The x-ray absorption spectrum of the propargyl radical C3H3●

We report a combined experimental and computational study of the near-edge X-ray absorption fine structure (NEXAFS) spectrum of the propargyl radical, C3H3●. As a central intermediate in the formation of polycyclic aromatic hydrocarbons, the propargyl radical is a species of considerable relevance in combustion and astrochemistry and was here generated by pyrolysis from propargyl bromide. The NEXAFS spectrum shows a pronounced band at 282.2 eV corresponding to transitions from carbon 1s orbitals to singly occupied molecular orbitals. Ab initio calculations reveal that two transitions to the lowest-lying states 1 A12 and 2 A12, which take place from the C1s orbital of the two terminal carbon atoms, contribute to this band. In addition, a 420 meV spacing of the first band is visible and is assigned to a vibrational progression in the symmetric CH2 stretch. Transitions at higher energies are also described reasonably well by theory. The fragmentation pattern was investigated at the different resonant transitions and shows the cleavage of one as well as both C-C bonds.

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Journal
The Journal of Chemical Physics
Published
2026-06-26
DOI
https://doi.org/10.1063/5.0328356
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
0.00

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article

The x-ray absorption spectrum of the propargyl radical C3H3●

Michele Alagia, Emil Karaev, Theo Juncker von Buchwald, Ingo Fischer et al.
The Journal of Chemical Physics
Astrophysics and Star Formation Studies
article

The x-ray absorption spectrum of the propargyl radical C3H3●

Michele Alagia, Emil Karaev, Theo Juncker von Buchwald, Ingo Fischer, Stefano Stranges, Sonia Coriani, Dorothee Schaffner, Jacob Pedersen, Valentin Laffert, Andreas Rasp, Alessio Bruno
article en

Abstract

We report a combined experimental and computational study of the near-edge X-ray absorption fine structure (NEXAFS) spectrum of the propargyl radical, C3H3●. As a central intermediate in the formation of polycyclic aromatic hydrocarbons, the propargyl radical is a species of considerable relevance in combustion and astrochemistry and was here generated by pyrolysis from propargyl bromide. The NEXAFS spectrum shows a pronounced band at 282.2 eV corresponding to transitions from carbon 1s orbitals to singly occupied molecular orbitals. Ab initio calculations reveal that two transitions to the lowest-lying states 1 A12 and 2 A12, which take place from the C1s orbital of the two terminal carbon atoms, contribute to this band. In addition, a 420 meV spacing of the first band is visible and is assigned to a vibrational progression in the symmetric CH2 stretch. Transitions at higher energies are also described reasonably well by theory. The fragmentation pattern was investigated at the different resonant transitions and shows the cleavage of one as well as both C-C bonds.

The Journal of Chemical PhysicsVol. 164(24)
Norwegian University of Science and Technology (NO), University of Würzburg (DE), Istituto Officina dei Materiali (IT), Sapienza University of Rome (IT), Technical University of Denmark (DK)
Fonds der Chemischen Industrie, Deutsche Forschungsgemeinschaft, Danmarks Tekniske Universitet, Novo Nordisk Fonden, Hamburg Centre for Ultrafast Imaging
Openalex Percentile: Top 7%
Astrophysics and Star Formation Studies
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