Exohedral η5 and η6 transition-metal organometallic complexes of C60 and C70: a theoretical study

Jemmis, Eluvathingal D. ; Manoharan, Mariappan ; Sharma, Pankaz K. (2000) Exohedral η5 and η6 transition-metal organometallic complexes of C60 and C70: a theoretical study Organometallics, 19 (10). pp. 1879-1887. ISSN 0276-7333

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Official URL: http://pubs.acs.org/doi/abs/10.1021/om9905355?prev...

Related URL: http://dx.doi.org/10.1021/om9905355

Abstract

Suitable transition-metal fragments are proposed to overcome the unfavorable interaction arising from the splayed out π-orbitals of the five- and six-membered rings of C60 and C70 in complex formation. Computations carried out at the semiempirical PM3(tm) level on a series of C60MCnHn and C70MCnHn complexes suggest that it is possible to stabilize η6 complexes of C60 and C70 using appropriate transition-metal fragments. Isodesmic equations of the type CmHmMCnHn + Ck → CkMCnHn + CmHm, where k = 60, 70, m = 5, 6, and n = 3-6, indicate that C3H3Co and C3H3Rh are ideal fragments for stabilizing η6-C60 complexes. Model studies at HF/LANL2DZ and B3LYP/LANL2DZ levels on C6H6MLn complexes with C6H6 constrained so as to mimic the C60 geometry support these results. Single-point calculations at these same levels on complexes of sumanene (C21H12) using geometry optimized at the PM3(tm) method also lead to similar conclusions. η5 complexes are less favorable in comparison; structural modifications such as those in the recently synthesized C60Ph6 should readily help in η5 bonding. However, the difficulty of formation of the mononuclear η5-C60MLn complex is reduced considerably if all 12 five-membered rings are used in η5 bonding as in C60(NiC3H3)12. For C70, however, the stability of the exohedral complexes depends on the position and curvature of the five- and six-membered rings. Capping on the flattest six-membered face leads to maximum stability.

Item Type:Article
Source:Copyright of this article belongs to American Chemical Society.
ID Code:13515
Deposited On:12 Nov 2010 15:26
Last Modified:04 Jun 2011 06:09

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