Ab initio molecular orbital calculations at the MP2/6-31G\*//MP2/6-31G\* + ZPE level have been performed in order to explore the reaction between CH 3 OH 2 + and CH 3 OH. The detailed mechanism of proton transfer, CH 3 OH 2 + + CH 3 OH ® CH 3 OH + CH 3 OH 2 + , and of cationic nucleophilic substitut
Proton-transfer reactions within ionized methanol clusters: Mass spectrometric and molecular orbital studies
✍ Scribed by Sun Young Lee; Dong Nam Shin; Soo Gyeong Cho; Kyung-Hoon Jung; Kwang Woo Jung
- Publisher
- John Wiley and Sons
- Year
- 1995
- Tongue
- English
- Weight
- 743 KB
- Volume
- 30
- Category
- Article
- ISSN
- 1076-5174
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✦ Synopsis
Abstract
Proton‐transfer reactions that proceed within methanol cluster ions were studied using an electron impact time‐of‐flight mass spectrometer. When CH~3~OH seeded in helium is expanded and ionized by electron impact, the protonated species, (CH~3~OH)~n~H^+^, are the predominant cluster ions in the low‐mass region. In CH~3~OD clusters, both (CH~3~OD)~n~H^+^ and (CH~3~OD)~n~D^+^ ions are observed. The ion abundance ratios, (CH~3~OD)~n~H^+^/(CH~3~OD)~n~D^+^, show a tendency to decrease as the methanol concentration increases, which is apparently related to the cluster structure and reaction energetics. The results suggest that the effective formation of (CH~3~OD)~n~H^+^ ions at low concentration of CH~3~OD in the expansion is the result of the relatively facile rotation of methanol molecules within the smaller clusters that tend to form at low CH~3~OD concentration. Ab initio molecular orbital calculations were carried out to investigate the rearrangement and dissociative pathways of ionized methanol dimer. Ion‐neutral complexes, [CH~3~OH~2~^+^…O(H)CH~2~] and [CH~3~OH~2~^+^…OCH~3~], are found to play an important role in the low‐energy pathways for production of CH~3~OH~2~^+^ + CH~2~OH (and OCH~3~) from ionized methanol dimer.
📜 SIMILAR VOLUMES
Cluster size distribution and collision-induced dissociation (CID) studies of protonated methanol and protonated methanol-water clusters yield information on the structure and energetics of such ions. Ions were formed at atmospheric pressure in a corona discharge source, and were subjected to CID in