C. Femoni, M. C. Iapalucci, G. Longoni, S. Zacchini
FULL PAPER
trumOne interferometer in CaF2 cells. 1H NMR spectra were re-
corded with a Varian Mercury 400 MHz spectrometer, and refer-
enced to internal TMS. The structure figures were drawn with
Concluding Remarks
The calculated average radius of the interstitial Ga atoms
in the title icosahedral compounds is comprised in the nar- SCHAKAL99.[21] EHMO calculations have been carried out with
CACAO.[14]
row 1.20–1.21 Å range of values, which is very close to the
accepted covalent radius of Ga (1.22 Å)[19] and corresponds
[NnBu4]3[Ni14.3Ga(CO)24.3]:
A
solution of GaCl3 (0.37 g,
to ca. 91% of the radii of the surrounding Ni atoms. There-
fore, both steric and electronic (viz. the above EHMO dia-
gram) factors seemed favourable but turned out to be not
sufficient to grant multivalence, as well as stability in a dif-
2.10 mmol) in dichloromethane (20 mL) was added in portions to
[NnBu4]2[Ni6(CO)12] (1.85 g, 1.58 mmol) dissolved in dichlorome-
thame (50 mL) with stirring. The mixture was left to react for 24 h,
until IR monitoring showed disappearance of [Ni6(CO)12]2– from
ferent ligand shell, to the [Ni12(µ12-Ga)(CO)22]3– icosahe- solution. The resulting dark-brown suspension was evaporated to
dral cluster, as it instead occurs for [Ni11(µ6-E)2(CO)18]4– (E
dryness and washed with water (3ϫ15 mL) and isopropyl alcohol
= Sb, Bi) and [Rh12(µ12-Sn)(CO)25]4–.
(2ϫ20 mL). The residual brown material was extracted in dichlo-
romethane (20 mL) and Ni(CO)4 (0.2 mL) was added. Precipitation
The difference between Ni-centred and E-centred Ni
by slow diffusion of isopropyl alcohol (60 mL) gave dark-brown
clusters is particularly striking. In spite of their different
crystals of [NnBu4]3[Ni14.3Ga(CO)24.3]·2CH2Cl2 (yield 0.654 g,
compositions, the two architectures feature identical num-
bers of Ni–Ni (30, dotted bonds in Figure 6) and Ni–E (12,
blackened bonds) interactions and similar EHMO dia-
grams. The only noticeable difference between the two
architectures in EHMO calculations is represented by a sig-
39.7% based on Ni). The salt is soluble in CH2Cl2, THF, acetone,
acetonitrile, DMF and DMSO, sparingly soluble in alcohols and
insoluble in nonpolar solvents. IR (CH Cl ): ν = 2009 (s), 1879
˜
CO
2
2
(m, br.), 1822 (sh.) cm–1. [NnBu4]3[Ni14.3Ga(CO)24.3]·2CH2Cl2:
calcd. Ni 33.76, C 35.89, H 4.51, N 1.69; found Ni 33.89, C 35.71,
nificant increase in the average overlap population (OP) of H 4.46, N 1.71.
Ni–E bonds, on going from group 13 or 14 (OP ca. 0.2) to
[NnBu4]3[Ni12Ga(CO)22]: Solid [NnBu4]3[Ni14.3Ga(CO)24.3] (0.521 g,
group 15 (OP ca. 0.3) elements. Besides, in all cases, the
umbrella sticks of geometry A in Figure 6 show ca. 45% of
the rib’s OP, whereas the opposite trend is observed in B.
0.21 mmol) was dissolved in dichloromethane (30 mL) in a 200-mL
flask and stirred under a static carbon monoxide atmosphere. The
initial dark red-brown colour of the solution slowly turned green-
brown. The resulting solution was evaporated to dryness to elimin-
ate Ni(CO)4, and the residue was dissolved in dichloromethane
(15 mL). Precipitation by diffusion of isopropyl alcohol (30 mL)
gave [NnBu4]3[Ni12Ga(CO)22]·2CH2Cl2 within a few days as brown
crystals (0.39 g, 68.2% based on Ni). The salt is soluble in CH2Cl2,
THF, acetone, acetonitrile, DMF and DMSO, sparingly soluble or
insoluble in alcohols and insoluble in nonpolar solvents. IR
(CH Cl ): ν
= 1999 (s), 1790 (m) cm–1. [NnBu4]3[Ni12Ga-
˜
CO
2
2
(CO)22]·2CH2Cl2: calcd. Ni 30.78, C 37.80, H 4.89, N 1.84; found
Ni 30.91, C 37.73, H 4.72, N 1.82.
Figure 6. Schematic structure of [Ni12(µ12-E)(CO)22]n– and [Ni11(µ6-
E)2(CO)18]n– (E as black spheres), pointing out the Ni–E bonds
acting as sticks and ribs of the two differently oriented (head–head
in A and tail–tail in B) Ni6(µ6-E) umbrella.
[NnBu4]2[HNi12Ga(CO)22]: Solid [NnBu4]3[Ni12Ga(CO)22]·2CH2Cl2
(0.32 g, 0.14 mmol) was dissolved in THF and treated dropwise
whilst stirring with a solution of dilute acid (1 mL of 20% H2SO4
in 5 mL of THF) monitoring the reaction by IR spectroscopy. The
Such a trend formally explains the greater reactivity of resulting brown solution was evaporated under vacuum. The pre-
[Ni12(µ12-E)(CO)22]n– species under a CO atmosphere in
cipitate was washed several times with water and dried. The residue
was extracted in acetone (10 mL) and precipitated by diffusion of
comparison with [Ni11(µ6-E)2(CO)18]n–. In particular,
[Ni12(µ12-Ge)(CO)22]2– is quantitatively degraded by CO at
isopropyl alcohol (20 mL) to obtain black crystals of [NnBu4]2-
[HNi12Ga(CO)22] (0.28 g). The salt is soluble in CH2Cl2, THF, ace-
atmospheric pressure to
a pentagonal antiprismatic
tone, acetonitrile, DMF and DMSO and insoluble in nonpolar sol-
[Ni10(µ10-Ge)(CO)20]2–.[6] It may therefore be speculated
that the trend of Ni–E OP and the opposite orientation of
their umbrella concur in tightening geometry B and explain
the different stability of the above geometries also upon a
redox change.
vents. The compound is deprotonated to [Ni12Ga(CO)22]3– both in
1
DMF and DMSO. H NMR ([D6]acetone, 293 K): δ = –13.5 ppm.
IR (acetone): ν
= 2025 (s), 1826 (m) cm–1. [NnBu4][HNi12-
˜
CO
Ga(CO)22]: calcd. Ni 37.53, C 34.56, H 3.89, N 1.49; found Ni
37.46, C 34.49, H 3.91, N 1.47.
X-ray Crystallographic Studies: Crystal data and collection details
for [NnBu4]3[Ni12Ga(CO)22]·2CH2Cl2, [NnBu4]2[HNi12Ga(CO)22]
and [NnBu4]3[Ni14.3Ga(CO)24.3]·2CH2Cl2 are reported in Table 2.
The diffraction experiments were carried out with a Bruker APEX
II diffractometer equipped with a CCD detector by using Mo-Kα
radiation. Data were corrected for Lorentz polarization and ab-
sorption effects (empirical absorption correction SADABS).[22]
Structures were solved by direct methods and refined by full-matrix
least-squares based on all data using F2.[23] Hydrogen atoms were
fixed at calculated positions and refined by a riding model. All
Experimental Section
General: All reactions and sample manipulations were carried out
by using standard Schlenk techniques under a nitrogen atmosphere
and in dried solvents. The [Ni6(CO)12]2– salts were prepared accord-
ing to literature methods.[20] Analysis of Ni were performed by
atomic absorption on a Pye-Unicam instrument. Analyses of C,
H and N were obtained with a ThermoQuest FlashEA 1112NC
instrument. IR spectra were recorded with a Perkin–Elmer Spec-
1060
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Eur. J. Inorg. Chem. 2010, 1056–1062