Roland B. Piper*a,
Megumi Yoshidaa,
Daniel J. Farrellb,
Tony Khouryc,
Maxwell J. Crossleyc,
Timothy W. Schmidtc,
Saif A. Haquea and
N. J. Ekins-Daukesa
aCentre for Plastic Electronics, Imperial College London, London, UK. E-mail: roland.piper09@imperial.ac.uk; Tel: +44 (0)20 759 46682
bRCAST, The University of Tokyo, 4-6-1 Komaba, Meguro-ku, Tokyo 153-8904, Japan
cSchool of Chemistry, The University of Sydney, NSW 2006, Australia
First published on 14th January 2014
We demonstrate a transient rate model for photochemical upconversion that links the internal energy transfer and triplet–triplet annihilation processes to spectroscopically measurable quantities, such as delayed fluorescence and bleaching. We confirm that our model is able to reproduce published delayed fluorescence measurements extremely well. We then use transient absorption spectroscopy to directly observe the dynamics of triplet populations through clear observation of delayed bleaching of the emitter species, providing direct evidence of triplet energy transfer from sensitiser to emitter molecules. This more complex experiment is also well reproduced by our model.
The molecular upconversion energy step ladder is shown in Fig. 1. This method of upconverting light is particularly well suited for upconversion of the visible and near-IR wavelengths (γ1 < 700 nm). This is because sensitising dyes exhibit strong absorption in this region, providing a good way to get energy into the system. Metallated porphyrin molecules are often employed in this role. The excitation crosses rapidly into the triplet state (T1), typically within a few picoseconds and with an inter-system crossing (ISC) efficiency close to unity. Providing that the triplet energy level of a paired fluorescent, emitting, molecule is close to that of the sensitiser's, and that there is an excess of emitter in the mixture, the sensitiser triplet is rapidly transferred to a triplet state in an emitter molecule via Dexter energy transfer,10 also known as triplet energy transfer (TET). When two triplet-excited emitter molecules interact, they can undergo a triplet–triplet annihilation (TTA) process whereby the excited singlet level of one emitter is populated and the other emitter relaxes to its ground state. This triplet–triplet annihilation process has been found to be highly efficient and while the TTA process does obey spin-selection rules, the efficiency of that process is not limited by those rules.11
The steady state and kinetic properties of many of these emitter/sensitiser pairs have been thoroughly investigated in previous articles, for example Murakami et al.12 recently used delayed fluorescence measurements to examine the kinetics of the final output of an upconverting system and Deng et al.13 analyse transient absorption measurements in the same way. Further information on fluorescent emitters and frequently used sensitisers can be found in (ref. 14–18).
For efficient upconversion, the rate constants, k, associated with the Dexter energy transfer step (kTET) and the final annihilation step (kTTA) must be much faster than the associated loss mechanisms. Namely phosphorescence, kp, and non-radiative decay, kNR. In the model presented in this paper the two governing equations have been adapted from Aucketts work. These modified equations are presented below as eqn (1) and (2), where: [·] denotes concentration; X a sensitiser species; Y an emitter species; G and T ground and triplet states respectively; kϕ the flux of photons capable of exciting the sensitiser; kp the rate of phosphorescence; kNR the rate of non-radiative decay; kTET the rate of triplet energy transfer and kTTA the rate of triplet annihilation.
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We make two changes to the equations reported in (ref. 19). We split the original kTTA terms into kXYTTA, kYYTTA and kXXTTA to allow for the potential differences in annihilation rates between two emitter molecules, two sensitiser molecules and that between a sensitiser and an emitter. We also remove a factor of two from the homoannihilation of sensitiser triplets term to make it kTTA[XT]2. This reflects new understanding on recombination dynamics of these triplets: an unsuccessful annihilation event between two sensitiser molecules that does not necessarily depopulate both triplet levels. One sensitiser will be excited to a singlet state and undergo ISC once more, leaving one triplet state sensitiser and one ground state sensitiser.11 In our experimental section we find that these changes make very little difference to the output of our model in this experimental regime. These changes only become significant at impractically high irradiance levels, and impossibly high concentrations. We make them only to provide the most correct description of the molecular dynamics possible with our current understanding.
Previous studies have used experimental techniques to calculate these rate constants, for example using steady-state and transient techniques such as delayed fluorescence or phosphorescence measurements.11 In these experiments, the triplet concentrations must be back-calculated based on the framework of eqn (1) and (2), whereas in this paper we use transient absorption spectroscopy to measure the triplet concentrations directly, as presented in the following sections.
The time-dependant rate model that was developed for this work solves the rate eqn (1) and (2) numerically. This is done by using the ODE45 library in Matlab, which employs a Runge–Kutta order 4 method20 to solve eqn (1) and (2) at dynamically varying discrete time intervals (1–10 ns). This provides a time-dependent description of the population of triplet states on emitter and sensitiser molecules within the upconversion system. By choosing a constant kϕ and taking the values of [XT] and [YT] at long times, i.e. once
, our model reproduces the steady-state results presented in the original model.19 If we then include experimentally determined rate constants of a particular molecular system in the calculations, it is possible to predict or replicate steady state experimental results. Setting kϕ = 0 and starting the simulation with a non-zero [XT] to simulate the effect of an excitation pulse allows even pulsed laser experiments to be modelled. The value of [XT] is calculated by determining the number of molecules that would be excited by a laser pulse, we assume that ISC efficiency is 100% so this number is equal to the initial value of [XT].
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| Fig. 2 Top left: structure of palladium(II) tetrakisquinoxalinoporphyrin (PQ4Pd). Top right: Structure of rubrene. Bottom: peak optical transitions for each molecule, with λmax in nm. | ||
The PQ4Pd was synthesised at the University of Sydney.21 The rubrene was purchased from Sigma-Aldrich, and was used without further purification. Following dissolution in toluene to the required concentration, each solution was purged of oxygen by being left open in a nitrogen glovebox overnight. The reliability of this passive process is demonstrated here by experimentally determining the value of kTET for this system and comparing it to published data.11 We derive kTET through transient absorption spectroscopy. This is achieved by varying the concentration of rubrene in a PQ4Pd/rubrene sample and observing the recovery time of the ground state of the porphyrin after laser excitation. The Stern–Volmer eqn (3) is then used to extract the rate constant, as shown in Fig. 3, where we find that there is a 2% difference between our result and that which has been published previously.
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| Fig. 3 Plot of reciprocal of recovery time of sensitiser ground state with varying rubrene concentration. The fitted curve is a plot of y = k × x + c where k corresponds to kTET and have a value of 3.4 × 108. The value reported in (ref. 11) was 3.1 × 108. | ||
Transient Absorption Spectroscopy (TAS) is a pump-probe technique that allows for direct observation of excited state yields and dynamics, making it possible to understand the energy flow through a molecular upconversion system. In our experiments pump pulses were produced by a Photon Technology International GL-301 dye laser, pumped with a Photon Technology International GL-3300 Nitrogen laser source. These pulses had a pulse width of 2 ns at a repetition rate of 4 Hz. The output from a Xe lamp was passed through a monochromator to provide the probe beam. Samples were sealed in a 1 mm quartz cuvette and placed at the conjunction of the probe beam and pump pulses.
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| Fig. 4 Comparison of model output, stars, with a fit to experimental data from (ref. 11), solid curve. | ||
Pumping PQ4Pd at its ground state absorption peak (λ = 660 nm) forms a long lived triplet state on that species. This excited state also has a characteristic absorption spectrum, shown in Fig. 5. Here it can be seen that, along with the expected bleach of the PQ4Pd ground state, there is a broad absorption feature induced between 530 and 600 nm, which we attribute to optical excitation up the triplet channel of the porphyrin. This PQ4Pd specific absorption feature overlaps the ground state absorption of the rubrene emitter, also shown in Fig. 5. The overlap between the excited sensitiser's induced absorbance and the ground state emitters absorbance spectrum has important implications when considering the TAS spectra of these species when mixed.
From Fig. 3 we see that sensitiser triplet lifetime decreases as higher concentrations of emitter molecules are incorporated into the system. This is because a triplet quenching pathway is introduced by the emitter. The decrease in lifetime does not, in itself, provide direct evidence of TET. To provide that we must probe at the ground state absorption of rubrene, while the pump remains at 660 nm. Fig. 6 shows the result of this experiment: a mixture of [0.1 mM] PQ4Pd and [2 mM] rubrene in toluene was pumped at 660 nm, where rubrene does not absorb, and the probe wavelength was chosen as 535 nm, corresponding to the λmax of ground state rubrene.
We attribute the initial induced absorption seen in Fig. 6 to the previously observed optical triplet excitation of the sensitiser, shown in Fig. 5. The decay of this induced absorption proceeds at a rate comparable to the regeneration of the sensitiser ground state, as indicated in Fig. 3. The delayed bleach in the rubrene ground state that follows this induced absorption then directly shows the process of triplet energy transfer from sensitiser to emitter molecules.
The solid line in Fig. 6 shows the result of running our model with known experimental parameters and the published rate constants for this system as inputs.19 The value of ΔOD was calculated from eqn (4): where TSabs is the contribution of one triplet excited sensitiser molecule to the induced absorption and GEabs is the contribution of one molecule to the ground state absorbance of our emitter, or its molar extinction coefficient. These values are then normalised. The rise time of the induced absorbance is taken to be instantaneous, as the ISC process is complete within a few 10 s of ps. The rate of the subsequent decay is primarily determined by two terms in eqn (1): kp[XT] and kTET[XT][YG]. As [XT] is always small, the kXXTTA[XT]2 term has little impact. After the delayed bleach builds, it then decays at some rate, determined by terms in eqn (2): at high [YT], the 2kYYTTA[YT]2 term is dominant, and at longer times the kNR[YT] term takes over.
| ΔOD = [XT] × TSabs − [YT] × GEabs | (4) |
It is clear that at each stage of the curve our rate model fits the experimental data well, showing that each regime is described by the model in a physically consistent way. The principal source of uncertainty in this calculation is the value of GEabs. The probe beam produces much lower intensity at shorter wavelengths, from which GEabs is derived. A more accurate measurement of GEabs would not alter the dynamics of the decay curve, it would simply scale the normalised ΔOD axis.
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