Communications
residue extracted with hexane (25 mL). Filtration, concentration to
approximately 10 mL, and storage at 58C afforded bright yellow
crystals suitable for X-ray analysis (0.29 g, 49%). Elemental analysis
calcd (%) for C24H31InN2O: C 60.26, H 6.55, N 5.86; found: C 62.26, H
HOMO is a bu orbital that is nonbonding with regard to In–In
contact. The degenerate HOMO-1 and -2 provide a level of
p overlap between the indium centers and the nitrogen donor
atoms of the chelated ligands. The HOMO-3 is an In–In s-
bonding orbital of Ag symmetry. This ag orbital thus provides
the primary bonding interaction between the metal centers.
This view of the metal–metal bonding within 6 is qualitatively
similar to that which has been evinced for alkene analogues of
the heavier Group 14 elements and some multiply bonded
gallium species.[1,9–13,27] The bu HOMO in these cases has been
variously interpreted as a “slipped” p bond or as possessing
lone-pair or even antibonding character. Experimental and
theoretical studies of heavier Group 14 R2EER2 species
indicate that, despite increased lone-pair character with
increased atomic mass of E, the p-bonding bu HOMO acts
to provide a minor augmentation of the overall bonding
interaction between the metal centers.[1] A similar rationale
has been applied to the recently completed series of REER
derivatives.[4] The data presented herein and the somewhat
limited literature precedents highlight some notable contrasts
within Group 13. The experimental data indicate that In–In
bonding with p character within 6 is feeble at best, or indeed
destructive. A further calculation based on the separation of
[{In[(N(H)C(H)]2CH}2] into two singlet indanediyl fragments
provided a bond-dissociation energy of only 2 kcalmolꢀ1. This
extremely low value is commensurate with values calculated
(ca. 3 kcalmolꢀ1) for the separation of the two {InH} frag-
ments of [In2H2] and suggests that the notion of “multiple
bonding” within molecules such as 6 is fallacious if the only
expectation is an augmentation of the overall bond
strength.[28] The weakness of the Ga–Ga bonding within the
neutral complex [{(2,6-dipp)2C6H3Ga}2] was similarly attrib-
uted to the large energy difference between the lone pair on
the singlet Gai center and the p orbitals.[14] This situation is
likely to be exacerbated in the current case by N–In
p interactions within the planar b-diketiminato chelates and
indicates that the “multiple bonding” present within 6
actually represents an overall bond order of less than unity.
This view of the HOMO within homonuclear bonding in
Group 13 elements has been emphasized previously by
calculations carried out on the hypothetical cationic species
[MeGaGaMe]+.[11] In this case, removal of an electron from
the bu HOMO of [MeGaGaMe] caused a decrease of
1
5.47, N 5.42 (partially decomposed in transit); H NMR (270 MHz,
3
[D6]benzene, 258C): d = 1.14 (d, 6H, JHH = 6.9 Hz; CH(CH3)2), 1.21
3
(d, 6H, JHH = 6.9 Hz; CH(CH3)2), 1.75 (s, 3H; CCH3), 1.90 (s, 3H;
3
CCH3), 3.20 (m, 2H, JHH = 6.9 Hz; CH(CH3)2), 3.25 (s, 3H; OCH3),
5.06 (s, 1H; CH), 6.50 (d, 1H; ArH), 6.88–6.96 (m, 2H; ArH), 7.15–
7.16 ppm (m, 4H; ArH); 13C{1H} NMR (125.8 MHz, [D6]benzene):
d = 23.8 (CH(CH3)2), 25.7 (CCH3), 28.2 (CH(CH3)2), 28.6 (CH-
(CH2)2), 55.1 (OCH3), 98.7 (g-CH), 111.8, 121.3, 123.3, 123.9, 124.5,
125.2, 125.5, 125.8, 126.7, (ArH) 142.3 (o-C(dipp)), 145.2 (i-C(dipp)),
155.6 (i-Ar-2-OCH3), 163.6 (CN), 163.9 ppm (CN).
6: This compound was made by the same general method
employing III-H (0.69 g, 2.07 mmol), InI (0.50 g, 2.07 mmol), and
KN(SiMe3)2 (0.42 g, 2.10 mmol) to afford pale yellow rectangular
crystals suitable for X-ray analysis (0.42 g, 45%). Elemental analysis
(%) calcd for C46H58In2N4: C 61.62, H 6.53, N 6.25; found: C 61.68, H
6.47, N 6.18; 1H NMR (500 MHz, [D6]benzene, 258C): d = 1.59 (s, 6H;
CCH3), 2.03 (s, 12H; o-CH3), 2.12 (s, 6H; p-CH3), 4.92 (s, 1H; CH),
6.76 ppm (s, 4H; m-ArH); 13C{1H} NMR (125.8 MHz, [D6]benzene):
d = 19.3 (o-CH3), 20.9 (p-CH3), 23.6 (CCH3), 98.2 (g-CH), 129.5 (m-
ArH), 133.4 (p-Ar), 137.4 (o-Ar), 146.0 (i-Ar), 163.4 ppm (CN).
Data for the X-ray structural analyses of 5 and 6 were collected
on a KappaCCD diffractometer (l(MoKa) = 0.71073 ꢀ), solved by
direct methods (SHELXS-97), and refined against all F2 using
SHELXL-97) with non-hydrogen atoms anisotropic and hydrogen
atoms in riding mode. An absorption correction (MULTISCAN) was
applied. For 5, the diffraction was weak and limited in extent.
Crystallographic data for 5 (C24H31InN2O) at 173(2) K: Mr = 478.33,
crystal dimensions 0.25 ꢁ 0.10 ꢁ 0.05 mm3, orthorhombic, space group
P21212 (no. 18), a = 11.6183(8), b = 22.8982(14), c = 8.7686(6) ꢀ, V=
2332.8(3) ꢀ3, Z = 4, 1calcd = 1.36 Mgmꢀ3, m = 1.03 mmꢀ1; of 10481
reflections measured (3.41 < q < 23.268), 3304 were independent
(Rint = 0.067); wR2 = 0.253 (all data), R1 = 0.100 (for 2765 reflections
with I > 2s(I)), 254 parameters, GOF = 1.114. Crystallographic data
for 6 (C46H58In2N4) at 173(2) K: Mr = 896.6, crystal dimensions 0.10 ꢁ
3
¯
0.10 ꢁ 0.05 mm , triclinic, space group P1 (no. 2), a = 8.6847(3), b =
9.9683(3), c = 13.5822(5) ꢀ, a = 71.003(2), b = 82.758(2), g =
81.907(2)8, V= 1096.67(6) ꢀ3, Z = 1, 1calcd = 1.36 Mgmꢀ3
,
m =
1.09 mmꢀ1; of 17033 reflections measured (3.54 < q < 26.068), 4316
were independent (Rint = 0.053); wR2 = 0.072 (all data), R1 = 0.031
(for 3783 reflections with I > 2s(I)), 241 parameters, GOF = 1.031.
CCDC-264672 and -264673 (5 and 6) contain the supplementary
crystallographic data for this paper. These data can be obtained free
of charge from the Cambridge Crystallographic Data Centre via
Received: March 1, 2005
Published online: June 2, 2005
ꢀ
approximately 0.2 ꢀ in the computed Ga Ga bond length.
Preliminary calculations on the [{In[(N(H)C(H)]2CH}2]+
species indicated a similar and pronounced contraction of
Keywords: carbenoids · Group 13 elements ·
ꢀ
the In In bond length to approximately 3 ꢀ and highlighted
.
indium · metal–metal interactions · multiple bonds
the fact that the bu HOMO may also possess antibonding
character. Experiments to assess the validity of this hypoth-
esis and further studies on the reactivity of these unusual
species are in progress.
[1] a) P. P. Power, Chem. Rev. 1999, 99, 3463; b) P. P. Power, J. Chem.
Soc. Dalton Trans. 1998, 2939.
[2] A. Sekiguchi, R. Kinjo, M. Ichinohe, Science 2004, 305, 1755.
[3] a) P. J. Davidson, M. F. Lappert, J. Chem. Soc. Chem. Commun.
1973, 317; b) D. E. Goldberg, D. H. Harris, M. F. Lappert, K. M.
Thomas, J. Chem. Soc. Chem. Commun. 1976, 261; c) D. E.
Goldberg, P. B. Hitchcock, M. F. Lappert, K. M. Thomas, A. J.
Thorne, T. Fjeldberg, A. Haarland, B. E. R. Schilling, J. Chem.
Soc. Dalton Trans. 1986, 2387.
Experimental Section
5: Precooled THF (20 mL) was added at ꢀ788C to a rapidly stirred
mixture of II-H (0.45 g, 1.25 mmol), InI (0.30 g, 1.25 mmol), and
KN(SiMe3)2 (0.24 g, 1.25 mmol) in the absence of light. The reaction
mixture was stirred for 3 h and allowed to warm to room temperature
to produce a gray slurry. Volatiles were removed and the gray solid
[4] For a review of REER structure and bonding, see: P. P. Power,
Chem. Commun. 2003, 2091.
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ꢀ 2005 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim
Angew. Chem. Int. Ed. 2005, 44, 4231 –4235