Early-type galaxies as probes of galaxy formation and cosmology

The goal of this thesis is to analyze the possibility of using early-type galaxies to place evolutionary and cosmological constraints, by both disentangling what is the main driver of ETGs evolution between mass and environment, and developing a technique to constrain H(z) and the cosmological parameters studying the ETGs age-redshift relation. The (U-V) rest-frame color distribution is studied as a function of mass and environment for two sample of ETGs up to z=1, extracted from the zCOSMOS survey with a new selection criterion. The color distributions and the slopes of the color-mass and color-environment relations are studied, finding a strong dependence on mass and a minor dependence on environment. The spectral analysis performed on the D4000 and Hδ features gives results validating the previous analysis. The main driver of galaxy evolution is found to be the galaxy mass, the environment playing a subdominant but non negligible role. The age distribution of ETGs is also analyzed as a function of mass, providing strong evidences supporting a downsizing scenario. The possibility of setting cosmological constraints studying the age-redshift relation is studied, discussing the relative degeneracies and model dependencies. A new approach is developed, aiming to minimize the impact of systematics on the “cosmic chronometer” method. Analyzing theoretical models, it is demonstrated that the D4000 is a feature correlated almost linearly with age at fixed metallicity, depending only minorly on the models assumed or on the SFH chosen. The analysis of a SDSS sample of ETGs shows that it is possible to use the differential D4000 evolution of the galaxies to set constraints to cosmological parameters in an almost model-independent way. Values of the Hubble constant and of the dark energy EoS parameter are found, which are not only fully compatible, but also with a comparable error budget with the latest results.

Investigations on maar-diatreme volcanoes by inversion of magnetic and gravity data from the Eifel area, Germany

A study of maar-diatreme volcanoes has been perfomed by inversion of gravity and magnetic data. The geophysical inverse problem has been solved by means of the damped nonlinear least-squares method. To ensure stability and convergence of the solution of the inverse problem, a mathematical tool, consisting in data weighting and model scaling, has been worked out. Theoretical gravity and magnetic modeling of maar-diatreme volcanoes has been conducted in order to get information, which is used for a simple rough qualitative and/or quantitative interpretation. The information also serves as a priori information to design models for the inversion and/or to assist the interpretation of inversion results. The results of theoretical modeling have been used to roughly estimate the heights and the dip angles of the walls of eight Eifel maar-diatremes — each taken as a whole. Inversemodeling has been conducted for the Schönfeld Maar (magnetics) and the Hausten-Morswiesen Maar (gravity and magnetics). The geometrical parameters of these maars, as well as the density and magnetic properties of the rocks filling them, have been estimated. For a reliable interpretation of the inversion results, beside the knowledge from theoretical modeling, it was resorted to other tools such like field transformations and spectral analysis for complementary information. Geologic models, based on thesynthesis of the respective interpretation results, are presented for the two maars mentioned above. The results gave more insight into the genesis, physics and posteruptive development of the maar-diatreme volcanoes. A classification of the maar-diatreme volcanoes into three main types has been elaborated. Relatively high magnetic anomalies are indicative of scoria cones embeded within maar-diatremes if they are not caused by a strong remanent component of the magnetization. Smaller (weaker) secondary gravity and magnetic anomalies on the background of the main anomaly of a maar-diatreme — especially in the boundary areas — are indicative for subsidence processes, which probably occurred in the late sedimentation phase of the posteruptive development. Contrary to postulates referring to kimberlite pipes, there exists no generalized systematics between diameter and height nor between geophysical anomaly and the dimensions of the maar-diatreme volcanoes. Although both maar-diatreme volcanoes and kimberlite pipes are products of phreatomagmatism, they probably formed in different thermodynamic and hydrogeological environments. In the case of kimberlite pipes, large amounts of magma and groundwater, certainly supplied by deep and large reservoirs, interacted under high pressure and temperature conditions. This led to a long period phreatomagmatic process and hence to the formation of large structures. Concerning the maar-diatreme and tuff-ring-diatreme volcanoes, the phreatomagmatic process takes place due to an interaction between magma from small and shallow magma chambers (probably segregated magmas) and small amounts of near-surface groundwater under low pressure and temperature conditions. This leads to shorter time eruptions and consequently to structures of smaller size in comparison with kimberlite pipes. Nevertheless, the results show that the diameter to height ratio for 50% of the studied maar-diatremes is around 1, whereby the dip angle of the diatreme walls is similar to that of the kimberlite pipes and lies between 70 and 85°. Note that these numerical characteristics, especially the dip angle, hold for the maars the diatremes of which — estimated by modeling — have the shape of a truncated cone. This indicates that the diatreme can not be completely resolved by inversion.

Climate signatures in corals of the tropical-temperate transition zone (Late Miocene, Crete/Greece)

The present study describes a Late Miocene (early Tortonian - early Messinian) transitional carbonate system that combines elements of tropical and cool-water carbonate systems (Irakleion Basin, island of Crete, Greece). As documented by stratal geometries, the submarine topography of the basin was controlled by tilting blocks. Coral reefs formed by Porites and Tarbellastrea occurred in a narrow clastic coastal belt along a „central Cretan landmass“, and steep escarpments formed by faulting. Extensive covers of level-bottom communities existed in a low-energy environment on the gentle dip-slope ramps of the blocks that show the widest geographical distribution within the basin. Consistent patterns of landward and basinward shift of coastal onlap in all outcrop studies reveal an overriding control of 3rd and 4th order sea level changes on sediment dynamics and facies distributions over block movements. An increasingly dry climate and the complex submarine topography of the fault block mosaic kept sediment and nutrient discharge at a minimum. The skeletal limestone facies therefore reflects oligotrophic conditions and a sea surface temperature (SST) near the lower threshold temperature of coral reefs in a climatic position transitional between the tropical coral reef belt and the temperate zone. Stable isotope records (δ18O, δ13C) from massiv, exceptionally preserved Late Miocene aragonite coral skeletons reflect seasonal changes in sea surface temperature and symbiont autotrophy. Spectral analysis of a 69 years coral δ18O record reveals significant variance at interannual time scales (5-6 years) that matches the present-day eastern Mediterranean climate variability controlled by the Arctic Oscillation/North Atlantic Oscillation (AO/NAO), the Northern Hemisphere’s dominant mode of atmospheric variability. Supported by simulations with a complex atmospheric general circulation model coupled to a mixed-layer ocean model, it is suggested, that climate dynamics in the eastern Mediterranean and central Europe reflect atmospheric variability related to the Icelandic Low 10 million years ago. Usually, Miocene corals are transformed in calcite spar in geological time and isotope values are reset by diagenetic alteration. It is demonstrated that the relicts of growth bands represent an intriguing source of information for the growth conditions of fossil corals. Recrystallized growth bands were measured systematically in massive Porites from Crete. The Late Miocene corals were growing slowly with 2-4 mm/yr, compatible with present-day Porites from high latitude reefs, a relationship that fits the position of Crete at the margin of the Miocene tropical reef belt. Over Late Miocene time (Tortonian - early Messinian) growth rates remained remarkably constant, and if the modern growth temperature relationship for massive Porites applies to the Neogene, minimum (winter) SST did not exceed 19-21°C.

Accretion disk winds in active galactic nuclei: an X-ray view

This Thesis focuses on the X-ray study of the inner regions of Active Galactic Nuclei, in particular on the formation of high velocity winds by the accretion disk itself. Constraining AGN winds physical parameters is of paramount importance both for understanding the physics of the accretion/ejection flow onto supermassive black holes, and for quantifying the amount of feedback between the SMBH and its environment across the cosmic time. The sources selected for the present study are BAL, mini-BAL, and NAL QSOs, known to host high-velocity winds associated to the AGN nuclear regions. Observationally, a three-fold strategy has been adopted: - substantial samples of distant sources have been analyzed through spectral, photometric, and statistical techniques, to gain insights into their mean properties as a population; - a moderately sized sample of bright sources has been studied through detailed X-ray spectral analysis, to give a first flavor of the general spectral properties of these sources, also from a temporally resolved point of view; - the best nearby candidate has been thoroughly studied using the most sophisticated spectral analysis techniques applied to a large dataset with a high S/N ratio, to understand the details of the physics of its accretion/ejection flow. There are three main channels through which this Thesis has been developed: - [Archival Studies]: the XMM-Newton public archival data has been extensively used to analyze both a large sample of distant BAL QSOs, and several individual bright sources, either BAL, mini-BAL, or NAL QSOs. - [New Observational Campaign]: I proposed and was awarded with new X-ray pointings of the mini-BAL QSOs PG 1126-041 and PG 1351+640 during the XMM-Newton AO-7 and AO-8. These produced the biggest X-ray observational campaign ever made on a mini-BAL QSO (PG 1126-041), including the longest exposure so far. Thanks to the exceptional dataset, a whealth of informations have been obtained on both the intrinsic continuum and on the complex reprocessing media that happen to be in the inner regions of this AGN. Furthermore, the temporally resolved X-ray spectral analysis field has been finally opened for mini-BAL QSOs. - [Theoretical Studies]: some issues about the connection between theories and observations of AGN accretion disk winds have been investigated, through theoretical arguments and synthetic absorption line profiles studies.

The coupling between electron transfer and Protein/Solvent Dynamics in Photosynthetic Reaction Centers: Spectroscopic Studies in Amorphous Matrices

We investigated at the molecular level protein/solvent interactions and their relevance in protein function through the use of amorphous matrices at room temperature. As a model protein, we used the bacterial photosynthetic reaction center (RC) of Rhodobacter sphaeroides, a pigment protein complex which catalyzes the light-induced charge separation initiating the conversion of solar into chemical energy. The thermal fluctuations of the RC and its dielectric conformational relaxation following photoexcitation have been probed by analyzing the recombination kinetics of the primary charge-separated (P+QA-) state, using time resolved optical and EPR spectroscopies. We have shown that the RC dynamics coupled to this electron transfer process can be progressively inhibited at room temperature by decreasing the water content of RC films or of RC-trehalose glassy matrices. Extensive dehydration of the amorphous matrices inhibits RC relaxation and interconversion among conformational substates to an extent comparable to that attained at cryogenic temperatures in water-glycerol samples. An isopiestic method has been developed to finely tune the hydration level of the system. We have combined FTIR spectral analysis of the combination and association bands of residual water with differential light-minus-dark FTIR and high-field EPR spectroscopy to gain information on thermodynamics of water sorption, and on structure/dynamics of the residual water molecules, of protein residues and of RC cofactors. The following main conclusions were reached: (i) the RC dynamics is slaved to that of the hydration shell; (ii) in dehydrated trehalose glasses inhibition of protein dynamics is most likely mediated by residual water molecules simultaneously bound to protein residues and sugar molecules at the protein-matrix interface; (iii) the local environment of cofactors is not involved in the conformational dynamics which stabilizes the P+QA-; (iv) this conformational relaxation appears to be rather delocalized over several aminoacidic residues as well as water molecules weakly hydrogen-bonded to the RC.

Generating vegetation-spectra as a basis for global monitoring of annual vegetation cycles using DOAS satellite observations

Vegetation-cycles are of general interest for many applications. Be it for harvest-predictions, global monitoring of climate-change or as input to atmospheric models.rnrnCommon Vegetation Indices use the fact that for vegetation the difference between Red and Near Infrared reflection is higher than in any other material on Earth’s surface. This gives a very high degree of confidence for vegetation-detection.rnrnThe spectrally resolving data from the GOME and SCIAMACHY satellite-instrumentsrnprovide the chance to analyse finer spectral features throughout the Red and Near Infrared spectrum using Differential Optical Absorption Spectroscopy (DOAS). Although originally developed to retrieve information on atmospheric trace gases, we use it to gain information on vegetation. Another advantage is that this method automatically corrects for changes in the atmosphere. This renders the vegetation-information easily comparable over long time-spans.rnThe first results using previously available reference spectra were encouraging, but also indicated substantial limitations of the available reflectance spectra of vegetation. This was the motivation to create new and more suitable vegetation reference spectra within this thesis.rnThe set of reference spectra obtained is unique in its extent and also with respect to its spectral resolution and the quality of the spectral calibration. For the first time, this allowed a comprehensive investigation of the high-frequency spectral structures of vegetation reflectance and of their dependence on the viewing geometry.rnrnThe results indicate that high-frequency reflectance from vegetation is very complex and highly variable. While this is an interesting finding in itself, it also complicates the application of the obtained reference spectra to the spectral analysis of satellite observations.rnrnThe new set of vegetation reference spectra created in this thesis opens new perspectives for research. Besides refined satellite analyses, these spectra might also be used for applications on other platforms such as aircraft. First promising studies have been presented in this thesis, but the full potential for the remote sensing of vegetation from satellite (or aircraft) could bernfurther exploited in future studies.

Towards the 3D attenuation imaging of active volcanoes: methods and tests on real and simulated data

The purpose of my PhD thesis has been to face the issue of retrieving a three dimensional attenuation model in volcanic areas. To this purpose, I first elaborated a robust strategy for the analysis of seismic data. This was done by performing several synthetic tests to assess the applicability of spectral ratio method to our purposes. The results of the tests allowed us to conclude that: 1) spectral ratio method gives reliable differential attenuation (dt*) measurements in smooth velocity models; 2) short signal time window has to be chosen to perform spectral analysis; 3) the frequency range over which to compute spectral ratios greatly affects dt* measurements. Furthermore, a refined approach for the application of spectral ratio method has been developed and tested. Through this procedure, the effects caused by heterogeneities of propagation medium on the seismic signals may be removed. The tested data analysis technique was applied to the real active seismic SERAPIS database. It provided a dataset of dt* measurements which was used to obtain a three dimensional attenuation model of the shallowest part of Campi Flegrei caldera. Then, a linearized, iterative, damped attenuation tomography technique has been tested and applied to the selected dataset. The tomography, with a resolution of 0.5 km in the horizontal directions and 0.25 km in the vertical direction, allowed to image important features in the off-shore part of Campi Flegrei caldera. High QP bodies are immersed in a high attenuation body (Qp=30). The latter is well correlated with low Vp and high Vp/Vs values and it is interpreted as a saturated marine and volcanic sediments layer. High Qp anomalies, instead, are interpreted as the effects either of cooled lava bodies or of a CO2 reservoir. A pseudo-circular high Qp anomaly was detected and interpreted as the buried rim of NYT caldera.

Multicentre study for a robust protocol in single-voxel spectroscopy: quantification of MRS signals by time-domain fitting algorithms

Magnetic Resonance Spectroscopy (MRS) is an advanced clinical and research application which guarantees a specific biochemical and metabolic characterization of tissues by the detection and quantification of key metabolites for diagnosis and disease staging. The "Associazione Italiana di Fisica Medica (AIFM)" has promoted the activity of the "Interconfronto di spettroscopia in RM" working group. The purpose of the study is to compare and analyze results obtained by perfoming MRS on scanners of different manufacturing in order to compile a robust protocol for spectroscopic examinations in clinical routines. This thesis takes part into this project by using the GE Signa HDxt 1.5 T at the Pavillion no. 11 of the S.Orsola-Malpighi hospital in Bologna. The spectral analyses have been performed with the jMRUI package, which includes a wide range of preprocessing and quantification algorithms for signal analysis in the time domain. After the quality assurance on the scanner with standard and innovative methods, both spectra with and without suppression of the water peak have been acquired on the GE test phantom. The comparison of the ratios of the metabolite amplitudes over Creatine computed by the workstation software, which works on the frequencies, and jMRUI shows good agreement, suggesting that quantifications in both domains may lead to consistent results. The characterization of an in-house phantom provided by the working group has achieved its goal of assessing the solution content and the metabolite concentrations with good accuracy. The goodness of the experimental procedure and data analysis has been demonstrated by the correct estimation of the T2 of water, the observed biexponential relaxation curve of Creatine and the correct TE value at which the modulation by J coupling causes the Lactate doublet to be inverted in the spectrum. The work of this thesis has demonstrated that it is possible to perform measurements and establish protocols for data analysis, based on the physical principles of NMR, which are able to provide robust values for the spectral parameters of clinical use.

Indagine sperimentale sulla risposta dinamica di provini piatti in lega d'alluminio sottoposti a diverse tipologie di eccitazione vibratoria non-gaussiana

Negli ultimi anni va sempre più affermandosi l’idea che nei test a fatica utilizzati in ambito industriale per testare la resistenza di numerosi prodotti, riprodurre profili vibratori con distribuzioni gaussiane non sia sufficientemente realistico. Nell’indagine sperimentale riportata in questo trattato vengono confrontati gli effetti generati da sollecitazioni leptocurtiche ottenute da misurazioni reali, con profili vibratori gaussiani a parità di RMS e forma della PSD (Power Spectral Density) verificando la validità della “Papoulis rule”. A partire da questi profili vibratori si è effettuata una progettazione ad hoc dalla quale sono stati ricavati dei provini piatti in lega di alluminio a cui è collegata una massa ausiliaria. Quest’ultimi montati a sbalzo su uno shaker elettrodinamico, sono caratterizzati da una variazione di sezione che localizza la sezione critica in prossimità dell’incastro. I provini sono stati inoltre caratterizzati attraverso prove a trazione e test accelerati a fatica, ricavandone la caratteristica a trazione del materiale ed il diagramma di Wohler. In seguito alla descrizione di tali prove viene riportata un’analisi dei provini sollecitati da due profili vibratori, uno gaussiano e uno ad elevato valore di kurtosis, monitorando tramite l’impiego di accelerometri i valori dell’eccitazione e la risposta. Vengono inoltre verificati i valori delle deformazioni dovute alle sollecitazioni imposte collocando due estensimetri in corrispondenza della sezione critica di due provini (uno per ogni tipologia di input).

Amphotericin B nano-formulations : development, characterisation and suitability for oral administration

In der Form von Nanokapseln (AmB-HST), Nanoemulsion beziehungsweise multilamellaren Vesikeln (MLV) wurden drei Amphotericin-B-Formulierungen für die orale Applikation entwickelt, charakterisiert und verglichen. Die neuartige homogene Nanokapsel-Formulierung des hydrophoben Polyen-Antimykotikums Amphotericin B wurde in Analogie zu einem für Simvastatin und andere Arzneistoffe etablierten Prozess aus der Reinsubstanz, Lezithin und Gelatine mit Hilfe des HST-Verfahrens hergestellt. Photometrische Untersuchungen zeigten, dass das Endprodukt aus Monomeren aufgebaut ist. Mittels Mikroskopie ließen sich die Aggregate vor der Umhüllung mit Lezithin und Gelatine im Ausgangsmaterial als individuelle kugelförmige Arzneistoffpartikel darstellen. Strukturuntersuchungen mit dynamischer licht streuung (DLS) zeigten eine enge Größenverteilung der verkapselten Partikel von ca. 1 µm. Die Struktur der Hülle der HST-Partikel wurde erstmalig mit Neutronenstreuung unter Verwendung der Deuterium-basierten Lösungsmittel kontrastmethode aufgeklärt. Durch die teilweise Kontrastmaskierung des Partikelkerns bei der Neutronenstreuung konnte die Lezithin-Gelatine-Hülle als eine dünne, 5,64 ± 0.18 nm dicke Schicht aufgelöst werden, welche der biologischen Lipidmembran ähnlich, im Vergleich aber geringfügig größer ist. Dieses Resultat eröffnet Wege für die Optimierung der Formulierung von pharmazeutischen Nanopartikeln, z.B. durch Oberflächenmodifizierungen. Weitere Untersuchungen mittels Kleinwinkelneutronenstreuung unter Verwendung der D-Kontrastvariation deuten darauf hin, dass die Komponenten der Nanokapseln nicht den gleichen Masseschwerpunkt haben, sondern asymmetrisch aufgebaut sind und dass die stärker streuenden Domänen weiter außen liegen. Die Partikel sind im Vergleich zu Liposomen dichter. In-Vitro Freisetzungsstudien belegen das Solubilisierungsvermögen des HST-Systems, wonach die Freisetzung des Arzneistoffes aus der Formulierung zu allen gemessenen Zeitpunkten höher als diejenige der Reinsubstanz war. rnDie Nanoemulsion-Formulierung von Amphotericin B wurde mit einem Öl und Tensid system, jedoch mit unterschiedlichen Co-Solvenzien, erfolgreich entwickelt. Gemäß der Bestimmung der Löslichkeit in verschiedenen Hilfsstoffen erwies sich der Arzneistoff Amphotericin B als nicht-lipophil, gleichzeitig aber auch als nicht-hydrophil. Die zur Ermittlung der für die Emulsionsbildung notwendigen Hilfstoffkonzentrationen erstellten ternären Diagramme veranschaulichten, dass hohe Öl- und Tensidgehalte zu keiner Emulsionsbildung führten. Dementsprechend betrug der höchste Ölgehalt 10%. Die Tröpfchengröße wuchs mit zunehmender Tensidkonzentration, wobei die Co-Solventmenge der Propylenglykol-haltigen Nanoemulsion indirekt verringert wurde. Für die Transcutol®P-haltige Nanoemulsion hingegen wurde das Gegenteil beobachtet, nämlich eine Abnahme der Tröpfchengröße bei steigenden Tensidkonzentrationen. Durch den Einschluss des Arzneistoffes wurde nicht die Viskosität der Formulierung, sondern die Tröpfchengröße beeinflusst. Der Wirkstoffeinschluss führte zu höheren Tröpfchengrößen. Mit zunehmender Propylenglykolkonzentration wurde der Wirkstoffgehalt erhöht, mit zunehmender Transcutol®P-Konzentration dagegen vermindert. UV/VIS-spektroskopische Analysen deuten darauf hin, dass in beiden Formulierungen Amphotericin B als Monomer vorliegt. Allerdings erwiesen sich die Formulierungen Caco-2-Zellen und humanen roten Blutkörperchen gegenüber als toxisch. Da die Kontrollproben eine höhere Toxizität als die wirkstoffhaltigen Formulierungen zeigten, ist die Toxizität nicht nur auf Amphotericin, sondern auch auf die Hilfsstoffe zurückzuführen. Die solubilisierte Wirkstoffmenge ist in beiden Formulierungen nicht ausreichend im Hinblick auf die eingesetzte Menge an Hilfsstoff nach WHO-Kriterien. Gemäß diesen Untersuchungen erscheinen die Emulsions-Formulierungen für die orale Gabe nicht geeignet. Dennoch sind Tierstudien notwendig, um den Effekt bei Tieren sowie die systemisch verfügbare Wirkstoffmenge zu ermitteln. Dies wird bestandskräftige Schlussfolgerungen bezüglich der Formulierung und Aussagen über mögliche Perspektiven erlauben. Nichtsdestotrotz sind die Präkonzentrate sehr stabil und können bei Raumtemperatur gelagert werden.rnDie multilamellar-vesikulären Formulierungen von Amphotericin B mit ungesättigten und gesättigten neutralen Phospholipiden und Cholesterin wurden erfolgreich entwickelt und enthielten nicht nur Vesikel, sondern auch zusätzliche Strukturen bei zunehmender Cholesterinkonzentration. Mittels Partikelgrößenanalyse wurden bei den Formulierungen mit gesättigten Lipiden Mikropartikel detektiert, was abhängig von der Alkylkettenlänge war. Mit dem ungesättigten Lipid (DOPC) konnten hingegen Nanopartikel mit hinreichender Verkapselung und Partikelgrößenverteilung gebildet werden. Die Ergebnisse der thermischen und FTIR-spektroskopischen Analyse, welche den Einfluss des Arzneistoffes ausschließen ließen, liefern den Nachweis für die mögliche, bereits in der Literatur beschriebene Einlagerung des Wirkstoffs in lipid- und/oder cholesterinreiche Membranen. Mit Hilfe eines linearen Saccharosedichtegradienten konnte die Formulierung in Vesikel und Wirkstoff-Lipid-Komplexe nach bimodaler Verteilung aufgetrennt werden, wobei der Arzneistoff stärker mit den Komplexen als mit den Vesikeln assoziiert ist. Bei den Kleinwinkelneutronenstreu-Experimenten wurde die Methode der Kontrastvariation mit Erfolg angewendet. Dabei konnte gezeigt werden, dass Cholesterol in situ einen Komplex mit Amphotericin B bildet. Diesen Sachverhalt legt unter anderem die beobachtete Differenz in der äquivalenten Streulängendichte der Wirkstoff-Lipid- und Wirkstoff-Lipid-Cholesterin-haltigen kleinen unilamellaren Vesikeln nahe. Das Vorkommen von Bragg-Peaks im Streuprofil weist auf Domänen hin und systematische Untersuchungen zeigten, dass die Anzahl der Domänen mit steigendem Cholesteringehalt zunimmt, ab einem bestimmten Grenzwert jedoch wieder abnimmt. Die Domänen treten vor allem nahe der Außenfläche der Modellmembran auf und bestätigen, dass der Wirkstoff in den Cholesterinreichen Membranen vertikal eingelagert ist. Die Formulierung war sowohl Caco-2-Zellen als auch humanen roten Blutkörperchen gegenüber nicht toxisch und erwies sich unter Berücksichtigung der Aufnahme in Caco-2-Zellen als vielversprechend für die orale Applikation. Die Formulierung zeigt sich somit aussichtsreich und könnte in Tabletten weiterverarbeitet werden. Ein Filmüberzug würde den Wirkstoff gegen die saure Umgebung im Magen schützen. Für die Bestimmung der systemischen Verfügbarkeit der Formulierung sind Tierstudien notwendig. Die entwickelten multilamellaren Formulierungen einschließlich der Wirkstoff-Cholesterin-Komplexe bieten somit gute Aussichten auf die mögliche medizinische Anwendung. rnrn

Multifrequency VLBA observations of two compact symmetric objects

In this thesis the results of the multifrequency VLBA observations of the GPS 1944+5448 and the HFP J0111+3906 are presented. They are compact objects smaller than about 100 pc, completely embedded in the host galaxy. The availability of multi-epoch VLBI observations spanning more than 10 years, allowed us to compute the hot spot advance speed in order to obtain the kinematic age of both sources. Both radio sources are young, in agreement with the idea that they are in an early evolutionary stage. The spectral analysis of each source component, such as the lobes, the hot spots, the core and the jets, making a comparison with the theoretical ones is described. In addition the physical parameters derived from VLBA images as the magnetic field, the luminosity, the energy and the ambient medium density of both sources are discussed.

Misure di rumore in corrente in un circuito per la generazione di un campo magnetico stabile

Questo lavoro di Tesi, svolto nell’ambito dell’esperimento BEC3 presso il LENS, costituisce il primo approccio al problema della stabilizzazione del campo magnetico di bias in una trappola per atomi ultra-freddi. Stabilizzare il campo magnetico generato da una coppia di bobine si traduce nello stabilizzare la corrente che le attraversa e il primo passo verso la soluzione di questo problema consiste nello stimare lo spettro di potenza del rumore in corrente del circuito. A questo scopo è stata misurata la PSD (Power Spectral Density) del segnale ai capi di diversi sensori per alcuni valori di corrente erogata da due diversi alimentatori. La PSD è stata misurata sia in maniera diretta, che indiretta, attraverso la trasformata di Fourier della Funzione di Autocorrelazione del segnale, misurata nelle stesse condizioni descritte. I dati raccolti costituiscono la base da cui partire per la progettazione e la realizzazione del circuito di stabilizzazione.

Mission synthesis of sine-on-random excitations for accelerated vibration qualification testing

In most real-life environments, mechanical or electronic components are subjected to vibrations. Some of these components may have to pass qualification tests to verify that they can withstand the fatigue damage they will encounter during their operational life. In order to conduct a reliable test, the environmental excitations can be taken as a reference to synthesize the test profile: this procedure is referred to as “test tailoring”. Due to cost and feasibility reasons, accelerated qualification tests are usually performed. In this case, the duration of the original excitation which acts on the component for its entire life-cycle, typically hundreds or thousands of hours, is reduced. In particular, the “Mission Synthesis” procedure lets to quantify the induced damage of the environmental vibration through two functions: the Fatigue Damage Spectrum (FDS) quantifies the fatigue damage, while the Maximum Response Spectrum (MRS) quantifies the maximum stress. Then, a new random Power Spectral Density (PSD) can be synthesized, with same amount of induced damage, but a specified duration in order to conduct accelerated tests. In this work, the Mission Synthesis procedure is applied in the case of so-called Sine-on-Random vibrations, i.e. excitations composed of random vibrations superimposed on deterministic contributions, in the form of sine tones typically due to some rotating parts of the system (e.g. helicopters, engine-mounted components, …). In fact, a proper test tailoring should not only preserve the accumulated fatigue damage, but also the “nature” of the excitation (in this case the sinusoidal components superimposed on the random process) in order to obtain reliable results. The classic time-domain approach is taken as a reference for the comparison of different methods for the FDS calculation in presence of Sine-on-Random vibrations. Then, a methodology to compute a Sine-on-Random specification based on a mission FDS is presented.

A study of extended radio galaxies in the Shapley concentration core

Extended cluster radio galaxies show different morphologies com- pared to those found isolated in the field. Indeed, symmetric double radio galaxies are only a small percentage of the total content of ra- dio loud cluster galaxies, which show mainly tailed morphologies (e.g. O’Dea & Owen, 1985). Moreover, cluster mergers can deeply affect the statistical properties of their radio activity. In order to better understand the morphological and radio activity differences of the radio galaxies in major mergeing and non/tidal-merging clusters, we performed a multifrequency study of extended radio galax- ies inside two cluster complexes, A3528 and A3558. They belong to the innermost region of the Shapley Concentration, the most massive con- centration of galaxy clusters (termed supercluster) in the local Universe, at average redshift z ≈ 0.043. We analysed low frequency radio data performed at 235 and 610 MHz with Giant Metrewave Radio Telescope (GMRT) and we combined them with proprietary and literature observations, in order to have a wide frequency range (150 MHz to 8.4 GHz) to perform the spectral analysis. The low frequency images allowed us to carry out a detailed study of the radio tails and diffuse emission found in some cases. The results in the radio band were also qualitatively compared with the X-ray information coming from XMM-Newton observations, in order to test the interaction between radio galaxies and cluster weather. We found that the brightest central galaxies (BCGs) in the A3528 cluster complex are powerful and present substantial emission from old relativistic plasma characterized by a steep spectrum (α > 2). In the light of observational pieces of evidence, we suggest they are possible re-started radio galaxies. On the other hand, the tailed radio galaxies trace the host galaxy motion with respect to the ICM, and our find- ings is consistent with the dynamical interpretation of a tidal interaction (Gastaldello et al. 2003). On the contrary, the BCGs in the A3558 clus- ter complex are either quiet or very faint radio galaxies, supporting the hypothesis that clusters mergers quench the radio emission from AGN.

Nanoscale switching characteristics of nearly tetragonal BiFeO3 thin films

We have investigated the nanoscale switching properties of strain-engineered BiFeO(3) thin films deposited on LaAlO(3) substrates using a combination of scanning probe techniques. Polarized Raman spectral analysis indicates that the nearly tetragonal films have monoclinic (Cc) rather than P4mm tetragonal symmetry. Through local switching-spectroscopy measurements and piezoresponse force microscopy, we provide clear evidence of ferroelectric switching of the tetragonal phase, but the polarization direction, and therefore its switching, deviates strongly from the expected (001) tetragonal axis. We also demonstrate a large and reversible, electrically driven structural phase transition from the tetragonal to the rhombohedral polymorph in this material, which is promising for a plethora of applications.