[B30]−: A Quasiplanar Chiral Boron Cluster
Chirality is vital in chemistry. Its importance in atomic clusters has been recognized since the discovery of the first chiral fullerene, the D2 symmetric C76.1 A number of gold clusters have been found to be chiral,2 raising the possibility to use them as asymmetric catalysts. The discovery of clus...
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Published in | Angewandte Chemie International Edition Vol. 53; no. 22; pp. 5540 - 5545 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Weinheim
WILEY-VCH Verlag
26.05.2014
WILEY‐VCH Verlag Wiley Subscription Services, Inc |
Edition | International ed. in English |
Subjects | |
Online Access | Get full text |
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Summary: | Chirality is vital in chemistry. Its importance in atomic clusters has been recognized since the discovery of the first chiral fullerene, the D2 symmetric C76.1 A number of gold clusters have been found to be chiral,2 raising the possibility to use them as asymmetric catalysts. The discovery of clusters with enantiomeric structures is essential to design new chiral materials with tailored chemical and physical properties.3 Herein we report the first inherently chiral boron cluster of [B30]− in a joint photoelectron spectroscopy and theoretical study. The most stable structure of [B30]− is found to be quasiplanar with a hexagonal hole. Interestingly, a pair of enantiomers arising from different positions of the hexagonal hole are found to be degenerate in our global minimum searches and both should co‐exist experimentally because they have identical electronic structures and give rise to identical simulated photoelectron spectra.
Holey chiral: The [B30]− cluster was characterized by photoelectron spectroscopy and ab initio calculations. A pair of planar structures with a hexagonal hole at different positions are found to be degenerate with identical electronic structures. These two isomers are enantiomers, suggesting that [B30]− is the first chiral boron cluster. |
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Bibliography: | NKBRSF - No. 2011CB932401 U.S. National Science Foundation - No. CHE-1263745 This work was supported by the U.S. National Science Foundation (CHE-1263745 to L.S.W) and NKBRSF (2011CB932401) and NSFC (21221062, 91026003) of China. The calculations were performed using the Supercomputer Center of the Computer Network Information Center, Chinese Academy of Sciences and the Shanghai Supercomputing Center. NSFC - No. 21221062; No. 91026003 ark:/67375/WNG-0D75KNMT-M istex:1DBF365ACD9871A2BF3485BF871AB1D3FD702EBD ArticleID:ANIE201402488 This work was supported by the U.S. National Science Foundation (CHE‐1263745 to L.S.W) and NKBRSF (2011CB932401) and NSFC (21221062, 91026003) of China. The calculations were performed using the Supercomputer Center of the Computer Network Information Center, Chinese Academy of Sciences and the Shanghai Supercomputing Center. ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
ISSN: | 1433-7851 1521-3773 |
DOI: | 10.1002/anie.201402488 |