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.

Paparazzo, E., Fanfoni, M., Severini, E., Priori, S. (1992). Evidence of SI-OH soecies at the surface of aged silica. In JOURNAL OF VACUUM SCIENCE & TECHNOLOGY A-VACUUM SURFACES AND FILMS (pp.2892-2896). WOODBURY : AMER INST PHYSICS.

Evidence of SI-OH soecies at the surface of aged silica

FANFONI, MASSIMO;
1992-01-01

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.
38TH NATIONAL SYMP OF THE AMERICAN VACUUM SOCIETY
SEATTLE, WA
NOV 11-15, 1991
AMER VACUUM SOCIETY
Rilevanza internazionale
contributo
1992
Settore FIS/03 - FISICA DELLA MATERIA
English
X-RAY PHOTOELECTRON; ELECTRON-SPECTROSCOPY; XPS; SENSITIVITY; NICKEL
Intervento a convegno
Paparazzo, E., Fanfoni, M., Severini, E., Priori, S. (1992). Evidence of SI-OH soecies at the surface of aged silica. In JOURNAL OF VACUUM SCIENCE & TECHNOLOGY A-VACUUM SURFACES AND FILMS (pp.2892-2896). WOODBURY : AMER INST PHYSICS.
Paparazzo, E; Fanfoni, M; Severini, E; Priori, S
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/45848
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