Fabrizio Ortu1,2, Simon Randall1, David J Moulding1, Adam W Woodward1,3, Andrew Kerridge4, Karsten Meyer5, Henry S La Pierre5,6,7, Louise S Natrajan1,3. 1. Centre for Radiochemistry Resesarch, Department of Chemistry, School of Natural Sciences, The University of Manchester, Oxford Road, Manchester M13 9PL, U.K. 2. School of Chemistry, University of Leicester, University Road, Leicester LE1 7RH, U.K. 3. Photon Science Institute, The University of Manchester, Oxford Road, Manchester M13 9PL, U.K. 4. Department of Chemistry, Lancaster University, Lancaster LA1 4YB, U.K. 5. Friedrich-Alexander-University Erlangen-Nürnberg (FAU), Department of Chemistry and Pharmacy, Inorganic Chemistry, Egerlandstr. 1, 91058 Erlangen, Germany. 6. School of Chemistry and Biochemistry, Georgia Institute of Technology, Atlanta, Georgia 30332-0400, United States. 7. Nuclear and Radiological Engineering and Medical Physics Program, School of Mechanical Engineering, Georgia Institute of Technology, Atlanta, Georgia 30332-0400, United States.
Abstract
Pentavalent uranyl species are crucial intermediates in transformations that play a key role for the nuclear industry and have recently been demonstrated to persist in reducing biotic and abiotic aqueous environments. However, due to the inherent instability of pentavalent uranyl, little is known about its electronic structure. Herein, we report the synthesis and characterization of a series of monomeric and dimeric, pentavalent uranyl amide complexes. These synthetic efforts enable the acquisition of emission spectra of well-defined pentavalent uranyl complexes using photoluminescence techniques, which establish a unique signature to characterize its electronic structure and, potentially, its role in biological and engineered environments via emission spectroscopy.
Pentavalent uranyl species are crucial intermediates in transformations that play a key role for the nuclear industry and have recently been demonstrated to persist in reducing biotic and abiotic aqueous environments. However, due to the inherent instability of pentavalent uranyl, little is known about its electronic structure. Herein, we report the synthesis and characterization of a series of monomeric and dimeric, pentavalent uranyl amide complexes. These synthetic efforts enable the acquisition of emission spectra of well-defined pentavalent uranyl complexes using photoluminescence techniques, which establish a unique signature to characterize its electronic structure and, potentially, its role in biological and engineered environments via emission spectroscopy.
The aqueous chemistry
of uranium is dominated by the uranyl dication,
[UVIO2]2+.[1−4] Therefore, understanding its physicochemical
properties is vital to the successful implementation of adequate nuclear
waste management strategies.[5−9] Despite its inherent stability, uranyl can undergo a number of transformations
in the environment, the cornerstone of which is the reduction of soluble
uranyl(VI) to insoluble U4+.[10] This transformation has been postulated to proceed via a disproportionation
mechanism, which involves the formation of transient uranyl(V) species,
{[UVO2]+} (n = 1 or 2).[11,12] The detection
of this transient species in the environment and in biological systems
remains a challenging goal due to its redox instability and lability.[13]In aqueous media, [UVO2]+ has
been observed in acidic solutions (pH 2–3)[14] and in concentrated carbonate solutions.[15] Molecular [UVO2]+ compounds
have also been stabilized by operating in the rigorous exclusion of
air and moisture.[9,16,17] Quite remarkably, they have recently been isolated and studied in
aqueous media.[18−20] Since 2003,[21] there have
been a number of reports on the structural and chemical properties
of the once elusive [UVO2]+ cation.[9,16,17,22−29] Nevertheless, there is a remarkable paucity of information regarding
the electronic structure and photophysical properties of [UVO2]+.[30] This is
in contrast to the extensive studies of the [UVIO2]2+ dication. In prior seminal reports on the emission
spectra of [UVO2]+ species,[31,32] [UVO2]+ was generated in situ using
photolytic or electrolytic reduction and analysis required deconvolution
of the luminescence spectra. Very recently, Mazzanti and co-workers
reported the emission spectra of a water-stable dipicolinate [UVO2]+ complex.[20] However, the photophysical properties of the [UVO2]+ cation remain unassigned. We have previously
shown that the application of photoluminescence techniques to [UVIO2]2+ can provide detailed information
regarding the behavior of uranyl, particularly its coordination, speciation,
and nuclearity including the existence of “cation–cation”
interactions (CCIs).[33] Therefore, the application
of this approach to discrete molecular [UVO2]+ compounds can offer a essential diagnostic tools for
understanding its physicochemical properties.[13] Herein, we report the synthesis and structural authentication of
a series of pentavalent uranyl complexes and the detailed characterization
of their photoluminescence properties.
Experimental
Section
General Methods
All manipulations were carried out using standard Schlenk techniques
or in an Inert Purelab HE 2GB glovebox. Solvents were dried by refluxing
over potassium and were distilled and degassed before use. All solvents
were stored over potassium mirrors (with the exception of THF and
DME, which were stored over activated 4 Å molecular sieves).
[K(THF)3][UO2(N″)3] (1), [K(crypt)][UO2(N″)3] (2-crypt), [UO2(N″)2(THF)2] (4) were prepared following literature procedures.[34]1H, 13C{1H},
and 29Si{1H} NMR spectra were recorded at 298
K on a Bruker Avance 400 spectrometer operating at 400.2, 100.6, and
79.5 MHz, respectively; chemical shifts are quoted in ppm and are
relative to TMS. FTIR spectra were recorded as Nujol mulls in KBr
discs using a Shimadzu IRAffinity-1S spectrometer. Raman spectra were
recorded using a XploRAPLUS Horiba Scientific spectrometer. Electronic
absorption spectra were recorded in sealed 10 mm path length cuvettes
using a Shimadzu UV-2600 spectrometer.
Synthesis
[K(18-crown-6)][UO2(N″)3] (2–18C6)
A Schlenk flask fitted with magnetic
stir bar was charged with 4 (1.225 g, 1.7 mmol), KN″
(0.356 g, 1.8 mmol) and 18-crown-6 (0.467 g, 1.8 mmol); the flask
was cooled to −50 °C, THF (15 mL) was added and the orange
solution stirred for 16 h at room temperature. Volatiles were removed
under reduced pressure and the solid washed with hexane (10 mL), then
dried in vacuo for 2 h at room temperature, affording 2–18C6 as an orange powder. Yield: 1.416 g, 1.3 mmol, 80%. Anal. Calc’d
(%) for C30H78KN3O8Si6U: C 34.17, H 7.45, N 3.98; Found: C 34.14, H 7.44, N 3.61. 1H NMR (pyridine-d6, 298 K, 400
MHz) δ 0.79 (s, 36H, Si(CH3)3), 3.50 (s, 24H, 18-crown-6–CH2). 13C{1H} NMR (pyridine-d6, 298 K, 100 MHz) δ 6.86 (Si(CH3)3), 70.95 (18-crown-6-CH2). 29Si{1H} (pyridine-d6, 298 K, 79.5 MHz) δ −8.52 (Si(CH3)3). FTIR (ATR microcrystalline)
ν̃ 2945 (w), 2892 (w), 1352 (w), 1233 (m), 1103 (s), 959
(vs, U=Oasym), 833 (vs), 770 (w), 689 (w), 658 (s),
607 (s) cm–1. FTIR (ATR) ν̃ 2971 (br,
m), 2859 (br, m), 1454 (w), 1352 (w), 1233 (w), 1107 (m), 1066 (vs),
961 (s, U=Oasym), 907 (w), 834 (vs), 768 (w), 668
(w), 661 (m), 605 (m). Raman (Solid, 638 nm, 100%) ν̃
2904 (br, 799), 1474 (640), 1278 (600), 1247 (479), 1135 (492), 802
(2257) (U=Osym), 280 (1256) cm–1 (counts). UV/vis (0.05 mM, THF) λmax (ε/mol–1 cm–1): 497 (270), 370 (2632), 324
(4018), 230 (5262), 212 (5026) nm. 2–18C6-THF: Crystals were
grown form a THF solution layered with hexane and stored at −25
°C several days. 2–18C6-Tol: Crystals were grown from
cooling of a boiling toluene solution. 2–18C6-CHCl3: Crystals were grown from a saturated solution in CHCl3 at room temperature.
[K(2.2.2-cryptand)][UO2N″3] (2-crypt)
A Schlenk flask fitted with
magnetic stir
bar was charged with 1 (1.701 g, 1.7 mmol) and 2.2.2-cryptand
(0.636 g, 1.7 mmol); DME (20 mL) was added and the reaction stirred
for 4 h. The deep red solution was concentrated to 5 mL and stored
at −30 °C, affording 2-crypt as bright red
crystals (1.595 g, 1.4 mmol, 80%). Spectroscopic data matched that
previously reported in the literature.[34]
[K(18-crown-6)(DME)]2[UO2(N″)3] (3–18C6)
A Schlenk flask with
a stirrer bar was charged with 2–18C6 (0.836 g,
0.79 mmol). Additionally, a separate flask was charged with a mixture
of 18-crown-6 (0.220 g, 0.83 mmol) and KC8 (0.109 g, 0.80
mmol). Both flasks were cooled to −50 °C and DME (5 mL
each) was added. Both mixtures were stirred for 5 min, then the slurry
of 18-crown-6 and KC8 was added quickly to the solution
of 1–18C6. More DME (2 mL) was added in order
to collect the rest of the KC8 slurry and complete the
addition. The reaction was allowed to stir at −50 °C for
5 min and then left to settle for 2 min. The suspension was then filtered
into a precooled Schlenk flask (−50 °C) affording an emerald
green solution. Subsequent concentration of the mother liqueur at
−30 °C (ca. 5 mL) followed by layering with pentane (7
mL) and storage at −30 °C led to emerald green crystals
of 3–18C6. Yield: 0.344 g, 0.21 mmol, 27%. 1H NMR (tetrahydrofuran-d8, 298
K) δ −8.64 (br, ν1/2 = 52 Hz, 18H, Si(CH)3), −4.94
(br, ν1/2 = 340 Hz, 9H, Si(CH)3), 3.28 (s, ν1/2 = 3 Hz, 12H, DME), 3.44
(s, ν1/2 = 4 Hz, 8H, DME), 6.44 (br, ν1/2 = 44 Hz, 24H,
crown–CH2). 13C{1H} NMR (tetrahydrofuran-d8, 298
K) δ 6.29 (s, Si(CH3)3), 6.50 (s, Si(CH3)3), 58.95
(s, DME), 72.83 (s, DME), 73.35 (br, 18-crown-6-CH2). 29Si{1H} NMR (d8-THF, 298 K) δ −10.87 (Si(CH3)3). μeff (Evans method,
298 K, tetrahydrofuran-d8) 2.68 μB. FTIR (ATR microcrystalline) ν̃ 2889 (br, m),
1452 (w), 1352 (m), 1233 (m), 1103 (vs), 1025 (s), 958 (s), 873 (m,
U=O(yl) asym), 821 (vs), 758 (s), 695 (w),
650 (s), 591 (w) cm–1. Raman (solid, 638 nm, 10%)
(Smoothed) ν̃ 2893 (br, s), 1475 (w), 1282 (w), 1142 (w),
837 (m), 727 (br, s, U=O(yl) sym), 609 (w),
415 (br, m), 282 (br, w). Anal. Calc’d (%) for C46H112K2N3O16Si6U·C4H10O2: C 38.15, H 7.80,
N 2.90; Found: C 37.92, H 7.83, N 2.57. UV/vis (2.65 mM, THF) λmax (ε/mol–1 cm–1): 773 (45), 650 (60), 622-shoulder (58), 567-shoulder (71) 496 (150)
nm.
[K(2.2.2-cryptand)]2[UO2(N″)3] (3-crypt)
A Schlenk flask fitted with
a stirrer bar was charged with 2-crypt (1.084 g, 0.9
mmol); a separate flask was charged with a mixture of 2.2.2-cryptand
(0.350 g, 0.9 mmol) and KC8 (0.126 g, 0.9 mmol). Both flasks
were cooled to −50 °C and DME (5 and 10 mL respectively)
was added. The slurry of 2.2.2-cryptand and KC8 was added
quickly to the solution of 2-crypt; more DME (5 mL) was added in order
to collect the rest of the KC8 slurry and complete the
addition. The reaction was allowed to stir at −50 °C and
then filtered in a precooled Schlenk flask (−50 °C), affording
a bright green solution. The solution was stored at −25 °C,
affording 3-crypt as emerald green crystals (0.791 g,
0.5 mmol, 51%). 1H NMR (tetrahydrofuran-d8, 298 K, 400 MHz) δ −8.47 (br, ν1/2 = 60 Hz, 5H, N(SiCH3)2), −4.75 (br, ν1/2 = 324 Hz, 36H, N(SiCH3)2), −0.09 (s, ν1/2 = 4 Hz, 9H, N(SiCH3)2), 0.33 (s, ν1/2 = 4 Hz, 4H, N(SiCH3)2), 6.72 (br, ν1/2 = 24
Hz, 24H, crypt–CH2), 8.17 (br,
ν1/2 = 36 Hz, 24H, crypt–CH2), 8.71 (br, ν1/2 = 40 Hz, 24H, crypt–CH2) ppm. 13C{1H} NMR (tetrahydrofuran-d8, 298 K, 100 MHz) δ 6.39 (N(SiCH3)2), 7.09 (N(SiCH3)2), 58.66 (crypt-CH2), 72.64 (crypt-CH2), 75.90 (crypt-CH2) ppm. 29Si{1H} (tetrahydrofuran-d8, 298 K, 79.5 MHz) δ −103.12 ppm.
μeff (Evans method, 298 K, tetrahydrofuran-d8) 2.47 μB. Anal. Calcd (%)
for C54H126K2N7O14Si6U: C 40.99, H 8.03, N 6.20; found: C 40.92, H 8.31,
N 6.09. UV/vis (3.1 mM, DME) λmax (ε/mol–1 cm–1): 649 (136), 622
(57), 490 (37) nm. FTIR (KBr disc in Nujol mull) ν̃ 1722
(w), 1622 (w), 1362 (s),1296 (s), 1261 (m), 1236 (m), 1223 (m), 1175
(w), 1101 (br s w/shoulder), 1030 (br s), 949 (m), 932 (w), 872 (m,
U=Oasym), 816 (br s), 762 (m w/shoulder), 698 (w),
662 (m), 648 (m), 582–360 (br s) cm–1. Raman
(50 mM in THF) ν̃ 753(544), 829(705) cm–1 (counts), (U=O(yl) sym); Raman (solid, 532
nm, 100%) ν̃ 164(127), 192(158), 488(636), 709(279), 790(126),
1416(74) cm–1 (counts).
[K(18-crown-6)(DME)]2[{UO(μ-O)(N″)2}2] (5) and [K(18-crown-6)(DME)]2[{UO2(μ-O2)(N″)2}2] (6)
In the glovebox, to a vial
containing a magnetic stirrer bar was added 4 (250 mg,
0.34 mmol) and 10 mL of 1:1 THF:hexane. The mixture was stirred and
the dark orange solution transferred to a–35 °C freezer.
KC8(46 mg, 0.34 mmol) and 2.2.2-cryptand (0.128 mg, 0.34
mmol) were weighed into separate vials, the crypt dissolved in 4 mL
of THF and the vials stored at −35 °C. After 30 min, the
THF/cryptand solution was transferred to the KC8 and the
resulting slurry added to the uranyl solution dropwise over 2 min
with vigorous stirring. Washings were transferred with an additional
2 mL of cold THF and the mixture stirred for a further minute before
being moved to the −35 °C freezer for 1 min. The slurry
was stirred and filtered through a fine porosity frit and the brown
filtrate concentrated to ca. 3 mL under reduced pressure and cooled
to −35 °C. The resultant brown solid was collected and
washed with cold THF/hexane (∼1:5, 50 mL) and dried in vacuo.
Crystals of 5 were obtained from a concentrated solution
in DME stored at −35 °C (Yield: 132 mg, 0.13 mmol, 38%).
When the reaction was attempted using Schlenk line techniques, small
crops of [K(18-crown-6)(DME)]2[{UO2(μ-O2)(N″)2}2] (6) were
also isolated and characterized via single crystal XRD. The high thermal
instability of 5 in solution precluded spectroscopic
characterization. Anal. Calc’d (%) for C60H144K2N8O16Si8U2: C 35.80, H 7.21, N 5.57; found: C 35.22, H 7.12, N 5.07.
[{U(μ-O)2(N″)2(μ-Cl)}{K(18-crown-6)}2] (7)
A Schlenk flask with a stirrer
bar was charged with 4 (0.735 g, 1 mmol). Additionally,
a separate flask was charged with a mixture of 18-crown-6 (0.529 g,
2 mmol), KC8 (0.137 g, 1 mmol) and KCl (0.087 g, 1.2 mmol).
Both flasks were cooled to −50 °C and DME (5 mL each)
was added. Both mixtures were allowed to stir for 5 min, at which
point the slurry of 2.2.2-cryptand and KC8 was added quickly
to the solution of 4. More DME (ca. 5 mL) was added in
order to collect the rest of the KC8 slurry and complete
the addition. The reaction was allowed to stir at −50 °C
for 5 min at which point stirring was stopped and the solution left
to settle for 2 min. The solution was then filtered into a precooled
Schlenk flask (−50 °C) affording an amber-brown solution.
Subsequent concentration of the mother liquor to ca. 5 mL followed
by layering with pentane (7 mL) and storage at −25 °C
lead to amber-brown crystals of 7. Yield: 0.378 g, 0.38
mmol, 38%). 1H NMR (tetrahydrofuran-d8, 298 K) δ −8.52 (br, ν1/2 =
55 Hz, Si(CH3)3, 5.18 (br,
ν1/2 = 51 Hz, crown–CH2). 13C{1H} NMR (tetrahydrofuran-d8, 298 K) δ 6.24 (Si(CH3)3), 72.15 (crown-CH2). 29Si{1H} NMR signal not observed.
μeff (Evans method, 298 K, tetrahydrofuran-d8) 2.44 μB. Anal. Calc’d
(%) for C36H84ClK2N2O14Si4U: C 35.07, H 6.87, N 2.27; Found: C 35.44,
H 7.08, N 2.17. FTIR (ATR microcrystalline) ν̃ 2865 (br
m), 1452 (w), 1352 (m), 1235 (m), 1103 (vs), 958 (s), 861 (m-shoulder,
U=O(yl) asym), 821 (s), 748 (w), 644 (w), 593
(w) cm–1. Raman (solid, 638 nm, 10%, smoothed) ν̃
2900 (br, s), 1472(m), 1274(m), 1140 (w), 869 (m), 784 (br s) (U=O(yl) sym), 434 (br m), 277 (m) cm–1.
UV/vis (5.63 mM, THF) λmax (ε/mol–1 cm–1): 841 (54), 655 (105),
495 (250) nm.
Results and Discussion
Synthesis and NMR Characterization
The sterically bulky
bis(trimethylsilyl)amide ligand, (N(SiMe3)2)−, (N″),[1−46] was selected to stabilize [UVO2]+ complexes, since the ligands lack strongly absorbing chromophores.
This approach has proven successful in enabling the identification
and characterization of the optical properties of U4+,
[NpVO2]+, and [NpVIO2]2+.[47] Uranyl(VI) silylamide
complexes [K(THF)3][UO2(N″)3(THF)] (1) and [UO2(N″)2(THF)] (4) were synthesized via salt metathesis between
[UO2(Cl)2(THF)2]2 and
ligand transfer reagent KN″ in a 1:3 (Scheme ) or 1:2 ratio (Scheme ). Complex 1 was converted to
[K(crypt)][UO2(N″)3] (2-crypt, crypt = 2.2.2-cryptand) by reaction with one equivalent of 2.2.2-cryptand,
while the analogous complex [K(18C6)][UO2(N″)3] (2–18C6, 18C6 = 18-crown-6) was obtained
by reacting 4 with one equivalent of KN″ and 18-crown-6.
The monomeric uranyl(V) derivatives [K(L)(DME)n]2[UO2(N″)3] (3-crypt, L
= crypt, n = 0; 3–18C6, L = 18C6, n = 1) were obtained in moderate crystalline yields via
reduction of 2-crypt or 2–18C6 with
one equivalent of KC8 in the presence of corresponding
sequestering agents (Scheme ). When the reactions were carried out in the absence of sequestering
agents, the only identifiable product was [K(DME)4][UO2(N″)3]. On the other hand, when the bis-amide
precursor 4 was reduced with KC8 and 2.2.2-cryptand,
the uranyl(V) dimer [K(crypt)]2[(UO(μ-O)(N″)2)2] (5) was obtained in low yields
(Scheme ). The isolation
of 5 is rather challenging, due to its inherent instability
and the concomitant formation of the peroxo byproduct [K(crypt)]2[(UO2(N″)2)2(μ-O2)] (6). When the same reduction was attempted
in the presence of 18-crown-6, the uranyl(V) ate-complex [(UO2(N″)2)(μ-Cl)(K(18C6))2]
(7) was obtained; its formation was likely due to the
presence of KCl in the starting material. Therefore its preparation
was purposely attempted by reacting 4 with an equimolar
ratio of KCl and 18-crown-6, which resulted in the formation of 7 in moderate yields (Scheme ). All compounds were thoroughly characterized via
spectroscopic and analytical techniques, with the exception of 5 and 6: the former is a highly unstable compound
which readily decomposes above −30 °C, while the latter
was never isolated as an analytically pure species and has very low
solubility in most laboratory solvents.
Scheme 1
Synthesis of Uranyl(VI)
Tris-amides, 2-crypt and 2-18C6, and Reduction
to Monomeric Uranyl(V) Complexes 3-crypt and 3-18C6
Scheme 2
Reduction of Uranyl(VI) Bis-amide 4 and to Dimeric Uranyl(V)
Complex 5 and Monomeric Uranyl(V) Complex 7
In comparison with the diamagnetic
precursors 1 and 2, the 1H NMR
spectrum of 3-crypt displays
a broadening of the spectral lines, which is in agreement with the
presence of a paramagnetic metal center. Two resonances are identified
for the SiMe3 protons (δH = −8.47
and −4.77 ppm), displaying a noticeable line broadening (δH = −8.47 ppm, ν1/2 = 60 Hz; δH = −4.75 ppm, ν1/2 = 324 Hz). Additionally,
three broad resonances each integrating for 24 protons are present
in the downfield region of the spectrum (δH = 6.72
ppm, ν1/2 = 24 Hz; δH = 8.17 ppm,
ν1/2 = 36 Hz; δH = 8.71 ppm, ν1/2 = 40 Hz). It is noteworthy that 3-crypt displays
a relatively high instability in solution at room temperature. After
48 h, the decomposition is particularly enhanced and visible in the 1H NMR spectrum, in conjunction with a significant shift of
the 2.2.2-cryptand signals and the appearance of several other decomposition
peaks (see SI, Figure S11).The 13C{1H} NMR spectrum of 3-crypt displays
characteristic resonances for the SiMe3 groups
(δC = 6.39 and 7.09 ppm) and CH2 fragments
belonging to the cryptand macrocycle (δC = 58.66,
72.64, and 75.90 ppm). 1H and 13C{1H} spectra of 3–18C6 are very similar to those
of 3-crypt, with different signals accounting for the
presence of a different sequestering agent (18c6) and DME. Additionally,
one signal was observed in the 29Si{1H} NMR
spectra of both 3-crypt and 3–18C6, resonating at −103.12 and −115.49 ppm respectively.The 1H NMR spectrum of 7 displays two broad
signals for the SiMe3 protons (δH = −8.52
ppm, ν1/2 = 55 Hz) and CH2 protons of
the crown (δH = −51 ppm, ν1/2 = 51 Hz), with additional diamagnetic impurities similar to those
observed for 3-crypt. The corresponding signals are also
observed in the 13C{1H} NMR spectrum, with peaks
resonating at 6.24 (SiMe3) and 72.15 (18-crown-6). Unlike
for 3-crypt and 3–18C6, no clear
signal was visible in the 29Si{1H} NMR. Line
broadening is typically observed in the 1H and 13C NMR spectra of U(V) species. This is also detected in the 1H NMR spectra of uranyl(V) species with various supporting
ligands[48−51] and bis-imido analogues, while 13C data is rarely reported.[52−54] Interestingly, full width half maxima of the 1H NMR signals
of 3-crypt (ν1/2 range = 24–324
Hz) are significantly narrower than those observed in bis-imido complexes
[UV(NDipp)2(bipyR2)2(X)]
(Dipp = 2,6-iPr2C6H2;
bipyR2 = 4,4′-dialkyl-2,2′-bipyridine; R=
Me, tBu; X = Cl, Br, I) (ν1/2 range =
154–2701 Hz).[53]Despite their
instability in solution, we were able to determine
the magnetic moment, μeff, of 3-crypt and 3–18C6 at room temperature via the Evans
method.[55] These were measured at 2.45 μB and 2.67 μB respectively, thus falling within
the range expected for monometallic U(V)[56] and close to the predicted magnetic moment of the U5+ free ion (μeff = 2.54 μB).[57] Noticeably, the magnetic moment values obtained
for 3-crypt and 3–18C6 are higher
than those of other uranyl(V) species measured with similar methods,
such as [K(18-crown-6][UO2(salan-tBu2)(py)] and [K(18-crown-6][UO2(salophen-tBu2)(py)K] (μeff = 2.14–2.25 μB) reported by Mazzanti and co-workers[50]—though it is noteworthy that the values
reported by these authors are significantly lower than those obtained
with solid state magnetic susceptibility measurements (2.57–2.60
μB).
Structural Characterization
The
identity of these complexes
was established through single-crystal X-ray diffraction (SC-XRD)
experiments, which demonstrated the formulation of the anionic [UO2N″3]2– fragment with two
cationic [K(L)]+ counterions to balance the overall charge
in 3-crypt and 3–18C6 and a trigonal
bipyramid geometry around the metal center, close to that observed
for precursors 1(34) and 2 (Figure and S37–S39).[34] The U=O distances of the [UVO2]+ fragment in 3-crypt [1.829(3)–1.843(3)
Å and 3–18C6 [1.853(3)–1.855(3) Å]
are longer than those previously reported for monomeric [UVO2]+ species [1.736–1.821 Å] (Tables S4–S5) and may be a reflection
of the strong sigma donating ability of the amide ligands.[21,25] The [UVO2]+ fragment is perfectly
linear in all polymorphs, together with a near perfect trigonal planar
arrangement around the equatorial coordination plane. Slight elongations
of the U–N distances are also observed in 3-crypt [2.430(3)–2.476(4) Å] with respect to the [UVIO2]2+ precursors 1 and 2-crypt [2.310(4)–2.333(4) Å]. This trend is in-line with changes
in the ionic radii of the uranium ion.[58] In the case of 7, the U=O distances are statistically
identical with those of 3-crypt and 3–18C6[1.846(5)–1.848(5) Å], while the U–N bond lengths
are shorter [2.409(6)–2.412(6) Å]. Interestingly, the
O=U=O deviates slightly from linearity [171.8°(2)]
owing to the interaction between K cations and the uranyl(V) unit.
Figure 1
Molecular
structures of 3-crypt, 5, 6, and 7 determined by SC-XRD. Thermal ellipsoids
are shown at 50% probability for all structures. Hydrogen atoms and
outer-sphere cations are omitted for clarity. Black, blue, red, orange,
green, magenta and aqua represent carbon, nitrogen, oxygen, silicon,
chlorine, potassium and uranium, respectively.
Molecular
structures of 3-crypt, 5, 6, and 7 determined by SC-XRD. Thermal ellipsoids
are shown at 50% probability for all structures. Hydrogen atoms and
outer-sphere cations are omitted for clarity. Black, blue, red, orange,
green, magenta and aqua represent carbon, nitrogen, oxygen, silicon,
chlorine, potassium and uranium, respectively.Single crystals of 5 reveal two [UO2N″2]+ fragments joined through a CCI, thereby forming
an oxo-bridged dimer with diamond-shaped [UO2]2 core [U···O = 2.327(13) and 2.330(13) Å] (Figure ). Such a conformation
is rare but has been previously observed in [UVO2]+ species.[17] Analogously to 3, the U–O distances in 5 are elongated
[1.868(13)–1.959(13) Å] with respect to its [UVIO2]2+ precursor, 4, and both O=U=O
units in the dimer are significantly bent [168.5(7) and 168.8(7)].
Additionally, the distances of the terminal U–O interactions
[1.940(13) and 1.959(13) Å] are significantly shorter than those
bridging between the two [UVO2]+.
In contrast to previously reported examples, in which the CCI was
favored by additional interactions of the actinyl fragment,[25,29,59] the formation of the diamond-shaped
core in 5 is unsupported.
Electronic Structure Investigation
and Analysis
The
UV–vis–nIR absorption spectra of 3-crypt in DME further demonstrate the presence of pentavalent uranyl (Figure A). The spectrum
shows a broad, intense feature centered at υmax =
22 000 cm–1 extending to higher energies,
plus a series of sharper electronic transitions at approximately 15 600,
13 300, 12 500, 10 000, and 1440 cm–1 (λmax = 641 (ε = 145 M–1 cm–1)), 752 (ε = 20 M–1 cm–1), 800 (ε = 15 M–1 cm–1), 1000 (ε = 15 M–1 cm–1) and 6944 (ε = 145 M–1 cm–1) nm) at lower energies (Figure S41 and S42 (SI)). These transitions are assigned as
admixtures of 5f ← U=O(yl), 5f ← amide,
intraligand, intra 5f, 6d ← 5f, and 7s ← 5f transitions
by comparison with the calculated excitations in 3-crypt (see Figure S80 and Table S6, SI for full assignments). In comparison
with experimental findings on related systems[30] and theoretical calculations for the bare [UO2]+ ion,[61,64−69] the excitations can be approximately
assigned as transitions involving the σuφuδu (15 600 cm–1),
σu2π*u (13 300
cm–1), σu2π*u/σu2φu/σu2δu (12 500 cm–1/10 000 cm–1) electronic configurations
(Figure ).
Figure 2
Representative
spectra of 3-crypt: (A). Electronic
UV–vis–nIR absorption spectrum (2.9 mM, DME). (B) Corrected
steady state emission spectrum recorded (295 K, 2-Me-THF, λexc = 280 nm). (C) Corrected steady state emission spectrum
recorded at 77 K (frozen 2-Me-THF, λexc = 300 nm).
(D) Corrected excitation spectrum recorded at 77 K (frozen 2-Me-THF,
λem = 475 nm). (E) Corrected steady state emission
spectrum of ground powder recorded (295 K, λexc =
280 nm). * denotes scattered light. (F) Spectrally sliced time-resolved
emission spectra (Figure S51) of powdered 3-crypt (295 K, 230 nm excitation, recorded over a 400 μs
time domain).
Figure 3
Computed MO
diagram of 3-crypt in the ground state.
For clarity, ligand orbitals are not explicitly shown. The principal
excitation promotes an electron from the σu/L(N2p) to the 5fδu orbital(s) (labeled as 5f
above, leaving an unpaired electron in the σu, 5f
δδ, and 5fδu orbitals).
Representative
spectra of 3-crypt: (A). Electronic
UV–vis–nIR absorption spectrum (2.9 mM, DME). (B) Corrected
steady state emission spectrum recorded (295 K, 2-Me-THF, λexc = 280 nm). (C) Corrected steady state emission spectrum
recorded at 77 K (frozen 2-Me-THF, λexc = 300 nm).
(D) Corrected excitation spectrum recorded at 77 K (frozen 2-Me-THF,
λem = 475 nm). (E) Corrected steady state emission
spectrum of ground powder recorded (295 K, λexc =
280 nm). * denotes scattered light. (F) Spectrally sliced time-resolved
emission spectra (Figure S51) of powdered 3-crypt (295 K, 230 nm excitation, recorded over a 400 μs
time domain).Solvatochromism of 3-crypt is further evidence the
charge-transfer character of absorptions in the visible region: dissolution
in pyridine converges the energies of the visible and nIR absorption
bands that span the 16 000 to 9000 cm–1 range
(625–1110 nm, see Figure S42 (SI)).The diagnostic spectroscopic features of [UVO2]+ were further defined via vibrational spectroscopy,
including the first reported Raman spectra for well-defined molecular
pentavalent uranyl species. Solid-state Raman spectra of 1 and 2-crypt have been previously reported with U=O(yl) symmetric stretching modes at 802 and 809 cm–1, respectively. A progression is often observed with the archetypal
uranyl(VI) σu ← δu/φuLMCT emission (←λmax ∼ 510
nm). In the solid-state Raman spectrum of 3-crypt several
signals are observed (Figure S25), including
the equivalent U=O(yl) symmetric stretching mode
at 753 cm–1 in THF solution, with a shoulder peaking
between 682 and 697 cm–1 (this feature is resolved
in 3–18C6 at 727 cm–1). The
shift of the ν1(U=O(yl)) symmetric
stretch between [UVIO2]2+ and [UVO2]+ species is consistent with a decrease
in the nuclear charge at uranium. This effect can also be quantified
by calculating the relative stretching and interaction force constants
(k1 and k12).[34,70,71] The uranyl(VI)
precursors 2–18C6 and 2-crypt have
stretching force constants of 6.85 and 6.94 mdyn Å–1 respectively. As expected, the force constants decrease for 3–18C6 and 3-crypt and are measured at
5.66 and 5.53 mdyn Å–1, respectively.[72] These experimental spectra are well-reproduced
by DFT calculations (geometry optimization and vibrational analysis, Figure S81).This vibrational analysis
sets the stage for the detailed understanding
of the photoluminescence spectra.[62,63] Prior to this
work, observation of uranyl(V) species has thus far been limited to
in situ studies of species generated from uranyl(VI).[31,32] In both instances, emission spectroscopy revealed broad featureless
emission bands centered at 405 and 440 nm respectively following 255
nm excitation. with luminescence lifetimes attributed to uranyl(V)
carbonate emission of 140 μs at 153 K and at pH 2.4, for the
aqua ion 1.1 μs at 298 K (compared to 0.9 μs for the equivalent
uranyl(VI) species also present in the solution at room temperature).Very recently, Mazzanti and co-workers reported the emission properties
of a water-soluble uranyl(V) dipicolinic acid (dpa) complex [K(2.2.2.crypt)]2{[KUO2(dpa)2]}.[18] in this system, the emission spectrum exhibits
a broad profile with two maxima at 404 and 459 nm following excitation
at 360 nm, with corresponding excitation peaks for the 404 nm emission
band at 335 and 360 nm. Upon excitation at 459 nm, the second maxima
is shifted to lower energy. At low temperatures (77 K), it was observed
that the emission profile becomes well resolved with seven distinguishable
vibrationally resolved lines in addition to lower intensity vibrationally
resolved emission up to 550 nm; the excitation spectra also exhibit
four sharp lines centered at ca. 360 nm. The decay kinetics showed
bi- or multiexponential behavior, with the longest component resolved
as 11 μs. These data are broadly in agreement with those observed
for 3-crypt reported herein.The photophysical
properties of the uranyl(VI) tris amide precursor, 2-crypt, [K(2.2.2-cryptand)][UO2{N(SiMe3)2}3]are shown in Figures S56–S60. The principal peak positions in the emission
spectrum are typical of uranyl(VI) and are 528 nm (18 939 cm–1), 550 nm (18 797 cm–1),
554 nm (18 182 cm–1), 576 nm (17 361
cm–1), with vibrational spacings measured as 757
and 821 cm–1. Here, the emission maximum is significantly
red-shifted (550 nm) compared to aqueous uranyl salts (ca. 510–520
nm) due to the strong amide sigma donors located in the equatorial
plane.[33,47]Continuous-wave UV excitation (230–300
nm) of mM, room temperature
DME, THF and 2-Me-THF solutions of 3-crypt (Figure B) results in broad
emission spectra, which are comprised of two principal bands centered
at 355 and 475 nm (26 170 and 21 050 cm–1). In room temperature 2-Me-THF, the 475 nm-feature displays discernible
vibrational progression. Upon freezing to a glass at 77 K in 2-Me-THF,
this vibrational fine structure becomes pronounced revealing seven
vibronic transitions with peak-to-peak separations of 737, 772, 717,
669, 757, and 760 cm–1 (average = 735 cm–1, Figure C). The
apparent zero-phonon (E0–0) transition
estimated between the first and second highest energy vibronic transitions
at 737 cm–1 matches well with the U=O(yl) symmetric stretch measured experimentally by Raman spectroscopy
(753 cm–1) and predicted computationally (711 cm–1) for the modes that possesses the most symmetric
U=O(yl) stretching character. However, this vibration
also possesses a degree of U–N{(SiMe)3}2 character, and computational analysis suggests that all of the other
vibrations with symmetric stretching character are coupled to other
molecular motions (723, 725, 728, and 732 cm–1).
The amide N–(SiMe)3 vibrations contribute to the
vibrations at frequencies of 724, 728, and 736 cm–1, where the latter is the most pronounced.[60,61] Therefore, more than one vibrational progression may be contributing
to the spectrum.The excitation spectra of 3-crypt (frozen 2-Me-THF)
monitored at the lowest energy emission maximum (475 nm) reveal three
separate excitation regions centered at 275, 324, and 390 nm (Figure D), whereas an excitation
band at 220 nm is responsible for the emission at 355 nm. In the excitation
spectrum, the lower energy absorptions appear to exhibit vibrational
fine structure. This feature is particularly pronounced in the lowest
energy excitation band (390 nm), with six measurable maxima (frequency
difference between the two lowest energy peaks is 490 cm–1, average peak-to-peak separation, 533 cm–1). These
features are reminiscent of the vibrationally resolved LMCT absorptions
exhibited in many [UVIO2]2+ compounds,
but here may, in principle, arise from the multiple different excitations
predicted in this region (Figure S80 and Table S6).The luminescence lifetimes recorded
at the emission maxima (475
nm) of 3-crypt in a frozen glass at 77 K (Figure C and Figure S44, Table ) are biexponential with the short component resolved as 1.02 μs
(25%), and the longer one at 8.22 μs (75%). This observation
implies that there are several excited states contributing to the
observed emission (as supported by theory). At room temperature (295
K), the corresponding lifetimes of the 475 nm band are much shorter
(2.1 and 9.5 ns) and could only be measured accurately following pulsed
picosecond excitation (375 nm).
Table 1
Summary of Lifetime
Data for 2-Crypt, 3-Crypt, 5, and 7a
complex
λex (nm)
λem (nm)
τ1 (μs)/(%)
τ2 (μs)/(%)
τ3 (μs)/(%)
χ2
2-cryptb
250
550
5.9
40.8
176.7
1.6
(34)
(37)
(27)
3-cryptb
280
320
3.7
24.0
186.4
1.3
(56)
(44)
(29)
280
360
4.3
77.5
153.3
1.2
(12)
(51)
(36)
280
492
5.2
41.2
204.1
1.0
(11)
(31)
(58)
280
580
6.9
44.2
198.7
1.3
(11)
(36)
(53)
3-cryptc
300
420
1.7
7.1
–
1.2
(47)
(53)
300
475
1.02
8.22
–
1.3
(25)
(75)
5b
230
370
109.5
–
–
1.3
(100)
230
440
130.1
–
–
1.2
(100)
230
550
5.2
57.4
160.5
1.0
(1)
(9)
(90)
5c
260
430
1.0
8.2
–
2.1
(22)
(78)
260
535
55.1
148.0
–
1.1
(28)
(72)
260
590
51.9
139.2
–
1.3
(27)
(73)
7c
325
480
11.0
102.9
–
1.1
(10)
(90)
325
550
45.6
202.5
–
1.2
(78)
(32)
Estimated
error ± 10%.
Sample
measured at 295 K in the
solid state.
Sample measured
at 77 K in a frozen
2-Me-thf glass.
Estimated
error ± 10%.Sample
measured at 295 K in the
solid state.Sample measured
at 77 K in a frozen
2-Me-thf glass.To forestall
contribution of any dynamic exchange and speciation
effects, the optical properties of solid-state 3-crypt were examined in detail. The steady-state spectrum of 3-crypt as a powdered sample (295 K), (Figure E) shows a similar emission profile to those
recorded in fluid solution and in a frozen glass, with overlapping
broad features (λem = 320, 420, and 475 nm). Again,
the emission band at 475 nm appears to exhibit vibrational progression,
where the estimated E0–0 is 772
cm–1 (average = 743 cm–1). The
kinetic profiles were also investigated by time-resolved emission
spectroscopy (TRES, Figure F, S51). Notably, as a function
of delay time, the emission profile of the 475 nm band resolves into
two components with peak maxima at 400 and 475 nm. The longest-lived
of these emission profiles is centered at 475 nm and exhibits biexponential
decay behavior (τ1 = 4.31 μs (12%) and τ2 = 127 μs (88%)), whereas the emissive feature at 400
nm is vibrationally broadened and is also modeled with a biexponential
decay function (τ1 = 5.56 μs (2%), τ2 = 117 μs (82%)).By analogy with reported experimental
and theoretical data of uranyl(V)[19,20,64,73] and neptunyl(VI)[47] 5f1 species
(where the emission with An = O(yl) to actinide charge
transfer character has been observed at 405, 440, and 438 nm respectively
in experiments), the equivalent lowest energy U ← U=O(yl) LMCT transition is expected to lie in the UV and be blue-shifted
with respect to that in uranyl(VI). In a complex of pseudo
D3 symmetry, as in 2 (L) and 3 (L), this transition is predicted to be formally
Laporte-forbidden but may be relaxed in part with respect to the free
ion of higher symmetry (D∞) due to the removal of the inversion symmetry by the inclusion
of the equatorial ligands. For comparison, in the neptunyl(VI) complex
[NpO2(TPIP)2(Ph3PO)] (TPIP = tetraphenylimidodiphoshinate),[47] the visible LMCT emission centered at 438 nm
also exhibits vibrational fine structure that corresponds to a N–P
vibration. The electronic excitations responsible for this emission
were shown by analogous calculations to be combination of Np ←
TPIP and Np ← O(yl)LMCT charge transfer.Computed MO
diagram of 3-crypt in the ground state.
For clarity, ligand orbitals are not explicitly shown. The principal
excitation promotes an electron from the σu/L(N2p) to the 5fδu orbital(s) (labeled as 5f
above, leaving an unpaired electron in the σu, 5f
δδ, and 5fδu orbitals).To investigate the origin of the emission in 3-crypt further, TD-DFT calculations were performed using
linear response
theory in the absence of point group symmetry, and a total of 100
excited states were evaluated. In preliminary studies to benchmark
methods on free uranyl including hybrid-GGA (e.g., PBE0, B3LYP) and
Coulomb-attenuated hybrids (e.g., CAM-B3LYP) with wave functions based
methods (CASPT2) indicate little variation with respect to functional,[74−79] and hence PBE0 was selected in an effort to minimize dependence
of the simulation data on parameters not optimized for the system
of interest. From a computational perspective, f-f transitions were
assigned on the basis of visual inspection of electron density difference
plots between ground and excited states (Figure ).
Figure 4
Plot of density differences between the ground
and excited state
for the 3-crypt. There are transitions with O(yl)-f character at 356, 352, 345, 312, and 302 nm. The light regions
indicate charge depletion and the blue areas charge accumulation.
Plot of density differences between the ground
and excited state
for the 3-crypt. There are transitions with O(yl)-f character at 356, 352, 345, 312, and 302 nm. The light regions
indicate charge depletion and the blue areas charge accumulation.Indeed, for the bare uranyl(VI) ion in the gas
phase, our DFT simulations
(PBE0/def2-TZVP) show the triplet state with single occupation of
the 5fδu orbital (a fair approximation to the optically
accessible excited state),[80] whereas for
the uranyl(V) cation, the equivalent excitation produces a quartet
with occupation of each of the degenerate 5fδu orbitals.
In both cases, the σu orbital has been deoccupied
(Figure ). The energy
difference between these LMCT excitations are calculated as 2.29 eV
(18 484 cm–1, 541 nm) for uranyl(VI) and
2.82 eV (22 779 cm–1, 439 nm) for uranyl(V)
consistent with previous observations.[20,31,32,64]Time-dependent
DFT simulations of the excited states of 3-crypt show
numerous excitations between 200–300 nm with oscillator
strengths >10–3 (Figure , Table S6). Of
these, a number of excitations with 5f ← Oyl character
(356, 352, 345, 312, 302 nm) were identified (Figure S80). Energetically, these are not well separated from
the intra f-f transitions and oscillator strengths of all are typically
∼10–4. Higher energy excitations <45 450
cm–1 (220 nm) are characterized as being localized
on the amide ligands, while those between 220 and 265 nm are associated
with charge-transfer from the amide ligands to the uranium nonbonding
5fδu orbitals.Attempts to investigate the
luminescence properties of 3–18C6 by excitation
into the UV and visible absorption bands (220–650
nm), in both solution (2-Me-THF, DME) and in the solid state were
unsuccessful, with no discernible emission or excitation seen even
at 77 K. This is in stark contrast to 3-crypt. The lack
of detectable emission under the same conditions in 3–18C6 may suggest that this complex is not as thermally and/or photochemically
stable as 3-crypt and rapidly reacts or decomposes to
form a nonemissive (or dark) thermal or photoproduct. Indeed, this
difference in stability was observed by 1H NMR spectroscopy
as noted above. Very similar observations were seen in the luminescence
experiments of the uranyl(VI) peroxo complex 6 (Figure S76).The emission properties of
the uranyl(V) complexes 5 and 7, were also
investigated, where we anticipated
that any U=O(yl)LMCT emission bands in particular
would be red-shifted slightly compared to 3-crypt due
to elongation/disruption of the linear uranyl unit.[13] For dimeric 5, the spectra are broader than
in 3-crypt in frozen solution and the solid state following
UV excitation (280–360 nm), with peak maxima at ca. 370, 410,
and 480 nm at 295 and 77 K (Figures S61–S75). The instability of 5 in optically dilute solutions
and in the solid state over prolonged acquisition times precluded
accurate and full data collection in addition to any data collection
in fluid solution at room temperature. However, representative spectra
in frozen solution at 77 K and in the solid state (Figures S61–S75) exhibit features attributable to uranyl(V)
centered around 470 nm, albeit much broader as expected. There is
also evidence for relatively stronger emission at higher energies
(ca. 400 nm) in line with that observed for 3-crypt.
Nevertheless, the steady state emission spectra of 5 points
toward the fact that higher nuclearity complexes of uranyl(V) may
be observable by optical spectroscopy and show a unique spectral and
temporal profile, especially when recorded at lower temperatures.Finally for complex, 7, the emission spectrum (Figures S77–S79) appears to be a combination
of uranyl(V) and uranyl(VI), where typical uranyl(VI) emission bands
(ca. 530 nm) displaying vibrational fine structure (E0–0 = 769 cm–1) alongside a broader
feature centered at ca. 480 nm. However, the origin of this emission
is not clear by examining the excitation spectra, and may be a result
of uranyl(VI) LMCT from the equatorial amide/chloride donors or a
mixture of uranyl(VI) LMCT and uranyl(V) LMCT emission.Of note,
we observed no emission in the near-infrared region of
the electromagnetic spectrum with our current instrumentation by exciting
across the UV–visible spectrum (300–850 nm). This result
is in contrast to the near-infrared emission observed from NpO22+ in D2O and in the polyoxometalate complex [Na2(NpVIO2)2(GeW9O34)2]14- reported by Faulkner
and co-workers.[72] Here, emission between
1452 and 1580 nm was observed following ns pulsed laser excitation
at 337 nm (N2 laser). This difference may be rationalized
at least in part, by examining the respective absorption spectra,
where there is a larger energy gap between the UV–visible absorptions
(neptunyl(VI) LMCT and the polyoxometalate LMCT which acts to sensitize
the emission in the complex) and the near-infrared absorption at ca.
1230 nm which is the characteristic absorption and assigned as an
interconfigurational 5f-f transition of neptunyl(VI); i.e., they are
more energetically well separated. In contrast, in 3-crypt and the other uranyl(V) complexes reported herein, there are several
broad absorptions that lie in the visible region which may preclude
effective population of any near-infrared excited states. Future work
is directed at examining the luminescence properties of uranyl(V)
complexes using higher powered laser excitation and at temperatures
below that of liquid N2.
Conclusion
In
conclusion, this study reports the first photoluminescence and
Raman spectra of well-defined monomeric [UVO2]+ complexes. Experimental and theoretical studies support
the assignment of the excited states in [UVO2]+ as principally a quartet, whose origin is an admixture
of amide to U(5f) and O(yl) to U(5f) with a unique vibrational
progression (with smaller contributions from intra 5f excitations)
where the emission band at 475 nm is best described computationally
as an open-shell doublet or quartet with a high degree of mixing (compared
to the well-defined triplet 5fδu excited state in
uranyl(VI)). Overall, the clear definition of these luminescence steady-state
and time-resolved features of the [UVO2]+ moiety in monomeric and dimeric complexes[20,30−32] should enable detailed studies of [UVO2]+ in biological and engineered environments.[18−20,73,81,82]
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