Excited-State Relaxation in Luminescent Molybdenum(0) Complexes with Isocyanide Chelate Ligands

: Diisocyanide ligands with a m -terphenyl backbone provide access to Mo 0 complexes exhibiting the same type of metal-to-ligand charge transfer (MLCT) luminescence as the well-known class of isoelectronic Ru II polypyridines. The luminescence quantum yields and lifetimes of the homoleptic tris(diisocyanide) Mo 0 complexes depend strongly on whether methyl- or tert -butyl substituents are placed in α -position to the isocyanide groups. The bulkier tert -butyl substituents lead to a molecular structure in which the three individual diisocyanides ligated to one Mo 0 center are interlocked more strongly into one another than the ligands with the sterically less demanding methyl substituents. This rigidiﬁcation limits the distortion of the complex in the emissive excited-state, causing a decrease of the nonradiative relaxation rate by one order of magnitude. Compared to Ru II polypyridines, the molecular distortions in the luminescent 3 MLCT state relative to the electronic ground state seem to be smaller in the Mo 0 complexes, presumably due to delocalization of the MLCT-excited electron over greater portions of the ligands. Temperature-dependent studies indicate that thermally activated nonradiative relaxation via metal-centered excited states is more signiﬁcant in these homoleptic Mo 0 tris(diisocyanide) complexes than in [Ru(2,2 (cid:48) -bipyridine) 3 ] 2 + .


Introduction
Hexacarbonyl complexes of Cr 0 , Mo 0 , and W 0 are prototypical coordination compounds obeying the 18-electron rule with a low-spin d 6 valence electron configuration. Isocyanides (CNR) are formally isoelectronic with CO, and consequently it is unsurprising that hexakis(isocyanide) complexes of the abovementioned d 6 metals as well as some heteroleptic complexes comprising both CO and CNR ligands have long been known [1][2][3][4][5][6][7]. The isocyanides are less π-accepting than CO, yet the ligand field remains very strong (even in the Cr 0 complexes), and all 6 d-electrons are paired in the t 2g -set of d-orbitals, which represent the HOMO in octahedral symmetry. In arylisocyanides, there is some π-conjugation between the C≡N group and the aryl π-system, and consequently antibonding ligand-based orbitals become the LUMO in hexakis(arylisocyanide) complexes of Cr 0 , Mo 0 , and W 0 [1,2]. The resulting electronic structure with a metal-based HOMO and a ligand-centered LUMO is closely related to that encountered for isoelectronic Ru II and Os II polypyridine complexes. Thus, in analogy to this well-known class of precious metal-based complexes, arylisocyanide complexes of Cr 0 , Mo 0 , and W 0 have energetically low-lying metal-to-ligand charge transfer (MLCT) absorptions. An early investigation already reported luminescence from a 3 MLCT state in W 0 arylisocyanide complexes [2], and more recent work demonstrated that high luminescence quantum yields and long excited-state lifetimes are achievable by optimizing the ligand design [8][9][10]. Moreover, these W 0 lifetimes are achievable by optimizing the ligand design [8][9][10]. Moreover, these W 0 complexes with monodentate arylisocyanide ligands are very strong photoreductants, capable, for example, of reducing anthracene to its radical anion form. Many different kinds of metal complexes with isocyanide ligands have been explored over the past few decades [11][12][13][14][15], but metals with the d 6 or d 10 electron configurations are unique in their ability to show luminescence from a 3 MLCT excited state.
Whilst structurally more flexible, multidentate isocyanide chelate ligands had been known for some time [16], we found that chelating diisocyanide ligands based on a m-terphenyl backbone permit the synthesis of homoleptic tris(diisocyanide) complexes of Cr 0 and Mo 0 that luminesce from 3 MLCT excited states (Figure 1) [17]. The molecular and the electronic structures of these compounds are reminiscent of Fe II and Ru II polypyridine complexes, which have been investigated extensively in the past. Until now, no convincing case of steady-state MLCT luminescence from a Fe II complex has been reported despite significant advances in extending their 3 MLCT lifetimes in recent years [18][19][20][21][22][23]; hence, our Cr 0 complex currently seems to be the only example of a first-row d 6 -metal complex showing MLCT luminescence in solution at room temperature under steady-state photo-irradiation [24]. The Mo 0 diisocyanide complexes are not only emissive, but they can furthermore be employed in photoredox catalysis of thermodynamically challenging reductions, which cannot be performed with more widely known photoreductants such as fac-[Ir(ppy)3] (ppy = 2-phenylpyridine) [25]. Thus, the Mo 0 diisocyanide complexes represent Earth-abundant alternatives to precious-metal based luminophores and photoredox catalysts, and in our view, there is interesting fundamental photophysics and photochemistry to be explored in this field [26].  [17,24,25,27].
Recently we reported that the [Mo(L tBu )3] complex exhibits much more favorable photophysical properties than the closely related [Mo(L Me )3] compound, and we demonstrated that [Mo(L tBu )3] is more widely applicable in photoredox catalysis due to greater photo-robustness [27]. The present article focuses on the origin of the photophysical differences between these two complexes and attempts to identify possible reasons for the very favorable luminescence behavior of [Mo(L tBu )3] in comparison to [Ru(bpy)3] 2+ (bpy = 2,2′-bipyridine) and related Ru II polypyridines. Herein, we provide the first analysis of relevant 3 MLCT excited-state distortions in tris(diisocyanide) Mo 0 complexes, and new temperature-dependent luminescence lifetime data give insight into thermally activated nonradiative relaxation via metal-centered excited states.  [17,24,25,27].
Recently we reported that the [Mo(L tBu ) 3 ] complex exhibits much more favorable photophysical properties than the closely related [Mo(L Me ) 3 ] compound, and we demonstrated that [Mo(L tBu ) 3 ] is more widely applicable in photoredox catalysis due to greater photo-robustness [27]. The present article focuses on the origin of the photophysical differences between these two complexes and attempts to identify possible reasons for the very favorable luminescence behavior of [Mo(L tBu ) 3 ] in comparison to [Ru(bpy) 3 ] 2+ (bpy = 2,2 -bipyridine) and related Ru II polypyridines. Herein, we provide the first analysis of relevant 3 MLCT excited-state distortions in tris(diisocyanide) Mo 0 complexes, and new temperature-dependent luminescence lifetime data give insight into thermally activated nonradiative relaxation via metal-centered excited states.

Results and Discussion
The [Mo(L Me ) 3 ] and [Mo(L tBu ) 3 ] complexes differ only by the substituents in orthoand para-position to the isocyanide groups, yet their photoluminescence properties are very disparate (Table 1) [27]. Whilst the emissive excited state is of 3 MLCT-type in both cases, the luminescence quantum yield (ϕ em ) for [Mo(L tBu ) 3 ] (in de-aerated solution at 20 • C) is an order of magnitude higher than for [Mo(L Me ) 3 ] under identical conditions. Similarly, the 3 MLCT lifetime (τ) is roughly a factor of 10 longer for [Mo(L tBu ) 3 ] compared to [Mo(L Me ) 3 ]. (In a prior study we already noted that the tert-butyl decorated complex exhibits bi-exponential luminescence decays and transient absorption kinetics in all solvents investigated, and this is likely due to conformational equilibria in solution [27]). The parallel combined trends in luminescence quantum yields and lifetimes indicate that the rate for nonradiative 3 MLCT relaxation (k nr ) decreases by circa a factor of 10 between [Mo(L Me ) 3 ] and [Mo(L tBu ) 3 ], whereas the radiative relaxation rate (k r ) remains similar. Using Equations (1) and (2), this effect can be quantified and the resulting rate constants can be compared to [Ru(dmb) 3 ] 2+ (dmb = 4,4 -dimethyl-2,2 -bipyridine) [28], which is an isoelectronic analogue of our molybdenum complexes ( Table 2). τ −1 = k r + k nr (1) The radiative rate constants of the two Mo 0 complexes are roughly a factor of 2 larger than for the Ru II complex. This is in line with more strongly absorbing MLCT features for [Mo(L Me ) 3 ] and [Mo(L tBu ) 3 ] (with ε max up to 27,000 M −1 cm −1 ) compared to [Ru(dmb) 3 ] 2+ (ε max ≈ 16,500 M −1 cm −1 , ε max is the extinction coefficient at the 1 MLCT absorption band maximum) [27]. However, it should be kept in mind that these are 1 MLCT absorption bands whereas the k r values are for 3 MLCT relaxation. As anticipated above, k nr is indeed 10 times smaller for [Mo(L tBu ) 3 ] than for [Mo(L Me ) 3 ] (last column in Table 2). In principle, a slower rate for nonradiative relaxation in the tert-butyl decorated complex is in line with the energy gap law [29], because this complex emits at somewhat shorter wavelengths (λ max = 585 nm, Table 1) than the methyl-substituted congener (λ max = 607 nm, Table 1). Yet, the factor of 10 difference in k nr seems large in relation to the difference in 3 MLCT excited-state energies (ca. 600 cm −1 when using the emission band maxima as a proxy).
Mere consideration of energy gaps is a very simplified view, and it is clear that the molecular distortions occurring in an excited state have a big influence on the rates for nonradiative relaxation [29].
The analysis of luminescence band shapes can provide deeper insight into excited-state distortions and nonradiative relaxation [30], and consequently it seemed meaningful to perform such analyses with the emission spectra of [Mo(L Me ) 3 ] and [Mo(L tBu ) 3 ] ( Figure 2); such analyses had not been performed before on our Mo 0 complexes. Ideally, vibrational fine structure would directly indicate the relevant distortion modes [31], but the lack thereof is common for MLCT luminescence and does not preclude emission band shape analysis [28]. ; such analyses had not been performed before on our Mo 0 complexes. Ideally, vibrational fine structure would directly indicate the relevant distortion modes [31], but the lack thereof is common for MLCT luminescence and does not preclude emission band shape analysis [28]. Suitable models describe the emission spectrum as a superposition of vertical transitions between the electronically excited state and the ground state [32]. The intensity of each transition is determined by the Franck-Condon factor, which quantifies the overlap between the vibrational wave functions of the initial and the final state ( Figure 3a). In this picture, the integral over all relevant vibronic transitions then makes up the experimentally observable emission band shape. Whilst several vibrations can in principle couple to an electronic transition [33], it is common to use single configurational coordinate models in which only one (weighted average) vibrational mode is considered, particularly when vibrationally unresolved (MLCT) luminescence spectra (at room temperature) are analyzed. In this limit, the emission intensity I(ν) at a given energy ν is described by Equation (3), where ħ•ωM is the average energy of the vibrational mode that couples to the luminescence transition [28,34].
E0 is the difference between the zero-point energies of the ground and the excited state, whereas SM is the Huang-Rhys parameter describing the extent of molecular distortion occurring between the two respective electronic states. The term ν1/2 is the homogeneously broadened bandwidth associated with the vibronic transitions. For the simulation of the spectra, the quantum number νM runs over the number of relevant vibrational levels of ħ•ωM, which serve as final states in the electronic ground state. Suitable models describe the emission spectrum as a superposition of vertical transitions between the electronically excited state and the ground state [32]. The intensity of each transition is determined by the Franck-Condon factor, which quantifies the overlap between the vibrational wave functions of the initial and the final state ( Figure 3a). In this picture, the integral over all relevant vibronic transitions then makes up the experimentally observable emission band shape. Whilst several vibrations can in principle couple to an electronic transition [33], it is common to use single configurational coordinate models in which only one (weighted average) vibrational mode is considered, particularly when vibrationally unresolved (MLCT) luminescence spectra (at room temperature) are analyzed. In this limit, the emission intensity I(ν) at a given energy ν is described by Equation (3), whereh·ω M is the average energy of the vibrational mode that couples to the luminescence transition [28,34].
E 0 is the difference between the zero-point energies of the ground and the excited state, whereas S M is the Huang-Rhys parameter describing the extent of molecular distortion occurring between the two respective electronic states. The term ∆ν 1/2 is the homogeneously broadened bandwidth associated with the vibronic transitions. For the simulation of the spectra, the quantum number ν M runs over the number of relevant vibrational levels ofh·ω M , which serve as final states in the electronic ground state. For the simulations in Figure 2, we summed over νM values from 0 to 3 and adapted E0, SM and ħ•ωM to match the experimentally observed emission spectra as closely as possible. The outcomes are included in Figure 2 as dotted gray traces, and the fitting parameters are summarized in Table 3 along with those reported previously for the [Ru(dmb)3] 2+ complex [28]. The experimental emission spectra are somewhat affected by an instrumental artefact at 15,400 cm −1 [24], which renders the simulations on the low energy side of the luminescence bands imperfect. Of key interest in this analysis are the Huang-Rhys parameter (SM) and the (average) vibrational frequency (ħ•ωM). The respective values for the [Ru(dmb)3] 2+ complex are quite typical for Ru II and Os II polypyridines [28,30,32,34,35]. The vibrational frequency ħ•ωM of ca. 1300 cm −1 for this class of compounds is usually interpreted as a dominance of polypyridine ring stretching modes in defining the relevant excited-state distortion of the emissive 3 MLCT state relative to the electronic ground state. Huang-Rhys parameters in the range of 0.6 to 1.2 are very common for Ru II and Os II polypyridines [28,30,32,34]. By contrast, our isoelectronic Mo 0 complexes yield markedly lower Huang-Rhys parameters combined with a significantly higher average vibrational frequency (Table 3). Specifically, our simulations provide ħ•ωM values near 1600 cm −1 , suggesting that isocyanide CN stretch vibrations (ca. 1950 cm −1 ) [25,27] contribute substantially to the weighted average of all modes that are responsible for the excited-state distortion, presumably along with lower frequency aryl ring stretch modes. This interpretation is compatible with recent computational work on W 0 complexes with monodentate arylisocyanide ligands, which demonstrated that distortion along a normal coordinate involving the CN stretch is important [10]. Furthermore, previous work discussed the coupling of the CN group to the aromatic π-system of arylisocyanides [1,2], and it For the simulations in Figure 2, we summed over ν M values from 0 to 3 and adapted E 0 , S M and h·ω M to match the experimentally observed emission spectra as closely as possible. The outcomes are included in Figure 2 as dotted gray traces, and the fitting parameters are summarized in Table 3 along with those reported previously for the [Ru(dmb) 3 ] 2+ complex [28]. The experimental emission spectra are somewhat affected by an instrumental artefact at 15,400 cm −1 [24], which renders the simulations on the low energy side of the luminescence bands imperfect. Of key interest in this analysis are the Huang-Rhys parameter (S M ) and the (average) vibrational frequency (h·ω M ). The respective values for the [Ru(dmb) 3 ] 2+ complex are quite typical for Ru II and Os II polypyridines [28,30,32,34,35]. The vibrational frequencyh·ω M of ca. 1300 cm −1 for this class of compounds is usually interpreted as a dominance of polypyridine ring stretching modes in defining the relevant excited-state distortion of the emissive 3 MLCT state relative to the electronic ground state. Huang-Rhys parameters in the range of 0.6 to 1.2 are very common for Ru II and Os II polypyridines [28,30,32,34]. By contrast, our isoelectronic Mo 0 complexes yield markedly lower Huang-Rhys parameters combined with a significantly higher average vibrational frequency (Table 3). Specifically, our simulations provideh·ω M values near 1600 cm −1 , suggesting that isocyanide C≡N stretch vibrations (ca. 1950 cm −1 ) [25,27] contribute substantially to the weighted average of all modes that are responsible for the excited-state distortion, presumably along with lower frequency aryl ring stretch modes. This interpretation is compatible with recent computational work on W 0 complexes with monodentate arylisocyanide ligands, which demonstrated that distortion along a normal coordinate involving the C≡N stretch is important [10]. Furthermore, previous work discussed the coupling of the C≡N group to the aromatic π-system of arylisocyanides [1,2], and it seems plausible that any distortion along the C≡N coordinate will automatically also affect the aromatic π-system and associated ring stretching vibrations. On this basis,h·ω M values near 1600 cm −1 for the Mo 0 complexes can be rationalized.
The Huang-Rhys parameters obtained for [Mo(L Me ) 3 ] and [Mo(L tBu ) 3 ] are considerably lower than that for [Ru(dmb) 3 ] 2+ (Table 3) and for many other Ru II polypyridines [35]. This is a somewhat surprising finding, which presumably reflects the fundamentally dissimilar molecular structures of the diisocyanide and α-diimine ligands. Thus, in the Mo 0 complexes, the 3 MLCT excited-state distortion seems considerably weaker than in the Ru II and Os II polypyridines, but this distortion occurs along vibrational modes with significantly higher average frequency. The combination of these two opposing effects results in rate constants for nonradiative relaxation (k nr ) that are within one order of magnitude the same for the Mo 0 and [Ru(dmb) 3 ] 2+ complexes (last column of Table 2).
The energy gap E 0 corresponds to the peak maximum of the first member of the vibrational progression in theh·ω M distortion mode [30], and as such does not strictly correspond to the 3 MLCT energy (E 00 ) used, for example, for the estimation of excited-state redox potentials from ground-state potentials [36]. However, the two quantities are related to one another by Equation (4), in which k B is Boltzmann's constant and T is temperature [28].
This relationship yields E 00 values (  [25,27]. Lastly, we note that the ∆ν 1/2 values for our Mo 0 diisocyanide complexes are similar to those obtained for the previously investigated Ru II and Os II polypyridines [28,30,32,34,35]. Aside from the comparison between the spectral band fitting parameters obtained for the Mo 0 and Ru II complexes (Table 3), the comparison between the obtained parameter sets for [Mo(L Me ) 3 ] and [Mo(L tBu ) 3 ] is interesting. The emissive 3 MLCT excited state is at slightly higher energy in the complex with tert-butyl-substituted ligands (ca. 300 cm −1 ) and its Huang-Rhys parameter is 35% lower than that of the complex with methyl-substituted ligands ( Table 3). Both of these findings are in line with the higher luminescence quantum yield for [Mo(L tBu ) 3 ] compared to [Mo(L Me ) 3 ] ( Table 1). The lower Huang-Rhys parameter for [Mo(L tBu ) 3 ] translates into a smaller distortion of the 3 MLCT excited state relative to the 1 A 1g ground state along the nuclear coordinate Q e (Figure 3a), which in turn leads to weaker overlaps between vibrational functions of the 3 MLCT and 1 A 1g states (grey shaded areas in Figure 3a). This makes nonradiative relaxation less efficient than in [Mo(L Me ) 3 ], where the excited-state distortion is stronger. The magnitude of the (equilibrium) distortion, ∆Q e , is related to the Huang-Rhys parameter by Equation (5), where M is the reduced mass of the oscillator and ω M is the vibrational frequency.
Since multiple normal coordinates contribute to S M in our Mo 0 complexes, and because we are lacking information regarding their relative importance, the ∆Q e values for the relevant individual normal coordinates cannot be calculated here. If vibrational fine structure were observable in the emission spectra, this would be possible [33].
The above emission band shape analysis serves to rationalize nonradiative relaxation occurring directly from the emissive 3 MLCT manifold to the electronic ground state. However, in Ru II polypyridine complexes there is usually additional nonradiative relaxation from the 3 MLCT via the 3 T 1g excited state (Figure 3b) [37,38]. Depending on ligand design [39], this metal-centered state can be energetically very close and nonradiative relaxation becomes very rapid, and this is the  2+ (tpy = 2,2 :6 ,2"-terpyridine) is essentially non-emissive in solution at room temperature [40]. Conversely, when the 3 T 1g state is located energetically sufficiently above the 3 MLCT manifold, high luminescence quantum yields and long excited state lifetimes are achievable [41]. In [Ru(bpy) 3 ] 2+ that energy difference amounts to ca. 3600 cm −1 [42], but for emissive Mo 0 isocyanide complexes this important aspect has not been explored before.
In order to gain insight into thermally activated 3 MLCT relaxation via the 3 T 1g state, we therefore performed temperature-dependent luminescence lifetime studies (τ(T), open circles in Figure 4) Figure 4 are weighted averages from bi-exponential fits. Equation (6) and the simplified model illustrated by Figure 3b have been used previously to determine the 3 MLCT-3 T 1g energy gap ∆E for [Ru(bpy) 3 ] 2+ [42], and the solid lines in Figure 4a,b is fits with the same model to the experimental data for our Mo 0 complexes. τ(T) = [k r + k nr,1 + k nr,2 · exp(−∆E/k·T)] −1 (6) isocyanide complexes this important aspect has not been explored before. In order to gain insight into thermally activated 3 MLCT relaxation via the 3 T1g state, we therefore performed temperature-dependent luminescence lifetime studies (τ(T), open circles in Figure 4). The 3 MLCT lifetimes of both [Mo(L Me )3] and [Mo(L tBu )3] decrease by roughly a factor of 4 between 283 and 338 K, in line with a thermally activated nonradiative decay process. The luminescence decays of [Mo(L tBu )3] remain bi-exponential at all temperatures measured (see above), and the τ(T)-values reported in Figure 4 are weighted averages from bi-exponential fits. Equation (6) and the simplified model illustrated by Figure 3b have been used previously to determine the 3 MLCT-3 T1g energy gap E for [Ru(bpy)3] 2+ [42], and the solid lines in Figure 4a,b are fits with the same model to the experimental data for our Mo 0 complexes. τ(T) = [kr + knr,1 + knr,2 • exp(−E/k•T)] −1 (6) The sum kr + knr,1 (reflecting the total 3 MLCT decay rate constant, Figure 3b) was fitted along with knr,2 and E. The results from such 3-parameter fits are listed in Table 4 along with those reported previously for [Ru(bpy)3] 2+ [42]. Of key interest is the comparison of E-values. The 3 MLCT-3 T1g energy gap is largest in [Ru(bpy)3] 2+ (3559 cm −1 ); hence, that compound features the highest barrier for thermally activated nonradiative relaxation via a metal-centered excited state. For the more strongly emissive [Mo(L tBu )3] complex E is ca. 19% larger than for [Mo(L Me )3] (2934 vs. 2472 cm −1 , last column in Table 4). Thus, the Mo 0 complex with the tert-butylated ligand features less efficient nonradiative relaxation than the Mo 0 complex with the methylated ligand, both via direct 3 MLCT relaxation to the electronic ground state (Figure 3a) and via thermal activation of metal-centered excited states (Figure 3b). It seems plausible that the greater overall rigidity of the [Mo(L tBu )3] complex compared to [Mo(L Me )3] is responsible for that. An X-ray crystal structure of [Mo(L tBu )3] is not available, but when considering the X-ray structure of the analogous Cr 0 compound in Figure 5b, it seems evident that the bulkier tert-butyl-substituents lead to a mutually more interlocked ligand framework than in the case of [Mo(L Me )3] (Figure 5a).   The sum k r + k nr,1 (reflecting the total 3 MLCT decay rate constant, Figure 3b) was fitted along with k nr,2 and ∆E. The results from such 3-parameter fits are listed in Table 4 along with those reported previously for [Ru(bpy) 3 ] 2+ [42]. Of key interest is the comparison of ∆E-values. The 3 MLCT-3 T 1g energy gap is largest in [Ru(bpy) 3 ] 2+ (3559 cm −1 ); hence, that compound features the highest barrier for thermally activated nonradiative relaxation via a metal-centered excited state. For the more strongly emissive [Mo(L tBu ) 3 ] complex ∆E is ca. 19% larger than for [Mo(L Me ) 3 ] (2934 vs. 2472 cm −1 , last column in Table 4). Thus, the Mo 0 complex with the tert-butylated ligand features less efficient nonradiative relaxation than the Mo 0 complex with the methylated ligand, both via direct 3 MLCT relaxation to the electronic ground state (Figure 3a) and via thermal activation of metal-centered excited states (Figure 3b). It seems plausible that the greater overall rigidity of the [Mo(L tBu ) 3 ] complex compared to [Mo(L Me ) 3 ] is responsible for that. An X-ray crystal structure of [Mo(L tBu ) 3 ] is not available, but when considering the X-ray structure of the analogous Cr 0 compound in Figure 5b, it seems evident that the bulkier tert-butyl-substituents lead to a mutually more interlocked ligand framework than in the case of [Mo(L Me ) 3 ] (Figure 5a).

Materials and Methods
The [Mo(L Me )3] and [Mo(L tBu )3] complexes were available from two recent studies and were stored under an Argon atmosphere at 4 °C [25,27]. Samples of both complexes (25 μM in dry toluene) were degassed by three freeze-pump-thaw cycles prior to measurements. The new temperaturedependent luminescence lifetime data were obtained using an LP920-KS spectrometer from Edinburgh Instruments, employing a Nd:YAG laser (Quantel Brilliant b) with an OPO (Opotek) as excitation source. The excitation wavelength was 500 nm with a typical pulse energy of 7 mJ. Singlewavelength kinetics were recorded using a photomultiplier tube. Spectral band shape analysis occurred with the Igor Pro software. The method by Parker and Rees was applied when converting the emission spectra from wavelength to wavenumbers [43].

Conclusions
The new analyses and additional temperature-dependent lifetime data reported herein are useful to understand why [Mo(L tBu )3] exhibits much more favorable photophysical properties than [Mo(L Me )3]. Furthermore, the direct comparison between these tris(diisocyanide)molybdenum(0) complexes and the isoelectronic and structurally related tris(α-diimine)ruthenium(II) compounds made herein is insightful.
In both compound classes the 3 MLCT relaxation is coupled to ring stretch vibrations (ca. 1300 cm −1 ) of the ligand backbone, but in the Mo 0 diisocyanides there seems to be additional coupling to CN vibrations, manifesting in a higher average frequency (1600-1650 cm −1 ) of all modes responsible for excited-state distortion. The disadvantage of coupling to a higher frequency mode in the Mo 0 complexes seems to be compensated by significantly smaller Huang-Rhys factors compared to Ru II polypyridines. Thus, the combination of weaker distortion along higher frequency modes is likely responsible for the finding that the Mo 0 diisocyanide complexes have similarly favorable luminescence properties as the [Ru(bpy)3] 2+ parent compound. In future work, it will be desirable to complement these findings by time-dependent density functional theory calculations to get clearer insight into the relevant excited-state distortions.

Materials and Methods
The [Mo(L Me ) 3 ] and [Mo(L tBu ) 3 ] complexes were available from two recent studies and were stored under an Argon atmosphere at 4 • C [25,27]. Samples of both complexes (25 µM in dry toluene) were degassed by three freeze-pump-thaw cycles prior to measurements. The new temperature-dependent luminescence lifetime data were obtained using an LP920-KS spectrometer from Edinburgh Instruments, employing a Nd:YAG laser (Quantel Brilliant b) with an OPO (Opotek) as excitation source. The excitation wavelength was 500 nm with a typical pulse energy of 7 mJ. Single-wavelength kinetics were recorded using a photomultiplier tube. Spectral band shape analysis occurred with the Igor Pro software (version 6.3.7.2). The method by Parker and Rees was applied when converting the emission spectra from wavelength to wavenumbers [43].

Conclusions
The new analyses and additional temperature-dependent lifetime data reported herein are useful to understand why [Mo(L tBu ) 3 ] exhibits much more favorable photophysical properties than [Mo(L Me ) 3 ]. Furthermore, the direct comparison between these tris(diisocyanide)molybdenum(0) complexes and the isoelectronic and structurally related tris(α-diimine)ruthenium(II) compounds made herein is insightful.
In both compound classes the 3 MLCT relaxation is coupled to ring stretch vibrations (ca. 1300 cm −1 ) of the ligand backbone, but in the Mo 0 diisocyanides there seems to be additional coupling to C≡N vibrations, manifesting in a higher average frequency (1600-1650 cm −1 ) of all modes responsible for excited-state distortion. The disadvantage of coupling to a higher frequency mode in the Mo 0 complexes seems to be compensated by significantly smaller Huang-Rhys factors compared to Ru II polypyridines. Thus, the combination of weaker distortion along higher frequency modes is likely responsible for the finding that the Mo 0 diisocyanide complexes have similarly favorable luminescence properties as the [Ru(bpy) 3 ] 2+ parent compound. In future work, it will be desirable to complement these findings by time-dependent density functional theory calculations to get clearer insight into the relevant excited-state distortions.
The barrier for thermal 3 MLCT deactivation via metal-centered excited states is 18-30% smaller in the two investigated Mo 0 complexes than in [Ru(bpy) 3 ] 2+ . For [Mo(L Me ) 3 ] that barrier is 19% lower than for [Mo(L tBu ) 3 ], and the spectral band shape analysis points to a significantly greater 3 MLCT excited-state distortion in [Mo(L Me ) 3 ] relative to [Mo(L tBu ) 3 ]. These two new findings can explain why nonradiative relaxation is roughly 10 times slower in the tert-butylated than in the methylated complex. Differences in the rigidity of the molecular structures of these two complexes provide a plausible rationale for this behavior. The sterically more demanding tert-butyl substituents lead to a molecular structure of [Mo(L tBu ) 3 ], in which the three individual ligands are considerably more interlocked into one another than in [Mo(L Me ) 3 ] where only methyl-groups are present. The use of sterically demanding substituents at the ligand periphery that lead to a compact molecular structure could represent a more generally valid design principle for minimizing undesirable excited state distortions, particularly in photoactive complexes of Earth-abundant metals [44,45].