Choudhary, V. R. ; Patil, V. P. ; Jana, P. ; Uphade, B. S. (2008) Nano-gold supported on Fe2O3: a highly active catalyst for low temperature oxidative destruction of methane green house gas from exhaust/waste gases Applied Catalysis A: General, 350 (2). pp. 186-190. ISSN 0926-860X
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Official URL: http://linkinghub.elsevier.com/retrieve/pii/S09268...
Related URL: http://dx.doi.org/10.1016/j.apcata.2008.08.008
Abstract
A number of nano-gold catalysts were prepared by depositing gold on different metal oxides (viz. Fe2O3, Al2O3, Co3O4, MnO2, CeO2, MgO, Ga2O3 and TiO2), using the homogeneous deposition precipitation (HDP) technique. The catalysts were evaluated for their performance in the combustion of methane (1 mol% in air) at different temperatures (300-600°C) for a GHSV of 51,000 h-1. The supported nano-gold catalysts have been characterized for their gold loading (by ICP) and gold particle size (by TEM/HRTEM or XRD peak broadening). Among these nano-gold catalysts, the Au/Fe2O3 (Au loading = 6.1% and Au particle size = 8.5 nm) showed excellent performance. For this catalyst, temperature required for half the methane combustion was 387°C, which is lower than that required for Pd(1%)/Al2O3 (400°C) and Pt(1%)/Al2O3 (500°C) under identical conditions. A detailed investigation on the influence of space velocity (GHSV = 10,000-100,000 cm3 g-1 h-1) at different temperatures (200-600°C) on the oxidative destruction of methane over the Au/Fe2O3 catalyst has also been carried out. The Au/Fe2O3 catalyst prepared by the HDP method showed much higher methane combustion activity than that prepared by the conventional deposition precipitation (DP) method. The XPS analysis showed the presence of Au in the different oxidation states (Au0, Au1+ and Au3+) in the catalyst.
Item Type: | Article |
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Source: | Copyright of this article belongs to Elsevier Science. |
Keywords: | Methane Combustion; Supported Nano-gold Catalysts; Au/FeO; Deposition Precipitation; Homogeneous Deposition Precipitation |
ID Code: | 10689 |
Deposited On: | 04 Nov 2010 07:14 |
Last Modified: | 28 May 2011 09:45 |
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