An efficient Jeans modelling of axisymmetric galaxies with multiple stellar components

Dynamical models of stellar systems represent a powerful tool to study their internal structure and dynamics, to interpret the observed morphological and kinematical fields, and also to support numerical simulations of their evolution. We present a method especially designed to build axisymmetric Jeans models of galaxies, assumed as stationary and collisionless stellar systems. The aim is the development of a rigorous and flexible modelling procedure of multicomponent galaxies, composed of different stellar and dark matter distributions, and a central supermassive black hole. The stellar components, in particular, are intended to represent different galaxy structures, such as discs, bulges, halos, and can then have different structural (density profile, flattening, mass, scale-length), dynamical (rotation, velocity dispersion anisotropy), and population (age, metallicity, initial mass function, mass-to-light ratio) properties. The theoretical framework supporting the modelling procedure is presented, with the introduction of a suitable nomenclature, and its numerical implementation is discussed, with particular reference to the numerical code JASMINE2, developed for this purpose. We propose an approach for efficiently scaling the contributions in mass, luminosity, and rotational support, of the different matter components, allowing for fast and flexible explorations of the model parameter space. We also offer different methods of the computation of the gravitational potentials associated of the density components, especially convenient for their easier numerical tractability. A few galaxy models are studied, showing internal, and projected, structural and dynamical properties of multicomponent galaxies, with a focus on axisymmetric early-type galaxies with complex kinematical morphologies. The application of galaxy models to the study of initial conditions for hydro-dynamical and $N$-body simulations of galaxy evolution is also addressed, allowing in particular to investigate the large number of interesting combinations of the parameters which determine the structure and dynamics of complex multicomponent stellar systems.

Unveiling the unknown of cool stars with high-resolution spectroscopy

Cool giant and supergiant stars are among the brightest populations in any stellar system and they are easily observable out to large distances, especially at infrared wavelengths. These stars also dominate the integrated light of star clusters in a wide range of ages, making them powerful tracers of stellar populations in more distant galaxies. High-resolution near-IR spectroscopy is a key tool for quantitatively investigating their kinematic, evolutionary and chemical properties. However, the systematic exploration and calibration of the NIR spectral diagnostics to study these cool stellar populations based on high-resolution spectroscopy is still in its pioneering stage. Any effort to make progress in the field is innovative and of impact on stellar archaeology and stellar evolution. This PhD project takes the challenge of exploring that new parameter space and characterizing the physical properties, the chemical content and the kinematics of cool giants and supergiants in selected disc fields and clusters of our Galaxy, with the ultimate goal of tracing their past and recent star formation and chemical enrichment history. By using optical HARPS-N and near-infrared GIANO-B high-resolution stellar spectra in the context of the large program SPA-Stellar Population Astrophysics: the detailed, age-resolved chemistry of the Milky Way disk” (PI L. Origlia), an extensive study of Arcturus, a standard calibrator for red giant stars, has been performed. New diagnostics of stellar parameters as well as optimal linelists for chemical analysis have been provided. Then, such diagnostics have been used to determine evolutionary properties, detailed chemical abundances of almost 30 different elements and mixing processes of a homogeneous sample of red supergiant stars in the Perseus complex.

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.

Exploring the internal kinematics of Galactic Globular Cluster cores

Globular clusters (GCs) are traditionally described as simple quasi-relaxed non-rotating stellar systems, characterized by spherical symmetry and isotropy in velocity space. However, recent studies have shown deviations from isotropic velocity distributions and significant internal rotation in many GCs, suggesting that their internal structure and kinematics are more complex than previously thought. The aim of this thesis is to investigate the internal kinematics of Galactic Globular Clusters (GGCs) as part of the Multi-Instrument Kinematic Survey (MIKiS), which exploits the capabilities of different ESO-VLT spectrographs to obtain comprehensive velocity dispersion (VD) and rotation profiles of GGCs. Moreover, this thesis has the particular goal of unraveling the kinematics of GC cores, which are still largely unexplored, by taking advantage of the exceptional spatial resolution of the adaptive-optics assisted integral-field spectrograph MUSE/NFM. The thesis presents a thorough kinematic study of three GGCs NGC 1904, NGC 6440, and NGC 6569. By combining the data sets acquired with four different spectrographs, we obtained the radial velocity (RV) of more than 1000 individual stars in each cluster, sampling from the innermost to the outermost regions. This allowed us to obtain the entire VD profile of each cluster and exclude the presence of an intermediate-mass black hole in the core of NGC 1904, at odds with previous findings obtained from integrated-light spectra. The studies also revealed signatures of internal rotation in each of the GCs studied. These results, supported by those of N-body simulations, prove that GCs were born with a significant initial rotation that they gradually lost through internal two-body relaxation and angular momentum loss carried away by escaping stars. Furthermore, we derived the structural parameters of NGC 6440 and NGC 6569, obtaining a comprehensive overview of the internal kinematics and structure of these GCs, which is necessary to properly reconstruct the evolutionary history of these systems.

Cross-population radio galaxies as a test of the jet-accretion relationship

Radio galaxies (RGs) are extremely relevant in addressing important unknowns concerning the interaction among black hole accretion, radio jets, and the environment. In the classical scheme, their accretion rate and ejection of relativistic jets are directly linked: efficient accretion (HERG) is associated with powerful edge-brightened jets (FRIIs); inefficient accretion (LERG) is associated with weak edge-darkened jets (FRIs). The observation of RGs with an inefficient engine associated with edge-brightened radio emission (FRII-LERGs) broke this scheme. FRII-LERGs constitute a suitable population to explore how accretion and ejection are linked and evaluate the environment's role in shaping jets. To this aim, we performed a multiwavelength study of different RGs catalogs spanning from Jy to mJy flux densities. At first, we investigated the X-ray properties of a sample of 51 FRIIs belonging to the 3CR catalog at z<0.3. Two hypotheses were invoked to explain FRII-LERGs behavior: evolution from classical FRIIs; the role of the environment. Next, we explored the mJy sky by studying the optical-radio properties of hundreds of RGs at z<0.15 (Best & Heckman 2012 sample). FRII-LERGs appear more similar to the old FRI-LERGs than to the young FRII-HERGs. These results point towards an evolutive scenario, however, nuclear time scale changes, star population aging, and kpc-Mpc radio structure modification do not agree. The role of the Mpc environment was then investigated. The Wen et al. 2015 galaxy clusters sample, built exploiting the SDSS survey, allowed us to explore the habitat of 7219 RGs at z<0.3. Most RGs are found to live in outside clusters. For these sources, differences among RG classes are still present. Thus, the environment is not the key parameter, and the possibility of intrinsic differences was reconsidered: we speculated that different black hole properties (spin and magnetic field at its horizon) could determine the observed spread in jet luminosity.

New indicators of star cluster dynamical evolution

This thesis presents a study of globular clusters (GCs), based on analysis of Monte Carlo simulations of globular clusters (GCs) with the aim to define new empirical parameters measurable from observations and able to trace the different phases of their dynamical evolution history. During their long term dynamical evolution, due to mass segregation and and dynamical friction, massive stars transfer kinetic energy to lower-mass objects, causing them to sink toward the cluster center. This continuous transfer of kinetic energy from the core to the outskirts triggers the runaway contraction of the core, known as "core collapse" (CC), followed by episodes of expansion and contraction called gravothermal oscillations. Clearly, such an internal dynamical evolution corresponds to significant variations also of the structure of the system. Determining the dynamical age of a cluster can be challenging as it depends on various internal and external properties. The traditional classification of GCs as CC or post-CC systems relies on detecting a steep power-law cusp in the central density profile, which may not always be reliable due to post-CC oscillations or other processes. In this thesis, based on the normalized cumulative radial distribution (nCRD) within a fraction of the half-mass radius is analyzed, and three diagnostics (A5, P5, and S2.5) are defined. These diagnostics show sensitivity to dynamical evolution and can distinguish pre-CC clusters from post-CC clusters.The analysis performed using multiple simulations with different initial conditions, including varying binary fractions and the presence of dark remnants showed the time variations of the diagnostics follow distinct patterns depending on the binary fraction and the retention or ejection of black holes. This analysis is extended to a larger set of simulations matching the observed properties of Galactic GCs, and the parameters show a potential to distinguish the dynamical stages of the observed clusters as well.

Unveiling the expansion history of the universe with cosmic chronometers and gravitational waves

This Thesis explores two novel and independent cosmological probes, Cosmic Chronometers (CCs) and Gravitational Waves (GWs), to measure the expansion history of the Universe. CCs provide direct and cosmology-independent measurements of the Hubble parameter H(z) up to z∼2. In parallel, GWs provide a direct measurement of the luminosity distance without requiring additional calibration, thus yielding a direct measurement of the Hubble constant H0=H(z=0). This Thesis extends the methodologies of both of these probes to maximize their scientific yield. This is achieved by accounting for the interplay of cosmological and astrophysical parameters to derive them jointly, study possible degeneracies, and eventually minimize potential systematic effects. As a legacy value, this work also provides interesting insights into galaxy evolution and compact binary population properties. The first part presents a detailed study of intermediate-redshift passive galaxies as CCs, with a focus on the selection process and the study of their stellar population properties using specific spectral features. From their differential aging, we derive a new measurement of the Hubble parameter H(z) and thoroughly assess potential systematics. In the second part, we develop a novel methodology and pipeline to obtain joint cosmological and astrophysical population constraints using GWs in combination with galaxy catalogs. This is applied to GW170817 to obtain a measurement of H0. We then perform realistic forecasts to predict joint cosmological and astrophysical constraints from black hole binary mergers for upcoming gravitational wave observatories and galaxy surveys. Using these two probes we provide an independent reconstruction of H(z) with direct measurements of H0 from GWs and H(z) up to z∼2 from CCs and demonstrate that they can be powerful independent probes to unveil the expansion history of the Universe.

Gli effetti della terapia di resincronizzazione cardiaca in pazienti con fibrillazione atriale permanente sulla sopravvivenza a lungo-termine: l'importanza dell'ablazione del nodo atrio-ventricolare

La terapia di resincronizzazione cardiaca (TRC) è un presidio non farmacologico che riduce la mortalità e la morbosità nei pazienti con scompenso refrattario alla terapia medica. La maggior parte dei dati riguardanti gli effetti della TRC coinvolgono i pazienti con le indicazioni consolidate seguenti: classe NYHA III-IV, ritardo della conduzione ventricolare (QRS>opp= 20 msec), disfunzione sistolica ventricolare sinistra (frazione di eiezione ventricolare sinistra >opp= 35%) e ritmo sinusale (RS). Mentre è noto che la fibrillazione atriale permanente (FA) sia presente in una porzione consistente dei pazienti con scompenso cardiaco, vi sono pochi dati riguardanti la sopravvivenza e gli effetti a lungo-termine della TRC in pazienti con scompenso cardiaco e fibrillazione atriale (FA); la maggior parte degli studi sono osservazionali ed hanno dimostrato che la TRC potrebbe conferire dei benefici a corto e medio termine anche in pazienti con FA permanente. Solo recentemente un ampio studio osservazionale ha descritto che, a lungo-termine, la TRC migliora significativamente la capacità funzionale, la frazione di eiezione e induce il rimodellamento inverso del ventricolo sinistro solamente in quei pazienti con FA dove la TRC viene combinata con l’ablazione del nodo atrio-ventricolare (NAV). La strategia ablativa del NAV infatti conferendo una stimolazione completa e costante, permette di eliminare gli effetti del ritmo spontaneo di FA (ritmo irregolare e tendenzialmente tachicardico) cheinterferisce in maniera importante con la stimolazione biventricolare in particolare durante gli sforzi fisici. Sulla base di queste premesse il presente studio si propone di valutare gli effetti a lungo-termine della TRC su pazienti con scompenso cardiaco e FA permanente focalizzando su due aspetti principali: 1) confrontando la sopravvivenza di pazienti con FA permanente rispetto ai pazienti in RS; 2) confrontando la sopravvivenza di pazienti in FA suddivisi secondo la modalità di controllo della frequenza con somministrazione di farmaci antiaritmici (gruppo FA-farm) oppure mediante controllo ablazione del NAV (gruppo FA-abl). Metodi e risultati: Sono presentati i dati di 1303 pazienti sottoposti consecutivamente ad impianto di dispositivo per la TRC e seguiti per un periodo mediano di 24 mesi. Diciotto pazienti sono stati persi durante il follow-up per cui la popolazione dello studio è rappresentata da una popolazione totale di 1295 pazienti di cui 1042 in RS e 243 (19%) in FA permanente. Nei pazienti con FA il controllo della frequenza cardiaca è stato effettuato mediante la somministrazione di farmaci anti-aritmici (gruppo FA-farm: 125 pazienti) oppure mediante ablazione del NAV (FA-abl: 118 pazienti). Rispetto ai pazienti in RS, i pazienti in FA permanente erano significativamente più vecchi, più spesso presentavano eziologia nonischemica, avevano una frazione di eiezione più elevata al preimpianto, una durata del QRS minore e erano più raramente trattati con un defibrillatore. Lungo un follow-up mediano di 24 mesi, 170/1042 pazienti in RS e 39/243 in FA sono deceduti (l’incidenza di mortalità a 1 anno era di 8,4% e 8,9%, rispettivamente). I rapporti di rischio derivanti dall’analisi multivariata con il 95% dell’intervallo di confidenza (HR, 95% CI) erano simili sia per la morte per tutte le cause che per la morte cardiaca (0.9 [0.57-1.42], p=0.64 e 1.00 [0.60-1.66] p=0.99, rispettivamente). Fra i pazienti con FA, il gruppo FA-abl presentava una durata media del QRS minore ed era meno frequentemente trattato con il defibrillatore impiantabile rispetto al gruppo FA-farm. Soli 11/118 pazienti del FA-abl sono deceduti rispetto a 28/125 nel gruppo FA-farm (mortalità cumulativa a 1 anno di 9,3% e 15,2% rispettivamente, p<0.001), con HR, 95% CI per FA-abl vs FA-farm di 0.15 [0.05-0.43],,p<0.001 per la mortalità per tutte le cause, di 0.18 [0.06-0.57], p=0.004 per la mortalità cardiaca, e di 0.09 [0.02-0.42], p<0.002 per la mortalità da scompenso cardiaco. Conclusioni: I pazienti con scompenso cardiaco e FA permanente trattati con la TRC presentano una simile sopravvivenza a lungo-termine di pazienti in RS. Nei pazienti in FA l’ablazione del NAV in aggiunta alla TRC migliora significativamente la sopravvivenza rispetto alla sola TRC; questo effetto è ottenuto primariamente attraverso una riduzione della morte per scompenso cardiaco.

Effetti dell'acido urico sulle cellule glomerulari mesangiali: meccanismi intracellulari di trasduzione del segnale e possibili implicazioni nella progressione del danno renale e nella sindrome infiammatoria in corso di nefropatie croniche

Uric acid is a major inducer of inflammation in renal interstitium and may play a role in the progression of renal damage in hyperuricemic subjects with primary nephropathies, renal vascular disease, and essential hypertension. At the same time, UA also acts as a water-soluble scavenger of reactive oxygen species. We evaluated the cellular effects of UA on cultured HMC as a potential interstitial target for abnormally elevated levels in acute and chronic renal disease. Intracellular free Ca2+ ([Ca2+]i) was monitored by microfluorometry of fura 2-loaded cells, while oxidation of intracellularly trapped non-fluorescent 2’,7’-dichlorofluorescein diacetate (DCFHDA, 20 uM) was employed to assess the generation of reactive oxygen species during 12-hr incubations with various concentrations of UA or monosodium urate. Fluorescent metabolites of DCFH-DA in the culture media of HMC were detected at 485/530 nm excitation/emission wavelengths, respectively. UA dose-dependently lowered resting [Ca2+]i (from 102±9 nM to 95±3, 57±2, 48±6 nM at 1-100 uM UA, respectively, p <0.05), leaving responses to vasoconstrictors such as angiotensin II unaffected. The effect was not due to Ca2+/H+ exchange upon acidification of the bathing media, as acetate, glutamate, lactate and other organic acids rather increased [Ca2+]i (to max. levels of 497±42 nM with 0.1 mM acetate). The decrease of [Ca2+]i was abolished by raising extracellular Ca2+ and not due to effects on Ca2+ channels or activation of Ca2+-ATPases, since unaffected by thapsigargin. The process rather appeared sensitive to removal of extracellular Na+ in combination with blockers of Na+/Ca2+ exchange, such as 2’,4’-dichlorobenzamil, pointing to a countertransport mechanism. UA dose-dependently prompted the extracellular release of oxidised DCFH (control 37±2 relative fluorescence units (RFU)/ml, 0.1uM 47±2, 1 uM 48±2, 10 uM 51±4, 0.1 mM 53±4; positive control, 10 uM sodium nitroprusside 92±5 RFU/ml, p<0.01). In summary, UA interferes with Ca2+ transport in cultured HMC, triggering oxidative stress which may initiate a sequence of events leading to interstitial injury and possibly amplifying renal vascular damage and/or the progression of chronic disease.

Valutazione della persistenza in trattamento antiipertensivo: un’analisi multilivello paziente-medico attraverso modelli con effetti casuali

Introduzione L’importanza clinica, sociale ed economica del trattamento dell’ipertensione arteriosa richiede la messa in opera di strumenti di monitoraggio dell’uso dei farmaci antiipertensivi che consentano di verificare la trasferibilità alla pratica clinica dei dati ottenuti nelle sperimentazioni. L’attuazione di una adatta strategia terapeutica non è un fenomeno semplice da realizzare perché le condizioni in cui opera il Medico di Medicina Generale sono profondamente differenti da quelle che si predispongono nell’esecuzione degli studi randomizzati e controllati. Emerge, pertanto, la necessità di conoscere le modalità con cui le evidenze scientifiche trovano reale applicazione nella pratica clinica routinaria, identificando quei fattori di disturbo che, nei contesti reali, limitano l’efficacia e l’appropriatezza clinica. Nell’ambito della terapia farmacologica antiipertensiva, uno di questi fattori di disturbo è costituito dalla ridotta aderenza al trattamento. Su questo tema, recenti studi osservazionali hanno individuato le caratteristiche del paziente associate a bassi livelli di compliance; altri hanno focalizzato l’attenzione sulle caratteristiche del medico e sulla sua capacità di comunicare ai propri assistiti l’importanza del trattamento farmacologico. Dalle attuali evidenze scientifiche, tuttavia, non emerge con chiarezza il peso relativo dei due diversi attori, paziente e medico, nel determinare i livelli di compliance nel trattamento delle patologie croniche. Obiettivi Gli obiettivi principali di questo lavoro sono: 1) valutare quanta parte della variabilità totale è attribuibile al livello-paziente e quanta parte della variabilità è attribuibile al livello-medico; 2) spiegare la variabilità totale in funzione delle caratteristiche del paziente e in funzione delle caratteristiche del medico. Materiale e metodi Un gruppo di Medici di Medicina Generale che dipendono dall’Azienda Unità Sanitaria Locale di Ravenna si è volontariamente proposto di partecipare allo studio. Sono stati arruolati tutti i pazienti che presentavano almeno una misurazione di pressione arteriosa nel periodo compreso fra il 01/01/1997 e il 31/12/2002. A partire dalla prima prescrizione di farmaci antiipertensivi successiva o coincidente alla data di arruolamento, gli assistiti sono stati osservati per 365 giorni al fine di misurare la persistenza in trattamento. La durata del trattamento antiipertensivo è stata calcolata come segue: giorni intercorsi tra la prima e l’ultima prescrizione + proiezione, stimata sulla base delle Dosi Definite Giornaliere, dell’ultima prescrizione. Sono stati definiti persistenti i soggetti che presentavano una durata del trattamento maggiore di 273 giorni. Analisi statistica I dati utilizzati per questo lavoro presentano una struttura gerarchica nella quale i pazienti risultano “annidati” all’interno dei propri Medici di Medicina Generale. In questo contesto, le osservazioni individuali non sono del tutto indipendenti poiché i pazienti iscritti allo stesso Medico di Medicina Generale tenderanno ad essere tra loro simili a causa della “storia comune” che condividono. I test statistici tradizionali sono fortemente basati sull’assunto di indipendenza tra le osservazioni. Se questa ipotesi risulta violata, le stime degli errori standard prodotte dai test statistici convenzionali sono troppo piccole e, di conseguenza, i risultati che si ottengono appaiono “impropriamente” significativi. Al fine di gestire la non indipendenza delle osservazioni, valutare simultaneamente variabili che “provengono” da diversi livelli della gerarchia e al fine di stimare le componenti della varianza per i due livelli del sistema, la persistenza in trattamento antiipertensivo è stata analizzata attraverso modelli lineari generalizzati multilivello e attraverso modelli per l’analisi della sopravvivenza con effetti casuali (shared frailties model). Discussione dei risultati I risultati di questo studio mostrano che il 19% dei trattati con antiipertensivi ha interrotto la terapia farmacologica durante i 365 giorni di follow-up. Nei nuovi trattati, la percentuale di interruzione terapeutica ammontava al 28%. Le caratteristiche-paziente individuate dall’analisi multilivello indicano come la probabilità di interrompere il trattamento sia più elevata nei soggetti che presentano una situazione clinica generale migliore (giovane età, assenza di trattamenti concomitanti, bassi livelli di pressione arteriosa diastolica). Questi soggetti, oltre a non essere abituati ad assumere altre terapie croniche, percepiscono in minor misura i potenziali benefici del trattamento antiipertensivo e tenderanno a interrompere la terapia farmacologica alla comparsa dei primi effetti collaterali. Il modello ha inoltre evidenziato come i nuovi trattati presentino una più elevata probabilità di interruzione terapeutica, verosimilmente spiegata dalla difficoltà di abituarsi all’assunzione cronica del farmaco in una fase di assestamento della terapia in cui i principi attivi di prima scelta potrebbero non adattarsi pienamente, in termini di tollerabilità, alle caratteristiche del paziente. Anche la classe di farmaco di prima scelta riveste un ruolo essenziale nella determinazione dei livelli di compliance. Il fenomeno è probabilmente legato ai diversi profili di tollerabilità delle numerose alternative terapeutiche. L’appropriato riconoscimento dei predittori-paziente di discontinuità (risk profiling) e la loro valutazione globale nella pratica clinica quotidiana potrebbe contribuire a migliorare il rapporto medico-paziente e incrementare i livelli di compliance al trattamento. L’analisi delle componenti della varianza ha evidenziato come il 18% della variabilità nella persistenza in trattamento antiipertensivo sia attribuibile al livello Medico di Medicina Generale. Controllando per le differenze demografiche e cliniche tra gli assistiti dei diversi medici, la quota di variabilità attribuibile al livello medico risultava pari al 13%. La capacità empatica dei prescrittori nel comunicare ai propri pazienti l’importanza della terapia farmacologica riveste un ruolo importante nel determinare i livelli di compliance al trattamento. La crescente presenza, nella formazione dei medici, di corsi di carattere psicologico finalizzati a migliorare il rapporto medico-paziente potrebbe, inoltre, spiegare la relazione inversa, particolarmente evidente nella sottoanalisi effettuata sui nuovi trattati, tra età del medico e persistenza in trattamento. La proporzione non trascurabile di variabilità spiegata dalla struttura in gruppi degli assistiti evidenzia l’opportunità e la necessità di investire nella formazione dei Medici di Medicina Generale con l’obiettivo di sensibilizzare ed “educare” i medici alla motivazione ma anche al monitoraggio dei soggetti trattati, alla sistematica valutazione in pratica clinica dei predittori-paziente di discontinuità e a un appropriato utilizzo della classe di farmaco di prima scelta. Limiti dello studio Uno dei possibili limiti di questo studio risiede nella ridotta rappresentatività del campione di medici (la partecipazione al progetto era su base volontaria) e di pazienti (la presenza di almeno una misurazione di pressione arteriosa, dettata dai criteri di arruolamento, potrebbe aver distorto il campione analizzato, selezionando i pazienti che si recano dal proprio medico con maggior frequenza). Questo potrebbe spiegare la minore incidenza di interruzioni terapeutiche rispetto a studi condotti, nella stessa area geografica, mediante database amministrativi di popolazione. Conclusioni L’analisi dei dati contenuti nei database della medicina generale ha consentito di valutare l’impiego dei farmaci antiipertensivi nella pratica clinica e di stabilire la necessità di porre una maggiore attenzione nella pianificazione e nell’ottenimento dell’obiettivo che il trattamento si prefigge. Alla luce dei risultati emersi da questa valutazione, sarebbe di grande utilità la conduzione di ulteriori studi osservazionali volti a sostenere il progressivo miglioramento della gestione e del trattamento dei pazienti a rischio cardiovascolare nell’ambito della medicina generale.

Effetti del chitosano su composti polifenolici in colture cellulari di vite: aspetti molecolari e metabolici

Polyphenols, including flavonoids and stilbenes, are an essential part of human diet and constitute one of the most abundant and ubiquitous group of plant secondary metabolites. The level of these compounds is inducible by stress or fungal attack, so attempts are being made to identify likely biotic and abiotic elicitors and to better understand the underlying mechanism. Resveratrol (3,5,4’-trihydroxystilbene), which belongs to the stilbene family, is a naturally occurring polyphenol, found in several fruits, vegetables and beverages including red wine. It is one of the most important plant polyphenols with proved benefic activity on animal health. In the last two decades, the potential protective effects of resveratrol against cardiovascular and neurodegenerative diseases, as well as the chemopreventive properties against cancer, have been largely investigated. The most important source of polyphenols and in particular resveratrol for human diet is grape (Vitis vinifera). Since stilbenes and flavonoids play a very important role in plant defence responses and enviromental interactions, and their effects on human health seem promising, the aim of the research of this Thesis was to study at different levels the activation and the regulation of their biosynthetic pathways after chitosan treatment. Moreover, the polyphenol production in grape cells and the optimisation of cultural conditions bioreactor scale-up, were also investigated. Cell suspensions were obtained from cv. Barbera (Vitis vinifera L.) petioles and were treated with a biotic elicitor, chitosan (50 μg/mL, dissolved in acetic acid) to promote phenylpropanoid metabolism. Chitosan is a D-glucosamine polymer from fungi cell wall and therefore mimes fungal pathogen attack. Liquid cultures have been monitored for 15 days, measuring cell number, cell viability, pH and grams of fresh weight. The endogenous and released amounts of 7 stilbenes (trans and cis isomers of resveratrol, piceid and resveratroloside, and piceatannol), gallic acid, 6 hydroxycinnamic acids (trans-cinnamic, p-coumaric, caffeic, ferulic, sinapic and chlorogenic acids), 5 catechines (catechin, epicatechin, epigallocatechin-gallate (EGCG), epigallocatechin and epicatechin-gallate) and other 5 flavonoids (chalcon, naringenin, kaempferol, quercetin and rutin) in cells and cultural medium, were measured by HPLC-DAD analysis and total anthocyanins were quantified by spectrophotometric analysis. Chitosan was effective in stimulating trans-resveratrol endogenous accumulation with a sharp peak at day 4 (exceeding acetic acid and water controls by 36% and 63%, respectively), while it did not influence the production of the cis-isomer. Compared to both water and acetic acid controls, chitosan decreased the release of both trans- and cis-resveratrol respect to controls. No effect was shown on the accumulation of single resveratrol mono-glucoside isomers, but considering their total amount, normalized for the relative water control, it was possible to evidence an increase in both accumulation and release of those compounds, in chitosan-treated cells, throughout the culture period and particularly during the second week. Many of the analysed flavonoids and hydroxycinnamic acids were not present or detectable in trace amounts. Catechin, epicatechin and epigallocatechin-gallate (EGCG) were detectable both inside the cells and in the culture media, but chitosan did not affect their amounts. On the contrary, total anthocyanins have been stimulated by chitosan and their level, from day 4 to 14, was about 2-fold higher than in both controls, confirming macroscopic observations that treated suspensions showed an intense brown-red color, from day 3 onwards. These elicitation results suggest that chitosan selectively up-regulates specific biosynthetic pathways, without modifying the general accumulation pattern of other flavonoids. Proteins have been extracted from cells at day 4 of culture (corresponding to the production peak of trans-resveratrol) and separated by bidimensional electrophoresis. The 73 proteins that showed a consistently changed amount between untreated, chitosan and acetic acid (chitosan solvent) treated cells, have been identified by mass spectrometry. Chitosan induced an increase in stilbene synthase (STS, the resveratrol biosynthetic enzyme), chalcone-flavanone isomerase (CHI, that switches the pathway from chalcones to flavones and anthocyanins), pathogenesis-related proteins 10 (PRs10, a large family of defence proteins), and a decrease in many proteins belonging to primary metabolisms. A train of six distinct spots of STS encoded by the same gene and increased by chitosan, was detected on the 2-D gels, and related to the different phosphorylation degree of STS spots. Northern blot analyses have been performed on RNA extracted from cells treated with chitosan and relative controls, using probes for STS, PAL (phenylalanine ammonia lyase, the first enzyme of the biosynthetic pathway), CHS (chalcone synthase, that shares with STS the same precursors), CHI and PR-10. The up-regulation of PAL, CHS and CHI transcript expression levels correlated with the accumulation of anthocyanins. The strong increase of different molecular weight PR-10 mRNAs, correlated with the 11 PR-10 protein spots identified in proteomic analyses. The sudden decrease in trans-resveratrol endogenous accumulation after day 4 of culture, could be simply explained by the diminished resveratrol biosynthetic activity due to the lower amount of biosynthetic enzymes. This might be indirectly demonstrated by northern blot expression analyses, that showed lower levels of phenylalanine ammonia lyase (PAL) and stilbene synthase (STS) mRNAs starting from day 4. Other possible explanations could be a resveratrol oxidation process and/or the formation of other different mono-, di-glucosides and resveratrol oligomers such as viniferins. Immunolocalisation experiments performed on grape protoplasts and the subsequent analyses by confocal microscope, showed that STS, and therefore the resveratrol synthetic site, is mostly associated to intracellular membranes close to the cytosolic side of plasma membrane and in a smaller amount is localized in the cytosol. STS seemed not to be present inside vacuole and nucleus. There were no differences in the STS intracellular localisation between the different treatments. Since it was shown that stilbenes are largely released in the culture medium and that STS is a soluble protein, a possible interaction of STS with a plasma membrane transporter responsible for the extrusion of stilbenes in the culture medium, might be hypothesized. Proteomic analyses performed on subcellular fractions identified in the microsomial fraction 5 proteins taking part in channel complexes or associated with channels, that significantly changed their amount after chitosan treatment. In soluble and membrane fractions respectively 3 and 4 STS and 6 and 3 PR-10 have been identified. Proteomic results obtained from subcellular fractions substantially confirmed previous result obtained from total cell protein extracts and added more information about protein localisation and co-localisation. The interesting results obtained on Barbera cell cultures with the aim to increase polyphenol (especially stilbenes) production, have encouraged scale up tests in 1 litre bioreactors. The first trial fermentation was performed in parallel with a normal time-course in 20 mL flasks, showing that the scale-up (bigger volume and different conditions) process influenced in a very relevant way stilbenes production. In order to optimise culture parameters such as medium sucrose amount, fermentation length and inoculum cell concentration, few other fermentations were performed. Chitosan treatments were also performed. The modification of each parameter brought relevant variations in stilbenes and catechins levels, so that the production of a certain compound (or class of compounds) could be hypothetically promoted by modulating one or more culture parameters. For example the catechin yield could be improved by increasing sucrose content and the time of fermentation. The best results in stilbene yield were obtained in a 800 mL fermentation inoculated with 10.8 grams of cells and supplemented with chitosan. The culture was fed with MS medium added with 30 g/L sucrose, 25 μg/mL rifampicin and 50 μg/mL of chitosan, and was maintained at 24°C, stirred by marine impeller at 100 rpm and supplied of air at 0.16 L/min rate. Resveratroloside was the stilbene present in the larger amount, 3-5 times more than resveratrol. Because resveratrol glucosides are similarly active and more stable than free resveratrol, their production using a bioreactor could be a great advantage in an hypothetical industrial process. In my bioreactor tests, stilbenes were mainly released in the culture medium (60-80% of the total) and this fact could be another advantage for industrial applications, because it allows recovering the products directly from the culture medium without stopping the fermentation and/or killing the cells. In my best cultural conditions, it was possible to obtain 3.95 mg/L of stilbenes at day 4 (maximum resveratrol accumulation) and 5.13 mg/L at day 14 (maximum resveratroloside production). In conclusion, chitosan effect in inducing Vitis vinifera defense mechanisms can be related to its ability to increase the intracellular content of a large spectrum of antioxidants, and in particular of resveratrol, its derivates and anthocyanins. Its effect can be observed at transcriptional, proteomic (variation of soluble and membrane protein amounts) and metabolic (polyphenols production) level. The chitosan ability to elicit specific plant matabolisms can be useful to produce large quantities of antioxidant compounds from cell culture in bioreactor.

Conoscenza e consapevolezza sugli effetti biologici degli ultrasuoni nella pratica clinica in Italia: risultati di una inchiesta con questionario tra ecografisti della socetà italiana di ultrasonologia in medicina e biologia (S.I.U.M.B.)

Background New potential hazards in the use of ultrasound (US) are implied in new diagnostic applications of US, such as contrast enhanced US. Aim To assess the level of awareness and knowledge on safety issues of clinical use of US among physicians who are members of the Italian National Society for Ultrasound (SIUMB) Materials and methods A questionnaire including 11 multiple choice quiz was sent by e-mail to members of SIUMB, who preliminarly agreed to participate in this initiative. The answers were received anonimously and statistically analyzed. Results The number of returned valid questionnaires was 97 (8 were considered not valid for less than 10 answers filled). Mean age of the responders was 44 years old, and the average time the physician has been performing ultrasound examinations was 13 years. The principal workplace (70%) was a public Hospital. Physicians seemed to know the general definitions of principal safety-parameters, but few of them knew the definition of specific indexes. There was a general knowledge about the safe use of ultrasound in obstetrics, but there was a poor knowledge of biological effects of US: only about 37% answered correctly to questions about damage of vasculature of lung by high Mechanical Index US investigation and about the increase of temperature under the probe, according to the thermal indexes. Conclusion In conclusion the present findings indicate that greater efforts of National Ultrasound Societies are warranted in disseminating knowledge about the bio-effects of diagnostic ultrasound modalities among their members to prevent possible hazards.