The conjugate base of methyl 3-oxobutanoate as an antenna ligand in visible-emitting photoluminescent lanthanide complexes

Marco Bortoluzzi*a, Andrea Reolona, Jesús Castroc, Francesco Enrichiab, Gabriele Albertina and Carlo Bragatoa
aDipartimento di Scienze Molecolari e Nanosistemi, Università Ca' Foscari Venezia, Via Torino 155, 30170 Mestre, Venezia, Italy. E-mail: markos@unive.it
bCNR-IFN, Istituto di Fotonica e Nanotecnologie, Laboratorio CSMFO, via alla Cascata 56/C, 38123 Povo, Trento, Italy
cDepartamento de Química Inorgánica, Universidade de Vigo, Facultade de Química, Edificio de Ciencias Experimentais, 36310 Vigo, Galicia, Spain

Received 20th January 2016 , Accepted 20th March 2016

First published on 24th March 2016


Abstract

Coordination compounds with the formulae [Y(MAA)3]x (1Y), [Ln(MAA)3]x (1Ln), [Y(MAA)3(phen)] (2Y) and [Ln(MAA)3(phen)] (2Ln) (Ln = Sm, Eu, Tb, Dy, Yb; MAA = conjugate base of methyl 3-oxo-butanoate; phen = 1,10-phenantroline) were synthesized and characterized, and X-ray diffraction data were collected for [Tb(MAA)3(phen)] (2Tb) and [Yb(MAA)3(phen)] (2Yb). Most of the lanthanide derivatives showed appreciable luminescence in the solid state upon excitation with near-UV light. Strong emissions were observed in particular for complexes of lanthanide ions with high-energy resonance levels. Visible-emitting [Ln(MAA)3(phen)] compounds were successfully used as dopants for the preparation of luminescent poly(methylmethacrylate) samples. Similar derivatives of the conjugate base of dimethyl malonate (DMM), with formulae [Y(DMM)3(phen)] (3Y) and [Ln(DMM)3(phen)] (3Ln) (Ln = Eu, Tb, Dy), were also synthesized and their photoluminescence behaviour was compared to that of the analogous methyl 3-oxo-butanoato-complexes.


Introduction

β-Diketonates are among the most used organic ligands in lanthanide coordination chemistry, and a huge number of neutral and charged complexes is known. The most usual substituents are alkyls, aryls, thiophene-based rings and perfluorinated chains, and the common coordination numbers are eight and nine. Even if the coordination sphere can be composed by only β-diketonates, often other ligands are present, usually mono- and polydentate oxygen and nitrogen donors. Besides their use as NMR shift reagents, MOCVD precursors and catalysts for organic reactions, these compounds have been studied in detail as luminescent materials. Several β-diketonate complexes of trivalent lanthanide ions are of current interest for the preparation of advanced materials for frontier technology applications, such as novel devices for light conversion and amplification and new biomedical sensors.1

Quite surprisingly, lower attention has been devoted to other anionic bidentate O-donor ligands comparable to β-diketonates. As an example, we recently reported the synthesis and photophysical characterization of lanthanide derivatives with the conjugate bases of nitromalonaldehyde and bromomalonaldehyde, their use as dopants for luminescent plastic materials and the electrochemical tuning of photoluminescence of an europium complex of bromomalonalehyde.2

Other examples of ligands of potential interest for the preparation of new lanthanide complexes are the conjugate bases of methyl 3-oxo-butanoate (methyl acetoacetate, MAA) and dimethyl malonate (DMM). To the best of our knowledge no lanthanide compound with MAA is actually reported in the literature, even if some complexes of group 4 elements have been synthesized and characterized.3 For what concerns DMM and similar ligands, dinuclear dysprosium complexes of the type [Dy{ROC(O)CHC(O)OR}3]2 (R = Me, Et, iPr, tBu, SiMe3) and heteroleptic species having formulae [Dy{ROC(O)CHC(O)OR}3(bpy)] (R = Et, tBu, SiMe3; bpy = 2,2′-bipyridine) and [Dy{Me3SiOC(O)CHC(O)OSiMe3}3(py)] (py = pyridine) have been prepared and used as MOCVD precursors, but no photophysical study has been carried out.4 In the framework of our interest towards new luminescent lanthanide complexes and polymeric materials containing lanthanide derivatives,5 the lack of experimental data regarding the use of methyl 3-oxo-butanoate as antenna-ligand towards lanthanide ions prompted us to start a research in this field. The results are summarized in this paper, together with comparative outcomes concerning new DMM-based lanthanide complexes.

Results and discussion

Synthesis and characterization of the complexes

Complexes having formulae [Y(MAA)3]x (1Y) and [Ln(MAA)3]x (1Ln) (MAA = conjugate base of methyl 3-oxo-butanoate; Ln = Sm, Eu, Tb, Dy, Yb) were obtained by reacting YCl3 or LnCl3 with three equivalents of K[MAA] in THF at room temperature, as depicted in Scheme 1. The elemental analyses agree with the proposed formulations. The IR spectra are all similar and show a quite intense signal involving the C[double bond, length as m-dash]O moieties at wavenumbers comprised between 1625 and 1644 cm−1. The 1H NMR spectra of the MAA derivatives in (CD3)2SO or CDCl3 show three signals attributable to the CH, C(O)CH3 and OCH3 groups of the coordinated ligands, which are therefore equivalent on the NMR timescale (see the ESI file, Fig. S1–S6). These resonances are affected by paramagnetic shift and relaxation in lanthanide derivatives, in particular when the metal centre has high magnetic moment. As an example, the δ values for the diamagnetic derivative 1Y in deuterated dimethylsulfoxide are 4.62, 3.44 and 1.69 ppm, while the chemical shift values for 1Tb are 99.25, 78.19 and −32.30 ppm. No signal corresponding to coordinated THF is present and conductivity measurements have ruled out the formation of ionic compounds. Three MAA ligands are not able to saturate the coordination sphere of the yttrium and lanthanide ions, therefore the formation of oligomers is expected. On considering the dinuclear structure of the dialkyl malonate complexes [Dy{ROC(O)CHC(O)OR}3]2 already reported in the literature,4 where two [Dy{ROC(O)CHC(O)OR}3] units are bridged by two oxygen atoms, one from an OR group and the other from a C[double bond, length as m-dash]O moiety, we can tentatively suppose a comparable structure also for the new compounds 1Y and 1Ln.
image file: c6ra01741j-s1.tif
Scheme 1 Synthesis of [Y(MAA)3]x (1Y), [Ln(MAA)3]x, (1Ln), [Y(MAA)3(phen)] (2Y), [Ln(MAA)3(phen)] (2Ln), [Y(DMM)3(phen)] (3Y) and [Ln(MAA)3(phen)] (3Ln).

Addition of 1,10-phenanthroline (phen) to THF solutions of 1Y or 1Ln at room temperature led to the formation of the complexes [Y(MAA)3(phen)] 2Y and [Ln(MAA)3(phen)] 2Ln (Ln = Sm, Eu, Tb, Dy, Yb), as depicted in Scheme 1. The elemental analyses confirm the proposed formulations and conductivity measurements indicate that these complexes are neutral. The IR stretching involving the C[double bond, length as m-dash]O moieties falls between 1616 and 1622 cm−1, at slightly lower wavenumbers with respect to the homoleptic precursors. All the 1H NMR spectra, recorded using CDCl3 or (CD3)2SO as solvents, show three signals for the CH, C(O)CH3 and OCH3 groups of MAA and four resonances attributable to phen (see the ESI file, Fig. S7–S12). As for 1Y and 1Ln, no signal due to coordinated THF is observable. Paramagnetic shift and relaxation strongly influence the resonances of all the coordinated ligands. For example, the 1H NMR signals of 2Tb and 2Dy at 298 K are spread over a range of about 140 ppm. The relative simplicity of the 1H NMR spectra can be explained on admitting a fast fluxional behaviour of the complexes in solution, which makes the three MAA ligands equivalent on the NMR timescale. In the cases of 2Tb and 2Yb crystals suitable for X-ray diffraction were obtained from dichloromethane/diethylether solutions.

The asymmetric units of both 2Tb and 2Yb contain two molecules with similar geometrical parameters, only one of them is shown in Fig. 1. For each Ln(III), the coordination environment includes six O atoms from three methyl 3-oxobutanoato-O,O′ ligands and two N atoms from the 1,10-phenanthroline neutral ligand. Selected bond lengths and angles are set out in Table 1.


image file: c6ra01741j-f1.tif
Fig. 1 Left: ORTEP6 view (20% probability level) of one of the molecules 2Tb found in the asymmetric unit. Right: ORTEP6 view (30% displacement level) of one of the molecules found in the asymmetric unit of 2Yb. For clarity, only one of the methyl 3-oxobutanoato ligands was labelled.
Table 1 Selected bond lengths [Å] and angles [°] for 2Tb and 2Yb
  2Tb 2Yb
Ln(1)–O(11) 2.323(4) 2.309(3)
Ln(1)–O(12) 2.330(4) 2.247(3)
Ln(1)–O(21) 2.298(5) 2.249(3)
Ln(1)–O(22) 2.406(5) 2.313(3)
Ln(1)–O(31) 2.315(4) 2.311(3)
Ln(1)–O(32) 2.348(4) 2.276(3)
Ln(1)–N(41) 2.633(5) 2.533(3)
Ln(1)–N(42) 2.605(5) 2.525(3)
Ln(2)–O(51) 2.305(6) 2.298(3)
Ln(2)–O(52) 2.398(5) 2.278(3)
Ln(2)–O(61) 2.316(4) 2.250(3)
Ln(2)–O(62) 2.345(5) 2.320(3)
Ln(2)–O(71) 2.314(4) 2.279(3)
Ln(2)–O(72) 2.352(5) 2.274(3)
Ln(2)–N(81) 2.592(6) 2.522(3)
Ln(2)–N(82) 2.633(7) 2.498(3)
O(11)–Ln(1)–O(12) 72.37(14) 74.73(10)
O(21)–Ln(1)–O(22) 72.37(16) 74.07(12)
O(31)–Ln(1)–O(32) 72.15(15) 73.18(11)
N(41)–Ln(1)–N(42) 61.90(16) 64.52(10)
O(51)–Ln(2)–O(52) 72.25(19) 73.18(11)
O(61)–Ln(2)–O(62) 72.11(17) 73.92(13)
O(71)–Ln(2)–O(72) 72.19(15) 74.11(15)
N(81)–Ln(2)–N(82) 61.81(18) 64.84(10)


The coordination polyhedron of the LnN2O6 was approximately assigned by using the SHAPE software7 and the calculation indicated that the LnN2O6 coordination polyhedron resulted to be different for each lanthanide. In the case of 2Tb the polyhedron is best described as “triangular dodecahedron”, as seen in Fig. 2, with SHAPE values of 0.343 and 0.420 for the two molecules, while other possibilities8 as elongated trigonal prism are bigger than 2.5. The output of the SHAPE program are given in Table 2.


image file: c6ra01741j-f2.tif
Fig. 2 Polyhedron (dodecahedron) around the Tb atom in 2Tb.
Table 2 Output of the SHAPE software for 2Tb and 2Yba
Structure [ML8] (*) OP HPY HBPY CU SAPR TDD JGBF JETBPY JBTPR BTPR JSD TT ETBPY
a Note that there are two molecules in the asymmetric unit in both compounds. (*) OP D8h octagon; HPY C7v heptagonal pyramid; HBPY D6h hexagonal bipyramid; CU Oh cube; SAPR D4d square antiprism; TDD D2d triangular dodecahedron; JGBF D2d Johnson gyrobifastigium J26; JETBPY D3h Johnson elongated triangular bipyramid J14; JBTPR C2v biaugmented trigonal prism J50; BTPR C2v biaugmented trigonal prism; JSD D2d Snub disphenoid J84; TT Td triakis tetrahedron; ETBPY D3h elongated trigonal bipyramid.
Tb1 33.409 24.288 15.162 8.110 3.116 0.343 15.224 29.231 3.308 2.744 3.144 8.831 25.273
Tb2 32.318 23.826 15.081 8.248 2.266 0.420 14.946 29.489 3.113 2.571 3.263 8.996 24.948
Yb1 29.333 22.793 16.868 10.327 0.391 2.107 16.038 27.550 2.385 1.984 4.765 11.124 23.641
Yb2 29.897 22.486 16.290 9.964 0.477 2.282 15.925 27.651 2.692 2.086 4.852 10.785 24.326


The Tb–O bond lengths vary in the range of 2.298(5) to 2.406(5) Å, similar (although in a slightly wide range) to that found in the acetylacetonate compound [Tb(acac)3(tdzp)] where tdzp represents a substituted phenanthroline, between 2.320(2) and 2.385(2) Å,9 and the Tb–N bond distances are between 2.592(6) and 2.633(7) Å, slightly longer than the Tb–N distances (2.563 and 2.567 Å) found for other Tb(1,10-phen) complexes.10

Methyl 3-oxo-butanoato-O,O′ ligands are chelating the Tb(III) forming five membered rings almost planar11 with root-mean-square deviation for these plane less than 0.0512 Å. Phenanthroline ligand is coordinated without any bending, and the Tb atoms are situated at less than 0.156(1) Å out of the phenanthroline best plane [that is, the angles between the phenanthroline best plane and the Tb–N bonds are between 2.7(2) and 2.9(2)°]. The O–Tb–O angles are in the range of 72.1(2) to 72.4(2)°, (five membered rings) whereas the N–Tb–N ones are 61.9(2) and 61.8(2)° (four membered rings) and these chelate rings are forming a paddle-wheel structure (Fig. 3) with dihedral angles rings of average 82.24°.


image file: c6ra01741j-f3.tif
Fig. 3 Left: paddle-wheel structure for 2Tb. Right: paddle-wheel structure for 2Yb. Only chelate rings atoms were drawn.

Regarding with 2Yb, once more the coordination environment of each Yb(III) is formed by six O atoms from three methyl 3-oxo-butanoato-O,O′ ligands and two N atoms from the 1,10-phenanthroline neutral ligand. However compounds 2Tb and 2Yb are not isomorphous. The SHAPE software7 provides for the coordination environment the data show in Table 2 which let us to conclude for this compound a “square antiprismatric polyhedron”. The two square planes consisting, for Yb1 of atoms N(41)/N(42)/O(11)/O(12) and O(31)/O(32)/O(21)/O(22), and for Yb2 of atoms N(81)/N(82)/O(71)/O(72) and O(51)/O(52)/O(61)/O(62) with a deviation of the root-mean-square of 0.0699, 0.0308, 0.0387 and 0.0770 Å, respectively. These square planes are rotated by an angle of almost 45° with respect to each other (see Fig. 4) and the distance between the centroids of the two square planes are about 2.54 Å. Yb(III) atoms are situated at about 1.34 Å from the N2O2 plane and at 1.18 Å from the O4 plane.


image file: c6ra01741j-f4.tif
Fig. 4 Square antiprism around Yb metal for 2Yb. In yellow the square planes.

Methyl 3-oxo-butanoato-O,O′ ligands are chelating the Yb(III) forming five membered rings and they are strongly bent coordinated, in a different manner that occurs with the related Tb compound 2Tb, with root-mean-square deviation for these plane of average 0.122 Å. If the metal atom is not considered in the calculation of the best plane, such atom deviated from the OCCO plane in average 0.56 Å, between 0.463(6) and 0.663(6) Å. Also the 1,10-phenathroline is coordinated in a bending mode, in such a way that the Yb atoms are situated at 0.467(1) and 0.536(1) Å from the phenanthroline best plane [that is, the angles between the phenanthroline best planes and the Yb–N bonds are between 9.7(2) and 11.7(2)°]. These deviations are clearly showed on the paddle-wheel structure shown in Fig. 3.

The Yb–O bond lengths are between 2.247(3) and 2.320(3) Å, as usual shorter than the Yb–N bond lengths, which range between 2.498(3) and 2.533(3) Å. These values are shorter to those in the terbium complex as expected due the well known lanthanide contraction. No important differences with other octacoordinated Yb(III) complexes are found.12

The replacement of K[MAA] with the potassium salt of dimethyl malonate, K[DMM], using the previously described experimental conditions allowed to isolate the complexes [Y(DMM)(phen)], 3Y and [Ln(DMM)(phen)], 3Ln (Ln = Eu, Tb, Dy), as depicted in Scheme 1. Elemental analyses and conductivity measurements support the proposed formulations. All the IR spectra are closely comparable and show a quite intense band between 1661 and 1667 cm−1 attributable to the stretching of the carboxylic moieties. As for the previously described complexes 2Y and 2Ln, fluxional behaviour in solution led to quite simple 1H NMR spectra, where only two resonances for DMM and four signals for phenanthroline are present, affected by meaningful paramagnetic shift in the case of 3Eu (see Fig. 5). Unfortunately, paramagnetic relaxation did not allow to observe resolved resonances for the 3Tb and 3Dy derivatives. It is likely to suppose that also 3Ln complexes are mononuclear, on considering the X-ray structures reported in the literature for the dysprosium derivatives [Dy{ROC(O)CHC(O)OR}3(bpy)] (R = Et, tBu, SiMe3; bpy = 2,2′-bipyridine).4


image file: c6ra01741j-f5.tif
Fig. 5 1H NMR spectra of 3Y and 3Eu (CDCl3, 298 K).

Preliminary electrochemical investigations on solutions of the europium derivatives suggested that the f-orbitals involved in the reduction of Eu3+ to Eu2+ are screened by the coordinated O-donor ligands, a behaviour already observed in the past for europium β-diketonates and nitromalonaldeyde complexes.1a,2a A typical cyclic voltammogram is reported as an example in Fig. S13.

Photoluminescence measurements on complexes and doped polymers

Photoluminescence studies were initially carried out on 1Ln complexes. Compound 1Eu is weakly luminescent in the red region upon excitation with UV light. The emission spectrum (see Fig. 6) shows that the most intense transition is the 5D07F2, centred at 611 nm (73.7%). The high 5D07F2/5D07F1 ratio, 10[thin space (1/6-em)]:[thin space (1/6-em)]1, suggests a low symmetry of the inner coordination sphere.13 The luminescence decay curve is mono-exponential and the measured lifetime (τ) is 0.255 ms, quite low if compared to the τ values of several homoleptic β-diketonate europium complexes.14 An intrinsic quantum yield (Qi) around 18% has been estimated from the τ value and the relative intensity of the 5D07F1 transition.
image file: c6ra01741j-f6.tif
Fig. 6 Emission spectra (solid samples, 298 K) of 1Eu (red plot, λexcitation = 319 nm), 1Tb (green plot, λexcitation = 325 nm) and 1Dy (yellow plot, λexcitation = 365 nm).

MAA showed to be an efficient antenna-ligand towards the Tb3+ ion. 1Tb is an intense green-emitting compound under UV light. The typical 5D47FJ (J = 6–0) transitions can be observed in the emission spectrum of 1Tb and the most intense is the 5D47F5 one, centred at 544 nm (Fig. 6). The photoluminescence excitation spectrum indicates that the antenna-effect from the coordinated ligands is the dominant process of population of the resonance level of Tb3+ and occurs for λexcitation below 380 nm, the maximum being reached around 305 nm (see Fig. S14). The observed lifetime for the terbium emission in 1Tb is 0.965 ms, corresponding to a Qi value of about 20% by accepting 4.75 ms as the τrad value for Tb3+.15

The photoluminescence measurements were in turn extended to the samarium derivative 1Sm, but no resolved emission spectrum was collected. Despite the fact that the transitions in the visible range of Sm3+ and Eu3+ fall at comparable wavelengths, the samarium compounds are more influenced by non-radiative decay because of the lower energy gap between the resonance level and the highest ground-state SO level (Sm3+: 7400 cm−1; Eu3+: 12[thin space (1/6-em)]300 cm−1 (ref. 16)). This fact, combined with the hygroscopic character of 1Sm, could explain the very poor photoluminescence exhibited by this compound.

Similar problems were expected for 1Dy, even if the lower ionic radius17 makes this compound meaningfully less hygroscopic than 1Sm. Quite surprisingly, an appreciable yellowish-white luminescence was observed for samples of 1Dy under near-UV light, and the emission spectrum of 1Dy (Fig. 6) shows resolved bands due to the transitions from 4F9/2 to 6HJ (J = 15/2–11/2), the most intense being the hypersensitive 4F9/26H13/2 centred at 572 nm (72.9%). The measured lifetime of this emission, 26 μs at room temperature, is quite long if compared to the few data present in the literature. For example, a τ value of 7 μs has been reported for the compound [Dy(PM)3(TPPO)2] (PM = 1-phenyl-3-methyl-4-isobutyryl-5-pyrazolone; TPPO = triphenylphosphine oxide).18 The observed lifetime for the tris(benzoylacetonate) complex of dysprosium at 77 K is 12.3 μs.19 By admitting a τrad value for the Dy3+ ion around 400 μs,20 the intrinsic quantum yield of 1Dy is around 6–7%.

We tried to explain the good performances exhibited by the MAA complexes of emitters having high-energy resonance levels by performing DFT and TD-DFT calculations on the diamagnetic model system [Lu(MAA)3] and, for comparative purposes, on [Lu(acac)3] (acac = acetylacetonate). The Cartesian coordinates of the two optimized geometries are collected in the ESI. The computed average Lu–O bond lengths, 2.195 Å for [Lu(acac)3], 2.183 Å and 2.201 Å for [Lu(MAA)3] respectively relative to the Lu-OC(CH3) and Lu-OC(OCH3) interactions, are closely comparable to experimental data reported in the literature for similar compounds. As an example, Inoue et al. reported an average Lu–O distance of 2.19 Å for the tris(2,2,6,6-tetramethylheptane-3,5-dionato)lutetium(III).21

MAA is formally an acetylacetonate derivative where one –CH3 group is replaced by a –OCH3 moiety. DFT outcomes predict a meaningful raise of both the first excited singlet (S) and triplet (T) states from [Lu(acac)3] (S: 31[thin space (1/6-em)]600 cm−1; T: 23[thin space (1/6-em)]900 cm−1) to [Lu(MAA)3] (S: 35[thin space (1/6-em)]800 cm−1; T: 26[thin space (1/6-em)]900 cm−1), attributable to the introduction of an electron-withdrawing group. The computed values support the idea of an easier energy transfer from MAA towards the resonance levels of Tb3+ (20[thin space (1/6-em)]430 cm−1) and Dy3+ (20[thin space (1/6-em)]960 cm−1)1d with respect to acac. The long lifetimes recorded for 1Tb and 1Dy can be therefore attributed to the favourable excited-state energies of coordinated MAA, besides the lack of high-energy oscillators close to the lanthanide centres.

The addition of 1,10-phenanthroline to the coordination sphere on the lanthanide ions caused an increase of light harvesting in the UV range. Moreover, the observed lifetime for the 2Eu derivatives is 0.828 ms, meaningfully higher than that of 1Eu (see Fig. 7 for the luminescence decay curve of 2Eu). The intrinsic quantum yield is 67% and makes 2Eu a bright red-luminescent compound under excitation with near-UV light. The measured lifetime appears quite long if compared to the τ values of the phen-europium derivatives of dibenzoylmethane, dimethoxydibenzoylmethane, benzoylacetone and 4-methylbenzoyl-2-furanoylmethane, ranging from 0.34 to 0.47 ms.22 The same Qi value was obtained in the past for the complex [Eu(NMA)3(terpy)] (NMA = nitromalonaldehyde; terpy = 2,2′:6′,2′′-terpyridine).2b The most intense band in the emission spectrum is the 5D07F2 one (62.1%) and, as for 1Eu, the 5D07F2/5D07F1 ratio is around 10[thin space (1/6-em)]:[thin space (1/6-em)]1 (Fig. 8). It is likely to suppose that the 7F1 level is composed by three sublevels, even if two of them overlap in Fig. 8, and that the 7F2 is separated in five sublevels, the last one corresponding to the weak transition at 631 nm. This would agree with the very low symmetry of the first coordination sphere observed in the X-ray structures of the analogues 2Tb and 2Yb derivatives.13c The photoluminescence excitation spectrum indicates antenna-effect over about all the UV range, as observable in Fig. 7. Comparable excitation spectra for wavelengths below 400 nm have been recorded for all the other 2Ln derivatives (see Fig. S15–S18). As a minor point, it is to be highlighted the high intensity of the hypersensitive 5D27F0 transition at 464 nm in the PLE spectrum reported in Fig. 7, if compared to the 5L67F0 band at 394 nm.


image file: c6ra01741j-f7.tif
Fig. 7 Luminescence decay curve of 2Eu (solid sample, 298 K, λexcitation = 325 nm, λemission = 613 nm). Inset: excitation spectrum of 2Eu (solid sample, 298 K, λemission = 610 nm).

image file: c6ra01741j-f8.tif
Fig. 8 Emission spectra (solid samples, 298 K) of 2Sm (orange plot, λexcitation = 350 nm), 2Eu (red plot, λexcitation = 338 nm), 2Tb (green plot, λexcitation = 310 nm) and 2Dy (yellow plot, λexcitation = 365 nm).

Also in the case of terbium the coordination of 1,10-phenanthroline caused an increase of luminescence. The observed lifetime of 2Tb is 1.212 ms, meaningfully higher than that of 1Tb, and corresponds to an estimated Qi of 26%. The bright green emission of this complex is related to the 5D47FJ (J = 6–0) transitions, the most intense (67.6%) occurring for J = 5 and centred between 541 and 547 nm (Fig. 8).

Differently from the precursor 1Sm, the compound 2Sm is perceptibly photoluminescent. The bands in the 550–750 nm range, observable in Fig. 8, are associated to the 4G5/26HJ (J = 5/2–11/2) transitions. The most intense emission is the hypersensitive one around 645 nm, corresponding to J = 9/2, as already reported for β-diketonate derivatives of samarium.23 Having the 4G5/26H5/2 transition predominant magnetic dipole character, an elevated 4G5/26H9/2/4G5/26H5/2 intensity ratio indicates low symmetry and high polarizability of the first coordination sphere. In the case of 2Sm this ratio is 7.7, higher than those of [Sm(Tp)3] and [Sm(DPA)3]3− (Tp = tris(pyrazol-1-yl)-borate; DPA = dipicolinate), which are comprised between 4 and 5. Ratios greater than 10 have been however obtained for several tetrakis-β-diketonates.5c,23a The τ value measured for 2Sm, 31 μs, is a bit lower than that reported for [Sm(hfa)3(phen)] (hfa = hexafluoroacetylacetonate).24 On the basis of the τrad values present in the literature for Sm3+, around 3 ms,25 the intrinsic quantum yield of 2Sm is about 1%.

Even if the photoluminescence of 2Dy appears enhanced by the increased absorption due to the coordination of 1,10-phenantholine, the measured τ value is 3 μs, meaningfully lower than that obtained for the precursor 1Dy. As for the homoleptic compound, the yellow-whitish emission is attributable to the 4F9/26HJ (J = 15/2–9/2) transitions, in particular the 4F9/26H15/2 (29%) at about 484 nm and the 4F9/26H13/2 (66.2%) centred at 576 nm, as observable in Fig. 8. This is the only case here reported of a reduction of lifetime caused by the coordination of phenanthroline ligand. It is worth noting that the triplet state of 1,10-phenanthroline is around 22[thin space (1/6-em)]100 cm−1 in the free molecule.26 On considering the previously described TD-DFT results, coordinated 1,10-phenanthroline should be the ligand with the lowest triplet state energy in the coordination sphere of 2Dy. The decrease of the observed lifetime from 1Dy to 2Dy could be therefore attributed to the closeness of the Dy3+ emitting level 4F9/2 (20[thin space (1/6-em)]960 cm−1 (ref. 1d)) to the triplet state of the N-donor ligand.

After examining the photoluminescent features of the 1Ln and 2Ln complexes of visible-emitting lanthanide ions, attention has been devoted to the ytterbium derivatives 1Yb and 2Yb. Both the compounds showed the typical 7F5/22F7/2 transition at around 1000 nm upon excitation with UV light, as observable in Fig. 9. The emission spectrum is more resolved for compound 2Yb, probably because of the lower hygroscopic character due to the saturation of the coordination sphere. In both the cases, however, the luminescence resulted too weak to allow the measurement of the lifetime.


image file: c6ra01741j-f9.tif
Fig. 9 Emission spectra (solid samples, 298 K) of 1Yb (light gray plot, λexcitation = 326 nm) and 2Yb (dark gray plot, λexcitation = 351 nm).

The good photoluminescent features of the 2Ln complexes of europium, terbium and dysprosium prompted us to prepare and characterize the corresponding DMM derivatives 3Ln. In all the cases compounds with appreciable luminescence in the visible range upon excitation with UV light were isolated. The emission spectra of 3Tb and 3Dy are roughly comparable to those previously described for the 2Ln complexes of the same elements. In the case of the europium complex, even if the 5D07F2 transition remains the most intense one, the intensity ratio 5D07F2/5D07F1 of 3Eu is meaningfully lower with respect to 2Eu, being about 5.5[thin space (1/6-em)]:[thin space (1/6-em)]1. The change of chelating O-donor ligand also influences the observed luminescence lifetimes. The τ values measured for 3Tb and 3Dy at room temperature are respectively 1.268 ms and 6 μs, a bit longer than those recorded for the analogous 2Ln compounds, this suggesting a slight increase of intrinsic quantum yield. On the other hand, the lifetime of the emission of 3Eu is 0.540 ms, meaningfully shorter than that reported for 2Eu. On considering the change of relative intensity of the 5D07F1 transition, the Qi value estimated for 3Eu is 25%. The measured lifetimes of 1Ln, 2Ln and 3Ln compounds are summarized for clarity in Table 3.

Table 3 Observed lifetimes (μs) of complexes and doped plastic materials (298 K)
  1Ln 2Ln 2Ln@PMMA 2Ln@PVP 3Ln 3Ln@PMMA
a Freshly prepared sample.
Sm   31 36      
Eu 255 828 337 686a 540  
Tb 965 1212 342   1268 28
Dy 26 3 5   6  


The phen-complexes having luminescence in the visible range were studied as dopants for the preparation of photoluminescent poly(methylmethacrylate), PMMA. The samples were obtained by adding a known amount of the proper complex to a solution of PMMA in dichloromethane and subsequent slow removal of the solvent. The complex: PMMA ratios considered in this work range from 10 to 50 μmol gPMMA−1. The 2Ln@PMMA samples (Ln = Sm, Eu, Tb, Dy) showed appreciable luminescence if irradiated with UV light. The relative intensities of the Ln3+ transitions in the emission spectra are roughly similar to those observed for the pure compounds and do not depend upon the concentration of the complex in the matrix, this suggesting that the embedding in PMMA does not meaningfully change the first coordination sphere of the complexes. The presence of PMMA chains has however a variable influence on the observed lifetimes (see Table 3). For the derivatives of the metal centres most affected by non-radiative decay, i.e. samarium and dysprosium, a small increase of the τ values is caused by the encapsulation in the polymer matrix (τ = 36 μs for 2Sm@PMMA, 5 μs for 2Dy@PMMA), probably because the complexes are protected from moisture. On the other hand, the measured lifetimes of 2Eu@PMMA and 2Tb@PMMA are meaningfully lower than those of the pure compounds, respectively 0.337 ms and 0.342 ms. This result can be tentatively explained on the basis of an incremented competition of luminescence from the excited states of the ligands. In fact, as clearly observable in Fig. 10 for Ln = Eu, a broad band in the violet-blue region appears in the emission spectrum of the doped polymer, which is absent in that of the pure complex. All the 2Ln@PMMA doped polymers exhibited negligible variations of the lifetimes on changing the concentration of the complexes in the corresponding materials.


image file: c6ra01741j-f10.tif
Fig. 10 Comparison of the emission spectra of solid 2Eu (red line) and 2Eu@PMMA (purple line) at 298 K. λexcitation = 338 nm.

Also 3Ln complexes were studied as dopants for the preparation of luminescent poly(methylmethacrylate), PMMA. Unfortunately, photophysical measurements on 3Tb@PMMA suggest that the complex is decomposed by the polymer chains. Even if the emission spectrum shows the typical transitions of the Tb3+ ion, the measured lifetime is extremely low, around 28 μs, corresponding to an intrinsic quantum yield below 1%.

Besides PMMA, another polymer that was considered is polyvinylpyrrolidone PVP, which has recently shown to be a good matrix for the preparation of photoluminescent plastics doped with lanthanide β-diketonates.27 Preliminary experiments using 2Eu as luminescent species indicate that the coordination sphere is progressively altered by PVP. In fact, the photoluminescence of 2Eu@PVP quenches almost completely in few days. Emission and excitation measurements on freshly prepared samples showed a relative increase of the 5D07F1 and 5D07F4 transitions with respect to pure 2Eu and a reduction of about 50 nm of the excitation spectrum in the near-UV range.

Conclusions

In this paper we reported new coordination compounds of trivalent yttrium and lanthanide ions with the conjugate base of methyl 3-oxo-butanoate. This ligand resulted able to sensitize several luminescent lanthanide ions and good performances were observed in particular for homoleptic complexes of the high-energy emitters Tb3+ and Dy3+, a result probably attributable to the raise of the excited states with respect to common β-diketonates caused by the presence of an electron-withdrawing moiety. The introduction of 1,10-phenanthroline in the coordination sphere enhanced the luminescence of the samarium, europium and terbium complexes, but the τ value of [Dy(MAA)3(phen)] resulted meaningfully lower than that of [Dy(MAA)3]n. Visibly luminescent plastic materials were obtained from the embedding of [Ln(MAA)3(phen)] complexes in PMMA, but luminescence from the coordinated ligands became competitive for the derivatives of europium and terbium. Polyvinylpyrrolidone resulted not suited as matrix for the preparation of plastic materials doped with these compounds. Finally, some dimethyl malonato-complexes of the type [Ln(DMM)3(phen)] were isolated and characterized. The photoluminescence features of the terbium and dysprosium complexes resemble those of the analogous methyl 3-oxo-butanoate derivatives, while the sensitization of Eu3+ is less efficient. Preliminary experiments indicated that these last compounds are strongly altered by encapsulation in PMMA.

Experimental section

Materials and methods

The reagents used for the preparation of the lanthanide complexes and the doped polymers were Aldrich products used without further purifications, with the exception of the anhydrous YCl3 and LnCl3 salts (Strem). The synthesis of the complexes was carried out under inert atmosphere (N2, < 5 ppm O2, < 1 ppm H2O) in a MBraun glove-box. Solvents were purified using common techniques.28 The potassium salt K[MAA] was prepared by slowly adding potassium tert-butoxide (1.040 g, 9.3 mmol) in anhydrous methanol (20 mL) to a solution of methyl 3-oxo-butanoate (1.0 mL, 9.3 mmol) in 30 mL of methanol, kept at 0 °C. At the end of the addition, the solvent was removed under reduced pressure and diethylether (30 mL) was added. The white solid obtained was filtered and dried. Yield 95%. The salt K[DMM] was prepared by adding 2.0 mL (17.5 mmol) of dimethyl malonate to 1.960 g (17.5 mmol) of potassium tert-butoxide in 100 mL of frozen, anhydrous THF. The reaction mixture was allowed to slowly reach room temperature, then the solvent was removed by evaporation under reduced pressure and diethylether (50 mL) was added. The solid which separated out was collected by filtration and dried. Yield 95%.

Conductivity measurements were carried out at 298 K on 10−3 mol dm−3 solutions using a radiometer Copenhagen CDM 83 instrument. Voltammetric experiments were performed at room temperature in an air-tight, three-electrode cell, which was located in a Faraday cage to avoid external noise. Glassy carbon working electrodes (1.5 mm radius) were employed. A platinum spiral was used as counter electrode, and aqueous Ag/AgCl saturated with KCl was used as reference electrode. All working electrodes were polished mechanically with graded alumina powder on a polishing microcloth. All voltammetric measurements were carried out using a CH Instruments 760b bipotentiostat. Elemental analyses were performed at the University of Padua using either a Fison EA1108 or a Thermo Scientific FLASH 2000 CHNS-O microanalyzer. NMR spectra were recorded at variable temperature on a Bruker Avance 300 or a Bruker AC 200 spectrometer using CDCl3 or (CD3)2SO as solvents. 1H chemical shifts are reported relative to tetramethylsilane. The solvent signals, quoted with respect to TMS (δ = 0 ppm), were used as internal references. IR spectra were recorded from 4000 to 400 cm−1 using a Perkin Elmer Spectrum One spectrophotometer. Samples were dispersed in KBr or nujol. Photoluminescence emission (PL) and excitation (PLE) measurements were carried out on solid samples at room temperature by a Horiba Jobin Yvon Fluorolog-3 spectrofluorometer. A xenon arc lamp was used as continuous-spectrum source selecting the excitation wavelength by a double grating Czerny-Turner monochromator. A single grating monochromator coupled to a R928 Hamamatsu photomultiplier tube (PMT) was used as detection system for optical emission measurements. Excitation and emission spectra were corrected for the instrumental functions. Time-resolved analyses were performed in Multi Channel Scaling modality (MCS) by using a tuneable pulsed Nd:YAG laser system as excitation source. The luminescence lifetimes were derived from the luminescence decay curves, fitting the data with the least squares method by using mono-exponential equation for all the materials. The intrinsic quantum yield (Qi) was estimated on the basis of eqn (1), where τ is the measured luminescence lifetime. τrad was obtained for the europium-based compounds from eqn (2), where η indicates the refractive index of the sample and the value of 1.5 is assumed in this work for comparative purposes. I(5D07FJ)/I(5D07F1) is the ratio between the total integrated emission from the Eu(5D0) level to the 7FJ manifold and the integrated intensity of the transition 5D07F1.29 The τrad values for the samarium, terbium and dysprosium ions were taken from the literature (Sm3+: 3 ms;25 Tb3+: 4.75 ms;15 Dy3+: 400 μs (ref. 19)).

 
image file: c6ra01741j-t1.tif(1)
 
image file: c6ra01741j-t2.tif(2)

Synthesis of [Y(MAA)3]x (1Y) and [Ln(MAA)3]x (1Ln) (Ln = Sm, Eu, Tb, Dy, Yb)

In a typical preparation, solid K[MAA] (0.463 g, 3.0 mmol) was slowly added at room temperature under inert atmosphere to 1.0 mmol of anhydrous YCl3 or LnCl3 in 20 mL of THF under vigorous stirring. The resulting reaction mixture was allowed to react at room temperature for 12 hours, then the solids were separated by centrifugation and the solvent was evaporated under reduced pressure. The residual white solid was triturated with diethylether (10 mL), filtered and dried under vacuum. Yield >70% in all the cases.
Characterization of 1Y. C15H21O9Y: calcd C 41.49, H 4.87; found C 41.30, H 5.00. IR (KBr): νCO = 1630 cm−1. 1H NMR ((CD3)2SO, 298 K, δ): 4.62 (s, 1H, CH); 3.44 (s, 3H, OCH3); 1.69 (s, 3H, C(O)CH3). 1H NMR (CDCl3, 315 K, δ): 4.71 (s, 1H, CH); 3.56 (s, 3H, OCH3); 1.81 (s,3H, C(O)CH3).
Characterization of 1Sm. C15H21O9Sm: calcd C 36.35, H 4.27; found 36.19, H 4.37. IR (nujol): νCO = 1626 cm−1. 1H NMR ((CD3)2SO, 315 K, δ): 5.44 (s, slightly br, 1H, CH); 3.16 (s, slightly br, 3H, OCH3); 2.26 (s, 3H, C(O)CH3).
Characterization of 1Eu. C15H21O9Eu: calcd C 36.23, H 4.26; found 36.18, H 4.40. IR (KBr): νCO = 1644 cm−1. 1H NMR ((CD3)2SO, 295 K, δ): 6.07 (s, slightly br, 3H, OCH3); −0.82 (s, br, 1H, CH); −4.23 (s, slightly br, 3H, C(O)CH3). 1H NMR ((CD3)2SO, 324 K, δ): 6.79 (s, slightly br, 3H, OCH3); −0.6 (s, very br, CH); −3.16 (s, br, 3H, C(O)CH3). PL (solid sample, 298 K, λexcitation = 319 nm, nm): weak, 578 (5D07F0, 0.7%); 591 (5D07F1, 7.2%); 611 (5D07F2, 73.7%); 652 (5D07F3, 3.8%); 690, 701 (5D07F4, 14.6%). PLE (solid sample, 298 K, λemission = 611 nm, nm): max 319 (ligand excitation); 393, 464 (Eu3+ excitation). Emission decay time (solid sample, λexcitation = 325 nm, λemission = 612 nm): τ = 0.255 ms. Qi = 18%.
Characterization of 1Tb. C15H21O9Tb: calcd C 35.73, H 4.20; found 35.59, H 4.38. IR (KBr): νCO = 1644 cm−1. 1H NMR ((CD3)2SO, 298 K, δ): 99.25 (s, br, 1H, CH); 78.19 (s, br, 3H, CH3); −32.30 (s, br, 3H, CH3). 1H NMR ((CD3)2SO, 310 K, δ): 89.65 (s, br, 1H, CH); 70.12 (s, br, 3H, CH3); −30.59 (s, br, 3H, CH3). PL (solid sample, 298 K, λexcitation = 305 nm, nm): medium, 487, 494 (5D47F6, 21.2%); 541, 546 (5D47F5, 65.3%); 582, 591 (5D47F4, 7.4%); 617, 622 (5D47F3, 4.7%); 635–695 (5D47F2, 5D47F1, 5D47F0, 1.4%). PLE (solid sample, 298 K, λemission = 546 nm, nm): max 305 (ligand excitation). Emission decay time (solid sample, λexcitation = 325 nm, λemission = 545 nm): τ = 0.965 ms. Qi = 20%.
Characterization of 1Dy. C15H21O9Dy: calcd C 35.48, H 4.17; found 35.37, H 4.30. IR (nujol): νCO = 1628 cm−1. 1H NMR ((CD3)2SO, 319 K, δ): 54.1 (s, very br, 1H, CH); 38.1 (s, very br, 3H, CH3); −55.0 (s, very br, 3H, CH3). PL (solid sample, 298 K, λexcitation = 365 nm, nm): strong, 478 (4F9/26H15/2, 19.9%); 572 (4F9/26H13/2, 72.9%); 662 (4F9/26H11/2, 7.2%). Emission decay time (solid sample, λexcitation = 350 nm, λemission = 585 nm): τ = 26 μs. Qi = 7%.
Characterization of 1Yb. C15H21O9Yb: calcd C 34.76, H 4.08; found 34.61, H 4.12. IR (KBr): νCO = 1625 cm−1. 1H NMR ((CD3)2SO, 319 K, δ): 14.18, 8.27, −15.59 (3s, br, MAA). PL (solid sample, 298 K, λexcitation = 326 nm, nm): weak, 950–1060, max 978 (2F5/22F7/2). PLE (solid sample, 298 K, λemission = 1000 nm, nm): max 327 (ligand excitation).

Synthesis of [Y(MAA)3(phen)] (2Y) and [Ln(MAA)3(phen)] (2Ln) (Ln = Sm, Eu, Tb, Dy, Yb)

Solid K[MAA] (0.463 g, 3.0 mmol) was slowly added at room temperature under inert atmosphere to 1.0 mmol of anhydrous YCl3 or LnCl3 in 20 mL of THF under vigorous stirring. The resulting reaction mixture was left under stirring at room temperature for 6 hours, then a solution of anhydrous 1,10-phenantholine (0.180 g, 1.0 mmol) in 5 mL of THF was added drop by drop. The reaction mixture was allowed to react overnight at room temperature, then the solids were removed by centrifugation, the solvent was evaporated under reduced pressure and diethylether (5 mL) was added. The solid which separated out was filtered, washed with 5 mL of cold diethylether and dried under vacuum. Yield >75% in all the cases.
Characterization of 2Y. C27H29N2O9Sm: calcd C 52.78, H 4.76, N 4.56; found 52.59, H 4.80, N 4.61. IR (KBr): νCO = 1622 cm−1. 1H NMR (CDCl3, 298 K, δ): 9.50 (d, 2H, 3JHH = 4.5 Hz, phen-H2/H9); 8.36 (d, 2H, 3JHH = 8.3 Hz, phen-H4/H7); 7.85 (s, 2H, phen-H5/H6); 7.76 (dd, 2H, 3JHH = 4.5 Hz, 3JHH = 8.3 Hz, phen-H3/H8); 4.69 (s, 3H, CH); 3.39 (s, 9H, OCH3); 1.79 (s, 9H, C(O)CH3).
Characterization of 2Sm. C27H29N2O9Sm: calcd C 47.98, H 4.32, N 4.14; found 47.90, H 4.48, N 4.24. IR (KBr): νCO = 1616 cm−1. 1H NMR (CDCl3, 298 K, δ): 9.20 (s, br, 3H, CH); 8.28 (d, slightly br, 2H, 3JHH = 7.8 Hz, phen-H4/H7); 7.82 (s, 2H, phen-H5/H6); 7.66 (m, slightly br, 2H, phen-H3/H8); 7.55 (s, br, 2H, phen-H2/H9); 3.30 (s, slightly br, 9H, OCH3); 2.35 (s, br, 9H, C(O)CH3). PL (solid sample, 298 K, λexcitation = 345 nm, nm): strong, 558, 564 (4G5/26H5/2, 7.2%); 593, 599, 604, 608 (4G5/26H7/2, 26.9%); 639, 646, 650 (4G5/26H9/2, 55.1%); 703, 711 (4G5/26H11/2, 10.8%). PLE (solid sample, 298 K, λemission = 646 nm, nm): max 310–357 (ligand excitation); 403, 418 (Sm3+ excitation). Emission decay time (solid sample, λexcitation = 320 nm, λemission = 646 nm): τ = 31 μs. Qi = 1%.
Characterization of 2Eu. C27H29N2O9Eu: calcd C 47.87, H 4.31, N 4.13; found 47.69, H 4.50, N 4.04. IR (KBr): νCO = 1616 cm−1. 1H NMR (CDCl3, 298 K, δ): 10.88 (d, 2H, 3JHH = 7.8 Hz, phen-H4/H7); 10.62 (s, 2H, phen-H5/H6); 9.21 (s, slightly br, 2H, phen-H2/H9); 8.58 (dd, slightly br, 2H, 3JHH = 4.0 Hz, 3JHH = 7.8 Hz, phen-H3/H8); 5.85 (s, 9H, OCH3); 0.09 (s, 3H, CH); -3.42 (s, 9H, C(O)CH3). 1H NMR (CDCl3, 315 K, δ): 10.56 (d, slightly br, 2H, phen-H4/H7); 10.26 (s, slightly br, 2H, phen-H5/H6); 9.20 (s, br, 2H, phen-H2/H9); 8.40 (m, slightly br, 2H, phen-H3/H8); 5.80 (s, 9H, OCH3); 0.82 (s, 3H, CH); −3.04 (s, 9H, C(O)CH3). 1H NMR (CDCl3, 324 K, δ): 10.34 (s, br, 2H, phen-H4/H7); 10.08 (s, br, 2H, phen-H5/H6); 9.18 (s, br, 2H, phen-H2/H9); 8.31 (s, br, 2H, phen-H3/H8); 5.74 (s, 9H, OCH3); 1.18 (s, 3H, CH); −2.82 (s, 9H, C(O)CH3). PL (solid sample, 298 K, λexcitation = 338 nm, nm): very strong, 578 (5D07F0, 0.6%); 590, 594 (5D07F1, 6.1%); 610, 613, 619, 624, 631 (5D07F2, 62.1%); 649, 654 (5D07F3, 3.5%); 685, 694, 701, 705 (5D07F4, 27.7%). PLE (solid sample, 298 K, λemission = 610 nm, nm): max 307–346 (ligand excitation); 394, 464 (Eu3+ excitation). Emission decay time (solid sample, λexcitation = 325 nm, λemission = 613 nm): τ = 0.828 ms. Qi = 67%.
Characterization of 2Tb. C27H29N2O9Tb: calcd C 47.38, H 4.27, N 4.09; found 47.21, H 4.43, N 3.96. IR (KBr): νCO = 1616 cm−1. 1H NMR ((CD3)2SO, 298 K, δ): 109.61 (s, br, 2H, phen); 99.03 (s, br, 2H, phen); 77.64 (s, br, 3H, CH); 62.97 (s, br, 9H, CH3); 7.84 (s, slightly br, 2H, phen); −21.08 (s, slightly br, 2H, phen); −31.65 (s, 9H, CH3). PL (solid sample, 298 K, λexcitation = 310 nm, nm): very strong, 486, 490, 496 (5D47F6, 19.2%); 541, 547 (5D47F5, 67.6%); 581, 590 (5D47F4, 6.7%); 617, 621 (5D47F3, 4.2%); 635–695 (5D47F2, 5D47F1, 5D47F0, 2.3%). PLE (solid sample, 298 K, λemission = 548 nm, nm): max 307–351 (ligand excitation). Emission decay time (solid sample, λexcitation = 325 nm, λemission = 545 nm): τ = 1.212 ms. Qi = 26%.
Characterization of 2Dy. C27H29N2O9Dy: calcd C 47.13, H 4.25, N 4.07; found 46.97, H 4.45, N 3.95. IR (KBr): νCO = 1619 cm−1. 1H NMR (CDCl3, 298 K, δ): 86.2 (s, very br, 3H, CH); 9.03 (s, slightly br, 2H, phen); 8.33 (s, slightly br, 2H, phen); 7.88 (s, slightly br, 2H, phen); 7.63 (s, slightly br, 2H, phen); −50.04 (s, br, 9H, CH3); −55.47 (s, br, 9H, CH3). PL (solid sample, 298 K, λexcitation = 365 nm, nm): strong, 481, 486 (4F9/26H15/2, 29.0%); 576 (4F9/26H13/2, 66.2%); 663 (4F9/26H11/2, 3.4%); 751 (4F9/26H9/2, 1.4). PLE (solid sample, 298 K, λemission = 576 nm, nm): max 307–355 (ligand excitation). Emission decay time (solid sample, λexcitation = 373 nm, λemission = 576 nm): τ = 3 μs. Qi = 1%.
Characterization of 2Yb. C27H29N2O9Yb: calcd C 46.42, H 4.18, N 4.01; found 46.29, H 4.30, N 3.90. IR (KBr): νCO = 1622 cm−1. 1H NMR ((CD3)2SO, 315 K, δ): 20.30 (s, br, 2H, phen); 19.08 (s, br, 2H, phen); 14.36 (s, br, 3H, CH); 13.05 (s, br, 2H, phen); 9.00 (s, br, 2H, phen); 8.33 (s, br, 9H, CH3); −16.52 (s, br, 9H, CH3). PL (solid sample, 298 K, λexcitation = 351 nm, nm): medium, 978, 1010, 1040 (2F5/22F7/2). PLE (solid sample, 298 K, λemission = 1000 nm, nm): max 351 (ligand excitation).

Synthesis of [Y(DMM)3(phen)] (3Y) and [Ln(DMM)3(phen)] (3Ln) (Ln = Eu, Tb, Dy)

The experimental procedure for the preparation of 3Y and 3Ln is the same above described for 2Y and 2Ln, replacing K[MAA] with K[DMM] (0.511 g, 3.0 mmol). Yield >75% in all the cases.
Characterization of 3Y. C27H29N2O12Y: calcd C 48.95, H 4.41, N 4.23; found 48.79, H 4.52, N 4.15. IR (nujol): νCO = 1667 cm−1. 1H NMR (CDCl3, 298 K, δ): 9.52 (dd, 2H, 3JHH = 4.8 Hz, 4JHH = 1.7 Hz, phen-H2/H9); 8.41 (dd, 2H, 3JHH = 8.2 Hz, 4JHH = 1.7 Hz, phen-H4/H7); 7.89 (s, 2H, phen-H5/H6); 4.19 (s, 3H, CH); 3.47 (s, 9H, OCH3).
Characterization of 3Eu. C27H29N2O12Eu: calcd C 44.70, H 4.03, N 3.86; found 44.57, H 4.20, N 3.91. IR (nujol): νCO = 1661 cm−1. 1H NMR (CDCl3, 298 K, δ): 12.87 (d, slightly br, 2H, 3JHH = 3.5 Hz, phen-H2/H9); 10.00 (d, 2H, 3JHH = 8.1 Hz, phen-H4/H7); 9.28 (s, 2H, phen-H5/H6); 8.78 (dd, 2H, 3JHH = 3.5 Hz, 3JHH = 8.1 Hz, phen-H3/H8); 3.56 (s, 18H, OCH3); 0.06 (s, 3H, CH). 1H NMR (CDCl3, 298 K, δ): 12.15 (s, slightly br, 2H, phen-H2/H9); 9.79 (d, slightly br, 2H, 3JHH = 8.1 Hz, phen-H4/H7); 9.06 (s, 2H, phen-H5/H6); 8.55 (m, 2H, phen-H3/H8); 3.54 (s, 18H, OCH3); 0.66 (s, 3H, CH). PL (solid sample, 298 K, λexcitation = 365 nm, nm): medium, 579 (5D07F0, 1.1%); 588, 591, 596 (5D07F1, 10.8%); 610, 615, 619 (5D07F2, 59.2%); 651 (5D07F3, 3.8%); 700, 707 (5D07F4, 25.1%). Emission decay time (solid sample, λexcitation = 350 nm, λemission = 616 nm): τ = 0.540 ms. Qi = 25%.
Characterization of 3Tb. C27H29N2O12Tb: calcd C 44.27, H 3.99, N 3.82; found 44.35, H 4.20, N 3.90. IR (nujol): νCO = 1664 cm−1. No NMR data available because of paramagnetic relaxation. PL (solid sample, 298 K, λexcitation = 365 nm, nm): very strong, 489 (5D47F6, 14.7%); 546 (5D47F5, 62.0%); 582, 588 (5D47F4, 9.9%); 620 (5D47F3, 7.7%); 635–695 (5D47F2, 5D47F1, 5D47F0, 5.7%). Emission decay time (solid sample, λexcitation = 350 nm, λemission = 557 nm): τ = 1.268 ms. Qi = 27%.
Characterization of 3Dy. C27H29N2O12Dy: calcd C 44.06, H 3.97, N 3.81; found 43.90, H 4.13, N 3.69. IR (nujol): νCO = 1664 cm−1. No NMR data available because of paramagnetic relaxation. PL (solid sample, 298 K, λexcitation = 365 nm, nm): strong, 480, 487 (4F9/26H15/2, 22.7%); 575 (4F9/26H13/2, 70.8%); 662 (4F9/26H11/2, 6.5%). Emission decay time (solid sample, λexcitation = 350 nm, λemission = 588 nm): τ = 6 μs. Qi = 1–2%.

Preparation of doped polymers

2Ln@PMMA (Ln = Sm, Eu, Tb, Dy) and 3Tb@PMMA samples were prepared by adding under N2 atmosphere a known amount of a freshly prepared 10−4 M solution of the proper complex in CH2Cl2 to a solution of 1.00 g of poly(methylmethacrylate) (PMMA, atactic, average Mw = 86[thin space (1/6-em)]000 g mol−1) in 50 mL of dichloromethane, to obtain complex: PMMA ratios ranging from 10 to 50 μmol gPMMA−1. The solutions were then concentrated to ca. 5 mL by evaporation under reduced pressure and transferred in a plastic polyethylene holder having 20 mm diameter. The residual solvent was allowed to evaporate overnight at room temperature and then the samples were kept under 10−3 torr pressure for 6 hours. Plastic glasses having about 2–3 mm thickness were obtained. A similar procedure was used for the preparation of 2Eu@PVP (PVP = polyvinylpyrrolidone, average Mw = 10[thin space (1/6-em)]000 g mol−1), using anhydrous methanol instead of dichloromethane as solvent.
Characterization of 2Sm@PMMA. PL (solid sample, 298 K, λexcitation = 356 nm, nm): strong, 564 (4G5/26H5/2, 5.5%); 599, 606, 609 (4G5/26H7/2, 25.4%); 646, 653 (4G5/26H9/2, 63.2%); 709 (4G5/26H11/2, 5.9%). Emission decay time (solid sample, λexcitation = 350 nm, λemission = 646 nm): τ = 36 μs. Qi = 1%.
Characterization of 2Eu@PMMA. PL (solid sample, 298 K, λexcitation = 338 nm, nm): very strong, 578 (5D07F0, 1.6%); 588, 592, 595 (5D07F1, 8.6%); 611, 616, 623 (5D07F2, 71.4%); 651 (5D07F3, 3.5%); 691, 703 (5D07F4, 14.9%). PLE (solid sample, 298 K, λemission = 610 nm, nm): max 335 (ligand excitation); 464 (Eu3+ excitation). Emission decay time (solid sample, λexcitation = 325 nm, λemission = 613 nm): τ = 0.337 ms. Qi = 19%.
Characterization of 2Tb@PMMA. PL (solid sample, 298 K, λexcitation = 310 nm, nm): very strong, 489, 496 (5D47F6, 24.3%); 545 (5D47F5, 64.6%); 583, 589 (5D47F4, 6.5%); 620 (5D47F3, 3.2%); 635–695 (5D47F2, 5D47F1, 5D47F0, 1.4%). PLE (solid sample, 298 K, λemission = 545 nm, nm): max 308–345 (ligand excitation). Emission decay time (solid sample, λexcitation = 325 nm, λemission = 544 nm): τ = 0.342 ms. Qi = 7%.
Characterization of 2Dy@PMMA. PL (solid sample, 298 K, λexcitation = 365 nm, nm): strong, 481, 484 (4F9/26H15/2, 17.9%); 575 (4F9/26H13/2, 75.4%); 662 (4F9/26H11/2, 6.7%). Emission decay time (solid sample, λexcitation = 350 nm, λemission = 573 nm): τ = 5 μs. Qi = 1%.
Characterization of 2Eu@PVP. PL (freshly prepared solid sample, 298 K, λexcitation = 294 nm, nm): strong, 578 (5D07F0, 0.5%); 591 (5D07F1, 10.2%); 614, 618 (5D07F2, 53.0%); 650 (5D07F3, 1.8%); 687, 694, 697 (5D07F4, 34.5%). PLE (freshly prepared solid sample, 298 K, λemission = 616 nm, nm): max 273, 294 (ligand excitation). Emission decay time (freshly prepared solid sample, λexcitation = 325 nm, λemission = 613 nm): τ = 0.686 ms. Qi = 33%.
Characterization of 3Tb@PMMA. PL (solid sample, 298 K, λexcitation = 365 nm, nm): medium, 488 (5D47F6, 18.4%); 544 (5D47F5, 54.5%); 583, 588 (5D47F4, 14.5); 621 (5D47F3, 8.5%); 635–695 (5D47F2, 5D47F1, 5D47F0, 4.1%). Emission decay time (solid sample, λexcitation = 350 nm, λemission = 544 nm): τ = 0.028 ms. Qi < 1%.

Theoretical calculations

The computational geometry optimization of the lutetium model complexes Lu(MAA)3 and Lu(acac)3 was carried out without symmetry constrains using the hybrid DFT B3PW91 functional30 in combination with the ECP-based basis set SDD, where the 4f shell of the lanthanide centre is included in a relativistic pseudopotential.31 The relative energies of the excited states were obtained from single-point time-dependent DFT calculations on the equilibrium geometries, using the previously described DFT functional and basis set.32 All the calculations were performed on a Intel-based x86-64 workstation and the software used was Gaussian '09.33

Crystal structure determination of 2Tb and 2Yb

Crystallographic data for 2Tband 2Yb were collected at room temperature using a Bruker Smart 6000 CCD detector and Cu-Kα radiation (λ = 1.54178 Å) generated by a Incoatec microfocus source equipped with Incoatec Quazar MX optics. The software APEX2 (ref. 34) was used for collecting frames of data, indexing reflections, and the determination of lattice parameters, SAINT34 for integration of intensity of reflections, and SADABS34 for scaling and empirical absorption correction. The crystallographic treatment was performed with the Oscail program.35 The structures were solved by charge flipping in arbitrary dimensions [Superflip program]36 and refined by a full-matrix least-squares based on F2.37 Non-hydrogen atoms were refined with anisotropic displacement parameters. Hydrogen atoms were included in idealized positions and refined with isotropic displacement parameters. For 2Yb, the Squeeze program38 was used to correct the reflection data for the diffuse scattering due to disordered molecule present in the unit cell. And also for latter 2Yb some positional disorder was found, but it was not modelled. In fact, all the methyl 3-oxo-butanoato-O,O′ ligand labelled as O71, O72, O73, C71, C72… is disordered over two positions, but the model including both positions does not improve the agreement factors, so only one position was refined, although BUMP and SIMU restrains were applied. CCDC 1448054 (2Tb) and 1448055 (2Yb) contain the ESI crystallographic data for this paper. Details of crystal data and structural refinement are given in Table 4.
Table 4 Crystal data and structure refinement
Identification code 2Tb 2Yb
Empirical formula C27H29N2O9Tb C27H29N2O9Yb
Formula weight 684.44 698.56
Temperature 296(2) K 296(2) K
Wavelength 1.54178 Å 1.54178 Å
Crystal system Triclinic Triclinic
Space group P[1 with combining macron] P[1 with combining macron]
Unit cell dimensions a = 9.3684(2) Å a = 13.1594(6) Å
b = 16.6936(3) Å b = 16.6828(8) Å
c = 18.2672(4) Å c = 16.7793(8) Å
α = 83.1135(10)° α = 88.5817(16)°
β = 88.7925(10)° β = 72.2913(14)°
γ = 87.0863(8)° γ = 66.8382(14)°
Volume 2832.25(10) Å3 3207.3(3) Å3
Z 4 4
Density (calculated) 1.605 Mg m−3 1.447 Mg m−3
Absorption coefficient 12.743 mm−1 5.803 mm−1
F(000) 1368 1388
Crystal size 0.154 × 0.121 × 0.108 mm 0.171 × 0.144 × 0.087 mm
Θ range for data collection 2.437 to 68.172° 2.781 to 68.480°
Index ranges −11 ≤ h ≤ 11 −15 ≤ h ≤ 15
−20 ≤ k ≤ 20 −18 ≤ k ≤ 19
−21 ≤ l ≤ 21 −20 ≤ l ≤ 20
Reflections collected 57[thin space (1/6-em)]616 91[thin space (1/6-em)]364
Independent reflections 10[thin space (1/6-em)]084 [R(int) = 0.0612] 11[thin space (1/6-em)]448 [R(int) = 0.0443]
Reflections observed (>2σ) 7399 10[thin space (1/6-em)]211
Data completeness 0.973 0.970
Absorption correction Semi-empirical from equivalents
Max. and min. transmission 0.7531 and 0.3489 0.7531 and 0.4872
Refinement method Full-matrix least-squares on F2
Data/restraints/parameters 10[thin space (1/6-em)]084/0/714 11[thin space (1/6-em)]448/42/714
Goodness-of-fit on F2 1.063 1.036
Final R indices [I > 2σ(I)] R1 = 0.0496 R1 = 0.0350
wR2 = 0.1252 wR2 = 0.0998
R indices (all data) R1 = 0.0698 R1 = 0.0385
wR2 = 0.1436 wR2 = 0.1043
Largest diff. peak and hole 1.174 and −1.413 e Å−3 1.307 and −0.644 e Å−3


Acknowledgements

Ca' Foscari University of Venice is gratefully acknowledged for financial support (Progetti di Ateneo 2014). We also thank to the CACTI (University of Vigo) for X-ray data collection.

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Footnote

Electronic supplementary information (ESI) available: 1H NMR spectra of the 1Y, 1Ln, 2Y and 2Ln derivatives (Fig. S1–S12); plot of a typical voltammogram of an europium MAA derivative (Fig. S13); selected excitation spectra (Fig. S14–S18). Cartesian coordinates of the DFT-optimized structures of Lu(acac)3 and Lu(MAA)3. CCDC 1448054 and 1448055. For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/c6ra01741j

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