Table 1 Results of the EDA calculations of complex 3a using (1Dg)
Sn2 and 2 :C{N(Me)C(H)}2 as interacting fragments. The energy
values are given in kcal molꢀ1 (C2h symmetry)
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DEint
DEPauli
DEelstat
DEOrb
DE(ag)
DE(bg)
DE(au)
DE(bu)
ꢀ84.1
251.3
ꢀ213.6
ꢀ121.2
ꢀ56.6
ꢀ1.5
(63.7%)
(36.3%)
(46.3%)
(1.3%)
(6.6%)
(45.5%)
ꢀ8.1
ꢀ55.7
DEprep (NHC)
DEprep (Sn2)
6.5
15.7
ꢀDe (X3Sꢀ
)
g
ꢀ61.9
the DEorb term was obtained. The major contribution comes
from plus (46.3%) and minus (45.5%) combinations of the
carbon lone-pair orbitals (C-Sn), while donation from the
occupied out of plane p MO of Sn2 into the empty p(p) orbitals
of the carbene carbon atoms (DE(au)) provides only 6.6% of
DEorb. Therefore, there is apparently very little Sn-C p-back-
bonding occurring in 3a.
In conclusion, the first NHC complex of a row 5 element (viz.
tin) in its diatomic form has been prepared. A combination of
spectroscopic, crystallographic and computational analyses of the
diamagnetic compound indicate that it is best considered as an
NHC adduct of the singlet state, doubly bonded tin(0) fragment,
:SnQSn:. Because the compound decomposes at close to room
temperature in solution and the solid state, yielding tin metal, it
has potential to act as a soluble source of elemental tin in its
further reactions. We are exploring this potential, in addition to
using more sterically hindered NHCs in attempts to prepare
isolable lead(0) dimers of the type, [(NHC)PbPb(NHC)].
CJ and AS gratefully acknowledge financial support from
the Australian Research Council. GF thanks the Deutsche
Forschungsgemeinschaft.
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19 As determined from a survey of the Cambridge Crystallographic
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obtain the crystalline form of [(IPr)GeQGe(IPr)]
2 that is
isomorphous to 3, to allow more direct structural comparisons
between the compounds. While this was not successful, two new
structural modifications of 2 were obtained (see ESIw for details).
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current study is 15.6 kcal molꢀ1
.
c
This journal is The Royal Society of Chemistry 2012
Chem. Commun., 2012, 48, 9855–9857 9857