Synthesis of Cs2AgSbCl6 and improved optoelectronic properties of Cs2AgSbCl6/TiO2 heterostructure driven by the interface effect for lead-free double perovskites solar cells
Double perovskites Cs2AgSbCl6 have been synthesized via the solution state for applications as a promising photovoltaic absorber. Considering TiO2 as an electron transport layer (ETL), Cs2AgSbCl6/TiO2 heterojunction nanoparticles have also been prepared by the hydrothermal process to study the inter...
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Veröffentlicht in: | Applied physics letters 2017-10, Vol.111 (15) |
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Sprache: | eng |
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Zusammenfassung: | Double perovskites Cs2AgSbCl6 have been synthesized via the
solution state for applications as a promising photovoltaic absorber. Considering
TiO2 as an electron transport layer (ETL),
Cs2AgSbCl6/TiO2 heterojunction nanoparticles have also
been prepared by the hydrothermal process to study the interface effect. Experimental
measurements show that Cs2AgSbCl6 has a cubic structure with the
lattice constant of 10.699 Å. The absorption peaks in the optical spectrum of the Ag and
Sb-based double perovskites agree well with our density functional theory calculations.
The Cs2AgSbCl6/TiO2 heterostructure exhibits enhanced
optical absorption in the visible-light region compared to that of
Cs2AgSbCl6, which is caused by the formation of the interface
states and the decreased bandgap, thus facilitating the photo-induced optical transition
in the visible-light region. From the charge transfer analysis of two interfaces
(Ag2Sb2Cl8/TiO2 and
Cs4Cl4/TiO2 interfaces), we find that the efficient
separation of photo-induced carriers can be achieved at the
Cs4Cl4/TiO2 interface, with electron flowing from the
double perovskite layer to the TiO2 ETL, which is beneficial for improving the
power conversion efficiency of solar cells. The combined study of theory and experiments
indicates that the double perovskites Cs2AgSbCl6 would be a
promising light-absorbing material in contact with TiO2 for the lead-free
perovskite-based solar cell devices. |
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ISSN: | 0003-6951 1077-3118 |
DOI: | 10.1063/1.4999192 |