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Sonstige beteiligte Institutionen
- Bavarian Center for Applied Energy Research (ZAE Bayern), 97074 Würzburg, Germany (1)
- Biomedizinische NMR Forschungs GmbH am Max-Planck-Institut fuer biophysikalische Chemie (1)
- Genelux Corporation, San Diego Science Center, 3030 Bunker Hill Street, Suite 310, San Diego, California 92109, USA (1)
- MRB Forschungszentrum für Magnet-Resonanz-Bayern e.V., Am Hubland, D-97074 Würzburg (1)
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- D-1250-2010 (1)
Background
The aortic pulse-wave velocity (PWV) is an important indicator of cardiovascular risk. In recent studies MRI methods have been developed to measure this parameter noninvasively in mice. Present techniques require additional hardware for cardiac and respiratory gating. In this work a robust self-gated measurement of the local PWV in mice without the need of triggering probes is proposed.
Methods
The local PWV of 6-months-old wild-type C57BL/6J mice (n=6) was measured in the abdominal aorta with a retrospectively triggered radial Phase Contrast (PC) MR sequence using the flow-area (QA) method. A navigator signal was extracted from the CMR data of highly asymmetric radial projections with short repetition time (TR=3 ms) and post-processed with high-pass and low-pass filters for retrospective cardiac and respiratory gating. The self-gating signal was used for a reconstruction of high-resolution Cine frames of the aortic motion. To assess the local PWV the volume flow Q and the cross-sectional area A of the aorta were determined. The results were compared with the values measured with a triggered Cartesian and an undersampled triggered radial PC-Cine sequence.
Results
In all examined animals a self-gating signal could be extracted and used for retrospective breath-gating and PC-Cine reconstruction. With the non-triggered measurement PWV values of 2.3±0.2 m/s were determined. These values are in agreement with those measured with the triggered Cartesian (2.4±0.2 m/s) and the triggered radial (2.3±0.2 m/s) measurement. Due to the strong robustness of the radial trajectory against undersampling an acceleration of more than two relative to the prospectively triggered Cartesian sampling could be achieved with the retrospective method.
Conclusion
With the radial flow-encoding sequence the extraction of a self-gating signal is feasible. The retrospective method enables a robust and fast measurement of the local PWV without the need of additional trigger hardware.
Atomare Ketten, sogenannte Nano-Drähte, entstehen durch Selbstorganisation adsorbierter Metallatome auf einer Halbleiteroberfläche. Aufgrund der starken räumlichen Einschränkung der Ladungsträger innerhalb dieser Ketten entsteht dabei oftmals eine metallische Bandstruktur mit starker Anisotropie. Im Falle phononischer Ankopplung an das Substrat kann so ein eindimensionales (1D) Metall instabil gegen eine periodische Gitterverzerrung werden, bei der es zu einer Ausbildung einer Energielücke kommt. Dieser Metall-Isolator-Übergang wird dabei als Peierls Übergang bezeichnet. Für verschwindend geringe Kopplung der Ketten untereinander bzw. an das Substrat, d.h. im strikt eindimensionalen Fall, bricht das Fermi Flüssigkeitsmodell für dreidimensionale (3D) Metalle zusammen. Dessen Quasiteilchen werden durch kollektive Anregungen von Spin und Ladung ersetzt. Diesen Zustand bezeichnet man als Tomonaga-Luttinger Flüssigkeit. Beide Phänomene, Peierlsübergang und Tomonaga-Luttinger Flüssigkeit lassen sich anhand der elektronischen Bandstruktur experimentell nachweisen. Bei dem hier untersuchten Probensystem handelt es sich um Gold-induzierte Nandrähte auf der Germanium (001)-Oberfläche, kurz Au/Ge(001). Deren Wachstum erfolgt epitaktisch entlang der durch das Substrat vorgegebenen Dimer-Reihen, welche die freie Germaniumoberfläche in Form einer (2×1)-Symmetrie einnimmt. Die abwechselnde Stapelfolge ABAB des Substrates führt dabei zu zwei unterschiedlichen Drahtrichtungen, die jeweils um 90° zueinander gedreht sind, wenn man eine Einfachstufe von 1.4 A von einer A-Terrasse auf eine B-Terrasse oder umgekehrt geht. Die vorherrschende Kinetik während der Gold-Deposition bzw. das Benetzungsverhalten ermöglicht dabei eine vollständige Bedeckung der vormals freien Oberfläche mit Nanodrähten, deren Abmessungen einzig und allein durch Defekte bzw. die Größe der darunterliegenden Ge-Terrasse begrenzt sind. Um die Längenskala der Subtrat-Terrassen zu optimieren, wurde eine Reinigungsprozedur für Ge (001) entwickelt, bei der nass-chemisches Ätzen mit anschliessender Trocken-Oxidation zum Einsatz kommt. Die darauf aufbauenden Nanodrähte wurden im Anschluss mittels winkelaufgelöster Photoelektronenspektroskopie auf ihre elektronische Bandstruktur untersucht. Dabei wurden zwei neuartige Zustände beobachtet: ein metallischer, zweidimensionaler Loch-Zustand, der seinen Ursprung höchstwahrscheinlich in tieferen Schichten des Germaniums hat; und ein eindimensionaler Oberflächenzustand mit elektronenartiger Dispersion, dessen bandintegrierte Spektralfunktion von der einer Fermiflüssigkeit abweicht. Stattdessen wird ein exponentieller Abfall des spektralen Gewichtes als Funktion der Energie zum Ferminiveau hin beobachtet. Dieses Verhalten kann über einen weiten Temperaturbereich beobachtet werden und lässt sich mit der Tomonaga-Luttinger Flüssigkeit für strikt eindimensionale Systeme erklären. Zum weiteren theoretischen Verständnis dieses Phänomes, beispielsweise durch Bandstrukuturrechnungen mittels Dichte-Funktional-Theorie, bedarf es der genauen Kenntnis der atomaren Struktur dieser Ketten. Selbige wurde mittels Oberflächenröntgenbeugung (engl. surface x-ray diffraction, SXRD) untersucht. Auf Basis der gewonnenen Patterson-Karte lassen sich Rückschlüsse auf die interatomaren Abstände der Goldatome untereinander in der Einheitszelle ziehen. Dies stellt einen ersten wichtigen Schritt auf dem Weg zu einem vollständigen Strukturmodell dar. Darüber hinaus wurden erste vielversprechende Schritte unternommen, das Nanodrahtsystem kontrolliert zu manipulieren. Durch geringfügige, zusätzliche Deposition von Kalium konnte dabei eine schrittweise Erhöhung der Bandfüllung erzielt werden. Für weitergehende Kaliumanlagerungen im (Sub-)Monolagenbereich konnte sogar eine neue Rekonstruktion erzielt werden.
Continuously increasing energy prices have considerably influenced the cost of living over the last decades. At the same time increasingly extreme weather conditions, drought-filled summers as well as autumns and winters with heavier rainfall and worsening storms have been reported. These are possibly the harbingers of the expected approaching global climate change. Considering the depletability of fossil energy sources and a rising distrust in nuclear power, investigations into new and innovative renewable energy sources are necessary to prepare for the coming future.
In addition to wind, hydro and biomass technologies, electricity generated by the direct conversion of incident sunlight is one of the most promising approaches. Since the syntheses and detailed studies of organic semiconducting polymers and fullerenes were intensified, a new kind of solar cell fabrication became conceivable. In addition to classical vacuum deposition techniques, organic cells were now also able to be processed from a solution, even on flexible substrates like plastic, fabric or paper.
An organic solar cell represents a complex electrical device influenced for instance by light interference for charge carrier generation. Also charge carrier recombination and transport mechanisms are important to its performance. In accordance to Coulomb interaction, this results in a specific distribution of the charge carriers and the electric field, which finally yield the measured current-voltage characteristics. Changes of certain parameters result in a complex response in the investigated device due to interactions between the physical processes. Consequently, it is necessary to find a way to generally predict the response of such a device to temperature changes for example.
In this work, a numerical, one-dimensional simulation has been developed based on the drift-diffusion equations for electrons, holes and excitons. The generation and recombination rates of the single species are defined according to a detailed balance approach. The Coulomb interaction between the single charge carriers is considered through the Poisson equation. An analytically non-solvable differential equation system is consequently set-up. With numerical approaches, valid solutions describing the macroscopic processes in organic solar cells can be found. An additional optical simulation is used to determine the spatially resolved charge carrier generation rates due to interference.
Concepts regarding organic semiconductors and solar cells are introduced in the first part of this work. All chapters are based on previous ones and logically outline the basic physics, device architectures, models of charge carrier generation and recombination as well as the mathematic and numerical approaches to obtain valid simulation results.
In the second part, the simulation is used to elaborate issues of current interest in organic solar cell research. This includes a basic understanding of how the open circuit voltage is generated and which processes limit its value. S-shaped current-voltage characteristics are explained assigning finite surface recombination velocities at metal electrodes piling-up local space charges. The power conversion efficiency is identified as a trade-off between charge carrier accumulation and charge extraction. This leads to an optimum of the power conversion efficiency at moderate to high charge carrier mobilities. Differences between recombination rates determined by different interpretations of identical experimental results are assigned to a spatially inhomogeneous recombination, relevant for almost all low mobility semiconductor devices.
In the presented thesis, the various excited states encountered in conjugated organic semiconductors are investigated with respect to their utilization in organic thin-film solar cells. Most of these states are spin-baring and can therefore be addressed by means of magnetic resonance spectroscopy. The primary singlet excitation (spin 0), as well as positive and negative polaronic charge carriers (spin 1/2) are discussed. Additionally, triplet excitons (spin 1) and charge transfer complexes are examined, focussing on their differing spin-spin interaction strength. For the investigation of these spin-baring states especially methods of electron paramagnetic resonance (EPR) are best suited. Therefore according experimental methods were implemented in the course of this work to study conjugated polymers, fullerenes and their blends with continuous wave as well as time-resolved EPR and optically detected magnetic resonance.
The present thesis is concerned with the impact of alkali metal-doping on the electronic structure of semiconducting organic thin films. The organic molecular systems which have been studied are the polycyclic aromatic hydrocarbons picene, pentacene, and coronene. Motivated by reports about exceptional behavior like superconductivity and electronic correlations of their alkali metal-doped compounds, high quality films fabricated from the above named molecules have been studied. The electronic structure of the pristine materials and their doped compounds has been investigated using photoelectron spectroscopy. Core level and valence band studies of undoped films yield excellent photoemission spectra agreeing with or even outperforming previously reported data from the literature. Alkali metal-doping manifests itself in a uniform manner in the electronic structure for all probed samples: Opposed to reports from the literature about metallicity and even superconductivity in alkali metal-doped picene, pentacene, and coronene, all films exhibit insulating nature with an energy gap of the order of one electron-volt. Remarkably, this is independent of the doping concentration and the type of dopant, i.e., potassium, cesium, or sodium. Based on the interplay between narrow bandwidths in organic semiconductors and sufficiently high on-molecule Coulomb repulsion, the non-metallicity is attributed to the strong influence of electronic correlations leading to the formation of a Mott insulator. In the case of picene, this is consolidated by calculations using a combination of density functional theory and dynamical mean-field theory. Beyond the extensive considerations regarding electronic correlations, further intriguing aspects have been observed. The deposition of thin picene films leads to the formation of a non-equilibrium situation between substrate and film surface. Here, the establishment of a homogeneous chemical potential is hampered due to the only weak van der Waals-interactions between the molecular layers in the films. Consequently, spectral weight is measurable above the reference chemical potential in photoemission. Furthermore, it has been found that the acceptance of additional electrons in pentacene is limited. While picene and coronene are able to host up to three extra electrons, in pentacene the limit is already reached for one electron. Finally, further extrinsic effects, coming along with alkali metal-doping, have been scrutinized. The oxidation of potassium atoms induced by the reaction with molecular oxygen in the residual gas of the ultra-high vacuum system turned out to significantly influence the electronic structure of alkali metal-doped picene and coronene. Moreover, also the applied X-ray and UV irradiation caused a certain impact on the photoemission spectra. Surprisingly, both effects did not play a role in the studies of potassium-doped pentacene.
The present thesis deals with the fabrication, optimization of growth process and characterization of silicon based materials with molecular beam epitaxy. Two material systems are investigated in the course of this work: silicon/silicon suboxide multilayer structures and mono manganese silicide thin films. Mono manganese silicide (MnSi) is grown on Si(111) substrates with an hydrogen passivated surface, that is prepared by wet chemical processes. The growth start is performed by deposition of an amorphous Mn wetting layer that is subsequently annealed to form a MnSi seed layer on which the MnSi molecular beam epitaxy (MBE) is achieved. An amorphous or a crystalline Si cap layer is deposited onto the MnSi film to finalize the growth process and protect the sample from oxidation. With Raman spectroscopy it is shown that the crystalline cap layer is in fact single crystalline silicon. Results of x-ray diffraction and Raman spectroscopy confirm the growth of mono manganese silicide in contrast to other existing manganese silicide phases. In addition, in-plane and out-of-plane residual strain, and twinning of the MnSi thin film is detected with x-ray diffraction of symmetric and asymmetric reflections. Orientation between the Si substrate and the MnSi film is determined with the parallel lattice planes MnSi(210) and Si(511). Transport measurements show a T^2 dependence of the resistivity below 30K and metallic behavior above, a magneto resistance of 0.9% and an unusual memory like effect of the resistance for an in-plane magnetic field sweep measurement. Silicon/Silicon suboxide (SiOx) multilayer structures are grown on Si(100) by interrupting the Si growth and oxidizing the surface with molecular oxygen. During oxidation the RHEED pattern changes from the Si(2x1) reconstruction to an amorphous pattern. When silicon growth is resumed a spotty RHEED pattern emerges, indicating a rough, three dimensional surface. The rough surface can be smoothed out with Si growth at substrate temperatures between 600°C and 700°C. Measurements with transmission electron microscopy show that a silicon suboxide layer of about 1nm embedded in single crystalline silicon is formed with the procedure. Multilayer structures are achieved by repeating the oxidation procedure when the Si spacer layer has a smooth and flat surface. The oxygen content of the suboxide layers can be varied between 7.6% and 26.8%, as determined with secondary ion mass spectrometry and custom-built simulations models for the x-ray diffraction. Structural stability of the multilayer structures is investigated by x-ray diffraction before and after rapid thermal annealing. For temperatures up to 1000°C the multilayer structures show no modification of the SiOx layer in x-ray diffraction.
In the context of this thesis, the novel method soft X-ray energy-dispersive NEXAFS spectroscopy was explored and utilized to investigate intermolecular coupling and post-growth processes with a temporal resolution of seconds. 1,4,5,8- naphthalene tetracarboxylic acid dianhydride (NTCDA)multilayer films were the chosen model system for these investigations. The core hole-electron correlation in coherently coupled molecules was studied by means of energy-dispersive near-edge X-ray absorption fine-structure spectroscopy. A transient phase was found which exists during the transition between a disordered condensed phase and the bulk structure. This phase is characterized by distinct changes in the spectral line shape and energetic position of the X-ray absorption signal at the C K-edge. The findings were explained with the help of theoretical models based on the coupling of transition dipole moments, which are well established for optically excited systems. In consequence, the experimental results provides evidence for a core hole-electron pair delocalized over several molecules. Furthermore, the structure formation of NTCDA multilayer films on Ag(111) surfaces was investigated. With time-resolved and energy-dispersive NEXAFS experiments the intensity evolution in s- and p-polarization showed a very characteristic behavior. By combining these findings with the results of time-dependent photoemission measurements, several sub-processes were identified in the post- growth behavior. Upon annealing, the amorphous but preferentially flat-lying molecules flip into an upright orientation. After that follows a phase characterized by strong intermolecular coupling. Finally, three-dimensional islands are established. Employing the Kolmogorov-Johnson-Mehl-Avrami model, the activation energies of the sub-processes were determined.
The present thesis studies the (Ga,Mn)As material in terms of optimization of very thin (4 nm) (Ga,Mn)As layers, epitaxially fabricated by the molecular beam epitaxy (MBE) technology. First of all, the ferromagnetic semiconductor (Ga,Mn)As with its structural, magnetic and electrical properties is introduced. The influences of point defects, interface and surface effects on bulk and thin (Ga,Mn)As layers are discussed by simplified self-consistent band alignment calculations. The experimental part is divided in three blocks: The first part studies the influence of epitaxial growth parameter conditions on electrical and magnetic properties of bulk (70 nm) (Ga,Mn)As layers. The second part introduces an alternative, parabolical Mn doping-profile instead of a 4 nm layer with a homogeneous Mn doping-profile. Improved properties of the parabolic layer have been observed as well as comparable magnetic and electrical properties to bulk (Ga,Mn)As layers, both with a Mn content of 4%. MBE growth parameters for the (Ga,Mn)As layers with a parabolically graded Mn profile and lowered nominal Mn content of 2.5% have been investigated. A narrow growth window has been found in which low-temperature (LT) layer properties are improved. The last part of this thesis presents an application of magnetic anisotropy control of a bulk (Ga,Mn)As layer.
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.
In this work, we take a look at the connection of gamma-ray bursts (GRBs) and ultra-high-energy cosmic rays (UHECR) as well as the possibilities how to verify this connection. The currently most promising approach is based on the detection of high-energy neutrinos, which are associated with the acceleration of cosmic rays. We detail how the prompt gamma-ray emission is connected to the prediction of a neutrino signal. We focus on the interactions of photons and protons in this regard. At the example of the current ANTARES GRB neutrino analysis, we show the differences between numerical predictions and older analytical methods. Moreover, we discuss the possibilities how cosmic ray particles can escape from GRBs, assuming that UHECR are entirely made up of protons. For this, we compare the commonly assumed neutron escape model with a new component of direct proton escape. Additionally, we will show that the different components, which contribute to the cosmic ray flux, strongly depend on the burst parameters, and test the applicability on some chosen GRBs. In a further step, we continue with the considerations regarding the connection of GRBs and UHECR by connecting the GRB source model with the cosmic
ray observations using a simple cosmic ray propagation code. We test if it is possible to achieve the observed cosmic ray energy densities with our simple model and what the consequences are regarding the prompt GRB neutrino flux predictions as well as the cosmogenic neutrinos. Furthermore, we consider the question of neutrino lifetime and how it affects the prompt GRB neutrino flux predictions. In a final chapter, we show that it is possible to apply the basic source model with photohadronic interactions to other types of sources, using the example of the microquasar Cygnus X-3.