4 research outputs found
Diffusion of Oxygen in Ceria at Elevated Temperatures and Its Application to H<sub>2</sub>O/CO<sub>2</sub> Splitting Thermochemical Redox Cycles
Determination of reaction and oxygen
diffusion rates at elevated
temperatures is essential for modeling, design, and optimization of
high-temperature solar thermochemical fuel production processes, but
such data for state-of-the-art redox materials, such as ceria, is
sparse. Here, we investigate the solid-state reduction and oxidation
of sintered nonstoichiometric ceria at elevated temperatures relevant
to solar thermochemical redox cycles for splitting H<sub>2</sub>O
and CO<sub>2</sub> (1673 K ≤ <i>T</i> ≤ 1823
K, 3 × 10<sup>–4</sup> atm ≤ <i>p</i><sub>O<sub>2</sub></sub> ≤ 2.5 × 10<sup>–3</sup> atm). Relaxation experiments are performed by subjecting the sintered
ceria to rapid oxygen partial pressure changes and measuring the
time required to achieve thermodynamic equilibrium state. From such
data, we elucidate information regarding ambipolar oxygen diffusion
coefficients through comparison of experimental data to a numerical
approximation of Fick’s second law based on finite difference
methods. In contrast to typically applied analytical approaches, where
diffusion coefficients are necessarily concentration independent,
such a numerical approach is capable of accounting for more realistic
concentration dependent diffusion coefficients and also accounts for
transient gas phase boundary conditions pertinent to dispersion and
oxygen consumption/evolution. Ambipolar diffusion coefficients are
obtained in the range 1.5·10<sup>–5</sup> cm<sup>2</sup> s<sup>–1</sup> ≤ <i>D̃</i> ≤
4·10<sup>–4</sup> cm<sup>2</sup> s<sup>–1</sup> between 1673 and 1823 K. These results highlight the rapid nature
of ceria reduction to help guide the design of redox materials for
solar reactors, the importance of accounting for transient
boundary conditions during relaxation experiments (either mass based
or conductivity based), and point to the flexibility of using a numerical
analysis in contrast to typical analytical approaches
Thermal Reduction of Ceria within an Aerosol Reactor for H<sub>2</sub>O and CO<sub>2</sub> Splitting
An aerosol reactor
was tested for the thermal reduction of ceria
as part of a solar thermochemical redox cycle for producing H<sub>2</sub> and CO from H<sub>2</sub>O and CO<sub>2</sub>. The design
is based on the downward aerosol flow of ceria particles, counter
to an argon sweep gas, which are rapidly heated and thermally reduced
within residence times of less than 1 s. When operating in the temperature
range of 1723–1873 K and at oxygen partial pressures between
5 × 10<sup>–5</sup> and 1.2 × 10<sup>–4</sup> atm, reduction extents of small particles (<i>D</i><sub>v50</sub> = 12 μm) approached those predicted by thermodynamics.
However, heat- and mass-transfer effects were found to limit their
conversion when the ceria mass flow rate was increased above 100 mg
s<sup>–1</sup>. This reactor concept inherently results in
separation of the reduced ceria and evolved O<sub>2</sub>(g), operates
isothermally throughout the day, and decouples the reduction and oxidation
steps in both space and time for potential 24-h syngas generation
Diffusion of Oxygen in Ceria at Elevated Temperatures and Its Application to H<sub>2</sub>O/CO<sub>2</sub> Splitting Thermochemical Redox Cycles
Determination of reaction and oxygen
diffusion rates at elevated
temperatures is essential for modeling, design, and optimization of
high-temperature solar thermochemical fuel production processes, but
such data for state-of-the-art redox materials, such as ceria, is
sparse. Here, we investigate the solid-state reduction and oxidation
of sintered nonstoichiometric ceria at elevated temperatures relevant
to solar thermochemical redox cycles for splitting H<sub>2</sub>O
and CO<sub>2</sub> (1673 K ≤ <i>T</i> ≤ 1823
K, 3 × 10<sup>–4</sup> atm ≤ <i>p</i><sub>O<sub>2</sub></sub> ≤ 2.5 × 10<sup>–3</sup> atm). Relaxation experiments are performed by subjecting the sintered
ceria to rapid oxygen partial pressure changes and measuring the
time required to achieve thermodynamic equilibrium state. From such
data, we elucidate information regarding ambipolar oxygen diffusion
coefficients through comparison of experimental data to a numerical
approximation of Fick’s second law based on finite difference
methods. In contrast to typically applied analytical approaches, where
diffusion coefficients are necessarily concentration independent,
such a numerical approach is capable of accounting for more realistic
concentration dependent diffusion coefficients and also accounts for
transient gas phase boundary conditions pertinent to dispersion and
oxygen consumption/evolution. Ambipolar diffusion coefficients are
obtained in the range 1.5·10<sup>–5</sup> cm<sup>2</sup> s<sup>–1</sup> ≤ <i>D̃</i> ≤
4·10<sup>–4</sup> cm<sup>2</sup> s<sup>–1</sup> between 1673 and 1823 K. These results highlight the rapid nature
of ceria reduction to help guide the design of redox materials for
solar reactors, the importance of accounting for transient
boundary conditions during relaxation experiments (either mass based
or conductivity based), and point to the flexibility of using a numerical
analysis in contrast to typical analytical approaches
Synthesis, Characterization, and Thermochemical Redox Performance of Hf<sup>4+</sup>, Zr<sup>4+</sup>, and Sc<sup>3+</sup> Doped Ceria for Splitting CO<sub>2</sub>
We
present results on the thermochemical redox performance and
analytical characterization of Hf<sup>4+</sup>, Zr<sup>4+</sup>, and
Sc<sup>3+</sup> doped ceria solutions synthesized via a sol–gel
technique, all of which have recently been shown to be promising for
splitting CO<sub>2</sub>. Dopant concentrations ranging from 5 to
15 mol % have been investigated and thermally cycled at reduction
temperatures of 1773 K and oxidation temperatures ranging from 873
to 1073 K by thermogravimetry. The degree of reduction of Hf and Zr
doped materials is substantially higher than those of pure ceria and
Sc doped ceria and increases with dopant concentration. Overall, 10
mol % Hf doped ceria results in the largest CO yields per mole of
oxide (∼0.5 mass % versus 0.35 mass % for pure ceria) based
on measured mass changes during oxidation. However, these yields were
largely influenced by their rate of reoxidation, not necessarily thermodynamic
limitations, as equilibrium was not achieved for either Hf or Zr doped
samples after 45 min exposure to CO<sub>2</sub> at all oxidation temperatures.
Additionally, sample preparation and grain size strongly affected
the oxidation rates and subsequent yields, resulting in slightly decreasing
yields as the samples were cycled up to 10 times. X-ray diffraction,
Raman, FT-IR, and UV/vis spectroscopy in combination with SEM-EDX
have been applied to characterize the elemental, crystalline, and
morphological attributes before and after redox reactions