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Article

Crystal Structure Complexity and Approximate Limits of Possible Crystal Structures Based on Symmetry-Normalized Volumes

1
Department of Geoscience, University of Nevada, Las Vegas, NV 89154, USA
2
Institute of Geological Sciences, University of Bern, 3012 Bern, Switzerland
*
Author to whom correspondence should be addressed.
Materials 2024, 17(11), 2618; https://doi.org/10.3390/ma17112618
Submission received: 6 May 2024 / Revised: 22 May 2024 / Accepted: 25 May 2024 / Published: 29 May 2024
(This article belongs to the Special Issue Development and Application of Advanced Inorganic Composites)

Abstract

:
Rules that control the arrangement of chemical species within crystalline arrays of different symmetry and structural complexity are of fundamental importance in geoscience, material science, physics, and chemistry. Here, the volume of crystal phases is normalized by their ionic volume and an algebraic index that is based on their space-group and crystal site symmetries. In correlation with the number of chemical formula units Z, the normalized volumes exhibit upper and lower limits of possible structures. A bottleneck of narrowing limits occurs for Z around 80 to 100, but the field of allowed crystalline configurations widens above 100 due to a change in the slope of the lower limit. For small Z, the highest count of structures is closer to the upper limit, but at large Z, most materials assume structures close to the lower limit. In particular, for large Z, the normalized volume provides rather narrow constraints for the prediction of novel crystalline phases. In addition, an index of higher and lower complexity of crystalline phases is derived from the normalized volume and tested against key criteria.

1. Introduction

The relation between crystal structure and composition of chemical species is at the heart of the science of condensed matter, whether it is the chemistry or physics of solids, the mineralogy and petrology of rocks, or material engineering. The problem may be cast in the principal question of whether there is a general relation that correlates symmetry, volume, and composition of all chemically possible compounds and their solid solutions. More specifically, it is asked for actual limits for possible crystal structures and the existence of forbidden zones in the correlation of symmetry, density, and composition. The existence of such limits is evident from the existence of the gaseous and the liquid state, but it is worth exploring if, within a range of plausible densities, narrower constraints are obtainable. This question receives additional interest through the search for new large, porous, multi-component structures, which are essential in the chemical industry as catalysts or catalyst matrices [1,2], detergents [3], filter materials [3,4], battery membrane materials [5], to mention just a number of applications.
More recently, powerful algorithms have been developed that provide crystal structures for a given chemical compound in a given unit cell shape [6] and, thus, address part of the question that we ask here, although under the constraint of fully occupied lattice sites, given cell shape, and for pure compounds only. Computational assessment of structures with very large unit cells, such as those of nano- and mesoporous materials, is computationally costly.
Within the range of crystalline materials, minerals pose additional problems but also serve as a repository for material synthesis: There is barely a material of industrial importance that does not occur in nature or has natural analogs. As they occur in nature, minerals are commonly multi-component phases that have formed within multiphase systems [7,8]. Commonly, minerals carry minor and trace element concentrations. While applied solid-state science has focused on synthesis with limited sets of chemical ingredients for a long time, the wealth of multivariant solid solutions in natural systems provides a vast repository of materials that guide material science where properties are controlled by dopants.
The distribution of crystalline phases among the seven crystal systems has been assessed with statistical measures [9,10,11,12]. Hummer [12] observed that within uncertainty, the distribution of mineral species among the 32 point groups obeys a power law. The assessment of structural complexity has been based on the distribution of atoms on distinct sites [13], computational weight [14], or, quite successfully, based on network topologies and probability [15,16]. The problems of the statistics of symmetry distribution and of the complexity of structures are related but not equivalent: A statistics of symmetry that is based on the seven crystal systems neglect essential features of crystal complexity. For instance, phases of structures as simple as gold and as complex as the zeolite paulingite are thus ranked as equally highly symmetric because both are cubic. Statistics of the symmetries of crystalline phases that is based on point groups [12] is more distinctive, but it still places phases like sphalerite, ZnS, and zunyite, Al13Si5O20(OH,F)18Cl, into one category because they assume the same point group, although their structural complexity is vastly different in terms of the sizes of their asymmetric units.
The distribution of crystalline species across space groups and compositional ranges and the size of their asymmetric units implicitly carry information about symmetry-based constraints on possible structures, but none of the measures of symmetry and complexity that are mentioned above make these constraints explicit. The network topology of structures [15,16] provides quantitative rankings of structural complexity, but by principle, it does not carry information about the energetic constraints on possible structures, which are, foremost, controlled by their density at given conditions of pressure and temperature. Consequently, this approach does not provide predictions on possible structures and volumes for a given chemical composition, which is the question that we ask in this paper.
Here, it is shown that a combination of unit cell volume, ionic volume, and an algebraic index of crystal complexity provide tentative upper and lower limits of possible crystalline phases as a function of Z, the number of chemical formula units. In addition, an index of the complexity of crystal structures can be derived from this correlation that does not reduce actual crystal structures but is based on Wyckoff multiplicities, Z, and ionic volume

2. Materials and Methods

First, a general reference volume of chemical species that disregards sterical or symmetrical constraints and possible asymmetry of bond polyhedra is defined by the total crystal ionic volume ([17], hereafter: ‘ionic volume’). The crystal radii represent the radial part of the electron wavefunctions of bonded atoms [18] and are based on a vast set of empirical data for each ion [19]. Thus, the cubes of the crystal radii are the primary space-filling entity for any given structure, while the angular part of the wavefunctions and geometric constraints cause deviations from closed packings. Thus, the reference ionic volume abstracts from the geometric constraints and the directional dependence of valence electron distributions, and it is defined here for a compound AiBjCk… where i, j, k, … gives the stoichiometry of the chemical species A, B, C, … as
V i o n = 4 π / 3 ( i · r A 3 + j · r B 3 + k · r C 3 + )
and the radii rA,B,C,… are the crystal radii for given valence and coordination and spin state [19]. Although this reference ionic volume neglects directional contributions to bonds and any sterical and geometrical constraints that avail for crystalline phases, it correlates with the unit cell volume Vuc and the number of chemical formula units Z as
V u c = 1.87 7 · Z · V i o n
with an adjusted R2 of 0.989 for all minerals and phases that are listed in Table 1. The correlation is shown in Figure 1.
In this comparison, minerals and phases with unit cell volumes between 70 and 9 × 104 Å3 and Z between 1 and 192 were selected, including sulfides, arsenides, oxides, silicates, borates, phosphates, and arsenates (Table 1). It is noteworthy that the correlation is quite good considering the wide variety of composition, structure, and size of the asymmetric units of the minerals and phases examined here (Table 1). On the other hand, the mean deviation of ~39% is significant. This large mean deviation is intrinsic to the large variation in structures and composition of the materials that are compared here, whose specific structural differences find an indirect expression in the discrepancies between ionic and actual volume. The concept of correspondence of states in the sense of the van der Waals equation finds its limitation for solids here. This fact, but in combination with the observation of an overall strong correlation between ionic and unit cell volumes, is used here as a basis for a more general assessment of structural complexity.
In the second step, an algebraic index of the intrinsic symmetry of the phases has to be defined. The criteria for a useful index are chosen as follows:
(1)
The index should correlate with the complexity of structures within structure families, e.g., the coupled substitution that derives bixbyite- and pyrochlore-type phases from fluorite-type oxides or tetrahedrite-type phases from the sphalerite-structure should be reflected by the index.
(2)
Polymorphs that are the result of structural transitions that obey the Landau criteria should also have higher indices. For instance, the transitions from cubic to rhombohedral and from cubic to tetragonal to orthorhombic ABO3–perovskites should be reflected by the index.
The above two criteria provide straightforward measures of the merit of a crystal symmetry index because they are based on well-defined concepts of the structural evolution of solids. In addition, it is required that:
(3)
The index should generally scale with increasing structural complexity as defined by the size of the asymmetric unit, and, more specifically, it should rank solids that assume the same space group but with vastly different sizes of their asymmetric units accordingly higher or lower.
Here, the following symmetry index is defined:
I S G = i n i · M i · S O F i M m a x · i n i
where ni is the number of occupied sites for chemical species i, Mi is the Wyckoff multiplicity of that site, Mmax is the maximal Wyckoff multiplicity that is possible in that space group, and SOFi is the site fraction occupancy of the site by species i.
Thus, ISG is the ratio of the sum of the orders of the subgroups of a space group that correspond to occupied sites in a structure, divided by the order of the space group itself times the number of occupied sites, that is, the lowest possible symmetry and maximal multiplicity. ISG is an isomorphic mapping from the space groups onto the field of rational numbers. The numbers quantify the deviation of the assumed symmetry from the lowest possible symmetry. Thus, generally ISG ≤ 1. Generally, the higher the complexity of a structure, the closer ISG is to unity. Partially vacant sites reduce ISG. In particular, ISG = 1 for any structure in space group 1 as long as all sites are fully occupied because all Mi’s equal Mmax; this is independent of the size of the asymmetric unit and, thus, limits the information about structural complexity that is represented by ISG.
This point and the functionality of ISG as a measure of structural complexity and discriminator for symmetry reductions, in general, is illustrated by some examples: The case of α- and β-quartz is illustrative. With Equation (3), ISG is
I S G   ( α ) = 3 + 6 6 + 6 = 3 4
for α-quartz and
I S G   β = 6 + 12 × 0.5 12 + 12 = 1 2
for β-quartz; therefore, the high-temperature, higher-symmetric polymorph is assigned to a smaller index and, thus, lesser structural complexity, reflecting the higher vibrational part of the free energy of β-quartz compared to α-quartz. It is noted that the lower index ISG of β-quartz results from the partial occupancy of site 12c, which, however, is essential in establishing the higher symmetry of the beta-phase. Thus, the index ISG behaves in accordance with the crystal physics of the two quartz polymorphs. For pyrite and marcasite, one finds ISG = ¼ and ¾, respectively (Table 1), which is in agreement with the crystal physics of these two polymorphs of FeS2. Substituting half of S with As gives arsenopyrite, FeAsS, with reduced crystal symmetry and ISG = 1 (Table 1). Further examples are given in Table 1: arsenopyrite has index 1, but so do enargite, panguite, anorthite, and, as mentioned, any crystalline phase that assumes space group P1 with all sites fully occupied.
Thus, ISG quantifies higher or lower symmetry within groups of related structures but does not discriminate between the intrinsic symmetry of very different structures. This issue is addressed further below in the Discussion. However, first of all, the results show that in combination with relation (2), ISG is instrumental in assessing limits for possible structures that are approximately quantitative (and it further outlines a path for making them fully quantitative).

3. Results

Correlating V, Vion, and ISG with Z, the number of chemical formula units defines allowed and forbidden fields of possible crystal structures independent of composition (as far as explored here). This is shown in Figure 2: Relation (2) is recast as ratio Vuc/Vion but multiplied with the inverse of ISG to give a normalized, dimensionless volume (hereafter: ‘symmetry-normalized volume’). In addition, the symmetry-normalized volume Vsym is weighted by the average slope of (2).
V s y m 1 1.87 · I S G · V u c V i o n
Vsym is related to Z, the number of chemical formula units per cell, as shown in Figure 2. As implied by the large deviations of individual values around the linear correlation (2), the values of Vsym occupy a large range of values between ≤2 and 1000. However, Figure 2a also shows rather well-defined upper and lower bounds for possible correlations between Vsym and Z. Figure 2b depicts the same data in a linear-logarithmic plot to better show the distribution of Vsym at small Z. Furthermore, the examined data (Table 1) indicate a distribution statistic for crystalline species within those bounds. The upper and lower bounds are discussed first.
Figure 2. (a) Correlation of normalized volume Vsym = Vuc/(1.87 ISGVion) and the number of chemical formula units Z, based on the data given in Table 1. Extensive forbidden zones of mechanically unstable low-density structures and of overly compact high-density structures are visible. Straight lines represent the upper and lower boundaries between the allowed and the forbidden zones. These lines are calculated based on the equations given in Table 2. The dashed lines represent the tentative limits for the low-density limit at large Z > 80 (Table 2). (b) Same but in linear-logarithmic plotting to make the data at low Vsym and Z better visible. The meaning of the lines and symbols is the same as in (a).
Figure 2. (a) Correlation of normalized volume Vsym = Vuc/(1.87 ISGVion) and the number of chemical formula units Z, based on the data given in Table 1. Extensive forbidden zones of mechanically unstable low-density structures and of overly compact high-density structures are visible. Straight lines represent the upper and lower boundaries between the allowed and the forbidden zones. These lines are calculated based on the equations given in Table 2. The dashed lines represent the tentative limits for the low-density limit at large Z > 80 (Table 2). (b) Same but in linear-logarithmic plotting to make the data at low Vsym and Z better visible. The meaning of the lines and symbols is the same as in (a).
Materials 17 02618 g002aMaterials 17 02618 g002b
Table 2. Tentative upper and lower boundaries of the correlation between Z and symmetry-normalized volume. The upper bounds were obtained by fits through the uppermost data points in Figure 2. For the lower bound, a fitted equation was modified so that it does not cut through the smallest Z data. The lower bound may have more terms that are influential at small Z, but this cannot be assessed using the given data. The adjusted R2 of fits are 0.97, 0.99, and 0.92, respectively (top to bottom), and the linear relation has not been fitted.
Table 2. Tentative upper and lower boundaries of the correlation between Z and symmetry-normalized volume. The upper bounds were obtained by fits through the uppermost data points in Figure 2. For the lower bound, a fitted equation was modified so that it does not cut through the smallest Z data. The lower bound may have more terms that are influential at small Z, but this cannot be assessed using the given data. The adjusted R2 of fits are 0.97, 0.99, and 0.92, respectively (top to bottom), and the linear relation has not been fitted.
BoundaryZVsym
Lower *>10.5 Z1.15
Upper1–8060 Z0.27
>800.03 Z1.97
or: 6.92 Z−400
* There is probably another term that limits this boundary to the symmetry-normalized volume around 2.

4. Discussion

4.1. Constraints on Possible Crystal Structures, Statistics, and Crystal Structure Prediction

Figure 2 shows large apparently forbidden zones of volume–symmetry correlations for inorganic compounds. This is less surprising than it may seem: for instance, the value of Vsym = 10 at Z = 48 falls within the lower forbidden zone. For a hypothetical phase of silica, these values give a density of 16.5 g/cm3 if ISG = 1, and for a cubic metric, for ISG = 0.75 and Z = 24, the density would be 11 g/cm3 in a cubic cell. In the upper forbidden zone, with, for example, Z = 48 and ISG = 1, a cubic phase of silica with Vsym = 300 assumes a density of 0.52 g/cm3. Thus, the forbidden zones represent regions where the available Wyckoff sites do not allow for stable structures either because at low density they are mechanically unstable toward collapse into denser structures or at high density they require extreme compression (very high inner energy, respectively), over which structures of smaller Z and lower density are favourable.
It is worth examining the boundaries between the allowed and the forbidden zones because they define the range where within inorganic crystalline structures are possible. Since the data set is limited (Table 1), these upper and lower boundaries are tentative. No strict evaluation of their functional dependence on Z and their uncertainties is attempted here. The approximate boundaries that are depicted in Figure 2 are summarized here in Table 2: All boundaries follow approximate power-law dependences of Z and provide tentative constraints on possible structures. In particular, at large Z, there are strong constraints on structures that are close to the high-density limit, and such crystalline phases may occur only sporadically. For instance, for a hypothetical polymorph of silica at Z = 144, Vsym = 146, and with ISG = 0.5625, the volume of the unit cell is about 2300 Å3, and a phase in space group Nr. 228 would have a density around 6.5 g/cm3 with Si and O on sites of multiplicities 48 + 96, and 96 + 192, respectively. ISG = 1 gives about twice the volume, but no cubic space group is compatible with this symmetry index, Z, and a stoichiometry 1:2. However, a rhombohedral phase of silica with Z = 144 and all atoms on special positions is compatible with the upper limit for a density of 3.5 g/cm3, which is between coesite and stishovite. These assessments shall only illustrate the rather strong constraints that are imposed by the high-density limit of the correlation Z ∝ Vsym (Figure 2, Table 2) and, hence, are made without any consideration of physical bond distances and -angles, which pose additional constraints, nor with any consideration of the free energy of such very large and dense polymorphs of silica.
The low-density limit is a positive monotonous correlation between the symmetry-normalized volume Vsym and Z, which simply states that the higher the number of chemical formula units, the larger the unit cell volume of possible crystalline structures that is stable towards spontaneous collapse into denser structures. The low-density limit obeys a power law with a slope of ~0.27 up to about Z = 80, where the slope changes to almost 2 (Table 2). However, instead of a fitted power-law relation for these data above Z = 80, a limiting linear relation (Table 2) is also consistent with the observed data (Figure 2). The divergence between the Z1.97 and the linear limiting relation becomes significant above Z = 200. This uncertainty about the actual functional relation between Vsym and Z above Z = 80 is a consequence of the limited statistics and emphasizes that the limiting relations in Table 2 are approximate. In any case, it is clear from Figure 2 that there is a change in slope for the low-density limit of the Vsym-Z correlation.
The extrapolation of the small-Z 0.27-power limit intersects the high-density limit around Z = 225 (Figure 2), implying that no crystalline structures are possible beyond that value, if these limits would hold for any Z. However, the crossover from 0.27 to ~2 widens the field of possible structures between the upper and lower boundary for Z > 90. Moreover, Figure 2 shows that the convergence of the Z0.27 small-Z, low-density limit towards the high-density limit causes a narrowing of the field of possible structures before the crossover of the power of the Z-dependence.

4.2. Effect of Pressure and Temperature

It was shown recently [22] that the measured pressure-dependent volumes and the pressure-dependent ionic volumes are strictly linearly correlated (at least for oxides and at least above 1–3 GPa) because the non-linear compressibility beyond Hooke’s law is dominated by the non-linear compression of the anions [17]. Thus, the ratio Vuc/Vion remains constant upon compression within narrow uncertainties and does not shift any of the phases in Figure 2.
Since ionic volumes are temperature-invariant by definition, Vsym increases with increasing temperature. Because thermal expansivity remains generally small up to the 1 bar melting point, Vsym remains below the upper limit of Figure 2. Examples are corundum at 300 and 2170 K; forsterite, Mg2SiO4, at 300 and 948 K; and protoenstatite, MgSiO3, at 1633 K (Table 1). It is expected that crossing the upper limit of the Z-Vsym relation is correlated with structural rearrangements or with melting, but this remains to be examined for a larger set of materials and data obtained at sufficiently high temperatures.

4.3. Statistical Distribution of Structures

The examined data provide only limited statistics for the count of structures across Z and structural complexity. It appears that at Z between 1 and 20, the maximum of existing structures is close to the high-density limit of the symmetry-normalized volume (Figure 2), and this is physically quite plausible because the crystallizing compounds are expected to minimize volume under the given sterical constraints imposed by the composition, ion size, and directional distribution of valence electrons. At large Z, it appears that the few available hydrogen-free inorganic solids are closer to the low-density limit than the high-density limit—in fact, no material appears to be close to the high-density limit for Z > 100. Based on the examples that are given above, this is plausible: the upper limit implies rather high densities for most compounds and space groups, thus limiting the number of possible structures. Figure 3a depicts the distribution of different chemical compound classes within the allowed range of Z-Vsym. Simple oxides and sulfides are more abundant in the low-Z range, where sulfides appear to be closer to the high-density oxides closer to the low-density limit. Silicates with small Z occupy the middle to close to the high-density limit but extend to large Z where they are close to—or at the low-density limit, whereas framework structures based on phosphate-, arsenate- or molybdate-groups are closer to the high-density limit up to Z ~ 80. In light of the discussion in Section 4.1., this observation provides a tentative explanation for, or at least a quantitative assessment of, the comparatively lesser number of such framework structures compared to those built from silica and alumosilicate networks.
The apparent high count of small Z silicates of higher density compared to simple oxides is not expected but finds a tentative explanation by the easier accommodation of constituent vacancies in high-temperature simple oxides, but this observation may well be biased by the very limited statistics.
The possible occurrence of very dense phases with very high Z is limited to accordingly very high pressures. Inside Earth, however, the geothermal gradient poses an entropic constraint on the formation of such phases. An additional constraint arises from the mobility of chemical elements in depth of Earth where no partial melts occur and where only metasomatosis through supercritical fluids acts as a potential means of mobilizing and segregating less common elements [23]. Moreover, chemically bonded water augments the number of potential mineral species in general [11,24].
Figure 3. (a) Figure 2 with key for different compound groups: red = silica and silicates, blue = simple oxides, titanates, aluminates; green = sulfides and arsenides. All others: Hollow diamonds. The remaining high Z data that are not silicates are phosphate-, arsenate-, borate-, or molybdate framework structures. As indicated in the discussion, these phases fall closer to the high-density limit of the Z-Vsym correlation than the silica-based large frameworks. (b) Figure 2 with key for different crystal systems: black = cubic; magenta = tetragonal; blue = trigonal and hexagonal; red = orthorhombic; green = monoclinic; hollow diamonds = triclinic. No strong correlation is visible for the examined set of data. There appears to be a tentative preference for cubic symmetry among the high Vsym phases and a preference for monoclinic phases at small Z and close to the high-density limit (see Table 2). The small number of triclinic phases is likely a bias from the limited number of phases and the exclusion of compounds with H-bonds [24,25]. An apparent preference for high crystal symmetry at high Z is noteworthy and deserves future study.
Figure 3. (a) Figure 2 with key for different compound groups: red = silica and silicates, blue = simple oxides, titanates, aluminates; green = sulfides and arsenides. All others: Hollow diamonds. The remaining high Z data that are not silicates are phosphate-, arsenate-, borate-, or molybdate framework structures. As indicated in the discussion, these phases fall closer to the high-density limit of the Z-Vsym correlation than the silica-based large frameworks. (b) Figure 2 with key for different crystal systems: black = cubic; magenta = tetragonal; blue = trigonal and hexagonal; red = orthorhombic; green = monoclinic; hollow diamonds = triclinic. No strong correlation is visible for the examined set of data. There appears to be a tentative preference for cubic symmetry among the high Vsym phases and a preference for monoclinic phases at small Z and close to the high-density limit (see Table 2). The small number of triclinic phases is likely a bias from the limited number of phases and the exclusion of compounds with H-bonds [24,25]. An apparent preference for high crystal symmetry at high Z is noteworthy and deserves future study.
Materials 17 02618 g003

4.4. Index of Crystal Complexity

It was stated in Methods that ISG does not discriminate between structurally unrelated crystalline phases. It should also be noted that Vuc/Vion does not provide a measure of crystalline complexity along the lines defined in Methods. For instance, Sc2O3 in the cubic bixbyite-type structures has a higher ratio Vuc/Vion than panguite, Ti2O3, a ‘collapsed bixbyite’, that is clearly the more complex structure, according to the three criteria established in Methods. Similarly, the Vuc/Vion of rhombohedral ABO3 perovskite LaAlO3 is higher than that of the orthorhombic perovskite CaTiO3. Thus, Vuc/Vion does not match the fundamental criteria of a physically meaningful index, and this statement holds for a variety of combinations of parameters that suggest plausible indices at first glance.
However, a general measure of structural complexity is obtained by combining ISG with the number of chemical formula units Z and the ionic volume as:
I S G · Z · V i o n 4 π / 3 · r B 3 = I c m p l x
where rB is the Bohr radius. Obviously, Icmplx is closely linked to relation (2) and to the correlation between Z and the symmetry-normalized volumes in Figure 2. Based on an algebraic index, ISG, and being dimensionless, Icmplx serves itself as an index. The term Σni in the denominator of ISG is divisible by Z, and (6) may be reformulated accordingly, but for clarity, it is better to keep Z as an explicit parameter. The full list of Icmplx’s is given in Table 1.
With Icmplx as a measure of structural complexity, the ambiguity of the unity values of the index ISG for structures with all atoms on sites of lowest possible symmetry in a space group vanishes. This and the other properties of Icmplx are illustrated through a number of examples that serve as tests of the three criteria established in Methods.
The minerals, enstatite (MgSiO3), anorthite (CaAl2Si2O8), sapphirine, and the clathrate framework silica phase Si264O528 all assume ISG = 1 despite obviously different structural complexity but their Icmplx’s are 403, 746, 724, and 39,889, respectively (Table 1), thus discriminating these structures in a quantitative fashion through assigning a single but unique number to each of them, in accordance with the third criterion in Methods.
The polymorphic Ca-alumosilicates anorthite and dmisteinbergite have both ISG = 1, but Icomplx assumes the values 1202.27 and 283.74 (Table 1), respectively, thus discriminating the ordered, low symmetric polymorph anorthite from the less ordered, high-temperature polymorph dmisteinbergite. Thus, Icmplx matches the fine-scale ranking of complexity that is obtained through topological network analysis [15] in this and in many other cases.
Corundum assumes Icmplx = 111.62 but ilmenite Icmplx = 115.48, representing the symmetry breaking imposed by the splitting of the cation site, in accordance with the first and second criterion of a meaningful index (see Section 2). γ-Al2O3 gives Icmplx = 40.36, which correctly reflects the lower complexity of this high-T polymorph of Al2O3 compared to corundum. The Ga2O3-type κ-Al2O3 has Icmplx = 331 due to an asymmetric unit that is large compared to corundum and to its low space group symmetry. A phase with low symmetry but modestly large asymmetric unit like the sodium chromate lopezite assumes ISG = 1 because all atoms reside on special positions; its Icmplx is 536.16, which ranks this Na-chromate between the inosilicates enstatite and clinoenstatite (both MgSiO3, see below and Table 1). This seems plausible since the structures of the latter two are based on tetrahedral chains with larger cations residing between these chains on distorted polyhedra with higher coordination, whereas in lopezite dimers of tetrahedra are arranged in linear arrays, like chains where every third tetrahedron is omitted, with likewise large low symmetric polyhedra occupied by Na.
For the series of K-Al-silicates kalsilite, nepheline, and panunzite, the Icmplx’s are 64.09, 446.23, and 2030.3, respectively, in accordance with the different sizes of the asymmetric units. ISG of marcasite, FeS2, and cubanite, CuFe2S3, are both 0.75, but their Icmplx’s are 102.8 and 324.1, correctly representing the difference in structural complexity between an AB2- and an ACB2-stoichiometry and a rutile-derived versus a sphalerite-derived tetrahedral superstructure. Isocubanite, (Cu,Fe)S, which is isotypic with sphalerite, ZnS, ranks very low with Icmplx = 6.0 as a highly symmetric and disordered high-T phase of very low complexity.
It is worth noting that Icmplx ranks complexity not always according to expectations that are based on the crystal metric. For instance, high-temperature clinoenstatite has lower Icmplx than enstatite despite its lower crystal symmetry. However, as a high-temperature phase, clinoenstatite has ~½ the unit cell of enstatite, which forms by condensation of phonons of the clinoenstatite lattice. Thus, Icmplx reflects the thermodynamic relation between both polymorphs of inosilicate MgSiO3 correctly (or more specifically, the first and second Landau criterion, and this is owed to the factor Z in Icmplx). The same statement holds for perovskites and for order-disorder induced symmetry breaking, such as for CoAsS, as well as for symmetry-reducing coupled substitutions for thorianite- and sphalerite-derived structures (see Table 1). Hence, Icmplx is an indirect measure of degrees of freedom in structures and fulfills criteria 1 and 2 that were outlined in Methods. Further examples of high–low T polymorphs and the according relations of their Icmplx’s are listed in Table 1.

4.5. Limitations of Icmplx

As defined, the index Icmplx is limited to solids where crystal radii can be applied at least as limiting cases of bonding, and that excludes proper metals and molecular materials. It has been shown previously [26] that at least pressure-induced polymorphism in elemental metals obeys simple relations between their volumes, number of valence shell electrons, and their principal and orbital quantum numbers, quite similar to the relations found for the radial part of valence states in ions that define crystal radii [18,27,28]. Thus, it is very likely that the concept of Icmplx can be expanded to metals and alloys.
Hydrogen poses a different problem. The apparent crystal radius of H+ is negative [19], which indirectly represents the effect of the H-bond averaged for many inorganic crystalline species. However, this effect should initially not be included in the ionic volumes as defined here. Therefore, in the present paper, the H-bearing phases are not considered. Vsym of H-bearing phases is expected to show a systematic shift toward lower values compared to non-H-bearing phases, which is indirectly expressed in the apparent negative crystal radius of H+ [19]. Icmplx is expected to be shifted to larger values [25].
Finally, molecular materials are not considered here and are expected to deviate systematically by the role of dissipative forces that control the intermolecular distances. It is noted that apparent ionic volumes of metallorganic network phases show a similar relation to actual molar volumes upon compression as inorganic phases [22], despite the markedly directional bonding in those compounds. Thus, the calculation of an apparent ionic volume of molecular phases may still be instructive but is beyond the scope of this study.

4.6. Tentative Statistics of Crystalline Phases Based on Icmplx

Due to the rather limited set of crystallographic data examined here, the distribution of Icmplx among the inorganic compound classes remains tentative: simple sulfides and oxides have overall lowest values of Icomplx between 1 and 200 (Table 1), complex sulfides assume in part much higher values. Salts with non-polymerized complex anions like carbonates and chromates have low to modest complexity with Icomplx’s of 50 to 300 (Table 1). Silicates assume values mostly between 200 and 1000, with the exception of framework structures, which extend to numbers as high as 40,000 (Table 1, Figure 2). Similarly, high numbers are obtained by frameworks that are based on molybdate, phosphate, arsenate, and borate groups. The apparent greater richness of large frameworks of silicates and phosphates compared to arsenates and molybdates is tentatively explained through the fact that the high-density limit of possible structures poses rather narrow constraints at large Z, while the latter two substance classes are placed closer to this upper than the lower density limit. This distribution is depicted in Figure 3a, which shows the same data as Figure 2 but with a key for different chemical compound classes.
It is noted that this tentative classification by Icmplx agrees well with that by Krivovichev [15]. Even the numerical values are mostly quite similar. This is not incidental because the network topology of crystalline phases is strongly correlated with the homotopic structure defined by the subgroup splitting of space groups that underlies the symmetry index ISG and, thus, Icmplx. A more rigorous mathematical discussion of this point is beyond the frame of this paper.
No strong correlation is visible for the distribution of crystal systems across Vsym for the examined set of data. This is shown in Figure 3b. There appears to be a tentative preference for cubic symmetry among the high Vsym phases and a preference for monoclinic phases at small Z and close to the high-density limit (see Table 2). The small number of triclinic phases is likely a bias from the limited number of phases and the exclusion of compounds with H-bonds [24,25]. An apparent preference for high crystal symmetry at high Z is noteworthy and deserves future study.

5. Conclusions

A general correlation between unit cell and ionic volume and an algebraic index ISG of crystal structure space group symmetry are combined into a symmetry-normalized volume Vsym that defines approximate upper and lower limits for possible crystal structures. These limits are tentatively fitted as power laws of Z. The lower limit is defined by the mechanical stability of low-density structures and follows a power law that crosses over from power 0.27 to either a linear or a nearly quadratic relation above Z = 80. In the relationship between Z and Vsym, most of the examined materials crystallize in small Z structures fall close to the upper limit, whereas it is shown that at large Z, the upper limit is more prohibitive for the formation of structures of physically possible densities and structures close to the low-density limit appear favourable. Based on these observations, an index of crystal structure complexity Icmplx is defined that properly scales with parameters such as order-disorder processes, symmetry reduction by coupled substitutions, 2nd order transitions, topological hierarchy, and number of atoms in the asymmetric unit. Icmplx is based on Wyckoff multiplicities, Z, and ionic volume only. It allows for categorizing classes of compounds by average complexity.

Author Contributions

Conceptualization, O.T. and M.B.; methodology, validation, analysis, and data curation, O.T and M.B.; validation and writing, O.T. and M.B. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Data Availability Statement

All data are listed in the tables in the paper.

Conflicts of Interest

The authors declare no conflicts of interest.

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Figure 1. Correlation between ionic and unit cell volume, both in Å3. The correlation is based on the inorganic solids and minerals given in Table 1.
Figure 1. Correlation between ionic and unit cell volume, both in Å3. The correlation is based on the inorganic solids and minerals given in Table 1.
Materials 17 02618 g001
Table 1. List of examined phases, Z, symmetry index ISG, measure of structural complexity Icmplx, ionic, and unit cell volumes. The records are ordered by increasing complexity index Icmplx (see Section 4). For natural crystalline phases, the mineral names are given; for zeolite frameworks, the common name is given; ISG and Icmplx are calculated according to Formulas (3) and (6). Ionic volumes are calculated based on Equation (1) using crystal radii from [19]. Unit cell volumes are averages based on data given in [20]. Because of ubiquitous polymorphism and in agreement with common practice, mineral names are used for phases that occur as such. Information about formation conditions is found in ref. [21].
Table 1. List of examined phases, Z, symmetry index ISG, measure of structural complexity Icmplx, ionic, and unit cell volumes. The records are ordered by increasing complexity index Icmplx (see Section 4). For natural crystalline phases, the mineral names are given; for zeolite frameworks, the common name is given; ISG and Icmplx are calculated according to Formulas (3) and (6). Ionic volumes are calculated based on Equation (1) using crystal radii from [19]. Unit cell volumes are averages based on data given in [20]. Because of ubiquitous polymorphism and in agreement with common practice, mineral names are used for phases that occur as such. Information about formation conditions is found in ref. [21].
PhaseZIcmplxISGVion3]V [Å3]
CaSiO3 Davemaoite12.138720.0347238.2354474.1
Cu1−xFexS4 Isocubanite45.997510.0416722.3364148.04
FeS, NiAs-type26.017460.0783323.8412961.19
ThO2 Thorianite47.667960.0312538.0769175.92
FeS Mackinawite29.089260.12522.5673267.92
SiO2 Stishovite29.588960.187515.87246.61
SiO2 β-Quartz328.05730.515.48049113.53
(Ni,Fe)9S8 Pentlandite237.255510.03186362.91611032.6
γ-Al2O31040.360820.0972225.7689500.94
MgAl2O4 Spinel842.763560.0972234.12799527.28
SiO2 α-Quartz356.11460.7515.48049113.25
KAlSiO4 Kalsilite264.08790.4040449.22811200.51
(Fe,Ni)3+xS4 Smythite364.917540.1458392.10339359.76
FeS2 Pyrite468.526110.2542.53511159.04
MgCO3 Magnesite672.068150.2777826.8402279.43
Cu2FeSnS4 Stannite275.309750.2593.49162317.98
SiO2 α-Cristobalite476.711650.7515.872153.15
CaCO3 Calcite682.27670.2777830.64215366.63
CuFeS2 Chalkopyrite495.730910.333344.57059291.57
LaAlO36102.08120.2777838.01764326.93
FeS2 Markasite2102.78920.7542.5351181.63
(Ca1.29, U0.50…) (Ti1.09, Nb0.79…) O6 (O0.98, F0.02) Betafite8105.4480.1041778.541141081.21
Al2O3 Corundum6111.62130.4166727.71396255.89
Al2O3 Corundum 2170K6111.62140.4166727.71396269.66
Al2O3 Corundum 11736111.62220.4166727.71396260.6
CoAsS Pa34112.46990.2777762.83221173.93
CaTiO3 Perovskite4117.05920.62529.0641224.63
CaCO3 Aragonite4130.71080.62532.45361226.97
CoAsS P234134.95410.333362.83221173.93
Mg2SiO4 Forsterite4135.40820.5833336.02152289.58
Forsterite 948K4138.24440.5833336.77582295.83
FeTiO3 Ilmenite6155.48430.5555628.95314315.84
Na6(AlSi O4)6 Sodalite, anhydrous1177.3540.4583240.2053759.05
Mg2Al3(AlSi5O18) Cordierite2215.83680.4524148.0691771.68
SiO2 Moganite12276.16190.915.872455.99
MgSiO3 Protoenstatite 1633K8276.5730.8333325.75101447.57
Ca(Al2Si2O8) Dmisteinbergite4283.74050.4848590.81244333.67
Ca(Al2Si2O8) Svyatoslavite2292.6064190.81244355.23
SiO2 Coesite16319.91360.821415.10948549.47
CuFe2S3 Cubanite4324.12240.7567.06243447.97
MgSiO3 Clinoenstatite (LP)8324.7162125.19448418.16
κ-Al2O38331.0387125.68504361.3
Al13Si5O20(OH,F)18Cl Zunyite4339.00250.2788188.68692665.61
K(AlSi3O8) Orthoclase4399.07780.812576.21943715.15
CoAsS Cobaltite4404.9029162.83221173.93
FeAsS Arsenopyrite4407.2117163.19049175.46
Cu6(Cu4Fe2)Sb4S13Tetrahedrite24450.22917602.651071.23
Na3K(Al4Si4O16)Nepheline2446.22870.90909152.3392726.25
Sc2O3 Kangite16470.42550.5555632.8497954.1
Si24O4824477.98920.8181815.109481386.3
Na4Al3Si9O24Cl Marialite2482.8120.6406233.91211093.33
SiO2 Linde-L framework1513.0610.45076706.50852204.67
SiO2 Chabasite36525.78930.615.109482337.86
K2Cr2O7 Lopezite4536.1572183.20006733.82
Mg3Al2Si3O12 Pyrope8604.43170.41667112.55371503.48
MgSiO3 Enstatite16649.4323125.19448832.49
NaMg3Al6(Si6O18)(BO3)3(OH)3(OH) Dravite3744.51940.631244.12761600
SiO2 ZSM4848751.13080.6428615.109482409.07
SiO2 PTS_244755.47740.70536166.20432395.23
SiO2 Ferrierite36788.68390.915.109481952.36
Cu3AsS4 Enargite2921.181285.89293.97
K0.04Al0.06Si0.44O STA-301441018.3650.51418.538564428.3
SiO2641099.6860.7058815.109483680.06
Fe7S841132.5780.9375187.4685696.84
Mg4(Mg3Al9)O4[Si3Al9O36] Sapphirine41166.7241181.05041312.11
CaAl2Si2O8 Anorthite81202.271193.283291342
SiO2 SSZ_58741315.50.730315.109484035.5
Ti2O3 Panguite161317.65151.11772938.69
Fe1−x S Pyrrhotite-5C41441.1060.951235.15111181.93
KAlSi2O6 Leucite161578.023161.218822356
SiO2 EU1-framework1121846.860.6774215.109486169.52
SiO2 ZSM11-framework961911.9570.8181815.109485400.4
Na2B2Si2O6241938.9140.7566.861723058
SiO2 Dodecasile1362009.820.607115.109487303.64
(K,Na)AlSiO4 Panunzite322030.2740.87545.007843110.17
SiO2 ZSM5-framework 70K882212.0320.9473816.469335394.38
SiO2 ZSM5-framework962413.1250.9473816.469335386.53
Si0.73Al0.27O2 Linde-Y1922595.8430.52615.9544914451.9
Cs7AsMo8O3082677.8220.5415.54036773.13
Si152O29212691.4340.756762207.5929088.23
K3YB6O12152794.1090.797145.07264583.29
LiRbP2O6323437.44166.677094586.48
KCoPO4483620.86146.82334736.48
Pb4Zn8P8O3283862.8821299.71815793.63
CuP2O4F4484027.0210.888958.58438454.3
SiO2 Faujasite14206.3140.92901.0214292
Mn11Na4.35(PO4)9124254.5940.891246.99648859.67
Na96(BePO4)9614258.520.743572.05812,760.41
LiPbB9O15244269.3650.852129.59976978.43
Cs12Zn4B20O4044305.4961668.12034947.65
CsTi2P3O12324681.9970.7037129.0587891.3
CsTi2As3O12324838.5740.7037133.37418608.82
Rb3Sc2As3O12165756.5230.765291.92444805.33
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Tschauner, O.; Bermanec, M. Crystal Structure Complexity and Approximate Limits of Possible Crystal Structures Based on Symmetry-Normalized Volumes. Materials 2024, 17, 2618. https://doi.org/10.3390/ma17112618

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Tschauner O, Bermanec M. Crystal Structure Complexity and Approximate Limits of Possible Crystal Structures Based on Symmetry-Normalized Volumes. Materials. 2024; 17(11):2618. https://doi.org/10.3390/ma17112618

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Tschauner, Oliver, and Marko Bermanec. 2024. "Crystal Structure Complexity and Approximate Limits of Possible Crystal Structures Based on Symmetry-Normalized Volumes" Materials 17, no. 11: 2618. https://doi.org/10.3390/ma17112618

APA Style

Tschauner, O., & Bermanec, M. (2024). Crystal Structure Complexity and Approximate Limits of Possible Crystal Structures Based on Symmetry-Normalized Volumes. Materials, 17(11), 2618. https://doi.org/10.3390/ma17112618

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