Abstract
We recently demonstrated that, in gas phase clusters containing aluminum and iodine atoms, an Al13 cluster behaves like a halogen atom, whereas an Al14 cluster exhibits properties analogous to an alkaline earth atom. These observations, together with our findings that Al13− is inert like a rare gas atom, have reinforced the idea that chosen clusters can exhibit chemical behaviors reminiscent of atoms in the periodic table, offering the exciting prospect of a new dimension of the periodic table formed by cluster elements, called superatoms. As the behavior of clusters can be controlled by size and composition, the superatoms offer the potential to create unique compounds with tailored properties. In this article, we provide evidence of an additional class of superatoms, namely Al7−, that exhibit multiple valences, like some of the elements in the periodic table, and hence have the potential to form stable compounds when combined with other atoms. These findings support the contention that there should be no limitation in finding clusters, which mimic virtually all members of the periodic table.
Keywords: 3d periodic table, cluster, jellium
The formation of materials with properties different from those of the constituent atoms is a known phenomenon in nature. For example, the formation of NaCl molecules/solid with characteristics different from its constituent elements, Na and Cl, is a classic example. One of the objectives of the research on superatoms (1–3) is to explore if one can carry out, what nature does, in a more facile and controlled manner. Developing an understanding of the factors governing the chemical behavior of clusters (4–10) and demonstrating that this knowledge can be used to design stable building blocks for new materials is critical for translating this concept into practice. For metal clusters, a simple electronic shell model called jellium (11) is routinely used to describe the global features of the electronic structure. In this model, the nuclei together with the innermost electrons form a positive-charged background, whereupon the valence electrons coming from individual atoms are then subjected to this potential. For pure metal clusters, within a spherical jellium background, this approach results in a shell structure where the electrons are arranged in electronic shells 1s2, 1p6, 1d10, 2s2, 1f14, 2p6 … compared with 1s2, 2s2, 2p6, 3s2, 3p6, 4s2, 3d10 … in individual atoms. Similar shell structure is also obtained for square well and harmonic forms of background potential (12), indicating that the shells derived within a jellium picture represent generic features of electronic states in a confined free electron gas. Clusters containing 2, 8, 18, 20, 34, 40 … electrons correspond to filled electronic shells and exhibit enhanced stability as seen via abundances in mass spectra of simple metal clusters, higher ionization potential, lower electron affinity, and chemical inertness seen in reactivity experiments. In this respect, an Al13 cluster with 39 valence electrons and an electronic structure of 1s2, 1p6, 1d10, 2s2, 1f14, 2p5 lacks a single electron as do halogen atoms, which, upon addition of a single electron, acquire a filled shell status (13). Indeed, previous studies (14, 15) have shown that Al13 has an electron affinity comparable to halogen atoms, indicating a chemical behavior reminiscent of halogen atoms. In a similar vein, we had recently shown that in cluster compounds with iodine, an Al14 cluster exhibits behavior analogous to alkaline earth atoms (3). We had shown that Al14I3− is a stable species and that its stability can be reconciled by considering Al14 in a + 2 valence state (3). The electronic shell structure, outlined above, does become modified (16) for compound clusters as the combination of atoms with different electronegativities can rearrange their geometry and influence the electronic shells. In particular, the shell closings at 18 and 20 are sensitive to the nature of the compound cluster.
Although the above developments bring out a close analogy between atoms and superatoms, one of the most important features characterizing atoms is that numerous elements in the periodic table exhibit multiple valence states. For example, carbon exhibits both divalent and tetravalent characteristics and, strongly binds with O or Si atoms forming CO and SiC, both of which are highly stable. Are there superatoms that share this commonality to atoms?
In this article we present the results of a synergistic effort that combines first-principles' theoretical calculations and the reactive stability of selected clusters to demonstrate an additional member of the superatom family, namely Al7−. What is truly remarkable is that unlike previous members, this superatom exhibits multiple valence states, enabling it to form stable compound clusters when combined with diverse atoms. In particular, we first demonstrate (8) the exceptional stability of Al7C− through the production of AlnC− clusters in reactions of aluminum clusters with benzene, and subsequent reactions of the clusters with oxygen to identify the stable species. The mass spectra show the Al7C− peak to be even more pronounced than Al13−, another member of the superatom family, which we have previously identified, and studied extensively (1–3). Theoretical considerations indicate that a superatom concept enables one to understand the electronic origin of the exceptional stability often observed for these species. The same considerations also predict stability of other species such as Al7O−, Al7S−, Al7I2−, and Al7+. Unlike Al7C−, however, the stability of Al7O−, Al7S−, and Al7I2− cannot be ascertained by O2 etching experiments. The Al7O− and Al7S− clusters are not stable toward the formation of AlO2− or Al2O2; Al7I2− is unstable toward the formation of Al2O2. Consequently, their stability has to be verified by a reactant less harsh than O2. Experimental mass spectra, however, do show the stability of Al7+ in oxygen-etching experiments. The present investigations provide further extensive support to the general nature of the superatom concept and show Al7− to be a member of the multivalent superatom family.
Results and Discussion
In brief, the clusters are produced by vaporizing a rotating and translating aluminum rod in a helium atmosphere. The production of mixed clusters is then accomplished by mixing the ablation species with a small percentage of the carrier gas containing the desired precursor. For example, AlnC− clusters are produced by adding benzene. To identify the stable species, the generated clusters are subsequently exposed to increasing amounts of etching gas introduced into the flow reactor in which the clusters are transported. In this way, the reactive anions are oxidized and often etched into smaller more stable fragments. The reacted species are mass-analyzed, thus spectra contain the stable species generated in the original mass distribution and the stable products generated in the oxidation and etching reactions. In this way, the peaks in the mass spectra of the reacted species identify the stable species.
Fig. 1 shows the mass spectra of AlnC− clusters obtained by reacting the aluminum plasma with benzene and subsequently exposing the generated AlnC− clusters to >200 standard cubic centimeters per minute of oxygen. Fig. 1 shows that Al7C− is the only cluster containing one C atom (at small sizes) that survives in the mass spectra. The peak at Al7C− is conspicuously large and even more prominent than Al13−, known to be resistant to oxygen because of its closed shell structure. It was suggested earlier (17) that the stability of Al7C− could be reconciled within a jellium model framework where the cluster could be looked upon as a compound jellium formed out of an Al6, with a closed shell of 18 electrons and AlC− with a closed shell of 8 electrons. Such a picture does have difficulties. The electron affinity of AlC (1.1 eV) is less than that of Al6 (2.5 eV). Our calculations show that, whereas it takes only 3.76 eV to remove an Al atom from Al7C−, it will take 9.09 eV to break it into Al6 and AlC−. The C atom in Al7C− is located inside the Al7 cage bonded to all of the Al sites, whereas one would expect it to bind to a single Al atom if it were a combination of Al6 and AlC−.
We begin by demonstrating that the true reason for the stability of Al7C− lies in the multiplet nature of Al7−. Fig. 2 shows the geometry deduced for Al7C−. Note that the cluster features an endohedral C atom as obtained in earlier studies. To examine the stability, we calculated the gain in energy, ΔE,
as a function of size as successive Al atoms are added to the preceding size Aln−1C−. Here E is the total energy of the cluster. The results are shown in Fig. 2b. A peak in ΔE is a signature of stability as it implies a larger gain in energy in forming the stable species from the preceding size and lower energy in breaking the higher size to form the stable species. Note that there is a peak at Al7C− indicating its preferred formation from the growth of Al6C− and from the fragmentation of Al8C−. Fig. 2b also shows the gap between the highest occupied molecular orbital (HOMO) and the lowest unoccupied molecular orbital (LUMO). In metallic clusters, the gap is generally indicative of stability and chemical inertness. Note that Al7C− has the highest HOMO–LUMO gap.
We now discuss the stability of Al7C− and other aluminum-based clusters toward etching by O2 more quantitatively. The possible fragmentation pathways involve the formation of AlO2, AlO2−, or Al2O2. Note that because the clusters are first thermalized, then exposed to molecular O2, the OO bond is protected by a barrier and remains intact in the formation of AlO2, AlO2−, or Al2O2. Our calculations show that the binding energy (BE) of AlO2 and AlO2− with OO bond intact is 2.83 and 5.72, eV respectively, whereas the energy required for breaking an Al2O2 into two Al atoms and an O2 molecule is 6.75 eV. These calculations show that those aluminum-based clusters, where it takes (i) <2.83 eV to remove a single Al, (ii) <5.72 eV to remove an Al−, or (iii) <6.75 eV to remove two Al atoms, will be energetically unstable toward etching by O2. In this way, the stability of clusters can be tested, as less stable clusters are oxidized and often etched into smaller more stable fragments. In the case of Al7C−, the removal of an Al atom requires 3.76 eV, and the removal of an Al− requires 6.40 eV, whereas the removal of two Al atoms requires 6.78 eV of energy. The corresponding studies based on the Naval Research Laboratory Molecular Orbital Library (NRLMOL) show that the energy required to remove two Al atoms is 7.04 eV, whereas the BE of Al2O2 toward breaking into two Al atoms and an O2 is 6.92 eV. Al7C− is therefore stable toward these fragmentation pathways and hence is not etched by O2. The same considerations also explain the observation of Al7+ in etching of the pure Aln+ cations by oxygen. In this case, whereas it takes 4.32 eV to remove an Al atom, it takes 7.22 eV to remove two Al atoms. Why is Al7C− so stable? Can Al7− combine with other atoms to create stable species?
To answer the above questions, we outline the mechanism by which the Al7− cluster combines with other atoms to form stable compounds. An Al atom has a valence electronic configuration of 3s2 3p1, and it has been proposed that Aln clusters undergo a transition (18) from monovalent to trivalent starting around n = 6. The trivalent character in Al7 is further established (19) by the mass spectra of the reacted Aln+ cations that exhibit a sharp peak at Al7+, indicative of a shell closing at 20 electrons within a jellium picture of the confined free electron gas. If instead, it was monovalent in character, it would display prominence as an eight-electron system, which it does not (13). An Al7−, on the other hand, has 22 valence electrons. Within the jellium picture, the cluster has an electronic configuration of 1s2, 1p6, 1d10, 2s2, 1f2, and Fig. 3 shows the one-electron levels in the free cluster. The molecular orbitals have been labeled by using the jellium classification (the levels roughly correspond to the overall shape of the molecular orbitals). A carbon atom has a valence structure of 2s2, 2p2 with four vacancies in the p-shell, and Fig. 3 shows the one-electron levels in carbon. To discuss the formation of Al7C−, let us start with the one-electron levels in Al7C− also shown in Fig. 3. The 2s filled state of carbon is far below the manifold of Al7− and becomes the 1s state of Al7C−. Consequently, the 1s and 2s states of pure Al7− become the 2s and 3s states of the combined system and are pushed up in energies (the resulting 3s is high in energy and is not shown). The partially filled p-states of carbon are around the same energy as 1p states of Al7− and form the bonding and antibonding combinations. The bonding combination leads to the 1p state of Al7C−, whereas the antibonding combination leads to the 2p state that characterizes the group of highest occupied molecular states in Al7C−. Because a carbon atom has four unfilled p-states, the occupation of the p-states can be looked on as the transition of four electrons from the 1f and the 2s states of Al7− to these unfilled states. The 1f unfilled states are pushed up in energy, and Fig. 3 shows the revised level structure in Al7C−. Note that the p-states of C form bonding orbitals with Al7− states; hence it is not a charge transfer but a population of these bonding states. A better description is the transition of Al7− toward a + 4 valence state, which is similar to the transition of Al14 toward a + 2 state reported previously (3). Obviously such a transition cannot be identified through Mulliken or other charge analysis, as recently undertaken by some authors (20). Fig. 2c shows the electron charge density in the HOMO orbital. As the bonding states are deep in energy, the occupation of bonding states stabilizes the cluster whereas the movement of unoccupied states opens a large HOMO–LUMO gap of 1.69 eV consistent with the stability and inertness of Al7C−. A similar model would also account for the previously known (21, 22) enhanced stability of neutral Al7N because Al7 has 21 electrons, and the N states can be filled by occupation of three bonding orbitals.
The key issue is whether such simple electronic counting rules and shell filling can be used to describe the stability of other members of the second row of the periodic table. Because the confined free electron gas exhibits shell closing at 18 and 20 electrons, the above arguments would suggest that Al7M− clusters should exhibit enhanced stability for cases where the M atom would require two or four electrons to fill the deep p-bonding orbitals. This criterion would indicate that Al7O− should also be quite stable, and Fig. 3 shows the levels in this cluster and an O atom (2s state of oxygen is deep in energy and is not shown). The bonding then proceeds as for Al7C−, with the only difference being that only 1f electrons of Al7− are transferred to bonding states between Al7− and O. To examine quantitatively the stability, we investigated the AlnO− clusters containing five to eight Al atoms and computed ΔE and the HOMO–LUMO gap (shown in Fig. 2 d and e). Note that ΔE peaks at Al7O−, indicating enhanced stability. Fig. 2f also shows the HOMO orbital. Although Al7O− is stable, it is not resistant to etching by O2 because it takes 6.10 eV to remove two Al atoms.
It is now interesting to inquire as to whether the above considerations could be extended to other elements. In particular, could one use the above model to understand the bonding of Al7− to other elements in the second, third, and fourth row of the periodic table. To this end, we have calculated the BE of all of the atoms in the second, third, and fourth rows with Al7− using the equation
Here E(Al7−), E(M), and E(Al7M−) are the total energies of the Al7−, M, and Al7M− species, respectively. For cases where M is a halogen atom, the BE was calculated by breaking into Al7 and M− fragments. In these calculations, the atoms were initially located at different positions around the Al7 motif. The geometry was optimized by moving atoms in the direction of forces until the forces dropped below a threshold value of 3 × 10−4 a.u. Several spin multiplicities were tried to locate the ground state. Three different types of geometries were obtained. For B, C, and N we obtain an endohedral structure (Fig. 2a). For Li, Be, O, F, Na, Mg, Al, P, S, Cl, Cu, Zn, Ga, Ge, As, Se, and Br we obtain an external geometry (Fig. 2d), and for Si we obtained a capped geometry where the Al7 opens up to accommodate the additional atom.
In Fig. 4a, we show the variation of BE for all of the anionic clusters. In each case, we have marked the total number of valence electrons. Note that Al7C− and Al7O− are not only stable with respect to addition of Al atoms, as discussed earlier, they also have the highest BE across the entire second row of the periodic table. What is quite amazing is that the same trend continues for the anions of the third-row and fourth-row elements. S in the third row and Se in the fourth row exhibit larger gain in BE than previous sizes, again indicative of their stability. In addition to the BE, we examined the variation of the HOMO–LUMO gap (Fig. 4b). Significantly, the HOMO–LUMO gap follows the stability trend, indicating a chemical inertness. For Si and Ge that correspond to a shell filling at 18, the BE only exhibits a shoulder whereas the HOMO–LUMO gap exhibit minor peaks. This behavior could be caused by the highly directional nature of the bonds from these atoms. To further confirm this extensive nature of the multivalence concept and reiterate the theoretical picture, AlnS− clusters were generated by reacting Aln clusters with SO2. The mass spectra of the resulting clusters contained Al7S− clusters, including other sulfur-containing clusters as well. When the clusters were exposed to O2, however, all of the clusters, including Al7S−, were etched away. The etching of Al7S− is understandable, noting that the energy required to remove two Al atoms is only 5.78 eV whereas energy gain in forming Al2O2 is 6.75 eV. Further, it will take 5.73 eV to remove an Al− atom, making the formation for AlO2− a resonant reaction. The corresponding studies based on the NRLMOL, however, indicate that it will take 5.68 eV to remove an Al− atom, whereas the gain in energy in forming AlO2− is 6.07 eV, opening this channel for fragmentation. In either case, Al7S− is unstable toward oxidation. We further calculated the electron affinity of the Al7M− clusters for M covering all of the third-row and fourth-row atoms. Al7S− and Al7Se− had the highest electron affinity, attesting to their closed electronic shell character.
A critical test of the multiple valence would be to combine Al7− with atoms that have only one vacancy in the p-level (3) and a high electron affinity. The formation of the bonding states would then remove one electron at a time whereupon the effect of the 2f and 2s depopulation could be mapped out with the number of atoms. To carry out this important test, we considered anionic Al7Im− clusters. An I atom has an electron affinity of 3.06 eV that is considerably higher than the measured electron affinity (15) of 2.43 for Al7. One would therefore expect each additional I atom to combine with one electron from the Al7 core. In Fig. 4c we show the variation of the BE and HOMO–LUMO gap as successive I atoms are added to the cluster. Note that Al7I2− leading to a core of 20 electrons is particularly prominent compared with other sizes, again verifying the shell closures discussed above. More importantly, the corresponding HOMO–LUMO gap shows the same trend. The chemical features together with the BE again point to the valence status. To examine whether the stability of Al7I2− is borne out by experiments, the aluminum clusters anions were reacted with iodine gas. Fig. 5 shows the mass spectra of the bare and reacted species. Note that the mass spectra indeed exhibits a peak at Al7I2−, confirming the theoretical prediction. We note that the variations in BE and HOMO–LUMO gap in Fig. 4c indicate Al7I4− to be more stable than neighboring sizes, consistent with a shell closure at 18 electrons; however, it is not seen in Fig. 5. The reason is that it is energetically unstable toward the reaction
by 0.31 eV. Although Al7I− and Al7I3− are less stable than Al7I4−, as discussed in a previous paper (23), their observation is linked to the enhanced stability of the corresponding neutral species. Al7I2− is, however, unstable toward etching by O2 as it takes 6.76 eV to remove two Al atoms, making the formation of Al2O2 a resonant reaction. Corresponding studies based on the NRLMOL indicate the formation of Al2O2 to be exothermic by 0.03 eV.
To summarize, we have demonstrated that bonding patterns of Al7− can be understood by regarding it as a superatom that exhibits multiple valence. The valence of 2 and 4 would make it analogous to C or Si. The stability of Al7C− on the one hand and that predicted for Al7O− and Al7S− on the other hand could then be correlated with the stability of SiC and CO, respectively. In the past we have shown that Al13 and Al14 could be regarded as superhalogen and alkaline earth superatoms. Importantly, unlike Al13− and Al14, Al7− exhibits multiple valence, thus adding an additional dimension to the chemistry of superatoms.
Materials/Methods
Experimental Methods.
Al7C− species were created by ablating an aluminum rod in a flow of 8,000 standard cubic centimeters per minute of high-purity helium. Benzene vapor was added restrictively to the source to maximize the population of AlnC− species. The clusters and helium carrier gas merged into a laminar flow regime where they became thermalized. The clusters were then reacted with molecular oxygen, and products were extracted, mass-analyzed by a quadrupole mass filter, and detected by a channel electron multiplier. The Al7I2− species were created by ablating an aluminum rod in a flow of 8,000 standard cubic centimeters per minute of high-purity helium. Molecular iodine was added externally to the source by flowing a small amount of helium through a sublimation cell containing molecular iodine.
Theoretical Methods.
The theoretical studies were carried out by using first-principles electronic structure calculations performed within a density functional formalism (24) that incorporates exchange and correlation using the generalized gradient approximation functional proposed by Perdew, Burke, and Ernzerhof (25). In particular, Gaussian basis sets were used to construct the atomic wave function, whereas the cluster wave function was formed from a linear combination of atomic orbitals. All calculations were performed with deMon2k software (26). Here, an auxiliary basis set was used for the variational fitting of the Coulomb potential (27, 28). The numerical integration of the exchange-correlation energy and potential were performed on an adaptive grid (29). The minimum structures were fully optimized in delocalized internal coordinates without constraints using the rational function optimization method and the Broyden, Fletcher, Goldfarb, and Shanno update (30). The double zeta valence polarized and the GEN-A2 auxiliary basis sets were used (31). To eliminate any uncertainty from the basis set or the numerical procedure, in selected cases we carried out supplementary calculations by using the NRLMOL developed by Pederson and coworkers (32–34) using the same density functional. For details, see refs. 3 and 32–34.
Acknowledgments
This work was supported by U.S. Air Force Office of Scientific Research Grant F49620-01-1-0328 (to A.W.C. and P.J.R.) for the experimental work on Al7C− and Al7In−, U.S. Air Force Office of Scientific Research Grant FA9550-05-1-0186 (to J.U.R. and S.N.K.) for the theoretical work on these systems, and U.S. Department of Energy Grant DE-FG02-02ER46009 for the systematic studies on Al7X− clusters for X covering the second, third, and fourth rows of the periodic table. S.N.K. thanks Virginia Commonwealth University for providing a study/research leave.
Abbreviations
- HOMO
highest occupied molecular orbital
- LUMO
lowest unoccupied molecular orbital
- BE
binding energy
- NRLMOL
Naval Research Laboratory Molecular Orbital Library.
Footnotes
The authors declare no conflict of interest.
References
- 1.Khanna SN, Jena P. Phys Rev Lett. 1992;69:1664–1667. doi: 10.1103/PhysRevLett.69.1664. [DOI] [PubMed] [Google Scholar]
- 2.Bergeron DE, Castleman AW, Jr, Morisato T, Khanna SN. Science. 2004;304:84–87. doi: 10.1126/science.1093902. [DOI] [PubMed] [Google Scholar]
- 3.Bergeron DE, Roach PJ, Castleman AW, Jr, Jones NO, Khanna SN. Science. 2005;307:231–235. doi: 10.1126/science.1105820. [DOI] [PubMed] [Google Scholar]
- 4.Zhao J, Xie R-H. Phys Rev B. 2003;68:035401-1–035401-5. [Google Scholar]
- 5.Zheng W, Nilles JM, Radisic D, Bowen KH. J Chem Phys. 2005;122:071101-1–071101-4. doi: 10.1063/1.1851984. [DOI] [PubMed] [Google Scholar]
- 6.Baruah T, Pederson MR, Zope RR, Beltran MR. Chem Phys Lett. 2004;387:476–480. [Google Scholar]
- 7.Kumar V, Kawazoe Y. Appl Phys Lett. 2003;80:859–861. [Google Scholar]
- 8.Ashman C, Khanna SN, Pederson MR, Kortus J. Phys Rev B. 2000;62:16956–16961. [Google Scholar]
- 9.Rao BK, Khanna SN, Jena P. J Cluster Sci. 1999;10:477–491. [Google Scholar]
- 10.Thomas OC, Zheng WJ, Bowen KH. J Chem Phys. 2001;114:5514–5519. [Google Scholar]
- 11.Knight WD, Clemenger K, de Heer WA, Saunders WA, Chou MY, Cohen ML. Phys Rev Lett. 1984;52:2141–2143. [Google Scholar]
- 12.de Heer WA, Knight WD, Chou MY, Cohen ML. Solid State Phys. 1987;40:93–181. [Google Scholar]
- 13.Leuchtner RE, Harms AC, Castleman AW., Jr J Chem Phys. 1989;91:2753–2754. [Google Scholar]
- 14.Pederson MR. In: Physics and Chemistry of Finite Systems: From Clusters to Crystals. Jena P, Khanna SN, Rao BK, editors. Vol II. Dordrecht, The Netherlands: Kluwer; 1992. pp. 861–866. [Google Scholar]
- 15.Li X, Wu H, Wang X-B, Wang L-S. Phys Rev Lett. 1998;81:1909–1912. [Google Scholar]
- 16.Janssens E, Neukermans S, Lievens P. Curr Opin Solid State Mater Sci. 2004;8:185–193. [Google Scholar]
- 17.Leskiw BD, Castleman AW., Jr Chem Phys Lett. 2000;316:31–36. [Google Scholar]
- 18.Rao BK, Jena P. J Chem Phys. 1999;111:1890–1904. [Google Scholar]
- 19.Leuchtner RE, Harms AC, Castleman AW., Jr J Chem Phys. 1991;94:1093–1101. [Google Scholar]
- 20.Han Y-K, Jung J. J Chem Phys. 2006;125:084101-1–084101-8. doi: 10.1063/1.2236114. [DOI] [PubMed] [Google Scholar]
- 21.Leskiw BD, Castleman AW, Jr, Ashman C, Khanna SN. J Chem Phys. 2001;114:1165–1169. [Google Scholar]
- 22.Guo L, Wu H-S. Int J Quant Chem. 2006;106:1250–1257. [Google Scholar]
- 23.Bergeron DE, Roach PJ, Castleman AW, Jr, Jones NO, Reveles JU, Khanna SN. J Am Chem Soc. 2005;127:16048–16053. doi: 10.1021/ja050338z. [DOI] [PubMed] [Google Scholar]
- 24.Kohn W, Sham LS. Phys Rev. 1965;140:A1133–A1138. [Google Scholar]
- 25.Perdew JP, Burke K, Ernzerhof M. Phys Rev Lett. 1996;77:3865–3868. doi: 10.1103/PhysRevLett.77.3865. [DOI] [PubMed] [Google Scholar]
- 26.Köster AM, Calaminici P, Casida M, Flores-Moreno R, Geudtner G, Goursot A, Heine T, Ipatov A, Janetzko F, Patchkovskii S, et al. deMon2k, version 1.8. Cinvestan, Mexico: The International deMon Developers Community; 2005. [Google Scholar]
- 27.Dunlap BI, Connolly JWD, Sabin JR. J Chem Phys. 1979;71:4993–4999. [Google Scholar]
- 28.Mintmire JW, Dunlap BI. Phys Rev A. 1982;25:88–95. [Google Scholar]
- 29.Köster AM, Flores-Moreno R, Reveles JU. J Chem Phys. 2004;121:681–690. doi: 10.1063/1.1759323. [DOI] [PubMed] [Google Scholar]
- 30.Reveles JU, Köster AM. J Comp Chem. 2004;25:1109–1116. doi: 10.1002/jcc.20034. [DOI] [PubMed] [Google Scholar]
- 31.Godbout N, Salahub DR, Andzelm J, Wimmer E. Can J Chem. 1992;70:560–571. [Google Scholar]
- 32.Pederson MR, Jackson KA. Phys Rev B. 1990;41:7453–7461. doi: 10.1103/physrevb.41.7453. [DOI] [PubMed] [Google Scholar]
- 33.Jackson KA, Pederson MR. Phys Rev B. 1990;42:3276–3281. doi: 10.1103/physrevb.42.3276. [DOI] [PubMed] [Google Scholar]
- 34.Porezag DV, Pederson MR. Phys Rev A. 1999;60:2840–2847. [Google Scholar]