TY - JOUR
T1 - Millimeter wave spectroscopy of propynal isotopologues and structure determination
AU - Robertson, Evan G.
AU - Ruzi, Mahmut
AU - McNaughton, Don
AU - Margulès, Laurent
AU - Motiyenko, Roman A.
AU - Guillemin, Jean Claude
N1 - Funding Information:
We are grateful to Dominique Appadoo and the staff at the Australian synchrotron THz/Far–IR beamline for facilitating the FTIR measurements. We acknowledge a La Trobe University Scholarship for MR. Quantum chemical calculations have been carried out using Australia's National Computing Infrastructure (NCI), project k02. LM, RM and JCG thank the Programme National “Physique et Chimie du Milieu Interstellaire” (PCMI) of CNRS/INSU with INC/INP co-funded by CEA and CNES.
Publisher Copyright:
© 2023
PY - 2023/4
Y1 - 2023/4
N2 - 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.
AB - 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.
KW - Ab initio calculations
KW - Density function theory
KW - far-IR spectroscopy
KW - Interstellar medium
KW - Isotopic substitution
KW - Millimeter wave spectroscopy
KW - Molecular structure
UR - http://www.scopus.com/inward/record.url?scp=85159596725&partnerID=8YFLogxK
U2 - 10.1016/j.jms.2023.111786
DO - 10.1016/j.jms.2023.111786
M3 - Article
AN - SCOPUS:85159596725
SN - 0022-2852
VL - 394
JO - Journal of Molecular Spectroscopy
JF - Journal of Molecular Spectroscopy
M1 - 111786
ER -