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Kinetics of CO2 Reduction over Nonstoichiometric Ceria
Author(s) -
Simon Ackermann,
Laurent Sauvin,
Roberto Castiglioni,
Jennifer L. M. Rupp,
Jonathan R. Scheffe,
Aldo Steinfeld
Publication year - 2015
Publication title -
the journal of physical chemistry c
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.401
H-Index - 289
eISSN - 1932-7455
pISSN - 1932-7447
DOI - 10.1021/acs.jpcc.5b03464
Subject(s) - raman spectroscopy , kinetics , stoichiometry , sintering , materials science , oxygen , analytical chemistry (journal) , reducing atmosphere , activation energy , oxide , atmospheric temperature range , inorganic chemistry , chemistry , mineralogy , thermodynamics , metallurgy , organic chemistry , physics , chromatography , quantum mechanics , optics
The kinetics of CO 2 reduction over nonstoichimetric ceria, CeO 2-δ , a material of high potential for thermochemical conversion of sunlight to fuel, has been investigated for a wide range of nonstoichiometries (0.02 ≤ δ ≤ 0.25), temperatures (693 ≤ T ≤ 1273 K), and CO 2 concentrations (0.005 ≤ p CO 2 ≤ 0.4 atm). Samples were reduced thermally at 1773 K to probe low nonstoichiometries (δ < 0.05) and chemically at lower temperatures in a H 2 atmosphere to prevent particle sintering and probe the effect of higher nonstoichiometries (δ < 0.25). For extents greater than δ = 0.2, oxidation rates at a given nonstoichiometry are hindered for the duration of the reaction, presumably because of near-order changes, such as lattice compression, as confirmed via Raman Spectroscopy. Importantly, this behavior is reversible and oxidation rates are not affected at lower δ. Following thermal reduction at very low δ, however, oxidation rates are an order of magnitude slower than those of chemically reduced samples, and rates monotonically increase with the initial nonstoichiometry (up to δ = 0.05). This dependence may be attributed to the formation of stable defect complexes formed between oxygen vacancies and polarons. When the same experiments are performed with 10 mol % Gd 3+ doped ceria, in which defect complexes are less prevalent than in pure ceria, this dependence is not observed.

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