During the development of phosphors with metal-centered emission from electric dipole forbidden transitions, including f-f transitions and d-d transitions, many phosphors with co-doped sensitizer and activator ions have been designed to pursue a higher color rendering index in lighting and a larger color gamut in display [1-4]. Trivalent cerium ion (CeⅢ) is a typical sensitizer ion with absorption bands from spin- and parity-allowed f-d transition, and has been widely applied in phosphors containing divalent manganese ion (MnⅡ) to enhance the MnⅡ-center emission from spin- and parity-forbidden d-d transition through energy transfer (ET) (Scheme 1a) [5-11]. Since effective ET is crucial to achieve a high photoluminescence quantum yield (PLQY) and a predictable emission spectrum, exploration of the ET mechanism is of great importance [12-15]. However, though much work on the ET mechanism in CeⅢ-MnⅡ solid phosphors has been reported, no consistent conclusion has been achieved. A dipole-quadrupole (dq) interaction mechanism was proposed in most cases [8,9,16-27] but dipole-dipole (dd) interaction [11,28-31] and exchange (ex) interaction [7,32-34] were also accounted to be the dominant mechanisms.
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Scheme 1. (a) The schematic diagram of CeⅢ-MnⅡ sensitization; EX, excitation, EM, emission, ET, energy transfer. (b) The indirect method and (c) the direct method for identifying the ET mechanism in CeⅢ-MnⅡ; C, concentration; R, distance; PET, energy transfer probability. |
Dexter’s theory elucidates the relations between the ET probability and the distance between the donor and the acceptor under different mechanisms [35]. Because the distance between CeⅢ and MnⅡ in solid phosphors could not be definitely measured, an indirect parameter, i.e. concentration (C), is utilized as the substitute to build the correlation with the ET efficiency (Scheme 1b). The ET efficiency is usually represented by overall parameters like emission intensities [9] and weighted-average lifetimes [34] of CeⅢ. And the identification of the ET mechanism in CeⅢ-MnⅡ is usually carried out following this indirect method firstly proposed by Reisfeld [36]. Naturally, one would wonder about investigating the ET mechanism based on the direct method with a parameter of the distance between CeⅢ and MnⅡ. Inspired by a heteronuclear EuⅡ-MnⅡ complex in our previous work [37], we realized that luminescent heteronuclear CeⅢ-MnⅡ complexes have clear and definite distances between CeⅢ and MnⅡ and could provide an ideal platform for the investigation on the ET mechanism (Scheme 1c).
On the construction of luminescent heteronuclear CeⅢ-MnⅡ complexes, macrocyclic ligands with size selectivity were chosen to build chelate cations containing CeⅢ while green-emitting MnBr42− acted as the anion, considering the significant difference between the radii of CeⅢ (114 pm) and MnⅡ (67 pm) [38]. The chosen ligands, N8 (1,4,7,10,13,16,21,24-octaazabicyclo[8.8.8]hexacosane) and N2O6 (4,7,13,16,21,24-hexaoxa-1,10-diazabicyclo[8.8.8]hexacosane), also provide rigid coordination environment to protect CeⅢ from non-radiative decay pathways. Based on this, complex Ce-N8-Mn and complex Ce-N2O6-Mn were designed and synthesized. In order to estimate the lifetimes and emission spectra of CeⅢ with similar coordination environment while free of inter-metal-centered ET, two control complexes, Ce(N8)Br3 and Ce(N2O6)Br3, were also prepared. Based on systematic characterizations and analysis of these complexes, dipole-quadrupole interaction was proposed to dominate the ET mechanism in CeⅢ-MnⅡ.
Ligand N8 can be facilely synthesized following previous reported routes [39] and ligand N2O6 is commercially available. Ce(N8)Br3 was synthesized by mixing ligand N8 and CeBr3 in methanol and Ce-N8-Mn was crystalized from the mixture solution of Ce(N8)Br3 and MnBr2 in methanol. Ce(N2O6)Br3 and Ce-N2O6-Mn were prepared similarly. The chemical composition and purity were confirmed by elemental analysis and single crystal X-ray diffraction. More details about synthesis were shown in Supporting information.
Single crystals of Ce(N8)Br3, Ce-N8-Mn, Ce(N2O6)Br3, and Ce-N2O6-Mn suitable for X-ray diffraction test were obtained by evaporation crystallization. Acetonitrile, dichloromethane and methanol were suitable for Ce(N8)Br3, Ce(N2O6)Br3 and two heteronuclear complexes, respectively. Ce(N8)Br3 crystalizes in a triclinic space group of P−1 and shows ten-coordinated geometry where two Br− ions coordinate directly to CeⅢ and the last one acts as a counterion (Fig. 1a, Table S1 and Fig. S1 in Supporting information). When MnBr2 is introduced, the counterion Br− and one of coordinated Br− are seized to build MnBr42−. As a result, the coordination number of CeⅢ decreases to nine in Ce-N8-Mn (Fig. 1b, Table S2 and Fig. S2 in Supporting information). In Ce-N8-Mn with an orthorhombic space group of P212121, the average bond length of Mn-Br is 2.465 Å and the minimum distance between CeⅢ and neighboring MnⅡ is 6.421 Å. Ce(N2O6)Br3 shares similar coordination geometry with Ce(N8)Br3 but crystalizes in a monoclinic space group of P2/n (Fig. 1c, Table S3 and Fig. S3 in Supporting information). Unlike Ce-N8-Mn, Ce-N2O6-Mn maintains ten-coordinated geometry of CeⅢ with one methanol molecule as an inner ligand and crystalizes in a monoclinic space group of P21 (Fig. 1d, Table S4 and Fig. S4 in Supporting information). The preference for ten-coordinated geometry of Ce-N2O6-Mn could be attributed to the lack of hindrance in N2O6, as that brought by N—H bonds in ligand N8. In Ce-N2O6-Mn, the average bond length of Mn-Br is 2.476 Å and the minimum distance between CeⅢ and neighboring MnⅡ is 6.607 Å. Both parameters become a little larger compared to those in Ce-N8-Mn, which results from the larger volume of the cation with a coordinating methanol molecule (Fig. S5 in Supporting information). Similarly, the shortest distance between two MnⅡ ions also lengthens from 7.651 Å in Ce-N8-Mn to 8.783 Å in Ce-N2O6-Mn.
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Fig. 1. Molecular structures of (a) Ce(N8)Br3, (b) Ce-N8-Mn, (c) Ce(N2O6)Br3, and (d) Ce-N2O6-Mn. Thermal ellipsoids are drawn at 50% probability. Hydrogen atoms and the solvent molecules are omitted for clarity. The distances (Å) between CeⅢ and MnⅡ in Ce-N8-Mn and Ce-N2O6-Mn were marked in green. It should be noted that Ce(N2O6)Br3 has two similar types of structures in one asymmetry unit (Fig. S3) and only one type is exhibited here for concision. Color scheme: C, black; N, blue; O, red; Ce, yellow; Mn, purple; Br, orange. |
Ce-N8-Mn exhibits dual emission in solid state, with a dominant emission peaking at 523 nm and a full width at half maximum of 62 nm (Fig. 2a and Table S5 in Supporting information). The lifetime (τ) of this peak is 304 µs (Fig. 2b), indicating that this green emission originates from the spin- and parity-forbidden 4T2 → 6A1 transition of MnⅡ in MnBr42− [40-42]. The weak emission at blue region displays remarkably double-peak characteristics and the higher of the two peaks centers at 424 nm (Fig. S6a in Supporting information). This double-peak emission has a mono-exponential decay lifetime of 1.04 ns (Fig. 2c and Fig. S6b in Supporting information), which is much shorter than that of the green emission. From the double-peak profile and the ns-level short lifetime, one can attribute this blue emission to the parity-allowed 5d → 4f transition of CeⅢ [43-46]. This identification is further supported by the emission spectrum and the lifetime of Ce(N8)Br3 in solid state (the maximum emission wavelength λmax = 408 nm and τ = 56.2 ns, Figs. 2a and c, and Fig. S6c in Supporting information).
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Fig. 2. (a) Emission spectra of Ce-N8-Mn and Ce(N8)Br3. (b) Emission decay curve of MnⅡ-center emission in Ce-N8-Mn. (c) Emission decay curves of CeⅢ-center emission in Ce-N8-Mn and Ce(N8)Br3. (d) Excitation spectra of Ce-N8-Mn. (e) Emission spectra of Ce-N2O6-Mn and Ce(N2O6)Br3. (f) Excitation spectra of Ce-N2O6-Mn. For Ce-N8-Mn and Ce-N2O6-Mn, the detecting wavelengths of emission decay curves and excitation spectra were marked in the legend. |
Under the aforementioned ascription of emission peaks, the overlap between the excitation spectra of MnⅡ-center emission and those of CeⅢ-center emission in the region of 250–400 nm indicates an ET from CeⅢ to MnⅡ in Ce-N8-Mn (Fig. 2d and Fig. S6d in Supporting information). The excitation peaks near 450 nm could be ascribed to the 6A1 → 4A1/4E(G) (436 nm), 4T2(G) (451 nm), and 4T1(G) (472 nm) transitions of MnⅡ and stand for the direct excitation [47,48]. The overlap under 400 nm means excited states on CeⅢ could relax to the emission state on MnⅡ. In other words, energy could be transferred from CeⅢ to MnⅡ. This conclusion is further confirmed by the shorter lifetime of CeⅢ-center emission in Ce-N8-Mn compared with that in Ce(N8)Br3 (1.04 ns vs. 56.2 ns), because the emergence of ET accelerates the overall deactivation process of the emission state on CeⅢ.
Similar conclusions as aforementioned could be obtained on Ce-N2O6-Mn and Ce(N2O6)Br3 (Figs. 2e and f, Fig. S7 and Table S5 in Supporting information), and only some differences would be discussed here for clarity. First of all, because longer average bond length of Mn-Br weakens the coordinating field in MnBr42−, the MnⅡ-center emission in Ce-N2O6-Mn is a little red-shifted (548 nm, Fig. S8 in Supporting information). In contrast, Ce-N2O6-Mn and Ce(N2O6)Br3 show remarkably blue-shifted CeⅢ-center emission (348 nm and 322 nm) for O atom produces weaker coordinating field than N atom does. As a result, the excitation spectra of MnⅡ-center emission in Ce-N2O6-Mn contain more direct excitation peaks (6A1 → 4T1(P) (362 nm) and 4E(D) (373 nm)). Another noteworthy feature about the emission spectrum of Ce-N2O6-Mn is that the relative intensity of CeⅢ-center emission is much stronger, which means the ET process is less complete.
Thanks to the compact protection brought by macrocyclic ligands, both Ce(N8)Br3 and Ce(N2O6)Br3 have a near-unity PLQY (Table S5). When the whole emission spectra are integrated, the PLQY of Ce-N8-Mn is 62% whereas the PLQY of Ce-N2O6-Mn is about 100%. Considering the almost 100% PLQYs of mononuclear complexes Ce(N2O6)Br3 and Ce(N8)Br3, which mean the non-radiative transition processes on the CeⅢ centers are negligible, this difference on PLQY originates most likely from the MnⅡ centers (Fig. S9 in Supporting information). This conclusion is further supported by the differences on lifetime (304 µs vs. 567 µs). According to literature [49,50], the higher PLQY of Ce-N2O6-Mn is caused by the longer distance between two adjacent MnⅡ centers (8.783 Å vs. 7.651 Å in Ce-N8-Mn). As a new example of Mn-containing complex with recording PLQY, Ce-N2O6-Mn reveals the feasibility of 4f-3d sensitization for the design of highly luminescent metal complexes with forbidden d-d transitions.
Based on aforementioned characterizations, the ET mechanism in heteronuclear CeⅢ-MnⅡ complexes was investigated as follows. Firstly, under the assumption that the dominant mechanisms are dd, dq, and ex interaction, respectively, we would separately calculate the theoretical ratio of ET probability in Ce-N8-Mn to that in Ce-N2O6-Mn. Then, we would compare these calculated results with the experimental result and draw a conclusion.
According to Dexter’s theoretical analysis [35], the ET probability of dd interaction (PET(dd)) could be strictly expressed (Eq. S1 in Supporting information). However, in systems with the same acceptor (MnBr42−) and different donors, the following simplified relation is sufficient for discussion (Eqs. 1 and 2)
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(1) |
① Fc stands for the overlap integral between the emission spectra of the donor (fd(E), normalized) and the absorption spectra of the acceptor (Fa(E), normalized) and has the formula as
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(2) |
In our system, the fd(E) of CeⅢ in the heteronuclear complex is estimated by the emission spectrum profile of the mononuclear complex and the Fa(E) of MnⅡ is estimated by the excitation spectrum profile of a reported SrⅡ-MnⅡ complex without energy donors (Fig. S10 in Supporting information) [37]. Since originating from the same d-d transitions, the excitation spectra of luminescent MnBr42− salts have similar profiles and contain nearly the same information as the absorption spectra do. Thus, it is reasonable to estimate the Fa(E) with the excitation spectra. Herein, the SrⅡ-MnⅡ complex was selected for its structural similarity with CeⅢ-MnⅡ complexes and its ready-made spectrum data in literature. The convolution spectrum profiles (Fig. S11a in Supporting information) showed that more energy levels of MnⅡ could be reached via ET in Ce-N8-Mn than in Ce-N2O6-Mn. Thus, the calculated Fc in Ce-N8-Mn (1.61 × 10−22) is larger than that in Ce-N2O6-Mn (2.87 × 10−23).
② R represents the distance between CeⅢ and MnⅡ. Herein, only the minimum distance between CeⅢ and neighboring MnⅡ was considered for the minimum distance represented the maximum ET probability and dominated the ET processes. According to the crystal structures, R in Ce-N8-Mn and Ce-N2O6-Mn were 6.421 Å and 6.607 Å, respectively.
③ τd is the lifetime of the donor without ET. Herein, τd was estimated by the lifetime of CeⅢ-center emission in the mononuclear complex, which is 56.2 ns for Ce(N8)Br3 and 19.8 ns for Ce(N2O6)Br3.
Inserting the corresponding values of Fc, R and τd into Eq. 1, we got the calculated ratio of PET(dd) in Ce-N8-Mn to PET(dd) in Ce-N2O6-Mn to be 2.35. This result indicates that if dd interaction was the dominant ET mechanism in CeⅢ-MnⅡ, the experimental ratio of ET probabilities of the two heteronuclear complexes should be close to 2.35.
For the dq interaction mechanism, the ET probability (PET(dq)) has a similar relation (Eq. 3):
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(3) |
where the main difference is the power of R compared with Eq. 1.
In the same way, inserting the corresponding values of Fc, R and τd into Eq. 3 gave the calculated ratio of PET(dq) in Ce-N8-Mn to PET(dq) in Ce-N2O6-Mn to be 2.48. That is to say, if dq interaction was the dominant ET mechanism in CeⅢ-MnⅡ, the experimental ratio of ET probabilities of the two heteronuclear complexes should be close to 2.48.
The ET probability of exchange interaction (PET(ex)) could be estimated as follows (Eqs. 4 and 5).
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(4) |
where
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(5) |
and l represents the effective average Bohr radius for the excited states of CeⅢ and the ground states of MnⅡ. Herein, l was estimated to the value of 0.461 Å as reported in CeⅢ-MnⅡ via exchange interaction ET mechanism [32]. Fex was calculated under the same condition as Fc and similar convolution spectrum profiles were obtained (Fig. S11b in Supporting information). The calculated Fc in Ce-N8-Mn and Ce-N2O6-Mn were 4.48 × 10−5 and 1.75 × 10−5, respectively.
Likewise, inserting the corresponding values of Fex, R and l into Eq. 4 gave the calculated ratio of PET(ex) in Ce-N8-Mn to PET(ex) in Ce-N2O6-Mn to be 5.75. If ex interaction was the dominant ET mechanism in CeⅢ-MnⅡ, the experimental ratio of ET probabilities should be close to 5.75.
In practice, the experimental ET probability (PET) is calculated as follows (Eq. 6).
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(6) |
where τET and τd are the lifetimes of CeⅢ-center emission in the heteronuclear complex and the mononuclear complex, respectively (Table S5). Apparently, other nonradiative processes are neglected. This approximation is reasonable because Ce-N2O6-Mn has a near-unity PLQY and light losses of Ce-N8-Mn are thought to happen on MnⅡ as discussed above. The PET in Ce-N8-Mn and Ce-N2O6-Mn were 9.44 × 108 s−1 and 3.80 × 108 s−1, respectively. Thus, the experimental ratio of PET in Ce-N8-Mn to PET in Ce-N2O6-Mn was 2.48.
By comparing the experimental value (2.48) with the calculated theoretical values of three mechanisms (2.35, 2.48, and 5.75 for dd, dq, and ex interaction, respectively), one could find that the simulated result of dq interaction matched best (Fig. 3a). This result is consistent with our preliminary judgement of Förster resonance energy transfer in the EuⅡ-MnⅡ complex for the distance is too long for efficient ET via exchange interaction [37,51,52]. The dependence on R of PET (Fig. 3b, normalized at 6.607 Å) showed the different amplification extents of PET caused by the shortening of R from 6.607 Å to 6.421 Å. Though the numerical difference between dq interaction and dd interaction is small, the experiment reproduced the calculated theoretical result precisely. Therefore, we proposed that dipole-quadrupole interaction dominated the ET mechanism from CeⅢ to MnⅡ. It is worth noting that the ET mechanism would be different if the distances between metal centers are in different ranges. For example, in an inorganic system with EuⅡ-MnⅡ ET where many EuⅡ centers only have slow ET processes caused by long distances, dd interaction was proposed [53].
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Fig. 3. (a) The experimental and calculated theoretical ratio of ET probability (PET) in Ce-N8-Mn to that in Ce-N2O6-Mn. (b) The dependence on the distance (R) of ET probability (PET); dd, dq, and ex stand for dipole-dipole, dipole-quadrupole, and exchange interaction, respectively. |
In summary, we prepared two luminescent heteronuclear CeⅢ-MnⅡ complexes with macrocyclic ligands chelating CeⅢ specifically. Both complexes exhibit efficient energy transfer from CeⅢ to MnⅡ and a near-unity PLQY was achieved in Ce-N2O6-Mn. This is the first time that CeⅢ-MnⅡ energy transfer was constructed and found in a molecular complex. Moreover, we proposed a new method in which direct correlations of the energy transfer probability to the distance, the spectral overlap integral, and the lifetime were taken as evidences of the energy transfer mechanism. By this way, dipole-quadrupole interaction mechanism was supported by the experimental data. One more time, this work demonstrated the feasibility of 4f-3d sensitization for preparing highly luminescent metal complexes with forbidden d-d transitions. The research method on the energy transfer mechanism in CeⅢ-MnⅡ developed here also brought the opportunity for the investigation of other energy transfer processes between metal centers.
Declaration of competing interestThe authors declare the following financial interests/personal relationships which may be considered as potential competing interests: A patent has been filed on this paper.
CRediT authorship contribution statementHuanyu Liu: Writing – original draft, Methodology, Investigation, Conceptualization. Gang Yu: Writing – review & editing, Methodology, Funding acquisition. Ruoyao Guo: Investigation. Hao Qi: Investigation. Jiayin Zheng: Investigation. Tong Jin: Investigation. Zifeng Zhao: Funding acquisition. Zuqiang Bian: Writing – review & editing, Project administration, Funding acquisition. Zhiwei Liu: Writing – review & editing, Supervision, Project administration, Funding acquisition, Conceptualization.
AcknowledgmentsThe authors gratefully acknowledge the financial support from the National Key R&D Program of China (Nos. 2022YFB3503702, 2023YFB3506901, 2021YFB3501800) and the National Natural Science Foundation of China (Nos. 92156016, 62104013, 22071003).
Supplementary materialsSupplementary material associated with this article can be found, in the online version, at doi:10.1016/j.cclet.2024.110296.
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