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In der vorliegenden Arbeit wurde die Wechselwirkung reaktiver Sauerstoffspezies (ROS) mit organischen Molekülen anhand zweier unterschiedlicher Systeme analysiert. Während einerseits der Einfluss von ROS auf eine organische Monoschicht am Beispiel des synthetischen, kationischen Polyelektrolyten Polyethylenimin (PEI) untersucht wurde, stand andererseits die Wechselwirkung von ROS mit einem DNS-Molekül, dem Biopolyelektrolyten pBR322 im Fokus des Interesses. Für die Untersuchungen der ROS-PEI-Wechselwirkung wurde zunächst verzweigtes PEI flach (RMS-Rauigkeit < 1 nm) auf einem Silizium-Substrat adsorbiert. Mit Hilfe der Fenton-Reaktion wurde die PEI-Monoschicht dem Einfluss von ROS ausgesetzt. Anhand von Kraft-Abstands-Kurven (KAK) konnte gezeigt werden, dass die flache Konformation der PEI-Monoschicht nach dem ROS-Einfluss erhalten bleibt. Des Weiteren konnte mittels Adsorption negativ geladener Gold-Nanopartikel (AuNP) demonstriert werden, dass die PEI-Oberfläche auch nach der Wechselwirkung mit ROS positiv geladene Gruppen enthält. Darüber hinaus konnte mit Hilfe der KAK gezeigt werden, dass sowohl die Oberflächenladungsdichte (OFL) als auch das Oberflächenpotential (OFP) unter ROS-Einfluss um einen Faktor 0,5 reduziert wurden. Es wurde gezeigt, dass die Reduzierung von OFL bzw. OFP auf die Abspaltung positiv geladener Gruppen der PEI-Monoschicht zurückgeführt werden kann. Mit Hilfe der dreidimensionalen Kraftspektroskopie wurde gezeigt, dass OFL und OFP auf einer Längenskala von 1,8 bis 30 µm lateral homogen sind. Darüber hinaus wurde anhand der AuNP-Belegungsdichte demonstriert, dass die Ladungsträger innerhalb der PEI-Oberfläche auf einer Längenskala oberhalb von 36 nm homogen verteilt sind. Hinsichtlich kleiner Längenskalen (< 36 nm) kann konstatiert werden, dass aufgrund einer verzögerten Adsorptionskinetik der AuNP nach der ROS-PEI-Wechselwirkung mit einer partiell reduzierten Bindungswahrscheinlichkeit zu rechnen ist. Vermutlich bewirkt der ROS-Einfluss eine inhomogene Verteilung der positiven Ladungsträger innerhalb der PEI-Monoschicht auf einer Längenskala von einigen nm. Experimentell ergibt sich darüber hinaus, dass eine 50 %ige Reduzierung des PEI-Oberflächenpotentials einer Abnahme von etwa 10 % der maximalen, anteiligen AuNP-Belegungsdichte entspricht. Diese experimentell bestimmten Parameter konnten unter Einbeziehung eines erweiterten drei-Körper RSA-Modelles erklärt werden. Im zweiten Teil der vorliegenden Arbeit wurde eine neue Methode der Quantifizierung ROS-induzierter DNS-Schäden eingeführt. Dazu wurden die DNS-Moleküle zunächst mittels Fenton-Reaktion dem Einfluss von ROS ausgesetzt, auf Polyallylamin-Hydrochlorid-funktionalisiertem Glimmer adsorbiert und mittels des RKM im intermittierenden Modus (RKM-IM) abgebildet. Die Klassifizierung der DNS-Moleküle erfolgt unter Berücksichtigung des Kettenhöhenunterschiedes von doppelsträngiger- (dsDNS) und einzelsträngiger (esDNS) DNS. Als ROS-induzierter DNS-Schaden wird hierbei der Konformationsübergang von dsDNS (intakt) in esDNS (defekt) identifiziert. Die zentrale Messgröße der vorgestellten Methode ist demnach die DNS-Kettenhöhe, welche sich im Falle immobilisierter DNS-Moleküle mit einer Genauigkeit im Sub-Ångström-Bereich mit Hilfe des RKM-IM bestimmen lässt. Für die automatisierte Quantifizierung der Flächen, welche mit dsDNS respektive esDNS belegt sind, wurde ein Höhengrenzwert-basierter Auswertungs-Algorithmus konstruiert. Neben der Variation der Stärke der ROS-DNS-Wechselwirkung mittels verschiedener H2O2-Konzentrationen innerhalb der Fenton-Reaktion, wurde der Einfluss eines Radikalfängers am Beispiel des Natriumacetats (NaOAc) auf diese Wechselwirkung untersucht. Mit der Quantifizierung der ROS-DNS-NaOAc-Wechselwirkung wurde gezeigt, dass der anteilige DNS-Schaden mit wachsender H2O2-Konzentration zunimmt und mit steigender NaOAc-Konzentration abnimmt. Darüber hinaus wurde die Anwendbarkeit der in dieser Arbeit eingeführten Quantifizierung ROS-induzierter DNS-Schäden mit Hilfe eines reaktionskinetischen Ansatzes unter Verwendung des Modelles der kompetitiven Hemmung analysiert. Auf diese Weise wurden Ratenkonstanten der Wechselwirkung zwischen NaOAc mit Hydroxylradikalen verifiziert und somit die Validität des eingeführten Konzeptes demonstriert. Des Weiteren ermöglicht die automatisierte Datenanalyse einen vergleichsweise hohen Datendurchsatz und eignet sich daher gut für die Untersuchung der komplexen Wechselwirkung zwischen ROS, Radikalfänger und DNS. Anhand eines Vergleiches mit den etablierten Methoden zur Quantifizierung ROS-induzierter DNS-Schäden ergibt sich unter Einbeziehung des, in dieser Arbeit eingeführten Analyseverfahrens, ein komplementäres Verständnis der ROS-DNS-Wechselwirkung über einen großen Längenskalenbereich.
A central point of this thesis is the investigation of surface structure and surface forces, which are created by single layers of linear polyelectrolytes (PE). In detail, the properties of cationic poly(allylamine)hydrochloride (PAH) and poly-l-lysine (PLL) and anionic sodium poly(styrene sulfonate) (PSS) are determined, which have been physisorbed onto oppositely charged silica surfaces in presence of a predefined salt concentration IAds. For these investigations, a new averaging method for colloidal probe (CP) force profiles is developed, which leads to an ultimate force resolution of 1 pN after the data processing, (signal to noise ratio of > 1000). Furthermore, a new kind of tapping mode imaging is presented (so called colloidal probe tapping mode, CPTM), which uses a CP instead of a sharp tip and hence which allows to resolve lateral inhomogeneously distributed surface forces. The basics to understand such-like obtained tapping mode images are developed. For adsorption from salt-free solution (IAds = 0) the dominance of an electrostatic double layer repulsion is observed, which is commonly attributed to the adsorption of the PE chains into a rather flat and compact layer and which is in full agreement with theoretical predictions and enormous experimental data available in literature. However, even a small addition of salt to the deposition solution (i.e. IAds > 1 mM NaCl) introduces a new contribution to the surface force, which is attributed to PE chains that are non-flatly physisorbed. Using scaling considerations, it is shown for all investigated PE that this non-flat conformation can be described by brush-like chain adsorption (cf. Section 3.3.5); other conformations like mushroom or pancake are excluded (cf. Section 5.3). Interestingly, these non-flatly physisorbed chains combine properties of neutral and PE brushes: (i) The force is very well described by the theory of Alexander and de Gennes (AdG, cf. Section 5.4). By fitting the AdG force law to the data, it is possible to determine the (brush) thickness L of the PE layer and the average distance s between brush-like physisorbed chains. Although the chains are charged the electrostatic contribution to the surface forces is too small to be noticeable (cf. Section 5.4.2). (ii) The thickness L of this PE layer is much larger compared to the compact layer (observed for salt-free adsorption) and is also subject to a pronounced swelling and shrinking if the bulk salt concentration I is decreased or increased, respectively. Surprisingly, all measurements indicate that L follows a scaling law known for salted end-grafted PE brushes, i.e. L ~ N (I s^2)^(-1/3) (with N denoting the degree of polymerization). Furthermore, the osmotic brush phase is never observed in the experiments, but chain stretching up to 1 / 3 of the contour length is regularly achieved. CPTM imaging applied to PSS shows that the brush-like physisorbed chains are not homogenously distributed over the surface, but form brush domains which coexist with flatly physisorbed chains (cf. sections 5.5 and 5.6). This clearly shows that PSS generally physisorbs in two distinct phases, which differ in conformation (flat vs. brush) and the surface force caused (electrostatic vs. steric repulsion). The force profile of the two phase system is in good approximation simply the superposition of a steric and an electrostatic repulsion, whereby their respective contribution to the composed force profile is given by their area fraction. The quantitative analysis reveals that L and s of the brush phase are independent on IAds. This is remarkable, as a change in IAds is known to induce a continuous transition between a stretched (low IAds) and coiled chain conformation (high IAds) in the deposition solution (cf. [Fleer1993, Yashiro2002]). Hence, one can conclude that the conformation in solution does not necessarily correspond to the conformation after adsorption. It is also shown that the area fraction A of the brush domains strongly depends on N and IAds. For example, for constant N the scaling relation A ~ sqrt(IAds) is determined, which is very similar to the common observation that the surface coverage %Gamma of adsorbed PE layers increases also with %Gamma ~ sqrt(IAds) [Schmitt1996, Cosgrove1986, Ahrens2001, Yim2000, Gopinadhan2007, Cornelson2010]. This suggest that brush-like physisorbed PE chains are responsible for the increase in %Gamma. In fact, Section 5.6 shows that the mass of the brush phase is approx. 0.5 mg/m² which is comparable to the increase in %Gamma reported in literature for IAds = 1 M NaCl [Cosgrove1986, Schmitt1996, Ahrens2001]. As a change in IAds does not affect L and s, but solely the brush area fraction A, it is argued in Section 5.6 that an increase in IAds can be understood as a phase transition from the (disordered) flat phase towards the (ordered and extended) brush phase. Here, further theoretical considerations would be desirable.
Bei moderaten sinusförmigen Betriebsspannungen tritt in reinem Stickstoff der diffuse Townsend-Modus (APTD) auf. Das elektrische Feld ist hier über den Entladungsspalt annähernd konstant, weshalb ein anodengerichteter exponentieller Anstieg der Intensität der Emission beobachtet wird. Dementsprechend ist das Intensitätsmaximum direkt vor der Anode lokalisiert. Überraschenderweise lässt sich die APTD unter den gegebenen experimentellen Bedingungen (Breite des Entladungsspalts d_Spalt=1 mm und sinusförmige Betriebsspannung) ebenfalls in einer Helium-BE genieren. Für gewöhnlich wird jedoch in einer Helium-Entladung der diffuse Glimmentladungs-Modus (APGD) beobachtet, wobei der Entladungsspalt zwischen 2-5 mm breit ist. Das Emissionsmaximum einer solchen Entladung befindet sich durch die Ausbildung eines Kathodenfallgebiets vor der Kathode. Die geringe Breite des Entladungsspalts verhindert hier jedoch die Ausbildung der APGD. Entsprechend kann sich das Kathodenfallgebiet nicht entwickeln, wodurch die Spaltspannung nur schwach einbricht. Das Intensitätsmaximum der Emissionsentwicklung befindet sich wie bei der diffusen Stickstoff-BE direkt vor der Anode. Die Zünd- und Brennspannung ist in Stickstoff größer als in Helium, da die Vibrationszustände des Stickstoffs effizient durch Elektronen angeregt werden und diesen dabei Energie entzogen wird. Helium hat jedoch keine Vibrationszustände, weshalb die Elektronentemperatur ansteigt und die Zünd- und Brennspannung deutlich geringer ist. Eine Erhöhung des Spannungsanstiegs dU/dt beeinflusst signifikant die Entladungsentwicklung in der diffusen Helium-Entladung. So führt eine Variation von der Sinus- zur Rechteckspannung zu einem Wechsel des Entladungsmodus, nämlich von der APTD zur APGD. Die Ursache hierfür ist der deutlich höhere Energieeintrag, was sich auf die Ionisationsprozesse auswirkt. Die Verwendung einer Sägezahnspannung stellt in Bezug auf den Spannungsanstieg dU/dt eine Kombination aus der Sinus- und der Rechteckspannung dar. Mit dieser Betriebsspannung war es erstmals möglich, in einer Entladungsperiode entsprechend der Spannungsgradienten beide Entladungsformen (APTD und APGD) zu beobachten und zu studieren. Durch die Oberflächenladungsmessung konnte nachgewiesen werden, dass die während eines elektrischen Durchbruchs im Entladungsvolumen transferierte Ladung vollständig auf den Dielektrika akkumuliert wird. Der Vergleich der phasenaufgelösten Oberflächenladungsdichtemessung mit der zeitlichen Integration der Stromdichte zeigt, dass die Akkumulation von Oberflächenladungen instantan mit dem Auftreten eines Strompulses stattfindet. Nach einem Entladungsstrompuls bleiben die Oberflächenladungen unabhängig vom Entladungsmodus auf dem Dielektrikum konstant, bis die Entladung in der nächsten Halbwelle erneut zündet. In der filamentierten Entladung markieren die Oberflächenladungen den Auftreffpunkt der einzelnen Mikroentladungen. Die Oberflächenladungen sind an diesen Stellen stark lokalisiert. Die gemittelten radialen Oberflächenladungsdichteprofile haben gezeigt, dass diese sowohl für die negativen als auch für die positiven Oberflächenladungen einer Gauß-Verteilung folgen. Die volle Halbwertebreite der entsprechenden Oberflächenladungsdichteprofile unterscheidet sich. Die negativen Oberflächenladungen nehmen eine größere Fläche ein als die positiven Oberflächenladungen. Es konnte erstmals gezeigt werden, dass Mikroentladungen über viele Entladungsperioden immer wieder an der gleichen Stelle zünden, wo sich aus einer vorhergehenden Entladung ein lokalisierter Oberflächenladungsfleck entgegengesetzter Polarität befand. Dieses Phänomen wird als Memory-Effekt bezeichnet. Durch zeitlich definiertes Abschalten der Entladung konnten die Lebensdauern von Oberflächenladungen beider Polaritäten auf dem BSO-Kristall gemessen werden. Es konnte gezeigt werden, dass der Abbau der Oberflächenladungen in zwei Zerfallsprozesse k_1 und k_2 unterteilt ist. Während des Prozesses k_1 nimmt die Oberflächenladungsdichte innerhalb einiger weniger Sekunden deutlich ab. Die Zeitkonstante k_1 ist trotz der photoleitenden Eigenschaft des BSO-Kristalls unabhängig von der Beleuchtungsfrequenz des Kristalls ist. Der zweite deutlich langsamer ablaufende Prozess zeigte hingegen eine starke Abhängigkeit von der Beleuchtungsfrequenz der BSO-Kristalls. Wurde der Kristall kontinuierlich beleuchtet, verschwanden die Oberflächenladungen unabhängig von ihrer Polarität nach wenigen Sekunden vollständig. Je kleiner die Beleuchtungsrate des Kristalls ist, desto länger waren die Oberflächenladungen nachweisbar. Der Zerfallsprozess k_2 beruht auf intrinsischen Transportprozessen. Hierbei wird davon ausgegangen, dass die negativen Oberflächenladungen durch Elektronen nahe der Oberfläche gebildet werden. Die positiven Oberflächenladungen sind Löcher im Valenzband, die durch Elektronen-Ionen-Rekombination entstehen.
Magnetic reconnection is a fundamental plasma process where a change in field line connectivity occurs in a current sheet at the boundary between regions of opposing magnetic fields. In this process, energy stored in the magnetic field is converted into kinetic and thermal energy, which provides a source of plasma heating and energetic particles. Magnetic reconnection plays a key role in many space and laboratory plasma phenomena, e.g. solar flares, Earth’s magnetopause dynamics and instabilities in tokamaks. A new linear device (VINETAII) has been designed for the study of the fundamental physical processes involved in magnetic reconnection. The plasma parameters are such that magnetic reconnection occurs in a collision-dominated regime. A plasma gun creates a localized current sheet, and magnetic reconnection is driven by modulating the plasma current and the magnetic field structure. The plasma current is shown to flow in response to a combination of an externally induced electric field and electrostatic fields in the plasma, and is highly affected by axial sheath boundary conditions. Further, the current is changed by an additional axial magnetic field (guide field), and the current sheet geometry was demonstrated to be set by a combination of magnetic mapping and cross-field plasma diffusion. With increasing distance from the plasma gun, magnetic mapping results in an increase of the current sheet length and a decrease of the width. The control parameter is the ratio of the guide field to the reconnection magnetic field strength. Cross-field plasma diffusion leads to a radial expansion of the current sheet at low guide fields. Plasma currents are also observed in the azimuthal plane and were found to originate from a combination of the field-aligned current component and the diamagnetic current generated by steep in-plane pressure gradients in combination with the guide field. The reconnection rate, defined via the inductive electric field, is shown to be directly linked to the time-derivative of the plasma current. The reconnection rate decreases with increasing ratio of the guide field to the reconnection magnetic field strength, which is attributed to the plasma current dependency on axial boundary conditions and the plasma gun discharge. The above outlined results offer insights into the complex interaction between magnetic fields, electric fields, and the localized current flows during reconnection.
Turbulence is a state of a physical system characterized by a high degree of spatiotemporal disorder. Turbulent processes are driven by instabilities exhibiting complex nonlinear dynamics, which span over several spatial as well as temporal scales. Apart from fluids and gases, turbulence is observed in plasmas. While turbulent mixing of a system is sometimes a desired effect, often turbulence is an undesired state. In hot, magnetically confined plasmas, envisaged for energy generation by thermonuclear fusion, plasma turbulence is clearly a problem, since the magnetic confinement time is drastically deteriorated by turbulent transport. Hence, a control mechanism to influence and to suppress turbulence is of significance for future fusion power devices. An important area of plasma turbulence is drift wave turbulence. Drift waves are characterized by currents parallel to the ambient magnetic field, that are tightly coupled to a coherent mode structure rotating in the perpendicular plane. In the present work, the control of drift waves and drift wave turbulence is experimentally investigated in the linear magnetized helicon experiment VINETA. Two different open-loop control systems - electrostatic and electromagnetic - are used to drive dynamically parallel currents. It is observed that the dynamics of the drift waves can be significantly influenced by both control schemes. If the imposed mode number as well as the rotation direction match those of the drift waves, classical synchronization effects like, e.g., frequency locking, frequency pulling, and Arnold tongues are observed. These confirm the nonlinear interaction between the control signal and the drift wave dynamics. Finally, the broadband drift wave turbulence, and thereby turbulent transport, is considerably reduced if the applied control signal is sufficiently large in amplitude.
The central aim of this thesis was the investigation of protein/polyanion interaction using circular dichroism (CD) spectroscopy, enzyme immune assay (EIA), isothermal titration calorimetry (ITC) and flow cytometry (FC). A further aim was to understand why an endogenous protein becomes immuno-genic when forming a complex. The focus was on the protein platelet factor (PF4), which gained wide interest in the clinical field, due to its role in the life-threatening, immune-driven, adverse drug effect heparin-induced thrombocytopenia (HIT). PF4 is a small homotetrameric chemokine with several basic amino acids on its surface, forming a positively charged ring. The antibodies that are formed during HIT recognize an epitope exposed on PF4, when it is in a complex with heparin at a certain molar ratio at which, PF4 tetramers are aligned on the heparin and forced into close approximation. The main results and conclusions of the thesis are summarized below: 5.1 Evolutionary Conservation of PF4 (Paper I – PF4/Evolution) By carrying out an amino acid sequence survey we found that the positively charged amino acids contributing to the heparin binding site on the surface of PF4 and related proteins are highly conserved in all vertebrates, including fish species. PF4 interacts with the phospholipid lipid A, the innermost part of the lipopolysaccharide (LPS) of Gram negative bacteria. We showed that the shorter the sugar chain of the O antigen, outer and inner core of the LPS were the more PF4 was binding. The interaction of PF4 with lipid A is inhibited by heparin, suggesting that the amino acids known to contribute to heparin binding are also involved in binding to lipid A. 5.2 PF4 Interaction with Polyanions (PA) of varying Length and Degree of Sulfation (Paper II – PF4/PA) CD spectroscopy was found to be a powerful technique to monitor structural changes of PF4 caused by binding to various clinically relevant polyanions. Therefore PF4 was titrated with different PA to investigate the dependencies: i. impact of the PF4:PA molar ratio, ii. degree of polymerization of the PA and iii. degree of sulfation of the PA. In all cases, exposure of HIT-relevant epitope(s) was only observed for PA that also induced changes in secondary structure of PF4. A comparison of results of an immune ¬assay with CD spectroscopic data showed that the extent of complex anti¬genicity correlates well with the magnitude of changes in PF4 secondary structure, and that the structural changes of PF4 have to exceed a certain threshold to achieve PF4/PA complex antigenicity. These findings allowed us to calculate expectation intervals for complex antigenicity solely using CD spectroscopic data. To our knowledge, this was the first demonstration that the capability of drugs to induce antigenicity of PF4 can be assessed without the necessity of in vivo studies or the use of antibodies obtained from immunized patients specific for the antigens. The antigenicity of PF4 in complex is not restricted to negative charges originating from sulfate groups, PA with phosphate groups are also capable (binding to phospholipids). We investigated inorganic polyphosphates (polyP) with a chain length of 75 Pi and showed that the induced secondary structural changes are even higher compared to the changes induced by the different heparins and that the PF4/P75 complexes are antigenic as well. 5.3 PF4 Interaction with defined oligomeric Heparins (Paper III – PF4/defined Heparins) We tested highly purified, monodisperse heparins. In contrast to the clinically relevant but relatively undefined (high polydispersity index) glycosamino glycans reported in paper II (PF4/PA). The defined heparins induced higher secondary structural changes. Here we showed for the first time that strong conformational changes during PF4/PA complex formation are necessary but not sufficient for to the expression of the anti-PF4/heparin antibody binding site. Also, the size of the complexes is not the only prerequisite for anti-PF4/heparin antibody binding (tested by atomic force microscopy). By ITC we found that antigenicity is only induced if the PF4/PA complex has a high binding enthalpy and the complex formation leads to a negative change in entropy. 5.4 PF4/Polyphosphates (polyP) Complex Antigenicity and Interaction with Escherichia coli (E. coli, Paper IV – PF4/polyP) PolyP with chain lengths of 45 Pi and 75 Pi induced remarkable secondary structural changes in the PF4 molecule, thereby exposing the epitope recognized by anti-PF4/heparin antibodies. The induced conformational changes were similar to the changes induced by the defined heparins. Again a high binding enthalpy was observed but here in connection with a positive change in entropy. Further we showed that polyP (≥45 Pi) enhance PF4 binding to the surface of Gram negative E. coli at intermediate concentration and disrupt the binding at elevated polyP concentrations. The increased amounts of PF4 on the bacterial surface also improved the binding of anti-PF4/heparin antibodies and thereby the phagocytosis of the bacteria by poly¬morpho¬nuclear leucocytes. 5.5 Nucleic acid based Aptamers induce structural Changes in the PF4 Molecule (Paper V – PF4/Aptamer) Nucleic acids are another class of molecules containing phosphate groups. Especially after cell damage their extra¬cellular concentration can be locally quite high (>2 mg/ml). We found that certain aptamers form complexes with PF4 and thereby inducing anti-PF4/aptamer antibodies which cross-react with PF4/heparin complexes. Moreover by CD spectroscopy we showed that the protein C-aptamer caused similar secondary structural changes of PF4 like heparin, but already at much lower concentration. The maximally induced changes by the protein-C aptamer were even higher and persisted over a broader concentration range. 5.6 Protamine Interaction with Heparin (Paper VI – PS/Heparin) After the intensive investigation of the complex formation between PF4 and many different classes of PA we assessed another protein for structural changes upon complex formation with heparin. Protamine (PS) a protein in routinely used in post-cardiac surgery to reverse the anticoagulant effects of heparin was found to unfold but not to refold with increasing concentration of PA in solution. 5.7 Conclusion and Outlook When starting this thesis, it was believed that repetitive structures formed by PF4 on a heparin chain mold the epitope recognized by antibodies inducing HIT. These repetitive structures might exhibit similarities with viral capsids and are therefore recognized by the immune system of some patients. We found that induced by the close approximation PF4 changes its conformation, thereby exposing a neoepitope. The conserved positively charged amino acids of the heparin binding site and the involvement of these amino acids in the binding to lipid A confirm our hypothesis of PF4 as part of an ancient immune-mediated host defense mechanism. As possible consequence of the “primitive mechanism of defense” the highly variable O-antigens of LPS might have significantly contributed to an efficient escape mechanism by hiding the structures that made the bacteria vulnerable. In turn polyP might be an adaption of the host improve pathogen recognition by PF4 and further by antibodies inducing phagocytosis of the PF4-marked objects. Although shown only for PF4 and PS, our findings might be applicable to other proteins that also express epitopes upon changes in their secondary structure. Our physicochemical methods may further be applied: i. to drug development for the prediction of antigenicity induced by polyanionic drugs, ii. to guide the development of synthetic heparins and other polyanion based drugs, e.g. aptamers, that do not lead to HIT and iii. to provide relevant aspects for other biological functions of heparins.
Impurity ions pose a potentially serious threat to fusion plasma performance by affecting the confinement in various, usually deleterious, ways. Due to the creation of helium ash during fusion reactions and the interaction of the plasma with the wall components, which makes it possible for heavy ions to penetrate into the core plasma, impurities can intrinsically not be avoided. Therefore, it is essential to study their behaviour in the fusion plasma in detail. Within the framework of this thesis, different problems arising in connection with impurities have been investigated. 1. Collisional damping of zonal flows in tokamkas: The effect of impurities on the collisional damping of zonal flows is investigated. Since the Coulomb collision frequency increases with increasing ion charge, heavy, highly charged impurities play an important role in this process. The effect of such impurities on the linear response of the plasma to an external potential perturbation, as caused by zonal flows, is calculated with analytical methods and compared with numerical simulations, resulting in good agreement. 2. Impurity transport driven by microturbulence in tokamaks: Fine scale turbulence driven by microinstabilities is a source of particle and heat transport in a fusion reactor. A semi-analytical model is presented describing the resulting impurity fluxes and the stability boundary of the underlying mode. The results are compared with numerical simulations. Both the impurity flux and the stability boundary are found to depend strongly on the plasma parameters such as the impurity density and the temperature gradient. 3. Pfirsch-Schlüter transport in stellarators: Due to geometry effects, collisional transport plays a much more prominent role in stellarators than in tokamaks. Analytical expressions for the particle and heat fluxes in an impure, collisional plasma are derived from first principles. Contrary to the tokamak case, where collisional transport is exclusively caused directly by friction, in stellarators an additional source of transport exists, namely pressure anisotropy. Since this term is, contrary to the contribution from friction, non-ambipolar, it plays an important role regarding the ambipolar electric field. Furthermore, the behaviour of heavy impurities in the presence of strong radial temperature and density gradients is studied, which lead to a redistribution of the impurities on the flux surfaces. As a consequence, the radial impurity flux is decreased considerably compared with a plasma in which the impurities are evenly distributed on the flux surfaces.
The thesis deals with ions stored in an electrostatic ion beam trap. In the first part of the thesis the so-called self-synchronization effect is discussed. It is demonstrated that the time a bunch of injected ions is conserved by the self-synchronization effect depends on the number of injected ions. In the second part of the thesis the cooling of small anionic cobalt and copper clusters is addressed. Measurements on anionic copper clusters consisting of four to seven atoms are presented and the decay of hot clusters is observed in order to draw conclusions on the internal temperature and the cooling process itself. Afterwards measurements on Co4- are discussed and a measurement scheme based on laser induced delayed electron emission is presented enabling to monitor the internal energy distribution of the clusters over storage time in a temperature-controlled environment. The cooling of initially hot clusters as well as the heating of initially cold clusters were observed.
In the present work, mass determinations of the eleven neutron-deficient nuclides (99-109)Cd, of ten neutron-rich silver nuclides (112-114,121,123)Ag, and seven neutron-rich cadmium nuclides (114,120,122-124,126,128)Cd are reported. Due to the clean production of the neutron-deficient nuclides it was possible to reduce the experimental uncertainties down to 2 keV, whereas the measurements of neutron-rich nuclides were hampered by the presence of contaminations from more stable In and Cs nuclides. In the case of 99Cd and 123Ag the masses were determined for the first time and for the other nuclides the mass uncertainties could be reduced by up to a factor of 50 as in the case of 100Cd. In the case of a potential isomeric mixture as for (115,117,119)Ag and 123Cd, where no assignment to either the ground state or the excited state was possible, the experimental results were adjusted accordingly. Afterwards all results were included in the framework of the atomic-mass evaluation and thus linked and compared with other experimental data. In the case of the neutron-deficient Cd nuclides a conflict between the mass values obtained in the present work and those published by the JYFLTRAP group could be solved by performing an atomic-mass evaluation. These mass measurements are an important step towards an understanding of the physics of the rp process that will enable a more reliable determination of the composition of the produced material at A = 99. It has been shown that the mass of 99Cd strongly affects the A = 99 production in an X-ray burst model, and that uncertainties have been significantly reduced from more than an order of magnitude to about a factor of 3. The dominant source of uncertainty is now the mass of 100In. In principle, other uncertainties will also contribute. These include those of masses of lighter Cd isotopes, where similar rp-process branchpoints occur and which might affect feeding into the 99Cd branchpoint. In addition, nuclear reaction rate uncertainties will also play a role. However, as reaction rates affect branchings in a linear fashion, while mass differences enter exponentially, mass uncertainties will tend to dominate. Also, which reaction rates are important depends largely on nuclear masses. For example, for low Sp(100In) a (p,γ)-(γ,p) equilibrium will be established between 99Cd and 100In and the 100In(p,γ) reaction rate would affect the A = 99 production, while for larger Sp(100In) the 99Cd(p,γ) reaction rate might be more relevant. Therefore, the mass uncertainties should be addressed first. The presented results are relevant for any rp-process scenario with a reaction flow through the 99Cd region. Here, an X-ray burst model has been used to investigate in detail the impact of the present measurements on such an rp process. The νp process in core collapse supernovae might be another possible scenario for an rp process in the 99Cd region. It it is planed to also explore whether in that case mass uncertainties have a similar impact on the final composition. On the neutron-rich side of the valley of stability for the Cd and Ag chains of nuclides, the r process has not yet been reached. Further technical development on suppression of contaminants are required. This includes improvements on the ISOLDE side, e.g., by improving the selectivity of the transfer line or on the ISOLTRAP setup by implementing an electrostatic ion beam trap for a fast and efficient isobaric selection. Nevertheless the obtained results contribute to the knowledge of nuclear structure. The trends in the two-neutron separation-energy S2n and the interaction between the last neutrons and last protons ΔVpn were corrected to more smooth evolutions, as already seen in other regions of the nuclear chart. The strongest corrections have been observed for even-N nuclides, were more new experimental data are available. Thus, new measurements on odd-N nuclides are suggested. This also is underlined by the trends observed in the Garvey-Kelson relations for the neutron-rich Cd nuclides. Furthermore, it has been shown, that the prominent structure of the ΔVpn for an entire chain of nuclides including inflexion points can be reproduced by using simple relations between quantum numbers of the occupied orbits. This approach connects ten values for each nuclide with only one adjusted parameter. This has been investigated for 63 ΔVpn values of even-even nuclides in the vicinity of Z = 50 and 50 ≤ N ≤ 82. The simple model works remarkably well for the elements Cd, Sn, and Te. Small deviation have been observed for the Xe and Pd nuclides which were explained with the limitations of the model to the vicinity of the close shells, where the nuclides have only few valence protons and neutrons.
Diese Arbeit untersucht experimentell den Einfluss des metastabilen Zustandes Xe(1s3) und des Resonanzzustandes Xe(1s2) auf die VUV-Strahlungserzeugung in Helium-Xenon-Glimmentladungen (He:Xe = 98:2). Für die Bestimmung der Atomdichten wurde eine experimentelle Anordnung geschaffen, mit der, basierend auf der Methode der Laser-Atom-Absorptionsspektroskopie, orts- und zeitaufgelöste Messungen von optischen Dichten im Säulenplasma durchgeführt wurden. Als Hintergrundstrahlungsquelle kam ein durchstimmbarer Diodenlaser zum Einsatz. Die bereitgestellten Laserwellenlängen von 820 nm bzw. 826 nm entsprechen optischen Übergängen zwischen den Xenonzuständen 6s' 1/2[1/2]0 --> 6p' 1/2[3/2]1 (1s3 --> 2p4) und 6s' 1/2[1/2]1 --> 6p' 1/2[1/2]1 (1s2 --> 2p2).
Den Ausgangspunkt der Untersuchungen stellte die Messung der Absorptionslinienprofile beider Nahinfrarot-Übergänge dar. In Abhängigkeit von den Entladungsparametern Gasdruck, Entladungsstrom und Betriebsweise (Gleichstrom-, gepulste und Wechselstromentladung) wurden daraus die Dichten der angeregten Atome auf der Entladungsachse ermittelt. Durch die Analyse des Abklingens der Besetzungsdichten im Afterglow von gepulst betriebenen Entladungen mit Hilfe eines Systems von gekoppelten Ratengleichungen konnten die dominanten Stoßprozesse für die betrachteten Zustände identifiziert werden. Erstmalig ist in dieser Arbeit die radiale Verteilung der angeregten Spezies Xe(1s3) und Xe(1s2) in He-Xe-Glimmentladungen untersucht worden. Damit ist die VUV-Strahlungsleistung der 129 nm-Linie aus der Dichteverteilung der Resonanzatome ermittelbar.