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Characterization of Rh films on Ta(110)

Journal Article · · Journal of Vacuum Science and Technology, A (Vacuum, Surfaces and Films); (USA)
DOI:https://doi.org/10.1116/1.576694· OSTI ID:6820948
; ;  [1]
  1. Physics Department, Brookhaven National Laboratory, Upton, NY (USA)

The surface and electronic structure of Rh films on Ta(110) up to several monolayers thick on Ta(110) are characterized by photoemission, Auger emission, low-energy electron diffraction (LEED) and low-energy ion scattering (LEIS). From the variation of the Rh Auger peak-to-peak intensity as a function of evaporation time, Rh appears to grow in the Stranski--Krastanov mode at room temperature. However, the LEIS data show that the Rh adatoms begin to cluster on Ta(110) before growth of the monolayer is completed. Diffuse LEED scattering suggests that the Rh films are disordered. Photoemission shows that Rh chemisorption on Ta(110) generates two peaks located at {minus}1.5 and {minus}2.5 eV binding energy during the initial phase of thin-film growth (0{lt}{theta}{lt}0.5 ML). By 0.75 ML Rh coverage, these states merge into a broad structure centered near {minus}2 eV binding energy. Photoemission peaks typical of a Rh(111) surface are seen at higher coverages ({theta}{gt}3.7 ML). CO dissociates on the Rh/Ta(110) surface for Rh coverages{lt}2.5 ML and the surface develops a site capable of molecular CO adsorption above 0.3-ML Rh coverage.

DOE Contract Number:
AC02-76CH00016
OSTI ID:
6820948
Journal Information:
Journal of Vacuum Science and Technology, A (Vacuum, Surfaces and Films); (USA), Journal Name: Journal of Vacuum Science and Technology, A (Vacuum, Surfaces and Films); (USA) Vol. 8:3; ISSN JVTAD; ISSN 0734-2101
Country of Publication:
United States
Language:
English