ARTICLE IN PRESS
J. Walker et al. / Journal of Solid State Chemistry 180 (2007) 2290–2297
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NiO [26], Al2O3 [27], Cr2O3, ZrO2, WO3, as well as
numerous other transition metals [28].
the ethanol. (The estimate of 1.6 mmol of Ru was
calculated by using the exact formula of the Ru precursor,
RuCl3.37 ꢀ 2.5H2O, having a molecular weight of 265.6 g/
mol, which was obtained after performing elemental
analysis on the as-bought RuCl3 ꢀ xH2O salt. However,
the commercially available hydrated ruthenium-(III) chlor-
ide is a mixture of several phases, including the hydrate of
ruthenium-(IV) oxide derivatives [29].) Then a 1.2 mL
allotment of the weak base, propylene oxide, was added as
the gelation chemical to the solution and stirred. The time
to gelation was monitored and recorded after the addition
of the gelation chemical. After gelation occurred, the gel
was covered and allowed to age for 24 h. Then the aged gel
was allowed to dry in a fume hood under ambient
conditions to allow solvents to evaporate. To complete
solvent evaporation, the sample was placed under vacuum
for an additional 48 h.
Our particular interest in exploiting these properties lies
in the design of metal oxide matrices for energetic
materials. Such energetic materials are comprised of a
particulate metal fuel (e.g., Al, Fe, Cr) closely mixed with
metal oxide particles, which, after a stress-induced oxida-
tion–reduction reaction, result in a substantial exothermic
heat release. In these materials, reactions between different
metal oxide networks (oxidants) and dispersed metallic
particles (fuels) will result in different energetic release
rates. The efficiency of the exothermic output of the
energetic reaction is also governed by the interfacial area
and reactivity between the metal fuel and the metal oxide
particles and hence, reducing the size of the metal oxide
(oxidant) network as well as the size of the particulate
metal fuel to the nanometer scale, will dramatically
increase the interfacial area and will directly translate into
a higher efficiency of the oxidation–reduction reaction.
In this work, we extend the sol–gel synthesis of hydrous
ruthenium oxide involving the addition of an epoxide, e.g.,
propylene oxide, to a hydrated ruthenium chloride
precursor solution, to generate a porous ruthenium oxide
xerogel with nanoscale dimensions of the oxide particles.
Unlike the work of Suh et al. [13] that is specifically
focusing on the formation of highly porous ruthenium
oxide aerogels by carbon dioxide supercritical drying, our
interest lies mainly in the formation and thermal behavior
of the denser xerogel material. In view of the potential
application of such oxides as energetic materials, the main
factor of interest in our case is the possibility of formation
of tight reactive interfaces between the ruthenium oxide
‘‘nanonetwork’’ and the fuel nanoparticles, and the
influence of the increase in the local temperature on
the chemistry of the reactants. Despite the fact that the
electronic configuration of Ru is similar to that of Fe,
the chemistry of its oxides bears little resemblance to that
of iron. While there is extensive chemistry associated with
the MxOy (M ¼ Fe or Ru) species for both elements, the
higher oxidation states of Ru are much more easily
obtained than for iron. Hence, in this paper, we set out
to probe the synthesis, thermal stability, and reactivity of
hydrous ruthenium oxide nanonetworks as the potential
oxidation moiety in energetic materials systems.
2.2. Physical characterization of synthesized material
The dried xerogel material was ground into a fine
powder using a ceramic mortar and pestle. XPS scans of
powder samples were taken using a Surface Science
Laboratories SSX-100 ESCA Spectrometer using mono-
chromatic AlKa radiation (1486.6 eV). The system oper-
ated at a pass energy of 50 eV. Powder samples were
housed in aluminum foil during analysis and a flood gun
was used at a voltage of 3 eV. The operating pressure of the
vacuum chamber was less than 3 ꢂ 10ꢃ8 Torr. General
scans covered the binding energy range of 0–1100 eV.
Thirty high-resolution C(1s)/Ru(3d5/2) scans were run with
a central binding energy (CBE) of 285 eV with a window
width of 20 eV at a spot size of 400 mm. Also, 30 high-
resolution O(1s) scans were run at a CBE of 532 eV using a
spot size of 400 mm and a window width of 20 eV. Each
high-resolution scan possessed a 0.1 eV per step interval.
Curve fitting of the data was accomplished using the
program Spectral Data Processor, Version 4.1.
XRD of the samples was performed on a Philips PW
1800 X-ray diffractometer. Patterns from 201 to 851 were
examined with a step size of 0.021 using monochromatic
˚
CuKa X-rays with a wavelength of 1.54056 A. Powder
samples were analyzed using a zero background sample
holder.
HRTEM images were obtained from a Hitachi HF 2000
FE TEM operating at an accelerating voltage of 200.0 keV.
Elemental analysis of the material was performed by
Atlantic Microlabs, Norcross, GA. Quantitative values of
carbon, hydrogen, oxygen, and chlorine were determined
through experimental measures. The balance of the
compositional make-up of the sample was assigned as
ruthenium. Lower temperature DSC data were compiled
from a TA Instruments Q100 DSC up to temperatures of
550 1C. Samples were placed in aluminum pans and heated
at 10 1C/min with a nitrogen purge at 20.00 mL/min. High-
temperature DTA/TGA data (4600 1C) was determined
using a Netzsch STA 449-Jupiter TGA-DSC. Powder
2. Experimental
2.1. Synthesis of hydrous ruthenium oxide gels
Ruthenium-(III) chloride hydrate, RuCl3 ꢀ xH2O; and
propylene oxide, C3H6O, were purchased from Fisher
Scientific and used as received. Stock absolute ethanol was
obtained from Aldrich and used as received. The synthesis
was performed in a 20 mL glass scintillation vial under
ambient conditions by adding 0.42 g (1.6 mmol) RuCl3 ꢀ
xH2O to 3.5 mL of ethanol and stirring until the powdered
ruthenium chloride component was completely dissolved in