Back to Search Start Over

Dissociative recombination of protonated methanol

Authors :
H. Roberts
Tom J. Millar
Vitali Zhaunerchyk
Anders Källberg
M. Kaminska
Jacek Semaniak
Fredrik Hellberg
M. Larsson
Wolf D. Geppert
F. Österdahl
Richard D. Thomas
M. af Ugglas
Ansgar Simonsson
Mathias Hamberg
Anneli Ehlerding
Source :
Faraday Discuss.. 133:177-190
Publication Year :
2006
Publisher :
Royal Society of Chemistry (RSC), 2006.

Abstract

The branching ratios of the different reaction pathways and the overall rate coefficients of the dissociative recombination reactions of CH3OH2+ and CD3OD2+ have been measured at the CRYRING storage ring located in Stockholm, Sweden. Analysis of the data yielded the result that formation of methanol or deuterated methanol accounted for only 3 and 6% of the total rate in CH3OH2+ and CD3OD2+, respectively. Dissociative recombination of both isotopomeres mainly involves fragmentation of the C-O bond, the major process being the three-body break-up forming CH3, OH and H (CD3, OD and D). The overall cross sections are best fitted by sigma = 1.2 +/- 0.1 x 10(-15) E(-1.15 +/- 0.02) cm2 and sigma = 9.6 +/- 0.9 x 10(-16) E(-1.20 +/- 0.02) cm2 for CH3OH2+ and CD3OD2+, respectively. From these values thermal reaction rate coefficients of k(T) = 8.9 +/- 0.9 x 10(-7) (T/300)(-0.59 +/- 0.02) cm3 s(-1) (CH3OH2+) and k(T) = 9.1 +/- 0.9 x 10(-7) (T/300)(-0.63 +/- 0.02) cm3 s(-1) (CD3OD2+) can be calculated. A non-negligible formation of interstellar methanol by the previously proposed mechanism via radiative association of CH3+ and H2O and subsequent dissociative recombination of the resulting CH3OH2+ ion to yield methanol and hydrogen atoms is therefore very unlikely.

Details

ISSN :
13645498 and 13596640
Volume :
133
Database :
OpenAIRE
Journal :
Faraday Discuss.
Accession number :
edsair.doi.dedup.....ca116efe6e2aa8e8f20f80906c571139
Full Text :
https://doi.org/10.1039/b516010c