The 130 to 375 GHz Rotational Spectroscopy of <i>s</i>-<i>trans</i>-(<i>Z</i>)-1-Cyano-1,3-butadiene (C<sub>5</sub>H<sub>5</sub>N): Analysis of the Lowest-Energy Vibrationally Excited Dyad (ν<sub>19</sub> and ν<sub>27</sub>)

The rotational spectra and analysis of the two lowest-energy vibrationally excited states, ν<sub>19</sub> (A', 126 cm<sup>-1</sup>, MP2) and ν<sub>27</sub> (A″, 133 cm<sup>-1</sup>, MP2), of <i>s-trans-(Z)</i>-1-cyano-1,3-butadiene from 130 to 375 GHz is presented. The state symmetries allow <i>a-</i> and <i>b-</i>type Coriolis coupling, the effects of which are observed due to the close energy spacing of these states. A combined total of 6744 transitions were modeled (σ<sub>fit</sub> < 60 kHz) with a partial-octic two-state A-reduced Hamiltonian including eight coupling parameters (<i>G</i><sub><i>a</i></sub>, <i>G</i><sub><i>a</i></sub><sup><i>J</i></sup>, <i>F</i><sub><i>bc</i></sub>, <i>F</i><sub><i>bc</i></sub><sup><i>J</i></sup>, <i>G</i><sub><i>b</i></sub>, <i>G</i><sub><i>b</i></sub><sup><i>J</i></sup>, <i>G</i><sub><i>b</i></sub><sup><i>JJ</i></sup>, and <i>G</i><sub><i>b</i></sub><sup><i>K</i></sup>). The vibration-rotation interaction constants, Coriolis ζ terms, and energy difference between the states were determined experimentally and are compared to predicted values (B3LYP/6-311+G(2d,p) and MP2/6-311+G(2d,p)). The coupled-state analysis affords a precise vibrational energy difference of 5.753 373 1 (25) cm<sup>-1</sup> between the two fundamental states. Several matching pairs of <i>a</i>- and <i>b</i>-type resonant transitions, as well as many formally forbidden, nominal interstate transitions, are included in the final least-squares fit. (<i>E</i>)- and (<i>Z</i>)-1-Cyano-1,3-butadiene are possible precursors to or degradation products of pyridine, a fundamental aromatic molecule of interest in the interstellar medium. There is currently some uncertainty concerning the reported identifications of other cyanobutadiene isomers in the interstellar medium. Combined with our previously reported ground-state spectroscopic constants, the vibrationally excited-state constants provided herein enable possible extraterrestrial identification of multiple vibrational states of <i>s-trans-(Z)</i>-1-cyano-1,3-butadiene.

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Journal
The Journal of Physical Chemistry A
Published
2025-09-04
DOI
https://doi.org/10.1021/acs.jpca.5c04066
Primary Topic
Molecular Spectroscopy and Structure
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article
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article

The 130 to 375 GHz Rotational Spectroscopy of s-trans-(Z)-1-Cyano-1,3-butadiene (C5H5N): Analysis of the Lowest-Energy Vibrationally Excited Dyad (ν19 and ν27)

Robert J. McMahon, Brian J. Esselman, P. Matisha Dorman, R. Claude Woods et al.
The Journal of Physical Chemistry A
Molecular Spectroscopy and Structure
article

The 130 to 375 GHz Rotational Spectroscopy of s-trans-(Z)-1-Cyano-1,3-butadiene (C5H5N): Analysis of the Lowest-Energy Vibrationally Excited Dyad (ν19 and ν27)

Robert J. McMahon, Brian J. Esselman, P. Matisha Dorman, R. Claude Woods, Andrew N. Owen
article en

Abstract

The rotational spectra and analysis of the two lowest-energy vibrationally excited states, ν<sub>19</sub> (A', 126 cm<sup>-1</sup>, MP2) and ν<sub>27</sub> (A″, 133 cm<sup>-1</sup>, MP2), of <i>s-trans-(Z)</i>-1-cyano-1,3-butadiene from 130 to 375 GHz is presented. The state symmetries allow <i>a-</i> and <i>b-</i>type Coriolis coupling, the effects of which are observed due to the close energy spacing of these states. A combined total of 6744 transitions were modeled (σ<sub>fit</sub> < 60 kHz) with a partial-octic two-state A-reduced Hamiltonian including eight coupling parameters (<i>G</i><sub><i>a</i></sub>, <i>G</i><sub><i>a</i></sub><sup><i>J</i></sup>, <i>F</i><sub><i>bc</i></sub>, <i>F</i><sub><i>bc</i></sub><sup><i>J</i></sup>, <i>G</i><sub><i>b</i></sub>, <i>G</i><sub><i>b</i></sub><sup><i>J</i></sup>, <i>G</i><sub><i>b</i></sub><sup><i>JJ</i></sup>, and <i>G</i><sub><i>b</i></sub><sup><i>K</i></sup>). The vibration-rotation interaction constants, Coriolis ζ terms, and energy difference between the states were determined experimentally and are compared to predicted values (B3LYP/6-311+G(2d,p) and MP2/6-311+G(2d,p)). The coupled-state analysis affords a precise vibrational energy difference of 5.753 373 1 (25) cm<sup>-1</sup> between the two fundamental states. Several matching pairs of <i>a</i>- and <i>b</i>-type resonant transitions, as well as many formally forbidden, nominal interstate transitions, are included in the final least-squares fit. (<i>E</i>)- and (<i>Z</i>)-1-Cyano-1,3-butadiene are possible precursors to or degradation products of pyridine, a fundamental aromatic molecule of interest in the interstellar medium. There is currently some uncertainty concerning the reported identifications of other cyanobutadiene isomers in the interstellar medium. Combined with our previously reported ground-state spectroscopic constants, the vibrationally excited-state constants provided herein enable possible extraterrestrial identification of multiple vibrational states of <i>s-trans-(Z)</i>-1-cyano-1,3-butadiene.

The Journal of Physical Chemistry AVol. 129(37)
University of Wisconsin–Madison (US)
National Science Foundation
Openalex Percentile: Top 79%
Molecular Spectroscopy and Structure
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