Siddhartha K.
Purkayastha
a,
Shahnaz S.
Rohman
b,
Pattiyil
Parameswaran
*b and
Ankur K.
Guha
*a
aAdvanced Computational Chemistry Centre, Cotton University, Panbazar, Guwahati, Assam 781001, India. E-mail: ankurkantiguha@gmail.com
bDepartment of Chemistry, National Institute of Technology Calicut, Kozhikode, 673601, India. E-mail: param@nitc.ac.in
First published on 28th March 2024
Transition metal–carbonyl bonds are rationalized by M ← CO σ donation and M → CO π back donation where the d orbital of the transition metal is involved. This bonding model provided by Dewar, Chatt and Duncanson (DCD) has rationalized many transition metal–ligand bonds. The involvement of p orbital in such a DCD model can be intriguing. Alkaline earth metals with ns2np0 configuration may appear suitable as ns0np2 excitation has been recognized in many complexes. Herein, a theoretical study is presented for the Be(CO)n (n = 1–4) complex to verify this assumption. Detailed electronic structure analyses confirmed the involvement of the p orbital of beryllium in M → CO π back donation, thereby supporting the hypothesis. EDA-NOCV results reveal that the π-back donation from the central Be atom to CO ligands significantly predominates over the σ donation from the ligands for both Be(CO)3 and Be(CO)4. Our calculations reveal that Be(CO)4 is the highest carbonyl that may be experimentally detected.
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Scheme 1 Bonding situation in (a) transition metal carbonyls where d orbitals are involved and (b) bonding situation in metal carbonyls where s and p orbital of metal are involved. |
Generally, transition metal having d orbital is best suited for this type of bonding, which favours backdonation from the filled d orbital to π* orbital of the CO ligand. However, an alternative situation may also be envisioned where the metal uses its filled pz-orbital for the M → CO (π*) back donation (Scheme 1b) and vacant s, px and py orbitals of metal for M ← CO σ donation. To realize this, the choice of the metal is very crucial. One such obvious choice is alkaline earth metal, among which beryllium is very lucrative. Braunschweig and co-workers have reported the first example of neutral zero valent beryllium complex L–Be–L (L = cyclic (alkyl)(amino)carbene).4 The bonding situation was described as a donor–acceptor interaction between the ground state of L ligands and Be(0), which is in 1s22s02p2 electronic configuration.4 Similarly, the OCBe(CO)3 complex has also been reported by Chen et al.5 This indicates that beryllium can show a bonding feature involving its excited 1s22s02p2 electronic configuration where the valence 2s orbital is empty and 2p orbital is filled, a perfect match to fulfill the hypothetical bonding situation in Scheme 1b. It should be noted that Be(0) compounds have been predicted theoretically.6,7 However, to the best of our knowledge, such a connection between the p-orbital analogy of the DCD model has never been highlighted in those Be(0) compounds; however, in this study, the beryllium carbonyl complex, Be(CO)n (n = 1–4), has been theoretically studied, and it shows such a bonding situation. Involvement of beryllium 2s, 2px and 2py orbitals in M ← CO σ donation and 2pz orbital in M → CO (π*) back donation is clearly established.
Energy decomposition analysis16 in conjunction with the natural orbital for chemical valence17 (EDA-NOCV) was performed at the BP86/TZ2P level18 using the ADF2020.102 program package19 on TPSSh optimized geometries. The interaction energy between fragments A and B in the molecule A–B can be considered as an indicator of bond strength between the two fragments under consideration. EDA mainly focuses on the intrinsic interaction energy (ΔEint). This interaction energy is related to another physical observable, the bond dissociation energy (De), as can be seen in the following equation:
ΔEint = −De + ΔEprep |
The fragments A and B in their respective ground states are excited to the frozen electronic and geometric states in the molecule A–B by providing them the required excitation energy (ΔEprep). EAGS and EBGS refer to the electronic energy of the fragments A and B in their respective ground states, while EA and EB refer to the electronic energy of the corresponding fragments in their frozen geometries of the molecule.
The instantaneous interaction energy (ΔEint) of a bond A–B is partitioned into chemically meaningful components as follows:
ΔEint = ΔEelect + ΔEPauli + ΔEorb + ΔEdisp. |
The term ΔEelect refers to the quasi-classical electrostatic interactions. The frozen electron density distribution of the fragments in the geometry of the molecules is calculated by quantum mechanics, and the interaction between the nuclei and electrons is calculated by classical laws. It is usually an attractive component and gives an estimate of electrostatic interactions that are excluded from the orbital-based analysis. ΔEPauli corresponds to the repulsive interactions between fragments of like spin as they approach each other. However, note that this term is not indicative of ionic bonding and is calculated by the anti-symmetrization and renormalization of the Kohn–Sham determinant of the orbitals. ΔEorb is associated with the stabilization of orbitals during bond formation and is an attractive component. It includes the effects of charge transfer, relaxation, and polarization by deformation of the charge distribution of the fragments during bond formation.
Developed by Mitoraj and Michalak, the EDA-NOCV scheme further decomposes ΔEorb term into contributions from each irreducible representation in the point group of the interacting system. The natural orbitals for chemical valence (NOCV) provide insight into each specific orbital interaction between the fragments and the contribution of each pair of the interacting orbitals (Ψ−n/Ψn) to the total bond energy. Within this scheme, ΔEorb is expressed in terms of NOCVs as
Let us turn our attention now to Be(CO)4. It adopts a perfectly square planar geometry in its singlet electronic ground state (Fig. 2a). The triplet state is 10.7 kcal mol−1 higher in energy at TPSSh/def2-TZVP and 14.2 kcal mol−1 at the CCSD(T)/cc-pVTZ//TPSSh/def2-TZVP level. The tetrahedral geometry is also a saddle point on the potential energy surface. All other manually constructed isomers are also saddle points on the potential energy surface. It implies that the square planar geometry of Be(CO)4 is the lowest energy structure. While BeCO has a triplet ground state,20 the ground state of Be(CO)4 is a closed-shell singlet. Moreover, while the triplet electronic states of BeCO and Be(CO)2 are more stable, singlet electronic states become more stable for Be(CO)3 and Be(CO)4 complexes. All Be–C bond lengths in Be(CO)4 are equal (1.811 Å) at the TPSSh level. Moreover, M06-2X level produces similar Be–C distances (1.816 Å). Mayer's bond order for the Be–C bond is 0.83, indicating significant covalency and a stronger Be–CO bond. The computed Hirshfeld charge at the Be atom is near zero (−0.05 e) and slightly positive (0.1 e) at the carbon atom indicating that the bonding situation should not be described as Be+(CO)4− or Be2+(CO)42−, rather as common DCD model, which recovers covalency in the metal–ligand bond.1,2 The CO bond is elongated by 0.013 Å compared to its length in the free form (1.129 Å). This reflects Be → CO back donation, which is also evident from the lowering of the IR active stretching frequency (unscaled) of the CO group (2027 cm−1) compared to its free value (2184 cm−1). The calculated bond dissociation energy for the loss of four molecules of CO from Be(CO)4 is 65.6 kcal mol−1 (46.2 kcal mol−1 at CCSD(T)/cc-pVTZ level), indicating that the Be–CO bonds are stronger. This indicates that the possibility of its experimental observation may be in the low-temperature neon matrix where the isolation of M(CO)8 (M = Ca, Sr or Ba) has been reported.22
Fig. 2b shows the shapes of the highest occupied molecular orbital (HOMO) and HOMO−1 of Be(CO)4 complex. HOMO represents the Be → CO π* back donation and is delocalized among all four carbon centres. This delocalization stabilizes the square planar geometry over the tetrahedral one. HOMO−1 represents the CO → Be σ donation, thereby establishing the synergism observed in the common DCD model. Interestingly, the Be → CO π* back donation involves Be 2pz orbital. Thus, the present bonding situation can be considered as a p-orbital analog of the DCD model. Electron localization function (ELF)12,13 analysis also reveals the presence of disynaptic V(Be,C) basins with a population greater than 2.00 |e| (Fig. 2c), indicating a partial double Be–C bonding character. The bonding situation is exactly similar to that observed for the experimentally observed neutral zero valent beryllium complex L–Be–L (L = cyclic (alkyl)(amino)carbene)4 and OCBe(CO)3 complex5 and theoretically proposed Be(0) compounds.6,7
Are higher carbonyl complexes possible? We tried to optimize Be(CO)n with n = 5–8 in both singlet and triplet electronic states. However, geometry optimisation leads to dissociation of CO ligand(s). This indicates that the beryllium atom can accommodate a maximum of four CO groups.
To gain an insight into the quantitative nature of the bonding description in Be(CO)3 and Be(CO)4, we carried out energy decomposition analysis coupled with natural orbital for chemical valence (EDA-NOCV). In both the systems, the central beryllium atom in 1s22s02pz2 electronic state is considered as one fragment and the ground state singlet carbonyl ligands, namely, three CO ligands in Be(CO)3 and four CO ligands in Be(CO)4, as another fragment. The bonding scheme considered here features purely dative interactions, with σ-donations from the CO ligands and π-back donations from the central beryllium atom (Table 1).
Be(CO)3 | Be(CO)4 | |||
---|---|---|---|---|
a The values in parentheses give the percentage contribution to the total attractive interactions ΔEelstat + ΔEorb. b The values in parentheses give the percentage contribution to the total orbital interactions ΔEorb. c ΔErest = ΔEorb − (ΔEσ + ΔEπ). d Dissociation energy (De). | ||||
Fragment 1 | Be(1s22s02pz2) | Be(1s22s02pz2) | ||
Fragment 2 | 3CO | 4CO | ||
ΔEint | −256.3 | −266.8 | ||
ΔEPauli | 69.2 | 37.9 | ||
ΔEelstata | −87.0 (26.9%) | −78.7 (26%) | ||
ΔEdisp | −1.8 | −1.9 | ||
ΔEorba | −236.7 (73.1%) | −224.1 (74%) | ||
ΔEσb | ΔEσ(+ + +)b | −17.1 (7.2%) | ΔEσ(+ + + +)b | −18.2 (8.1%) |
ΔEσ(+ − +)b | −40.3 (17.0%) | ΔEσ(· + · −)b | −32.8 (14.6%) | |
ΔEσ(+ · −)b | −40.3 (17.0%) | ΔEσ(+ · − ·)b | −32.8 (14.6%) | |
ΔEσ(+ − + −)b | −8.1 (3.6%) | |||
ΔEπb | −128.3 (54.2%) | −123.7 (55.3%) | ||
ΔErestc | −10.7 (4.6%) | −8.5 (3.8%) | ||
ΔEprep | 179.2 | 196.6 | ||
−Ded | −77.1 | −70.2 |
The interaction energy ΔEint, which can be considered as a measure of the Be–C bond strength, is found to be only slightly higher for Be(CO)4 (−266.8 kcal mol−1) as compared to Be(CO)3 (−256.3 kcal mol−1). Note that the total attractive component of interaction energy is higher for Be(CO)3. The slightly higher value of ΔEint for Be(CO)4 mainly arises from the significantly lower value of Pauli repulsion (37.9 kcal mol−1). The orbital stabilization energy, ΔEorb in Be(CO)3 and Be(CO)4 are found to be −236.7 and −224.1 kcal mol−1, respectively, which contributes significantly to the attractive component of the interaction energy (73.1% in Be(CO)3 and 74.0% in Be(CO)4).
The beryllium in the excited state with 1s22s02pz2 electronic configuration has three vacant in-plane orbitals, which can form σ bonds with three CO ligands. Hence, the Be–C bonds in Be(CO)3 can be considered formal 2c–2e bonds. However, the multicentre bonding concept needs to be invoked to explain four Be–C σ-bonds in Be(CO)4. This is corroborated by the geometrical pattern where the Be–C bonds in Be(CO)3 (1.655 Å) are shorter than those in Be(CO)4 (1.811 Å).
To understand the variation in σ and π interaction among Be(CO)3 and Be(CO)4, we decomposed the ΔEorb into the contribution from atomic orbitals of beryllium. Since Be(CO)3 and Be(CO)4 are perfectly trigonal planar (D3h) and square planar (D4h) molecules, the ligand group orbitals of (CO)3 and (CO)4 are similar to those shown in Scheme 1. The all (+) combination of the ligand group orbital (a′1 for Be(CO)3 and a1g for Be(CO)4) are right symmetry to interact with the 2s orbital of the Be atom. Note that the energy stabilization due to this interaction is only slightly higher for Be(CO)4. The second σ(+ − +) and third set σ(+ · −) of the ligand group orbitals of (CO)3 are right symmetry to interact with 2py and 2px, respectively (Scheme 2).
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Scheme 2 Atomic orbitals of Be atom in the excited state (1s22s02pz2) interacting with ligands group orbitals of (CO)3 and (CO)4 fragments in Be(CO)3 and Be(CO)4. |
The energy stabilization due to this interaction is more than two times that of the former interaction in Be(CO)3 (Table 1). Hence, we wish to propose that 2p orbitals of beryllium atoms are better σ acceptors as compared to the 2s orbital. Similarly, the second σ(+ · − ·) and third σ(· + · −) set of ligand group orbitals of (CO)4 also have the right symmetry to interact with 2py and 2px orbitals of the Be atom. The corresponding energy stabilization is lower than those in Be(CO)3. Nevertheless, the energetics indicate that 2p orbitals are better σ acceptors as compared to 2s orbitals. The deformation densities corresponding to σ and π interactions in both the systems are shown in Fig. 3. Δρ2 – Δρ4 shows the accumulation of red region around ligand group orbitals along with an accumulation of blue region in the direction of 2s/2p orbitals of central Be atom. Thus, the flow of charge density from red → blue reaffirms σ donation from CO ligands to the Be centre.
The fourth combination of ligand group orbital of (CO)4 does not have a right symmetrical orbital to interact with beryllium. The energy stabilization for this interaction arises from the polarization of ligand orbitals towards a more electropositive beryllium centre. The total orbital stabilization energy due to σ-donation from the CO group in Be(CO)3 is −97.7 kcal mol−1, whereas the corresponding value for Be(CO)4 is −91.9 kcal mol−1. The π-back donation from central Be atom to CO ligands (ΔEπ = −128.3 kcal mol−1 and −123.7 kcal mol−1 in Be(CO)3 and Be(CO)4 respectively) considerably predominates over the σ donation for both Be(CO)3 and Be(CO)4. The deformation density Δρ1 in Fig. 3 represents a π-back donation from the 2pz orbital of Be to the π-symmetric ligand group orbitals. Important NOCV pairs of orbitals Ψ−n/Ψn associated with respective deformation densities are plotted in Fig. S1 and S2 of ESI.†
Footnote |
† Electronic supplementary information (ESI) available: Fig. S1 and S2 and cartesian coordinates of all the optimized geometries. See DOI: https://doi.org/10.1039/d4cp00908h |
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