- 1. Introduction
- 2. Some peculiarities of complex f.c.c. intermetallics
- 3. Structures with space-group symmetry F[\bar{4}]3m
- 4. Structures with space-group symmetry Fd[\bar{3}]m
- 5. Structures with other space-group symmetries
- 6. First-principles studies
- 7. Conclusions
- Supporting information
- References
- 1. Introduction
- 2. Some peculiarities of complex f.c.c. intermetallics
- 3. Structures with space-group symmetry F[\bar{4}]3m
- 4. Structures with space-group symmetry Fd[\bar{3}]m
- 5. Structures with other space-group symmetries
- 6. First-principles studies
- 7. Conclusions
- Supporting information
- References
feature articles
Structural building principles of complex face-centered cubic intermetallics
aLaboratory of Crystallography, Department of Materials, ETH Zurich, Wolfgang-Pauli-Strasse 10, 8093 Zurich, Switzerland
*Correspondence e-mail: steurer@mat.ethz.ch
Fundamental structural building principles are discussed for all 56 known intermetallic phases with approximately 400 or more atoms per p. The atoms on this set of layers, which intersect each other, form pentagon face-sharing endohedral fullerene-like clusters arranged in a face-centered cubic packing (f.c.c.). Due to their topological layer structure, all these crystal structures can be described as (p × p × p) = p3-fold superstructures of a common basic structure of the double-diamond type. The parameter p, with p = 3, 4, 7 or 11, is determined by the number of layers per repeat unit and the type of cluster packing, which in turn are controlled by chemical composition.
and space-group symmetry , , , or . Despite fundamental differences in chemical composition, bonding and electronic band structure, their complex crystal structures show striking similarities indicating common building principles. We demonstrate that the structure-determining elements are flat and puckered atomic {110} layers stacked with periodicities 21. Introduction
Why and how do complex intermetallic phases form with up to thousands of atoms per
or even in a quasiperiodic way without a unit cell? How do all these atoms find their sites during crystal growth? How do their structures depend on chemical composition and do they have anything in common? All these questions are in the focus of our long-term study of the crystallography of complex intermetallics, periodic as well as quasiperiodic ones. In this first comprehensive classification of intermetallics with giant unit cells, we discuss all known f.c.c. structures in the range from approximately 400 up to more than 23 000 atoms per unit cell.Structural complexity can result from:
In some cases complex structures can be described as modulations or superstructures of rather simple basic structures. We distinguish two classes of modulations: a simple modulation is a correlated displacement or substitution of atoms leading to a comparatively small deviation of the actual structure from the underlying basic structure, resulting in a (in)commensuratly modulated structure. A complex modulation on the other hand results from a correlated displacement or substitution of atoms leading to the local formation of clusters yielding a cluster-modulated structure; as we will show, this is the case for all structures discussed in the following.
There is no unique way to classify, describe and visualize the ) for the definition of AETs, which can be seen, in some cases, as the first shell of a multi-shell cluster. However, there are not usually such simple rules for higher-order cluster shells. Furthermore, even if one finds a topologically elucidating cluster-based description, this does not mean that it is supported from a crystal-chemical point of view, i.e. that the chemical bonds between atoms within a cluster differ from those outside a cluster. For a more detailed discussion of this problem see Steurer (2006) and Henley et al. (2006).
of a complex intermetallic compound. One should keep in mind that the visualization of a in terms of clusters (in the meaning of structural building blocks) or structure modules can be quite arbitrary. There are some conventions and rules, such as the maximum-gap rule (Brunner & Schwarze, 1971In the following we will pragmatically utilize this kind of cluster description that proves to be most useful. This is the case when it allows for a simpler representation of a structure which is simpler than any other geometrical description; it is particularly justified if the clusters used are constituents of more than just a single structure type. A useful cluster-based description relates complex structures to simpler ones, thereby reducing the degree of complexity and unveiling the underlying packing principles. In this case of f.c.c. structures, the fundamental endohedral pentagon face-sharing fullerene-like clusters form cubic close packing with the octahedral voids filled with a second type of cluster. The choice of this kind of cluster is particularly justified because it allows the family of giant unit-cell structures cF444-Al63.6Ta36.4, cF(5928-x)-Al56.6Cu3.9Ta39.5 and cF(23256-x)-Al55.4Cu5.4Ta39.1 (Weber et al., 2009; Conrad et al., 2009) to be described in a unique way.
We want to emphasize that our goal is the crystallographic description of complex structures, to identify their structural building units and connectivities. A detailed analysis of chemical bonding and the identification of chemically relevant subunits such as polyanionic frameworks is beyond the scope of this study.
The paper is organized in the following way: in §2 we describe the data basis of the present study and introduce the general packing principles and peculiarities we derived for f.c.c. structures with giant unit cells; in §§3, 4 and 5 we apply our concept of cluster description, layer decomposition and average structure derivation to the 56 intermetallics grouped according to their symmetries (39), (9), (1), (4) or (3); in §6 we discuss the results of ab initio calculations of representatives of the two most frequent structure types and show that chemical bonding and electronic band structure differ significantly between all these geometrically closely related structures.
2. Some peculiarities of complex f.c.c. intermetallics
Our study is based on structures taken from Pearson's Crystal Data database (PCD; Villars & Cenzual, 2009/10). Full structural information is only available for 10 655 of the 41 788 intermetallics1 included in this database. However, these numbers refer to database entries and not necessarily to structures of different compounds; for some compounds, more than one entry may exist based on different structure determinations. We restrict our study to the fully determined structures and start with the analysis of 1891 entries with cubic symmetry and focus first on the 842 with f.c.c. lattice symmetry: (4 entries), (1 entry), (305 entries), (249 entries), (76 entries) and (207 entries).2
The histogram in Fig. 1 lists the number of database entries of f.c.c. structures as a function of the number of atoms per Obviously, the majority of f.c.c. structures has unit cells with less than 200 atoms. Another significant clustering of structures is found at around 400 atoms per while even larger structures are sparse. These are the structures we will focus on in the following, taking into account both their comparably high frequency and complexity. In this survey, we also consider the two recently discovered structures cF(5928-x)-Al56.6Cu3.9Ta39.5 and cF(23256-x)-Al55.4Cu5.4Ta39.1 (Weber et al., 2009; Conrad et al., 2009), with space-group symmetry , which are not included in the databases yet, as well as structures taken directly from the literature and another database, the ICSD (Belsky et al., 2002). Most of the 56 structures selected (Table 1) belong to just two space groups, and , with 39 and 9 entries. , and are represented altogether by eight entries only. These 56 complex intermetallics differ strongly in their chemical properties. They range from Zintl phases to transition metal aluminides, from alkali-metal/alkaline-earth metal compounds to ones just between transition metals. Consequently, since their crystal structures are similar they are dominated by geometrical packing principles rather than by the significantly differing chemical bonding or electronic interactions.
|
A short comment on preferred space-group symmetries: the
of a cluster centered at a given is that of this special site; of course, the symmetry of a cluster is controlled by the most energetically favorable atomic arrangement under the constraint of optimum cluster packing and not by the Wyckoff symmetry of the The symmetry of a cluster determines the type of it can be described with and constrains the number of possible space groups characterizing its packing. In other words, the space-group symmetry of a structure is a consequence, and not the origin of the best possible packing of atoms, AETs or clusters under the constraint of free-energy minimization.In the case of the most frequent space-group symmetries among the structures we chose for examination and , the AETs most useful for the structural description will be tetrahedra (t) and truncated tetrahedra (tt) decorated with atoms, AETs or clusters. Only a single packing of uniform polyhedra exists that shows global tetrahedral symmetry, , which is just a packing of these two types of regular polyhedra.
2.1. Packings of tetrahedra, truncated tetrahedra and endohedral clusters
The tt is one of the AETs constituting the Frank–Kasper (FK) phases. In most cases the tt are centered by one type of atom, A, while all 12 vertices are occupied by another type, B; four more atoms of type A cap the h(exagon) faces of the tt. This gives a total (CN) of 16 for the central A atom. Therefore, this AET is usually termed CN16 FK polyhedron or Friauf polyhedron FK2816. Hereafter Frank–Kasper polyhedra will be expressed by FKFV if they exhibit F triangle faces and V vertices. The size of the tt is determined by the distance dB—B = a between B atoms, where a is the edge length of the tt; dA—A = a/2 ≃ 1.22474a and dA—B = a/4 ≃ 1.17260a. In case types A and B atoms correspond to hard spheres with radii a/4 ≃ 0.61237a and a/2; all atoms would only touch atoms of the same type. Consequently, Friauf polyhedra are energetically more favorable if attractive A—A and B—B interactions are stronger than A—B interactions. The ideal ratio of the atomic radii corresponds to . The difference between dA—B and the summed-up radii of atoms A and B is 0.06023a, which would be the gap width in the case of equally sized hard spheres. In an atomic arrangement this gives the tt some flexibility to distort and allows for a large variety of packings.
Layers of tt/t can be stacked to give cubic or hexagonal structures with the general composition AB2 such as the Laves phases cF24-MgCu2, hP16-MgZn2 and hP24-MgNi2. A different stoichiometry results from three-dimensional frameworks or spherical clusters of tt/t (e.g. the Samson cluster). While tetrahedral symmetry prevails in the first case, pentagonal arrangements are typical for the second. The outer shell of B atoms forms fullerene-like structures (fullerenes, for short) FFV with 12 p(entagon) faces plus H h faces (F = 12+H) and V = 20+2H vertices. H equals the number of Friauf polyhedra constituting the cluster shell. The outer A atoms form generalized FK polyhedra FKFV with V faces and F vertices (deltahedra, covered by only triangular faces with either five- or sixfold vertex symmetry; Alvarez, 2005, 2006). The inner cluster shell formed by the triangle faces of the Friauf polyhedra is a FK polyhedron with H faces.
2.2. description
All the complex intermetallic structures discussed in this work can be regarded as (p×p×p)-fold (or p3-fold) superstructures of a basic structure (p = 3, 4, 7, 11). The easiest way to recognize a smaller unit underlying the periodic cell is by evaluating the diffraction pattern with respect to the strongest reflections. This is obvious from the calculated diffraction patterns as they are shown in Fig. 2 for the mentioned superstructures and possible basic structures (see below). Therein, the strongest reflections of structures considered as being p3-fold superstructures with p = 3, 4, 7, 11 bear the indices 6 6 0, 8 8 0, 14 14 0 and 22 22 0, corresponding to face-centered unit cells of the respective metric.
The fact that the compounds investigated are superstructures can be easily visualized by their distinct average structures, as shown in the respective sections (§§3.1, 3.3, 4 and 5). The average structure of a results if it is projected into one of the basic structure. Previously the structures were usually discussed as (2×2×2)-fold superstructures of the -brass structure type, cI52-Cu5Zn8 (Johansson & Westman, 1970; Arnberg et al., 1976; Booth et al., 1977; Fornasini et al., 1978; Lidin et al., 1994; Thimmaiah et al., 2003; Berger et al., 2008). This structural relationship seemed obvious since the structures also feature 26-atom groups that were previously identified as constituents of -brasses. On the other hand, the -brass structure itself can be considered as already being a (3×3×3)-fold of the cP2-CsCl structure type, with two sites of this vacant. Accordingly, the structures with p = 3 () can also be regarded as (6×6×6)-fold superstructures of the cP2-CsCl type.
Using the example of cF444-Al63.6Ta36.4 Fig. 3 shows the as well as the different average structures projected along [001]. The corresponding basic structures have space-group symmetries (23-fold of cP52-P-cell--brass), (33-fold of a cF16-NaTl derivative) or (63-fold of a cP2-CsCl-type structure). The symmetry relations can be directly read from the diagram in Fig. 4. They are also listed in detail in Section 1 of the supplementary material.3 Accordingly, the indices of the group–subgroup relations are easily determined as 2, 27 and 108.
Using the cF16 for the basic structure we not only preserve the maximum () but also the centering. Alternatively, the CsCl structure type may be used, however, involving the loss of F-centering. The -brass structure does not appear to be the ideal choice for a simple reason: the superstructures with p = 8, 14, 22 with regard to the cP2-CsCl-type cannot be described as superstructures of -brass, which itself is a (p = 3)-fold of cP2-CsCl. Hence we choose the cF16-NaTl structure type as the basic structure for a unifying description with maximum symmetry.
As mentioned before, another indication of an underlying basic structure is based on the intensity distribution of the diffraction patterns: the shows the calculated diffraction patterns of representative structures for all unit-cell dimensions discussed here.4 Obviously, the reflections of highest intensity are the same for all structures. Their indices are also given in the graph and increase with increasing unit-cell size, while the sets of net planes they refer to remain the same. Consequently, all the structures discussed here can be regarded as superstructures of a cF16-NaTl-like cell. In principle, they can also be regarded as superstructures of cP2-CsCl (the same is true for cF16-NaTl and -brass-type structures).
of a features a subset of strong reflections related to the average structure along with a much larger number of weak reflections caused by deviations from the basic structure. Fig. 22.3. Basic structures
The basic structures of all the cubic compounds discussed here are of the cF16-NaTl structure type () or of one of its derivatives with lower symmetry. The details and symmetry of these basic structures are given in Section 1 of the supplementary material.
For the p = 3 superstructures with space groups and the symmetries of the basic structures with the cF16 are the same as for the respective superstructures.
The basic structures of the p = 4 superstructures are of the type cP16, geometrically similar to the previously discussed cF16-NaTl structure type but with different site relationships. The average structure of cF1124-Cu56.9Cd43.1 (), with , looks more scattered in comparison to the p = 3 ones. The average structures of cF(1192-40)-Cd66.7Na33.3 and cF(1192-23)-Al53.6Mg46.4 () look similar to that of cF1124-Cu56.9Cd43.1 and also exhibit a reduction in lattice symmetry, but in this case to . The same is true for the p = 4 superstructures in space groups and such as cF(944-22)-Zn67.1Sn20.8Mo12.1. The basic structure of the superstructures with symmetry can be described in the , which is a translationengleiche of .
Fig. 4 illustrates the group–subgroup relations between all relevant space groups of the f.c.c. complex intermetallics and their average (and basic) structures. Each prototype structure is represented by its and – if available – the name of the structure type, a representative or a very similar structure. Direct symmetry transitions are shown by arrows, pointing from super- to and bearing a symbol which expresses the type of – t for translationengleiche and k for klassengleiche – as well as its index.
The symmetry graph starts with the cI2-W structure type (). The average structure types discussed above are derived via the cP2-CsCl type and other intermediate structures. They exhibit space groups , and in the case of (p = 4)-superstructures (cP16) and space groups and for the other compounds (cF16). The space groups of the average structures are marked in green and the space groups in red in Fig. 4. The structure types found to be related to the displayed prototype structures are given in Table 2 of the supplementary material. The atomic sites in the different space groups and their interrelations are given in Tables 3–17 of the supplementary material.
|
2.4. Fundamental sets of atomic layers and the concept
All crystal structures in thermodynamic equilibrium show n-dimensional lattice symmetry, with n = 3 for regular crystals and for aperiodic crystals such as quasicrystals or incommensurate crystals.
The topological decomposition of crystal structures into atomic layers parallel to low-indexed lattice planes frequently gives insight into the structural building principles.
It has already been pointed out by Samson (1964) that every special (crystallographic orbit) of the space groups F23, , F432, and places at least one point on the (110) plane, which he named the `most useful plane' for structure analysis. With some restrictions, this is also true for the cubic space groups F4132, and .5
In the projected structures a clear layer structure can be seen. There are 2p (110) layers per period. For p = 3, for instance, one flat layer, located on a mirror plane, is sandwiched between two puckered layers. Each adjacent pair of such three-layer stacks (3S) is related by a glide plane yielding the stacking sequence 3S–3S′–3S–3S′ along [110], with 3S′ representing the three-layer stack symmetrically equivalent to 3S.
Since the set of {110} layers consists of a framework of six, mutually intersecting, symmetrically equivalent layers, there are not so many left for decorating the layers properly, i.e. with reasonable atomic distances. In the case of an energetically favorable formation of particular AETs and larger clusters, additional constraints are imposed. The unit-cell dimensions of the discussed complex intermetallic phases are controlled by the number of layers, which in turn depends on the cluster size and their way of packing.
In the case of layer structures, we can expect the existence of average structures. In other words, the actual structures can be seen as superstructures or modulated structures. In the case at hand, the underlying basic structure common to all structures is related to a type of double-diamond structure. Taking the actual structure modulo the hkl and h,k,l = 3n have particularly high intensities (Fig. 2, see §2.3).
of the basic structure gives the average structure. Thereby each three-layer stack is projected into a single flat layer located on a mirror plane. This approach is obvious in There the Bragg reflections with indicesIn the case of some structures with p = 4, the {100} layers are also quite important. In the case of the {110} layers are no longer relevant, only the {100} ones (as can be seen in §5.2). This structure can certainly be seen as cluster-dominated, which is also reflected in the average structure.
3. Structures with space-group symmetry F3m
Of the 39 complex intermetallics crystallizing in the (3×3×3)-fold superstructures of a double-diamond-type basic structure with unit-cell parameters similar to those of the (fictitious) cubic Laves phase in the respective system. The others, cF1124-Cu56.9Cd43.1 (Samson, 1967), cF(5928-20)-Al56.6Cu3.9Ta39.5 and cF(23256-122)-Al55.4Cu5.4Ta39.1 (Weber et al., 2009; Conrad et al., 2009), correspond to p3-fold superstructures with p = 4, 7 and 11.
, all but three can be regarded asFor the 36 structures with p = 3, certain similarities – of chemical as well as purely geometrical type – become apparent immediately. Since they share a considerable amount of common atomic sites, they can be grouped into four different subtypes of one (Table 1). In Fig. 5 the projected unit cells are shown for one representative of each subtype together with its average structure. The atomic coordinates of an average structure can be obtained by taking all atomic coordinates modulo the of the basic structure: (xav,yav,zav) = (px,py,pz) mod (1). The basic structure in turn is related to cF16-NaTl.6
| Figure 5 . The projection of the along the |
In Table 1 the Pearson symbols for the different structural subtypes are shown with the number of atoms for fully occupied atomic sites minus x, the total number of missing atoms [e.g. cF(432-x)]. In the case of partially occupied sites, on average x need not be an integer. For the mixed subtypes I/II the set union is given and part of the sites are bound to be unoccupied in order to produce a physically valid structure. The variants II′ and III′ include additional sites increasing the number of atoms per unit cell.
3.1. (3 × 3 × 3)-fold superstructures – cF(464 − x)
The four subtypes of (3×3×3)-fold superstructures have in common a formed by a subset of eight atomic sites (see upper part of Table 2). The rather small standard deviations of the averaged atomic coordinates (obtained by averaging the respective coordinates of all 36 structures with symmetry ) indicate that these four structures are quite similar variants of one and the same There are only small differences in the occupancies and/or the way of splitting some sites. The sites whose occupations differ among the different structural subtypes are given in the lower part of Table 2.
Consequently, all representatives of the (3×3×3)-fold class show a cluster structure similar to that of cF444-Al63.6Ta36.4 (Conrad et al., 2009), which can be seen as cubic close packing of three-shell clusters with the shape of a F4076 fullerene (with 40 faces and 76 vertices) and tetrahedral symmetry. These clusters share their 12 p faces with their neighbors. The second cluster shell is formed by a FK7640 polyhedron (76 triangle faces and 40 vertices) dual to the fullerene shell.7 The first (innermost) shell corresponds either to a CN14 rhombic dodecahedron or a CN16 Friauf polyhedron (Fig. 6), which are centered by an atom in some structures and in others are not.
This main cluster is centered at one of the four points of highest symmetry, , in i.e. the Wyckoff positions 4a 0,0,0, 4b , 4c or 4d . They are essentially interchangeable, as the space-group symmetry is invariant with respect to origin shifts of , or . With this in mind, all these sites are equally considered as centers of significant clusters.
,3.1.1. First cluster shell
The rd) around the points of highest symmetry, subtype II three rhombic dodecahedra and one Friauf polyhedron (F), subtype III two of each kind and subtype IV three Friauf polyhedra and only one rhombic dodecahedron. The arrangement of these first-shell clusters along the body diagonal of the – at 0,0,0; ; ; – is the following:
structure corresponds to the union of the different subtypes. Subtype I contains only rhombic dodecahedra (In the actual structures reduced rd forms are also observed when some sites remain unoccupied, resulting in either an octahedron with only half of its faces capped or a cube. Some structures between the subtypes are also found, Zn89.1Ir10.9, Zn90.5Ir9.5 and Zn91.1Ir8.9, which exhibit a partially occupied Friauf polyhedron and a rhombic dodecahedron centered on the same site. Corresponding to the often disordered first cluster shells, the positions of the central atoms are disordered in numerous cases.
3.1.2. Second cluster shell
The second cluster shell has the same shape in all subtypes of the FK7640 polyhedron is found for all structures at sites 4a–4d. The corresponding atomic positions build the which is common to all cF464 structures in the .
the3.1.3. Third cluster shell
Contrary to the second cluster shell, the third shell varies in shape from subtype to subtype. All different versions, as well as their respective types of faces (triangles t, quadrangles q, pentagons p and hexagons h) are given in Fig. 6.
In subtype I the third cluster shell is the same for all alternative sites (4a–4d): a 58-vertex polyhedron. The third-shell polyhedra go through a series of changes with evolving structural subtypes, as shown in Fig. 6. (The exact changes of the third-shell cluster throughout the different subtypes are listed in Table 20 of the supplementary material.) The noticeable F4076 fullerene-like polyhedron is found on position 4c in subtypes III and IV.
The sites forming the different cluster shells are given in Table 18 of the supplementary material. Also given are their occupations for all discussed compounds in Tables 24 and 25 of the supplementary material.
3.2. Comment on the definition of cluster types
In connection with the description of the cF(464-x) structures as superstructures of the -brass structure type (see above), the atomic sites closest to the four Wyckoff positions 4a–4d were directly referred to as `clusters'. Their packing was evaluated and their divided into simpler polyhedra, directly apparent from the respective site symmetries (Johansson & Westman, 1970; Arnberg et al., 1976; Booth et al., 1977; Fornasini et al., 1978; Chabot et al., 1980; Fornasini et al., 1986; Thimmaiah et al., 2003; Hornfeck et al., 2004). In this approach the atomic distances in the outer `shells' become much larger than the sum of the atomic radii. In our cluster description, on the contrary, we only allow for polyhedra with edge lengths in the range of atomic interactions close to nearest-neighbor distances in the compound.
For comparing clusters, identifying different cluster shells and evaluating their spacing and their thickness/sphericity, a histogram of the interatomic distances can be quite useful. The number of atoms constituting the cluster shells must increase quadratically with the radius to keep their density constant (and also atomic distances).
The analysis of the interatomic distances in Al63.6Ta36.4 shows that the separation of cluster shells becomes increasingly difficult with increasing distances from the central atom. The first shell is quite easily recognizable around sites of all symmetries, while the definition of the second shell becomes quite ambiguous around low-symmetry sites. Fig. 7 shows the histograms corresponding to the highest symmetric atomic environments of sites 4b, 4c and 4d, as well as the unoccupied site 4a. In these diagrams the displayed atomic sites are specified, as well as the thicknesses of the three cluster shells around each of these positions. They can be separated to a different degree: the second and third shell at site 4d are not separated and around 4a and 4d the third shell is already overlapping with atomic sites belonging to the outer region. The best separation is found between the clusters at site 4c, which show larger distances between atoms of different cluster shells than the other ones. The distances between different shells are also larger than those within shells (which is not the case for the cluster around 4b) and, generally, the thickness of the shells is small. These findings support the kind of cluster description introduced by Conrad et al. (2009).
In general, it should be added that a cluster choice is in the first instance reasonable if the cluster shells chosen are as spherical as possible and well separated with respect to the distances between atoms in different cluster shells and the center of the nested clusters. Another important point is the occurrence of a certain cluster type: if clusters can be found independently in different structure types, this makes a good case for their significance. This type of more general cluster was for example found in the family of cubic Al–Cu–Ta compounds in the form of an Al76 fullerene-like cluster shell (Conrad et al., 2009).
3.3. Higher-order superstructures – cF1124, cF5928 and cF23256
The three largest intermetallic structures known in cF1124-Cu56.9Cd43.1, cF5928-Al56.6Cu3.9Ta39.5 and cF23256-Al55.4Cu5.4Ta39.1, with lattice parameters of a around 25, 45 and 71 Å (Samson, 1967; Weber et al., 2009). Projections of the unit cells as well as of their average structures are shown in Fig. 8; for completeness, the structure of cF444-Al63.6Ta36.4 is also shown. In the description the structures are classified as (3×3×3)-, (7×7×7)- and (11×11×11)-fold superstructures of cF16-NaTl in the case of the Al-(Cu)-Ta compounds and as a (4×4×4)-fold one of an analogous cP16-type in the case of cF1124-Cu56.9Cd43.1.
are3.3.1. Al–Cu–Ta structures
The close relationship between the three structures of the Al–Cu–Ta system is apparent: they are all superstructures of a double-diamond type basic structure with unit-cell parameters of the related cubic Laves phase. From a purely mathematical point of view, (p×p ×p)-fold superstructures of a basic structure with the same symmetry can exist for all prime numbers . The observed structures in the Al–Cu–Ta system, however, exhibit only three-, seven- and 11-fold supercells, e.g. fivefold supercells have not been found so far. This can be explained as follows.
The dominant feature in this group of structures is the endohedral cluster with the F4076 third cluster shell. It is closely packed in the smallest structure (p = 3), whereas tetrahedrally assembled building blocks of four and ten such clusters are found in the medium and large structures with p = 7 and p = 11. These building blocks correspond to tetrahedra with edge lengths of two and three clusters. Therefore, it seems obvious that the three phases found are the only representatives of this family of structures and no intermediate superstructures can exist, although p = 5 would be equivalent from a group-theoretical perspective. On the other hand, superstructures with even bigger unit cells could be possible, at least geometrically.
3.3.2. cF1124-Cu56.9Cd43.1
The structure of cF1124-Cu56.9Cd43.1 has been reinvestigated several times after its first publication by Samson (1967). The structure was originally determined based on a `packing map' of the structure – a cut through the structure along the (110) plane. It was described by two interpenetrating three-dimensional frameworks, composed of Friauf polyhedra and icosahedra, respectively, arranged in a diamond-like network (Samson, 1967). The Friauf network consists of tt sharing their hexagonal faces; the icosahedral network fits into its cavities and shares vertices with tt.
An alternative description interprets the structure in terms of octahedra and tetrahedra in addition to Friauf polyhedra (Andersson, 1980). That author also pointed out that complex phases like those discussed here are built up from structural features which are also found in simpler metallic structures. He also discusses that in the case of the Cu–Cd system the complex structure is packed more efficiently than the corresponding elementary metals and exhibits smaller interatomic distances. Both this description and the original one by Samson were analyzed later in conjunction with other complex structures explained as polyhedral frameworks by Hellner & Pearson (1987).
Kreiner & Schäpers (1997) pointed to the relationship between cF1124-Cu56.9Cd43.1 and the metastable icosahedral structure found in the Cd–Cu system with similar composition. The description as a hybrid structure by Samson (1967) is maintained, whereas the icosahedral network is explained in detail by means of the so-called I3-cluster concept. They identified the periodic structure to be an approximant structure of the i.e. to consist of the same type of clusters.
We employed the cluster approach to cF1124-Cu56.9Cd43.1 similar to the structures discussed above (see Fig. 9). The cluster shells found around the points of highest symmetry () are less regular when their centers are formed by more than one atom. The positions 4a 0,0,0 and 4d are surrounded by octahedra, which are not considered to be full cluster shells but rather a somewhat large cluster center; in this case not even the first cluster shell exhibits any considerable regularity. Around 4b , where a small tetrahedron is centered that cannot be regarded as an independent cluster shell either, a quite low cluster symmetry is also observed: already the first shell is a rather irregular 22-atom polyhedron with tetrahedral symmetry and only triangular faces. The second shell is a F2240 fullerene-like polyhedron with only partially capped p and h faces. The cluster shells around 4c , occupied by a Cd atom, are the most regular ones: first – a Friauf polyhedron FK2816; second – a F1628 fullerene-like cluster with all 12 p faces capped by one atom each and the four h faces by three atoms each, thus producing a 52-atom cluster shell; third – a 70-atom polyhedron consisting of 12 triangles, 36 pentagons and four hexagons, capped yielding a 110-atom polyhedron FK266110. The 70-atom polyhedra around 4c and F2240 around 4b share hexagonal faces and build an infinite three-dimensional network. This packing and the cluster shells involved are shown in Fig. 9. The rest of the structure is explained by the icosahedral network as discussed in the previous work on this compound (Samson, 1967; Kreiner & Schäpers, 1997).
3.4. (110) layers
As already mentioned above, the (110) layers play a major role in structures with symmetry . They contain atomic positions belonging to all special Wyckoff sites and therefore are representative of the structure as a whole. The (110) layers of the five structure variants with space-group symmetry and are shown in Fig. 10.
If the framework of symmetry elements in f) and puckered layers (p), stacked f, p, −p′, f′, p′, −p, f.8
is considered, it is obvious that the atomic arrangement on the (110) plane is not only repeated with translations [110] or but also and . These layers coincide with mirror planes and therefore are flat. Halfway between two mirror planes, a glide plane is located. On both sides of it, puckered atomic layers can be found in the investigated structures. As a result, the whole can be described by flat (Thus, between two symmetrically related flat layers two puckered ones are found for the (3×3×3)-fold superstructures. In the case of higher-order superstructures with p = 7 and p = 11, six and ten layers are sandwiched between two flat ones. This corresponds to three and five symmetrically independent puckered layers on one side of the glide plane. This means that two, four and six symmetrically independent layers are needed to describe the (p = 3, 7, 11) structures along a [110] direction; one of these is always a flat layer. The layer-stacking period thus corresponds directly to the order of the superstructure.
4. Structures with space-group symmetry Fdm
Among the nine intermetallic compounds on our list with cF(1192-23)-Al53.6Mg46.4 and the closely related structure cF(1192-40)-Cd66.7Na33.3, also found by Samson (1962, 1965). The remaining seven compounds are (3×3×3)-fold superstructures of what seems to be a similar basic structure to the previously discussed compounds in , which is a of index 2 of .
symmetry , two have significantly larger unit cells than the others: the famous Samson phase4.1. (3 × 3 × 3)-fold superstructures – cF464
The six p3-fold superstructures (p = 3) in are listed in Table 1; their lattice parameters ( Å) are in the same range as those of the lower-symmetric compounds. The atomic sites featured in those structures are strikingly similar (Table 3). Only cF472-Zn61.0Ca35.6Ni3.4 shows minor deviations: Ni atoms are located at the 16d rather than 8a. The and average structure of one representative of this structure type is shown in Fig. 11.
|
| Figure 11 along the |
The Wyckoff positions in
obviously have double multiplicity with respect to the owing to the symmetrically equivalent positions created by the inversion center added at . To compare structures in both symmetries, origin choice 1 has been used in the case of , as it directly corresponds to the setting of .Looking for a cluster structure similar to that introduced for cF444-Al63.6Ta36.4 (Conrad et al., 2009), one finds a quite regular three-shell cluster centered at 8a (see Fig. 12). Its innermost shell is a Friauf polyhedron, followed by a capped fullerene-like polyhedron F1628, a truncated triakistetrahedron which is the dual of a Friauf polyhedron.
The third cluster shell, a fullerene of type F4484, is again the dual of the capped F1628 polyhedron. These outer cluster shells already interpenetrate each other, while the second shells share all their hexagonal faces (see Fig. 12), which results in a tetrahedral coordination of every F1628 with four polyhedra of the same type. This network is completed with a second type of cluster, centered at the generally empty sites of 16d , with an icosahedron as the first shell and a pentagonal dodecahedron around it, as shown in Fig. 12. Four of these dodecahedra meet at 8b and, together with the F1628 polyhedra, completely fill space.
The sites of this structure type with e.g. around 4c, sites 16e2 and 48h1–48h3 constitute the FK7640 cluster and only 48h3 has to be omitted to obtain a distorted version of F1628.
can largely be related directly to sites of the corresponding structures in . Therefore, their cluster descriptions should be similar. The corresponding inner cluster shells are easily recognizable: only the Friauf polyhedra have to be taken into account, not the alternative rhombic dodecahedra in subtypes I–IV. The second shell can be directly related by atomic sites:The sites forming the different clusters as well as their correspondence to the sites in supplementary material.
are given in Tables 22 and 23 of the4.2. (4 × 4 × 4)-fold superstructures – cF1192
The first structure of this cF(1192-40)-Cd66.7Na33.3 (Samson, 1962). It was found to be built up of Friauf polyhedra, arranged in five-rings, as usually described by their tt skeleton. Six of these five-rings are again arranged centered at the vertices of a tetrahedrally distorted octahedron and produce four more Friauf polyhedra at the vertices of a tetrahedron around their common center. The whole structure is made up by this arrangement, complemented by even more Friauf polyhedra between them as well as 32 additional atoms. For the structure solution of this highly complex structure, so-called packing maps were employed (Samson, 1964). Later, similar coordinates resulting in an improved structure model could be calculated from coincidence site lattice theory (Yang et al., 1987). The purely geometrical understanding of the structure was recently complemented by quantum-mechanical calculations (Lee et al., 2007; Fredrickson et al., 2007), indicating that the structure can be divided into electron-rich and -poor substructures.
size to be reported wasThe more famous `Samson phase' cF(1192-23)-Al53.6Mg46.4 (Samson, 1965) can be regarded as isostructural with cF(1192-40)-Cd66.7Na33.3 and is also nearly exclusively built from Friauf polyhedra, although it exhibits a considerable degree of disorder. Samson attributed this to the formation of a large number of icosahedra in the structure, which finally outnumber the Friauf polyhedra by far. An extensive re-investigation and further analysis of Al53.6Mg46.4 with respect to structure and related properties was recently carried out and confirmed the previous structure model in detail (Feuerbacher et al., 2007). A description of the structure by layers was done by Wolny et al. (2008), where also the interplay between these layers and previously described clusters is discussed (Sikora et al., 2008).
The two isostructural compounds can be described in a similar way to the smaller structures by the cluster approach (see Fig. 13). Projections of the unit cells, as well as of their average structures are shown in the overview in Fig. 11. The clusters centered at 8a 0,0,0 (around a small tetrahedron that cannot be regarded as an independent cluster shell) do not exhibit a high degree of symmetry: the first shell is a rather irregular 22-atom cluster with tetrahedral symmetry and only triangular faces. The second shell is an incompletely capped fullerene-like F2240 polyhedron; this cluster is similar to that found in cF1124-Cu56.9Cd43.1 centered at site 4b (see Fig. 9).
The cluster centered around 8b (where atoms are located in both mentioned compounds), on the other hand, is fairly regular and has the following cluster shells: first – a Friauf polyhedron FK2816; second – a F1628 fullerene-like cluster with all faces capped yielding a FK8444 polyhedron; third – a F4076 cluster with all faces capped resulting in a FK228116 polyhedron (fourth – a 114-atom shell consisting of 76 triangles, 12 pentagons and 28 hexagons). The second cluster shells around 8b do not touch each other, but the third cluster shells overlap. The F4076 polyhedron and the two-shell clusters around 8a together describe all atomic positions of the discussed structures. Hereby the F4076 clusters, which are identical to those found in subtypes III and IV of the cF464 structures in , are arranged on a diamond-like lattice and overlap with their third shells. The configuration of cluster centers as well as the clusters' first two (8a) or three (8b) shells are shown in Fig. 13.
5. Structures with other space-group symmetries
Besides the 48 structures on our list with symmetries and , only eight more are known with other cubic symmetries; their projections are shown in Fig. 14.
5.1. Four structures in Fmm – (4 × 4 × 4)-fold superstructures
The structure of cF(1208-64)-Dy40.9Sn39.2Co19.9 was determined in without any in-depth discussion of its building units (Salamakha et al., 2001). It is closely related to cF1124-Tb41.6Ge39.9Fe18.5 (Pecharskii et al., 1987) as well as the corresponding structures in the Pr–Sn–Co and Gd–Ge–Fe systems. Here we discuss a possible cluster description of the structure (see Fig. 15).
Around 4a 0,0,0, occupied by a Dy atom, the following cluster shells are found: first, a disordered rhombic dodecahedron/capped cuboctahedron (in Tb41.6Ge39.9Fe18.5, only the latter is present); second, a capped rhombicuboctahedron/deltoidal icositetrahedron; third, an 80-atom polyhedron with six quadrangular and 144 triangular faces. Around 4b , occupied by a Co atom, the cluster shells are as follows: first, a cube; second, a capped rhombicuboctahedron/deltoidal icositetrahedron; third, a 48-atom polyhedron with eight triangular and 42 quadrangular faces.
The sites of 8c and are each occupied by an atom, surrounded by a 22-atom cluster shell with triangular faces, just as found in the and compounds of similar unit-cell size at positions 4b and 8a. The second shell is the same 28-atom cluster as was previously found in the cF(464-x) compounds: a tetrahedrally truncated rhombic dodecahedron, with capping atoms resulting in a FK7640 polyhedron.
The two three-shell clusters at positions 4a (cluster 1) and 4b (cluster 2) and the four-shell cluster at 8c (cluster 3) pack densely describing these two structures entirely. The first two clusters share quadrangular faces along all directions and are aligned alternately in those directions. The cubic interstices in this structure are filled with 8c polyhedra, which share one triangular face with each neighboring three-shell cluster at 4b and six triangular faces with each cluster at 4a. The clusters and their arrangement are shown in Fig. 15.
5.2. Three structures in Fmc
The structure of cF(944-22)-Zn67.1Sn20.8Mo12.1 was described in the (Hillebrecht et al., 1997). It looks somewhat unusual with respect to the number of atoms per compared with the other structures discussed here containing either or atoms per Furthermore, it has a rather ill-defined (4×4×4)-fold superstructure.
The cluster structure has already been introduced by Hillebrecht et al. (1997) and features the following nested clusters around the two highest-symmetric sites (see Fig. 16): at 8a ; a centered rhombic dodecahedron within a snub cube9 with a 60-atom third-shell cluster, consisting of 24 pentagonal, six quadrangular and 24 triangular faces (cluster 1); and around 8b 0,0,0 and a centered icosahedron within an icosidodecahedron with atoms capping all pentagonal faces within a small rhombicosidodecahedron10 (cluster 2). The symmetrically inequivalent three-shell clusters overlap and cover all sites within the If one considers a two-shell cluster on one of the sites 8a and 8b and a three-shell cluster on the other, they form a packing which describes the structure entirely. The different cluster shells as well as both packing alternatives are shown in Fig. 16.
The structures cF(968-32)-Zn57.3Ru22.2Sb20.5 and cF(992-125)-Zn76.9Ru12.0Sb11.1 were found to be nearly isostructural to cF(944-22)-Zn67.1Sn20.8Mo12.1 (Xiong et al., 2010). They exhibit minor differences, as well as a certain range of compositions in the latter case, leading to a with exchange of Sb and Zn, as described in detail by Xiong et al. (2010).
5.3. One structure in Fd – a (4 × 4 × 4)-fold superstructure
The structure of cF1392-Cd86.2Eu13.8, with symmetry , is an approximant structure to the binary icosahedral quasicrystals in the Ca–Cd and Yb–Cd systems (Gómez & Lidin, 2004). It was described by two symmetrically inequivalent triacontahedra with the following inner shells (from inside to outside): tetrahedron, dodecahedron, icosahedron and icosidodecahedron. Additionally, interstitial atoms had to be introduced.
In our cluster description (see Fig. 17), the tetrahedron forms the cluster center and the surrounding dodecahedron the first cluster shell. The next two polyhedra are joined so that the second cluster shell is an icosidodecahedron whose pentagonal faces are capped (by the Eu atoms which – according to the previous description – belong to the icosahedron). The third cluster shell then consists of the atomic sites which were previously discussed as building a triacontahedron and belonging to some interstitial cubes. All of those atoms build a fullerene-like shell F4280 with icosahedral symmetry. There are two symmetrically inequivalent versions of this three-shell cluster, which overlap with each other as well as with clusters of the symmetrically non-related type. The cluster centers are located at the positions 8a 0,0,0 and 8b , and arranged in a double-diamond lattice. The three-shell clusters around one of these centers already overlap in the outer shell. The clusters, as well as their arrangement in the are shown in Fig. 17. The three-shell cluster around 8a and the two-shell cluster around 8b together describe all the atoms present in the published structure.11
6. First-principles studies
The electronic properties of the structures were studied by ab initio calculations. With respect to computational feasibility, these were restricted to compounds with less than 500 atoms per f.c.c. thus not including the Samson phase and structures of higher complexity. Prior to calculations, the structures were transformed to their primitive rhombohedral setting using the matrix
resulting in not more than 116 atoms per
with lattice parameters and . All calculations discussed in the following are based on these primitive unit cells.Due to the already large number of atoms per supplementary material.
we could not increase the number of unit cells in our calculations to treat structural disorder properly. Consequently, our structure models had to be idealized for the calculations. For that purpose partially occupied and split positions were condensed into fully occupied, single ones and occupancies of deficient sites were rounded to full or zero occupancy. Mixed positions were assumed to be fully occupied by the majority element on the respective site. Details on the performed idealization are given in Tables 27 and 28 of theThe structures of cF(416-16)-Cu73.9Sn23.2Ni2.9 and cF(416-1)-Zn86.6Fe6.7Ni6.7 had to be calculated in the variants Cu76.8Sn23.2, Zn86.6Fe13.4 and Zn86.6Ni13.4, because the Ni sites had not been specified explicitly by the authors (Booth et al., 1977; Lidin et al., 1994). Also the structure of cF464-Ga53.4Li31.0Cu8.6In6.9 was reduced to Ga62.1Li31.0Cu8.6, and thus a ternary compound, since In atoms were only found as minority elements on shared sites (Chahine et al., 1995).
The calculations were performed with the VASP (Vienna ab initio simulation package) code (Kresse & Furthmüller, 1996a,b). The generalized gradient approximation (GGA; Perdew et al., 1996) together with the projector-augmented wave (Blöchl, 1994) method have been applied to optimize the structures and calculate the charge distribution (at 0 K). In all calculations the projector-augmented wave (PAW) potentials and a 4×4×4 Monkhorst–Pack scheme (Monkhorst & Pack, 1976) for the sampling, as provided by the code, were employed. The positions of all atoms were relaxed with the conjugate gradient method. For the cut-off of the plane wave representation of the wavefunction, the default values were used. The energy minimization procedure is iterative and proceeds until self-consistency within a prescribed tolerance of 10−4 eV per for electronic optimization and 10−3 eV per for atomic relaxation.
6.1. Electron localization function
The electron localization function (ELF; Becke & Edgecombe, 1990; Silvi & Savin, 1994) is a measure of the likelihood of finding an electron in the neighborhood space of a reference electron located at a given point and with the same spin. Physically this measures the extent of spatial localization of the reference electron and provides a method for the mapping of electron pair probability in multi-electronic systems. The ELF represents the organization of chemical bonding in It is a dimensionless localization index that expresses electron localization with respect to the uniform electron gas, whereas ELF = 1 corresponds to perfect localization and ELF = 0.5 to the electron gas. In most metals there would not be any ELF maxima between the atoms but only around their centers, reflecting the shell structure of the core electrons. The ELF was calculated with the corresponding module provided with the VASP code. For an overview, see the ELF website (https://www.cpfs.mpg.de/ELF).
Even though the underlying structural building principles are the same, the ELF maps are quite diverse. Structures with the same chemical environment locally will of course exhibit the same ELF map behavior, but the overall ELF map can change significantly simply with a change of composition, e.g. the Zn–Pt system in subtype I of the structures, depicted in Fig. 4 of the supplementary material. On the other hand, structures with almost the same electronic composition such as Mg-(Ir,Pd,Rh,Ru) exhibit almost identical ELF maps, depicted in Fig. 3 of the supplementary material.
In our case the calculated ELF maps can be roughly divided into two groups: one with significant electron localization and another without. Structures of the second category include nearly all compounds with majority elements Zn and Cu as well as cF432-Li64.3In26.5Ag9.2. Representative ELF maps of the first group of structures are shown in Fig. 18 and discussed in the following. The ELF maps of all discussed structures are given in Figs. 3, 4, and 5 of the supplementary material.
In the following the most distinct features in the different ELF maps are given:
|
6.2. Bader charge analysis
The Bader analysis (Bader, 1990; Henkelman et al., 2006) is an intuitive way of dividing molecules into atoms. The definition of an atom is based purely on the electronic charge density, with zero-flux surfaces being used to divide atoms. A zero-flux surface is a two-dimensional surface on which the charge density is a minimum perpendicular to the surface. Typically in molecular systems the charge density reaches a minimum between atoms and this is a natural place to separate atoms from each other.
The Bader analysis is used to calculate the volume that a single atom is going to occupy in the structure; additionally the charge within this volume can be integrated, leading to the effective Bader charge on the atom. This allows an estimation of how covalent/ionic/metallic the atom is going to be in the structure. Alternatively, localized charges, not positioned on atoms, can be analyzed, to further investigate the nature of bonding in the structures.
This Bader charge analysis corresponds very well with the ELF maps of the previous section, giving numbers to the visual interpretation of the maps. No general trends over all structures can be observed. However, within the subtypes and within similar electronic compositions the Bader charges are comparable.
The calculated electron-density distributions were evaluated by means of Bader charge analysis. An overview of the results is given in Table 4. Detailed results are listed in Tables 29 and 30 of the supplementary material.
|
Some particular features are found in the following compounds:
|
In summary, a few distinct characteristics can be identified in some of the investigated structures, but they are not consistent throughout one subtype. No overall commonalities can be found for these very similar compounds.
6.3. Electronic density of states
Almost all quasicrystals with icosahedral symmetry have been considered as Hume–Rothery electron compounds, and it has been shown theoretically that the existence of a pseudogap contributes to the stabilization of quasicrystals (Smith & Ashcroft, 1987). This also holds true for phases related to quasicrystals with different constituents and different atomic concentrations, because they are electron compounds with similar electron-per-atom ratios. The pseudogap formation in the across the EF can be explained in two possible ways; one is by the interaction between the quasi-Brillouin zone (q-BZ) boundary and the Fermi sphere (FS), i.e. the Hume–Rothery mechanism (HRM), and the other is by sp-d (Fujiwara & Yokokawa, 1991; Mizutani, 2011; Friedel, 1988; de Laissardière et al., 1995). A pseudogap near the reduces the total band energy. Due to the almost spherical symmetry of the q-BZs the HRM works most effectively in icosahedral quasicrystals. In aluminium transition-metal quasicrystals, the d states of a transition metal element are strongly hybridized with the s and p states of Al. This sp–d further enhances the pseudogap formed by the q-BZ-FS interaction. The deep pseudogap in the vicinity of EF is a contribution to the stabilization of icosahedral quasicrystals.
The electronic DOS) as well as its projection onto the orbitals of the atoms were calculated as implemented in the VASP package. The projection scheme is not perfect; the sum over all projections does not add up to the total of the DOS. This is due to the fact that VASP does not use localized orbital basis sets but plane waves as the basis for the electron density. Hence the projected DOS is calculated by weighting the DOS with the projected integrated partial charges, integrated over the volumes of the `atomic spheres'. As space cannot be filled by spheres completely, there will always be some discrepancy and the projected DOS just gives a qualitative picture.
(The DOS was calculated for a group of representative structures of the cF(464-x) class. The DOS graphs are shown in Fig. 19 in the relevant range around the All structures show a clear metallic behavior, i.e. with significant electron density at the The plots are obviously very diverse on first glance. On closer inspection, most calculated DOS have a pseudogap in the proximity of the EF.
The DOS of all calculated structures shows a strong tendency to form dense spiky peaks. Theoretical (Fujiwara et al., 1994; Hippert et al., 1999) and experimental (Escudero et al., 1999) studies on quasicrystals and their structure approximants have observed a similar spikiness in their DOS. These spiky features could be associated with the confinement of electrons in clusters (de Laissardière & Mayou, 1997), and lead to a spiky DOS with the involvement of many clusters. An assembly of the complete DOS plots is shown in Fig. 6 of the supplementary material.
Finally, a word of caution has to be issued when addressing the DOS calculations and their interpretation with respect to all compounds. Due to the inherent periodicity and absoluteness of the atoms in the density-functional theory calculations used here, it is very hard to calculate structures with mixed-atom positions. On the other hand, if the mixed occupancy is ordered and can be described in a it can be calculated, but of course with a largely increased amount of computing time due the non-linear scaling of density functional theory calculations. Hence all structures with disorder or mixed occupancies on certain positions have been idealized, i.e. the occupancies have been rounded to zero or to one. For structures in real space this may have minuscule differences, but it can influence the DOS at specific points. Especially when dealing with transition metal compounds, the addition or subtraction of certain atoms and their respective electrons in the d orbitals changes the DOS near the Fermi surface and can move the position of the pseudogap along the DOS.
As already mentioned, the DOS at the Fermi surface and the pseudogap may vary from the real measured structures; this is mostly a result of the varying occupancy of the d states of the transition metals. The overall features of the DOS will however remain unchanged, as can be seen for instance when comparing Ga53.4Li31.0Cu8.6In6.9 and Ga47.5Mg31.2Cu21.3 in Fig. 6 of the supplementary material, which differ in their composition only through the exchange of Mg with Li.
In the following we discuss the DOS of the structures according to their subtypes in the idealization, as listed in Tables 27 and 28 of the supplementary material. An interesting point here is that in general, the DOS of the structures are very diverse. This is astonishing as the principle building scheme of the structures is the same. Only when comparing structures which are in the same subtype and have a similar composition (at least when considering the number of electrons involved in bondings), like Zn82.7Pt17.3 and Zn89.1Ir10.9 in subtype I, are the overall characteristics of the DOS the same, but one can clearly see the effect of the different number of electrons in the d states, leading to a different DOS at the and shifting the pseudogap above the for Zn82.7Pt17.3.
6.3.1. Subtype I
In the DOS of cF420-Li81.0Pb19.0, the pseudogap at approximately −0.2 eV from EF is very pronounced, while just above it an energetically unfavorable maximum arises at the Taking a partial occupancy of the Pb sites into account (Goward et al., 2001), the could be lowered into this pseudogap. Thus, via vacancies and disordered sites, the structure may tune the DOS to the most favorable configuration. The DOS of two more representatives of subtype I, cF(416-16)-Zn82.7Pt17.3 and cF(416-4)-Cu78.6Sn21.4, exhibit clear pseudogaps at approximately +0.2 eV. The heavily disordered compound cF(452-36)-Zn89.1Ir10.9 again features a very narrow but deep pseudogap at ca −0.2 eV.
6.3.2. Subtype II
The two isostructural subtype II compounds cF408-Na86.3Tl13.7 and cF408-Sc86.3Os13.7 exhibit very spiky DOS with a couple of minima which could be interpreted as pseudogaps. cF408-Mg86.3Rh13.7 and cF408-Zn78.4Fe21.6 show distinct pseudogaps at around −0.2 eV. The DOS of cF(412-28)-Al65.3Cu18.1Cr16.6 has a very narrow and deep gap located directly at the In the DOS of cF480-Zn67.5Ce16.7Mg15.8 the significant contribution of the Ce-f-states has its onset at around −0.2 eV. A broad and low minimum can be observed approximately at the Fermi level,
6.3.3. Subtypes III and IV
The DOS of cF444-Al63.6Ta36.4 has already been shown by Conrad et al. (2009) and another representative of subtype III, cF(448-4)-Mg83.6Gd16.4, also does not exhibit any clear features around EF. In the very spiky DOS of cF448-Cd80.4Sm19.6, a broad pseudogap can be found at around −0.3 eV and a rather narrow one at approximately +0.1 eV. The only structure belonging to subtype IV, cF456-Na49.1Sn26.3In24.6, is again quite spiky and has a very narrow pseudogap at EF; the broad minimum at −0.6 eV could be interpreted to be a pseudogap as well.
6.3.4. Fdm
cF464-In70.7K29.3, the only binary compound in the group of cF464 structures crystallizing in , exhibits an actual gap in the DOS at +0.4 eV. The DOS of cF444-Ga50.0Na29.3In20.7 exhibits a striking pseudogap at −1.0 eV, while two less deep ones are found at −0.6 and −0.1 eV. The DOS of cF(464-4)-Ga48.9Na30.4Cd20.7 shows a pseudogap directly at EF. The DOS of cF464-Ga53.4Li31.0Cu8.6In6.9 shows a significant rise of the overall level at the just below, at −0.1 eV, a pseudogap can be found. No hint towards any pseudogaps, however, can be found in the DOS plot of cF(464-13)-Ga47.5Mg31.2Cu21.3.
7. Conclusions
The most striking result of our analysis of f.c.c. complex intermetallics with giant unit cells is that all of them follow the same building principles regardless of significant differences in chemical composition and bonding. The structures discussed here are mainly binary (29) and ternary (26), with one quaternary compound also included. The unit-cell dimensions seem to be determined by the type of layer structure under the constraint of cluster formation, as well as the size of the fundamental clusters and their packing principle.
The packing appears to be stabilized by an energetically favorable stoichiometry, which is specific for a certain system; many of the binary compounds, for example, have compositions of around A85B15. The respective composition then makes the formation of a simpler structure in the phase diagram impossible, but instead allows for a simple packing of bigger structural units – the clusters – which are more flexible with regard to composition.
Another interesting result is that all these structures can be seen as p3-fold superstructures with p = 3, 4, 7 or 11 depending on their lattice parameters. The underlying basic structure of the cF16-NaTl-type is indicated by the set of most intense Bragg peaks in their diffraction patterns. This means that the slightly puckered atomic layers of the average structure are not only strongly scattering X-rays but also electrons, which can lead to pseudogaps in the DOS. Indeed, almost all structures in all subtypes display pseudogaps in the vicinity of the and a very spiky DOS.
It is also remarkable that the structures can also be interpreted as topological layer structures. The number of one flat and p-1 puckered (110) layers per period equals p, the period in the description. The three-dimensional framework of interpenetrating layer stackings along all six symmetrically equivalent [110]-directions determines the kind of clusters and their packing that is compatible with it. The cluster structure found builds by decoration and puckering of the layers, whereas the cluster centers again mostly arrange on atomic positions corresponding to a cF16-NaTl-unit cell.
To summarize, intermetallic compounds are prone to form giant unit cells if their odd stoichiometry favors the formation of clusters that pack in a way allowing the formation of a three-dimensional framework of atomic layers. The existence of an underlying basic structure is a consequence of these structural building principles.
Supporting information
Extra tables and figures. DOI: https://doi.org/10.1107/S0108768111025390/sn5103sup1.pdf
Footnotes
1All elements were considered as possible components of intermetallic compounds except the following: H, He, B, C, N, O, F, Ne, Si, P, S, Cl, Ar, As, Se, Br, Kr, Te, I, Xe, At and Rn.
2Remarkably, no structures of intermetallics were found with space groups F23, F432, F4132, or .
3Supplementary data for this paper are available from the IUCr electronic archives (Reference: SN5103). Services for accessing these data are described at the back of the journal.
4These are cP2-CsCl, cF16-NaTl, cP52-Al4Cu9, cF444-Al63.6Ta36.3, cF1192-Al53.6Mg46.4, cF5928-Al56.6Ta39.5Cu3.9 and cF23256-Al55.4Ta39.1Cu5.4.
5Within the scope of this work only the face-centered space groups are listed. These considerations also hold true for P213 and , and with minor restrictions for P4332 and P4132.
6It can also be seen as the structure of cF24-MgCu2 with the additionally occupied 8b .
7A dual polyhedron corresponds to the original one by replacing faces by vertices and vice versa. The dual of a dual is the original polyhedron.
8Here p and −p lie on opposing sides of a mirror plane and p′ is generated from p after a glide operation.
9A snub cube is an Archimedean solid with 32 triangular and six square faces, and 24 vertices.
10This polyhedron is often simply called rhombicosidodecahedron (r), but is referred to as `small r'. Also termed `truncated r' in order to distinguish it from the `great r' (Cundy & Rollett, 1961).
11The Wyckoff positions in correspond directly to those in , with the exception of two of the highest multiplicities (, ).
12This feature was also observed in Zn95.3Mo4.7 at the same position, but below the threshold for significant ELF values of 0.5.
13These ELF maxima connect pairs of Sc atoms with interatomic distances of 4.0–4.6 Å. The shortest Sc—Sc distances in this structure, however, range from 3.0 to 3.9 Å.
14The bond basins found by Bader analysis do not, however, cover all maxima assigned to parts from the ELF.
Acknowledgements
We would like to gratefully acknowledge the extensive and very helpful comments given by the referees during the review process.
References
Alvarez, S. (2005). Dalton Trans. 13, 2209–2233. Web of Science CrossRef PubMed Google Scholar
Alvarez, S. (2006). Dalton Trans. 17, 2045–2051. Web of Science CrossRef PubMed Google Scholar
Andersson, S. (1980). Acta Cryst. B36, 2513–2516. CrossRef CAS IUCr Journals Web of Science Google Scholar
Arnberg, L., Jonsson, A. & Westman, S. (1976). Acta Chem. Scand. A, 30, 187–192. CrossRef Web of Science Google Scholar
Bader, R. F. W. (1990). Atoms in Molecules – A Quantum Theory. Oxford University Press. Google Scholar
Becke, A. D. & Edgecombe, K. E. (1990). J. Chem. Phys. 92, 5397–5403. CrossRef CAS Web of Science Google Scholar
Belsky, A., Hellenbrandt, M., Karen, V. L. & Luksch, P. (2002). Acta Cryst. B58, 364–369. Web of Science CrossRef CAS IUCr Journals Google Scholar
Berger, R. F., Lee, S., Johnson, J., Nebgen, B., Sha, F. & Xu, J. (2008). Chem. Eur. J. 14, 3908–3930. Web of Science CrossRef PubMed CAS Google Scholar
Blase, W., Cordier, G. & Vogt, T. (1991). Z. Anorg. Allg. Chem. 606, 79–90. CrossRef CAS Web of Science Google Scholar
Blöchl, P. E. (1994). Phys. Rev. B, 50, 17953–17979. CrossRef Web of Science Google Scholar
Bonhomme, F. & Yvon, K. (1995). J. Alloys Compd. 227, L1–L3. CrossRef CAS Web of Science Google Scholar
Booth, M. H., Brandon, J. K., Brizard, R. Y., Chieh, C. & Pearson, W. B. (1977). Acta Cryst. B33, 30–36. CrossRef CAS IUCr Journals Web of Science Google Scholar
Brunner, G. O. & Schwarzenbach, D. (1971). Z. Kristallogr. 133, 127–133. CrossRef CAS Web of Science Google Scholar
Chabot, B., Cenzual, K. & Parthé, E. (1980). Acta Cryst. B36, 2202–2205. CrossRef CAS IUCr Journals Web of Science Google Scholar
Chahine, A., Tillard-Charbonnel, M. & Belin, C. (1995). Z. Kristallogr. 210, 80. CrossRef Web of Science Google Scholar
Conrad, M., Harbrecht, B., Weber, T., Jung, D. Y. & Steurer, W. (2009). Acta Cryst. B65, 318–325. Web of Science CrossRef CAS IUCr Journals Google Scholar
Cordier, G. & Müller, V. (1993a). Z. Kristallogr. 205, 353–354. CrossRef CAS Web of Science Google Scholar
Cordier, G. & Müller, V. (1993b). Z. Kristallogr. 205, 133–134. CrossRef CAS Web of Science Google Scholar
Cundy, H. M. & Rollett, A. P. (1961). Mathematical Models. Oxford University Press. Google Scholar
Escudero, R., Lasjaunias, J., Calvayrac, Y. & Boudard, M. (1999). J. Phys. Condens. Matter, 11, 383–404. Web of Science CrossRef CAS Google Scholar
Feuerbacher, M. et al. (2007). Z. Kristallogr. 222, 259–288. CAS Google Scholar
Fornasini, M. L., Chabot, B. & Parthé, E. (1978). Acta Cryst. B34, 2093–2099. CrossRef CAS IUCr Journals Web of Science Google Scholar
Fornasini, M. L., Manfrinetti, P. & Gschneidner, K. A. (1986). Acta Cryst. C42, 138–141. CrossRef CAS Web of Science IUCr Journals Google Scholar
Fredrickson, D. C., Lee, S. & Hoffmann, R. (2007). Angew. Chem. Int. Ed. 46, 1958–1976. Web of Science CrossRef CAS Google Scholar
Friedel, J. (1988). Helv. Phys. Acta, 61, 538–556. CAS Google Scholar
Fujiwara, T., de Laissardière, G. & Yamamoto, S. (1994). Mater. Sci. Eng. A, 179, 118–121. CrossRef Google Scholar
Fujiwara, T. & Yokokawa, T. (1991). Phys. Rev. Lett. 66, 333–336. CrossRef PubMed CAS Web of Science Google Scholar
Gómez, C. P. & Lidin, S. (2004). Chem. Eur. J. 10, 3279–3285. PubMed Google Scholar
Goward, G. R., Taylor, N. J., Souza, D. C. S. & Nazar, L. F. (2001). J. Alloys Compd. 329, 82–91. Web of Science CrossRef CAS Google Scholar
Gribanov, A. V., Seropegin, Y. D., Bodak, O. I., Pavlyuk, V. V., Akselrud, L. G., Nikiforov, V. N. & Velikhovski, A. A. (1993). J. Alloys Compd. 202, 133–136. CrossRef CAS Google Scholar
He, W., Zhang, J., Yan, J., Fu, Y. & Zeng, L. (2010). J. Alloys Compd. 491, 49–52. Web of Science CrossRef CAS Google Scholar
He, W., Zhang, J. & Zeng, L. (2007). Powder Diffr. 22, 312–315. Web of Science CrossRef CAS Google Scholar
Hellner, E. & Pearson, W. B. (1987). Z. Kristallogr. 179, 175–186. CrossRef CAS Web of Science Google Scholar
Henkelman, G., Arnaldsson, A. & Jónsson, H. (2006). Comput. Mater. Sci. 36, 354–360. Web of Science CrossRef Google Scholar
Henley, C. F., de Boissieu, M. & Steurer, W. (2006). Philos. Mag. 86, 1131–1151. Web of Science CrossRef CAS Google Scholar
Hillebrecht, H., Kuntze, V. & Gebhardt, K. (1997). Z. Kristallogr. 212, 840–847. Web of Science CrossRef CAS Google Scholar
Hippert, F., Simonet, V., de Laissardière, G., Audier, M. & Calvayrac, Y. (1999). J. Phys. Condens. Matter, 11, 10419–10450. Web of Science CrossRef CAS Google Scholar
Hornfeck, W., Thimmaiah, S., Lee, S. & Harbrecht, B. (2004). Chem. Eur. J. 10, 4616–4626. Web of Science CrossRef PubMed CAS Google Scholar
Johansson, A. & Westman, S. (1970). Acta Chem. Scand. 24, 3471–3479. CrossRef CAS Web of Science Google Scholar
Koster, A. S. & Schoone, J. C. (1981). Acta Cryst. B37, 1905–1907. CrossRef CAS Web of Science IUCr Journals Google Scholar
Kreiner, G. & Schäpers, M. (1997). J. Alloys Compd. 259, 83–114. CrossRef CAS Web of Science Google Scholar
Kresse, G. & Furthmüller, J. (1996a). Comput. Mater. Sci. 6, 15–50. CrossRef CAS Web of Science Google Scholar
Kresse, G. & Furthmüller, J. (1996b). Phys. Rev. B, 54, 11169–11186. CrossRef CAS Web of Science Google Scholar
Laissardière, G. de & Mayou, D. (1997). Phys. Rev. B, 55, 2890–2893. Google Scholar
Laissardière, G. T. de, Manh, D. N., Maagaud, L., Julien, J. P., Cyrot-Lackmann, F. & Mayou, D. (1995). Phys. Rev. B, 52, 7920–7933. Google Scholar
Lee, S., Hoffmann, R. & Fredrickson, D. C. (2007). Angew. Chem. 119, 2004–2023. Google Scholar
Lidin, S., Jacob, M. & Larsson, A.-K. (1994). Acta Cryst. C50, 340–342. CrossRef CAS Web of Science IUCr Journals Google Scholar
Lin, Q. & Corbett, J. D. (2005). Inorg. Chem. 44, 512–518. Web of Science CrossRef PubMed CAS Google Scholar
Mahne, S. & Harbrecht, B. (1994). J. Alloys Compd. 203, 271–279. CrossRef CAS Web of Science Google Scholar
Mizutani, U. (2011). Hume–Rothery Rules for Structurally Complex Alloy Phases. Boca Raton: CRC Press. Google Scholar
Monkhorst, H. J. & Pack, J. D. (1976). Phys. Rev. B, 13, 5188–5192. CrossRef Web of Science Google Scholar
Nasch, T. & Jeitschko, W. (1999). J. Solid State Chem. 143, 95–103. Web of Science CrossRef CAS Google Scholar
Pavlyuk, V., Solokha, P., Zelinska, O., Paul-Boncour, V. & Nowik-Zając, A. (2008). Acta Cryst. C64, i50–i52. Web of Science CrossRef IUCr Journals Google Scholar
Pavlyuk, V. V., Dmytriv, G. S., Tarasiuk, I. I., Pauly, H. & Ehrenberg, H. (2007). Intermetallics, 15, 1409–1415. CrossRef CAS Google Scholar
Pecharskii, V. K., Bodak, O. I., Bel'skii, V. K., Starodub, P. K., Mokra, I. R. & Gladyshevskii, E. I. (1987). Sov. Phys. Crystallogr. 32, 194–196. Google Scholar
Perdew, J. P., Burke, K. & Ernzerhof, M. (1996). Phys. Rev. Lett. 77, 3865–3868. CrossRef PubMed CAS Web of Science Google Scholar
Salamakha, P., Sologub, O., Bocelli, G., Otani, S. & Takabatake, T. (2001). J. Alloys Compd. 314, 177–180. Web of Science CrossRef CAS Google Scholar
Samson, S. (1962). Nature, 195, 259–262. CrossRef CAS Google Scholar
Samson, S. (1964). Acta Cryst. 17, 491–495. CrossRef CAS IUCr Journals Web of Science Google Scholar
Samson, S. (1965). Acta Cryst. 19, 401–413. CrossRef CAS Web of Science IUCr Journals Google Scholar
Samson, S. (1967). Acta Cryst. 23, 586–600. CrossRef CAS IUCr Journals Web of Science Google Scholar
Samson, S. (1972). Acta Cryst. B28, 936–945. CrossRef CAS IUCr Journals Google Scholar
Samson, S. & Hansen, D. A. (1972). Acta Cryst. B28, 930–935. CrossRef CAS IUCr Journals Google Scholar
Sikora, W., Malinowski, J., Kuna, A. & Pytlik, L. (2008). J. Phys. Condens. Matter, 104, 012023. Google Scholar
Silvi, B. & Savin, A. (1994). Nature, 371, 683–686. CrossRef CAS Web of Science Google Scholar
Smetana, V., Babizhetskyy, V., Vajenine, G. & Simon, A. (2006). Z. Anorg. Allg. Chem. p. 2115. CrossRef Google Scholar
Smith, A. P. & Ashcroft, N. W. (1987). Phys. Rev. Lett. 59, 1365–1368. CrossRef PubMed CAS Web of Science Google Scholar
Steurer, W. (2006). Philos. Mag. 86, 1105–1113. Web of Science CrossRef CAS Google Scholar
Stojanovic, M. & Latturner, S. E. (2007). J. Solid State Chem. 180, 907–914. Web of Science CrossRef CAS Google Scholar
Sugiyama, K., Saito, H. & Hiraga, K. (2002). J. Alloys Compd. 342, 148–152. Web of Science CrossRef CAS Google Scholar
Thimmaiah, S. & Miller, G. J. (2010). Chem. Eur. J. 16, 5461–5471. CrossRef CAS PubMed Google Scholar
Thimmaiah, S., Richter, K. W., Lee, S. & Harbrecht, B. (2003). Solid State Sci. 5, 1309–1317. Web of Science CrossRef CAS Google Scholar
Tillard-Charbonnel, M. & Belin, C. (1992). Mater. Res. Bull. 27, 1277–1286. CAS Google Scholar
Tillard-Charbonnel, M., Chahine, A. & Belin, C. (1993). Z. Kristallogr. 208, 372–373. CAS Google Scholar
Tursina, A. I., Nesterenko, S. N., Noël, H. & Seropegin, Y. D. (2005). Acta Cryst. E61, i99–i101. Web of Science CrossRef IUCr Journals Google Scholar
Villars, P. & Cenzual, K. (2009/10). Pearson's Crystal Data. Ohio: ASM International. Google Scholar
Weber, T., Dshemuchadse, J., Kobas, M., Conrad, M., Harbrecht, B. & Steurer, W. (2009). Acta Cryst. B65, 308–317. Web of Science CrossRef CAS IUCr Journals Google Scholar
Westin, L. & Edshammar, L.-E. (1971). Acta Chem. Scand. 25, 1480–1481. CrossRef CAS Web of Science Google Scholar
Westin, L. & Edshammar, L.-E. (1972). Acta Chem. Scand. 26, 3619–3626. CrossRef CAS Web of Science Google Scholar
Westin, L. & Edshammar, L.-E. (1973). Chem. Scr. 3, 15–22. CAS Google Scholar
Wolny, J., Kozakowski, B., Duda, M. & Kusz, J. (2008). Philos. Mag. Lett. 88, 501–507. Web of Science CrossRef CAS Google Scholar
Xiong, D.-B., Zhao, Y., Schnelle, W., Okamoto, N. L. & Inui, H. (2010). Inorg. Chem., 49, 10788–10797. Web of Science CrossRef CAS PubMed Google Scholar
Yang, Q.-B., Andersson, S. & Stenberg, L. (1987). Acta Cryst. B43, 14–16. CrossRef CAS Web of Science IUCr Journals Google Scholar
© International Union of Crystallography. Prior permission is not required to reproduce short quotations, tables and figures from this article, provided the original authors and source are cited. For more information, click here.