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Electron-withdrawing groups as property tuners in functionalized terpyridine-based ligands in Eu(III) and Tb(III) complexes

Oksana Fizer a, Sina Chiniforoush b, Thomas J. Summers b, Mohammad Zafar Abbas a, David C. Cantu b and Ana de Bettencourt-Dias *a
aDepartment of Chemistry, University of Nevada, Reno, 1664 N. Virginia Street, Reno, NV 89557, USA. E-mail: abd@unr.edu
bDepartment of Chemical and Materials Engineering, University of Nevada, Reno, 1664 N. Virginia Street, Reno, NV 89557, USA

Received 8th October 2025 , Accepted 13th November 2025

First published on 24th November 2025


Abstract

Three terpyridine derivatives with electron-withdrawing groups in the ortho-position of terpyridine, –NO2 (terpyNO2), –CHO (terpyCHO) and –Br (terpyBr), were isolated and the influence of these substituents on the chemical and photophysical characteristics of the corresponding Eu(III), Tb(III) and Dy(III) complexes was assessed and compared with the complexes with unsubstituted terpyridine. A direct correlation between the complex stability constants and the second pKa2 values of the free ligands was found. Emission quantum yields indicate moderate ability to sensitize the metal-centered emission. Judd–Ofelt intensity parameters and energy transfer rates were calculated for all complexes. A direct correlation was found between the forward energy transfer rates and the sensitization efficiency for the Eu(III) complexes. For the Tb(III)-based complexes back-energy transfer from the metal ion to the ligands’ triplet level dominates. At 298 K, the Eu(III) complexes displayed emission lifetimes in the range 1.49–1.68 ms, while for the Tb(III) complexes the lifetimes were in the range 0.71–1.17 ms. The lifetimes of all the complexes could be fit with a single exponential at this temperature. However, at 77 K, double-exponential decay was observed. Nuclear magnetic resonance (NMR) analysis and density functional theory (DFT) calculations, modeled on the Eu(III)-terpyNO2 complex are consistent with decomplexation and subsequent rotation of one of the ligand's pyridine rings, which lead to the observed two species in frozen solution.


Introduction

The interest in luminescent lanthanide (Ln(III)) ion complexes is dictated by the metal ions’ unique optical properties,1 which make them useful for a variety of functional materials,2–5 such as OLEDs and lighting,6–10 biosensors,11–15 and chemical sensors.16 Moreover, Ln(III) ion complexes have interesting metal-based magnetic properties, and are explored as single-molecule magnets17–19 and as magnetic resonance imaging contrast agents; they have also garnered interest as therapeutic agents in chemotherapy.20,21 While the magnetic and optical properties are metal-based, variation of the ligand structure enables fine-tuning the properties of the complexes depending on the application.22–27

The molecular design of ligands for lanthanide-based complexes is a powerful approach to developing new materials and compounds with predefined and tuned properties. While searching for design criteria for enhancing magnetic hysteresis of Dy(III) single-molecule magnets (SMMs), Yu et al. found that replacing the ligand butoxide with a more hindered phenylethanolate in [Dy(OR)2(py)5][BPh4] leads to reduced quantum tunnelling at low temperatures and thus higher temperature of magnetic hysteresis.28 Corner et al. showed that adding one halobenzene PhX (X = F, Cl, Br) as additional equatorial ligand in a dysprosocenium-based SMM reduces the magnetic hysteresis temperature compared to the unsubstituted compound, due to an increase in the Orbach and two-phonon relaxation mechanisms, which correlate with the presence of the halide atoms bound to the metal ion.29 In the presence of two equatorial halobenzenes, a significant bending of the Cp*⋯Dy⋯Cp* moiety occurs, which promotes relaxation mechanisms.30 Building on the dysprosocenium architecture, Ullah et al. showed that it was possible to tune the blocking temperature of dysprosocenium-type SMMs by varying the cyclopentadienyl ring substituents.31 Photoluminescence can be modulated as well through ligand substitution, as demonstrated by Romanova et al., who showed the use of the substituted 2-phenoxy-1,10-phenanthroline sensitizer for improved Eu(III) luminescence.32

In the search for efficient sensitizers for Ln(III) ion emission, and unique modes of coordination for Ln(III) ion complexes, our group isolated several complexes with ligands bearing a –NO2 functional group, including a terpyridine functionalized at the ortho-position, terpyNO2. We found that the nitro moiety coordinated to the metal ion through one of its oxygen atoms and that the ligand sensitized metal-centred emission for both Eu(III) and Tb(III), yet yielded relatively weak luminescence.33

With the purpose of investigating the influence of other electron-withdrawing groups (EWGs) in the ortho-position of terpyridine ligands on the spectroscopic properties of their complexes with Eu(III), Tb(III) and Dy(III) ions, we isolated terpyBr, terpyCHO and compared the photophysical properties of their complexes with the complexes of terpyNO2 and the unsubstituted terpy. Our focus on these systems was made due to versatility of terpyridine heterocyclic system in coordination chemistry of Ln(III),34–36 and the ease of functionalization.37–39 While the selected EWGs should decrease the electron density on the terpyridine system and thus decrease its complexation ability, their localization at the ortho-position should allow to form an additional coordination bond to the central Ln(III) ion, thus increasing complex stability and decreasing the ability of solvent molecules to coordinate to the metal ion, which frequently results in vibrational quenching of the emission.

Experimental

General information

Starting materials purchased from commercial sources were used as received without further purification, unless otherwise indicated, and the solvents were dried by standard methods. All lanthanide salts were dried under reduced pressure at 60 °C for 12 h. Stock solutions of the Ln(III) (Ln = Eu(III), Gd(III), Tb(III) and Dy(III)) nitrate salts were prepared in spectroscopic grade acetonitrile. Concentration of the Ln(III) salt solutions was determined by complexometric titrations with EDTA (0.01 M) using xylenol orange as indicator.40 Unless otherwise indicated, all reactions were done under inert atmosphere.

NMR spectra were recorded on Varian 400 and 500 MHz spectrometers, and the chemical shifts were reported (ppm) against tetramethylsilane (TMS, 0.00 ppm) as the reference.

Mass spectra were recorded using an Agilent Technologies 6230 TOF LC/MS system with an electrospray ionization source.

Spectroscopic characterization

Absorption data were collected on a Perkin Elmer Lambda 35 spectrometer equipped with deuterium and tungsten halogen lamps and a concave grating with 105 lines per mm. Spectra were collected using a scan speed of 480 nm min−1 in the range 190–700 nm with a photodiode detector. All spectra were background corrected using solvent as the blank.

The emission and excitation spectra of the complexes were recorded on a Perkin Elmer LS-55 spectrometer equipped with a 450 W xenon discharge lamp at 298 and 77 K. All spectra were collected in the 200–800 nm range with a maximum scan speed of 250 nm min−1. Emission lifetimes were measured on the same instrument using the Short Phosphorescence Decay software package.

Standards used for emission quantum yield measurements were Cs3[Eu(dpa)3] (ϕstd = 24%, 7.5 × 10−5 M in TRIS/HCl buffer (0.1 M, pH ∼ 7.4) and Cs3[Tb(dpa)3] in TRIS/HCl buffer (ϕstd = 22%, A279 ≈ 0.18, 6.5 × 10−5 M)41 The excitation wavelength for the standards was 279 nm, while for the samples the excitation wavelength was 335 nm. The concentration of the samples was adjusted to have an absorption value A < 0.10. The quantum yield of the samples was determined by the dilution method using eqn (1), which accounts for the need to use of different excitation wavelengths of sample (x) and standard (std).

 
image file: d5dt02417j-t1.tif(1)

Grad is the slope of the plot of the integrated emission as a function of absorbance, n is the refractive index of the solvent, I is the intensity of the excitation source at the excitation wavelength and ϕ is the quantum yield.

The intrinsic quantum yield ϕLnLn was determined using eqn (2).42

 
image file: d5dt02417j-t2.tif(2)
ktot is the total emission rate (ktot = krad + knrad = 1/τexp), krad is the radiative rate constant, knrad is the non-radiative rate constant and τexp is the observed excited state lifetime. In the case of the Eu(III) complexes, krad can be determined using eqn (3).42–44
 
image file: d5dt02417j-t3.tif(3)

I tot and IMD are the total integrated emission spectrum and integrated intensity of the magnetic dipole-allowed 5D07F1 transition of the Eu(III) ion, respectively, and AMD,0 is the Einstein coefficient of spontaneous emission in vacuum (14.65 s−1).

Due to our inability to measure the absorption spectra of the f–f transitions for the Tb(III) complexes and thus determine τrad experimentally,42–44 its value was taken as 4 ms, as proposed by Klink et al.45

The sensitization efficiency (ηsens) was determined using eqn (4).42,43

 
image file: d5dt02417j-t4.tif(4)

Unless otherwise indicated, all data were collected at 25.0 ± 0.1 °C and are the average of at least three independent measurements.

Synthesis of compounds

Synthesis of [2,2′:6′,2″-terpyridine]-6-carbaldehyde (terpyCHO)46,47. Following a modified literature procedure, 6-bromo-2,2′-bipyridine (0.971 g, 4.13 mmol, 1.0 eq.),48 2-(1,3-dioxolan-2-yl)-6-(tributylstannyl)pyridine (1.99 g, 4.54 mmol, 1.1 eq.)49 and Pd(PPh3)4 (0.286 g, 0.25 mmol, 0.06 eq.) were stirred to reflux in dry toluene (30 ml) for 72 h. The solvent was removed under reduced pressure, 20 ml 4 M HCl was added, and the reaction mixture was stirred overnight at 60 °C. After cooling to room temperature, the mixture was neutralized with 2 M NaHCO3. The suspension was extracted with CHCl3 (3 × 30 ml), the organic phase separated, washed with water (3 × 30 ml), and brine (1 × 40 ml) and dried over magnesium sulphate. The isolated solid was purified by flash chromatography (ethylacetate[thin space (1/6-em)]:[thin space (1/6-em)]hexanes 1[thin space (1/6-em)]:[thin space (1/6-em)]2) to give the desired product in 12% yield (95 mg, 0.36 mmol).

1H-NMR (500 MHz, CDCl3) δ 7.32–7.26 (m, 1H), 7.81 (td, J = 7.7, 1.8 Hz, 1H), 8.01–7.91 (m, 3H), 8.45 (d, J = 7.8 Hz, 1H), 8.55 (d, J = 7.7 Hz, 2H), 8.66 (d, J = 4.8 Hz, 1H), 8.81 (d, J = 7.6 Hz, 1H), 10.13 (s, 1H) ppm (Fig. S1).

13C-NMR (126 MHz, CDCl3) δ 193.76, 156.78, 156.00, 155.61, 154.21, 152.34, 149.25, 138.10, 137.86, 136.89, 125.21, 123.91, 121.64, 121.44, 121.19, 121.13 ppm (Fig. S3).

ESI-MS (Fig. S12): terpyCHO. ESI-MS: [terpyCHO + H2O]; m/z: 279.101 (calc), 279.088 (exp).

Synthesis of 6-bromo-2,2′;6′,2′′-terpyridine (terpyBr)50. Following a modified literature procedure, to a solution of 2,6-dibromopyridine (2.0 g, 4.5 mmol) and Pd(PPh3)4 (0.26 g, 0.225 mmol) in dry toluene, 6-(tributylstannyl)-2,2′-bipyridine (1.006 g, 4.5 mmol) was added and the mixture was heated to reflux overnight. The reaction mixture was cooled, diluted with water, mixed with a concentrated aqueous solution of caesium fluoride (3.3 g, 22.2 mmol) and stirred for 30 min at room temperature. The mixture was filtered through a Celite pad and extracted with toluene (3 × 30 ml) and the combined organic layer was dried over magnesium sulfate, filtered and the solvent removed under reduced pressure. The product was obtained as an off-white solid in 10% yield (126 mg, 0.40 mmol) after flash column chromatography with hexane[thin space (1/6-em)]:[thin space (1/6-em)]ethylacetate (3[thin space (1/6-em)]:[thin space (1/6-em)]1) as the eluent.

1H-NMR (500 MHz, CDCl3): δ 8.71 (d, J = 5.2 Hz, 1H), 8.58 (d, J = 7.9 Hz, 2H), 8.49–8.43 (m, 2H), 7.96 (t, J = 7.7 Hz, 1H), 7.86 (td, J = 7.7, 1.8 Hz, 1H), 7.71 (t, J = 7.7 Hz, 1H), 7.51 (d, J = 7.8 Hz, 1H), 7.37–7.31 (m, 1H) ppm (Fig. S2).

13C-NMR (126 MHz, CDCl3): δ 157.44, 156.02, 155.47, 149.20, 141.58, 139.14, 138.01, 136.86, 128.00, 123.86, 121.58, 121.41, 121.12, 119.77 ppm (Fig. S4).

ESI-MS (Fig. S8): terpyBr. ESI-MS: [terpyBr] + m/z: 312.014 (calc), 312.012 (exp).

Synthesis of 6-nitro-2,2′;6′,2′′-terpyridine (terpyNO2)33. Following a literature procedure, 6-tributylstannyl-2,2′-bipyridine (1.0 g, 2.25 mmol) and 2-bromo-6-nitropyridine (0.50 g, 2.47 mmol) were mixed with 1 mol% Pd(PPh3)4 and LiCl (0.24 g, 5.6 mmol) and toluene were added. The mixture was heated to 110 °C overnight. The solvent was removed under reduced pressure and the reaction mixture purified by flash chromatography with hexane[thin space (1/6-em)]:[thin space (1/6-em)]ethylacetate (2[thin space (1/6-em)]:[thin space (1/6-em)]1) as eluent to afford a brown solid, which was washed with a small volume of acetonitrile to give the desired product as a white solid. Yield: 0.056 g (0.2 mmol, 9%).

1H-NMR (500 MHz, CDCl3): δ 7.34–7.30 (m, 1H), 7.86–7.82 (m, 1H), 7.97 (t, J = 7.8 Hz, 1H), 8.12 (t, J = 7.8 Hz, 1H), 8.20 (d, J = 7.8 Hz, 1H), 8.47 (d, J = 7.8 Hz, 1H), 8.53 (t, J = 7.8 Hz, 2H), 8.71–8.67 (m, 1H), 9.00–8.97 (m, 1H) ppm.

Synthesis of metal complexes

Equimolar solutions of terpyR (R = H, NO2, Br, CHO) and the Ln(NO3)3 (Ln = Eu, Tb, Dy, and Gd) were refluxed for 24 h in acetonitrile. Each solution was filtered, and the solvent removed under reduced pressure. The obtained solid was washed with chloroform and dried under reduced pressure to afford the corresponding metal complexes in 80–86% yield. No yield is indicated when the complexes were not isolated, and the solutions were used as is for spectroscopy.

Eu-terpy. ESI-MS (Fig. S5): [Eu(terpy)(NO3)2(CH3CN)]+; m/z: 509.991 (calc), 509.996 (exp).

Tb-terpy. ESI-MS (Fig. S6): [Tb(terpy)2(NO3)2]+; m/z: 749.092 (calc), 749.094 (exp).

Dy-terpy. ESI-MS (Fig. S7): [Dy(terpy)2(NO3)2]+; m/z: 754.091 (calc), 754.101 (exp).

Eu-terpyCHO. Yield: 82%. ESI-MS (Fig. S13): [Eu(terpyCHO)(NO3)2]+; m/z: 536.987 (calc), 536.973 (exp).

Tb-terpyCHO. Yield: 85%. ESI-MS (Fig. S14): [Tb(terpyCHO)(CH3CN)(NO3)2]+; m/z: 585.018 (calc), 584.995 (exp).

Dy-terpyCHO. Yield: 80%. ESI-MS (Fig. S15): [Dy(terpyCHO)(CH3CN)(NO3)2]+; m/z: 590.022 (calc), 590.012 (exp).

Eu-terpyNO 2 . ESI-MS (Fig. S16): [Eu(terpyNO2)2(NO3)2]+; m/z: 835.056 (calc), 835.061 (exp).

Tb-terpyNO 2 . ESI-MS (Fig. S17): [Tb(terpyNO2)(NO3)2]+; m/z: 560.981 (calc), 560.986 (exp).

Dy-terpyNO 2 . ESI-MS (Fig. S18): [Dy(terpyNO2)(NO3)2]+; m/z: 565.981 (calc), 565.982 (exp).

Eu-terpyBr. ESI-MS (Fig. S9): [Eu(terpyBr)(NO3)2(CH3CN)(H2O)]+; m/z: 646.938(calc), 647.055 (exp).

Tb-terpyBr. ESI-MS (Fig. S10): [Tb(terpyBr)2(NO3)3]+; m/z: 969.908 (calc), 969.902 (exp).

Dy-terpyBr. ESI-MS (Fig. S11): [Dy(terpyBr)(NO3)2]+; m/z: 598.907 (calc), 598.907 (exp).

Computational methods

Molecular geometries were optimized using the M06 functional.51 For Eu, effective core potentials and the corresponding basis set (Stuttgart RSC Segmented + ECP)52 were used, and the CC-PVTZ[thin space (1/6-em)]53 basis set was used for the rest of the atoms. The thermal contribution to the Gibbs free energy was computed using vibrational frequencies obtained from frequency calculations.

To compute the energies of the optimized structures, the M06 functional was used in combination with the relativistic DKH-def2-TZVPP54 basis set for non-metal atoms and SARC-DKH-TZVP for the Eu atom.54–56 The relativistic Hamiltonian DKH2 was utilized during the calculations.57 The solvent effect of the acetonitrile medium was modeled with the conductor-like polarizable continuum (CPCM) model in geometry optimizations and single point calculations.58 Solvent molecules were explicitly included in cases where their coordination was expected.

ChemAxon59 online program was used for the prediction of pKa values of the terpyR ligands. LUMPAC60–62 was used to obtain the experimental and theoretical Judd–Ofelt parameters and energy transfer rates for the Eu-based complexes. Quantum chemical calculations needed for the LUMPAC algorithm were performed with RM1-Sparkle59,60 and ZINDO/S levels of theory using MOPAC2016[thin space (1/6-em)]63 and ORCA,64 respectively. Judd–Ofelt parameters and energy transfer rates for the complexes were obtained with JOYSpectra.65

The distortion parameter δ of the central polyhedron from the ideal polyhedron in RM1-Sparkle-optimized Ln-complexes was calculated with the Polynator program.66 Complex stoichiometry in solution and corresponding stability constants were obtained from UV-VIS spectrophotometric titrations and estimated using the SupraFit software.67

Results and discussion

Complex formation and stability

Previous work by us33,47 and others68–78 showed that the terpyridine scaffold can bind Ln(III) ions and sensitize their luminescence. Moreover, its ease of functionalization provides opportunities to tune electronic and structural properties of the resulting metal complexes. In this work, we focused on three known terpy-based compounds with EWG groups, namely, 6 nitro-2,2′;6′,2′′-terpyridine (terpyNO2),33 6-bromo-2,2′;6′,2′′ terpyridine (terpyBr),50 and [2,2′:6′,2′′]-terpyridine-]-6-carbaldehyde (terpyCHO).46 terpyNO2 was studied by our group and showed its ability to function as a tetradentate ligand and as a sensitizer in Eu(III) and Tb(III) complexes.33,39 terpyCHO and terpyBr were intermediates in the synthesis of other terpy-based compounds, namely in the synthesis of oligopyridylimines49 and of a ruthenium complex with a terpy-substituted porphyrin,79 respectively. terpyBr was used to add the terpy moiety during the synthesis of polypyridyl-containing ligands80,81 The vibrational energy features of terpyCHO were explored via two-dimensional infrared spectroscopy.47 Despite a general interest in terpyridine-based ligands to sensitize Ln(III)-centred emission,82–84 neither terpyCHO nor terpyBr had been studied in this context. This could stem from the known lability of lanthanide complexes with the terpyridine ligand (vide infra).

Nine complexes (Fig. 1) were isolated with these three functionalized terpyridine-based ligands with the nitrate salts of Eu(III), Tb(III), and Dy(III) in acetonitrile. We also synthesized the known terpyridine (terpy) complexes85 of the same metal ions for comparison purposes. All complexes showed 1[thin space (1/6-em)]:[thin space (1/6-em)]1 stoichiometry (Fig. S19 and S30) with stability constants (Table 1) that decreased in the order terpy > terpyCHO > terpyBr > terpyNO2. While the stability constants of the Gd(III) complexes were not determined, they were prepared as well, to determine singlet and triplet state energies (vide infra).


image file: d5dt02417j-f1.tif
Fig. 1 Complexes studied here.
Table 1 Experimentally determined stability constants (log[thin space (1/6-em)]K) for the [Ln(terpyR)]3+ (R = H, NO2, CHO, Br; Ln(III) = Eu(III), Tb(III), Dy(III)) complexes in acetonitrile and ionic radii (rion)
Ln(III) r ion[thin space (1/6-em)]86 [Å] log[thin space (1/6-em)]K
terpy terpyNO2 terpyBr terpyCHO
Eu 1.120 8.1 ± 0.2, 7.9 (ref. 77) 5.2 ± 0.4 5.5 ± 0.1 6.6 ± 0.1
Tb 1.095 7.9 ± 0.4 5.4 ± 0.5 5.5 ± 0.2 6.4 ± 0.1
Dy 1.083 7.9 ± 0.3 5.2 ± 0.5 5.4 ± 0.1 6.8 ± 0.4


The log[thin space (1/6-em)]K values of the substituted terpyridines, in the range 5.24–6.84, are smaller than the ones obtained for terpy, despite the possibility of tetradentate coordination. For the latter, the obtained value log[thin space (1/6-em)]K of 8.1 is in line with the reported value of 7.9;77 the small difference is likely due to the different experimental conditions used, namely the 3[thin space (1/6-em)]:[thin space (1/6-em)]1 stoichiometry of the terpy complexes and our use of nitrate counter-ions, that are reported to successfully compete in acetonitrile for binding to the metal ion.26 We do not observe statistically significant differences between stabilities of complexes of the same ligand with different metal ions, consistent with the similar sizes of the ions. Of the three terpyR ligands, terpyCHO binds Ln(III) most strongly.

To unravel the observed trend in log[thin space (1/6-em)]K, we studied the protonation of the ligands and found that the protonation of the outer unsubstituted pyridine ring appears most favourable (Table 2). For terpy, the calculated value of 4.46 compares well with the reported value of 4.54.87 In the case of the substituted terpyridines, the calculated pKa1 of 4.17 indicates that the R-substituent has negligible influence on the electronics of this ring. The second protonation step is more complex; in the case of terpy, it occurs on the other outer pyridine ring and the calculated value of 3.85 agrees well with the reported value of 3.57.87 In the case of the bromo- and nitro-substituted ligands, the protonation occurs on the middle pyridine ring, with pKa2 values of 0.37 and 0.22, respectively. In the case of terpyCHO, the pKa2 of 1.67 corresponds to the protonation of the first, functionalized pyridine ring. We attribute this difference to the high electron-withdrawing effect of the Br- and NO2-groups, which decrease the basicity of the neighbouring ring, and absence of protonation of the substituted ring. Despite this discrepancy, pKa2 correlates well with log[thin space (1/6-em)]K (Fig. 2a). Similar arguments involving substituent electronegativity χ, following the scale developed by Dailey and Shoolery,88 indicate that χ decreases for NO2 > Br > CHO > H and tracks with log[thin space (1/6-em)]K (Fig. 2b).


image file: d5dt02417j-f2.tif
Fig. 2 Correlation of log[thin space (1/6-em)]K of the Ln(III) (Ln = Eu, Tb, Dy) complexes with (a) pKa2, and (b) electronegativity χ of the ligands. The connecting lines are visual aids.
Table 2 Protonation constants of the terpyR ligands, electronegativity (χ) of the R-groups
R= –H –NO2 –Br –CHO
a n.a. – calculation did not converge.
pKa1 4.46 (ring 3), 4.54 (ref. 87) 4.17 (ring 3) 4.17 (ring 3) 4.17 (ring 3)
pKa2 3.85 (ring 1), 3.57 (ref. 87) 0.22 (ring 2) 0.37 (ring 2) 1.67 (ring 1)
pKa3 n.a.a (ring 2) n.a.a (ring 1) n.a.a (ring 1) −1.70 (ring 2)
χ (ref. 88) 1.71 3.91 2.94 2.61


Photophysical characterization

All substituted terpyR sensitized the emission of Eu(III), Tb(III) and Dy(III). Absorption, emission, and excitation spectra of acetonitrile solutions of the Eu(III)-based complexes are shown in Fig. 3, those of the Tb(III)-based complexes are in Fig. S31–S34 and those of the Dy(III)-based complexes are in Fig. S35–S37. The analogous spectra at 77 K are shown in Fig. S38–S48. The absorption was most red-shifted for the complexes with terpyCHO and most blue-shifted for the complexes with terpyBr. As all complexes absorbed around 335 nm, the complexes were excited at this wavelength in all cases. The corresponding emission spectra display peaks at 588, 595, 617, 656, and 685 nm characteristic of the Eu(III)-centred 5D07FJ (J = 0, 1, 2, 3, 4) transitions, 490, 545, 583, 623 nm, 5D47FJ (J = 6, 5, 4, 3) for the Tb(III)-centred and 482, 575, 663 nm, 4F9/26HJ (J = 15/2, 13/2, 11/2) for the Dy(III)-centred transitions.
image file: d5dt02417j-f3.tif
Fig. 3 Absorption (a), excitation (b), and emission (c) spectra of Eu-terpyR complexes [R = H (green), NO2 (black), Br (blue), and CHO (red)] in acetonitrile at 298 K. λexc = 335 nm, λem = 617 nm, slit widths excitation = emission = 5 nm; scan rate = 250 nm min−1; gain = 650 V; [complexes] = 0.10 mM.

Table 3 summarizes the photophysical data for the Eu(III) and Tb(III) complexes. The 1S and 3T excited-state energies for terpy, determined in this work, were 27[thin space (1/6-em)]950 and 22[thin space (1/6-em)]200 cm−1, respectively, higher than the reported values of 26[thin space (1/6-em)]178 and 20[thin space (1/6-em)]041 cm−1.77 This difference is likely due to the slightly different complex used by the authors, namely 3[thin space (1/6-em)]:[thin space (1/6-em)]1 [La(terpy)3]ClO4,77 as well as slight differences in the deconvolution of the experimental spectra. For terpyNO2, terpyBr and terpyCHO 1S energies were 27[thin space (1/6-em)]900, 27[thin space (1/6-em)]330 and 28[thin space (1/6-em)]000 cm−1, respectively, and 3T energies were 22[thin space (1/6-em)]200, 22[thin space (1/6-em)]860, 21[thin space (1/6-em)]740, and 21[thin space (1/6-em)]880 cm−1, respectively. All 1S–3T gaps are larger than 5000 cm−1, which facilitates the intersystem crossing.90 The 3T states are higher in energy than the emissive states of both Eu(III) and Tb(III), consistent with their ability to sensitize the metal-centered emission. The sensitized emission efficiency ϕLLn of the Eu(III) complexes is highest for terpyBr and terpyCHO, which have 3T-f* gaps of 4510 and 4650 cm−1, respectively, and lowest for terpy and terpyNO2, which have the largest 3T-f* gaps, at 4970 and 5630 cm−1, respectively. For all Eu(III) complexes we observed that the sensitization efficiency ηsens correlates inversely with the energy of the triplet state (Fig. 4a).


image file: d5dt02417j-f4.tif
Fig. 4 Correlation between sensitization efficiency ηsens, the triplet state energy and the donor–acceptor distance RL(3T) for the (a) Eu(III) complexes and (b) Tb(III) complexes.
Table 3 Energies (E) of singlet (1S) and triplet (3T) states of the ligands, distance (RL) between acceptor (Ln(III)) and singlet (1S) or triplet (3T) states of the donor ligand, bandwidths (γ) of the peaks corresponding to 1S and 3T states of the ligands, emission lifetimes (τ) at 77 and 298 K, quantum yields of sensitized emission (ϕLLn), intrinsic quantum efficiency (ϕLnLn) and sensitization efficiency (ηsens) for the Ln-terpyR (Ln = Eu, Tb, R = H, NO2, CHO, Br) complexes
  terpy terpyNO2 terpyBr terpyCHO
a Indicated as the 0–0 transition after deconvolution of the fluorescence or phosphorescence spectra at 77 K (Fig. S57–S64).89 b Determined as the full width at half maximum of the 0–0 transition. c Calculated assuming τrad(Tb(III)) = 4 ms.45 d Calculations yielded an unrealistically high value of 124 ± 34, the more realistic lower limit value is presented in the table. Likely, this value is due to the assumed free ion τrad of 4 ms.
E(1S)a [cm−1] 27[thin space (1/6-em)]950 ± 130 (lit. 26[thin space (1/6-em)]178)77 27[thin space (1/6-em)]900 ± 50 27[thin space (1/6-em)]330 ± 200 28[thin space (1/6-em)]000 ± 120
E(3T)a [cm−1] 22[thin space (1/6-em)]200 ± 50 (lit. 20[thin space (1/6-em)]041)77 22[thin space (1/6-em)]860 ± 40 21[thin space (1/6-em)]740 ± 40 21[thin space (1/6-em)]880 ± 50
ΔES–T [cm−1] 5750 5040 5590 6120
ΔET-f*
 Eu 4970 5630 4510 4650
 Tb 1700 2360 1240 1380
R L(1S) [Å] 3.8071 3.8378 3.7071 3.8378
R L(3T) [Å] 4.0296 4.1221 3.9202 3.9694
ϕ LLn [%]
 Eu 9 ± 6 (lit. 1.3 (ref. 77)) 26 ± 4 29 ± 6 29 ± 5
 Tb 16 ± 6 (lit. 4.7 (ref. 77)) 2 ± 2 22 ± 6 16 ± 4
ϕ LnLn [%]
 Eu 15 ± 1 53 ± 2 41 ± 3 46 ± 2
 Tb 32.5 ± 0.3 20.3 ± 0.3 17.8 ± 0.3 29.3 ± 0.3
η sens [%]
 Eu 60 ± 40 49 ± 8 71 ± 16 63 ± 11
 Tbc 49 ± 18 10 ± 10 >90%d 55 ± 14
γ (1S)b [cm−1] 1120 490 1870 1560
γ (3T)b [cm−1] 770 400 890 750
τ [ms] (77 K)
 τ1 (population) Eu 0.30 ± 0.01 (70%) 0.40 ± 0.01 (61%) 0.75 ± 0.02 (44%) 0.25 ± 0.01 (69%)
 τ2 (population) 0.93 ± 0.01 (30%) 1.55 ± 0.01 (39%) 2.14 ± 0.02 (56%) 0.73 ± 0.01 (31%)
 τ1 (population) Tb 0.42 ± 0.06 (15%) 0.24 ± 0.01 (30%) 0.79 ± 0.02 (63%) 0.53 ± 0.01 (21%)
 τ2 (population) 1.14 ± 0.03 (85%) 1.13 ± 0.01 (70%) 2.04 ± 0.01 (37%) 1.23 ± 0.01 (79%)
τ av [ms] (77 K)
 Eu 0.49 ± 0.01 0.85 ± 0.01 1.53 ± 0.04 0.40 ± 0.01
 Tb 1.03 ± 0.03 0.86 ± 0.01 1.25 ± 0.02 1.08 ± 0.01
τ [ms] (298 K)
 Eu 0.92 ± 0.01 1.49 ± 0.01 1.66 ± 0.01 1.68 ± 0.01
 Tb 1.30 ± 0.01 0.81 ± 0.01 0.71 ± 0.01 1.17 ± 0.01
k rad [s−1]
 Eu 164.0 ± 9.2 358.0 ± 21.9 246.9 ± 5.3 272.6 ± 11.2
 Tbc 250.0 250.0 250.0 250.0
k nrad [s−1]
 Eu 923.0 ± 9.2 313.1 ± 21.9 355.5 ± 5.3 322.6 ± 11.2
 Tb 519.2 984.6 1158.5 604.7


Tb(III), with its 5D4 emissive level at 20[thin space (1/6-em)]500 cm−1, is most efficiently sensitized by terpyBr, for which the 3T-f* gap is 1240 cm−1. This is, surprisingly, the narrowest gap, and should yield a substantial degree of back-energy transfer.91 In fact, the narrow gaps observed for all systems should lead to substantial back-energy transfer for all except terpyNO2, which has a gap of 2360 cm−1 (vide infra). A similar inverse correlation between ηsens and the triplet energies is seen for the Tb(III) complexes (Fig. 4b).

While the 3T-f* gap91 is frequently cited as the main criterion for efficient Ln(III) emission, it has been demonstrated that RL, the distance between emissive state of the acceptor (Ln(III)) and the excited state of the donor (ligand) involved in the energy transfer to the Ln(III), also impacts the sensitization process.92,93 Assuming that the energy transfer occurs mostly through the triplet, an increase in RL(3T) is observed in the order terpyBr (3.9202 Å) < terpyCHO (3.9694 Å) < terpy (4.0296 Å) < terpyNO2 (4.1221 Å). If the singlet is considered, the RL(1S) are in the order terpyBr (3.7071 Å) < terpy (3.8071 Å) < terpyNO2 (3.8378 Å) = terpyCHO (3.8378 Å). These values show a good correlation of the triplet energy, with ηsens and RL(3T) for Eu(III) (Fig. 4a) and Tb(III) (Fig. 4b) complexes.

The room temperature emission lifetimes τ of the Eu(III) complexes (Table 3 and Fig. S49a–S56a), measured in acetonitrile, range from 0.92 to 1.68 ms; they could be fit to a single exponential, and are within the expected for this type of complexes. We attribute the longer lifetimes of the substituted ligands to increased steric hindrance around the metal ion. Overall, the lifetimes for the Tb(III) complexes (Table 3 and Fig. S49–S56(a)) are in the range 0.71–1.30 ms. They are shorter than those of the Eu(III) complexes, except in the case of the terpy-based complexes. We attribute this difference to the slight size decrease of Tb(III) with respect to Eu(III); the structure of the terpyNO2 complexes showed a slightly better fit of Eu(III) in the ligand cavity than Tb(III).33 The lifetimes of the terpy-based complexes, 0.92 ms and 1.30 ms for the Eu(III) and Tb(III) complexes, are shorter than the reported values of 2.31 ms and 1.20 ms,77 consistent with different ligand-to-metal ion stoichiometry of the complexes studied here (1[thin space (1/6-em)]:[thin space (1/6-em)]1), and by Mürner et al. (3[thin space (1/6-em)]:[thin space (1/6-em)]1).77 At 77 K the emission decay (Fig. S49–S56b) is best fit with a double exponential for both ions, which is consistent with two conformations of the Ln(III)-complexes, as is discussed below.

The radiative (krad) and non-radiative (knrad) rate constants are similar for all substituted Eu-terpyR complexes. In contrast, the corresponding rate constants for the terpy complex are approximately 2 times lower for krad and about 2.5–3 times higher for knrad. This indicates that adding an EWG to the terpyridine ortho-position, regardless of its nature, leads to a simultaneous increase in luminescence emission rates and a decrease in non-radiative luminescence quenching. In the case of the Tb-complexes, the non-radiative processes dominate, particularly in the case of the highly electronegative groups –NO2 and –Br.

Determination of the Judd–Ofelt parameters and energy transfer rates

To further unravel the complexity of the photophysical properties, we determined the experimental and theoretical Judd–Ofelt parameters Ω2, Ω4, and Ω6 (Table 4). We used, as starting geometries for all complexes, the known X-ray single crystal structures of Eu-terpyNO2 and Tb-terpyNO2.33 A good match between the calculated and experimental geometries (Fig. S65), and the calculated and experimental parameters Ω2 and Ω4 (Table 4) was obtained.
Table 4 Coordination polyhedra around the Eu(III) ion (yellow – Eu, red – O, blue – N, purple – Br), distortion of the experimental polyhedra (δ), and experimental and theoretical Judd–Ofelt parameters Ω2, Ω4, Ω6, for the Eu(III) and Tb(III) complexes of terpyR (R = H, NO2, Br, CHO)
Coordination number, polyhedron 9, monocapped square antiprism 10, bicapped square antiprism
Complex

image file: d5dt02417j-u1.tif

image file: d5dt02417j-u2.tif

image file: d5dt02417j-u3.tif

image file: d5dt02417j-u4.tif

δ 18.1 20.2 14.7 21.4
Eu-terpyR experimental parameters
Ω 2 [×10−20 cm2] 3.76 ± 0.25 8.57 ± 0.26 10.35 ± 0.50 12.83 ± 0.10
Ω 4 [×10−20 cm2] 4.29 ± 0.19 2.65 ± 0.07 1.56 ± 0.28 4.50 ± 0.241
Eu-terpyR theoretical (RM1 Sparkle) parameters
Ω 2 [×10−20 cm2] 3.76 8.57 10.36 12.83
Ω 4 [×10−20 cm2] 4.29 2.65 2.14 3.30
Ω 6 [×10−20 cm2] 2.22 0.98 0.46 2.25
Tb-terpyR theoretical (RM1 Sparkle) parameters
Ω 2 [×10−20 cm2] 4.61 9.10 10.16 6.75
Ω 4 [×10−20 cm2] 7.89 5.07 2.84 7.02
Ω 6 [×10−20 cm2] 3.31 1.59 0.58 2.42


These spectral intensity parameters reflect numerous crystal field effects between the Ln(III) ion and its ligand environment; Ω2 is very sensitive to distortions of the coordination sphere symmetry and changes in covalency of the Ln-ligand bonds, while Ω4 and Ω6 are more affected by bulk properties such as viscosity and rigidity.5,94 For Eu(III) complexes, Ω2 is strongly related to the hypersensitive 5D07F2 emission peak.94 The observed differences in Ω2 correlate with the distortion parameter δ from the ideal polyhedron; the larger δ for a coordination polyhedron with the same coordination number, the larger the value of Ω2. Lower values of Ω4 and Ω6 correspond to higher molecular rigidity. Based on this, the Eu(III) complexes with terpyBr and terpyCHO should have the longest emission lifetimes, which is observed experimentally.

The calculated forward W and back-energy Wb transfer rates involve transitions from the singlet (1S → Ln (WS)) (Fig. 5a) and triplet (3T → Ln (WT)) (Fig. 5b) states to the Ln(III) excited states and from those back to the ligand singlet (Ln → S (WSb)) and triplet (Ln → 3T (WTb)) states; their calculated numerical values, along with the Ln(III) energy levels participating in the transitions, are summarized in Tables S1–S2. WS and corresponding WSb are higher in the case of Tb(III) complexes. Oppositely, WT of Tb-complexes are considerably lower comparing to the Eu-terpyR, except Eu-terpyNO2, for which WT value is also very low. Thus, WTb are higher than WT for all Tb-terpyR, whereas in the case of Eu-terpyR, WT are higher than WTb.


image file: d5dt02417j-f5.tif
Fig. 5 Forward (W) and back energy transfer rates (Wb) related to 1S–Ln (S) (a) and 3T–Ln (T) transitions; (a) for Eu(III) complexes and (b) for Tb(III) complexes.

Predominance of back-transfer processes in Tb(III) complexes correlates with the expectation that an efficient ligand-to-metal energy transfer with negligible back energy transfer is expected if the ligand's triplet state is >1850 cm−1 higher than the Tb(III) 5D4 level (20[thin space (1/6-em)]500 cm−1).91 This explains the higher values for Tb-terpyR WTb than WT as the ligands’ triplets energies lie in the range 21[thin space (1/6-em)]740–22[thin space (1/6-em)]860 cm−1, close to the 5D4 level. For Eu(III), experimental data indicates that ligands with a minimum triplet state energy of 19[thin space (1/6-em)]800 cm−1 should easily transfer energy to the metal.95–97

Despite significant WTb, the sensitization of Tb still takes place, as evidenced by relatively large values of sensitization efficiency ηsens (Table 3). This includes an overestimated ηsens for Tb-terpyBr, likely caused by simplifying the estimate of this value with the assumption that τrad = 4 ms. Overall, the determined ηsens values correlate with the total rate of forward energy transfer WS+T values, as shown in Fig. 6. An increase in total rate of energy transfer from ligand to Ln(III) increases ηsens (Fig. 6a and d). Conversely, WS+T decreases with an increase in 3T and RL(3T) (Fig. 6b, c, e and f).65 Moreover, as WS+T depends on 1/RL[thin space (1/6-em)]4 and 1/RL,6 a modest increase of acceptor-donor distance leads to an increase in total WS+T of almost two orders of magnitude from 7.9 × 106 to 3.7 × 108 s−1.


image file: d5dt02417j-f6.tif
Fig. 6 Correlation between energy transfer rates and different parameters. Correlations related to the Eu(terpyR) complexes, between the logarithm of total forward transfer rates and sensitization efficiency (a), ligand triplet energy (b), donor–acceptor distance (c). Correlations related to the Tb(terpyR) complexes, between the logarithm of total forward transfer rates and sensitization efficiency (d), ligand triplet energy (e), and donor–acceptor distance (f).

A Jabłoński diagram for the Eu-terpyBr complex (Fig. 7), which exhibits the highest efficiency of sensitized emission ϕLLn = 29% (Table 3), summarizes that the rates of forward energy transfer are higher than those of back energy transfer. Jabłoński diagrams for the other Eu complexes are presented in the SI (Fig. S66–S68). A similar predominance of forward energy transfer is seen for the complexes Eu(terpyNO2), and Eu(terpyCHO), which have efficiencies of sensitized emission close to 30%. The efficiency is smaller for Eu(terpy) (9%); while for this complex the forward rates are also higher, knrad is significantly larger than krad and thus also has the lowest intrinsic emission efficiency ϕLnLn of 15%, while for the other Eu complexes this value is close to 50%, indicating a better vibrational shielding of the emissive state with the tetradentate ligands.


image file: d5dt02417j-f7.tif
Fig. 7 Jabłoński diagram for Eu(terpyBr) (a) and Tb(terpyBr) (b)with energy transfer (red dashed lines and numbers) and back transfer (blue dashed lines and numbers) rates.

Tb(terpyBr) also displays the largest efficiency of sensitized emission ϕLLn = 22% (Table 3) and its Jabłoński diagram is shown in Fig. 7b. The analogous diagrams for the remaining Tb complexes are shown in Fig. S69–S71. For all four complexes, uniformly the rates of back-energy transfer to the 3T state are higher than the forward energy transfer, consistent with the small 3T-f* gap (Table 3). Moreover, large values of knrad lead to low values of ϕLLn for these complexes. The diagrams in Fig. 6 demonstrate that the triplet energy of the studied ligands decreases in the order NO2 > CHO > Br. This trend inversely correlates with the forward energy transfer rates, which in turn directly correlate with the sensitization efficiency. Consequently, among the substituents considered, the sensitization efficiency of terpy ligands for Eu(III) and Tb(III) increases in the order NO2 < H ≈ CHO < Br. However, this trend is not apparent from other properties, such as the complex stability constants (Table 1) or the distortions of the metal coordination sphere (Table 4). These observations highlight the importance of continuing the search for suitable synthetic modifications to design efficient Ln(III) sensitizers, as not only the energies of the singlet and triplet states influence energy transfer and sensitization efficiency, but also the donor–acceptor distances RL and, as discussed below, the coordination environment around the Ln(III) ion.

Species leading to double-exponential emission lifetimes

While at room temperature the emission lifetimes fit a single exponential, at 77 K the emission lifetimes of all complexes could be fit with a double exponential. Chapman and co-workers98 reported two conformations for terpy complexes of Ln(III), consistent with decomplexation and the rotation of one of the outside pyridine rings. These authors observed the coordination of terpyridine to Eu(III) in acetonitrile as a tridentate ligand in a ciscis–cis conformation, and as a bidentate ligand with a ciscistrans conformation, with an acetonitrile molecule completing the coordination sphere. To assess the presence here of two species we calculated representatively, via a higher level of theory (relativistic Hamiltonian DKH2DFT), the isomerization for the Eu(terpyNO2) complexes via the partial decomplexation of one of the pyridine rings followed by rotation of the pyridine ring away from the metal ion (Fig. 8a), either the unsubstituted ring, or the one containing the NO2 group. From geometry optimization, we found that an acetonitrile solvent molecule coordinates to the Eu(III) ion.
image file: d5dt02417j-f8.tif
Fig. 8 (a) Three structures considered for the Eu(terpyNO2) complex representing isomerization via decomplexation. (b) The free energy surface for the de-coordination of the pyridine nitrogen in the Eu(terpyNO2)(NO3)3 complex. The structure on the left, right and middle are the geometries of the bound complex, unbound complex and the transition state structure respectively.

Multiple coordination modes for the coordinated acetonitrile molecule were considered for the structure of the Eu(terpyNO2) complex in the partially coordinated conformations, as there are multiple binding sites for the acetonitrile. The partially complexed isomer with the lowest computed relative free energy is 4.2 kcal mol−1 higher in energy than the completely coordinated complex. In this conformation, the NO2-containing pyridine ring rotates, followed by a re-arrangement of the nitrate and acetonitrile molecules. Additionally, three other partially uncoordinated conformers with free energies at 5.9, 6.2, and 6.5 kcal mol−1 were found. Assuming the activation free energy of rotation for these different coordination modes are similar, the presence of multiple different coordination mode shifts the equilibrium further towards the uncomplexed systems.

The activation free energy for the rotation of the pyridine ring was found to be 7.6 kcal mol−1 (Fig. 8b). Using the Arrhenius equation, and assuming a pre-exponential factor in the order of kBT/h, the rate constants of forward and backward reactions at 77 K are in the order of 10−9 s−1 and 103 s−1, respectively. This is in contrast with the much higher rates of 107 s−1 and 1010 s−1 for the forward and backward reactions at 300 K. This indicates that the interconversion between the fully coordinated complex and the partially uncoordinated complex isomers is orders of magnitude faster at 300 K than 77 K, which enables the presence of the two species at the lower temperature and is consistent with the double exponential decay.

Further experimental evidence for these two species was procured by 1H-NMR spectroscopy. Comparison of spectra of Eu(terpy)(NO3)3 and Eu(terpyNO2)(NO3)3 at room temperature (Fig. 9I and 9II), respectively) and at −30 °C (Fig. 9VII and 9VIII, respectively) show a splitting of peaks at the lower temperature, consistent with the formation of different structures. A noticeable downfield shift of the signal of the meta-hydrogen in the pyridine ring (denoted as Hd) was observed upon cooling. In the case of Eu(terpy)(NO3)3 the downfield shift of Hd is not easily observable due to overlapping signals. The signals corresponding to the Hd protons (8.67 ppm, ddt, J = 7.99, 1.16, 1.16 Hz) and the Ha protons (8.72 ppm, ddd, J = 4.83, 1.86, 0.98 Hz) are easily distinguishable (Fig. 9III). Lowering the temperature causes the appearance of additional peaks in between these two, resulting in a multiplet at 8.69 ppm (Fig. 9V).


image file: d5dt02417j-f9.tif
Fig. 9 1H-NMR spectra of Eu(terpy)(NO3)3 at (II) +24 °C and (IV) −30 °C and Eu(terpyNO2)(NO3)3 at (VI) +24 °C and (VIII) −30 °C. Corresponding structural formulas (I, III, V, VII) are presented for clarity.

For this complex, Ha (8.71 ppm, d, J = 4.79 Hz) and Hd (m, 8.66 ppm) can be easily distinguished at room temperature (Fig. 9IV); however, they overlap at −30 °C (Fig. 9VI). The shifts of other peaks are less prominent, consistent with the assumption that the distance between Hd and Eu(III) shortens upon rotation of the pyridine ring at lower temperature.

Conclusions

In this paper, we synthesized terpyridine ligands with different electron-withdrawing functional groups to study how the nature of these groups influences the formation of Eu and Tb complexes and the efficiency of sensitized emission in these complexes. We found that the higher stability constants of the complexes are obtained for the ligands with the highest pKa2, the second protonation constant of the terpyridine-based ligands. All complexes display Ln(III)-centred emission. Especially in the case of Eu(III), we found that the more distorted the structure of the polyhedron around the metal ion, the largest the Ω2 Judd–Ofelt parameter, and such distortions were largest for the terpyBr and terpyCHO complexes; these also display the largest efficiency of sensitized emission for Eu(III). Lifetime measurements indicated the formation of two species at 77 K, which were explained, through DFT calculation and supported by 1H-NMR measurements, by the formation of partially decomplexed structures, as had been previously observed for other terpy-based lanthanide complexes. Overall, these findings provide valuable design principles for designing terpyridine-based ligands to optimize the luminescence properties of lanthanide complexes. Ultimately, they highlight the complexity of tailoring ligand properties for sensitization of Ln(III)-centred emission; in addition to the energies of singlet and triplet states, coordination environment and donor–acceptor distances also play an important role.

Author contributions

Oksana Fizer: spectroscopic measurements, methodology writing – original draft. Sina Chiniforoush: computations, writing – original draft. Thomas J. Summers: computations. Mohammad Zafar Abbas: synthesis, writing – original draft. David C. Cantu: conceptualization, methodology, supervision. Ana de Bettencourt-Dias: conceptualization, methodology, writing – original draft & editing, supervision.

Conflicts of interest

There are no conflicts to declare.

Data availability

The data supporting this article have been included as part of the supplementary information (SI). Supplementary information: NMR and mass spectra, spectrophotometric titrations, absorption, excitation and emission spectra, emission decay curves, calculated energy transfer rates and calculated geometries. See DOI: https://doi.org/10.1039/d5dt02417j.

Acknowledgements

This work was financially supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Created by the Competitive Research Incentive Program under grant number DE-SC0022178.

References

  1. Luminescence of Lanthanide Ions in Coordination Compounds and Nanomaterials, ed. A. de Bettencourt-Dias, John Wiley and Sons, Hoboken, 2014 Search PubMed.
  2. C. M. Granadeiro, D. Julião, S. O. Ribeiro, L. Cunha-Silva and S. S. Balula, Coord. Chem. Rev., 2023, 476, 214914 CrossRef.
  3. S. Zhang, W. Yin, Z. Yang, Y. Yang, Z. Li, S. Zhang, B. Zhang, F. Dong, J. Lv, B. Han, Z. Lei and H. Ma, ACS Appl. Mater. Interfaces, 2021, 13(4), 5539–5550 CrossRef PubMed.
  4. C. Chen, Y. Zhuang, X. Li, F. Lin, D. Peng, D. Tu, A. Xie and R. J. Xie, Adv. Funct. Mater., 2021, 31(25), 2101567 CrossRef.
  5. V. X. Quang, P. Van Do, N. X. Ca, L. D. Thanh, V. P. Tuyen, P. M. Tan, V. X. Hoa and N. T. Hien, J. Lumin., 2020, 221, 117039 CrossRef.
  6. V. V. Utochnikova, A. N. Aslandukov, A. A. Vashchenko, A. S. Goloveshkin, A. A. Alexandrov, R. Grzibovskis and J.-C. G. Bünzli, Dalton Trans., 2021, 5(37), 1286–12813 Search PubMed.
  7. K. Nehra, A. Dalal, A. Hooda, S. Bhagwan, R. K. Saini, B. Mari, S. Kumar and D. Singh, J. Mol. Struct., 2022, 1249, 131531 CrossRef.
  8. A. Barkanov, A. Zakharova, T. Vlasova, E. Barkanova, A. Khomyakov, I. Avetissov, I. Taydakov, N. Datskevich, V. Goncharenko and R. Avetisov, J. Mater. Sci., 2022, 57(18), 8393–8405 CrossRef.
  9. F. Zinna, M. Pasini, F. Galeotti, C. Botta, L. Di Bari and U. Giovanella, Adv. Funct. Mater., 2017, 27(1), 1603719 CrossRef.
  10. A. de Bettencourt-Dias, Dalton Trans., 2007, 22, 2229–2241 RSC.
  11. X. Qiu, J. Xu, M. Cardoso Dos Santos and N. Hildebrandt, Acc. Chem. Res., 2022, 55(4), 551–564 CrossRef PubMed.
  12. L. Yu, Z. Gao, Q. Xu, X. Pan and Y. Xiao, Biosens. Bioelectron., 2022, 210, 114320–114320 CrossRef PubMed.
  13. J. Wang, T. Sheng, X. Zhu, Q. Li, Y. Wu, J. Zhang, J. Liu and Y. Zhang, Mater. Chem. Front., 2021, 5(4), 1743–1177 RSC.
  14. Y. Li, C. Chen, F. Liu and J. Liu, Mikrochim. Acta, 2022, 189(3), 109–109 CrossRef PubMed.
  15. H. Pham and L. W. Miller, in Methods in Enzymology, Academic Press, 2021, ch. 9 Search PubMed.
  16. H. Min, S. Wu, Z. Han, Z. Chen, T. Sun, W. Shi and P. Cheng, Chem. – Eur. J., 2021, 27(69), 17459–17464 CrossRef PubMed.
  17. Y.-C. Chen and M.-L. Tong, Chem. Sci., 2022, 13(3), 8716–8726 RSC.
  18. R. Marin, G. Brunet and M. Murugesu, Angew. Chem., Int. Ed., 2021, 60(4), 1728–1746 CrossRef CAS PubMed.
  19. Z. Zhu and J. Tang, Natl. Sci. Rev., 2022, 9(12), nwac194 CrossRef PubMed.
  20. Tamanna and V. Mutreja, Mater. Today: Proc., 2022, 2214–7853 Search PubMed.
  21. M. Patyal, K. Kaur, N. Bala, N. Gupta and A. K. Malik, J. Trace Elem. Med. Biol., 2023, 80, 127277–127277 CrossRef CAS.
  22. J. H. S. K. Monteiro, A. de Bettencourt-Dias, I. O. Mazali and F. A. Sigoli, New J. Chem., 2015, 39(3), 1883–1891 RSC.
  23. A. de Bettencourt-Dias and J. S. K. Rossini, Inorg. Chem., 2016, 55, 9954–9963 CrossRef CAS.
  24. A. K. Duncan, C. N. McBride, T. G. R. Benjamin, M. P. Madsen, K. T. Bowers, A. de Bettencourt-Dias and E. J. Werner, Polyhedron, 2016, 114, 451–458 CrossRef CAS.
  25. A. de Bettencourt-Dias, J. S. K. Rossini and J. A. Sobrinho, Dalton Trans., 2020, 49, 17699–17708 RSC.
  26. J. H. S. K. Monteiro, N. R. Fetto, M. J. Tucker and A. de Bettencourt-Dias, Inorg. Chem., 2020, 59, 3193–3199 CrossRef CAS.
  27. P. S. Barber, A. de Bettencourt-Dias, K. R. Johnson and J. H. S. K. Monteiro, Ligand design in lanthanide complexes for luminescence, therapy, and sensing, in Handbook on the Physics and Chemistry of Rare Earths, ed. J.-C. G. Bünzli and S. Kauzlarich, Elsevier, 2024, vol. 65 Search PubMed.
  28. K.-X. Yu, J. G. C. Kragskow, Y.-S. Ding, Y.-Q. Zhai, D. Reta, N. F. Chilton and Y.-Z. Zheng, Chem, 2020, 6(7), 1777–1793 CAS.
  29. S. C. Corner, G. K. Gransbury, I. I. J. Vitorica-Yrezabal, G. F. S. Whitehead, N. F. Chilton and D. P. Mills, Inorg. Chem., 2024, 63(21), 9552–9561 CrossRef CAS.
  30. S. C. Corner, G. K. Gransbury, I. I. J. Vitorica-Yrezabal, G. F. S. Whitehead, N. F. Chilton and D. P. Mills, Inorg. Chem., 2024, 63(21), 9562–9571 CrossRef CAS PubMed.
  31. A. Ullah, J. S. Cerdá, J. J. Baldoví, S. A. Varganov, J. Aragó and A. Gaita-Ariño, In Silico, J. Phys. Chem. Lett., 2019, 10(24), 7678–7683 CrossRef CAS.
  32. J. Romanova, R. Lyapchev, M. Kolarski, M. Tsvetkov, D. Elenkova, B. Morgenstern and J. Zaharieva, Molecules, 2023, 28(10), 4113 CrossRef CAS PubMed.
  33. A. de Bettencourt-Dias, S. Bauer, S. Viswanathan, B. C. Maull and A. M. Ako, Dalton Trans., 2012, 41, 11212–11218 RSC.
  34. Y. Bretonnière, M. Mazzanti, J. Pécaut and M. M. Olmstead, J. Am. Chem. Soc., 2002, 124(31), 9012–9013 CrossRef.
  35. X.-Y. Chen, Y. Bretonnière, J. Pécaut, D. Imbert, J.-C. Bünzli and M. Mazzanti, Inorg. Chem., 2007, 46(3), 625–637 CrossRef CAS PubMed.
  36. Y. Sakai, S. Mizuta, A. Kumagai, M. S. O. Tagod, H. Senju, T. Nakamura, C. T. Morita and Y. Tanaka, Cells, ChemMedChem, 2017, 12(23), 2006–2013 CrossRef CAS.
  37. P. J. Vallett and N. H. Damrauer, J. Phys. Chem., 2011, 115(14), 3122–3132 CrossRef CAS.
  38. A. de Bettencourt-Dias, S. Bauer, S. Viswanathan, B. C. Maull and A. M. Ako, Dalton Trans., 2012, 41(36), 11212–11218 RSC.
  39. T. J. Summers, J. A. Sobrinho, A. de Bettencourt-Dias, S. D. Kelly, J. L. Fulton and D. C. Cantu, Inorg. Chem., 2023, 62(13), 5207–5218 CrossRef CAS PubMed.
  40. J. A. Mattocks, J. L. Tirsch and J. A. Cotruvo Jr, Methods Enzymol., 2021, 651, 23–61 CAS.
  41. A.-S. Chauvin, F. Gumy, D. Imbert and J.-C. G. Bünzli, Spectrosc. Lett., 2004, 37(5), 517–532 CrossRef CAS.
  42. S. I. Klink, G. A. Hebbink, L. Grave, P. G. B. Alink, F. C. J. M. van Veggel and M. H. V. Werts, J. Phys. Chem. A, 2002, 106(15), 3681–3689 CrossRef CAS.
  43. A. Aebischer, F. Gumy, J. C. G. Bünzli, A. Aebischer and F. Gumy, Phys. Chem. Chem. Phys., 2009, 11(9), 1346–1353 RSC.
  44. M. H. V. Werts, R. T. F. Jukes and J. W. Verhoeven, Phys. Chem. Chem. Phys., 2002, 4, 1542–1548 RSC.
  45. S. I. Klink, L. Grave, D. N. Reinhoudt, F. C. J. M. van Veggel, M. H. V. Werts, F. A. J. Geurts and J. W. Hofstraat, J. Phys. Chem. A, 2000, 104(23), 5457–5468 CrossRef CAS.
  46. Y. D. M. Champouret, R. K. Chaggar, I. Dadhiwala, J. Fawcett and G. A. Solan, Tetrahedron, 2006, 62, 79–89 CrossRef CAS.
  47. C. J. Mallon, M. Hassani, M. Fizer, S. A. Varganov, A. de Bettencourt-Dias and M. J. Tucker, Phys. Chem. A, 2025, 129(20), 4374–4383 CrossRef CAS.
  48. Y. Toya, K. Hayasaka and H. Nakazawa, Organometallics, 2017, 36(9), 1727–1735 CrossRef CAS.
  49. Y. D. M. Champouret, R. K. Chaggar, I. Dadhiwala, J. Fawcett and G. A. Solan, Tetrahedron, 2006, 62(1), 79–89 CrossRef CAS.
  50. O. Kuleshova, S. Asako and L. Ilies, ACS Catal., 2021, 11(10), 5968–5973 CrossRef CAS.
  51. Y. Zhao and D. G. Truhlar, Theor. Chem. Acc., 2008, 119(5–6), 525–525 Search PubMed.
  52. X. Cao and M. Dolg, J. Mol. Struct., 2002, 581(1), 139–147 CrossRef CAS.
  53. T. H. Dunning, J. Chem. Phys., 1989, 90(2), 1007–1023 CrossRef CAS.
  54. D. Aravena, F. Neese and D. A. Pantazis, J. Chem. Theory Comput., 2016, 12(3), 1148–1156 CrossRef CAS PubMed.
  55. A. Z. de Oliveira, I. B. Ferreira, C. T. Campos, F. E. Jorge and P. A. Fantin, Mol. Model., 2019, 25(2), 38–39 CrossRef CAS.
  56. F. E. Jorge, L. S. C. Martins and M. L. Franco, Chem. Phys. Lett., 2016, 643, 84–88 CrossRef CAS.
  57. M. Reiher, WIREs: Comput Mol Sci, 2012, 2(1), 139–149 CAS.
  58. M. Cossi, N. Rega, G. Scalmani and V. Barone, J. Comput. Chem., 2003, 24(6), 669–681 CrossRef CAS.
  59. K. Mansouri, N. F. Cariello, A. Korotcov, V. Tkachenko, C. M. Grulke, C. S. Sprankle, D. Allen, W. M. Casey, N. C. Kleinstreuer and A. J. Williams, J. Cheminf., 2019, 11(1), 60–20 Search PubMed.
  60. J. D. L. Dutra, T. D. Bispo and R. O. Freire, J. Comput. Chem., 2014, 35(10), 772–775 CrossRef CAS.
  61. M. A. M. Filho, J. D. L. Dutra, G. B. Rocha, R. O. Freire and A. M. Simas, RSC Adv., 2013, 3(37), 16747–16755 RSC.
  62. A. B. Ganaie and K. Iftikhar, ACS Omega, 2021, 6(33), 21207–21226 CrossRef CAS PubMed.
  63. J. J. P. Stewart, Stewart Computational Chemistry, Colorado Springs, CO, USA, 2016. https://openmopac.net/ Search PubMed.
  64. F. Neese, Software update: The ORCA program system—Version 5.0, Wiley Interdiscip. Rev.:Comput. Mol. Sci., 2022, 12(5), e1606 Search PubMed.
  65. R. T. Moura Jr, A. N. Carneiro Neto, E. C. Aguiar, C. V. Santos-Jr, E. M. de Lima, W. M. Faustino, E. E. S. Teotonio, H. F. Brito, M. C. F. C. Felinto, R. A. S. Ferreira, L. D. Carlos, R. L. Longo and O. L. Malta, Opt. Mater.:X, 2021, 11, 100080 CAS.
  66. L. Link and R. Niewa, J. Appl. Crystallogr., 2023, 56(6), 1855–1864 CrossRef CAS.
  67. C. Hübler, Chem.:Methods, 2022, 2(7), e202200006 Search PubMed.
  68. I. Hemmila, V. M. Mukkala, M. Latva and P. Kiilholma, J. Biochem. Biophys. Methods, 1993, 26(4), 283–290 CrossRef CAS PubMed.
  69. M. Latva, H. Takalo, V.-M. Mukkala and J. Kankare, Inorg. Chim. Acta, 1998, 267(1), 63–72 CrossRef CAS.
  70. G. Muller, J.-C. G. Bünzli, J. P. Riehl, D. Suhr, A. von Zelewsky and H. Muerner, Chem. Commun., 2002, 14, 1522–1523 RSC.
  71. Y. Bretonniere, M. Mazzanti, J. Pecaut and M. M. Olmstead, J. Am. Chem. Soc., 2002, 124(31), 9012–9013 CrossRef CAS.
  72. L. J. Charbonnière, S. Mameri, D. Flot, F. Waltz, C. Zandanel and R. F. Ziessel, Dalton Trans., 2007, 22, 2245–2253 RSC.
  73. X. Y. Chen, Y. Bretonnière, J. Pecaut, D. Imbert, J. C. G. Bünzli and M. Mazzanti, Inorg. Chem., 2007, 46(3), 625–637 CrossRef CAS PubMed.
  74. S. A. Cotton, O. E. Noy, F. Liesener and P. R. Raithby, Inorg. Chim. Acta, 2003, 344, 37–42 CrossRef.
  75. A. Escande, L. Guénée, K.-L. Buchwalder and C. Piguet, Inorg. Chem., 2009, 48(3), 1132–1147 CrossRef PubMed.
  76. C. Mallet, R. P. Thummel and C. Hery, Inorg. Chim. Acta, 1993, 210, 223–231 CrossRef.
  77. H.-R. Mürner, E. Chassat, R. P. Thummel and J.-C. G. Bünzli, Dalton Trans., 2000, 2809–2816 RSC.
  78. B. Song, G. Wang, M. Tan and J. Yuan, J. Am. Chem. Soc., 2006, 128(41), 13442–13450 CrossRef PubMed.
  79. K. Mizuno, M. Kurihara, S. Takagi and H. Nishihara, Chem. Lett., 2003, 32(9), 788–789 CrossRef.
  80. M. Ichikawa, T. Yamamoto, H.-G. Jeon, K. Kase, S. Hayashi, M. Nagaoka and N. Yokoyama, J. Mater. Chem., 2012, 22(14), 6765–6773 RSC.
  81. A. R. Stefankiewicz, M. Wałęsa-Chorab, J. Harrowfield, M. Kubicki, Z. Hnatejko, M. Korabik and V. Patroniak, Dalton Trans., 2013, 42(5), 1743–1751 RSC.
  82. Q.-R. Wu, J.-J. Wang, H.-M. Hu, Y.-Q. Shangguan, F. Fu, M.-L. Yang, F.-X. Dong and G.-L. Xue, Inorg. Chem. Commun., 2011, 14(3), 484–488 CrossRef.
  83. J. K. Molloy, Z. Pillai, J. Sakamoto, P. Ceroni and G. Bergamini, Asian J. Org. Chem., 2015, 4(3), 251–255 CrossRef.
  84. X. Yu, Y. Hu, C. Guo, Z. Chen, H. Wang and X. Li, Supramol. Mater., 2022, 1, 100017 Search PubMed.
  85. D. A. Durham, G. H. Frost and F. A. Hart, J. Inorg. Nucl. Chem., 1969, 31(3), 833–838 CrossRef.
  86. R. D. Shannon, Acta Crystallogr., Sect. A, 1976, 32, 751–767 CrossRef.
  87. E. Farkas, É.A Enyedy, G. Micera and E. Garribba, Polyhedron, 2000, 19(14), 1727–1736 CrossRef.
  88. B. P. Dailey and J. N. Shoolery, J. Am. Chem. Soc., 1955, 77(15), 3977–3981 CrossRef.
  89. G. A. Crosby, R. E. Whan and R. M. Alire, J. Chem. Phys., 1961, 34(3), 743–748 CrossRef.
  90. F. J. Steemers, W. Verboom, D. N. Reinhoudt, E. B. van der Tol and J. W. Verhoeven, J. Am. Chem. Soc., 1995, 117(37), 9408–9414 CrossRef CAS.
  91. M. Latva, H. Takalo, V.-M. Mukkala, C. Matachescu, J. C. Rodriguez-Ubis and J. Kankare, J. Lumin., 1997, 75, 149–169 CrossRef CAS.
  92. J. H. Monteiro, A. de Bettencourt-Dias and F. A. Sigoli, Inorg. Chem., 2017, 56(2), 709–712 CrossRef CAS.
  93. A. N. Carneiro Neto, L. S. D. Carlos, O. L. Malta, M. Sanadar, A. Melchior, E. Kraka, S. Ruggieri, M. Bettinelli and F. Piccinelli, Inorg. Chem., 2022, 61(41), 16333–16346 CrossRef CAS PubMed.
  94. C. K. Jørgensen and R. Reisfeld, J. Less-Common Met., 1983, 93(1), 107–112 CrossRef.
  95. X. Zhai, P. Feng, N. Song, G. Zhao, Q. Liu, L. Liu, M. Tang and Y. Tang, Inorg. Chem. Front., 2022, 9(7), 146–1415 RSC.
  96. X. Mi, D. Sheng, Y. E. Yu, Y. Wang, L. Zhao, J. Lu, Y. Li, D. Li, J. Dou, J. Duan and S. Wang, ACS Appl. Mater. Interfaces, 2019, 11(8), 7914–7926 CrossRef CAS PubMed.
  97. C. H. Hossack, R. J. Butcher, C. L. Cahill and C. Besson, Inorg. Chem., 2021, 60(20), 15724–15743 CrossRef CAS PubMed.
  98. R. D. Chapman, R. T. Loda, J. P. Riehl and R. W. Schwartz, Inorg. Chem., 1984, 23, 1652–1657 CrossRef CAS.

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