2013
DOI: 10.1021/jp3122616
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The Structure and Spectroscopy of Cyanate and Bicarbonate Ions. Astrophysical Implications

Abstract: Cyanate and bicarbonate are two ions that play active roles in many fields of physics and chemistry, including biological sciences and astrochemistry. We present here a comprehensive study of these species covering a range of phases and methodologies. We have performed theoretical calculations on the isolated ions and their hydrates with one to four water molecules, and in clusters with 15 water molecules. The predicted infrared spectra are compared with observed spectra from experiments where liquid droplets … Show more

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Cited by 4 publications
(5 citation statements)
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References 41 publications
(60 reference statements)
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“…In addition to COMs, ions such as OCN − (cyanate ion), HCOO − and NH + 4 have been proposed to be present in interstellar ices mostly as part of salts produced by acid-base reactions (e.g., Geballe 1984;Grim & Greenberg 1987;Schutte et al 1999;Schutte & Khanna 2003;Gálvez et al 2010;Maté et al 2012;Moreno et al 2013;Bergner et al 2016;Kruczkiewicz et al 2021). The presence of OCN − in ice mantles can be considered a secure detection based on comprehensive laboratory experiments and extensive analysis toward several protostars (e.g., Geballe 1984;van Broekhuizen et al 2004) and toward background stars (McClure et al 2023), and the good correlation between gas-phase abundances of HNCO and OCN − ice (Öberg et al 2009a).…”
Section: Introductionmentioning
confidence: 99%
“…In addition to COMs, ions such as OCN − (cyanate ion), HCOO − and NH + 4 have been proposed to be present in interstellar ices mostly as part of salts produced by acid-base reactions (e.g., Geballe 1984;Grim & Greenberg 1987;Schutte et al 1999;Schutte & Khanna 2003;Gálvez et al 2010;Maté et al 2012;Moreno et al 2013;Bergner et al 2016;Kruczkiewicz et al 2021). The presence of OCN − in ice mantles can be considered a secure detection based on comprehensive laboratory experiments and extensive analysis toward several protostars (e.g., Geballe 1984;van Broekhuizen et al 2004) and toward background stars (McClure et al 2023), and the good correlation between gas-phase abundances of HNCO and OCN − ice (Öberg et al 2009a).…”
Section: Introductionmentioning
confidence: 99%
“…Specifically, for the NCSe – ·H 2 O case, calculations point to the existence of two isomers, whose energies are very close to each other. Similar to previously reported results for NCO – ·H 2 O and NCS – ·H 2 O, the lowest energy structure (Iso I) is characterized by water forming one hydrogen bond (HB) with the N-terminal of NCSe – . The calculated VDE and SO splitting (3.762 eV and 1671 cm –1 ) suggest that it is Iso I that gives rise to the main experimental peak at 3.70 eV with an SO splitting of 1653 cm –1 (Table ).…”
Section: Results and Discussionmentioning
confidence: 99%
“…Gas-phase ion spectroscopy coupled with high-level quantum chemical computations has been demonstrated as an ideal technique to obtain the geometric and electronic structure information for microsolvated clusters and to provide a molecular-level understanding of solute–solvent and solvent–solvent interactions. The method has been shown to provide a sensitive probe of subtle solvation differences between different yet overall similar solutes, such as CN – · n H 2 O, , NCO – · n H 2 O, and NCS – · n H 2 O. , It also allows one to examine different solvation behaviors with different solvent molecules, e.g., water (H 2 O) versus acetonitrile (CH 3 CN), two common but very different solvents with their respective solvation binding motifs driven by the formation of hydrogen bonding in H 2 O , and charge–dipole interaction in CH 3 CN. , …”
Section: Introductionmentioning
confidence: 99%
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