1986
DOI: 10.1021/ja00275a011
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Predictions of relative stabilities among series of carborane isomers by the criterion of topological charge stabilization

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Cited by 87 publications
(54 citation statements)
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“…Thus, the carbon‐germanium triangulenes 1g – 4g substantially differ from carbon triangulenes 1a – 4a , they have non‐planar structure preventing effective delocalization of the unpaired electrons (see Table for exchange coupling constants) and are characterized by significant loss of aromaticity. These results are in accord with the rule of topological charge stabilization and the conclusion on that in mixed‐composition triangulenes more electronegative atoms prefer to take a‐positions.…”
Section: Resultssupporting
confidence: 90%
“…Thus, the carbon‐germanium triangulenes 1g – 4g substantially differ from carbon triangulenes 1a – 4a , they have non‐planar structure preventing effective delocalization of the unpaired electrons (see Table for exchange coupling constants) and are characterized by significant loss of aromaticity. These results are in accord with the rule of topological charge stabilization and the conclusion on that in mixed‐composition triangulenes more electronegative atoms prefer to take a‐positions.…”
Section: Resultssupporting
confidence: 90%
“…1 The method of topological charge stabilization assigns preferred locations for electronegative heteroatoms based on simple atomic charge distributions calculated for a common isostructural, isoelectronic, but homoatomic analog.2'3 Other authors have also predicted the order of stabilities of carborane isomers using empirical valence t h e~r y~-~ or a fragment molecular orbital a p p r o a~h .~ Although our predictions agree with all available experimental evidence we were able to assess the relative stabilities of many higherenergy isomers which are unknown experimentally. Therefore, to test our qualitative predictions, we have performed ab initio SCF MO calculations for each case.…”
Section: Introductionmentioning
confidence: 99%
“…32,36,[40][41][42] At least Si 4 C 2 H 2 , and perhaps other members of this series of clusters is very probable to exist in interstellar space. 32,36,[40][41][42] At least Si 4 C 2 H 2 , and perhaps other members of this series of clusters is very probable to exist in interstellar space.…”
Section: Discussionmentioning
confidence: 99%
“…32,36,[40][41][42] At least Si 4 C 2 H 2 , and perhaps other members of this series of clusters is very probable to exist in interstellar space. [40][41][42] It would be perhaps interesting to further investigate the extent of this "dramatic" similarity, at least in three possible directions: ͑1͒ in the direction of increasing n, ͑2͒ in the direction of the possible electrophylic substitutions ͑in analogy to carboranes͒, and ͑3͒ toward other possible similar species, such as C 4 Si n H 4 in analogy to C 4 B n H n+4 . By removing the H atoms and reoptimizing the geometry, the lowest energy structures of the corresponding nonhydrogenated clusters can be obtained ͑not from the global energy minimum structure͒.…”
Section: Discussionmentioning
confidence: 99%
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