Vapor hydration of a simulated borosilicate nuclear waste glass in unsaturated conditions at 50 °C and 90 °C

A. Ait Chaou*a, A. Abdelouasa, Y. El Mendilia, R. Bouakkaza, S. Utsunomiyab, C. Martinc and X. Bourbonc
aSUBATECH, UMR 6457CNRS-IN2P3, Ecole des Mines de Nantes, Université de Nantes, 4 rue Alfred Kastler, BP 20722, 44307 Nantes Cedex 03, France. E-mail: aitchaou@subatech.in2p3.fr
bDepartment of Chemistry, Faculty of Science, Kyushu University, 6-10-1 Hakozaki Higashi-ku, Fukuoka 812-8581, Japan
cFrench National Radioactive Waste Management Agency (ANDRA), 1/7, rue Jean Monnet, Parc de la Croix-Blanche, 92298 Châtenay-Malabry Cedex, France

Received 26th June 2015 , Accepted 10th July 2015

First published on 10th July 2015


Abstract

Vapor hydration of a simulated typical French nuclear intermediate-level waste (ILW) glass in unsaturated conditions has been studied in order to simulate its behaviour under repository conditions before complete saturation of the disposal site. The experiments were conducted for one year at 50 °C and 90 °C and the relative humidity (RH) was maintained at 92% and 95%. The glass hydration was followed by Fourier Transform Infra-Red spectroscopy (FTIR). The surface of the reacted glass was characterised by Scanning Electron Microscopy (SEM) and Transmission Electron Microscopy (TEM). The chemical and mineralogical composition of the alteration products were studied by Energy Dispersive X-ray Spectroscopy (EDX) and μ-Raman spectroscopy, respectively. The glass hydration increased with temperature and RH and led to the formation of a depolymerized gel layer depleted in alkalis. The glass hydration rate decreased with time and remained almost unchanged for the last three months of exposure. Overall, the ILW glass hydration rate was similar to that obtained with the SON68 high-level waste glass.


1. Introduction

In France borosilicate glasses have been considered for high-level and certain intermediate-level waste confinement. Final geological disposal in a deep and stable rock seems to be the best option to guarantee safety over a long period of time. Accordingly, in France the nuclear waste forms are expected to be disposed in Callovo-Oxfordian claystone.

When in contact with an aqueous solution and/or humid air environment, borosilicate glass is subject to chemical attack that results in progressive alteration of the glass matrix. Constituent elements of the glass dissolve into solution, elements initially in the solution diffuse into or are absorbed onto the solid and new phases may appear. These processes lead to the formation of surface layers on the corroded glass. Dissolution kinetics of High Level Waste (HLW) borosilicate glasses in pure water, but also in clayey groundwater have been extensively reported in the literature.1–8 As regards alteration of nuclear glasses, in particular the French inactive SON68 glass, in aqueous media, dedicated studies have identified several alteration steps characterized by different mechanisms: interdiffusion, alteration at the maximal alteration rate (rhydro), slowdown of the alteration rate and a residual alteration rate (rr). Studies of the alteration kinetics of nuclear glasses have long attributed the observed slowdown in the rate to chemical affinity mechanisms (affinity laws).9–11 However, this theory has been called into question.12–14 The mechanism currently taken into consideration by the The French Alternative Energies and Atomic Energy Commission (CEA) is the development of a protective gel forming a diffusion barrier for reactive species.15,16 Silicon retention within the gel is also considered to be one of the parameters affecting the protective properties of the gel layer.17

Studies have also been conducted on ILW borosilicate glass alteration in a cementitious medium.18,19 Depierre et al.18,19 studied the influence of Ca-enriched solution on glass alteration mechanisms and kinetics and the Ca–Si interaction processes. The authors suggest that four main mechanisms control the glass durability depending on the pH, the reaction progress and the Ca concentration. The authors shown that a Ca-enriched solution presents antagonist effects according to the relative importance of these parameters. Strong similarities were noted between glass alteration in a Ca rich high-pH solution and cement hydration. The characterization to determine the properties of the thin passivating layer formed at the glass or cement grain surface, which is assumed to account for the rate-limiting step, is a technical challenge today.20,21 Depierre et al.19 shows that three main factors affect the glass dissolution rate: S/V, the pH and the Ca concentration in solution. The Ca concentration is the most important parameter controlling the growth rate and also the growth mode of C–S–H.22,23

Under deep geological disposal conditions, vapor hydration may be also an important corrosion process of both HLW and ILW nuclear waste glasses in a hydrologically unsaturated geological repository:24 (i) hydrogen production induced by the anoxic corrosion of metallic components in HLW disposal cells is likely to prevent a fast resaturation of the voids within the waste packages; (ii) during the operating period of the ILW disposal zone (up to 100 years), concrete components (waste disposal packages, concrete vaults…) will be ventilated in order to guarantee operating safety and to contribute to the evacuation of residual heat from the waste. In these two cases, the resaturation process will then be very slow and as a consequence, glass vapor hydration may occur before pore water has completely infiltrated the container. However, only a few studies were dedicated to glass vapor hydration.25–31 Recent papers on the vapor hydration of borosilicate glasses have been published by McKeown et al.32,33 and Buechele et al.34 The authors used state-of-art spectroscopic techniques to investigate the glass alteration layer. Hence, Raman and X-ray absorption spectroscopic studies showed that, at high temperature (200 °C) and short time periods (3–20 days), the major hydration product is a depolymerized hydrated altered glass with some crystals of analcime and leucite. Furthermore, Buechele et al.34 and McKeown et al.33 found that during vapor hydration tests of a technetium-doped glass, Tc7+ was largely reduced into highly immobile Tc4+.

In the presence of water vapor, an aqueous film is formed on the glass surface, whose thickness depends on the relative humidity, the composition of the glass and its surface condition. The alteration of glass by water vapor leads also to rapid precipitation of secondary phases, but the thickness of the hydrated glass is lower compared to the alteration in liquid water.28 According to the studies carried out on the alteration kinetics of U.S. nuclear glasses by water vapor, the alteration can not begin at relative humidities below 50%.27 Abrajano et al.28 showed that alteration of SRL 131 glass is negligible for a relative humidity of 70%, even at a temperature of 202 °C. In general, the number of layers of water adsorbed on the glass surface changes slightly depending on the relative humidity up to about 80–90% and then increases sharply from 90% leading to a maximum glass hydration.25,26 For this reason, we chose in this study to work under 92% and 95% of relative humidity.

In this work, we studied the vapor hydration of a simulated French ILW nuclear glass under unsaturated conditions and we studied how the exposure to water vapor changes the chemical and/or physical characteristics of the glass surface. The hydration kinetics and the alteration layers were studied. We chose to study both relative humidity 92% and 95% based on the results of the previous studies and two temperatures 50 °C and 90 °C, expected under disposal conditions.

2. Materials and experimental techniques

2.1. Materials and samples preparation

2.1.1. Materials. The inactive surrogate of an ILW nuclear glass (CSD-B glass), also studied by Depierre,18 was provided by The French Alternative Energies and Atomic Energy Commission (CEA) and its composition is given in Table 1 together with that of the SON68 glass (inactive surrogate of the French R7T7 HLW glass) for comparison. The main difference is that the ILW glass is less rich in oxides simulating fission products compared to HLW, but richer in Si, Al and Na oxides.
Table 1 Composition in weight percentage of the simulated French nuclear waste glasses SON68 and CSD-B
Oxide SON68 CSD-B
SiO2 45.1 50.33
B2O3 13.9 14.44
Al2O3 4.9 8.70
Na2O 9.8 12.58
Li2O 2.0 2.17
Cr2O3 0.5 0.07
CaO 4.0 3.10
Fe2O3 2.9 2.84
P2O5 0.3 0.42
ZnO 2.5  
NiO 0.4 0.33
ZrO2   1.99
MoO3   0.69
RuO2   0.12
BaO   0.36
MnO2   0.19
CoO   0.27
SO3   0.19
Oxides (fission products + Zr + actinides) 13.7  
Oxides (fission products + actinides)   0.47
Other   0.74
Total 100 100


Glass monoliths with dimensions of 25 mm × 25 mm × 0.5 mm were cut from a rectangular prism, polished to 3 μm and cleaned with ethanol before use.

2.1.2. Hydration experiments. The hydration experiments were performed in stainless steel autoclaves with a Teflon liner (39 mL). The glass monolith was placed on a Teflon holder that fits into the Teflon liner.29,35 8 mL of saline solution was placed underneath the holder. The autoclave was placed in a 2 cm thick aluminium container to prevent temperature gradients that may cause vapor condensation on the glass sample during the heating and cooling processes. The hydration was conducted at two temperatures, 50 °C and 90 °C. The relative humidity was controlled by varying the concentration of NaCl in the solution. Thus, 92% and 95% of relative humidity were respectively obtained with 13 and 6 weight% of NaCl in the solutions.36 Two types of experiments were conducted: short-term (35 days) and long-term (365 days). A list of all the experiments can be seen in Table 2.
Table 2 Experimental conditions for hydration experiments. The corresponding techniques used to analyse each sample are also listed
Relative humidity (%) Temperature (°C) Alteration time (days) Analytical techniques
92 50 365 FTIR, SEM, EDX, micro-Raman, TEM
92 90 365
95 50 365
95 90 365
92 50 35
92 90 35
95 50 35
95 90 35


Four samplings were conducted in the first month, two the following month and then one sampling every month. To do so, the autoclaves, including the overpack, were removed from the oven and left to cool down for six hours at room temperature. Then, the glass monolith was analysed using Fourier Transform-Infrared (FTIR) spectroscopy. After the FTIR measurements, the monoliths were placed back onto the sample holder. After each sampling, the saline solution was replaced by a fresh one. No significant change of pH or of the mass of the saline solution was observed.

2.2. Characterization techniques

Glass hydration was followed using FTIR Spectroscopy. The glass monoliths, which are transparent to the laser beam, were analysed using a 8400 Shimadzu FTIR between 4000 and 2500 cm−1. This range allowed the observation of the concentration and speciation of water in the glass.37,38 After spectra deconvolution, the error was estimated to 2%.

At the end of the experiments, hydrated glass samples were collected from the reactor and characterised by scanning electron microscope (SEM) (JEOL JSM 5800 LV and 7600 LV, 15 kV). We carried out direct observations of the altered surface to view the crystallised secondary phases. The cross-sectional samples were prepared by polishing cross-sections of cuts perpendicular to the original surface to obtain a large-scale morphological overview, as well as to observe the chemographic relationships of the surface layers and for thickness measurements of the glass alteration layer.

The SEM is coupled with an energy dispersive X-ray spectrometer (EDX), making quantitative chemical analysis possible on the carbon-metallised specimens. The final compositions were calculated assuming oxide stoichiometry and normalization to 100%. The EDX detected the presence of K-lines associated with Al, Si, Ca, Na, Cr, Fe, Ni and while L-lines were used for Zr and Ru. Two light elements that are important constituents of CSD-B glass, Li and B, are not detectable using this technique.

The hydrated glass was analysed using micro-Raman spectroscopy. Confocal micro-Raman was employed because it ensures a great facility of use and because of its great advantages for microanalysis of mineral phases.29 Measurements were performed at room temperature in the backscattering configuration on a T64000 Jobin-Yvon/Labraham spectrometer equipped with a diffraction grating of 600 lines per mm under a microscope (Olympus Bx41) with a 100× objective focusing the 514 nm line from an argon–krypton ion laser. With the 100× objective, the spot size of the laser was estimated at 0.8 μm. A Peltier-based cooled CCD records the spectrum and the resolution given by the spectrometer setting is around 2 cm−1. Raman measurements were carried out at very low laser power to minimize possible sample deterioration. All spectra were recorded twice in the wavenumber 100–2000 cm−1 region with an integration time of 360 s. We used Origin software and Gaussian curves as elementary fitting functions. The compositions of the mineral phases were determined by comparing the collected Raman signals to values reported in literature. The error is estimated to 5%.

The altered glass was also analysed using High Resolution TEM (HRTEM) with EDX and HAADF-STEM using a JEOL JEM-ARM200F double Cs-corrected transmission electron microscope with an acceleration voltage of 200 kV. FEI TIA software was used to control the STEM-EDX mapping. The best spatial resolution in STEM mode is 82 pm. The point-to-point resolution for TEM is 110 pm, in the ADF-STEM image we used, a probe size of 1 nm was used to obtain better X-ray counts. EDX software controlling the acquisition of elemental map is JEOL Analysis Station 3.8. The specifications of the STEM were: CS of 1.0 mm and probe size of 1.0 nm. The condenser aperture was 20 mm in diameter. TEM specimens were prepared by dispersing the sample on a holey carbon thin film supported by a Cu mesh grid. For each sample, the thickness measurement of the hydrated layer was performed over several images and in different locations within the sample. Mean and standard deviation were calculated on the hydration layer thickness and the initial and long-term hydration rates. The error is 7 to 14% for the hydrated samples for 365 days and up to 27% for samples hydrated at 50 °C for 35 days.

3. Results and discussion

3.1. Infrared results

In the work of Efimov et al.39 and Navarra et al.40 on the hydration of silicate glasses, the existence of the following infrared bands was observed:

• ≈3595–3605 cm−1 attributed to OH stretching mode in SiOH.

• ≈3515–3518 cm−1 attributed to OH stretching mode in the bound water silanol groups.

• ≈3400–3415 cm−1 attributed to symmetrical stretching OH mode in the free water molecule.

• ≈3170–3185 cm−1 attributed to OH stretching mode in bound water silanol groups.

• ≈2700 cm−1 attributed to silica matrix.

To study the FTIR spectra, we performed a deconvolution with five Gaussian using the Origin 8.0 software (OriginLab). Fig. 1 shows an example of deconvolution. Note that all spectra have been normalised to their maximum and minimum intensity (Imax and Imin). We can see the quality of deconvolution obtained by the Origin 8.0 software with five Gaussian. Thus, each vibration mode can be followed.


image file: c5ra12384d-f1.tif
Fig. 1 Infrared spectra of CSD-B glass hydrated 1 day at 90 °C under 92% of relative humidity. The spectra were deconvoluted with five Gaussian.

The SiOH absorbance was used to study the glass hydration (hydrolysis) with time.25,26,29,30 The authors found a correspondence between the hydration thickness measured by SEM/TEM and the SiOH absorbance at different experimental conditions obtained by FTIR, which allowed hydration kinetics with time exposure to be obtained.

3.1.1. Effect of relative humidity. FTIR spectra were taken for each hydrated sample and the absorbance was plotted as a function of time at 50 °C and 90 °C for various relative humidities. We chose to follow the evolution of the absorption band at 3595 cm−1 corresponding to the vibration of the silanol group (SiOH), this band is indicative of the silicate hydrolysis. Fig. 2 shows the evolution of the absorption of the silanol band as a function of hydration time at 50 °C and 90 °C, for different values of relative humidities. The absorbance values were normalised using the SiOH absorbance of pristine glass.
image file: c5ra12384d-f2.tif
Fig. 2 Evolution with alteration time of the absorbance (band at 3595 cm−1 assigned to SiOH) for different relative humidity at 50 °C (a) and 90 °C (b).

At 50 °C or 90 °C, the initial hydration rate is linear with time. After 1 to 4 months of alteration, depending on the experimental conditions, there is a significant change in the regime with a significant drop in the hydration kinetics. This does not seem to depend on the relative humidity.

The absorbance (i.e., the hydration rate) of the SiOH band (3595 cm−1) increases between 92% and 95% relative humidity and the increase is more pronounced at 90 °C. However, the effect of relative humidity is very low after the change of hydration regime and the rate seems very similar for all conditions studied here.

3.1.2. Effect of temperature. Fig. 3 shows the absorbance relative to the Si–OH band as a function of time for the CSD-B glass hydrated under 92% and 95% of relative humidity at two temperatures (50 °C and 90 °C). We can see a strong increase of absorbance of the Si–OH band with the temperature. An order of magnitude is noted between the alteration kinetics at 50 °C and 90 °C for the same relative humidity. The surface reactivity and the transfer of water through the surface layers may explain these differences.
image file: c5ra12384d-f3.tif
Fig. 3 Evolution with alteration time of the absorbance (band at 3595 cm−1 assigned to SiOH) for different temperatures under 95% (a) and 92% (b) relative humidity.

Additional short term hydration experiments were conducted for 35 days in the same conditions in order to study the surface layer. The absorbance of the Si–OH band as a function of time are represented in Fig. 4 at 50 °C and 90 °C under 92% and 95% RH. For these short-term experiments we obtain similar absorbance values for the same hydration time compared to the long-term experiments, showing the good reproducibility of our experiments and the high accuracy of FTIR measurements.


image file: c5ra12384d-f4.tif
Fig. 4 Evolution with alteration time of the absorbance (band at 3595 cm−1 assigned to SiOH) for experiments conducted for 35 days at different temperatures and relative humidities.
3.1.3. Comparison of the alteration of CSD-B and SON68 glasses. The hydration of CSD-B glass was compared to that of SON68.41 Fig. 5 shows the absorbance corresponding to the Si–OH band as a function of time for CSD-B and SON68 glasses at 90 °C under 92% and 95% RH. As we can see, the hydration of SON68 is a little lower than CSD-B especially under 95% relative humidity. However, this initial rate is followed by a low long-term hydration rate in both CSD-B (this work, Fig. 3) and SON68 glasses.41 This suggests that similar hydration mechanisms are controlling the long-term hydration of these two borosilicate glasses.
image file: c5ra12384d-f5.tif
Fig. 5 Evolution with alteration time of the absorbance (band at 3595 cm−1 assigned to SiOH) for the CSD-B and SON68 glasses at 90 °C under 92% and 95% relative humidity.

3.2. Cross sectional TEM analyses

Cross-sectional analyses of the altered glasses were performed using TEM. Typical TEM cross sections, with elemental maps are given in Fig. 6 to 8 for samples hydrated for 35 and 365 days at 50 and 90 °C under 92% and 95% RH. The figures show clearly hydration layers of a few hundred nm after 35 days increasing to more than 1 μm for samples hydrated 1 year. The Ca, Na, Si, Fe and Ni mapping and EDX analyses performed on hydrated samples show that the hydrated layer is enriched in Si and depleted in Na and Ca in comparison to the pristine glass. This elemental distribution indicates that glass components can migrate through the alteration layer perhaps via a water-saturated gel layer. The concentration of Fe and Ni is remarkably constant.
image file: c5ra12384d-f6.tif
Fig. 6 TEM photographs of CSD-B glass hydrated 35 days at 90 °C and (a) 95% and (b) 92% RH. The Na, Si, Ca, Fe, Ni and Zr maps of the sample hydrated 35 days at 90 °C and 92% RH are also represented.

image file: c5ra12384d-f7.tif
Fig. 7 TEM photographs of CSD-B glass hydrated 365 days at 90 °C and (a) 92% and (b) 95% RH. The Na, Si, Ca, Fe and Zr maps of the sample hydrated 365 days at 90 °C and 95% RH are also represented.

image file: c5ra12384d-f8.tif
Fig. 8 TEM photographs of CSD-B glass hydrated 365 days at 90 °C and 95% RH.

The TEM observations allowed the FTIR water absorbance data to be linked with the alteration layer thickness. The correspondence TEM-FTIR is deduced from the whole experimental duration. For all experiments we obtained an average of 0.1 SiOH absorbance unit per 1 μm of alteration layer measured by TEM. This correspondence is close to that obtained by Neeway et al.25,26 for the SON68 glass (0.09 a.u μm−1) and the value obtained by Abdelouas et al.29 for the ISG glass (0.11 a.u μm−1).

3.2.1. Short-term hydration. Fig. 6 shows the TEM photographs and elemental maps (Na, Ca, Si, Fe, Ni, Zr) of glass hydrated 35 days at 90 °C under 92 and 95% RH. The elemental maps show a depletion of Na and Ca in the hydrated layer. However, the concentrations of Fe, Zr and Ni remain unchanged compared to the pristine glass.

For the sample hydrated at 90 °C under 92% RH the thickness of the hydration layer is estimated to be about 205 ± 29 nm. Evidence of glass dissolution and porosity formation can be seen in Fig. 6 with a clear interface between the pristine and the hydrated glasses. The hydration rate, calculated by dividing the thickness by the glass density (2.5 g cm−3), is 1.5 × 10−2 ± 2.1 × 10−3 g m−2 per d (Table 3).

Table 3 The thickness of the reaction layer given by TEM and FTIR. The TEM value was obtained from cross sections. The FTIR values were calculated using the correspondence TEM-FTIR (0.1 a.u μm−1) based on TEM observations for samples hydrated for 365 days
Sample TEM FTIR
Layer thickness (nm) rhydro (g m−2 per d) Layer thickness (nm) rhydro (g m−2 per d)
90 °C, 92% RH, 35 days 205 ± 29 1.5 × 10−2 ± 2.1 × 10−3 333 ± 7 2.8 × 10−2 ± 5.6 × 10−4
90 °C, 95% RH, 35 days 225 ± 24 1.6 × 10−2 ± 1.7 × 10−3 625 ± 13 4.4 × 10−2 ± 8.8 × 10−4
50 °C, 92% RH, 35 days 65 ± 21 4.6 × 10−3 ± 1.5 × 10−3 51 ± 1 4.3 × 10−3 ± 8.6 × 10−5
50 °C, 95% RH, 35 days 80 ± 21 5.7 × 10−3 ± 1.5 × 10−3 77 ± 2 7.1 × 10−3 ± 1.4 × 10−4


For the CSD-B glass hydrated for 35 days at 90 °C and 95% RH, the thickness of the altered layer is estimated to about 225 ± 24 nm, giving a hydration rate of 1.6 × 10−2 ± 1.7 × 10−3 g m−2 per d (Table 3). This rate is in the same order of magnitude as that calculated at 90 °C and 92% RH and is similar to that found by Bouakkaz et al.41 for the SON68 glass hydrated in the same conditions (1.20 × 10−2 g m−2 per d).

The determination of the hydrated layer thickness at 50 °C for the short term experiments (35 days) is delicate because it is very thin and the chemical contrast between the pristine and hydrated glass layer is very low. Nevertheless, we were able to estimate the hydration layer to about 80 ± 21 nm at 50 °C and 95% RH. This corresponds to an initial hydration rate of 5.7 × 10−3 ± 1.5 × 10−3 g m−2 per d (Table 3). This rate is 3 times lower than that calculated at 90 °C for the same relative humidity. For the glass hydrated at 50 °C and 92% RH, the hydrated layer is estimated to 65 ± 21 nm, which corresponds to the alteration rate of 4.6 × 10−3 ± 1.5 × 10−3 g m−2 per d (Table 3).

3.2.2. Long-term hydration. TEM observations show a highly porous hydration layer with a hydration front, showing strong dissolution evidence at the interface glass/hydration layer. Elemental mapping confirms a strong loss of Na and Ca while heavy elements such as Fe and Ni remain unchanged.

The results of TEM thickness measurements for long-term experiments could not directly be used to calculate a long-term hydration rate because the total thickness also includes that corresponding to the short-term rate. However, the long term hydration rate, corresponding to the period starting from the second inflection of the glass hydration until the end of the experiment, was calculated from the FTIR data (Fig. 2 and 3) and using the correspondence TEM–FTIR (0.1 a.u μm−1) (Table 4). The long-term rate is in the order of 10−3 g m−2 per d at 90 °C and 5.0 × 10−5 g m−2 per d at 50 °C. These rates are one order of magnitude lower than the initial rates and in the same order of magnitude as that found for the SON68 glass.25,41 For example for the sample hydrated at 90 °C and 95% RH, we found a long-term rate of 1.2 × 10−3 ± 2.3 × 10−5 g m−2 per d for the CSD-B glass compared to 1.6 × 10−3 g m−2 per d for the SON68 glass.41 Table 5 summarizes the short and long-term hydration rates of CSD-B and SON68 glasses and indicates the similarity between these two glasses.

Table 4 The long-term reaction rate calculated from FTIR absorbance using the correspondence TEM–FTIR (0.1 a.u μm−1)
Sample Long-term calculated layer thickness (nm)a rhydro L.T (g m−2 per d) Total layer thickness by TEM (nm)
a The data correspond to the period starting from the inflection of the glass hydration until the end of the experiment.
90 °C, 92% RH, 365 days 237 within the last 267 days 2.3 × 10−3 ± 4.6 × 10−5 695 ± 75
90 °C, 95% RH, 365 days 119 within the last 267 days 1.2 × 10−3 ± 2.3 × 10−5 1500 ± 104
50 °C, 92% RH, 365 days 5 within the last 226 days 5.5 × 10−5 ± 1.1 × 10−6 150 ± 22
50 °C, 95% RH, 365 days 4 within the last 226 days 4.4 × 10−5 ± 8.8 × 10−7 270 ± 23


Table 5 The initial and long-term hydration rate of the CSD-B and SON68 glasses
Sample CSD-B SON68 (ref. 41)
rhydro (g m−2 per d) rhydro L.T (g m−2 per d) rhydro (g m−2 per d) rhydro L.T (g m−2 per d)
90 °C, 92% RH 1.5 × 10−2 ± 2.1 × 10−3 2.3 × 10−3 ± 4.6 × 10−5 9.8 × 10−3 2.3 × 10−3
90 °C, 95% RH 1.6 × 10−2 ± 1.7 × 10−3 1.2 × 10−3 ± 2.3 × 10−5 1.2 × 10−2 1.6 × 10−3
50 °C, 92% RH 4.6 × 10−3 ± 1.5 × 10−3 5.5 × 10−5 ± 1.1 × 10−6 5.2 × 10−3 9.2 × 10−4


3.3. SEM imaging and EDX analyses

The CSD-B glass hydrated 35 days and 365 days was observed by SEM and analysed by EDX after carbon metallisation. To check the sensitivity of EDX, we analysed the pristine glass and the analysed composition is compared to the theoretical composition in Table 1. The measured composition is in good agreement with the initial glass composition and shows the high sensitivity of the device used. Note that the measured composition is normalised to 83.39% to take into account the boron and lithium percentage unmeasured by EDX.

Fig. 9a and b show the SEM photograph and EDX spectra of CSD-B glass hydrated for the short term (35 days) at 50 °C and 90 °C under 92% and 95% RH. The EDX microanalyses in Table 6 show no significant difference between the composition of the hydrated and pristine glass. This is probably due to the small thickness of the hydrated layers for all experiments (65–225 nm), which is much less than the analysed thickness (1 μm). We can notice the presence of dissolution evidence on the glass surface in all experiments.


image file: c5ra12384d-f9.tif
Fig. 9 SEM photograph of the surface of altered CSD-B glass, (a) 35 days at 90 °C and 92% RH, (b) 35 days at 50 °C and 95% RH, (c) 365 days at 90 °C and 92% RH, (d) 365 days at 90 °C and 95% RH showing the gel formation and Ru particles, (e) 365 days at 50 °C and 95% RH, (f) 365 days at 50 °C and 92% RH.
Table 6 EDX microanalysis of the surface of the CSD-B glass hydrated 35 days at 50 °C and 90 °C and 92% and 95% RH. The data correspond to an average of 6 spot analyses
Oxide Pristine glass 92% RH, 50 °C, 35 d 95% RH, 50 °C, 35 d 92% RH, 90 °C, 35 d 95% RH, 90 °C, 35 d
SiO2 63.6 ± 0.61 65.2 ± 0.41 63.3 ± 0.10 64.2 ± 0.14 66.4 ± 0.04
Al2O3 10.7 ± 0.22 11.0 ± 0.10 10.7 ± 0.03 10.5 ± 0.09 10.8 ± 0.06
Na2O 12.3 ± 0.19 12.0 ± 0.30 11.6 ± 0.03 12.4 ± 0.21 10.8 ± 0.28
Cr2O3 0.3 ± 0.19 0.4 ± 0.03 0.4 ± 0.04 0.0 ± 0.05 0.5 ± 0.03
CaO 3.8 ± 0.16 3.8 ± 0.05 3.9 ± 0.04 3.3 ± 0.07 3.5 ± 0.06
Fe2O3 3.2 ± 0.15 3.1 ± 0.08 3.3 ± 0.11 3.3 ± 0.06 3.2 ± 0.04
P2O5 0.4 ± 0.26 0.4 ± 0.03 0.3 ± 0.04 0.4 ± 0.05 0.5 ± 0.06
NiO 0.3 ± 0.22 0.3 ± 0.04 0.3 ± 0.02 0.5 ± 0.06 0.3 ± 0.04
ZrO2 3.2 ± 0.17 3.5 ± 0.11 3.6 ± 0.09 3.3 ± 0.20 3.1 ± 0.23
La2O3 0.2 ± 0.12 0.0 ± 0.0 0.0 ± 0.0 0.0 ± 0.0 0.0 ± 0.0
Ce2O3 1.2 ± 0.11 1.2 ± 0.10 1.2 ± 0.10 1.2 ± 0.14 1.1 ± 0.13
Nd2O3 0.7 ± 0.34 0.7 ± 0.07 0.7 ± 0.03 0.5 ± 0.08 0.7 ± 0.11
RuO2 0.0 ± 0.0 0.0 ± 0.0 0.0 ± 0.0 0.0 ± 0.0 0.0 ± 0.0
Total 100 100 100 100 100


Fig. 9 shows the SEM photographs of CSD-B glass hydrated 365 days at 50 °C and 90 °C under 92% and 95% RH. The SEM photographs show alteration layers consisting of a gel-like layer with cracks. The formation of gel is more advanced for higher temperatures (90 °C) and RH (95%). However, there is no significant difference between 92% and 95% RH. We also see the formation of ruthenium particles (Fig. 9) in the case of experiments conducted at 90 °C. The RH had no effect on layer composition while the temperature influenced the gel composition (Table 7). Hence, the gel composition shows the loss of Na and Ca compared to the pristine glass. These results are in good agreement with the TEM data. The concentration of ZrO2 and Fe2O3 is remarkably constant in all samples regardless of temperature and RH underlying the low mobility of these elements often observed during the aqueous corrosion of nuclear glasses.25,26

Table 7 EDX microanalysis of the surface of the CSD-B glass hydrated at 50 °C and 90 °C for 365 days and a relative humidity of 92% and 95%. The data correspond to an average of 6 spot analyses
Oxide Pristine glass 92% RH, 50 °C, 365 d 95% RH, 50 °C, 365 d 92% RH, 90 °C, 365 d 95% RH, 90 °C, 365 d
SiO2 63.6 ± 0.61 63.2 ± 0.95 63.0 ± 0.72 67.9 ± 0.62 69.9 ± 0.92
Al2O3 10.7 ± 0.22 10.4 ± 0.05 10.5 ± 0.07 12.8 ± 0.08 11.8 ± 0.11
Na2O 12.3 ± 0.19 13.9 ± 0.53 13.0 ± 0.61 6.8 ± 0.45 6.5 ± 0.35
Cr2O3 0.3 ± 0.19 0.1 ± 0.09 0.4 ± 0.07 0.3 ± 0.08 0.2 ± 0.06
CaO 3.8 ± 0.16 3.2 ± 0.41 3.4 ± 0.52 1.5 ± 0.33 1.3 ± 0.43
Fe2O3 3.2 ± 0.15 3.1 ± 0.16 3.5 ± 0.20 3.9 ± 0.19 3.9 ± 0.13
P2O5 0.4 ± 0.26 0.7 ± 0.12 0.2 ± 0.14 0.7 ± 0.21 0.8 ± 0.15
NiO 0.3 ± 0.22 0.5 ± 0.10 0.2 ± 0.09 0.5 ± 0.08 0.4 ± 0.11
ZrO2 3.2 ± 0.17 2.3 ± 0.05 3.1 ± 0.08 3.0 ± 0.07 2.9 ± 0.06
La2O3 0.2 ± 0.12 0.3 ± 0.09 0.0 ± 0.0 0.1 ± 0.08 0.1 ± 0.07
Ce2O3 1.2 ± 0.11 1.4 ± 0.13 1.1 ± 0.11 1.3 ± 0.09 1.2 ± 0.10
Nd2O3 0.7 ± 0.34 0.6 ± 0.08 0.9 ± 0.07 0.9 ± 0.08 0.8 ± 0.11
RuO2 0.0 ± 0.0 0.1 ± 0.03 0.3 ± 0.05 0.1 ± 0.07 0.0 ± 0.0
Total 100 100 100 100 100


At 50 °C, the EDX analyses of hydrated glass are similar to those of the pristine glass, regardless of the RH, which is attributed to the small thickness of the gel layer at 50 °C (150 to 270 nm), which is largely below the analysed depth (1 μm).

3.4. Micro-Raman analyses

The Raman spectroscopy of borosilicate glasses is one of the non-destructive tools to determine the glass structure. The Raman analysis may be successfully applied to a large variety of glass as encountered in the field of craft history and archaeology. The structure of the silicate network in a glass is mainly determined by the degree of polymerization of the silicate tetrahedra and described by the abundance of different Qn species, where Qn denotes a tetrahedron linked by bridging O atoms to n adjacent tetrahedra. The range of n is 0 (isolated tetrahedra) to 4 (fully polymerized three-dimensional network). Therefore, the analyses of the stretching band of the Si–O bond species Qn in the silicate glass envelope of a given silicate can then provide useful information about its microstructure. It was proposed by Colomban42,43 that the relative intensities of the bending and stretching bands can provide a good indication of the degree of polymerization of a silicate because of modification of the partial charge of oxygen atoms involved in the Si–O bonds.44

The Raman vibration modes present in this type of glass have been widely studied. We will report those present in the literature:

– The broad band around 490 cm−1 is assigned to the stretching modes of Si–O–Si.45–47

– The centered peak at 680 cm−1 is attributed to vibrations involving danburite type rings B2O7–Si2O7.48,49

– The broad band between 850 and 1200 cm−1 is associated with the symmetric stretching modes of Si–O bond species Qn in silicate glasses. Qn species are defined as consisting of SiO4 tetrahedra n bridging oxygens:

• The Q0 species are centered at 870 cm−1.

• The Q1 species are centered at 900 cm−1.

• The Q2 species are located at 950–1100 cm−1.

• The Q3 species are located at 1050 to 1100 cm−1.

• The Q4 species are located at 1100–1200 cm−1.

– The broad band centered around 1430–1450 cm−1 is assigned to the stretching vibration modes of BO-binding.50–56

3.4.1. The CSD-B pristine glass. Fig. 10 shows the spectrum of CSD-B pristine glass. The refinement of the Raman spectrum was possible with 9 Gaussian. Table 8 presents the refined values.
image file: c5ra12384d-f10.tif
Fig. 10 Raman spectrum of the CSD-B glass reference. Example of Raman spectrum deconvolution with 9 Gaussian.
Table 8 Refined parameters for Gaussian functions calculated for the Raman spectrum of pristine CSD-B glass
Peak Vibration mode Center (cm−1) %
1 BO-binding 1427 9.2
2 Q3 1085 10.2
3 Q2 965 17.6
4 Q1 917 1.1
5 Si–O stretching 785 1.6
6 Danburite B2O7–Si2O7 690 3.7
7 Si–O–Si stretching 488 2.5
8 O–(Al, Si)–O bending 475 43.4
9 Ca–O polyhedra 318 10.6
Total 100


The CSD-B glass is composed of several oxides, which does not make the detailed analysis and direct attribution of vibration bands easy. However, we can show the presence of broad bands corresponding to the vibration modes of the Q1, Q2 and Q3, species localized at 917, 965 and 1085 cm−1. The vibration mode at 318 cm−1 was attributed to the Raman vibrations involving Ca–O polyhedra.57 The broad band at 488 cm−1 is assigned to the vibration modes of twisting and stretching of the Si–O–Si.45–47 Other band contributions were present in the spectrum, such as the vibration mode at 690 cm−1 attributed to a poorly crystalline calcium silicate.58,59 The broad band centered around 1427 cm−1 is assigned to the stretching vibration modes of BO-binding. The spectra are dominated by the bending modes at 475 cm−1 witch correspond to O–(Al, Si)–O bending.46,47 The band at 785 cm−1 is assigned to Si–O stretching vibration with a dominant Si motion.60

3.4.2. The CSD-B glass after hydration. For the first time we analyzed the structural properties of CSD-B glass before (CSD-B pristine glass) and after hydration (CSD-B gel glass).

The Raman spectra of CSD-B glass before and after hydration (35 and 365 days) are presented in Fig. 11 and Table 9 presents the refined values obtained for the stretching band of Si–O bond species Qn in our silicate glasses. The Raman spectrum of pristine glass shows that the vibrations of the edge groups in structural units Q3 and Q2 are dominant in the CSD-B glasses.


image file: c5ra12384d-f11.tif
Fig. 11 Raman spectrum of the CSD-B glass before and after hydration (90 °C and 95% RH). The symmetric stretching modes of Si–O bond species Qn in CSD-B glasses before and after hydration.
Table 9 Refined parameters for Gaussian functions calculated for the symmetric stretching modes of Si–O bond species Qn in CSD-B glass
Peak Vibration mode Peak center (cm−1) % of Qn peaks in the gel layer
Pristine glass After 35 days After 365 days
1 Q3 1080–1090 35.3 32.3 23.8
2 Q2 950–965 60.9 56.6 53.9
3 Q1 917–923 3.8 11.1 22.3
Total 100 100 100


With increasing vapor hydration time, the abundance of Q3 and Q2 units in the glass clearly decreases (Table 9). The structure of the glass is thus depolymerized, presumably by formation of Si–OH groups from bridging O atoms according to the equation:

Si–O–Si + H2O → Si–OH + HO–Si

The formation of Si–OH groups has been associated with the increase of a Q1 species peak around 920 cm−1 at the expense of Q3 and Q2 in hydrous silicate glasses. This suggests that water reacts with O atoms bridging two Q3 tetrahedra according to Q3 – Q3 → Q2 – Q2 → Q1 – Q1.

3.4.3. The minerals formed on the CSD-B gel glass surface. Raman spectra of the mineral phases formed after 35 and 365 days on CSD-B glass monolith surface are shown in Fig. 12. The only mineral phases detected with Raman spectroscopy are a few particles of calcite (CaCO3), apatite Ca5(PO4)3(OH) and elemental Ru.
image file: c5ra12384d-f12.tif
Fig. 12 Raman spectra of the precipitated products formed on CSD-B glass monolith hydrated at 90 °C and 95% RH (a) after 35 days and (b) after 365 days.

The Raman spectrum of apatite is dominated by the stretching vibration of the P–O bonds. The band at around 962 cm−1 corresponds to the symmetric stretching vibration (ν1) of phosphate (PO43−) and is the strongest marker of apatite. The spectra displayed other Raman PO43− vibration bands such as the ν2 symmetrical bending centred at 433 cm−1, ν4 symmetrical bending centred at 590 cm−1, and ν3 asymmetrical stretching mode centred at 1044 cm−1. The peak at 1073 cm−1 was formed by the carbonate (CO32−) vibrational mode and indicated the extent of carbonate incorporated into the apatite lattice. The 1070 cm−1 band historically has been assigned to the A1g mode of carbonate.61–65 Recently, however, Antonakos et al.,66 Mason et al.,67 and Brooker et al.68 have suggested that this carbonate-induced band is an asymmetric ν3 phosphate stretch.

For calcite, there are basically five Raman bands at ambient conditions. The most intense band is the A1g mode at 1085 cm−l.69,70 Two sets of doubly degenerate internal Eg modes are observed at 712 and 1434 cm−l, and the external Eg or lattice modes occur at 282 and, 156 cm−l. The external modes are associated with librations of the carbonate ions in the primitive cell around axes normal to the C3 axis and translations of the CO32− ions normal to the C3 axis, respectively. The precipitation of carbonate minerals in these systems can affect the physical properties of the subsurface such as porosity and permeability.

Raman spectrum of the minerals formed on a CSD-B glass monolith after 365 days is shown in Fig. 12b. The Raman spectrum shows the precipitation of elemental Ru particles as we have seen by SEM/EDS analysis. The spectral features at the low-frequency region (<300 cm−1) are very similar to those reported by Slebodnick et al.71 who attributed the vibrations modes at low-frequency to Ru–Ru stretching deformation. It’s important to notice that apatite and calcite are also present on the surface of CSD-B glass after 365 days of hydration.

4. Conclusions

Borosilicate CSD-B glass vapor hydration has been studied at 50 and 90 °C, and 92% and 95% relative humidities (RH) for up to one year. The glass hydration increased with temperature and RH. After a few weeks with a linear initial rate (∼2 × 10−2 g m−2 per d at 90 °C and ∼5 × 10−3 g m−2 per d at 50 °C) a drastic drop in hydration rate occurred in all experiments where the rate did not change between 255 and 365 days. The kinetic data are similar to those obtained with the French reference high-level nuclear waste glass SON68. The major hydration product is a depolymerized gel layer depleted in Na and Ca in addition to a few particles of calcite and apatite precipitated on the glass surface. Future work should focus on understanding of the mechanisms responsible for the hydration process (initial rate, final rate) and the chemical balance of leachable elements including Ca and Na to better simulate the glass behaviour under long-term disposal conditions in particular under non-saturated water conditions.

Acknowledgements

The authors acknowledge Andra for the financial support, CEA and Areva NC for the supply of ILW glass samples. Special thanks to Nicolas Stephant and Eric Gautron from Institut des Matériaux de Nantes (IMN) for SEM and TEM analyses.

References

  1. D. E. Clark, C. G. Pantano Jr and L. L. Hench, Corrosion of Glass, Magazines for Industry, New York, 1979 Search PubMed.
  2. R. G. Newton, Glass Technol., 1985, 26, 21 CAS.
  3. B. C. Bunker, Mater. Res. Soc. Symp. Proc., 1987, 84, 493 CAS.
  4. D. E. Clark, R. L. Schulz, G. G. Wicks and A. R. Lodding, Mater. Res. Soc. Symp. Proc., 1994, 333, 107 CrossRef CAS.
  5. W. H. Casey and B. C. Bunker, in Mineral Water Interface Geochemistry, ed. M. F. Hochella Jr and A. F. White, Mineralogical Society of America, 1990, vol. 23, p. 397 Search PubMed.
  6. G. Leturcq, G. Berger, T. Advocat and E. Vernaz, Chem. Geol., 1999, 160, 39 CrossRef CAS.
  7. P. Jollivet, P. Frugier, G. Parisot, J. P. Mestre, E. Brackx, S. Gin and S. Schumacher, J. Nucl. Mater., 2012, 420(1–3), 508 CrossRef CAS PubMed.
  8. P. Jollivet, S. Gin and S. Schumacher, Chem. Geol., 2012, 330–331, 207–217 CrossRef CAS PubMed.
  9. P. Aagard and H. C. Helgeson, Am. J. Sci., 1982, 282, 237 CrossRef.
  10. B. Grambow, Mater. Res. Soc. Symp. Proc., 1985, 44, 15 CrossRef CAS.
  11. T. Advocat, Ph.D thesis, University Louis Pasteur of Strasbourg, 1991.
  12. C. Jégou, Ph.D thesis, University of Montpellier II, 1998.
  13. Y. Linard, Ph.D thesis, University Denis Diderot, 2000.
  14. S. Gin, Mater. Res. Soc. Symp. Proc., 2001, 663, 207 CrossRef.
  15. G. Berger, C. Claparols, C. Guy and V. Daux, Geochim. Cosmochim. Acta, 1994, 58(22), 4875 CrossRef CAS.
  16. N. Valle, Ph.D thesis, Institut National Polytechnique de Lorraine, 2000.
  17. S. Gin and J.-P. Mestre, J. Nucl. Mater., 2001, 295, 83 CrossRef CAS.
  18. S. Depierre, Ph.D thesis, University of Montpellier, 2012.
  19. S. Mercado-Depierre, F. Angeli, F. Frizon and S. Gin, J. Nucl. Mater., 2013, 441(1–3), 402 CrossRef CAS PubMed.
  20. F. Bellmann, T. Sowoidnich, H. M. Ludwig and D. Damidot, Cem. Concr. Res., 2012, 42, 1189 CrossRef CAS PubMed.
  21. S. Gin, J. V. Ryan, D. K. Schreiber, J. Neeway and M. Cabié, Chem. Geol., 2013, 349–350, 99–109 CrossRef CAS PubMed.
  22. S. Garrault-Gauffinet and A. Nonat, J. Cryst. Growth, 1999, 200, 565 CrossRef CAS.
  23. S. Garrault, E. Finot, E. Lesniewska and A. Nonat, Mater. Struct., 2005, 38, 435 CrossRef CAS.
  24. J. K. Bates, M. G. Seitz and M. J. Steindler, Nucl. Chem. Waste Manage., 1984, 5(1), 63 CrossRef CAS.
  25. J. Neeway, A. Abdelouas, B. Grambow, S. Schumacher, C. Martin, M. Kogawa, S. Utsunomiya, S. Gin and P. Frugier, J. Non-Cryst. Solids, 2012, 358, 2894 CrossRef CAS PubMed.
  26. J. Neeway, Ph.D thesis, University of Nantes, 2010.
  27. T. A. Abrajano, J. K. Bates and J. J. Mazer, J. Non-Cryst. Solids, 1989, 108, 269 CrossRef CAS.
  28. T. A. Abrajano, J. K. Bates and C. D. Byers, J. Non-Cryst. Solids, 1986, 84(1–3), 251 CrossRef CAS.
  29. A. Abdelouas, Y. El Mendili, A. Aït Chaou, G. Karakurt, C. Hartnack and J.-F. Bardeau, Int. J. Appl. Glass Sci., 2013, 4(4), 307 CrossRef CAS PubMed.
  30. A. Ait Chaou, A. Abdelouas, Y. El Mendili, R. Bouakkaz and C. Martin, Procedia Mater. Sci., 2014, 7, 179 CrossRef CAS PubMed.
  31. W. L. Gong, L. M. Wang, R. C. Ewing, E. Vernaz, J. K. Bates and W. L. Ebert, J. Nucl. Mater., 1998, 254, 249 CrossRef CAS.
  32. D. A. McKeown, A. C. Buechele, C. Viragh and I. L. Pegg, J. Nucl. Mater., 2010, 399(1), 13 CrossRef CAS PubMed.
  33. D. A. McKeown, A. C. Buechelee, W. W. Lukens, D. K. Shuh and I. L. Pegg, Environ. Sci. Technol., 2007, 41(2), 431 CrossRef CAS.
  34. A. C. Buechele, D. A. McKeown, W. W. Lukens, D. K. Shuh and I. L. Pegg, J. Nucl. Mater., 2012, 429(1–3), 159 CrossRef CAS PubMed.
  35. A. Ait Chaou, A. Abdelouas, G. Karakurt and B. Grambow, J. Nucl. Mater., 2014, 448(1–3), 206 CrossRef CAS PubMed.
  36. K. S. Pitzer and D. J. Bradley, in Thermodynamics of High Temperature Brines, Lawrence Berkeley Lab., Univ. California, Berkeley, CA, USA, 1979, p. 40 Search PubMed.
  37. K. M. Davis and M. Tomozawa, J. Non-Cryst. Solids, 1996, 201, 177 CrossRef CAS.
  38. K. Ferrand, A. Abdelouas and B. Grambow, J. Nucl. Mater., 2006, 355, 54 CrossRef CAS PubMed.
  39. A. M. Efimov, V. G. Pogareva and A. V. Shashkin, J. Non-Cryst. Solids, 2003, 332, 93 CrossRef CAS PubMed.
  40. G. Navarra, I. Iliopoulos, V. Militello, S. G. Rotolo and M. Leone, J. Non-Cryst. Solids, 2005, 351, 1796 CrossRef CAS PubMed.
  41. R. Bouakkaz, Ph.D thesis, University of Nantes, 2014.
  42. P. Colomban, J. Non-Cryst. Solids, 2003, 323, 180 CrossRef CAS.
  43. P. Colomban and O. Paulsen, J. Am. Ceram. Soc., 2005, 88, 390 CrossRef CAS PubMed.
  44. M. Henry, in Modelling of Minerals and Silicated Materials, ed. B. Silvi and P. D’Arco, Kluwer Academic Publishers, 2002, p. 273 Search PubMed.
  45. D. W. Matson, S. K. Sharma and J. A. Philpotts, J. Non-Cryst. Solids, 1983, 58, 323 CrossRef CAS.
  46. F. L. Galeener, J. Non-Cryst. Solids, 1982, 49, 53 CrossRef CAS.
  47. P. McMillan, Am. Mineral., 1984, 69, 622 CAS.
  48. N. Ollier, Ph.D thesis, University of Lyon 1, 2002.
  49. B. C. Bunker, D. R. Tallant, R. J. Kirkpatrick and G. L. Turner, Phys. Chem. Glasses, 1990, 31, 30 CAS.
  50. H. Li, Y. Su, L. Li and D. M. Strachan, J. Non-Cryst. Solids, 2001, 292, 167 CrossRef CAS.
  51. T. Furukawa and W. B. White, J. Am. Ceram. Soc., 1981, 64, 443 CrossRef CAS PubMed.
  52. B. Gasharova, B. Mihailova and L. Konstantinov, Eur. J. Mineral., 1997, 9, 935 CrossRef CAS.
  53. E. I. Kamitsos, M. A. Karakassides and G. D. Chryssikos, J. Phys. Chem., 1987, 91, 1073 CrossRef CAS.
  54. H. Li, P. Hrma, J. D. Vienna, M. Qian, Y. Su and D. E. Smith, J. Non-Cryst. Solids, 2003, 331, 202 CrossRef CAS PubMed.
  55. A. K. Hassan, L. M. Torell, L. Börjesson and H. Doweidar, Phys. Rev. B: Condens. Matter Mater. Phys., 1992, 45, 12797 CrossRef CAS.
  56. S. Nonnemenn, Master of Science thesis, UCF, 2003.
  57. B. O. Mysen, D. Virgo and C. M. Scarfe, Am. Mineral., 1980, 65, 690 CAS.
  58. C.-S. Deng, C. Breen, J. Yarwood, S. Habesch, J. Phipps, R. Craster and G. Maitland, J. Mater. Chem., 2002, 11, 3105 RSC.
  59. S. Martinez-Ramirez, M. Frías and C. Domingo, J. Raman Spectrosc., 2006, 37, 555 CrossRef CAS PubMed.
  60. D. W. Matson, S. K. Sharma and J. A. Philpotts, J. Non-Cryst. Solids, 1983, 58, 323 CrossRef CAS.
  61. I. L. Botto, V. L. Barone, J. L. Castiglioni and I. B. J. Schalamuk, J. Mater. Sci., 1997, 32, 6549 CrossRef CAS.
  62. J. D. Cotter-Howells, P. E. Champness and J. M. Charnock, Mineral. Mag., 1999, 63, 777 CAS.
  63. J. A. Ryan, Z. P. Hang, D. Hesterberg, J. Chou and D. E. Sayers, Environ. Sci. Technol., 2001, 35, 3798 CrossRef CAS.
  64. A. Nakamoto, Y. Urasima, S. Sugiura, H. Nakano, T. Yachi and K. Tadokoro, Mineral. J., 1969, 6(1–2), 85 CrossRef CAS.
  65. J. A. Crowley and N. A. Radford, Mineral. Rec., 1982, 13, 273 CAS.
  66. A. Antonakos, E. Liarokapis and T. Leventouri, Biomaterials, 2007, 28, 3043 CrossRef CAS PubMed.
  67. H. E. Mason, A. Kozolowski and B. I. Phillips, Chem. Mater., 2008, 20, 294 CrossRef CAS.
  68. M. H. Brooker, S. Sunder, P. Taylor and V. J. Lopata, Can. J. Chem., 1983, 61, 494 CrossRef CAS.
  69. H. G. M. Edwards, S. E. Jorge Villar, J. Jehlicka and T. Munshi, Spectrochim. Acta, Part A, 2005, 61, 2273 CrossRef PubMed.
  70. B. E. Scheetz and W. B. White, Am. Mineral., 1977, 62, 36 CAS.
  71. C. Slebodnick, J. Zhao, R. Angel, B. E. Hanson, Y. Song, Z. Liu and R. J. Hemley, Inorg. Chem., 2004, 43(17), 5245 CrossRef CAS PubMed.

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