"Analysis Of The Coriolis- And Fermi-coupled Triad Near 315 <span Class=""roman"">cm</span>^&#8722;1&nbsp;&nbsp;of Benzonitrile (<span Class=""roman"">c</span>_{<span Class=""roman"">6</span>}<span Class=""roman"">h</span><sub><span Class=""roman"""

Zdanovskaia, Maria

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https://hdl.handle.net/2142/111595 Copy

Description

Title

"Analysis Of The Coriolis- And Fermi-coupled Triad Near 315 cm⁻¹  of Benzonitrile (c₆h

Author(s)

Zdanovskaia, Maria

Contributor(s)

• Kisiel, Zbigniew
• McMahon, Robert J.
• Woods, R. Claude
• Esselman, Brian J.

Issue Date

2021-06-22

Keyword(s)

Comparing theory and experiment

Abstract

We previously presented the least-squares fit of the benzonitrile (\chem{C_6H_5CN}, C$_{2v}$, $\mu$$_{a}$ = 4.5 D) ground vibrational state, which was fit to a partial octic Hamiltonian, as well as the first analysis of its two Coriolis-coupled, lowest-energy fundamental states, \nub{22} and \nub{33}.$^{1}$ Herein, we present the continuation of this work: the analysis and fitting of the Coriolis- and Fermi-coupled triad of the overtone and combination states (\nub{22} = 2, \nub{33} = 2, and \nub{22} + \nub{33}) near 315 \wn. Approximately 3000 transitions are assigned for each state, including multiple resonances, and their least-squares fitting results in precise energy separations that are in agreement with those expected based on the energy separation determined for \nub{22} and \nub{33}. $\\$ $\\$ 1. Zdanovskaia, M. A.; Esselman, B. J.; Lau, H. S.; Bates, D. M.; Woods, R. C.; McMahon, R. J.; Kisiel, Z. The 103 - 360 GHz Rotational Spectrum of Benzonitrile, the First Interstellar Benzene Derivative Detected by Radioastronomy. $\it{J. Mol. Spectrosc}$. $\textbf{2018}$, 351, 39-48.

Publisher

International Symposium on Molecular Spectroscopy

Type of Resource

Text

Language

eng

Permalink

http://hdl.handle.net/2142/111595

DOI

10.15278/isms.2021.TE01

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