Abstract

The symmetry of the Diels–Alder transition state depends on the interplay of orbital interactions, aromaticity, which favors a C s structure, and strain, which tends to break symmetry. Twenty Diels–Alder reactions are examined at MP4SDTQ/6-312G(d)//B3LYP/6-31G(d). The substituents utilized are alkyl groups in order to minimize the effect of orbital interactions. The underlying assumptions are examined and appropriate caveats discussed. These computations provide, as a first approximation, an estimate of 10 kcal mol −1 for the aromatic stabilization energy in the Diels–Alder TS.

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