The Marcus equation for electron transfer has been widely applied to atom transfer reactions, but the equation
does not seem to work well for very endothermic or very exothermic reactions. In this paper, a modified
model is proposed. The modified model assumes that the potential energy surface can be written as a sum of
the potentials for the individual molecules and an intermolecular potential that keeps the reactants apart. The
activation barrier predicted by the model is within 3 kcal/mol of that predicted by the Marcus electron transfer
equation when −1 ≤ ΔH
r/4E
°≤ 1, where ΔH
r is the heat of reaction and E
° is the intrinsic barrier.
However, there are significant deviations when ΔH
r/4E
° < −1 and when ΔH
r/4E
° > 1. The modified model
predicts that the activation barrier should equal ΔH
r/4E
° in the very endothermic limit, (i.e., ΔH
r/4E
° > 1),
while the Marcus electron transfer equation predicts that the activation energy, E
a, should diverge from ΔH
r.
Data shows that E
a approaches ΔH
r. The modified model predicts that the activation barrier goes to zero for
very exothermic reactions, (i.e., ΔH
r/E
° < −1) while the Marcus electron transfer equation predicts large
barriers. Data shows, though, that the barriers approach zero. We also compare to the Marcus hyperbolic
cosine expression and find that the modified model is within 3 kcal/mol of the Marcus hyperbolic cosine
expression over the entire energy range. The modified model predicts that the barriers to reaction are associated
with Pauli repulsions and not with bond stretching. That prediction agrees with recent ab initio calculations,
and the VB model but not with the intersecting parabola model. Overall, the modified model seems to extend
the original Marcus equation to very endothermic and very exothermic reactions. Also, it gives predictions
similar to the Marcus hyperbolic cosine expression over the entire energy range.