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Título : | Effect of Argon on the Properties of Copper Nitride Fabricated by Magnetron Sputtering for the Next Generation of Solar Absorbers |
Autor : | Figueira, Carla. A. Del Rosario, G. Plugiese, D. Rodríguez-Tapiador, M.I. Fernández, S |
Palabras clave : | copper nitride reactive RF magentron sputtering gaseous environment solar absorber |
Fecha de publicación : | 15-dic-2022 |
Editorial : | Fabrizio Roccaforte |
Citación : | Figueira, C.A.; Rosario, G.D.; Pugliese, D.; Rodríguez-Tapiador, M.I.; Fernández, S. Effect of Argon on the Properties of Copper Nitride Fabricated by Magnetron Sputtering for the Next Generation of Solar Absorbers. Materials 2022, 15, 8973. https://doi.org/10.3390/ma15248973 |
Citación : | volumen;15 |
Resumen : | Copper nitride, a metastable semiconductor material with high stability at room
temperature, is attracting considerable attention as a potential next-generation earth-abundant thinfilm
solar absorber. Moreover, its non-toxicity makes it an interesting eco-friendly material. In this
work, copper nitride films were fabricated using reactive radio frequency (RF) magnetron
sputtering at room temperature, 50 W of RF power, and partial nitrogen pressures of 0.8 and 1.0 on
glass and silicon substrates. The role of argon in both the microstructure and the optoelectronic
properties of the films was investigated with the aim of achieving a low-cost absorber material with
suitable properties to replace the conventional silicon in solar cells. The results showed a change in
the preferential orientation from (100) to (111) planes when argon was introduced in the sputtering
process. Additionally, no structural changes were observed in the films deposited in a pure nitrogen
environment. Fourier transform infrared (FTIR) spectroscopy measurements confirmed the
presence of Cu–N bonds, regardless of the gas environment used, and XPS indicated that the
material was mainly N-rich. Finally, optical properties such as band gap energy and refractive index
were assessed to establish the capability of this material as a solar absorber. The direct and indirect
band gap energies were evaluated and found to be in the range of 1.70–1.90 eV and 1.05−1.65 eV,
respectively, highlighting a slight blue shift when the films were deposited in the mixed gaseous
environment as the total pressure increased. |
URI : | http://documenta.ciemat.es/handle/123456789/2999 |
ISSN : | 1996-1944 |
Aparece en las colecciones: | Artículos de Energía
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