Photocatalytic properties of porous titania grown by oblique angle deposition

M. J. Riley, B. Williams, G. Y. Condon, J. Borja, T. M. Lu, W. N. Gill, J. L. Plawsky

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

Resumen

High surface area nanorods of titanium dioxide were grown by oblique angle deposition on a transparent substrate to investigate their effectiveness as photocatalytic agents for the destruction of organic contaminants in air and water. Optical transmission measurements were made that allowed for an estimation of the porosity of the film (75-78). Comparing transmission measurements with those from a dense anatase film showed that the penetration depth for the light into the nanorod film was 2.5 times that in a dense, anatase film. The photocatalytic degradation of indigo carmine dye on the porous films was shown to depend on film thickness and annealing conditions. The effectiveness of the film was assessed by observing the change in absorbance of the dye at 610 nm over time and quantifying the film performance using a pseudo-first-order reaction rate model. Reaction rates increased as the film thickness increased from 600 nm to 1000 nm, but leveled out or decreased at thicknesses beyond 1500 nm. A transport/reaction model was used to show that there exists an optimal geometry that maximizes the overall reaction rate and that such a geometry can be simply produced using glancing angle deposition. The nanorod films were benchmarked against nanoparticle films and were shown to perform as well as 0.73 g/L of 25-nm-diameter anatase nanoparticles with surface area of 50 m 2/g.

Idioma originalInglés
Número de artículo074904
PublicaciónJournal of Applied Physics
Volumen111
N.º7
DOI
EstadoPublicada - 1 abr. 2012
Publicado de forma externa

Nota bibliográfica

Funding Information:
This work was supported in part by the Engineering Research Centers Program of the National Science Foundation under NSF Cooperative Agreement No. EEC-0812056 and in part by New York State under NYSTAR contract C090145. This material is also based upon work supported by the National Science Foundation under Grant No. 0333314.

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