The
OH radical plays an important role in combustion, and isopentanol
(3-methylbutan-1-ol) is a promising sustainable fuel additive and
second-generation biofuel. The abstractions of H atoms from fuel molecules
are key initiation steps for chain branching in combustion chemistry.
In comparison with the more frequently studied ethanol, isopentanol
has a longer carbon chain that allows a greater number of products,
and experimental work is unavailable for the branching fractions to
the various products. However, the site-dependent kinetics of isopentanol
with OH radicals are usually experimentally unavailable. Alcohol oxidation
by OH is also important in the atmosphere, and in the present study
we calculate the rate constants and branching fractions of the hydrogen
abstraction reaction of isopentanol by OH radical in a broad temperature
range of 298–2400 K, covering temperatures important for atmospheric
chemistry and those important for combustion. The calculations are
done by multipath variational transition state theory (MP-VTST). With
a combination of electronic structure calculations, we determine previously
missing thermochemical data. With MP-VTST, a multidimensional tunneling
approximation, multiple-structure anharmonicity, and torsional potential
anharmonicity, we carried out more realistic rate constant calculations
than can be computed by conventional single-structure harmonic transition
state theory or by the empirical relations that are currently used
in atmospheric and combustion modeling. The roles of
various factors in determining the rates are elucidated, and we show
that recrossing, tunneling, and multiple structures are all essential
for accurate work. We conclude that the multiple structure anharmonicity
is the most important correction to conventional transition state
theory for this reaction, although recrossing effects and tunneling
are by no means insignificant and the tunneling depends significantly
on the path. The thermodynamic and kinetics data determined in this
work are indispensable for the gas-phase degradation of alcohols in
the atmosphere and for the detailed understanding and prediction of
ignition mechanisms of biofuels in combustion.