AI Article Synopsis

  • Trifluoroacetyl chloride (CFCOCl) is produced in the atmosphere from the breakdown of hydrochlorofluorocarbons and can generate reactive halogen radicals.
  • This study investigates how CFCOCl molecules and their clusters react when exposed to electron ionization and attachment using a combination of experiments and quantum chemical calculations.
  • The findings reveal that ionization leads to significant fragmentation, with specific bond dissociations producing various ions, and that electron attachment causes different reactions depending on the energy levels, which could have implications for atmospheric chemistry.

Article Abstract

Trifluoroacetyl chloride, CFCOCl, is produced in the Earth's atmosphere by photooxidative degradation of hydrochlorofluorocarbons, and represents a potential source of highly reactive halogen radicals. Despite considerable insight into photochemistry of CFCOCl, its reactivity towards electrons has not been addressed so far. We investigate the electron ionization and attachment in isolated CFCOCl molecules and (CFCOCl), max. ≥ 10, clusters using a molecular beam experiment in combination with quantum chemical calculations. The ionization of the molecule at 70 eV electron energy leads to strong fragmentation: weakening of the C-C bond yields the CF and COCl ions, while the fission of the C-Cl bond produces the major CFCO fragment ion. The cluster spectra are dominated by M·COCl and M·CFCO ions (M = CFCOCl). The electron attachment at energies between 1.5 and 11 eV also leads to the dissociation of the molecule breaking either the C-Cl bond at low energies below 3 eV yielding mainly Cl ions, or dissociating the C-C bond at higher energies above 4 eV leading mainly to CF ions. In the clusters, the intact M ions are stabilized after electron attachment at low energies with contribution of M·Cl fragment ions. At higher energies, the M·Cl fragments dominate the spectra, and C-C bond dissociation occurs as well yielding M·CF. Interestingly, M·Cl ions appear in the spectra at higher energies. We briefly discuss possible atmospheric implications.

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Source
http://dx.doi.org/10.1039/d3cp05387cDOI Listing

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