English

High-resolution ro-vibrational and rotational spectroscopy of the open-shell, linear CCH$^+$ ion ($^3\Pi$)

Chemical Physics 2026-05-04 v1 Astrophysics of Galaxies

Abstract

In this work, we report on the high-resolution infrared spectrum of CCH+^+ (3Π^3\Pi) recorded in the range 306631843066-3184~cm1^{-1} by means of leak-out spectroscopy. This spectral range covers the fundamental of the CH stretching mode and a highly excited bending vibrational mode. Based on this data (385 ro-vibrational lines), accurate spectroscopic descriptions of the ground and the two vibrationally excited states of CCH+^+ were obtained. Besides the band origins, spin-orbit coupling constants, rotational constants, centrifugal distortion constants and Λ\Lambda-doubling constants for the ground and excited vibrational states have been derived. This effective Hamiltonian analysis allowed a search for pure rotational lines of CCH+^+ in its electronic and vibrational ground state using a two-color millimeterwave - infrared scheme. We observed all rotational transitions from J=2J^{\prime\prime} = 2 up to J=6J^{\prime\prime} = 6 within the Ω=2\Omega = 2 lowest energy fine structure component with resolved hyperfine splittings. This data has already guided the first detection of CCH+^+ in space toward the Orion Bar photo-dissociation region, and has the potential to support further astronomical searches for CCH+^+ either through radio or infrared spectroscopy, for example with the James Webb Space Telescope.

Keywords

Cite

@article{arxiv.2605.00564,
  title  = {High-resolution ro-vibrational and rotational spectroscopy of the open-shell, linear CCH$^+$ ion ($^3\Pi$)},
  author = {Kim Steenbakkers and Weslley G. D. P. Silva and Oskar Asvany and Gerrit C. Groenenboom and Pavol Jusko and Britta Redlich and Sandra Brünken and Stephan Schlemmer},
  journal= {arXiv preprint arXiv:2605.00564},
  year   = {2026}
}

Comments

34 pages, 5 figures, supplementary information available on the journal webpage