Skip to main content
Wiley Open Access Collection logoLink to Wiley Open Access Collection
. 2019 Oct 17;58(48):17365–17374. doi: 10.1002/anie.201908572

Transition‐Metal Chemistry of Alkaline‐Earth Elements: The Trisbenzene Complexes M(Bz)3 (M=Sr, Ba)

Qian Wang 1,, Sudip Pan 2,4,, Yan‐Bo Wu 3,, Guohai Deng 1, Jian‐Hong Bian 3, Guanjun Wang 1, Lili Zhao 2, Mingfei Zhou 1,, Gernot Frenking 2,4,
PMCID: PMC6900055  PMID: 31498532

Abstract

We report the synthesis and spectroscopic identification of the trisbenzene complexes of strontium and barium M(Bz)3 (M=Sr, Ba) in low‐temperature Ne matrix. Both complexes are characterized by a D 3 symmetric structure involving three equivalent η6‐bound benzene ligands and a closed‐shell singlet electronic ground state. The analysis of the electronic structure shows that the complexes exhibit metal–ligand bonds that are typical for transition metal compounds. The chemical bonds can be explained in terms of weak donation from the π MOs of benzene ligands into the vacant (n−1)d AOs of M and strong backdonation from the occupied (n−1)d AO of M into vacant π* MOs of benzene ligands. The metals in these 20‐electron complexes have 18 effective valence electrons, and, thus, fulfill the 18‐electron rule if only the metal–ligand bonding electrons are counted. The results suggest that the heavier alkaline earth atoms exhibit the full bonding scenario of transition metals.

Keywords: 18-electron rule, alkaline earth metals, benzene complexes, bonding analysis, matrix isolation spectroscopy


Bonding scenarios: The synthesis and spectroscopic identification of the trisbenzene complexes of strontium and barium M(Bz)3 (M=Sr, Ba) in a low‐temperature Ne matrix is reported. The complexes exhibit metal–ligand bonds that are typical for transition‐metal compounds. The results suggest that the heavier alkaline‐earth atoms exhibit the full bonding scenario of transition metals.

graphic file with name ANIE-58-17365-g010.jpg

Introduction

The alkali metals and the alkaline earth elements with a (n)s1 or (n)s2 valence shell configuration, respectively, are the most electropositive elements in the periodic table. These classical s‐block main group elements were for a long time considered to be among the rather uninteresting elements in terms of chemical bonding due to preconceived notions about their valence orbitals, their reactivity and handling.1 They readily lose the outermost (n)s electron(s) to form ionic compounds in the +1 and +2 oxidation states. But recent reports showed that the alkali and alkaline earth elements have a much richer chemistry than hitherto thought.2, 3, 4, 5, 6, 7, 8, 9, 10, 11 In particular, the heavier alkaline earth atoms M=Ca, Sr, Ba may use their (n−1)d functions as genuine valence orbitals in the octa‐coordinated complexes M(CO)8 7 and M(N2)8.11 The cubic (O h) adducts possess metal–ligand bonds that are typical for transition‐metal complexes. The participation of the (n−1)d atomic orbitals (AOs) of barium in chemical bonding had been suggested already in earlier theoretical studies12, 13, 14, 15, 16, 17 and barium was even called by Pyykkö an “honorary transition metal”.17 Recent investigations demonstrated that (n−1)d AO bonding is not restricted to Ba only and that the heavier atoms Ca, Sr, Ba exhibit a transition metal chemistry to a much larger extent than ever known so far.7, 8, 9, 10, 11 Here, we report the isolation and spectroscopic identification of the trisbenzene complexes of heavier alkaline earth atoms M(Bz)3 (M=Sr, Ba). The synthesis of the first transition metal benzene complex Cr(Bz)2 by Fischer and Hafner in 1955 was a milestone in transition metal chemistry.18 The isolation of Sr(Bz)3 and Ba(Bz)3 now opens the door to another chapter of metal complexes.

Results and Discussion

The strontium and barium–benzene complexes were prepared by co‐deposition of laser‐evaporated strontium and barium atoms with benzene molecules in excess neon at 4 K.19 The experiments were performed using relatively low laser energy to avoid the formation of multinuclear species. A series of experiments were performed using different benzene concentrations ranging from 0.025–0.5 %. The IR spectra in the 1650–600 cm−1 region from co‐deposition of laser‐evaporated strontium atoms with 0.1 % C6H6 are represented in Figure 1.

Figure 1.

Figure 1

Infrared absorption spectra of strontium–benzene complexes in the 1650–600 cm−1 region from co‐deposition of laser‐evaporated strontium atoms with 0.1 % C6H6 in neon. a) 30 min of sample deposition at 4 K, b) after annealing at 12 K, c) after 20 min of visible light irradiation.

A group of metal‐dependent product absorptions are observed after sample deposition at 4 K, remain almost unchanged on sample annealing to 12 K and increase under 20 min of visible light excitation using a high pressure mercury arc lamp with a 495 nm long‐wavelength pass filter (λ=495–600 nm). Since some bands are partially overlapped by the benzene absorptions, a difference spectrum taken from the spectrum after visible light excitation minus the spectrum after 12 K annealing is obtained, as shown in Figure 2. The upward bands represent the product absorptions, while the downward bands are due to benzene absorptions. It clearly shows the formation of the product absorptions with the consumption of the benzene absorptions. The bands are quite broad and some bands show site absorptions. Laser evaporation of alkaline earth metal targets might easily lead to formation of cations. In order to verify whether the observed species is a cation or a neutral, additional experiments were performed by adding a trace of CCl4 in the reactant gas to serve as an electron trap.20 CCl4 captures most of electrons produced by laser ablation during sample deposition, and thus would facilitate the survival of more cation products. The spectra from the experiment with 0.01 % CCl4 added to the neon matrix gas are compared to the spectra from the experiment without CCl4 doping in Figure S1 of Supporting Information. The results show that the observed product absorptions are reduced relative to other absorptions, indicating that these product absorptions are due to a neutral species rather than a cation.

Figure 2.

Figure 2

Difference spectra of strontium–benzene complexes in the 1600–500 cm−1 region from co‐deposition of laser‐evaporated strontium atoms with isotopic‐labeled benzene in excess neon (the spectrum taken after 20 min of visible light irradiation minus the spectrum taken after 12 K annealing). a) 0.1 % C6H6, b) 0.2 % 13C6H6, and c) 0.2 % C6D6.

Isotopic substitution experiments (13C6H6, C6D6, and 12C6H6 + 13C6H6) were performed for product identification based on isotopic shifts and absorption splitting. As shown in Figure 2, all the absorptions are shifted with the 13C6H6 and C6D6 samples. The assignment of these product absorptions to the tris(benzene)strontium complex is based on the isotopic splitting of the most intense band at 924.9 cm−1, which is due to the benzene ring breathing mode based on the isotopic data. The spectrum from the experiment using an equimolar mixture of 12C6H6 and 13C6H6 shows that a quartet with two weak intermediates is produced (The low frequency intermediate band is partially overlapped by the strong absorption of Sr(13C6H6)3, See Figure 3). This mixed isotopic spectral feature indicates that the 924.9 cm−1 band is due to a doubly degenerate benzene ring breathing mode of a tris(benzene) complex involving three equivalent benzene ligands. The positions and mode assignment of the observed bands are listed in Table 1. Besides the most intense ring breathing mode, the second most intense band at 1534.8 cm−1 is assigned to the C−C stretching mode. The third strongest band at 1159.1 cm−1 is attributed to the C−H in‐plane bending mode. The remaining bands are weak. The bands at 1332.6 and 1320.1 cm−1 are assigned to mixed modes involving C−C stretching and in‐plane C−H bending. The bands at 933.8 and 810.7 cm−1 are attributed to the out‐of‐plane C−H bending modes.

Figure 3.

Figure 3

Infrared absorption spectra of strontium–benzene complexes in the 960‐860 cm−1 region from co‐deposition of laser‐evaporated strontium atoms with isotopic‐labeled benzene in excess neon (the spectra were taken 20 min of visible light irradiation). a) 0.1 % C6H6, b) 0.15 % 12C6H6 + 0.15 % 13C6H6, and c) 0.2 % 13C6H6.

Table 1.

Experimental infrared absorptions (cm−1) of Sr(C6H6)3, Sr(13C6H6)3 and Sr(C6D6)3 in solid neon and calculated values at the M06‐2X(D3)/def2‐TZVPP level (D 3 symmetry). Calculated IR intensities (km mol−1) are given in parentheses.

Mode

Experimental

Calculated

12C6H6

13C6H6

Δ[a]

12C6D6

Δ[a]

12C6H6

13C6H6

Δ[a]

12C6D6

Δ[a]

C=C stretch

1534.8

1483.0

−51.8

1487.6

−47.2

1556.8

(700)

1506.8

(608)

−50.0

1504.1

(812)

−52.7

C=C stretch and C‐D in‐plane bend

1382.1

1399.6

(54)

C=C stretch and C‐D in‐plane bend

1366.0

1372.2

(21)

C=C stretch and C−H in‐plane bend

1332.6

1286.4

−46.2

1365.3

(49)

1317.5

(47)

−47.8

C=C stretch and C−H in‐plane bend

1320.1

1274.2

−45.9

1346.4

(34)

1299.7

(32)

−46.7

C−H(D) in‐plane bend

1159.1

1151.6

−7.5

844.6

−314.5

1173.3

(119)

1163.4

(155)

−9.9

860.8

(50)

−312.5

C−H(D) in‐plane bend

1094.6

1080.6

−14.0

832.6

−262.0

1141.6

(15)

1129.0

(17)

−12.6

848.5

(65)

−293.1

C−H(D) out‐of‐plane bend

933.8

766.8

−167.0

993.6

(5)

809.0

(53)

−184.6

Ring breath

924.9

895.5

−29.4

898.1

−26.8

968.0

(415)

935.4

(374)

−32.6

936.8

(203)

−31.2

C−H(D) out‐of‐plane bend

810.7

803.1

−7.6

662.0

−148.7

853.1

(58)

845.5

(53)

−7.6

690.2

(50)

−162.9

[a] Shift with respect to 12C6H6.

The Sr(C6H6)3 absorptions are the only product absorptions observed in the experiments using different benzene concentrations as well as laser energy. The spectra from experiments using different laser energy are shown in Figure S2. There is no any experimental evidence of formation of the Sr(C6H6) and Sr(C6H6)2 complexes in these experiments.

Similar absorptions are also observed in the barium experiments. The IR spectra are shown in Figure 4. All the absorptions are observed on sample deposition and increase on sample annealing to 10 K and 12 K, and remain almost unchanged under visible light irradiation (λ=495–600 nm), but decrease upon UV‐visible light irradiation using the high pressure mercury arc lamp without filters (λ=250–600 nm). The band positions are only slightly blue‐ or red‐shifted with respect to the corresponding modes of tris(benzene)strontium (within 10 cm−1 difference). The spectra from the isotopic‐labeled experiments are shown in Figures S3 and S4. The band positions are listed in Table 2. No similar product absorptions are observed in the experiments with calcium.

Figure 4.

Figure 4

Infrared absorption spectra of barium–benzene complexes in the 1650–600 cm−1 region from co‐deposition of laser‐evaporated barium atoms with 0.1 % C6H6 in neon. a) 30 min of sample deposition at 4 K, b) after annealing at 10 K, c) after annealing to 12 K, and d) after 20 min of UV‐visible light irradiation.

Table 2.

Experimental infrared absorptions (cm−1) of Ba(C6H6)3, Ba(13C6H6)3 and Ba(C6D6)3 in solid neon and calculated values at the M06‐2X(D3)/def2‐TZVPP level (D 3 symmetry). Calculated IR intensities (km mol−1) are given in parentheses.

Mode

Experimental

Calculated

12C6H6

13C6H6

Δ[a]

12C6D6

Δ[a]

12C6H6

13C6H6

Δ[a]

12C6D6

Δ[a]

C=C stretch

1529.0

1479.5

−49.5

1486.7

−42.3

1575.0

(651)

1523.7

(562)

−51.3

1523.1

(769)

−51.9

C=C stretch and C‐D in‐plane bend

1382.2

1438.9

(124)

C=C stretch and C‐D in‐plane bend

1360.7

1386.8

(50.2)

C=C stretch and C−H in‐plane bend

1327.1

1281.9

−45.2

1360.3

(76)

1312.0

(70)

−48.3

C=C stretch and C−H in‐plane bend

1318.4

1272.2

−46.2

1343.6

(18)

1296.9

(17)

−46.7

C−H(D) in‐plane bend

1153.6

1145.0

−8.6

845.2

−308.4

1172.7

(152)

1163.1

(180)

−9.6

858.4

(40)

−314.3

C−H(D) in‐plane bend

1084.6

1073.0

−11.6

838.7

−245.9

1144.1

(2)

1130.5

(3)

−13.6

853.8

(98)

−290.3

C−H(D) out‐of‐plane bend

932.2

766.9

−165.3

986.5

(8)

801.5

(70)

−185.0

Ring breath

925.8

894.8

−31

899.2

−26.6

969.4

(472)

937.0

(430)

−32.4

937.8

(224)

−31.6

C−H(D) out‐of‐plane bend

813.8

806.8

−7.0

665.1

−148.7

831.2

(11)

824.3

(11)

−6.9

659.4

(4)

−171.8

[a] Shift with respect to 12C6H6.

We calculated the trisbenzene complexes M(Bz)3 (M=Ca, Sr, Ba) and analyzed their electronic structures with quantum chemical methods using density functional theory (DFT) at the M06‐2X(D3)/def2‐TZVPP level of theory, which considers also dispersion interactions. Details of the methods are given in Supporting Information. The calcium complex was also included in the theoretical work in order to provide a comparison with the experimentally observed strontium and barium adducts.

The geometry optimizations give D 3 symmetric M(Bz)3 equilibrium structures with a singlet (1A1) electronic state as energy minima (Figure 5 a). The benzene ligands are distorted from their D 6h geometry in the free molecules to C 2 symmetric fragments with two C−C distances being significantly longer (1.420–1.423 Å) than in free benzene (1.388 Å), while the other C−C bond lengths are only slightly altered. Calculations with enforced D 3h symmetry give structures being marginally higher in energy than the D 3 form (Figure 5 b). The D 3h structures of Ca(Bz)3 and Sr(Bz)3 have 3 imaginary frequencies, but the D 3h form of Ba(Bz)3 is calculated as energy minimum, which is only 0.2 kcal mol−1 less stable than the D 3 structure. The D 3h structures of M(Bz)3 have four C−C bonds that are clearly longer (1.411–1.412 Å) than in free benzene while two C−C bonds are a bit shortened (1.382–1.384 Å). The corresponding triplet states of M(Bz)3 posses C 1 symmetry for M=Ca and C 2 symmetry for M=Sr, Ba and they are 0.6–3.8 kcal mol−1 higher in energy than the singlet D 3 structures (see Figure S5).

Figure 5.

Figure 5

Calculated geometries of M(Bz)3 and M(Bz)2 complexes (M=Ca, Sr, Ba) at M06‐2X‐D3/def2‐TZVPP. Bond distances are in Å, Relative energies are in kcal mol−1.

Table 3 shows the bond dissociation energies (BDEs) of M(Bz)3 for the loss of one or all three benzene ligands. The calculations suggest that the BDE of one ligand ranges between D e=19.4 kcal mol−1 for M=Ca and D e=26.1 kcal mol−1 for M=Sr. The BDEs at room temperature become smaller after correcting for thermodynamic contributions, having values between ΔG 298=6.5 kcal mol−1 (Ca) and ΔG 298=14.2 kcal mol−1 (Sr). The total BDEs for fragmentation into three benzene molecules are between D e=38.6 kcal mol−1 (Ca) and D e=46.0 kcal mol−1 (Ba), but the free energies at room temperature are significantly smaller having values between ΔG 298=8.7 kcal mol−1 (Ca) and ΔG 298=19.5 kcal mol−1 (Ba). Note that the latter process includes the electronic relaxation of the metal atoms to the 1S electronic ground state. The lower BDE of the calcium complex may be the reason why Ca(Bz)3 could not be observed experimentally.

Table 3.

Calculated bond dissociation energies of M(Bz)3 complexes for the loss of one Bz and three Bz molecules at the M06‐2X‐D3/def2‐TZVPP level. The D e values give the electronic energies, the D 0 data include the corrections by zero‐point vibrational frequencies and the ΔG 298K values consider the thermodynamic and vibrational corrections at room temperature.

Reaction

M

D e

D 0

ΔG 298K

M(Bz)3 (D 3, 1A1) → M(Bz)2 (C 2v, 1A1) + Bz

Ca

19.4

18.3

6.5

Sr

26.1

25.3

14.2

Ba

24.0

23.6

13.4

M(Bz)3 (D 3, 1A1) → M (1S) + 3 Bz

Ca

38.6

38.3

8.7

Sr

39.2

39.7

11.0

Ba

46.0

47.1

19.5

The calculated infrared signals of the M(Bz)3 complexes and their 13C and deuterated isotopes in the region >600 cm−1 as well as the frequency shifts are shown in Tables 1 and 2. The agreement of the computed unscaled values of the harmonic frequencies with the experimental values of the anharmonic mode is quite good. The calculated isotopic frequency shifts are also in very good accord with the recorded spectra. The comparison between the calculated and observed IR spectra leaves no doubt that the experimentally observed species are the neutral trisbenzene complexes M(Bz)3 (M=Sr, Ba). The radical cations [M(Bz)3]+ (M=Sr, Ba) were also calculated. The optimized structures are shown in Figure S6. Both cations are predicted to have D3 symmetric structures with a doublet (2A1) electronic ground state. The calculated vibrational frequencies and intensities are listed in Tables S1 and S2, respectively. Both cations are predicted to have two intense well‐separated C=C stretching modes. Therefore, the assignment of the experimentally observed species to the radical cations can clearly be ruled out, as only one C=C stretching band is observed experimentally.

The complexes M(Bz)3 (M=Ca, Sr, Ba) are formally 20‐electron species possessing a singlet (1A1) electronic ground state. Our previously reported isoelectronic alkaline earth complexes M(CO)8 7 and M(N2)8 11 are 18‐electron adducts with cubic (O h) symmetry that possess a triplet (3A1g) ground state. The latter molecules have two singly occupied degenerate orbitals and one lower lying ligand‐based molecular orbital (MO) with a2u symmetry that has zero coefficient at the metal, because it has no valence AO having proper symmetry. We earlier reported the observation of the 20‐electron transition metal octa‐carbonyl anions [TM(CO)8] (TM=Sc, Y, La).21 These complexes also have cubic symmetry but a singlet (1A1g) ground state, where the degenerate HOMO is fully occupied. The 18‐electron rule first suggested by Langmuir22 remains valid in the above complexes, if only the metal–ligand bonding electrons are counted.

Figure 6 a shows the orbital correlation diagram for the splitting of the (n)s(n)p(n−1)d AOs of alkaline earth atoms in the D 3h field of three benzene ligands along with plots of the associated occupied MOs of M(Bz)3. In the D 3h symmetry field, the five d orbitals of metal split into three irreducible representations (a1′ + e′ + e′′). The a1′ orbital, which is the dz2 AO of the metal, provides backdonation to the antibonding π* orbital of the benzene ligands leading to the bonding MO (2a1′). The remaining eight metal AOs serve as acceptor orbitals for the charge donation from the bonding π orbitals of the benzene ligands. There are nine symmetry‐adapted linear combination orbitals from the bonding π orbitals of three benzene ligands. The 1a2′ MO remains as a ligand‐only orbital, because there is no valence AO of the metal possessing this symmetry. All of these bonding and nonbonding orbitals are doubly occupied, resulting in a closed‐shell singlet ground state. Thus, the M(Bz)3 complexes have a total of 20 valence electrons, but the metal centers have only 18 effective valence electrons, and thus still fulfill the 18‐electron rule if only the metal–ligand bonding electrons are considered.

Figure 6.

Figure 6

MO correlation diagram of the valence (n)s(n)p(n−1)d AOs of M and (C6H6)3 in a) D 3h symmetry and b) D 3 symmetry. Shapes of the MOs of Ba(Bz)3 are also shown.

Figure 6 b shows the related orbital diagram for M(Bz)3 in the D 3 field of the benzene ligands at the equilibrium geometries and the shape of the occupied MOs of M(Bz)3. Comparing the latter MOs with the D 3h orbitals shows only negligible differences. The 2a2 MO of the D 3 form takes the position of the 2a2′ MO of the D 3h form and could, in principle, mix with one (n)p AO of the metal. Inspection of the MO coefficients shows that the contribution of the (n)p AO of the metal is nearly zero. Thus, the pattern of the orbital interaction of the D 3 structures is very similar to the D 3h form. We think that the deviation from perfect D 3h geometry of the M(Bz)3 complexes is due to weak steric interactions between the benzene ligands, which have a negligible effect on the orbital interactions. This corresponds to the reduction of the energy difference between the D 3 and D 3h forms of M(Bz)3 having the order of Ca>Sr>Ba, because the metal–ligand bonds and thus the ligand–ligand distances increase (Figure 5).

On the basis of above bonding analysis, it is clear that the M(Bz)3 complexes can be regarded as being formed via the interactions between the metal atoms in the singlet excited state with an (n−1)d2ns0np0 electron configuration and three benzene ligands in the singlet state. The strength of the pairwise orbital interactions can be estimated with the EDA‐NOCV (energy decomposition analysis in combination with natural orbitals for chemical valence) method.23 Details of the method have been described in the literature.24, 25, 26 The calculations at M06‐2X with the Slater basis functions TZ2P of the ADF program for M in the singlet excited state with d2 configuration did not converge. Therefore, we used the BP86‐D3(BJ) functional in conjunction with the TZ2P basis set. Our experience in numerous studies has shown that the EDA‐NOCV calculations are not very sensitive to the functional.27, 28, 29, 30, 31, 32, 33, 34, 35, 36, 37 Table 4 gives the numerical results of the calculations of M(Bz)3 (M=Ca, Sr, Ba) at the D 3 equilibrium structures.

Table 4.

Results of EDA‐NOCV calculations at BP86‐D3(BJ)/TZ2P for M(Bz)3 (D 3, 1A1) complexes using neutral atoms M in the singlet state with ns0np0(n−1)d2 electron configuration and (Bz)3 (singlet) as interacting fragments.

Term

Interaction

Ca (S, 4s04p03d2) + (Bz)3 (S)

Sr (S, 5s05p04d2) + (Bz)3 (S)

Ba (S, 6s06p05d2) + (Bz)3 (S)

ΔE int

−197.4

−191.5

−135.5

ΔE Pauli

124.5

140.5

156.8

ΔE disp [a]

−7.1 (2.2 %)

−8.4 (2.5 %)

−16.8 (5.7 %)

ΔE elstat [a]

−82.7 (25.7 %)

−88.8 (26.8 %)

−116.4 (39.8 %)

ΔE orb [a]

−232.1 (72.1 %)

−234.7 (70.7 %)

−159.1 (54.4 %)

ΔE orb(1) [b] (2a1)

(Bz)3←M(d) backdonation

−191.8 (82.6 %)

−189.9 (80.9 %)

−119.9 (75.4 %)

ΔE orb(2) [b] (3e)

(Bz)3→M(d) donation

−14.0 (6.0 %)

−16.8 (7.2 %)

−16.8 (10.6 %)

ΔE orb(3) [b] (2e)

(Bz)3→M(d) donation

−13.6 (5.9 %)

−15.0 (6.4 %)

−11.8 (7.4 %)

ΔE orb(4) [b] (1a1)

(Bz)3→M(s) donation

−2.7 (1.2 %)

−2.9 (1.2 %)

−2.1 (1.3 %)

ΔE orb(5) [b] (1a2)

(Bz)3→M(p) donation

−1.4 (0.6 %)

−1.3 (0.6 %)

−0.8 (0.5 %)

ΔE orb(6) [b] (1e)

(Bz)3→M(p) donation

−3.2 (1.4 %)

−2.4 (1.0 %)

−0.8 (0.5 %)

ΔE orb(7) [b] (1a2)

Polarization

−1.3 (0.6 %)

−1.8 (0.8 %)

−2.5 (1.6 %)

ΔE orb(rest) [b]

−4.1 (1.8 %)

−4.6 (2.0 %)

−4.4 (2.8 %)

[a] The values in parentheses give the percentage contribution to the total attractive interactions ΔE elstat + ΔE orb + ΔE disp. [b] The values in parentheses give the percentage contribution to the total orbital interactions ΔE orb.

The data in Table 4 suggest that the M‐(Bz)3 attractive interactions come mainly from the covalent term ΔE orb, which provides between 72 % (M=Ca) and 54 % (M=Ba) to the total attraction. The breakdown of ΔE orb into pairwise orbital interactions shows that the dominant contribution ΔE orb(1) comes from the backdonation of the occupied (n−1)d AO of the metal into the vacant π* orbitals of the ligands denoted as (Bz)3←M(d). This orbital interaction contributes between 83 % (M=Ca) and 75 % (M=Ba) to ΔE orb. The following terms ΔE orb(2) and ΔE orb(3) also involve the (n−1)d AOs of the metals. They are due to the donation from two sets of degenerate occupied π MOs of the ligands into vacant (n−1)d metal AOs denoted as (Bz)3→M(d). Thus, the valence AOs of the metals that contribute to the metal–ligand bonding are dominated by the (n−1)d orbitals.

The assignment of the ΔE orb(1) interaction to (Bz)3←M(d), which has a1 symmetry, may be questioned because the MO diagram shows that the metal (n)s AO correlates in a D 3 environment also with a1 symmetric MOs (Figure 6 b). Inspection of the related deformation density Δρ 1 and the associated orbitals reveals that the contribution of the metal (n)s AO to the 2a1 MO is negligible. Also, the EDA‐NOCV calculation of the D 3h structures of M(Bz)3 gives values that are very similar to the D 3 analysis. The numerical results of the EDA‐NOCV calculation using the D 3h structures are shown in Table S3. Figure 7 displays the shape of the deformation densities Δρ 1−Δρ 7 of Ba(Bz)3 which nicely illustrate the charge alteration due to the pairwise orbital interactions ΔE orb(1)−ΔE orb(7). The color code of the charge flow is red → blue. The deformation densities Δρ 1−Δρ 7 of M(Bz)3 calculated with D 3h symmetry are displayed in Figures S7–S9. The shape of Δρ 7 clearly reveals that the small stabilization energy ΔE orb(7) is solely due to the polarization of the ligand orbitals. The deformation densities Δρ 1−Δρ 7 of Ca(Bz)3 and Sr(Bz)3 closely resemble those of Ba(Bz)3. They are shown in Figures S10 and S11.

Figure 7.

Figure 7

Shape of the deformation densities Δρ (1)‐(7), which are associated with the orbital interactions ΔE orb(1)‐(7) between neutral fragments Ba and (Bz)3 in Ba(Bz)3 (D 3, 1A1) complex, using Ba (S, 6s06p05d2) + (Bz)3 (S) as interacting complexes (Table 4), and eigenvalues |νn| of the charge flow. The color code of the charge flow is red → blue. The isosurface values are 0.002 for Δρ (1), 0.0005 for Δρ (2)‐(4) and 0.0004 for Δρ (5)‐(7).

One referee pointed out that the choice of the electronic reference states of the fragments is somewhat arbitrary and that the same state can be obtained from a ground state metal atom and excited benzene molecules, which would yield a different pattern of donation and back‐donation. This is a justified objection, which needs to be addressed. The electronic ground state of the metal atoms has the electron configuration (n)s2, which transforms to a1′ in D 3h symmetry. But the shape of the occupied 1a1′ MO of the complex Ba(Bz)3 shown in Figure 6 a reveals that the 6s AO of Ba has a negligible coefficient in the molecular orbital of the complex, which has only slightly distorted ligand orbitals. The same situation is found in the D 3 symmetric structure (Figure 6 b). The visual impression is supported by EDA‐NOCV calculations of the complexes M(Bz)3 using the atoms M in the electronic ground state configuration (n)s2 and (Bz)3 in the doubly excited singlet state with two electrons in the π* MO. It has been shown by us in numerous studies that those fragments, which give the smallest absolute values for the orbital term ΔE orb, are the most suitable species to represent the bonding of the complex, since they change the least in the formation of the bond. This method has proven to be very helpful for a large number of chemical compounds whose nature is not directly apparent.27, 28, 29, 30, 31, 32, 33, 34, 35, 36, 37 Tables S4–S6 show that the ΔE orb values using atom M in the electronic ground state and (Bz)3 in the excited state are significantly larger than those in Table 4.

However, there is an alternative option for the choice of the interacting fragments. The calculated partial charges of M(Bz)3 using the NBO 6.0 method38 suggest large positive charges for the metal atoms of 1.47 for Ca, 1.46 for Sr and 1.40 for Ba. The choice of neutral fragments in the electronic references states for M(Bz)3 follows the Dewar–Chatt–Duncanson (DCD) model for transition metal compounds, which considers the metal atom and the ligands prior to bond formation.39 But the formation of chemical bonds can lead to large charge transfers, resulting in an electronic structure of the molecule that differs greatly from the initial components.

We carried out EDA‐NOCV calculations using charged fragments as interacting moieties. We found that the lowest ΔE orb value is given when the singly charged species M+ in the doublet state with the electron configuration (n−1)d1ns0np0 and doublet (Bz)3 are employed as interacting fragments. Fragments with other charges or electron configurations give larger ΔE orb values (see the numerical results in Tables S4–S6 in Supporting Information). Table 5 shows the numerical EDA‐NOCV results for the M+‐(Bz)3 interactions.

Table 5.

Results of EDA‐NOCV calculations at BP86‐D3(BJ)/TZ2P for M(Bz)3 (D 3, 1A1) complexes using positively charged atoms M+ in the doublet state with ns0np0(n−1)d1 electron configuration and negatively charged (Bz)3 (D) as interacting fragments.

Term

Interaction

Ca+ (D, 4s04p03d1) + (Bz)3 (D)

Sr+ (D, 5s05p04d1) + (Bz)3 (D)

Ba+ (D, 6s06p05d1) + (Bz)3 (D)

ΔE int

−232.9

−228.9

−207.0

ΔE Pauli

71.4

85.6

110.1

ΔE disp [a]

−7.1 (2.3 %)

−8.4 (2.7 %)

−16.8 (5.3 %)

ΔE elstat [a]

−155.0 (50.9 %)

−159.0 (50.6 %)

−176.7 (55.8 %)

ΔE orb [a]

−142.2 (46.7 %)

−147.0 (46.8 %)

−123.4 (38.9 %)

ΔE orb(1) [b] (2a1)

(Bz)3‐M(d) electron‐sharing

−70.9 (49.9 %)

−76.7 (52.2 %)

−53.7 (43.5 %)

ΔE orb(2) [b] (3e)

(Bz)3→M(d) donation

−20.4 (14.3 %)

−22.0 (15.0 %)

−24.2 (19.6 %)

ΔE orb(3) [b] (2e)

(Bz)3→M(d) donation

−19.4 (13.6 %)

−19.4 (13.2 %)

−18.4 (14.9 %)

ΔE orb(4) [b] (1a1)

(Bz)3→M(s) donation

−5.5 (3.9 %)

−5.1 (3.5 %)

−4.0 (3.2 %)

ΔE orb(5) [b] (1a2)

(Bz)3→M(p) donation

−3.3 (2.3 %)

−2.7 (1.8 %)

−2.4 (1.9 %)

ΔE orb(6) [b] (1e)

(Bz)3→M(p) donation

−6.6 (4.6 %)

−3.0 (2.0 %)

−3.8 (3.1 %)

ΔE orb(7) [b] (1a2)

Polarization

−2.6 (1.8 %)

−3.0 (2.0 %)

−4.3 (3.5 %)

ΔE orb(rest) [b]

−13.5 (9.5 %)

−15.1 (10.3 %)

−12.6 (10.2 %)

[a] The values in parentheses give the percentage contribution to the total attractive interactions ΔE elstat + ΔE orb + ΔE disp. [b] The values in parentheses give the percentage contribution to the total orbital interactions ΔE orb.

The data in Table 5 show that the covalent term ΔE orb is now a bit smaller than the Coulombic attraction ΔE elstat. The strongest pairwise orbital interaction ΔE orb(1) between the fragments in the electronic doublet state comes from the electron‐sharing bond formation between the unpaired electrons of M+ and (Bz)3 . It is interesting to see that the associated deformation density Δρ 1 shown in Figure 8 exhibits a very similar shape as the dative interaction of ΔE orb(1) when neutral fragments are used (Figure 7). It means that the electron‐sharing interactions between the (n−1)d electron of M+ and the unpaired electron of (Bz)3 have a polarity from the metal towards the ligands. As can be expected, the associated eigenvalue υ1, which indicates the magnitude of the net charge flow, is much smaller for the charged fragments than for the neutral fragments. The relative contribution of the 2a1 orbital interaction between the charged fragments is smaller than the dominating 2a1 term of the neutral fragments, whereas the 2e and 3e orbital terms that come from (Bz)3→M(d) π donation are larger when charged fragment are used. But the most relevant results is the finding that the (n−1)d AOs of the metal are still clearly the most important valence orbitals for covalent metal‐(Bz)3 binding even when charged fragments are used for the EDA‐NOCV calculations.

Figure 8.

Figure 8

Shape of the deformation densities Δρ (1)‐(7), which are associated with the orbital interactions ΔE orb(1)‐(7) in Ba(Bz)3 (D 3, 1A1) complex, using Ba+ (D, 6s06p05d1) + (Bz)3 (D) as interacting complexes (Table 5), and eigenvalues |νn|of the charge flow. The color code of the charge flow is red → blue. The isosurface values are 0.001 for Δρ (1), 0.0005 for Δρ (2)‐(4)and 0.0004 for Δρ (5)‐(7). aNet charge flow of the electron‐sharing interactions.

The two sets of EDA‐NOCV results in Tables 4 and 5 address two different questions. The dissociation of M(Bz)3 gives neutral atoms M and three neutral ligands Bz and the data in Table 4 provide information about the total charge flow taking place during bond formation. The latter results directly refer to the DCD model and to orbital correlation diagrams, which always take the orbitals of the fragments prior to bond formation for explaining molecular structures and reactivities.40 The data in Table 5 give information about the best description of the bonding situation in the eventually formed complexes, which is given in terms of interactions between the metal ion M+ and the negatively charged ligand cave (Bz)3 . EDA‐NOCV calculations using the doubly charged fragments M2+ and (Bz)3 2− give larger ΔE orb values (Tables S4–S6, last columns) than singly charged fragments. The results in Tables 4 and 5 demonstrate the variability of the EDA‐NOCV method, which provides quantitative answer to the questions about the binding interactions between fragments prior and after the bond formation. The difference between the two situations is sometimes not recognized, which has led to a misunderstanding of the EDA‐NOCV results by some authors.41

Benzene is an excellent ligand in the organometallic chemistry of low‐valent transition metals. Since the first synthesis of bis(benzene)chromium Cr(Bz)2,18 a large number of sandwich or half‐sandwich transition metal compounds involving one or two benzene ligands have been reported.42 Although main group metal cation–benzene complexes43 as well as organometallic complexes of the alkaline earth cations such as metallocene complexes that feature ionic bonding with no propensity for π backbonding are quite common,44, 45, 46, 47, 48 sandwich complexes of neutral alkaline earth metals, in particular with three η6‐bound benzene ligands, are unprecedented. In the literature, only very few metallocene complexes of actinides involving three η5‐bound cyclopendadienyl ligands have been reported.49 The successful synthesis of trisbenzene complexes of heavier alkaline earth metals may open the door to another chapter of metal complexes.

The observation of the alkaline earth trisbenzene complexes M(Bz)3 is not just a surprising finding of some exotic species. It seems that the bonding situation of the arene complexes plays also an important role in some intermediates of alkaline earth catalyzed reactions. Alonso, Harder and co‐workers recently reported the alkene hydrogenation catalyzed by simple compounds of the alkaline earth elements Ca, Sr, Ba.4 The calculated reaction profile identified a species D3 where Ca is sandwiched between two aromatic rings (Figure 9). The structure of D3 closely resembles the metal–ligand bonds in M(Bz)3. A similar situation was reported by the group for the alkaline earth catalyzed imine hydrogenation.5 The involvement of the valence‐d orbitals of Ca may also be involved in the recently reported organocalcium‐mediated nucleophilic alkylation of benzene.3 The transition‐metal like chemical reactivity of Ca, Ba, Sr is perhaps more relevant for synthetic chemistry than hitherto thought.

Figure 9.

Figure 9

Calculated structure D3 of a calcium compound sandwiched between two aromatic rings, which is relevant in the hydrogenation of alkene catalyzed by alkaline earth atoms. The Figure is adapted from reference 4.

Conclusion

In summary, we report the synthesis and spectroscopic identification of the unprecedented trisbenzene complexes M(Bz)3 (M=Sr, Ba) featuring three equivalent η6‐bound benzene ligands in low‐temperature Ne matrix. The analysis of the electronic structure shows that the complexes exhibit metal–ligand bonds that are typical for transition metal compounds. The chemical bonds can be explained in terms of weak donation from the π MOs of benzene ligands into the vacant (n−1)d AOs of M and strong backdonation from the occupied (n−1)d AO of M into vacant π* MOs of benzene ligands. The metals in these 20‐electron complexes have 18 effective valence electrons, and thus still fulfill the 18‐electron rule, because two valence electrons occupy a ligand‐based MO that has zero coefficient at the metal. The results suggest that the heavier earth alkaline atoms Ca, Sr, Ba may exhibit the full bonding scenario of transition metals.

Conflict of interest

The authors declare no conflict of interest.

Supporting information

As a service to our authors and readers, this journal provides supporting information supplied by the authors. Such materials are peer reviewed and may be re‐organized for online delivery, but are not copy‐edited or typeset. Technical support issues arising from supporting information (other than missing files) should be addressed to the authors.

Supplementary

Acknowledgements

The experimental work was supported by the National Natural Science Foundation of China (grant numbers 21688102 and 21433005). L.Z. and G.F. acknowledge financial support from Nanjing Tech University (grant numbers 39837123, 39837132) and SICAM Fellowship from Jiangsu National Synergetic Innovation Center for Advanced Materials, Natural Science Foundation of Jiangsu Province for Youth (grant number BK20170964), National Natural Science Foundation of China (grant number 21703099). S.P. thanks Nanjing Tech University for a postdoctoral fellowship and the High Performance Center of Nanjing Tech University for the computational resources. Y.W. thanks National Natural Science Foundation of China (grant number 21273140) for financial support and the High Performance Center of Shanxi University for the computational resources.

Q. Wang, S. Pan, Y.-B. Wu, G. Deng, J.-H. Bian, G. Wang, L. Zhao, M. Zhou, G. Frenking, Angew. Chem. Int. Ed. 2019, 58, 17365.

Dedicated to Professor Christian Reichardt on the occasion of his 85th birthday

Contributor Information

Mingfei Zhou, Email: mfzhou@fudan.edu.cn.

Gernot Frenking, Email: frenking@chemie.uni-marburg.de.

References

  • 1. Chirik P. J., Organometallics 2019, 38, 195–197. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 2. Schafer L., Hill M., Tonks I., Organometallics 2018, 37, 4311–4312. [Google Scholar]
  • 3. Wilson A. S. S., Hill M. S., Mahon M. F., Dinoi C., Maron L., Science 2017, 358, 1168–1171. [DOI] [PubMed] [Google Scholar]
  • 4. Bauer H., Alonso M., Fischer C., Rösch B., Elsen H., Harder S., Angew. Chem. Int. Ed. 2018, 57, 15177–15182; [DOI] [PubMed] [Google Scholar]; Angew. Chem. 2018, 130, 15397–15402. [Google Scholar]
  • 5. Bauer H., Alonso M., Färber C., Elsen H., Pahl J., Causero A., Ballmann G., De Proft F., Harder S. J., Nat. Catal. 2018, 1, 40–47. [Google Scholar]
  • 6. Wu X., Zhao L., Jiang D. D., Fernandez I., Berger R., Zhou M. F., Frenking G., Angew. Chem. Int. Ed. 2018, 57, 3974–3980; [DOI] [PubMed] [Google Scholar]; Angew. Chem. 2018, 130, 4038–4044. [Google Scholar]
  • 7. Wu X., Zhao L., Jin J. Y., Pan S., Li W., Jin X. Y., Wang G. J., Zhou M. F., Frenking G., Science 2018, 361, 912–916. [DOI] [PubMed] [Google Scholar]
  • 8. Armentrout P. B., Science 2018, 361, 849–850. [DOI] [PubMed] [Google Scholar]
  • 9. Yang X. M., Nat. Sci. Rev. 2019, 6, 8–9. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 10. Chi C. X., Pan S., Meng L. Y., Luo M. B., Zhao L., Zhou M. F., Frenking G., Angew. Chem. Int. Ed. 2019, 58, 1732–1738; [DOI] [PubMed] [Google Scholar]; Angew. Chem. 2019, 131, 1746–1752. [Google Scholar]
  • 11. Wang Q., Pan S., Lei S. J., Jin J. Y., Deng G. H., Wang G. J., Zhao L. L., Zhou M. F., Frenking G., Nat. Commun. 2019, 10, 3375. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 12. Kaupp M., Schleyer P. v. R., Stoll H., Preuss H., J. Am. Chem. Soc. 1991, 113, 6012–6020. [Google Scholar]
  • 13. Kaupp M., Schleyer P. v. R., Stoll H., Preuss H., J. Chem. Phys. 1991, 94, 1360–1366. [Google Scholar]
  • 14. Kaupp M., Schleyer P. v. R., J. Am. Chem. Soc. 1992, 114, 491–497. [Google Scholar]
  • 15. Pyykko P., J. Chem. Soc. Faraday Trans. 2 1972, 75, 1256. [Google Scholar]
  • 16. Gagliardi L., J. Am. Chem. Soc. 2002, 124, 8757–8761. [DOI] [PubMed] [Google Scholar]
  • 17. Gagliardi L., Pyykko P., Theor. Chem. Acc. 2003, 110, 205–210. [Google Scholar]
  • 18. Fischer E. O., Hafner W., Z. Naturforsch. B 1955, 10, 665. [Google Scholar]
  • 19. Wang G. J., Zhou M. F., Int. Rev. Phys. Chem. 2008, 27, 1–25. [Google Scholar]
  • 20. Zhou M. F., Andrews L., J. Am. Chem. Soc. 1998, 120, 11499–11503. [Google Scholar]
  • 21. Jin J. Y., Yang T., Xin K., Wang G. J., Wang X. F., Zhou M. F., Frenking G., Angew. Chem. Int. Ed. 2018, 57, 6236–6241; [DOI] [PubMed] [Google Scholar]; Angew. Chem. 2018, 130, 6344–6349. [Google Scholar]
  • 22. Langmuir I., Science 1921, 54, 59–67. [DOI] [PubMed] [Google Scholar]
  • 23. Mitoraj M. P., Michalak A., Ziegler T., J. Chem. Theory Comput. 2009, 5, 962–975. [DOI] [PubMed] [Google Scholar]
  • 24. Zhao L., Schwarz W. H. E., Frenking G., Nat. Rev. Chem. 2019, 3, 48–63. [Google Scholar]
  • 25. Zhao L., von Hopffgarten M., Andrada D. M., Frenking G., WIREs Comput. Mol. Sci. 2018, 8, e1345. [Google Scholar]
  • 26. Frenking G., Bickelhaupt F. M. in The Chemical Bond. Fundamental Aspects of Chemical Bonding (Eds.: G. Frenking, S. Shaik), Wiley-VCH, Weinheim, 2014, p. 121–158. [Google Scholar]
  • 27. Zhang Q., Li W.-L., Xu C., Chen M., Zhou M., Li J., Andrada D. M., Frenking G., Angew. Chem. Int. Ed. 2015, 54, 11078–11083; [DOI] [PubMed] [Google Scholar]; Angew. Chem. 2015, 127, 11230–11235. [Google Scholar]
  • 28. Andrada D. M., Frenking G., Angew. Chem. Int. Ed. 2015, 54, 12319–12324; [DOI] [PubMed] [Google Scholar]; Angew. Chem. 2015, 127, 12494–12500. [Google Scholar]
  • 29. Mohapatra C., Kundu S., Paesch A. N., Herbst-Irmer R., Stalke D., Andrada D. M., Frenking G., Roesky H. W., J. Am. Chem. Soc. 2016, 138, 10429–10432. [DOI] [PubMed] [Google Scholar]
  • 30. Scharf L. T., Andrada D. M., Frenking G., Gessner V. H., Chem. Eur. J. 2017, 23, 4422–4434. [DOI] [PMC free article] [PubMed] [Google Scholar]
  • 31. Hermann M., Frenking G., Chem. Eur. J. 2017, 23, 3347–3356. [DOI] [PubMed] [Google Scholar]
  • 32. Georgiou D. C., Zhao L., Wilson D. J. D., Frenking G., Dutton J. L., Chem. Eur. J. 2017, 23, 2926–2934. [DOI] [PubMed] [Google Scholar]
  • 33. Wu Z., Xu J., Sokolenko L., Yagupolskii Y. L., Feng R., Liu Q., Lu Y., Zhao L., Fernández I., Frenking G., Trabelsi T., Francisco J. S., Zeng X., Chem. Eur. J. 2017, 23, 16566–16573. [DOI] [PubMed] [Google Scholar]
  • 34. Petz W., Andrada D. M., Hermann M., Frenking G., Neumüller B., Z. Anorg. Allg. Chem. 2017, 643, 1096–1099. [Google Scholar]
  • 35. Andrada D. M., Casalz-Sainz J. L., Pendas A. M., Frenking G., Chem. Eur. J. 2018, 24, 9083–9089. [DOI] [PubMed] [Google Scholar]
  • 36. Jerabek P., Schwerdtfeger P., Frenking G., J. Comput. Chem. 2019, 40, 247–264. [DOI] [PubMed] [Google Scholar]
  • 37. Saha R., Pan S., Merino G., Chattaraj P. K., Angew. Chem. Int. Ed. 2019, 58, 8372–8377; [DOI] [PubMed] [Google Scholar]; Angew. Chem. 2019, 131, 8460–8465. [Google Scholar]
  • 38. Glendening E. D., Landis C. R., Weinhold F., J. Comput. Chem. 2013, 24, 1429–1437. [DOI] [PubMed] [Google Scholar]
  • 39. 
  • 39a. Dewar M. J. S., Bull. Soc. Chim. Fr. 1951, 18, C79; [Google Scholar]
  • 39b. Chatt J., Duncanson L. A., J. Chem. Soc. 1953, 2939–2947; [Google Scholar]
  • 39c. Frenking G., Fröhlich N., Chem. Rev. 2000, 100, 717–774; [DOI] [PubMed] [Google Scholar]
  • 39d. Frenking G., J. Organomet. Chem. 2001, 635, 9–23. [Google Scholar]
  • 40. Albright T. A., Burdett J. K., Whangbo M.-H., Orbital Interactions in Chemistry , 2nd ed., Wiley, New York, 2013. [Google Scholar]
  • 41. 
  • 41a. Landis C. R., Hughes R. P., Weinhold F., Organometallics 2015, 34, 3442–3449; [Google Scholar]
  • 41b.see also the recent controversy about the nature of the chemical bonds in the alkaline earth octacarbonyls in Landis C. R., Hughes R. P., Weinhold F., Science 2019, 10.1126/science.aay2355; [DOI] [Google Scholar]
  • 41c. Zhao L., Pan S., Zhou M., Frenking G., Science 2019, 10.1126/science.aay5021. [DOI] [PubMed] [Google Scholar]
  • 42. 
  • 42a. Seyferth D., Organometallics 2002, 21, 2800–2820; [Google Scholar]
  • 42b. Duncan M. A., Int. J. Mass Spectrom. 2008, 272, 99–118. [Google Scholar]
  • 43. 
  • 43a. van Heijnsbergen D., Jaeger T. D., von Helden G., Meijer G., Duncan M. A., Chem. Phys. Lett. 2002, 364, 345–351; [Google Scholar]
  • 43b. Reishus K. N., Brathwaite A. D., Mosley J. D., Duncan M. A., J. Phys. Chem. A 2014, 118, 7516–7525; [DOI] [PubMed] [Google Scholar]
  • 43c. Cabarcos O. M., Weinheimer C. J., Lisy J. M., J. Chem. Phys. 1999, 110, 8429–8435; [Google Scholar]
  • 43d. Jaeger J. B., Pillai E. D., Jaeger T. D., Duncan M. A., J. Phys. Chem. A 2005, 109, 2801–2808. [DOI] [PubMed] [Google Scholar]
  • 44. Hanusa T. P., Chem. Rev. 1993, 93, 1023–1036. [Google Scholar]
  • 45. Jutzi P., Burford N., Chem. Rev. 1999, 99, 969–990. [DOI] [PubMed] [Google Scholar]
  • 46. Hanusa T. P., Coord. Chem. Rev. 2000, 210, 329–367. [Google Scholar]
  • 47. 
  • 47a. Westerhausen M., Angew. Chem. Int. Ed. 2001, 40, 2975–2977; [DOI] [PubMed] [Google Scholar]; Angew. Chem. 2001, 113, 3063–3065; [Google Scholar]
  • 47b. Rayón V. M., Frenking G., Chem. Eur. J. 2002, 8, 4693–4707. [DOI] [PubMed] [Google Scholar]
  • 48. Roşca S. C., Caytan E., Dorcet V., Roisnel T., Carpentier J. F., Sarazin Y., Organometallics 2017, 36, 1269–1277. [Google Scholar]
  • 49. Brennan J. G., Andersen R. A., Zalkin A., Inorg. Chem. 1986, 25, 1761–1765. [Google Scholar]

Associated Data

This section collects any data citations, data availability statements, or supplementary materials included in this article.

Supplementary Materials

As a service to our authors and readers, this journal provides supporting information supplied by the authors. Such materials are peer reviewed and may be re‐organized for online delivery, but are not copy‐edited or typeset. Technical support issues arising from supporting information (other than missing files) should be addressed to the authors.

Supplementary


Articles from Angewandte Chemie (International Ed. in English) are provided here courtesy of Wiley

RESOURCES