Photoluminescence characterization of a high-efficiency Cu2ZnSnS4 device

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We report on low-temperature (4 K) photoluminescence of an 8.3% efficient Cu2ZnSnS4 photovoltaic device. Measurements were recorded as a function of excitation intensity, and the evolution of the resulting spectra is discussed. The spectra indicate that the radiative recombination is characteristic of heavily compensated material with a high quasi donor-acceptor pair density, as determined by the relationship between peak height, peak position, and excitation intensity, as well as the carrier lifetimes at different wavelengths. The blue-shift of the defect-derived peak position is used to estimate the quasi donor-acceptor pair spacing and density. The data indicate an average pair spacing of roughly 3.3 nm, yielding an overall total radiative-defect density of similar to 1.3 x 10(19) cm(-3). (C) 2013 AIP Publishing LLC.
Publisher
AMER INST PHYSICS
Issue Date
2013-10
Language
English
Article Type
Article
Keywords

SOLAR-CELLS; THIN-FILMS; DEFECTS

Citation

JOURNAL OF APPLIED PHYSICS, v.114, no.15

ISSN
0021-8979
DOI
10.1063/1.4825317
URI
http://hdl.handle.net/10203/191134
Appears in Collection
MS-Journal Papers(저널논문)
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