Author
Listed:
- Jacob Stamm
(Michigan State University)
- Swati S. Priyadarsini
(Michigan State University)
- Shawn Sandhu
(Michigan State University)
- Arnab Chakraborty
(Michigan State University)
- Jun Shen
(Michigan State University)
- Sung Kwon
(Michigan State University)
- Jesse Sandhu
(Michigan State University)
- Clayton Wicka
(Michigan State University)
- Arshad Mehmood
(Stony Brook University
Stony Brook University)
- Benjamin G. Levine
(Stony Brook University
Stony Brook University)
- Piotr Piecuch
(Michigan State University
Michigan State University)
- Marcos Dantus
(Michigan State University
Michigan State University)
Abstract
The formation of $${\rm H}_{3}^{+}$$ H 3 + following the double ionization of small organic compounds via a roaming mechanism, which involves the generation of H2 and subsequent proton abstraction, has recently garnered significant attention. Nonetheless, a cohesive model explaining trends in the yield of $${\rm H}_{3}^{+}$$ H 3 + characterizing these unimolecular reactions is yet to be established. We report yield and femtosecond time-resolved measurements following the strong-field double ionization of CH3X molecules, where X = OD, Cl, NCS, CN, SCN, and I. These measurements, combined with double-ionization-potential equation-of-motion coupled-cluster ab initio calculations used to determine the geometries and energetics of CH3X2+ dications, are employed to identify the key factors governing the formation of $${\rm H}_{3}^{+}$$ H 3 + in certain doubly ionized CH3X species and its absence in others. We also carry out ab initio molecular dynamics simulations to obtain detailed microscopic insights into the mechanism, yields, and timescales of $${\rm H}_{3}^{+}$$ H 3 + production. We find that the excess relaxation energy released after double ionization of CH3X molecules combined with substantial geometrical distortion that favors H2 formation prior to proton abstraction boost the generation of $${\rm H}_{3}^{+}$$ H 3 + . Our study provides useful guidelines for examining alternative sources of $${\rm H}_{3}^{+}$$ H 3 + in the universe.
Suggested Citation
Jacob Stamm & Swati S. Priyadarsini & Shawn Sandhu & Arnab Chakraborty & Jun Shen & Sung Kwon & Jesse Sandhu & Clayton Wicka & Arshad Mehmood & Benjamin G. Levine & Piotr Piecuch & Marcos Dantus, 2025.
"Factors governing $${\rm H}_{3}^{+}$$ H 3 + formation from methyl halogens and pseudohalogens,"
Nature Communications, Nature, vol. 16(1), pages 1-14, December.
Handle:
RePEc:nat:natcom:v:16:y:2025:i:1:d:10.1038_s41467-024-55065-5
DOI: 10.1038/s41467-024-55065-5
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