4.2 Article

Phosphorus and silicon analogs of isocyanic acid: Microwave detection of HPCO and HNSiO

Journal

JOURNAL OF MOLECULAR SPECTROSCOPY
Volume 310, Issue -, Pages 119-125

Publisher

ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.jms.2014.12.019

Keywords

Isocyanic acid; Phosphaketene; Silaisocyanic acid; Fourier transform microwave spectroscopy; Coupled-cluster calculations

Funding

  1. Deutsche Forschungsgemeinschaft (DFG) [TH 1301/3-2]
  2. NASA [NNX13AE59G]
  3. DFG
  4. NASA [NNX13AE59G, 474607] Funding Source: Federal RePORTER

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Phosphaketene, HPCO, and silaisocyanic acid, HNSiO, have been characterized in the gas phase for the first time, employing Fourier transform microwave spectroscopy. Besides the parent isotopic species, the rare isotopologs (HPCO)-C-13, (HNSiO)-Si-29, and (HNSiO)-Si-30 were also observed. The molecular parameters derived experimentally agree very well with results of new quantum-chemical calculations performed at the coupled-cluster level of theory. Other derivatives of HNCO, in which one atom is replaced with its third-row counterpart, or two atoms are replaced with their second-row counterparts, may be detectable using the same combined theoretical/experimental approach. Because both isocyanic acid, HNCO, and its sulfur variant HNCS are abundant in molecule-rich astronomical sources, HPCO and HNSiO are good candidates for future radio astronomical searches. (C) 2015 Elsevier Inc. All rights reserved.

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