Formation of hydroxide anions in amorphous astrophysical ices and recombination with protons: a quantum chemical study

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Abstract

Quantum chemical cluster calculations employing density functional theory and correlation consistent basis sets reveal the following pathways by which hydroxide anions (OH ) may form in amorphous astrophysical ices: (1) hydroxyl radicals (OH), which may arise in ice via ultraviolet photolysis, can capture electrons; (2) adsorbed hydrogen atoms can capture electrons to form H , which reacts with water to yield H 2 and OH ; (3) NaOH deposited on ice dissociates into Na + and OH ; (4) NaH deposited on ice dissociates into Na + and H ; H then reacts with water to yield H 2 and OH as above. The IR spectrum of ice-bound OH is presented, based on nine clusters containing up to 31H 2O and 1–2 OH anions. The interaction of OH in ice with cations is also explored. Prior work shows that when HCO + is deposited on pure amorphous water clusters, it reacts with H 2O to form formic acid (HCOOH) and the hydronium (H 3O +). When HCO + is deposited on a cluster containing OH , the reaction proceeds in almost the same manner, but the H 3O + and OH charge centres migrate through the water network toward each other and tend to neutralize one another by forming H 2O. This occurred in all but one of seven cases considered; migration occurred even when the oxygen atom attacked by HCO + is over 10 Å from the oxygen atom in OH . Cations and anions can interact in ice via pathways not present in the gas phase or incorporated in current models.

Original languageEnglish (US)
Article numberstad3242
Pages (from-to)1357-1363
Number of pages7
JournalMonthly Notices of the Royal Astronomical Society
Volume527
Issue number1
Early online dateOct 23 2023
DOIs
StatePublished - Jan 1 2024

Keywords

  • astrochemistry
  • ISM: molecules
  • methods: numerical
  • molecular processes

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