The Hidden Path to the Resonance-Stabilized Fulvenallenyl Radical (C <sub>7</sub> H <sub>5</sub> ) via the Bimolecular Reaction of Tricarbon (C <sub>3</sub> , X <sup>1</sup> Σ <sub>g</sub> <sup>+</sup> ) with 1,3-Butadiene (C <sub>4</sub> H <sub>6</s

We report a novel bimolecular reaction pathway forming the resonance-stabilized fulvenallenyl radical (C<sub>7</sub>H<sub>5</sub>) <i>via</i> the gas-phase reaction of tricarbon (C<sub>3</sub>, X<sup>1</sup>Σg<sup>+</sup>) with 1,3-butadiene (C<sub>4</sub>H<sub>6</sub>, X<sup>1</sup>A<sub>g</sub>). Crossed molecular beam experiments combined with high-level electronic structures and statistical calculations reveal a rich potential energy surface. The reaction proceeds <i>via</i> tricarbon addition to a double bond of 1,3-butadiene, overcoming a 30 kJ mol<sup>-1</sup> barrier, followed by ring closure, isomerizations (ring opening/closures, hydrogen shifts), and eventual hydrogen atom loss, yielding the fulvenallenyl radical (<b>p1</b>) almost exclusively via two dominant pathways. Considering the entrance barrier, this reaction may occur in high-temperature environments, like circumstellar envelopes of carbon stars, but is suppressed in colder regions such as molecular clouds and Titan's atmosphere. These findings highlight the unexpected reactivity of small carbon clusters in shaping the molecular complexity of our universe, from the flicker of a flame to the death of a star.

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Journal
The Journal of Physical Chemistry Letters
Published
2026-01-29
DOI
https://doi.org/10.1021/acs.jpclett.5c03004
Primary Topic
Astrophysics and Star Formation Studies
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article
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article

The Hidden Path to the Resonance-Stabilized Fulvenallenyl Radical (C 7 H 5 ) via the Bimolecular Reaction of Tricarbon (C 3 , X 1 Σ g + ) with 1,3-Butadiene (C 4 H 6</s

Anatoliy A. Nikolayev, Shane J. Goettl, Iakov A. Medvedkov, A. M. Mebel et al.
The Journal of Physical Chemistry Letters
Astrophysics and Star Formation Studies
article

The Hidden Path to the Resonance-Stabilized Fulvenallenyl Radical (C 7 H 5 ) via the Bimolecular Reaction of Tricarbon (C 3 , X 1 Σ g + ) with 1,3-Butadiene (C 4 H 6</s

Anatoliy A. Nikolayev, Shane J. Goettl, Iakov A. Medvedkov, A. M. Mebel, Ralf I. Kaiser
article en

Abstract

We report a novel bimolecular reaction pathway forming the resonance-stabilized fulvenallenyl radical (C<sub>7</sub>H<sub>5</sub>) <i>via</i> the gas-phase reaction of tricarbon (C<sub>3</sub>, X<sup>1</sup>Σg<sup>+</sup>) with 1,3-butadiene (C<sub>4</sub>H<sub>6</sub>, X<sup>1</sup>A<sub>g</sub>). Crossed molecular beam experiments combined with high-level electronic structures and statistical calculations reveal a rich potential energy surface. The reaction proceeds <i>via</i> tricarbon addition to a double bond of 1,3-butadiene, overcoming a 30 kJ mol<sup>-1</sup> barrier, followed by ring closure, isomerizations (ring opening/closures, hydrogen shifts), and eventual hydrogen atom loss, yielding the fulvenallenyl radical (<b>p1</b>) almost exclusively via two dominant pathways. Considering the entrance barrier, this reaction may occur in high-temperature environments, like circumstellar envelopes of carbon stars, but is suppressed in colder regions such as molecular clouds and Titan's atmosphere. These findings highlight the unexpected reactivity of small carbon clusters in shaping the molecular complexity of our universe, from the flicker of a flame to the death of a star.

The Journal of Physical Chemistry LettersVol. 17(10)
University of Hawaiʻi at Mānoa (US), Florida International University (US), Samara National Research University (RU)
Openalex Percentile: Top 71%
Astrophysics and Star Formation Studies
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