Published March 7, 2012 | Version v1
Journal article

The effect of step geometry in copper oxidation by hyperthermal O2 molecular beam: Cu(511) vs Cu(410)

  • 1. Department of Chemistry, Graduate School of Science, Osaka University, 1-1 Machikaneyama-cho, Toyonaka, Osaka 560-0043 (Japan)
  • 2. Renovation Center of Instruments for Science Education and Technology, Osaka University, 8-1 Mihogaoka, Ibaraki, Osaka 560-0047 (Japan)
  • 3. Dipartimento di Fisica dell'Universita di Genova and IMEM-CNR, Via Dodecaneso 33, 16146 Genova (Italy)
  • 4. Surface Reaction Dynamics Research Group, Quantum Beam Science Directorate, Japan Atomic Energy Agency, 1-1-1 Kouto, Sayo-cho, Sayo-gun, Hyogo 679-5148 (Japan)

Description

Steps are known to be often the active sites for the dissociation of O2 molecules and the nucleation sites of oxide films since they provide paths for subsurface migration and oxygen incorporation. In order to unravel the effect of their morphology on the oxidation of Cu surfaces, we present here a detailed investigation of the O2 interaction with Cu(511) and compare it with previous results for Cu(410), a surface exhibiting terraces of similar size and geometry but different step morphology. As for Cu(410) we find, by x-ray photoemission spectroscopy performed with synchrotron radiation, that Cu2O formation gradually starts above half a monolayer oxygen coverage and that the ignition of oxidation can be lowered to room temperature by dosing O2 via a supersonic molecular beam at hyperthermal energy. The oxidation rate for Cu(511) comes out to be lower than for Cu(410) at normal incidence, about the same when the O2 molecules impinge towards the ascending step rise, but higher when they hit the surface along trajectories even slightly inclined towards the descending step rise. These findings can be rationalized by a collision induced absorption mechanism.

Additional details

Identifiers

Publishing Information

Journal Title
Journal of Chemical Physics
Journal Volume
136
Journal Issue
9
Journal Page Range
p. 094704-094704.8
ISSN
0021-9606
CODEN
JCPSA6

Optional Information

Notes
(c) 2012 American Institute of Physics