The ground-state potential energy surface of C6H63-+ was explored by ab initio molecular orbital calculations using the split valence 3-21G basis set. Various isomers were located as minima, the most stable corresponding to the fulvene tricat-.... 0 -1 3+ β’ β’ ion (1). The heat of formation of 1 Is e
Ab initio computational study of selected C60H6 isomers
β Scribed by Paul A. Cahill
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 348 KB
- Volume
- 254
- Category
- Article
- ISSN
- 0009-2614
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β¦ Synopsis
The relative energies of 18 isomers of C6oH 6 have been determined through geometry-optimized ab initio calculations. HF/6-31G* computations on the two lowest energy structures determined at the HF/3-21G level indicate that 1,2,4,11,15,30-C6oH 6 (18, with a C6oBr6-1ike structure) lies only 0.4 kcal/mol higher in energy than 1,2,3,4,9i,10-C6oH (4). This remarkably close energy spacing was unexpected because, unlike in 4 in which addition occurs exclusively to 6,6 ring fusions, H 2 addition in 18 occurs both 1,2 to a 6,6 ring fusion and 1,4 across 6-rings so as to place two double bonds into 6,5 ring fusions.
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