Ph.D. Thesis: Dissociative Recombination of Astrochemically Interesting Ions
by
Mathias Hamberg(Stockholm University, Department of Physics)
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Europe/Stockholm
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Description
In this thesis the major work described concerns experimental determination of the dissociative
recombination (DR) reaction for several molecular ions of astrochemical interest. DR is the process
where an electron recombines with a molecular ion to form an excited neutral that disintegrates into
two or more neutral fragments to release the gained excess energy. It is very efficient under cold
conditions and therefore ubiquitously occurring in interstellar environments such as dark clouds
and plays an important role in aeronomical plasmae, lightnings and in man-made plasmas such as
in combustion engines and fusion reactors. Although DR reactions are crucial processes in all these
environments, product branching fractions of DR reactions have proven to be very unpredictable
and present one of the great remaining challenges for theoreticians. The experimental work includes
determination of reaction rates and product distribution of DR of complex ions such as protonated
alcohols and ethers. The following species have been investigated and are discussed in this thesis:
CH3OH2+ (protonated methanol), CD3OD2+ (deuteronated methanol), CD3OCD2+ (methoxymethyl cation), CD3CDOD+ (deuteronated acetaldehyde), CH3CH2OH2+ (protonated
ethanol) and (CD3)2OD+ (deuteronated dimethyl ether).
The results of these measurements are used in astrochemical model calculations in which therates used hitherto greatly have been based on educated guesses. Employing the outcome of the
DR investigations of the CH3OH2
+ and CD3OD2
+ ions have shown a great impact on such models.
The DR investigations have been followed up by astronomical observations. Theoretical models
and laboratory experiments show that methanol should be formed from CO on cold grains. This
scenario was tested by astronomical observations of gas associated with young stellar objects
(YSOs). Two independent tests were showing consistency with methanol formation on grain
surfaces.