Análise de imagens na avaliação de danos mecânicos em sementes de soja

A injúria mecânica é um dos mais importantes fatores na redução da qualidade de sementes de soja. Neste contexto, este trabalho objetivou avaliar a influência da pressão de impacto e o teor de água em sementes, bem como a aplicabilidade da técnica de análise de imagens, na ocorrência de danos mecânicos em sementes de soja. Sementes das cultivares Vencedora e Monsoy 8001, com teores de água de 13% e 18%, foram submetidas a danos mecânicos, com a utilização de equipamento simulador de impactos (551,6 KPa e 965,3 KPa). Posteriormente, as sementes foram secas a 32ºC, até atingirem 12% de teor de água. Imediatamente após os impactos e após cinco meses de armazenamento, as sementes foram avaliadas pelos testes de tetrazólio e raios X. A pressão de impacto e o teor de água nas sementes exerceram efeitos diretos na severidade do dano mecânico, porém, o local do impacto exerceu maior influência do que aqueles fatores. A técnica de análise de imagens foi de grande utilidade na avaliação de danos mecânicos em sementes de soja, possibilitando a análise detalhada dos efeitos de diferentes fatores.

Brain activity and medical diagnosis: an EEG study

Abstract Background Despite new brain imaging techniques that have improved the study of the underlying processes of human decision-making, to the best of our knowledge, there have been very few studies that have attempted to investigate brain activity during medical diagnostic processing. We investigated brain electroencephalography (EEG) activity associated with diagnostic decision-making in the realm of veterinary medicine using X-rays as a fundamental auxiliary test. EEG signals were analysed using Principal Components (PCA) and Logistic Regression Analysis Results The principal component analysis revealed three patterns that accounted for 85% of the total variance in the EEG activity recorded while veterinary doctors read a clinical history, examined an X-ray image pertinent to a medical case, and selected among alternative diagnostic hypotheses. Two of these patterns are proposed to be associated with visual processing and the executive control of the task. The other two patterns are proposed to be related to the reasoning process that occurs during diagnostic decision-making. Conclusions PCA analysis was successful in disclosing the different patterns of brain activity associated with hypothesis triggering and handling (pattern P1); identification uncertainty and prevalence assessment (pattern P3), and hypothesis plausibility calculation (pattern P2); Logistic regression analysis was successful in disclosing the brain activity associated with clinical reasoning success, and together with regression analysis showed that clinical practice reorganizes the neural circuits supporting clinical reasoning.

Constitutive gene expression profile segregates toxicity in locally advanced breast cancer patients treated with high-dose hyperfractionated radical radiotherapy

[EN] Breast cancer patients show a wide variation in normal tissue reactions after radiotherapy. The individual sensitivity to x-rays limits the efficiency of the therapy. Prediction of individual sensitivity to radiotherapy could help to select the radiation protocol and to improve treatment results. The aim of this study was to assess the relationship between gene expression profiles of ex vivo un-irradiated and irradiated lymphocytes and the development of toxicity due to high-dose hyperfractionated radiotherapy in patients with locally advanced breast cancer. Raw data from microarray experiments were uploaded to the Gene Expression Omnibus Database http://www.ncbi.nlm.nih.gov/geo/ (GEO accession GSE15341). We obtained a small group of 81 genes significantly regulated by radiotherapy, lumped in 50 relevant pathways. Using ANOVA and t-test statistical tools we found 20 and 26 constitutive genes (0 Gy) that segregate patients with and without acute and late toxicity, respectively. Non-supervised hierarchical clustering was used for the visualization of results. Six and 9 pathways were significantly regulated respectively. Concerning to irradiated lymphocytes (2 Gy), we founded 29 genes that separate patients with acute toxicity and without it. Those genes were gathered in 4 significant pathways. We could not identify a set of genes that segregates patients with and without late toxicity. In conclusion, we have found an association between the constitutive gene expression profile of peripheral blood lymphocytes and the development of acute and late toxicity in consecutive, unselected patients. These observations suggest the possibility of predicting normal tissue response to irradiation in high-dose non-conventional radiation therapy regimens. Prospective studies with higher number of patients are needed to validate these preliminary results.

Statistical properties of Radio Halos and the re-acceleration model

Galaxy clusters occupy a special position in the cosmic hierarchy as they are the largest bound structures in the Universe. There is now general agreement on a hierarchical picture for the formation of cosmic structures, in which galaxy clusters are supposed to form by accretion of matter and merging between smaller units. During merger events, shocks are driven by the gravity of the dark matter in the diffuse barionic component, which is heated up to the observed temperature. Radio and hard-X ray observations have discovered non-thermal components mixed with the thermal Intra Cluster Medium (ICM) and this is of great importance as it calls for a “revision” of the physics of the ICM. The bulk of present information comes from the radio observations which discovered an increasing number of Mpcsized emissions from the ICM, Radio Halos (at the cluster center) and Radio Relics (at the cluster periphery). These sources are due to synchrotron emission from ultra relativistic electrons diffusing through µG turbulent magnetic fields. Radio Halos are the most spectacular evidence of non-thermal components in the ICM and understanding the origin and evolution of these sources represents one of the most challenging goal of the theory of the ICM. Cluster mergers are the most energetic events in the Universe and a fraction of the energy dissipated during these mergers could be channelled into the amplification of the magnetic fields and into the acceleration of high energy particles via shocks and turbulence driven by these mergers. Present observations of Radio Halos (and possibly of hard X-rays) can be best interpreted in terms of the reacceleration scenario in which MHD turbulence injected during these cluster mergers re-accelerates high energy particles in the ICM. The physics involved in this scenario is very complex and model details are difficult to test, however this model clearly predicts some simple properties of Radio Halos (and resulting IC emission in the hard X-ray band) which are almost independent of the details of the adopted physics. In particular in the re-acceleration scenario MHD turbulence is injected and dissipated during cluster mergers and thus Radio Halos (and also the resulting hard X-ray IC emission) should be transient phenomena (with a typical lifetime <» 1 Gyr) associated with dynamically disturbed clusters. The physics of the re-acceleration scenario should produce an unavoidable cut-off in the spectrum of the re-accelerated electrons, which is due to the balance between turbulent acceleration and radiative losses. The energy at which this cut-off occurs, and thus the maximum frequency at which synchrotron radiation is produced, depends essentially on the efficiency of the acceleration mechanism so that observations at high frequencies are expected to catch only the most efficient phenomena while, in principle, low frequency radio surveys may found these phenomena much common in the Universe. These basic properties should leave an important imprint in the statistical properties of Radio Halos (and of non-thermal phenomena in general) which, however, have not been addressed yet by present modellings. The main focus of this PhD thesis is to calculate, for the first time, the expected statistics of Radio Halos in the context of the re-acceleration scenario. In particular, we shall address the following main questions: • Is it possible to model “self-consistently” the evolution of these sources together with that of the parent clusters? • How the occurrence of Radio Halos is expected to change with cluster mass and to evolve with redshift? How the efficiency to catch Radio Halos in galaxy clusters changes with the observing radio frequency? • How many Radio Halos are expected to form in the Universe? At which redshift is expected the bulk of these sources? • Is it possible to reproduce in the re-acceleration scenario the observed occurrence and number of Radio Halos in the Universe and the observed correlations between thermal and non-thermal properties of galaxy clusters? • Is it possible to constrain the magnetic field intensity and profile in galaxy clusters and the energetic of turbulence in the ICM from the comparison between model expectations and observations? Several astrophysical ingredients are necessary to model the evolution and statistical properties of Radio Halos in the context of re-acceleration model and to address the points given above. For these reason we deserve some space in this PhD thesis to review the important aspects of the physics of the ICM which are of interest to catch our goals. In Chapt. 1 we discuss the physics of galaxy clusters, and in particular, the clusters formation process; in Chapt. 2 we review the main observational properties of non-thermal components in the ICM; and in Chapt. 3 we focus on the physics of magnetic field and of particle acceleration in galaxy clusters. As a relevant application, the theory of Alfv´enic particle acceleration is applied in Chapt. 4 where we report the most important results from calculations we have done in the framework of the re-acceleration scenario. In this Chapter we show that a fraction of the energy of fluid turbulence driven in the ICM by the cluster mergers can be channelled into the injection of Alfv´en waves at small scales and that these waves can efficiently re-accelerate particles and trigger Radio Halos and hard X-ray emission. The main part of this PhD work, the calculation of the statistical properties of Radio Halos and non-thermal phenomena as expected in the context of the re-acceleration model and their comparison with observations, is presented in Chapts.5, 6, 7 and 8. In Chapt.5 we present a first approach to semi-analytical calculations of statistical properties of giant Radio Halos. The main goal of this Chapter is to model cluster formation, the injection of turbulence in the ICM and the resulting particle acceleration process. We adopt the semi–analytic extended Press & Schechter (PS) theory to follow the formation of a large synthetic population of galaxy clusters and assume that during a merger a fraction of the PdV work done by the infalling subclusters in passing through the most massive one is injected in the form of magnetosonic waves. Then the processes of stochastic acceleration of the relativistic electrons by these waves and the properties of the ensuing synchrotron (Radio Halos) and inverse Compton (IC, hard X-ray) emission of merging clusters are computed under the assumption of a constant rms average magnetic field strength in emitting volume. The main finding of these calculations is that giant Radio Halos are naturally expected only in the more massive clusters, and that the expected fraction of clusters with Radio Halos is consistent with the observed one. In Chapt. 6 we extend the previous calculations by including a scaling of the magnetic field strength with cluster mass. The inclusion of this scaling allows us to derive the expected correlations between the synchrotron radio power of Radio Halos and the X-ray properties (T, LX) and mass of the hosting clusters. For the first time, we show that these correlations, calculated in the context of the re-acceleration model, are consistent with the observed ones for typical µG strengths of the average B intensity in massive clusters. The calculations presented in this Chapter allow us to derive the evolution of the probability to form Radio Halos as a function of the cluster mass and redshift. The most relevant finding presented in this Chapter is that the luminosity functions of giant Radio Halos at 1.4 GHz are expected to peak around a radio power » 1024 W/Hz and to flatten (or cut-off) at lower radio powers because of the decrease of the electron re-acceleration efficiency in smaller galaxy clusters. In Chapt. 6 we also derive the expected number counts of Radio Halos and compare them with available observations: we claim that » 100 Radio Halos in the Universe can be observed at 1.4 GHz with deep surveys, while more than 1000 Radio Halos are expected to be discovered in the next future by LOFAR at 150 MHz. This is the first (and so far unique) model expectation for the number counts of Radio Halos at lower frequency and allows to design future radio surveys. Based on the results of Chapt. 6, in Chapt.7 we present a work in progress on a “revision” of the occurrence of Radio Halos. We combine past results from the NVSS radio survey (z » 0.05 − 0.2) with our ongoing GMRT Radio Halos Pointed Observations of 50 X-ray luminous galaxy clusters (at z » 0.2−0.4) and discuss the possibility to test our model expectations with the number counts of Radio Halos at z » 0.05 − 0.4. The most relevant limitation in the calculations presented in Chapt. 5 and 6 is the assumption of an “averaged” size of Radio Halos independently of their radio luminosity and of the mass of the parent clusters. This assumption cannot be released in the context of the PS formalism used to describe the formation process of clusters, while a more detailed analysis of the physics of cluster mergers and of the injection process of turbulence in the ICM would require an approach based on numerical (possible MHD) simulations of a very large volume of the Universe which is however well beyond the aim of this PhD thesis. On the other hand, in Chapt.8 we report our discovery of novel correlations between the size (RH) of Radio Halos and their radio power and between RH and the cluster mass within the Radio Halo region, MH. In particular this last “geometrical” MH − RH correlation allows us to “observationally” overcome the limitation of the “average” size of Radio Halos. Thus in this Chapter, by making use of this “geometrical” correlation and of a simplified form of the re-acceleration model based on the results of Chapt. 5 and 6 we are able to discuss expected correlations between the synchrotron power and the thermal cluster quantities relative to the radio emitting region. This is a new powerful tool of investigation and we show that all the observed correlations (PR − RH, PR − MH, PR − T, PR − LX, . . . ) now become well understood in the context of the re-acceleration model. In addition, we find that observationally the size of Radio Halos scales non-linearly with the virial radius of the parent cluster, and this immediately means that the fraction of the cluster volume which is radio emitting increases with cluster mass and thus that the non-thermal component in clusters is not self-similar.

Funzionalizzazione della mandibola dopo ricostruzione con lembo libero rivascolarizzato di fibula "single strut". Al di là del deficit di verticalità.

Obiettivi: Valutare la modalità  più efficace per la riabilitazione funzionale del limbo libero di fibula "single strut", dopo ampie resezioni per patologia neoplastica maligna del cavo orale. Metodi: Da una casistica di 62 ricostruzioni microvascolari con limbo libero di fibula, 11 casi sono stati selezionati per essere riabilitati mediante protesi dentale a supporto implantare. 6 casi sono stati trattati senza ulteriori procedure chirurgiche ad eccezione dell'implantologia (gruppo 1), affrontando il deficit di verticalità  della fibula attraverso la protesi dentaria, mentre i restanti casi sono stati trattati con la distrazione osteogenetica (DO) della fibula prima della riabilitazione protesica (gruppo 2). Il deficit di verticalità  fibula/mandibola è stato misurato. I criteri di valutazione utilizzati includono la misurazione clinica e radiografica del livello osseo e dei tessuti molli peri-implantari, ed il livello di soddisfazione del paziente attraverso un questionario appositamente redatto. Risultati: Tutte le riabilitazioni protesiche sono costituite da protesi dentali avvitate su impianti. L'età  media è di 52 anni, il rapporto uomini/donne è di 6/5. Il numero medio di impianti inseriti nelle fibule è di 5. Il periodo massimo di follow-up dopo il carico masticatorio è stato di 30 mesi per il gruppo 1 e di 38.5 mesi (17-81) di media per il gruppo 2. Non abbiamo riportato complicazioni chirurgiche. Nessun impianto è stato rimosso dai pazienti del gruppo 1, la perdita media di osso peri-implantare registrata è stata di 1,5 mm. Nel gruppo 2 sono stati riportati un caso di tipping linguale del vettore di distrazione durante la fase di consolidazione e un caso di frattura della corticale basale in assenza di formazione di nuovo osso. L'incremento medio di osso in verticalità è stato di 13,6 mm (12-15). 4 impianti su 32 (12.5%) sono andati persi dopo il periodo di follow-up. Il riassorbimento medio peri-implantare, è stato di 2,5 mm. Conclusioni: Le soluzioni più utilizzate per superare il deficit di verticalità  del limbo libero di fibula consistono nell'allestimento del lembo libero di cresta iliaca, nel posizionare la fibula in posizione ideale da un punto di vista protesico a discapito del profilo osseo basale, l'utilizzo del lembo di fibula nella versione descritta come "double barrel", nella distrazione osteogenetica della fibula. La nostra esperienza concerne il lembo libero di fibula che nella patologia neoplastica maligna utilizziamo nella versione "single strut", per mantenere disponibili tutte le potenzialità  di lunghezza del peduncolo vascolare, senza necessità  di innesti di vena. Entrambe le soluzioni, la protesi dentale ortopedica e la distrazione osteogenetica seguita da protesi, entrambe avvitate su impianti, costituiscono soluzioni soddisfacenti per la riabilitazione funzionale della fibula al di là  del suo deficit di verticalità . La prima soluzione ha preso spunto dall'osservazione dei buoni risultati della protesi dentale su impianti corti, avendo un paragonabile rapporto corona/radice, la DO applicata alla fibula, sebbene sia risultata una metodica con un numero di complicazioni più elevato ed un maggior livello di riassorbimento di osso peri-implantare, costituisce in ogni caso una valida opzione riabilitativa, specialmente in caso di notevole discrepanza mandibulo/fibulare. Decisiva è la scelta del percorso terapeutico dopo una accurata valutazione di ogni singolo caso. Vengono illustrati i criteri di selezione provenienti dalla nostra esperienza.

Untersuchung der Wirkung von Schwerionenstrahlen auf menschliche Hautfibroblasten unter besonderer Berücksichtigung chromosomaler Veränderungen

In der vorliegenden Arbeit wurden humane diploide Vorhaut-Fibroblasten u.a. auf Chromosomensch?den hin untersucht. Die konfluenten Zellen wurden mit d?nnionisierender R?ntgen-und Kohlenstoffstrahlung, sowie mit dichtionisierendenKohlenstoff- und Nickelionen bestrahlt und der chromosomaleSchaden in Intervallen bis zu 100 h nach Bestrahlungbestimmt. Dabei wurde nach dichtionisierender Strahlung ein deutlicher Anstieg in der Frequenz aberranter Zellen undAberrationen je Metaphase mit der Sammelzeit gefunden. Dieszeigt, dass gesch?digte Zellen von Zellzyklusverz'ogerungenst?rker betroffen sind als ungesch?digte Zellen.Durch Integration ?ber die Zeit wurde der genetische Gesamt-schaden in der proliferierenden Zellpopulation bestimmt. Dabei zeigte sich, dass ein Grossteil der Zellen nachTeilchenbestrahlung einen permanenten Zellzyklusarrest bzw.eine beschleunigte Differenzierung erf?hrt. Nur ein kleinerTeil erreicht die 1. Mitose nach Bestrahlung, so dass nurein geringer Teil der genetischen Sch?den auf die folgendenGenerationen ?bertragen wird. Der beobachtete Gesamtschadenist viel kleiner, als anhand von Daten aus Experimenten mitV79-Zellen abgesch?tzt wurde. Die direkte Extrapolation vonDaten etablierter Nagerzellen auf prim?re menschliche Zellenist demnach nicht m?glich. F?r die Beurteilung vonErgebnissen aus Tierexperimenten w?re es w?nschenswert zuwissen, ob die Unterschiede auf der Art der Zellen, alsoetablierten und prim?ren Zellen beruhen, oder von derSpezies abh?ngen.

Synthesis and characterization of polymers containing oligothiophenes

In the present work a series of thiophene oligomers of three and six thiophene units were synthesized, starting from thiophene, and characterized. Polymers containing these electroative side groups were then prepared by two strategies. The oligomers were attached to existing polymer systems and were connected to a polymerizable unit leading to monomer containing the oligothiophenes as side groups. Subsequently the properties of the monomers and the polymers were investigated. A butylcellulose derivative carrying terthienyl side chains (BCTTE, 26) was synthesized starting from cellulose acetate and 5-(2-chloroethyl)-2,2':5',2'-terthiophene (4). The polymer had a degree of substitution (DS) of the butyl and terthienyl side chains of DSbutyl = 1.9 and DSterth = 0.35, respectively. It was successfully spread on a Langmuir-Blodgett (LB) trough and then transferred to several solid substrates. X-rays reflectometry showed an ordered architecture of the cellulose backbones. However, the terthiophene side groups were found as isotropically aligned by polarized UV-Vis spectroscopy. When used as anode material in the electropolymerization of 3-pentylthiophene (28), polythiophene was grafted onto the cellulose backbone through the terthienyl side groups. The polythiophene chains showed an average anisotropic alignment of 20 % along the LB dipping direction, calculated by means of polarized UV-Vis spectroscopy. A second butylcellulose derivative carrying sexithienyl side chains (BCST) was synthesized and investigated, starting from butylcellulose and 2-[b ', b ''-dipentyl-5'''-(2-hydroxyethyl)-2,2': 5',2':5',2'':5'',2'':5'',2'''-sexithiophen-5-yl]-ethyl p-toluensulfonate (7). The polymer showed formation of stable LB monolayers at the air-water interface, but its transfer onto solid substrates was not successful. A poly(p-phenylene-ethynylene) bearing sexithienyl side chains (BzAcST, 31) was prepared by reaction of the two monomers 2-[b ', b ''-dipentyl-5'''-(2-hydroxyethyl)-2,2': 5',2':5',2'':5'',2'':5'',2'''-sexithiophen-5-yl]-ethyl 2,5-diiodobenzoate (15) and 2-[b', b ''-dipentyl-5'''-(2-hydroxyethyl)-2,2':5',2':5',2'':5'',2'':5'',2'''-sexithiophen-5-yl]-ethyl 2,5-diethynylbenzoate (18). The polymer was obtained as insoluble product. Upon oxidation with FeCl3 (doping) of the polymer suspension, BzAcST showed an electrical conductivity of ó = 2.5 . 10 -6 S/cm, a typical value for semiconductors. The IR spectrum of the doped polymer presented the diagnostic bands of oxidized sexithiophene in good agreement with literature results. Along with the monomer and polymer synthesis, an a,a '-disubstituted sexithiophene, b ', b ''-dipentyl-5,5'''-bis-(2-hydroxyethyl)-2,2':5',2':5',2'':5'',2'':5'',2'''-sexithiophene (6a),was synthesized and characterized. The UV-Vis absorption of the chromophore wasinvestigated as a function of temperature and different solvents, showing a blue-shift of the absorption maximum with increasing temperature and a red-shift changing the solvent from hexane to ethanol to toluene. Monitoring the change of the UV-Vis spectrum upon electrochemical oxidation, the oxidized chromophore showed a new broad absorption band, red shifted with respect to the p -p* transition of the neutral state. Upon reduction, the new band disappeared and the UV-Vis spectrum of the chromophore was restored. Such oxidation-reduction cycles were totally reversible. This feature, together with the absorption maximum falling in the visible region, makes this chromophore a suitable compound for the development of an electrochemical sensor.Attempts to polymerize acrylic monomers carrying sexythienyl side chains both via radical polymerization, as in the case of 2-[b ', b ''-dipentyl-5'''-(2-hydroxyethyl)-2,2': 5',2':5',2'':5'',2'':5'',2'''-sexithiophen-5-yl]-ethyl acrylate (8), and anionic polymerization, as in the case of 2-{b ', b ''-dipentyl-5'''-[2-(tertbutyldimethylsiloxy)ethyl]-2,2':5',2':5',2'':5'',2'': 5'',2''' -sexithiophen-5-yl}-ethylacrylate (29), were not successful, probably due to the steric hindrance of the oligothiophene side group. However, due to the time consuming and therefore restricted availability of the monomers, a screening of the polymerization conditions towards the formation of polymeric material was not possible.

Schwerionenbestrahlung zwei- und dreidimensionaler Zellsysteme

Aufgaben der vorliegenden Untersuchungen waren die Etablierung von planaren Multilayern aus mensch­lichen Tumorzellen (WiDr und SiHa) und die Testung dieses Zellsystems als Bestrahlungsmodell solider Tumoren. Neben der konventionellen Röntgenbestrahlung (250 kV) wurde auch das Überle­ben nach Schwerionenbestrahlung (12C6+) und nach Behandlung mit dem Chemotherapeutikum Etoposid unter­sucht. Multilayer aus beiden Zelllinien zeigten ein geringeres Überleben nach Röntgen- und Schwerionenbestrah­lung als die entsprechenden Monolayer. Die hier beschriebene multizelluläre Sensitivierung steht aller­dings im Ge­gensatz zu der in der Literatur beschriebenen multizellulären Resistenz der Sphäroide, dem sog. Kontakteffekt. Nach durchflußzytometrischen Mes­sungen arretierten die bestrahlten SiHa-Zellen in der G2/M-Phase. Im Gegen­satz zum transienten Block der Monolayer verweilten die Multilayer in einem per­manenten Arrest. Im Vergleich zur Röntgenbe­strahlung verlän­gerte sich die Arrestzeit der Mono­layer nach Schwerionenbestrahlung im Bragg-Peak um 12-24 h. Auch waren mehr Zellen betroffen. Im Gegensatz dazu war kein Unterschied zwischen beiden Bestrahlungsmo­dalitäten bei den Multi­layern bis zum Ende des Beobachtungszeit­raumes zu verzeichnen. Nach Etoposid-Behandlung verhielten sich die Multilayer deutlich resistenter als die Monolayer. Somit zeigten Multilayer interessan­terweise nach Bestrahlung eine Sensitivierung und nach Etoposid-Behandlung eine Resistenz. Die Unterschiede im Überleben der beiden Kultivierungs­formen beruhen zum Großteil auf den Differenzen in der Zellzyk­lusverteilung. Besonders deutlich wurde dieser Zusam­men­hang zwischen Überleben und Zell­zyklusvertei­lung durch Wie­deraussaat- und Synchronisations-Experi­mente.

Performance evaluation of detectors for digital radiography

To date the hospital radiological workflow is completing a transition from analog to digital technology. Since the X-rays digital detection technologies have become mature, hospitals are trading on the natural devices turnover to replace the conventional screen film devices with digital ones. The transition process is complex and involves not just the equipment replacement but also new arrangements for image transmission, display (and reporting) and storage. This work is focused on 2D digital detector’s characterization with a concern to specific clinical application; the systems features linked to the image quality are analyzed to assess the clinical performances, the conversion efficiency, and the minimum dose necessary to get an acceptable image. The first section overviews the digital detector technologies focusing on the recent and promising technological developments. The second section contains a description of the characterization methods considered in this thesis categorized in physical, psychophysical and clinical; theory, models and procedures are described as well. The third section contains a set of characterizations performed on new equipments that appears to be some of the most advanced technologies available to date. The fourth section deals with some procedures and schemes employed for quality assurance programs.

A panchromatic view of the evolution of supermassive black holes

This PhD Thesis is devoted to the accurate analysis of the physical properties of Active Galactic Nuclei (AGN) and the AGN/host-galaxy interplay. Due to the broad-band AGN emission (from radio to hard X-rays), a multi-wavelength approach is mandatory. Our research is carried out over the COSMOS field, within the context of the XMM-Newton wide-field survey. To date, the COSMOS field is a unique area for comprehensive multi-wavelength studies, allowing us to define a large and homogeneous sample of QSOs with a well-sampled spectral coverage and to keep selection effects under control. Moreover, the broad-band information contained in the COSMOS database is well-suited for a detailed analysis of AGN SEDs, bolometric luminosities and bolometric corrections. In order to investigate the nature of both obscured (Type-2) and unobscured (Type-1) AGN, the observational approach is complemented with a theoretical modelling of the AGN/galaxy co-evolution. The X-ray to optical properties of an X-ray selected Type-1 AGN sample are discussed in the first part. The relationship between X-ray and optical/UV luminosities, parametrized by the spectral index αox, provides a first indication about the nature of the central engine powering the AGN. Since a Type-1 AGN outshines the surrounding environment, it is extremely difficult to constrain the properties of its host-galaxy. Conversely, in Type-2 AGN the host-galaxy light is the dominant component of the optical/near-IR SEDs, severely affecting the recovery of the intrinsic AGN emission. Hence a multi-component SED-fitting code is developed to disentangle the emission of the stellar populationof the galaxy from that associated with mass accretion. Bolometric corrections, luminosities, stellar masses and star-formation rates, correlated with the morphology of Type-2 AGN hosts, are presented in the second part, while the final part concerns a physically-motivated model for the evolution of spheroidal galaxies with a central SMBH. The model is able to reproduce two important stages of galaxy evolution, namely the obscured cold-phase and the subsequent quiescent hot-phase.

Development and performance assessment of a Plasma Focus electron beam generator for Intra-Operative Radiation Therapy

The Plasma Focus is a device designed to generate a plasma sheet between two coaxial electrodes by means of a high voltage difference. The plasma is then driven to collapse into a “pinch”, where thermonuclear conditions prevail. During the “pinch phase” charged particles are emitted, with two main components: an ion beam peaked forward and an electron beam directed backward. The electron beam emitted backward by Plasma Focus devices is being investigated as a radiation source for medical applications, using it to produce x-rays by interaction with appropriate targets (through bremsstrahlung and characteristic emission). A dedicated Plasma Focus device, named PFMA-3 (Plasma Focus for Medical Applications number 3), has been designed, put in operation and tested by the research groups of the Universities of Bologna and Ferrara. The very high dose rate (several gray per discharge, in less than 1 µs) is a peculiarity of this device that has to be investigated, as it might modify the relative biological effectiveness (RBE). Aim of this Ph.D. project was to investigate the main physical properties of the low-energy x-ray beams produced by a Plasma Focus device and their potential medical applications to IORT treatments. It was necessary to develop the optimal geometrical configuration; to evaluate the x-rays produced and their dose deposited; to estimate the energy electron spectrum produced in the “pinch phase”; to study an optimal target for the conversion of the x-rays; to conduct simulations to study the physics involved; and in order to evaluate the radio-biological features of the beam, cell holders had to be developed for both irradiations and cell growth conditions.

Einfluss einer Schwerionenbestrahlung auf das Migrationsverhalten von Tumorzellen

Die Bildung von Metastasen und Rezidiven stellt ein großes Problem für eine erfolgreiche Therapie solider maligner Tumoren dar. Dabei ist die Rolle der angewendeten Therapiever-fahren in der Induktion metastasierender Zellen vor allem für eine Schwerionentherapie noch weitestgehend unklar. Die für die Metastasierung entscheidende Tumorzellmigration wurde daher unter dem Einfluss von Röntgen- und Schwerionenstrahlung untersuchen. Dazu wurden drei humane Tumorzelllinien (Gliomzelllinie U87 und kolorektale Zelllinien HCT116 und HCT116 p21-/-) unter standardisierten Bedingungen in einer Boydenkammer direkt und 24 Stunden nach Bestrahlung in vitro auf ihr Migrationsverhalten untersucht. Um mögliche Än-derungen migrationsrelevanter Proteine zu bestimmen, wurden zu denselben Zeitpunkten Zelllysate hergestellt und die Expression der Integrine b1 und b3 sowie der Proteinkinase B Isoformen Akt1 und Akt2 und deren Phosphorylierung untersucht. Gezeigt werden konnten sowohl zelllinien- als auch strahlenspezifische Unterschiede in der Migration und der Proteinexpressionen. Dabei konnten die beobachteten Migrationsänderungen nur zum Teil (vor allem nach Röntgenbestrahlung) durch die veränderte Expressionen der untersuchten Proteine erklärt werden. Daher ist zu vermuten, dass den strahleninduzierten Veränderungen der Migration der verwendeten Zelllinien verschiedene Mechanis-men zugrunde liegen, die auf der Expression unterschiedlicher Proteine beruhen. Bestrahlungen mit 12C-Ionen scheinen prinzipiell andere Expressionsmuster zu induzieren als konventionelle Strahlung und die hier untersuchten Proteine in der Migration der Zellen daher nur eine untergeordnete Rolle zu spielen. Auffällig waren die deutlich zelllinienspezifischen Unterschiede in der Migration nach Röntgenbestrahlung. Dort wurde ein zum Teil erhöhtes Migrationspotential nach klinisch relevanten Bestrahlungsdosen von U87 Gliomzellen festgestellt. Die Migrationsaktivität von kolorektalen Zelllinien hingegen nahm nach Bestrahlung ab. Nach Schwerionenbestrahlung wurden für alle Zelllinien signifikante Abnahmen der Migration festgestellt. Die hier erhaltenen Ergebnisse können aufgrund einer Vielzahl pro- und antimigratorischer Signale im Tumorgewebe nicht direkt in die in vivo Situation übertragen werden, doch können sie durchaus als Hinweise für die Abschätzung eines veränderten Metastasierungsrisikos dienen. Für kolorektale Zellen, unabhängig von ihrem p21-Status scheint eine Behandlung mit Röntgenstrahlen eher nicht mit einem erhöhten Migrationsrisiko einherzugehen. Anders ist dies bei den hier untersuchten Gliomzellen U87. Hier kann ein strahleninduziertes Metastasierungsrisiko aufgrund der erzielten Ergebnisse keinesfalls ausgeschlossen werden. Aus dieser Sicht scheint eine Behandlung von Gliomen mit 12C-Ionen vorteilhafter, da eine sehr gute reproduzierbare strahlenvermittelte Migrationshemmung beobachtet wurde.

A chemical approach to Heusler compounds and nanoparticles

Heusler Materialien wurden bisher vor allem in Volumen- und Dünnfilmproben aufgrund ihrer technischen Bedeutung untersucht. In dieser Arbeit berichtet über die experimentellen Untersuchungen der chemischen Synthese, Struktur, und der magnetischen Eigenschaften von ternären Heusler-Nanopartikeln. Die grundlegenden Aspekte der Physik, Chemie und Materialwissenschaft bezüglich der Heusler Nanopartiikel wurden untersucht. Außerdem wurde eine silicatgestützte Herstellungsmethode für Karbon-ummantelte, ternäre intermetallische Co2FeGa Nanopartikel entwickelt. Die Bildung der L21 Co2FeGa Phase wurde mit Röntgenbeugung (XRD), Extended X-ray Absorption Fine Structure Spektroskopie (EXAFS), und 57Fe Mössbauer Spektroskopie bestätigt. Die Abhängigkeit der Phase und der der Größe der Co2FeGa Nanopartikel vom der Zusammensetzung der Precursor und des Silicats wurden untersucht. Durch das Koppeln der aus Transmissions-Elektronen-Mikroskopie (TEM) gewonnen Teilchengröße und der Mössbauerspektroskopie konnte die kritische Größe für den Übergang von superparamgnetischem zu ferromagnetischem Verhalten von Co2FeGa Nanopartikel ermittelt werden. Die silicatgestützte chemische Synthese von Co2FeGa Nanopartikeln besitzt großes Potential für eine generelle Herstellungsmethode für Co-basierte Heuser Nanopartikel. Des weiteren wurde auch eine chemische Herstellungsmethode von metallischen Nanopartikeln mit Synchrotronstrahlung untersucht, die so gewonnen Nanopartikel sind vielversprechende Materialien für die Nanobiotechnologie und die Nanomedizin.

Transport Properties and Novel Sensing Applications of Organic Semiconducting Crystals

The present thesis is focused on the study of Organic Semiconducting Single Crystals (OSSCs) and crystalline thin films. In particular solution-grown OSSC, e.g. 4-hdroxycyanobenzene (4HCB) have been characterized in view of their applications as novel sensors of X-rays, gamma-rays, alpha particles radiations and chemical sensors. In the field of ionizing radiation detection, organic semiconductors have been proposed so far mainly as indirect detectors, i.e. as scintillators or as photodiodes. I first study the performance of 4HCB single crystals as direct X-ray detector i.e. the direct photon conversion into an electrical signal, assessing that they can operate at room temperature and in atmosphere, showing a stable and linear response with increasing dose rate. A dedicated study of the collecting electrodes geometry, crystal thickness and interaction volume allowed us to maximize the charge collection efficiency and sensitivity, thus assessing how OSSCs perform at low operating voltages and offer a great potential in the development of novel ionizing radiation sensors. To better understand the processes generating the observed X-ray signal, a comparative study is presented on OSSCs based on several small-molecules: 1,5-dinitronaphthalene (DNN), 1,8-naphthaleneimide (NTI), Rubrene and TIPS-pentacene. In addition, the proof of principle of gamma-rays and alpha particles has been assessed for 4HCB single crystals. I have also carried out an investigation of the electrical response of OSSCs exposed to vapour of volatile molecules, polar and non-polar. The last chapter deals with rubrene, the highest performing molecular crystals for electronic applications. We present an investigation on high quality, millimeter-sized, crystalline thin films (10 – 100 nm thick) realized by exploiting organic molecular beam epitaxy on water-soluble substrates. Space-Charge-Limited Current (SCLC) and photocurrent spectroscopy measurements have been carried out. A thin film transistor was fabricated onto a Cytop® dielectric layer. The FET mobility exceeding 2 cm2/Vs, definitely assess the quality of RUB films.

Ein neuartiges Interferometer zur Messung magneto-optischer Effekte an L-Absorptionskanten von ferromagnetischen Metallen mit linearpolarisierter Undulatorstrahlung

Am Mainzer Mikrotron MAMI wurde ein neuartiges Interferometer entwickelt und getestet, mit dem magneto-optische Effekte an dünnen, freitragenden Folien von 3d-Übergangsmetallen wie Eisen, Kobalt oder Nickel an den L_{2,3}-Absorptionskanten (im Spektralbereich der weichen Röntgenstrahlung) gemessen werden können. Es handelt sich um eine Weiterentwicklung eines an MAMI erprobten Interferometers, das im wesentlichen aus einer kollinearen Anordnung zweier identischer Undulatoren, zwischen die die dünne Probefolie eingebracht wird, und einem Gitterspektrometer besteht. Aus den als Funktion des Abstands der Undulatoren beobachtbaren Intensitätsoszillation lassen sich das Dekrement des Realteils δ und der Absorptionskoeffizient β des komplexen Brechungsindex bestimmen.rnIm Rahmen der vorliegenden Arbeit wurde die Apparatur derart weiterentwickelt, dass auch die magnetisch zirkulare Doppelbrechung Δδ und der magnetisch zirkulare Dichroismus Δβ an den L_{2,3}-Absorptionskanten von Übergangsmetallen gemessen werden können. Der zweite Undulator wurde um die Elektronenstrahlachse um den Winkel Ψ = ±107° drehbar gemacht. Damit dient er auch als Analysator der aus der Folie austretenden elliptisch polarisierten weichen Röntgenstrahlung, für die - wie bei der Faraday-Rotation - die Polarisationsebene gedreht ist. Weiterhin kann die Spaltbreite der 10-poligen Hybrid-Undulatoren mit einer Periodenlänge von 12 mm und damit der Undulatorparameter über eine Antriebsmechanik kontinuierlich variiert werden, wodurch eine optimale Anpassung der Amplituden der Undulatorstrahlung aus den beiden Undulatoren möglich wird. Der maximale Undulatorparameter beträgt K = 1.1. Auch das Spektrometer, das auf einem selbstfokussierenden Gitter mit variierter Liniendichte (im Mittel 1400 Linien / mm) basiert, wurde weiterentwickelt. Als Detektor kommt jetzt eine fensterlose CCD mit 1024 x 1024 Pixeln und einer Pixelgröße von 13 μm x 13 μm zum Einsatz, die im Bildmodus betrieben wird, was die gleichzeitige Messung eines Energieintervalls von ca. 50 eV ermöglicht. Die totale Linienbreite wurde bei einer vertikalen Strahlfleckausdehnung von σ_y = 70 μm (rms) am Neon 1s-3p Übergang bei (867.18 ±0.02) eV zu Δħω = (0.218 ±0.002) eV (FWHM) gemessen. Das hohe Auflösungsvermögen von 4000 und die Möglichkeit der Eichung gegen den 1s-3p Übergang von Neon wurden ausgenutzt, um die Energie der Maxima an den Absorptionskanten von Nickel (weiße Linien) neu zu bestimmen. Die Ergebnisse E_{L_2}=(869.65_{-0.16}^{+0.27}) eV und E_{L_3}=(852.37_{-0.11}^{+0.16}) eV stellen eine Verbesserung früherer Messungen dar, die große Streuungen aufwiesen.rnAus systematischen Messungen als Funktion des Abstandes der Undulatoren und des Drehwinkels Ψ wurden die magnetisch zirkulare Doppelbrechung Δδ im Energiebereich 834 eV ≤ ħω ≤ 885 eV an einer freitragenden, bis zur Sättigung magnetisierten Nickelfolie der Dicke von (96.4 ±2.7) nm gemessen. Sowohl das Auflösungsvermögen als auch die Genauigkeit der Messungen für Δδ übersteigen bekannte Literaturangaben signifikant, so dass eine bisher nicht bekannte Feinstruktur gefunden werden konnte. Außerdem wurde der Betrag des magnetisch zirkularen Dichroismus |Δβ| im Bereich des Maximums an der L_3-Absorptionskante mit hoher Genauigkeit gemessen.rn