Johann A Hlina1, James R Pankhurst1, Nikolas Kaltsoyannis2,3, Polly L Arnold1. 1. EaStCHEM School of Chemistry, University of Edinburgh , Joseph Black Building, The King's Buildings, Edinburgh EH9 3FJ, U.K. 2. Department of Chemistry, University College London , 20 Gordon Street, London, WC1H 0AJ, U.K. 3. School of Chemistry, University of Manchester , Oxford Road, Manchester, M13 9PL, U.K.
Abstract
Heterobimetallic complexes containing short uranium-group 10 metal bonds have been prepared from monometallic IU(IV)(OAr(P)-κ(2)O,P)3 (2) {[Ar(P)O](-) = 2-tert-butyl-4-methyl-6-(diphenylphosphino)phenolate}. The U-M bond in IU(IV)(μ-OAr(P)-1κ(1)O,2κ(1)P)3M(0), M = Ni (3-Ni), Pd (3-Pd), and Pt (3-Pt), has been investigated by experimental and DFT computational methods. Comparisons of 3-Ni with two further U-Ni complexes XU(IV)(μ-OAr(P)-1κ(1)O,2κ(1)P)3Ni(0), X = Me3SiO (4) and F (5), was also possible via iodide substitution. All complexes were characterized by variable-temperature NMR spectroscopy, electrochemistry, and single crystal X-ray diffraction. The U-M bonds are significantly shorter than any other crystallographically characterized d-f-block bimetallic, even though the ligand flexes to allow a variable U-M separation. Excellent agreement is found between the experimental and computed structures for 3-Ni and 3-Pd. Natural population analysis and natural localized molecular orbital (NLMO) compositions indicate that U employs both 5f and 6d orbitals in covalent bonding to a significant extent. Quantum theory of atoms-in-molecules analysis reveals U-M bond critical point properties typical of metallic bonding and a larger delocalization index (bond order) for the less polar U-Ni bond than U-Pd. Electrochemical studies agree with the computational analyses and the X-ray structural data for the U-X adducts 3-Ni, 4, and 5. The data show a trend in uranium-metal bond strength that decreases from 3-Ni down to 3-Pt and suggest that exchanging the iodide for a fluoride strengthens the metal-metal bond. Despite short U-TM (transition metal) distances, four other computational approaches also suggest low U-TM bond orders, reflecting highly transition metal localized valence NLMOs. These are more so for 3-Pd than 3-Ni, consistent with slightly larger U-TM bond orders in the latter. Computational studies of the model systems (PH3)3MU(OH)3I (M = Ni, Pd) reveal longer and weaker unsupported U-TM bonds vs 3.
Heterobimetalliccomplexes containing short uranium-group 10 metal bonds have been prepared from monometallic IU(IV)(OAr(P)-κ(2)O,P)3 (2) {[Ar(P)O](-) = 2-tert-butyl-4-methyl-6-(diphenylphosphino)phenolate}. The U-M bond in IU(IV)(μ-OAr(P)-1κ(1)O,2κ(1)P)3M(0), M = Ni (3-Ni), Pd (3-Pd), andPt (3-Pt), has been investigated by experimental andDFT computational methods. Comparisons of 3-Ni with two further U-Nicomplexes XU(IV)(μ-OAr(P)-1κ(1)O,2κ(1)P)3Ni(0), X = Me3SiO (4) and F (5), was also possible via iodide substitution. All complexes were characterized by variable-temperature NMR spectroscopy, electrochemistry, and single crystal X-ray diffraction. The U-M bonds are significantly shorter than any other crystallographically characterizedd-f-block bimetallic, even though the ligand flexes to allow a variable U-M separation. Excellent agreement is found between the experimental andcomputed structures for 3-Ni and3-Pd. Natural population analysis and natural localized molecular orbital (NLMO) compositions indicate that U employs both 5f and 6d orbitals in covalent bonding to a significant extent. Quantum theory of atoms-in-molecules analysis reveals U-M bondcritical point properties typical of metallic bonding and a larger delocalization index (bond order) for the less polar U-Ni bond than U-Pd. Electrochemical studies agree with the computational analyses and the X-ray structural data for the U-X adducts 3-Ni, 4, and 5. The data show a trend in uranium-metal bond strength that decreases from 3-Nidown to 3-Pt and suggest that exchanging the iodide for a fluoride strengthens the metal-metal bond. Despite short U-TM (transition metal) distances, four other computational approaches also suggest low U-TM bond orders, reflecting highly transition metal localized valence NLMOs. These are more so for 3-Pd than 3-Ni, consistent with slightly larger U-TM bond orders in the latter. Computational studies of the model systems (PH3)3MU(OH)3I (M = Ni, Pd) reveal longer and weaker unsupported U-TM bonds vs 3.
The nature of the bonding
in f-block metal–ligand bonds
is still far from fully understood, and bonding between f-block metals
and other metalcations even less so. By contrast, studies of the
bonding between d-block and other metalcations are 50 years old andhave furthered our understanding of d-orbital interactions and generated
some unique small molecule activation chemistry andcatalyzed reactions
not seen in single metalchemistry.[1] The
few complexes that feature bonds between an f-block andd-block cation[2−4] have begun to help to improve our understanding of metal–metal
bonding and to challenge andhelp the development of computational
methods; however, the challenges associated with their synthesis andcharacterization have precluded the systematic study of any families
of heterobimetallics that would enable the prediction of trends in
other systems. The 5f orbitals have a suitable spatial extension but
not yet a predictability of participation in bonding that makes the
d–f heterobimetallic bond a particularly interesting target
to improve our understanding of the relative involvement of f- andd-orbital participation. A better understanding of the subtleties
of the 5f/6dcontributions to actinide bonding in general is important
in the handling of nuclear materials, where differences in behavior
are dominated by small covalency differences in bonding.Compounds
with a uranium–transition metal bond are limited
to iron,[5−7] ruthenium,[5,8] cobalt,[9−11] rhenium,[12−14] andsilver.[15] The first
pair, Cp3U-MCp(CO)2 (M = Fe, Ru), was reported
in 1987,[5] prepared via salt metathesis
from Cp3UCl and Na[MCp(CO)2]. The investigation
confirmed the presence of a metal–metal bond rather than an
isocarbonyl bridge, but without crystallographicdata, further analyses
were difficult. We were able to isolate and structurally confirm the
stable lanthanide analogue, (L)(N″)NdFeCp(CO)2 [L
= ButNCH2CH2{C(NCSiMe3CHNBut)}; N″ = N(SiMe3)2],
the first complex with an unsupported 4f–3dmetal–metal
bond.[16] Liddle andco-workers translated
this chemistry back to a uranium-supported bond by the tris(amido)
tren framework[17] and extended the range
of unsupporteduranium–transition metalcomplexes further to
cobalt andrhenium.[8,9,12−14]Complementary to unsupported f/d-block metal
bonds, which intrinsically
rely on a negatively charged, ligating d-block fragment, bridging
ligands can provide more robust molecules. The Group 10 metal–thoriumderivatives (Cp*)2Th(μ-PPh2)2Ni(CO)2 and (Cp*)2Th(μ-PPh2)2PtPMe3 (Cp* = C5Me5) have unusual geometries and short Th–M distances of 3.206(2)
and 2.984(1) Å, respectively,[18,19] the latter
being described by calculations as a donor–acceptor bond from
the pseudotrigonal-bipyramidal M0 to the redox-inactive
ThIVcenter.The groups of Bart and Thomas reporteduranium–cobaltcompounds
with bridging heterobidentate monoanionicPN ligands.[10] At 2.874(3) Å, ICo(μ-Ph2PNPri-κ1P,κ1N)3UI (A) exhibits the shortest
uranium–transition metal bond reported prior to this study;
in this most instructive work, the analogue withPr2iPNMes ligands (Mes = C6H2Me3-2,4,6) was proposed from voltammetric experiments to have a stronger
Co → U dative interaction than the relatively modest one in A, although the changes at both ends of the bidentate ligand
make the components difficult to separate, and the latter complex
was not structurally characterized. One of the arguments for using
heterobidentate ligands has been to expand the variety of synthetic
routes to M–M′ bonds; the photolytic release of CO from
the isocarbonyl U–OC–Co moiety upon photolysis is arguably
the most inventive synthesis yet, forming a 3.0319(7) Å U(IV)–Co(I)
bond within the rigid NP scaffold N[ο-(NHCH2PPr2i)C6H4]3 and with the suggestion of a close contact between the U
center and another Co-boundCO ligand, while vibrational data suggest
stronger donation of Co electron density to uranium through the bond
than through the original isocarbonyl link, although the coordination
of additional phosphineshas also changed the ancillary ligand set
somewhat.[11]For comparison, the shortest
distance yet found between an f and
a d block metal is in the lutetium–platinumcomplex (C5Me4SiMe2CH2PPh2)Lu(μ-CH2SiMe2CH2)(OC4H8)PtMe2, 2.7668(5) Å,[20] which shows interesting intramolecular C–H
bondcleavage chemistry at elevated temperatures.Even though
the heterobimetallicchemistry of rare-earth transition-metalcompounds has now begun to receive considerable attention, examples
with late transition metals are still rare.[2−4] Roesky also
usedphosphinoamido ligands to combine palladium withyttrium andlutetium in bi- andtrimetalliccompounds with 2.9898(6) Å (Y–Pd),
2.9712(8) Å (Lu–Pd), and 3.141(13) Å (Y–Pd2) bond lengths for the trimetalliccompound.[21]We have targetedphosphine-functionalized aryloxide
analogues of
U(IV)(OAr)3X (OAr = 2,6-di-tert-butylphenoxide)
first reported in the 1980s, anticipating binding of a secondmetal
by the incorporatedphosphine groups, and since then work by others
and us has shown that the U–OAr bonds are sufficiently robust
to allow many X-substitution reactions without ligand scrambling that
can dominate f-block coordination chemistry.[22−27] Other robust ligand sets, such as bis(permethylcyclopentadienyl)
or polydentate chelates, can be insufficiently mobile to allow the
M–M′ distance to change according to metal size or electronic
preference. We also considered that the X ligand in the trans position
to a ligatedmetal ion would provide the possibility to exploit the
inverse trans influence (ITI) in the formation of stronger bonds to
an atom (here the secondmetal) in the position trans to X, the phenomenon
whereby mutually trans-ligands bindcloser and more tightly to a uraniumcenter than they would in a d-block system, since the available (pseudocore)
U 6p orbitals can mix with the valence 5f.[28−31]We present a set of new
heterobimetallicuranium–group 10
metalcomplexes using these simple ligands, the first study of an
actinide–M bond for a complete transition-metal group and the
first set of differently trans-ligand-functionalizeduranium–metal
bonds. We show how the ligand supports the shortest 5f–ndmetal–metal bonds yet stabilized and preserves
the metal–metal bond while allowing steric/electronic variation
of the metal-bound X-ligand. These features have enabled a thorough
study of the electronic structure of the metal–metal bond and
its variation from 3d to 5d, and with ancillary ligand, for the first
time.
Synthesis
Preparation of the Ligand and Monometallic
Compounds
The base-free potassium salt of the heterobidentate
ligand2-tert-butyl-4-methyl-6-(diphenylphosphino)phenolate
(1, KOArP) may be prepared by deprotonation
of 2-tert-butyl-4-methyl-6-(diphenylphosphino)phenol[32] in THF with KH.The reaction of 3 mol
equiv of 1 withuranium(IV) iodide etherate in THF gives
IU(OC6H2-6-But-4-Me-2-PPh2-κ2O,P)3 [IU(OArP-κ2O,P)3, 2] as a bright green powder
in 78% yield (Scheme ).[25] Compound 2 is moderately
soluble in benzene andtoluene; 1H NMR spectroscopy shows
broad overlapping resonances at ambient temperature but seven resonances
at elevated temperatures, although even at 370 K these are still broad.
No 31P NMR resonance is observed at 300 or 370 K, similarly
to other uranium phosphinecomplexes, e.g., U(dmpe)2X4 (X = Cl, OPh, Me).[33,34] This could indicate a persistent coordination of the phosphine groups
to the paramagneticuranium or a more dynamic process that broadens
the resonances to baseline. The room-temperature magnetic moment (Evans’
method) of 2 is 2.4 μB.
Scheme 1
Synthesis
of Uranium(IV) Tris(aryloxide) Iodide 2
Green crystals of 2 suitable for
single-crystal X-ray
diffraction were grown from a benzene solution at ambient temperature.
The solid-state structure shows a coordination number of 7 for the
uraniumcenter with three bidentate phosphino-aryloxides (Figure ). The U–O
and U–I distances (ranging from 2.150(3) to 2.162(3) and 3.0414(6)
Å, respectively) are slightly longer than those previously reported
for IU(OC6H3-2,6-But2)3 [U–O, 2.092(8)–2.114(11) Å; U–I,
3.011(2) Å].[24] The difference is probably
due to the three additional phosphinedonor atoms in 2. The U–P bonds lie between 3.041(1) and 3.056(1) Å.
To the best of our knowledge there are no other examples of triarylphosphineuraniumcomplexes; hence, a comparison is limited to the few crystallographically
characterizedtrialkylphosphine uranium compounds. The U–P
bonddistances in 2 are similar to those of U(dmpe)2X4 (X = Cl, OPh, Me).[33,34] The related U(IV)(Pr2iPNMes-κ2P,N)3UI has U–Pdistances between 2.8662(12) and 2.8828(4) Å.[10]
Figure 1
Molecular structure of 2. Solvent molecules and hydrogen
atoms are omitted, and peripheral carbon atoms are depicted as a wireframe,
for clarity. Thermal ellipsoids are drawn at 50% probability. Selected
distances (Å) and angles (deg): U–I, 3.0414(6); U–O,
2.150(3)–2.162(3); U–P, 3.041(1)–3.056(1); O–U–P,
62.93(8)–63.14(8); O–U–I, 79.98(2)–82.43(2),
119.43(8)–124.53(8).
Molecular structure of 2. Solvent molecules andhydrogen
atoms are omitted, and peripheral carbon atoms are depicted as a wireframe,
for clarity. Thermal ellipsoids are drawn at 50% probability. Selecteddistances (Å) and angles (deg): U–I, 3.0414(6); U–O,
2.150(3)–2.162(3); U–P, 3.041(1)–3.056(1); O–U–P,
62.93(8)–63.14(8); O–U–I, 79.98(2)–82.43(2),
119.43(8)–124.53(8).
Preparation of the Bimetallic Compounds
The reaction
of 2 with low oxidation state group 10 metalcompounds
incorporates the respective metal throughphosphine ligation. The
uranium(IV)–nickel(0) derivative is prepared by treatment of 2 with an equimolar amount of Ni0(cod)2 (cod = 1,5-cyclooctadiene) in toluene at ambient temperature (Scheme ). An immediate color
change to dark red indicates fast displacement of cod by the triarylphosphinedonor groups. The new heterobimetallic IU(μ-OArP-1κ1O,2κ1P)3Ni (3–Ni) is isolated as dark redcrystals
in excellent yield and exhibits similar solubility to the parent compound 2.
Scheme 2
Preparation of the Bimetallic Uranium(IV) Complex 3–Ni, 3–Pd, and 3–Pt
For the preparation of the
heavier congeners, palladium(0) andplatinum(0) phosphines proved to be suitable precursors, whereas Pd2(dba)3 (dba = dibenzylideneacetone) was unsuitable
due to the ketone functional group [see the Supporting Information (SI)]. Reactions between equimolar amounts of 2 and tetrakis(triphenylphosphine)M(0) (M = Pd, Pt) in toluene
at 80 °C give the bimetallicuranium(IV)–palladium(0)
complex IU(μ-OArP-1κ1O,2κ1P)3Pd (3–Pd) anduranium(IV)–platinum(0) complex IU(μ-OArP-1κ1O,2κ1P)3Pt (3–Pt), respectively
(Scheme ). All three
bimetalliccomplexes 3–Ni, 3–Pd, and 3–Pt show remarkable thermal stability.Upon introduction of the group 10 metalcenters, the magnetic moment
decreases from 2.4 μB in 2 to 1.9 μB (3–Ni), 1.8 μB (3–Pd), and 2.0 μB (3–Pt), respectively. The similarity of the values for the bimetallic
systems might indicate analogous interaction between the different
d10-metals anduranium. However, a comparison of this group
trend with previously reported systems is not possible, since no magneticdata were given for the only pair of complexes in which the ligand
system remained unchanged between different transition-metalderivatives,
Cp3UMCp(CO)2 (M = Fe, Ru).[5] Our observation contrasts with that of the groups of Bart
and Thomas and of Arnold and Lu, who reported an increase of the magnetic
susceptibility after introduction of the cobaltcenter into the amidophosphine-ligateduraniumcompounds.[10,11]Single crystals suitable
for X-ray diffraction studies of the bimetalliccompounds were grown at ambient temperature by vapor diffusion of
hexane into benzene solutions. The solid-state structures of the bimetalliccomplexes 3–Ni, 3–Pd, and 3–Pt are similar and are shown in Figure . Selecteddistances and angles
are collected in Table along with the data from the DFT calculations described below. The
agreement between experiment and theory is very good.
Figure 2
Thermal ellipsoid plot
for 3–Ni, 3–Pd, and 3–Pt. Solvent molecules and hydrogen atoms
are omitted, and selected carbon atoms are depicted as a wireframe,
for clarity. Thermal ellipsoids are drawn at 50% probability, and
only one independent molecule out of nine in the asymmetric unit is
shown. Selected bond distances (Å) and angles (deg) are shown
in Table .
Table 1
Selected Bond Distances (Å) and
Angles (deg) of the Solid-State Structures of 3–Ni, 3–Pd, and 3–Pt and the
Calculated Values, Respectivelya
3–Ni
3–Pd
3–Pt
expl
calcd
expl
calcd
expl
U–M (Å)
2.527(2)–2.540(2)
2.534
2.686(2)–2.694(1)
2.701
2.706(1)–2.709(1)
U–I (Å)
3.007(1)–3.012(1)
3.008
2.994(1)–3.007(1)
3.014
3.007(1)–3.014(1)
U–O (Å)
2.134(8)–2.16(1),
2.166 (av)
2.12(1)–2.14(1)
2.162 (av)
2.125(5)–2.15(1)
M–P (Å)
2.222(5)–2.239(4)
2.264 (av)
2.361(3)–2.368(3)
2.396 (av)
2.320(4)–2.330(3)
I–U–M (deg)
178.94(5)–179.58(6)
178.0
178.90(5)–179.34(4)
178.3
178.80(3)–179.13(3)
U–M–P (deg)
91.7(1)–94.3(1)
90.36(9)–92.68(8)
91.11(7)–93.57(7)
O–U–M–P (deg)
26.4(3)–31.8(3)
25.3(2)–30.2(2)
24.6(2)–29.3(2)
Torsion angles are given for
oxygen and phosphorus atoms bound to the same bridging ligand.
Thermal ellipsoid plot
for 3–Ni, 3–Pd, and 3–Pt. Solvent molecules andhydrogen atoms
are omitted, and selectedcarbon atoms are depicted as a wireframe,
for clarity. Thermal ellipsoids are drawn at 50% probability, and
only one independent molecule out of nine in the asymmetric unit is
shown. Selected bonddistances (Å) and angles (deg) are shown
in Table .Torsion angles are given for
oxygen andphosphorus atoms bound to the same bridging ligand.Despite the C3-symmetry of the individual
molecules, the structures of 3–Ni and 3–Ptcould be refined only in the triclinic space group P1. The asymmetric unit of eachcontains nine molecules of the compound
along with three benzene molecules each. The individual molecules
show slightly different orientations andcould not be refined using
a space group of higher symmetry. Complex 3–Pd was solved and refined in the trigonal space group P32 andcontains three molecules of complex, with three
benzene molecules per complex, in the asymmetric unit. The U–M
bonddistances increase from 2.527(2)–2.540(2) Å in 3–Ni to 2.686(2)–2.694(1) Å in 3–Pd and 2.706(1)–2.709(1) Å in 3–Pt (Figure ). The intermetallic
bonddistances are significantly shorter than those of any other crystallographically
characterizedd- and f-block bimetalliccompound previously reported.
[The shortest, Lu–Pt, noted above, is 2.7668(5) Å.[20]] The only other actinide–group 10 derivatives
reported are Cp*Th(μ-PPh2)2Ni(CO)2 andCp*Th(μ-PPh2)2PtPMe3, featuring intermetallicdistances of 3.206(2) and 2.984(1) Å,
respectively.[18,19] To the best of our knowledge,
no other uranium–group 10 derivatives have been reported; comparison
with the bimetallic UIV–CoI ICo(μ-Ph2PNPri-1κ1P,2κ1N)3U[η2-Ph2PNPri] and ICo(μ-Ph2PNPri-1κ1P,2κ1N)3UI reported by the groups of Bart and Thomas
is most instructive.[10] The short intermetallic
bonds are accompanied by U–M–P bond angles larger than
90°: 91.7(1)–94.3(1)° (3–Ni),
90.36(9)–92.68(8)° (3–Pd), and 91.11(7)–93.57(7)°
(3–Pt). The increase in U–M bond lengthcaused by the increased atomic radius in the series from nickel to
platinum appears to be compensated by a decrease in O–U–M–P
torsion angle, leaving the anionic ligand sphere around the uraniumcenters virtually unaffected.The U–I bonds of 3–Ni, 3–Pd, and 3–Pt are shorter than those in the parent
monometallicderivative 2 by around 0.04 Å in all
cases. It is tempting to attribute this to the ITI. However, it could
simply be a result of the lower coordination number in the bimetalliccomplexes (5-coordinate at U, including the M–M bond) compared
to the phosphine-ligated parent compound (7-coordinate at U) since
the effective ionic radius of the 5-coordinate U will be up to 0.1
Å smaller.[35]The compounds 3–Ni, 3–Pd, and 3–Pt show paramagnetically shifted1H NMR resonances in the
range 3.56–11.82 ppm (3–Ni), 5.32–15.44
ppm (3–Pd), and 1.99–10.95 ppm (3–Pt). Again, the C3-symmetry of the solid-state
structures is
evident in solution, but the interconversion of the Δ and Λ
isomers can now be observed using variable-temperature (VT) NMR spectroscopic
experiments in the range 300–370 K (Figure for 3–Ni), withcoalescence
relating to the interconversion shown in Figure , which requires the breaking of the U–M
bond.
Figure 3
Stacked variable-temperature 1H NMR spectra of 3–Ni in toluene-d8 from
3.2 to 6.6 ppm over a temperature range of 300–370 K. Asterisks
indicate resonances of phenyl hydrogen atoms observable at 300 and
370 K.
Figure 4
Simplified Newman projection illustrating the
helicity of the bimetallic
complexes.
Stacked variable-temperature 1H NMR spectra of 3–Ni in toluene-d8 from
3.2 to 6.6 ppm over a temperature range of 300–370 K. Asterisks
indicate resonances of phenyl hydrogen atoms observable at 300 and
370 K.Simplified Newman projection illustrating the
helicity of the bimetalliccomplexes.In the case of 3–Ni, two sets of distinct resonances
are observed at ambient temperature for the two phenyl groups on the
diphenylphosphine substituents. These can be accounted for by the
two orientations of the rings either close to perpendicular or along
the metal–metal axis, which are visible at elevated temperatures
(see the SI). For 3–Pd, no phenyl resonances are observed at ambient temperature and for 3–Pt they are strongly broadened.The coalescence
temperatures (TC) were
highest for 3–Ni at ca. 332 K followed by 3–Pt at around 314 and 300 K for 3–Pd. In the case of 3–Pt, strong broadening and
overlapping of unrelated shifts allow only a rough estimation of TC. This agrees with the other data, making U–Ni
the hardest bond and U–Pt the easiest bond to break to interconvert
the isomers. Unfortunately, the presence of the paramagnetic U center
precludes the calculation of the energy associated with these dynamic
processes due to the additional temperature dependence of the chemical
shifts.The broadened31P{1H} resonances
appear at
300 K at 93.2 ppm (3–Ni), 68.0 ppm (3–Pd), and 85.5 ppm (3–Pt), with the latter compound
showing a 31P–195Ptcoupling constant
of 3742 Hz. These chemical shifts are all higher than the 31P NMR resonances for the “naked equivalent” group 10
metalcomplexes M(PPh3)3, M = Ni (21 ppm), Pd
(23 ppm), Pt [50 ppm, 1J(31P–195Pt) = 4438 Hz], but the influence from the
uranium paramagnet cannot be quantified. In the absence of paramagnetism,
a related shift to higher frequency on incorporation of the more electropositive
metalhas been used as an (unquantified) indication of group 10 metal
→ metal electron donation.[17,18,36,37,18,19,38] The significantly lower 31P–195Ptcoupling
constant in 3–Ptcompared to Pt(PPh3)3 can also be taken as an indication of a 4-coordinate
platinum(0).[19]
Computational Investigation
of 3–Ni and 3–Pd
In order to probe the uranium–TM
(transition metal) bonding within 3–M, we turned
to density functional theory (DFT) at the PBE level. Calculated geometricdata for 3–Ni and 3–Pd are
collected in Table .[39] As noted above, the agreement between
the calculated and experimental structures is excellent, the largest
discrepancy being <0.04 Å (for the average Ni–Pdistances
in 3–Ni).Natural population analysis (NPA)
data are presented in Table , from which it can be seen that the two systems have very
similar electronic structures at the NPA level. The spindensities
are very much in keeping with a U(IV) system. Partial charges rarely
tally well with formal oxidation state, but those calculatedhere
show that the actinide atoms are much more positive than the transition
metals and are very close to zero for the latter, in keeping with
an M(0) formalism. The population analysis shows that the 10 electrons
expected for Ni(0) andPd(0) are located mainly in the 3d and 4d orbitals,
with a small 4s/5s population. The uranium populations show the expected
buildup in 5f and 6d, 1.12/1.08 and 1.50/1.46 electrons, respectively, above the value expected for
U(IV) (data for 3–Pd in italics). Such buildups
are often taken as a measure of the extent to which the 5f and 6d
orbitals are involved in covalent bonding with the surrounding ligand
framework.[39−41] We are happy to adopt this approach for the early
part of the 5f series, and the present data indicate significant involvement
of both f- andd-orbitals.
Table 2
Natural Population
Analysis Data for 3–Ni and, in Italics, 3–Pd
spin density
partial charge
atomic populations
U
2.146
1.079
5f3.126d1.507s0.217p0.01
U
2.137
1.198
5f3.086d1.467s0.197p0.01
Ni
–0.075
0.091
3d9.394s0.48
Pd
–0.032
0.050
4d9.445s0.47
I
–0.038
–0.277
5s1.885p5.395d0.01
I
–0.040
–0.298
5s1.895p5.405d0.01
P (av)
0.000
0.881
P (av)
–0.003
0.872
O (av)
–0.018
–0.700
O (av)
–0.018
–0.708
Further insight into 3–Ni is provided by analysis
of the valence natural localized molecular orbitals (NLMOs), the compositions
andcharacters of an α spin selection of which are collected
in Table and shown
pictorially in Figure . NLMOs 110 and 111 are the two U 5f electrons. NLMOs 113 and 114
are strongly iodine-localized (ca. 92%) andpπ in character,
while NLMO 128 is I pσ, with a significantly larger (ca. 20%)
uraniumcontribution than the pπ levels. The remaining orbitals
(115–118 and 129) are nickel 3d-based. Together with the five
β spin equivalents, these NLMOs house the 10 nickel electrons
located by the NPA. They separate into σ + 2π + 2δ
with respect to the U–Ni axis, withdiffering contributions
from the actinide. The δ orbitals (115 and 116) have essentially
no uraniumcontribution, while the π orbitals (117 and 118),
also strongly nickel-localized, have slightly larger uraniumcontributions
(similar to those of the iodinepπ-localized orbitals). Finally,
NLMO 129 is nickeldσ, withca. 10% uraniumcharacter. The uraniumcontributions to the iodine-based NLMOs are more 6d-based than 5f,
while the reverse is true for the nickel-localized orbitals.
Table 3
Compositions (%) and Principal Characters
of Selected α Spin Valence NLMOs of 3–Ni and, in Italics, 3–Pd
Selected valence NLMOs of 3–Ni. Isosurface
value = 0.04. Atom colors: iodine = purple, uranium = lighter blue,
oxygen = red, nickel = darker blue, phosphorus = yellow, and carbon
= gray. Hydrogen atoms are omitted for clarity.
Selected valence NLMOs of 3–Ni. Isosurface
value = 0.04. Atom colors: iodine = purple, uranium = lighter blue,
oxygen = red, nickel = darker blue, phosphorus = yellow, andcarbon
= gray. Hydrogen atoms are omitted for clarity.In order to probe further the nature of the U–Ni and
U–Pd
bonds, we turned to the quantum theory of atoms-in-molecules (QTAIM)
approach, which we have used extensively to study the electronic structure
of 5f molecules.[26,41−43] Bondcritical
point (BCP) data are collected in Table , together with five different measures of
U–TM bond order. The BCP electron and energy densities and
the electron density Laplacian (ρ, H, and ∇2ρ) are very similar for the two target systems and very
much in keeping with the extensive previous QTAIM studies of metal–metal
bonds, in both bulk metals and polynuclear complexes.[44−57] These have suggested that metal–metal bonding should not
be pigeon-holed as either closed-shell or shared-shell, but that “metallic”
bonding has a topological behavior of its own, possessing neither
ionic nor covalent features; metal–metal bonds are identified
by relatively low electron density at the BCP and positive ∇2ρ (normally associated withclosed shell or ionic bonding)
and negative H (usually typical of shared shell or
covalent bonding).
Table 4
QTAIM U–TM
BCP Parameters and
Delocalization Indices and Bond Orders for 3–Ni and 3–Pd and Model Compounds 3–Ni(m) and 3–Pd(m) [(PH3)3MU(OH)3I (M = Ni, Pd)]a
3–Ni
3–Pd
3–Ni(m)
3–Pd(m)
ρ
0.068
0.065
0.043
0.041
∇2ρ
0.144
0.128
0.064
0.078
H
–0.019
–0.018
–0.010
–0.008
ε
0.024
0.028
0.019
0.012
δ(U,TM)
0.955
0.777
0.633
0.514
Wiberg bond
order
0.720
0.625
0.457
0.403
atom–atom net linear NLMO/NPA bond order
0.813
0.685
0.446
0.363
Mayer bond order
0.831
0.598
0.716
0.489
Gopinathan–Jug bond order
0.911
0.640
0.595
0.411
ρ, H,
and ∇2ρ are in atomic units.
The BCP ellipticity ε is a measure
of the cylindrical symmetry
of a bond. Values close to zero are associated with either single
or triple bonds, while significant deviations from zero (up to ca.
0.45) are typical of double bondcharacter.[58] For both 3–Ni and 3–Pd,
ε is very close to zero. The highly nickel localized nature
of NLMOs 115–118 and 129 of 3–Ni strongly
suggests that these ellipticities are not indicative of the higher,
i.e., triple bond order, and this is supported by the QTAIM delocalization
indices δ(U,TM), which are measures of bond order and which
are below 1 for both 3–Ni and 3–Pd. Table also provides
four further U–TM bond order metrics. All of these agree that
the U–Ni bond order is less than 1 and that that of U–Pd
is smaller than for the 3d analogue. The lower bond orders found for
the Pd system are in keeping with the composition of the NLMOs (Table ). Specifically, the
TM-baseddσ anddπ orbitals are even more localized on
the transition metal in 3–Pd than in 3–Ni, leading to reduced U–TM covalency. Althoughmetal–metal
bonding interactions typically increase down a transition-metal group,[59] the present NLMO data are consistent with the
electronegativities of Ni, Pd, and U, 1.91, 2.20, and 1.38, respectively,
on the Pauling scale.[60] The more electronegative
4d element has a more polar interaction with the actinide than does
Ni, leading to reduced bond order.ρ, H,
and ∇2ρ are in atomic units.To the best of our knowledge, there
are no comparable computational
analyses of the bond order in zero oxidation state group 10 complexes
containing a homobimetallicmetal–metal bond, so we carried
out our own calculations on a previously reported low oxidation state
system with an unconstrained Ni–Ni (or Pd–Pd) bond,
[(η5-Cp)M(PEt3)]2.[61] Unfortunately, while geometry optimization of
the 3d system proceeded smoothly, that for the Pddimer did not, collapsing
to a nonsensical solution. Thus, comparative M–M bonddata
are not available.In summary, we conclude that the U–Ni
and U–Pd interactions
have topological features typical of metal–metal bonds. Analysis
of the localized orbital structure locates MOs of σ and π
symmetry between the actinide and the transition metals, but these
are heavily polarized toward the latter, resulting in small orders. 3–Pd features consistently smaller bond orders than 3–Ni, in agreement with greater TM σ and π
NLMO localization.In order to probe the extent to which the
U–TM interaction
is a function of the geometricconstraints placed on the metal atoms
by the bidentate ligand framework, we have optimized the geometries
of the model compounds 3–Ni(m) and 3–Pd(m) [(PH3)3MU(OH)3I (M = Ni, Pd)],
i.e., with the chelate bridge broken, to ascertain whether L really
does flex/twist sufficiently to enable the “ideal” M–M
separation. The U–I distances are very similar to those calculated
for 3–Ni and 3–Pd, 2.993 and
2.995 Å, respectively. By contrast, there is a significant lengthening
of the U–TM distances, to 2.784 and 2.932 Å, respectively,
for 3–Ni(m) and 3–Pd(m), an
increase of ca. 0.25 Å vs 3–Ni and 3–Pd. This lengthening is reflected in the QTAIM and
bond order metrics for the U–TM interaction, collected in Table , which are all smaller
(in an absolute sense) than in 3–Ni and 3–Pd. As with the full molecules, all of the bond orders
are smaller in the model Pd system than the Ni one.The data
on these model compounds therefore indicate that the very
short uranium–TM bonds observed in 3–Ni and 3–Pd are partly a function of the ligand
framework. In the absence of constraining ligands, the 5f–nd bonds lengthen, thoughuranium–TM interactions
are clearly still present. The bond orders in the unchelatedcompounds
are, in general, a little more than half of those calculated for 3–Ni and 3–Pd.
Derivatization
of the Bimetallic Compounds
In addition
to the variation of the d-metalcenter, we investigated the effect
on the metal–metal bond of exchanging the iodide for other
ligands, focusing on the smaller Ni because of its stronger U–Ni
bond. For this purpose it seemed reasonable to substitute the large,
polarizable iodide for the more electronegative and strongly bonding
fluoride. In order to differentiate between electronic and steric
effects, we also included a sterically demanding andhard O-donor
ligandtrimethylsiloxide (OSiMe3). Treatment of 3–Ni withsodium trimethylsiloxide yields the corresponding uranium(IV)
siloxidecompound 4 (Scheme ) andsodium iodide. The reaction of 3–Ni withcesium fluoride results in the elimination
of cesium iodide to give the F–UIV–Ni0complex 5 (Scheme ). Reaction monitoring via 1H
and31P NMR spectroscopy shows quantitative formation of 4 and 5, respectively, within 24 h. Attempts
to use silver fluoride instead of cesium fluoride resulted in decomposition
of the bimetallic species and release of an oxidizednickel(II)complex
NiII(OArP-κ2O,P)2 (6), which was characterizedcrystallographically (see the SI). Adaptation
of a published preparation allowed 6 to be prepared independently
by reaction of 2 equiv of HOArP with 1 equiv of Ni(cod)2 in toluene (see the SI).[62] Reactions of 3–Ni aimed
at the formation of a cationiccompound using silver tetraphenylborate
or potassium tetraphenylborate gave 6 or no conversion,
respectively (see the SI). A bis(trimethylsilyl)amidoderivative of 3–Ni was also targeted, but the
reaction between 3–Ni andpotassium bis(trimethylsilyl)amidedid not show any conversion (see the SI).
Scheme 3
Preparation of Bimetallic Trimethylsiloxide (4) and
Fluoride Derivatives (5)
Dark redcrystals of 4 suitable for X-ray
crystallography
were grown from a benzene/hexane solution at ambient temperature.
Single crystals of 5 were obtained from a benzene-layeredTHF solution. The two bimetalliccomplexes feature U–Ni bonddistances of 2.556(1) Å (4) and 2.520(1) Å
(5) (Figures and 7), respectively. For 4, this is slightly longer than in 3–Ni, likely
a result of the increased spatial demand of the OSiMe3 substituent
compared with the iodide and thus a greater stericclash with the tert-butyl groups of the aryl oxide ligands. However, the
exchange of iodide for the smaller, more electronegative fluoride
in 5 is accompanied by a decrease of the intermetallic
bonddistance. While this could be associated with a reorganization
of the OArP ligand set, it could also be attributed to
the inverse trans influence. The siloxide U–O bonddistance
of 2.093(6) Å in 4 is significantly shorter than
the U–OAr bonds but within the range of previously
reported values for uranium(IV) trimethylsiloxides.[63−68] The U–F distance of 2.091(5) Å in 5 is
within the range of other nonbridging uranium(IV) fluoridecompounds.
The Ni–P bonds in 4, 2.208(1)–2.221(2)
Å, and 5, 2.212(2)–2.225(3) Å, are slightly
shorter than in the parent compound, indicating increased back-bonding
via the σ*(Ni–P) orbitals.[69] In the solid state, both the U1–O4–Si1 [174.9(4)°]
and Ni1–U1–O4 [178.6(2)°] angles in 4 are nearly linear. The F–U–Ni angle in 5 is 178.8(2)°, similar to that of its congener. The U–F
bonddissociation energy is measured to be around 50% stronger than
the other U–halide bonds in UX4, and the U–Ni
bond lengthdecreases in the order SiO–U–Ni > I–U–Ni
> F–U–Ni (i.e., 4 > 3–Ni > 5). The ITI would predict a stronger than usual
U–O
bond in the linearly boundsiloxide 4. If the MM strength
order predicted by electrochemistry (vide infra) (SiO–U–Ni
> F–U–Ni > I–U–Ni, i.e., 4 > 5 > 3–Ni) directly correlated
with M–M bond length, then the solid-state and solution methods
would agree on the halide ordering, perhaps indicating the strongest
ITI in the fluoridecomplex 5.[70] However, the stericcongestion around the U–siloxide evidenced
by the solid-state structure and the NMR spectra of 4 suggests that in this instance there is insufficient space for an
(ITI-facilitated) closer approach of the O and Ni atoms to U.
Figure 6
Thermal
ellipsoid plots for 4 and 5.
Solvent molecules and hydrogen atoms are omitted, and selected carbon
atoms are depicted as a wireframe, for clarity. Thermal ellipsoids
drawn at 50% probability. Selected bond distances (Å) and angles
(deg) for 4: U1–Ni1, 2.556(1); U1–O1, 2.210(6);
U1–O2, 2.188(6); U1–O3, 2.160(6); U1–O4, 2.093(6);
Ni1–P1, 2.208(2); Ni1–P2, 2.213(3); Ni1–P3, 2.221(2);
O4–U1–Ni1, 178.6(2); U1–Ni1–P1, 87.85(7);
U1–Ni1–P2, 97.84(7); U1–Ni1–P3, 94.95(7);
O1–U1–Ni1–P1, 37.4(2); O2–U1–Ni1–P2,
18.4(2); O3–U1–Ni1–P3, 28.1(2). For 5: U1–Ni1, 2.520(1); U1–F1, 2.091(5); U1–O1,
2.159(8); U1–O2, 2.174(6); U1–O3, 2.199(5); Ni1–P1,
2.225(3); Ni1–P2, 2.215(3); Ni1–P3, 2.212(2); F1–U1–Ni1,
178.8(2); U1–Ni1–P1, 96.16(7); U1–Ni1–P2,
91.56(7); U1–Ni1–P3, 91.82(7); O1–U1–Ni1–P1,
22.2(2); O2–U1–Ni1–P2, 30.1(2); O3–U1–Ni1–P3,
29.1(2).
Figure 7
Thermal ellipsoid plot
for 3–Ni (left) and 4 (right) viewed
along the U–Ni bond axes. Solvent
molecules and hydrogen atoms are omitted and selected carbon atoms
are depicted as a wireframe for clarity. Thermal ellipsoids are drawn
at 50% probability.
The aryloxide U–O bonds in both 4 and 5 are longer than they are in 3–Ni [2.160(6)
to 2.210(6) Å in 4 and 2.159(8) to 2.199(5) Å
in 5], a feature whichcould be attributed to the preferential
shortening of the trans X–U–Ni unit, even for the sterically
demanding OSiMe3 group. The top-view of the solid-state
structures of the U–Ni iodide andsiloxide (3–Ni and 4, respectively) are also shown in Figure to highlight the C3-propeller shape and similarity of the overall structures.Thermal
ellipsoid plots for 4 and 5.
Solvent molecules andhydrogen atoms are omitted, and selectedcarbon
atoms are depicted as a wireframe, for clarity. Thermal ellipsoids
drawn at 50% probability. Selected bonddistances (Å) and angles
(deg) for 4: U1–Ni1, 2.556(1); U1–O1, 2.210(6);
U1–O2, 2.188(6); U1–O3, 2.160(6); U1–O4, 2.093(6);
Ni1–P1, 2.208(2); Ni1–P2, 2.213(3); Ni1–P3, 2.221(2);
O4–U1–Ni1, 178.6(2); U1–Ni1–P1, 87.85(7);
U1–Ni1–P2, 97.84(7); U1–Ni1–P3, 94.95(7);
O1–U1–Ni1–P1, 37.4(2); O2–U1–Ni1–P2,
18.4(2); O3–U1–Ni1–P3, 28.1(2). For 5: U1–Ni1, 2.520(1); U1–F1, 2.091(5); U1–O1,
2.159(8); U1–O2, 2.174(6); U1–O3, 2.199(5); Ni1–P1,
2.225(3); Ni1–P2, 2.215(3); Ni1–P3, 2.212(2); F1–U1–Ni1,
178.8(2); U1–Ni1–P1, 96.16(7); U1–Ni1–P2,
91.56(7); U1–Ni1–P3, 91.82(7); O1–U1–Ni1–P1,
22.2(2); O2–U1–Ni1–P2, 30.1(2); O3–U1–Ni1–P3,
29.1(2).According to NMR spectroscopy,
both 4 and 5 differ significantly in solution
from the parent compound 3–Ni. The 1H NMR resonances for the aryl
oxide ligands are in the range from −15.28 to 19.44 ppm for 4 and from −11.70 to 19.04 ppm for 5,
with a more strongly pronounced paramagnetic influence on the ligand
sphere compared with 3–Ni. The proton chemical
shift of the trimethylsiloxide group of 4 is 48.67 ppm.
Further, the 31P resonances are strongly shifted to high
frequencies, 469.4 ppm (4) and 474.5 ppm (5) (compared with 92.3 ppm for 3–Ni). Having studied
the NLMOs of the complexes involved and not found any significant
differences, we attribute the large chemical shift difference to two
factors. First, the extensive electronicdifferences of I vs F/TMSO.
Second, the slightly shorter Ni–P bonds in 4 than 5 that indicate stronger Ni–P backbonding. Both of
these wouldcombine to enhance the through-bond paramagnetic influence
from the f2-uraniumcenter. Resonances for the heteronuclei 19F and29Sicould not be observed within the spectral
range from −740 to 620 and −1050 to 870 ppm, respectively.
VT NMR experiments of 4 and 5 show that
bothhave rigid structures in solution as high as 100 °C. This
represents a significantly higher energy barrier to the interconversion
of Δ and Λ isomers compared with 3, supporting
the ITI-induced stronger U–M bond being formed when the more
electronegative X-ligands are uranium-bound. The replacement of the
iodidechanges the magnetic moment values from 1.9 μB (3–Ni) to 2.8 μB (4) and 2.1 μB (5), respectively. Similarity
of magnetic moment throughout series of U(IV) aryl oxide andamidecomplexes withdifferent halideshas been reported.[71−73] The value of
the trimethylsiloxidederivative 4 is similar to that
of other R3SiO-ligateduraniumcomplexes, U(OSiBu3t)4 (2.83 μB) and U(OSiMe3)2I2(bipy)2 (bipy = 2,2′-bipyridine)
(2.7 μB).[65,74] To account for these
increases, and the strongly paramagnetically shifted31Pchemical shifts for 4 and 5, we compared
the composition of the two f-based NLMOs for the iodide (3–Ni) andfluoride (5) to look for different U 5f contributions
that would lead to larger paramagnetic shifts for the Ni-bound atoms.
For the iodide, they are 99.18% U (99.56% 5f) and 94.81% U (97.24
5f, 2.05 s, 1.75% total contribution from P) (see also Table S4 of the SI for a comparison of the predominantly
Ni d-σ and π NLMOs). For the fluoride they are 99.22%
U (99.68% 5f) and 92.54% U (97.58 5f, 1.63 s, 2.48% total contribution
from P). While these data indicate a marginally greater through-bond
mixing of unpaired 5f electron with the phosphorus, there is really
very little difference between the two systems.Thermal ellipsoid plot
for 3–Ni (left) and 4 (right) viewed
along the U–Ni bond axes. Solvent
molecules andhydrogen atoms are omitted and selectedcarbon atoms
are depicted as a wireframe for clarity. Thermal ellipsoids are drawn
at 50% probability.The electronic absorption
spectra of toluene solutions of the compounds 2–5 were recorded to locate potential
metal–metalcharge transfer bands (see the SI). UV–vis spectra of monometallic 2 show
several weak U(IV) f–f transitions[75] up to ca. 700 nm and more intense π–π* charge-transfer
processes below 500 nm.[76,77] The secondmetalation
to form 3–Ni, 3–Pd, and 3–Ptcauses a bathochromic shift of the predominately
ligand-based absorption at short wavelengths. In the visible region,
the nickelderivative 3–Ni differs significantly
from 3–Pd and 3–Pt, with an
absorption at 511 nm (ε 598 M–1 cm–1) that is much stronger than that in 4 and 5, with weaker absorptions at 527 nm (ε 103 M–1 cm–1) and 533 nm (ε 90 M–1 cm–1), respectively. In the NIR region the monometalliccomplex 2 shows several absorption bands in the 850–2060
nm region (ε 18–45 M–1 cm–1). The NIR spectra of 3–Ni, 3–Pd, and 3–Pt are similar to each other but feature
fewer absorption bands. As such, an unambiguous assignment of absorptions
in this region to a metal–metalcharge transfer appears to
be not possible.
Electrochemistry
The electronic
structures of complexes 2–5 were
investigated using a range of voltammetric techniques
(Figure and the SI). In the electrochemical window provided by
THF/[nBu4N][BPh4], a single reduction
process was observed for 2 during the cyclic voltammetry
(CV) experiment, at Epc −2.87
V versus Fc+/Fc, assigned to the U(IV)/U(III) couple and
it is irreversible. The U(IV)/U(III) redox couple is sensitive to
the ligand environment andhas been reported in the range from −1.83
to −2.78 V for metallocene andacetylacetonate (acac) complexes.[78−80]
Figure 8
Cyclic
voltammograms for 3–Pt, 3–Pd, 3–Ni, 4, and 5. All
measured in THF using 0.1 M [nBu4N][BPh4] as the supporting electrolyte, at a scan rate of 100 mV
s–1. The currents are normalized against the peak
height of reduction process I for 3–Pt.
Cyclic
voltammograms for 3–Pt, 3–Pd, 3–Ni, 4, and 5. All
measured in THF using 0.1 M [nBu4N][BPh4] as the supporting electrolyte, at a scan rate of 100 mV
s–1. The currents are normalized against the peak
height of reduction process I for 3–Pt.Incorporation of the group 10
transition metal alters the electrochemistry
significantly. The CVs of 3–Ni, 3–Pd, and 3–Pt are qualitatively very similar, having
three reduction processes each, suggesting a common electronic structure.
The electrochemical behavior of 3–Pt will be described
as a representative example. The first reduction (denoted I) at Epc −1.92 V is irreversible;
two further quasi-reversible reduction processes are observed as overlapping
cathodic waves at Epc −2.39
and −2.55 V, denoted II and III, respectively. Determination
of the peak areas in the CV of 3–Pt reveals that
the charge passedduring reduction I is equal to that passedduring
II and III combined, indicating that process I is a two-electron reduction,
whereas II and III are single-electron reduction processes.The electrochemical experiments with 3–Ni and 3–Pd generated identical conclusions, and in the series 3, the reduction potentials for all three processes are cathodically
shifted when the transition metal is changed from Pt to Pd to Ni.
The Kohn–Sham α spin LUMOs of both 3–Ni and 3–Pd are primarily U–M antibonding,
so we ascribe reduction I to the filling of this orbital andconclude
that the cathodic shift of the reduction process moving up the group
10 metals is due to a strengthening of the metal–metal bond.[81] This agrees with the computational results that
showedhigher bond order for 3–Ni compared to 3–Pd and also correlates with the shorter M–M′
distance determinedcrystallographically.The CV of 5, the fluoride analogue of 3–Ni, shows only an
irreversible reduction at Epc −2.39 V, but square-wave voltammetry (SWV)
reveals a second process at the edge of the electrochemical window, Epc −2.81 V. This implies that 5 displays similar electrochemical behavior to the iodocomplexes,
albeit at more negative potentials; i.e., replacing the iodide with
a fluoride strengthens the metal–metal bond trans to it.The replacement of iodide withsiloxide to make 4 cathodically
shifts the reduction I further still, to Epc −2.50 V; no other reduction processes are observed
by CV or SWV. This reduction is now quasi-reversible and suggests
that the reduced species is stabilized to a certain degree. A reversible
oxidation process is also observed at E1/2 −0.20 V, denoted IV. The area of the anodicCV wave for IV
is approximately equal to the area of the cathodic wave for reduction
I, and both processes therefore involve two electrons. It is not known
whether this oxidation IV is unique to 4; it may be that
this oxidation is possible for all but lies outside of the electrochemical
window.Thus, we infer from the electrochemical data that the
metal–metal
bond strength increases in the series 3–Pt < 3–Pd < 3–Ni < 5 < 4.
Conclusions
The use of a relatively
rigidheterobidentate phosphinoaryl oxide
ligand that forms strong U–O bonds and weak, labile U–P
bonds in the new complex IUIV(OArP-κ2O,P)3 has allowed
the systematic incorporation of Ni(0), Pd(0), or Pt(0) via phosphinecoordination, and the replacement of the iodide anion with Me3SiO– or F–, to form a
set of five heterobimetallic U–M complexes XUIV(μ-OArP-1κ1O,2κ1P)3M0 (X = I, OSiMe3, F; M = Ni, Pd, Pt), all of whichhave shorter An−TM bonds
than any previously reported example. The synthesis of a complete
set of adducts from a single group for the first time and the solution
and solid-state structural characterization of the complexes have
enabled a thorough study of the uranium–metal bond. The U–I
bond length in the starting material 2 becomes significantly
shorter upon formation of the U–M complexes 3,
but the coordination number changes from 7 to 5 (replacing three phosphines
with one metalcenter), so inferences of the inverse trans influence
(ITI) cannot be made here. Upon introduction of the group 10 metalcenters, the magnetic moment decreases from 2.4 μB to around 1.9 μB in 3, respectively,
an opposite change in moment to that reported upon secondary metalation
of U complexes by CoI as a donor.[10]Although the changes in magnetic moment and UV–vis–NIR
spectra cannot yet be interpreted in terms of bonding trends in the
series, the combination of experimental electrochemistry andcomputation
is particularly informative. A cathodic shift of the first reduction
process observed upon moving from U–Pt up to U–Ni indicates
a strengthening of the metal–metal bond in the order 3–Ni > 3–Pd > 3–Pt. This correlates with the shortening of the internuclear distance
determinedcrystallographically. Natural population analysis and natural
localized molecular orbital compositions indicate that U employs both
its 5f and 6d orbitals in covalent bonding to a significant extent,
and this agrees with experimental data that the oxidation states of
the metals are best described as U(IV) and zero for the group 10 atoms.
Quantum theory of atoms-in-molecules analysis yields bondcritical
point properties in keeping with many previous studies of transition-metal–metal
bonds in both bulk metals and polynuclear clusters (relatively low
electron density, positive ∇2ρ, and negative H). Replacing the uranium-boundiodide trans to the nickelcenter with the more electronegative fluoride andsiloxide also results
in NMR spectroscopic and electrochemical responses consistent with
a strengthening of the U–Ni bond and with the existence of
an ITI. If an ITI is influencing the M–M′ bond strength,
then this is also borne out by the crystallographicdata for 3 and 5, which show a shorter U–Ni bond
in the F–U–Ni (5) than in I–U–Ni
(3) complexes. Despite the short U–M distances,
the bond orders are calculated by five different approaches to be
small; less than 1 in all cases. All bond order metrics are smaller
for U–Pd than U–Ni, in agreement with the electrochemical
and QTAIM bondcritical point data and with population analysis of
the U–TM σ and π NLMOs which, while heavily localized
on the TM in bothcases, are even more so for the 4d system than the
3d, in keeping with the larger electronegativity difference between
U andPd vs U and Ni. Calculations on a monodentate analogue of 3 show that in the absence of the constraining ligand geometry
there is clearly still a U–TM interaction, but it is enhanced
by about 0.25 Å in the constraining ligand framework.Thus,
by combining the spectroscopic, computational, electrochemical,
and structural studies, the U–M bond strengthcan be placed
in increasing order: 3–Pt < 3–Pd < 3–Ni < 5 < 4, i.e., I–U–Pt < I–U–Pd < I–U–Ni
< F–U–Ni < SiO–U–Ni.
Experimental Section
General Details
All manipulations
were carried out
under a dry, oxygen-free atmosphere of nitrogen using standard Schlenk
and glovebox technique. Benzene was distilled from potassium and stored
over 4 Å molecular sieves. Hexane, THF, andtoluene were degassed
and purified by passage through activated 4 Å molecular sieves
or activatedalumina towers and stored over 4 Å molecular sieves.
Deuterated solvents, benzene-d6 andtoluene-d8, were boiled over potassium, vacuum-transferred,
and freeze–pump–thaw degassed prior to use. 1H, 13C, 19F, 29Si, and31P NMR spectra were recorded on Bruker AVA400, AVA500, or PRO500 spectrometers
at 300 K. Variable-temperature NMR spectra were recorded on a Bruker
AVA400 spectrometer between 300 and 370 K. Chemical shifts are reported
in parts per million, δ, referenced to residual proton resonances,
andcalibrated against external TMS. Magnetic moment values were determined
by Evans’ method using a sealedbenzene-d6capillary as reference.[82−85] UV–vis–NIR spectra
were recorded on a JASCO V-670 spectrophotometer using a sealed quartz
cuvette with 0.02–5 mM toluene solutions. Artifacts at 1650–1750
nm relate to solvent absorption. Electrochemical measurements were
made on 1–10 mM of the analyte in 12 cm3 THF, 0.1
M [nBu4N][BPh4], in a N2-filled glovebox using an Autolab ECO Chemie PGSTAT potentiostat,
glassy-carbondisk (d = 3 mm) working electrode,
Pt-gauze counter electrode, Ag-wire quasi-reference electrode, andferrocenium/ferrocene (Fc+/Fc = 0 V) standard.[86] Scan details are in the SI, anddata were processed using GPES Manager 4.9. Elemental
analyses were carried out at London Metropolitan University, London,
UK, andPascher Labor, Remagen, Germany. UI4(dioxane)1.5,[87] HOC6H2-6-But-4-Me-2-PPh2,[32] andAgBPh4[88] were prepared
according to published procedures. All other reagents were from commercial
sources and used as received.
KOC6H2-6-But-4-Me-2-PPh2 (KL, 1)
A Schlenk flask was charged
with6-tert-butyl-4-methyl-2-(diphenylphosphino)phenol
(5.92 g, 17.0 mmol, 1 equiv), potassium hydride (682 mg, 17.0 mmol,
1 equiv), and a stir bar andcooled in an ice bath. THF (40 mL) was
added under vigorous stirring, and the mixture was allowed to warm
to 20 °C after 30 min, and no further H2 evolution
was observable. After storage at 5 °C for 18 h, the colorless
solids were isolated via filtration, washed withhexane (3 ×
10 mL), anddried in vacuo to give 1 as a colorless powder
(5.33 g, 81%). 1H NMR (THF-d8): 1.40 (s, 9H, tBu), 1.93 (s, 3H, Me), 5.99 (m,
1H, ArH), 6.79 (d, 4JH,H 2.4
Hz), 7.20–7.26 (m, 6H, Ph), 7.30–7.34 (m, 4H, Ph). 13C NMR (THF-d8): 21.4, 30.4, 35.4
(d, 4JC,P 2.3 Hz), 116.8 (d, 3JC,P 3.1 Hz), 122.4 (d, 1JC,P 13.8 Hz), 128.6 (d, 2JC,P 6.5 Hz), 128.6, 135.0 (d, 3JC,P 18.8 Hz), 136.2 (d, 3JC,P 1.5 Hz), 142.2 (d, 1JC,P 11.5 Hz), 171.1 (d, 1JC,P 17.2 Hz). 31P{1H}
NMR (THF-d8): −15.0. Anal. Calcd
for C23H24KOP: C 71.47. H 6.26. Found: C 71.56,
H 6.31.
IU(μ-OC6H2-6-But-4-Me-2-PPh2-κ2O,P)3 (IUL3, 2)
A Schlenk flask
was charged withUI4(Et2O)2 (2.68
g, 3.00 mmol), a stir bar, andTHF (20 mL). Under vigorous stirring
a THF solution of 1 (3.48 g, 9.00 mmol, 3.00 equiv, 30
mL) was added via syringe. The green mixture was stirred at room temperature
for 16 h, followed by evaporation of volatiles under reduced pressure.
The green residue was extracted four times with warm toluene. The
green extract was concentrated to 40 mL and stored at −30 °C,
giving 3.28 g (78%) of 2 as a bright green powder. 1H NMR (toluene-d8): 4.96 (v br). 1H NMR (toluene-d8, 370 K): 1.83
(br), 4.88 (br), 5.12, 5.30 (br), 6.54 (v br), 8.89 (v br), 15.10
(v br). Evans’ method (C6D6): 2.4 μB. UV–vis–NIR [λ in nm (ε in M–1 cm–1)]: 300 (1.8 × 104), 516 (38), 550 (18), 598 (16), 633 (26), 895 (29), 976 (19),
1023 (27), 1069 (31), 1102 (35), 1139 (32), 1175 (27), 1198 (26),
1351 (22), 1406 (27), 1484 (18), 1829 (10), 2055 (45). Anal. Calcd
for C69H72IO3P3U: C 58.89.
H 5.16. Found: C 59.03, H 5.06.
IUIVL3Ni0 (3–Ni)
A Schlenk flask
equipped with a stirring bar was charged
with 2 (422 mg, 0.300 mmol) andbis(1,8-cyclooctadiene)nickel
(28 mg, 0.30 mmol, 1.0 equiv). The reagents were dissolved in toluene
(20 mL) to give a red solution and stirred at ambient temperature
for 18 h, during which time the mixture turneddark red anddeposited
a metal mirror. After removal of volatiles under reduced pressure,
the dark red residue was extracted with warm toluene (3 × 5 mL).
The combined extracts were concentrated to ca. 10 mL and stored at
−30 °C for 1 d. Dark redcrystals of 3–Ni were isolated, washed withhexane, anddried in vacuo. Yield: 316
mg (72%). 1H NMR (toluene-d8): 3.51 (s, 9H, ArMe), 4.05 (s, 6H, PPhH), 4.66 (s, 6H, PPhH), 4.97 (s, 6H, PPhH), 5.74 (s, 6H, PPhH), 5.93 (s, 30H, tBu/PPhHp), 6.29 (s, 3H, PPhHp), 6.35 (s, 3H, ArH), 11.65 (s, 3H,
ArH). 1H NMR (toluene-d8, 370 K): 3.30 (s, 9H, ArMe), 4.61 (s,
12H, PPhH), 5.07 (s, 27H, tBu),
5.57 (s, 6H, PPhH), 6.22 (s, 6H, PPhHp), 6.32 (s, 3H, ArH), 11.03 (s, 3H,
ArH). 31P{1H} NMR (C6D6): 92.3. Evans’ method (C6D6): 1.9 μB. UV–vis–NIR [λ in
nm (ε in M–1 cm–1)]: 305
(3.4 × 104), 511 (598), 666 (41), 709 (51), 814 (8),
948 (13), 1056 (25), 1120 (36), 1202 (39), 1411 (13), 1547 (15), 1649
(14), 1748 (15), 1754 (15). Anal. Calcd for C69H72INiO3P3U: C 56.54. H 4.95. Found: C 56.65,
H 5.01.
IUIVL3Pd0 (3–Pd)
A Schlenk flask was charged with 2 (141 mg,
0.100 mmol), tetrakis(triphenylphosphine)palladium (116 mg, 0.100
mmol, 1.00 equiv), a stir bar, andtoluene (5 mL) and the solution
stirred at 80 °C for 3 d. The red mixture was cannula filtered,
layered withhexane, and allowed to stand at ambient temperature.
Orange crystals of 3–Pd grew over 5 d and were
isolated by decanting, washed withhexane, anddried under vacuum.
Yield: 53 mg (35%). 1H NMR (toluene-d8): 5.32 (s, 9H, ArMe), 7.23 (s, 3H, ArH), 9.89 (s, 27H, tBu), 15.44 (s, 3H, ArH). 1H NMR (toluene-d8, 370
K): 3.21 (s, 12H, o-HPhP), 4.63 (s, 9H, ArMe), 5.60 (s, 12H, m-HPhP), 6.11 (s, 6H, p-HPhP), 7.11 (s, 3H, ArH), 7.83 (s, 27H,
tBu), 13.69 (s, 3H, ArH). 31P{1H} NMR (C6D6): 68.4. 31P{1H} NMR (toluene-d8): 68.0. Evans’
method (C6D6): 1.8 μB. UV–vis–NIR
[λ in nm (ε in M–1 cm–1)]: 300 (3.4 × 104), 527 (103), 576 (27), 661 (22),
686 (29), 722 (11), 891 (9), 948 (13), 1060 (19), 1114 (34), 1151
(23), 1175 (19), 1431 (11), 1455 (12), 1540 (16), 1750 (11), 1776
(12), 2045 (12), 2086 (13). Anal. Calcd for C69H72IO3P3PdU: C 54.75. H 4.79. Found: C 54.82,
H 4.88.
IUIVL3Pt0 (3–Pt)
This compound was prepared in an analogous procedure to
that of 3–Pd (see the SI) to give orange crystals in 66% yield.
Me3SiOUIVL3Ni0 (4)
A scintillation
vial was charged with 3–Ni (147 mg, 0.100 mmol),
sodium trimethylsilanolate (11 mg, 0.10 mmol,
1.0 equiv), a stir bar, andTHF (3 mL). The red mixture was stirred
for 16 h at ambient temperature and then evaporation of volatiles
under reduced pressure, affording a dark red residue which was suspended
in a minimal amount of benzene, centrifuged, and filtered. Dark redcrystals of 4 were isolated from the benzene filtrate
by hexane vapor diffusion (83 mg, 58%). 1H NMR (toluene-d8): −15.47 (s, 27H), −7.59 (s,
3H), −7.20 (br s, 3H), −4.74 (t, 3H, J 7.5 Hz), −3.95 (s, 9H), 7.65 (s, 3H), 16.82 (t, 3H, J 7.5 Hz), 19.47 (br s, 3H), 48.83 (s, 9H). 1H NMR (toluene-d8, 370 K): −11.57
(s, 27H), −4.23 (s, 3H), −4.13 (br s, 3H), −3.83
(vbr s, 3H), −2.59 (s, 9H), −2.15 (br s, 3H), 7.29 (s,
3H), 14.56 (t, 3H, J 7.5 Hz), 16.56 (s, 6H), 30.38
(vbr s, 6H), 37.77 (s, 9H). 469.4. 31P{1H} NMR
(toluene-d8): 476.4. Evans’ method
(C6D6): 2.8 μB. UV–vis–NIR
[λ in nm (ε in M–1 cm–1)]: 302 (2.9 × 104), 520 (296), 559 (148), 659 (50),
692 (28), 837 (6), 966 (22), 1098 (31), 1150 (38), 1287 (16), 1410
(10), 1578 (20), 1751 (22), 1781 (31), 1885 (48), 2039 (7), 2075 (4).
Anal. Calcd for C72H81O4P3SiU: C 60.55. H 5.72. Found: C 60.43. H 5.81.
FUIVL3Ni0 (5)
A scintillation
vial was charged with 3–Ni (58
mg, 0.040 mmol, 1.0 equiv), cesium(I) fluoride (6 mg, 0.040 mmol,
1.0 equiv), a stir bar, andTHF (2 mL). The red solution was stirred
for 1 d at ambient temperature. Some colorless solids that formed
were removed by filtration. Volatiles were removed under reduced pressure,
the red residue was suspended in benzene, and the solution was centrifuged
and then filtered. Crystallization by hexane vapor diffusion into
the filtrate afforded redcrystals (32 mg, 59%) of 5. 1H NMR (toluene-d8): −11.88
(s, 27H), −7.35 (s, 3H), −7.25 (s, 4H), −4.74
(s, 3H), −4.25 (s, 9H), 5.73 (br s, 2H), 6.54 (s, 3H), 16.58
(s, 3H), 19.16 (v br s, 6H), 30.00 (v br s, 4H). 1H NMR
(toluene-d8, 370 K): −8.60 (s,
27H), −4.06 (br s, 12H), −2.86 (s, 9H), −2.10
(br s, 2H), 5.10 (s, 3H), 6.36 (s, 2H), 14.37 (s, 3H), 16.31 (br s,
4H), 30.00 (v br s, 4H). 31P{1H} NMR (C6D6): 474.5. Evans’ method (C6D6): 2.1 μB. UV–vis–NIR
[λ in nm (ε in M–1 cm–1)]: 303 (2.5 × 104), 655 (147), 691 (118), 841 (73),
952 (75), 1042 (64), 1087 (75), 1150 (82), 1202 (48), 1254 (49), 1412
(35), 1447 (29), 1580 (39), 1751 (57), 1777 (77), 1835 (81), 1880
(66), 2035 (15), 2072 (12). Anal. Calcd for C69H72FO3P3U: C 61.03. H 5.34. Found: C 60.89, H
5.23.
Computational Details
Density
functional theory calculations
were carried out using the PBE functional, as implemented in Gaussian
09, Rev. C.01 andD.01,[89] andADF 2014[90−92] quantum chemistry codes. For the Gaussian calculations, the cc-pVDZ
basis set was used for all atoms except U, I, andPd. For these elements,
a Stuttgart–Bonn variety relativistic pseudopotential was employed,
together with segmented valence basis sets; (14s13p10d8f)/[10s9p5d4f]
for U,[93] (16s12p4d1f)/[3s3p2d1f] for I,[94,95] and (8s7p6d2f)/[6s5p3d1f] for Pd.[95,96] The ultrafine
integration grid was employed. natural bond orbital calculations were
performed using the NBO6 code, interfaced with Gaussian revision D.01.[97] QTAIM analyses were performed using the AIMAll
program package,[98] with .wfx files generated
in Gaussian used as input.Single-point calculations, at the
Gaussian-optimized geometries, were run in the ADFcode in order to
obtain Mayer[99] and Gopinathan–Jug[100] bond orders. For these calculations, the zeroth-order
regular approximation (ZORA) Hamiltonian was used. Slater-type orbital
ZORA basis sets of TZP quality were used for U, Ni, Pd, and I, withDZP ZORA basis sets for all other atoms. The frozen core approximation
was employed, with U(5d), I(4p), Pd(3d), Ni(2p), P(2p), and 1s for
all other atoms, bar H. The default SCFconvergence criteria were
used, together with an integration grid of 4.5.
Authors: Dipti Patel; Fabrizio Moro; Jonathan McMaster; William Lewis; Alexander J Blake; Stephen T Liddle Journal: Angew Chem Int Ed Engl Date: 2011-09-14 Impact factor: 15.336
Authors: Franziska Völcker; Felix M Mück; Konstantinos D Vogiatzis; Karin Fink; Peter W Roesky Journal: Chem Commun (Camb) Date: 2015-07-28 Impact factor: 6.222
Authors: David M King; Floriana Tuna; Eric J L McInnes; Jonathan McMaster; William Lewis; Alexander J Blake; Stephen T Liddle Journal: Nat Chem Date: 2013-05-05 Impact factor: 24.427
Authors: Erli Lu; Ashley J Wooles; Matthew Gregson; Philip J Cobb; Stephen T Liddle Journal: Angew Chem Int Ed Engl Date: 2018-04-27 Impact factor: 15.336