Millimeter wave spectroscopy of propynal isotopologues and structure determination

Evan G. Robertson, Mahmut Ruzi, Don McNaughton, Laurent Margulès, Roman A. Motiyenko, Jean Claude Guillemin

Research output: Contribution to journalArticleResearchpeer-review

1 Citation (Scopus)

Abstract

Rotational transitions of propynal (HCCCHO) have been measured in the 150–900 GHz region by millimeter wave spectroscopy and in the far infrared region by high resolution FTIR spectroscopy using a synchrotron source. For the parent isotopologue, assignment of MMW transitions up to very high quantum numbers (J = 100, Ka = 25) reveals evidence of extensive perturbations in the ground vibrational state due to Fermi-asymmetry resonance with an excited vibrational state. A fit to nearly 3000 ground state transitions yields effective constants that are suitable for describing relatively unperturbed rotational levels up to Ka = 13. Over 1000 transitions were assigned and fitted for each singly substituted 13C species and nearly 400 transitions for the 18O variant. Re-analysis of literature data on deuterated species, aided by centrifugal distortion constants from hybrid density functional theory calculations at the B2PLYP/aug-cc-pVTZ level, provides a further set of rotational constants. This allows determination of a Rm(2) structure for propynal with the following geometry: r(C≡C) = 1.2066(15), r(C[sbnd]C) = 1.4486(14), r(CO) = 1.2087(10), r(C­H ald) = 1.1069(8), r(C­H acet) = 1.0578(13), θ(CCC) = 176.71(22), θ(OCC) = 123.23(7), θ(HCC ald) = 114.43(31), θ(HCC acet) = 178.45(16). A new Rs structure was also derived.

Original languageEnglish
Article number111786
Number of pages10
JournalJournal of Molecular Spectroscopy
Volume394
DOIs
Publication statusPublished - Apr 2023

Keywords

  • Ab initio calculations
  • Density function theory
  • far-IR spectroscopy
  • Interstellar medium
  • Isotopic substitution
  • Millimeter wave spectroscopy
  • Molecular structure

Cite this