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dc.contributor.authorPeeters, J.
dc.contributor.authorNguyen, V.S.
dc.contributor.authorMuller, J.-F.
dc.date2015
dc.date.accessioned2016-03-24T11:19:59Z
dc.date.available2016-03-24T11:19:59Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2733
dc.descriptionThe atmospheric oxidation of vinyl alcohol (VA) produced by photoisomerization of acetaldehyde (AA) is thought to be a source of formic acid (FA). Nevertheless, a recent theoretical study predicted a high rate coefficient k1(298 K) of ≈10–14 cm3 molecule–1 s–1 for the FA-catalyzed tautomerization reaction 1 of VA back into AA, which suggests that FA buffers its own production from VA. However, the unusually high frequency factor implied by that study prompted us to reinvestigate reaction 1. On the basis of a high-level ab initio potential energy profile, we first established that transition state theory is applicable, and derived a k1(298 K) of only ≈2 × 10–20 cm3 molecule–1 s–1, concluding that the reaction is negligible. Instead, we propose and rationalize another important VA sink: its uptake by aqueous aerosol and cloud droplets followed by fast liquid-phase tautomerization to AA; global modeling puts the average lifetime by this sink at a few hours, similar to oxidation by OH.
dc.languageeng
dc.titleAtmospheric Vinyl Alcohol to Acetaldehyde Tautomerization Revisited
dc.typeArticle
dc.subject.frascatiChemical sciences
dc.audienceScientific
dc.source.titleJournal of Physical Chemistry Letters
dc.source.volume6
dc.source.issue20
dc.source.page4005-4011
Orfeo.peerreviewedYes
dc.identifier.doi10.1021/acs.jpclett.5b01787


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