Negative hyperconjugation and red-, blue- or zero-shift in X-Z Y complexesElectronic supplementary information (ESI) available: Coordinates of the model complexes and evidence for proper and pro-improper nature of model systems. See DOI: 10.1039/c4fd00183d
A generalized explanation is provided for the existence of the red- and blue-shifting nature of X-Z bonds (Z = H, halogens, chalcogens, pnicogens, etc. ) in X-Z Y complexes based on computational studies on a selected set of weakly bonded complexes and analysis of existing literature data. The addit...
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Sprache: | eng |
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Zusammenfassung: | A generalized explanation is provided for the existence of the red- and blue-shifting nature of X-Z bonds (Z = H, halogens, chalcogens, pnicogens,
etc.
) in X-Z Y complexes based on computational studies on a selected set of weakly bonded complexes and analysis of existing literature data. The additional electrons and orbitals available on Z in comparison to H make for dramatic differences between the H-bond and the rest of the Z-bonds. The nature of the X-group and its influence on the X-Z bond length in the parent X-Z molecule largely controls the change in the X-Z bond length on X-Z Y bond formation; the Y-group usually influences only the magnitude of the effects controlled by X. The major factors which control the X-Z bond length change are: (a) negative hyperconjugative donation of electron density from X-group to X-Z σ* antibonding molecular orbital (ABMO) in the parent X-Z, (b) induced negative hyperconjugation from the lone pair of electrons on Z to the antibonding orbitals of the X-group, and (c) charge transfer (CT) from the Y-group to the X-Z σ* orbital. The exchange repulsion from the Y-group that shifts partial electron density at the X-Z σ* ABMO back to X leads to blue-shifting and the CT from the Y-group to the σ* ABMO of X-Z leads to red-shifting. The balance between these two opposing forces decides red-, zero- or blue-shifting. A continuum of behaviour of X-Z bond length variation is inevitable in X-Z Y complexes. |
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ISSN: | 1359-6640 1364-5498 |
DOI: | 10.1039/c4fd00183d |