ArXiv TLDR

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

🐦 Tweet
2605.00564

Kim Steenbakkers, Weslley G. D. P. Silva, Oskar Asvany, Gerrit C. Groenenboom, Pavol Jusko + 3 more

physics.chem-phastro-ph.GA

TLDR

High-resolution infrared and millimeter-wave spectroscopy of the CCH$^+$ ion provides crucial data for its astronomical detection and characterization.

Key contributions

  • Recorded high-resolution infrared spectrum of CCH$^+$ (3066-3184 cm⁻¹) using leak-out spectroscopy.
  • Derived accurate spectroscopic constants for CCH$^+$ ground and excited vibrational states.
  • Observed pure rotational lines of CCH$^+$ in its ground state with resolved hyperfine splittings.
  • This data guided the first astronomical detection of CCH$^+$ in the Orion Bar photo-dissociation region.

Why it matters

This work provides essential, highly accurate spectroscopic data for the CCH$^+$ ion, a key interstellar molecule. This data has already enabled its first astronomical detection and will support future searches using telescopes like JWST, advancing our understanding of astrochemistry.

Original Abstract

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 $J^{\prime\prime} = 2$ up to $J^{\prime\prime} = 6$ 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.

📬 Weekly AI Paper Digest

Get the top 10 AI/ML arXiv papers from the week — summarized, scored, and delivered to your inbox every Monday.