| AVS 66th International Symposium & Exhibition | |
| Surface Science Division | Friday Sessions |
| Session SS+HC+PS-FrM |
| Session: | Planetary, Ambient, and Operando Environments |
| Presenter: | Daniel Killelea, Loyola University Chicago |
| Authors: | D.R. Killelea, Loyola University Chicago M.E. Turano, Loyola University Chicago R.G. Farber, The University of Chicago K.D. Gibson, The University of Chicago S.J. Sibener, The University of Chicago W. Walkosz, Lake Forest College R.A. Rosenberg, Argonne National Laboratory |
| Correspondent: | Click to Email |
Understanding the interaction of oxygen with transition metal surfaces is important in many areas including corrosion and catalysis. Of interest to us is the formation and chemistry of subsurface oxygen (Osub); oxygen atoms dissolved in the near-surface region of catalytically active metals. The goal of these studies is to understand how incorporation of Osubinto the selvedge alters the surface structure and chemistry. The oxygen – Ag system, in particular, has been studied extensively both experimentally and theoretically because of its role in two important heterogeneously catalyzed industrial reactions: the epoxidation of ethylene to produce ethylene oxide and the partial oxidation of methanol to produce formaldehyde. In addition, the O/Rh and O/Ag systems serve as models for the dissociative chemisorption of diatomic molecules on close packed metal surfaces. Despite extensive research, there remain questions about the fundamental chemistry of the O/Ag system. Rh is also used in partial oxidation reactions, and its response to adsorbed oxygen provides an interesting complement to Ag. Where Ag extensively reconstructs, Rh does not. In particular, the structure of the catalytically active surface remains poorly understood under conditions of high oxygen coverages or subsurface oxygen. To improve our understanding of this system, we use ultra-high vacuum (UHV) surface science techniques to characterize Ag and Rh surfaces after exposure to atomic oxygen (AO) to obtain O coverages in excess of 1 ML. AO is generated by thermally cracking molecular O2. We then use low-energy electron diffraction (LEED) and UHV Scanning Tunneling Microscopy (UHV-STM) to further characterize the various oxygenaceous structures produced, and quantify the amount of oxygen with temperature programmed desorption (TPD). We have found that the surface temperature during deposition is an important factor for the formation of Osuband the consequent surface structures. Finally, we have recently found that Rh surfaces are significantly more reactive towards CO oxidation when Osub is present. This enhanced reactivity is located at the interface between the less reactive RhO2oxide and O-covered metallic Rh. These results reveal the conditions under which Osubis formed and stable, and show that Osubalso leads to enhanced reactivity of oxidized metal surfaces.