Ionic Fragmentation Mechanisms of 2,2,2-Trifluoroethanol Following Excitation with Synchrotron Radiation

Gaseous 2,2,2‐trifluoroethanol (TFE) is excited with synchrotron radiation between 10 and 1000 eV and the ejected electrons and positive ions are detected in coincidence. In the valence‐electron energy region, the most abundant species is CH2OH+. Other fragments, including ions produced by atomic re...

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Published inChemphyschem Vol. 16; no. 2; pp. 322 - 330
Main Authors Bava, Yanina B., Berrueta Martínez, Yanina, Moreno Betancourt, Angélica, Erben, Mauricio F., Cavasso Filho, Reinaldo L., Della Védova, Carlos O., Romano, Rosana M.
Format Journal Article
LanguageEnglish
Published Weinheim WILEY-VCH Verlag 02.02.2015
WILEY‐VCH Verlag
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Summary:Gaseous 2,2,2‐trifluoroethanol (TFE) is excited with synchrotron radiation between 10 and 1000 eV and the ejected electrons and positive ions are detected in coincidence. In the valence‐electron energy region, the most abundant species is CH2OH+. Other fragments, including ions produced by atomic rearrangements, are also detected; the most abundant are COH+, CFH2+ and CF2H2+. The energies of electronic transitions from C 1 s, O 1 s and F 1 s orbitals to vacant molecular orbitals are determined. A site‐specific C 1 s excitation is observed. The photofragmentation mechanisms after the excitation of core‐shell electrons are inferred from analysis of the shape and slope of the coincidence between two charged fragments in the bi‐dimensional coincidence spectra. The spectra are dominated by islands that correspond to the coincidence of H+ with several charged fragments. One of the most important channels leads to the formation of CH2OH+ and CF3+ in a concerted mechanism. Breaking it down: The most important photofragmentation channel of gaseous 2,2,2‐trifluoroethanol (TFE) after photoionization in the valence‐electron energy region results in CH2OH+ and CF3. (see figure). After core‐shell electron excitations, several fragmentation mechanisms involving two positive ions are observed, the most abundant of which produce H+.
Bibliography:istex:D1EB4B1264FF17409FEAC2AB3FF8BF225E21F8BB
Universidad Nacional de La Plata, República Argentina
Consejo Nacional de Investigaciones Científicas y Técnicas
ArticleID:CPHC201402669
Comisión de Investigaciones Científicas de la Provincia de Buenos Aires
Brazilian Synchrotron Light Source - No. SGM-11670; No. SGM-15206; No. TGM-15163
Agencia Nacional de Promoción Científica y Tecnológica
ark:/67375/WNG-NPX63TGQ-W
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:1439-4235
1439-7641
DOI:10.1002/cphc.201402669