2.1. XRD Analysis
A previous study [
27] shows that calcination at 700 °C leads to the formation of the minor phases
m-ZrO
2 and
r-TiO
2 for pure ZrO
2 and TiO
2, respectively. However, for Zr-Ti solid solutions, the crystal structure is hardly changed, remaining in a pure tetragonal phase at 700 °C. In addition, an increase to the Ti proportion (≥50 mol%) in Zr-Ti solid solutions results in an incomplete crystallization, which is evident in very broad XRD peaks. As a result, in this study, calcination at 600 °C is selected to produce
t-ZrO
2,
a-TiO
2 and
t-Zr-Ti solid solutions with Ti ≤ 25 mol%.
Since the purposes of this work are to achieve a higher specific surface area and to focus on the Zr-Ti solid solutions while the powders possess a tetragonal structure, two series of samples are investigated, as shown in
Table 1. One set of samples is composed of ZrO
2, Zr
0.875Ti
0.125O
2 (Z
7T
1), Zr
0.75Ti
0.25O
2 (Z
3T
1) and TiO
2, with a silica-to-(Zr,Ti)O
2 weight ratio of 1:2. Another series of samples are Z
3T
1 solid solutions with silica-to-Z
3T
1 weight ratios ranging from 0 to 1:1.
Figure 1 shows the XRD patterns of the silica-leached powders, with all samples possessing a tetragonal crystal structure. Both ZrO
2 (Z-1/2) and Zr-rich (Zr,Ti)O
2 (Z
7T
1-1/2 and Z
3T
1-1/2) have a tetragonal structure with XRD reflections at (101), (002), (110), (102), (112), (200), (103), (211), (202) and (220) in the range of 25–80° (2
θ). The crystallite size of ZrO
2 is calculated using the Scherrer equation to be 7.9 nm, and it increases to 8.9 and 10 nm (
Table 1) when Ti fractions increase to 12.5 and 25 mol%, respectively. A larger crystallite size is generally desired, so Zr
3Ti
1 composition materials with varying silica content are used for further study. TiO
2 (T-1/2) represents a pure tetragonal anatase phase with XRD reflection peaks indexed as (101), (004), (200), (105), (211), (204), (116), (220) and (215), and the crystallite size is 7.7 nm. The crystallite sizes of the counterpart powders having identical chemical compositions without the introduction of silica are in the range ~23–25 nm [
27], suggesting the presence of silica inhibits crystal growth.
The effect of silica on the crystallization of the solid solution Z3T1 is further investigated. The powder without addition of the silica (Z3T1-0) exhibits sharp and intense XRD peaks, indicating higher crystallinity of the material and a larger crystallite size (21 nm). With a gradual increase in silica-to-Z3T1 weight ratios from 1:4 (Z3T1-1/4) to 1:3 (Z3T1-1/3) and 1:2 (Z3T1-1/2), all powders indicate the tetragonal structure; however, the broadening of XRD peaks at higher weight ratios suggests structural distortion and/or smaller crystallite sizes. It is apparent that the crystallite size decreases progressively from 21 nm for Z3T1-0 to 12, 11 and 10 nm when silica-to-Z3T1 weight ratios increase from 1:4 to 1:3 and 1:2. When the weight ratio reaches 2:3, the XRD pattern shows a low degree of crystallinity, with only a few XRD peaks observed, and the crystallite size is calculated to be 4.8 nm. Further increasing the silica such that it equals Z3T1 in weight leads to a very low crystallized powder, but not a completely amorphous phase, as the crystallite size is estimated, with low confidence, to be 1.4 nm and the very broad XRD peaks indicate the loss of the long-range order. The formation of the stable tetragonal phase is important for nuclear applications, which generally require the applied materials to have high radiation resistance features.
These results with respect to Z
3T
1 materials are similar to phenomena observed by Abel et al., who investigated the silica effect on the formation of
t-ZrO
2 calcined at 650 °C with different Si mole fractions (0–27 mol%) [
8]. In their study, Ludox
® AS 40 colloidal silica is used, which has a surface area of ~135 m
2·g
−1 and a calculated colloid size of ~20.3 nm. Without Si,
m-ZrO
2 is predominantly formed. Almost pure
t-ZrO
2 is obtained at 8 mol% Si and above. At higher Si molar fractions,
t-ZrO
2 reflections become visibly broad, until an X-ray amorphous material is formed at 27 mol% Si. It is also observed that as the Si mole fraction increases, the calculated crystallite sizes decrease from 23.7 nm (pure ZrO
2) to 7.5 nm (19 mol% Si). As a result, they conclude that no XRD reflections observed at 27 mol% Si mole fraction are likely due to even smaller crystallite sizes, as an amorphous, growth-constraining SiO
2 network forms around the ZrO
2 crystallites [
8]. In our case, for Z
3T
1 samples, distinct tetragonal structures are formed until a Si mole fraction at 48.3 mol% (sample Z
3T
1-1/2 in
Table 1), weaker and broader XRD peaks are observed for Z
3T
1-2/3 with 55.5 mol% Si and the Z
3T
1-1/1 powder becomes the least crystallized at 65.2% Si mole fraction, possibly due to a very small crystallite size. Hence, using colloidal silica of different sizes and/or incorporating Ti in zirconia enable the tetragonal crystal structure to be maintained at higher Si mol fractions than in the previous investigation of Abel et al. [
8].
Figure S1 in the Supplementary Materials (SI) shows the XRD patterns of the calcined powders prior to leaching silica hard templates. These patterns are similar to those of the counterpart samples shown in
Figure 1, suggesting silica is in an amorphous state and does not incorporate inside the tetragonal crystal structure.
The crystallite size of t-(Zr,Ti)O2 formed on a colloidal silica particle surface depends on the concentration of (Zr,Ti)O2 per nm2 of silica surface. A high number (N) of (Zr,Ti)O2 molecules on the silica surface (N·nm−2) would lead to a bigger crystallite size. Taking Z3T1 composition as an example, there are 97 Z3T1 molecules per nm2 of silica surface for Z3T1-1/4. When the number of molecules of Z3T1 is ~37 (Z3T1-2/3), the crystallite size is only ~4.8 nm. Very small crystallites will be formed when the number of molecules is lower than ~30 per nm2 of silica surface. The formation mechanisms of t-ZrO2 or t-Z3T1 in the presence of Si may be different with respect to Si introduced as colloidal silica (SiO2) and silicon alkoxide at molecules level. When silica nanoparticles are used, the interaction between Si and Zr or Zr-Ti occurs on the surface of the silica colloids. The silanol groups (Si–O–H) on the silica surface are functional active sites for any chemical reactions. The hydroxyl groups (–OH) on colloidal silica react with hydroxyl groups on zirconia (Zr–OH) followed by a dehydration condensation reaction, resulting in the formation of chemical bonds between ZrO2 and silica (Zr–O–Si). In this case, the greater the number of silica colloids presented, the higher the surface area of the silica and, as such, the greater the number of reaction sites. Under a fixed amount of the Zr or Zr-Ti molecule, fewer Zr or Zr-Ti reactants presented in a fixed silica surface area lead to smaller crystallite or crystal grains.
Previous studies show that the introduction of silicon is able to stabilize
t-ZrO
2 [
30,
31,
32,
33]. The stabilization is attributed to either the constraining effect of the amorphous silica on ZrO
2 particles at high SiO
2 content (>30% mol) [
30,
31] or the decreased kinetics of ZrO
2 grain growth induced by silica as low as 2 mol% SiO
2 [
32,
33]. High-temperature calcination normally leads to the formation of
m-ZrO
2 [
27]. When a small amount of silica is introduced, it does not crystallize but forms silica-rich glassy phase concentrates at the triple junctions of the
m-ZrO
2 crystallites [
34]. This amorphous silica-rich phase contains many substitution defects and might have considerable acidity [
35]. So the introduction of silica will increase the phase transformation temperature from tetragonal to monoclinic.
Because the silicon atom is small and strongly prefers tetrahedral coordination, its dissolution within the ZrO
2 lattice seems less probable than at the superficial location [
22]. It is evidenced [
22] that the zirconia textural can be stabilized by siliceous species, and this effect is due to smearing of the siliceous species over the precipitate surface. This support surface is strongly enriched by silicon; at a Si content as low as 4 wt%, the solids show properties similar to pure silica catalytic supports for both noble metal- and sulfide-catalyzed reactions [
22], indicating Si-stabilized zirconia possessing a substantial surface area and thus a high concentration of active sites (–OH) [
8]. This observation is very important for further reaction with other species via either hydrogen bonding or electrostatic force.
2.2. Raman and FTIR Analyses
Complementary to XRD analysis, which focuses on long-range cation order–disorder of the crystal structure, the Raman technique is used to study the short-range atomic arrangement of the metal oxides by monitoring the metal–oxygen vibrations. The active modes for
t-ZrO
2 polymorph with space group
P4
2/
nmc ≡ D
4h include six Raman peaks (
A1g + 2
B1g + 3
Eg) and three IR bands (
A2u + 2
Eu), with two molecules per unit cell [
36]. Raman spectra are generally well defined and very useful for characterization of the metal oxides, while middle range IR spectra are more difficult to interpret.
Figure 2 shows the Raman spectra of two series of powders after leaching silica. The zirconia (Z-1/2) displays well-defined Raman peaks, including 148, 270, 314, 461 and 642 cm
−1, and weak shoulder peak at ~604 cm
−1. These peak positions of the silica-leached powder are very similar to those of the pure ZrO
2 sample (146, 272, 316, 461, 645 and shoulder 604 cm
−1) studied previously [
27], suggesting that the presence of silica during formation of ZrO
2 has no apparent effect on the short-range order; i.e., Zr–O vibrations. More importantly, a weak and broad peak detected at ~190 cm
−1 in the pure ZrO
2 sample is highly likely due to
m-ZrO
2 phase [
27]; however, it is barely visible for silica-leached ZrO
2 (Z-1/2). This may indirectly confirm that silica might increase the temperature of phase transformation from
t- to
m-ZrO
2. The
Eg mode at 148 cm
−1 is assigned to O–Zr–O and Zr–O–Zr bending vibrations. The 270 cm
−1 band is the
A1g mode, which is mainly due to the Zr–O stretching vibration. Raman bands at 461 cm
−1 (
Eg mode) and 314 cm
−1 (
B1g mode) can be assigned to a combination of bending and stretching vibrations. The 642 cm
−1 peak (
Eg mode) and very weak shoulder at 604 cm
−1 (
B1g mode) are attributed to the Zr–O stretching vibrations [
27].
Tetragonal
a-TiO
2 is also characterized by six Raman active vibrations (
A1g + 2
B1g + 3
Eg) [
27]. Sample T-1/2 exhibits three
Eg modes located at 145, 199 and 638 cm
−1. The
B1g mode is found at 397 cm
−1 and a combination band (
A1g +
B1g) is observed at 517 cm
−1. These Raman peak positions are similar to those observed for pure titania powder (144, 195, 397, 517 and 640 cm
−1) [
27], indicating that silica does not affect the formation of the
a-TiO
2 crystal structure.
When 12.5 and 25 mol% of Zr are replaced by Ti for Z
7T
1-1/2 and Z
3T
1-1/2, respectively, the location of two
Eg modes at ~640 and 148 cm
−1 is hardly changed; however, peak broadening is clearly noticeable for both Raman bands. The major Raman band centered at ~320 cm
−1 appears in both samples and most likely is due to a combination of Zr–O and Ti–O stretching vibrations. The broadening of this Raman peak may be due to the deformation of the tetragonal structure with the incorporation of Ti in a ZrO
2 unit cell, rather than the crystallite size effect. The Raman spectra of the silica-leached samples with various silica-to-Z
3T
1 weight ratios are also shown in
Figure 2. Both crystallite size and structure deformation have impacts on the Raman spectra for these powders. The continuous broadening of the major peak observed at ~320 cm
−1 is due to the gradual decrease in the crystallite size [
37]. With a further increasing of the silica-to-Z
3T
1 weight ratio to ≥2:3, the Raman spectrum becomes featureless. The extremely small crystallite size could be responsible for this observation, in addition to the dis-ordered nature of these samples because of the incorporation of 25 mol% of Ti.
The IR spectroscopy is employed to determine if Zr/Ti–O–Si bonds are formed at the Zr/Ti oxide interface. The principal absorption frequencies in both ZrO
2 and TiO
2 are routinely observed in the IR region below 800 cm
−1. The IR spectrum of SiO
2, on the other hand, is characterized by several main absorption bands, including a very strong peak at 1100–1000 cm
−1 owing to the Si–O–Si asymmetric stretching vibration [
38,
39]. The FTIR spectra of the silica-leached powders are presented in
Figure 3 and
Figure S2 in the Supplementary Materials. As expected, all samples display a strong IR absorption below 850 cm
−1, which is due to the M–O–M (M = Zr or Ti) bond vibration modes.
From
Figure 3, the IR spectra display strong absorption at 957–941 cm
−1, reflecting the presence of the O–Si bond. It is noted that the frequency of the O–Si stretching band in these synthesized materials is significantly lower than the band corresponding to the same type of vibration in amorphous silica (~1100 cm
−1) [
38,
39]. This behavior manifests the presence of an elevated number of Zr–O–Si and/or Ti–O–Si bonds in the samples. The phenomena have been observed for ZrO
2-SiO
2 powders [
33,
40,
41]. The IR peak ~990 cm
−1 is observed for amorphous ZrO
2-SiO
2 powders prepared by hydrolysis of a liquid aerosol and dried at 50 °C [
40,
41]. For ZrO
2/SiO
2 binary oxides thermally treated at 600 °C [
33], the typical stretching peak of Zr–O–Si shifts progressively from 1075 cm
−1 for silica-rich (10 mol% ZrO
2 + 90 mol% SiO
2) to 1002 cm
−1 for zirconia-rich (90 mol% ZrO
2 + 10 mol% SiO
2) materials. In addition, it is reported that the band corresponding to Ti–O–Si vibrations is usually observed in the 950–970 cm
−1 zone for TiO
2–SiO
2 nanocomposites [
42], which is also lower than 1100 cm
−1.
With the gradual increase of the Ti component in zirconia samples Z-1/2, Z7T1-1/2 and Z3T1-1/2, the IR band responsible for O–Si bond vibrations not only shifts to lower wavenumbers, but also becomes less intense. These results suggest that the Zr/Ti ratio has a strong impact on O–Si bond vibrations when it is chemically bonded with Zr/Ti. ZrO2 and TiO2 have a similar specific surface area in our study, which will be discussed later. The intense IR peak at ~957 cm−1 for Z-1/2 may indicate that zirconia has a stronger affiliation with silica than titania (T-1/2).
The weak-to-medium IR peaks at 1348–1360 cm
−1 (
Figure 3) are ascribed to δ(Si–OH) groups of hydrated silica. This band is routinely observed at ~1400 cm
−1 [
39] and its shifting to lower wavenumbers may indicate that Si–OH groups are chemically bonded on (Zr,Ti)O
2 surfaces. Furthermore, weak and broad IR bands located at ~1600 cm
−1 are due to free –OH vibrations (water within the metal oxide structure) [
39].
It is expected that powder materials with a higher specific surface area will account for a higher number of Zr/Ti–O–Si and Si–OH species. Thus, for Z3T1 solid solutions with a higher amount of silica, intense IR peaks at 941 and 1348 cm−1 suggest higher concentrations of surface Si–O–Si and Si–OH groups. For material without the addition of silica, both IR peaks are not observed.
When these porous materials are used as adsorbents for nuclear applications such as radionuclide generation and radioactive waste separation, the presence of the active Si–OH groups on particle surfaces is of great importance. The high number of –OH groups can directly associate with radioactive species with high efficiency; they can also further graft organic ligands to improve selectivity.
2.3. SEM and TEM Analyses
The overall morphology of the powders imaged by secondary SEM is presented in
Figure 4. The particulate shape is irregular and the size ranges from sub-micron to tens of microns. The high magnification SEM images (
Figure 4 inset) display an interconnected porous network structure (like ‘necked millet seeds’) with the mesopores originated from remaining voids after leaching silica. The glucose introduced acts as a dispersant agent during drying and calculation, leading to the formation of the aggregated/agglomerated crystalized particles, not a completely gelled monolith. The hydroxyl groups on the glucose may associate with the metal oxide surfaces by a weak chemical bond. On the other hand, the nonpolar organic part of the glucose on the fringe of the complex-building species yields steric repulsion, which inhibits the complete coalescence/’fusion’ of the particulates [
27,
28,
29]. It is expected that particulate morphology, including particle size and size range, can be controlled by judiciously selecting the type and quantity of the dispersant agent.
The energy dispersive spectroscopy (EDS) results analyzed by SEM for samples with different compositions are given in
Table 2. Element Na is derived from the remaining NaOH used during the leaching process. A high level of Na (5.1 mol%) for Z
3T
1-1/1 is possibly due to the high surface area of the sample. A thin layer of SiO
2 is chemically bonded on Zr/Ti oxide surfaces via a Zr/Ti–O–Si bond, as evidenced by IR results (
Figure 3). SiO
2 is more likely to associate with the ZrO
2 surface (2.7 mol% Si) than with TiO
2 (0.7 mol% Si), which is also consistent with the IR observation. It is not clear whether the bonding between silica and the (Zr,Ti)O
2 surface is homogeneous or not, but the smearing of the siliceous species leads to the powder exhibiting properties similar to pure amorphous silica [
8,
22], which is then easy to be functionalized for industrial applications. In addition, it is not surprising that more Si on sample Z
3T
1-1/1 (5.1 mol% Si) is observed than on Z
3T
1-1/2 (2.5 mol% Si), as the former possesses a higher specific surface area.
The microstructures of the samples after removing silica and the primary grain sizes of the particulates are observed using TEM.
Figure 5 and
Figures S3 and S4 in the Supplementary Materials show the TEM bright field images of the particles at different magnifications. The TEM images display ceramic particulates composed of the aggregated primary nanoparticles with diameters of ~5–10 nm (
Figure S3 in Supplementary Materials). This observation is consistent with the crystallite estimation obtained by XRD analysis.
Figure 6 shows the selected area diffraction rings generated from the selected aperture area, which includes many nano-sized grains with different crystal orientations. The patterns belong to the tetragonal crystalline structure. The Z-1/2 and Z
3T
1-1/2 exhibit the same SAED ring patterns; i.e., (101), (002), (112) and (211) with space group
P4
2/
nmc. Z
3T
1-1/1 only shows the three inner rings, indicating the same crystal structure as Z-1/2 and Z
3T
1-1/2, but relatively lower crystallinity and/or smaller crystallites. T-1/2 shows the ring pattern with four diffraction rings; i.e., (101), (004), (200) and (121) in space group
I4
1/
amd. The space distances calculated from the (101) plane ring via TEM are 0.297, 0.296 and 0.354 nm for Z-1/2, Z
3T
1-1/1 and T-1/2, respectively, whereas the d-spacings of the (101) plane measured by XRD are 0.2929 nm (2
θ = 30.523°), 0.2938 nm (2
θ = 30.424°) and 0.3483 nm (2
θ = 25.573°) for the corresponding samples. The d-spacing of the (002) plane for Z
3T
1-1/2 is estimated by TEM to be 0.261 nm while the value is measured by XRD to be 0.2599 nm (2
θ = 34.516°).
HRTEM images shown in
Figure 7 demonstrate the lattice structures of the crystal. The d-spacings of lattice planes based on the HRTEM estimation are in good consistency with XRD data, with a value discrepancy of <2%. The results confirm the full crystallization of the materials for most samples, with crystallite grains exhibiting a similar scale to the primary particles. Although the TEM images and SAED patterns show the specimen features of small areas whereas the XRD results reflect the characteristics of the bulk materials, the d-spacing measurements by TEM match well with the XRD results. As a result, both techniques are used complementarily to better understand the microstructure and overall structure of the materials.
2.4. Nitrogen Sorption Analysis
Specific surface area, pore volume and pore size of the silica-leached powders are determined by nitrogen sorption analysis. The adsorption and desorption isotherms, the corresponding pore width distribution and cumulative pore volume with respect to pore diameter are shown in
Figure 8 for tetragonal ZrO
2, TiO
2 and two solid solutions, with a 1:2 silica-to-(Zr,Ti)O
2 weight ratio. All sorption diagrams exhibit the characteristic features of the Type IV isotherm using the IUPAC classification scheme [
43,
44], and the hysteresis loops correspond mainly to the presence of the mesopores (2–50 nm). The detailed porosity data are summarized in
Table 3. In general, there is no significant variation for specific surface area, which is in the range of 171–191 m
2·g
−1 and 166–187 m
2·g
−1 as analyzed by BET and DFT, respectively. The pore volume for ZrO
2 (Z-1/2) is ~0.3 cm
3·g
−1, which increases by ~10% when 12.5 mol% of Zr is replaced by Ti (Z
7T
1-1/2). Further increasing the Ti content in a solid solution (Z
3T
1-1/2) leads to a higher pore volume, ~0.36 cm
3·g
−1, a similar value to pure TiO
2 (T-1/2). The pore size distribution profiles shown in
Figure 8 demonstrate predominantly mesoporous pores (2–50 nm), with the volume being ~97–99% of the total pores (
Table 3). The average pore size estimated by BET is ~7–9 nm, while the pore size determined by DFT is ~10 nm for most samples. The contribution from micropores (pore size < 2 nm) to pore volume is less than 2.2%. In most cases, there are two pore size peaks at ~5 and 10 nm within the mesopore size range. It is expected that the 5 nm pores are derived from the voids between (Zr,Ti)O
2 crystallites, while 10 nm pores are originated from the spaces occupied by colloidal silica before leaching. Overall, the Zr/Ti ratio has minimal impact on the porous structure under a fixed silica-to-(Zr,Ti)O
2 weight ratio.
For silica-leached Z
3T
1 samples at various silica-to-Z
3T
1 weight ratios, the nitrogen sorption isotherms, pore size distributions and corresponding cumulative pore volumes are shown in
Figure S5 in the Supplementary Materials and detailed pore structure data are listed in
Table 4. All isotherm diagrams demonstrate Type IV nitrogen sorption characteristics [
43,
44]. By increasing the silica-to-Z
3T
1 weight ratio from 0 to 1:1, the specific surface area increases from approximately 20 to 230 m
2·g
−1. Specifically, a linear relationship is expressed between the specific surface area and a silica/Z
3T
1 weight ratio in the range of 0 to 0.5 (
Figure 9a). With a further increase to the weight ratio of 0.5 to 1.0, the specific surface area still increases gradually, but at a slower pace compared to samples having less silica.
In addition, it is apparent that total pore volume is increased linearly with respect to the silica-to-Z
3T
1 weight ratio within the 0–0.67 range (
Figure 9b). The pore volume of the sample without adding silica is 0.04 cm
3·g
−1. When the silica-to-Z
3T
1 weight ratio is 2:3 (Z
3T
1-2/3), the pore volume increases to ~0.45 cm
3·g
−1, which is about 11 times higher than that of Z
3T
1-0. Further increasing the weight ratio from 2:3 to 1:1, the pore volume increases by ~10% to ~0.50 cm
3·g
−1. The average pore diameter estimated by BET is ~8 nm, whereas the pore size determined by DFT is about 10 nm for all silica-leached samples,
For Z
3T
1-0, there is only one pore size peak of ~7 nm (
Figure S5 in the Supplementary Materials), which is the void spaces between crystalline grains. For all silica-leached samples, two pore size peaks are observed at ~5 and 10 nm (
Figure S5 in the Supplementary Materials). The smaller pores are the voids between ceramic grains, while the larger pores are the remaining spaces after leaching silica.
It can be seen from SEM and TEM images (
Figure 4 and
Figure 5) that the particulates of the powder are composed of nanocrystalline ‘building blocks’/primary particles. The specific surface area of the porous powder determined by nitrogen sorption is mainly contributed by the surface area of the nano grains, even though there might be open pores on the grains which would be in small proportion. The total surface area of the crystallites can be calculated, with the results shown in
Table S1 in the Supplementary Materials, under the assumption that the crystals are spherical. For Z
3T
1-1/4, Z
3T
1-1/3 and Z
3T
1-2/3, the calculated figures are close to the experimental results, suggesting that the crystal grain size is close to the crystallite size. The calculated figure for Z
3T
1-0 is more than double the experimental value, indicating that each crystal grain consists of several crystallites, which can be observed from the TEM images. For Z
3T
1-1/2, the higher value of the experimental result compared to the calculation may suggest that the real grain size is smaller than the calculated crystallite size and/or that crystal grains are highly porous. For Z
3T
1-1/1, the estimated crystallite size is ~1.4 nm, which may be much smaller than the true value. As a result, a higher calculated surface area is obtained.
Certainly, one (Zr,Ti)O
2 grain may contain several crystallites and colloidal silica may undergo aggregation and/or coalescence during sample preparation. In both cases, the surface areas of the (Zr,Ti)O
2 grains and the number of the silica nanoparticles will be decreased. In general, the silica covers ~60–70% of the surface area of Z
3T
1 powder, regardless of the silica-to-Z
3T
1 weight ratios (except low-confidence sample Z
3T
1-1/1). Hence, it is reasonable to assume that the presence of silica inhibits the growth of the ceramic grains and that approximately two-thirds of the Z
3T
1 surface area is covered by silica (
Table S1).
The tetragonal ZrO
2, TiO
2 and Zr-Ti solid solutions are synthesized using a solution combustion method in the presence of an organic fuel only [
27]. The maximum specific surface area of ~50 m
2·g
−1 is observed for ZrO
2, which decreased to ~34 and ~10 m
2·g
−1 for Zr
0.75Ti
0.25O
2 and TiO
2, respectively. The pore volumes are <0.04 cm
3·g
−1 for all these powders. By combining a ‘soft’ dispersant and a hard colloidal template, crystalline ternary metal oxides have been produced. Pyrochlore Y
2Ti
2O
7 powders [
28] are composed of ~25–30 nm nanoparticles, with a specific surface area up to 70 m
2·g
−1 and a pore volume of ~0.35 cm
3·g
−1. Brannerite CeTi
2O
6 polycrystalline materials [
29] are assembled by primary particles of ~20–30 nm and exhibit a slightly higher specific surface area (up to ~100 m
2·g
−1) and pore volume (~0.4 cm
3·g
−1) than those of the porous pyrochlore [
28]. In the present work, the pore structure features have been significantly improved compared with previous studies [
27,
28,
29]. The optimal sample in terms of porosity and crystallinity was Zr
3Ti
1-1/2, as this sample demonstrates the highest surface area and pore volume while still maintaining a tetragonal crystal structure. Increasing the silica content further increases the porosity but results in poor crystallinity. More importantly, the existence of the Zr/Ti–O–Si bonds and, thus, the active Si–OH groups on the surface of the materials pave the way for further studies. As a result, these materials attain several critical features for potential applications. A tetragonal crystal structure is radiation resistant, and its high porosity ensures a high concentration of –OH groups on the particle surface, which provides active sites for post-grafting organic ligands or directly conjugating with other species.