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Published on: August 18, 2017
Valence Threshold Photoionization Spectra of C 5 $_5$ H and C 5 $_5$ H 2 $_2$ Isomers
Ugo Jacovella1, Myriam Drissi2, Bérenger Gans1
1Université Paris-Saclay, CNRS, Institut des Sciences Moléculaires d'Orsay, Orsay, France.
This study characterizes C5Hx isomers, crucial in forming large carbon molecules. High-resolution spectra differentiate linear and cyclic structures, providing benchmarks for combustion and astrochemistry.
Area of Science:
- Physical Chemistry
- Chemical Physics
- Spectroscopy
Background:
- C5Hx species are vital intermediates in the synthesis of complex carbonaceous molecules.
- Understanding their structure is key to modeling combustion processes and interstellar chemistry.
Purpose of the Study:
- To record and assign mass-selected threshold photoelectron spectra (TPES) for linear and cyclic C5Hx isomers.
- To establish reliable methods for distinguishing between different C5Hx isomers using high-resolution spectroscopy.
- To provide benchmarks for identifying these reactive intermediates in various chemical environments.
Main Methods:
- Double-imaging photoelectron-photoion coincidence spectroscopy was employed to obtain TPES.
- Transient C5Hx species were generated in situ via hydrogen abstraction reactions using fluorine atoms in a discharge flow-tube reactor.
- Ab initio calculations and Franck-Condon simulations were used for spectral assignment and ionization energy determination.
Main Results:
- TPES for l-C5H and c-C3H-CCH were reported for the first time.
- Accurate adiabatic ionization energies were determined for the studied C5Hx isomers.
- The study demonstrated that high-resolution TPES effectively distinguishes between linear and cyclic C5Hx isomers, surpassing photoion yield methods.
Conclusions:
- The developed TPES method provides a robust fingerprint for identifying C5Hx isomers.
- These findings offer critical data for understanding hydrocarbon formation in combustion and astrochemical settings.
- Similar isomeric distributions were observed from distinct precursors, suggesting common formation pathways.
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