Understanding the role of acidity on the surface exchange reaction in mixed conductors: The case for water species
George Harrington a
a University of Bath, Bath BA2 7AY, United Kingdom, United Kingdom
Proceedings of 24th International Conference on Solid State Ionics (SSI24)
Fundamentals: Experiment and simulation
London, United Kingdom, 2024 July 14th - 19th
Organizers: John Kilner and Stephen Skinner
Invited Speaker, George Harrington, presentation 206
Publication date: 10th April 2024

The surface exchange reaction is, while technologically relevant, poorly described for many mixed ionic-electronic conductors (MIECs). Due to the complex, multi-step nature of the exchange reaction, over the years there have been efforts to develop empirical correlations between the exchange reaction and properties that are easier to measure, calculate, or engineer. These include, concentrations of defects, diffusion coefficients, and the position of the conduction band, valance band or Fermi level. All suffer from the same limitations: they are based on bulk properties.

Given that the oxygen exchange reaction takes place on the outer surface, it is not surprising that the surface chemistry plays a significant role in the oxygen exchange rate. Intuitively, one might expect increases in the exchange rate to come from the addition of redox-active transition metal species, however, recently Nicollet et al. demonstrated that the surface exchange rate of Pr0.1Ce0.9O2 (PCO) could be altered by more than 5 orders of magnitude by the infiltration of nominally inert, isovalent binary oxides, and that the change in the exchange rate is correlated with the acidity of the infiltrated species.[1] Experimental work from Riedl et al. have confirmed these findings,[2] and an increasing body of work have shown that this correlation extends to multiple MIEC systems.

Attempts to provide a mechanistic explanation have primarily focused on the role of electron transfer between the modified surface and adsorbed oxygen species. In this work, based on experimental data from model MEICs systems and an analysis of literature, we present an alternative hypothesis, which considers, instead, the role of water species from the gas atmosphere.  

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