| Literature DB >> 20411529 |
Willem-Jan van Zeist, F Matthias Bickelhaupt.
Abstract
We respond to a paper by Fernández, Frenking, and Uggerud (FFU: Chem. Eur. J. 2009, 15, 2166) in which they conclude that not steric hindrance but reduced electrostatic attraction and reduced orbital interactions are responsible for the S(N)2 barrier, in particular in the case of more highly substituted substrates, for example, F(-) + C(CH(3))(3)F. We disagree with this conclusion, which we show is the result of neglecting geometry relaxation processes that are induced by increased Pauli repulsion in the sterically congested S(N)2 transition state.Entities:
Year: 2010 PMID: 20411529 DOI: 10.1002/chem.200902337
Source DB: PubMed Journal: Chemistry ISSN: 0947-6539 Impact factor: 5.236