X-Ray studies of the physics of matter around super-massive black-holes in nearby Seyfert galaxies

Seyfert galaxies are the closest active galactic nuclei. As such, we can use them to test the physical properties of the entire class of objects. To investigate their general properties, I took advantage of different methods of data analysis. In particular I used three different samples of objects, that, despite frequent overlaps, have been chosen to best tackle different topics: the heterogeneous BeppoS AX sample was thought to be optimized to test the average hard X-ray (E above 10 keV) properties of nearby Seyfert galaxies; the X-CfA was thought the be optimized to compare the properties of low-luminosity sources to the ones of higher luminosity and, thus, it was also used to test the emission mechanism models; finally, the XMM–Newton sample was extracted from the X-CfA sample so as to ensure a truly unbiased and well defined sample of objects to define the average properties of Seyfert galaxies. Taking advantage of the broad-band coverage of the BeppoS AX MECS and PDS instruments (between ~2-100 keV), I infer the average X-ray spectral propertiesof nearby Seyfert galaxies and in particular the photon index (~1.8), the high-energy cut-off (~290 keV), and the relative amount of cold reflection (~1.0). Moreover the unified scheme for active galactic nuclei was positively tested. The distribution of isotropic indicators used here (photon index, relative amount of reflection, high-energy cut-off and narrow FeK energy centroid) are similar in type I and type II objects while the absorbing column and the iron line equivalent width significantly differ between the two classes of sources with type II objects displaying larger absorbing columns. Taking advantage of the XMM–Newton and X–CfA samples I also deduced from measurements that 30 to 50% of type II Seyfert galaxies are Compton thick. Confirming previous results, the narrow FeK line is consistent, in Seyfert 2 galaxies, with being produced in the same matter responsible for the observed obscuration. These results support the basic picture of the unified model. Moreover, the presence of a X-ray Baldwin effect in type I sources has been measured using for the first time the 20-100 keV luminosity (EW proportional to L(20-100)^(−0.22±0.05)). This finding suggests that the torus covering factor may be a function of source luminosity, thereby suggesting a refinement of the baseline version of the unifed model itself. Using the BeppoSAX sample, it has been also recorded a possible correlation between the photon index and the amount of cold reflection in both type I and II sources. At a first glance this confirms the thermal Comptonization as the most likely origin of the high energy emission for the active galactic nuclei. This relation, in fact, naturally emerges supposing that the accretion disk penetrates, depending to the accretion rate, the central corona at different depths (Merloni et al. 2006): the higher accreting systems hosting disks down to the last stable orbit while the lower accreting systems hosting truncated disks. On the contrary, the study of the well defined X–C f A sample of Seyfert galaxies has proved that the intrinsic X-ray luminosity of nearby Seyfert galaxies can span values between 10^(38−43) erg s^−1, i.e. covering a huge range of accretion rates. The less efficient systems have been supposed to host ADAF systems without accretion disk. However, the study of the X–CfA sample has also proved the existence of correlations between optical emission lines and X-ray luminosity in the entire range of L_(X) covered by the sample. These relations are similar to the ones obtained if high-L objects are considered. Thus the emission mechanism must be similar in luminous and weak systems. A possible scenario to reconcile these somehow opposite indications is assuming that the ADAF and the two phase mechanism co-exist with different relative importance moving from low-to-high accretion systems (as suggested by the Gamma vs. R relation). The present data require that no abrupt transition between the two regimes is present. As mentioned above, the possible presence of an accretion disk has been tested using samples of nearby Seyfert galaxies. Here, to deeply investigate the flow patterns close to super-massive black-holes, three case study objects for which enough counts statistics is available have been analysed using deep X-ray observations taken with XMM–Newton. The obtained results have shown that the accretion flow can significantly differ between the objects when it is analyzed with the appropriate detail. For instance the accretion disk is well established down to the last stable orbit in a Kerr system for IRAS 13197-1627 where strong light bending effect have been measured. The accretion disk seems to be formed spiraling in the inner ~10-30 gravitational radii in NGC 3783 where time dependent and recursive modulation have been measured both in the continuum emission and in the broad emission line component. Finally, the accretion disk seems to be only weakly detectable in rk 509, with its weak broad emission line component. Finally, blueshifted resonant absorption lines have been detected in all three objects. This seems to demonstrate that, around super-massive black-holes, there is matter which is not confined in the accretion disk and moves along the line of sight with velocities as large as v~0.01-0.4c (whre c is the speed of light). Wether this matter forms winds or blobs is still matter of debate together with the assessment of the real statistical significance of the measured absorption lines. Nonetheless, if confirmed, these phenomena are of outstanding interest because they offer new potential probes for the dynamics of the innermost regions of accretion flows, to tackle the formation of ejecta/jets and to place constraints on the rate of kinetic energy injected by AGNs into the ISM and IGM. Future high energy missions (such as the planned Simbol-X and IXO) will likely allow an exciting step forward in our understanding of the flow dynamics around black holes and the formation of the highest velocity outflows.

Experimental analysis of coaxial jets: instability, flow and mixing characterization

The velocity and mixing field of two turbulent jets configurations have been experimentally characterized by means of cold- and hot-wire anemometry in order to investigate the effects of the initial conditions on the flow development. In particular, experiments have been focused on the effect of the separation wall between the two streams on the flow field. The results of the experiments have pointed out that the wake behind a thick wall separating wall has a strong influence on the flow field evolution. For instance, for nearly unitary velocity ratios, a clear vortex shedding from the wall is observable. This phenomenon enhances the mixing between the inner and outer shear layer. This enhancement in the fluctuating activity is a consequence of a local absolute instability of the flow which, for a small range of velocity ratios, behaves as an hydrodynamic oscillator with no sensibility to external perturbations. It has been suggested indeed that this absolute instability can be used as a passive method to control the flow evolution. Finally, acoustic excitation has been applied to the near field in order to verify whether or not the observed vortex shedding behind the separating wall is due to a global oscillating mode as predicted by the theory. A new scaling relationship has been also proposed to determine the preferred frequency for nearly unitary velocity ratios. The proposed law takes into account both the Reynolds number and the velocity ratio dependence of this frequency and, therefore, improves all the previously proposed relationships.

Il cibo come creatore di circoli virtuosi. Slow Food e Terra Madre, eccellenze nello sviluppo sostenibile del territorio.

Punto di partenza per il lavoro presentato, sono le tematiche legate alle pratiche di consumo di cibo in un’ottica che superi una semplice visione utilitaristica delle stesse, mentre viene evidenziato invece il più profondo rapporto uomo-cibo e i fenomeni di socializzazione che ne scaturiscono. Si trovano pertanto a coniugarsi la sociologia dei consumi e la sociologia della cultura. La base per questa visione del cibo e delle pratiche di produzione e consumo ad esso collegate è l’ipotesi che nel rapporto uomo-cibo sia individuabile un livello di significato superiore al mero utilitarismo/nutrizionismo, che si compone di una dimensione strutturale, una dimensione simbolica ed una dimensione metaforica. Il cibo, e di conseguenza tutte le pratiche ad esso collegate (produzione, elaborazione, consumo), rientrano pertanto in maniera naturale nella categoria “cultura”, e quindi, accostandoci al paradigma del passaggio da natura a società, attraverso il cibo si crea e si alimenta la socialità del consorzio umano, e quindi l’umanità stessa. Accostando a queste concettualizzazioni l’idea che il consumo in generale possa diventare una prassi tramite cui esperire una più diffusa ricerca di sostenibilità nello sviluppo del territorio, (facendosi carico delle conseguenze socio-ambientali derivanti dalla fruizione di determinati oggetti piuttosto che altri), si è sviluppata l’ipotesi che al consumo alimentare possa competere un ruolo precipuamente attivo nella definizione di pratiche sociali orientate alla sostenibilità, capaci cioè di integrare attraverso il consumo – e in relazione all’indebolimento delle tradizionali agenzie di socializzazione – quella perdita di senso civico e solidarietà organizzata che sperimentiamo nelle prassi di vita quotidiana. Sul piano operativo, la tesi è articolata in sei capitoli: • Il percorso presentato prende le mosse dalla considerazione che il cibo, inteso in un’ottica sociologica, costituisce un fattore culturale non irrilevante, anzi fondamentale per il consorzio umano. Si fornisce quindi una breve descrizione del ruolo del cibo nei suoi accostamenti con la definizione di un territorio (e quindi con la sua storia, economia e società), con le arti visive, con il cinema, con la musica, ma anche con la sfera sensoriale (tatto, gusto, olfatto) ed emotivo-cognitiva (psiche) dell’uomo. • Successivamente, si analizza nello specifico la funzione socializzante delle pratiche alimentari, ripercorrendo le tappe principali degli studi classici di sociologia e antropologia dell’alimentazione e introducendo anche l’idea di cibo come simbolo e metafora, che si riflettono sul piano sociale e sulle relazioni tra gli individui. La constatazione che le pratiche legate al cibo sono le uniche attività umane da sempre e per sempre irrinunciabili è un chiaro indicatore di come esse giochino un ruolo fondamentale nella socializzazione umana. • Nel terzo capitolo, la prospettiva simbolico-metaforica è la base di un’analisi di tipo storico delle pratiche alimentari, nello specifico delle pratiche di consumo di cibo, dalle origini dell’umanità ai giorni nostri. Viene presentato un excursus essenziale in cui l’attenzione è focalizzata sulla tavola, sui cibi ivi serviti e sugli eventi di socializzazione che si sviluppano attorno ad essa, considerando situazioni storico-sociali oggettive di cui si è in grado, oggi, di ricostruire le dinamiche e le fasi più significative. • Il quarto capitolo costituisce un momento di riflessione teorica intorno al tema della globalizzazione nella contemporaneità. Sia per una logica progressione cronologica all’interno del lavoro presentato, sia per la rilevanza in quanto inerente alla società attuale in cui viviamo, non si è potuto infatti non soffermarsi un po’ più a fondo sull’analisi delle pratiche alimentari nella contemporaneità, e quindi nella società generalmente definita come “globalizzata” (o “mcdonaldizzata”, per dirla alla Ritzer) ma che in realtà è caratterizzata da un più sottile gioco di equilibri tra dimensione locale e dimensione globale, che si compenetrano come anche nel termine che indica tale equilibrio: il “glocale”. In questo capitolo vengono presentati i principali riferimenti teorici relativi a queste tematiche. • Nel quinto capitolo è stata analizzata, quindi, la declinazione in senso “alimentare” della relazione tra globale e locale, e quindi non solo i mutamenti intercorsi nella contemporaneità nelle pratiche di produzione, scambio e consumo di cibo con particolare riferimento ai sistemi culturali e al territorio, ma anche alcune proposte (sia teoriche che pratiche) a garanzia di uno sviluppo sostenibile del territorio, che trovi i suoi fondamenti sulla perpetuazione di modalità tradizionali di produzione, commercio e consumo di cibo. • Nel sesto capitolo viene analizzato un caso di studio significativo, (il movimento Slow Food, con il suo progetto Terra Madre) senza la pretesa di confermare o smentire né le ipotesi di partenza, né i concetti emersi in itinere, ma semplicemente con l’intenzione di approfondire il percorso svolto attraverso l’esemplificazione operativa e la ricerca entro un piccolo campione composto da testimoni significativi e intervistati, sottoposti a colloqui e interviste incentrate su item inerenti i temi generali di questo lavoro e sul caso di studio considerato. La scelta del caso è motivata dalla considerazione che, alla luce delle filosofia che lo anima e delle attività che svolge, il movimento Slow Food con il progetto Terra Madre costituisce una vera e propria eccellenza nella pianificazione di uno sviluppo sostenibile del territorio e delle sue risorse, tanto economiche quanto sociali e culturali. L’intera analisi è stata condotta tenendo presente l’importanza della comparazione e della collocazione del singolo caso non solo nel contesto sociale di riferimento, ma anche in sintonia con l’ipotesi della ricerca, e quindi con l’assunto che le pratiche alimentari possano guidare uno sviluppo sostenibile del territorio. Per analizzare la realtà individuata, si è in primo luogo proceduto alla raccolta e all’analisi di dati e informazioni volte alla ricostruzione della sua storia e del suo sviluppo attuale. Le informazioni sono state raccolte attraverso l’analisi di materiali, documenti cartacei e documenti multimediali. Si è poi proceduto con colloqui in profondità a testimoni significativi individuati nell’ambito delle attività promosse da Slow Food, con particolare riferimento alle attività di Terra Madre; le informazioni sono state elaborate con l’ausilio dell’analisi del contenuto. Alla luce di quanto analizzato, tanto a livello teorico quanto a livello empirico, la tesi si conclude con alcune considerazioni che, in linea con la finalità dichiarata di approfondire (più che di confermare o smentire) le ipotesi di partenza circa un ruolo fondamentale delle pratiche alimentari nello sviluppo sostenibile del territorio, non possono comunque non tendere ad una convalida dei concetti introduttivi. Si individuano pertanto spunti importanti per affermare che nelle pratiche alimentari, nei tre momenti in cui trovano specificazione (la produzione, lo scambio, il consumo), siano individuabili quei semi valoriali che possono dare solidità alle ipotesi di partenza, e che quindi - nell’intento di operare per uno sviluppo sostenibile del territorio - sia possibile farne un valido strumento al fine di costruire dei veri e propri percorsi di sostenibilità ancorati ai concetti di tutela della tradizione locale, recupero e salvaguardia dei metodi tradizionali di produzione e conservazione, certificazione di tipicità, controllo della distribuzione, riscatto e promozione delle modalità tradizionali di consumo con particolare riferimento alle culture locali.

The gaseous environment of radio galaxies: a new perspective from high-resolution x-ray spectroscopy

It is known that massive black holes have a profound effect on the evolution of galaxies, and possibly on their formation by regulating the amount of gas available for the star formation. However, how black hole and galaxies communicate is still an open problem, depending on how much of the energy released interacts with the circumnuclear matter. In the last years, most studies of feedback have primarily focused on AGN jet/cavity systems in the most massive galaxy clusters. This thesis intends to investigate the feedback phenomena in radio--loud AGNs from a different perspective studying isolated radio galaxies, through high-resolution spectroscopy. In particular one NLRG and three BLRG are studied, searching for warm gas, both in emission and absorption, in the soft X-ray band. I show that the soft spectrum of 3C33 originates from gas photoionized by the central engine. I found for the first time WA in 3C382 and 3C390.3. I show that the observed warm emitter/absorbers is not uniform and probably located in the NLR. The detected WA is slow implying a mass outflow rate and kinetic luminosity always well below 1% the L(acc) as well as the P(jet). Finally the radio--loud properties are compared with those of type 1 RQ AGNs. A positive correlation is found between the mass outflow rate/kinetic luminosity, and the radio loudness. This seems to suggest that the presence of a radio source (the jet?) affects the distribution of the absorbing gas. Alternatively, if the gas distribution is similar in Seyferts and radio galaxies, the M(out) vs rl relation could simply indicate a major ejection of matter in the form of wind in powerful radio AGNs.

Sulforaphane as a multifunctional neuroprotective molecule to prevent and slow down the progression of Alzheimer’s disease

Oxidative stress has been implicated in the pathogenesis of a number of diseases including neurodegenerative disorders, cancer, ischemia, etc. Alzheimer’s disease (AD) is histopathologically characterized by the presence of extracellular senile plaque (SP), predominantly consisting of fibrillar amyloid-peptide (Aβ), intracellular neurofibrillary tangles (NFTs), composed of hyperphosphorylated tau protein, and cell loss in the selected regions of the brain. However, the pathogenesis of AD remains largely unknown, but a number of hypothesis were proposed for AD mechanisms, which include: the amyloid cascade, excitotoxicity, oxidative stress and inflammation hypothesis, and all of them are based, to some extent on the role of A. Accumulated evidence indicates that the increased levels of ROS may act as important mediators of synaptic loss and eventually promote formation of neurofibrillary tangles and senile plaques. Therefore a vicious circle between ROS and Aaccumulation may accelerate progression of AD. For these reasons, growing attention has focused on oxidative mechanism of Atoxicity as well as the search for novel neuroprotective agents. A strategy to prevent the oxidative stress in neurons may be the use of chemopreventive agents as inducers of antioxidant and phase 2 enzymes. Sulforaphane (SF), derived from corresponding glucoraphanin, glucosinolate found in abundance in cruciferous vegetables, has recently gained attention as a potential neuroprotective compound inducer of antioxidant phase 2 enzymes. Consistent with this evidence, the study is aimed at identifying the SF ability to prevent and counteract the oxidative damage inducted by oligomers of Aβ (1-42) in terms of impairment in the intracellular redox state and cellular death in differentiated human neuroblastoma and microglia primary cultures. In addition we will evaluated the mechanism underlying the SF neuroprotection activity.

Analysis of the Slow Food movement impact on the farmers and rural areas’ sustainable development

The evaluation of the farmers’ communities’ approach to the Slow Food vision, their perception of the Slow Food role in supporting their activity and their appreciation and expectations from participating in the event of Mother Earth were studied. The Unified Theory of Acceptance and Use of Technology (UTAUT) model was adopted in an agro-food sector context. A survey was conducted, 120 questionnaires from farmers attending the Mother Earth in Turin in 2010 were collected. The descriptive statistical analysis showed that both Slow Food membership and participation to Mother Earth Meeting were much appreciated for the support provided to their business and the contribution to a more sustainable and fair development. A positive social, environmental and psychological impact on farmers also resulted. Results showed also an interesting perspective on the possible universality of the Slow Food and Mother Earth values. Farmers declared that Slow Food is supporting them by preserving the biodiversity and orienting them to the use of local resources and reducing the chemical inputs. Many farmers mentioned the language/culture and administration/bureaucratic issues as an obstacle to be a member in the movement and to participate to the event. Participation to Mother Earth gives an opportunity to exchange information with other farmers’ communities and to participate to seminars and debates, helpful for their business development. The absolute majority of positive answers associated to the farmers’ willingness to relate to Slow Food and participate to the next Mother Earth editions negatively influenced the UTAUT model results. A factor analysis showed that the variables associated to the UTAUT model constructs Performance Expectancy and Effort Expectancy were consistent, able to explain the construct variability, and their measurement reliable. Their inclusion in a simplest Technology Acceptance Model could be considered in future researches.

Inverse Static Analysis of Massive Parallel Arrays of Three-State Actuators via Artificial Intelligence

Massive parallel robots (MPRs) driven by discrete actuators are force regulated robots that undergo continuous motions despite being commanded through a finite number of states only. Designing a real-time control of such systems requires fast and efficient methods for solving their inverse static analysis (ISA), which is a challenging problem and the subject of this thesis. In particular, five Artificial intelligence methods are proposed to investigate the on-line computation and the generalization error of ISA problem of a class of MPRs featuring three-state force actuators and one degree of revolute motion.

The evolution of massive clumps in star forming regions

In this thesis two related arguments are investigated: - The first stages of the process of massive star formation, investigating the physical conditions and -properties of massive clumps in different evolutionary stages, and their CO depletion; - The influence that high-mass stars have on the nearby material and on the activity of star formation. I characterise the gas and dust temperature, mass and density of a sample of massive clumps, and analyse the variation of these properties from quiescent clumps, without any sign of active star formation, to clumps likely hosting a zero-age main sequence star. I briefly discuss CO depletion and recent observations of several molecular species, tracers of Hot Cores and/or shocked gas, of a subsample of these clumps. The issue of CO depletion is addressed in more detail in a larger sample consisting of the brightest sources in the ATLASGAL survey: using a radiative tranfer code I investigate how the depletion changes from dark clouds to more evolved objects, and compare its evolution to what happens in the low-mass regime. Finally, I derive the physical properties of the molecular gas in the photon-dominated region adjacent to the HII region G353.2+0.9 in the vicinity of Pismis 24, a young, massive cluster, containing some of the most massive and hottest stars known in our Galaxy. I derive the IMF of the cluster and study the star formation activity in its surroundings. Much of the data analysis is done with a Bayesian approach. Therefore, a separate chapter is dedicated to the concepts of Bayesian statistics.

Study and implementation of control strategies for polymerization processes assisted by atmospheric pressure plasma jets

In recent years, polymerization processes assisted by atmospheric pressure plasma jets (APPJs) have received increasing attention in numerous industrially relevant sectors since they allow to coat complex 3D substrates without requiring expensive vacuum systems. Therefore, advancing the comprehension of these processes has become a high priority topic of research. This PhD dissertation is focused on the study and the implementation of control strategies for a polymerization process assisted by an atmospheric pressure single electrode plasma jet. In the first section, a study of the validity of the Yasuda parameter (W/FM) as controlling parameter in the polymerization process assisted by the plasma jet and an aerosolized fluorinated silane precursor is proposed. The surface characterization of coatings deposited under different W/FM values reveals the presence of two very well-known deposition domains, thus suggesting the validity of W/FM as controlling parameter. In addition, the key role of the Yasuda parameter in the process is further demonstrated since coatings deposited under the same W/FM exhibit similar properties, regardless of how W/FM is obtained. In the second section, the development of a methodology for measuring the energy of reactions in the polymerization process assisted by the plasma jet and vaporized hexamethyldisiloxane is presented. The values of energy per precursor molecule are calculated through the identification and resolution of a proper equivalent electrical circuit. To validate the methodology, these energy values are correlated to the bond energies in the precursor molecule and to the properties of deposited thin films. It is shown that the precursor fragmentation in the discharge and the coating characteristics can be successfully explained according to the obtained values of energy per molecule. Through a detailed discussion of the limits and the potentialities of both the control strategies, this dissertation provides useful insights into the control of polymerization processes assisted by APPJs.

A hydrodynamical view on the mass accretion onto massive halos

This Thesis presents the results of my work on how galaxy clusters form by the accretion of sub-clumps and diffuse materials, and how the accreted energy is distributed in the X-ray emitting plasma. Indeed, on scales larger than tens of millions of light years, the Universe is self-organised by gravity into a spiderweb, the Cosmic Web. Galaxy clusters are the knots of this Cosmic Web, but a strong definition of filaments (which link different knots) and their physical proprieties, is still uncertain. Even if this pattern was determined by studying the spatial distribution of galaxies in the optical band, recently, also in the X-rays probes of filamentary structures around galaxy clusters were obtained. Therefore, given these observational facilities, the galaxy clusters’ outskirts are the best candidate regions to detect filaments and study their physical characteristics. However, from X-rays observations, we have only a few detections of cosmic filaments to date. On the other hand, it is crucial to understand how the accreted energy is dissipated in the baryon content of galaxy clusters and groups. Indeed, it is well known that in the central region of galaxy clusters and groups, the baryon fraction increases with the halo mass. On the outer region, the lack of X-rays constraints influences our understanding of the evolution of baryons in the halos volume. The standard assumption of “closed-box” system, for which the baryon fraction should approach the cosmological ratio Omega_bar/Omega_m, for galaxy clusters and groups seems to be too strong, especially for less massive objects. Moreover, a complete redshift evolution of baryons in galaxy clusters and groups is still missing.

Grant-free protocols for massive multiple access

In next generation Internet-of-Things, the overhead introduced by grant-based multiple access protocols may engulf the access network as a consequence of the proliferation of connected devices. Grant-free access protocols are therefore gaining an increasing interest to support massive multiple access. In addition to scalability requirements, new demands have emerged for massive multiple access, including latency and reliability. The challenges envisaged for future wireless communication networks, particularly in the context of massive access, include: i) a very large population size of low power devices transmitting short packets; ii) an ever-increasing scalability requirement; iii) a mild fixed maximum latency requirement; iv) a non-trivial requirement on reliability. To this aim, we suggest the joint utilization of grant-free access protocols, massive MIMO at the base station side, framed schemes to let the contention start and end within a frame, and succesive interference cancellation techniques at the base station side. In essence, this approach is encapsulated in the concept of coded random access with massive MIMO processing. These schemes can be explored from various angles, spanning the protocol stack from the physical (PHY) to the medium access control (MAC) layer. In this thesis, we delve into both of these layers, examining topics ranging from symbol-level signal processing to succesive interference cancellation-based scheduling strategies. In parallel with proposing new schemes, our work includes a theoretical analysis aimed at providing valuable system design guidelines. As a main theoretical outcome, we propose a novel joint PHY and MAC layer design based on density evolution on sparse graphs.