English

Gas phase detection and rotational spectroscopy of ethynethiol, HCCSH

Astrophysics of Galaxies 2018-12-03 v1 Chemical Physics

Abstract

We report the gas-phase detection and spectroscopic characterization of ethynethiol (HCCSH\mathrm{HCCSH}), a metastable isomer of thioketene (H2C2S\mathrm{H_2C_2S}) using a combination of Fourier-transform microwave and submillimeter-wave spectroscopies. Several aa-type transitions of the normal species were initially detected below 40 GHz using a supersonic expansion-electrical discharge source, and subsequent measurement of higher-frequency, bb-type lines using double resonance provided accurate predictions in the submillimeter region. With these, searches using a millimeter-wave absorption spectrometer equipped with a radio frequency discharge source were conducted in the range 280 - 660 GHz, ultimately yielding nearly 100 transitions up to rR0(36)^rR_0(36) and rQ0(68)^rQ_0(68). From the combined data set, all three rotational constants and centrifugal distortion terms up to the sextic order were determined to high accuracy, providing a reliable set of frequency predictions to the lower end of the THz band. Isotopic substitution has enabled both a determination of the molecular structure of HCCSH\mathrm{HCCSH} and, by inference, its formation pathway in our nozzle discharge source via the bimolecular radical-radical recombination reaction SH+C2H\mathrm{SH + C_2H}, which is calculated to be highly exothermic (-477 kJ/mol) using the HEAT345(Q) thermochemical scheme.

Keywords

Cite

@article{arxiv.1811.12798,
  title  = {Gas phase detection and rotational spectroscopy of ethynethiol, HCCSH},
  author = {Kin Long Kelvin Lee and Marine-Aline Martin-Drumel and Valerio Lattanzi and Brett A. McGuire and Paola Caselli and Michael McCarthy},
  journal= {arXiv preprint arXiv:1811.12798},
  year   = {2018}
}

Comments

Accepted for publication in Molecular Physics. 29 pages, 4 tables, 6 figures. Supporting information is available