Journal of the Chemical Society Faraday Transactions 2 Molecular and Chemical Physics · 1976 · 94 citations · 0 references
Natural SciencesChemistryMaterials ScienceInorganic ChemistrySpectroscopySurface ScienceCarbon MonoxideInorganic SpectroscopyMetal OxidesPhotochemistryReactive Oxygen SpeciesCarbon Monoxide PhotochemistryHyperfine Selection RulesHyperfine SpectroscopyParamagnetic CentersParamagnetic ComplexesParamagnetic SpeciesTitanium Oxides
Oxygen absorbed on TiO2 when subjected to u.v. irradiation gives rise to three different paramagnetic species. The first species, A, has been identified as O–2(g1= 2.021, g2= 2.009 and g3= 2.001 and C1≈C2≈ 0 Oe, C3= 77 Oe for 17O hyperfine spliting), the second species, C, as O–3(g1= 2.014, g2= 2.009 and g3= 2.003, no detected hyperfine lines due to 17O) and the third, B, as O3–3(g∥= 2.008 and g⊥= 2.001, no detectable hyperfine lines due to 17O). The latter species reacts readily with CO at 77 K and gives rise to species D, identified as OI–OII–CO–III according to the reaction: O3–3+ CO → O2–latt.+ O—O—CO– where the two directly bonded oxygen atoms originate from the absorbed molecular oxygen. The e.p.r. parameters of species D are : g1= 2.0465, g2= 2.006, g3= 2.001, C1≃ 6 Oe ± 0.5C2≈C3≈ 4 Oe ± 0.5 for 13C hyperfine interaction, CI1≈CI2≈ 0 and CI3= 104 Oe, CII1C≈II2 0 and CII3≃ 42.5 Oe and CIII1≈CIII2≈CIII3≈ 0 for 17O hyperfine splitting constants of the three oxygen nuclei. It is mainly the characterization of species, D, which enables us to postulate the nature of species, B.