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Asymmetrical capacitively coupled RF discharges in oxygen, argon and hydrogen have been experimentally investigated with the innovative technique of the phase resolved optical emission spectroscopy. This diagnostic tool allows to measure spatio-temporally resolved emission intensities of electronically excited species with a high resolution. The spatial (axial) resolution was better than 1 mm and a temporal resolution of about 1.5 ns has been achieved. Therefore the plasma induced optical emission within the RF cycle (TRF = 73.75 ns) from the RF sheath region with a typical mean sheath thickness of about 5mm has been studied. Spatio-temporally resolved optical emission patterns of the following optical transitions have been measured for a total gas pressure in the range of 20 to 100 Pa and self-bias voltages between -50 and -550 V: Oxygen plasma Emission at 777.4 nm and 844.6 nm (atomic oxygen) Argon plasma Emission at about 751 nm and 841 nm (argon) Hydrogen plasma Emission at 656.3nm (atomic hydrogen, H alpha-line) These transitions are the most prominent ones of the investigated excited species in these plasmas as could be shown from overview spectra of the plasma induced optical emission in the range from 350 to 850 nm. For the first time such extensive PROES measurements in oxygen CCRF plasmas are presented in this work. The additional investigations of argon and hydrogen plasmas serve as a reference and for a direct comparison with results from the literature. The temporal behavior of the emission intensity is influenced by the effective lifetime of the emitting states which is on the order of the nanosecond time scale of the RF cycle. Therefore, it does not represent the real temporal behavior of the excitation. A simple method has been applied to calculate relative excitation rates from the measured emission intensities to distinguish different excitation mechanisms and their correct relative temporal behavior. In a close collaboration within the framework of the Sonderforschungsbereich Transregio 24 'Fundamentals of Complex Plasmas' a newly 1d3v PIC-MCC code for simulations of capacitive RF discharges in oxygen has been developed by Matyash et al. The very close coupling of experiment and modeling allowed a really detailed and microscopic understanding of the processes and dynamics from the sheath to the bulk plasma in CCRF discharges. The spatio-temporally resolved excitation rate profiles show four different excitation structures (I-IV). Excitation processes due to the following mechanisms in CCPs could be identified and characterized: I Electrons expelled from growing sheath II Electrons detached from negative ions (collisions with neutrals) + secondary electrons from the electrode surface (ion bombardment) III Field-reversal effect, reduced mobility of electrons (electron-neutral collisions) IV Heavy-particle collisions These excitation mechanisms are characterized by different temporal and spatial behaviors of the excitation rate within the RF cycle. Additionally it has been shown that the excitation by electron impact in the investigated oxygen plasmas results mainly from dissociative electron impact excitation (O2 + e -> O + O* + e) and not from direct electron impact excitation (O + e -> O* + e). Actinometry measurements show that the results are not really credible. Thus actinometry is not applicable on the investigated oxygen RF plasma. A challenge in interpretation is the observed excitation pattern IV. Pattern IV has to be caused in connection with heavy particle collisions nearby the electrode surface and could be observed in all the three plasmas oxygen, argon and hydrogen. It is located directly in front of the powered electrode and appears during almost the whole RF cycle. The temporal modulation is nearly sinusoidal and weak in comparison to the first three patterns. This is due to the weak RF modulation of the ion flux towards the electrode surface which has been proven by a PIC simulation. It could be shown that the modulation degree of pattern IV depends on the transition time of the corresponding positive ions through the RF sheath which is influenced by the ion mass. In oxygen as well as in argon CCRF plasmas pattern IV is less modulated than in hydrogen CCRF plasmas due to the heavier ions in oxygen and argon. Additionally the modulation degree increases with increasing pressure due to the more confined plasma at higher pressures which is yielding in a stronger modulated ion current towards the powered electrode.
In the present work, mass determinations of the eleven neutron-deficient nuclides (99-109)Cd, of ten neutron-rich silver nuclides (112-114,121,123)Ag, and seven neutron-rich cadmium nuclides (114,120,122-124,126,128)Cd are reported. Due to the clean production of the neutron-deficient nuclides it was possible to reduce the experimental uncertainties down to 2 keV, whereas the measurements of neutron-rich nuclides were hampered by the presence of contaminations from more stable In and Cs nuclides. In the case of 99Cd and 123Ag the masses were determined for the first time and for the other nuclides the mass uncertainties could be reduced by up to a factor of 50 as in the case of 100Cd. In the case of a potential isomeric mixture as for (115,117,119)Ag and 123Cd, where no assignment to either the ground state or the excited state was possible, the experimental results were adjusted accordingly. Afterwards all results were included in the framework of the atomic-mass evaluation and thus linked and compared with other experimental data. In the case of the neutron-deficient Cd nuclides a conflict between the mass values obtained in the present work and those published by the JYFLTRAP group could be solved by performing an atomic-mass evaluation. These mass measurements are an important step towards an understanding of the physics of the rp process that will enable a more reliable determination of the composition of the produced material at A = 99. It has been shown that the mass of 99Cd strongly affects the A = 99 production in an X-ray burst model, and that uncertainties have been significantly reduced from more than an order of magnitude to about a factor of 3. The dominant source of uncertainty is now the mass of 100In. In principle, other uncertainties will also contribute. These include those of masses of lighter Cd isotopes, where similar rp-process branchpoints occur and which might affect feeding into the 99Cd branchpoint. In addition, nuclear reaction rate uncertainties will also play a role. However, as reaction rates affect branchings in a linear fashion, while mass differences enter exponentially, mass uncertainties will tend to dominate. Also, which reaction rates are important depends largely on nuclear masses. For example, for low Sp(100In) a (p,γ)-(γ,p) equilibrium will be established between 99Cd and 100In and the 100In(p,γ) reaction rate would affect the A = 99 production, while for larger Sp(100In) the 99Cd(p,γ) reaction rate might be more relevant. Therefore, the mass uncertainties should be addressed first. The presented results are relevant for any rp-process scenario with a reaction flow through the 99Cd region. Here, an X-ray burst model has been used to investigate in detail the impact of the present measurements on such an rp process. The νp process in core collapse supernovae might be another possible scenario for an rp process in the 99Cd region. It it is planed to also explore whether in that case mass uncertainties have a similar impact on the final composition. On the neutron-rich side of the valley of stability for the Cd and Ag chains of nuclides, the r process has not yet been reached. Further technical development on suppression of contaminants are required. This includes improvements on the ISOLDE side, e.g., by improving the selectivity of the transfer line or on the ISOLTRAP setup by implementing an electrostatic ion beam trap for a fast and efficient isobaric selection. Nevertheless the obtained results contribute to the knowledge of nuclear structure. The trends in the two-neutron separation-energy S2n and the interaction between the last neutrons and last protons ΔVpn were corrected to more smooth evolutions, as already seen in other regions of the nuclear chart. The strongest corrections have been observed for even-N nuclides, were more new experimental data are available. Thus, new measurements on odd-N nuclides are suggested. This also is underlined by the trends observed in the Garvey-Kelson relations for the neutron-rich Cd nuclides. Furthermore, it has been shown, that the prominent structure of the ΔVpn for an entire chain of nuclides including inflexion points can be reproduced by using simple relations between quantum numbers of the occupied orbits. This approach connects ten values for each nuclide with only one adjusted parameter. This has been investigated for 63 ΔVpn values of even-even nuclides in the vicinity of Z = 50 and 50 ≤ N ≤ 82. The simple model works remarkably well for the elements Cd, Sn, and Te. Small deviation have been observed for the Xe and Pd nuclides which were explained with the limitations of the model to the vicinity of the close shells, where the nuclides have only few valence protons and neutrons.
The experimental determination of the electron energy distribution of a low pressure glow discharge in neon from emission spectroscopic data has been demonstrated. The method extends an approach by Fischer and Dose [5]. The spectral data were obtained with a simple overview spectrometer and analyzed using a strict probabilistic, Bayesian data analysis. It is this Integrated Data Analysis (IDA) approach, which allows the significant extraction of non-thermal properties of the electron energy distribution function (EEDF). The results bear potential as a non-invasive alternative to probe measurements. This allows the investigation of spatially inhomogeneous plasmas (gradient length smaller than typical probe sheath dimensions) and plasmas with reactive constituents. The diagnostic of reactive plasmas is an important practical application, needed e.g. for the monitoring and control of process plasmas. Moreover, the experimental validation of probe theories for magnetized plasmas as a long-standing topic in plasma diagnostics could be addressed by the spectroscopic method.
The WEGA stellarator is used to confine low temperature, overdense (densities exceeding the cut-off density of the heating wave) plasmas by magnetic fields in the range of B=50-500 mT. Microwave heating systems are used to ignite gas discharges using hydrogen, helium, neon or argon as working gases. The produced plasmas have been analyzed using Langmuir and emissive probes, a single-channel interferometer and ultra-high resolution Doppler spectroscopy. For a typical argon discharge in the low field operation, B=56 mT, the maximum electron density is n_e~10^18m^{-3} with temperatures in the range of T=4-12 eV. The plasma parameters are determined by using Langmuir probes and are cross-checked with interferometry. It is demonstrated within this work that the joint use of emissive probes and ultra-high resolution Doppler spectroscopy allows a precise measurement of the radial electric field. Here the floating potential measurements using emissive probes have been compared to measurements of the poloidal rotation of the plasma which is also linked to the radial electric field. In order to alter the plasma parameters a biasing probe setup has been used during this work. The focus of this work is on demonstrating the ability to modify the existing radial electric field in a plasma by using the biasing probe. This technique is in principle not new, as it has been around for decades. Looking at details, it turns out that describing low field operation WEGA argon plasmas in connection with biasing is not covered by the present set of theoretical approaches and experimental cognition. This work will commence with a basic approach and first establishes the diagnostic tools in a well-known discharge. Then the perturbation caused by the biasing probe is assessed. Following the characterization of the unperturbed plasmas, plasma states altered by the operation of the energized biasing probe will be characterized. It is demonstrated that modifying the existing radial electric field can be achieved and reliably diagnosed using spectroscopy and probe measurements. In order to verify the different approaches for determining the radial electric field the diagnostics are cross-checked against another whenever possible. During biasing the plasma two different stable plasma states have been found. Stable here refers to the state existing much longer than the confinement time for WEGA. The presence of a calorimetric limiter placed in the scrape-off layer has an impact on the type of the plasma state. The two observed plasma states differ in plasma parameter profiles, such as density, temperature, electric field and confined energy. The results are compared to two simple models. One model relies on the relevant atomic processes and a second one is based on neoclassical theory. Both models can be used to derive the particle and power flux from the plasma. The losses predicted by the atomic models can be tested using bolometry. It can be shown that both models agree well in the description of the particle balance of the electrons for large regions of the plasma. By comparing the models the neoclassical heat flux turns out to be small compared to the energy fluxes caused by atomic processes. For the reference discharge taking the energy flux due to the atomic processes and balancing it by the input microwave power is satisfying the energy balance, without the need for transport. For the biased discharges it turns out that neoclassical transport can be neglected as well, but the additional biasing power has to be taken into account. A simple model for the biasing power is motivated and tested. An agreement in the energy balance can be reached in this way as far as the models are applicable. The models also allow drawing conclusions on the amount of absorbed microwave power.
Turbulence is a state of a physical system characterized by a high degree of spatiotemporal disorder. Turbulent processes are driven by instabilities exhibiting complex nonlinear dynamics, which span over several spatial as well as temporal scales. Apart from fluids and gases, turbulence is observed in plasmas. While turbulent mixing of a system is sometimes a desired effect, often turbulence is an undesired state. In hot, magnetically confined plasmas, envisaged for energy generation by thermonuclear fusion, plasma turbulence is clearly a problem, since the magnetic confinement time is drastically deteriorated by turbulent transport. Hence, a control mechanism to influence and to suppress turbulence is of significance for future fusion power devices. An important area of plasma turbulence is drift wave turbulence. Drift waves are characterized by currents parallel to the ambient magnetic field, that are tightly coupled to a coherent mode structure rotating in the perpendicular plane. In the present work, the control of drift waves and drift wave turbulence is experimentally investigated in the linear magnetized helicon experiment VINETA. Two different open-loop control systems - electrostatic and electromagnetic - are used to drive dynamically parallel currents. It is observed that the dynamics of the drift waves can be significantly influenced by both control schemes. If the imposed mode number as well as the rotation direction match those of the drift waves, classical synchronization effects like, e.g., frequency locking, frequency pulling, and Arnold tongues are observed. These confirm the nonlinear interaction between the control signal and the drift wave dynamics. Finally, the broadband drift wave turbulence, and thereby turbulent transport, is considerably reduced if the applied control signal is sufficiently large in amplitude.
In der Frequenz kontinuierlich veränderbare Laser sind interessante Lichtquellen für wissenschaftliche Forschung, Industrie und Technik. In diesem Zusammenhang zeigen insbesondere Diodenlaser mit externem Resonator (ECDL) vorteilhafte Eigenschaften. Weit verbreitet ist der Littrow-Laser, da er aufgrund seines einfachen Designs kostengünstig, kompakt und robust ist und zudem eine geringe Linienbreite aufweist. Das bei ihm eingesetzte Reflexions-Gitter fungiert gleichzeitig als Reflektor und Frequenzfilter. Die Durchstimmung erfolgt mechanisch durch Drehung des Gitters mittels eines Piezo-Aktuators. Diese Vorgehensweise begrenzt sowohl die erreichbare Repetitionsrate als auch Durchstimmbereich und -geschwindigkeit. Um diese Probleme zu umgehen, bietet sich der Einsatz zweier akusto-optischer Modulatoren (AOM) als Deflektor im externen Resonator an. Die Durchstimmung eines solchen AOM-Lasers erfolgt durch Ablenkung des Strahls auf rein nicht-mechanischem Weg. Dazu ist allerdings eine geeignete Ansteuerung der AOMs vonnöten. Im Rahmen dieser Arbeit wurde ein theoretisches Modell entworfen, welches grundlegende Eigenschaften eines AOM-Lasers beschreibt. Darauf basierend konnte ein Algorithmus zur Berechnung der für eine kontinuierliche Durchstimmung notwendigen AOM-Ansteuersignale entwickelt werden. Dieses Modell zeigt zudem, dass zur Realisierung einer Durchstimmung mit gleichzeitig akzeptabler Laser-Linienbreite hohe Anforderungen an die Ansteuerelektronik, insbesondere bezüglich Jitterfreiheit (< 5 ps), gestellt werden, was nur durch eine vollständig digitale Erzeugung der Ansteuersignale mittels sogenannter DDS-ICs (Direct-Digital-Synthesis) erfüllt werden kann. Andere untersuchte Schaltungen zeigten schlechtere Eigenschaften. Aufgrund der guten Übereinstimmung zwischen dem aufgestellten Modell und dem praktischen AOM-Laseraufbau können im roten Spektralbereich kontinuierliche (modensprungfreie) Durchstimmbereiche von bis zu 220 GHz erreicht werden. Die maximale Durchstimmgeschwindigkeit liegt 1.5 GHz/µs. Eine Repetitionsrate von 25 kHz ist realisierbar. Die 0.2-ms-Linienbreite liegt bei 450 kHz. Der Laser konnte außerdem in einem Bereich von 6 nm (4 THz) ohne mechanische Nachjustage operieren. Eine genaue Analyse zeigt, dass trotz der schon sehr guten Performance des Lasersystems durch Verfeinerung des Modells und eine weitere Verbesserung der Komponenten die genannten Leistungsparameter um einen Faktor 5 - 10 gesteigert werden könnten.
In this work, the investigation of dusty plasma by means of tunable diode laser spectroscopy was carried out. Special interest was focused on the interactions of dust particles and metastable atoms. At first, Al density and temperature in dc and pulsed magnetron discharges were measured. Measurements with argon as working gas show an expected behavior of the measured atom density and temperature. Decrease of absorption signal was observed in argon/oxygen and argon/methane mixtures. A small admixture of oxygen leads to a complete disappearance of the absorption signal indicating vanishing Al atom density. The effect is believed to be caused by the oxidation of the magnetron target. This decrease reveals typical hysteresis behavior caused by poisoning of the target. Significant difference between critical oxygen flow value in dc and pulsed modes was registered. Then dust formation and plasma behaviors in hydrocarbon containing plasmas were analysed. The dust growing plasmas (Ar/C2H2, Ar/CH4 and Ar/C3H6 rf plasmas) were characterized by laser transmission and scattering methods, ion energy distribution function and mass spectrum evolution by plasma processing monitor, and the spatial distribution in pristine plasma and the temporal behavior of the metastable atom density in processing plasma using TDLAS. Pristine plasma were then characterized in term of metastable density and temperature. The radial distribution of neon metastable atom density in capacitive coupled rf discharge can be approximated to a Gaussian profile with the width smaller than plasma chamber radius. The diffusion flow of metastable atoms deduced from their spatial density distribution gives the loss of metastable atom in the plasma sheath. Argon metastable density was measured in rf plasma and compared with a simple model for metastable density. The model explains well the trend of metastable density with respect to the change of plasma input power. Metastable density of dusty plasma with injected dust particles was measured and compared to that of pristine plasma. The particle heating by metastable atoms was strongly evidenced. The power absorbed by dust particles due to bombardment of metastable atoms onto a dust particle surface in our experiments is about 0.04 Wm-2 for the low dust density case and lower for higher dust density which is in the same order as the contributions of kinetic energy of ions and electrons and the energy released by their recombination on the grain surface. The influence of dust particle density and size on metastable density was studied. Through measuring metastable density, TDLAS can be used as a tool to study the dust growth process in processing plasma.
Diese Arbeit widmet sich dem Nachweis und der Analyse lateraler Strukturen in molekular dünnen Polyelektrolytschichten an der Luft-Wasser-Grenzfläche. Sie dient insbesondere der Suche nach den Parametern, welche zu Bildung und Zerfall solcher Strukturen führen sowie deren Eigenschaften beeinflussen. Im Zentrum des Interesses stehen dabei zwei sich in geometrischer Hinsicht unterscheidende Systeme: Flach adsorbierte Polyelektrolyte und senkrecht zur Oberfläche ausgerichtete Ketten in Polyelektrolytbürsten. Die zu charakterisierenden Schichten werden durch Spreiten geeigneter Lösungen auf der Wasseroberfläche präpariert und anschließend systematisch veränderten Bedingungen ausgesetzt. Als universelles Werkzeug kommt dabei die Filmwaage zum Einsatz. Sie wird einerseits zur Untersuchung der thermodynamischen Eigenschaften der Schichten verwendet, andererseits können gezielt Umgebungsbedingungen, wie molekulare Fläche, Lateraldruck, Temperatur oder Ionengehalt der Wassersubphase, eingestellt und für die Dauer der strukturanalytischen Messungen aufrecht erhalten werden. Die Charakterisierung des Elektronendichteprofils senkrecht zur Oberfläche erfolgt durch Messung der einfallswinkelabhängigen Intensität spekular reflektierter Röntgenstrahlen. Örtliche Periodizitäten in der Oberflächenebene werden mittels Röntgendiffraktion bei streifendem Einfall aufgelöst. Bei Adsorption des anionischen Polyelektrolyts PSS (Polystyrolsulfonat) aus einer Lösung mit geringer Monomerkonzentration (0.001 bis 1 mmol/l) heraus an eine Monoschicht des kationischen Lipids DODAB (Dioctadecyldimethylammonium Bromid) können sowohl in flüssiger als auch in kondensierter Lipidphase Braggpeaks beobachtet werden, die parallel ausgerichteten Polyelektrolytketten zuzuordnen sind. Damit gelingt erstmals der experimentelle Nachweis der theoretisch vorhergesagten, elektrostatisch stabilisierten, zweidimensionalen lamellaren Phase semiflexibler Polyelektrolytketten. Der Flächenanteil der Bereiche mit parallel ausgerichteten Ketten nimmt bei steigender Monomerkonzentration ab und verschwindet für Monomerkonzentrationen >1 mmol/l. Als zerstörerisch für die zweidimensionale lamellare Phase erweisen sich kurzreichweitige attraktive Kräfte, deren Beiträge mit zunehmender Belegungsdichte und abnehmendem Kettenabstand steigen und die sogar zur Aggregation der Ketten führen können. Zur Erforschung der kurzreichweitigen attraktiven Kräfte sind Polyelektrolytbürsten mit ihren vertikal zur Oberfläche gestreckten Ketten geeignet. Die Bürsten bestehen aus den in die Subphase ragenden anionischen Polyelektrolyten (PSS136 bzw. PAMPS158), welche mit einem Ende an einen flüssigen hydrophoben Ankerblock (PEE144 bzw. PBA76) kovalent gebunden sind. Durch laterale Kompression und Expansion der hydrophoben Schicht kann die Dichte der Ankerpunkte, die ein zweidimensionales hexagonales Gitter bilden, eingestellt werden. Die Ketten formen dabei bündelförmige Aggregate, deren Form und Größe vom Ionengehalt in der wässrigen Subphase abhängt. Bei Erhöhung der Konzentration monovalenter Kationen sind zwei gegenläufige Trends zu beobachten: Der Durchmesser der Bündel vergrößert sich durch steigende Zahl aggregierter Ketten während die Länge der Bündel abnimmt. Beide Effekte sind Folge der durch die Kationen abgeschwächten inter- und intramolekularen elektrostatischen Repulsion. In der osmotischen Bürstenphase mit monovalenten Na+- und Cs+-Gegenionen sind für beide Polyelektrolyte zwei Ketten pro Bündel zu beobachten. Die Länge der Bündel reduziert sich bei Monolayerkompression von 50 Angström auf 25 Angström. In der Salzbürstenphase steigt die Zahl der aggregierten Ketten auf 17 und die Länge bleibt konstant bei 20 Angström, vergleichbar mit der Persistenzlänge einer neutralen Polystyrolkette im Wasser. Divalente Kationen bewirken ionenspezifische Effekte. Bei Austausch von Ca2+ mit Sr 2+ verdoppelt sich die Anzahl der Ketten pro Bündel von 4 auf 8 für PEE144PSS136 bzw. von 2 auf 4 für PBA76PAMS158. Die Länge der Bündel beträgt rund 20 Angström und ist unabhängig von der Ionen- und Polyelektrolytsorte. Bestimmend für die Bündelbildung ist die Balance zwischen langreichweitiger elektrostatischer Repulsion und kurzreichweitiger Attraktion. Die Elektrostatik wird durch die Kettenladungen und die Ionenstärke der Gegenionen beeinflusst. Als anziehende Komponente kommen hydrophober Effekt und/oder van-der-Waals-Kräfte in Frage. Im Gegensatz zu monovalenten Ionen können divalente Kationen darüber hinaus weitere attraktive Beiträge vermitteln.
Titanaluminide auf der Basis von gamma-TiAl können aufgrund der etwa halb so großen Dichte und der guten mechanischen Eigenschaften im Temperaturbereich von 700 bis 900°C die Nickelsuperlegierungen in Teilbereichen als Hochtemperaturwerkstoff in der Gasturbine ablösen. Bei Einsatztemperaturen oberhalb von 750°C weist gamma-TiAl allerdings eine geringe Oxidationsbeständigkeit auf. Daher ist es notwendig, das Oxidationsverhalten dieses Materials zu kennen und Maßnahmen zum Schutz vor zu starker Oxidation und somit einem möglichen Materialversagen zu treffen. In dieser Arbeit ist an der Niob-haltigen Legierung Ti-45Al-8Nb (at.%) zunächst die Mikrostrukturentwicklung der sich bildenden Oxidschicht bei Hochtemperaturauslagerungen in unterschiedlichen Atmosphären genauer untersucht worden. Rasterelektronenmikroskopische Analysen lieferten detaillierte Erkenntnisse über den Aufbau und das Wachstum der komplexen Oxidlage, die im Wesentlichen aus TiO2 sowie Al2O3 besteht und sich an der Grenzfläche zum Grundmaterial mit einem Übergangsbereich aus Nitriden, Aluminiumoxidausscheidungen und intermetallischen Phasen auszeichnet. In einem weiteren Schritt sind zur gezielten Verbesserung der Oxidationsbeständigkeit von gamma-TiAl spezielle Schutzschichten entwickelt und mittels Magnetron-Sputtern auf dem Substratmaterial abgeschieden worden. Ziel war es, durch eine Unterdrückung der Titanoxid-Bildung einen hohen Widerstand gegen oxidative Angriffe zu erreichen. Umgesetzt wurde dies, indem die aufgebrachten Schichten entweder die Aluminiumaktivität derart erhöhten, dass sich eine schützende Aluminiumoxid-Deckschicht bilden konnte oder die Aktivität von Titan so verringert wurde, dass die Wachstumsgeschwindigkeit von Titanoxid stark reduziert war. Als dritte Möglichkeit ist eine Kombination dieser beiden Konzepte untersucht worden. Der Oxidationswiderstand der getesteten Schichtsysteme wurde über eine vergleichende quantitative Analyse der Oxidationskinetiken bewertet. Dazu sind neuartige Erkenntnisse aus im Rahmen dieser Arbeit durchgeführten theoretischen Betrachtungen zur Wachstumskinetik von Oxidschichten herangezogen und auf deren Basis eine Messwertanalyse vorgenommen worden. Zur Erweiterung des Einsatzpotentials von gamma-TiAl ist in einem weiterführenden Schritt die Anwendbarkeit von elektronenstrahlaufgedampften Wärmedämmschichten ohne und mit Oxidationsschutz als Zwischenschicht auf gamma-TiAl getestet worden. Kernpunkt war hier die detaillierte Untersuchung von möglichen Einflüssen der keramischen Thermalschutzschicht auf den Oxidbildungsprozess des beschichteten Materialsystems.