662 Inorganic Chemistry, Vol. 40, No. 4, 2001
Table 1. Crystallographic Data for 1
Mitzel et al.
and vibrational frequency calculations were performed from analytic
first and second derivatives at the SCF and MP2 levels of theory.
Different basis sets of increasing size were employed, namely, the
standard basis sets 3-21G(d), 6-31G(d), and 6-31G(d,p) as well as the
more extended 6-311G(d,p) basis set.14 For calculations involving tin
atoms 3-21G(d) and a basis set of double-ú quality by Dunning were
employed.15
C2H9NOGe
fw 135.69
space group Pnma
T ) 153(2) K
λ ) 0.71073 Å
Fcalc ) 1.616 g cm-3
5.350 mm-1
a ) 8.1280(12) Å
b ) 9.7037(15) Å
c ) 7.0722(12) Å
V ) 557.8(2) Å3
Z ) 4
R1(Fo) ) 0.0249
2
wR2(Fo ) ) 0.0638
Results and Discussion
The stoichiometrically simple N,N-dimethylaminoxygermane,
H3GeONMe2 (1), was prepared from bromogermane and N,N-
dimethylaminoxy lithium (eq 1). Due to the instability of
monohalogenogermanes, the preparation of N,N-dimethylami-
noxygermane (1) had to be conducted at -96 °C. Dimethyl ether
(bp -24 °C) was advantageously applied as a solvent, as its
volatility exceeds that of all starting materials and products and
thus allows complete separation. H3GeONMe2 is obtained as a
To reduce the steric and electronic influences at the germa-
nium center, we decided to study the simplest possible GeON
compound that can be prepared, H3GeONMe2. The absence of
steric repulsion in this compound and its C, Si, and Sn
homologues allows comparison of the E‚‚‚N distances and
E-O-N angles and so the assessment of the influence of the
group 14 atom on the molecular structure of the E-O-N units.
Experimental Section
H3GeBr + LiONMe2 f LiBr + H3GeONMe2
(1)
General. The experiments were carried out using a standard Schlenk
line or a vacuum line with greaseless stopcocks (Young taps), directly
attached to the gas cell in an FTIR spectrometer (Midac Prospect FTIR).
All NMR spectra were recorded at 21 °C on a JEOL JNM-LA400 spec-
trometer in sealed tubes with C6D6 as solvent directly condensed onto
the sample from K/Na alloy. Bromogermane was prepared according
to a literature procedure from GeH4 and HBr in the presence of AlBr3.8
(N,N-Dimethylaminoxy)germane (1). At -50 °C n-butyllithium
(0.3 g, 5 mmol, 1.8 M in hexane) was added dropwise to a solution of
N,N-dimethylhydroxylamine (0.6 mL, 0.5 g, 8 mmol) in pentane (25
mL). The mixture was slowly warmed to ambient temperature, and
all volatiles were pumped off. Dimethyl ether (30 mL) and 0.86 g
of bromogermane (5.5 mmol) were condensed onto the remaining
LiONMe2 (0.33 g, 4.9 mmol). The mixture was stirred for 10 h at -96
°C while H3GeBr was carefully washed off the flask wall. (N,N-
Dimethylaminoxy)germane was isolated in low yield as a colorless,
air and temperature sensitive liquid (mp -22 °C) by fractionated
condensation through a series of cold traps held at -20, -96, -196
colorless liquid in moderate yield by trap-to-trap distillation. It
is highly sensitive to air and unstable at ambient temperature.
Decomposition of the compound can be observed even near
the melting point of -22 °C by the occurrence of a yellow-
brownish color and later by formation of a red-brown precipitate.
The compound has been identified by gas-phase IR spec-
troscopy and NMR spectroscopy of the nuclei 1H, 13C, 15N, and
17O. The Ge-H stretching vibrational mode corresponds to an
absorption at 2101 cm-1 in the IR spectrum, and correct relative
intensities of the proton signals and the occurrence of the
expected quartet of quartet splitting in the proton-coupled 13C
NMR proved the identity of H3GeONMe2. An attempt to record
a
73Ge NMR spectrum failed as well as attempts to obtain a
mass spectrum and a reliable elemental analysis.
Despite having the different elements bound to the ONMe2
unit, the 15N and 17O NMR chemical shifts of H3GeONMe2
(-234.0 and 112 ppm) and H3SiONMe2 (-237.9 and 113
ppm)16 are surprisingly similar. This indicates that the bonding
situations in the two compounds are similar.
The decomposition of H3GeONMe2 can be monitored by
recording proton NMR spectra at suitable time intervals. Figure
1 displays two spectra of a freshly prepared sample in C6D6
°C. The product was retained in the -96 °C trap. 1H NMR: δ ) 2.41
1
(s, 6H, H3C), 5.11 (s, 3H, H3Ge). 13C NMR: δ ) 49.6 (q q, JCH
)
3
134.4 Hz, JCNCH ) 5.7 Hz, CH3). 15N{1H} NMR: δ ) -237.9 (s).
17O{1H} NMR: δ ) 113 (s). IR (gas): 2101 cm-1 (s, νGeH).
Crystal Structure Determination of 1. A single crystal of 1 was
grown in situ by slowly cooling the melt in sealed capillaries after
generation of a suitable seed crystal. The crystal and refinement data
are listed in Table 1.
Gas-Phase Electron Diffraction of 1. Electron scattering intensity
data for 1 were recorded on Kodak Electron Image plates using the
Edinburgh electron diffraction apparatus and a wavelength of 0.06016
Å.9 Scattering data for benzene were recorded concurrently and used
to calibrate the electron wavelength and camera distances. Three
exposures were taken at each camera distance. Data were obtained in
digital form using the microdensitometer at the Institute of Astronomy
at Cambridge.10 The data analysis followed standard procedures, using
established data reduction and least-squares refinement programs11 and
the scattering factors established by Fink and co-workers.12 The
experimental conditions are summarized in Table 2. The refined
molecular parameters, their definitions and the applied restraints, a list
of selected interatomic distances including vibrational amplitudes and
applied restraints, and elements of the correlation matrix are given in
Tables 2, 4, and 6.
(12) Ross, A. W.; Fink, M.; Hilderbrandt, R. In International Tables for
X-Ray Crystallography; Wilson, A. J. C., Ed.; Kluwer Academic
Publishers: Dordrecht, Boston, 1992; Vol. C., p 245.
(13) Frisch, M. J.; Trucks, G. W.; Schlegel, H. B.; Scuseria, G. E.; Robb,
M. A.; Cheeseman, J. R.; Zakrzewski, V. G.; Montgomery, J. A., Jr.;
Stratmann, R. E.; Burant, J. C.; Dapprich, S.; Millam, J. M.; Daniels,
A. D.; Kudin, K. N.; Strain, M. C.; Farkas, O.; Tomasi, J.; Barone,
V.; Cossi, M.; Cammi, R.; Mennucci, B.; Pomelli, C.; Adamo, C.;
Clifford, S.; Ochterski, J.; Petersson, G. A.; Ayala, P. Y.; Cui, Q.;
Morokuma, K.; Malick, D. K.; Rabuck, A. D.; Raghavachari, K.;
Foresman, J. B.; Cioslowski, J.; Ortiz, J. V.; Baboul, A. G.; Stefanov,
B. B.; Liu, G.; Liashenko, A.; Piskorz, P.; Komaromi, I.; Gomperts,
R.; Martin, R. L.; Fox, D. J.; Keith, T.; Al-Laham, M. A.; Peng, C.
Y.; Nanayakkara, A.; Gonzalez, C.; Challacombe, M.; Gill, P. M. W.;
Johnson, B.; Chen, W.; Wong, M. W.; Andres, J. L.; Gonzalez, C.;
Head-Gordon, M.; Replogle, E. S.; Pople, J. A., Gaussian 98, revision
A.7; Gaussian, Inc.: Pittsburgh, PA, 1998.
(14) (a) Binkley, J. S.; Pople, J. A.; Hehre W. J. J. Am. Chem. Soc. 1980,
102, 939. (b) Gordon, M. S.; Binkley, J. S.; Pople, J. A.; Pietro, W.
J.; Hehre W. J. J. Am. Chem. Soc. 1982, 104, 2797. (c) Pietro, W. J.;
Francl, M. M.; Hehre, W. J.; Defrees, D. J.; Pople, J. A.; Binkley J.
S. J. Am. Chem. Soc. 1982, 104, 5039. (d) 6-31G(d): Hariharan, P.
C.; Pople J. A. Theor. Chim. Acta 1973, 28, 213. (e) Hariharan, P. C.;
Pople, J. A. Chem. Phys. Lett. 1972, 66, 217. (f) 6-311G(d): Krishnan,
R.; Frisch, M. J.; Pople, J. A. Chem. Phys. 1980, 72, 4244.
(15) Dunning, T. H. Unpublished work.
Ab Initio Calculations. Ab initio molecular orbital calculations were
carried out using the Gaussian 98 program.13 Geometry optimizations
(8) Dennis, L. M.; Judi, P. R. J. Am. Chem. Soc. 1929, 51, 2321.
(9) Huntley, C. M.; Laurenson G. S.; Rankin, D. W. H. J. Chem. Soc.,
Dalton Trans. 1980, 945.
(10) Lewis, J. R.; Brain P. T.; Rankin, D. W. H. Spectrum 1997, 15, 7.
(11) Mitzel, N. W.; Brain, P. T.; Rankin, D. W. H. ED96, version 2.0,
1998. A program developed on the basis of formerly described ED
programs: Boyd, A. S. F.; Laurenson, G. S.; Rankin, D. W. H. J.
Mol. Struct. 1981, 71, 217.
(16) Mitzel, N. W.; Losehand, U. Angew. Chem., Int. Ed. Engl. 1997, 36,
2807.