H<sub>2</sub> roaming chemistry and the formation of H<sub>3</sub><sup>+</sup> from organic molecules in strong laser fields.
basic_science · Level V
Where this comes from
- Record sourced from PubMed, PMID 30518927.
- Also identified by DOI 10.1038/s41467-018-07577-0 and PMC identifier 6281587.
- Licence recorded as CC BY.
- The licence permits redistribution, so the abstract is shown in full and the full text is available from the publisher.
Abstract
Roaming mechanisms, involving the brief generation of a neutral atom or molecule that stays in the vicinity before reacting with the remaining atoms of the precursor, are providing valuable insights into previously unexplained chemical reactions. Here, the mechanistic details and femtosecond time-resolved dynamics of H<sub>3</sub><sup>+</sup> formation from a series of alcohols with varying primary carbon chain lengths are obtained through a combination of strong-field laser excitation studies and ab initio molecular dynamics calculations. For small alcohols, four distinct pathways involving hydrogen migration and H<sub>2</sub> roaming prior to H<sub>3</sub><sup>+</sup> formation are uncovered. Despite the increased number of hydrogens and possible combinations leading to H<sub>3</sub><sup>+</sup> formation, the yield decreases as the carbon chain length increases. The fundamental mechanistic findings presented here explore the formation of H<sub>3</sub><sup>+</sup>, the most important ion in interstellar chemistry, through H<sub>2</sub> roaming occurring in ionic species.