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The transport of optically excited states, called excitons, as well as their conversion into charges define the two major steps allowing for the operation of organic photovoltaic (OPV) devices. Hence, a deep understanding of these processes, the involved mechanisms as well as possible loss channels is crucial for further improving the efficiency of organic solar cells. For studying the aforementioned processes spectroscopic methods like absorption and emission measurements are useful tools. As many of the processes take place on a sub-nanosecond (ns) timescale ultrafast spectroscopic methods are required. Due to this reason two experiments based on a femtosecond laser system were built and employed in this work, namely picosecond (ps) time-resolved photoluminescence (PL) and transient absorption (TA) spectroscopy.
By analyzing the PL decay dynamics in the prototypical organic semiconductor rubrene, the feasibility of a new approach for improving the efficiency of organic solar cells by harvesting triplet excitons generated by singlet fission was examined. Singlet fission describes a process where two triplet excitons are generated via a photoexcited singlet exciton precursor state if the energy of the two triplets is comparable with the energy of the singlet. For this purpose the influence of characteristic length scales on the exciton dynamics in different rubrene morphologies exhibiting an increasing degree of confinement was analyzed. The results show that the quenching at interfacial states efficiently suppresses the desired fission process if these states are reached by excitons during migration. Since interfacial states are expected to play a significant role in thin film solar cells and are easily accessible for the migrating excitons, the results have to be considered for triplet-based OPV.
While the aforementioned approach is only investigated for model systems so far, the efficiency of disordered organic bulk heterojunction (BHJ) solar cells could be significantly enhanced in the last couple of years by employing new and more complex copolymer donor materials. However, little is known about the photophysics and in particular the excitation dynamics of these systems. By carrying out a systematic optical study on the prominent copolymer PCDTBT and its building blocks we were able to identify the nature of the two characteristic absorption bands and the coupling mechanism between these levels. The latter mechanism is based on an intrachain partial charge transfer between two functional subunits and our time-resolved measurements indicate that this coupling governs the photophysical properties of solar cells based on these copolymers. The efficient coupling of functional subunits can be seen as a key aspect that guarantees for the success of the copolymer approach.
Another important issue concerns the optimization of the morphology of BHJ solar cells. It arises from the discrepancy between the exciton diffusion length \mbox{($\approx$ 10 nm)} and the absorption length of solar irradiation ($\approx$ 100 nm). Due to this reason, even for devices based on new copolymer materials, processing parameters affecting the morphology like annealing or employing processing additives are of major importance. In our combined optical, electrical and morphological study for solar cells based on the high-efficient copolymer PBDTTT-C we find a direct correlation between additive content and intermixing of the active layer. The observed maximum in device efficiency can be attributed to a morphology guaranteeing for an optimized balance between charge generation and transport. Our results highlight the importance of understanding the influence of processing parameters on the morphology of the BHJ and thus on the efficiency of the device.
In the course of this dissertation, we have presented the interest of using spectroscopic methods to unravel the physics of polymer semiconductors in photovoltaic applications. Applying photoluminescence and photoinduced absorption spectroscopy to the reference system P3HT:PCBM has enabled us to study the major steps of photocurrent generation in organic bulk heterojunctions, from excitons generation to charges extraction and loss mechanisms and thus to improve the understanding of those mechanisms.
The exciton binding energy, is the first obstacle to overcome for photocurrent generation in organic solar cell and the reason for the use of two materials, whose heterojunction act as a driving force for charge separation. We developed an original photoluminescence-detected field-induced exciton quenching method to investigate this energy. Absorption and photoluminescence spectra of pure P3HT show that, while both amorphous and crystalline domains participate in
absorption, the energy is then transferred to the crystalline domains, from where the photoluminescence is exclusively originating. The field dependence of this photoluminescence showed that an energy of no less than 420 meV is necessary to split excitons into non photon-emitting species. Comparing those results with energy levels obtained by absorption and photoelectron spectroscopies, confirmed that the formation of those species is only a first step toward dissociation into free charges. Indeed, photoemission spectroscopy and the onset
of photocurrent upon increasing the photon energy in a pure P3HT solar cell, concomitantly show that the energy level of a pair of free polarons is located 0.7 eV above the one of the exciton. The comprehensive analysis of those results originating from those different method enable us to draw a global picture of the states and energies involved in free polarons generation in pure material. This work has been widely acknowledged by the scientific community, published in Physical Review B in 2010 [1] and presented in national [2] and international [3] conferences.
The spectroscopy of excited states is used to detect the presence of wanted species (charges) and potentially unwanted neutral species upon photoexcitation. As such, it offers us the possibility to qualify the efficiency of charge generation and, if any, identify the competing processes and the generation of unwanted species. In the frame of the European Marie Curie Research Network SolarNType,[4] this possibility was used - in combination with morphological,
charge transport and devices characterizationsn - to study a number of new donor:acceptor blends. Thanks to those techniques, we were able to not only quantify the potential of those blends, but also to provide the chemist laboratories with a precious and detailed feedback on the strengths and weakness of the molecules, regarding charge generation, transport and extraction. The detailed study of terrylene-3,4:11,12-bis(dicarboximide) as electron acceptor for
solar cells application was published in the peer review journal Synthetic Metals and was chosen to illustrate the cover page of the issue [5].
Finally, in the last chapter, we have used time resolved photoinduced absorption to improve the understanding of the charge carrier loss mechanisms in P3HT:PCBM active layers. This comprehension is of prime importance because, the fact that this recombination is far weaker than expected from the Langevin theory, enable polarons to travel further without recombining and thus to build thicker and more efficient devices. A comprehensive analysis of steady-state
PIA spectra of pure P3HT, indicates that probing at 980 nm at a temperature between 140 and 250 K enables to monitor specifically polaron densities in both neat P3HT and P3HT:PCBM. Applying this finding to transient absorption enabled us to monitor, for the first time, the bimolecular recombination in pure P3HT, and to discover that - in sharp contrast with the blend - this recombination was in agreement with the Langevin theory. Moreover, it enables us to pinpoint the important role played by the existence of two materials and of energetical traps in the slow recombination and high recombination orders observed in the blend. This work has been published in the Journal of Applied Physics.[6]
Those new insights in the photophysics of polymer:fullerene photoactive layers could have a strong impact on the future developement of those materials. Consistent measurements of the binding energy of excitons and intermediate species, would enable to clarify the role played by excess thermal energy in interfacial states dissociation. Better understanding of blends
morphology and its influence on solar cells parameters and in particular on recombination could enable to reproduce the conditions of limited recombination on material systems offering some promising performances but with only limited active layer thicknesses. However, due to the number of parameters involved, further experimentation is required, before we can reach a quantitative modeling of bimolecular recombination.
[1] Deibel et al., Phys. Rev. B, 81:085202, 2010
[2] Gorenflot et al., Deutsche Physikalische Gesellschaft Frühjahrstagung 2010, CPP20:10, Regensburg, Germany, 2010
[3] Gorenflot et al., International Conference of Synthetic Metals, 7Ax:05, Kyoto, Japan, 2010
[4] Marie-Curie RTN "SolarNTyp" Contract No. MRTN-CT-2006-035533
[5] Gorenflot et al., Synth. Met., 161(23{24):2669-2676, 2012
[6] Gorenflot et al., J. Appl. Phys., 115(14):144502, 2014
In this work, three different material systems comprising carbon were researched: (i) Organic polymers and small molecules, in conjunction with fullerene molecules for applications in organic photovoltaics (OPV), (ii) single walled semiconducting carbon nanotubes and (iii) silicon carbide (SiC), whose defect color centers are recently in the limelight as candidates for quantum applications. All systems were analyzed using the optically detected magnetic resonance (ODMR) spectroscopy.
In the OPV chapter, first the intrinsic parameters and orientations of high spin excitons were analyzed in the materials P3HT, PTB7 and DIP. Specifically the influence of ordering in these organic systems was adressed. The second part of the OPV chapter is concerned with triplet generation by electron back transfer in the high-efficiency OPV material combination PTB7:PC71BM.
The carbon nanotube chapter first shows the way to the first unambiguous proof of the existence of triplet excitons in semiconducting (6,5) single-walled carbon nanotubes (SWNT) by ODMR spectroscopy. A model for exciton kinetics, and also orientation and intrinsic parameters were propoesed.
The last part of this work is devoted to spin centers in silicon carbide (SiC). After a brief introduction, the spin multiplicity of the V2 and V3 silicon vacancies, and also of a Frenkel pair and an unassigned defect UD in 6H SiC, and of the V2 vacancy and the Frenkel pair in 4H SiC, was shown to be S=3/2. The spin polarized pumping of the 3/2 manifold of the quartet ground state of the silicon vacancies allows stimulated microwave emission. Furthermore, in 6H SiC, the UD and Frenkel pair were shown to have a large dependence of their intrinsic zero field interaction parameters on the temperature, while the vacancies are temperature independent. The application of the UD and Frenkel pair as temperature sensor, and of the vacancies as a vector magnetic field sensor is discussed.