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Possible spectroscopic manifestation of the angular group induced bond alteration (AGIBA) effect in toluene
Author(s) -
Kirillov S. A.,
Morresi A.,
Paolantoni M.,
Sassi P.
Publication year - 2007
Publication title -
journal of physical organic chemistry
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.325
H-Index - 66
eISSN - 1099-1395
pISSN - 0894-3230
DOI - 10.1002/poc.1208
Subject(s) - chemistry , toluene , raman spectroscopy , aromaticity , ring (chemistry) , wavenumber , crystal (programming language) , double bond , methyl group , spectral line , group (periodic table) , computational chemistry , crystallography , crystal structure , stereochemistry , organic chemistry , molecule , physics , astronomy , computer science , optics , programming language
The most obvious consequence of the concept of aromaticity is the common confidence that in aromatic compounds, bond lengths do not alternate and are between typical to the single and double ones. However, in 1994, performing crystal structure investigations of substituted pyridines and their salts, Krygowski and co‐workers have discovered a very surprising angular group induced bond alteration (AGIBA) effect: It appears that some angular substituents, like methoxy or nitrozo groups, can induce bond alternation in aromatic rings. Crystal studies do not allow one to operate with liquids that are more common in organic chemistry. This paper presents the first possible evidence of spectroscopic manifestations of the AGIBA effect. Raman spectra of the liquid toluene are analyzed. It is found that instead of being single, the line corresponding to the ring breathing vibrations is clearly split by 1.0–1.4 cm −1 , thus indicating the presence of two ( cis ‐ and trans ‐) AGIBA isomers. The energy difference between these isomers estimated in temperature dependent Raman studies is found equal to 6.68 kJ mol −1 . The low‐wavenumber line therefore corresponds to the cis ‐AGIBA isomer and the high‐wavenumber line to the trans ‐AGIBA isomer stabilized by the AGIBA effect. Copyright © 2007 John Wiley & Sons, Ltd.