Open Access Article
Alexander
Gehlhaar
a,
Hanns Micha
Weinert
a,
Christoph
Wölper
a,
Nina
Semleit
b,
Gebhard
Haberhauer
*b and
Stephan
Schulz
*ac
aInstitute of Inorganic Chemistry, University of Duisburg-Essen, 45117 Essen, Germany. E-mail: stephan.schulz@uni-due.de
bInstitute of Organic Chemistry, University of Duisburg-Essen, 45117 Essen, Germany. E-mail: gebhard.haberhauer@uni-due.de
cCenter for Nanointegration Duisburg-Essen (Cenide), University of Duisburg-Essen, Carl-Benz-Straße 199, 47057 Duisburg, Germany
First published on 12th May 2022
peri-Substituted naphthalene complexes (Trip2Pn)2Naph (Pn = Sb 1, Bi 2) were synthesised and their redox behaviour investigated. Oxidation of 1 with [Fc][BArF] (BArF = B(C6F5)4) yielded [(Trip2Sb)(TripSb)Naph][BArF] (3) containing the stibane-coordinated stibenium cation [(Trip2Sb)(TripSb)Naph]+. Subsequent reduction of 3 with KC8 yielded distibane (TripSb)2Naph (4). 1–4 were characterised by NMR (1H, 13C) and IR spectroscopy as well as single-crystal X-ray diffraction (sc-XRD), while their electronic structures were analysed by quantum chemical computations.
Neutral donor–acceptor complexes R3Pn–Pn′R′3 of Lewis basic phosphanes PR3 (R = alkyl, aryl) and Lewis acidic phosphanes PX3 (X = halide)6 as well as their heavier homologues are well known.7–9 Since donor–acceptor interaction strengths typically decrease with increasing atomic number, neutral complexes of heavy pnictogens tend to dissociate to either the neutral Lewis acid and Lewis base or with formation of ionic species [R3Pn–Pn′R′2]+[R′]− (Fig. 1), which are often more stable toward Pn–Pn′ bond dissociation due to the increased Lewis acidity of the pnictenium (Pn′R′2+) cation.8–11peri-Substituted naphthalene and acenaphthene complexes, in which the pnictogen atoms are fixed in 1,8-position, are also promising candidates to study Pn(III)–Pn(III) donor–acceptor interactions since they can not separate into two individual species. While complexes of this type containing lighter pnictogens are known,12 those of the heaviest elements of group 15, Sb and Bi, are still rare, and they exclusively contain rather strong phosphane donors.13
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| Fig. 1 Known intermolecular- and intramolecular stabilised pnictenium cations and peri-substituted heavy pnictenium complexes reported herein. | ||
We recently reported on dipnictanes Pn2Naph2 (Pn = As, Sb, Bi)14 and bis(diphenylpnicta)naphthalenes (Ph2Pn)2Naph (Pn = Sb, Bi)15 of the heaviest group 15 elements. Due to our general interest in pnictogen-centered radicals,16 we investigated single electron transfer reactions of the latter. Unfortunately, reactions with several oxidants failed to give defined reaction products. We therefore replaced the Ph groups by bulky Trip groups (Trip = 2,4,6-i-Pr3C6H2), which successfully stabilised Trip3Pn˙+ radical cations,17 in order to kinetically stabilise likely-formed radical cations. (Trip2Pn)2Naph (Pn = Sb 1, Bi 2) were synthesized by reaction of Trip2PnCl (Pn = Sb, Bi) with Li2Naph at −78 °C (1) and −30 °C (2), respectively (Scheme 1).
The 1H NMR spectrum of 2 at ambient temperature shows the expected number of signals due to the Naph and Trip substituents, indicating a symmetric molecule in solution, whereas that of 1 exhibits several signals of the Trip groups, pointing to a molecule of lower symmetry. Variable temperature (VT) NMR studies showed that the septet of the ortho i-Pr group first splits into two broad signals, which further split into two septets. ΔG≠ values of 15.6 and 15.9 kcal mol−1 were calculated from the coalescence temperatures (50 °C, 70 °C).182 also shows coalescence points (0 °C, ΔG≠ = 12.9 kcal mol−1; −60 °C, ΔG≠ = 13.3 kcal mol−1) at lower temperatures. The hindered rotation most likely stems from ligand–ligand interactions of the large Trip groups, which are expected to be larger in 1 due to the smaller Sb atoms compared to the Bi atoms in 2, resulting in larger rotational barriers in 1.
Single crystals of 1 (Fig. 2A) and 2 (Fig. S26, ESI†) were grown from saturated solutions in ethanol upon storage at +4 °C. 1 and 2 crystallise in the orthorhombic and monoclinic space groups P21212 (1) and C2/c (2) with two (1) and four (2) molecules per unit cell, respectively. Selected bond lengths and angles are given in Table 1.
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| Fig. 2 Solid-state structures of 1 (A), 3 (B), and 4 (C) with displacement ellipsoids drawn at the 50% probability level. Hydrogen atoms (1, 3) and the [BArF] anion (3) are omitted for clarity. | ||
| 1 | 2 | 3 | 4 | |
|---|---|---|---|---|
| Pn⋯Pn | 3.2327(2) | 3.6742(4) | 2.7980(4) | 2.7991(6) |
| Pn–C | 2.1769(11), 2.2019(11), 2.1902(10) | 2.318(4), 2.326(5), 2.326(5) | 2.1170(15), 2.1367(15), 2.1465(15), 2.1647(17), 2.1708(17) | 2.149(6), 2.196(6), 2.153(6), 2.192(6) |
| C–Pn–Pn | 80.89(3), 93.23(3), 167.59(3) | 74.73(11), 102.87(13), 164.20(13) | 91.26(4), 80.51(4), 137.25(4), 98.29(4), 106.31(4) | 86.18(16), 100.81(17), 85.91(15), 102.91(15) |
| C–Pn–C | 106.84(4), 101.51(4), 97.64(4) | 107.53(16), 96.72(17), 92.31(9) | 113.07(6), 113.33(6), 107.08(6), 102.86(6) | 100.7(2), 99.9(2) |
The pnictogen atoms adopt trigonal-pyramidal coordination spheres, and the sum of bond angles (306.02° 1, 296.56° 2) indicate a high p-orbital character of the bonding electrons. The Sb–C (2.1769(11) Å, 2.2019(11) Å, 2.1902(10) Å) and Bi–C (2.318(4) Å, 2.326(5) Å, 2.326(5) Å) bonds are rather long due to the large steric crowding in 1 and 2. Despite the increased steric hindrance, the Sb⋯Sb distance in 1 (3.2327(2) Å) is shorter than that in (Ph2Sb)2Naph (3.2983(6) Å),15 indicating stronger attractive forces, i.e. ligand⋯ligand dispersion interactions of the i-Pr groups of the Trip substituents. In marked contrast, the Bi⋯Bi distance in 2 (3.6742(4) Å) is significantly elongated compared to that in (Ph2Bi)2Naph (3.4461(4) Å).15 The elongation of the Pn⋯Pn distance in 2 compared to 1 points to stronger repulsive interactions between the Bi atoms, which is also reflected by the larger distortion of the Naph ligand in 2 (dihedral angles: 12.78(7)° 1, 28.13(29)° 2). In addition, intramolecular CH⋯π contacts are found for 1 and 2 (Fig. S29, ESI†).
We performed cyclic voltammetry (CV) studies with 1 and 2 to study their redox properties (Fig. S21–S24, ESI†). Two oxidation events were observed for 1, with a pseudo-reversible first one (E1/2(Fc0/+1) = −0.1 V) as indicated by the peak-to-peak distance ΔEp value, which increased significantly with faster scan rates, followed by an irreversible second event (Ep,a(Fc0/+1) = 0.74 V). In contrast, only one irreversible oxidation event was observed for 2 (Ep,a(Fc0/+1) = 0.66 V), which occurred at a slightly lower voltage than the irreversible event of 1. The reduction event found at Ep,c = −0.79 V was observed only when the sample was scanned in the oxidative direction. The CV studies indicate that 1 can be oxidised by a mild oxidant, and 1 was therefore reacted with [Fc][BArF].19 The reaction immediately resulted in a color change (Scheme 2), and green crystals were isolated after workup, which did not show any paramagnetic behaviour. They were identified as [(Trip2Sb)(TripSb)Naph][BArF] (3) and TripH was formed as a by-product. Analogous reactions in thf or CH2Cl2, which are easier to deprotonate than benzene, proceeded much faster, hence we assume that the Trip anion is protonated by the solvent. The splitted signals for the Naph protons in the 1H NMR spectrum of 3 indicate an unsymmetric species. In addition, both sharp and broad signals in a 2
:
1 ratio are observed for the Trip protons. VT 1H NMR studies showed a coalescence temperature of −70 °C for the sharp signals. The calculated rotational barrier (ΔG≠ = 10.1 kcal mol−1) is roughly 5 kcal mol−1 smaller than that in 1, which is in line with the reduced steric hindrance due to removal of one Trip ligand. Comparable oxidation reactions were performed with 2. Due to the higher oxidation potential, [NO][SbF6] was chosen as the oxidant. The resulting reaction mixture showed high activity toward the polymerization of thf, but unfortunately, any attempts to isolate a product failed.
To transfer cation 3 into a radical species, we attempted a reduction with KC8. A yellow solid was isolated after work-up and identified as (TripSb)2Naph (4) (Scheme 2), while TripH and K[BArF] formed as by-products. The 1H NMR spectrum of 4 shows the expected signals for a highly symmetric species.
Single crystals of 3 (Fig. 2B) and 4 (Fig. 2C) were grown from saturated solutions in 2 mL of CH2Cl2 layered with 30 mL of n-hexane (3) and in n-hexane (4) upon storage at +4 °C. 3 crystallises in the triclinic space group P
with two molecules per unit cell and 4 in the orthorhombic space group Pbca with eight molecules per unit cell. The Sb–C bonds in 3 and 4 are shorter than those in 1 as was expected, but the tetrahedrally-coordinated Sb1_1 atom in 3 (2.1170(5), 2.1367(15), 2.1465(15) Å) surprisingly shows slightly shorter Sb–C bonds than the three-coordinated Sb2_1 centers in 3 (2.1647(17), 2.1708(16) Å) and 4 (2.149(6), 2.196(6), 2.153(6), 2.192(6) Å), respectively. The Sb–Sb distance in 3 (2.7980(4) Å) is significantly shorter compared to that of 1 (3.2327(2) Å) and in the range of typical Sb(II)–Sb(II) bond lengths, indicating a strong Sb⋯Sb charge-transfer interaction. The Sb⋯Sb distance in 3 is virtually identical to the “regular” Sb–Sb single bond in 4 (2.7991(6) Å), and both are at the shorter end of the Sb–Sb bond length range reported for distibanes.20
To interpret these experimental findings, quantum chemical computations were performed both for compounds 1–4 and the Ph-substituted reference systems S1–S4 (see Fig. 3 and ESI†).
In the latter, the ligands at the Pn centers are not connected, so the Pn⋯Pn interactions can be determined by dividing the systems into two fragments. A comparison of the calculated data confirms that the Sb–Sb bond lengths in 3 (2.806 Å) and in S3 (2.848 Å) are slightly shorter than that in 4 (2.820 Å) and in S4 (2.860 Å), suggesting that the Sb–Sb binding in the cationic donor–acceptor compounds (3, S3) is stronger than in the distibanes (4, S4) containing a “regular” Sb–Sb covalent bond. Indeed, the total binding energy (ΔE in Fig. 3) obtained from a bond energy analysis calculation is higher for S3 (Fig. 3, −64.2 kcal mol−1) than for S4 (−46.9 kcal mol−1). A glance at the individual attractive energy terms for the Sb–Sb bonds in S3 and S4 reveals that they are very similar and quite different from the van der Waals interaction of the fragments in S1 (Fig. 3). Thus, the relative sizes of the individual terms are not significantly different; in fact, in S4 the electrostatic term is slightly larger than in S3; in other words, the dative Sb–Sb bond in S3 is stronger than the covalent bond in S4 due to orbital interactions. NBO analysis of S3 and S4 shows that the Sb–Sb bond in S3 is strongly polarised (Fig. 3): the tetravalent Sb atom has a higher fraction (64%) and the s character of the orbital is significantly higher (22%) than that at the trivalent Sb atom (4%). As expected, a symmetric Sb–Sb bond with high p fraction (95%) of the interacting orbitals is found for S4. Quantum theory of atoms in molecules (QTAIM)21 analysis of S3, S4, 3 and 4 confirms these findings (Tables S10–S12 and Fig. S34–S39, ESI†). The Laplacian of the electron density (∇2ρCP) at the bond critical points (BCP) between the Sb atoms is in all cases negative which corresponds to polar covalent interactions. Furthermore, the BCPs in S3 and 3 are closer to the tetravalent than to the trivalent Sb atom, indicating a polarised bond. A stabilising effect resulting from ligand–ligand dispersion interactions in 3/S3 relative to 4/S4 is negligible for the strength of the Sb–Sb bond.
To conclude, stepwise single-electron oxidation and reduction reactions transformed the peri-substituted bisstibanaphthalene (Trip2Sb)2Naph (1) via [(Trip2Sb)(TripSb)Naph][BArF] (3) to the distibane (TripSb)2Naph (4). A very strong donor–acceptor interaction is observed for the stibane-coordinated stibenium cation (3-An), resulting in a short Sb⋯Sb distance that is typical for regular Sb–Sb single bonds. According to quantum chemical calculations, the dative Sb–Sb bond in the related Ph-substituted system S3 is stronger than the covalent Sb–Sb bond in S4 due to orbital interactions.
Financial support by the DFG (SCHU1069/19-2) is acknowledged.
Footnote |
| † Electronic supplementary information (ESI) available: Experimental procedures, NMR and IR spectra, elemental analysis, crystallographic data and details of theoretical study. CCDC 2157418 (1), 2157419 (2), 2157420 (3), and 2157421 (4). For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d2cc01986h |
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