth, resulting in CZTSSe absorbers with lm thickness ∼ 1 µm. This process has been described in greater detail in our previous work (Qu et al, 2016b). The crystal structure of both types of lm is kesterite in nature determined from X-ray diraction (XRD).…”
Section: Methodsmentioning
confidence: 99%
“…The resulting nanoparticle inks were then deposited on molybdenum substrates via spin coating to form the CZTS precursor thin film with a thickness of ∼1 µm. Thereupon, CZTS precursor thin films were annealed in a selenium atmosphere to introduce grain growth, resulting in CZTSSe absorbers 33 41 and metallic ratios Zn/Sn: 1.02, Cu/(Zn+Sn): 0.85. Buffer layers of CdS (∼60 nm) and In 2 S 3 (∼70 nm) were prepared by chemical bath deposition (CBD).…”
Section: Methodsmentioning
confidence: 99%
“…• C. This temperature was then held for 20 minutes before being cooled down rapidly (∼ 20 • C /min) as detailed elsewhere (Qu et al, 2016b GD-proler 2) using an Ar plasma with a crater size of 4 mm in diameter.…”
Section: Theorymentioning
confidence: 99%