Infrared spectrum of HCl–O2 dimer and tentative assignment of HCl–(O2)3 tetramer

A A. J. Barclay (Department of Physics and Astronomy, University of Calgary 1 , 2500 University Drive North West, Calgary, Alberta T2N 1N4,) A A. R. W. McKellar (National Research Council of Canada 2 , Ottawa, Ontario K1A 0R6,) N N. Moazzen-Ahmadi (Department of Physics and Astronomy, University of Calgary 1 , 2500 University Drive North West, Calgary, Alberta T2N 1N4,)

Abstract

Spectra of the weakly bound dimer HCl–O2 were studied in the mid-infrared region of the HCl fundamental band (≈2890 cm−1) using a tunable optical parametric oscillator source to probe a pulsed supersonic slit jet expansion. This is the first reported gas-phase spectrum of HCl–O2 in any region. Over 180 H35Cl–O2 and H37Cl–O2 rotational transitions were assigned and interpreted in terms of four sub-states: a Σ ground state, a Π state at about 2.3 cm−1, another Σ state at about 3.3 cm−1, and another Π state at an unknown energy (possibly 1–2 cm−1). For each isotopologue, rotational energies for 75 levels in the ground and excited vibrational states [v(H–Cl) = 0 and 1] were derived directly from the spectra. Efforts to interpret the spectra using an existing theory of weakly bound dimers containing O2 were not very successful, probably due to the presence of large amplitude intermolecular motions. Spectra of two larger clusters, likely each containing one HCl and multiple O2 molecules, were also assigned. One of these spectra, is well simulated by a symmetric top molecule with B = 0.028 cm−1 and is likely due to the tetramer HCl–(O2)3. Although the other spectrum is not understood at all, its dependence on O2 concentration and apparent B-value (≈0.045 cm−1) suggest that it could be due to the trimer HCl–(O2)2.

Article Details

Volume / Issue Vol. 164, Issue 24
Published June 28, 2026
ISSN 0021-9606
Publisher American Institute of Physics

Journal Info

The Journal of Chemical Physics

American Institute of Physics

ISSN: 0021-9606 Physical Sciences

Authors (3)

A

A. J. Barclay

Department of Physics and Astronomy, University of Calgary 1 , 2500 University Drive North West, Calgary, Alberta T2N 1N4,

A

A. R. W. McKellar

National Research Council of Canada 2 , Ottawa, Ontario K1A 0R6,

N

N. Moazzen-Ahmadi

Department of Physics and Astronomy, University of Calgary 1 , 2500 University Drive North West, Calgary, Alberta T2N 1N4,