Literature DB >> 26290966

Two Isomers of Protonated Isocyanic Acid: Evidence for an Ion-Molecule Pathway for HNCO ↔ HOCN Isomerization.

Valerio Lattanzi1, Sven Thorwirth2, Carl A Gottlieb1, Michael C McCarthy1.   

Abstract

Ion-molecule reactions are thought to play a crucial role in the formation of metastable isomers, but relatively few protonated intermediates beyond HNCH(+) have been characterized at high spectral resolution. We present here laboratory measurements of the rotational spectra of protonated isocyanic acid in two isomeric forms, the ground state H2NCO(+) with C2v symmetry and a low-lying bent chain HNCOH(+), guided by coupled cluster calculations of their molecular structure. Somewhat surprisingly, HNCOH(+) is found to be more abundant than H2NCO(+), even though this metastable isomer is calculated to lie approximately 15-20 kcal/mol higher in energy. In the same way that HCNH(+) serves as a key intermediate in ion-molecule reactions that form HNC via dissociative electron recombination in cold dense interstellar molecular clouds, HNCOH(+) may play an analogous role in the conversion of HNCO to HOCN.

Entities:  

Keywords:  bonding; molecular structure; quantum-chemical calculations; radio astronomy; rotational spectroscopy

Year:  2012        PMID: 26290966     DOI: 10.1021/jz301520s

Source DB:  PubMed          Journal:  J Phys Chem Lett        ISSN: 1948-7185            Impact factor:   6.475


  3 in total

1.  Water-assisted isomerization of the [H, C, N, O] system.

Authors:  Jia Cao; Zhi Xiang Wang; Lou Jun Gao; Feng Fu
Journal:  J Mol Model       Date:  2015-03-05       Impact factor: 1.810

2.  Discovery of the acetyl cation, CH3CO+, in space and in the laboratory.

Authors:  J Cernicharo; C Cabezas; S Bailleux; L Margulès; R Motiyenko; L Zou; Y Endo; C Bermúdez; M Agúndez; N Marcelino; B Lefloch; B Tercero; P de Vicente
Journal:  Astron Astrophys       Date:  2021-02-05       Impact factor: 5.802

3.  Discovery of the elusive radical NCO and confirmation of H2NCO+ in space.

Authors:  N Marcelino; M Agúndez; J Cernicharo; E Roueff; M Tafalla
Journal:  Astron Astrophys       Date:  2018-05-10       Impact factor: 5.802

  3 in total

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