Yttria ceramics named and prepared.
The evaluation of plasma resistance and the characteristics of yttria ceramics fabricated by calcination yttria as a starting material without dopants under an oxidation atmosphere were investigated. Regardless of the starting materials, as-received and calcined yttria powder, XRD patterns showed that all samples have Y2O3 phase. The three cycling processes inhibited a large grain, which occurs frequently during the yttria sintering, and a high-density ceramic with a homogeneous grain size was obtained. The smaller the grain size, the larger were the Young’s modulus and KIC. Compared to Al2O3 and ZrO2 ceramics, yttria ceramics showed 3 times larger plasma resistance and 1.4–2.2 times lower weight loss during the plasma etching test, respectively. The characteristics of pure hot-pressed yttria ceramics tempered in an oxidation atmosphere are also investigated. Even though the color variation of the hot-pressed Y2O3 ceramics was due to the sintering temperatures, the oxidation process turned the color of the Y2O3 ceramics into white. In addition, oxygen defects also affected the weight change and microstructure of the Y2O3 ceramics. The Y2O3 ceramic sintered at 1600°C had obtained a full density. As the sintering temperature increased, small homogeneous grains grew to large grains which affected the Vickers hardness.
- as-received yttria
- calcined yttria
- three-repeated cycle sintering
- homogeneous grain
- plasma resistance
- hot-pressed yttria ceramics
- homogeneous grain
- full density
1. Approach to sintering a yttria monolith to full density by surface and interfacial engineering
Yttria, Y2O3, has great potential as a host material for solid-state lasers such as yttrium aluminum garnet-doped neodymium, Nd:YAG, and yttrium oxide doped with ytterbium, Yb:Y2O3 [1, 2]. Other commonly known oxides, such as Al2O3, MgO, and ZrO2 ceramics, have attracted more interest than yttria [3, 4]. Therefore, the application of yttria ceramics in modern industry has been limited. Yttria ceramics are strongly dependent on not only their intrinsic properties but also their crystal structure. Yttria, which has a C-type rare earth sesquioxide structure, needs to be derived from the cubic fluorite-type structure by removing one quarter of the oxygen atoms . Yttria has 32 yttrium and 48 oxygen ion sites per unit cell. This structure has large interstitial sites with the same size as an oxygen ion in the anion sublattice. Yttria has a cubic or alpha-type crystal structure until the temperature reaches 2325°C. The phase transition to a tetragonal crystal structure also occurs at 2325°C. A stable phase, known as hexagonal or beta-type, is maintained until it reaches the melting temperature, 2340°C .
Recently, yttria, which is used widely in partially stabilized zirconia and sintering aids, was the center of attention in the semiconductor industry because yttria is superior to quartz, Al2O3, ZrO2, BN, and SiC in terms of its radical or cationic resistance activated by plasma  and sintering-limiting property .
Nevertheless, when the synthesis of nanoparticles using coprecipitation was carried out and the influence of precursors or additives was examined, it was reported that yttria, sintered under vacuum or hydrogen conditions, was close to the theoretical density [8, 9, 10]. The additives affected the grain boundary migration. This compensated for the charge, cation diffusion, solute transport, and additive-defect interaction [11, 12]. According to Huang et al. , the theoretical density of yttria ceramic was obtained by the two-step sintering and vacuum sintering of a lanthanum-doped yttria ceramic combination. Previous studies [14, 15, 16] attempted to improve the yttria transmittance and electrical conduction of the body sintered using special techniques, such as spark plasma sintering, microwave-flash combustion synthesis, hot isostatic pressing, and the addition of tri- or tetravalent additives. Therefore, it is necessary to examine the intrinsic sintering characteristics of yttria itself. More recently, Choi et al.  reported not only the behavior, color, and density of yttria ceramics but also the weight change due to oxygen vacancies and oxygen diffusion in a sintered body as a function of the sintering temperature. They suggested that the changes in color, density, weight, and microstructure of grains according to the sintering temperature were related to the volatilization of yttrium ions at oxygen vacancies in the lattice site at high temperatures [8, 10, 11]. On the other hand, the sintering property of the starting material, calcined yttria, from which the hydration reaction had been eliminated, as expressed in Eq. (1), but oxygen diffusion in oxygen vacancies and yttria powder, which removes gas spouting of the precursor, occurred continuously up to 1250°C, is unknown [13, 15]:
To determine the effects of oxygen vacancies and hydration on the sintering properties of yttria, this study studied the sintering characteristics of yttria calcined without a gas or hydration reaction containing a hydration reagent of precursors. In addition, when oxygen diffusion occurred in the oxygen vacancies, the yttria powder was heated repeatedly to adopt the result of density and increasing weight. The plasma resistivity of the yttria ceramic was compared with that of the control group.
1.2 Y2O3 as a host material and fabrication methods for the potential applications
1.2.1 Y2O3 structure and dopant
Y2O3 has a C-type cubic structure of rare earth oxides. The C-type structure is due to the bixbyite (space group Ia3 (Th7) with X = 16) and is similar to the fluorite (CaF2)-type structure, in which there is a quarter of empty anion sites and they are arranged regularly (Figure 1).
Three quarters of the cations are in cubes, in which the missing oxygen ions are along the face diagonal. One quarter of the cations are in cubes, in which the missing oxygen ions are along the body diagonal. The unit cell contains 48 oxygen and 32 yttrium ions. Yttrium ions are located at the center of an approximate cube, and oxygen ions are located at six of the eight vertices [1, 18]. In three quarters of these sites, the missing oxygen ions are located on a face diagonal of the mini-cube, and the rest are located at the ends of a body diagonal. The full unit cell contained 4 × 4 × 4 of these mini-cubes. Here, only a 2 × 2 × 1 part is shown for clarity of presentation. As an oxide, yttria showed broad transmittivity from 280 nm to 8 μm. Y2O3 melts at 2430°C, but the C-type structure was only stable up to 2325°C . The H-type structure has a hexagonal form at high temperatures. The high melting temperature and this polymorphic transition make the growth of yttria single crystals difficult. Like fluorite-structured oxides, oxygen vacancies and interstitials are the major defects in pure yttrium oxide .
In fluorite-structured oxides, Y2O3 can dissolve a large amount of aliovalent cations. This is accompanied by the formation of charge-compensation oxygen vacancies when accepted dopants are present and donor dopants are present in the oxygen interstitials. These anion defects facilitate oxygen diffusion. Indeed, oxygen anion diffusion was much faster than yttrium cation diffusion in pure Y2O3. Therefore, cation diffusion is the rate control step for grain boundary migration at all compositions. Because cation doping can be conducted readily within the solubility limit, Y2O3 like CeO is a good candidate for examining the cation dopant effects on grain boundary mobility . The cubic symmetry of this oxide further ensured a lack of strong anisotropy in grain boundary mobility, which could otherwise complicate grain growth behavior.
Dopants of both donor and acceptor types as additives for sintering yttria at lower temperatures include Mg2+, Sr2+, Sc3+,Yb3+, Gd2+, La3+, Ti4+, Zr4+, Ce4+, and Nb5+ [19, 20]. The role of the dopant in yttria is similar to fluorite-structured oxide estimated from several important features. The grain boundary mobility by cation diffusion involves an interstitial mechanism. Solute drag could suppress grain boundary mobility at high dopant concentrations. Grain boundary mobility is influenced by a dopant-defect interaction, which is charge and size dependent. Moreover, undersized dopants have a tendency to enhance grain boundary mobility markedly due to distortion of the surrounding lattice that apparently facilitates defect migration [12, 18]. According to Kingery et al. , the diffusion of oxygen anions in yttria is much faster than that of yttrium cations. Hence, yttrium cation interstitial diffusion is the rate control step for grain boundary migration.
1.2.2 Yttria ceramic fabrication
Yttria has potential applications, such as missile domes and bulb envelopes because of its optical transparency and a host material for solid-state lasers and high-resistance materials for etching plasma. Several studies have focused on obtaining full-density or high-transparency polycrystalline yttria ceramics. In the former, several methods have attempted to control the particle size and its distribution, coprecipitation, dopants or additives, and homogeneity, through hydrothermal methods. In the latter, a novel sintering method was studied. A combination of vacuum sintering and hot isostatic pressing methods was based on the low-temperature sintering process to suppress grain growth without sacrificing densification. The pores can be removed completely after hot isostatic pressing. These results are based on the addition of additives in yttria. Ikegami et al.  reported the fabrication of transparent ceramics by the two-temperature sintering of yttrium hydroxide with near theoretical total transmittance. Haung et al.  synthesized lanthanum-doped yttria ceramic by a combination of two-step sintering and vacuum sintering. A two-step strategy was proposed to produce materials with near theoretical total transmittance, and these studies focused on transparent ceramics used as infrared windows.
1.3 Sample fabrication
The sample preparation was as follows. Yttria powder (99.9%, UUHP, Shin-Etsu Chemical Co. Ltd., Japan) was used as the starting material of as-received yttria. ASY and CY powder was prepared by calcination at 1250°C for 48 h. The powder of fused yttria, FY (Mirae Materials Co. Korea), by induction melting was ball milled with 300 μm zirconia ball media for 24 h. After milling, the powder mixtures were dried at 500°C for 24 h and sieved with 325 mesh to achieve uniform particle sizes. Here, the graphite mold having a diameter of 60 mm was filled with 100 g of the starting material. After forming one axis at 200 kg, cold isostatic pressing (CIP) was performed at a 300 bar pressure to increase the green density. The heating and cooling rates were 5°C/min. The sintered specimens listed in Table 1 were obtained by the thermal history shown in Figure 2.
|CY||Calcined yttria, at 1250°C for 24 h in air|
|FY||Fused yttria by induction melting|
|HY ||Hot-pressed, at 1600°C for 8 h under Ar gas|
In the crystal phase, a coarse grain microstructure, and a microstructure of specimen, the specimens were observed using X-ray diffraction (XRD, D/MAX-2550V, Rigaku, Japan), polarizing microscope (Eclipse LV100, Nikon, Japan), and scanning electron microscope (SEM, JSM-6700F, Jeol, Japan), respectively, while bulk density of the sintered specimens was measured according to the ASTM D6683-14 method. The modulus of elasticity of the sintered specimens was observed using a pulse echo device (5800 Pulser/Receiver, Panametrics, Japan) with an oscilloscope (Tektronix, TDS3012, Japan) of X- and Y-modulation, longitudinal, and transverse waves. KIC (HV-100, Mitutoyo, Japan) was measured by applying a load of 500 g on average of 10 times or more after the specimen surface was polished with 0.2 μm diamond paste. The etching depth and the weight reduction rate were obtained by surface roughness (Surfcorder ET3000, Kosaka Lab., Japan) after plasma etching for 60 min by using an inductively coupled plasma system (Versiline, UNAXIS Co., USA). Sintering properties and plasma evaluation were compared with yttria ceramics sintered, Al2O3 (99.6%, Semiconductor Wafer, Inc., Taiwan), ZrO2 (Semiconductor Wafer, Inc., Taiwan), Si wafer (Sumco Co., Japan), and quartz (General Electric (GE), USA), respectively.
1.4 Characteristic evaluation of yttria ceramics sintered by three-repeated cycle
Table 1 lists the names of yttria ceramic specimens. Figure 3 shows the XRD crystal phase of the yttria ceramic sintered under the conditions in Figure 2. X-ray diffraction analysis (XRD, D/MAX-2550V, Rigaku, Japan) was conducted to determine the crystal structure of the prepared yttria ceramics sintered using CuKα1 radiation between 5 and 70° (2θ) at room temperature. The crystal phase of CY, the calcined starting material, was identified as Y2O3, but ASY contained both Y2O3 and YO1.335.
The difference in the crystallographic phase depending on the starting material is believed to be the effect of the oxygen vacancies, which was about one-fourth of the 48 standard positions [5, 11, 15].
The starting material calcined at 1250°C for 48 h was exposed to hydration and precursor gases, whereas ASY exhibited continuous volatilization of precursors up to 1250°C [10, 16]. Rhodes et al.  examined the continuous volatilization of methane gas. They observed not only the release of carbon or water impurities but also carbonization and hydration reactions until the temperature reached 1200°C. At higher temperatures, the calcined starting material was found to be free from the influence of the adsorption gas and hydration reaction of the precursor [5, 9, 10, 16]. A mixture phase of Y2O3 and YO1.335 in ASY was obtained after the sintering, and the relative oxygen filling was less than CY . Based on this, similar study results were reported; the self-diffusion coefficient and activation energy at 1050–1250°C were 6 × 10−6 cm2/s and 82 kJ/mole, respectively . Swamy et al.  suggested the possibility of a fluorite crystal phase formation due to the irregular oxygen vacancies in the unit lattice according to high-temperature XRD equipment. In addition, there was a difference between the results in that the additive affected only the change in transmittance, YO1.401 or YO1.335 phase formation, and the crystalline phase of the monoclinic were mixed depending on the heat treatment conditions. On the other hand, these results are common in that it originated from oxygen vacancies in the yttria regular site [13, 18, 24]. The density of the CY specimen was 4.9 g/cm3, which is higher than that of ASY, 4.8 g/cm3, as shown in Figure 4. On the other hand, CY, calcined yttria, and ASY, repeated-cycle sintering yttria, corresponding to the density of commercial yttria (Y0100A, Kyocera, Japan) and 4.9 g/cm3 were effective sintering methods, despite being lower than the theoretical density (5.01 g/cm3) of the HY specimen.
Figure 5 shows a coarse grain microstructure of the CY specimen, in which the surface of the specimen was polished with a 0.2 μm diamond paste, regardless of the starting material condition. The microstructure after repeated-cycle sintering revealed a large number of open pores, in which the hydration reactant and precursor gas of formula (1) were observed, but no coarse particles were observed in the ASY specimen in Figure 6(a) [9, 24].
In addition, the CY specimen showed a relatively dense microstructure, as shown in Figure 6(b). The coarse particles in the initial stage changed to uniform particles after repeat-cycle sintering of yttria in air (see Figures 5 and 6(a)). Because Y2O3 is an oxygen-deficient complex, it is easy to deviate from the stoichiometric Y:O ratio of 40:60 (at.%) due to oxygen vacancies [13, 25]. The majority phase of YO1.335 with oxygen deficiencies appeared in only the ASY specimen observed in XRD patterns in Figure 3.
A thermodynamically stable liquid phase formed locally at 1522°C when the Y:O ratio was 60:40 (at.%), which resulted in pyrolysis of the liquid phase in the repeated heat treatment . The reasons why the rough particles of Figure 5, which appeared at the initial stages of less-pressure sintering of yttria, changed to homogeneous particles like the microstructure in Figure 6(a) after repeated sintering are as follows. As Y2O3 is an oxygen-deficient body, it is easy to deviate from the stoichiometric Y:O ratio range of 40:60 (at.%) due to oxygen vacancies . In Figure 3(a), which showed the XRD crystal phase, only the YO1.335 crystal phase with oxygen deficiencies appeared in the ASY specimen. The liquid phase was thermodynamically stable, formed locally at 1522°C and decomposed thermally in the repeated heat treatment, resulting in a crystal when the Y:O ratio was in 60:40 (at.%). The coarse particles in Figure 5 were prepared by the liquid phase formation when the Y:O ratio was 60:40 (at.%) at 1522°C.
This liquid phase changed stoichiometrically at a Y:O ratio of 40:60 (at.%) due to oxygen diffusion in the lattice during repeated sintering. Therefore, the coarse particles in Figure 4 disappear because it could change into a crystalline phase rather than exist in the liquid phase [25, 26]. Figure 7 shows the Y-O phase diagram at 1522°C when the Y:O ratio was 60:40 (at.%); coarse particles support the validity of liquid phase formation hypothesis. This liquid phase changed stoichiometrically at a Y:O ratio (at.%) of 40:60 due to oxygen diffusion in the lattice during the repeated sintering. Therefore, it is believed that the coarse particles shown in Figure 4 disappear because the crystalline phase was more stable than the liquid phase, but this hypothesis will be proven through further studies. Figure 8(a) and (b) showed the Vickers indentation results of the ASY and CY specimens. Stress propagation along the cleavage plane and the low-level mist shape were distinct from the HY specimen, which was similar to the glass-like microstructure in Figure 8(c).
The Young’s modulus increased with decreasing particle size, as listed in Table 2, where average values of the indentation of the specimens, KIC, were measured to apply a 500 g load more than ten times. On the other hand, the HY specimen KIC appeared to be relatively high regardless of the particle size because the dense microstructure, crystal phase, and the amorphous phase were mixed as shown in Figures 6(c) and 8(c) [26, 27]. Figure 9 presents the plasma resistivity profiles of the sintered specimens and the control group. From Eqs. (2) and (3), the etching depth and weight reduction rate were obtained by surface roughness after plasma etching for 60 min using an inductively coupled plasma system by masking the abrasive specimen.
|Name||Grain size (μm)||Young’s modulus (GPa)||KIC (GPa)|
|ASY||<2||146||3.27 ± 0.6|
|CY||1||153||2.28 ± 0.5|
|HY ||>5||168||1.2 ± 0.5|
The sintering properties and plasma evaluation of yttria ceramic were compared with Al2O3 (Semiconductor Wafer, Inc., Taiwan), ZrO2 (Semiconductor Wafer, Inc., Taiwan), Si wafer (Sumco Co., Japan), and quartz (General Electric) . The etch rate and weight loss rate, which are related directly to the plasma resistance, were calculated as follows. The evaluation of plasma etching was performed using simple equations:
Quartz and Si wafer (100) were etched at a depth of 2.94–3.14 μm within 10 min of plasma irradiation, and then the etching evaluation was completed. On the other hand, the etching depth of Al2O3 and ZrO2 irradiated with plasma for 60 min was 1.31–1.45 μm. The resistivity of the yttria was 0.41–0.54 μm, which was three times higher than that of the control.
The etching depth and etch rate of the control and yttria specimens was in the order of Si wafer, quartz, ZrO2, Al2O3, and Y2O3, as shown in Figure 10(a). The weight loss rate of Al2O3 and ZrO2 was 12 times higher than that of Y2O3, as shown in Figure 10(b). In the present study, there was no difference in plasma resistance between the specimens according to the starting materials.
The plasma resistance and characteristics of the yttria ceramics were investigated in terms of calcination and three-step sintering. The crystal phase of the calcined yttria ceramics was identified as Y2O3, but as-received yttria ceramics contained both Y2O3 and YO1.335 phase on the XRD pattern have been demonstrated.
The coarse particles in the initial stage changed to uniform particles after repeat-cycle sintering of yttria in air. In the repeated heat treatment process, the liquid phase with local differences in the Y:O ratio was converted to a uniform crystal grain.
The stress propagation along the cleavage plane and the low-level mist shape appeared to the hot-pressed specimen. The Young’s modulus increased with decreasing particle size, and KIC appeared to be relatively high regardless of the particle size because the dense microstructure, crystal phase, and the amorphous phase were mixed. The etching depth and etch rate of the control and yttria specimens were in the order of Si wafer, quartz, ZrO2, Al2O3, and Y2O3. The weight loss rate of Al2O3 and ZrO2 was 12 times higher than that of yttria ceramics. There was no difference in plasma resistance between the specimens according to the starting materials. The calcination and three-repeated cycle could be suggested as one of effective sintering methods of yttria.
2. Characteristics of thermal oxidation on hot-pressed pure yttria ceramics
Fundamental studies on the forming process that affects the sintering behavior of yttria ceramics and powder synthesis techniques to obtain full density have attracted considerable interest. In particular, the sintering temperature has direct effects on the porosity, density, microstructure or crystal phase, and grain boundary migration. Yttria is used widely as a liquid sintering additive in AlN, SiC, SiAlON, and ZrO2 [7, 12]. Yttria itself, however, is a sintering-limit material when heated and can induce abnormal grain growth during the sintering process .
Finely divided yttria, having a purity at least 99.9%, was pressed into compacts, sintered in a dry hydrogen atmosphere or a partial vacuum to 2150–2300°C, and refired in wet hydrogen at 1950–2300°C to redoxidize any yttria that had been reduced to yttrium during sintering . The resulting polycrystalline yttria ceramics were examined to determine if there was any improvement in the intrinsic properties of yttria.
The previously studied yttria ceramics were divided into three groups. The first was developed from the control of yttria particles, such as 5 nm Y2O3 synthesized from a 50 to 120 nm Y2O3 powder and Y(OH)3 using a coprecipitation method [9, 24]. The second group was a transparent yttria ceramic used as an infrared window to examine the electrical properties of yttria ceramics with additives, Th, Nd, and Er [15, 28, 29]. The last group involved the development of unconventional sintering techniques, such as triaxial isostatic press, hot isostatic pressing, or vacuum sintering, to fabricate full-density polycrystalline yttria ceramics [13, 30].
Most studies reported that the synthesis of nano-yttria particles was dependent only on the process variables. On the other hand, derivation of a common denominator for the properties of yttria is more complex because of the sintering methods of yttria ceramics, sintering property, and grain boundary migration by dopants such as La, Sr, and Sc [25, 31].
Nevertheless, the purity of the starting material and packing behavior as a function of the particle size used in the granule preparation together with the particle surface area affects the sintering characteristics . These are important factors in the synthesis of dense sintered bodies. When yttria powders are induced on the nanoscale and have high purity, the fine particles or submicron-sized secondary particles agglomerate easily. Although deformation occurs in most agglomerated particles under applied stresses, strongly agglomerated secondary particles maintain their agglomerated shapes. Because the green compact containing secondary agglomerated particles produces discontinuous microstructures at the interface of the agglomerated zones to show a difference in heat transfer, its evasion is desirable.
From this point of view, a high-purity 99.9% Y2O3 powder as a starting material and a hot isostatic pressing method (hot-pressed), which are useful for obtaining a fully dense ceramic, were used to observe the sintering behavior as a function of temperature.
A foundation study was performed through comparisons between the microstructure of hot-pressed yttria ceramics as a function of temperature and that of the density, crystal phase, weight loss, Vickers hardness, the behavior of indentation, flexural strength, etc.
2.2 Characteristics of the hot-pressed yttria ceramics
Figure 11 shows the X-ray diffraction (XRD) patterns of hot-pressed yttria ceramics as a function of temperature. The sintering temperature in hot isostatic pressing (FRET-18, Fuji Denfa, Japan) was increased from 1300 to 1800°C at 100°C intervals, where the heating rate, holding time, and Ar gas flow were 5°C/min, 8 h, and 3 kgf/cm2, respectively.
The hot isostatic pressing (hot-pressed) yttria ceramic specimens were oxidized at 1200°C for 12 h. XRD revealed the characteristic peaks of cubic yttria (JCPDS 41-1105), as shown in Figure 11(a) and (b), irrespective of the sintering temperature and oxidation reaction at 1200°C.
In previous studies using a conventional sintering method, the crystallite phase of yttria could not be described precisely as the yttria phase because the YO1.401 (JCPDS39-1064) and YO1.335 (JCPDS 39-10,654) phases were also detected in the XRD pattern [25, 31]. This was based on the possibility that lattice distortion due to cation invasion into the oxygen vacancies or the Y-O ions can escape the regular lattice . On the other hand, yttria ceramics containing Sc, Gd, La, Yb, and Mg were accompanied by a change in translucency and grain boundary migration, but the crystal phase was not changed .
The change in the intensity ratio reversed the peak at 48 and 57° in the high-temperature region, 1800°C, as shown in Figure 11(b). Therefore, it was necessary to further examine the fraction of the crystal lattice due to the decomposition and volatilization of the yttria component [19, 31]. This means that the yttria crystalline phase varied according to the synthesis conditions and sintering methods, but the Y2O3 crystal phase identified in hot-pressed yttria ceramics means that the sintering temperature and oxidation reaction had no effect [18, 33].
Figure 12 shows the hot-pressed yttria ceramics sintered as a function of temperature. As the sintering temperature was increased, the color of the sintered body changed to black. This is dependent on the weight deviation and change in color due to an increase in oxygen defect concentration and Y:O ratio variation [12, 18]. This suggests that the black samples obtained from a traditional sintering method are due to the oxygen released in the lattice site during the sintering process.
In addition, the proposed hot-pressed yttria ceramics could be applied to marking samples with a crystalline structure and full density, because it has a larger effect on the color change than repeat-cycle sintering or conventional sintering. The oxidation reaction specimens were converted to white regardless of the sintering temperature, which suggests that oxygen diffusion affects the oxygen vacancies in the lattice directly . The 1500°C specimen was translucent and showed the considerable development of a glassy phase with increasing sintering temperature.
The weight of the specimens after the oxidation of yttria ceramics showed a tendency to increase with increasing temperature in Figure 13. The self-diffusion coefficient of yttrium, Do, and activation energy, Q, for polycrystalline Y2O4 with a density of 99.9% at 1400–1700°C were reported to be 1.65 × 10−2 cm2/s and 289 J/mole, respectively . The Do and Q values in the interstitial mechanism at 1050–1250°C were >6 × 10−6 cm2/s and 82 kJ/mole, respectively . The self-diffusion coefficient was expressed as D = Do exp(−Q/RT). O had 3.5 times the activation energy of Y, and the self-diffusion of oxygen ions was relatively higher than yttrium. In addition, the diffusion of oxygen anions means that they occur relatively quickly because the interstitial diffusion of yttrium cations was similar to the rate of grain boundary migration [5, 18, 21]. Therefore, the diffusion rate during the oxidation of the hot-pressed yttria ceramics was higher than that of Y atom, and the oxygen vacancy showed preferential filling. This suggests that the weight increases with increasing weight of oxygen (see Figure 14).
This tendency corresponded to an approximate 35% reduction in weight due to gas evolution and volatilization in the precursor at temperatures up to 1250°C . The density of the hot-pressed yttria ceramics of 1600°C was close to those of the theoretical density of yttria, 5.03 g/cm3, and the density tended to decrease with increasing temperature. Figure 15 presents SEM images of the microstructure according to the sintering temperature.
The initial 0.5 μm uniform crystal grains changed to a glassy phase, in which the grain size was unclear depending on the sintering temperature, as shown in Figure 15(a)–(d). Figure 15(e) and (f) presents the grain shape of the pentagonal or hexagonal of 15 μm grain size in yttria ceramics hot pressed at 1700°C. Grain growth tended to show a continuous increase with increasing temperature, which has a direct effect on the porosity, density, and crystal phase (see Figure 15(a′)–(f′)). On the other hand, the microstructure of hot-pressed yttria ceramics had an obscurity grain boundary like a glassy phase after the sintering process, which was illustrated by the change in density and weight from Figure 15(e′) and (f). The Young’s modulus of 120–170 GPa measured by the pulse echo method using an oscilloscope with X and Y modulation in Figure 16 is believed to be dependent on the yttria ceramic microstructure. Figure 17 shows the behavior of Vickers indentation of the specimen sintered as a function of temperature.
The indentation shape of the 1400°C specimen showed slightly ragged edges and interior surface, whereas in the 1500°C specimen, the origin, mirror, and mist-like noncrystalline fracture surface were distinguished clearly. The relationship between the grain size and crystal phase was examined by measuring the shape and length of the indentation according to the sintering temperature. This tendency increased with increasing indentation crack length when the crystal grains of the MgAl2O4 ceramics were grown from 0.4 to 24 μm and were attributed to the presence of local cracks acting as grain spalling . Figure 18 shows the KIC and Vickers hardness measured by applying a load of 500 g according to JIS R1610 method. KIC was calculated to be 1.2–1.9 MPa. The displacement point of KIC is dependent on the crystal phase according to the sintering temperature. The Vickers hardness of hot-pressed yttria ceramics was 28 GPa, indicating similar properties to those of the conventional polycrystalline yttria ceramics in Figure 18(b) .
The Vickers hardness of the hot-pressed yttria ceramics had high hardness because the particle size was smaller due to the Hall-Petch effect, but the hardness behavior tended to decrease with increasing particle size [27, 34]. The correlation between KIC and the hardness in hot-pressed yttria ceramics was affected by the grain size and the presence or absence of pores. The mean bending strength of five samples for each specimen was determined according to the JIS R1601 method. Figure 19 shows the bending strength of the specimen. The specimens before heat treatment showed high strength in the high-temperature region, and those after heat treatment showed relatively high strength in the low-temperature region. The bending strength of the hot-pressed yttria ceramics was approximately 140 MPa, and it was similar to that of fused silica in Table 3.
|Materials||Fracture toughness (MPa)||Strength (MPa)|
|Zirconia (3 mol% Y2O3)||7.0–12.0||800–1500|
|Glass ceramics (Pyroceram)||1.6–2.1||123–370|
|Borosilicate glass (Pyrex)||0.77||69|
|Polyethylene terephthalate (PET)||5.0||59.3|
This study examined the characteristics of hot-pressed pure yttria ceramic that was annealed in an oxidation atmosphere. As the sintering temperature was increased, the color of the sintered body changed to black. The weight of the specimens after the oxidation of yttria ceramics showed a tendency to increase with increasing temperature. The hot-pressed yttria ceramics could be applied to marking samples with a crystalline structure and full density. Grain growth tended to show a continuous increase with increasing temperature, which has a direct effect on the porosity, density, and crystal phase. The relationship between the grain size and crystal phase increased with increasing indentation crack length and was attributed to the presence of local cracks acting as grain spalling. KIC was calculated to be 1.2–1.9 MPa, and the Vickers hardness of hot-pressed yttria ceramics was 28 GPa. The specimens before heat treatment showed high strength in the high-temperature region, and those after heat treatment showed relatively high strength in the low-temperature region. The bending strength of the hot-pressed yttria ceramics was approximately 140 MPa. The yttria crystalline phase varied according to the synthesis conditions and sintering methods, but the Y2O3 crystal phase identified in hot-pressed yttria ceramics means that the sintering temperature and oxidation reaction had no effect.