English

Hyperfine structure of methanol lines at 25 GHz

Atomic Physics 2023-10-13 v1 Cosmology and Nongalactic Astrophysics

Abstract

High-dispersion (channel width 0.015 km s^-1) laboratory spectroscopy of the torsion-rotation lines J_2 - J_1 (J = 2 - 6) in the ground torsional state (vt = 0) of the E-type methanol demonstrates multicomponent hyperfine splitting patterns at 25 GHz. The observed patterns are compared with simulations of CH3OH emission lines based on ab initio quantum-mechanical models. A substantial disparity between the laboratory and simulated patterns is revealed. The observed morphology of the line shapes is not reproduced in the model profiles. The found inconsistency requires further refinement of the current quantum-mechanical models to fit the observed hyperfine splitting patterns at 25 GHz.

Keywords

Cite

@article{arxiv.2310.08231,
  title  = {Hyperfine structure of methanol lines at 25 GHz},
  author = {J. S. Vorotyntseva and S. A. Levshakov},
  journal= {arXiv preprint arXiv:2310.08231},
  year   = {2023}
}

Comments

10 pages, 3 figures, Proc. of the conference "Physics of the ISM: from local cloud to early galaxies", dedicated to the memory of N.G. Bochkarev, Moscow, May 25-26, 2023; to appear in AApTr, vol. 34, N 2, 2023