(Institución)
 
 

Docu-menta > Energía > Artículos de Energía >

Por favor, use este identificador para citar o enlazar este ítem: http://documenta.ciemat.es/handle/123456789/2999

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

Ficheros en este ítem:

Fichero Descripción Tamaño Formato
materials-15-08973-publicado.pdf888.99 kBAdobe PDFVisualizar/Abrir
View Statistics

Los ítems de Docu-menta están protegidos por una Licencia Creative Commons, con derechos reservados.

 

Información y consultas: documenta@ciemat.es | Documento legal