Germanium Nanowires
A R T I C L E S
(VLS) growth,20 templated supercritical fluid,21-24 and combina-
tion of these techniques. The VLS technique is most widely
used among these methods. Modified VLS techniques, such as
solution-liquid-solid (SLS) and supercritical-fluid-liquid-
solution (SFLS)6,25-27 growth techniques, have also been
developed. While these routes can yield Ge0 nanowires, they
require the use of metal catalysts (e.g., Au0 or Fe0) or
nonmetallic, high-boiling-point catalysts (e.g., trioctylamine) as
seed materials to initiate the growth and to define the growth
direction of Ge0 nanowires.28,29 Also, the use of high temperature
and pressure coupled with the volatility of the precursor could
be potentially hazardous.21 For the synthetic routes described
above, the typical Ge precursors are in the +4 oxidation state,
such as GeH4, GeI4,7 Ge(CH3)4,6 or GexFe1-x alloy.19 More
recently, a Ge precursor in the +2 oxidation state has found
utility in a CVD and SLS systems, using Fe0 or Bi0 as the
catalyst material.18,30 Despite the success of producing Ge0
nanowires by these techniques, the presence of foreign seed
particles adds complexity to the production of pure Ge0
nanowires and influences their electrical and optical properties.
In comparison, select solution routes can be simple and
effective for the production of high-quality Ge0 nanoparticles.
To date, very limited information has been available for the
production of Ge0 nanowires from these solution routes.31,32 One
reported solution route to Ge0 nanowires involves the reduction
of GeCl4 and phenyl-GeCl3 by Na0 in an alkane solvent at
elevated temperature and pressure.8 In this solution route, the
complexity of the reaction as well as the potential contamination
by metal reducing agents and salt byproducts limits the direct
use of the as-produced Ge0 nanowires for novel devices. An
ideal case for the synthesis of Ge0 nanowires would be a simple
synthesis conducted under relatively benign conditions associ-
ated with low pressure, low temperature, and no salt byproduct.
In this paper, we report a solution synthesis of Ge0 nanowires
from a newly characterized Ge2+ precursor, Ge(DBP)2 (1),
where DBP represents 2,6-OC6H3(C(CH3)3)2. Our approach
hinges on molecularly designed precursors to control their
reactivity and resulting nanostructure morphology. This con-
ceptual approach has been introduced in the synthesis of several
other systems, such as CdSe,33 PbSe, and Au.34,35 Previously,
we described the utility of Ge(N(SiMe3)2)2 to produce Ge0
nanocrystals.31 Herein, we tailor the precursor reactivity by the
use of 1 to form Ge0 nanowires. The synthesis and characteriza-
tion of both 1 and the subsequent Ge0 nanowires are described
below.
Experimental Details
The synthesis was conducted at 285-315 °C under 1 atm of Ar in
a vacuum/Schlenk line setup, typically used for solution synthesis of
nanoparticles and nanowires.36 Note: no metal catalysts were used, and
no salt byproducts were formed. All anhydrous solvents were purchased
in sure-seal bottles. The following chemicals were purchased from
Aldrich and used without further purification: GeCl2‚dioxane, LiN-
(SiMe3)2, and oleylamine. Ge(N(SiMe3)2)2 was synthesized following
literature reports.37
Fourier transform infrared (FTIR) transmission spectra were obtained
on a Bruker Vector 22 spectrometer using KBr pellets pressed under
an Ar atmosphere and handled under an atmosphere of flowing N2.
Elemental analyses were performed on a Perkin-Elmer 2400 CHN-
S/O elemental analyzer. Thermogravimetry analysis and differential
thermal analysis (TGA/DTA) were performed on a TA Instrument STD
2960 at 15 °C/min ramp rate under Ar atmosphere. Nuclear magnetic
resonance (NMR) data were collected on flame-sealed samples dis-
solved in toluene-d8 using a Bruker 250 MHz NMR.
Ge(OC6H3(C(CH3)3)-2,6)2 (1). A solution of DBP-H (0.525 g, 2.54
mmol) dissolved in toluene was slowly added by pipet to a stirring
solution of Ge(N(SiMe3)2)2 (0.500 g, 1.27 mmol) in toluene. The
mixture was heated to 50 °C for 15 min to drive the reaction into
completion and then allowed to cool to room temperature. X-ray quality
pale yellow crystals of 1 were isolated by slow evaporation of the
1
volatile component of the mixture. Yield: 0.335 g (67.0%). H NMR
(400.1 MHz, tol-d8): δ 7.37-7.29 (br m, 3-H, OC6H3(C(CH3)3)2) and
1.54 (s, 18 H, OC6H3(C(CH3)3)2)). 13C{1H} NMR (100.0 MHz, tol-
d8); δ 140.6, 125.9 (partial, OC6H3(C(CH3)3)2), 35.44 (OC6H3-
(C(CH3)3)2), and 32.9 (OC6H3(C(CH3)3)2). FTIR (KBr, cm-1): 3088(s),
2965(sh, s), 2380(s), 2044(s), 1914(s), 1859(s), 1794(s), 1696(s), 1641-
(s), 1578(s), 1469(sh, s), 1414(m), 1359(sh, s), 1316(s), 1218(m), 1109-
(m), 1019(s), 844(m), 746(m), 659(s), and 583(s). Elemental analysis
calculated for C20H26GeO2: 69.59% C and 8.76% H. Found 69.36% C
and 8.78% H.
General X-ray Crystal Structure Information. Using a Bruker
AXS diffractometer, a single crystal of 1 was mounted onto a thin glass
fiber from a pool of Fluorolube and immediately placed under a liquid
N2 stream. The radiation source was graphite-monochromatized Mo
KR (λ ) 0.7107 Å). The lattice parameters were optimized from a
least-squares calculation on carefully centered reflections. Lattice
determination and data collection were carried out using SMART
Version 5.054 software. Data reduction was performed using SAINT
Version 6.01 software. The structure refinement was performed using
XSHELL 3.0 software. The data were corrected for absorption, using
the SADABS program within the SAINT software package. General
collection parameters for 1 are shown in Table 1. Additional information
concerning the structure of these compounds can be found in the
Supporting Information or by accessing the final CIF files through the
Cambridge Crystallographic Data Base.
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The structure was solved using direct methods, which yielded the
heavy atoms, along with a number of the C and O atoms. Subsequent
Fourier synthesis yielded the remaining atom positions. The H atoms
were fixed in positions of ideal geometry and refined within the
XSHELL software. These idealized H atoms had their isotropic
temperature factors fixed at 1.2 or 1.5 times the equivalent isotropic U
of the C atoms to which they were bonded. The final refinement of
each compound included anisotropic thermal parameters on all non-
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