Abstract
Triplet-triplet annihilation upconversion (TTA-UC) has great potential for significantly improving the light harvesting capabilities of photovoltaic cells, as well as being sought after for biomedical applications. Many factors combine to influence the overall efficiency of TTA-UC, the most fundamental of which is the spin statistical factor, η, that gives the probability that a bright singlet state is formed from a pair of annihilating triplet states. Using solid rubrene as a model system, we reiterate why experimentally measured magnetic field effects prove that annihilating triplets first form weakly exchange-coupled triplet-pair states. This is contrary to conventional discussions of TTA-UC that implicitly assume strong exchange coupling and we show that it has profound implications for the spin statistical factor η. For example, variations in intermolecular orientation tune η from 2/5 to 2/3 through spin mixing of the triplet-pair wavefunctions. Since the fate of spin-1 triplet-pair states is particularly crucial in determining η, we investigate it in rubrene using pump-push-probe spectroscopy and find additional evidence for the recently reported high-level reverse intersystem crossing channel. We incorporate all of these factors into an updated model framework in which to understand the spin statistics of TTA-UC, and use it to rationalise the differences in reported values of η amongst different common annihilator systems. We suggest that harnessing high-level reverse intersystem crossing channels in new annihilator molecules may be a highly promising strategy to exceed any spin statistical limit.
Supplementary materials
Title
Supplementary Information for "Spin statistics for triplet-triplet annihilation upconversion: exchange coupling, intermolecular orientation and reverse intersystem crossing"
Description
Includes:
* Further analysis of transient absorption data
* Pump-push-probe spectroscopy of a polycrystalline rubrene film (including discussion of alternative explanations for the pump-push-probe data why we discount them)
* Rate equations and constants for the extended kinetic scheme
* Literature values of spin statistical factors and energy levels.
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