Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
5354361 | Applied Surface Science | 2015 | 35 Pages |
Abstract
Each of the several Ru core XPS spectra characterized (3d, 3p and 3s) was found to be composed of three symmetric components. Together with two metal oxide O1s components, these give evidence of a rather complex, previously unidentified oxide that is initially formed. The Ru valence band (4d and 5s) spectra clearly demonstrate a loss of metallicity, a simultaneous increase of the Kubo gap, and an abrupt transfer in valence electron density from the 4d to the 5s orbitals (known as electron spill-over), as the NP size decreases below 0.5Â nm. TEM photomicrographs, as a function of deposition rate, show that, at a rate that gives insufficient time for the NP condensation energy to dissipate, the initially well-separated NPs are capable of diffusing laterally and aggregating. This indicates weak NP bonding to the HOPG substrate. Carbide is formed, at both high and low deposition rates, at Ru deposition thicknesses greater than 0.25Â nm, its formation explained by Ru NPs reacting with residual hydrocarbon vapor, under the influence of the heat of condensation released on Ru deposition, and not by Ru reacting with the HOPG substrate.
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Physical Sciences and Engineering
Chemistry
Physical and Theoretical Chemistry
Authors
R. Bavand, A. Yelon, E. Sacher,