Qiaomu Yang†
a,
Xiaojuan Yu
b,
Ekaterina Lapsheva‡
a,
Pragati Pandey§
a,
Patrick W. Smith
c,
Himanshu Gupta
a,
Michael R. Gaua,
Patrick J. Carrolla,
Stefan G. Minasian
c,
Jochen Autschbach
*b and
Eric J. Schelter
*ade
aP. Roy and Diana T. Vagelos Laboratories, Department of Chemistry, University of Pennsylvania, 231 S. 34th St., Philadelphia, PA 19104, USA. E-mail: schelter@sas.upenn.edu
bDepartment of Chemistry, University at Buffalo, State University of New York, 732 Natural Sciences Complex, Buffalo, NY 14260, USA. E-mail: jochena@buffalo.edu
cLawrence Berkeley National Laboratory, 1 Cyclotron Rd, Berkeley, CA 94720, USA
dDepartment of Chemical and Biomolecular Engineering, University of Pennsylvania, 220 S. 33rd St., 311A Towne Building, Philadelphia, PA 19104, USA
eDepartment of Earth and Environmental Science, University of Pennsylvania, 251 Hayden Hall, 240 South 33rd Street, Philadelphia, PA 19104, USA
First published on 11th August 2025
Organometallic cerium(IV) complexes have been challenging to isolate and characterize due to the strongly oxidizing nature of the cerium(IV) cation. Herein, we report two cerium(IV) alkynyl complexes, [Ce(TriNOx)(CC-SiMe3)] (1-CeTMS) and [Ce(TriNOx)(C
C-Ph)] (1-CePh) (TriNOx3− = tris(2-tert-butylhydroxylaminato)benzylamine), that include terminal alkyne moieties. The isostructural thorium analogue [Th(TriNOx)(C
C-SiMe3)] (1-ThTMS) was also synthesized and compared with 1-CeTMS in bond distance, 13C-NMR spectra, vibrational spectra and electronic structure. The Ce–C bond distances were 2.501(3) Å for 1-CePh and 2.513(5) Å for 1-CeTMS on the shorter end of the few reported CeIV–C single bonds (2.478(3)–2.705(2) Å), possibly indicating significant Ce 5d- and 4f-orbital involvement. 13C-NMR spectroscopy was also consistent with Ce–C covalency, with significantly deshielded resonances ranging from 185–213 ppm. Such 13C-NMR shifts demonstrate a strong influence from spin–orbit coupling (SOC) effects, corroborated by computational studies. Raman analysis showed νC
C stretching frequencies of 2000 cm−1 (1-CeTMS) and 2052 cm−1 (1-CePh), indicating the cerium(IV)–alkynyl interaction, compared to the parent HC
CPh (IR = 2105 cm−1 and Raman = 2104 cm−1). L3-edge X-ray absorption measurements revealed a predominant Ce(IV) electronic configuration, and magnetic measurements revealed temperature-independent paramagnetism. Electrochemical studies similarly revealed the electron donating ability of the alkynyl ligands, stronger than either fluoride or imido ligands for the Ce(IV)(TriNOx)-framework, with a cerium(IV/III) reduction potential of Epc = −1.58 to −1.66 V vs. Fc/Fc+. Evidence for a trans-influence has been observed by evaluating a series including previously reported [CeIV(TriNOx)X]+/0 complexes with axial ligands X = THF, I−, Br−, Cl−, F−, −C
C-Ph, −C
C-SiMe3, −NH(3,5-(CF3)2-Ar), −OSiPh3, −N(M(L))(3,5-(CF3)2-Ar) [M(L) = Li(TMEDA), K(DME)2 or Cs(2,2,2-crypt)]. These data stand in contrast with previous reports of an inverse trans-influence at cerium(IV) and point to differences in involvement of cerium 4f- versus 5d-orbitals in the electronic structures of the complexes.
Organo-cerium(IV) complexes are generally rare,2 and their scarcity is likely due to redox chemistry, with carbanions prone to oxidation and cerium(IV) cations prone to reduction. Notable examples in the field include metallocene Ce(IV) complexes, heteroatom-stabilized Ce(IV)–C compounds, and Ce(IV) complexes with monodentate carbanion ligands. Metallocene complexes include cerium(IV) cyclopentadienides,19,20 cerium(IV) cyclooctatetraenes such as [Ce(COT)2],15,21–23 or cerium(IV) bispentalenides, with important examples reported between 1976 and 2010.24 Progress has also been made in heteroatom-stabilized cerium(IV)–carbon complexes. Furthermore, Arnold and coworkers reported the use of N-heterocyclic carbene ligands featuring CeIV–Csp2 bonds in 2009,25 and Liddle and coworkers studied the bis(iminophophorano)methandiide (BIPM) ligand in [CeIV(BIPMTMS)2] featuring a CeIV–Csp2 bond in 2013 (Fig. 1).3,14 Our group reported [CeIV(κ2-ortho-oxa)(MBP)2]− in 2021,2 where ortho-oxa = dihydrodimethyl-2-[4-(trifluoromethyl)phenyl]-oxazolide and MBP = 2,2′-methylenebis(6-tert-butyl-4-methylphenolate). The complex featured a CeIV–aryl (Csp2) bond supported by a chelating oxazolide group. Recent progress has been made in Ce–C single bond chemistry, without supporting chelating groups using monodentate supporting ligands. Chen, Li, Tamm, et al. recently used an imidazolin-2-iminato (ImN−) ligand featuring a CeIV–alkynyl (Csp) bond in [CeIV(CC-Ph)(ImN)3] complexes in 2024.26 In the same work, the team also realized compounds featuring CeIV–aryl (Csp2) and CeIV–alkyl (Csp3) bonds. Independently and at the same time, La Pierre and co-workers employed a tri-tert-butyl imidophosphorane ligand on [CeIV(Alkyl)(NP(tert-butyl)3)3] featuring CeIV–alkyl (Csp3) bonds, where alkyl is neopentyl (Npt) or benzyl (Bn).27 Furthermore, a CeIV–cyclopropenyl complex featuring a CeIV–Csp2 bond and ring-open isomerization was recently disclosed by us.28
![]() | ||
Fig. 1 Recent examples of cerium(IV)–carbon containing complexes, including heteratom-stabilized Ce(IV) compounds, or Ce(IV) complexes with monodentate carbanion ligands. |
In pursuit of cerium(IV) organometallic complexes, three primary synthetic strategies have been employed: the use of a supporting ligand with electron-donating groups to stabilize the CeIV oxidation state, the use of multidentate ligands with both a carbanion and electronically supporting heteroatoms coordinating to the CeIV cation, and tethering of ligands with a steric bulk to kinetically inhibit the homolysis of the CeIV–C bond.2 In this study, we sought to employ the first strategy to further expand the scope of CeIV–C chemistry and realize CeIV–alkynyl complexes. The TriNOx3− ligand has been used by us for the stabilization of the Ce(IV) oxidation state and a series of [CeIV(TriNOx)X]+/0 axial complexes, X = THF, I−, Br−, Cl−, F−,29 anilide,12 imide,6,12,13,30 siloxide,13 carbamate,30 and oxo,6,13 were synthesized previously. For the current work, H–CC-SiMe3 and H–C
C-Ph have been used as two alkyne precursors. As a result, compounds with CeIV–Csp bonds were obtained without heteroatom stabilization and without steric hindrance provided by bulky substituents. This approach also provided the opportunity for a more direct analysis of the cerium(IV)–carbon bonding interactions without the influence of conjugated heteroatoms.
Herein, we report the isolation of Ce(IV)–Csp compounds with terminal carbon atom coordination (Fig. 1). The complexes provide opportunities for spectroscopic characterization of the –CC– vibrations and electronic structure calculations. The observed 13C-NMR chemical shifts of the title compounds are remarkably downfield because of effects originating from the relativistic spin–orbit interaction. The alkynyl moiety is also found to be a strong donor for stabilizing cerium(IV) with metal redox potentials of −1.49 and −1.57 V vs. Fc/Fc+ (Fc = Fe(C5H5)2). The information obtained in the present study has been applied to complete a trans influence series for related [CeIV(TriNOx)X]+/0 complexes with axial ligands X including THF, halide, alkynyl, amide, siloxide, and imide ligands. These results provide important opportunities for improving our understanding of the bonding involving lanthanides in high oxidation states.
![]() | ||
Fig. 2 Syntheses of (A) CeIV–alkynyl complexes (1-CePh and 1-CeTMS) and (B) ThIV–alkynyl complex (1-ThTMS). |
These CeIV–Csp bond distances are shorter than the previously reported CeIII–Csp bond distances in cerium–cyanide complexes (2.596(15)–2.736(17) Å),31 such as ([NnBu4]2[(C5Me5)2CeIII(CN)3]); alkynyl complexes (2.549(3)–2.71(2) Å),32 such as [(C5Me5)2Ce(CCtBu)2Li(THF)]; and a cerium(III) phenolate alkynyl complex (2.652(9) Å),33 Na[Ce(CCPh)(bdmmp)3] (bdmmp = 2,6-bis-(dimethylamino)-4-methylphenolate). The shorter distances of the CeIV–Csp bonds in 1-CePh and 1-CeTMS are consistent with the ∼0.1 Å smaller ionic radius of the cerium(IV) ion compared to cerium(III) with similar coordination numbers.34 The interatomic distance is summarized into a table (see Table 1 and the SI).
Bond type | Bond distance (Å) | Reference |
---|---|---|
CeIII–Ccyanide | 2.596(15)–2.736(17) | 31 |
CeIII–Calkynyl | 2.549(3)–2.71(2) | 32 |
CeIII–Calkynyl | 2.652(9) | 33 |
CeIV–Ccarbene | 2.652(7)–2.705(2) | 25 |
CeIV–Caryl | 2.571(7)–2.5806(19) | 2 |
CeIV–Caryl | 2.539(3) | 26 |
CeIV–Calkyl | 2.515(4) | 26 |
CeIV–Calkyl | 2.508(2)–2.562(2) | 27 |
CeIV–Calkynyl | 2.478(3)–2.523(10) | 26 |
CeIV–Calkynyl | 2.513(5) | 1-CePh |
CeIV–Calkynyl | 2.501(3) | 1-CeTMS |
CeIV–Cheter-atom supported multiple bond | 2.385(2)–2.441(5) | 14 |
These CeIV–Csp bond distances are also shorter than those of previously reported single CeIV–C bonds in CeIV N-heterocyclic carbene complexes (2.652(7)–2.705(2) Å),25 such as CeIV[OCMe2CH2(1-C{NCHCHNiPr})]4; CeIV oxazolide aryl complexes (2.571(7)–2.5806(19) Å),2 such as [Li(DME)3][CeIV{κ2-dihydrodimethyl-2-[4-(trifluoromethyl)phenyl]-oxazolide}](2,2′-methylenebis(6-tert-butyl-4-methylphenolate)2); CeIV tris(imidazoline-2-iminato) alkyl complexes (2.515(4) Å) and aryl complexes (2.539(3) Å);26 CeIV imidophosphorane alkyl complexes (2.508(2)–2.562(2) Å),27 such as CeIV benzyl tris(tri-tert-butyl imidophosphorane). However, our CeIV–Csp bond distances are similar to the CeIV–C bond distances in CeIV tris(imidazoline-2-iminato) alkynyl complexes (2.478(3)–2.523(10) Å)26 and are longer than the CeIV and carbon bond distances in heteroatom-supported bis(iminophosphorano)methandiide complexes (2.385(2)-2.441(5) Å),14 such as Ce{C[PPh2N(SiMe3)]}[O(2,6-diisopropylphenyl)]2 (Fig. 1). The short CeIV–Csp distances possibly indicate appreciable cerium(IV)–carbon interactions, especially considering that the coordination of the alkynyl moieties to the cerium is unsupported in the case of the compounds reported here.
X-ray crystallography experiments confirmed the molecular structure of related 1-ThTMS was isostructural to 1-CeTMS. There are two independent molecules of 1-ThTMS in the asymmetric unit with minor differences, with Th–Csp bond distances of 2.593(14) and 2.605 (14) Å. Thorium(IV)–alkynyl complexes were reported previously,35–39 where the reported ThIV–C bond lengths ranged from 2.450(7) to 2.642(5) Å. The ThIV–C bond distance in 1-ThTMS is similar to or slightly longer than these literature values, likely due to the electron-donating TriNOx3− ligand. This bond length in 1-ThTMS is also 0.086 Å longer than the Ce–C distance in 1-CeTMS, consistent with a slightly larger ionic radius of thorium(IV) of 1.05 Å than cerium(IV) of 0.97 Å, with an oxidation state of +4 and a coordination number of 8.34
We also observed previously that the 1H-NMR chemical shifts of the diastereotopic benzylic resonances (CH2) and tert-butyl (tBu) resonances in the TriNOx3− arms were sensitive to the axial ligand identity. The –CH2 and –tBu proton resonances were used to differentiate inner- or outer-sphere coordination to the [Ce(TriNOx)]+ fragment in the solution phase.29 For example, [Ce(TriNOx)]I exhibits 1H-NMR CH2 resonances between 4.73–4.67 and 4.07–4.03 ppm and a tBu resonance at 0.72 ppm, features that were confirmed to correspond to an outer-sphere iodide anion, whereas the [Ce(TriNOx)Cl] complex has an inner-sphere chloride axial ligand in solution with –CH2 proton resonances spanning 4.66–4.62 and 3.16–3.12 ppm and characteristic tBu resonance at 0.94 ppm. In particular, the larger differences in the diastereotopic –CH2 chemical shift ranges were correlated with the geometry difference between inner- and outer axial ligand coordination. In the current work, the chemical shifts of 1-CePh and 1-CeTMS resemble those of the inner-sphere [Ce(TriNOx)Cl] at around 3.1 and 0.9 ppm (Fig. 4A). Thus, the chemical shift indicates, as expected, that the alkynyl is coordinated to the cerium(IV) cation in solution, consistent with the result from cyclic voltammetry, vide infra. The thorium(IV) alkynyl complex 1-ThTMS resembles the cerium analogue 1-CeTMS in C6D6 (see the SI) and was also assigned as an inner-sphere alkynyl complex.
Considering the 1H-NMR resonances of 1-CePh and 1-CeTMS it is noteworthy that the upfield chemical shift of the –CH2 signals corresponded to a relatively stronger bonding interaction of the axial ligand with the cerium(IV) cation. The trend was noted by us previously for [Ce(TriNOx)Br] (4.71–4.62, 3.34–3.30 ppm), [Ce(TriNOx)Cl] (4.66–4.62, 3.16–3.12 ppm), and [Ce(TriNOx)F] (4.64–4.60, 3.08–3.04 ppm) in pyridine-d5.29 In comparison, the –CH2 1H-NMR resonances for 1-CePh (4.62–4.59, 3.08–3.05 ppm) are similar to those for [Ce(TriNOx)F], while the –CH2 resonance for 1-CeTMS (4.57–4.54 and 3.03–3.00 ppm) is further upfield. This result indicates the stronger electron donating ability of –CC-SiMe3 than –C
C-Ph for the CeIV cation, consistent with the cerium(III/IV) electrochemistry results, the 13C-NMR spectroscopy results, and the observations of a trans-influence for the system (vide infra).
After confirming the chemical structures and the 1H-NMR spectra of 1-CeTMS, 1-CePh and 1-ThTMS, we turned to investigations of 13C-NMR spectra. Atoms directly bound to closed-shell heavy metal centers with formally empty d- and/or f-shells, especially actinides, are known to have a characteristic and often large downfield shift.40,41 This deshielding effect has been correlated with the degree of covalency in the metal–ligand bond.41–43 The effect has been found, for example, for Csp3, Csp2 and hydrogen atoms in diamagnetic Th(IV) and U(VI) complexes.7,44–48 For thorium, the largest 13C-NMR spectroscopy chemical shift δ 230.8 ppm was observed for Th(2-C6H4CH2NMe2)4,48 while the largest 1H-NMR chemical shift was estimated using DFT calculations at 20.3 ppm for ThH[N(SiMe3)2]3.49 Recent progress in obtaining isolable cerium(IV)–carbon bonded complexes has demonstrated similar downfield shifts to those in actinide compounds,2,3,14,25 where the largest 13C chemical shift of δ 343.5 ppm was observed for a CeIV[C(Ph2PNSiMe3)2]2 complex.3 Notably, this cerium(IV) complex had a Ce–C bond supported by heteroatom coordination and conjugation, including two phosphorus atoms bound at the central carbon, qualifying a direct comparison.
In the current cases (Fig. 4B), the 13C chemical shifts are 184.7 ppm for 1-CePh in CD2Cl2 and 207.0 ppm for 1-CeTMS in CD2Cl2 (and 213.0 ppm in C6D6), well outside the typical range for alkynyl resonances (65–90 ppm).50 Thus, the strong downfield shift indicates potentially a large spin–orbit coupling contribution to the chemical shift, as with other cerium(IV)–carbon moieties.7 This observation also reflects the strong cerium–alkynyl bonding interactions. [Ce(TriNOx)(CC-Ph)] has larger 13C-NMR shifts at 184.7 ppm than those reported in the CeIV–Csp complex [CeIV(ImN)3(C
C-Ph)] at 176.4 ppm by Chen and Li.26 It should be noted that these 13C-NMR shifts are smaller than those reported in the CeIV–Caryl complex (255.6 ppm for a cerium oxazolide complex) by us previously.2 This is presumably because the 13Csp2-NMR chemical shift (100–170 ppm for arenes)2 is intrinsically larger than the 13Csp-NMR chemical shift (60–100 ppm for alkynes).
To understand the CeIV/ThIV–C bonding interactions and the influence of spin–orbit coupling, computational analyses were carried out, including calculations of the carbon NMR chemical shifts. Density functional theory (DFT) calculations were initially performed for 1-CeTMS, 1-CePh, and 1-ThTMS using the B3LYP hybrid functional. Complete computational details are provided in the SI. B3LYP is frequently used for molecular structure optimizations and bonding studies and therefore we used it for these purposes in the present investigation.51,52 Selected optimized bond distances of 1-CeTMS, 1-CePh, and 1-ThTMS are compared to the experimental crystal structure data in Table S3. The optimized M–C bond metrics align closely with the experimental data, with deviations of only 0.001 Å and 0.03 Å for the Ce–C and Th–C distances, respectively, confirming the reliability of the chosen computational model.
To explore the nature of the M–C interactions, we employed natural localized molecular orbital (NLMO) analyses to assess the covalency resulting from the σ donation in 1-CeTMS, 1-CePh, and 1-ThTMS. Relevant orbitals are depicted in Fig. 5, and atomic hybrid contributions in the NLMOs and bond order analysis representing the important bonding interactions are listed in Tables S4 and S5. Given the similarity in the bonding characteristic of 1-CeTMS and 1-CePh, we mainly focused on 1-CeTMS versus 1-ThTMS. For 1-CeTMS, the NLMO analysis reveals a σ(Ce–Cα) bond with 17% total Ce density weight (18% 6s; 62% 5d; 20% 4f), along with two orthogonal π(Cα–Cβ) bonds showing negligible Ce weights (1% each). In other words, there is a Ce—Cα σ bond which is polarized toward carbon. The 17% density weight on Ce means that electron density corresponding to about 0.34 electrons is donated to Ce (the NLMO is doubly occupied). In contrast, the σ(Th–Cα) NLMO for 1-ThTMS exhibits 14% (60% 6d; 15% 5f) Th weight, i.e., lower than that of the Ce analogue. The calculations therefore indicate that the extent of metal–ligand covalent bonding with the ligands studied herein is somewhat more pronounced for Ce(IV)- than for Th(IV)-carbon bonds, which is in line with reported data for thorium(IV)-imido versus cerium(IV)-imido complexes from our group.53 These results and a growing body of evidence suggest that the notion that lanthanide bonding is not covalent is inappropriate.
The 13C-NMR chemical shifts for complexes 1-CeTMS and 1-CePh were calculated using a functional denoted here as PBE0(40) (a PBE-based hybrid with 40% exact exchange), without and with inclusion of the SO interaction. This functional was previously shown to accurately predict 13C-NMR chemical shifts in organometallic cerium complexes.2,54,55 A summary of calculated shielding constants and chemical shifts is listed in Table S6. The calculated and experimental 13C chemical shifts are in excellent agreement. For example, the calculated Cα shift for 1-CeTMS is 207.3 ppm (expt. = 207.0 ppm), which includes a 19.4 ppm deshielding contribution due to SO effects that is primarily attributed to the strong SO coupling within the Ce 4f (and 5d) shell and its involvement in the chemical bond with Cα.
For comparison, the calculated Cα shift for 1-ThTMS is 195.5 ppm (expt. = 193.2 ppm), with a 25.4 ppm shift due to SO coupling. This is consistent with a weaker covalency of thorium compared with cerium but stronger SO coupling for Th due to the higher nuclear charge. In another comparison, the calculated Cα shift for 1-CePh is 186.8 ppm (expt. = 184.7 ppm), which includes a 20.4 ppm deshielding from the SO interaction. The similar SOC deshielding in 1-CePh relative to 1-CeTMS is commensurate with its similar Ce–Cα bond covalency.
No vibrational spectra of cerium(IV)–alkynyl complexes have previously been reported. Here, we collected the infrared (IR) absorption and Raman spectra of 1-CeTMS, 1-CePh, and 1-ThTMS to identify the vibrational frequencies of the –CC– moiety (Fig. 6 and the SI) and compared them with those of other metal–alkynyl complexes. For the M–C
C-TMS complexes, the observed νC
C Raman stretching frequencies were 2000 and 2003 cm−1 for 1-CeTMS and 1-ThTMS respectively. The notably weak Raman signal for 1-CeTMS was intrinsic and observed over multiple samples/measurements. The reasons for the lower Raman signal strength for 1-CeTMS compared to 1-ThTMS are, as yet, unclear. For M–C
CPh, 1-CePh (Raman = 2052 cm−1) was shown to have a νC
C stretching frequency that was lower than that in HC
CPh (IR = 2105 cm−1 and Raman = 2104 cm−1). Vibrational spectra of related metal–acetylide complexes reported in the literature include Yb(C
CPh)(C5H5)2 (IR = 2040 cm−1)63 and Zr(C
CPh)2(C5Me5)2 (IR = 2073 cm−1).57 Based on these reported results, the vibrational frequency of the alkynyl moiety reflects the metal–alkynyl σ-bond interactions (Fig. S48). We contend that the νC
C stretching frequencies for 1-CeTMS, 1-CePh, and 1-ThTMS are approximately intermediate between those observed for more purely ionic f-block (low frequency) and relatively more covalent d-block (high frequency) metal congeners.1,16,21
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Fig. 6 Raman spectra of 1-CeTMS, 1-CePh, and 1-ThPh, and comparison with a lithium–acetylide complex and protonated alkyne. |
The Ce L3-edge (Ce 2p → 5d) X-ray absorption near edge structure (XANES) spectra of 1-CeTMS and 1-CePh are shown in Fig. S56–S57. A characteristic double-peaked structure is observed, which is attributed to excitations of the core hole electron (2p) to 4f15d1 and 4f05d1 final states, where
indicates a hole (vacancy) at the ligand.6,17 The intensities of both peaks were evaluated using established curve-fitting methods, which indicated that the weight of the 4f05d1 configuration had statistically equivalent values for both complexes, with relative weights of 0.43(3) for 1-CeTMS and 0.46(3) for 1-CePh. These configuration weights are comparable to those of other cerium(IV) complexes, such as cerium(IV) TriNOx3− imido complexes (0.37(3)–0.45(3))6 and cerium(IV) TriNOx3− oxo complexes (0.39(3)–0.41(3)).6 Although fitting was unable to quantify any difference, visual inspection of the normalized spectra shows that the feature at higher energy is more intense for 1-CePh. We reach the qualitative determination that the 4f electron density at Ce is lower for 1-CePh relative to 1-CeTMS.
Having evaluated the amount of charge transfer for 1-CeTMS and 1-CePh, we next turned to temperature dependent magnetic studies of the compounds. Van Vleck temperature-independent paramagnetism (TIP) has been observed for molecules, formally cerium(IV) complexes,6,66–68 arising from small energy differences between the open-shell singlet ground state and admixed, low-lying triplet excited states.67 Magnetometry studies were carried out on 1-CePh. The variable field magnetization was collected for 1-CePh at 2 K, which shows the presence of a negligible magnetic impurity that saturates below M < 0.01 μB (Fig. S52), indicating the +IV oxidation state of cerium in 1-CePh. A variable temperature magnetic susceptibility plot for 1-CePh was collected at a 1.0T applied field (Fig. S53 and S54). The susceptibility plot of χT vs. T shows a linear decrease from high (300 K) to low temperature (2 K). After accounting for the intrinsic diamagnetic contribution using Pascal's constants, the TIP value for this cerium(IV) complex was determined to be 6.34(1) × 10−4 emu mol−1. This value is similar to, or larger than, those of reported cerium(IV) complexes such as cerocene (1.4(2) × 10−4 emu mol−1),68 [NEt4]2[CeCl6] (1.6(2) × 10−4 emu mol−1),66 and [K(DME)2][Ce(TriNOx)(NArF)] (2.2(2) × 10−4 emu mol−1).6 UV-vis absorption spectra were recorded for both 1-CeTMS and 1-CePh, where 1-CeTMS showed a peak at 358 nm and 1-CePh showed a peak at 382 nm, and both were attributed to LMCT (Fig. S50). Overall, our experimental data confirm pure cerium(IV) oxidation states and reveal the electronic structure and configuration for the cerium–alkynyl complex.
The relatively negative Epc values of the cerium(IV) alkynyl complexes indicate the strong electron donating character of the alkynyl ligand, notably stronger than that of the fluoride ligand, with a ∼0.2 V more negative redox potential. It should be noted that although the cerium(IV) imido complexes have a Epc values less negative than that of the alkynyl analogues: [M(L)x][Ce(TriNOx) = N–Ar] (–Ar = –(3,5-(CF3)2C6H3), Epc = −1.39 to −1.45 V), this observation is likely due to the reduction of the imido ligand instead of a cerium(IV) cation. Indeed, the imido ligand is a better electron-donating ligand, as indicated in the trans-influence section, vide infra. In comparison, they have a similar reduction potential to [Li(THF)4][Ce(κ2-ortho-oxa)(MBP)2],26 while [CeIV(Alkyl)(NP(tert-butyl)3)3] has a much more negative reduction potential (−2.55 V to −2.92 V) due to the strong electron donating –NP(tert-butyl) moiety in addition to an alkyl ligand.27 In general, these electrochemical data provide supporting evidence for a strong interaction between the Ce(IV) cation and –C
C–R moieties (–R = –SiMe3 or –Ph).
Reduction waves (Epc) for 1-CeTMS and 1-CePh demonstrate the reduction of the Ce(IV) alkynyl complexes to corresponding Ce(III) moieties (Fig. 7A and Table 2). However, this process is largely irreversible due to an accompanying chemical process. In this process, the reduced species, [CeIII(CC–R)(TriNOx)]−, is not stable and the alkynyl ligand presumably dissociates under the electrochemical conditions employed, similar to reported results for [CeIIICl(TriNOx)]−.29 Following the cathodic features of 1-CeTMS and 1-CePh, the subsequent anodic sweeps (Epa) indicate the oxidation of the newly generated Ce(III) species, likely “[CeIII(TriNOx)]”, based on the observed oxidation potential and comparison with our previous results.29
Complex | Epc | E1/2 |
---|---|---|
a Ep stands for redox potential from differential pulse voltammetry (DPV) instead of E1/2.b The scan rate was unknown, while other Epc values were measured at a 100 mV s−1 scan rate. | ||
[Ce(TriNOx)](OTf) | −1.04 V | −0.95 V |
[Ce(TriNOx)]I | −1.04 V | — |
[Ce(TriNOx)Br] | −1.16 V (−1.04 V) | — |
[Ce(TriNOx)Cl] | −1.26 V | — |
[Ce(TriNOx)F] | −1.40 V | −1.36 V |
[M][Ce(TriNOx)![]() |
−1.39 V to −1.45 V | — |
[Ce(TriNOx)(C![]() |
−1.58 V | −1.49 V (Ep)a |
[Ce(TriNOx)(C![]() |
−1.66 V | −1.57 V (Ep)a |
[NnBu4]2[Ce(NO3)6] | — | 0.62 V |
[CeCl6]2− | — | 0.03 V |
[Ce[N(SiMe3)2]3Cl] | — | −0.30 V |
[Ce(COT)2] | — | −1.40 V |
[Ce(BIPMTMS)2] | — | −1.63 V |
[Li(THF)4][Ce(κ2-ortho-oxa)(MBP)2] | −1.67 V | — |
[CeIV(Alkyl)(NP(tert-butyl)3)3] | b−2.55 V to −2.92 V | — |
Differential pulse voltammetry (DPV) experiments70 were also used to determine potential values for the redox processes of 1-CeTMS and 1-CePh, where Ep = −1.57 V for 1-CeTMS and −1.49 V for 1-CePh vs. Fc/Fc+ (Fig. 7B), for comparison with the measured E1/2 values (Table 2).29,71 These observed Ep values are more negative than those of some commonly observed cerium(IV) complexes and are comparable with those of other organo-cerium(IV) complexes such as [Ce(COT)2] or [CeIV(BIPMTMS)2].2,3,14
Axial ligand X to [Ce(TriNOx)]+ | Computed distance (Å) | Bond order | Energy | |
---|---|---|---|---|
Ce–N(4) | Ce–X | Ce–N(4) | ELUMO (Hartree) | |
THF | 2.826 | 0.2564 | 0.2590 | −0.1884 |
I− | 3.082 | 0.7353 | 0.1821 | −0.0873 |
Br− | 3.111 | 0.9373 | 0.1712 | −0.0820 |
Cl− | 3.129 | 0.9726 | 0.1695 | −0.0821 |
F− | 3.147 | 1.0430 | 0.1559 | −0.0767 |
−C![]() |
3.082 | 0.8552 | 0.1660 | −0.0710 |
−C![]() |
3.069 | 0.8506 | 0.1691 | −0.0772 |
−NHAr | 3.071 | 0.7999 | 0.1711 | −0.0831 |
−OSiPh3 | 3.187 | 0.8972 | 0.1485 | −0.0758 |
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3.228 | 1.1970 | 0.1359 | −0.0520 |
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3.335 | 1.5158 | 0.1151 | −0.0383 |
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3.510 | 1.7020 | 0.0774 | 0.0550 |
In the current work, a trans-position has been studied for the current and previously reported, structurally conserved [CeIV(TriNOx)X] complexes, considering the axial nitrogen atom N(4) from the tridentate TriNOx3− ligand and terminal X− (or L) ligand (Fig. 8). For example, X− in 1-CeTMS/1-CePh indicates the alkynyl ligands. The angles of X–Ce–N(4)TriNOx of the complexes range from 173.8(3)° to 179.34(8)° in the crystal structures and range from 172.84° to 179.98° in the DFT optimized structures, indicating the validity for the trans-position of X− and N(4) atoms on the cerium atom. A series of X− (or L) ligands for the complexes have been compared from weakly coordinating to strongly coordinating: -THF, -halide (iodide, bromide, chloride, and fluoride), -alkynyl, -anilide, -siloxide, and -imide (Li-capped, K-capped and uncapped imides) (see the SI). The Ce(IV)–N(4) bonding interaction is understood to be weak but nevertheless an important and diagnostic metric on axial bonding in this system. It should be noted that, in the solution phase, the iodide ligand is an outer-sphere and bromide ligand is partially outer-sphere (in chemical equilibrium between the inner- and outer-sphere). But these two ligands, I− and Br−, were considered inner spheres for the structures considered in this study. The complexes were ranked by increasing Ce–N(4) distance, excepting the halides. Among halide complexes [CeIV(TriNOx)X, X = F−, Cl−, Br−, I−], only the Cl− complex was previously characterized by crystallography, while the rest were characterized by elemental analysis and NMR.29 Here, all the halide complexes were used as model complexes for computational studies. It should also be noted that these computational studies on the trans-influence used methods, with the B3LYP hybrid functional, that were chosen for consistency with previous work on the [CeIV(TriNOx)X] system.29
We posited that the most telling case for the trans influence in the current system would be made with multiple lines of experimental and computational metrics that incorporate X-ray structural and computational electronic structural aspects concurrently (Fig. 8).43 The computational methods undertaken here are different from those described in previous sections of the current work and a description of the trans influence computational study is also provided in the SI. As described before,29 the accuracy between the computed distance of Ce–OTriNOx and experimental result indicates an acceptable computational model performance. The Ce–X distances exhibit a good correlation between the experimental and computed results, with differences less than 0.08 Å, except for the chloride complex (0.12 Å). The Ce–N(4)TriNOx distances also demonstrated reasonable agreement between experimental and computed values, except for chloride (Fig. 8A). We also observed a negative correlation between computed Ce–N(4) bond distance and Mayer bond order (Fig. 8B), consistent with a stronger bond with a shorter distance.
Mayer bond order has been used to compare the halide derivatives of [CeIV(TriNOx)X] complexes.29 Based on the computational results in Fig. 8C, it is evident that a larger Mayer bond order of Ce–X (or L) exhibits a trans-influence and results in a smaller Mayer bond order of CeIV–N(4), indicating the stronger donating ability of the X/L ligand on cerium resulting in a weaker bond between Ce and N(4). The LUMO of these complexes primarily consists of 4f character and the LUMO energies are correlated with the electron donating ability of the ligands.84 We observe a similar trend between the LUMO energy and Ce–N(4) distance, where a stronger Ce–X bond and longer but weaker Ce–N(4) bond result in a higher LUMO energy (Fig. 8D), similar to previous observation.29
To better illustrate the trans-influence, this phenomenon can be interpreted using the Ce–N(4) experimental bond distances (Table S1). Weakly coordinated THF resulted in a Ce–N(4) bond length of 2.717(9)–2.787(8) Å and the chloride (Cl−) ligand resulted in a Ce–N(4) bond length of 2.825(3) Å. The relatively strong sigma-donating alkynyl ligands yielded a Ce–N(4) bond length of 2.906(2) Å for [Ce(TriNOx)(CC-Ph)] and 2.932 Å for [Ce(TriNOx)(C
C-TMS)], whereas the anilide ligand resulted in a bond length of 2.934(3) Å for [Ce(TriNOx)(NHAr)] (Ar = (3,5-(CF3)2C6H3)). Thus, notably, the alkynyl ligand exhibits a strong donating ability comparable to that of the anilide ligand, indicating a stronger bonding interaction between cerium and alkynyl moieties (see the SI). By way of comparison, the extraordinarily strongly coordinating uncapped imido ligand gives a bond distance of 3.335 Å for Ce–N(4) of [Cs(2,2,2-cryptand)][Ce(TriNOx)(NAr)]. To conclude, the bond distance and bond order well reflect the bonding interactions of the Ce–X and Ce–N(4) moieties and illustrate a structural trans-influence is operative in this series.
CCDC 2448118–2448120 contain the supplementary crystallographic data for this paper.85–87
The supplementary information includes NMR spectroscopic, X-ray crystallographic, electrochemical, vibrational spectroscopic, UV-vis spectroscopic, magnetometric, X-ray absorption spectroscopic, and computational data. See DOI: https://doi.org/10.1039/d5sc03222a.
Footnotes |
† Current address: 9700 S. Cass Avenue, The Center of Nanoscale Materials, Argonne National Lab, IL 60439 (USA). |
‡ Current address: 410 Forest Ave, Sheboygan Falls, Ereztech Labs, WI 53085. |
§ Current address: Group of Coordination Chemistry, Institut des Sciences et Ingénierie Chimiques, École Polytechnique Fédérale de Lausanne (EPFL), CH-1015 Lausanne, Switzerland. |
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