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In this thesis wave propagation in the whistler wave frequency range ωci≤ω≤ωce in the linear magnetized plasma experiment VINETA is investigated. The plasma is generated by a helicon antenna and has a diameter of about 10 cm. Whistler waves are launched by a loop antenna with a diameter of 4.5 cm and the fluctuating magnetic field is mapped by Ḃ-probes. Experiments are carried out for plasma parameters γ≤1/ √ 2 under which the only transversal polarized wave according to plane wave dispersion theory is the whistler wave. Due to the small collision frequencies ν≪1 cyclotron damping of whistler waves in this parameter regime is dominant and depends only on the electron plasma-β. The influence of the inhomogeneous plasma profile and excitation by a loop antenna is investigated by measurements of the fluctuating magnetic field perpendicular to the ambient magnetic field in azimuthal and radial axial planes. A mode characterized by the number of wave lengths m in the azimuthal direction is found. The mode structure is modified by the specific shape of the plasma density profile. Profiles with a homogeneous density inside the plasma radius are found to posses a comparably simple mode structure. An agreement in the mode structure of full-wave simulations in three dimensions, including a Gaussian density profile and excitation of the wave by a loop antenna, with the experimental results is found. Conclusions on the spatial structure of the excited mode are drawn using the simulations which predict excitation of an m=2 mode. The wave is found to be ducted within the plasma radius over a wide parameter range. A Helmholtz decomposition of the simulations electric field exhibits the fluctuating space charge as the dominant source for the electric field, while the contribution due to induction is negligible. The magnetic field is given partially by the electron and displacement current. Both contributions to the magnetic field are of the same order of magnitude. The frequency dependency of the excited modes spatial damping increment is investigated using measurements of the magnetic fluctuations along the symmetry axis of the plasma. In order to illustrate the parameter dependency, the electron plasma-β is varied over two orders in magnitude in the range β = 4·10-4 - 2.4·10-2. The experimental result for the spatial damping increment of the mode yields a strong damping for wave frequencies ω/ωce > 0.5 at maximum plasma-β, which shifts to higher frequencies with decreasing β. The parameter dependency of the damping for a fixed frequency is studied in an axial ambient magnetic field gradient. In both cases an excellent agreement between the experimental result and predictions for cyclotron damping from plane wave dispersion theory is found.
In der vorliegenden Arbeit wurden die Wechselwirkungen zwischen den reaktiven Sauerstoffspezies (ROS) und den Lipiden, die das Grundgerüst der Zellmembran bilden, sowie die daraus resultierenden chemischen und physikalischen Veränderungen der Membran untersucht. Außerdem wurde der Schutz einer Modellmembran durch Adsorption eines Polymers untersucht. Da natürliche Zellmembrane hoch komplexe Systeme sind, in und an denen chemische und strukturelle Prozesse häufig gleichzeitig ablaufen, wurden Lipidmonoschichten und Liposomen als Modellmembranen für die Untersuchungen gewählt. Die Radikale wurden mithilfe der Fenton-Reaktion erzeugt. Um ein vollständiges Bild des Radikalangriffs auf Modellmembrane zu erhalten, war es notwendig verschiedene Untersuchungsmethoden zu verwenden. Die Lipidmonoschichten und deren Phasenumwandlungen wurden vor und nach dem Radikalangriff mithilfe des Langmuir-Troges und den damit aufgenommenen Isothermen untersucht. Die Fluoreszenz- und die Brewsterwinkel-Mikroskopie wurde genutzt, um die Veränderungen des Phasenübergangs und somit die Veränderungen der Form und des Wachstums von Lipid-Domänen (flüssig-kondensierten Phase) durch den Radikalangriff zu beobachten. Die laterale periodische Struktur und das vertikale Elektronendichteprofil der Lipidmonoschicht wurden mit der Röntgendiffraktion und Röntgenreflexion vor und nach dem Radikalangriff untersucht. Mit der Infrarot-Reflexion-Absorption Spektroskopie (IRRAS) können Aussagen über die chemische Veränderungen der Lipide nach dem Radikalangriff getroffen werden. Die Liposomen wurden mit Differenzkalorimetrie untersucht, um die Verschiebung der Phasenübergangstemperatur durch den Radikalangriff zu beobachten. Der Radikalangriff auf Liposomen wurde mit Fluorenzmikroskopie verfolgt. Im ersten Teil der Arbeit wurde die Wechselwirkung von ROS mit zwitterionisch geladenen Lipiden untersucht. Die Modellmembranen bestanden aus Phosphatidylcholinen. Fasst man alle Ergebnisse der Untersuchungen zusammen, führt dies zum folgenden Resultat: Die Radikale reagieren bevorzugt mit der Kopfgruppe der zwitterionischen Phosphatidylcholinen. Es entstehen negativ geladene Phospholipide mit einer kleineren Kopfgruppe. Die Alkylketten bleiben nach dem Radikalangriff unverändert. Wie die Isothermen und die Brewsterwinkel-Mikroskopie bei Monoschichten sowie die Thermogramme bei Liposomen zeigen, hat die Reaktion keinen erkennbaren Einfluss auf das thermodynamische Verhalten. Erst durch Zugabe bzw. bei Vorhandensein von „freien“ Eisen-Ionen wird die Veränderung der Phosphocholine durch die Radikale beobachtbar. Die „freien“ Eisen-Ionen binden an die negativ geladenen Phospholipde. Dies führt im Fall von DPPC (1,2-dipalmitoyl-sn-glycero-3-phosphocholine) Monoschichten zu einer irreversiblen Verfestigung. Weiterhin kommt es zur Abnahme der molekularen Fläche in der flüssig-kondensierten Phase. Im Fall von DMPC (1,2-dimyristoyl-sn-glycero-3-phosphocholine) Liposomen führt der Radikalangriff, bei Vorhandensein von „freien“ Eisen-Ionen, ebenfalls zu einer Verfestigung. Am Ende des Radikalangriffs sind die Liposomen zerstört. Im zweiten Teil der Arbeit wurde die Wechselwirkung von ROS mit negativ geladenen Phospholipiden untersucht. Dabei wurde herausgefunden, dass die negative Ladung der Phospholipide nach dem Radikalangriff erhalten bleibt. Die Alkylkettenlänge bleibt konstant. Die durchgeführten IRRAS Messungen zeigen ebenfalls keine Veränderungen der Alkylketten. Aufgrund der Beobachtung, dass Eisen-Ionen negativ geladene Modellmembranen verfestigen, sollte im dritten Teil dieser Arbeit die Eisenanbindung an negativ geladene Monoschichten am Beispiel des Cardiolipin TMCL quantifiziert werden. Bei einem physiologischen pH-Wert führt eine Eisen-Ionen Konzentration im mikromolaren Bereich zu einer irreversiblen Verfestigung der Monoschicht. Der pH-Wert ist ein entscheidender Parameter. Eine irreversible Verfestigung der Monoschicht kann durch einen pH-Wert von 1,3 oder niedriger verhindert werden, wenn die Eisenkonzentration kleiner als 1000 µM ist. Bei höheren Eisenkonzentrationen tritt auch bei diesem pH-Wert eine Verfestigung ein. Im vierten Teil dieser Arbeit wurde die Wechselwirkung von ROS mit einer negativ geladenen Lipid-Monoschicht (DMPG) mit adsorbierten Polykationen (Polyethylenimin (PEI)) untersucht. Die adsorbierte Polymerschicht dient zum Schutz der Lipidmonoschicht. Der Radikalangriff wurde mit verschiedenen Fenton-Konzentrationen durchgeführt. Es war eine signifikant höhere Fenton-Konzentration als bei dem Radikalangriff auf eine DPPC Monoschicht notwendig, um Veränderungen zu induzieren.
The layer-by-layer method is a robust way of surface functionalization using a wide range of materials, e.g. synthetic and natural polyelectrolytes (PEs), proteins and nanoparticles. Thus, this method yields films with applications in diverse areas including biology and medicine. Sequential adsorption of different oppositely charged macromolecules can be used to prepare tailored films with controlled molecular organization. In biomedical research, electrically conductive coatings are of interest. In manuscript 1, we investigated films sequentially assembled from the polycation poly (diallyldimethyl-ammonium) (PDADMA) and modified carbon nanotubes (CNTs), with CNTs serving as the electrically conductive material. We assume that charge transport occurs through CNT contacts. We showed that with more than four CNT/PDADMA bilayers, the electrical conductivity is constant and independent of the number of CNT/PDADMA bilayers. A conductivity up to 4∙10^3 S/m was found. It is possible to control the conductivity with the CNT concentration of the CNT deposition suspension. A higher CNT concentration resulted in thicker CNT/PDADMA bilayers, but in a lower conductivity per bilayer. We suspect that an increased CNT concentration leads to a rapid CNT adsorption without the possibility to rearrange themselves. If PDADMA then adsorbs on the disordered CNTs in the next deposition step, the average thickness of the polymer layer is thicker than on the more ordered CNT layer from the dilute solution. This leads to an increased PE monomer/CNT ratio and lower conductivity. More polycations between the CNT layers leads to less CNT contacts. Thus, the controlled composition of films can be used to fulfill specific requirements.
For many applications of polyelectrolyte multilayers (PEMs), cheap PEs with a broad distribution of molecular weights are used. It was unknown whether the distribution of molecular weights of the PE in the adsorption solution is maintained during the adsorption process and hence in the film. To investigate this, the PSS adsorption solution in article 2 consisted of a binary mixture of short and long poly (styrene sulfonate) (PSS). A good model system to study layered films in terms of composition are PDADMA/PSS multilayers. Neutron reflectivity and in-situ ellipsometry measurements were carried out to determine the PSS composition in the film and the growth regimes. At a mole fraction of long PSS of 5 % or more in solution, the exponential growth (which is characteristic of short PSS) is totally suppressed, and only long PSS is deposited in the resulting multilayer. Variation of adsorption time of PSS showed that short PSS first adsorbs to the surface but is displaced by long PSS. Between 0 and 5 % of long PSS in the adsorption solution exponential growth occurs. The fraction of short PSS in the film continuously decreases with the increase of long PSS in the adsorption solution. In the assembly of films prepared from binary PSS mixtures, the short PSS leaves the film through adsorption/desorption steps both during PSS adsorption and during PDADMA adsorption (as PDADMA/PSS complexes). Both techniques show that the composition of the film does not correspond to that of the deposition solution. The composition and thus the properties of the resulting multilayer are influenced by the choice of adsorption time. Moreover, we conclude that a multilayer grown from a polydisperse polyelectrolyte contains fewer mobile low molecular weight polymers than the deposition solution.
In manuscript 1 and article 2, the composition of multilayers was studied. In manuscript 1 adsorption kinetics were important for the arrangement of CNTs on the surface. In article 2, the adsorption kinetics, i.e. the diffusion of the polyelectrolytes to the surface, was also investigated. In article 3, we investigated the influence of the composition of the film as well as the preparation condition on the mobility of PEs in the film. The molecular weight of the polycation PDADMA and the NaCl concentration of the deposition solution were varied. The vertical PSS diffusion constant D_PSS within the PDADMA/PSS multilayers was measured using neutron reflectivity. The salt concentration of the preparation solution defines the polymer conformation during deposition. The molecular weight of the polycation determines the degree of intertwining. Together, both parameters determine the polyanion-polycation coupling and thus the PSS mobility within the network. Log−log display of D_PSS vs the molecular weight of PDADMA and fits to two power laws (D_PSS ∝ X_n(PDADMA)^(-m) ∝ M_w(PDADMA)^(-m)) reveals for films built from 10 or 200 mM NaCl a kink. Below and above the kink, the dependence of D_PSS on M_w(PDADMA) can be described by different power laws. For Χ_n(PDADMA) < X_n,kink(PDADMA) ≈ 288, the exponents are consistent with the predictions of the sticky reptation model. X_n(PDADMA) ≈ 288 is the entanglement limit. For Χ_n(PDADMA) > X_n,kink(PDADMA) ≈ 288, the decrease of D_PSS with M_w(PDADMA) is larger than below the entanglement limit, which is indicative of sticky reptation and entanglement. The PSS diffusion constant of films built from 100 mM NaCl drops three orders of magnitude when increasing the molecular weight of PDADMA from 45 kDa to 72 kDa. To figure out if an immobile PSS fraction exists in the film built from 72 kDa PDADMA (beyond the entanglement limit), the film was annealed at different conditions in article 4: both temperature and salt concentration were varied. For data analysis, the simplest model with two PSS fractions with different diffusion constants was used. These diffusion constants increase as the temperature of the surrounding solution is increased. As assumed in article 3, an immobile PSS fraction exists when annealing at room temperature. At higher annealing temperatures, at least two diffusion processes must be distinguished: the diffusion of the highly mobile PSS fraction through the entire film and a slow PSS fraction, mowing in a limited way. The choice of preparation conditions determines whether a polyelectrolyte multilayer can intermix completely. It is not clear if complete intermixing will ever occur for films built with PDADMA beyond the entanglement limit. It is possible that the diffusion is more complex. Long-term measurements will clarify this question. Calculating scattering length density profiles with subdiffusive behavior would be interesting and is a challenge for the future. Furthermore, immobile fractions are only visible with long annealing times. We hypothesize that an immobile or nearly immobile fraction is present whenever the dependence of D_PSS on the molecular weight of PDADMA cannot be described by the sticky reptation. To verify this hypothesis, further studies are necessary.
All results presented and discussed in the manuscript and articles show that by varying the preparation conditions, tailored films can be built. The composition of the film is also determined by the adsorption kinetics. In addition, the mobility of the PEs within the multilayers can be controlled by varying the conformation, mingling and entanglement of the chains within the film. The influence of the salt concentration in the preparation solution on the growth regimes during film formation is part of our future research. It is planned to investigate films built of different PDADMA molecular weights under varied annealing conditions to better understand the mobile and immobile fractions.
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.
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.
Die Forschung an mikrowelleninduzierten Atmosphärendruckplasmen am INP führte zu verschiedenen potentiellen Applikationen. Dabei besitzt die mikrobiologische Dekontamination sowohl von thermolabilen Medizinprodukten als auch von Lebensmitteln schon zum jetzigen Zeitpunkt ein hohes industrielles Anwendungspotential. Den aufgeführten Anwendungen gemeinsam ist, dass für eine erfolgreiche Weiterentwicklung der Prozesse, sowie der Plasmaquelle, ein grundlegendes Verständnis der vorliegenden dynamischen Mikrowellenplasmawechselwirkung notwendig ist. Durch den begrenzten diagnostischen Zugang der zu untersuchenden Plasmaquelle wird ein kombinierter Ansatz aus diagnostischen Methoden und Modellierung gewählt. Die Entladung wird in Argon bei reduziertem Druck (ab 10 mbar) zur Vereinfachung des Modells betrieben. Daher musste die Plasmaquelle für diesen Einsatz weiterentwickelt werden. Dieses beinhaltet die Neuauslegung der Prozesswärmeabfuhr, auf Grund der nicht oder nur teilweisen Anwendbarkeit von etablierten Verfahren im Atmosphärendruck (hohe Gasflüsse, Wasserkühlung). Die Plasmamikrowellenwechselwirkung dieser Quelle ist anschließend mit Methoden zur Charakterisierung des Plasmas und des Mikrowellenfeldes für unterschiedliche Arbeitspunkte in Druck und Leistung untersucht worden. Zur Bestimmung der Elektronendichte des Plasmas wurde ein frequenzvariables Mikrowelleninterferometer auf Basis eines Vektornetzwerkanalysators erstmalig etabliert. Dieses neue Messsystem wurde im Vorfeld detailliert untersucht, um das korrekte Zusammenspiel aller Komponenten zu überprüfen. In diesem Zusammenhang wurde ein frequenzaufgelöstes Mikrowelleninterferometer zur Messung der Elektronendichte in einer Fluoreszenzlampe aufgebaut. Durch diesen neuartigen Ansatz konnte der Einfluss der dielektrischen Umhüllung (Glasrohr der Lampe) auf die Mikrowelleninterferometrie untersucht werden. In einer weiteren Untersuchung an einem Induktiv Gekoppelten Plasma wurden die Resultate dieses Messsystems mit denen von Langmuir-Sondenmessungen. Auf Grund der konstruktiven Gegebenheiten des Reaktors ist das Plasma nur über ein Fenster für das Mikrowelleninterferometer zugänglich. Der Vergleich der ermittelten Elektronendichten ergab einen Unterschied von Faktor zwei zwischen Interferometer und Langmuir-Sonde. Die Untersuchungen an der Fluoreszenzlampe und dem Induktiv Gekoppelten Plasma zeigten zum einen die korrekte Funktion des neu etablierten frequenzvariablen Mikrowelleninterferometers mit erreichbaren Phasenauflösungen unterhalb von 0,1 mrad. Zum anderen wurde festgestellt, dass die dielektrische Umhüllung des Plasmas zu einem systematischen Fehler von bis 53 % bei der Elektronendichtebestimmung führen kann. Diese gewonnenen Erkenntnisse hatten bei der Konzipierung des Mikrowelleninterferometers zur Untersuchung der Plasmamikrowellenwechselwirkung einen entscheidenden Einfluss. Neben der Untersuchung des Plasmas ist ebenfalls eine Diagnostik des Mikrowellenfeldes nötig, um die Plasmamikrowellenwechselwirkung dieser Entladung experimentell zu charakterisieren. Auf Grundlage dieser Daten können die Resultate des Modells bewertet werden, die einen Einblick in die Plasmaquelle und ihrer dynamischen Vorgänge erlaubt, was für die Weiterentwicklung der Applikationen essentiell ist. Aus diesem Grund ist ein heterodynes Reflektometer entwickelt worden. Dieses Messsystem wurde umfangreich getestet und kann mit einer maximalen Zeitauflösung von 100 ns den komplexen Reflektionsfaktor mit einer Phasengenauigkeit von 10 mrad bestimmen. Das Reflektometer erlaubt einen experimentellen Zugang zur aktiven Zone schon in der Frühphase der Entladung. Mit Hilfe der Diagnostiken zur Untersuchung des Plasmas und des Mikrowellenfeldes wurde die Entladung von der Zündung bis zur stationären Phase charakterisiert und mit den Ergebnissen des Modells verglichen. Es zeigte sich eine gute Übereinstimmung im Millisekundenzeitbereich, sowie eine starke Dynamik im Reflektionsfaktor in der ersten Millisekunde, hervorgerufen durch die Plasmamikrowellenwechselwirkung. Durch die hohe Zeitauflösung des Reflektometers konnten diese Vorgänge im Mikrosekundenzeitbereich erstmalig experimentell aufgelöst werden, was die Interpretation mittels des Modells möglich macht. Es konnten die Vorgänge während der Zündung des Plasmas detailliert untersucht werden und damit die Richtigkeit von Annahmen, die bei der Entwicklung der Zündtechnologie getroffen wurden, überprüft werden. Dieses erworbene grundlegende Verständnis ermöglicht eine Weiterentwicklung dieser Technologie. Mit Hilfe der erzielten Ergebnisse wurde eine neue Optimierungsstrategie für die Abstimmung der Mikrowellenplasmaquelle entwickelt. Dies führte zu einer wesentlichen Verbesserung der Reproduzierbarkeit der mikrobiologischen Ergebnisse. Darüber hinaus bilden die erzielten Ergebnisse eine solide Grundlage für weitere experimentelle und theoretische Untersuchungen dieser Entladung in beispielsweise anderen Arbeitsgasen.
Polyelektrolyt-Multischichten werden durch die sequentielle Adsorption von entgegengesetzt geladenen Polyelektrolyten auf einem festen Substrat hergestellt. Die Präparation layer-by-layer ermöglicht die Beschichtungen von Flächen im cm-Bereich mit Schichtdicken im µm-Bereich sowie einer Kontrolle der Molekülanordnung senkrecht zur Substratoberfläche im nm-Bereich. Aus diesen Eigenschaften ergeben sich zahlreiche Anwendungsmöglichkeiten. Ein Schwerpunkt dieser Arbeit ist die Analyse der Polyelektrolyt-Adsorption bei der Präparation von Multischichten bestehend aus dem Polykation Polyallylaminhydrochlorid (PAH) und dem Polyanion Polystyrolsulfonat (PSS) bzw. Polydiallyldimethylammonium (PDADMA) und PSS. Die Untersuchung der Multischichten unter in-situ Bedingungen erfolgt mittels Ellipsometrie. Zu diesem Zweck wird ein Formalismus der ellipsometrischen Datenauswertung entwickelt, um die Messgenauigkeit bei der Untersuchung dünner, transparenter Schichten zu optimieren. Im Fall von PDADMA/PSS-Multischichten verläuft das Schichtwachstum nicht-linear mit der Anzahl an adsorbierten Doppelschichten. Der nicht-lineare Verlauf wird mit der unterschiedlichen Linienladungsdichte zwischen einer PDADMA- und einer PSS-Kette in Verbindung gebracht. Die quantitative Analyse der ellipsometrischen in-situ-Messungen ergibt, dass alle untersuchten PDADMA/PSS-Multischichten (präpariert aus 0,1 mol/L NaCl-Lösung bei Raumtemperatur) mindestens zwei verschiedene Wachstumsregimes aufweisen: Erst wächst die Schichtdicke parabolisch mit der Anzahl an deponierten Polyanion/Polykation-Schichtpaaren, nach Nlin Schichtpaaren erfolgt ein Übergang in lineares Schichtwachstum, charakterisiert durch eine konstante Dicke pro Schichtpaar dBL. Das parabolische Wachstumsregime lässt sich mit einer Asymmetrie im Adsorptionsverhalten von PDADMA und PSS erklären: Während die adsorbierenden PSS-Moleküle die Oberflächenladung lediglich neutralisieren, führt ein PDADMA-Beschichtungsschritt zu einer Ladungsüberkompensation und hinterlässt eine effektiv positiv geladene Oberfläche. Die deponierte Stoffmenge nimmt mit jeder PDADMA/PSS-Doppelschicht zu, bis nach Nlin Doppelschichten die adsorbierenden PSS-Ketten nicht mehr imstande sind alle positiven Oberflächenladungen zu neutralisieren. Die beiden Wachstumsparameter Nlin und dBL hängen in einem linearen Zusammenhang voneinander ab, da beide einem gemeinsamen Mechanismus folgen: Je mehr Doppelschichten ein parabolisches Wachstumsverhalten zeigen (Nlin), desto höher ist die Oberflächenbelegungsdichte am Ende des parabolischen Wachstumsregimes und desto größer die Doppelschichtdicke dBL. Das Adsorptionsverhalten von PDADMA- und PSS-Ketten wird analysiert, indem das Molekulargewicht Mw beider Polyelektrolyte systematisch variiert wird (zwischen Mw(PDADMA) = 24 kDa ... 322 kDa sowie Mw(PSS) = 8,6 kDa ... 168 kDa). Die Flächenbelegungsdichte pro Doppelschicht wächst proportional zu Mw(PDADMA) an, bis ab dem Schwellwert Mw(PDADMA) = 80 kDa eine Sättigung eintritt und das Schichtwachstum unabhängig vom Wert des PDADMA-Molekulargewichts wird (Nlin = 15 Doppelschichten und dBL = (12,3 ± 1,3) nm). Die Daten legen nahe, dass unterhalb des PDADMA-Schwellwerts lediglich ein Teil einer PDADMA-Kette auf der PSS-terminierten Multischicht adsorbiert und der restliche Teil der adsorbierten Kette in Lösung ragt. Oberhalb des PDADMA-Schwellwertes adsorbiert mindestens noch ein zweiter Abschnitt der Kette und es ragt mindestens ein loop in Lösung. Dies führt zu einer konstanten Gleichgewichtsdicke der Monoschicht unabhängig vom Molekulargewicht. Unterschreitet das PSS-Molekulargewicht den Schwellwert Mw(PSS) = 25 kDa, so beobachtet man den gegenteiligen Effekt: beide Wachstumsparameter Nlin und dBL nehmen deutlich zu. Die größten gemessene Werte (unter Verwendung von 8,6 kDa PSS) lauten Nlin = 33 und dBL = 28,7 nm. Neutronenreflektionsmessungen zeigen, dass dieser Effekt mit der Diffusion der kurzen PSS-Ketten innerhalb der Multischicht einhergeht. Die Ausdehnung der Diffusionszone von 8,6 kDa PSS beträgt 80 nm und nimmt bis zum Erreichen des PSS-Schwellwertes monoton mit Mw(PSS) ab. Im Gegensatz dazu bilden PSS-Ketten mit einem Molekulargewicht oberhalb des Schwellwertes klar lokalisierte, lateral homogene Schichten (mit einer Grenzflächenunschärfe von 2 ... 4,6 nm). Entgegen der intuitiven Erwartung hat eine höhere Adsorptionszeit keinen Einfluss auf die Diffusionszone. Der limitierende Faktor ist die Diffusionszone selbst. In Übereinstimmung mit der theoretischen Erwartung führt die Diffusion von kurzen PSS-Ketten während der Multischicht-Präparation zu einem exponentiellen Wachstum der PDADMA/PSS-Multischichten, sobald Mw(PSS) < 25 kDa. In diesem Fall durchläuft das Schichtwachstum nacheinander erst ein exponentielles, dann ein parabolisches und schließlich ein lineares Regime.
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.
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.
The confinement of energy has always been a challenge in magnetic confinement fusion devices. Due to their toroidal shape there exist regions of high and low magnetic field, so that the particles are divided into two classes - trapped ones that are periodically reflected in regions of high magnetic field with a characteristic frequency, and passing particles, whose parallel velocity is high enough that they largely follow a magnetic field line around the torus without being reflected. The radial drift that a particle experiences due to the field inhomogeneity depends strongly on its position, and the net drift therefore depends on the path taken by the particle. While the radial drift is close to zero for passing particles, trapped particles experience a finite radial net drift and are therefore lost in classical stellarators. These losses are described by the so-called neoclassical transport theory. Recent optimised stellarator geometries, however, in which the trapped particles precess around the torus poloidally and do not experience any net drift, promise to reduce the neoclassical transport down to the level of tokamaks. In these optimised stellarators, the neoclassical transport becomes small enough so that turbulent transport may limit the confinement instead. The turbulence is driven by small-scale-instabilities, which tap the free energy of density or temperature gradients in the plasma. Some of these instabilities are driven by the trapped particles and therefore depend strongly on the magnetic geometry, so the question arises how the optimisation affects the stability. In this thesis, collisionless electrostatic microinstabilities are studied both analytically and numerically. Magnetic configurations where the action integral of trapped-particle bounce motion, J, only depends on the radial position in the plasma and where its maximum is in the plasma centre, so-called maximum-J configurations, are of special interest. This condition can be achieved approximately in quasi-isodynamic stellarators, for example Wendelstein 7-X. In such configurations the precessional drift of the trapped particles is in the opposite direction from the direction of propagation of drift waves. Instabilities that are driven by the trapped particles usually rely on a resonance between these two frequencies. Here it is shown analytically by analysing the electrostatic energy transfer between the particles and the instability that, thanks to the absence of the resonance, a particle species draws energy from the mode if the frequency of the mode is well below the charateristic bounce frequency. Due to the low electron mass and the fast bounce motion, electrons are almost always found to be stabilising. Most of the trapped-particle instabilities are therefore predicted to be absent in maximum- J configurations in large parts of parameter space. Analytical theory thus predicts enhanced linear stability of trapped-particle modes in quasi-isodynamic stellarators compared with tokamaks. Moreover, since the electrons are expected to be stabilising, or at least less destabilising, for all instabilities whose frequency lies below the trapped-electron bounce frequency, other modes might benefit from the enhanced stability as well. In reality, however, stellarators are never perfectly quasi-isodynamic, and the question thus arises whether they still benefit from enhanced stability. Here the stability properties of Wendelstein 7-X and a more quasi-isodynamic configuration, QIPC, are investigated numerically and compared with another, non-quasiisodynamic stellarator, the National Compact Stellarator Experiment (NCSX) and a typical tokamak. In gyrokinetic simulations, performed with the gyrokinetic code GENE in the electrostatic and collisionless approximation, several microinstabilities, driven by the density as well as both ion and electron temperature gradients, are studied. Wendelstein 7-X and QIPC exhibit significantly reduced growth rates for all simulations that include kinetic electrons, and the latter are indeed found to be stabilising when the electrostatic energy transfer is analysed. In contrast, if only the ions are treated kinetically but the electrons are taken to be in thermodynamic equilibrium, no such stabilising effect is observed. These results suggest that imperfectly optimised stellarators can retain most of the stabilising properties predicted for perfect maximum-J configurations. Quasi-isodynamic stellarators, in addition to having reduced neoclassical transport, might therefore also show reduced turbulent transport, at least in certain regions of parameter space.
We present a Green's function based treatment of the effects of electron-phonon coupling on transport through a molecular quantum dot in the quantum limit. Thereby we combine an incomplete variational Lang-Firsov approach with a perturbative calculation of the electron-phonon self energy in the framework of generalised Matsubara Green functions and a Landauer-type transport description. Calculating the ground-state energy, the dot single-particle spectral function and the linear conductance at finite carrier density, we study the low-temperature transport properties of the vibrating quantum dot sandwiched between metallic leads in the whole electron-phonon coupling strength regime. We discuss corrections to the concept of an anti-adiabatic dot polaron and show how a deformable quantum dot can act as a molecular switch.
Synopsis
C+60 has been proposed to be responsible for two of the diffuse interstellar bands (DIBs), the absorption features observed in the visible-to-near-infrared spectra of the interstellar medium. However, a confirmation requires laboratory gas-phase spectra, which are so far not available. We plan to develop a novel spectroscopy technique that will allow us to obtain the first gas-phase spectra of C+60, and that will be applicable to other complex organic molecules such as polycyclic aromatic hydrocarbons. The current status of the experimental setup, the ideas behind the measurement scheme and the preparatory work toward its implementation will be presented.
Experience in the construction of optimized stellarators shows the coil system is a significant challenge. The precision necessary allow the generation of accurate flux surfaces in recent experiments affected both cost and schedule negatively. Moreover, recent experiments at Wendelstein 7-X have shown that small field corrections were necessary for the operation of specific desired magnetic configurations. Therefore, robust magnetic configurations in terms of coil geometry and assembly tolerances have a high potential to facilitate swifter and less expensive construction of future, optimized stellarators. We present a new coil optimization technique that is designed to seek out coil configurations that are resilient against 3D coil displacements. This stochastic version of stellarator coil optimization uses the sampling average approach to incorporate an iterative perturbation analysis into the optimization routine. The result is a robust magnetic configuration that simultaneously reproduces the target magnetic field more accurately and leads to a better fusion performing coil configuration.
A novel method for time-resolved tuned diode laser absorption spectroscopy has been developed. In this paper, we describe in detail developed electronic module that controls time-resolution of laser absorption spectroscopy system. The TTL signal triggering plasma pulse is used for generation of two signals: the first one triggers the fine tuning of laser wavelength and second one controls time-defined signal sampling from absorption detector. The described method and electronic system enable us to investigate temporal evolution of sputtered particles in technological low-temperature plasma systems. The pulsed DC planar magnetron sputtering system has been used to verify this method. The 2" in diameter titanium target was sputtered in pure argon atmosphere. The working pressure was held at 2 Pa. All the experiments were carried out for pulse ON time fixed at 100 (is. When changing OFF time the discharge has operated between High Power Impulse Magnetron Sputtering regime and pulsed DC magnetron regime. The effect of duty cycle variation results in decrease of titanium atom density during ON time while length of OFF time elongates. We believe that observed effect is connected with higher degree of ionization of sputtered particles. As previously reported by Bohlmark et al., the measured optical emission spectra in HiPIMS systems were dominated by emission from titanium ions [1].
Abstract
Reactive high power impulse magnetron sputtering (HiPIMS) of a cobalt cathode in pure argon gas and with different oxygen admixtures was investigated by time-resolved optical emission spectroscopy (OES) and time-integrated energy-resolved mass spectrometry. The HiPIMS discharge was operated with a bipolar pulsed power supply capable of providing a large negative voltage with a typical pulse width of 100 μs followed by a long positive pulse with a pulse width of about 350 μs. The HiPIMS plasma in pure argon is dominated by Co+ ions. With the addition of oxygen, O+ ions become the second most prominent positive ion species. OES reveals the presence of Ar I, Co I, O I, and Ar II emission lines. The transition from an Ar+ to a Co+ ion sputtering discharge is inferred from time-resolved OES. The enhanced intensity of excited Ar+* ions is explained by simultaneous excitation and ionisation induced by energetic secondary electrons from the cathode. The intensity of violet Ar I lines is drastically reduced during HiPIMS. Intensity of near-infrared Ar I lines resumes during the positive pulse indicating an additional heating mechanism.
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'.
This thesis is devoted to experiments on three-dimensional dust clouds which are confined in low temperature plasmas. Such ensembles of highly electrically charged micrometer-sized particles reveal fascinating physics, such as self-excited density waves and vortices. At the same time, these systems are challenging for experimental approaches due to their three-dimensional character. In this thesis, new optical diagnostics for dusty plasmas have been developed and, in combination with existing techniques, have been used to study these 3D dusty plasmas on different size and time scales.
Ausgangspunkt aller Untersuchungen sind Langmuir-Monoschichten an der Wasser/Luftgrenzfläche. Denn mit diesen Monoschichten kann die Oberflächeladungsdichte eingestellt werden. Sie werden durch amphiphile Moleküle gebildet.Die hydrophoben Alkylketten sind zur Luftseite und die hydrophile Kopfgruppe zur Wasserseite orientiert.Die Phasen der Lipid- Monoschicht und die Belegungsdichte werden extern eingestellt. Die Lipid- Monoschicht kann je nach Anordnung der Alkylketten verschiedene unter- schiedliche Phasen zeigen. Um die adsorbierten Polyelekrolyte zu beschreiben zu können, benötigt man experimentelle Methoden, die in der Lage sind, Konformation und Be- legungsdichte von adsorbierten Polyelektrolyten an Oberflächen aufzulösen. Diese Strukturen, auf der Nanometerskala, werden mit Röntgenreflektion und Röntgendiffraktion unter streifendem Einfall untersucht.Die Strukturda- ten werden durch thermodynamische Untersuchungen ergänzt. Die Untersuchungen werden für elektrostatische Kräfte mit hoher Ampli- tude und langer Reichweite durchgeführt. Die Lösungen der Polyelektrolyte (c PSS = 0.01 mmol/L bezogen auf die Monomerkonzentration) sind so einge- stellt, dass eine fast vollständige Ladungskompensation (70-90%) stattfindet. Unter diesen Bedingungen adsorbieren PE entweder flach als 2-dimensionales Knäuel oder geordnet in einer 2-dimensionalen lamellaren Phase. Die Untersuchungen sollen herausfinden, welchen Einfluss die elektrostatische Wechselwirkung auf die Kettensteifigkeit von adsorbierten Polyelektrolyten,die durch die Persistenzlänge LP charakterisiert werden.So kann geklärt werden,ab welcher Konturlänge LK Polyelektrolyte nicht mehr stäbchenförmig sondern als 2-dimensionales Knäuel adsorbieren. Untersucht werden negativ geladene PSS (Polystyron Sulfonat) mit un- terschiedlichen Konturlängen LK.Diese adsorbieren an die positiv geladene DODA Lipid-Monoschicht (Dioctadeyldimethylammonium). Die Persistenzlänge LP für adsorbiertes PSS an DODA ist direkt aus den thermodynamischen Daten ermittelt worden. Als Funktion der Konturlänge LK wurde der Oberflächendruck π c sowie die erste Ableitung dπc /dT unter- sucht. Daraus läßt sich die Persistenzlänge des adsorbierten PSS LP ≈ 210 Å bestimmen. Die Oberflächenladungsdichte der Monoschicht wird durch die Kompression verdoppelt.Simultan wird der Abstand der Polyelektrolytketten dPE halbiert, so dass immer eine 70-90% Ladungskompensation erreicht wird. Es wird mit Röntgendiffraktion immer eine fache 2-dimensionale lamellare Phase der adsorbierten PSS Ketten detektiert.Hierbei bilden Konturlängen LK < 110 Å eine Ausnahme. Es wird keine 2-dimensionale lamellare Phase für geringe Oberflächenladungsdichte (LE Phase der Lipide) gefunden. Die Röntgenreflektion kann aber zeigen, dass PSS Ketten, unabhängig von der Konturlänge LK, immer flach an der Lipidmonoschicht adsorbieren. Wenn steife kurze Ketten (LK≤110Å<LP ) an der LC Phase der Lipid- Monoschicht adsorbieren, liegen sie aber in der 2-dimensionalen lamellare Phase. Der Übergang von der LE in die LC Phase der Lipid-Monoschichten erfolgt gleichzeitig mit dem Übergang von der ungeordneten flachen zur 2- dimensionalen lamellare Phase der adsorbierten kurzen PSS Ketten. Daher zeigt die Enthalpie ∆H des LE/LC Phasenübergangs ein Maximum bei L K =110 Å. Im nächsten Schritt wird die Elektrostatik zwischen der Lipid-Monoschicht und den Polyelektrolyte untersucht.Die maximale Oberflächenladungsdichte der Lipid-Monoschicht wird durch eine Mischung von geladenen DODA und ungeladenen DPPC (Dipalmitoylphosphatidylcholine) eingestellt. Röntgendiffraktionsmessungen zeigen bis zu einem DODA-Anteil von 75% die Ausbildung einer 2-dimensionalen lamellaren Phase an der LC Phase der Lipid-Monoschicht. Nimmt die maximale Oberflächenladungsdichte weiter ab, so wird keine Bildung der 2-dimensionalen lamellaren Phase beobachtet. Die Abnahme der maximalen Oberflächenladung führt zu einer niedrigen Belegungsdichte und so zu einem größerem Kettenabstand dPE. Die Linienladungsdichte wird durch unterschiedliches P−TrisAAx−rand−AMPS1−x auf 90% oder 50% verringert. Röntgendiffraktionsmessungen an PE mit unterschiedlichen Linienladungsdichten zeigen auch hier eine 2-dimensionale lamellare Phase. Die verringerte Linienladungsdichte erzwingt eine höhere Belegungsdichte um eine 70-90% Ladungskompensation zu erreichen. Dieses führt zu einem kleineren Kettenabstand dPE. Ein Grenzfall ist bei einer 50%-igen Linienladungsdichte zu beobachten. Dort konnte an der LC Phase der Lipid-Monoschicht keine 2-dimensionale lamellare Phase der PE beobachtet werden. Der Kettenabstand dPE ist so gering, dass er mit der Röntgendiffraktion nicht mehr aufgelöst werden kann.
In this thesis, I was able to provide answers to transport processes in lipid monolayers, which are ultimately, all of biological relevance. In particular, I was interested in lipid oxidation and dynamic compression/expansion processes of surfactant monolayers at the air-water interface:
Lipid oxidation was shown to be a consequence of the formation of a high concentration of reactive oxygen species (ROS) during cell respiration, which finally can lead to severe cell damage. It is not yet understood clearly, which part of the lipid molecules is especially prone to a ROS attack. I was particularly interested in the role of the double bonds of the acyl chains of the lipid molecules during oxidation. Further, I wanted to know the time scales of lipid interaction with the ROS.
Compared to lipid vesicles, lipid monolayers have the advantage that many parameters of the system can be adjusted easily. In our system, I made use of this by setting the lateral pressure to low values during H2O2 treatment, which facilitated the ROS to reach the double bonds in the acyl chains.
A prime example of biological systems out of thermal equilibrium was given in the alveolus surface, which is covered with a surfactant monolayer. During breathing, these monolayers undergo such a highly dynamic compression and expansion. Arising flows from breathing could disrupt a film and consequently, it would lose its protective role. One of my goals was to understand flows and their influence on domain shape. Dependent on the strength of the flows, I expected different growth regimes, with differing prevailing transport processes. Once understanding the underlying mechanisms in domain shaping would allow me to draw conclusions on biological systems.
In order to address these questions, I established two systems, both based on the compression of lipid monolayers. I used isotherms to study the phase behavior of the lipids:9 During compression, the lipids can undergo phase transitions from the gaseous phase to the liquid expanded phase (LE-phase) and further from the LE-phase to the liquid condensed phase (LC-phase). A coexistence regime is observed in between the LE-phase and the LC-phase, characterized by a flat increase of lateral pressure with decreasing molecular area. Some lipids exhibited LC-phase domains. These were further investigated with Brewster angle microscopy (BAM). The used BAM was equipped with an integrated Scheimpflug optics, enabling an overall focused image plane. Furthermore, time-resolved observation of the growth of the domains was possible by recording videos (20 frames per seconds).
The first system enabled the investigation of lipid peroxidation, when the lipids were exposed to ROS. I chose DMPC, POPC, DOPC and PLPC, since these are phospholipids differing in the number and position of double bonds in acyl chains, but not in the head group. I used a H2O2 enriched phosphate buffered saline (PBS) solution, which served as a precursor for more reactive ROS, like hydroxyls (.OH). PBS was chosen, since it resembles the cell environment best. During defined waiting times of H2O2 treatment, the ROS diffused vertically from the subphase towards the monolayer. The lipid molecules were in the LE-phase, which facilitated the ROS molecules to reach also the double bonds of the acyl chains. The oxidized monolayers were then compressed at constant compression speed. Since the corresponding isotherms could be measured with high precision, the relative area increase δA/A between oxidized and non-oxidized monolayer along the isotherm proved to be a good measure for lipid peroxidation. The area increase δA in the molecular area of the oxidized molecules was explained by the eventually added, more hydrophilic −OOH group at the position of a carbon atom adjacent to a double bond in the unsaturated acyl chain. The −OOH group is drawn to the hydrophilic head group of the lipid. This leads to a kink in the acyl chain, which increases the molecular area A by δA. A model, which explained this peroxidation process in lipid vesicles, could be adopted to monolayers.
I compared the oxidation of phospholipids, differing in the number and position of the double bonds of their acyl chains. I found that δA/A increased with the growing number of double bonds in one acyl chain. However, a comparison of DOPC with POPC also showed the importance of the position of the acyl chain. I determined a slow reaction kinetic. It could be estimated by a √t dependence of the number density N_surface, which denominates the ROS sticking on the monolayer. The transport of ROS towards the monolayer was found to be diffusive, because it was the slowest process in the reaction. This interpretation was reinforced by a comparison of the temperature dependence of the relative area increase δA/A with the Stokes-Einstein diffusion coefficient of water molecules. The initial ROS concentration c_0 in the trough could be traced back (c_0~ 50 nM), which is indeed a realistic value found in human cells.
Concluding, our results can be understood as a feasibility study. The complexity of the monolayer can be arbitrarily increased, for example by the addition of proteins, allowing the investigation of other oxidative processes occurring in the cell membrane.
The second system allowed the investigation of growth of LC domains during fast compression processes of monolayers. I chose erucic acid monolayers, due to its low line tension and a continuous nucleation phase, enabling the formation of fractal domains. The monolayers were investigated with isotherms and BAM videos. Since v_C (compression speed of the monolayer) was continuous over the whole compression time, I had a system with well-defined hydrodynamic conditions. This allowed me a complete analysis of the system, starting with descriptive features of the observed domains to a classification of the observed growth regimes by means of hydrodynamic theory, through to the distinction and quantification of different kind of flows and supersaturations, involving Ivantsov theory:
Dependent on the compression speed v_C, I observed seaweed or dendritic domains. The LE/LC phase transition pressure pi_t was slightly increased compared to pi_inf of the equilibrium isotherm. A high compression speed v_C induced a supersaturation Δc. I introduced the excess lateral pressure Δpi=pi-pi_inf as an appropriate quantity to describe the supersaturation Δc. I showed a linear behavior of Δc on Δpi. Δc is a macroscopic quantity since it is averaged over the whole monolayer area. I characterized the domains of the seaweed and dendritic regime with respect to tip radii, branch lengths, side branch separations and fractal dimensions. I calculated the growth speed of the main branches. A roughly doubling of the growth speed of dendritic domains, compared to seaweed domains was observed. This was an evidence of adjunctive (Marangoni) flow in the subphase.
For each monolayer, I observed drifts during domain growth, which I explained by an anisotropy in the LE-phase, caused by the continuous nucleation of the domains. These kind of surface flows were superimposed to bulk flows in the subphase. Since I had a well established system, I could analyze the influence of these surface flows on domain shape, in terms of magnitude, direction and duration of the surface flows. I therefore used FFT spectra and directionality histograms. At low flows, the FFT showed six-fold symmetry. Higher drifts exhibited incisions in the FFT, eventually leading to dumbbell shaped FFTs at very high drifts. The domains grew preferentially in the direction parallel to the incision.
I used directionality histograms to analyze the angular distribution of the growing domains. They showed that the drift direction always correlated with a minimum in the histogram. In order to analyze drift duration, I split the domain in downstream and upstream side. I could show that for small drift durations, downstream growth was preferred. However, for longer drift durations, the flows got more isotropic and consequently growth was more balanced then.
I could observe only a weak correlation between drift velocity v_D and compression speed v_C. However, dendrites were formed when the compression speed v_C was high, while seaweed domains were formed when v_C was small. Domain distortion occurred in the same way, independent if seaweed or dendritic domains were considered. I further showed that hydrodynamic flows in the subphase and surface flows are superimposed and scale differently. Consequently, they have different impact on domain shape: hydrodynamic flows act on μm scale and influence the domain morphology (distance between side branches, and tip radius) and the growth speed of the main branches. Surface flows act on the mm to cm scale, cause an anisotropic flow in the LE phase surrounding the domain, and thus affect the overall domain shape.
The anisotropy in the LE-phase led to a locally different degree of supersaturation. To take this into account, I introduced a local normalized supersaturation Δ, based on the Ivantsov solution. Therefore, I calculated Péclet numbers p of measured quantities of the system. I obtained values of 0.88 ≤Δ≤0.90 for the seaweed regime (p<5) and 0.93 ≤Δ≤0.96 for the dendritic regime (p>6). Since the Ivantsov solution can only be applied for purely diffusive processes, I applied a modified Ivantsov solution Δ_mod, which calculates Δ at a distance 𝛿 ahead of the dendrite tip. I was able to determine the progression of the diffusive layer 𝛿, however a quantitative determination failed.
Applying hydrodynamic theory allowed me to classify the two growth regimes with respect to the Boussinesq number Bq. Since for both growth regimes, I achieved values of Bq<1, bulk viscous losses dominated over surface viscous losses. Further, a cross-over length 𝜉 was calculated, from which one can distinguish, whether advective transport dominates over diffusion.
I further connected the two defined supersaturations Δ and Δc via the excess lateral pressure Δpi. From this, I saw differences in the seaweed and dendritic growth regimes: The local normalized supersaturation Δ of seaweed growth seemed to be quite stable for a further increase of the lateral excess pressure Δpi, whereas it reacted quite sensitive in the dendritic regime. This was found to be an indication of a non-equilibrium regime, caused by the strong coupling of the monolayer to the subphase. It reinforces therefore the theory of Marangoni-flow.
The findings of this thesis emphasize the importance of understanding highly dynamic compression/expansion processes arising in surfactant monolayers. Using the example of the compression of the alveolus surface, it can be seen that a more realistic model of the pulmonary alveolus is not only enabled by increasing the complexity of the surfactant monolayer (e.g. by adding specific proteins or lipid mixtures to the monolayer). Equally important is the understanding in transport processes and the consequences for the monolayer structure. By the analysis of domain shapes, I presented a method, which is suitable for such a study.
The first Therapeutic ROS and Immunity in Cancer (TRIC) meeting was organized by the excellence research center ZIK plasmatis (with its previous Frontiers in Redox Biochemistry and Medicine (FiRBaM) and Young Professionals’ Workshop in Plasma Medicine (YPWPM) workshop series in Northern Germany) and the excellence research program ONKOTHER-H (Rostock/Greifswald, Germany). The meeting showcased cutting-edge research and liberated discussions on the application of therapeutic ROS and immunology in cancer treatment, primarily focusing on gas plasma technology. The 2-day hybrid meeting took place in Greifswald and online from 15–16 July 2021, facilitating a wide range of participants totaling 66 scientists from 12 countries and 5 continents. The meeting aimed at bringing together researchers from a variety of disciplines, including chemists, biochemists, biologists, engineers, immunologists, physicists, and physicians for interdisciplinary discussions on using therapeutic ROS and medical gas plasma technology in cancer therapy with the four main sessions: “Plasma, Cancer, Immunity”, “Plasma combination therapies”, “Plasma risk assessment and patients studies”, and “Plasma mechanisms and treated liquids in cancer”. This conference report outlines the abstracts of attending scientists submitted to this meeting.
In the present work, a time- and radial-dependent fluid model has been developed to describe the glow-to-arc transition of the positive column in the course of constriction. The self-consistent model comprises the particle balance equations for the relevant species, the balance equation of the mean electron energy and the heavy particle temperature in the plasma, the Poisson equation for the space-charge potential, and a current balance determining the axial electric field. The model adopts the nonlocal moment method, i.e., the system of the balance equations resulting from the moments of the radially dependent Boltzmann equation is solved. The electron transport and rate coefficients are adapted as functions of the mean energy of the electrons, the gas temperature and the ionization degree. The model is applied to a description of the constriction of the dc positive column in argon, for a wide range of pressures and applied currents. Pronounced nonlocal features of the mean electron energy balance are found and their influence on the constricted argon positive column is analyzed. Different assumptions concerning the electron velocity distribution function (EVDF) have been considered in the present model. The assumption of a Maxwellian distribution for the electrons was found to be inappropriate, while the assumption of a Druyvesteyn distribution for the electrons was found to be suitable for describing qualitatively the glow-to-arc transition. However, the standard model using the EVDF obtained from the solution of the steady-state, spatially homogeneous electron Boltzmann equation including electron-electron collisions allows to describe the constriction effect and provides best agreement with experimental data and other available modelling results. The fluid model has also been used to study a medium-pressure pulsed positive column in xenon at conditions of the contracted discharge. The simulation results provide a detailed insight in the physical mechanisms of xenon discharges in pulsed mode. The stepwise ionization of the excited atoms, the conversion of the atomic ions into molecular ions as well as the dissociative recombination of the molecular ions are found to be the most important processes for the pulsed positive column in xenon plasmas at conditions of the contracted discharge. The comparison of the model predictions with experimental results generally shows good agreement. In particular, the model predictions are suitable for qualitative reproduction of the significant increase of low-lying atomic levels densities as well as of the higher and of the relaxed lowest vibrational states of the Xe2* excimers in the afterglow phase of the pulse.
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.
AbstractThe efficient operation of a tokamak is limited by several constraints, such as the transition to high confinement or the density limits occurring in both confinement regimes. These particular boundaries of operation are derived in terms of a combination of dimensionless parameters describing interchange-drift-Alfvén turbulence without any free adjustable parameter. The derived boundaries describe the operational space at the separatrix of the ASDEX Upgrade tokamak, which is presented in terms of an electron density and temperature existence diagram. The derived density limits are compared against Greenwald scaling. The power threshold and role of ion heat flux for the transition to high confinement are discussed.
This thesis highlights the impact of surface charges and negative ions on the pre-ionization, breakdown mechanism, and lateral structure of dielectric barrier discharges operated in binary mixtures of helium with nitrogen or electronegative oxygen. Sophisticated diagnostic methods, e.g., non-invasive optical emission spectroscopy and the electro-optic Pockels effect as well as invasive laser photodetachment and laser photodesorption, were applied at one plane-parallel discharge configuration to investigate both relevant volume and surface processes. Moreover, the experimental findings were supported by numerical fluid simulations of the discharge. For the first time, the memory effect of the measured surface charge distribution was quantified and its impact on the local self-stabilization of discharge filaments was pointed out. As well, it turned out that a few additional seed electrons, either desorbed from the charged dielectric surface or detached from negative ions in the volume, significantly contribute to the pre-ionization resulting in a reduced voltage necessary for discharge breakdown. Finally, effective secondary electron emission coefficients of different dielectrics were estimated from the measured breakdown voltage using an analytical model.
In future fusion reactors disruptions must be avoided at all costs. Disruptions due to the density limit (DL) are typically described by the power-independent Greenwald scaling. Recently, a power dependence of the disruptive DL was predicted by several authors (Zanca et al 2019 Nucl. Fusion 59 126011; Giacomin et al 2022 Phys. Rev. Lett. 128 185003; Singh and Diamond 2022 Plasma Phys. Control. Fusion 64 084004; Stroth et al 2022 Nucl. Fusion 62 076008; Brown and Goldston 2021 Nucl. Mater. Energy 27 101002). It is investigated whether this increases the operational range of the tokamak. Increasing the heating power in the L-mode can induce an L-H transition, and therefore a power-dependent DL and the L-H transition cannot be considered independently. The different models are tested on a data base for separatrix parameters at the separatrix of ASDEX Upgrade and compared with the concept (SepOS) presented in Eich and Manz (2021 Nucl. Fusion 61 086017). The disruptive separatrix density scales with the power ne ∝ P0.38±0.08 in good agreement to all models. Also the back transition from high to low (H-L) confinement shows an approximately Greenwald scaling with an additional power dependence ne ∝ P0.4 according to the SepOS concept. For future devices operating at much higher heating power such a power scaling may allow operation at much higher separatrix densities than are common in H-mode operation. Preconditions to extrapolation for future devices are discussed.
The heaviest actinide elements are only accessible in accelerator-based experiments on a one-atom-at-a-time level. Usually, fusion–evaporation reactions are applied to reach these elements. However, access to the neutron-rich isotopes is limited. An alternative reaction mechanism to fusion–evaporation is multinucleon transfer, which features higher cross-sections. The main drawback of this technique is the wide angular distribution of the transfer products, which makes it challenging to catch and prepare them for precision measurements. To overcome this obstacle, we are building the NEXT experiment: a solenoid magnet is used to separate the different transfer products and to focus those of interest into a gas-catcher, where they are slowed down. From the gas-catcher, the ions are transferred and bunched by a stacked-ring ion guide into a multi-reflection time-of-flight mass spectrometer (MR-ToF MS). The MR-ToF MS provides isobaric separation and allows for precision mass measurements. In this article, we will give an overview of the NEXT experiment and its perspectives for future actinide research.
This work describes the recent scientific and technical achievements obtained at the high-precision Penning trap mass spectrometer SHIPTRAP. The scientific focus of the SHIPTRAP experiment are mass measurements of short-lived nuclides with proton number larger than 100. The masses of these isotopes are usually determined via extrapolations, systematic trends, predictions based on theoretical models or alpha-decay spectroscopy. In several experiments the masses of the isotopes 252-255No and 255,256Lr have been measured directly. With the obtained results the region of enhanced nuclear stability at the deformed shell closure at the neutron number 152 was investigated. Furthermore, the masses have been used to benchmark theoretical mass models. The measured masses were compared selected mass models which revealed differences between few keV/c² up to several MeV/c² depending on the investigated nuclide and model. In order to perform mass measurements on superheavy nuclei with lower production rates, the efficiency of the SHIPTRAP setup needs to be increased. Currently, the efficiency is 2% and mainly limited by the stopping- and extraction efficiency of the buffer gas cell. The stopping and extraction efficiency of the current buffer gas cell is 12%. To this end, a modified version of the buffer gas cell was developed and characterized with 223Ra ion source. Besides a larger stopping volume and a coaxial injection the new buffer gas cell is operated at a temperature of 40K. The operation at cryogenic temperatures increases the cleanliness of the buffer gas. From extraction measurements and simulations an overall efficiency of 62(3)% was determined which results in an increase by a factor of 5 in comparison to the current buffer gas cell. Aside from high-precision mass measurements of heavy radionuclides the mass differences of metastable isobars was measured to identify candidates for the neutrinoless double-electron capture. Neutrinoless double-electron capture can only occur if the neutrino is its own antiparticle and a physics beyond the standard model exists since the neutrinoless double-electron capture violates the conservation of the lepton number. Due to its expected long half-life this decay has not yet been observed. However, the decay rate is resonantly enhanced if mother and daughter nuclide are degenerate in energy. Suitable candidates for the search of the neutrinoless double-electron capture have been identified with mass difference measurements uncertainties of about 100eV/c². In this work the results of the mass difference measurements of 12 possible candidates are presented.
Abstract
The laser photodetachment experiment in a diffuse helium–oxygen barrier discharge is evaluated by a 1D fluid simulation. As in the experiment, the simulated discharge operates in helium with
400
ppm
oxygen admixture at
500
mbar
inside a discharge gap of
3
mm
. The laser photodetachment is included by the interaction of negative ions with a temporally and spatially dependent photon flux. The simulation with the usually applied set of reactions and rate coefficients provides a much lower negative ion density than needed to explain the impact on the discharge characteristics in the experiment. Further processes for an enhanced negative ion formation and their capabilities of reproducing the experimental results are discussed. These further processes are additional attachment processes in the volume and the negative ion formation at the negatively charged dielectric. Both approaches are able to reproduce the measured laser photodetachment effect partially, but the best agreement with the experimental results is achieved with the formation of negative ions at the negatively charged dielectric.
Abstract
Based on the analysis of electron density Ne profiles (Grahamstown ionosonde), a case study of the height‐dependent ionospheric response to two 27‐day solar rotation periods in 2019 is performed. A well‐defined sinusoidal response is observed for the period from 27 April 2019 to 24 May 2019 and reproduced with a Thermosphere‐Ionosphere‐Electrodynamics General Circulation Model simulation. The occurring differences between model and observations as well as the driving physical and chemical processes are discussed based on the height‐dependent variations of Ne and major species. Further simulations with an artificial noise free sinusoidal solar flux input show that the Ne delay is defined by contributions due to accumulation of O+ at the Ne peak (positive delay) and continuous loss of O2+ ${\mathrm{O}}_{2}^{+}$ in the lower ionosphere (negative delay). The neutral parts' 27‐day signatures show stronger phase shifts. The time‐dependent and height‐dependent impact of the processes responsible for the delayed ionospheric response can therefore be described by a joint analysis of the neutral and ionized parts. The return to the initial ionospheric state (and thus the loss of the accumulated O+) is driven by an increase of downward transport in the second half of the 27‐day solar rotation period. For this reason, the neutral vertical winds (upwards and downwards) and their different height‐dependent 27‐day signatures are discussed. Finally, the importance of a wavelength‐dependent analysis, statistical methods (superposed epoch analysis), and coupling with the middle atmosphere is discussed to outline steps for future analysis.
This study evaluated the impact of a defined plasma treated water (PTW) when applied to various stages within fresh-cut endive processing. The quality characteristic responses were investigated to establish the impact of the PTW unit processes and where PTW may be optimally applied in a model process line to retain or improve produce quality. Different stages of application of PTW within the washing process were investigated and compared to tap water and chlorine dioxide. Fresh-cut endive (Cichorium endivia L.) samples were analyzed for retention of food quality characteristics. Measurements included color, texture, and nitrate quantification. Effects on tissue surface and cell organelles were observed through scanning electron and atomic force microscopy. Overall, the endive quality characteristics were retained by incorporating PTW in the washing process. Furthermore, promising results for color and texture characteristics were observed, which were supported by the microscopic assays of the vegetal tissue. While ion chromatography detected high concentrations of nitrite and nitrate in PTW, these did not affect the nitrate concentration of the lettuce tissue post-processing and were below the concentrations within EU regulations. These results provide a pathway to scale up the industrial application of PTW to improve and retain quality characteristic retention of fresh leafy products, whilst also harnessing the plasma functionalized water as a process intervention for reducing microbial load at multiple points, whether on the food surface, within the process water or on food-processing surfaces.
AbstractThe 2022 Roadmap is the next update in the series of Plasma Roadmaps published by Journal of Physics D with the intent to identify important outstanding challenges in the field of low-temperature plasma (LTP) physics and technology. The format of the Roadmap is the same as the previous Roadmaps representing the visions of 41 leading experts representing 21 countries and five continents in the various sub-fields of LTP science and technology. In recognition of the evolution in the field, several new topics have been introduced or given more prominence. These new topics and emphasis highlight increased interests in plasma-enabled additive manufacturing, soft materials, electrification of chemical conversions, plasma propulsion, extreme plasma regimes, plasmas in hypersonics, data-driven plasma science and technology and the contribution of LTP to combat COVID-19. In the last few decades, LTP science and technology has made a tremendously positive impact on our society. It is our hope that this roadmap will help continue this excellent track record over the next 5–10 years.
AbstractMagneto-optical (MO) effects, viz. magnetically induced changes in light intensity or polarization upon reflection from or transmission through a magnetic sample, were discovered over a century and a half ago. Initially they played a crucially relevant role in unveiling the fundamentals of electromagnetism and quantum mechanics. A more broad-based relevance and wide-spread use of MO methods, however, remained quite limited until the 1960s due to a lack of suitable, reliable and easy-to-operate light sources. The advent of Laser technology and the availability of other novel light sources led to an enormous expansion of MO measurement techniques and applications that continues to this day (see section 1). The here-assembled roadmap article is intended to provide a meaningful survey over many of the most relevant recent developments, advances, and emerging research directions in a rather condensed form, so that readers can easily access a significant overview about this very dynamic research field. While light source technology and other experimental developments were crucial in the establishment of today’s magneto-optics, progress also relies on an ever-increasing theoretical understanding of MO effects from a quantum mechanical perspective (see section 2), as well as using electromagnetic theory and modelling approaches (see section 3) to enable quantitatively reliable predictions for ever more complex materials, metamaterials, and device geometries. The latest advances in established MO methodologies and especially the utilization of the MO Kerr effect (MOKE) are presented in sections 4 (MOKE spectroscopy), 5 (higher order MOKE effects), 6 (MOKE microscopy), 8 (high sensitivity MOKE), 9 (generalized MO ellipsometry), and 20 (Cotton–Mouton effect in two-dimensional materials). In addition, MO effects are now being investigated and utilized in spectral ranges, to which they originally seemed completely foreign, as those of synchrotron radiation x-rays (see section 14 on three-dimensional magnetic characterization and section 16 on light beams carrying orbital angular momentum) and, very recently, the terahertz (THz) regime (see section 18 on THz MOKE and section 19 on THz ellipsometry for electron paramagnetic resonance detection). Magneto-optics also demonstrates its strength in a unique way when combined with femtosecond laser pulses (see section 10 on ultrafast MOKE and section 15 on magneto-optics using x-ray free electron lasers), facilitating the very active field of time-resolved MO spectroscopy that enables investigations of phenomena like spin relaxation of non-equilibrium photoexcited carriers, transient modifications of ferromagnetic order, and photo-induced dynamic phase transitions, to name a few. Recent progress in nanoscience and nanotechnology, which is intimately linked to the achieved impressive ability to reliably fabricate materials and functional structures at the nanoscale, now enables the exploitation of strongly enhanced MO effects induced by light–matter interaction at the nanoscale (see section 12 on magnetoplasmonics and section 13 on MO metasurfaces). MO effects are also at the very heart of powerful magnetic characterization techniques like Brillouin light scattering and time-resolved pump-probe measurements for the study of spin waves (see section 7), their interactions with acoustic waves (see section 11), and ultra-sensitive magnetic field sensing applications based on nitrogen-vacancy centres in diamond (see section 17). Despite our best attempt to represent the field of magneto-optics accurately and do justice to all its novel developments and its diversity, the research area is so extensive and active that there remains great latitude in deciding what to include in an article of this sort, which in turn means that some areas might not be adequately represented here. However, we feel that the 20 sections that form this 2022 magneto-optics roadmap article, each written by experts in the field and addressing a specific subject on only two pages, provide an accurate snapshot of where this research field stands today. Correspondingly, it should act as a valuable reference point and guideline for emerging research directions in modern magneto-optics, as well as illustrate the directions this research field might take in the foreseeable future.
Abstract
Identifying materials with an efficient spin-to-charge conversion is crucial for future spintronic applications. In this respect, the spin Hall effect is a central mechanism as it allows for the interconversion of spin and charge currents. Spintronic material research aims at maximizing its efficiency, quantified by the spin Hall angle and the spin-current relaxation length . We develop an all-optical contact-free method with large sample throughput that allows us to extract and . Employing terahertz spectroscopy and an analytical model, magnetic metallic heterostructures involving Pt, W and Cu80Ir20 are characterized in terms of their optical and spintronic properties. The validity of our analytical model is confirmed by the good agreement with literature DC values. For the samples considered here, we find indications that the interface plays a minor role for the spin-current transmission. Our findings establish terahertz emission spectroscopy as a reliable tool complementing the spintronics workbench.
The absolute density of the metastable N2(A,v=0) molecule was extensively studied in nitrogen barrier discharges at 500 mbar. For the detection of the metastables laser-induced fluorescence spectroscopy (LIF) was used, at which for the calibration of the absoute metastables density a comparison with Rayleigh scattering was performed. To get the ratio of the LIF signal to the Rayleigh signal it is shown that the LIF signal is the convolution of the Rayleigh signal with an exponential decay. Besides, the different cross sections are calculated and the ratio of the detection sensitivities at the laser and fluorescence wavelength is determined. As a first step on the way to atmospheric pressure barrier discharges, the laser-induced fluorescence spectroscopy was implemented in low pressure capacitively coupled radio-frequency discharges. The determined metastables density in the capacitively coupled radio-frequency discharge is somewhat below 10^12 cm^(-3) at 40 Pa and somewhat below 10^13 cm^(-3) at 1000 Pa. The axial density profiles show a nearly symmetric shape due to the long lifetime of the metastable state. At a pressure of 500 mbar the two discharge modes of the barrier discharge, the filamentary and the diffuse mode, were analysed. The filamentary mode was mainly investigated in an asymmetric discharge configuration. Typical densities in the detection volume are in the range of 10^13 cm^(-3), resulting in maximal densities of up to 10^15 cm^(-3) in the microdischarge channel. Such large densities are in agreement with the fast decay by the pooling reaction after the maximum of the metastables density in the afterglow of the discharge pulse. The time dependent measurements in the afterglow of single microdischarges offer a delay of the metastables production with respect to the discharge current. This delay indicates that the metastables production takes place mostly by cascades from higher triplet states, which are in turn excited by electron impact. The axial density profiles show a maximum in metastables density in front of the anode in agreement with optical emission spectroscopy, but which cannot be clearly identified because of the asymmetric discharge configuration. The measurements for the diffuse discharge mode were performed in a symmetric discharge configuration. The metastables density is in the range of 10^13 cm^(-3). It increases during the current pulse of the discharge and decays afterwards. The maximum of the metastables density is delayed with respect to the maximum of the discharge current. The depletion of metastables in the early discharge afterglow is dominated by the pooling reaction, afterwards quenching by nitrogen atoms becomes important assuming a nitrogen atom density in the order of 10^14 cm^(-3). As for the filamentary mode, the losses by diffusion are negligible for the measurement positions. The measured axial density profiles show an accumulation of metastables in front of the anode, whereas the density in front of the cathode is below the detection limit. To calculate the metastables current density to the dielectrics after the discharge pulse a simulation is developed including the dominant volume processes for the depletion of metastables and the axial diffusion. Starting point for the simulation is the axial metastables density distribution at the end of the discharge pulse. The calculated metastables current density at the dielectrics is in the range of 10^14 cm^(-2)s^(-1). With the use of recently calculated secondary electron emission coefficients a comparison of the secondary electron emission by metastables with the discharge current is done. It is figured out that the secondary electron emission current is large enough to be important during the discharge ignition. To expand the simulation to the whole voltage cycle, the excitation of metastables is assumed to be proportional to the discharge current and electron density. Using this model, the measured time dependences of the metastables density are well reproduced for the investigated parameter variations. This is not the case for the axial profiles, where a metastables loss process is missed to explain the formation of a density plateau in front of the anode during the discharge pulse. The intended calculation of the metastables current density shows that the delay of the metastables production with respect to the discharge current might be responsible for the ignition of microdischarges at the beginning of the discharge pulse.
This thesis contains studies on a special class of topological insulators, so called anomalous Floquet topological insulators, which exclusively occur in periodically driven systems. At the boundary of an anomalous Floquet topological insulator, topologically protected transport occurs even though all of the Floquet bands are topologically trivial. This is in stark contrast to ordinary topological insulators of both static and Floquet type, where the topological invariants of the bulk bands completely determine the chiral boundary states via the bulk-boundary correspondence. In anomalous Floquet topological insulators, the boundary states are instead characterized by bulk invariants that account for the full dynamical evolution of the Floquet system.
Here, we explore the interplay between topology, symmetry, and non-Hermiticity in two-dimensional anomalous Floquet topological insulators. The central results of this exploration are (i) new expressions for the topological invariants of symmetry-protected anomalous Floquet topological phases which can be efficiently computed numerically, (ii) the construction of a universal driving protocol for symmetry-protected anomalous Floquet topological phases and its experimental implementation in photonic waveguide lattices, (iii) the discovery of non-Hermitian boundary state engineering which provides unprecedented possibilities to control and manipulate the topological transport of anomalous Floquet topological insulators.
Surface Stoichiometry and Depth Profile of Tix-CuyNz Thin Films Deposited by Magnetron Sputtering
(2021)
This work study a monolayer of branched poly(ethyleneimine (PEI) adsorbed onto oppositely charged surfaces with iron chelates or iron ions in the absorption solution. The conformation of adsorbed PEI is explored in the dependence of the composition of the adsorption solution by measuring the surface forces using atomic force microscopy (AFM) with the colloidal probe (CP) at different ionic strengths (INaCl) in surrounding aqueous solution. The surface coverage of these layers is investigated using X-ray reflectivity.
PEI solutions show different pH values with iron chelates (pH = 3), iron ions (pH = 4.67) or pure water (pH = 9.3) at room temperature. Low surface coverage of PEI at pH = 3 adjusted by monovalent ions was also observed. However, adsorbing PEI with iron ions or iron chelates and washing with pure water shifts the pH, leading to an adsorbed PEI layer with high coverage. In our observation, the influence of iron ions and iron chelates on the surface coverage of PEI film is stronger than the pH effect. PEI adsorbed from a pure water solution shows flat conformation. Surface force measurements with CP show that PEI adsorbed from solutions containing iron chelates or iron ions cause almost identical steric forces. The thickness of the brush L is determined as a function of the ionic INaCl in the measuring solution. It scales as a polyelectrolyte brush.
The maximum number density of gold nanoparticles (AuNPs) adsorbed onto the PEI brushes was identical and larger than on flatly adsorbed PEI. On the PEI layer with the larger surface coverage, the AuNPs aggregate; on the PEI layer with the lower surface coverage they do not aggregate. Taken together, these results contribute to understanding the mechanisms determining surface coverage and conformation of PEI and demonstrate the possibility of controlling surface properties, which is highly desirable for potential future applications.
In this thesis, we also investigate the top layer (PSS and PDADMA) of polyelectrolyte multilayer (PEM) films. PEM films were prepared by sequential adsorption of oppositely charged PEs on solid substrates. PEM films consist of polydiallyldimethylammonium (PDADMA) as polycation and the polystyrene sulfonate (PSS) as polyanion. PDADMA has a smaller linear charge density than PSS. For this system, two different growth regimes are known: parabolic and linear. I studied the top layer (PSS and PDADMA) conformation of PEM films and how the structure of this top layer is affected by increasing the number of PDADMA/PSS layer pairs N and the addition of salt to the surrounding solution.
The INaCl was changed during the force-distance measurements. PSS terminated films always show electrostatic forces at INaCl < 0.1 M and flat conformation. The surface charge density is always negative at INaCl < 0.1 M. The surface charge of the PSS top layer starts to turn from negative to positive at N ≥ 14. At N between 13 and 15, adsorbed PSS cannot compensate all the excess PDADMA charge. This leads to an accumulation of the positive extrinsic sites within the PSS terminated film beyond a specific N. At INaCl ≈ 0.1 M, an exponential decaying force was measured. This is an indication of unusual long-ranged hydration force (decay length λ-1 ≈ 0.2-0.5 nm), and PSS terminated film shows zwitterionic or neutral surface. At INaCl > 0.1 M, a non-electrostatic action occurs and the PSS terminated film reswells in solution.
PDADMA terminated surface consisting of few layers show a flat conformation and the electrostatic forces were measured. For N ≥ 9 and INaCl ≤ 0.1 M, steric forces were measured. The force-distance profiles are well-explained by Alexander and de Gennes theory. PDADMA chains show a maximum L that is around 40-45 % of the contour length. For INaCl ≈ 0.1 M, and N > 9, a flat, neutral or zwitterionic surface is found (λ-1 ≈ 0.3-0.9 nm). For N = 9 and INaCl > 0.1 M, a strong screening of electrostatic interaction and attractive forces are observed. For N > 9 and INaCl > 0.1 M, the ion adsorption into the PE chains leads to an increase in the monomer size and as a result, the L increases and PDADMA brushes reswell again into the solution.
These data show that by varying N and INaCl, different surface forces can be obtained: Electrostatic forces (flat chains) both positive and negative, steric forces (brush), hydration force (flat, neutral or zwitterionic surface), and effects not yet explained (reswelling brush).
The concept of the electron surface layer introduced in this thesis provides a framework for the description of the microphysics of the surplus electrons immediately at the wall and thereby complements the modelling of the plasma sheath. In this work we have considered from a surface physics perspective the distribution and build-up of an electron adsorbate on the wall as well as the effect of the negative charge on the scattering of light by a spherical particle immersed in a plasma. In our electron surface layer model we treat the wall-bound electrons as a wall-thermalised electron distribution minimising the grand canonical potential and satisfying Poissons equation. The boundary between the electron surface layer and the plasma sheath is determined by a force balance between the attractive image potential and the repulsive sheath potential and lies in front of the crystallographic interface. Depending on the electron affinity x, that is the offset of the conduction band minimum to the potential in front of the surface, two scenarios for the wall-bound electrons are realised. For x<0 electrons do not penetrate into the solid but are trapped in the image states in front of the surface where they form a quasi two-dimensional electron gas. For x>0 electrons penetrate into the conduction band where they form an extended space charge. These different scenarios are also reflected in the electron kinetics at the wall which control the sticking coefficient and the desorption time. If x<0 electrons from the plasma cannot penetrate into the solid. They are trapped in the image states in front of the surface. The transitions between unbound and bound states are due to surface vibrations. Trapping of electrons is mediated by one-phonon transitions and takes place in the upper bound states. Owing to the large binding energy of the lowest bound state transitions from the upper bound states to the lowest bound state are due to multi-phonon processes. For low surface temperatures relaxation to the lowest bound state takes place while for higher temperature a relaxation bottleneck emerges. Desorption occurs in cascades for systems without relaxation bottleneck and as a one-way process in systems with a relaxation bottleneck. From the perspective of plasma physics the most important result is that the sticking coefficient for electrons is relatively small, typically on the order of 0.001. For x>0 electron physisorption takes place in the conduction band. For this case sticking coefficients and desorption times have not been calculated yet but in view of the more efficient scattering with bulk phonons, responsible for electron energy relaxation in this case, we expect them to be larger than for the case of x<0. Finally, we have studied the effects of surplus electrons on the scattering of light by a spherical particle. For x<0 the electrons form a spherical electron gas around the particle and their electrical conductivity modifies the boundary condition for the magnetic field. For x>0 the electrons in the bulk of the particle modify the refractive index through their bulk electrical conductivity. In both cases the conductivity is limited by scattering with surface or bulk phonons. Surplus electrons lead to an increase of absorption at low frequencies and, most notably, to a blue-shift of an extinction resonance in the infrared. This shift is proportional to the charge and is strongest for submicron-sized particles. The particle charge is also revealed in a blue-shift of the rapid variation of one of the two polarisation angles of the reflected light. From our work we conclude that the electron affinity is an important parameter of the surface which should affect the charge distribution as well as the charge-up. Therefore, we encourage experimentalists to study the charging of surfaces or dust particles as a function of x. Interesting in this respect is also if or under what conditions the electron affinity of a surface exposed to a plasma remains stable. Moreover, we suggest to use the charge signatures in Mie scattering to measure the particle charge optically. This would allow a charge measurement independent of the plasma parameters and could be applied to nano-dust where conventional methods cannot be applied.
Surface charge measurements on different dielectrics in diffuse and filamentary barrier discharges
(2017)
Abstract
Previously, we reported on the measurement of surface charges during the operation of barrier discharges (BDs) using the electro-optic Pockels effect of a bismuth silicon oxide (BSO) crystal. With the present work, the next milestone is achieved by making this powerful method accessible to various dielectrics which are typically used in BD configurations. The dynamics and spatial distribution of positive and negative surface charges were determined on optically transparent borosilicate glass, mono-crystalline alumina and magnesia, respectively, covering the BSO crystal. By variation of the nitrogen admixture to helium and the pressure between 500 mbar and 1 bar, both the diffuse glow-like BD and the self-stabilized discharge filaments were operated inside of a gas gap of 3 mm. The characteristics of the discharge and, especially, the influence of the different dielectrics on its development were studied by surface charge diagnostics, electrical measurements and ICCD camera imaging. Regarding the glow-like BD, the breakdown voltage changes significantly by variation of the cathodic dielectric, due to the different effective secondary electron emission (SEE) coefficients. These material-specific SEE yields were estimated using Townsend’s criterion in combination with analytical calculations of the effective ionization coefficient in helium with air impurities. Moreover, the importance of the surface charge memory effect for the self-stabilization of discharge filaments was quantified by the recalculated spatio-temporal behavior of the gap voltage.
The active screen plasma nitrocarburizing (ASPNC) technology is a state-of-the-art plasma-assisted heat treatment for improving surface hardness and wear resistance of metallic workpieces based on thermochemical diffusion. In comparison to conventional plasma nitrocarburizing, the use of an active screen (AS) improves thermal homogeinity at the workload and reduces soot formation. Further it can serve as a chemical source for the plasma processes, e.g. by use of an AS made of carbon-fibre reinforced carbon. This compilation of studies investigates the plasma-chemical composition of industrial- and laboratory-scale ASPNC plasmas, predominantly using in-situ laser absorption spectroscopy with lead-salt tuneable diode lasers, external-cavity quantum cascade lasers, and a frequency comb. In this way the temperatures and concentrations of the dominant stable molecular species HCN, NH3, CH4, C2H2, and CO, as well as of less prevelant species, were recorded as functions of e.g. the pressure, the applied plasma power, the total feed gas flow and its composition. Additionally, the diagnostics were applied to a chemically similar plasma-assisted process for diamond deposition.
Resulting from this thesis are new insights into the practical application of an AS made of CFC, the plasma-chemistry involving hydrogen, nitrogen, and carbon, and the particular role of CO as an indicator for reactor contamination. The effect of the feed gas composition on the resulting nitrogen- and carbon-expanded austenite layers was proven by combination of in-situ laser absorption spectroscopy with post-treatment surface diagnostics. Furthermore this work marks the first use of frequency comb spectroscopy with sub-nominally resolved Michelson interferometry for investigation of a low-pressure molecular discharge. This way the rotational bands of multiple species were simultaneously measured, resulting in temperature information at a precision hitherto not reached in the field of nitrocarburizing plasmas.
The stratospheric aerosol layer plays an important role in the radiative balance of Earth primarily through scattering of solar radiation. The magnitude of this effect depends critically on the size distribution of the aerosol. The aerosol layer is in large part fed by volcanic eruptions strong enough to inject gaseous sulfur species into the stratosphere. The evolution of the stratospheric aerosol size after volcanic eruptions is currently one of the biggest uncertainties in stratospheric aerosol science. We retrieved aerosol particle size information from satellite solar occultation measurements from the Stratospheric Aerosol and Gas Experiment III mounted on the International Space Station (SAGE III/ISS) using a robust spectral method. We show that, surprisingly, some volcanic eruptions can lead to a decrease in average aerosol size, like the 2018 Ambae and the 2021 La Soufrière eruptions. In 2019 an intriguing contrast is observed, where the Raikoke eruption (48∘ N, 153∘ E) in 2019 led to the more expected stratospheric aerosol size increase, while the Ulawun eruptions (5∘ S, 151∘ E), which followed shortly after, again resulted in a reduction in the values of the median radius and absolute distribution width in the lowermost stratosphere. In addition, the Raikoke and Ulawun eruptions were simulated with the aerosol climate model MAECHAM5-HAM. In these model runs, the evolution of the extinction coefficient as well as of the effective radius could be reproduced well for the first 3 months of volcanic activity. However, the long lifetime of the very small aerosol sizes of many months observed in the satellite retrieval data could not be reproduced.
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.
In this thesis, a stereoscopic camera system is presented that is designed for the use on parabolic flights for the investigation of dusty plasmas under microgravity conditions. This camera system consists of three synchronously triggered high-speed cameras observing a common volume of approximately (15 × 15 × 15) mm³ size. In this volume, the three-dimensional trajectories of a large number of particles surrounded by a dense dust cloud were reconstructed. For this task an intricate set of reconstruction algorithms has been developed, including a four-frame linking algorithm and a complex combined 2D/3D tracking algorithm for a reliable tracking of 3D particles. Furthermore, these algorithms effectively suppress so-called ghost particles in the evaluation process which are reconstructed from falsely identified 2D particle correspondences. Dusty plasmas under microgravity conditions are of special interest due to their complex structure and the variety of observable dynamic phenomena. Under typical discharge conditions, a central dust-free void is formed, surrounded by a dense particle cloud. Since the void is inherently dust-free, particles shot into the void can be uniquely identified and used to probe plasma properties inside this region. In the dust cloud itself, processes like self-excited dust-density waves can be observed under suitable experimental conditions. Using the presented camera setup and reconstruction algorithms, two parts of a dusty plasma under microgravity on parabolic flights are investigated. Initially, the force field creating and sustaining the central void is deduced and characterized. The combination of ion drag and electric field force is measured and compared to current models of the ion drag, showing a good agreement with these models. While previous investigations on the forces were limited to two-dimensional slices through the void, our measurements represent the first three-dimensional quantitative analysis of a large fraction of the void region. From this analysis the structure of the force field is determined and separated into a radial and a non-radial (or orthogonal) contribution. It is shown that the radial contribution dominates in the central void, while non-radial forces increase in magnitude close to the void edge. The radial domination is also observed in the velocity distribution of the probe particles which is significantly shifted to radially outward directed velocities for particles leaving the void. Assuming a strictly radial force profile in the horizontal mid-plane of the void, the friction coefficient determining the interaction of the probe particles with the neutral gas background is experimentally determined and shown to match the theoretical expectation. Subsequently, particles at the outer surface of the dust cloud are reconstructed. There, the particles are found to oscillate due to dust-density waves propagating through the high-density dust cloud. For the investigation of the correlation between waves and oscillating particles, the instantaneous wave and oscillation properties are determined and the instantaneous phase difference is obtained. Modeling the probe particles as driven, damped harmonic oscillators, these phase differences between waves and particles are interpreted with respect to the resonance frequency of the oscillating particles. Spatial variations of the phase difference are observed that may be attributed to different frequencies of the dust-density waves, or to changes of the resonance frequency induced by changing local plasma parameters. From a few measurements of particles oscillating at their resonance frequency, information about the surrounding plasma or properties of the particles themselves can be deduced. However, a larger number of reconstructed trajectories is necessary in order to interpret the phase differences on a reliable data basis. The presented camera setup in combination with the evaluation algorithms is a flexible system for the investigation of three-dimensional dusty plasmas. Its robust construction allows the operation of the system in challenging environments such as on parabolic flights, where spatial limitations and vibrations produced by the aircraft make special demands on such a diagnostic tool. This versatility makes our stereoscopic camera setup and the reconstruction process a suitable standard diagnostic for the application with dusty plasmas; this system will therefore be used in future research amongst other things for the investigation of boundary layers in extended three-dimensional dust clouds under microgravity.
In this work, 2-dimensional measurements in the THz frequency range with self-made spintronic THz emitters were presented. The STE were used to optimize the spatial resolution and determine the magnetization in geometric shapes. At the beginning, various combinations of FM and NM layers were produced and measured to achieve an optimal composition of the STE. The layer thickness of the ferromagnetic CoFeB layer and the nonmagnetic PT layer was also varied. The investigations have shown that a layer combination of 2 nm thick CoFeB and 2 nm thick Pt, applied to a fused silica glass substrate and covered with a 300 nm thick SiO2 layer, emits the highest THz amplitude. Based on these, a structured sample, consisting of an STE and an additional layer system of 5 nm Cr and 100 nm Au, was produced. Further, three wedge-shaped structures were removed from the gold layer by an etching process so that the THz radiation generated by the STE can pass through these areas. This enables the optimization of the resolution of the system. For this purpose, the sample was moved perpendicular to the laser beam by two stepping motors with a step size of 5 μm and imaged 2-dimensionally. By reducing the step size to 0.2 μm, the beam diameter could be measured at the edge of the structure using the knife-edge method. Based on this measurement, the resolution of the system could be determined as 5.1 ± 0.5 μm at 0.5 THz, 4.9 ± 0.4 μm at 1 THz, and 5.0 ± 0.5 μm at 1.5 THz. These results are confirmed by simulations considering the propagation of THz wave packets through the SiO2. The expansion of the FWHM of the waves, passing through the 300 nm thick layer, is about 1%. Only a SiO2 layer with a thickness in the μm range occurs an expansion of around 10%. This shows that it is possible to perform 2-dimensional THz spectroscopy with a resolution in the dimension of the exciting laser beam by using near-field optics. Afterward, the achieved spatial resolution was used to investigate the influence of external magnetic fields on the STE and the emitted THz radiation. By implementing a pair of coils above the sample, an external magnetic field could be applied parallel to the pattern. The used sample was designed in such a way that only certain geometric areas on the fused silica glass substrate were coated with an STE so that THz radiation is emitted only in those areas. The 2-dimensional images show the geometric structures for f = 1.0 THz and f = 1.5 THz clearly. By applying a permanent, positive magnetic field (+M), a positive course of the THz amplitude can be seen. A rotation of the magnetic field by 180° (-M) leads to a reversal of the orientation of the emitted THz radiation, whereby the magnetic field does not influence the corresponding frequency spectrum. By using minor loops, the sample was demagnetized by the constant reduction of the magnetic field strength with alternating magnetic field direction. The 2-dimensional representation of the pattern with a step size of 10 μm shows that the sample was demagnetized since both, positively and negatively magnetized structures, could be imaged. In addition, in the 2nd row from the top, a completely demagnetized circle and a rectangle with a division into two domains can be seen. These structures have both positive and negative magnetized areas, which are separated by a domain wall. To investigate this in more detail a 2-dimensional measurement of the divided regions was made with a step size of 2.5 μm. These images confirm the division of the structures into positive and negative domains, separated by a domain wall, which was verified by Kerr-microscope measurements. Both data show a similar course of the domains and the domain wall. However, to be able to examine the domain wall more precisely using 2-dimensional THz spectroscopy, the resolution of the system must be improved to a range of a few nm, because the expected domain wall width is between 𝑙𝑊 = 12.56 nm and 𝑙𝑊 = 125.6 nm. The improved resolution would make it possible to image foreign objects, such as microplastics in biological cells or tissue. For this purpose, different plastics, such as polypropylene, polyethylene, and polystyrene, were investigated in the THz frequency range up to 4 THz. While no specific absorption could be determined for PP, characteristic absorption peaks were found for PE and PS. The energy of the photons with a frequency of about 2.2 THz excites lattice vibrations in the PE. Therefore, this frequency is specifically absorbed, and the intensity in the transmission spectrum is lower than for other frequencies. PS absorbs especially THz radiation with a frequency of 3.2 THz. In addition, all of the investigated plastics are mostly transparent for THz radiation, which makes imaging of these materials feasible. Based on these basic properties, it will be possible to image and identify these types of plastic.
We investigate local THz field generation using spintronic THz emitters to enhance the resolution for micrometer-sized imaging. Far-field imaging with wavelengths above 100 µm limits the resolution to this order of magnitude. By using optical laser pulses as a pump, THz field generation can be confined to the area of laser beam focusing. The divergence of the generated THz beam due to laser beam focusing requires the imaged object to be close to the generation spot at a distance below the THz field wavelength. We generate THz-radiation by fs-laser pulses in CoFeB/Pt heterostructures, based on spin currents, and detect them by commercial low-temperature grown-GaAs (LT-GaAs) Auston switches. The spatial resolution of THz radiation is determined by applying a 2D scanning technique with motorized stages allowing step sizes in the sub-micrometer range. Within the near-field limit, we achieve spatial resolution in the dimensions of the laser spot size on the micrometer scale. For this purpose, a gold test pattern is evaporated on the spintronic emitter separated by a 300 nm SiO2 spacer layer. Moving these structures with respect to the femtosecond laser spot, which generates THz radiation, allows for resolution determination. The knife-edge method yields a full-width half-maximum beam diameter of 4.9 +- 0.4 µm at 1 THz. The possibility to deposit spintronic emitter heterostructures on simple glass substrates makes them attractive candidates for near-field imaging in many imaging applications.
Three-dimensional (3D) dynamical properties of fast particles being injected into the void region of a dusty plasma under microgravity conditions have been measured. For that purpose, a stereoscopic camera setup of three cameras has been developed that is able to track and reconstruct the 3D trajectories of individual dust particles. From more than 500 particle trajectories, the force field inside the void region and its influence on particle movement are derived and analyzed in 3D. It is shown that the force field is dominated by forces pointing radially out of the void and that this radial character is reflected in the velocity distributions of particles leaving the void. Furthermore, the structure of the force field is used for measuring the neutral gas friction for the particles inside the void.