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Disentangling the complex spectrum of the ethynyl cation
B Mehnen1, R Linguerri2, S Ben Yaghlane3
1Université Paris-Est, Laboratoire Modélisation et Simulation Multi Echelle, MSME UMR 8208 CNRS, 5 bd Descartes, 77454 Marne-la-Vallée, France. roberto.linguerri@u-pem.fr and Laboratoire de Spectroscopie Atomique, Moléculaire et Applications LSAMA, Université de Tunis El Manar, Tunis, Tunisia.
The ethynyl cation (C2H+) plays a key role in astrophysics and combustion. Its complex electronic structure and interactions present a significant computational challenge, impacting organic compound formation and decomposition.
Area of Science:
- Theoretical Chemistry
- Astrophysical Chemistry
- Physical Chemistry
Background:
- The ethynyl cation (C2H+) is crucial in interstellar chemistry and combustion processes.
- It participates in the synthesis and degradation pathways of organic molecules.
Purpose of the Study:
- Investigate the low-lying electronic states of the ethynyl cation (C2H+).
- Analyze potential energy surfaces and electronic state interactions.
- Determine the adiabatic ionization energy of the ethynyl radical.
Main Methods:
- Utilized pure ab initio computational methodologies.
- Examined potential energy surfaces along stretching and bending coordinates.
- Analyzed electronic state density and wavefunction mixing.
Main Results:
- Identified a high density of electronic states leading to significant interactions.
- Characterized the ground state as 3Π symmetry and the lowest singlet state (1Π) as a Renner-Teller system.
- Calculated the adiabatic ionization energy of the ethynyl radical, matching experimental data.
Conclusions:
- The ethynyl cation exhibits complex electronic behavior due to multiple couplings (Renner-Teller, vibronic, spin-orbit).
- Accurate spectral predictions require accounting for these intricate interactions.
- Despite its small size, C2H+ remains a computationally demanding system.
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