Open Access Article
Mariusz
Michalczyk
*a,
Steve
Scheiner
b and
Wiktor
Zierkiewicz
a
aFaculty of Chemistry, Wrocław University of Science and Technology, Wybrzeże Wyspiańskiego 27, 50-370 Wrocław, Poland. E-mail: mariusz.michalczyk@pwr.edu.pl
bDepartment of Chemistry and Biochemistry, Utah State University Logan, Utah 84322-0300, USA
First published on 21st October 2025
The apex C atom of square pyramidane C(C4H4) is replaced by heavier tetrel T atoms Si, Ge, Sn, and Pb. The molecular electrostatic potential surrounding the substituted T-pyramidane features minima at both the apex and the square base. Quantum chemical calculations are conducted to examine the ability of these two sites to act as electron donors in H-bonds, halogen bonds, or osme bonds to group 8 metals Fe, Ru, and Os. Osme bonds are strongest, with some approaching 40 kcal mol−1, with a heavy covalent contribution, followed by halogen and then by hydrogen bonding. The latter are fairly weak, with interaction energies between 0.6 and 3.3 kcal mol−1. The apex T site is favored over the square base for osme bonds, but the base is preferred for H-bonds. There is a more delicate balance for halogen bonds, with Si preferred over the pyramid base, but the latter favored for Sn. The primary electron donor site at the apex is a pseudo-lone pair on T, while the π-electron system serves this function when the electrophile attacks the base of the pyramid.
Interest in the pyramidal T(C4R4) structure, where T = Si, Ge, Sn, Pb, has become the subject of experimental research.9–11 The following compounds have been synthetized: Si[C4(SiMe3)4]9 Ge[C4(SiMe3)4],11 Sn[C4(SiMe3)4],11 and
,10 where T = Ge, Sn, Pb, T′ = C, Si, Ge, and R = Me, MetBu2. Along with this work, there have been a number of theoretical predictions2,4,7,12–15 of their properties. Imagawa et al. synthesized several silapyramidanes, where Fe(CO)4 interacted directly with an apical Si atom.11 Borapyramidanes were synthesized by the Erker16 group in 2022. Pendas et al. carried out theoretical studies on the electronic structure2 of T[C4(SiMe3)4] pyramidanes, in which the apical T center was a tetrel atom, varying from C to Pb. Their analysis suggested that the interactions between apical and basal atoms changed from covalent to electrostatically driven as the tetrel atom size increased, with the exception of T = Si. Previous computational studies extended beyond isolated pyramidanes. For example, Veljkovic et al.14 scrutinized the interactions between pyramidanes and water molecules. The molecular electrostatic potential (MEP) in the vicinity of the apex C atom was found to be negative (ranging from −49 to −8 kcal mol−1) for a set of pyramidanes, depending on the substituents on the base C atoms. Such pyramidanes could thus behave as nucleophiles, interacting directly with H atoms of water. The study found strong O–H⋯C hydrogen bonds characterized by interaction energies reaching as high as −7.4 kcal mol−1.14 Decomposition of the interaction energy indicated the primary electrostatic character of these contacts.
A very recent computational work considered pyramidane in the context of other highly strained C atoms, and comparison was drawn with a set of propellanes.15 The carbon atom at the apex served as an electron donor to a variety of different noncovalent bonds, including hydrogen, halogen, chalcogen, pnicogen and tetrel bonds, by taking advantage of the σ-holes17,18 on the various electrophiles with which they were paired. Of the systems considered, the Sn⋯C tetrel bonds were strongest, up to 56 kcal mol−1, bordering on a covalent bond. To be sure, the concentration of electron density at carbon atoms has been observed in several contexts. What is particularly notable is the ability of the strained C of propellanes and pyramidanes to serve as an electron donor despite the absence of a formal lone pair. This participation is aided by the presence of what might be thought of as a pseudo-lone pair orbital on this center.10,15 It would thus appear that the electrostatic potential and electronic structure of the highly strained C of pyramidanes place it in the pantheon of electron sources for σ-hole bonds, joining the already established club of lone pairs and π- and σ-bonds.
The present work involves high-level calculations to better understand the origin of the curious interactions between pyramidanes and selected Lewis acids. In order to broaden the dataset which has largely concentrated on the C atom at the apex of the pyramid in the past, this C was replaced in turn by each of the larger tetrel T atoms (Si, Ge, Sn and Pb), which thus covers a wide range of atomic size and electronegativity, and response to bond strain. The type of bonding was also broadened by considering a set of nine different Lewis acids covering hydrogen, halogen, and osme bonding to group 8 metals Fe, Ru, and Os, one of the newly established types of noncovalent bonds.19–22 The choice of the latter was motivated by the observation of a pyramidane crystalline solid with an Fe(CO)4 group, which is stabilized by an Fe⋯Si osme bond.11 To further broaden the types of interactions that pyramidanes are capable of forming, the calculations presented here suggest the possibility that an approaching electrophile can interact not with the apex, but rather with the base of the pyramid. The comparison of the bonding to these two very different sites on these pyramids provides additional insights into the bonding capabilities of tetrel atoms, and also concerning intermolecular interactions in a more general sense.
| Monomer | R(C–C) | R(C–T) | h | V s,min(T) | V s,min(base) | I s,min(T) | I s,min(base) | q(T) |
|---|---|---|---|---|---|---|---|---|
| Si(C4H4) | 1.451 | 2.027 | 1.748 | −9.4 | −14.1 | 8.88 | 10.50 | 0.252 |
| Ge(C4H4) | 1.453 | 2.135 | 1.872 | −4.7 | −13.4 | 8.93 | 10.44 | 0.315 |
| Sn(C4H4) | 1.455 | 2.335 | 2.097 | +3.2 | −17.4 | 8.24 | 9.95 | 0.507 |
| Pb(C4H4) | 1.454 | 2.432 | 2.204 | +18.3 | −21.5 | 7.80 | 9.57 | 0.565 |
The overall MEP values surrounding the pyramidanes are shown in Fig. 1 for the Si and Pb variants. Each contains a minimum directly above the T atom, but this minimum is not necessarily negative in sign. As listed in the fourth column of Table 1, Vs,min on the 0.001 a.u. isodensity surface varies from a negative −9.4 kcal mol−1 for Si up to +18.3 kcal mol−1 for the more electropositive Pb. It is worth noting that there is another minimum at the base of each pyramid, which is more negative than that near T, as is clear from the next column of Table 1. As another perspective on this point, the ALIE (average local ionization energy) was computed as well. The results in Table 1 indicate that this quantity is smaller at the site of the apical tetrel atom than at the pyramid base. From this point of view, the former would be preferred over the latter as a site for electrophilic attack.
As another measure of the charge distribution, the last column of Table 1 displays the atomic polar tensor (APT) charges assigned to T. This charge is positive for all T, but becomes more so as the atom grows in size, consistent with the same trend in Vs,min(T). A similar pattern of more positive MEP for heavier T was reported earlier2 for the SiMe3 tetrasubstituted pyramidanes. For purposes of comparison, the MEP minimum near the apical C in C(C4H4) was computed earlier15 to be much more negative at −42.3 kcal mol−1, consistent with carbon's higher electronegativity. This highly negative potential on the apical C persists as substituents are added to the basal C atoms.14
Another perspective on the electron density distribution of each pyramidane entity is derived from ELF analysis. The ELF basins are presented in Fig. 2 for an isovalue of 0.85 a.u. These basins can be divided into monosynaptic, V(T) (a T lone pair), and disynaptic, V(C,C) or V(C,H), as labelled in Fig. 2.
![]() | ||
| Fig. 2 ELF diagrams of pyramidanes with ELF basins indicated by pink globular shapes at an isovalue of 0.85 a.u. | ||
Of particular interest are the lone pair V(T) basins that progressively weaken in the Si < Ge < Sn order, vanishing entirely for Pb at this particular isovalue. Average population numbers in V(T) basins are 2.74e (Si), 2.86e (Ge), 2.68e (Sn) and 2.76e (Pb), nearly the same for all tetrel atoms despite the different sizes of these basins. NBO localization of the wavefunction of each monomer leads to the appearance of an orbital that closely resembles a lone pair on each tetrel atom, as is clear from Fig. S1. This orbital is primarily of s character, roughly 90%. Consistent with the near equality of the ELF populations, the NBO lone pairs are similar in appearance for all T. While ELF designates these areas as encompassing high electron localization, NBO formalism refers to the localized orbital here as a lone pair. In either scenario, these electrons are available for bonding with an electrophile.
Three different types of Lewis acids were tested as partners for these pyramidanes. The HX series, with X = F, Cl, Br, were examined as proton donors in H-bonds to the apical T atom. Another type of interaction examined was halogen bonds via the FX series, where it is the σ-hole on the X center that might interact with T. A third category allows the pyramidane T to interact with the central M atom of M(CO)4 for the group 8 metals Fe, Ru, and Os in what might be classified as an osme bond. The values of Vs,max on these various electrophiles are provided in Table S1. As expected, the value on the H of HX becomes less positive with larger X, while the opposite is true for the X center of FX. The MEP on the central M atom of M(CO)4 is rather uniform for all three M, between 16.3 and 18.4 kcal mol−1.
| Si(C4H4) | Ge(C4H4) | Sn(C4H4) | |||||||
|---|---|---|---|---|---|---|---|---|---|
| R | θ | α | R | θ | α | R | θ | α | |
| a In osme bonded dimers, there are two variants of angle θ: θ1/θ2; see Fig. 3. | |||||||||
| HF | 2.524 | 179.6 | 179.0 | 2.599 | 179.7 | 178.9 | 2.770 | 180.0 | 179.0 |
| HCl | 2.719 | 179.2 | 178.9 | 2.797 | 180.0 | 178.3 | 2.984 | 176.7 | 178.2 |
| HBr | 2.742 | 177.3 | 177.5 | 2.833 | 175.9 | 177.8 | 3.020 | 172.5 | 172.6 |
| FCl | 2.390 | 179.9 | 179.9 | 3.054 | 180.0 | 179.9 | 3.212 | 179.9 | 179.8 |
| FBr | 2.488 | 180.0 | 180.0 | 2.830 | 179.8 | 179.9 | 3.152 | 179.7 | 179.9 |
| FI | 2.686 | 179.9 | 179.9 | 2.905 | 179.1 | 173.0 | 3.042 | 179.0 | 139.5 |
| Fe(CO)4 | 2.202 | 88.6/116.7a | 179.9 | 2.396 | 89.1/118.3a | 176.8 | 2.574 | 89.2/117.5a | 150.2 |
| Ru(CO)4 | 2.287 | 92.2/111.3a | 179.9 | 2.490 | 93.8/112.2a | 179.1 | 2.692 | 89.6/113.0a | 133.4 |
| Os(CO)4 | 2.294 | 100.8/101.7a | 179.9 | 2.448 | 93.8/111.3a | 176.7 | 2.614 | 91.5/113.7a | 144.7 |
Both the HBs and XBs are very close to linear with θ and α values close to 180°. The one exception occurs for the FI··Sn XB, where α is only 140°. The Fe and Ru osme bonds are also linear with α values close to 180° with the exception of Sn. The complexes involving the osme bonds are based on a trigonal pyramidal shape around the metal center, with the pyramidane occupying an equatorial site. θ1 refers to the angle made with one of the two axial C atoms, so it is close to 90° (89°–101°), whereas those involving the two equatorial C atoms are designated as θ2, which is about 113°. Not unexpectedly, the intermolecular distances R grow with the size of the T atom in the order of Si < Ge < Sn. The same is generally true for the XB complexes and the size of X, with the exception of Sn, where this distance contracts from Cl to I. There is little sensitivity of the osme bonds to the identity of the M atom.
The M062X interaction energies are collected in Table 3, along with the same quantity calculated at the higher CCSD(T) level.
| Si(C4H4) | Ge(C4H4) | Sn(C4H4) | ||||
|---|---|---|---|---|---|---|
| M062X | CCSD(T) | M062X | CCSD(T) | M062X | CCSD(T) | |
| HF | −3.33 | −2.93 | −2.37 | −1.86 | −1.39 | −0.50 |
| HCl | −1.93 | −1.97 | −1.34 | −1.34 | −0.68 | −0.53 |
| HBr | −1.73 | −1.86 | −1.18 | −1.31 | −0.61 | −0.61 |
| FCl | −10.13 | −5.83 | −3.36 | −1.67 | −2.72 | −0.69 |
| FBr | −13.91 | −10.03 | −5.98 | −3.95 | −4.50 | −2.18 |
| FI | −14.28 | −11.59 | −8.29 | −6.15 | −8.32 | −5.44 |
| Fe(CO)4 | −30.16 | −39.84 | −20.85 | −28.30 | −20.10 | −26.12 |
| Ru(CO)4 | −29.41 | −34.62 | −18.21 | −23.63 | −17.60 | −22.29 |
| Os(CO)4 | −38.04 | −39.66 | −25.02 | −28.00 | −27.08 | −29.49 |
The latter reproduces the trends of the former, although there are some quantitative differences. CCSD(T) halogen bond energies are a bit smaller than those of M062X but follow the same trend. The same is true for the osme bonds, except that here the CCSD(T) values are systematically slightly larger in magnitude. At either level of theory, the osme bonds are rather strong, in the range between 18 and 40 kcal mol−1. Os engages in the strongest of these, with Ru and Fe being comparable to one another. With respect to the pyramidanes, Si is the most potent electron donor. XBs are substantially weaker and HBs are weaker still, 3 kcal mol−1 or less. The XB pattern follows along with σ-hole depth on the electrophile: I > Br > Cl, and with Vs,min on T: Si > Ge > Sn. As a parenthetical comment, it may be noted that Sn engages in all three types of bonds, despite its positive Vs,min.
AIM analysis of the electron density within the complexes reveals a bond path between the apical T and the atom of the Lewis acid with which it interacts directly (H, X, or M), as illustrated in the molecular diagrams in Fig. S1. The three most important parameters of this bond path are associated with the bond critical point: density ρ, potential energy density V, and total energy density H, all of which pertain to bond strength and type, and are compiled in Table 4.
| Si(C4H4) | Ge(C4H4) | Sn(C4H4) | |||||||
|---|---|---|---|---|---|---|---|---|---|
| ρ | V | H | ρ | V | H | ρ | V | H | |
| HF | 0.015 | −0.008 | −0.001 | 0.013 | −0.006 | 0.000 | 0.011 | −0.005 | 0.000 |
| HCl | 0.011 | −0.005 | 0.000 | 0.010 | −0.004 | 0.001 | 0.008 | −0.003 | 0.001 |
| HBr | 0.011 | −0.005 | 0.000 | 0.009 | −0.004 | 0.001 | 0.008 | −0.003 | 0.001 |
| FCl | 0.066 | −0.047 | −0.022 | 0.018 | −0.010 | 0.001 | 0.016 | −0.008 | 0.001 |
| FBr | 0.064 | −0.045 | −0.020 | 0.034 | −0.021 | −0.004 | 0.022 | −0.012 | −0.001 |
| FI | 0.053 | −0.037 | −0.014 | 0.036 | −0.023 | −0.006 | 0.034 | −0.020 | −0.005 |
| Fe(CO)4 | 0.081 | −0.086 | −0.039 | 0.058 | −0.063 | −0.019 | 0.050 | −0.050 | −0.013 |
| Ru(CO)4 | 0.089 | −0.093 | −0.050 | 0.067 | −0.067 | −0.024 | 0.055 | −0.049 | −0.015 |
| Os(CO)4 | 0.096 | −0.104 | −0.060 | 0.080 | −0.082 | −0.034 | 0.070 | −0.068 | −0.024 |
Similar to the interaction energies, ρ is smallest for the HBs (0.008–0.015 a.u.), larger for the XBs (0.016–0.066 a.u.) and highest for the osme bonds (0.050–0.096 a.u.). The higher end of this spectrum approaches the 0.1 a.u. arbitrary border into covalency.40 These patterns in ρ also bear some resemblance to the energetic ordering from Si to Ge and Sn. In fact, the correlation coefficient R2 for a linear fit between these two quantities is 0.91. Similar patterns are observed for V, but of course with a different range of values. The correlation with Eint is even better for V with R2 = 0.96. A negative value of H is commonly taken as a sign that the interaction contains a significant degree of covalency. With the exception of the HBs in the upper segment of Table 4, H is mostly negative, particularly so for the osme bonds.
A decomposition of the interaction energy into several physically meaningful components provides further perspective on the nature of the bonding. The results of ALMO-EDA decomposition of the interaction energies are displayed in Table 5.
| Si(C4H4) | Ge(C4H4) | Sn(C4H4) | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| ES | POL | CT | DISP | ES | POL | CT | DISP | ES | POL | CT | DISP | |
| HF | 53 | 14 | 19 | 15 | 51 | 16 | 17 | 15 | 16 | 28 | 29 | 27 |
| HCl | 53 | 9 | 21 | 17 | 52 | 10 | 20 | 18 | 19 | 17 | 31 | 34 |
| HBr | 52 | 8 | 23 | 17 | 52 | 9 | 21 | 19 | 20 | 14 | 33 | 33 |
| FCl | 24 | 12 | 55 | 9 | 44 | 6 | 32 | 18 | 32 | 7 | 35 | 25 |
| FBr | 25 | 19 | 48 | 8 | 38 | 10 | 40 | 13 | 35 | 10 | 35 | 20 |
| FI | 43 | 17 | 29 | 11 | 42 | 12 | 32 | 14 | 39 | 12 | 34 | 15 |
| Fe(CO)4 | 44 | 18 | 30 | 8 | 51 | 16 | 24 | 9 | 58 | 13 | 19 | 11 |
| Ru(CO)4 | 58 | 12 | 24 | 6 | 60 | 9 | 24 | 7 | 57 | 10 | 23 | 9 |
| Os(CO)4 | 48 | 26 | 22 | 4 | 50 | 20 | 25 | 5 | 49 | 21 | 24 | 5 |
The entries refer to the percent contribution of each of the four attractive elements, electrostatic (ES), polarization (POL), charge transfer (CT) and dispersion (DISP), to the total of all four. Focusing first on the HB complexes, those involving Si and Ge show roughly 50% contribution from ES that is typical of HBs in general. But ES is way down, less than 20%, for the Sn complexes, where all three of the other attractive elements have increased to make up the difference. The patterns are internally consistent within the osme bonds. ES accounts for roughly half, DISP is quite small on the order of 10%, and POL and CT make up the remainder in roughly equal amounts, although the latter tends to be a bit larger than the former. The XB data are rather interesting. ES tends to be largest for Ge as compared to Si or Sn. CT is quite substantial as well, comparable to ES and exceeding it in some cases. DISP is generally small; however, it does increase a bit for the Sn XB dyads. Polarization energy makes up the smallest percentage in most cases.
NBO localization of the MOs participating in these interactions provides a framework by which to consider the fundamental aspects of the bonding. Fig. 4 depicts the orbitals directly involved in the intermolecular bonding of Sn(CH)4 as an example pyramidane. The Sn pseudo-lone pair is obvious for the HB and XB in Fig. 4(a) and (b), which donates a certain amount of charge to the σ* antibonding orbitals in HF and ClF as prototypical HB and XB, as indicated by the curved red arrow. The osme bonding with Ru(CO)4 is strong enough that NBO analyzes the density as containing a single entity, with the Ru–Sn bond shown in Fig. 4(c).
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| Fig. 4 Natural bond orbitals primarily responsible for the intermolecular bonding of Sn(CH)4 with (a) HF, (b) ClF, and (c) Ru(CO)4. Red arrows indicate the direction of electron flow. | ||
Another window into the nature of the bonding arises in connection with monitoring the way in which the electron density shifts when the two monomers approach so as to form the dyad. These maps were generated by subtracting the density of the two isolated monomers from that of the entire complex, and are displayed in Fig. 5 for several of these systems.
The green and red colors, respectively, signify areas of density accumulation and depletion resulting from the interaction. In each case, there is an extensive green region between the two subunits where the buildup of density helps to cement the two units together. A good deal of this extra density is extracted from the apical T atom, as indicated by the prominent red region encircling it. The polarizations occurring within the Lewis acid units are evident from the pattern of green and red lobes within each.
As in most complexation processes, the two monomers each undergo certain structural changes to accommodate their partner. The first column of Table 6 shows that there is a small stretch of the bonds between the four basal C atoms.
| Si(C4H4) | Ge(C4H4) | Sn(C4H4) | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Δr(C–C) | Δr(C–T) | ΔqT | CT | Δr(C–C) | Δr(C–T) | ΔqT | CT | Δr(C–C) | Δr(C–T) | ΔqT | CT | |
| a Average value. | ||||||||||||
| HF | +0.002 | −0.015 | −0.040 | 0.02 | +0.002 | −0.017 | −0.044 | 0.01 | +0.001 | −0.016 | −0.036 | 0.01 |
| HCl | +0.001 | −0.010 | −0.018 | 0.02 | +0.001 | −0.010 | −0.027 | 0.01 | +0.001 | −0.012 | −0.019 | 0.01 |
| HBr | +0.001 | −0.009 | −0.008 | 0.03 | +0.001 | −0.010 | −0.021 | 0.02 | +0.002 | −0.012 | −0.013 | 0.01 |
| FCl | +0.006 | −0.037 | 0.256 | 0.34 | +0.001 | −0.015 | 0.006 | 0.05 | +0.002 | −0.015 | 0.021 | 0.05 |
| FBr | +0.007 | −0.042 | 0.233 | 0.32 | +0.004 | −0.028 | 0.075 | 0.14 | +0.003 | −0.025 | 0.051 | 0.09 |
| FI | +0.007 | −0.041 | 0.158 | 0.25 | +0.009 | −0.043 | 0.062 | 0.15 | +0.011a | −0.012a | 0.102 | 0.20 |
| Fe(CO)4 | +0.006 | −0.039 | 0.649 | 0.66 | +0.011 | −0.044 | 0.473 | 0.51 | +0.006a | −0.006a | 0.529 | 0.55 |
| Ru(CO)4 | +0.004 | −0.036 | 0.634 | 0.65 | +0.005 | −0.035 | 0.447 | 0.49 | +0.015a | +0.005a | 0.459 | 0.52 |
| Os(CO)4 | +0.007 | −0.042 | 0.561 | 0.58 | +0.002 | −0.043 | 0.458 | 0.50 | +0.016a | +0.013a | 0.563 | 0.59 |
This stretch is minimal for the HBs but increases to as much as 0.016 Å for the osme-bonded dimers. Concomitant with the expansion of the base is a flattening of the pyramid as the four C–T bonds to the apical T contract by as much as 0.04 Å. The exceptions include the Sn-osme bonds to Ru and Os, where there is a small elongation. If one were to consider bond length changes as a barometer of bond strength, the three types of noncovalent bonds slightly weaken the C–C bonds within the square base, while strengthening the C–T bonds to the apex of the pyramid by a larger amount. The geometric changes caused by complexation raise the energy of each monomer relative to its fully optimized structure. This sum of deformation energies of the two subunits is collected in Table S2, where it can be seen to be fairly small in most cases, with the exception of the osme-bonded dimers, where Edef can exceed 8 kcal mol−1. When Edef is subtracted from the interaction energy, one has the binding energy Eb equal to the reaction energy from optimized monomers to the optimized dyad. These quantities are listed in Table S3, where it is clear that they follow the same pattern as that of Eint, even if a bit smaller in magnitude.
Also listed in Table 6 as ΔqT are the changes in the natural charge on the apical T atom when involved in the bond to each of the Lewis acids. This atom becomes more negative in the various HBs, particularly for the strong proton donor HF. This density increase is typical of HB proton acceptor atoms and is likely attributable in large measure to internal polarization within the pyramidane that makes the T a more attractive target for the positively charged bridging proton. The tetrel atom increases its positive charge for the XBs, especially noticeable for FI with its deep σ-hole on I. This density loss is consistent with the red regions surrounding T in Fig. 5. The increase in positive charge is very substantial for the osme-bonded complexes, roughly 0.5e. This large change is consistent with the high degree of covalent character of these bonds. The last column in each section of Table 6 lists the total amount of charge displaced from the pyramidane to the electrophilic molecule. This CT is small for the HBs, a bit larger for the stronger XBs, and very large, on the order of 0.5–0.7e, for the OsBs. These large intermolecular charge transfers are consistent with the density loss from T signaled by its substantially more positive charge, as well as the red areas in Fig. 5 within the pyramidanes. These effects are similar for the XBs, if a bit muted.
| Si(C4H4) | Ge(C4H4) | Sn(C4H4) | Pb(C4H4) | |||||
|---|---|---|---|---|---|---|---|---|
| M062X | CCSD(T) | M062X | CCSD(T) | M062X | CCSD(T) | M062X | CCSD(T) | |
| HF | −5.18 | −3.73 | −5.02 | −3.64 | −5.70 | −3.91 | −6.24 | −4.22 |
| HCl | −3.98 | −3.20 | −3.88 | −3.15 | −4.47 | −3.31 | −4.91 | −4.78 |
| HBr | −3.77 | −3.18 | −3.70 | −3.10 | −4.31 | −3.35 | −4.72 | −3.57 |
| FCl | −4.50 | −2.58 | −4.53 | −2.62 | −5.51 | −3.04 | −6.29 | −3.45 |
| FBr | −6.16 | −4.18 | −6.23 | −4.28 | −7.98 | −5.30 | −10.55 | −6.88 |
| FI | −7.89 | −5.61 | −7.98 | −5.77 | −10.36 | −7.42 | −13.03 | −9.24 |
| Fe(CO)4 | −12.64 | −13.64 | −12.66 | −13.82 | −15.48 | −16.90 | −17.03 | −18.48 |
| Ru(CO)4 | −8.65 | −8.56 | −8.77 | −8.83 | −10.44 | −10.42 | −11.67 | −11.57 |
| Os(CO)4 | −9.72 | −9.60 | −9.93 | −10.03 | −14.17 | −14.58 | −17.31 | −17.75 |
The AIM molecular diagrams are displayed on the right side of Fig. S2. They show bond paths leading to various elements of the base, either a C atom or a C–C bond midpoint. The AIM parameters for these intermolecular bond paths are collected in Table S6. The bond critical point densities remain clearly in the noncovalent range, all less than 0.05 a.u. The total energy density H hovers around zero, confirming only a minor degree of covalency.
NBO analysis of the density of each complex allows for a better understanding of the orbitals involved in the bonding. This protocol reapportions the total density into a series of orbitals that are highly localized. The C4 structure of the base of the pyramid is represented by a group of four σ(C–C) bonding orbitals, one for each pair of adjacent C atoms. This array is supplemented by one C–C π bonding orbital. The HB and XB complexes in Fig. 7(a) and (b) show the recipient orbital in each case to be the pertinent σ* orbital of the Lewis acid. The primary donor in the HCl case of Fig. 7(a) can be described as a Ge–C bonding orbital, comprising a C π-orbital, that overlaps nicely with the HCl σ*. The chief donor in the XB case is the π bonding orbital between a pair of C atoms in the base of the pyramid. The same CC π orbital is the primary donor to the Fe atom in Fig. 7(c). The orbital within Fe(CO)4, which accepts charge, is labeled by NBO as a vacant Fe lone pair orbital, primarily of p-character, with its main lobe pointing toward the pyramid base. This sort of osme bonding also contains a contribution from back-bonding. Specifically, some charge is transferred from the Fe d-orbital in Fig. 7(d) to a CC π* antibonding orbital within the pyramidane. The latter accounts for a second-order perturbation energy of 7.8 kcal mol−1, as compared to 20.8 kcal mol−1 for the main transfer in Fig. 7(c).
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| Fig. 7 Natural bond orbitals primarily responsible for the intermolecular bonding of Ge(CH)4 with (a) HCl, (b) BrF, and (c) and (d) Fe(CO)4. Red arrows indicate the direction of electron flow. | ||
As for the apical complexes, the effect of H-bonding on the basal C–C bond lengths is very little, as is evident from Table S7. On the other hand, the basal complexes do not manifest the substantial contraction of the r(C–T) bonds to the apex of the pyramid that is observed for the apical structures. The major geometrical changes within the pyramidanes occur within the context of the osme bonds, where the C–T bonds grow longer, in contrast to the contractions that were observed in the apical complexes. Whereas the charge on the T atom had become more negative for apical HBs, somewhat more positive for the XB, and very much more positive for OsB, the pattern is quite different for the basal complexes. The T atom grows more positive for each type of bond, and there are no dramatic differences from one bond type to the next. This increased positive charge is consistent with the idea that density is drawn away from the pyramidane and into the electrophile, as these noncovalent bonds are forged.
The interaction energy decompositions described in Table S8 are also consistent with the idea that all three electrophile types form basically similar noncovalent interactions. The ES percentage is about 50% for Si and Ge, and is reduced a bit for the heavier Sn and Pb. Dispersion contributes another 1/4 or so. POL and CT account for the remainder, with the latter generally being larger than the former.
There will be natural competition between the apical and basal sites for an incoming electrophile. The competitive advantage of the apical over the basal complexes is listed explicitly in Table 8, where the positive values signify the greater stability of the former. It is immediately apparent that the osme bonds greatly prefer the apical T atom, by amounts varying between 4.6 and 28.3 kcal mol−1. One can attribute this advantage to the presence of a strong and partially covalent bond to the T atom. The HBs show a consistent preference for the basal geometries, consonant with the more negative potential minimum at this location within the pyramidanes as compared to the T locale. The pattern is more interesting for the halogen bonds. The Si-pyramidanes favor association with the apical atom, whereas the base is favored over Sn. The situation is mixed for Ge: the lighter Cl and Br prefer the base, whereas I with its deeper σ-hole favors the Ge center. Of course, all three types of electrophiles favor the base of the Pb-pyramidanes as there are no complexes with the apical Pb, with its highly positive MEP.
| Si(C4H4) | Ge(C4H4) | Sn(C4H4) | ||||
|---|---|---|---|---|---|---|
| M062X | CCSD(T) | M062X | CCSD(T) | M062X | CCSD(T) | |
| HF | −1.85 | −0.80 | −2.65 | −1.78 | −4.31 | −3.41 |
| HCl | −2.05 | −1.23 | −2.54 | −1.81 | −3.79 | −2.78 |
| HBr | −2.04 | −1.32 | −2.52 | −1.79 | −3.70 | −2.74 |
| FCl | 5.63 | 3.25 | −1.17 | −0.95 | −2.79 | −2.35 |
| FBr | 7.75 | 5.85 | −0.25 | −0.33 | −3.48 | −3.12 |
| FI | 6.39 | 5.98 | 0.31 | 0.38 | −2.04 | −1.98 |
| Fe(CO)4 | 17.52 | 26.20 | 8.19 | 14.48 | 4.62 | 9.22 |
| Ru(CO)4 | 20.76 | 26.06 | 9.44 | 14.80 | 7.16 | 11.87 |
| Os(CO)4 | 28.32 | 30.06 | 15.09 | 17.97 | 12.91 | 14.91 |
The H-bonds are fairly weak, on the order of 3 kcal mol−1 or less, but the halogen bonds are considerably stronger but variable, covering the range between 3 and 14 kcal mol−1. Both the HBs and XBs follow the conventional trends in that the former grow stronger with the acidity of HF, and the latter strengthen as the X atom grows larger and becomes more electropositive. Strongest of all, between 18 and 38 kcal mol−1, and containing a significant degree of covalent character, are the osme bonds to Fe, Ru, and Os. Si engages in the strongest OsBs, with Ge and Sn roughly equivalent. Os forms stronger bonds than does either Fe or Ru. The HBs to Si and Ge are largely dominated by electrostatics, as is a common feature of most such bonds. However, the influence of dispersion grows in importance for Sn. The halogen bonds to the apical T place electrostatics and charge transfer on a roughly equal footing, except for Si where charge transfer plays the dominant role. The osme bonds all contain a heavy dose of electrostatics, regardless of the size of T, and dispersion is nearly negligible.
Because the MEPs of these pyramid shaped molecules are characterized by a negative region at their base, this site attracts the various electrophiles despite the absence of a lone pair in this position. The various electrophiles are drawn instead toward the C–C π-bonding orbitals, which serve as a reservoir of charge that is amenable to transfer. The bonding to the pyramid's base, whether the electrophile is an H, X, or group 8 metal atom, is controlled largely by electrostatics, which accounts for roughly half of the total attraction. Polarization and charge transfer make more minor contributions, even less than dispersion in some cases. Bonding to the group 8 metal atoms is clearly noncovalent and much weaker than when M attacks the T atom at the pyramid apex.
There is an interesting competition between the apex T atom and the all-C base of the pyramid. Perhaps due to their dependence on electrostatics, proton donors are drawn preferentially toward the pyramid base with its more negative potential. These HB energies lie in the 4–6 kcal mol−1 range, placing the pyramid base on the same scale as O and N lone pairs as electron donors. HBs to the apex of the pyramid are consistently weaker, some less than even 1 kcal mol−1. On the other end of the spectrum are the osme bonds to the group 8 metals. Their bonding to the pyramid base is substantive but clearly noncovalent, between 5 and 28 kcal mol−1. But their approach toward the apex T leads to much stronger bonding, with a significant covalent contribution. The interaction energies of these coordinate covalent bonds fall in the 18–38 kcal mol−1 range. This stronger bonding to the apex occurs despite a disadvantage in terms of a small negative, and even slightly positive, electrostatic potential at the T center. The halogen bonds present the most interesting mix of competitive bond strengths. While the Si apex is favored over the base, this balance shifts toward the base for the heavier Ge and Sn, with their much lower negative potential. Indeed, there are no stable apical complexes at all for Pb with its substantially positive potential.
The results for the various T apex atoms can be compared with prior calculations placing C at this position.15 The MEP at the C apex was measured to be −42.3 kcal mol−1, considerably larger in magnitude than any of the larger T atoms examined here. Like the systems discussed above, this apical C had associated with it a pseudo-lone pair, which was able to interact with a host of electrophiles. The interaction energies varied up to as high as 57 kcal mol−1 for the tetrel bond with SnF4. The C⋯HX HB energies were considerably stronger than those with larger T apices, more than 10 kcal mol−1. The same greater strength was observed for halogen bonds of nearly 30 kcal mol−1. Strongest of all were T⋯C tetrel bonds to various TF4 Lewis acids that exceeded 50 kcal mol−1. The bonding of the C-pyramidanes to any of these electrophiles contained a major contribution from electrostatics, in most cases well above 50%. This fraction exceeds that of a number of heavier T-pyramidanes examined here. Veljkovic et al. had computed HB energies for C-pyramidanes with water14 at the CCSD(T)/CBS level. Due to the much more negative potential on the C as opposed to the heavier tetrels here, the energies of these O–H⋯C HBs were a bit stronger, between −2.0 and −7.4 kcal mol−1. This strength was amplified by the substitution of electron-donating groups on the four basal C atoms.
Lee9,10et al. had considered other types of pyramidanes where both the apex and base atoms were replaced by tetrels other than C. They identified what they considered to be a high degree of ionicity in the bonds connecting the apex to the base atoms. AIM bond critical point densities for the bonds including the apex are uniformly smaller than those connecting base atoms to one another. This work verified the presence of a very high s-character lone pair on the apex atom. These results were validated in another study,2 which also provided ELF analyses that mirror our own picture in Fig. 2. Imagawa et al.11 placed Si at the apex and were able to bind this pyramidane with an Fe(CO)4 species and determine the structural data from the crystal. Their observed R(Si⋯Fe) distance of 2.211 Å was rather close to our calculated bond length of 2.202 Å, confirming the strength of this osme bond. The geometry was also consistent with our computed trigonal bipyramidal structure around the Fe. Other work has considered non-tetrel atoms at the apex of the pyramidane. In various bora[4]pyramidanes,41 the bond critical point density from B to the base C atoms was larger than 0.1.
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