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Bandgap tunable colloidal Cu-based ternary and quaternary chalcogenide nanosheets via partial cation exchange
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- Title
- Bandgap tunable colloidal Cu-based ternary and quaternary chalcogenide nanosheets via partial cation exchange
- Issued Date
- 2016
- Citation
- Ramasamy, Parthiban. (2016). Bandgap tunable colloidal Cu-based ternary and quaternary chalcogenide nanosheets via partial cation exchange. Nanoscale, 8(15), 7906–7913. doi: 10.1039/c5nr08666c
- Type
- Article
- Keywords
- ABSORPTION ; ATTACHMENT ; Cation Exchanges ; Colloidal Synthesis ; ELECTRICAL-PROPERTIES ; Energy Gap ; In-Situ Oxidation ; Low-Cost Photovoltaics ; NANOMATERIALS ; NANOPLATELETS ; NANOSCALE ; NANOSHEETS ; OPTOELECTRONICS ; Positive Ions ; Quaternary Chalcogenides ; Quaternary Semiconductors ; ROOM-TemPERATURE ; Semiconducting Selenium Compounds ; Synthesis (Chemical) ; Ternary Semiconductors ; THERMOELECTRIC APPLICATIONS ; Thickness Measurement ; Two Dimensional (2 D) ; ZN-S NANOCRYSTALS
- ISSN
- 2040-3364
- Abstract
-
Copper based ternary and quaternary semiconductor nanostructures are of great interest for the fabrication of low cost photovoltaics. Although well-developed syntheses are available for zero dimensional (0D) nanoparticles, colloidal synthesis of two dimensional (2D) nanosheets remains a big challenge. Here we report, for the first time, a simple and reproducible cation exchange approach for 2D colloidal Cu2GeSe3, Cu2ZnGeSe4 and their alloyed Cu2GeSxSe3-x, Cu2ZnGeSxSe4-x nanosheets using pre-synthesized Cu2xSe nanosheets as a template. A mechanism for the formation of Cu2-xSe nanosheets has been studied in detail. In situ oxidation of Cu+ ions to form a CuSe secondary phase facilitates the formation of Cu2-xSe NSs. The obtained ternary and quaternary nanosheets have average lateral size in micrometers and thickness less than 5 nm. This method is general and can be extended to produce other important ternary semiconductor nanosheets such as CuIn1-xGaxSe2. The optical band gap of these nanosheets is tuned from 1 to 1.48 eV, depending on their composition. © 2016 The Royal Society of Chemistry.
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- Publisher
- Royal Society of Chemistry
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