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The main objective of this work is to contribute to the understanding of the grafting of nitrogen and amino surface functional groups on polymers by means of plasmas containing nitrogen and hydrogen. For this purpose, many aspects of plasma surface modification were studied. In the frame of this work, a new, UHV-sealed plasma reactor system was put into operation. The system is special for its clean reaction environment and the possibility to perform quasi in situ XPS measurements. A comparison of the UHV system to a fine vacuum reactor showed that a clean reaction environment is mandatory for reproducible plasma processing and efficient nitrogen and amino functionalisation. A key motivation for the present work was the observation that the non-coating plasma processes reported in literature fail to graft primary amino groups on polymer surfaces with densities that significantly exceed 3 - 4% NH2/C. In order to investigate this phenomenon in detail, this work followed two experimental tracks: On the one hand, a broad systematic study of plasma processing parameters was performed. On the other, the surface diagnostics methods used for the quantification of amino groups were critically reviewed. For this, a numerical algorithm was developed to reconstruct the element depth profile from angle-resolved XPS data. In the scope of the process parameter study, cw and pulsed microwave (MW) plasma excitation was compared to radio-frequency (RF) excitation. The home-built MW source was studied and optimised with respect to ignition behaviour and power efficiency. The performance of the MW and RF plasmas in polymer surface modifications was studied in various gas mixtures containing NH3 and H,, or N2 and H,. Also the differences of glow and afterglow processing of polymers were investigated. Large variations of the nitrogen and primary amino grafting efficiencies were obtained. They triggered a number of new ideas for the underlying reaction mechanisms. Special attendance was devoted to the selectivity of the functionalisation processes for primary amino groups. Nitrogen-containing discharges that were rich in hydrogen achieved selectivities up to 100%. The upper limit of 3 - 4% amino groups on the surface, however, was not passed. Angle-resolved XPS measurements revealed a systematic problem for the definition of a surface density, which is capable of explaining the upper limit for amino groups. It is either due to a limited labelling depth of amino groups by the applied TFBA derivatisation reaction, or to a limited functionalisation depth of the plasma process. One very efficient nitrogen-grafting plasma process that was developed on polystyrene was applied to seven other unfluorinated polymers. The similarity of the resulting functionalisation demonstrated a good transfer-ability of plasma surface functionalisation processes. Plasma treatments of polymer surfaces, especially in hydrogen-containing gases, are known to be generally followed by uncontrollable oxidation phenomena. The properties of plasma-functionalised polymer surfaces were therefore studied in conjunction with ageing effects. Quasi in situ XPS analysis allowed to distinguish the influence of oxygen contamination during the plasma process from post-process oxidation due to contact of plasma-treated samples to atmospheric oxygen. The surface modification experiments were accompanied by several gas phase diagnostic techniques. In the scope of this work, the UHV reactor system was equipped with optical emission spectroscopy (OES), two-photon absorption laser-induced fluorescence (TALIF), and tunable diode laser absorption spectroscopy (TDLAS). A separate plasma source was setup to perform an absolute quantification of the vacuum-ultra-violet (VUV) emission intensity of hydrogen-containing MW-excited plasmas. The techniques were evaluated with respect to their contribution to an understanding of the plasma processing of polymers. The rich experimental data allowed to suggest new reaction mechanisms for the grafting of nitrogen- and amino functional groups. Surface passivation experiments in H, plasmas of nitrogen-functionalised surfaces initiated a re-evaluation and an extension of the mechanism of selective etching [1]. Together with two other new reaction mechanisms, a hypothetical reaction scheme was suggested. It was studied by the help of two numerical models for heterogenous reactions of radicals with the surface. In order to avoid the complexity of the fragmentation process of NH,, the models were restricted to discharges in N, and H9. Despite the sparse information on the composition of the gas phase, the data of two experimental series showed a very particular phenomenology that allowed a first test of the model. The test supports the newly-suggested reaction mechanisms. Especially the role of NH2 attachment to open reaction sites for the grafting of amino groups was emphasised. A more stringent test of the model is left to future experiments with extended gas phase diagnostic means.
The present experimental work investigates plasma turbulence in the edge region of magnetized high-temperature plasmas. A main topic is the turbulent dynamics parallel to the magnetic field, where hitherto only a small data basis existed, especially for very long scale lengths in the order of ten of meters. A second point of special interest is the coupling of the dynamics parallel and perpendicular to the magnetic field. This anisotropic turbulent dynamics is investigated by two different approaches. Firstly, spatially and temporally high-resolution measurements of fluctuating plasma parameters are investigated by means of two-point correlation analysis. Secondly, the propagation of signals externally imposed into the turbulent plasma background is studied. For both approaches, Langmuir probe arrays were utilized for diagnostic purposes. The main findings can be summarized as follows: Greatly elongated fluctuation structures exist in plasma edge turbulence. The structures are aligned along the confining magnetic field (k|| = 0). The correlation degree of fluctuations for a short connection length of 0.75m is greater than 80%. For much longer connection lengths of 23m and 66m, the correlation degree is reduced to approximately 40%. A conceptual interpretation of these observations is the coexistence of two different fluctuation components. One component has a correlation length parallel to the magnetic field below 20m and the other component a correlation length greater than 70m. Sine signals in the frequency range 1-100 kHz were injected into the turbulent plasma background. The propagation parallel and perpendicular to the magnetic field of the signals was studied. In poloidal direction, an asymmetry is observed, that can be explained by a copropagation of the signal with the background E × B-rotation of the plasma. The signal propagation parallel to the magnetic field shows no such asymmetry. As an advanced approach, spatio-temporal wave patters were injected into the edge plasma. The waves launched that way can be seen as test waves' in a turbulent background. The coupling strength of the imposed wave patterns to the background turbulence relies on the match of the imposed waves to the dynamics of turbulent structures. If the propagation direction of the imposed waves is parallel to the propagation direction of the background plasma, improved coupling is observed. This finding underlines the importance of the background plasma rotation for future attempts of controlling the plasma edge turbulence. Further optimization of frequency and wave vector of the imposed waves is probably a promising approach for achieving a significant and systematic influence of turbulence. Taking into account the present experimental state-of-the-art, for a deeper insight into the mechanism of the plasma edge turbulence of magnetized high-temperature plasmas a joint effort of numerical modeling and experimental results is a valuable approach. Such a cooperation should cover the explanation of the correlation observations as well as the experiments on signal injection into background turbulence. A quantitative comparison between the results presented in this work and a dedicated numerical drift wave simulation would be a significant step forward to a better understanding of plasma edge turbulence.
The role of large-scale fluctuation structures in electrostatic
drift-wave-type plasma turbulence is highlighted. In particular,
well-defined laboratory experiments allow one to study the
dynamics of drift wave mode structures as well as `eddies' in
drift wave turbulence. In the present paper we discuss the
mutual relationships between observations made in linear
magnetic geometry, purely toroidal geometry and magnetic
confinement. The simplest structure, a saturated, nonlinear
drift mode, is the starting point for a Ruelle-Takens-Newhouse
transition route to chaos and weakly developed turbulence. Both
spectral and phase space analysis are applied to characterize in
detail the transition scenario, which is enforced due to an
increased drive by the plasma equilibrium state. In addition to
direct multi-probe observation, statistical approaches are most
revealing for the systematic study of the spatiotemporal
dynamics in fully developed drift wave turbulence. In
particular, the propagation of large-scale `eddy' structures is
traced by conditional statistics methods. Finally, the control
of drift wave turbulence by spatiotemporal synchronization is
discussed.
Within the scope of this work, a versatile large linear magnetised plasma experiment was designed, constructed, and subsequently put into operation. The magnetised plasma was used to investigate the dispersion of whistler waves (circular polarised electromagnetic waves) with regard to the influence of the plasma boundaries. After a brief review over electromagnetic plasma waves and the three discharge modes of a helicon source, the experimental device and the diagnostic tools are explained in detail. Great attention is devoted to the identification of a reliable, calibrated magnetic fluctuation probe design. To the understanding of dynamical phenomena in ionospheric plasmas, whistler wave measurements in laboratory experiments may contribute significantly because of the ability to vary plasma parameters and to do measurements with high spatial and temporal resolution. However, the boundaries of laboratory experiments change the dispersion behaviour of whistler waves significantly if compared to the unbounded ionospheric situation. The influence of the plasma boundary is studied in the present work on three different levels of increasing complexity. First, a high density, small wavelength regime is established to make the effect of the boundary negligible. Measurements are in full agreement with whistler wave theory for unbounded plasma geometry. Measurements below the ion cyclotron frequency reveal the strong influence of the ion dynamics on whistler wave propagation, but are not straightforward to interpret in terms of dispersion theory. Second, the other limit case is examined: bounded plasma helicon modes. These waves are, mathematically speaking, eigenfunctions of the plasma-boundary system and are of great practical importance for high density plasma discharges, the helicon source. Careful measurements of the equilibrium plasma parameters as well as the magnetic fluctuation profiles of the helicon source are done in all three modes of operation, the capacitive, inductive, and helicon wave sustained mode. The first two modes are fairly well understood and the measurements are consistent with existing models. The high density helicon mode, however, is still a scientific case. The measurements partially confirm existing assumptions. It is demonstrated that the plasma production is detached from the antenna edge region. Moreover, it is shown that the plasma parameters are self-consistently determined by the antenna geometry and the discharge parameters according to basic helicon wave theory. Finally, it is ruled out that the plasma density is the control parameter determining the transition point into the high density helicon mode. The measurements rather suggest that the rf power density is the important value. As a third aspect, whistler waves in an intermediate wavelength regime are studied and the transition from unbounded to bounded plasma wave dispersion is systematically investigated. It is shown both experimentally and numerically that the wave dispersion in a plasma filled metal waveguide cannot be determined solely from wave vector measurements parallel to the magnetic field. For a correct description, the perpendicular mode profile has to be correctly taken into account. In contrast to simple helicon wave theory, it is demonstrated that the perpendicular mode profile is not only determined by the conducting vessel boundaries alone but the entire plasma-boundary system has to be considered as a unity. To summarise, this work has contributed to a better understanding of the physics of the propagation of whistler waves, where the particular role of metal boundaries acting as wave guides was highlighted. This basic science approach to the waves' dynamics is believed to be of significance in the course of the scientific debate on the physics principles of helicon discharges.
Two main aspects concerning drift wave dynamics in linear, magnetized plasma devices are addressed in the work: In part I of the thesis, drift waves are studied in a helicon plasma. The plasma parameter regime is characterized by comparably high collision frequencies and comparably high plasma-p exceeding the electron-ion mass ratio. Single Langmuir probes and a poloidal probe array are used for spatiotemporal studies of drift waves as well as for characterization of background plasma parameters. The main goals are the identification of a low-frequency instability and its major destabilization mechanisms. All experimentally observed features of the instability were found to be consistent with drift waves. A new code, based on a non-local cylindrical linear model for the drift wave dispersion, was used to gain more insight into the dominating destabilzation mechanisms, and also into dependencies of mode frequencies and growth rates on different parameters. In the experiment and in the numerical model, poloidal mode structures were found to be sheared. Part II of the thesis reports about mode-selective spatiotemporal synchronization of drift wave dynamics in a low-P plasma. Active control of the fluctuations is achieved by driving a preselected drift mode to the expense of other modes and broadband turbulence. It is demonstrated that only if a resonance between the driver signal and the drift waves in both space and time is reached, the driver has a strong influence on the drift wave dynamics. The synchronization effect is qualitatively well reproduced in a numerical simulation based on a Hasegawa-Wakatani model.
Low-pressure plasmas offer a unique possibility of confinement, control and
fine tailoring of particle properties. Hence, dusty plasmas have grown
into a vast field and new applications of plasma-processed dust particles
are emerging. There is demand for particles with special properties and
for particle-seeded composite materials. For example, the stability of
luminophore particles could be improved by coating with protective Al2O3
films which are deposited by a PECVD process using a metal-organic precursor gas.
Alternatively, the interaction between plasma and injected micro-disperse powder
particles can also be used as a diagnostic tool for the study of plasma surface
processes. Two examples will be provided: the interaction of micro-sized (SiO2)
grains confined in a radiofrequency plasma with an external ion beam as well as
the effect of a dc-magnetron discharge on confined particles during deposition
have been investigated.
Colossal magneto-resistance manganites are characterized by a complex interplay of charge, spin, orbital and lattice degrees of freedom. Formulating microscopic models for these compounds aims at meeting two conflicting objectives: sufficient simplification without excessive restrictions on the phase space. We give a detailed introduction to the electronic structure of manganites and derive a microscopic model for their low-energy physics. Focusing on short-range electron–lattice and spin–orbital correlations we supplement the modelling with numerical simulations.
This work studies different alternatives for parallelization of ground-state DMRG, with a focus on shared memory multiprocessor systems. Exploiting the parallelism in the dominant part of a DMRG calculation (diagonalization of the superblock Hamiltonian), speedups of 5 to 6 on 8-CPU machines can be achieved. A performance analysis gives hints as to which machine is best siuted for the task. The parallelized DMRG code is then applied to current problems in theoretical solid state physics with electronics, bosonic and spin degrees of freedom. Stripe-like modulations of the hole density in the ground state of doped Hubbard with cylindrical boundary conditions are idenficied in the thermodynamic limit using extrapolation techniques. In the 1D Holstein model of spinless fermions at half filling, Luttinger parameters and the charge structure factor are determinde in order to derive the phase diagram that had previously been established only on small lattices. For the 1D half-filled Holstein-Hubbard model, a finite size analysisof spine and charge excitation gaps in the relevant sectors (Mott insulator, Peierls band insulator and bipolaronic Peierls insulator) is able to yield the phase diagram as well. Finally, is the Heisenberg spin chain with dynamical phonons is considered as a relevant model for a spin-Peierls transition in Copper Germanate. Using DMRG, the relation between singlet-triplet excitation gap and dynamical dimeriaztion is calculated for the first time.
First-principle path integral Monte Carlo simulations were performed in order to analyze correlation effects in complex electron-hole plasmas, particularly with regard to the appearance of excitonic bound states. Results are discussed in relation to exciton formation in unconventional semiconductors with large electron hole mass asymmetry.
Collisional absorption of dense fully ionized plasmas in strong high-frequency laser fields is investigated in the non-relativistic case. Quantum statistical methods are used as well as molecular dynamics simulations. In the quantum statistical expressions for the electrical current density and the electron-ion collision frequency–valid for arbitrary field strength–strong correlations are taken into account. In addition, molecular dynamic simulations were performed to calculate the heating of dense plasmas in laser fields. Comparisons with the analytic results for different plasma parameters are given. Isothermal plasmas as well as two-temperature plasmas are considered.
We investigate the equilibration of nonideal plasmas from initial states where each species has already established a Maxwellian distribution, but the species temperatures and the chemical composition are not in equilibrium. On the basis of quantum kinetic equations, we derive hydrodynamic balance equations for the species densities and temperatures. The coupled density-temperature relaxation is then given in terms of the energy transfer between the subsystems and the population kinetics. We use the Landau-Spitzer approach for the energy transfer rates and a system of rate equations to describe the nonequilibrium plasma composition. Nonideality corrections are included in the rate coefficients and as potential energy contributions in the temperature equations on the simplest level of a Debye shift.
The relaxation of nonideal two-temperature plasmas is investigated with a kinetic approach. First the energy transfer between the electrons and ions is described using different approximations: the energy transfer through classical collisions (Landau-Spitzer approach) is reviewed; quantum diffraction and strong collisions are included by applying the quantum Boltzmann equation; the influence of collective modes is considered on the basis of the Lenard-Balescu equation (coupled modes) and with the Fermi-Golden-Rule approach (independent electron and ion modes). Finally, the evolution of the species temperature is investigated. In nonideal plasmas, changes in the correlation energy have to be taken into account during the relaxation. It is demonstrated that ionic correlations can significantly influence the relaxation particularly the evolution of the ion temperature).
The triple-trap mass spectrometer ISOLTRAP at ISOLDE/CERN has demonstrated the feasibility of mass spectrometry of in-trap-decay product ions. This novel technique gives access to radionuclides, which are not produced directly at ISOL-type radioactive ion beam facilities. As a proof of principle, the in-trap decay of 37K+ has been investigated in a Penning trap filled with helium buffer gas. The half-life of the mother nuclide was confirmed and the recoiling 37Ar+ daughter ion was contained within the trap. The ions of either the mother or the daughter nuclide were transferred to a precision Penning trap, where their mass was determined.
Diese Arbeit untersucht experimentell den Einfluss des metastabilen Zustandes Xe(1s3) und des Resonanzzustandes Xe(1s2) auf die VUV-Strahlungserzeugung in Helium-Xenon-Glimmentladungen (He:Xe = 98:2). Für die Bestimmung der Atomdichten wurde eine experimentelle Anordnung geschaffen, mit der, basierend auf der Methode der Laser-Atom-Absorptionsspektroskopie, orts- und zeitaufgelöste Messungen von optischen Dichten im Säulenplasma durchgeführt wurden. Als Hintergrundstrahlungsquelle kam ein durchstimmbarer Diodenlaser zum Einsatz. Die bereitgestellten Laserwellenlängen von 820 nm bzw. 826 nm entsprechen optischen Übergängen zwischen den Xenonzuständen 6s' 1/2[1/2]0 --> 6p' 1/2[3/2]1 (1s3 --> 2p4) und 6s' 1/2[1/2]1 --> 6p' 1/2[1/2]1 (1s2 --> 2p2).
Den Ausgangspunkt der Untersuchungen stellte die Messung der Absorptionslinienprofile beider Nahinfrarot-Übergänge dar. In Abhängigkeit von den Entladungsparametern Gasdruck, Entladungsstrom und Betriebsweise (Gleichstrom-, gepulste und Wechselstromentladung) wurden daraus die Dichten der angeregten Atome auf der Entladungsachse ermittelt. Durch die Analyse des Abklingens der Besetzungsdichten im Afterglow von gepulst betriebenen Entladungen mit Hilfe eines Systems von gekoppelten Ratengleichungen konnten die dominanten Stoßprozesse für die betrachteten Zustände identifiziert werden. Erstmalig ist in dieser Arbeit die radiale Verteilung der angeregten Spezies Xe(1s3) und Xe(1s2) in He-Xe-Glimmentladungen untersucht worden. Damit ist die VUV-Strahlungsleistung der 129 nm-Linie aus der Dichteverteilung der Resonanzatome ermittelbar.
In the present thesis, a systematic study of beam driven Alfvén eigenmodes in high-density and low-temperature plasmas of the W7-AS stellarator is performed. The device went out of operation in 2002 and the study is based on stored experimental data. Alfvén instabilities can roughly be divided into ideal MHD Alfvén eigenmodes and those existing due to kinetic effects. The spectrum of ideal MHD Alfvén waves in toroidal fusion devices consists of a continuum of stable waves that are strongly localized. Weakly damped, discrete eigenmodes can exist in gaps of the continuous spectrum which are formed by plasma inhomogeneities and the coupling of Alfvén continua. This allows an identification of ideal MHD Alfvén eigenmodes in terms of their frequency and mode numbers. Kinetic effects can modify this spectrum and cause additional types of eigenmodes, the kinetic Alfvén eigenmodes (KAE) and energetic particle modes (EPM). The goal of this thesis is twofold: (I) identification and description of fast particle driven Alfvén instabilities in W7-AS, and (II) study of energetic particle losses induced by Alfvén instabilities. The reconstruction of the ideal MHD plasma equilibrium for each discharge with sufficient accuracy is the very foundation of all subsequent steps. This is achieved, based on measured plasma parameter profiles that are further refined by validating them to the measurements of other, independent plasma diagnostics. The applied scheme is inspired by an approach of Integrated Data Analysis (IDA) to combine different diagnostic data and provide combined uncertainties. After mode number analysis and eigenmode identification, the theoretically expected, linear growth rate of the instability is calculated where possible, and the various contributions of the fast particle drive to the instability of the mode are identified. Alfvénic activity recorded by the Mirnov diagnostic is analyzed, which consists of a set of spatially distributed coils that measure magnetic fluctuations. On W7-AS, the probes are arranged in three poloidal arrays at different toroidal positions. The spacing between the probes is non-equidistant. In addition, the signals of one probe array are digitized with a different sample rate. These characteristics prohibit the straight-forward use of standard tools available for harmonic analysis. Instead, a new tool has been developed and thoroughly tested. It is a multi-dimensional extension of the Lomb periodogram, able to provide reliable time-resolved frequency and mode number spectra in the case of uneven datapoint spacing. Numerical studies of this periodogram show a good performance with respect to mode number resolution given the low number of available probes, and robustness against perturbations of the signal. Only two of the probe arrays can be used for the analysis of eigenmodes with frequencies >70 kHz, such that for high-frequency phenomena insufficient information about the mode numbers is available. A total of 133 different Alfvén eigenmodes is studied in discharges from different experimental campaigns. A restriction to discharges from various high-beta campaigns with neutral beam heating is required to allow for a realistic reconstruction of plasma equilibrium and velocity distribution functions of energetic particles. The discharges are characterized by high density, ne = 5 x 1019 m-3 to 2.5 x 1020 m-3 at relatively low temperatures of Te = Ti = 150 ... 600 eV. Alfvén eigenmodes often appear transiently in the startup phase of these discharges, where density and heating power are being ramped up. Occasionally, Alfvén eigenmodes are seen in the stationary, high-beta phase in the presence of considerable neutral beam heating. Most of the Alfvén eigenmodes are successfully classified as ideal MHD eigenmodes. 19 global, 47 toroidicity-induced and 8 ellipticity-induced Alfvén eigenmodes (GAEs, TAEs, and EAEs, respectively) are unambiguously identified by their mode numbers and frequencies. Excellent agreement between experimentally observed mode number spectra and theoretically calculated eigenmode structure is shown for a TAE example. Additional 13 events are found to have frequencies inside the EAE gap and could possibly be EAEs. Evidence for high-frequency Alfvén eigenmodes (mirror- and helicity-induced Alfvén eigenmodes) is seen, but can not be proven rigorously due to uncertain mode numbers and the complexity of the Alfvén continuum. The remaining 41 Alfvén eigenmodes can not be classified to be one of the above cases. Reasons are either high frequencies, mode numbers obscured by far-field effects, or mode numbers that could not be related to ideal MHD Alfvén eigenmodes. A selection of these shows indications of strong non-linear wave-particle interactions and are assumed to be EPMs. Kinetic Alfvén eigenmodes are not expected to exist in the experimental conditions that were studied. The radially resolved velocity distribution function is used to describe the parameter regimes in which the modes are observed in terms of the dimensionless parameters vb/vA (beam velocity normalized to the Alfvén velocity) and ßfast/ßth, where beta is the ratio of plasma pressure to magnetic pressure. The first parameter describes through which of the possible resonance velocities particles can interact with the eigenmode. A peculiarity of the fast particle dynamics in fusion devices is that they can resonantly interact with Alfvén eigenmodes through sideband resonances even if v < vA. The second parameter describes the energy content of the destabilizing fast particle population compared to the potentially stabilizing thermal plasma component. These parameters contain relevant information about the instability of an eigenmode and such diagrams are given for all observed modes. In addition to that, the expected linear growth rate of gap modes is calculated based on a theoretical model that extends the ideal MHD by a perturbative, drift-kinetic description of the energy exchange between waves and circulating particles, neglecting the effects of trapped particles. For the discharges under consideration the thermal electron speed is comparable to vA and the electrons provide a significant Landau damping contribution. Due to strong density gradients near the plasma boundary in most of the discharges, the thermal ions can provide a small drive via the spatial inhomogeneity which does not overcome the electron damping, however. The drive by spatial inhomogeneity of thermal ions requires a certain propagation direction of the mode and is equally stabilizing for opposite mode numbers. The fast particles also contribute to the growth rate via spatial inhomogeneity, velocity gradients and velocity anisotropy terms are negligible in W7-AS. Most of the observed GAE or EAE modes have negative mode numbers, which correspond to a propagation direction for which the spatial inhomogeneity of thermal and beam ions is predicted to be stabilizing. A fast particle drive of these modes is not confirmed, whereas the TAEs are found to be strongly destabilized by neutral beam injection. The distribution of plasma parameters for discharges showing TAEs in terms of the dimensionless stability parameters suggests an instability threshold that is qualitatively confirmed by an exploration of the parameter space with the theoretical model. Wave-induced, resonant losses of energetic ions scale linearly with the wave amplitude. To identify them, correlations between ion loss probe signals and wave amplitudes are searched, where correlation times in the order of the slowing-down time of energetic particles are expected. Significant correlations can be established only exceptionally for 3 of the identified ideal MHD Alfvén eigenmodes. Those Alfvén eigenmodes, however, which are assumed to be EPMs frequently show severe losses of energetic ions that are visible in the time traces of the plasma energy as well.
A fluorescent lamp driven with an 'instant start electronic control gear' starts in a glow mode. In the glow mode, which lasts typically for tens of milliseconds, the cathode fall exceeds hundreds of volts. This causes high energy ion bombardment of the electrode which heats the electrode, and induces a transition from glow to arc mode. In the arc mode the electrode emits thermionically and the cathode fall drops to the 12 – 15 V range. Unfortunately, the high energy ion bombardment during the glow mode leads also to intense sputtering of electrode material, including tungsten as well as emitter. Thus, instant started fluorescent lamps often suffer from early failures due to coil fracture. Therefore, the investigation of tungsten erosion during instant start is necessary and was the main goal of this work.
The density of neutral atomic tungsten is determined by laser-induced fluorescence (LIF) and optical emission spectroscopy measurements (OES). Investigations are performed on a low-pressure argon dc discharge and on commercial fluorescent lamps. To include the entire temperature profile along the electrode the diffuse and spot operation modes of the dc lamp are studied experimentally and theoretically. The measured dependencies of the cathode temperature along the coil on the discharge and heating parameters are compared with the calculated results. For the first time the tungsten erosion during instant start of commercial fluorescent lamps was experimentally investigated in this work. The erosion process could be related to sputtering. A reconstruction of the temporal evolution of the absolute tungsten population density of the ground state during the glow mode was presented. The sputtered tungsten density increases immediately with the ignition, reaches a maximum where the discharge contracts at the end of the glow mode, and decreases some milliseconds before the glow-to-arc transition takes place. The maximum tungsten density was observed within a region of a few hundred micrometers only located at the discharge attachment point. The main result achieved in this work is that during the whole glow mode tungsten is sputtered. Therefore, the lifetime of instant started fluorescent lamps can be enhanced by reducing the duration of the glow mode. Additionally, the need for the application of different types of diagnostics for the observation of lamp ignition was shown due to different results of LIF, AAS and OES: The observation of excited tungsten atoms by OES shows the maximum emission signal at the glow-to-arc transition whereas by LIF and AAS measurements of tungsten atoms in the ground state the maximum density is found during the whole glow mode. This can be explained by the fact that the intensity of the spontaneous emitted light is related not only to the density but also to the degree of excitation.
In magnetisierten Plasmen kommt dem Verständnis von magnetischen Fluktuationen eine tragende Rolle hinsichtlich der Plasmadynamik zu. Diese Fluktuationen treten in Form linearer und nichtlinearer Wellenphänomene oder auch als Änderung der magnetischen Topologie auf. Im Rahmen der vorliegenden Dissertation wurde der Einfluß von niederfrequenten elektromagnetischen Wellen und der von topologischen Magnetfeldänderungen durch magnetische Rekonnektion auf die Dynamik der Ionen experimentell untersucht. In dem linearen magnetisierten Laborexperiment VINETA wurden kinetische Alfvénwellen angeregt und durch detaillierte Messung der Dispersion mittels magnetischer Fluktuationsdiagnostiken eindeutig identifiziert. Für das Verständnis des Dispersionsverhaltens müssen die Berandung der Wellen und der Einfluß von Stößen einbezogen werden. Mittels laserinduzierter Fluoreszenz (LIF) wurde die Ionenenergieverteilungsfunktion (IEVF) gemessen. Dabei wurde das Schema dahingehend erweitert, daß bei periodischen Störungen des Plasmas phasenaufgelöste Messungen der IEVF durchgeführt werden können. Die elektrischen Felder der durch vergleichsweise kleine magnetische Störungen angeregten linearen Alfvénwellen sind jedoch in der Regel zu klein, um einen signifikanten Einfluß auf die Ionendynamik zu nehmen. Anders verhält es sich jedoch bei einem stark nicht-linearem Anregungssschema: Die Welle-Teilchen Wechselwirkung konnte für nichtlineare Anregung Alfvénischer Wellen durch amplitudenmodulierte Helikoneigenmoden mittels LIF nachgewiesen werden. In dem toroidalen Experiment VTF kann magnetische Rekonnektion periodisch und unter reproduzierbaren Bedingungen angetrieben werden. Diese Voraussetzungen ermöglichen systematische Untersuchungen der Rückwirkung magnetischer Rekonnektion auf die Ionendynamik mittels LIF. Dabei ist es zum ersten Mal gelungen, eine Ionenheizung als Folge von Rekonnektion direkt nachzuweisen. Ferner konnte gezeigt werden, daß diese Heizung stark lokalisiert ist und nur am magnetischen X-Punkt, dem Ort der Rekonnektion, auftritt. Mittels zeitaufgelöster Messungen konnte ein kausaler Zusammenhang zwischen der Rekonnektionsrate und der Ionenheizung gezeigt werden. Desweiteren wurden starke nicht-thermische Komponenten der IEVF diagnostiziert, die mit der beobachteten Ionenheizung korrelieren. Numerische Simulationen, basierend auf einem kinetischen Einteilchenbild, zeigen einen Transfer von magnetischer Energie zu kinetischer Energie der Ionen, der konsistent mit dem experimentell beobachteten Anstieg der Ionentemperatur ist.
The interaction of partially ionized plasmas with an electromagnetic field is investigated using quantum statistical methods. A general statistical expression for the current density of a plasma in an electromagnetic field is presented and considered in the high field regime. Expressions for the collisional absorption are derived and discussed. Further, partially ionized plasmas are considered. Plasma Bloch equations for the description of bound-free transitions are given and the absorption coefficient as well as rate coefficients for multiphoton ionization are derived and numerical results are presented.
Based on distributions of local Green's functions we present a stochastic approach to disordered systems. specifically we address Anderson localisation and cluster effects in binary alloys. Taking Anderson localisation of Holstein polarons as an example we discuss how this stochastic approach can be used for the investigation of interacting disordered systems.
Die vorliegende Arbeit widmet sich der plasmachemischen Herstellung und physikalisch-chemischen Charakterisierung von dünnen organischen Schichten auf der Basis von Ethylenglykol (Präkursor). Die Oberflächen können die Adsorption von Proteinen minimieren und daher als neues biokompatibles Material getestet werden. Im Schwerpunkt der Arbeit liegt die Entwicklung eines plasmachemischen RF-Reaktors (genannt Nevada) und einer innovativen Beschichtungstechnologie TFPD (Temperature Forced Plasma Deposition) als Erweiterung der PECVD (Plasma Enhanced Chemical Vapour Deposition). Ein Gemisch aus Ethylenglykol und Argon wurde als Modellsystem untersucht. Die Plasmabedingungen und die Oberflächentemperatur wurden optimiert und an Phaseneigenschaften von Ethylenglykol angepasst. Die komplexe Polykondensation steht für die plasmagestützte Umwandlung der Kondensatschicht zu einem stabilen Poly(Ethylenglykol)-ähnlichen Plasmapolymer. Der Prozess wurde durch die simultane Temperaturkontrolle und in situ FTIR-Spektroskopie analysiert. Zur Untersuchung der erzeugten Proben wurden weitere ex situ Oberflächenanalysen wie XPS, AFM, TDS, MALDI, XRD und die optische Ellipsometrie verwendet. Durch die neue Methode TFPD entstehen extrem glatte, amorphe und wasserunlösliche Schichten mit einem Potenzial für die Biokompatibilität.
Turbulenz ist allgegenwärtig in der Natur. Ein wichtiges Charakteristikum sind Fluktuationen auf einer Vielzahl von räumlichen und zeitlichen Skalen, die sowohl in neutralen Fluiden und gasförmigen Systemen, als auch in Plasmen beobachtet werden. Obwohl der elektromagnetische Charakter von Plasmen eine erhöhte Komplexität von Plasmaturbulenz bedingt, sind die grundlegenden Eigenschaften universell. In magnetisch eingeschlossenen Plasmen führen fluktuierende Plasmaparameter zu turbulentem Transport von Plasmateilchen und Energie, der die Einschlusszeit verringert und wichtige Aspekte zukünftiger Fusionskraftwerke beeinflusst. Der intermittente Charakter dieses konvektiven Teilchenflusses ist verbunden mit turbulenten Strukturen mit großen Amplituden, auch "blobs" genannt, die radial durch das Magnetfeld propagieren. Intermittente Fluktuationen im Randplasma von Experimenten mit linearer Magnetfeldgeometrie werden ebenfalls propagierenden turbulenten Strukturen zugeschrieben. Dabei ist der Mechanismus der radialen Propagation kaum verstanden. In dieser Arbeit wird die Bildung und Propagation von turbulenten Strukturen im linear magnetisierten Helikonexperiment Vineta untersucht. Durch Messungen der Fluktuationen in der azimuthalen Ebene mit multi-dimensionalen Sonden wird gezeigt, dass turbulente Strukturen in Driftwellenturbulenz im Gebiet des maximalen Dichtegradienten entstehen. Die turbulenten Strukturen propagieren hauptsächlich azimuthal in Richtung der Hintergrund ExB-Drift, aber sie besitzen auch eine starke radiale Geschwindigkeitskomponente. Die radiale Propagation wird durch das selbstkonsistente Potential der turbulenten Struktur verursacht, dass zu einem fluktuations-induzierten radialen Transport führt. Im Plasmarand werden die turbulenten Strukturen als intermittente Dichteeruptionen mit großen Amplituden beobachtet. Ein Vergleich der experimentellen Ergebnisse mit numerischen dreidimensionalen Fluid-Simulationen mit abgestimmten Geometrie- und Randbedingungen zeigt Übereinstimmung. Die Bildung der turbulenten Strukturen ist kausal mit einer quasi-kohärenten Driftmode verbunden und ihre radiale Propagation wird durch das selbstkonsistente elektrische Feld verursacht, dass aus der dreidimensionalen Dynamik resultiert. Zum Vergleich wird die Propagation von turbulenten Strukturen im Randplasma vom National Spherical Torus Experiment (NSTX) untersucht und mit theoretischen Propagationsmodellen verglichen.
The rapid neutron-capture or the r-process is responsible for the origin of about half of the neutron-rich atomic nuclei in the universe heavier than iron. For the calculation of the abundances of those nuclei, atomic masses are required as one of the input parameters with very high precision. In the present work, the masses of the neutron-rich Zn isotopes (A=71 to 81) lying in the r-process path have been measured in the ISOLTRAP experiment at ISOLDE/CERN. The mass of 81Zn has been measured directly for the first time. The half-lives of the nuclides ranged from 46.5 h (72Zn) down to 290 ms (81Zn). In case of all the nuclides, the relative mass uncertainty (∆m/m) achieved was in the order of 1E-8 corresponding to a 100-fold improvement in precision over previous measurements.
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.
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.
Multiply negatively charged aluminium clusters and fullerenes were generated in a Penning trap using the "electron-bath" technique. Aluminium monoanions were generated using a laser vaporisation source. After this, two-, three- and four-times negatively charged aluminium clusters were generated for the first time. This research marks the first observation of tetra-anionic metal clusters in the gas phase. Additionally, doubly-negatively charged fullerenes were generated. The smallest fullerene dianion observed contained 70 atoms.
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.
The present work is the first work dealing with turbulence in the WEGA stellarator. The main object of this work is to provide a detailed characterisation of electrostatic turbulence in WEGA and to identify the underlying instability mechanism driving turbulence. The spatio-temporal structure of turbulence is studied using multiple Langmuir probes providing a sufficiently high spatial and temporal resolution. Turbulence in WEGA is dominated by drift wave dynamics. Evidence for this finding is given by several individual indicators which are typical features of drift waves. The phase shift between density and potential fluctuations is close to zero, fluctuations are mainly driven by the density gradient, and the phase velocity of turbulent structures points in the direction of the electron diamagnetic drift. The structure of turbulence is studied mainly in the plasma edge region inside the last closed flux surface. WEGA can be operated in two regimes differing in the magnetic field strength by almost one order of magnitude (57mT and 500mT, respectively). The two regimes turned out to show a strong difference in the turbulence dynamics. At 57mT large structures with a poloidal extent comparable to the machine dimensions are observed, whereas at 500mT turbulent structures are much smaller. The poloidal structure size scales nearly linearly with the inverse magnetic field strength. This scaling may be argued to be related to the drift wave dispersion scale. However, the structure size remains unchanged when the ion mass is changed by using different discharge gases. Inside the last closed flux surface the poloidal ExB drift in WEGA is negligible. The observed phase velocity is in good agreement with the electron diamagnetic drift velocity. The energy in the wavenumber-frequency spectrum is distributed in the vicinity of the drift wave dispersion relation. The three-dimensional structure is studied in detail using probes which are toroidally separated but aligned along connecting magnetic field lines. As expected for drift waves a small but finite parallel wavenumber is found. The ratio between the average parallel and perpendicular wavenumber is in the order of 10^-2. The parallel phase velocity of turbulent structures is in-between the ion sound velocity and the Alfvènvelocity. In the parallel dynamics a fundamental difference between the two operational regimes at different magnetic field strength is found. At 500mT turbulent structures can be described as an interaction of wave contributions with parallel wavefronts. At 57mT the energy in the parallel wavenumber spectrum is distributed among wavenumber components pointing both parallel and antiparallel to the magnetic field vector. In both cases turbulent structures arise preferable on the low field side of the torus. Some results on a novel field in plasma turbulence are given, i.e. the study of turbulence as a function of resonant magnetic field perturbations leading to the formation of magnetic islands. Magnetic islands in WEGA can be manipulated by external perturbation coils. A significant influence of field perturbations on the turbulence dynamics is found. A distinct local increase of the fluctuation amplitude and the associated turbulent particle flux is found in the region of magnetic islands.
The term atomic cluster relates to compounds of at least two or three atoms. Thereby the physical properties are size dependent and the property transitions between single atoms and bulk material are not always smooth. Ion traps allow it to observe internal cluster properties independent from the influence of external forces. In this work the electron induced decay of singly negatively charged atomic clusters was observed. The dissociation cross section of the clusters is dominated by detachment of the only weakly bound outer electrons. For simple atoms at low electron energies a simple scaling law can be obtained that includes only the binding energies of the valence electrons. Nevertheless for larger sizes theoretical calculations predict so called "giant resonances" as dominant decay process in metal clusters. Due to mass limitations in storage rings exist so far only cross section measurements for simple anions and small negative molecules. In this work the electron detachment cross sections of small negatively charged carbon (Cn- n=2-12), aluminium (Aln- n=2-7) and silver clusters (Agn- n=1-11) were measured in an electrostatic ion beam trap. The classical scaling law, including only the binding energies of the valence electrons, turned out to be not sufficient, especially for larger clusters. In order to improve the correlation between measured and predicted values it was proposed to involve the influence of the cluster volume and the specific polarisability induced by long range coulomb interaction. For silver clusters the best agreement was obtained using a combination of the projected area reduced by the polarisability. The existence of "giant resonances" could not be confirmed. According to theory for clusters with a broad internal energy distribution, a power-law decay close to 1/time is expected. For some clusters the lifetime behaviour would be strongly quenched by photon emission. The thermionic evaporative decay of anionic aluminium and silver clusters in a size range from one to ten constituents was tested but a correlation could be only found incidentally for a few cluster sizes.
In this work we will analyse the capabilities of several numerical techniques for the description of different physical systems. Thereby, the considered systems range from quantum over semiclassical to classical and from few- to many-particle systems. For each case we address an interesting, partly unsolved question. Despite the different topics we address in the individual chapters, the problems under study are somehow related because we focus on the time evolution of the system. In chapter 1 we investigate the behaviour of a single quantum particle in the presence of an external disordered background (static potentials). Starting from the quantum percolation problem, we address the fundamental question of a disorder induced (Anderson-) transition from extended to localised single-particle eigenstates. Distinguishing isolating from conducting states by applying a local distribution approach for the local density of states (LDOS), we detect the quantum percolation threshold in two- and three-dimensions. Extending the quantum percolation model to a quantum random resistor model, we comment on the possible relevance of our results to the influence of disorder on the conductivity in graphene sheets. Furthermore, we confirm the localisation properties of the 2D percolation model by calculating the full quantum time evolution of a given initial state. For the calculation of the LDOS as well as for the Chebyshev expansion of the time evolution operator, the kernel polynomial method (KPM) is the key numerical technique. In chapter 2 we examine how a single quantum particle is influenced by retarded bosonic fields that are inherent to the system. Within the Holstein model, these bosonic degrees of freedom (phonons) give rise to an infinite dimensional Hilbert space, posing a true many-particle problem. Constituting a minimal model for polaron formation, the Holstein model allows us to study the optical absorption and activated transport in polaronic systems. Using a two-dimensional variant of the KPM, we calculate for the first time quasi-exactly the optical absorption and dc-conductivity as a function of temperature. Concerning the numerical technique, the close relation to the time evolution in the other chapters get clear if we identify temperature with an imaginary time. In chapter 3 we come back to the time evolution of a quantum particle in an external, static potential and investigate the capability of semiclassical approximations to it. Considering various one-dimensional geometries, we address basic quantum effects as tunneling, interference and anharmonicity. The question is, to which extend and at which numerical costs, several semiclassical methods can reproduce the exact result for the quantum dynamics, calculated by Chebyshev expansion. To this end we consider the linearised semiclassical propagator method, the Wigner-Moyal approach and the recently proposed quantum tomography. A conceptually very interesting aspect of the compared semiclassical methods is their relation to different representations of quantum mechanics (wave function/density matrix, Wigner function, quantum tomogram). Finally, in chapter 4 we calculate the dynamics of a classical many-particle system under the influence of external fields. Considering a low-temperature rf-plasma, we investigate the interplay of the plasma dynamics and the motion of dust particles, immersed into the plasma for diagnostic reasons. In addition to the huge number of involved particles, the numerical description of this systems faces the challenge of a large range of involved time and length scales. Exploiting the mass differences of plasma constituents and dust particles allows for separating the PIC description of the plasma from the MD simulation of the dust particles in the effective surrounding plasma.
The properties of the ion feature of the Thomson scattering signal are investigated. Firstly, the description of the atomic form factor by hydrogen-like wave functions is reviewed and better screening charges are obtained. Then the ionic structure in systems with several ion species is calculated from the HNC integral equation.
Interaction of injected dust particles with metastable neon atoms in a radio frequency plasma
(2008)
Spatial density and temperature profiles of neon metastables produced in a radio frequency (rf) discharge were investigated by means of tunable diode laser absorption spectroscopy. The experiments were performed in the PULVA1 reactor, which is designed for the study of complex (dusty) plasmas. The line averaged measured density is about 1.5×1015 m−3 in the bulk and drops almost linearly in the plasma sheath. The gas temperature is in the range of 370–390 K. The flow of metastable atoms in the plasma sheath deduced from the spatial density distribution is dominated by the flow towards the rf electrode. The sheath length is supposed as the effective diffusion length in the plasma sheath region. This approximation was used to investigate the interaction of injected particles with the plasma. The observations and estimation provide evidence for a significant interaction between metastable atoms and powder particles which is important for energy transfer from the plasma to the particles. The power per unit area absorbed by dust particles due to the collision of metastable atoms with the dust particle surface is in the range of a few tens of mW m−2.
In dieser Arbeit wurden Experimente an einem DC-Magnetron-Beschichtungsplasma zur (reaktiven) Abscheidung von Ti, TiNx und TiOx-Schichten durchgeführt. Das Ziel war es, durch Korrelation von Messungen des Ionen- und des Energieeinstroms auf das Substrat während des Beschichtungsvorgangs mit Analysen der abgeschiedenen Schichten Aussagen über die Zusammenhänge von Abscheidebedingungen und Schichteigenschaften zu treffen. Von besonderem Interesse waren hierbei die Unterschiede zwischen den beiden Betriebsmodi des eingesetzten Magnetrons (balanced mode und unbalanced mode), da sich über diesen Parameter der Ioneneinstrom auf das Substrat signifikant beeinflussen lässt, sowie der Einfluss hochenergetischer negativ geladener Ionen, die beim Einsatz von Sauerstoff im Gegensatz zu dem von Stickstoff als Reaktivgas auftreten. Die Maxima der mittels energieaufgelöster Massenspektrometrie gemessenen Energieverteilungen aller Ionenspezies liegen im unbalanced mode im Vergleich zum balanced mode bei um etwa 0,2...1 eV höherer Energie. Der im Wesentlichen von den einfach positiv geladenen Argonionen und bei hohem Reaktivgasfluss den molekularen Reaktivgasionen getragene Gesamtioneneinstrom auf das Substrat ist im unbalanced mode deutlich höher als im balanced mode. Der mit Hilfe einer Thermosonde gemessene Energieeinstrom auf das Substrat steigt linear mit der Entladungsleistung an. Im unbalanced mode ist er, bedingt durch den höheren Gesamtioneneinstrom auf das Substrat und die größere mittlere Energie aller Ionenspezies, um mehr als eine Größenordnung höher als im balanced mode. Eine Abhängigkeit des Energieeinstroms vom Reaktivgasfluss wurde nicht beobachtet. Die röntgenreflektometrisch gemessenen Beschichtungsraten steigen über der Entladungsleistung linear an und sind im unbalanced mode trotz geringerer Sputterraten am Target um ca. 10...20 % höher als im balanced mode. Die Begründung hierfür liefert der im unbalanced mode deutlich höhere Energieeinstrom auf das Substrat. Durch diesen erhöhten Energieeintrag in die aufwachsenden Schichten steht im unbalanced mode mehr Energie für Prozesse an der Oberfläche, wie die Oberflächendiffusion, zur Verfügung. Die somit verbesserte laterale Mobilität der Teilchen an der Oberfläche führt dazu, dass diese besser in die wachsende Kristallstruktur eingebaut werden können. Damit ergibt sich letztendlich im unbalanced mode trotz des geringeren Teilcheneinstroms in allen untersuchten Plasmen eine höhere Abscheiderate von Titan auf dem Substrat. Der Energieeinstrom auf das Substrat ist demnach durch seinen signifikanten Einfluss auf die laterale Mobilität der aufwachsenden Teilchen ein bestimmender Parameter für das Schichtwachstum. Die durch die Beimischung von Reaktivgas zum Plasma auftretende Targetnitrierung bzw. –oxidation verursacht ein deutliches Absinken der Sputterraten am Target und damit der Beschichtungsraten über dem Reaktivgasfluss. Messungen der chemischen Zusammensetzungen der Schichten mittels Röntgenphotoelektronenspektroskopie zeigen, dass die Menge des in die Schichten eingebauten Reaktivgases über dessen Konzentration im Beschichtungsplasma zu kontrollieren ist. Im Argon-Stickstoff-Plasma sind die Werte der aus den röntgenreflektometrisch erhaltenen Dichten bei den im unbalanced mode abgeschiedenen Schichten deutlich höher als bei den im balanced mode abgeschiedenen. Untersuchungen mittels Röntgendiffraktometrie zeigen für diese Schichten auch höhere makroskopische Spannungen. Offenbar führt der größere Energieeinstrom hier zu lokalen Temperaturunterschieden, aus denen aufgrund unterschiedlicher Ausdehnungskoeffizienten von Schicht und Substrat beim Abkühlen makroskopische Schichtspannungen resultieren. Insgesamt werden im Argon-Stickstoff-Plasma im unbalanced mode des Magnetrons kompaktere Schichten mit weniger Lücken abgeschieden als unter denselben Bedingungen im balanced mode. Im Argon-Sauerstoff-Plasma wird dieser positive Effekt des höheren Energieeintrags in die aufwachsenden Schichten durch den im unbalanced mode deutlich höheren Beschuss des Substrats mit hochenergetischen negativ geladenen Sauerstoffionen mehr als aufgehoben. Dadurch kommt es in diesem Betriebsmodus des Magnetrons zu einer erhöhten Lückenbildung in den aufwachsenden Schichten, die somit geringere makroskopische Spannungen und geringere mittlere Dichten aufweisen als die im balanced mode abgeschiedenen. Die Summe dieser Ergebnisse zeigt, dass die Eigenschaften der im hier untersuchten DC-Magnetronplasma abgeschiedenen Schichten maßgeblich von der Zusammensetzung des Beschichtungsplasmas und insbesondere von der Art und der Energie der auf das Substrat auftreffenden Ionen abhängen.
Infrared laser absorption spectroscopy (IRLAS) employing both tuneable diode and quantum cascade lasers (TDLs, QCLs) has been applied with both high sensitivity and high time resolution to plasma diagnostics and trace gas measurements.
TDLAS combined with a conventional White type multiple pass cell was used to detect up to 13 constituent molecular species in low pressure Ar/H2/N2/O2 and Ar/CH4/N2/O2 microwave discharges, among them the main products such as H2O, NH3, NO and CO, HCN respectively. The hydroxyl radical has been measured in the mid infrared (MIR) spectral range in-situ in both plasmas yielding number densities of between 1011 ... 1012 cm-3. Strong indications of surface dominated formation of either NH3 or N2O and NO were found in the H2-N2-O2 system. In methane containing plasmas a transition between deposition and etching conditions and generally an incomplete oxidation of the precursor were observed.
The application of QCLs for IRLAS under low pressure conditions employing the most common tuning approaches has been investigated in detail. A new method of analysing absorption features quantitatively when the rapid passage effect is present is proposed. If power saturation is negligible, integrating the undisturbed half of the line profile yields accurate number densities without calibrating the system. By means of a time resolved analysis of individual chirped QCL pulses the main reasons for increased effective laser line widths could be identified. Apart from the well-known frequency down chirp non-linear absorption phenomena and bandwidth limitations of the detection system may significantly degrade the performance and accuracy of inter pulse spectrometers. The minimum analogue bandwidth of the entire system should normally not fall below 250 MHz.
QCLAS using pulsed lasers has been used for highly time resolved measurements in reactive plasmas for the first time enabling a time resolution down to about 100 ns to be achieved. A temperature increase of typically less than 50 K has been established for pulsed DC discharges containing Ar/N2 and traces of NO. The main NO production and depletion reactions have been identified from a comparison of model calculations and time resolved measurements in plasma pulses of up to 100 ms. Considerable NO struction is observed after 5 ... 10 ms due to the impact of N atoms.
Finally, thermoelectrically cooled pulsed and continuous wave (cw) QCLs have been employed for high finesse cavity absorption spectroscopy in the MIR. Cavity ring down spectroscopy (CRDS) has been performed with pulsed QCLs and was found to be limited by the intrinsic frequency chirp of the laser suppressing an efficient intensity build-up inside the cavity. Consequently the accuracy and advantage of an absolute internal absorption calibration is not achievable. A room temperature cw QCL was used in a complementary cavity enhanced absorption spectroscopy (CEAS) configuration which was equipped with different cavities of up to ~ 1.3 m length. This spectrometer yielded path lengths of up to 4 km and a noise equivalent absorption down to 4 x 10-8 cm-1Hz-1/2. The corresponding molecular concentration detection limit (e.g. for CH4, N2O and C2H2 at 1303 cm-1/7.66 μm) was generally below 1 x 1010 cm-3 for 1 s integration times and one order of magnitude less for 30 s integration times. The main limiting factor for achieving even higher sensitivity is the residual mode noise of the cavity. Employing a ~ 0.5 m long cavity the achieved sensitivity was good enough for the selective measurement of trace atmospheric constituents at 2.2 mbar.
(A paperback version is published by Logos under ISBN 978-3-8325-2345-9.)
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.
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.
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.
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.
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 der vorliegenden Arbeit wurde die Katodenregion einer quecksilberfreien Helium-Xenon Niederdruckentladung im Brennfleckbetrieb experimentell untersucht. Diese Region ist von besonderem Interesse, da sich hier die Elektronenemission, die Erzeugung von Ionen und metastabilen Atomen sowie lebensdauerbegrenzende Prozesse abspielen. Um die Entladung im Brennfleckbetrieb zu realisieren, kam als Katode eine im Rahmen dieser Arbeit entwickelte neuartige planare Geflechtelektrode zum Einsatz. Mit der Methode der ortsaufgelösten Laser-Atom-Absorptionsspektroskopie (LAAS) wurden die absoluten Teilchendichten der zwei untersten angeregten Xe-Atome und die Gastemperatur in der Katodenregion bestimmt. Die Inhomogenität des Spot-Plasmas fand dabei besondere Berücksichtigung. Sowohl die Teilchendichten der zwei untersten angeregten Xe-Atome als auch die Gastemperatur sind unmittelbar vor dem Brennfleck maximal und fallen in axiale und radiale Richtung stark ab. Insbesondere die Gastemperatur beträgt in einem Abstand von 1 mm vor dem Brennfleck circa 650 K und liegt damit deutlich über Raumtemperatur. Des Weiteren ließ sich die Temperatur im Brennfleck auf der Katodenoberfläche mittels optischer Emissionsspektroskopie ermitteln. Dies geschah durch Anpassung des aufgenommenen Spektrums an die Plancksche Strahlungsgleichung. Die Brennflecktemperaturverteilung weißt ein ausgeprägtes Maximum auf, das je nach Entladungsstromstärke maximale Werte zwischen 1414 K bei 40 mA und 1524 K bei 80 mA annimmt. Von diesem Maximum aus wurde ein starker in alle Richtungen nahezu symmetrischer Temperaturabfall festgestellt. Ein technologisch wichtiger Aspekt hinsichtlich der Lebensdauer einer auf Xenon basierenden quecksilberfreien Lampe ist der negative Effekt der Xe-Gasaufzehrung. In dieser Arbeit wird gezeigt, dass die Gasaufzehrung unter Verwendung der planaren Geflechtelektrode im deutlichen Gegensatz zur industriell gefertigten Becherelektrode, wie sie vielfach in Lampen für Lichtwerbung vorkommt, vernachlässigbar klein ist. Dies wird auf die Ausbildung eines heißen Brennflecks und die damit verbundene hohe Katodentemperatur und niedrige Katodenfallspannung zurückgeführt.
This thesis constitutes a computational study of charge and ion drag force on micron-sized dust particles immersed in rf discharges. Knowledge of dust parameters like dust charge, floating potential, shielding and ion drag force is very crucial for explaining complex laboratory dusty plasma phenomena, such as void formation in microgravity experiments and wakefield formation in the sheaths. Existing theoretical models assume standard distribution functions for plasma species and are applicable over a limited range of flow velocities and collisionality. Kinetic simulations are suitable tools for studying dust charging and drag force computation. The main aim of this thesis is to perform three dimensional simulations using a Particle-Particle-Particle-Mesh ($P^3M$) model to understand how the dust parameters vary for different positions of dust in rf discharges and how these parameters on a dust evolve in the presence of neighboring dust particles. At first, rf discharges in argon have been modelled using a three-dimensional PIC-MCC code for the discharge conditions relevant to the dusty plasma experiments. All necessary elastic and inelastic collisions have been considered. The plasma background is found collisional, charge-exchange collisions between ions and neutrals being dominant. Electron and ion distributions are non-Maxwellian. The dominant heating mechanism is Ohmic. Then, simulations have been done to compute the dust parameters for various sizes of dust located at different positions in the rf discharges. Dust charge and floating potential in the presheath are slightly larger than the values in the bulk due to the higher electron flux to the dust particle in the presheath. From presheath to the sheath the charge and floating potential values decrease due to the decrease of the electron current to the dust. A linear dependence of dust potential on dust size has been found, which results in a nonlinear dependence of the dust charge with the dust size when the particle is assumed to be a spherical capacitor. This has been verified by independently counting the charges collected by the dust. %where indeed it has been noted that the dust charge %scales nonlinearly with the dust size. The computed dust parameters are also compared with theoretical models. Simulated dust floating potentials are comparable to values obtained from Allen-Boyd-Reynolds (ABR) and Khrapak models, but much smaller than the values obtained from Orbit Motion Limited (OML) model. The dust potential distribution behaves Debye-H\"{u}ckel-like. The shielding lengths are in between ion and electron Debye lengths. % indicating shielding by both ions and electrons. Further, the orbital drag force is typically larger than the collection drag force. The total drag force for the collisional case is larger than for the collisionless case and it scales nonlinearly with the dust size. The collection drag values and size-scaling agrees with Zobnin's model. The charging and drag force computation is then extended to two and multiple static dust particles in the rf discharge to study the influence of neighboring dust particles on the dust parameters. Initially, the dust parameters on two dust particles are computed for various interparticle separation distances and for dust particles placed at different locations in the rf discharge. It is observed that for dust separations larger than the shielding length the dust parameters for the two dust particles match with the single dust particle values. As the dust separation is equal to or less than the shielding length the ion drag force increases due to the buildup of a parallel drag force component. However, the main dust properties like charge, potential, vertical component of ion drag are not affected considerably. This is attributed to the smaller collection impact parameter values compared to the dust separation. %This is because the %collection impact parameter values in the sheath and the presheath are smaller %than the smallest dust separation and in case of the dust in the bulk, the %collection impact parameter is comparable with the dust separation. Then the dust charges on multiple dust particles located at different positions in the discharge and arranged along the discharge axis are also computed. It is found that the charges of the multiple dust particles in the bulk or presheath do not differ much from the single particle values at that location. But the dust charges of multiple dust particles located in the sheath drastically differ from the single dust parameter values. Due to ion focusing from dust particles in the upper layers, the ion current increases to dust particles in the lower layers resulting in smaller charge values. This is as well the case where dust particles are vertically aligned as in the standard experiments of dusty plasmas. In conclusion, this work used a fully kinetic (PIC and MD or $P^3M$) model to study the physics of dust charging in rf plasmas. Our simulations revealed that the dust parameters vary considerably from the bulk to the sheath. The CX collisions increase flux to the dust thereby affecting the dust parameters and their scaling with dust size. Also, a dust particle affects the charging dynamics of its neighbor only when their separation is within the shielding length. In the plasma sheath, ion focussing can cause great reduction in dust charges.
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.
Kinetik der Ladungsträger und neutralen Spezies in anisothermen, molekularen Entladungsplasmen
(2009)
In dieser Arbeit wurde die Kinetik geladener und neutraler Spezies in anisothermen, molekularen Niederdruckentladungsplasmen untersucht. Als Arbeitsgas wurde Sauerstoff gewählt, da es noch eine Reihe grundlegender Fragen zu beantworten gibt und da Sauerstoff für viele technische Anwendungen von Interesse ist. Für eine adäquate Beschreibung des Elektronensubsystems wurde die stationäre, räumlich inhomogene kinetische Gleichung der Elektronen gelöst und die Elektronengeschwindigkeitsverteilungsfunktion (EVDF) bestimmt. Auf der Grundlage einer Legendre-Polynomentwicklung wurde eine strikte Multiterm-Beschreibung entwickelt, mit deren Hilfe die EVDF unter Vorgabe realistischer Potentialverläufe zwischen den Elektroden und der Plasmazusammensetzung im Druckbereich von 1 bis ~100 Pa bestimmt wurde. Es konnte der wesentliche Einfluß der dissipativen Stoßterme zur räumlichen Relaxation der EVDF erstmals für Sauerstoff gezeigt werden. In Bereichen kleiner Drücke ist ein Verhalten zu finden, welches typisch für Strahlelektronen ist, d.h. die an der Kathode eingestreute Elektronengruppe wandert praktisch ohne Dämpfung bis zur Anode. Dies spiegelt sich auch in den makroskopischen Größen wider, die im gesamten Entladungsgebiet eine starke räumliche Struktur aufweisen. Bei einer Druckerhöhung ist eine schnelle räumliche Relaxation der EVDF zu beobachten, die bereits beim Verlassen des Kathodenfallgebiets annähernd abgeschlossen ist. Damit in Verbindung stehen räumlich konstante Transportgrößen für die Elektronen oder deren mittlere kinetische Energie. Weiterhin wurde ein System hydrodynamischer Bilanzgleichungen für die betrachteten Spezies in Sauerstoff-Glimmentladungen abgeleitet, welches gekoppelt mit der Poisson-Gleichung gelöst wurde. Somit konnten die Dichten und Ströme der Spezies sowie das elektrische Potential selbstkonsistent bestimmt werden. Für die Analysen wurde ein reaktionskinetisches Modell für Sauerstoff entwickelt, welches alle relevanten Spezies und die zugehörigen Reaktionskanäle enthält. Insbesondere können in den hier betrachteten Plasmen mit Drücken um 100 Pa O2(b 1Σg+), O3 sowie O+ und O2- vernachlässigt werden. Somit war es möglich, sowohl das Startverhalten als auch den stationären Zustand der betrachteten Sauerstoff-Entladungen zu charakterisieren. Dabei konnte festgestellt werden, daß die metastabilen Moleküle O2(a 1Δg) keinen Einfluß auf kurze anormale Glimmentladungen haben, da ihre Dichte im Vergleich zum Bereich der positiven Säule äußerst gering ist. Dagegen wirken sich die negativen Ionen O- merklich auf die Formierung des Raumladungsfelds aus und müssen Berücksichtigung finden. Anhand einer Radiofrequenzentladung konnte zudem der Einfluß der Lokalen-Feld-Näherung (LFA) als auch der Lokalen-Mittleren-Energie-Näherung (LMEA) für die elektronischen Größen auf das Entladungsverhalten gezeigt werden. Hierbei konnte in Übereinstimmung mit der kinetischen Analyse der Elektronen festgestellt werden, daß die LFA zu einer erheblichen Überschätzung der entsprechenden Größen führt und zur nichtlokalen Beschreibung ungeeignet ist. Daher ist die Anwendung der LMEA im Rahmen einer hydrodynamischen Beschreibung zu empfehlen. Weiterhin wurde ein Hybrid-Verfahren entwickelt, welches eine kinetische Beschreibung der Elektronenkomponente sowie eine hydrodynamische Beschreibung der Spezies beinhaltet. Diese Methode wurde angewendet, um den stationären Zustand einer anormalen Sauerstoff-Glimmentladung zu bestimmen. Dabei wurden die Ratenkoeffizienten der Elektronenstoßprozesse auf einem kinetischen Niveau bestimmt und in der hydrodynamischen Beschreibung verwendet, so daß die Qualität der theoretischen Beschreibung wesentlich verbessert wurde. Dieses Verfahren wurde für einen direkten Vergleich mit den bisher durchgeführten rein hydrodynamischen Rechnungen genutzt. Dabei konnte wiederum festgestellt werden, daß die Ratenkoeffizienten in der Lokalen-Feld-Näherung überschätzt werden, was zum einen zu hohe Raten und Teilchendichten zur Folge hat und zum anderen auch die Entladungsparameter für einen erfolgreichen Durchbruch nicht korrekt charakterisiert.
Application of quantum cascade laser absorption spectroscopy to studies of fluorocarbon molecules
(2009)
The recent advent of quantum cascade lasers (QCLs) enables room-temperature mid-infrared spectrometer operation which is particularly favourable for industrial process monitoring and control, i.e. the detection of transient and stable molecular species. Conversely, fluorocarbon containing radio-frequency discharges are of special interest for plasma etching and deposition as well as for fundamental studies on gas phase and plasma surface reactions. The application of QCL absorption spectroscopy to such low pressure plasmas is typically hampered by non-linear effects connected with the pulsed mode of the lasers. Nevertheless, adequate calibration can eliminate such effects, especially in the case of complex spectra where single line parameters are not available. In order to facilitate measurements in fluorocarbon plasmas, studies on complex spectra of CF4 and C3F8 at 7.86 μm (1269 – 1275 cm-1) under low pressure conditions have been performed. The intra-pulse mode, i.e. pulses of up to 300 ns, was applied yielding highly resolved spectral scans of ∼ 1 cm-1 coverage. Effective absorption cross sections were determined and their temperature dependence was studied in the relevant range up to 400 K and found to be non-negligible.
Fluorocarbon containing capacitively coupled radio frequency (cc-rf) plasmas are widely used in technical applications and as model systems for fundamental investigations of complex plasmas. Absorption spectroscopy based on pulsed quantum cascade lasers (QCL) was applied in the mid-IR spectral range of 1269-1275 cm-1. Absolute densities of the precursor molecule CF4 and of the stable product C3F8 were measured with a time resolution of up to 1 ms in pulsed CF4/H2 asymmetrical cc-rf (13.56 MHz) discharges. For this purpose both the non-negligible temperature dependence of the absorption coefficients and the interference of the absorption features of CF4 and C3F8 had to be taken into account in the target spectral range. Therefore, at two different spectral positions composite absorption spectra were acquired under the same plasma conditions in order to discriminate between CF4 and C3F8 contributions. A total consumption of∼ 12 % was observed for CF4 during a 1 s plasma pulse, whereas C3F8 appeared to be produced mainly from amorphous fluorocarbon layers deposited at the reactor walls. A gas temperature increase by ∼ 100 K in the plasma pulse was estimated from the measurements. Additionally, not yet identified unresolved absorption (potentially from the excited CF4 molecule) was found during the àon-phase'.
An interesting aspect in the research of complex (dusty) plasmas is the experimental study of the interaction of micro-particles with the surrounding plasma for diagnostic purposes. Local electric fields can be determined from the behaviour of particles in the plasma, e.g. particles may serve as electrostatic probes. Since in many cases of applications in plasma technology it is of great interest to describe the electric field conditions in front of floating or biased surfaces, the confinement and behaviour of test particles is studied in front of floating walls inserted into a plasma as well as in front of additionally biased surfaces. For the latter case, the behaviour of particles in front of an adaptive electrode, which allows for an efficient confinement and manipulation of the grains, has been experimentally studied in terms of the dependence on the discharge parameters and on different bias conditions of the electrode. The effect of the partially biased surface (dc and rf) on the charged micro-particles has been investigated by particle falling experiments. In addition to the experiments, we also investigate the particle behaviour numerically by molecular dynamics, in combination with a fluid and particle-in-cell description of the plasma.
A central point of this thesis is the investigation of surface structure and surface forces, which are created by single layers of linear polyelectrolytes (PE). In detail, the properties of cationic poly(allylamine)hydrochloride (PAH) and poly-l-lysine (PLL) and anionic sodium poly(styrene sulfonate) (PSS) are determined, which have been physisorbed onto oppositely charged silica surfaces in presence of a predefined salt concentration IAds. For these investigations, a new averaging method for colloidal probe (CP) force profiles is developed, which leads to an ultimate force resolution of 1 pN after the data processing, (signal to noise ratio of > 1000). Furthermore, a new kind of tapping mode imaging is presented (so called colloidal probe tapping mode, CPTM), which uses a CP instead of a sharp tip and hence which allows to resolve lateral inhomogeneously distributed surface forces. The basics to understand such-like obtained tapping mode images are developed. For adsorption from salt-free solution (IAds = 0) the dominance of an electrostatic double layer repulsion is observed, which is commonly attributed to the adsorption of the PE chains into a rather flat and compact layer and which is in full agreement with theoretical predictions and enormous experimental data available in literature. However, even a small addition of salt to the deposition solution (i.e. IAds > 1 mM NaCl) introduces a new contribution to the surface force, which is attributed to PE chains that are non-flatly physisorbed. Using scaling considerations, it is shown for all investigated PE that this non-flat conformation can be described by brush-like chain adsorption (cf. Section 3.3.5); other conformations like mushroom or pancake are excluded (cf. Section 5.3). Interestingly, these non-flatly physisorbed chains combine properties of neutral and PE brushes: (i) The force is very well described by the theory of Alexander and de Gennes (AdG, cf. Section 5.4). By fitting the AdG force law to the data, it is possible to determine the (brush) thickness L of the PE layer and the average distance s between brush-like physisorbed chains. Although the chains are charged the electrostatic contribution to the surface forces is too small to be noticeable (cf. Section 5.4.2). (ii) The thickness L of this PE layer is much larger compared to the compact layer (observed for salt-free adsorption) and is also subject to a pronounced swelling and shrinking if the bulk salt concentration I is decreased or increased, respectively. Surprisingly, all measurements indicate that L follows a scaling law known for salted end-grafted PE brushes, i.e. L ~ N (I s^2)^(-1/3) (with N denoting the degree of polymerization). Furthermore, the osmotic brush phase is never observed in the experiments, but chain stretching up to 1 / 3 of the contour length is regularly achieved. CPTM imaging applied to PSS shows that the brush-like physisorbed chains are not homogenously distributed over the surface, but form brush domains which coexist with flatly physisorbed chains (cf. sections 5.5 and 5.6). This clearly shows that PSS generally physisorbs in two distinct phases, which differ in conformation (flat vs. brush) and the surface force caused (electrostatic vs. steric repulsion). The force profile of the two phase system is in good approximation simply the superposition of a steric and an electrostatic repulsion, whereby their respective contribution to the composed force profile is given by their area fraction. The quantitative analysis reveals that L and s of the brush phase are independent on IAds. This is remarkable, as a change in IAds is known to induce a continuous transition between a stretched (low IAds) and coiled chain conformation (high IAds) in the deposition solution (cf. [Fleer1993, Yashiro2002]). Hence, one can conclude that the conformation in solution does not necessarily correspond to the conformation after adsorption. It is also shown that the area fraction A of the brush domains strongly depends on N and IAds. For example, for constant N the scaling relation A ~ sqrt(IAds) is determined, which is very similar to the common observation that the surface coverage %Gamma of adsorbed PE layers increases also with %Gamma ~ sqrt(IAds) [Schmitt1996, Cosgrove1986, Ahrens2001, Yim2000, Gopinadhan2007, Cornelson2010]. This suggest that brush-like physisorbed PE chains are responsible for the increase in %Gamma. In fact, Section 5.6 shows that the mass of the brush phase is approx. 0.5 mg/m² which is comparable to the increase in %Gamma reported in literature for IAds = 1 M NaCl [Cosgrove1986, Schmitt1996, Ahrens2001]. As a change in IAds does not affect L and s, but solely the brush area fraction A, it is argued in Section 5.6 that an increase in IAds can be understood as a phase transition from the (disordered) flat phase towards the (ordered and extended) brush phase. Here, further theoretical considerations would be desirable.
Es wurde ein Versuchsaufbau für die Behandlung von Titanproben mittels der Plasma-Immersions-Ionen-Implantation konzipiert, konstruiert und aufgebaut. Im Unterschied zu üblichen PIII-Anlagen wurde hier eine kapazitiv gekoppelte RF-Entladung als Hintergrundentladung mit zwei koplanaren Elektroden direkt über den zu behandelnden Titanproben benutzt. Auf diese Weise war es möglich unter Verwendung von Kupfer für die Elektroden und den Probenhalter, die Titanproben mit Kupfer zu dotieren und parallel, durch die Wahl geeigneter Prozessgase, zu oxidieren. Zusätzlich waren neben Prozessgaskontrollern auch Flüssigkeitskontroller vorhanden, so dass mit diesem Versuchsaufbau Gase, verdampfte Flüssigkeiten und erodierte Metalle in verschiedensten Kombinationen gleichzeitig als Prozessgas für die PIII zur Verfügung gestellt werden konnte. Wie bei PIII-Prozessen erforderlich, waren die Hochspannungshöhe und -dauer einstellbar. Der Strom wurde so gemessen, dass er die Ionendosis wider gibt und für die Temperaturmessung der Substratoberfläche wurde ein in-situ Pyrometer verwendet. Die relevanten elektrischen Parameter wurden mittels eines Oszilloskops bestimmt. Es stellte sich heraus, dass ein Gesamtionenstrom von bis zu 48mA implantiert werden konnte. Dies entspricht bis zu 3.5 x 1015 Ionen cm-2 s-1 und dementsprechend einem Energiestrom von bis zu 5 J cm-2 s-1. Die daraus resultierenden Temperaturen der Substratoberfläche betrugen bis zu 600 °C. Diese Parameter bewegen sich durchaus im Parameterfeld herkömmlicher Anlagen. Der erste inhaltliche Arbeitsgegenstand dieser Arbeit bestand darin, die Oberfläche der Titanproben unter Verwendung von Sauerstoff als Prozessgas mit einem ausreichend dicken und idealerweise kristallinen Titandioxid zu modifizieren. Auf diese Weise wurde die undefinierte natürliche Oxidschicht durch ein definiertes Oxid ausgetauscht. Röntgen-Diffraktometrie Messungen der modifizierten Proben ergaben neben alpha-Titan auch Rutil als primäre Kristallstruktur in der Oberfläche. Durch Variation der Prozessparameter, speziell des Duty-Cycle und damit des Ionenstroms bzw. der Temperatur der Titanproben, konnte die Konzentration an Rutil direkt gesteuert werden. Der zweite inhaltliche Arbeitsgegenstand bestand in der Modifikation des Prozesses und des Versuchsaufbaus zur Dotierung des Titans mit einem antimikrobiell wirksamen Metall, wobei Kupfer aufgrund seiner biologischen Eigenschaften favorisiert wurde. Um die positiven physikochemischen Eigenschaften der Titandioxidoberfläche bestmöglich zu nutzen, wurde parallel zur Dotierung mit Kupfer eine definierte Titandioxid-Schicht erzeugt. Als Prozessgas wurden dafür sauerstoffhaltige Gase, speziell Sauerstoff und Wasserdampf verwendet. Es zeigte sich, dass mit Sauerstoff aufgrund des hohen atomaren O Anteils CuO und TiO2 erzeugt, während mit Wasserdampf, aufgrund der reduzierenden Wirkung des Wasserstoffs, bis zu 30% metallisches Kupfer in die TiO2 Matrix eingebracht werden konnte. Zusätzlich konnte ein Übergang von alpha-Titan für kleine Ionendosen zu Rutil für Dosen oberhalb von 4 x 1018 Ionen cm-2 und 450 °C festgestellt werden. Weiterhin zeigten die Diffraktogramme Ti3O als Übergangsmodifikation, jedoch keine Kupfer- oder Kupferoxidkristalle. Durch geeignete Prozessparameterwahl ist es daher selbst bei geringen Implantationsspannungen von 10 kV möglich, einen bis zu 200nm dicken Verbund aus kristallinem TiO2 (Rutil) angereichert mit metallischem Kupfer zu erzeugen. Ein zusätzlicher Arbeitsgegenstand bestand in exemplarischen Zelltests mit Staphylococcus aureus (MRSA) und MG-63 Zellen als Vertreter für problematische Krankenhauskeime bzw. als Modellorganismus für Knochenzellen. Parallel zu diesen Versuchen wurde das Kupfer-Release der mit Kupfer dotierten Titanoberfläche bestimmt. Mit höheren Ionendosen während der Ionenimplantation konnten die Proben dahingehend modifiziert werden, dass eine höhere Kupferkonzentration aus dem Verbund ausgelöst wurde. Dieser Verlauf spiegelte sich auch in den Zelltests wieder. Während die Vitalität der MG-63 Zellen mit steigender Dosis abnahm, stieg die antibakterielle Wirkung an. So konnten über 95% der Bakterien getötet werden, wobei die Zellvitalität mit 80% im Vergleich zur Zelle auf dem Deckgläschen immer noch sehr hoch war. Weiterhin wurde eine brauchbare numerische Simulation erstellt, die ein besseres Verständnis der physikalischen Prozesse auf und unter der Oberfläche der zu modifizierenden Proben ermöglichte. Zusätzlich kann, basierend auf dieser Simulation, eine Prozessabstimmung geschehen. In die Simulation gingen die mit der Software TRIM simulierten Tiefenprofile, Sputterraten der einzelnen Oberflächenelemente, Elementanteile der Oberfläche sowie der einfliegenden Ionen und deren Energie mit ein. Dabei zeigte sich, dass die experimentell erhaltenen Tiefenprofile mit diesem Modell bis zu einem gewissen Genauigkeitsgrad qualitativ und quantitativ erklärt werden können.
This thesis presents the results of experimental investigations of the vertical and lateral properties of polyelectrolyte multilayer films (PEMs) adsorbed on a solid support. PEMs are a new class of organic thin films based on self-assembly layer-by-layer (LbL) processes of oppositely charged polyelectrolytes (charged polymers). The LbL assembly technique allows precise control of film thickness within a few nanometers and makes PEM systems especially interesting for technical applications. Thin films are prepared by alternating exposure of a hydrophilic substrate to solutions of oppositely charged polyelectrolytes. In this work, synthetic polycation poly (allylamine hydrochloride) (PAH) and polyanion poly (styrene sulfonate) (PSS) have been used. Range and amplitude of the electrostatic force during PEM build-up, has been shielded by use of high salt concentration in the deposition solution. As a foundation of any theory, role of non-elecrostatic (secondary) forces is explored. Four complementary methods have been combined to investigate the properties and composition of PEMs. X-ray reflectivity is sensitive to electron density gradients, and therefore provides information about film thickness, average electron density and interfacial roughness between materials of different electron densities (like PEM and air). Neutrons are the unique probe that is sensitive to the internal order of the multilayers (scattering length density variation) due to selective deuteration of the layers (PSS replaced by PSS_d). Therefore neutron reflectivity at V6 beamline, at the research reactor BER II, Helmholtz Centre for Materials and Energy (former Hahn-Meitner-Institute), was used in this work. Ultraviolet-visible (UV-Vis) light induces the characteristic absorption peak of polyelectrolytes and metallic nanoparticles, therefore with UV-Vis absorption spectroscopy is possible to probe the aggregation of metallic nanoparticles embedded into PEM by measuring their absorption spectra (imaginary part of the refraction index). Atomic force microscopy (AFM) allows to observe lateral structures at nano-level and to obtain surface topology of the films. Application of only small forces (pN) is achieved by use of a intermittent contact (tapping) mode in air. Summarizing the main results, the unambiguous parametrization of the investigated system for neutron reflectivity measurements enables to obtain detailed information about internal interfaces. New approach for polyelectrolyte multilayer architectures consisting of thick protonated and deuterated blocks can be used in order to distinguish different zones of the thin film growth which can be described as precursor and core zones. Thus, almost no bound water is found in precursor layers at 0% relative humidity, which suggests that water is mobile and the precursor layer is not in the glassy state like in the central zone of the PEM. Swelling behaviour of the PEMs (reversibility of the swelling) can be understood in terms of equilibrium reactions. Explored influence of temperature and type of salt used during preparation contributes to a better understanding of the formation of PEMs. The dependence of the film thickness on preparation temperature, concentration and the type of salt can be described by the hydrophobic nature of the effect. Experimental observations demonstrate that it is possible to decrease both the range and the amplitude of the electrostatic force by using an ion concentration of at least 0.1 mol/L in the solution. The role of secondary interactions such as hydrophobic attraction of the chains that can overcome electrostatic repulsion and become the major contributing factor for the layer formation and resulting structures is emphasized.
Tunable Diode Laser Absorption Spectroscopy in the mid InfraRed spectral range (IR-TDLAS) has been applied to investigate the behaviour of CF, CF2 and C2F4 species produced in pulsed CF4/H2 capacitively coupled radio frequency plasmas (13.56 MHz CCP). This experimental technique was shown to be suitable for temporally resolved measurements of the absolute number density of the target molecules in the studied fluorocarbon discharges. The temporal resolution of about 20…40 ms typically achieved in the standard data acquisition mode (“stream mode”) was sufficient for the real-time measurements of CF2 and C2F4, but not of CF whose kinetics was observed to be much faster. Therefore, a more sophisticated approach (“burst mode”) providing a temporal resolution of 0.94 ms was established and successfully applied to CF density measurements. In order to enable the TDLAS measurements of the target species, preliminary investigations on their spectroscopic data had been carried out. In particular, pure C2F4 has been produced in laboratory by means of vacuum thermal decomposition (pyrolysis) of polytetrafluoroethylene and used as a reference gas. Therefore, an absorption structure consisting of several overlapping C2F4 lines around 1337.11 cm-1 was selected and carefully calibrated, which provided the first absolute measurements of the species by means of the applied experimental technique. The absolute number density traces measured for CF, CF2 and C2F4 in the studied pulsed plasmas were then analysed, in which two differential balance equations were proposed for each of the species to describe their behaviour during both “plasma on” and “plasma off” phases. Analytical solutions of the balance equations were used to fit the experimental data and hence to deduce important information on the kinetics of the studied molecules. In particular, during the “plasma off” phase, the self-recombination of CF2 (CF2 + CF2 (+M) → C2F4 (+M)) was found to be dominant in the kinetics of the radical, but of minor importance for C2F4 production. A rapid consumption of CF observed within 7…25 ms after switching off the plasma was explained mainly by volume reaction with other species (most likely with CF3), whereas diffusion of the radical towards the reactor walls followed by sticking on the surfaces was found to contribute only at relatively low pressures (<10 Pa). Under certain discharge conditions, measured CF density traces exhibited significant overshoots in 50…150 ms after the plasma ignition, which had not been known from literature before. The electron impact fragmentation of C2F4 was shown to be essential for CF production at the beginning of the “plasma on” phase and therefore for formation of the observed CF density overshoots. Finally, the broad band FTIR spectroscopy was applied in order to better characterize the gas phase composition of the studied plasmas. Thus, absorption bands of CF4, C2F4, C2F6, C3F8, CHF3 and HF stable molecules were detected in the FTIR spectra recorded between 400 and 4000 cm-1. The spectra were then successfully deconvolved and the absolute concentration of the detected species was estimated. In particular, the absolute number density of C2F4 obtained from the FTIR measurements was in a good agreement with that achieved by means of the IR-TDLAS technique. The work was supported by the German Research Foundation (DFG) within the framework of the Collaborative Research Centre Transregio 24 “Fundamentals of Complex Plasmas” (SFB/TRR24, project section B5).