Hubert
Huppertz
*
Institute for General, Inorganic and Theoretical Chemistry, Innrain 52a, Leopold-Franzens-University Innsbruck, A-6020 Innsbruck, Austria. E-mail: hubert.huppertz@uibk.ac.at; Fax: +43(0)512507 2934; Tel: +43(0)512507 5100
First published on 21st September 2010
Most of the syntheses in solid-state chemistry are performed at constant pressure of ∼1 atm (about 105 Pa) by the manipulation of the thermodynamic parameters temperature and composition, leading to a rich variety of compounds. In contrast, the additional variation of pressure has remained virtually unexplored, due to the relatively large costs of maintaining high-pressure conditions and the inevitably tiny sample volumes. In the last two decades, technical advances, developed for studying the properties of minerals, have found access into the preparative solid-state chemistry, opening up tremendously large areas to synthesize new materials.
![]() Hubert Huppertz | Hubert Huppertz studied chemistry at the University of Bayreuth (Germany), followed by a PhD thesis in the field of nitridosilicates in the group of Prof. W. Schnick. For habilitation, he changed to the Department of Chemistry of the Ludwig-Maximilians-Universität München (Germany), establishing a high-pressure laboratory for the syntheses of solid-state materials, followed by a habilitation thesis on new oxoborates through multianvil high-pressure/high-temperature syntheses. Recently, he took up a Chair in Inorganic Chemistry at the University of Innsbruck (Austria), where he is now going to explore the high-pressure/high-temperature chemistry and synthesis of new solid-state materials. |
![]() | ||
| Fig. 1 Schematic assemblage of a high-pressure experiment: (a) cross section of the octahedral pressure cell; (b) finished octahedron; (c) eight truncated tungsten carbide cubes to compress the octahedron; (d) three wedges incorporate the cube; (e) additional wedges from the top; (f) containment ring; (g) cross section of the module with pressure distribution plates; (h) uniaxial 1000 ton press. | ||
With the Walker-type multianvil apparatus, it is now possible to perform experiments with pressures up to 25 GPa, considerably extending the experimental area and gaining new insights into the structural and synthetic possibilities of oxoborate chemistry. In the following, some examples from our research are presented, which can be devided into three sections: (1) the syntheses of new polymorphs of already existing ambient-pressure phases; (2) the syntheses of compounds with new compositions not attainable under ambient-pressure conditions; (3) the access to crystalline phases of borates, forming glasses under ambient-pressure conditions.
![]() | ||
| Fig. 2 Crystal structures of the four structure types of the rare-earth oxoborates RE(BO2)3. | ||
The crystal structure of the meta-oxoborates β-RE(BO2)3 (RE = Tb–Lu) consists of strongly corrugated layers, composed of corner-shared BO4 tetrahedra (Fig. 2, second from the top). Besides the bridging oxygen atoms (O[2]), the structure contains also threefold coordinated oxygen atoms O[3]. The further research with smaller rare-earth metal ions led to the result that only the dysprosium compound was attainable under normal-pressure conditions. For the synthesis of the remainder β-RE(BO2)3 series with RE = Ho–Lu using the corresponding rare-earth oxide and boron oxide as starting materials, high-pressure/high-temperature conditions of 7.5 GPa and 1000 °C were necessary.31
Due to the fact that the monoclinic phases α-RE(BO2)3 were built up from trigonal BO3 and tetrahedral BO4 groups, we assumed a possible transformation into a new modification by applying high-pressure conditions. This assumption was fulfilled by the synthesis of the orthorhombic phases γ-RE(BO2)3 (RE = La–Nd) at conditions of 7.5 GPa and 1000 °C.32,33 As expected for a high-pressure phase in oxoborate chemistry, the structure-type consists purely of corner-sharing BO4 tetrahedra, forming a three-dimensional network (Fig. 2, third from the top). In detail, the crystal structure contains layers of BO4 tetrahedra, further connected via zigzag chains of BO4 tetrahedra. Here, too, threefold coordinated oxygen atoms, O[3], are part of the layers. Naturally, the difference between normal-pressure and high-pressure of 7.5 GPa is remarkable. For example, the calcium borate CaB2O4 exhibits three phase transformations up to a pressure of 4 GPa. Therefore, we analyzed the pressure range below 7.5 GPa and discovered a fourth structure type designated as δ-RE(BO2)3 for RE = La and Ce at 5.5 GPa and 3.5 GPa, respectively.28,34 The crystal structure of these δ-phases is built up exclusively from BO4 tetrahedra, which are linked via common corners to form a network. Fig. 2 (bottom) gives a view of the crystal structure along [100], showing large ten-membered rings occupied by the rare-earth ions, and small, empty four-membered rings.
This example from the rare-earth oxoborates shows remarkably, how pressure can be used to enlarge structure types of known compounds. Additional structure types at higher pressures can be imagined, as the former mentioned high-pressure compounds were all synthesized below 8 GPa.
A second example of a new high-pressure polymorph comes from nonlinear optical (NLO) materials, which are used to generate new lasers with frequencies, that cannot be obtained directly. Since the discovery of the first effective borate material β-BaB2O4 (BBO) being suitable for frequency conversion, the potential of a large variety of borates has been investigated under ambient pressure.35 The most prominent compound in this system is bismuth triborate (BiB3O6, BIBO) because of its exceptional nonlinear optical properties, which has excited the materials community.36–39 In 2005, Liet al. synthesized two new polymorphs of BiB3O6.40 For the sake of clarity, the authors renamed the original bismuth triborate as α-BiB3O6 and the two new modifications as β- and γ-BiB3O6. In contrast to the α phase, which crystallizes in the non-centrosymmetric, monoclinic space groupC2, these modifications crystallize in the centrosymmetric space groupP21/n. Under high-pressure conditions of 5.5 GPa and a temperature of 820 °C, we successfully synthesized a fourth modification δ-BiB3O6 (from a stoichiometric mixture of Bi2O3 and B2O3), which has got again a non-centrosymmetric structure (space group: Pca21).41 As the interatomic spacing is reduced under pressure, one could expect a higher symmetry for the high-pressure phase δ-BiB3O6. However, the center of inversion is lacking in the space groupPca21, prompting to investigate the nonlinear optical properties. Fig. 3 gives a view of the four different modifications of BiB3O6.
![]() | ||
| Fig. 3 The four different polymorphs of BiB3O6. | ||
A comparison between α-, β-, and γ-BiB3O6 shows an increasing density (α: 5.033; β: 5.411; γ: 6.177 g cm−3), running parallel with a transformation of BO3 into BO4 groups. In the ambient-pressure modification α-BiB3O6, the ratio of BO3
∶
BO4 is 2
∶
1, and this ratio changes to 1
∶
2 in β-BiB3O6. The structure of γ-BiB3O6 shows only BO4 tetrahedra. As expected through the high-pressure synthesis, the new phase δ-BiB3O6 exhibits a denser structure (6.378 g cm−3) than the γ modification, prepared under ambient-pressure conditions. Due to the fact that the coordination of the oxygen atoms is identical in both structures (fraction of O[3]: 1/6), the bismuth coordination must be responsible for the higher density. In fact, δ-BiB3O6 has sevenfold-coordinated Bi3+ ions in contrast to sixfold-coordinated Bi3+ ions in γ-BiB3O6. A powder sample of δ-BiB3O6 was subjected to a qualitative powder second-harmonic-generation (SHG) measurement. The intensities of the second harmonics generated by δ-BiB3O6 and by the reference compound KDP, were nearly equal, thus corroborating the non-centrosymmetry of δ-BiB3O6 and indicating a considerable SHG effect of the compound. Interestingly, the structure types of δ- and γ-BiB3O6 are isostructural to the former mentioned compounds γ-RE(BO2)3 (RE = La–Nd) and δ-RE(BO2)3 (RE = La, Ce), respectively. A specific difference lies in the coordination sphere of the metal cations, which is caused by the sterically active lone pair, localized at each Bi3+ center.
Thus, the systematic investigation of the phase diagrams of known compounds, taking into account the parameter pressure, might give access to useful nonlinear optical materials. Therefore, we intend a systematic investigation of new noncentrosymmetric borates synthesized under high-pressure conditions. The question is, whether sufficient amounts of a specific compound can be synthesized for an industrial application? The artificial synthesis of diamond under extreme conditions of pressure and temperature indicates impressively that compounds in the scale of tons can be synthesized under high-pressure conditions, if they are of interest and the pressure does not exceed a value of 6–8 GPa. A second point is the access to small single crystals of the high-pressure phase, which could serve as a seed for crystal growth of the compound in question under ambient-pressure conditions. Third, the high-pressure synthesis can lead to low-temperature modifications, because often the high-pressure modification of a known compound corresponds to a not yet discovered low-temperature form at ambient-pressure conditions. In the case of δ-BiB3O6, Cong et al. were recently able to show that the high-pressure phase corresponds to the low-temperature form, which can be realized at ambient-pressure conditions via a phase transformation starting from β-BiB3O6 after 100 h annealing at 650–670 °C.42
The syntheses of new polymorphs of existing compositions is a highly interesting topic, which is often performed in diamond-anvil cells with the advantage of the in situdetection of phase transformations. A much more demanding challenge is the synthesis of new compositions, whose formation is indispensably based on high-pressure conditions during the syntheses—the topic of the next section.
∶
B2O3. Partly, several polymorphs of these compositions could be obtained at higher temperatures and pressures and a detailed reference list for all compounds can be found in ref. 43. Later on, the compositions REB5O9 and RE4B14O27 were discovered under normal-pressure conditions by Liet al. and Nikelski et al., respectively.44–46
∶
B2O3 (new compositions are shown in italics)
| Composition | RE |
RE2O3 : B2O3 |
RE : B |
|---|---|---|---|
| α-REB5O9 | Sm–Er | 1 : 5 |
0.2 |
| β-REB5O9 | La, Ce | 1 : 5 |
0.2 |
| RE4B14O27 | La | 1 : 3.5 |
0.285 |
| α-REB3O6 | La–Nd, Sm–Tb | 1 : 3 |
0.33 |
| β-REB3O6 | Nd, Sm, Gd–Lu | 1 : 3 |
0.33 |
| γ-REB3O6 | La–Nd | 1 : 3 |
0.33 |
| δ-REB3O6 | La, Ce | 1 : 3 |
0.33 |
| RE4B10O21 | Pr |
1 : 2.5
|
0.4 |
| α-RE2B4O9 | Sm–Ho |
1 : 2
|
0.5 |
| β-RE2B4O9 | Gd , Dy |
1 : 2
|
0.5 |
| RE3B5O12 | Er–Lu |
3 : 5
|
0.6 |
| RE4B6O15 | Dy , Ho |
2 : 3
|
0.67 |
| π-REBO3 | Y, Nd, Sm–Lu | 1 : 1 |
1 |
| μ-REBO3 | Y, Sm–Gd, Dy–Lu | 1 : 1 |
1 |
| λ-REBO3 | La–Nd, Sm, Eu | 1 : 1 |
1 |
| β-REBO3 | Sc, Er–Lu | 1 : 1 |
1 |
| ν-REBO3 | Ce–Nd, Sm–Dy | 1 : 1 |
1 |
| χ-REBO3 | Dy–Er | 1 : 1 |
1 |
| H-REBO3 | La, Ce, Nd | 1 : 1 |
1 |
| RE8.66O8(BO3)2(B2O5) | Ho | 8.66 : 4 |
2.165 |
| RE17.33O16(BO3)4(B2O5)2 | Y, Gd | ∼8.7 : 4 |
2.175 |
| RE3BO6 | Y, La, Pr–Lu | 3 : 1 |
3 |
| RE26O27(BO3)8 | La, Nd | 13 : 4 |
3.25 |
| RE31O27(BO3)3(BO4)6 | Ho |
31 : 9
|
3.44 |
Applying high-pressure/high-temperature conditions on stoichiometric mixtures of rare-earth oxides and boron oxide, we were able to synthesize five new compositions in this system, namely, RE3B5O12,47RE4B10O21,48,49RE31O27(BO3)3(BO4)6,43RE4B6O15,50,51 and RE2B4O952–56 (in italics in Table 1). These compounds possess a remarkable metastability up to 600–800 °C before they decompose into the corresponding ortho-borates or meta-borates under ambient-pressure conditions. For example, successive heating of Yb3B5O12 from the series RE3B5O12 (RE = Er–Lu) in the range of 800–900 °C led to a decomposition into a mixture of μ-YbBO3 and π-YbBO3. The compounds crystallize into a novel structure type, being homeotypic with the beryllosilicate mineral semenovite ((Fe2+, Mn, Zn, Ti)RE2Na0−2(Ca, Na)8(Si, Be)20(O, OH, F)48). Thus, the compounds RE3B5O12 (RE = Er–Lu) represent an outstanding example of complex silicate structures in the field of borates using high pressure.
With the high-pressure synthesis of RE4B10O21 (RE = Pr) at a relatively mild pressure of 3.5 GPa, we obtained a rare-earth oxoborate structure of BO3 and BO4 groups in the ratio 1
:
4, which are linked to a highly connected network in accordance with the relatively high amount of boron in the formula (RE2O3
:
B2O3 = 1
:
2.5).
On the other hand, we were able to synthesize the compound RE31O27(BO3)3(BO4)6 (RE = Ho) with the lowest percentage of boron in a trivalent rare-earth oxoborate up to now.43Fig. 4 shows the structure of Ho31O27(BO3)3(BO4)6, displaying isolated BO4 tetrahedra as dark hatched polyhedra and BO3 units in form of ball-and-stick models, embedded in a complex holmium oxide network.
![]() | ||
| Fig. 4 Crystal structure of Ho31O27(BO3)3(BO4)6. (BO3 groups are shown in form of a ball-and-stick model; BO4 tetrahedra are visualized through polyhedra; large spheres: Ho3+, small spheres: O2−). | ||
RE31O27(BO3)3(BO4)6 (RE = Ho) represents the most metal rich rare-earth oxoborate known up to now. Based on our experience, we would have expected exclusively BO4 tetrahedra for a compound, which was synthesized under the extreme pressure conditions of 11.5 GPa (pressure coordination rule).18,19 Nevertheless, Ho31O27(BO3)3(BO4)6 also contains trigonal-planar coordinated boron atoms, which are exceptional for a material synthesized under such conditions. In the past, all oxoborate compounds synthesized at pressures exceeding 8 GPa revealed exclusively BO4 tetrahedra. All the more it is astonishing that the BO3 group is stable in the structure of Ho31O27(BO3)3(BO4)6, especially in the plethora of oxygen atoms.
In this context, the general influence of increased pressure on the structure of new oxoborates attracts our intention. It was already mentioned that the coordination number of the boron atoms can be enhanced from three to four. Additionally, the metal cations and the oxygen anions (O[2] → O[3]) often reveal higher coordination numbers in comparison with compounds under normal pressure conditions. However, the most striking discovery was the structural motif of edge-sharing BO4 tetrahedra ([B2O6]6− units), which was observed for the first time in 2002 in the rare-earth borate Dy4B6O15 and two years later in the isotypic holmium phase Ho4B6O15.50,51Fig. 5 gives a view of the corresponding crystal structures.
![]() | ||
| Fig. 5 Crystal structures of the four known structure types in the chemistry of oxoborates, which exhibit the structural motif of edge-sharing BO4 tetrahedra (partially marked as red polyhedra). Except for KZnB3O6, these compounds were synthesized under high-pressure conditions. | ||
A second series of borates, having edge-sharing BO4 tetrahedra in a different structure type, could be synthesized with the composition α-RE2B4O9 (RE = Sm–Ho).52–54 In these examples, only a fraction of 1/3 (RE4B6O15 (RE = Dy, Ho)) or 1/10 (α-RE2B4O9 (RE = Sm–Ho)) of the BO4 tetrahedra bridge to a second tetrahedron via a common edge. The corresponding polymorphs β-RE2B4O9 (RE = Dy, Gd) did not show BO4 tetrahedra with common edges.55,56 The latest high-pressure experiments with transition-metal borates yielded a third structure type with edge-sharing tetrahedra. The special feature of the compound HP-NiB2O4 is that in contrast to the first two compounds, all tetrahedra are linked to each other via one common edge and two common corners.57 Meanwhile, it was possible to prepare the isotypic structures β-FeB2O458 and HP-CoB2O4.59 To our astonishment, the structural feature of edge-sharing BO4 tetrahedra was recently found in the compound KZnB3O6, which was synthesized under ambient-pressure conditions.60,61 This result means that the structural motif of edge-sharing BO4 tetrahedra is no longer a domain of high-pressure chemistry, but still favoured under these conditions, as there exist eleven different compounds with three structure types prepared under high-pressure and only one compound synthesized under ambient-pressure conditions. Fig. 5 summarizes all four structure types known up to now, in which the structural motif of edge-sharing BO4 tetrahedra was observed.
Additionally to the syntheses of new compounds with fascinating structural features, high-pressure gives us access into a variety of systems, which are normally glass formers. The next section will give a view of the power of high-pressure in glass forming systems.
In this context, we had a look into the ternary system Sn–B–O as a simplified variant of the tin-based amorphous composite oxides (TCO), materials in use as negative electrodes of lithium-ion rechargeable batteries. Several investigations were performed in this system and because all compounds in this area were glasses, the synthesis of crystalline approximands for a more detailed structural investigation would be favourable. In fact, the use of high-pressure/high-temperature of 7.5 GPa and 1100 °C led to the synthesis of the first crystalline tin borate β-SnB4O7.63Fig. 6 gives a view of the crystal structure of β-SnB4O7, which is purely built up of corner-sharing BO4 tetrahedra, being isotypic to the known high-pressure phases β-CaB4O722 and β-HgB4O7,24 as well as to the ambient-pressure phases SrB4O7,64,65PbB4O7,66 and EuB4O7.67
![]() | ||
| Fig. 6 Crystal structure of β-SnB4O7. | ||
Generally, we would expect that the nucleation and growth of a crystalline phase from the amorphous “SnB4O7” with increasing pressure gets impeded by a suppressed ionic mobility at higher pressures. However, these observations suggest that the reconstructive formation of the more densely packed compound β-SnB4O7 under pressure is kinetically not restricted at a temperature of 1100 °C.
In a further step, we had a look at the ternary systems Hf–B–O and Zr–B–O, where no defined crystalline materials could be obtained via conventional synthetic routes until then. The experiments in the ternary system Hf–B–O were successful with the synthesis of the first hafnium diborate β-HfB2O5 starting from a stoichiometric mixture of HfO2 and B2O3.68 Due to the fact that this compound is a high-pressure phase, we labelled it with the Greek character “β”. Later on, it became also possible to synthesize the isotypic zirconium phase β-ZrB2O5 under similar conditions.69 Attempts to synthesize the ambient-pressure hafnium diborate and zirconium diborate “α-MB2O5 (M = Zr, Hf)” are ongoing. Fig. 7 gives a view of the crystal structure of β-MB2O5 (M = Zr, Hf), showing layers of BO4 tetrahedra and M4+ (M = Zr, Hf) ions.
![]() | ||
| Fig. 7 Crystal structure of β-MB2O5 (M = Zr, Hf). | ||
The arrangement of the BO4 tetrahedra in β-MB2O5 (M = Zr, Hf), with four- and eight-membered rings, shows that the topology of the tetrahedra is identical to the arrangement in silicate minerals of the gadolinite group.70 Several important minerals and synthetic compounds belong to the gadolinite group (space groupP21/c), which can be represented by the general chemical formula A2Z2XSi2O8(O,OH)2. In this context, the compounds β-MB2O5 (M = Zr, Hf) can be considered as the simplest structural variant of all compounds belonging to the complex gadolinite family. For a more detailed discussion of the interesting structural relationships, the reader is referred to ref. 68.
The latter examples show impressively that pressure favours the formation of crystalline oxoborates in contrast to normal-pressure investigations, which often lead to amorphous compounds (glasses). In the future, we hope to have access to a large variety of other systems, of which no compounds exist until now.
In a first approach, it was possible to synthesize a new series of fluoride borates with the composition RE5(BO3)2F9 (RE = Er, Tm, Yb) (Fig. 8) starting from stoichiometric mixtures of RE2O3, REF3, and B2O3.80–82
![]() | ||
| Fig. 8 Crystal structure of the fluoride borates RE5(BO3)2F9 (RE = Er, Tm, Yb); BO3 groups are shown in the form of a ball-and-stick model; large spheres: RE3+, small spheres: F−. | ||
These rare-earth fluoride borates exclusively consist of isolated trigonal BO3 groups, rare-earth cations, and fluoride anions, closely related to the compounds RE3(BO3)2F3 (RE = Sm, Eu, Gd)83,84 and Gd2(BO3)F3.85 In fact, all three structure types can be described by different sequences of layers with the formal composition “REBO3” and “REF3”.
Since the compounds RE5(BO3)2F9 (RE = Er, Tm, Yb) contain only trigonal BO3 groups, it was attractive to synthesize a fluoride borate with BO4 groups by higher pressure. Consequently, we were able to synthesize Gd4B4O11F2, in which BO3 groups and BO4 tetrahedra were found, connected via common corners (Fig. 9).86
![]() | ||
| Fig. 9 Crystal structure of Gd4B4O11F2, showing the fundamental building block units, consisting of BO3 groups and BO4 tetrahedra. Large spheres: Gd3+, small spheres: F−. | ||
A much more complicated structure is found for the lanthanum fluoride borate La4B4O11F2, which shows the same formula but a different rare-earth cation.87 The crystal structure is fairly complicated with a large unit cell built up from BO4 tetrahedra interconnected with two BO3 groupsvia common vertices, B2O5-pyroborate units, and isolated BO3 groups. Fig. 10 gives a view of the crystal structure of La4B4O11F2.
![]() | ||
| Fig. 10 Crystal structure of La4B4O11F2, consisting of La3+ and F− ions, BO3 groups and BO4 tetrahedra. | ||
The b lattice parameter is about five times longer than the other cell edges. Looking at the structure along c, a wave-like modulation of the cations and the B–O-polyhedra with a formal wavelength λ = b was observed. In contrast to the well known Vernier phases,88–91 no separation into mismatching substructures was found in La4B4O11F2. In analogy to the meta-oxoborates, continuing experiments on the formation range of the compounds RE4B4O11F2 will be undertaken. It will be of great interest to see, which crystal structure is favoured by the rare-earth ions of intermediate size and whether it will be possible to obtain both structure types as polymorphs for one and the same cation.
In principle, most of the working areas in solid-state chemistry can be extended into the regime of high-pressure. This often results in interesting collaborations, e.g. in the field of gallium oxonitrides.
:
1. Later on, we systematically investigated the stability field of this spinel phase by reactions between hexagonal GaN and monoclinic β-Ga2O3 with different molar ratios under specific high-pressure/high-temperature conditions.99 Therewith, initial conditions of 2.5–11.5 GPa at temperatures between 1000–1300 °C could be stated as leading to the formation of cubic, spinel-type gallium oxonitride phases.
From one of these experiments, (GaN
:
Ga2O3 = 9
:
1; 5 GPa, 1250 °C), the isolation of single crystals of spinel-type gallium oxonitride became possible for the first time.100 The combination of energy dispersive X-ray spectroscopy (EDS) with electron energy-loss spectroscopy (EELS) allowed the quantification of nitrogen and oxygen for the structural refinement of the single-crystal data (N/O = 0.25 ± 0.06). The observation of a site occupation deficiency of the octahedral gallium site led to the composition Ga2.79□0.21(O3.05N0.76□0.19). In the literature on oxonitrides, crystal defects in spinel-type materials are handled with different models, mainly by the assumption of a constant anion model.101–103 The results of the single-crystal structure determination indicate that this model is doubtful, and one should take into account a model with both cation and anion vacancies. A more detailed discussion of the single-crystal refinement and the consequences for the occupation of the crystallographic sites can be found in ref. 100.
Furthermore, we performed in situdiamond anvil cell (DAC) investigations, using the end members w-GaN and β-Ga2O3 in a first route and an amorphous gallium oxonitride ceramic in a second one.104 Both approaches led to remarkable new insights into the formation tendencies of gallium oxonitride spinel-type compounds.
Footnote |
| † This article is part of the ‘Emerging Investigators’ themed issue for ChemComm. |
| This journal is © The Royal Society of Chemistry 2011 |