An Upgraded Line List for Radiative Transitions between the B <sup>2</sup>Σ<sup>+</sup>, A <sup>2</sup>Π, and X <sup>2</sup>Σ<sup>+</sup> States of the CN Radical

Abstract The global mass-invariant coupled-channel deperturbation model of the B 2 Σ + , A 2 Π, and X 2 Σ + states of the CN radical, which reproduces the overall rovibronic term values of mutually perturbed levels with almost spectroscopic accuracy, has been utilized to produce complete line lists of radiative transitions between the X 2 Σ + , B 2 Σ + , and A 2 Π 1/2;3/2 states of CN isotopologues. The Einstein A emission coefficients generated for the A − X , B − X , and B − A transitions provide both lifetimes of the excited states as well as the B → A / X branching ratios. The ab initio permanent and transition dipole moments required are revisited within the framework of the multireference configuration interaction and of the averaged coupled-pair functional methods. An upgraded line list is provided in ExoMol format and employed to simulate intensity distribution into the high-temperature air plasma B → X and A → X spectra as well as in the rotational resolved B → X / A emission bands undergoing strong local B ∼ A ∼ X perturbations. A comparison with laboratory and astronomical spectra shows that the present line list significantly improves the treatment of both locally perturbed and highly excited rotational levels of the B ∼ A ∼ X complex.

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Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2024-11-19
DOI
https://doi.org/10.3847/1538-4365/ad8b40
Citations
3
Primary Topic
Atmospheric Ozone and Climate
Type
article
Field-Weighted Citation Impact
1.13

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article

An Upgraded Line List for Radiative Transitions between the B 2Σ+, A 2Π, and X 2Σ+ States of the CN Radical

E. A. Pazyuk, В. А. Терашкевич, Sergei N. Yurchenko, S. V. Kozlov et al.
3 citations
The Astrophysical Journal Supplement Series
Atmospheric Ozone and Climate
1.13
article

An Upgraded Line List for Radiative Transitions between the B 2Σ+, A 2Π, and X 2Σ+ States of the CN Radical

E. A. Pazyuk, В. А. Терашкевич, Sergei N. Yurchenko, S. V. Kozlov, Jonathan Tennyson, A. V. Stolyarov
article en
3 citations

Abstract

Abstract The global mass-invariant coupled-channel deperturbation model of the B 2 Σ + , A 2 Π, and X 2 Σ + states of the CN radical, which reproduces the overall rovibronic term values of mutually perturbed levels with almost spectroscopic accuracy, has been utilized to produce complete line lists of radiative transitions between the X 2 Σ + , B 2 Σ + , and A 2 Π 1/2;3/2 states of CN isotopologues. The Einstein A emission coefficients generated for the A − X , B − X , and B − A transitions provide both lifetimes of the excited states as well as the B → A / X branching ratios. The ab initio permanent and transition dipole moments required are revisited within the framework of the multireference configuration interaction and of the averaged coupled-pair functional methods. An upgraded line list is provided in ExoMol format and employed to simulate intensity distribution into the high-temperature air plasma B → X and A → X spectra as well as in the rotational resolved B → X / A emission bands undergoing strong local B ∼ A ∼ X perturbations. A comparison with laboratory and astronomical spectra shows that the present line list significantly improves the treatment of both locally perturbed and highly excited rotational levels of the B ∼ A ∼ X complex.

The Astrophysical Journal Supplement SeriesVol. 275(2)
Lomonosov Moscow State University (RU), University College London (GB)
European Commission, Russian Science Foundation, Science and Technology Facilities Council, Central Laser Facility, Science and Technology Facilities Council, HORIZON EUROPE European Research Council
Openalex Percentile: Top 23%
Atmospheric Ozone and Climate
1.13
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