Giuseppe
Fisicaro
*a,
Bastian
Schaefer
b,
Jonas A.
Finkler
b and
Stefan
Goedecker
b
aConsiglio Nazionale delle Ricerche, Istituto per la Microelettronica e Microsistemi (CNR-IMM), Z.I. VIII Strada 5, I-95121 Catania, Italy. E-mail: Giuseppe.Fisicaro@imm.cnr.it
bDepartment of Physics, University of Basel, Klingelbergstrasse 82, CH-4056 Basel, Switzerland
First published on 28th February 2023
In this work we study isomers of several representative small clusters to find principles for their stability. Our conclusions about the principles underlying the structure of clusters are based on a huge database of 44000 isomers generated for 58 different clusters on the density functional theory level by Minima Hopping. We explore the potential energy surface of small neutral, anionic and cationic isomers, moving left to right across the third period of the periodic table and varying the number of atoms n and the cluster charge state q (Xqn, with X = {Na, Mg, Al, Si, Ge}, q = −1, 0, 1, 2). We use structural descriptors such as bond lengths and atomic coordination numbers, the surface to volume ratios and the shape factor as well as electronic descriptors such as shell filling and hardness to detect correlations with the stability of clusters. The isomers of metallic clusters are found to be structure seekers with a strong tendency to adopt compact shapes. However certain numbers of atoms can suppress the formation of nearly spherical metallic clusters. Small non-metallic clusters typically also do not adopt compact spherical shapes for their lowest energy structures. In both cases spherical jellium models are not any more applicable. Nevertheless for many structures, that frequently have a high degree of symmetry, the Kohn–Sham eigenvalues are bunched into shells and if the available electrons can completely fill such shells, a particularly stable structure can result. We call such a cluster whose shape gives rise to shells that can be completely filled by the number of available electrons an optimally matched cluster, since both the structure and the number of electrons must be special and match. In this way we can also explain the stability trends for covalent silicon and germanium cluster isomers, whose stability was previously explained by the presence of certain structural motifs. Thus we propose a unified framework to explain trends in the stability of isomers and to predict their structure for a wide range of small clusters.
Clusters can in principle be made of any number of atoms. The inspection of experimental mass spectra shows however that clusters of certain sizes can be found much more frequently than other sizes. For these sizes particularly low geometric ground states can be formed and they are called magic sizes. Numerous publications on the topic exist. We will extend the scope of these investigations by not only identifying geometric ground states as candidates for magic sizes, but by proposing general principles that also explain the relative stability of meta-stable isomers of clusters independently of whether they are magic sizes or not.
Two basic types of theories exist to explain the particular stability of clusters with magic sizes. The first theory is just based on purely geometrical considerations, while the second is based on the filling of electronic shells in a spherical jellium model.
For a simple pairwise potential icosahedral structures are highly stable. The smallest stable icosahedron can be formed by the 12 atoms located at the 12 corners of the icosahedron plus a central atom. The next two icosahedral structures then have one or two additional shells of atoms and consist of 55 and 147 atoms. So according to this geometrical theory the sizes containing 13, 55 and 147 atoms are predicted to be magic. Experimentally these sizes turn out to be magic sizes for rare gas atom clusters that are weakly interacting by van der Waals forces.22,23
The second theory establishes a connection between the number of valence electrons in the cluster and its stability. The concept of cluster electronic shells and the enhanced stability of clusters with completely filled shells starts from the work of Knight and co-workers on magic numbers in the mass spectra of free small sodium clusters.24 They detected a particular high stability for clusters containing 2, 8, 18, 20, 34, 40, 58… atoms. Knight and co-workers succeeded in rationalizing the experimental observations by means of the jellium model.25–27 The jellium model, an extension of the independent nuclear shell model,27 assumes that a gas of independent electrons is spatially confined by a model potential within a sphere. A uniform positive background charge mimics the ions in the cluster. The quantum mechanical energy levels of such a system together with their electronic occupations are given by |1s2|1p6|1d10|2s2|1f14|2p6|1g18|…, where s,p,d denote in the usual way the values l = 0, 1, 2 of the angular quantum number. The energetic ordering of the energy levels of electrons is however different from the one for a Coulombic potential. For most flat potentials27 the degenerate shells of jellium clusters can accommodate 2, 8, 18, 20, 34, 40, 58… electrons. Clusters with this number of valence electrons are considered magic clusters in this electronic theory.
For Na clusters it has been observed that for small sizes of up to 1500 atoms magic sizes are determined by electronic shell filling, whereas for larger sizes it is determined by complete geometrical shells.28 For the small clusters we are studying geometrical shell filling is in general not possible and only the Al−113 and the Al12Si exhibit this effect since they have a completely filled icosahedral shell.
Various generalizations of the jellium model have been proposed that take into account deviations from spherical symmetry. Distortions of the spherical shape lead to a splitting of energy levels with different quantum numbers, l.29 For weak distortions, the splitting is however relatively small30 so that they still can be lumped together into the levels of a spherical potential. Many of the early works on non-spherical metal clusters26,31,32 were not based on systematic structure predictions at the density functional theory (DFT) level. Since only this approach can reliably find the ground state geometries, it is therefore questionable whether the assumed shapes and resulting properties were the correct ones. Distorted jellium models fail for instance to predict the icosahedral shape of the Na55 cluster that is obtained from DFT calculations.33 The jellium model and its generalizations work best for clusters made out of alkaline and alkaline earth metals. As soon as atomic p orbitals come into play, such as in Al clusters, a jellium like shell structure is absent in most cases.34 It should also be pointed out that the jellium model fails for transition metal clusters.35
Trends in cluster properties are related according to the jellium model to the occupation of molecular electronic shells in much the same way as the occupation of the atomic shells govern the properties of the elements in the periodic table. This suggests that it is possible to regard particular clusters as superatoms.11,13,16,36–38 The concept of magic clusters paves the way to superatoms physics. Following the findings on the halogen character of the Al13 cluster, various research groups, such as the experimental group of Castleman and Khanna's theory group12,13,39 explored the concept of superatoms. For instance, adding an electron to the 39 valence electrons of the neutral cluster leads to a fully occupied shell of the jellium model. This leads to a high electron affinity of 3.6 eV which is comparable to that of the chlorine atom. Therefore, the cluster behaves in a similar way to an halogen atom.11,36,40,41
We propose in this study a theoretical framework which goes beyond the jellium model. It is based on geometrical arrangements of the nuclei that lead to electronic shells that can be filled completely by the number of available electrons. These shells are however in general quite different from the shells predicted by the jellium model as well as its extensions. In contrast to any kind of jellium model we do not have to assume that the nuclei are completely smeared out into a uniform background charge, but we can use real point like nuclei. Our approach is also not restricted to explain the stability of magic size ground states, but can explain the stability of any cluster.
In order to substantiate our model we explore and analyse the potential energy surface (PES) of various neutral and charged cluster isomers at the density functional theory level. The clusters are made out of elements of the third period of the periodic table and span the groups I to IV. In this way we can compare the behaviour of metallic and covalently bonded clusters. To understand the general principles of cluster stability we do not only consider systems that are experimentally known to be magic sizes. Instead we study in general the influence of the variation of the number of atoms and electrons on low energy meta-stable isomers. We do not consider in this work transition metal clusters. So if we refer in the following to metals we mean simple metals.
All structural searches were performed directly at the Kohn–Sham (KS) density functional theory level by coupling the MH method with the BigDFT package.47–49 BigDFT uses wavelets as basis functions, which are localized both in real and Fourier space and allows for an exact treatment of free boundary conditions without the need to introduce vacuum regions in the periodic dimensions for both neutral and charged systems. As a consequence, the code is well suited for the evaluation of the KS energies and forces for neutral and charged isolated clusters. Soft norm-conserving pseudo-potentials including non-linear core corrections50,51 were used. Except for Mg where we have used for backward compatibility7 the Local Density Approximation, the Perdew–Burke–Ernzerhof functional52 as implemented in the Libxc53 library was used. Spin polarized calculations were performed for all the clusters with an odd number of electrons. For a cluster with an even number of electrons, it was assumed that the electronic ground state is a singlet state, even though some exceptions to this rule are known.54 A zero electronic temperature was used for all the calculations, except for the Mg clusters with an odd number of electrons where a temperature of 3 × 10−3 Ha was used for faster convergence. All structures were relaxed using the Hellman–Feynman scheme until forces were less than 0.5 meV Å−1. We have made all data generated by this research, that are all structure coordinates of all minima found by the minima hopping method together with their structural and electronic properties, openly-available through the Materials Cloud Archive.55
Cluster | Number of electrons | Average bond distance [Å] | Shape factor S | Point group | Point group degeneracies | KS DFT degeneracies | Homo–Lumo gap [eV] | Chemical Hardness [eV] |
---|---|---|---|---|---|---|---|---|
Na−18 | 9 | 3.547 | 0.36 | D 2d | [1, 2] | [1, 2] | 0.40 | 1.25 |
Na 8 | 8 | 3.529 | 0.23 | D 2d | [1, 2] | [1, 2] | 1.08 | 1.84 |
Na+18 | 7 | 3.592 | −0.02 | C s | [1] | [1] | 0.48 | 1.67 |
Na−110 | 11 | 3.560 | 0.46 | D 2h | [1] | [1, 4*] | 0.33 | 1.23 |
Na10 | 10 | 3.571 | 0.51 | D 2d | [1, 2] | [1, 2] | 0.60 | 1.51 |
Na+110 | 9 | 3.587 | 0.36 | C 2v | [1] | [1] | 0.34 | 1.53 |
Na15 | 15 | 3.616 | −0.14 | C 1 | [1] | [1, 2*, 4*] | 0.31 | 1.25 |
Na+115 | 14 | 3.615 | −0.40 | D 3 | [1, 2] | [1, 2, 4*] | 0.79 | 1.54 |
Mg−110 | 21 | 3.191 | 0.28 | D 4d | [1, 2] | [1, 2] | 0.73 | 1.65 |
Mg 10 | 20 | 3.167 | 0.07 | C 3v | [1, 2] | [1, 2, 3*, 5*] | 1.29 | 2.11 |
Mg+110 | 19 | 3.185 | −0.17 | C 3v | [1, 2] | [1, 2, 3*] | 0.98 | 1.71 |
Mg +2 10 | 18 | 3.190 | −0.22 | C 3v | [1, 2] | [1, 2, 3*] | 0.89 | 2.06 |
Mg−111 | 23 | 3.192 | 0.30 | C s | [1] | [1, 2*, 4*] | 0.35 | 1.48 |
Mg11 | 22 | 3.172 | 0.35 | D 3h | [1, 2] | [1, 2, 4*] | 1.32 | 2.07 |
Mg+111 | 21 | 3.163 | 0.21 | C s | [1] | [1, 2*, 3*, 4*] | 0.33 | 1.73 |
Mg +2 11 | 20 | 3.112 | −0.07 | D 3h | [1, 2] | [1, 2, 3*] | 1.53 | 2.30 |
Mg−114 | 29 | 3.193 | 0.30 | C 2 | [1] | [1, 2*, 4*, 5*] | 0.41 | 1.40 |
Mg14 | 28 | 3.107 | −0.35 | C 2 | [1] | [1, 2*, 3*, 5*] | 0.57 | 1.66 |
Mg+114 | 27 | 3.147 | 0.31 | C 1 | [1] | [1, 2*, 3*] | 0.28 | 1.54 |
Mg+214 | 26 | 3.192 | 0.42 | C 1 | [1] | [1, 2*, 3*] | 0.84 | 1.87 |
Mg15 | 30 | 3.208 | 0.33 | D 3h | [1, 2] | [1, 2, 3*] | 0.50 | 1.56 |
Mg+115 | 29 | 3.208 | 0.32 | C 2v | [1] | [1, 2*, 3*] | 0.56 | 1.53 |
Mg+215 | 28 | 3.165 | 0.26 | C 1 | [1] | [1, 2*, 3*] | 0.46 | 1.66 |
Al−17 | 22 | 2.715 | 0.38 | C 3v | [1, 2] | [1, 2, 3*] | 0.74 | 2.05 |
Al7 | 21 | 2.711 | 0.28 | C 3v | [1, 2] | [1, 2, 3*] | 0.88 | 2.25 |
Al +17 | 20 | 2.735 | 0.06 | C 3v | [1, 2] | [1, 2, 3*] | 1.96 | 2.86 |
Al+27 | 19 | 2.759 | −0.06 | C 2v | [1] | [1, 2*, 3*] | 0.44 | 2.26 |
Al−110 | 31 | 2.742 | 0.14 | C s | [1] | [1, 2*, 3*] | 0.60 | 1.86 |
Al10 | 30 | 2.756 | 0.05 | C s | [1] | [1, 2*, 3*] | 0.59 | 1.97 |
Al+110 | 29 | 2.771 | −0.08 | C 1 | [1] | [1, 2*, 3*, 4*] | 0.55 | 2.01 |
Al+210 | 28 | 2.746 | 0.67 | D 2d | [1, 2] | [1, 2, 3*] | 1.26 | 2.38 |
Al −1 13 | 40 | 2.756 | 0.00 | I h | [1, 3, 4, 5] | [1, 3, 4, 5, 10*] | 1.88 | 2.52 |
Al13 | 39 | 2.771 | −0.05 | D 3d | [1, 2] | [1, 2, 3*, 4*, 7*, 9*] | 0.46 | 1.87 |
Al+113 | 38 | 2.747 | −0.16 | C s | [1] | [1, 2*, 4*, 5*] | 1.24 | 2.28 |
Al+213 | 37 | 2.763 | −0.16 | C s | [1] | [1, 2*, 3*, 4*, 5*] | 0.43 | 1.89 |
Al12Si−1 | 41 | 2.751 | 0.06 | D 5d | [1, 2] | [1, 2, 3*, 5*, 6*, 7*, 10*] | 0.47 | 1.88 |
Al12 Si | 40 | 2.735 | 0.00 | I h | [1, 3, 4, 5] | [1, 3, 4, 5, 6*, 7*] | 2.00 | 2.73 |
Al12Si+1 | 39 | 2.757 | −0.04 | D 3d | [1, 2] | [1, 2, 3*, 5*, 9*, 10*] | 0.49 | 1.96 |
Al12Si+2 | 38 | 2.739 | −0.16 | C s | [1] | [1, 2*, 5*, 7*] | 1.30 | 2.33 |
Al14−1 | 43 | 2.766 | 0.22 | C s | [1] | [1, 3*, 4*, 8*, 9*] | 0.50 | 1.75 |
Al14 | 42 | 2.757 | 0.22 | C 3v | [1, 2] | [1, 2, 3*, 4*, 9*] | 0.90 | 2.01 |
Al+114 | 41 | 2.780 | 0.09 | C 2v | [1] | [1, 3*, 4*, 8*, 10*] | 0.56 | 1.97 |
Al+214 | 40 | 2.778 | 0.01 | C 3v | [1, 2] | [1, 2, 3*, 5*, 7*] | 1.92 | 2.60 |
Al15 | 45 | 2.769 | 0.29 | C 2h | [1] | [1, 2*, 3*, 4*, 8*] | 0.41 | 1.77 |
Al+115 | 44 | 2.797 | 0.24 | D 2h | [1] | [1, 2*, 3*, 4*, 9*] | 1.22 | 2.20 |
Al+215 | 43 | 2.786 | 0.24 | C s | [1] | [1, 2*, 3*, 4*, 6*, 7*] | 0.48 | 1.85 |
Si 10 | 40 | 2.515 | 0.05 | C 3v | [1,2] | [1,2,3*,7*] | 2.09 | 2.94 |
Si+110 | 39 | 2.530 | −0.04 | C s | [1] | [1, 2*, 3*, 4*, 5*] | 0.70 | 2.31 |
Si+210 | 38 | 2.541 | −0.17 | C s | [1] | [1, 2*, 4*, 5*] | 1.55 | 2.76 |
Si15 | 60 | 2.528 | 0.31 | C 3v | [1, 2] | [1, 2, 3*, 6*] | 2.19 | 2.79 |
Si+115 | 59 | 2.529 | 0.29 | C s | [1] | [1, 2*, 3*, 4*, 5*, 10*, 11*] | 0.51 | 1.96 |
Si +2 15 | 58 | 2.522 | 0.23 | D 3h | [1, 2] | [1, 2, 5*] | 1.96 | 2.67 |
Si+315 | 57 | 2.512 | 0.81 | C 2 | [1] | [1, 2*, 3*, 5*, 6*, 8*] | 0.52 | 1.87 |
Si20 | 80 | 2.544 | 0.70 | C 3v | [1, 2] | [1, 2, 3*, 4*, 9*] | 1.78 | 2.36 |
Si+120 | 79 | 2.542 | 0.65 | C 2v | [1] | [1, 2*, 3*, 5*, 6*, 11*, 16*] | 0.31 | 1.66 |
Ge15 | 60 | 2.742 | 0.33 | C s | [1] | [1, 2*, 3*, 6*, 8*] | 1.59 | 2.39 |
Ge+115 | 59 | 2.739 | 0.31 | C 2v | [1] | [1, 2*, 4*, 5*, 8*, 12*] | 0.47 | 1.89 |
Ge +2 15 | 58 | 2.759 | 0.27 | C 1 | [1] | [1, 2*, 5*, 12*] | 1.20 | 2.25 |
Our global minimum structures for various cluster families are in agreement with previous structure prediction searches and experimental investigations. They are all shown in Fig. 1. The global minimum of Na8 agrees with previous Car–Parrinello simulations,58 the Na−110 and Na15 GMs agree with the GM structures found by means of the CALYPSO structural search coupled to the simulated photoelectron spectra.59 Magnesium neutral global minima agree with the ones found by the CALYPSO structure prediction code60 and with other DFT studies.61–63 Global minima for neutral and charged aluminium clusters agree with previous DFT calculations for Al7.64,65 All the global minima of aluminum clusters match the ones determined by means of a multistage search approach (genetic algorithm, basin hopping, minima hopping and “by hands constructions”).66–68 Silicon global minima agree with the one determined by infrared multiple phonon dissociation spectra.69 Si15 GM corresponds to the one found by genetic algorithm explorations coupled to ion mobility measurements70 and the one determined by vibrational IR spectra coupled to DFT calculations.71 Si20 GM agrees with the one found by single-parent evolution search,72 the one determined by the “big bang” optimization method73 or with previous MH structure predictions.9
(1) |
(2) |
The average coordination number ζ associated to a particular isomer is the average of ζk over all atoms k. The average bond distance is defined as the average over all atoms k of a cluster isomer of the average over all distances between the k atom and all the other atoms l used in the calculation of the coordination number ζk.
Fig. 2 shows the correlation between the Kohn–Sham energy EKS and the average coordination number ζ. Each sub-box is associated to a particular cluster family. The color scale for data dots indicates the average bond distance. The red dot represents the global minimum for each particular PES.
We notice a remarkable and nearly linear correlation between the Kohn–Sham energy EKS of the isomers and their average coordination number ζ for all examined simple metals. The global minima of all the metallic systems are characterized by a high average coordination number ζ with a value higher than five or six depending on the cluster size n. Even though, as already pointed out, we do not study transition metal clusters, let us add for completeness that our findings for simple metals clusters are certainly not transferable to transition metal clusters. As is well known both pure74 as well as decorated75 small gold clusters have for instance planar shapes.
For the non-metallic clusters, where directional covalent bonds dominate, no such correlation can be seen. Like the corresponding bulk materials, the metallic clusters have much larger coordination numbers than the non-metallic clusters.
Table 1 reports the average bond distance of all global minima found in our minima hopping runs for neutral and charged clusters. In all cases the global minima of metallic clusters (sodium, magnesium and aluminium) have a shorter average bond length than the bulk phases. This is due to a redistribution of the charge from the region outside the surface of the cluster to the centers between neighboring atoms in the cluster as can be seen from the panels in the second row in Fig. 3, corresponding to an isovalue of 0.004. This charge redistribution is possible in a metallic system and leads to a lowering of the energy since the additional electronic charge inside the cluster is fully surrounded by the positively charged nuclei, whereas outside the surface it would only interact with a much smaller number of surface nuclei. A higher charge density in between neighboring atoms leads accordingly to the Hellmann–Feynman theorem to shorter bond lengths. This mechanism, which leads to bond shortening, is also encountered for the clusters of the other two elements that we examined, namely Na and Mg, as shown in Fig. S1 and S2 of the ESI.†
Apart from this charge flow towards bond centers, the bonding properties of the elemental metallic solid and the cluster are quite similar. As can be seen from the top panels in the first row of Fig. 3 (isovalue 0.002), there is a ring shaped electronic cloud around the atoms with a peak in the middle between nearest neighbors.
On the other side, the global minima of the covalent systems (silicon and germanium) are characterized by larger average bond distances compared with the corresponding bulk materials. Due to the strong directional bonding in insulators arising from hybridized orbitals, the charge in a disordered structure cannot flow into the bond region between two atoms to the same extent as in a solid with a perfect tetrahedral bonding pattern. This is also illustrated in the bottom panels, third row, of Fig. 3 (isovalue 0.006). In the ground state diamond structure of bulk silicon the sp3 hybridisation allows the charge to accumulate in the four tetrahedral positions which are exactly the bond centers. In the case of a Si cluster, the non-tedrahedral arrangement of the nearest neighbors does not allow for this kind of optimal charge accumulation in the middle between two atoms. Instead the charge is distributed in some kind of irregular way in the interstitial region. If there is less charge, in between two atoms, the bond length is longer as a consequence of the Hellmann Feynman theorem. In addition one can find core atoms that have a much higher coordination than the bulk atoms.
For each isomer we computed the surface and volume of the associated soft-sphere cavity. Fig. 4 shows the correlation between the Kohn–Sham energy EKS of the isomers and their surface to the volume ratio of their associated soft-sphere cavity. The plots show a high degree of correlation for all metallic clusters. In most cases the correlation is linear and low-lying isomers have a lower surface to volume ratio with respect to higher energy structures. The global minimum (red dots) coincides in general with the geometrical arrangement that minimizes this descriptor. Since the volume to surface ratio is strongly size dependent one can of course use this descriptor only for comparing clusters with the same number of atoms, where one can expect the volumes to be nearly constant.
So for a given number of atoms, there is a strong tendency to adopt compact shapes, but forming a nearly spherical cluster is not possible for any number of atoms as can be seen from the atomic arrangements shown in Fig. 1. The ground states show in general significant deviations from a perfect spherical shape. The icosahedron made out of 13 atoms (12 atoms from the 12 corners of the icoshedron and 1 central atom) is an exceptional case where one can form a quasi spherical shape. But with 15 spheres it is for instance not possible to obtain an approximately spherical shape by close packing spherical atoms of nearly identical size. The ground states of Na15 and Mg15 are consequently non-spherical.
The non-metallic clusters Ge15, Si10, Si15 and Si20 show hardly any correlation between the energy and the surface to volume ratio. The strong directional bonding prevents the cluster from adopting a nearly spherical shape.
S = λ2/λ3 − λ1/λ2 | (3) |
The length of the structure along the eigenvectors of the inertia tensor, called the principal axes of inertia, is given by the reciprocal square root of the eigenvalues. For a strongly oblate structure, which has two long axes and a short one, we have λ1 ≈ λ2 ≪ λ3 and hence S ≈ −1. For a strongly prolate structure, which has one long axis and two short ones, we have λ1 ≪ λ2 ≈ λ3 and hence S ≈ 1. So S = 0 indicates a spherical shape whereas positive values of S indicate a prolate shape and negative values an oblate shape as shown in Fig. 5. The shape factor is actually not only zero for a sphere but for all Platonic solids (tetrahedron, cube, octahedron, dodecahedron and icosahedron). Such shapes are however not present in our data set, except the icosahedron which is indeed quite spherical.
Fig. 5 An oblate (left) and prolate (right) shape. Figure taken from: https://en.wikipedia.org/wiki/Spheroid. |
Fig. 6 shows the correlation between the Kohn–Sham energy EKS of a given cluster local minimum and its shape factor S defined by eqn (3). Values of the shape factor for all global minima are reported in Table 1. The preference for spherical shapes can be clearly seen for metallic clusters. Nevertheless many ground states, particularly with sizes in between the magic sizes of the jellium model, do not succeed to be close to spherical as can be deduced from the shape factors in Table 1. Higher energy metal cluster isomers typically adopt a prolate shape. While we limit our investigation to small clusters, a very similar behaviour based on geometrical shell completion was observed for a Na cluster with up to 147 atoms.6 For geometrically magic sizes of 55 and 147 atoms the ground state is a spherical icosahedron. For the sizes in between, disordered ground states were found that deviate significantly from a spherical shape. A non-spherical ground state was also reported for the Na34 cluster.33
Fig. 6 Correlation between the Kohn–Sham energy EKS of isomers and their shape factor S defined by eqn (3). Each box belongs to a particular cluster family. E0KS is the KS energy of the global minimum. The color scale for data dots is based on the average bond distance (Å). The red dot represents the global minimum for each PES. |
No clear trends can be seen for the non-metalic clusters. For the Si20 which has a prolate ground state, the energy rises continuously when the shape becomes more spherical.
The principal axes of inertia are frequently aligned with the structure's symmetry axes. If a rigid body has an axis of symmetry of order m, meaning it is invariant under rotations of 360°/m about the given axis, this axis is a principal axis. When m > 2, the rigid body is a symmetrical top. If a rigid body has at least two symmetry axes that are not parallel or perpendicular to each other, it is a spherical top.80 The more symmetric the structure is, the more S tends toward zero.
It is worth noticing that low-energy minima of clusters with a magic number of electrons (or near magic number, that is ±1 electrons with respect to a magic number) always have an almost zero shape factor. This holds, in particular, for the potential energy surface of the magic clusters Na8, Mg10, Mg+210, Mg+211, Al+17, Al−113, Al12 Si, Al+214, and Si10 (see Table 1). As a consequence, low-energy minima of magic clusters are highly symmetric and their arrangement tends toward a spherical top symmetry (see GM structures in Fig. 1). The spherical character of low lying isomers correlates with their higher coordination number ζ as shown in Fig. 2.
Only a weak correlation between the energy and fingerprint distance can be seen for the non-metallic clusters. Extensive annealing might be required experimentally to find the ground state and in some cases it might actually not be reachable.85
(4) |
Consequently the Kohn–Sham orbitals are eigenfunctions of both and , and the eigenfunctions, that can be mapped onto each other by a symmetry operation, are degenerate. Filling an entire set of degenerate orbitals with the same number of possibly fractional electrons results in a charge density with the same symmetry as the cluster. Higher symmetries lead on average to higher degeneracies.
Table 1 gathers various structural and electronic properties of all global minima. Clusters that have a number of valence electrons that would classify the cluster size as magic in the jellium model are highlighted in bold in Table 1. However, as can be seen from the shape factors in Table 1, the shape of most of these clusters is quite non-spherical and the jellium model is not expected to be applicable. The failure of the jellium model can be seen from the fact that either the ideal shell ordering (1s, 1p, 1d, 2s, 1f, 2p) is reversed and/or some of these levels are split due to the symmetry breaking. These two effects have been studied in detail for Al clusters34,86 and we have also found them in many of our clusters as can be seen from their DoS (Fig. 1). Nevertheless, in virtually all cases completely filled shells stabilize the ground state of the clusters.
The shells are frequently related to exact degeneracies arising from symmetry, but approximate degeneracies that arise from small symmetry reducing Jahn–Teller distortions, are even more important. We considered KS eigenvalues to have an approximate degeneracy if they differ by less then 10−2 Ha. The Al−113 cluster has for instance a high Ih symmetry. Removing one electron leads to a small relaxation (see Fig. 9) that reduces the symmetry to D3d. The exact 3 and 4-fold degeneracies that exist in the Ih group become approximate degeneracies (see Table 1) during the relaxation. The same effect can be seen in the non-metallic Si15 cluster. Removing one electron reduces the symmetry from C3v to Cs and the exact two fold degeneracy becomes an approximate degeneracy. Several other similar cases can be deduced from Table 1.
We call this process, which allows for the complete filling of shells formed by exact or approximate degeneracies, optimal matching, because the degeneracies of the occupied eigenvalues have to match the number of available electrons. The eigenvalue spectrum is of course determined by the structure of the cluster. So in an optimally matched cluster the atoms have to be able to find positions such that the resulting spectrum has shells that can be filled completely by the available number of electrons. We can see from Table 1 that it is not possible to find such an optimal matching for any number of atoms and electrons, using only the degeneracies related to symmetry. It is therefore not true that the ground state of a cluster is necessarily of high symmetry. We will later on discuss some clusters where the highest symmetry structure is only a low energy meta-stable structure but not the ground state. The systems for which such an optimal matching is possible are however in the majority of cases of higher symmetry, which results frequently from a moderate distortion of an even higher symmetry structure as discussed above. Approximate degeneracies are particularly important for small clusters with few electrons where a single approximate degeneracy can already have a large stabilizing effect.
When the optimal matching gives rise to a highly degenerate level, the cluster is particularly stable and is therefore expected to be found in large quantities in experimental spectra and to be thus a magic size. High degeneracy is in general related to high symmetry. The particularly low energy per atom of the ground state of optimally matched clusters is shown in Fig. 10 for the anionic Al clusters in the range between 10 and 22 atoms. This energy is on average of course decreasing as a function of cluster size and converging to the bulk value. Al−113 has the highest symmetry (Ih) and therefore by far the highest degree of degeneracy in the size range considered. As shown in Fig. 11, all the valence electrons are accommodated in seven shells arising from exact symmetries and in only five shells of near degeneracy. As a consequence it has the lowest energy per atom over a considerable range of cluster sizes.
Fig. 11 Structures and density of states of the series of anionic Al clusters. The high stability of Al−113 relative to other cluster sizes, shown in Fig. 10, clearly coincides with the high degeneracies of this cluster. See also Fig. S3 of the ESI† for a similar figure augmented by the data used to make the figure plus selected structural and electronic properties. |
Fig. 12 shows the density of states for various perturbed and unperturbed global minimum configurations. We consider the GM of Mg11, with a non-magic number of 22 valence electrons, and the GM of the clusters Al+214 and Si10, both with the magic number of 40 valence electrons. These GM are particularly stable as shown by the large energetic distance of the first meta-stable configurations relative to the ground state (sharp increase of EKS in the relative leftmost panels of Fig. 1) and their large HOMO–LUMO gap, reported in Table 1. For each system we extracted the electronic properties for the unperturbed (δ = 0.0 Å) structure as well as for structures where each atomic coordinate has been randomly displaced with an amplitude δ between 0.0 and 0.5 Å. Since we obtained the DoS plots by a convolution with a Gaussian of width 0.1 eV, the lifting of the degeneracies becomes visible only for random displacements with an amplitude of 0.5 Å or more. This random perturbation also has the side effect of reducing the HOMO–LUMO gap (see Fig. S4 of the ESI†). This analysis elucidates the process of structural adjustment towards the global minimum driven by an optimal matching condition for the nuclei configuration and valence electrons.
Fig. 12 Lifting of the KS eigenvalue degeneracies by random atomic displacements away from the global minima. The effect for two different displacement amplitudes δ is shown, δ = 0.01 and 0.5 Å. See also Fig. S4 of the ESI† for a similar figure augmented by the data used to make the figure plus selected structural and electronic properties. |
Among the meta-stable structures high symmetry structures with filled shells can also be found frequently as detailed in Table 2. Fig. 13 and 14 show that all the low energy structures of these metallic clusters try to be spherical and to form completely filled shells (see also Fig. S5 and S6 of the ESI† reporting additional structural and electronic data for the same structures). Moving from the eighth minimum to the GM of Al−113 in Fig. 14, the formation of electronic shells and the adoption of a spherical arrangement is clearly visible. However the high symmetry structures with completely filled shells get rarer with increasing energy of the isomers. As shown in the histogram of Fig. 15, the abundance of high symmetry structures in all meta-stable configurations is much lower than in the ground state structures. In the ground state structures the Cs and C3v symmetry dominate whereas the overwhelming majority of the meta-stable structures have no symmetry, i.e. belong to C1.
Cluster | Minimum | Number of electrons | Point group | Point group degeneracies | List of all KS DFT degeneracies |
---|---|---|---|---|---|
Mg10 | 1 (GM) | 20 | C 3v | [1, 2] | [1, 1, 2, 1, 2, 2, 1] |
2 | 20 | C 3v | [1, 2] | [1, 2, 1, 2, 1, 2, 1] | |
3 | 20 | D 4d | [1, 2] | [1, 1, 2, 1, 2, 2, 1] | |
4 | 20 | C 4v | [1, 2] | [1, 2, 1, 1, 2, 1, 1, 1] | |
6 | 20 | T d | [1, 2, 3] | [1, 3, 1, 3, 2] | |
12 | 20 | D 2d | [1, 2] | [1, 1, 2, 1, 2, 1, 1, 1] | |
Al−113 | 1 (GM) | 40 | I h | [1, 3, 4, 5] | [1, 3, 5, 1, 3, 3, 4] |
2 | 40 | C 3v | [1, 2] | [1, 1, 2, 2, 1, 2, 1, 2, 1, 2, 1, 1, 2, 1] | |
4 | 40 | C 3 | [1, 2] | [1, 1, 2, 1, 2, 1, 2, 1, 2, 2, 1, 2, 1, 1] | |
13 | 40 | C 3v | [1, 2] | [1, 1, 2, 1, 2, 2, 1, 1, 1, 2, 3*, 1, 2] | |
105 | 40 | C 3v | [1, 2] | [1, 1, 1, 2, 2, 1, 2, 1, 2, 1, 2, 1, 2, 1] |
Fig. 13 Structures and density of states of the first eight low-lying minima for the Mg10 cluster. See also Fig. S5 of the ESI† for a similar figure augmented by the data used to make the figure plus selected structural and electronic properties. |
Fig. 14 Structures and density of states of the first eight low-lying minima for the Al−113 cluster. See also Fig. S6 of the ESI† for a similar figure augmented by the data used to make the figure plus selected structural and electronic properties. |
The optimally matched clusters can also easily be recognized in the density of states plots in Fig. 1. In all these cases the density of states consists of a rather small number of narrow but high peaks arising from the degenerate shells and the Fermi level is in the middle of a large gap separating the fully occupied shells from the unoccupied shells. It does not matter whether the degeneracy comes from the spherically symmetric potential of the jellium model or whether it comes from another kind of high symmetry structure.
The energetically favorable high symmetry ground state structures always have several classes of equivalent atoms that see the same environment. In the Al−113 cluster there are for instance two classes. The first comprises the 12 surface atoms of the icosahedron, and the second class consists only of the central atom. To obtain an overall low energy structure, the characteristic environments of the atoms defining the different classes must lead to low energy. When one transforms a high symmetry ground state into a meta-stable structure, at least one atom has to be moved. Since it was in a low energy position, the energy will typically increase strongly in such a move. In addition the corresponding moves of another atom in the same equivalence class will either give rise to an identical meta-stable structure or to a structure related by a symmetry operation. In both cases the increase in energy will be identical. Hence we can expect that we find only a relatively small number of structures in the funnel of a high symmetry ground state and that the energy gap between the ground state and the first meta-stable structure is relatively large. In a ground state with low symmetry all, or at least most atoms, have different environments, which are not all energetically optimal. Hence there are many possibilities to generate meta-stable structures and the energy increase will frequently be smaller since the starting point was already higher in energy. These expectations are confirmed by our data. The leftmost panel of each line in Fig. 1, corresponding to a cluster with a fixed number of atoms, shows the energy with respect to the ground state, EKS–E0KS, for the energetically sorted meta-stable structures. Since EKS–E0KS increases rapidly for magic clusters, they have a deeper global minimum funnel containing a smaller number of meta-stable structures.
A more detailed description of a funnel can be obtained from a disconnectivity graph which also provides the height of the barriers that have to be crossed when hopping from one minimum of the potential energy surface to another one. The disconnectivity graphs in Fig. 16 show, in agreement with the EKS curves in the panels at the left of Fig. 1, that Si10 has the deepest funnel followed by the ionized Si10 clusters. In agreement with Fig. 7, the disconnectivity graphs also show that only Si10 and to a certain extent its ions are structure seekers whereas the other silicon clusters have a glassy energy landscape.
Since the spatial orbitals can always be filled with two electrons of opposite spin, a complete filling of the shells is only possible for clusters with an even number of electrons. For this reason all the magic clusters have an even number of electrons. If the neutral cluster has an odd number of electrons, the ionized cluster can sometimes be optimally matched. This is for instance the case in Al−113 where the 40 valence electrons can completely fill all the shells of the jellium model. A complete filling of the shells is also observed for other clusters: the GM of Mg+211 and Al+17 with 20 electrons; the GM of Al12 Si and Al+214 with 40 electrons.
For some well matched ground states, taking away or adding an electron can conserve up to slight distortions in the ground state such as in the Al13 cluster shown in Fig. 1 or 9. However in many cases the ground state configuration of the ionized cluster does not coincide with the ground state of the neutral cluster.9
Closely related to the HOMO–LUMO gap is the chemical hardness η, defined as
(5) |
Applying a three-point finite difference approximation, we can extract the chemical hardness from the vertical ionization energy EVi and the vertical electron affinity EVa
(6) |
In a single particle scheme, the hardness is identical to the HOMO–LUMO gap. The vertical ionization energy EVi is defined as the total energy difference between the (m − 1)-electron and the m-electron system with the cluster geometry kept fixed at the optimized m-electron configuration. Analogously, the vertical electron affinity EVa is defined as the energy difference between the m-electron and the (m + 1)-electron system at the frozen m-electron configuration.
The maximum hardness principle87 was originally proposed by Pearson. It states that “at equilibrium, chemical systems are as hard as possible”. The chemical hardness quantifies the resistance to the changes in the number of electrons in the system, or to changes in the electronic density. A value of zero denotes maximum softness. For lithium clusters it was already shown that the magic size clusters are characterized by a particularly high hardness.88
Even though the correlation of the total energy with neither the ionization energy nor the electron affinity is good, the correlation with the hardness is very good. As shown in Fig. 18 there is a clear linear correlation between the Kohn–Sham energy EKS and the chemical hardness η. In most of the cases, the global minimum (red dot on each subgraph, data reported in Table 1) lies in the high η region of the PES. This is especially true for magic clusters or, in general, clusters with filled shells like the GM of Mg11, Si10 and Si15.
In its ground state, the Mg11 cluster can fill with its 22 electrons all the shells arising from a strongly non-spherical structure with D3h symmetry. So optimal matching can explain this ground state, but since the structure is less compact than Mg clusters made out of a different number of atoms, it is not expected to be a magic size.
The competition between adopting a spherical shape and the complete filling of shells can be well observed in the Na8 and Mg10 clusters. The Td structure of Na8 (Fig. 19 or Fig. S7 of the ESI† reporting additional structural and electronic data for the same structures), which allows for complete filling of the two shells, is only the first meta-stable structure, while the ground state has three filled shells. For Mg10 (Fig. 13) the highest symmetry structure is the tetrahedron which is however only the sixth meta-stable structure. The lower symmetry C3v structure is the ground state. In both cases the ground states are slightly more compact than the more symmetric meta-stable structures.
Fig. 19 Structures and density of states of the first two low-lying minima for the Na8 cluster. The first meta-stable structure has higher degeneracies than the ground state, but is slightly more compact. See also Fig. S7 of the ESI† for a similar figure augmented by the data used to make the figure plus selected structural and electronic properties. |
Fig. 20 illustrates nicely the role of optimal matching in Al13. Starting from the Al−113 cluster which is an optimally matched cluster, we can either take away an electron while freezing the Ih structure or keep the 40 electrons but transform the structure into the quite similar D3d ground state structure of the neutral Al13. In both cases degeneracies are lifted. In the first case the reason is that the incomplete filling of the electronic shells leads to Hartree and exchange correlation potentials of lower symmetry. In the second case the ionic potential arising from the nuclei is of lower symmetry. Both processes reduce the stability of the cluster. See also Fig. S8 of the ESI† for a similar figure augmented by the data used to make the figure.
Fig. 20 Density of states of 40 (a) and 39 (b) valence electrons, distributed over a perfect icosahedron with point group Ih. This structure is the GM of Al−113 and has point group degeneracies [1, 3, 4, 5]. (c) The DoS of 40 electrons distributed over the slightly distorted icosahedron D3d, GM of Al13, which has point group degeneracies [1, 2]. See also Fig. S8 of the ESI† for a similar figure augmented by the data used to make the figure. |
Optimal matching emerges also in the global minimum series of Al14 with charge states q = −1, 0, 1, 2. Analysing how GM structures and DoS (Fig. 1), as well as the shape factor S (Table 1), change with a varying number of electrons, the optimal match of 40 electrons allows for a more stable spherical arrangement of the 14 atoms.
The Al12Si cluster should be extremely stable according to all criteria. It has a nearly perfect spherical shape, because of its high symmetry multiple degenerate shells, that are completely filled, as well as a very high HOMO—LUMO gap and hardness. According to general belief, it should therefore not be reactive. However it turns out that this cluster reacts easily with a second identical cluster. It is therefore not possible to build a cluster assembled material based on this cluster.89 When two clusters are brought into contact during the assembly of such a material, they do not stay intact but form chemical bonds that destroy the 12 atom cage structure. A similar coalescence tendency was found for the Na8 cluster.90 For this magic cluster it was also shown that its spherical shape is destroyed upon deposition on a surface.
We analyzed the density of states of various clusters obtained from the global minimum of Al−113, that is the icosahedron, replacing its central atom with elements of the IV and V groups: Al−113, Al12 C, Al12 Si, Al12 Ge, Al12 Sn, Al12N+1, Al12P+1, Al12As+1, and Al12Sb+1. All of them hold the same magic number of valence electrons, that is 40, and, after their geometry optimization, the same icosahedron Ih symmetry of the Al−113 global minimum is displayed. The KS DFT eigenvalue degeneracies are identical for all icosahedrons, and their DoS maintains an identical shell structure with respect to the one of the Al−113 global minimum. For some icosahedrons the order of appearance for the KS eigenvalue degeneracies or the distances between groups of degenerate eigenvalues are slightly modified. For example, comparing the KS eigenvalue degeneracies [1, 3, 5, 1, 3, 3, 4] of Al−113 with the [1, 3, 1, 5, 3, 4, 3] ones of Al12 C, we can notice an inversion of the third and fourth degeneracy levels. Similar differences appear when we compare other icosahedra. For all the Al12 X icosahedra, with X being one of elements investigated, exchanging the X central atom with a surface atom breaks the cluster symmetry and, as a consequence, reduces the KS DFT eigenvalue degeneracies. The structure is still meta-stable but the energy is considerably higher. These pieces of evidence can only be accounted for by the optimal matching description, not by a structure-less jellium model.
For non-metallic clusters we could not find any tendency for spherical shapes. Hence jellium models are not applicable. As a matter of fact the stability of covalent clusters such as Si or Ge clusters was up to now nearly exclusively discussed in terms of certain structural motifs. Our approach of optimally matched clusters can however also be used in such cases and it can explain the in general strongly non-spherical ground state structures.
The bond lengths in metallic clusters are always considerably shorter than in the bulk metal. This is due to a flow of charge from the outside of the cluster to centers between neighboring atoms in the cluster. The effect is strongest for the low energy isomers.
In covalent clusters, the bond lengths are always longer than in the crystalline phase, since because of the directional bonding, it is not possible to accumulate charge exactly between each atom and all its nearest neighbors.
For all clusters the hardness and the energy difference between the first meta-stable structure and the ground state are good indicators for stability. In both cases large values indicate high stability. We have however no indications that a large hardness suppresses the chemical reactivity of clusters.
Our fingerprint-distance energy plots show that metallic clusters are structure seekers that can easily find their ground state by crossing only low barriers along a trajectory where they gain a significant amount of energy after each hop over a barrier. Experimentally they should therefore adopt their ground state with moderate annealing. This is however not true for covalent clusters. There the experimentally observed structure may not be the ground state but a structure that is kinetically more easily accessible.85
Footnote |
† Electronic supplementary information (ESI) available: The file supplementary-information.pdf reports two additional analyses concerning the redistribution of the electronic charge density for selected Na and Mg clusters together with various figures from the main publication augmented by the data used to make the figure plus selected structural and electronic properties. See DOI: https://doi.org/10.1039/d2ma01088g |
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