Mo6 cluster-based compounds for energy conversion applications: comparative study of photoluminescence and cathodoluminescence.

We report the photoluminescence (PL) and cathodoluminescence (CL) properties of face-capped [Mo6Xi8La6]2- (X = Cl, Br, I; L = organic or inorganic ligands) cluster units. We show that the emission of Mo6 metal atom clusters depends not only on the nature of X and L ligands bound to the cluster and counter-cations, but also on the excitation source. Seven members of the AxMo6Xi8La6 series (A = Cs+, (n-C4H9)4N+, NH4+) were selected to evaluate the influence of counter-cations and ligands on de-excitation mechanisms responsible for multicomponent emission of cluster units. This study evaluates the ageing of each member of the series, which is crucial for further energy conversion applications (photovoltaic, lighting, water splitting, etc.).

Introduction

Energy supply is one of the greatest challenges of humankind. The current world energy consumption of ca. 16 TW is expected to increase to more than 30 TW by 2050 [1]. Meanwhile, as CO2 emissions are predicted to increase (around 43 billion metric tons by 2035) there is an urgent need for alternatives to fossil energy sources. In this frame, solar energy appears as the most relevant alternative by taking advantage of a quasi-infinite and renewable resource. On the other side, buildings are one of the major sources of energy consumption; our society is clearly facing the challenges of green buildings. Thus, novel materials and processes are needed to meet these challenges, and composite nanomaterials could be one way to answer it [2]. One promising strategy is the development of new nanocomposite materials and concepts for smart windows and solar devices. The challenge to achieve this goal is to find less toxic and more efficient phosphors than the currently available materials based on rare earth (RE) or heavy metals (HM). Among the possible candidates, metal clusters (MCs), which consist of less than a few dozens of metal atoms, are receiving more and more attention owing to their attractive properties and great flexibility in terms of composition and design [3-6]. In the past decades, Mo6 metal cluster compounds have shown interesting and rich complexity of structural and physico-chemical properties [7,8]. Their good solubility in various solvents provides a wide range of processing routes to elaborate molecular assemblies and nanocomposite materials [6]. Thus, a large variety of Mo6-based MCs have been investigated for potential applications in lighting [6,9-11], solar cells [12-14], and biotechnologies [15-19]. Additionally, their high chemical flexibility has already allowed the fabrication of transparent nanocomposite thin films in organic or inorganic matrices that can be easily coated on substrates for photonic applications [20,21] Moreover, in addition to their very interesting optical properties for energy conversion applications (molecule-like energy gaps, strong photoluminescence in near infrared (NIR) region, etc.), they have also some specific electronic and electrochemical properties with strong potential for energy storage and supply applications (superconductivity, battery, thermoelectricity, hydrogen affinity, etc.) [22-26].

Although Mo6 cluster-based compounds were reported in the literature a long time ago and they have recently shown great potential for advanced applications [34-37], there are still large possibilities of improvement for further implementation into energy and environment applications. In order to fully exploit MCs, it is necessary to have a better understanding of the relations between chemical compositions, structural arrangements, and physical properties in MC-based compounds for a better selection of targeted properties and applications, as well as to develop scalable and industrially viable processes. For instance, some of us showed recently the effects of centro-symmetry in the Cs2Mo6Cl14.xH2O system on second harmonic generation [28]. On the other hand, we reported the design of transparent inorganic thin films based on octahedral Mo6 MCs deposited on indium tin oxide (ITO) glass by electrophoretic deposition (EPD) within a short time interval and at low cost [21]. Recently, multicomponent emission of []2− cluster units has been reported [29]. Several excited triplet states resulting from complex de-excitation processes (breaking Kasha’s rule) have been evidenced. Quantum chemical studies suggest that the geometries of this excited triplet states are different from the ground state (S0) geometrical arrangement. These changes are either an elongation of one Mo-Mo bond or axial and non-axial elongations of one Mo apex. It turns out that absorption and emission properties of Mo6 cluster-based units are very sensitive to the nature of ligands and counter-ions, and more generally to matrix effects [9,30]. One of the goals of this work is to evidence if such a de-excitation cascade is also effective for another source of excitation (e-beam). Secondly, we aim at evaluating the luminescence efficiency over time upon highly energetic photon/electron irradiation (ageing), a key point to consider prior to effective applications such as energy conversion or field emission display (FED) applications [31]. To the best of our knowledge, no study of ageing of Mo6 cluster units upon different excitation sources has been reported to date. This work reports (i) the cathodoluminescence (CL) properties of representative face-capped []2− cluster unit-based compounds; (ii) systematic and quantitative comparisons of photoluminescence (PL) properties; (iii) the influence of the excitation wavelength on their quantum yields (QY), defined as the ratio of the number of absorbed exciting photons and the number of emitted photons; and (iv) their luminescence stability over irradiation time.

Experimental section

Description of the studied series

We have synthesized and investigated seven compounds in the series – namely (Cs)2[Mo6Cl14] (1), (Cs)2[Mo6Br14] (2), (Cs)2[Mo6I14] (3), (Cs)2[Mo6I8(OOCC2F5)6] (4), ((n-C4H9)4N)2[Mo6Br14] (5), (NH4)2[Mo6Br14] (6), and (NH4)2[Mo6Br8(NCS)6] (7), according to the procedures reported in the literature, and whose structural view can be viewed in Supporting Figure 1 [27,32,33]. Those systems have been chosen since (i) 1, 2, and 3 constitute a ternary series of MCs solid-state compounds for which only the halogen atoms differ (Cl, Br, I); (ii) in the 2, 5, and 6 series, the [Mo6Br14]2− cluster unit is kept unchanged, allowing study of the effect of counter-cations (Cs+, (n-C4H9)4N+ = TBA+, ); (iii) 1, 4, and 7 are the most emissive systems of the series. It may be noted that 4 and 7 contain an organic apical ligand (C2F5COO−) and SCN−, respectively, for which stability could be an issue. Actually, a continuous irradiation could affect the Mo-O and Mo-N bonds, respectively. Recently a lot of work has been devoted to the series of general formula (OOCCnF2n+1)a 6 (A = Cs+, (n-C4H9)4N+; n = 1, 2, and 3) owing to their remarkable luminescent properties. Among all face-capped clusters, the last-mentioned series exhibits the highest quantum yields [18,30,37-44].

Figure 1.

CL spectra of 1–7 compound series.

Description of the measurement techniques

The chemical composition and purity of all the compounds were monitored by X-ray diffraction (XRD) and scanning electron microscopy combined with energy-dispersive electron spectroscopy (SEM-EDS). QY measurements were made upon continuous irradiation of a 150 W Xe lamp, corresponding to a power density of ca. 0.5 μW cm−2, in standard atmosphere conditions using a system combining two-multichannel photodetectors (MCPD-9800: Otsuka Electronics) and a 3.3 inch integrating semi-sphere. Excitation wavelength was selected by a monochromator with an accuracy of ca. 3 nm. PL spectra were generated by combining UV–visible (250–800 nm) and IR data (800–1100 nm). The spectral resolution was 0.3 and 3 nm for UV–visible and IR, respectively. Time-dependent photo-irradiation was performed using a micro-PL system (HORIBA LabRam HR) equipped with fixed 325 nm He-Cd laser system (average source power of 20 mW and around 10 mW on the sample), corresponding to a power density of ca. 1000 mW cm−2, and a Perce type charge-coupled device (CCD) to investigate the PL evolution under photon excitation at ambient conditions. CL measurements were performed in a field emission SEM (Hitachi SU6600) equipped with a CL system (HORIBA MP32) at room temperature and 3 × 10−3 Pa. For CL measurements, a few milligrams of powders were deposited and hand-pressed on carbon tape for each composition. CL spectra were obtained at room temperature by a CCD (2048 channels, HORIBA Jobin-Yvon, Spectrum One), while CL mapping was carried out with a photomultiplier (Hamamatsu, R943–02). The applied voltage and beam current were set to 10 kV and 100 pA. The probe size was 12 nm, and the spectral resolution was about 0.2 nm.

Results and discussion

Cathodoluminescence properties of 1–7

The CL spectra of 1–7 are gathered in Figure 1. Except 3, all compounds exhibit CL properties on a large spectral window ranging from 550 nm to more than 900 nm. The all-iodide compound 3 that hardly shows CL will not be subsequently considered. We suspect that 3 decomposes under e-beam irradiation similarly as under UV irradiation. Except for 4, the CL spectra consist of an asymmetrical broad band with a maximum centered at around λmax = 720 nm. CL spectrum of 4 shows a narrower blue-shifted band than that of the other members of the series (λmax = 655 nm). For all the emission spectra except 4, a small depletion is observed around 725 nm.

Photoluminescence properties of 1–7 and quantum yield evolutions

PL spectra of 1–7 upon 325 nm excitation generated by a Xe lamp are shown in Figure 2. For 1, 2, 5, 6, and 7, the spectral PL shape consists of an asymmetric structured broad band centered roughly at λmax = 715 nm. It is worth noting that this shape is more asymmetric than that found for CL. One can note that spectra of 2, 5, and 6 are almost flat between 715 and 790 nm. Contrary to the other samples, the PL spectrum of 4 consists of a less asymmetric broad band centered at λmax = 655 nm, which is similar to that found in CL. As there is no observable PL emission for 3, it will not be discussed further. It may also be noted that, for all the clusters except 4, there is an inflexion point around 750 nm that may be related to self-absorption, as quantum chemical calculations performed on []2− relaxed excited states show absorption transitions in the NIR region (∼600, 750, 900 nm) [29]. It may be noted that the position of the inflexion point found for PL (750 nm) is different compared to that found for CL (725 nm). The full understanding of the origin of this position shift, probably related to the absorption of several excited triplet states, will require further combined and theoretical investigations.

Figure 2.

PL spectra of 1–7 compound series (λexc = 325 nm).

Figure 3 shows the QY excitation wavelength dependence (λexc = 300–550 nm) of 1, 2, and 4–7. The analysis of the curves reveals two behaviors: (i) for 1, 4, 5, and 6, a plateau with the maximum QY value is observed followed by a loss of efficiency as the excitation wavelength increases; (ii) for 2 and 7, a smooth increase of QY is observed from 300 nm to roughly 550 nm. These different behaviors evidence that the emission strongly depends on the environment of the metallic Mo6 clusters: on one hand, the effect of Xi inner and La apical ligands forming the []2− unit, and, on the other hand, the effect of counter-cations [45]. It is worth noting that for 2, 5, and 6 that are based on the same []2−cluster unit, but differing in the nature of counter-cations, the two behaviors are found. This unambiguously proves that there exists a significant effect of the cations in the de-excitation processes.

Figure 3.

QY of 1–2 and 4–7 vs. excitation wavelength (300–550 nm).

Here we report the evolution of QY for several members of the series as a function of the excitation wavelength. The measurements were carried out using the same experimental set-up and the same experimental conditions. series were reported in previous works using a single excitation wavelength. In acetonitrile solutions, QYs of (TBA)2[] and (TBA)2[] were reported by Maverick et al. to be 19% and 23% upon excitation at 436 nm [46]. Absolute quantum yields were estimated by comparison with solutions. On the other hand, Kirakci et al. reported, by a comparative method with cresyl violet as reference upon excitation at 440 nm, that the QYs of (TBA)2[], (TBA)2[], and (TBA)2[] in acetonitrile solution are 15%, 13%, and 12%, respectively [30]. More recently, the QY of (TBA)2[] measured on powder upon excitation at 400 nm was reported to be 10% [45]. It is worth noting that the QY of parent compound (4-ViBnNMe3)2[] (4-ViBnNMe3 = trimethyl(4-vinylbenzyl)ammonium) measured on powders by the same authors and in the same conditions as (TBA)2[] is only 1%. In the present study, QY could not be measured for Cs2[]. For iodide clusters, those previous measurements showed that counter-cations play a significant role in luminescent properties. Actually, changes in the luminescent properties observed for the bromine series 2, 5, and 6 are related to the nature of the counter-cations. Counter-cations drive the packing and stacking of []2− clusters units within the crystal, and we suspect that a dense packing favors reabsorption phenomena. Additionally to optical reabsorption, the strong absorbance of 3 probably induces decomposition by overheating upon continuous irradiation. Luminescence and QY of 3 could thus not be measured. The substitution of iodide apical ligands by organic substituents substantially decreases these phenomena. QYs of powder samples of Cs2[] and its derivative (TBA)2[] have been recently determined at 35% and 32%, respectively, by absolute photoluminescence QY measurement upon 380 nm excitation [44,47].

It has to be pointed out that except for 4, which incorporates an organic ligand, the rest of the series shows the maximum QY in a large range of excitation energy from UV to the lower-energy green-region. This excitation window combined with NIR emission properties makes Mo6 clusters relevant down-conversion phosphorescent dyes for the design of solar cell concentrators for photovoltaic applications as already demonstrated by Lunt et al. for a series of []2− based compounds [11,12]. Mo6 cluster compounds constitute an alternative to lead-based perovskites. Both families of compounds exhibit many analogies. It is worth mentioning that halogen ligands and cations play a significant role in optical properties of lead-based perovskites as demonstrated here for the series [48,49].

Comparative analysis of CL and PL results

As stressed above, except for 4, the spectral shape of the luminescence (PL and CL) deviates from the Gaussian function. This deviation is more pronounced for PL spectra. This is most probably related to the multicomponent nature of the emission. In order to quantify this matter, CL and PL spectra were normalized, and were then fitted with two Gaussian functions whose characteristics – maximum (Emax1, Emax2), full width at half maxima (FWHM1, FWHM2), and relative contributions (cont1, cont2) – are given in Table 1.

Table 1.

Parameters of the Gaussian functions used to fit CL and PL spectra of 1, 2, and 4–7: Emax1, Emax2, FWHM1, FWHM2 in eV; cont1 and cont2 percentages; coefficient of determination R 2. Values in italics were fixed (see text).

	E-beam excitation								Optical excitation
	Emax1	Emax2	FWHM1	FWHM2	cont1	cont2	R2		Emax1	Emax2	FWHM1	FWHM2	cont1	cont2	R2
1	1.396	1.740	0.097	0.349	1.5	98.5	0.9998		1.448	1.740	0.245	0.316	31.4	68.6	0.9983
2	1.401	1.721	0.128	0.333	3.3	96.7	0.9997		1.463	1.721	0.298	0.302	41.1	58.9	0.9958
4	1.796	1.909	0.240	0.174	44.4	55.6	0.9988		1.796	1.909	0.222	0.170	47.3	52.7	0.9971
5	1.400	1.716	0.126	0.339	3.4	96.6	0.9996		1.447	1.716	0.270	0.311	34.7	65.3	0.9962
6	1.394	1.704	0.099	0.333	2.3	97.7	0.9998		1.447	1.704	0.245	0.310	32.5	67.5	0.9908
7	1.398	1.736	0.112	0.342	2.1	97.9	0.9998		1.463	1.736	0.258	0.316	27.4	72.6	0.9954

Except for 4, all CL spectra are well fitted using a first Gaussian component centered at Emax1 ~ 1.40 ± 0.01 eV with a FWHM of ~ 0.11 ± 0.02 eV and a second one at Emax2 ~ 1.72 ± 0.02 eV with a FWHM of ~ 0.34 ± 0.01 eV, respectively. The first contribution is minor, representing less than 4% of the total spectra. A deeper analysis can be made taking into account the nature of the ligands and counter-cations. For compounds 2, 5, and 6, which contain the same cluster unit []2−, the energies and bandwidths of the two components are relatively similar with a maximum deviation of less than 0.02 eV. Changing the apical ligands from bromines (6) to thiocyanates (7) leads to a slight shift of Emax2 energy (1.704 to 1.736 eV). Changing the bromine apical and inner ligands in 2 by chlorine in 1 barely modifies the emission properties from the energetic point of view. Such behavior has been reported for the PL of (X = Cl, Br) [46]. Overall, one can conclude that the nature of the ligands and of the counter-cations for this group (1, 2, 5–7) plays a limited role on the energies of CL emissions, but, as previously highlighted, it has more noticeable effects on their emission intensities.

The CL properties of 4 are different from the rest of the series described above. One can note that: (i) the maximum of emission is blue-shifted; (ii) the emission intensity is the highest of the whole series; (iii) the two components are close in energy (Emax1 = 1.796 eV, Emax2 = 1.909 eV); and (iv) the first contribution reaches 44.4%, which strongly differs from other compounds for which the first component is minor. The substitution of apical iodides by pentafluoropropionates (C2F5COO−) going from 3 to 4 induces thus an incredible enhancement of emissive properties along with a strong blue-shift compared to the other member of the series. From this investigation and comparison between 4 and the other member of the series, it appears that, for the same [Mo6Xi 8]4+ cluster core, CL characteristics are more sensitive to the nature of apical ligands, in particular changing inorganic La ligands by organic pentafluoropropionate group, than to that of the counter-cations. This can be understood taking into account the molecular character of the []2− unit. Frontier molecular orbitals (MO) of the cluster unit (singlet ground state S0) depend on the nature of ligands [50-52]. Consequently, the triplet (T1+n) and singlet (S1+n) excited states are also strongly affected by the nature of the apical ligands since they formally result from S0 electronic MO transitions. On the other hand, counter-cations mainly affect the crystal packing and, to a much lower extent, the ionic character of the Mo-La bond and the excited-state geometry relaxations. Judicious choice of apical ligands would enable emissive properties of Mo6-based compounds to be enhanced and optimized.

CL fitting procedure was applied to the PL spectra. While in PL, one incident photon generates usually one electron-hole pair, in CL, one incident electron generates thousands of pairs. This leads to significant differences in the excited-state populations between optical and e-beam excitation, and results in different spectral shapes due to different non-radiative energy losses occurring before emission. Taking into account lifetime of the excited states, re-absorption can also occur [29]. As it can be seen in Supporting Figure 2, there is a good match between the CL and PL spectra in the high-energy region (>1.68 eV). This part of the emission corresponds to the second component of the CL spectra, which is very accurately defined since it covers 96% of CL (except for 4). For this reason, PL fits were performed by fixing Emax2 to the value obtained after CL refinements. The values of Εmax1, Εmax2, FWHM1, and FWHM2 and relative contributions (cont1, cont2) of the two Gaussian components are given in Table 1. It turns out that the present results for (Cs)2[Mo6Br14] (2) and ((n-C4H9)4N)2[Mo6Br14] (5) are in full agreement with previously reported PL steady state measurements, despite the fact that the experimental set-up and excitation sources are different [29]. In this previous work, the doublet nature of the emission of []2− in 2 and 5 metal cluster units has been demonstrated by a combined theoretical, steady-state and time-resolved PL investigation. Thus, from the PL excitation maps, the energies of the emission maxima (for λexc = 380 nm) of the two contributive emissions could be extracted as Emax1 = 1.463 eV and Emax2 = 1.721 eV (845 and 719 nm, respectively), and Emax1 = 1.447 eV and Emax2 = 1.716 eV (856 nm and 722 nm, respectively) for 2 and 5, respectively. The corresponding ratios between the first and second contributions (cont1/cont2) are ~41/59 for 2 and ~35/65 for 5. This set of convergent results proves the doublet structure of luminescence for two []2− cluster unit-based compounds differing by the counter-cation nature. The same behavior is suspected for the rest of the series. For the third compound of the all-bromide series, 6, the maxima of energy Εmax1 and Εmax2 are the same as those of 2 and 5. The ratio between each contribution is the same as that of 5 (~33/67 compared to ~35/65), revealing a similar impact of the counter-cation environment. This result is coherent with the fact that both 5 and 6 are ammonium-type cations ((n-C4H9)4N+ for 5; for 6). Going from 6 to 7, i.e. replacing apical bromine atoms by thiocyano groups, a blue-shift of both Εmax1 and Εmax2 is observed along with a decrease of cont1/cont2 ratio from ~33/67 to ~27/73. For the whole series, both components show rather similar FWHM, which are mainly due to vibrational phenomena (from 0.17 to 0.32 eV).

Similarly to CL, the PL properties of 3 and 4 are very different from those of the others members of the series. While 3 hardly emits, 4 exhibits a strong blue-shifted luminescence compared to the other member of the series. Moreover, since the PL and CL spectral shapes for 4 are very similar, both Emax1 and Emax2 were fixed to the values found in CL for PL fittings. The slight difference between PL and CL spectra for 4 is due to a very slight evolution of cont1/cont2 ratios (~47/53 for PL compared to ~44/56 found for CL). It suggests that, for 4, both types of excitation (photon and electron-beam) lead to the same emissive triplet states and thus most probably to similar non-radiative de-excitation pathways. The substitution of apical iodide by C2F5COO− going from 3 to 4 affords a modified [(OOCC2F5)]2− cluster unit with outstanding enhancement of emissive properties along with a strong blue-shift compared to the other members of the series.

Luminescence intensity decay upon continuous laser optical irradiation

The evolution in time of the PL intensity of the series of compounds under study upon high-power continuous laser irradiation at a wavelength of 325 nm is given in Figure 4. The experiment was performed over 300 s. Normalized curves are given as inset. The curves can be fitted with a double exponential: A1 exp(−x/τ1) + A2 exp(−x/τ2) + y0, whose A1/2 and τ1/2 are reported in Table 2. At this stage, it has to be pointed out that while no noticeable change in intensity emission over the time was observed during the QY measurements, which last roughly 10 min, important decreases of intensity are observed for all compounds in the present experiment. It may be related to a difference in light intensity, which was lower for QY measurements (Xe lamp). As previously reported, the absorption properties and notably the absorbance at 325 nm depend on the composition of each studied system. It means that the structural damage or decomposition phenomena originating from heat generation upon high-power irradiation differs from one composition to another [13,53,54]. In the halogenide series 1, 2, and 3, the heavier the halogen is, the higher its UV–visible absorbance is [55]. Compound 3 exhibits the strongest absorbance, and it appears to be the worst emitter. This result suggests that important non-radiative processes occur after excitation, self-reabsorption, or decomposition phenomena. For other cluster compositions, QY can be high with a weak absorbance leading to inferior luminescence properties.

Figure 4.

PL intensity decay at maximum of emission of 1, 2, and 4–7 upon continuous 325 nm laser irradiation (average source power of 20 mW – around 10 mW on the sample). Inset: normalized curves.

Table 2.

Fitting parameters by a double exponential of PL (Figure 4) and CL (Figure 5) intensity decays. The loss percentage after 300s irradiation and the QY at 325 nm (QY325nm in percentage) extracted from Figure 3 are also reported.

	A1	Optical excitation						A1	E-beam excitation
		τ1 (s)	A2	τ2 (s)	Loss (%)	QY325 nm (%)			τ1 (s)	A2	τ2 (s)	Loss (%)
1	0.42	15	0.58	226	29	26.3		3.03	13	1.67	87	90.2
2	0.11	17	0.04	207	45	9.4		0.75	24	0.62	144	76.6
4	3.05	8.1	0.53	76	94	19.3		34.5	4.2	1.21	28	99.5
5	2.81	13	1.13	114	79	12.6		2.00	6.6	1.14	210	71.6
6	0.07	13	0.04	1300	26	3.4		0.34	9.6	0.20	135	82.7
7	0.06	10	0.01	93	88	14.2		0.64	9.1	0.43	76	88.3

For the design of effective PL-based devices, good candidates should absorb strongly at the working excitation wavelengths, and have a high quantum yield resulting in high PL intensity (luminance). Ageing, e.g. loss of intensity, or change in energy of emission, is thus an element to consider for the selection of phosphorescent dyes. Laser irradiation can cause photo-induced phase transition and structural damages via local heat generation. Considering initial emission intensity, the best systems within the studied series are 1, 4, and 5 as shown in Figure 4. Additionally, if ageing is taken into account, the compound that is the most resistant to a strong and continuous photon irradiation is 1, with still 70% of luminescence intensity after 300 s of laser irradiation. For the two other best candidates, 4 and 5, the decay regime is very abrupt since more than 50% of their intensity is lost after only 60 s. The compounds 1 and 5 are the only ones for which the emission is still significant after 300 s. This conclusion could be different for another wavelength of irradiation since all processes (excitation and de-excitation) are wavelength-dependent (absorption, non-radiative decay, emissive and non-emissive excited-state population).

Luminescence intensity decay upon continuous e-beam irradiation

Ageing of a luminescent material can also be evaluated using e-beam excitation. Electron-induced damages can indifferently affect an organic or inorganic sample through electrostatic charging, heating, ionization damage (radiolysis), displacement damage, sputtering, or hydrocarbon contamination [56,57]. Luminescence intensity decay was studied for the whole series (Figure 5). CL decay characteristics are given in Table 2 together with those of PL (corresponding to Figure 4).

Figure 5.

CL intensity decay at maximum of emission of 1, 2, and 4–7 upon electron irradiation. Inset: normalized curves.

As shown in Figure 5, when a continuous e-beam is applied, one can observe a drastic decrease in intensity. Two decay regimes are found. For 4, an abrupt loss of intensity is found, leading to a total extinction of luminescence after roughly 120 s. For the rest of the series, a smoother decrease is measured. Only the [Mo6Br14]2− cluster unit-based compounds (2, 5, and 6) are still emitting at more than 40% of their initial intensity after 60 s of irradiation. After 300 s, the remaining intensity ranges from 10% to 30% of the initial intensity. Taking into account the absolute intensity, the most emissive compound after 300 s is 5 followed by 1 and 2. For the rest of the series, no significant CL is measured. These results suggest that for a targeted application, an compound could be tailor-made by a judicious choice of ligands and counter-cations. For applications requiring low-power photo-irradiation, 4 would give the highest emission intensity, while for those needing high-power or long-term photo-irradiation, 1 seems to be more relevant. Compounds 2 and 5 may be a better choice for FED applications.

Conclusions

The luminescence behaviors of seven representative members of the series were investigated in order to evaluate the influence of the nature of ligands bound to the Mo6 cluster, as well as the nature of counter-cations on QY, PL, CL, and ageing upon continuous light source and a continuous electron beam irradiation.

The PL multicomponent emission previously found for Mo6 cluster-based bromides (Cs)2[Mo6Br14] (2) and ((n-C4H9)4N)2[Mo6Br14] (5) has been enlarged to other members of . Moreover, while two peaks are observed in PL, the high-energy emission component is predominant in CL with the exception of (Cs)2[Mo6I8(OOCC2F5)6] (4), which exhibits a CL doublet. The latter shows blue-shifted emission spectra whatever the nature of the excitation source (photon or electron), revealing that the same emissive triplet states are populated. The intensity of luminescence of 4 is one of the most important among the series, but it decreases dramatically over time. It turns out that (Cs)2[Mo6Cl14] (1), 2, and 5 are the most robust systems upon irradiation.

Additionally, understanding ageing mechanisms is mandatory to improve the luminescence stability of the MCs and thus enlarge their potential application fields. For that purpose, predictive molecular engineering, combining theoretical and experimental approaches, may greatly contribute in the fine-tuning of the luminescence properties of cluster-based compounds [28,50,51]. Another strategy lies in materials engineering consisting in embedding MCs into a mediating (active) matrix. This should enhance the stability of the luminescence properties of the MCs by favoring heat dissipation and limiting non-radiative processes for long-term applications [10,47,58,59].

Disclosure statement

No potential conflict of interest was reported by the authors.

Funding

The study was financially supported by Saint-Gobain (France), CNRS, University of Rennes 1, and NIMS through the Laboratory for Innovative Key Materials and Structures (LINK UMI 3629). M.A.C. thanks ANR Clustomesogens ANR-13-BS07-0003-01.

Supplemental data

The supplemental material for this paper is available online at https://doi.org/10.1080/14686996.2017.1338496.

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