4.7 Article

Interplay of material thermodynamics and surface reaction rate on the kinetics of thermochemical hydrogen production

期刊

INTERNATIONAL JOURNAL OF HYDROGEN ENERGY
卷 42, 期 27, 页码 16932-16945

出版社

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.ijhydene.2017.05.184

关键词

Solar fuels; Thermochemical cycle; Kinetics; Ceria

资金

  1. Advanced Research Projects Agency - Energy of the U.S. Department of Energy [DE-AR0000182]
  2. EERE Postdoctoral Research Award
  3. NSF MRSEC [DMR-0080065]

向作者/读者索取更多资源

Production of chemical fuels using solar energy has been a field of intense research recently, and two-step thermochemical cycling of reactive oxides has emerged as a promising route. In this process, the oxide of interest is cyclically exposed to an inert gas, which induces (partial) reduction of the oxide at a high temperature, and to an oxidizing gas of either H2O or CO2 at the same or lower temperature, which reoxidizes the oxide, releasing H-2 or CO. Thermochemical cycling of porous ceria was performed here under realistic conditions to identify the limiting factor for hydrogen production rates. The material, with 88% porosity and moderate specific surface area, was reduced at 1500 degrees C under inert gas with 10 ppm residual O-2, then reoxidized with H2O under flow of 600 sccm g(-1) of 20% H2O in Ar to produce H-2. The fuel production process transitions from one controlled by surface reaction kinetics at temperatures below -4000 degrees C to one controlled by the rate at which the reactant gas is supplied at temperatures above -1100 degrees C. The reduction of ceria, when heated from 800 to 1500 degrees C, is observed to be gas limited at a temperature ramp rate of 50 degrees C min(-1) at a flow of 1000 sccm g(-1) of 10 ppm O-2 in Ar. Consistent with these observations, application of Rh catalyst particles improves the oxidation rate at low temperatures, but provides no benefit at high temperatures for either oxidation or reduction. The implications of these results for solar thermochemical reactors are discussed. (C) 2017 Hydrogen Energy Publications LLC. Published by Elsevier Ltd. All rights reserved.

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