Issue 34, 2011

Formation of Ag+–N–TiO2 nanochains and their HPA-composites as highly visible light-sensitive photocatalysts toward two-color solar cells

Abstract

Ag+-coupled N-doped TiO2 (Ag+–N–TiO2) nanochains were newly synthesized by combination of sol–gel and hydrothermal methods, and their structures were characterized by TEM, SEM, and XPS. The UV-visible diffuse reflectance absorption spectrum of Ag+–N–TiO2 nanochains was observed to absorb visible light in the broad range of 400–800 nm as compared to neat N–TiO2, exhibiting efficient visible light-photocatalytic activity. Their visible light absorption band became much broader and stronger upon formation of composites with heteropoly phosphotungstic acid (HPA), and their photocatalytic efficiency was observed to be further enhanced. The Ag+–N–TiO2 nanochains also exhibited improved photovoltaic performance with significantly high photoenergy conversion efficiency (PCE) (5.6%) under AM 1.5 (100 mW cm−2) as compared to N–TiO2 nanochains. The PCE was observed to be further enhanced to 7.6% by formation of HPA-composites. These results suggest that Ag and HPA play important roles in enhancement of PCE through the cooperative Z-scheme process of the electron transport triggered by two-color visible lights as in the plant photosynthetic system. The HPA-composites were also found to be useful for the dye-sensitized solar cells (DSSCs) as proved by synergistic enhancement of PCE to 10.2% as they are additionally incorporated with Ru-dye.

Graphical abstract: Formation of Ag+–N–TiO2 nanochains and their HPA-composites as highly visible light-sensitive photocatalysts toward two-color solar cells

Supplementary files

Article information

Article type
Paper
Submitted
06 Apr 2011
Accepted
31 May 2011
First published
11 Jul 2011

J. Mater. Chem., 2011,21, 12829-12835

Formation of Ag+–N–TiO2 nanochains and their HPA-composites as highly visible light-sensitive photocatalysts toward two-color solar cells

H. Lee, J. Lee, Y. Lee, J. Lee and M. Yoon, J. Mater. Chem., 2011, 21, 12829 DOI: 10.1039/C1JM11439E

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