Issue |
EAS Publications Series
Volume 46, 2011
PAHs and the Universe: A Symposium to Celebrate the 25th Anniversary of the PAH Hypothesis
|
|
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Page(s) | 241 - 249 | |
DOI | https://doi.org/10.1051/eas/1146026 | |
Published online | 30 March 2011 |
C. Joblin and A.G.G.M. Tielens (eds)
EAS Publications Series, 46 (2011) 241-249
Experimental studies of the dissociative recombination processes for the C6D6+ and C6D7+ ions
1 Department of Physics, Stockholm
University, SE-106
91
Stockholm,
Sweden ;
e-mail: mathias.hamberg@physto.se
2
Radboud University Nijmegen, Institute for Molecules and
Materials, PO Box
9010, 6500 GL
Nijmegen, The
Netherlands
3
Institute of Modern Physics, Chinese Academy of
Sciences, 509 Nanchang
Rd., Lanzhou
730000,
China
4
Department of Physics, Albert-Ludwigs Universität
Freiburg, Hermann-Herder-Str.
3, 79104
Freiburg,
Germany
5
Jan Kochanowski University, Świȩtokrzyska 15, 25406
Kielce,
Poland
6
Manne Siegbahn Laboratory, Frescativägen 26, 114 18
Stockholm,
Sweden
We have investigated the dissociative recombination (DR) of the C6D6+ and C6D7+ ions using the CRYRING heavy-ion storage ring at Stockholm University, Sweden. The dissociative recombination branching ratios were determined at minimal collision energy, showing that the DR of both ions was dominated by pathways keeping the carbon atoms together in one product. The absolute reaction cross sections for the titular ions are best fitted by σ(Ecm [eV]) = 1.3 ± 0.4 × 10-15 (Ecm [eV])−1.19 ± 0.02 cm2 (C6D6+) and σ(Ecm [eV]) = 1.1 ± 0.3 × 10-15(Ecm [eV])−1.33 ± 0.02 cm2 (C6D7+) in the intervals 3-300 meV and 3-200 meV respectively. The thermal rate constants of the titular reactions are best described by: k(T) = 1.3 ± 0.4 × 10-6(T/300)−0.69 ± 0.02 cm3s-1 for C6D6+ and k(T) = 2.0 ± 0.6 × 10-6 (T/300)−0.83 ± 0.02 cm3s-1 for C6D7+. These expressions correlates well with earlier flowing afterglow studies on the same process.
© EAS, EDP Sciences 2011