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 language | English (US) |
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Article number | stad3242 |
Pages (from-to) | 1357-1363 |
Number of pages | 7 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 527 |
Issue number | 1 |
Early online date | Oct 23 2023 |
DOIs | |
State | Published - Jan 1 2024 |
Keywords
- astrochemistry
- ISM: molecules
- methods: numerical
- molecular processes