1988
DOI: 10.1016/0368-2048(88)85005-9
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Fluorination effects on the inner-shell spectra of unsaturated molecules

Abstract: The applicability of the perfluoro effect to the X-ray spectra (300-800 eV) of unsaturated organic molecules is explored. The Cls and Fls (and 01s where appropriate) oscillator strength spectra of five fluoroethylenes, octafluorocyclopentene, formyl fluoride, carbonyl fluoride, hexafluorobutadiene, trifluoroacetic acid, heduorobutyne-2, hexafluoroacetone, and octatluoronaphthalene were derived from electron impact energy loss spectra recorded under electric-dipole scattering conditions. These spectra are analy… Show more

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Cited by 133 publications
(110 citation statements)
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“…This small excess could be associated with the high stabilization of COOH + due to charge resonance (charge migration) (Silverstein & Webster 1998) or a possible dissociation of CH + 3 into minor fragments. Other possibility is that the methyl carbon IP occurs at 291.6, 5 eV less than for the carboxyl carbon (see Robin et al 1988). As a consequence, the number of resonances to excited orbitals involving the carbon atom in the COOH site is higher than for the other carbon site at photon energies above the IP of the methyl carbon.…”
Section: Photodissociation and Formation Pathwaysmentioning
confidence: 99%
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“…This small excess could be associated with the high stabilization of COOH + due to charge resonance (charge migration) (Silverstein & Webster 1998) or a possible dissociation of CH + 3 into minor fragments. Other possibility is that the methyl carbon IP occurs at 291.6, 5 eV less than for the carboxyl carbon (see Robin et al 1988). As a consequence, the number of resonances to excited orbitals involving the carbon atom in the COOH site is higher than for the other carbon site at photon energies above the IP of the methyl carbon.…”
Section: Photodissociation and Formation Pathwaysmentioning
confidence: 99%
“…Figure 2 shows the mass spectrum of acetic acid obtained at photon energy of 288.3 eV. The C1s → π * resonance energy from C = O bond is 288.6 eV (Robin et al 1988). We can see the methyl fragment group (mass from 12 to 15 a.m.u), the C 2 group (24 to 27 a.m.u), the HCO group (28 to 31 a.m.u) and the CCO group (40 to 44 a.m.u).…”
Section: Methodsmentioning
confidence: 99%
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“…To further investigate the structural transformations and surface reactions occurring on a-C:H:Si:O upon sliding under different environmental conditions, imaging near edge X-ray absorption fine structure spectroscopy (NEXAFS) measurements, which are highly surface sensitive (for electron yield NEXAFS spectroscopy of low atomic number elements, the information depth, which is the specimen thickness measured normal to the surface from which a specified percentage of typically 95% of the detected signal originates, is usually less shows characteristic absorption features at 285.0±0.1 eV (due to the C1s→π * transition for disordered carbon-carbon bonds), ~286.5 eV (due to the C1s→π * transition for carbonyl groups), 287.5±0.1 eV (assigned to the C1s→σ * transition for carbon-hydrogen bonds), and 288.9±0.1 eV (assigned to the C1s→σ * transition for carbon-oxygen and carbon-silicon bonds, as well as to the C1s→π * transition for carboxyl groups) 25,26 . These assignments are summarized in Table 1.…”
Section: Friction Measurementsmentioning
confidence: 99%