1. Symmetry-resolved CO desorption and oxidation dynamics on O/Ru(0001) probed at the C K-edge by ultrafast x-ray spectroscopy
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Jerry LaRue, Boyang Liu, Gabriel L. S. Rodrigues, Chang Liu, Jose Antonio Garrido Torres, Simon Schreck, Elias Diesen, Matthew Weston, Hirohito Ogasawara, Fivos Perakis, Martina Dell’Angela, Flavio Capotondi, Devon Ball, Conner Carnahan, Gary Zeri, Luca Giannessi, Emanuele Pedersoli, Denys Naumenko, Peter Amann, Ivaylo Nikolov, Lorenzo Raimondi, Carlo Spezzani, Martin Beye, Johannes Voss, Hsin-Yi Wang, Filippo Cavalca, Jörgen Gladh, Sergey Koroidov, Frank Abild-Pedersen, Manuel Kolb, Piter S. Miedema, Roberto Costantini, Tony F. Heinz, Alan C. Luntz, Lars G. M. Pettersson, and Anders Nilsson
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General Physics and Astronomy ,ddc:530 ,Physical and Theoretical Chemistry - Abstract
The journal of chemical physics 157(16), 164705 (2022). doi:10.1063/5.0114399, We report on carbon monoxide desorption and oxidation induced by 400 nm femtosecond laser excitation on the O/Ru(0001) surface probed by time-resolved x-ray absorption spectroscopy (TR-XAS) at the carbon K-edge. The experiments were performed under constant background pressures of CO (6 × 10$^{−8}$ Torr) and O$_2$ (3 × 10$^{−8}$ Torr). Under these conditions, we detect two transient CO species with narrow 2$π^*$ peaks, suggesting little 2π* interaction with the surface. Based on polarization measurements, we find that these two species have opposing orientations: (1) CO favoring a more perpendicular orientation and (2) CO favoring a more parallel orientation with respect to the surface. We also directly detect gas-phase CO2 using a mass spectrometer and observe weak signatures of bent adsorbed CO2 at slightly higher x-ray energies than the 2$π^*$ region. These results are compared to previously reported TR-XAS results at the O K-edge, where the CO background pressure was three times lower (2 × 10$^{−8}$ Torr) while maintaining the same O$_2$ pressure. At the lower CO pressure, in the CO 2$π^*$ region, we observed adsorbed CO and a distribution of OC–O bond lengths close to the CO oxidation transition state, with little indication of gas-like CO. The shift toward “gas-like” CO species may be explained by the higher CO exposure, which blocks O adsorption, decreasing O coverage and increasing CO coverage. These effects decrease the CO desorption barrier through dipole–dipole interaction while simultaneously increasing the CO oxidation barrier., Published by American Institute of Physics, Melville, NY
- Published
- 2022
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