Comparative study of water and carbon dioxide adsorption on CuFeO$_{\mathrm{2}}$ and CuFe$_{\mathrm{1-x}}$Ga$_{\mathrm{x}}$O$_{\mathrm{2\thinspace }}$highly epitaxial thin films

ORAL

Abstract

Thermal programmed desorption (TPD) of CO$_{\mathrm{2}}$ and H$_{\mathrm{2}}$O from a 200 nm thick CuFeO$_{\mathrm{2}}$ and 52 nm thick CuFe$_{\mathrm{1-x}}$Ga$_{\mathrm{x}}$O$_{\mathrm{2\thinspace }}$delafossite surfaces was performed in a Ultra-high vacuum (UHV) chamber. The thin films with epitaxial quality were grown by Pulsed Laser Deposition (PLD) on Al$_{\mathrm{2}}$O$_{\mathrm{3}}$ (0001) substrates . The adsorption / desorption of CO2 and H2O process was also monitored with X-ray Photoelectron Spectroscopy (XPS) and Auger Electron Spectroscopy (AES). Our results revealed that carbon dioxide is preferentially chemisorbed by CuFe$_{\mathrm{1-x}}$Ga$_{\mathrm{x}}$O$_{\mathrm{2}}$ over water and we observed the opposite behavior with regard to chemisorption of CO$_{\mathrm{2}}$ and H$_{\mathrm{2}}$O over CuFeO$_{\mathrm{2}}$. Hydroxyls and metal carbonates were formed on the surface due to the chemisorption of H$_{\mathrm{2}}$O and CO$_{\mathrm{2}}$. Arrhenius plots for CO$_{\mathrm{2}}$ and H$_{\mathrm{2}}$O desorption were done and activation energy for desorption were obtained.

Authors

  • S. Rojas

    Instituto de Fisica, Pontificia Universidad Catolica de Chile

  • T. Joshi

    West Virginia University, Morgantown, WV, Department of Physics and Astronomy, West Virginia University, Morgantown

  • P. Borisov

    West Virginia University, Morgantown, WV, Department of Physics and Astronomy, West Virginia University, Morgantown

  • D. Lederman

    Department of Physics and Astronomy,West Virginia University,Department of Physics,University of California,Santa Cruz,95064, West Virginia University; University of California, Santa Cruz, West Virginia University, Morgantown, WV, University of California, Santa Cruz, CA, West Virginia Univ, University of California Santa Cruz, West Virginia University, Department of Physics and Astronomy, West Virginia University, Morgantown

  • A. L. Cabrera

    Instituto de Fisica, Pontificia Universidad Catolica de Chile