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LEED-IV study of the rutile TiO2(110)1×2 surface with a Ti-interstitial added-row reconstruction

M. Blanco-Rey, J. Abad, C. Rogero, J. Méndez, M. F. López, E. Román, J. A. Martín-Gago, and P. L. de Andrés
Phys. Rev. B 75, 081402(R) – Published 9 February 2007

Abstract

Upon sputtering and annealing in UHV at 1000K, the rutile TiO2(110) surface undergoes a 1×11×2 phase transition. The resulting 1×2 surface is Ti rich, formed by strands of double Ti rows as seen on scanning tunneling microscopic images, but its detailed structure and composition have been subject to debate in the literature for years. Recently, Park et al. [Phys. Rev. Lett. 96, 226105 (2006)] have proposed a model where Ti atoms are located on interstitial sites with Ti2O stoichiometry. This model, when it is analyzed using LEED-IV data [Phys. Rev. Lett. 96, 0055502 (2006)], does not yield an agreement between theory and experiment as good as the previous best fit for Onishi and Iwasawa’s model for the long-range 1×2 reconstruction. Therefore, the Ti2O3 added row is the preferred one from the point of view low-energy electron diffraction.

  • Figure
  • Figure
  • Received 22 November 2006

DOI:https://doi.org/10.1103/PhysRevB.75.081402

©2007 American Physical Society

Authors & Affiliations

M. Blanco-Rey1,*, J. Abad2, C. Rogero3, J. Méndez1, M. F. López1, E. Román1, J. A. Martín-Gago1, and P. L. de Andrés1

  • 1Instituto de Ciencia de Materiales (CSIC), Cantoblanco, 28049 Madrid, Spain
  • 2Centro de Investigación en Optica y Nanofísica, Universidad de Murcia, Campus Espinardo, 30100 Murcia, Spain
  • 3Centro de Astrobiología (CSIC-INTA), Carretera de Ajalvir km. 4, 28850 Torrejón de Ardoz, Madrid, Spain

  • *Present address: Department of Chemistry, University of Cambridge, Lensfield Road, Cambridge CB2 1EW, UK. Electronic address: mb633@cam.ac.uk

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Issue

Vol. 75, Iss. 8 — 15 February 2007

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