The X-ray absorption spectrum of the propargyl radical, C$_3$H$_3^{\cdot}$

Fuente: arXiv
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Autores principales: Schaffner, Dorothee, von Buchwald, Theo Juncker, Pedersen, Jacob, Rasp, Andreas, Karaev, Emil, von Laffert, Valentin, Bruno, Alessio, Alagia, Michele, Stranges, Stefano, Fischer, Ingo, Coriani, Sonia
Formato: Preprint
Publicado: 2026
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author Schaffner, Dorothee
von Buchwald, Theo Juncker
Pedersen, Jacob
Rasp, Andreas
Karaev, Emil
von Laffert, Valentin
Bruno, Alessio
Alagia, Michele
Stranges, Stefano
Fischer, Ingo
Coriani, Sonia
author_facet Schaffner, Dorothee
von Buchwald, Theo Juncker
Pedersen, Jacob
Rasp, Andreas
Karaev, Emil
von Laffert, Valentin
Bruno, Alessio
Alagia, Michele
Stranges, Stefano
Fischer, Ingo
Coriani, Sonia
contents We report a combined experimental and computational study of the near-edge X-ray absorption fine structure (NEXAFS) spectrum of the propargyl radical, C$_3$H$_3^{\cdot}$. 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 show that two transitions to the lowest lying states 1 $^2$A$_1$ and 2 $^2$A$_1$, 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 CH$_2$ 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.
format Preprint
id arxiv_https___arxiv_org_abs_2602_19356
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle The X-ray absorption spectrum of the propargyl radical, C$_3$H$_3^{\cdot}$
Schaffner, Dorothee
von Buchwald, Theo Juncker
Pedersen, Jacob
Rasp, Andreas
Karaev, Emil
von Laffert, Valentin
Bruno, Alessio
Alagia, Michele
Stranges, Stefano
Fischer, Ingo
Coriani, Sonia
Chemical Physics
We report a combined experimental and computational study of the near-edge X-ray absorption fine structure (NEXAFS) spectrum of the propargyl radical, C$_3$H$_3^{\cdot}$. 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 show that two transitions to the lowest lying states 1 $^2$A$_1$ and 2 $^2$A$_1$, 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 CH$_2$ 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.
title The X-ray absorption spectrum of the propargyl radical, C$_3$H$_3^{\cdot}$
topic Chemical Physics
url https://arxiv.org/abs/2602.19356