The effect of octahedral tilting on proton binding sites and transition states in pseudo-cubic perovskite oxides

Maria A. Gomez, Mary A. Griffin, Saryu Jindal, Kristin D. Rule, Valentino R. Cooper

Research output: Contribution to journalArticlepeer-review

101 Scopus citations

Abstract

Proton conducting oxide ceramics have shown potential for use in fuel cell technologies. Understanding the energy pathways for proton conduction could help us design more efficient fuel cell materials. This paper describes how octahedral tilting affects the relative energies of proton binding sites, transition states, and conduction pathways in cubic and pseudo-cubic perovskites. First, the structure for cubic and pseudo-cubic forms of BaTi O3, BaZr O3, CaTi O3, and CaZr O3, is found. Even when cubic symmetry is enforced, CaTi O3, and CaZr O3 exhibit octahedral tilting distortions characteristic of orthorhombic phases while BaTi O3 and BaZr O3 remain undistorted. Octahedral tilting gives rise to proton binding sites facilitating inter- and intra-octahedral proton transfer while the proton binding sites of undistorted perovskites facilitate only intra-octahedral proton transfer. The nudged elastic band method is used to find minimum energy paths between the proton binding sites. As distortions increase, inter-octahedral proton transfer barriers decrease while intra-octahedral proton transfer barriers increase. Concurrently, rotational barriers from oxygens facilitating inter-octahedral proton transfer increase while rotational barriers from oxygens facilitating intra-octahedral proton transfer decrease. Intra-octahedral transfer is the rate-limiting step to the lowest energy extended proton conduction pathway in all the perovskites considered.

Original languageEnglish
Article number094703
JournalJournal of Chemical Physics
Volume123
Issue number9
DOIs
StatePublished - Sep 1 2005
Externally publishedYes

Funding

This research was supported by Camille and Henry Dreyfus Faculty Start-up Grant Program for Undergraduate Institutions and an ACS PRF Type G Starter Grant. Computational resources were provided in part by the MERCURY supercomputer consortium (http://mars.hamilton.edu) under NSF Grant No. CHE-0116435.

FundersFunder number
National Science FoundationCHE-0116435
American Cancer Society
Camille and Henry Dreyfus Foundation

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