Abstract
We report experimental as well as theoretical evidence that suggests Au-CO complex formation upon the exposure of CO to active sites (step edges and threading dislocations) on a Au(111) surface. Room-temperature scanning tunneling microscopy (STM), X-ray photoelectron spectroscopy, transmission infrared spectroscopy, and density functional theory calculations point to Au-CO complex formation and migration. Room-temperature STM of the Au(111) surface at CO pressures in the range from 10-8 to 10-4 Torr (dosage up to 106 langmuir) indicates Au atom extraction from dislocation sites of the herringbone reconstruction, mobile Au-CO complex formation and diffusion, and Au adatom cluster formation on both elbows and step edges on the Au surface. The formation and mobility of the Au-CO complex result from the reduced Au-Au bonding at elbows and step edges leading to stronger Au-CO bonding and to the formation of a more positively charged CO (COδ+) on Au. Our studies indicate that the mobile Au-CO complex is involved in the Au nanoparticle formation and reactivity, and that the positive charge on CO increases due to the stronger adsorption of CO at Au sites with lower coordination numbers.
Original language | English |
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Pages (from-to) | 1518-1526 |
Number of pages | 9 |
Journal | Journal of the American Chemical Society |
Volume | 138 |
Issue number | 5 |
DOIs | |
State | Published - Feb 17 2016 |
Funding
STM measurements were conducted at the Center for Nanophase Materials Sciences (CNMS), which is a DOE Office of Science User Facility. We thank the DOE-Office of Basic Energy Sciences under grant number DE-FGOZ-09ER16080 for partial support of this research. This work was also partially supported by the Fluid Interface Reactions, Structures and Transport (FIRST) Center, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Science. We also thank AES Corp. for the AES Graduate Fellowship in Energy Research Program at the University of Virginia for Monica McEntee. We also gratefully thank the XSEDE computing resources from the Texas Advanced Computing Center and the San Diego Supercomputer Center for all of the DFT calculations.