Ab initio calculation of optical rotatory dispersion (ORD) curves: a simple and reliable approach to the assignment of the molecular absolute configuration
In this paper, both Hartree-Fock (HF) and density functional theory (DFT) methods have been
used to make ab initio calculations of the optical rotatory power of selected molecules at several wavelengths;
that is, part of the optical rotatory dispersion (ORD) curve has been predicted. This approach constitutes
a new, simple, and reliable method to assign the molecular absolute configuration, at least for rigid molecules
such as those studied in the present work. In fact, in this way, it is possible to overcome the difficulties
connected to some relevant cases, in particular that of (-)-â-pinene, for which even a very high-level (DFT/
B3LYP/6-311++G(2d,2p)) calculation affords the wrong sign of the optical rotation at 633 nm. On the
contrary, the predicted ORD curve, even using small basis sets, reproduces (below 400 nm) the experimental
trend well, allowing for the correct configurational assignment. This result clearly shows that to have a
reliable configurational assignment the comparison between experimental and predicted rotation values
must be carried out at different wavelengths and not at a single frequency. The reason for this is that
working at wavelengths approaching the absorption maximum the [R]ì values become larger and their
prediction becomes more reliable. Coupling the use of an inexpensive instrument (a polarimeter working
at a few wavelengths) with the use of a DFT-calculation package can also allow the experimental organic
chemist to arrive, quickly and reliably, at the assignment of the molecular absolute configuration
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