Abstract

Ring-shaped Re(I) multinuclear complexes (Re(I) rings) in which Re(I)-diimine-biscarbonyl complexes are connected to each other through bisphosphine bridging ligands exhibit very suitable photophysical and electrochemical properties as redox photosensitizers. We developed two approaches for synthesizing Re(I) rings connected with a Ru(II) complex: cyclization of a linear Re(I) trinuclear complex connected with a Ru(II) complex and Mizoroki–Heck coupling of a ring-shaped Re(I) trinuclear complex and a Ru(II) complex. Photophysical measurements of these heteromultinuclear complexes and comparisons with their model complexes indicated that they exhibit efficient light-harvesting abilities, where energy transfer from the excited ring-shaped Re(I) trinuclear complex unit to the Ru(II) complex unit proceeds efficiently.
Keywords: multinuclear complexes, luminescence, energy transfer, light-harvesting system, coupling reaction
Introduction
The systematic integration of emissive polypyridyl d6-transition-metal complexes potentially affords useful photophysical properties and/or photochemical behaviors that cannot be achieved using the corresponding mononuclear complexes, such as control of the direction and speed of excitation energy and/or electron transfer, photochemical multielectron accumulation, and good performance as redox photosensitizers or photocatalysts.1,2 As typical examples, wheel-type assemblies3 and dendrimers4,5 constructed with Ru(II) trisdiimine complexes; multiporphyrin arrays with Re(I) or Ru(II) ions;6−8 and linear-,9 square-,10−17 and ring-shaped18−23 multinuclear Re(I) complexes have been reported. Among them, ring-shaped Re(I) multinuclear complexes (Re(I) rings) in which Re(I)-diimine-biscarbonyl complexes are connected to each other through bisphosphine bridging ligands exhibit unique photophysical and electrochemical properties,18−20e.g., strong luminescence from the triplet metal-to-ligand charge transfer (3MLCT) excited state (emission quantum yield as high as 66%),20 a much longer lifetime (as high as 7.77 μs)20 and stronger oxidation power of the 3MLCT excited state compared with those of the corresponding mononuclear and linear-shaped multinuclear Re(I) complexes, and stability of both the excited state and the reduced state. Because of their excellent redox photosensitizer ability, the Re(I) rings have been used in the photocatalytic reduction of CO2. For example, a photocatalytic system comprising a trinuclear Re(I) ring as a redox photosensitizer and a Re(I) mononuclear complex as a catalyst exhibits the highest quantum yield of CO2 reduction in the reported photocatalytic systems (ΦCO = 82%).18,20 In addition, tetranuclear Re(I) rings can photochemically accumulate as many as four electrons per molecule and their reduced state is stable.21 These useful photofunctions are reinforced by interligand π–π interaction between the diimine ligands and phenyl groups in the phosphine ligands.24−27 Such interaction is substantially enhanced when the multinuclear complexes are cyclized because of the rigidity of the molecular structure and the limited rotation along the P–Re–P bonds.18,19
The synergistic connection of different photofunctional complexes to form heteromultinuclear complexes is a useful approach to creating new photofunctions that cannot be achieved using a simple mixture of the corresponding model complexes. The Re(I) rings should be fascinating candidates for such heteromultinuclear complexes because of their aforementioned unique photophysical and photochemical properties.
Therefore, synthetic methods to introduce into the Re(I) rings another metal complex that does not affect the Re(I) rings’ steric structures should be developed to create a new class of photofunctional molecules.
We herein report two methods for synthesizing such Re(I) rings connected with a Ru(II) trisdiimine complex28 which is another type of useful photofuctional metal complex ([Ring-Run]5+): (1) cyclization of linear-shaped Re(I) trinuclear complexes already connected to the Ru complex and (2) the Mizoroki–Heck reaction between a ring-shaped Re(I) trinuclear complex and a Ru(II) complex. The synthesized [Ring-Run]5+’s exhibit excellent light-harvesting functions: light energy absorbed by the Re(I)-ring unit is efficiently transferred to the Ru unit. Figure 1 illustrates the structures of the synthesized [Ring-Run]5+’s (n = 1, 2, 3) and the corresponding model complexes.
Figure 1.

Structures and abbreviations of [Ring-Run]5+’s and the model complexes. All are PF6– salts.
Results and Discussion
Synthesis
(1) Cyclization of Linear Re(I) Trinuclear Complexes Connected with a Ru Complex
To substitute both terminal CO ligands in the linear-shaped Re(I) trimer complexes, which is one of the critical processes for synthesizing the target complexes, we recently developed a selective method for removing the carbonyl ligand only in the trans-position to the phosphine ligand in fac-[Re(N^N)(CO)3(PR3)]+ (N^N = diimine ligand) using Me3NO as a decarbonylation reagent.20,23 Notably, the photochemical ligand substitution reaction,18,29 which is well-known as the other method to remove CO ligands, cannot be used in the case of linear Re(I) multinuclear complexes with a Ru(II) unit because efficient energy transfer proceeds from the excited Re units to the Ru unit.30 As a typical example, the synthetic scheme for [Ring-Ru1]5+ is illustrated in Scheme 1. A linear Re trimer in which one of the edge Re moieties is connected with a Ru(II) complex ([L3(4dmb)(trans-CO)2-Ru(4dmb,bpy2)]5+, 4dmb = 4,4′-dimethyl-2,2′-bipyridine, bpy = 2,2′-bipyridine) was synthesized via the reaction between the Re dimer with a labile ligand and a Ru–Re heterodinuclear complex in which the Re unit has a bisphosphine moiety as a monodentate ligand (process A in Scheme 1). To an acetone solution of the isolated [L3(4dmb)(trans-CO)2-Ru(4dmb,bpy2)]5+(PF6)5, 2 equiv of Me3NO was added at room temperature (process B). The solution immediately became dark brown, indicating rapid substitution of CO with a solvent molecule and/or Me3N. Panels a and b of Figure S1 show electrospray-ionization (ESI) mass spectra of the reaction solution before and after the addition of Me3NO, respectively. In this reaction, two carbonyl ligands in the trans-positions to the dppph ligands (dppph = 1,4-bis(diphenylphosphino)benzene), which are localized in both edge Re units, were selectively substituted, whereas the other carbonyl ligands and the Ru unit were not affected. One equivalent of dppph was added to the reaction solution, which was subsequently refluxed for 24 h, giving the target molecule [Ring-Ru1]5+ as the major product (process C), as indicated by size-exclusion chromatography (SEC) analysis of the reaction solution (Figure S1c).31 Through recycling size-exclusion chromatography (RSEC) and recrystallization, [Ring-Ru1](PF6)5 was isolated in 44% isolated yield. Its 1H NMR spectrum is shown in Figure 2. Similar procedures were applied to synthesize [Ring-Ru2](PF6)5 using [L3(5dmb)(trans-CO)2-Ru(5dmb3)](PF6)5 (Scheme S1, 5dmb = 5,5′-dimethyl-2,2′-bipyridine) instead of [L3(4dmb)(trans-CO)2-Ru(4dmb,bpy2)](PF6)5; the isolated yield was 38%.
Scheme 1. Synthesis of [Ring-Ru1]5+ via Decarbonylation with Me3NO and Subsequent Cyclization with Bidentate Phosphine Ligands.

Figure 2.

Aromatic region of the 1H NMR spectrum of [Ring-Ru1]5+ in CD3CN. The same numbering of the diimine moieties for the Ru complex is applied for the Re-ring.
(2) The Mizoroki–Heck Reaction between a Ring-Shaped Re(I) Trinuclear Complex and a Ru(II) Complex
We recently reported that a Pd-mediated Mizoroki–Heck reaction can be used to couple two different metal complexes that have either a bromo or vinyl group on the diimine ligands.32−35 We used this reaction as an alternative route for the synthesis of another ring-shaped Re(I) trinuclear complex connected with a Ru(II) complex [Ring-Ru3]5+, as illustrated in Scheme 2. A ring-shaped Re(I) trinuclear complex with two 5dmb and one 4-bromo-2,2′-bipyridine (Brbpy) ligands and with the Re(I) centers connected to each other by 1,2-bis(diphenylphosphino)ethane (dppet) ([(R3et(5dmb2,Brbpy)]3+) was first synthesized as a precursor using Me3NO for the decarbonylation followed by the cyclization step (Scheme S2).23,36 The Mizoroki–Heck reaction between [R3et(5dmb2,Brbpy)]3+ and 2 equiv of [Ru(4dmb)2(allyl-4dmb)]2+ proceeded in an MeCN solution containing 0.6 equiv of Pd(OAc)2 and 5 equiv of AcONa under reflux. Monitoring of the reaction solution using SEC showed that the reaction proceeded to a saturation point after 1 day even though both [R3et(5dmb2,Brbpy)]3+ and [Ru(4dmb)2(allyl-4dmb)]2+ remained in the reaction solution. At this point, black Pd particles precipitated in the solution. To promote further progress of the coupling, the reaction mixture was transferred to a fresh solution via a three-step procedure: removal of the precipitates by filtration, solvent evaporation, and then loading of new solvent and catalyst (in the same amount as the initial conditions). This solution was again refluxed for 48 h. These operations were repeated twice, resulting in almost complete consumption of [R3et(5dmb2,Brbpy)]3+, as shown in the SEC chromatograms in Figure S2, where the target compound ([Ring-Ru3]5+) and the starting Ru(II) complex were mainly detected. The yield of [Ring-Ru3]5+ was estimated to be 64% on the basis of the amount of [R3et(5dmb2,Brbpy)]3+ consumed, as determined by SEC analysis of the reaction solution. Purification using RSEC resulted in an isolated yield of 40%. Notably, the excess amount of [Ru(4dmb)2(allyl-4dmb)]2+ was necessary to suppress a competitive reaction, i.e., homocoupling of [R3et(5dmb2,Brbpy)]3+.34,36
Scheme 2. Synthesis of [Ring-Ru3]5+ by the Mizoroki–Heck Reaction.

These synthesized ring–Ru complexes [Ring-Run]5+s (n = 1, 2, 3) are the first examples of ring-shaped Re(I) multinuclear complexes modified with another metal complex. They were fully characterized by NMR, infrared (IR), and high-resolution mass spectroscopies. The corresponding trinuclear Re(I) rings without the Ru unit and the mononuclear Ru(II) trisdiimine complexes shown in Figure 1 were also synthesized as model compounds for clarifying photophysical processes of the ring–Ru complexes, as described in the next section.
Photophysical Properties
Figure 3 shows UV–Vis absorption spectra recorded in MeCN. The absorption spectra of all of the [Ring-Run]5+ (n = 1, 2, 3) complexes were similar to a 1:1 summation spectrum of the singlet metal-to-ligand charge transfer (1MLCT) absorption bands of the Re(I) ring and Ru(II) model complexes (i.e., [Ring1]3+ + [Ru1]2+, [Ring2]3+ + [Ru2]2+, and [Ring3]3+ + [Ru3]2+, respectively). These results indicate that no strong electronic interaction occurred between the Re ring and Ru units. Notably, in the spectra of all of the [Ring-Run]5+, the 1MLCT absorption band of the Ru(II) unit was observed at longer wavelengths compared with that of the Re(I)-ring unit.
Figure 3.

UV–vis absorption spectra of samples in MeCN: (a) [Ring-Ru1]5+ (blue), [Ring1]3+ (green), and [Ru1]2+ (red); (b) [Ring-Ru2]5+ (blue), [Ring2]3+ (green), and [Ru2]2+ (red); (c) [Ring-Ru3]5+ (blue), [Ring3]3+ (green), and [Ru3]2+ (red). The black dashed lines show corresponding 1:1 summation spectra of [Ringn]3+ + [Run]2+ (n = 1, 2, 3).
All of the [Ring-Run]5+ complexes are emissive in MeCN at ambient temperature. The photophysical properties of [Ring-Run]5+ and the corresponding model complexes are summarized in Table 1. Figure 4a shows the emission spectra of [Ring-Ru1]5+ as a typical example; these spectra were recorded using two different excitation wavelengths. The shape of the emission band varied according to the excitation wavelength: a shoulder was observed at λem ≈ 550 nm when [Ring-Ru1]5+ was excited at λex = 380 nm, whereas the shoulder decreased in intensity when the complex was excited at λex = 469 nm. Mainly the Re ring unit and partially the Ru unit absorb the light at λex = 380 nm, whereas the light at λex = 469 nm is mainly absorbed by the Ru unit (Figure 3a). The maximum emission wavelength (λemmax) was 622 and 624 nm when the complex was excited at λex = 380 and 469 nm, respectively. Therefore, even though the excitation light should be absorbed mainly by the Re ring unit of [Ring-Ru1]5+, the maximum emission wavelength was similar to that of [Ru1]2+ (λemmax = 630 nm) but not to that of [Ring1]3+ (λemmax = 581 nm) (Figure 4a). The emission spectrum of [Ring-Ru1]5+ recorded with λex = 380 nm was well-simulated with the emission spectra of [Ru1]2+ and [Ring1]3+ (Figure 4b). The simulation also reveals that the main component of the emission from [Ring-Ru1]5+ should be from the Ru unit but not from the Re ring unit and that the shoulder peak at λem = ∼550 nm in the emission band of [Ring-Ru1]5+ can be assigned to emission from the Re ring unit.
Table 1. Photophysical Properties of [Ring-Run]5+ and Their Model Complexes Measured in Degassed MeCN at 25°C.
| complex | λabsa (nm) | εb (×103 M–1 cm–1) | λemc (nm) | Φem (λex/nm) | τ1d (μs) | τ2d (μs) | τ3d (μs) |
|---|---|---|---|---|---|---|---|
| [Ring-Ru1]5+ | 424 | 23.1 | 622 | 0.11 ± 0.004 (380) | 0.016 ± 0.009 | 0.51 ± 0.007 | 0.73 ± 0.007 |
| [Ring1]3+ | 401 | 11.9 | 581 | 0.154 ± 0.001 (380) | 1.68 ± 0.005 | ||
| [Ru1]2+ | 454 | 15.5 | 630 | 0.091 ± 0.001 (380) | 0.75 ± 0.003 | ||
| [Ring-Ru2]5+ | 419 | 20.5 | 603 | 0.063 ± 0.003 (380) | 0.004 ± 0.001 | 0.22 ± 0.01 | 0.46 ± 0.01 |
| [Ring2]3+ | 398 | 11.4 | 553 | 0.44 ± 0.006 (380) | 3.40 ± 0.01 | ||
| [Ru2]2+ | 444 | 15.1 | 604 | 0.041 ± 0.002 (380) | 0.31 ± 0.001 | ||
| [Ring-Ru3]5+ | 427 | 22.0 | 633 | 0.060(380) 0.086 (460) | 0.023e | 0.14e | 0.98e |
| [Ring3]3+ | 412 | 12.3 | 622 | 0.042 ± 0.002 (390) | 0.13e | 0.84e | 4.8e,f |
| [Ring4]3+g | 409 | 571 | 0.41 | 5.4 | |||
| [Ru3]2+ | 458 | 14.9 | 633 | 0.089h | 0.85 ± 0.004 |
Maximum wavelength of the MLCT bands.
Molar extinction coefficients at λabs.
The values of [Ring-Run]5+ depend on λex; see main text.
The emission decay curves were fitted by a single- to triple-exponential function I = ΣAnexp(−t/τn), within proper χ2 values (1.0–1.1).
The lifetimes were determined by using the decay functions constructed as the numerical solutions of the set of rate equations and the “FindMinimum procedure” in Mathematica, which is described in the main text in detail.
τ3 was a very minor component in the emission and is likely emission from [Ring4]3+ as an impurity.
Ref (18).
Ref (37).
Figure 4.

(a) Normalized emission spectra of [Ring-Ru1]5+ in degassed MeCN measured using various wavelength excitation light: λex = 380 nm (light blue) and λex = 469 nm (blue dotted line). The emission spectra of [Ring1]3+ (green) and [Ru1]2+ (red) are also illustrated. (b) Emission spectrum of [Ring-Ru1]5+ (sky blue) and simulation of spectral deconvolution into individual emissions of [Ring1]3+ (green) and [Ru1]2+ (red) and their sum (black dotted line).
The emission quantum yield (Φem) was determined to be 11% (λex = 380 nm), which is slightly greater than that of [Ru1]2+ (Φem = 9%) but less than that of [Ring1]3+ (Φem = 15%). These results clearly indicate that energy transfer efficiently proceeded from the excited Re ring unit to the Ru unit in [Ring-Ru1]5+. Figure 5a shows an excitation spectrum of [Ring-Ru1]5+ measured at λem = 620 nm which is the emission maximum of [Ru1]2+. Its similarity to the absorption spectrum of [Ring-Ru1]5+ also suggests that the energy transfer from the excited Re ring unit to the Ru unit is efficient. This interpretation is reasonable because the lowest excited state of the Re ring unit has an excitation energy higher than that of the Ru unit.
Figure 5.

Normalized absorption (light blue line) and excitation spectra (black dotted line) of (a) [Ring-Ru1]5+ and (b) [Ring-Ru2]5+ in degassed MeCN. Each detection wavelength of excitation spectra is (a) 620 nm and (b) 600 nm, respectively.
The efficiency of the energy transfer (ηET), which indicates the percentage of the excited Re ring units that can transfer their excitation energy to the Ru unit, can be estimated by using eq 1:
| 1 |
where Asim(Ring-Run) and Aem(Ringn) are the areas of the emission spectra (normalized by the absorbed photon number at the excitation wavelength, λex) associated with the Re ring unit in the emission spectra of [Ring-Ru1]5+ and [Ring1]3+, respectively, and ε(Ringn) and ε(Run) are the molar absorption coefficients of [Ringn]3+ and [Run]2+ at λex, respectively. The emission spectrum of [Ring-Ru1]5+ excited at λex = 380 nm was deconvoluted using the emission spectra of [Ring1]3+ and [Ru1]2+ to estimate Asim(Ring-Ru1) (Figure 4b). From these analyses, ηET in the case of [Ring-Ru1]5+ was estimated to be 78%. Notably, such efficient intramolecular energy transfer is caused by the covalent linkage between the Re ring and the Ru complex units, as confirmed by energy transfer not being observed for an equimolar mixed solution of the model Re ring ([Ring1]3+) and the model Ru mononuclear complex ([Ru1]2+) (Figure S3).
We also investigated this excitation energy-transfer event in [Ring-Ru1]5+ by measuring the emission lifetimes and recording the corresponding transient emission spectra. Figure 6a shows the transient emission spectra of [Ring-Ru1]5+ acquired using the single-photon counting method. In the initial stage, rapid decay was observed at 480 ≤ λem ≤ 560 nm, and an increase of the emission intensity in the longer-wavelength region (λem > 570 nm) was observed in this time scale. The shape of the spectrum became similar to that of [Ru1]2+ within ∼20 ns after laser excitation. After this rapid change of the spectrum shape, the emission intensity at all wavelengths gradually decreased, accompanied by slow changes in the spectrum shape; that is, a slightly more rapid decay was observed at shorter wavelengths. Figure 6b shows time profiles of the emission at λem = 520 and 650 nm (λex = 380 nm). The decay curve recorded at λem = 520 nm (red) shows a two-step decrease, whereas the emission intensity at λem = 650 nm (blue) increases in the first stage and then decreases monotonically. As previously mentioned, the main component of the emission at λem = 520 and 650 nm is derived from the Re(I) ring unit and the Ru unit, respectively. Therefore, the increase in emission at λem = 650 nm also indicates efficient energy transfer from the excited Re ring unit to the Ru unit. The time profiles could be fitted with a triple-exponential function; the obtained lifetimes are τ1 = 16 ns, τ2 = 0.51 μs, and τ3 = 0.73 μs, and the pre-exponential factors strongly varied depending on the detection wavelength. The longest-lifetime component (τ3) is attributable to emission from the Ru(II) unit because of its similarity to the lifetime of [Ru1]2+ (τem = 0.75 μs) and the larger pre-exponential factor corresponding to the longer-wavelength region. Therefore, the two shorter lifetimes (τ1 and τ2) are attributed to emissions from the Re ring unit, both of which are shorter than that of [Ring1]3+ (τem = 1.68 μs). This difference is mainly caused by the excitation energy transfer from the Re ring unit to the Ru unit, as previously described. The two types of emission with different lifetimes is attributable to two different Re moieties in [Ring-Ru1]5+, i.e., the node-Re moiety connected with the Ru unit directly and the other peripheral Re moieties with a 4dmb ligand. Although energy migration among these Re moieties might proceed, it should be slower than the energy transfer from the excited Re ring unit to the Ru unit because the difference between τ1 and τ2 is large even though the excitation energy of each Re moiety is the same or very similar. If the energy migration among the Re moieties is assumed to not affect the photophysical properties of [Ring-Ru1]5+, the rates of energy transfer can be calculated on the basis of the emission lifetimes (Table 1) and eq 2 as kET1 = 6.2 × 107 s–1 and kET2 = 1.4 × 106 s–1 (Table 2).
| 2 |
where τ([Ringn]3+) is the lifetime of [Ringn]3+, e.g., 1.68 μs (n = 1). The efficiency of the energy transfers was estimated to be ηET1 = 99% and ηET2 = 70%, respectively, using eq 3:
| 3 |
The weighted average of ηET1 and ηET2 (ηET1 × 1/3 + ηET2 × 2/3 = 79%) well matches the value estimated by fitting the emission spectrum of [Ring-Ru1]5+ (78%), as previously described. We reasonably assumed that the node-Re moiety connected with the Ru unit was quenched more efficiently than the other Re moieties with 4dmb because of the direct connection via the ethylene chain and the short distance to the Ru unit. These excitation energy-transfer events of [Ring-Ru1]5+ are summarized in Figure 7a.
Figure 6.

(a) Transient emission spectra of [Ring-Ru1]5+ measured in MeCN with λex = 379 nm. (b) Emission decay curves of [Ring-Ru1]5+ recorded at 520 nm (red) and 650 nm (blue).
Table 2. Energy-Transfer Rate Constants and Efficiencies in the [Ring-Run]5+ Complexes in Degassed MeCN at 25°C.
|
k (×106 s–1)b |
||||||||
|---|---|---|---|---|---|---|---|---|
| complex | ηETa (%) | ET1c | ET1′d | ET2e | ET0f | ηET1g (%) | ηET2g (%) | ηETAveh (%) |
| [Ring-Ru1]5+ | 78 | 62 | – | 1.4 | – | 99 | 70 | 79 |
| [Ring-Ru2]5+ | 95 | 250 | – | 4.3 | – | >99 | 94 | 96 |
| [Ring-Ru3]5+ | – | 4.0 | 0.56 | 52 | 13 | –i | >99 | – |
| [Ring3]3+ | 98j | – | – | – | 7.6 | – | – | – |
The energy-transfer rate constant from the Re(n) unit to the Ru unit.
The energy-transfer rate constant from the Ru unit to the Re(n) unit.
The energy-transfer rate constant from the Re(p) unit to the Ru unit.
The energy-transfer rate constant from the Re(p) to the Re(n) unit.
Weighted average of ηET1 and ηET2.
The concentration ratio between the excited Ru unit and the excited Re(n) unit in the excited [Ring-Ru3]5+ was approximately 6.7:1 after equilibrium was reached.
The efficiency of the intraring energy transfer.
Figure 7.

Energy-transfer processes and their rate constants in (a) [Ring-Ru1]5+ and (b) [Ring-Ru2]5+.
Similar photophysical phenomena were observed in the case of [Ring-Ru2]5+ (Figures 5b and 8 and Table 1); that is, the maximum emission wavelength and the quantum yield (λemmax = 603 nm, Φem = 6.3%) are similar to those of [Ru2]2+ (λemmax = 604 nm, Φem = 4.1%) and dramatically different from those of [Ring2]3+ (λemmax = 553 nm, Φem = 44%). The excitation (Figure 5b: λem = 600 nm, close to the emission maximum of [Ru2]2+) and absorption spectra of [Ring-Ru2]5+ were similar to each other. The energy-transfer efficiency in the case of [Ring-Ru2]5+, which was determined from spectrum-fitting using the spectra of [Ru2]2+ and [Ring2]3+ in the same manner as for [Ring-Ru1]5+ (eq 1), was greater (ηET = 95%) than that of [Ring-Ru1]5+ (ηET = 78%).
Figure 8.

(a) Normalized emission spectra of [Ring-Ru2]5+ in degassed MeCN measured using excitation light with various wavelengths: λex = 380 nm (sky blue) and λex = 456 nm (blue dotted line). The emission spectra of [Ring2]3+ (green) and [Ru2]2+ (red) are also illustrated. (b) Emission spectrum of [Ring-Ru2]5+ (sky blue) and spectral deconvolution into individual emissions of [Ring2]3+ (green) and [Ru2]2+ (red) and their sum (black dotted line).
When [Ring-Ru2]5+ was excited at λex = 379 nm, the transient emission spectra of [Ring-Ru2]5+ also showed two-step decay at λem < 570 nm (Figure 9). This stepwise decay was likely caused by different rates of intramolecular energy transfer from the two different Re moieties, similar to the case of [Ring-Ru1]5+. The decay profiles were fitted with a triple-exponential function with τ1 = 4 ns, τ2 = 220 ns, and τ3 = 460 ns. Because the pre-exponential factor of τ3 was dominant at λem ≈ 700 nm, this longest component is attributable to emission from the Ru unit.
Figure 9.

(a) Transient emission spectra of [Ring-Ru2]5+ measured in MeCN with λex = 379 nm. (b) Emission decay curves of [Ring-Ru2]5+ recorded at 520 nm (red) and 650 nm (blue).
The energy-transfer rates in [Ring-Ru2]5+ were calculated as kET1 = 2.5 × 108 s–1 and kET2 = 4.3 × 106 s–1 using τ1 and τ2; these results are attributable to the lifetimes of the Re(I) ring unit (eq 2). These values indicate that the emission from each Re unit in the Re ring unit was quenched almost quantitatively (ηET1 > 99%, ηET2 = 94%). The weighted average of ηET1 and ηET2 (ηET1 × 1/3 + ηET2 × 2/3 = 96%) is similar to the value estimated by fitting the emission spectra using eq 1 (95%). The reason for the more efficient intramolecular energy transfer in [Ring-Ru2]5+ compared with that in [Ring-Ru1]5+ is discussed below. The energy-transfer processes and the corresponding rate constants are summarized in Figure 7b.
Figure 10a shows the emission spectra of [Ring-Ru3]5+. The emission behavior of [Ring-Ru3]5+ differs somewhat from those of [Ring-Ru1]5+ and [Ring-Ru2]5+. The emission spectrum of [Ring-Ru3]5+ differs from that of [Ru3]2+ and could be well fitted using the emission spectra of both [Ring3]3+ and [Ru3]2+. Because the Re complex unit with the bridging diimine ligand of [Ring-Ru3]5+ has a vinyl group that conjugates with the diimine moiety, the π* energy level of the orbitals of this bridging diimine ligand should be lower than those of [Ring-Ru1]5+ and [Ring-Ru2]5+. Actually, the emission maximum of [Ring3]3+, which has one Re complex unit with a conjugated vinyl group, was red-shifted and closer to that of [Ru3]2+ (Figure 10a) compared with [Ring1]3+ and [Ring2]3+. Because of this difference, [Ring-Ru3]5+ exhibited different photophysical behaviors from [Ring-Ru1]5+ and [Ring-Ru2]5+. The contributions of both model complexes to this fitting were similar to each other (Figure 10b); that is, the contribution of the model of the Re ring unit, i.e., [Ring3]3+, was much larger than that of the Re ring models in the fittings of [Ring-Ru1]5+ and [Ring-Ru2]5+ (Figures 4b and 8b).
Figure 10.

(a) Normalized emission spectra of [Ring-Ru3]5+ in degassed MeCN, as measured with excitation light of various wavelengths: λex = 380 nm (sky blue) and λex = 460 nm (blue dotted line). The emission spectra of [Ring3]3+ (green), [Ru3]2+ (red), and [Ring4]2+ (yellow green) are also illustrated. (b) Emission spectrum of [Ring-Ru3]5+ (blue, λex = 380 nm) and simulation of spectral deconvolution into individual emission spectra of [Ring3]3+ (green) and [Ru3]2+ (red) and their sum (black dotted line).
Before investigating the properties of the excited [Ring-Ru3]5+, we carefully checked the photophysical behaviors of [Ring3]3+. Notably, this analyzed sample contained a minimal amount of [Ring4]3+, which could not be removed and was detected as small peaks in the ESI mass spectrum (Figure S4). However, the effects of this impurity on the photophysical properties of the sample are easily corrected for, as described later. The transient emission spectra of [Ring3]3+ show a gradual red-shift of the maximum emission wavelength from λmax = 605 nm (5 ns) to λmax = 635 nm (1000 ns) (Figure 11a). The emission decay measured at λdet = 550 nm was drastically faster than that at λdet = 650 nm (Figure 11b). These results strongly suggest that intramolecular energy transfer proceeded among the Re complex units in [Ring3]3+. The emission decay curves could be fitted with a triple-exponential function; the obtained lifetimes were τ1 = 130 ns, τ2 = 840 ns, and τ3 = 5 μs, respectively. Because τ3 was a minor component in the emission, it likely originated from the [Ring4]3+ impurity because τ3 is very similar to the emission lifetime of [Ring4]3+ (τem = 5.4 μs). Therefore, the emission lifetimes from [Ring3]3+ itself should be τ1 = 130 ns and τ2 = 840 ns. The emission maximum of [Ring4]3+ (Figure 10a), which consists of only the Re complex units with 5dmb, was blue-shifted compared with that of [Ring3]3+ (Figure 10a) and the wavelength dependence of the pre-exponential factors of τ1 of [Ring3]3+ (Figure S5) was similar to the emission spectrum of [Ring4]3+ (yellow green spectrum in Figure 10a). These results strongly suggest that τ1 and τ2 are the emission lifetimes associated with the Re units with 5dmb and that with 4-vinyl-bpy (vbpy), respectively, and that the excitation energy was transferred from the Re units with 5dmb to that with vbpy. The rate constant of the energy transfer in [Ring3]3+ (kET0) was calculated as kET0 = 7.6 × 106 s–1 using eq 2 with τ1 and the emission lifetime of [Ring4]3+ (τ([Ring4]3+) = 5.4 μs, Figure 12a). According to eq 3, the efficiency of this intraring energy transfer was ηET = 98% (Figure 12a).
Figure 11.

(a) Transient emission spectra of [Ring3]3+ measured in MeCN with λex = 444 nm. (b) Emission decay curves of [Ring3]3+ recorded at 550 nm (red) and 650 nm (blue)
Figure 12.

Energy-transfer processes and their rate constants in (a) [Ring3]3+ and (b) [Ring-Ru3]5+.
Figure 13a shows the transient emission spectra of [Ring-Ru3]5+. The time profiles of the emission in the shorter-wavelength region (<600 nm) show a rapid decrease within 50 ns. This behavior is attributable to energy transfer from the Re units with the 5dmb ligand to other units in [Ring-Ru3]5+. Notably, this decay rate is much higher than that of the energy transfer from the Re units with the 5dmb ligand to the Re unit with the vbpy ligand in [Ring3]3+. This difference strongly suggests that energy transfers from the Re units with the 5dmb ligand directly to the Ru unit as well (red arrow in Figure 12b). In addition, from 50 to 400 ns, another slower and smaller change in the spectrum shape is observed, i.e., a decrease in the wavelength region <600 nm and an increase at ∼630 nm (Figure 13b); the transient spectrum then monotonically decays without a change in the spectrum shape after 400 ns. This spectrum shape recorded after 800 ns was well-fitted with the emission spectra of [Ru3]2+ and [Ring3]3+ (Figure S6). These results indicate that another energy transfer occurred from the Re unit with the vbpy ligand to the Ru unit in the time interval to 400 ns and that the reverse energy transfer from the Ru unit to the Re unit with the vbpy ligand simultaneously proceeded (green arrows in Figure 12b). These forward and backward energy-transfer processes should arrive at an equilibrium state at 400 ns after the laser irradiation. Figure 13c shows emission decay curves of [Ring-Ru3]5+ recorded at λem = 550 and 650 nm as typical examples (λex = 337 nm), which could be roughly fitted using a triple-exponential function with τ1 = 23 ns, τ2 = 140 ns, and τ3 = 980 ns. Notably, the pre-exponential functions of τ2 (A2) at >600 nm were negative values because of the slower energy transfer between 50 and 400 ns after laser irradiation (Figure 13d); in this time region, the ratio between the excited Re unit with the vbpy ligand and the excited Ru unit should be greater than that in the equilibrium state because the Ru unit has a slightly longer emission maximum than the Re unit with the vbpy ligand. This result also suggests that the process with τ2 = 140 ns involves a change in the concentration ratio between the excited Ru unit and the excited Re unit with the vbpy ligand. Because the lifetimes of the excited state of [Ru3]2+ and the Re unit with the vbpy ligand of [Ring3]3+ are similar to each other and also similar to the longest emission lifetime of [Ring-Ru3]5+ (Table 1), the emission with τ3 = 980 ns is attributed to both the excited Ru unit and the excited Re unit with the vbpy ligand.
Figure 13.

(a) Transient emission spectra of [Ring-Ru3]5+ in MeCN with λex = 337 nm. (b) Transient emission spectra of [Ring-Ru3]5+ normalized at 620 nm. (c) Emission decay curves of [Ring-Ru3]5+ recorded at 550 nm (red) and 650 nm (blue). (d) Wavelength dependence of the pre-exponential factors of τ1 (A1), τ2 (A2), and τ3 (A3).
To determine the exact rate constants of energy-transfer processes among the three different units in [Ring-Ru3]5+, i.e., the Ru unit, the Re units with the 5dmb ligand, and the node-Re unit directly connected with the Ru unit, we analyzed the emission decays measured at three different detection wavelengths (550, 575, and 650 nm). These emission decays are mainly associated with the Re units with the 5dmb ligand, a mixture of emissions from all of the units, and the Ru unit, respectively. We conducted the analyses using the rate equations based on the photophysical processes of [Ring-Ru3]5+ (Figure 14).
Figure 14.
Photophysical processes of [Ring-Ru3]5+. I0 is the sum of the initial concentrations of the excited states. αA, αB, and αC are the fractions of the initial concentrations. kA, kB, and kC are intrinsic decay rates of the excited states. ΦA, ΦB, and ΦC are intrinsic emission quantum yields of the excited states. τA, τB, and τC are the intrinsic emission decay lifetimes of the excited states. kET0, kET1, kET1′, and kET2 are the energy-transfer rate constant from the Re(p) (the Re units with the 5dmb ligand) to the Re(n) unit (the node-Re unit), that from the Re(n) unit to the Ru unit, that from the Ru unit to the Re(n) unit, and that from the Re(p) unit to the Ru unit, respectively.
The concentrations of the excited states of [Ring-Ru3]5+ at t seconds after excitation are abbreviated as A(t), B(t), and C(t), where the excited units are the Re unit with the 5dmb ligand (Re(p)), the Re unit directly connected to the Ru unit (Re(n)), and the Ru unit itself (Ru), respectively. These concentration changes can be formulated by the following set of rate equations (eqs 4–6):
| 4 |
| 5 |
| 6 |
The observed emission intensity Iem(λ, t) at the monitoring wavelength (λ) and time (t) was calculated using the concentrations of the excited states (J). The numerical parameters relate to their emission spectra and the spectral sensitivities of the apparatus as
| 7 |
where a(λ) is the apparatus constant of the instrument at wavelength λ, bJ(λ) the numerical constant of the emission spectral shape of the excited species J at wavelength λ, and J(λ, t) the concentration of the excited state J.
The set of rate equations was numerically solved, and the emission decays of the [Ring-Ru3]5+ measured at 550, 575, and 650 nm (Figure 15) were analyzed using the nonlinear model fit method in the Wolfram Mathematica 10 software (Wolfram Research Inc.) to minimize the deviation of the evaluated values from those in the emission decay data with the parameters, as previously described; both the precision goal and the accuracy goal were set to 10–8, and the experimentally obtained parameters from the measurement of the model species, [Ring3]3+, [Ring4]3+, and [Ru3]2+ (i.e., kA = 1.9 × 105 s–1, kB = 1.2 × 106 s–1, and kc = 1.0 × 106 s–1) were used. Reasonable fitting was obtained, as shown in Figure 15. The evaluated kinetic parameters are summarized along with other photophysical parameters in Table 2.
Figure 15.

Emission decay profiles of [Ring-Ru3]5+ monitored at (a) 550, (b) 575, and (c) 650 nm (red dots) with the simulated emission intensities (orange curves) and residuals (red dots). The calculated relative concentration changes of three excited states of [Ring-Ru3]5+ are presented in panel d.
Interestingly, the value of kET2 of [Ring-Ru3]5+, which is the energy-transfer rate from the excited Re unit with the 5dmb ligand to the Ru unit, is relatively large even though the length of the spacer between the Ru unit and the Re ring unit is the longest among the ring–Ru complexes. This result suggests that the Ru unit can collide with the Re units with 5dmb because of the flexibility of the long bridging chain. The obtained energy-transfer rate from the excited Re unit with the 5dmb ligand to the Re unit directly connected with the Ru unit in [Ring-Ru3]5+ (kET0 = 13 × 106 s–1) is slightly greater than that from the excited Re unit with the 5dmb ligand to the Re unit with the vbpy ligand in [Ring3]3+ (kET0 = 7.6 × 106 s–1). This difference might be caused by different conformations of the Re ring moiety in [Ring-Ru3]5+ and that of [Ring3]3+ because of the steric hindrance of the Ru unit and flexibility of the bridging bisphosphine ligands, i.e., dppet. The rate constant of forward energy transfer from the Re unit to the Ru unit, each of which is directly connected, was kET1 = 4.0 × 106 s–1, and that of the backward energy transfer was kET1′ = 0.56 × 106 s–1; therefore, the concentration ratio between the excited Ru unit and the excited Re(n) unit in the excited [Ring-Ru3]5+ was approximately 6.7:1 after equilibrium was established between them.
Conclusions
We developed two efficient synthetic strategies to construct covalently linked trinuclear Re(I) rings with the Ru(II)-trisdiimine mononuclear complex [Ring-Run]5+ (n = 1, 2, 3). These complexes exhibit strong absorption in the visible region because of different absorption behaviors of the Re complex and Ru complex units. They also show good light-harvesting ability because of the efficient intramolecular energy transfer among the Re units and between the Re ring and the Ru unit. Notably, both the Re rings and [Ru(diimine)3]2+ complexes function as excellent redox photosensitizers (photoredox catalysts), and [Ring-Run]5+ has both complex units. Therefore, this multinuclear complex can potentially function as good redox photosensitizers with stronger visible-light absorption than the Re rings and [Ru(diimine)3]2+ complexes. The synthesis methods of [Ring-Run]5+ should enable any diimine-coordinating metal complexes to be tethered to the Re ring, leading to the construction of novel Re rings with various metal complexes.
Experimental Section
Materials and Methods
Acetonitrile was dried over P2O5 three times and then distilled from CaH2 prior to use. Other anhydrous solvents were purchased from commercial sources. All reactions were carried out under an inert atmosphere and in dim light. Column chromatography was performed with Silica Gel 60 (40–50 μm, Kanto Chemical Co.), alumina (standardized, Merck), or Sephadex (GE Healthcare). 2,2′-Bipyridine (bpy), 4,4′-dimethyl-2,2′-bipyridine (4dmb), 5,5′-dimethyl-2,2′-bipyridine (5dmb), 1,2-bis(diphenylphoshino)ethane (dppet), Re2(CO)10, RuCl3·H2O, Me3NO, Pd(OAc)2 and other commercially available reagents were purchased from Kanto Chemical Co., Tokyo Kasei Co., Wako Pure Chemical Industries, and Aldrich Chemical Co. and were used as received. Syntheses of 4′-but-3-enyl-4-methyl-2,2′-bipyridyl (allyl-4dmb),38 1,2-bis(4′-methyl-[2,2′-bipyridin]-4-yl)ethane (4C2),39 and analogously 1,2-bis(5′-methyl-[2,2′-bipyridin]-5-yl)ethane (5C2), p-bis(diphenylphosphino)benzene (dppph),40 and Re(CO)5Br41 were reported elsewhere. The 4-(2-hydroxyethyl)-2,2′-bipyridine (OHbpy),42fac-Re(N^N)(CO)3Br-type,43fac-Re(N^N)(CO)3OTf-type,44 Ru(N^N)2Cl2-type,45 final model complexes of [Ru(N^N)3]2+-type,46 and dinuclear Re(I) complexes ([L2xx(N^N)]2+, xx = bisphosphine ligand)9 were synthesized according to the reported methods with some modification and using corresponding N^N ligands. Syntheses of the trinuclear ring complexes [R3ph(N^N)]3+(19) and [R3et(5dmb2,Brbpy)]3+(36) were published recently. All target complexes were obtained as PF6– salts.
Photochemical reactions were performed with a 500 W high-pressure Hg lamp EHBWI (Eikosha) with a uranium glass filter (>330 nm) in a Pyrex doughnut-form cell, with bubbling of N2 gas. During irradiation, both the reaction vessel and the light source were cooled with tap water. Separation of larger complexes was achieved by RSEC using a pair of Shodex PROTEIN KW-2002.5 columns (300 mm × 20.0 mm i.d.) with a KW-LG guard column (50 mm × 8.0 mm i.d.) and a JAI LC-9201 recycling preparative HPLC apparatus (Japan Analytical Industry Co.) with a JASCO 870-UV detector (the detection wavelength was chosen as 360 nm); the eluent was MeOH–MeCN (1:1 v/v) containing CH3COONH4 (0.15 M), and the flow rate was 6.0 mL min–1.31 For analytical SEC, two sequentially connected Shodex KW-402.5-4F columns (300 mm × 4.6 mm i.d.) were used, with a KW400G-4A guard-column (10 mm × 4.6 mm i.d.), a JASCO 880-51 degasser, an 880-PU pump, an MD-2010 Plus UV–Vis photodiode-array detector (λdet = 360 nm), and a Rheodyne 7125 injector. The column temperature was maintained at 40 °C using a JASCO 860-CO column oven. The eluent was MeOH–MeCN (1:1 v/v) containing CH3COONH4 (0.5 M), and the flow rate was 0.2 mL min–1. 1H NMR and 31P NMR spectra were acquired with a JEOL ECA400II spectrometer. Chemical shifts (δ/ppm) were referenced to the residual 1H signals of a deuterated solvent (1.94 ppm for CD3CN and 2.05 ppm for CD3COCD3) and the 31P-signal of PF6– (−145 ppm), respectively. All NMR spectra were recorded at room temperature. ESI mass spectrometry (ESI-MS) was conducted on a Shimadzu LCMS-2010A mass spectrometer. ESI time-of-flight mass spectrometry was undertaken with a Waters LCT Premier instrument. Fourier transform infrared (FT-IR) spectra were recorded with a JASCO FT/IR-610 spectrometer at 1 cm–1 resolution with a TGS detector.
UV–Vis absorption spectra were recorded with a JASCO V-565 or V-670 spectrophotometer. Emission spectra were recorded at 25 °C using a JASCO FP-6500 spectrofluorometer and were corrected for photomultiplier tube response. Emission quantum yields were determined with a calibrated integrating sphere (Absolute PL Quantum Yield Measurement System C9920-01, Hamamatsu Photonics k.k.) comprising a Xe lamp as an excitation source and a multichannel spectrometer (C10027). Emission lifetimes were measured at 25 °C using a HORIBA FluoroCube time-correlated single-photon counting system. The excitation light source was a NanoLED-560 (379 nm, <200 ps; 401 nm, <200 ps; 456 nm, <1.3 ns, or 510 nm, <100 ps). All measurements were performed in a quartz cubic cell (1 cm optical path length). The absorbances were adjusted to 0.1 at λex; otherwise, the photoluminescence responses were corrected to the number of absorbed photons in the case of using various excitation wavelengths of a single solution. Prior to measurements, the solutions were degassed using the pump–thaw–freeze method.
Syntheses
Synthesis of [Ring-Ru1]5+
[Ru(bpy)2(4C2)](PF6)2
Ru(bpy)2Cl2·2H2O (150 mg, 0.29 mmol) and 4C2 (420 mg, 1.16 mmol) were refluxed in MeOH (25 mL) overnight. The solvent was evaporated, and the resultant crude product was dissolved in H2O (30 mL) and filtered to remove the excess of 4C2. Solid NH4PF6 (excess) was added to the filtrate; extraction was performed with CH2Cl2 (2 × 50 mL), and the combined organic layers were evaporated to dryness. The crude solid was purified by column chromatography (alumina, CH2Cl2 and MeCN–CH2Cl2 8:1), yielding 280 mg of a red solid (90%). ESI-MS (CH3CN): m/z 389 [M–2PF6–]2+.
fac-[Re(CO)3Br(μ2-4C2)Ru(bpy)2](PF6)2
[Ru(bpy)2(4C2)](PF6)2 (280 mg, 0.26 mmol) and Re(CO)5Br (117 mg, 0.29 mmol) were refluxed in MeOH (40 mL) for 8 h. The solvent was evaporated, and the resultant crude product was purified by ion-exchange chromatography (SP Sephadex C-25, MeCN–H2O 1:1 containing NH4PF6 0–10 mM). After evaporation of the MeCN portion, the precipitated solid was collected by filtration, washed with H2O and EtOH, and then dried to furnish 140 mg of a red solid (38%). ESI-MS (CH3CN): m/z 564 [M–2PF6–]2+.
fac-[Re(CO)3(η1-dppph)(μ2-4C2)Ru(bpy)2](PF6)2(CF3SO3)
fac-[Re(CO)3Br(μ2-4C2)Ru(bpy)2](PF6)2 (140 mg, 0.1 mmol) was dissolved in anhydrous CH2Cl2 (25 mL); silver trifluoromethanesulfonate (AgOTf, 25 mg, 0.1 mmol) was added in one portion, and the mixture was gently refluxed for 3 h until the starting compound was consumed, as monitored by ESI-MS (m/z 364 Re(CO)3(CH3CN)(μ2-4C2)Ru(bpy)2]3+). The mixture was filtered through a pad of Celite and diluted with dry CH2Cl2 to a total volume of 100 mL; dppph (223 mg, 0.5 mmol) was added, and the resultant mixture was heated at 35 °C for 2 days. The mixture was evaporated and redissolved in MeCN, filtered to remove the excess dppph, and evaporated, affording a crude red solid that was used in the next step without further purification. ESI-MS (CH3CN): m/z 499 [M–2PF6––OTf–]3+.
[Re(4dmb)(CO)3(μ2-dppph)Re(4dmb)(CO)2(μ2-dppph)Re{(μ2-4C2)Ru(bpy)2}(CO)3](PF6)5 ([L3(4dmb)(trans-CO)2–Ru(4dmb,bpy2))]5+
[L2ph(4dmb)](OTf)2 (100 mg, 0.06 mmol) was irradiated in degassed CH2Cl2 (150 mL) for 35 min. After evaporation of the solvent, the crude red solid was dissolved in CH2Cl2 (25 mL) together with the crude fac-[Re(CO)3(η1-dppph)(μ2-4C2)Ru(bpy)2]3+ from the previous step and the solution was stirred at room temperature (rt) for 3 days. The solvent was evaporated, and the crude material was purified by RSEC. The fraction containing the product was collected, evaporated, and portioned between CH2Cl2 and NH4PF6 aqueous solution. The organic layer was washed once more with aqueous NH4PF6 solution, dried over Na2SO4, and evaporated to yield 60 mg of red crystals (28%, based on [L2ph(4dmb)]2+).31P NMR (161 MHz, CD3CN): δ 22.6, 21.5, 17.6, 17.3 ppm. FT-IR (CH3CN): νCO 2040, 1954, 1939, 1924, 1869 cm–1. ESI-MS (CH3CN): m/z 565 [M–5PF6–]5+, 742 [M–4PF6–]4+.
[–{Re(4dmb)(CO)2(μ2-dppph)}Re(4dmb)(CO)2(μ2-dppph)Re{(μ2-4C2)Ru(bpy)2}(CO)2–](PF6)5 ([Ring-Ru1]5+)
[L3(4dmb)(trans-CO)2–Ru(4dmb,bpy2)]5+ (60 mg, 0.017 mmol) was dissolved in acetone (15 mL); Me3NO (3 mg 0.04 mmol) was added in one portion, and the resultant solution was stirred at rt for 1 h. Afterward, dppph (8 mg, 0.018 mmol) was added and the resultant mixture was gently refluxed for 1 day. The solvent was evaporated, and the crude residue was purified by RSEC. The fraction containing the product was collected, evaporated, and portioned between CH2Cl2 and NH4PF6 aqueous solution. The organic layer was washed once more with aqueous NH4PF6 solution, dried over Na2SO4, and evaporated. Final recrystallization from EtOH–CH2Cl2 afforded 20 mg of bright-red crystals (30%).1H NMR (400 MHz, CD3CN): δ 8.60 (s, 1H, 4C2(Ru)-3), 8.54 (s, 1H, 4C2(Ru)-3′), 8.49 (m, 4H, bpy-3,3′), 8.22 (br s, 12H, P–C6H4–P), 8.06 (s, 1H, 4C2(Re)-3), 8.05–7.95 (m, 5H, 4C2(Re)-3′ + bpy-4,4′), 7.93 (d, J = 5.6 Hz, 1H, 4C2(Re)-6), 7.86 (s, 2H, 4dmba-3,3′), 7.84 (s, 2H, 4dmbb-3,3′), 7.83 (d, J = 6 Hz, 2H, 4dmba-6,6′), 7.80 (d, J = 6 Hz, 2H, 4dmbb-6,6′), 7.74 (d, J = 6 Hz, 3H, 4C2(Re)-6′ + bpya-6,6′), 7.70 (ddd, J = 4.6, 1.2 Hz, 2H, bpyb-6,6′), 7.63 (d, J = 5.6 Hz, 1H, 4C2(Ru)-6), 7.55 (d, J = 5.6 Hz, 1H, 4C2(Ru)-6′), 7.42–7.34 (m, 4H, bpy-5,5′), 7.30 (dd, J = 5.6, 1.6 Hz, 1H, 4C2(Ru)-5), 7.26 (dd, J = 6, 1.2 Hz, 1H, 4C2(Ru)-5′), 7.25–7.17 (m, 12H, Ph-p), 7.16–7.05 (m, 24H, Ph-m), 7.03–6.87 (br m, 24H, Ph-o), 6.66 (d, J = 5.6, 1.6 Hz, 1H, 4C2(Re)-5), 6.63 (dd, J = 6, 1.6 Hz, 1H, 4C2(Re)-5′), 6.59 (dd, J = 6 Hz, 4H, 4dmb-5,5′), 3.04–2.90 (m, 4H, 4C2–CH2–CH2), 2.57 (s, 3H, 4C2(Ru)–CH3), 2.36 (s, 3H, 4C2(Re)–CH3), 2.34 (s, 12H, 4dmb–CH3) ppm. 31P NMR (161 MHz): δ 22.2 (2P), 22.1 (4P) ppm. FT-IR (CH3CN): νCO 1936, 1877, 1867(sh) cm–1. ESI-MS (CH3CN): m/z 643 [M–5PF6–]5+, 840 [M–4PF6–]4+. HRMS (ESI-TOFMS): m/z [M–5PF6–]5+ calcd for C164H134N12O6P6Re3Ru, 643.1338; found, 643.1354; [M–4PF6–]4+ calcd for C164H134F6N12O6P7Re3Ru, 840.1583; found 840.1608.
Synthesis of [Ring-Ru2]5+
[Ru(5dmb)2(5C2)](PF6)2
Ru(5dmb)2Cl2·2H2O (160 mg, 0.28 mmol) and 5C2 (410 mg, 1.12 mmol) were refluxed in MeOH (30 mL) overnight. The solvent was evaporated, and the resulting crude product was dissolved in H2O (40 mL) and filtered to remove the excess of 5C2. Solid NH4PF6 (excess) was added to the filtrate and extracted with CH2Cl2 (2 × 50 mL), and the combined organic layers were evaporated to dryness. The crude solid was purified by column chromatography (alumina, CH2Cl2 and MeCN–CH2Cl2 8:1 v/v), yielding 268 mg of a red solid (85%). ESI-MS (CH3CN): m/z 418 [M–2PF6–]2+.
fac-[Re(CO)3Br(μ2-5C2)Ru(5dmb)2](PF6)2
[Ru(5dmb)2(5C2)](PF6)2 (268 mg, 0.24 mmol) and Re(CO)5Br (107 mg, 0.26 mmol) were refluxed in MeOH (40 mL) for 10 h. The solvent was evaporated, and the resultant crude product was purified by ion-exchange chromatography (SP Sephadex C-25, MeCN–H2O 1:1 containing NH4PF6 0–10 mM). After evaporation of the MeCN portion, the precipitated solid was collected by filtration, washed with H2O and EtOH, and dried to furnish 190 mg of a red solid (54%). ESI-MS (MeCN): m/z 593 [M–2PF6–]2+.
fac-[Re(CO)3(η1-dppph)(μ2-5C2)Ru(5dmb)2](PF6)2(CF3SO3)
fac-[Re(CO)3Br(μ2-5C2)Ru(5dmb)2](PF6)2 (190 mg, 0.13 mmol) was dissolved in anhydrous CH2Cl2 (30 mL); AgOTf (33 mg, 0.13 mmol) was added in a single portion, and the resultant mixture was gently refluxed for 2 h until the starting compound was consumed and Re(CO)3(CH3CN)(μ2-5C2)Ru(5dmb)2]3+ was formed, as monitored by ESI-MS (m/z 383). The mixture was filtered through a pad of Celite and diluted with dry CH2Cl2 to a total volume of 100 mL; dppph (290 mg, 0.65 mmol) was added, and the resultant mixture was heated at 35 °C for 2 days. The mixture was evaporated and redissolved in MeCN, filtered to remove the excess of dppph, and evaporated, affording a crude red solid that was used in the next step without further purification. ESI-MS (CH3CN): m/z 518 [M–2PF6––OTf–]3+.
[Re(5dmb)(CO)3(μ2-dppph)Re(5dmb)(CO)2(μ2-dppph)Re{(μ2-5C2)Ru(5dmb)2}(CO)3](PF6)5 ([L3(5dmb)(trans-CO)2–Ru(5dmb)3)]5+)
[L2ph(5dmb)](OTf)2 (120 mg, 0.073 mmol) was irradiated by a 500 W high-pressure mercury lamp with a uranium glass filter in degassed CH2Cl2 (200 mL) for 25 min. After evaporation of the solvent, the crude red solid was dissolved in CH2Cl2 (30 mL) together with the crude fac-[Re(CO)3(η1-dppph)(μ2-5C2)Ru(5dmb)2]3+ from the previous step, and the resultant solution was stirred at rt for 3 days. The solvent was evaporated, and the crude material was purified using RSEC. The fraction containing the product was collected, evaporated, and portioned between CH2Cl2 and NH4PF6 aqueous solution. The organic layer was washed once more with aqueous NH4PF6 solution, dried over Na2SO4, and evaporated to yield 43 mg of dark orange crystals (16%, based on [L2ph(5dmb)]2+). ESI-MS (CH3CN): m/z 576 [M–5PF6–]5+, 757 [M–4PF6–]4+.
[–Re(5dmb)(CO)2(μ2-dppph)Re(5dmb)(CO)2(μ2-dppph)Re{(μ2-5C2)Ru(5dmb)2}(CO)2–](PF6)5 ([Ring-Ru2]5+)
[L3(5dmb)(trans-CO)2–Ru(5dmb)3]5+ (43 mg, 0.012 mmol) was dissolved in acetone (10 mL); Me3NO (2 mg 0.025 mmol) was added in a single portion, and the resultant solution was stirred at rt for 1 h. Afterward, dppph (6 mg, 0.013 mmol) was added and the resultant mixture was gently refluxed for 2 days. The solvent was evaporated, and the crude residue was purified using RSEC. The fraction containing the product was collected, evaporated, and portioned between CH2Cl2 and NH4PF6 aqueous solution. The organic layer was washed once more with aqueous NH4PF6 solution, dried over Na2SO4, and evaporated. Final recrystallization from EtOH–CH2Cl2 afforded 18 mg of bright orange crystals (38%).1H NMR (400 MHz, CD3CN): δ 8.41–8.29 (m, 12H, 5dmb(Ru)-3,3′ + 5C2(Ru)-3,3′ + 5dmb(Re)-3,3′ + 5C2(Re)-3,3′), 7.94–7.85 (m, 11H, 5dmb(Ru)-4,4′ + 5C2(Ru)-4,4′) + 5dmb(Re)-4,4′) + 5C2(Re)-4′), 7.73 (dd, J = 8.4, 1.5 Hz, 1H, 5C2(Re)-4), 7.63 (s, 1H, 5C2(Re)-6), 7.54–7.41 (set of br s, 23H, 5dmb(Ru)-6,6′ + 5C2(Ru)-6,6′ + 5dmb(Re)-6,6′ + 5C2(Re)-6′ + P–C6H4–P), 7.25–7.18 (m, 12H, Ph-p), 7.15–7.09 (m, 24H, Ph-m), 7.05–6.87 (br m, 24H, Ph-o), 2.42–2.27 (m, 4H, 5C2-CH2–CH2), 2.25–2.22 (set of s, 12H, 5dmb(Ru)–CH3), 2.14 (s, 3H, 5C2(Ru)–CH3), 1.88 (s, 3H, 5dmb(Re)–CH3), 1.87 (s, 3H, 5dmb(Re)–CH3), 1.84 (s, 6H, 5dmb(Re)–CH3) ppm. 31P NMR (161 MHz): δ 23.4 (4P), 23.2 (2P) ppm. FT-IR (CH3CN): νCO 1938, 1879, 1869(sh) cm–1. ESI-MS (CH3CN): m/z 654 [M–5PF6–]5+, 854 [M–4PF6–]4+. HRMS (ESI-TOFMS): m/z [M–5PF6–]5+ Calcd for C168H142N12O6P6Re3Ru, 654.3463; found, 654.3484; [M–4PF6–]4+ calcd for C168H142F6N12O6P7Re3Ru, 854.1740; found 854.1796.
Synthesis of [Ring-Ru3]5+
[R3et(5dmb2,Brbpy)]3+ (10 mg, 3.4 μmol), [Ru(dmb)2(allyl-4dmb)](PF6)2 (6.6 mg, 6.8 μmol), Pd(OAc)2 (0.46 mg, 2.0 μmol), and AcONa (1.4 mg, 17 μmol) were dissolved in degassed MeCN (0.5 mL). The solution was heated at 65 °C for 2 days. After the solution cooled to rt, the precipitated Pd black was removed by filtration through a Millex LG 0.20 μm filter. The solvent was evaporated, and then a fresh MeCN solution containing Pd(OAc)2 (0.46 mg, 2.0 μmol) and AcONa (1.4 mg, 17 μmol) was added to the residue. The solution was heated at 65 °C for 1 d. This process was repeated once more with additional heating for 2 days. The obtained crude product was purified by RSEC, and the fraction containing the product was evaporated. The residue was dissolved in CH2Cl2 and twice washed with water containing NH4PF6. After evaporation of the organic layer, the obtained orange–red solid was dissolved in MeOH, and a concentrated MeOH solution of NH4PF6 was added. Some water was added to the solution, and an aliquot of MeOH was evaporated under reduced pressure. After product precipitation, an orange–red solid was collected, washed with water and Et2O, and dried under vacuum to afford 5.2 mg (40%) of product. 1H NMR (400 MHz, acetone-d6): δ 8.74 (s, 2H), 8.67 (d, J = 6.8 Hz, 1H), 8.64 (m, 3H), 8.61(s, 2H), 8.38 (s, 2H), 8.21 (s, 2H), 7.96–7.78 (m, 17H), 7.64–7.58 (m, 6H), 7.39–7.11 (m, 40H), 7.03–6.82 (m, 20H), 6.61 (m, 1H), 6.57 (m, 1H), 2.98–2.87 (m, 12H, P–CH2–CH2–P), 2.55–2.51 (m, 19H, – CH2–CH2–CH = CH–, 4dmb-CH3), 2.18 (s, 6H, 5dmb-CH3), 2.14 (s, 6H, 5dmb-CH3) ppm. 31P NMR (161 MHz, acetone-d6): δ 13.6 (4P), 13.5 (2P) ppm. FT-IR (CH3CN): νCO 1949(sh), 1932, 1880, 1867, 1851 cm–1. ESI-MS (CH3CN): m/z 627 [M–5PF6–]5+, 821 [M–4PF6–]4+). HRMS (ESI-TOFMS): m/z [M–5PF6–]5+ Calcd for C157H142N12O6P6Re3Ru 627.7470, Found 627.7444; [M–4PF6–]4+ Calcd for C157H142F6N12O6P7Re3Ru 820.9248; Found 820.9290.
Synthesis of [Ring3]3+
fac-[Re(OHbpy)(CO)3(η1-dppet)](CF3SO3)
fac-[Re(OHbpy)(CO)3OTf] (101 mg, 0.16 mmol) and dppet (248 mg, 0.62 mmol) was dissolved in degassed CH2Cl2 (50 mL). The solution was refluxed for 1 d. After the solution cooled to rt, the solvent was removed to yield a yellow solid. Some degassed MeOH was added, and unreacted dppet was removed by filtration. The combined MeOH solutions were evaporated, and the resultant crude product was purified twice by column chromatography with different eluents (silica gel, CH2Cl2 and MeOH–CH2Cl2 1:100 v/v) to afford 77 mg (23%) of yellow solid. ESI-MS (CH3CN): m/z 869 [M–OTf–]+.
[Re(5dmb)(CO)3(μ2-dppet)Re(5dmb)(CO)2(μ2-dppet)Re(OHbpy)(CO)3](PF6)3 ([L3et(5dmb2,OHbpy)]3+)
A solution of [L2et(5dmb)]2+ (187 mg, 0.12 mmol) in degassed CH2Cl2–acetone (1:1 v/v, 200 mL) was irradiated for 30 min. After evaporation of the solvent, the residue was dissolved in degassed acetone (60 mL) together with fac-[Re(OHbpy)(CO)3(η1-dppet)](OTf) (77 mg, 0.08 mmol), and refluxed for 20 h. The solvent was removed under vacuum, and the residue was purified by ion-exchange chromatography (CM Sephadex C-25, MeCN–H2O 1:1 containing NH4PF6 (0–8 mM)). After evaporation of the MeCN portion, a yellow solid was collected by filtration, washed with H2O, and dried to yield 151 mg (77%) of product. ESI-MS (CH3CN): m/z 716 [M–3PF6–]3+.
[−{Re(5dmb)(CO)2(μ2-dppet)}2Re(vbpy)(CO)2(μ2-dppet)−](PF6)3 ([Ring3]3+)
[L3et(5dmb2,OHbpy)]3+ (150 mg, 59 μmol) was dissolved in acetone (20 mL), and Me3NO (9 mg, 0.12 mmol) was added to the solution, which was then refluxed for 30 min. After a second loading of Me3NO (1.5 mg, 0.02 mmol), the solution was further refluxed for 1 h. To this solution, a degassed acetone solution (60 mL) containing dppet (26 mg, 65 μmol) was added, and the resultant mixture was refluxed for 1 d. After the solution cooled to rt, the solvent was removed under reduced pressure, and the orange residue was redissolved in MeCN (25 mL); TsCl (130 mg, 0.68 mmol) and trimethylamine (2 mL) were then added. The resultant solution was heated at 75 °C for 1 d. After the solution cooled to rt, the solvent was removed under vacuum and the crude product was purified by RSEC. The fraction containing the product was evaporated. The residue was dissolved in CH2Cl2 and twice washed with water containing NH4PF6. After evaporation of the organic layer, the obtained yellow solid was dissolved in MeOH and a concentrated MeOH solution of NH4PF6 was added. Some water was added to the solution, and an aliquot of MeOH was evaporated under reduced pressure. After product precipitation, a yellow solid was collected, washed with water and Et2O, and dried under vacuum to yield 62 mg (36%, three steps). 1H NMR (400 MHz, acetone-d6): δ 8.82 (d, J = 5.6 Hz, 1H), 8.63 (d, J = 6.0 Hz, 1H), 8.29 (s, 4H, 5dmb-6,6′), 8.04 (d, J = 8.0 Hz, 1H), 7.98 (s, 1H), 7.91 (d, J = 8.6 Hz, 4H, 5dmb-4,4′), 7.73 (m, 2H), 7.61 (d, J = 8.6 Hz, 4H, 5dmb-3,3′), 7.55–7.13 (m, 41H), 6.93–6.84 (m, 20H), 6.75 (dd, J = 10.8, 17.4 Hz, 1H), 6.23 (d, J = 17.4 Hz, 1H), 5.70 (d, J = 10.8 Hz, 1H), 3.00–2.96 (m, 12H, P–CH2–CH2–P), 2.18 (s, 6H, 5dmb-CH3) ppm. 31P NMR (161 MHz, acetone-d6): δ 13.4 (4P), 13.2 (2P). FT-IR (CH3CN): νCO 1950(sh), 1932, 1880, 1867, 1853 cm–1. ESI-MS (CH3CN): m/z 824 [M–3PF6–]3+. HRMS (ESI-TOFMS): m/z [M–3PF6–]3+ calcd for C120H106N6O6P6Re3, 824.1761; found, 824.1786.
Acknowledgments
This work was supported by JSPS KAKENHI Grant Numbers JP17K14526 and JP17H01198 and JST CREST Grant Number JPMJCR13L1.
Supporting Information Available
The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/jacsau.0c00114.
Synthetic scheme of [Ring-Ru2]5+, [R3et(5dmb2,Brbpy)]3+, and [Ring3]3+; ESI-MS spectra of the reaction solution for decarbonylation of [L3(4dmb)(trans-CO)2-Ru(4dmb,bpy2)]5+ before and after addition of Me3NO; SEC chromatogram of the reaction solution after cyclization of [L3(4dmb)-Ru(4dmb,bpy2)]5+ with dppph; SEC chromatogram of the crude reaction mixture after Mizoroki–Heck heterocoupling; emission spectrum of 1:1 mixture of [Ring1]3+ and [Ru1]2+; ESI-mass spectrum of a reaction solution before the dehydration reaction containing [−{Re(5dmb)(CO)2(μ2-dppet)}2Re(OHbpy)(CO)2(μ2-dppet)−](PF6)3; wavelength dependence of the pre-exponential factors observed in [Ring-Ru3]5+; transient emission spectrum of [Ring-Ru3]5+ recorded after 800 ns of excitation and simulation spectra; electrochemical properties of model complexes (PDF)
Author Present Address
# J.R.: Teva Czech Industries s.r.o., Ostravska 29, 747 70 Opava, Czech Republic.
Author Contributions
‡ Y.Y. and J.R. contributed equally.
The authors declare no competing financial interest.
Supplementary Material
References
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