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Vinyl alcohol, also called ethenol (IUPAC name; not ethanol) or ethylenol, is the simplest enol. With the formula Template:Chem2, it is a labile compound that converts to acetaldehyde immediately upon isolation near room temperature.<ref name=March>Template:March6th</ref> It is not a practical precursor to any compound.

SynthesisEdit

Vinyl alcohol can be formed by the pyrolytic elimination of water from ethylene glycol at a temperature of 900 °C and low pressure. Such processes are of no practical importance.<ref>Template:Cite book</ref>

Tautomerization of vinyl alcohol to acetaldehydeEdit

Under normal conditions, vinyl alcohol converts (tautomerizes) to acetaldehyde:

File:Ethenol–ethanal tautomérisation.svgTemplate:Clear left

At room temperature, acetaldehyde (Template:Chem2) is more stable than vinyl alcohol (Template:Chem2) by 42.7 kJ/mol.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> Vinyl alcohol gas isomerizes to the aldehyde with a half-life of 30 min at room temperature.<ref name=March/>

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File:WackerCycleKeith&HenryImp.png
The industrial synthesis of acetaldehyde (Wacker process) proceeds via the intermediacy of a vinyl alcohol complex.<ref name=K&H>Template:Cite journal</ref>

The uncatalyzed keto–enol tautomerism by a 1,3-hydrogen migration is forbidden by the Woodward–Hoffmann rules and therefore has a high activation barrier and is not a significant pathway at or near room temperature. However, even trace amounts of acids or bases (including water) can catalyze the reaction. Even with rigorous precautions to minimize adventitious moisture or proton sources, vinyl alcohol can only be stored for minutes to hours before it isomerizes to acetaldehyde. (Carbonic acid is another example of a substance that is stable when rigorously pure, but decomposes rapidly due to catalysis by trace moisture.)

The tautomerization can also be catalyzed via photochemical process. These findings suggest that the keto–enol tautomerization is a viable route under atmospheric and stratospheric conditions, relevant to a role for vinyl alcohol in the production of organic acids in the atmosphere.<ref>Template:Cite journal</ref><ref>Template:Cite journal</ref>

Vinyl alcohol can be stabilized by controlling the water concentration in the system and utilizing the kinetic favorability of the deuterium-produced kinetic isotope effect (kH+/kD+ = 4.75, kH2O/kD2O = 12). Deuterium stabilization can be accomplished through hydrolysis of a ketene precursor in the presence of a slight stoichiometric excess of heavy water (D2O). Studies show that the tautomerization process is significantly inhibited at ambient temperatures ( kt ≈ 10−6 M/s), and the half-life of the enol form can easily be increased to t1/2 = 42 minutes for first-order hydrolysis kinetics.<ref>Template:Cite journal</ref>

Relationship to poly(vinyl alcohol)Edit

Because of the instability of vinyl alcohol, the thermoplastic polyvinyl alcohol (PVA or PVOH) is made indirectly by polymerization of vinyl acetate followed by hydrolysis of the ester bonds (Ac = acetyl; HOAc = acetic acid):<ref name=Ullmann>Template:Ullmann</ref>

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As a ligandEdit

Several metal complexes are known that contain vinyl alcohol as a ligand. One example is Pt(acac)(η2-C2H3OH)Cl.<ref>Template:Cite journal</ref>

Occurrence in interstellar mediumEdit

Vinyl alcohol was detected in the molecular cloud Sagittarius B in 2001, the last of the three stable isomers of Template:Chem (after acetaldehyde and ethylene oxide) to be detected in space.<ref>Template:Cite press release</ref><ref name = SpaceVA /> Its stability in the (dilute) interstellar medium shows that its tautomerization does not happen unimolecularly,<ref name = SpaceVA>Template:Cite journal</ref> a fact attributed to the size of the activation energy barrier to the rearrangement being insurmountable at temperatures present in interstellar space.<ref name = ChemPhysChem2021 /> The vinyl alcohol to acetaldehyde rearrangement is the only keto-enol tautomerisation to have been detected in deep space, induced by the provision of secondary electrons from galactic cosmic rays.<ref name = ChemPhysChem2021>Template:Cite journal</ref>

ReferencesEdit

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