In this work, we report on the high-resolution infrared spectrum of CCH+ (3Π) recorded in the range 3066−3184~cm−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-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′′=2 up to J′′=6 within the Ω=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.
@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