Synchrotron radiation (SR) photoemission and x-ray photoelectron spectroscopy (XPS) are used to reveal the presence of Si-OH species at the surface of aged silica. SR Si 2p spectra, recorded in the photon energy range 130 eV less-than-or-equal-to hv less-than-or-equal-to 240 eV, show the coexistence of Si-O bonding states and Si-OH bonding states, the latter being marked by a component at 105.2 eV in binding energy. The intensity ratio I[Si-OH]/I[Si-O] varies monotonically from 0.24 to 0.77 with increasing photoelectron kinetic energy from 15 to 135 eV, respectively. On the contrary, no sign of silanol groups is evident in the XPS spectra, although some excess oxygen is measured in the nO/nSi atomic ratios. Combination of SR and XPS results suggest that the silanol groups lie in a region which extends approximately 16 to 21 angstrom from the surface, whereas the composition of the material is virtually that of silica for depths greater-than-or-equal-to 30 angstrom. Possible sources of uncertainty in the analysis of Si-OH species in silica are discussed.

EVIDENCE OF SI-OH SPECIES AT THE SURFACE OF AGED SILICA

PAPARAZZO E;PRIORI S
1992

Abstract

Synchrotron radiation (SR) photoemission and x-ray photoelectron spectroscopy (XPS) are used to reveal the presence of Si-OH species at the surface of aged silica. SR Si 2p spectra, recorded in the photon energy range 130 eV less-than-or-equal-to hv less-than-or-equal-to 240 eV, show the coexistence of Si-O bonding states and Si-OH bonding states, the latter being marked by a component at 105.2 eV in binding energy. The intensity ratio I[Si-OH]/I[Si-O] varies monotonically from 0.24 to 0.77 with increasing photoelectron kinetic energy from 15 to 135 eV, respectively. On the contrary, no sign of silanol groups is evident in the XPS spectra, although some excess oxygen is measured in the nO/nSi atomic ratios. Combination of SR and XPS results suggest that the silanol groups lie in a region which extends approximately 16 to 21 angstrom from the surface, whereas the composition of the material is virtually that of silica for depths greater-than-or-equal-to 30 angstrom. Possible sources of uncertainty in the analysis of Si-OH species in silica are discussed.
1992
Synchrotron radiation photoemission
XPS
silica
surface hydration
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/406471
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