TY - JOUR
T1 - Deposition of ultra thin CuInS2 absorber layers by ALD for thin film solar cells at low temperature (down to 150°C)
AU - Schneider, Nathanaelle
AU - Bouttemy, Muriel
AU - Genevée, Pascal
AU - Lincot, Daniel
AU - Donsanti, Frédérique
N1 - Publisher Copyright:
© 2015 IOP Publishing Ltd.
PY - 2015/6/6
Y1 - 2015/6/6
N2 - Two new processes for the atomic layer deposition of copper indium sulfide (CuInS2) based on the use of two different sets of precursors are reported. Metal chloride precursors (CuCl, InCl3) in combination with H2S imply relatively high deposition temperature (Tdep = 380°C), and due to exchange reactions, CuInS2 stoechiometry was only achieved by depositing In2S3 layers on a CuxS film. However, the use of acac- metal precursors (Cu(acac)2, In(acac)3) allows the direct deposition of CuInS2 at temperature as low as 150°C, involving in situ copper-reduction, exchange reaction and diffusion processes. The morphology, crystallographic structure, chemical composition and optical band gap of thin films were investigated using scanning electronic microscope, x-ray diffraction under grazing incidence conditions, x-ray fluorescence, energy dispersive spectrometry, secondary ion mass spectrometry, x-ray photoelectron spectroscopy and UV-vis spectroscopy. Films were implemented as ultra-thin absorbers in a typical CIS-solar cell architecture and allowed conversion efficiencies up to 2.8%.
AB - Two new processes for the atomic layer deposition of copper indium sulfide (CuInS2) based on the use of two different sets of precursors are reported. Metal chloride precursors (CuCl, InCl3) in combination with H2S imply relatively high deposition temperature (Tdep = 380°C), and due to exchange reactions, CuInS2 stoechiometry was only achieved by depositing In2S3 layers on a CuxS film. However, the use of acac- metal precursors (Cu(acac)2, In(acac)3) allows the direct deposition of CuInS2 at temperature as low as 150°C, involving in situ copper-reduction, exchange reaction and diffusion processes. The morphology, crystallographic structure, chemical composition and optical band gap of thin films were investigated using scanning electronic microscope, x-ray diffraction under grazing incidence conditions, x-ray fluorescence, energy dispersive spectrometry, secondary ion mass spectrometry, x-ray photoelectron spectroscopy and UV-vis spectroscopy. Films were implemented as ultra-thin absorbers in a typical CIS-solar cell architecture and allowed conversion efficiencies up to 2.8%.
KW - Atomic layer deposition
KW - Copper indium sulfide
KW - Thin film solar cells
U2 - 10.1088/0957-4484/26/5/054001
DO - 10.1088/0957-4484/26/5/054001
M3 - Article
AN - SCOPUS:84921038549
SN - 0957-4484
VL - 26
JO - Nanotechnology
JF - Nanotechnology
IS - 5
M1 - 054001
ER -