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Unsteady radiative heat transfer within a suspension of ZnO particles undergoing thermal dissociation
Authors:W Lipiński  A Steinfeld
Affiliation:a Department of Mechanical and Process Engineering, ETH Zurich, 8092 Zurich, Switzerland
b Solar Technology Laboratory, Paul Scherrer Institute, 5232 Villigen, Switzerland
Abstract:An emitting, absorbing, and anisotropically scattering plain medium containing a suspension of ZnO particles is considered, in which the particles are directly exposed to high-flux irradiation and undergo shrinkage during their endothermic dissociation into Zn(g) and O2 at above 2100 K. The unsteady energy equation that links the rate of radiative heat transfer to the rate of the chemical reaction is formulated and solved numerically by the finite volume technique and the explicit Euler time-integration scheme. The path-length Monte Carlo method is applied for modeling the radiative transfer within the suspension using the absorption/scattering coefficients and the scattering phase function obtained from the Mie theory. It is found that the particle suspension can be heated rapidly from its initial 300 K to over 1800 K in less than 0.1 s, resulting in a more uniform temperature profile as the reaction progresses, particles shrink, and the suspension becomes optically thinner. The chemical conversion increases with decreasing initial particle diameter and volume fraction due to the efficient radiative absorption.
Keywords:Zinc oxide  Thermal dissociation  Radiative transfer  Monte Carlo  Solar chemistry
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