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Surface and interstitial transition barriers in rutile (110) surface growth

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journal contribution
posted on 01.02.2013 by E. Sanville, Louis J. Vernon, Steven Kenny, Roger Smith, Y. Moghaddam, C. Browne, P. Mulheran
We present calculated surface and interstitial transition barriers for Ti, O, O2, TiO, and TiO2 atoms and clusters at the rutile (110) surface. Defect structures involving these small clusters, including adcluster and interstitial binding sites, were calculated by energy minimization using density-functional theory (DFT). Transition energies between these defect sites were calculated using the NEB method. Additionally, a modified SMB-Q charge equilibration empirical potential and a fixed-charge empirical potential were used for a comparison of the transition energy barriers. Barriers of 1.2–3.5 eV were found for all studied small cluster transitions upon the surface except for transitions involving O2. By contrast, the O2 diffusion barriers along the [001] direction upon the surface are only 0.13 eV. The QEq charge equilibration model gave mixed agreement with the DFT calculations, with the barriers ranging between 0.8 and 5.8 eV.

History

School

  • Science

Department

  • Mathematical Sciences

Citation

SANVILLE, E. ... et al., 2009. Surface and interstitial transition barriers in rutile (110) surface growth. Physical Review B (Condensed Matter and Materials Physics), 80 (23), 9 pp.

Publisher

© The American Physical Society

Version

VoR (Version of Record)

Publication date

2009

Notes

This article was published in the journal, Physical Review B (Condensed Matter and Materials Physics) [© The American Physical Society]. The definitive version is available at: http://dx.doi.org/10.1103/PhysRevB.80.235308

ISSN

1098-0121

Language

en

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