4.8 Article

Maximizing fuel production rates in isothermal solar thermochemical fuel production

Journal

APPLIED ENERGY
Volume 183, Issue -, Pages 1098-1111

Publisher

ELSEVIER SCI LTD
DOI: 10.1016/j.apenergy.2016.09.012

Keywords

Solar fuels; Thermochemical cycle; Kinetics; Thermodynamics; Ceria

Funding

  1. Advanced Research Projects Agency - Energy of the U.S. Department of Energy [DE-AR0000182]
  2. U.S. National Science Foundation [CBET-1038307]
  3. EERE Postdoctoral Research Award

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Production of chemical fuels by isothermal pressure-swing cycles has recently generated significant interest. In this process a reactive oxide is cyclically exposed to an inert gas, which induces partial reduction of the oxide, and to an oxidizing gas of either H2O or CO2, which reoxidizes the oxide, releasing H-2 or CO. At sufficiently high temperatures and sufficiently low gas flow rates, both the reduction and oxidation steps become limited only by the flow of gas across the material and not by material kinetic factors. In this contribution, we develop a numerical model describing fuel production rates in this gas-phase limited regime. The implications of this behavior are explored under all possible isothermal pressure-swing cycling conditions, and the outcome is optimized in terms of fuel production rate as well as fuel conversion and utilization of input gas of all types. Fuel production rate is maximized at infinitesimally small cycle times and attains a value that is independent of material thermodynamics. Gas utilization is maximized at infinitesimally small gas inputs, but the values can be made independent of cycle time, depending on manipulation of flow conditions. Gas-phase conditions (temperature, oxidant and reductant gas partial pressures, and CO2 vs H2O as oxidant) have a strong impact on fuel production metrics. Under realistic, finite cycle times, material thermodynamics play a measurable role in establishing fuel production rates. (C) 2016 Elsevier Ltd. All rights reserved.

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