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Besides established, conventional inorganic photovoltaics—mainly based on silicon—organic photovoltaics (OPV) are well on the way to represent a lowcost, environment friendly, complementary technology in near future. Production costs, solar cell lifetime and performance are the relevant factors which need to be optimized to enable a market launch of OPV. In this work, the efficiency of organic solar cells and their limitation due to charge carrier recombination are investigated. To analyze solar cells under operating conditions, time-resolved techniques such as transient photovoltage (TPV), transient photocurrent (TPC) and charge extraction (CE) are applied in combination with time delayed collection field (TDCF) measurements. Solution processed and evaporated samples of different material composition and varying device architectures are studied. The standard OPV reference system, P3HT:PC61BM, is analyzed for various temperatures in terms of charge carrier lifetime and charge carrier density for a range of illumination intensities. The applicability of the Shockley Equation for organic solar cells is validated in case of field-independent charge photogeneration. In addition, a consistent model is presented, directly relating the ideality factor to the recombination of free with trapped charge carriers in an exponential density of states. An approach known as j=V reconstruction enables to identify the performance limiting loss mechanism of as-prepared and thermally treated P3HT:PC61BM solar cells. This procedure, involving TPV, CE and TDCF measurements, is extended to samples based on the rather new, low-band gap polymer PTB7 in combination with PC71BM. While in the devices processed from pure chlorobenzene solution considerable geminate and nongeminate losses are observed, the use of a solvent additive facilitates efficient polaron pair dissociation minimizing geminate recombination. Finally, in collaboration with the IMEC institute in Leuven, the two main organic solar cell device architectures, planar and bulk heterojunction—both based on CuPc and C60—are directly compared in terms of nongeminate recombination and charge carrier distribution. Two experimental techniques, TPV and CE, as well as a macroscopic device simulation are applied to reveal the origin of different Voc vs. light intensity dependence.
Optical antennas work similar to antennas for the radio-frequency regime and convert electromagnetic radiation into oscillating electrical currents. Charge density accumulations form at the antenna surface leading to strong and localized near-fields. Since most optical antennas have dimensions of a few hundred nanometers, their near-fields allow the focusing of electromagnetic fields to volumes much smaller than the diffraction limit, with intensities several orders of magnitude larger than achievable with classical diffractive and refractive optical elements. The task to maximize the emission of a quantum emitter, a point-like entity capable of reception and emission of single photons, is identical to the task to maximize the field intensity at the position of the quantum emitter. Therefore it is desirable to optimize the capabilities of focusing optical antennas.
Radio-frequency-antenna designs scaled to optical dimensions of several hundred nanometers show already a decent performance. However, optical frequencies lie near the plasma frequency of the metals used for optical antennas and the mass of electrons cannot be neglected anymore. This leads to new physical phenomena. Light can couple to charge density oscillations, yielding a so-called Plasmon. Effects emerge which have no equivalent in the very advanced field of radio-frequency-technology, e.g.~volume currents and shortened effective wavelengths. Additionally the conductivity is not infinite anymore, leading to thermal losses. Therefore, the question for the optimal geometry of a focusing optical antenna is not easy to answer. However, up to now there was no evidence that there exist better alternatives for optical antennas than down-scaled radio-frequency designs.
In this work the optimization of focusing optical antennas is based on an approach, which often proved successful for radio-frequency-antennas in complex applications (e.g.~broadband and isotropic reception): evolutionary algorithms. The first implementation introduced here allows a large freedom regarding particle shape and count, as it arranges cubic voxels on a planar, square grid. The geometries are encoded in a binary matrix, which works as a genome and enables the methods of mutation and crossing as mechanism of improvement. Antenna geometries optimized in this way surpass a comparable dipolar geometry by a factor of 2. Moreover, a new working principle can be deduced from the optimized antennas: a magnetic split-ring resonance can be coupled conductively to dipolar antennas, to form novel and more effective split-ring-antennas, as their currents add up constructively near the focal point.
In a next step, the evolutionary algorithm is adapted so that the binary matrices describe geometries with realistic fabrication constraints. In addition a 'printer driver' is developed which converts the binary matrices into commands for focused ion-beam milling in mono-crystalline gold flakes. It is shown by means of confocal two-photon photo-luminescence microscopy that antennas with differing efficiency can be fabricated reliably directly from the evolutionary algorithm. Besides, the concept of the split-ring antenna is further improved by adding this time two split-rings to the dipole-like resonance.
The best geometry from the second evolutionary algorithm inspires a fundamentally new formalism to determine the power transfer between an antenna and a point dipole, best termed 'three-dimensional mode-matching'. Therewith, for the first time intuitive design rules for the geometry of an focusing optical antenna can be deduced. The validity of the theory is proven analytically at the case of a point dipole in from of a metallic nano sphere.
The full problem of focusing light by means of an optical antenna can, thus, be reduced to two simultaneous mode-matching conditions -- on the one hand with the fields of a point dipole, on the other hand with a plane wave. Therefore, two types of ideal focusing optical antenna mode patterns are identified, being fundamentally different from the established dipolar antenna mode. This allows not only to explain the functionality of the evolutionary antennas and the split-ring antenna, but also helps to design novel plamonic cavity antennas, which lead to an enhanced focusing of light. This is proven numerically in direct comparison to a classical dipole antenna design.
In this paper, we present results on the first MBE growth of HgSe. The influence of the GaAs substrate temperature as well as the Hg and Se fluxes on the growth and the electrical properties has been investigated. It has been found that the growth rate is very low at substrate temperatures above 120°C. At 120°C and at lower temperatures, the growth rate is appreciably higher. The sticking coefficient of Se seems to depend inversely on the Hg/Se flux ratio. Epitaxial growth could be maintained at 70°C with Hg/Se flux ratios between lOO and ISO, and at 160°C between 280 and 450. The electron mobilities of these HgSe epilayers at room temperature decrease from a maximum value of 8.2 x 10^3 cm2 /V' s with increasing electron concentration. The concentration was found to be between 6xlO^17 and 1.6x10^19 cm- 3 at room temperature. Rocking curves from X-ray diffraction measurements of the better epilayers have a full width at half maximum of 5S0 arc sec.
The molecular beam epitaxially growth of (001) Hg\(_{1-x}\) Cd\(_z\) Te-HgTe superlattices has been systematically investigated. The well width as well as the period were determined directly by X-ray diffraction. This was accomphshed for the well width by exploiting the high reflectivity from HgTe and the low reflectivity from CdTe for the (002) Bragg reflection. Knowing the well and barrier thicknesses we have been able to set an upper limit on the aver~ge composition of the barriers, Xl, by annealing the superlattice and then measuring the composition of the. resultmg alloy. Xb was shown to decrease exponentially with decreasing barrier width. Xb is appreciably smaller m. narrow barriers due to the increased significance of interdiffusion in the Hg\(_{1-x}\)Cd\(_x\) Te/HgTe interface in narrow barriers. The experimentally determined optical absorption coefficient for these superlattices is compared WIth theoretical calculations. The absorption coefficient was determined from transmission and reflection spectra at 300, 77 and 5 K. Using the thickness and composition of the barriers and wells, and an interface width due to interdiffusion, the complex refractive index is calculated and compared with the experimental absorption coefficient. The envelope function method based on an 8 x 8 second order k . p band model was used to calculate the superlattice states. These results when inserted into Kubo's formula, yield the dynamic conductivity for interband transitions. The experimental and theoretical values for the absorption coefficient using no adjustable parameters are in good agreement for most of the investigated superlattices. Furthermore the agreement for the higher energetic interband transitions is much worse if values for the barrier composition, which are appreciably different than the experimentally determined values, are used. The infrared photoluminescence was investigated at temperatures from 4.2 to 300 K. Pronounced photoluminescence was observed for all superlattices in this temperature range.
The outcomes of measurements on entangled quantum systems can be nonlocally correlated. However, while it is easy to write down toy theories allowing arbitrary nonlocal correlations, those allowed in quantum mechanics are limited. Quantum correlations cannot, for example, violate a principle known as macroscopic locality, which implies that they cannot violate Tsirelson’s bound. This paper shows that there is a connection between the strength of nonlocal correlations in a physical theory and the structure of the state spaces of individual systems. This is illustrated by a family of models in which local state spaces are regular polygons, where a natural analogue of a maximally entangled state of two systems exists. We characterize the nonlocal correlations obtainable from such states. The family allows us to study the transition between classical, quantum and super-quantum correlations by varying only the local state space. We show that the strength of nonlocal correlations—in particular whether the maximally entangled state violates Tsirelson’s bound or not— depends crucially on a simple geometric property of the local state space, known as strong self-duality. This result is seen to be a special case of a general theorem, which states that a broad class of entangled states in probabilistic theories—including, by extension, all bipartite classical and quantum states— cannot violate macroscopic locality. Finally, our results show that models exist that are locally almost indistinguishable from quantum mechanics, but can nevertheless generate maximally nonlocal correlations.
Diese Arbeit befasst sich mit der Konzeption, Umsetzung und Charakterisierung eines Rönt- genmikroskops für harte Röntgenstrahlung mit der Möglichkeit zur dreidimensionalen Bild- gebung. Der vorgestellte Aufbau basiert auf geometrischer Vergrößerung und verzichtet im Gegensatz zu anderen Röntgenmikroskopiemethoden auf den Einsatz optischer Elemente. Dreidimensionale Bildgebung wird durch einen linearlaminographischen Aufnahmemodus realisiert, bei dem unterschiedliche Durchstrahlungsrichtungen durch das Objekt durch eine relative Verschiebung von Quelle und Detektor zustande kommen. Die Röntgenquelle des Mikroskops besteht aus einer zu einer Nanofokusröntgenröhre um- gebauten Elektronenmikrosonde mit 30 kV Beschleunigungsspannung (dies entspricht einer Wellenlänge von bis zu 0,041 nm). Durch die Elektronenoptik kann ein intensiver Elektronen- strahl anstelle eine Probe auf ein Transmissionstarget fokussiert werden. In dieser Arbeit wird eine Möglichkeit evaluiert, die Schichtdicke der röntgenaktiven Schicht des Transmissionstar- gets für die gegebene Beschleunigungsspannung zu optimieren. Dabei werden eine Schichtdi- cke für maximale Röntgenleistung (700 nm Wolfram) und eine für maximale Röntgenleistung bezogen auf die entstehende Quellfleckgröße (100 nm Wolfram) identifiziert. Dadurch erreicht dieses System eine laterale Ortsauflösung von 197 nm, gemessen an einem Siemensstern. Diese ist eine Größenordnung besser als bei modernen SubμCT-Anlagen, die zur zerstörungsfrei- en Prüfung eingesetzt werden, und einen Faktor 2 besser als bei Laborröntgenmikroskopen basierend auf Fresnel’schen Zonenplatten. Abgesehen von der lateralen Auflösung bei hochkontrastigen Objekten werden auch die Abbil- dungseigenschaften für schwach absorbierende Proben mit Inline-Phasenkontrastbildgebung untersucht. Dazu wird eine Methode entwickelt mit der anhand der gegebenen Anlagenpara- meter der optimale Quell-Objekt-Abstand zur Maximierung des Fringe-Kontrasts gefunden werden kann. Dabei wird die Ausprägung des Fringe-Kontrasts auf die Phase −iα zurück geführt. Das vorgeschlagene Modell wird durch Messungen am Röntgenmikroskop und an einer weiteren Röngtenanlage verifiziert. Zur Beurteilung der dreidimensionalen Bildgebung mit dem vorgeschlagenen linearlaminogra- phischen Aufnahmemodus kann dieser auf eine konventionelle Computertomographie mit ein- geschränktem Winkelbereich zurückgeführt werden und so die maximal erreichbare Winkel- information bestimmt werden. Des Weiteren werden numerische Berechnungen durchgeführt, um die Einflüsse von Rauschen und geometrischen Vorgaben einschätzen zu können. Ein experimenteller Test des Laminographiesystems wird anhand eines hochkontrastigen (Fres- nel’sche Zonenplatte) und eines niederkontrastigen Objekts (Kohlefasergewebe) durchgeführt. Es zeigte sich, dass die laterale Auflösung während der dreidimensionalen Rekonstruktion gut erhalten bleibt, die Tiefenauflösung aber nicht die gleiche Qualität erreicht. Außerdem konnte festgestellt werden, dass die Tiefenauflösung sehr stark von der Geometrie und Zusammen- setzung des untersuchten Objekts abhängt.
Unter dem Gesichtspunkt kohärenter Wellenpaketdynamik werden in dieser Arbeit zwei Themenfelder untersucht: Zum einen die Auswirkungen von Kernfreiheitsgraden auf die zweidimensionale vibronische Spektroskopie (2D-Spektroskopie) und zum anderen photoinduzierte Energieverlustmechanismen in organischen Halbleitern. Im ersten Abschnitt wird am numerischen Beispiel zweiatomiger Moleküle gezeigt, dass sich die Anharmonizität der Wellenpaketbewegung durch Variation der Verzögerungszeit der Femtosekundenpulse in der komplexwertigen Spektralfunktion, die aus der störungstheoretischen Berechnung der Polarisationsfunktion hervorgeht, widerspiegelt. Die zeitliche Entwicklung besetzter Vibrationszustände zeigt sich in der Struktur des Signals anhand sogenannter Quantenphasen. Durch Variation der Pulsparameter und -reihenfolge kann dabei die Quantendynamik in unterschiedlichen elektronischen Zuständen charakterisiert werden. Im zweiten Teil der Arbeit wird für molekulare Aggregate (3,4,9,10-Perylentetracarbonsäurediimid und 3,4,9,10-Perylentetracarbonsäuredianhydrid) ein zeitaufgelöstes, atomistisches Bild intra- und intermolekularer Strukturverzerrungen vorgestellt. Letztere induzieren eine ultraschnelle Depopulation der durch Photoabsorption angeregten elektronischen Zustände, was mit einer deutlichen Abnahme der Anregungsenergie einhergeht.
Using k · p theory, we derive an effective four-band model describing the physics of the typical two-dimensional topological insulator (HgTe/CdTe quantum well (QW)) in the presence of an out-of-plane (in the z-direction) inversion breaking potential and an in-plane potential. We find that up to third order in perturbation theory, only the inversion breaking potential generates new elements to the four-band Hamiltonian that are off-diagonal in spin space. When this new effective Hamiltonian is folded into an effective twoband model for the conduction (electron) or valence (heavy hole) bands, two competing terms appear: (i) a Rashba spin–orbit interaction originating from inversion breaking potential in the z-direction and (ii) an in-plane Pauli term as a consequence of the in-plane potential. Spin transport in the conduction band is further analysed within the Landauer–Büttiker formalism. We find that for asymmetrically doped HgTe QWs, the behaviour of the spin-Hall conductance is dominated by the Rashba term.