Ayako
Yamamoto
*a,
Kimitoshi
Murase
a,
Takeru
Sato
a,
Kazumasa
Sugiyama
b,
Toru
Kawamata
b,
Yoshiyuki
Inaguma
c,
Jun-ichi
Yamaura
d,
Kazuki
Shitara
e,
Rie
Yokoi
e and
Hiroki
Moriwake
ef
aGraduate School of Engineering and Science, Shibaura Institute of Technology, 307 Fukasaku, Minuma, Saitama, 337-8570, Japan. E-mail: ayako@shibaura-it.ac.jp
bInstitute for Materials Research, Tohoku University, 2-1 Katahira, Aoba, Sendai, 980, Japan
cDepartment of Chemistry, Faculty of Science, Gakushuin University, 1-5-1 Mejiro, Toshima-ku, Tokyo 171-8588, Japan
dInstitute for Solid State Physics, University of Tokyo, Kashiwa, Chiba, 277-8581, Japan
eNanostructures Research Laboratory, Japan Fine Ceramics Center, 2-4-1 Mutsuno, Atsuta, Nagoya, 456-8587, Japan
fInternational Research Frontiers Initiative (IRFI), MDX Research Center for Element Strategy (MDXES), Tokyo Institute of Technology, SE-6, 4259 Nagatsuta-cho, Midori-ku, Yokohama, Kanagawa, 226-8501 Japan
First published on 1st April 2024
We synthesized a perovskite-type RbNbO3 at 1173 K and 4 GPa from non-perovskite RbNbO3 and investigated its crystal structure and properties towards ferroelectric material design. Single-crystal X-ray diffraction analysis revealed an orthorhombic cell in the perovskite-type structure (space group Amm2, no. 38) with a = 3.9937(2) Å, b = 5.8217(3) Å, and c = 5.8647(2) Å. This non-centrosymmetric space group is the same as the ferroelectric BaTiO3 and KNbO3 but with enhanced distortion. Structural transition from orthorhombic to two successive tetragonal phases (Tetra1 at 493 K, Tetra2 at 573 K) was observed, maintaining the perovskite framework before reverting to the triclinic ambient phase at 693 K, with no structural changes between 4 and 300 K. The first transition is similar to that of KNbO3, whereas the second to Tetra2, marked by c-axis elongation and a significant cp/ap ratio jump (from 1.07 to 1.43), is unique. This distortion suggests a transition similar to that of PbVO3, where an octahedron's oxygen separates along the c-axis, forming a pyramid. Ab initio calculations simulating negative pressure like thermal expansion predicted this phase transition (cp/ap = 1.47 at −1.2 GPa), aligning with experimental findings. Thermal analysis revealed two endothermic peaks, with the second transition entailing a greater enthalpy change and volume alteration. Strong second harmonic generation signals were observed across Ortho, Tetra1, and Tetra2 phases, similar to BaTiO3 and KNbO3. Permittivity increased during the first transition, although the second transition's effects were limited by thermal expansion-induced bulk sample collapse. Perovskite-type RbNbO3 emerges as a promising ferroelectric material.
Alkali metal niobates, ANbO3 (where A = Li, Na, and K), are classic examples of ferroelectrics or anti-ferroelectrics.1 Their structural stability and distortion types can be explained using the tolerance factor (t = (rA + rO)/√2(rB + rO)) in ABO3, assuming a perovskite structure. LiNbO3 with t = 0.80 adopts its original LiNbO3-type structure, while KNbO3 with t = 1.05 maintains a perovskite structure. Conversely, RbNbO3 with t = 1.07 deviates from the perovskite structure and forms a pseudo-one-dimensional structure3 due to the larger Rb ion size.
High-pressure synthesis methods have been instrumental in discovering new functional materials. In ABO3 compounds, simple and dense structures, such as the LiNbO3 and perovskite types, are stabilized at high pressures based on the ionic radii of A and B. For instance, ferroelectric LiSbO34 was stabilized as a LiNbO3-type at 7.7 GPa, and ferroelectric PbVO35 as a highly distorted perovskite-type was achieved at 4–6 GPa. The high-pressure approach is particularly advantageous for suppressing low vapor-pressure element volatilization, such as Na, K, Rb, Hg, Tl, and Pb, due to the synthesis in a closed cell.
An initial brief report on the high-pressure synthesis of perovskite RbNbO3 dates back to 1972.6 Over the decades, theoretical calculations have predicted the structural stability and ferroelectric properties of RbNbO3, assuming a perovskite structure.7 Recently, Fukuda and Yamaura reported on the structural transition of perovskite-type RbNbO3 from the orthorhombic to the tetragonal phase at 493 K and its dielectric properties below 300 K.8 In our study, we present our detailed findings from independent studies on the crystal structure and phase transitions over a broad temperature range (4–1100 K), along with thermal properties measured using thermogravimetry (TG), differential thermal analysis (DTA), and differential scanning calorimetry (DSC), optical properties measured using second harmonic generation (SHG), and dielectric properties. We also discuss ab initio calculations related to phonon dispersion and phase stability. These theoretical calculations explain our experimental results well.
Powder XRD (Cu Kα) measurements at 300–1100 K were carried out using a Bragg–Brentano diffractometer equipped with a furnace (Ultima, Rigaku) using a Pt sample holder (also serving as a heater). Measurements at 4–300 K were performed using a Bragg–Brentano diffractometer (SmartLab, Rigaku) with Cu Kα1 radiation on a Cu plate connected to a cold head. Lattice parameters were determined using the whole pattern profile fitting method. Diffraction patterns at 373 K (orthorhombic phase), 533 K (tetragonal phase), and 643 K (tetragonal phase) were analyzed using the Rietveld method using the Z-Rietveld software.12
Fig. 1 (a) Crystal structure models of the ambient-pressure phase (APP) and high-pressure phase (HPP) of RbNbO3; (b) powder XRD of APP and HPP of RbNbO3 and KNbO3. |
The lattice parameters of RbNbO3 were determined as a = 3.9937(2) Å, b = 5.8217(3) Å, and c = 5.8647(2) Å, and volume v = 136.35(2) Å3 by single-crystal analysis; consistent with the lattice parameters determined by Fukuda and Yamaura8 (a = 3.99152(2) Å, b = 5.82230(3) Å, and c = 5.86394(3) Å). These values are larger than those of KNbO3, reflecting the larger ionic size of Rb. The density change from 4.362 g cm−3 to 5.514 g cm−3 represents a significant volume reduction of 26%, much higher than typical volume reductions in metal complex oxide phase transitions. The orthorhombicity and Nb displacement exceed those of KNbO3, suggesting a higher dielectric polarization.
SEM images in Fig. 2(a–c) show the automorphic grain of HPP-RbNbO3. Most single crystals measured 10–30 μm on the edge length, as shown in Fig. 2(a and b). Most powders and crystals show cubic shapes, but an exception occurs in the case of the Rb-deficient precursor, as seen in Fig. 2(c). The rod-shaped automorphic grain of TTB-Rb1−xNbO3 (x ∼ 0.4) was confirmed based on both XRD and SEM images. EDX analysis of flat crystal surfaces of RbNbO3 revealed an Rb:Nb ratio of 50.6(4):49.4(4), close to the expected stoichiometry.
Atomic positions and displacement parameters in HPP-RbNbO3 were refined using a single-crystal XRD analysis and are listed in Tables 1 and S2.† Bond distances and angles were compared with those of KNbO3 and APP-RbNbO3 and are summarized in Table 2. Fig. 3(a) and (b) illustrate the Nb and Rb coordinations in RbNbO3, respectively. Although cell parameters of RbNbO3 are longer than those of KNbO3, the shortest Nb–O bond is shorter in RbNbO3. The Nb–O bond angles in RbNbO3 deviate more from the ideal 90° than those in KNbO3. A greater Nb shift in the ab plane occurring along the polar axis c than in KNbO3 was confirmed, resulting in two shorter Nb–O2 bonds and two longer Nb–O2 bonds. The findings suggest a greater polarization in RbNbO3 than that of KNbO3.
Fig. 3 Structure models of (a) Nb–O and (b) Rb–O coordination in RbNbO3. Numbers between atoms indicates the distance in Å. |
Atom | Site | Occ. | x | y | z | U iso (Å2) |
---|---|---|---|---|---|---|
Nb | 2b | 1 | 1/2 | 0 | 0.50570(9) | 0.00383(14) |
Rb | 2a | 1 | 0.0 | 0 | 0.02736(6) | 0.0062(2) |
O1 | 2a | 1 | 0.0 | 0 | 0.5487(6) | 0.0065(6) |
O2 | 4e | 1 | 1/2 | 0.2411(5) | 0.2992(5) | 0.0060(4) |
RbNbO3 (HPP) | KNbO3 | RbNbO3 (APP) | |
---|---|---|---|
Nb–O2 (Å) | 1.854(3) × 2 | 1.867(2) × 2 | Nb1–O, 1.794(5), 1.890(5), 1.948(6), 2.059(4), 2.073(6) |
Nb–O1 (Å) | 2.013(5) × 2 | 1.9968(3) × 2 | Nb2–O, 1.766(7), 1.912(5),1.996(4), 2.049(5), 2.093(3) |
Nb–O2 (Å) | 2.288(3) × 2 | 2.178(2) × 2 | — |
O1–Nb–O2 (°) | 84.60(8)/94.69(7) | 85.74(5)/94.58(6) | — |
O2–Nb–O2 (°) | 89.580(19) | 89.67(3) | — |
BVS (Rb/K) | +2.22 | +1.78 | +0.93(Rb1)/+1.20(Rb2)/+1.13(Rb3) |
BVS (Nb) | +4.57 | +4.63 | +4.88(Nb1)/+4.87(Nb2) |
BVS (O1) | −2.21 | −2.14 | −2.03(O1)/−1.28(O2)/−2.12(O3) |
BVS (O2) | −2.29 | −2.13 | −2.28(O4)/−2.15(O5)/−2.40(O6) |
t (given) | 1.07 | 1.05 | n/a |
t (obs.) | 1.00 | 1.00 | n/a |
The Bond Valence Sum (BVS) calculated21 for each site, based on the distances in Table 2, indicated that if a cation's BVS exceeds its formal valence, the lattice experiences compression from nearby anions or forms multiple bonds. The BVS value of Rb in HPP-RbNbO3 is exceptionally high at +2.22, indicating significant compressibility with the 12 coordination. In contrast, the BVS for Rb in APP ranged from +0.93–1.20, closer to the formal valence of +1.0. The BVSs of Nb and O1/O2 in HPP are +4.57 and −2.21/−2.29, despite having formal valences +5.0 and −2.0, respectively, suggesting dipole formation.
The t was calculated using both Shannon's ionic radii22 and observed experimental distances. The given t for RbNbO3 is slightly larger than for KNbO3. However, once stabilized under high pressure, both the observed t values for the Rb and K variants are 1.00, implying that Rb's ionic radius compacts significantly under high pressure, fitting well within the perovskite structure.
The temperature dependences of the lattice parameters of HPP-RbNbO3 are plotted in Fig. 5. The ortho-to-Tetra1 transition occurred at 493 K, almost the same temperature as in KNbO3.23 Note that the transition to another tetragonal phase, Tetra2, at 573 K involved lattice parameter c elongation, distinct from the tetra–cubic transition in KNbO3.23 A wide temperature range with coexisting Tetra1–Tetra2 phases was observed. In this range, c elongated, and the cp/ap ratio (ap and cp are taken from a basic perovskite cell) increased from 1.07 to 1.43, with cell volume expansion. As later discussed, the SHG was confirmed up to 650 K, proving that the Ortho, Tetra1, and Tetra2 phases are non-centrosymmetric. The space group of both the Tetra1 and Tetra2 phases was estimated as P4mm due to the reflection conditions and appearance of the SHG signal. The Rietveld analyses of powder XRD at 373 K, 533 K, and 643 K were performed, and reasonable parameters are shown in Fig. S2.† Local coordination around Nb in Tetra2 will be discussed later.
Fig. 5 Temperature dependence of lattice parameters of RbNbO3 at 300–670 K. a, b, c, and v taken from a basic perovskite cell. |
Powder XRD measurements at 4–300 K revealed no structural changes, unlike the transition to a rhombohedral phase below 220 K in KNbO3.24 This aligns with our predictions that the most stable phase, i.e., the lowest energy, of RbNbO3 is the orthorhombic cell, as shown in Table 3, while that of KNbO3 is a rhombohedral cell. The temperature dependences of the diffraction patterns are shown in Fig. S1.† The lattice parameters shrunk according to the regular thermal reduction with decreasing temperature. One possible reason why no phase transition occurred is that Rb substitution functions as chemical pressure. The orthorhombic phase is stable at lower temperatures, as observed in KNbO3 under external (physical) pressure.25
RbNbO3 | RbNbO37 | KNbO3 | BaTiO3 | |
---|---|---|---|---|
Space group | Energy (meV) | Energy (meV) | Energy (meV) | Energy (meV) |
Pmm | 0 | 0 | 0 | 0 |
P4mm | −61.76 | −46.5 | −22.4 | −20.4 |
Amm2 | −70.11 | −57.0 | −27.9 | −22.5 |
R3m | −70.08 | −58.6 | −28.9 | −27.1 |
Fig. 6 The second harmonic generation (SHG) signals of perovskite-type RbNbO3, KNbO3 and BaTiO3. The relative intensities were calibrated based on that of α-SiO2. |
The SHG intensity in relation to temperature was measured using a powdered sample, as shown in Fig. S2.† The intensity vs. temperature graph displays kinks around 500 K and 600 K in both the heating and cooling processes, with notable hysteresis. The decreasing intensity in the first run might be attributable to domain reformation. These kinks likely correspond to phase transitions from the Ortho to Tetra1 and from the Tetra1 to Tetra2 phases, respectively. This suggests that the Tetra2 structure maintains non-centrosymmetric symmetry similar to the orthorhombic and Tetra1 phases. Further investigation is necessary to clarify the reversibility and hysteresis of these transitions.
The dielectric constant of a disk-shaped bulk of HPP-RbNbO3 with gold electrodes was measured. The permittivity at 350 K was ca. 50 (f = 1 MHz), comparable to the value (76 at 200 K, f = 1 MHz) reported by Fukuda et al.8 It gradually increased, showing a sharp rise at the ortho-to-Tetra1 transition temperature, as plotted in Fig. S3.† With further temperature increases, samples collapsed at the Tetra1-to-Tetra2 transition, likely due to significant volumetric expansion. This collapse might be attributable to stress application during measurement, as the samples were fixed with clips. The packing density is about 75% for this measurement. The permittivity at room temperature was 60 at 1 kHz, markedly lower than that of KNbO3. However, we expect the intrinsic value to exceed that of KNbO3, considering the stronger distortion in the Tetra2 phase of RbNbO3 (cp/ap = 1.43) compared with the tetragonal phase of KNbO3 (cp/ap = 1.04). A bulk sample with higher density or a larger single crystal is required for accurate evaluation. The precise determination of this value is of significant interest for developing high-performance electronic devices.
Fig. 7(b) illustrates the DSC curves in the heating and cooling processes. The first peak, associated with the ortho–Tetra1 transition above 497 K, showed an enthalpy change (ΔH) of 457 J mol−1, comparable with the O–T transition in KNbO3. In contrast, the second peak above 582 K, corresponding to the Tetra1–Tetra2 transition, indicated a ΔH of 3350 J mol−1, approximately seven times larger than the first transition. This aligns with the observed substantial volume change and is significantly higher than the tetragonal-to-cubic transition in KNbO3,26 as listed in Table 4. No reversible thermal peaks corresponding to these phase transitions were observed.
Phase transition | RbNbO3 transition temp. (K) | RbNbO3 enthalpy (J mol−1) | KNbO3 transition temp. (K) | KNbO3 enthalpy (J mol−1) |
---|---|---|---|---|
Rhomb–Ortho | — | — | 260.4 | 72.47 |
Ortho–Tetra1 | 497 | 457 | 489 | 317.71 |
Tetra1−Tetra2 | 582 | 3,350 | — | — |
Tetra–Cubic | — | — | 702 | 506.89 |
Tetra2−Triclinic | 693 (DTA) | — | — | — |
Our experimentally obtained orthorhombic perovskite-type RbNbO3 at high pressure was consistent with our first-principles calculations. The calculated relative energies of RbNbO3 depending on symmetries are listed in Table 3. These data indicate the most stable symmetry for RbNbO3 at the lowest temperature is Amm2. The energy gap between P4mm and Pmm is significantly larger than those in KNbO3 and BaTiO3, corroborating that no cubic phase appeared experimentally.
Of further interest in perovskite RbNbO3 is the feasibility of stabilizing the high-temperature and high-pressure (HTHP) phase as a thin film. PbVO35 was first obtained as an HTHP phase at 4–6 GPa, and then it was obtained as a thin film28 using the pulsed laser deposition method. As an analogy, we expected that perovskite RbNbO3 could be stabilized as a thin film if we choose substrates with suitable lattice parameters such as KTaO3 (a = 3.989 Å).
The cp/ap ratio increased from 1.07 to 1.43, and the volume expanded by 12%. A similarly strong distortion was reported in tetragonal perovskite PbVO3 (cp/ap = 1.22)5 and BiCoO3 (cp/ap = 1.27)29 that led one tetrahedral oxygen to separate along the c-axis and form a pyramid. Using high-temperature XRD data and Rietveld analysis, as shown in Fig. S4,† we determined the preliminary structural parameters as presented in Table S3.† This transition notably includes one Nb–O bond lengthening from 2.2 Å to 3.0 Å, effectively forming a pyramidal five-coordination as illustrated in Fig. 9.
Fig. 9 Structure models of Nb–O coordination in RbNbO3. (a) Tetra1 (cp/ap = 1.07), and (b) Tetra2 (cp/ap = 1.43) phases. |
Such an elongation extent for c has yet to be reported in the ANbO3 series. However, our previous theoretical calculations predicted a tetragonal–tetragonal phase transition by applying negative pressure in an A′TiO3 (A′ = Ca, Sr, Ba, and Pb) series. The cp/ap ratio of the second tetragonal cell exceeds 1.2, maintaining the space group P4mm,29 which contrasts with the cubic cell with Pmm space group appearing at higher temperatures. For example, in CaTiO3, tetra–tetra phase transition occurs at −4.2 GPa.29 Inspired by such phase transitions, we calculated the phase stability of HPP-RbNbO3 by applying negative pressure. We found a similar phase transition at −1.2 GPa, as plotted in Fig. 10. The tetragonal phase caused by thermal expansion simulates the lattice expansion under negative pressure. A comparison of experimental lattice parameters and calculated ones assuming negative pressure is provided in Table 5. This suggests the possibility of stabilizing the tetragonal phase with a high cp/ap ratio, which is expected to have high permittivity as a thin film by manipulating the lattice size with a suitable substrate.
Phase, Temp. (K) | Exp. lattice parameters, a (Å), c (Å), and v (Å3) | Press. (GPa) | Cal. lattice parameters, a (Å), c (Å), and v (Å3) |
---|---|---|---|
Tetra1, 533 | a = 4.0080(14) | 0.0 | a = 3.992 |
c = 4.3073(15) | c = 4.223 | ||
v = 69.10(2) | v = 69.22 | ||
Tetra2, 643 | a = 3.8249(12) | –1.2 | a = 3.819 |
c = 5.4723(19) | c = 5.650 | ||
v = 80.06(2) | v = 82.45 |
Footnote |
† Electronic supplementary information (ESI) available. CCDC 2327355. For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d4dt00190g |
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