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.

Ruolo dell'elastometria pulsata monodimensionale ad ultrasuoni (fibroscan) nella stadiazione della fibrosi epatica in pazienti sottoposti a trapianto ortotopico di fegato con recidiva di epatite C

PREMESSA: La progressione della recidiva d’epatite C è accelerata nei pazienti sottoposti a trapianto di fegato e ciò ha portato alla necessità di sviluppare nuove e validate metodiche non invasive per la quantificazione e la misura della fibrosi epatica. SCOPI: Stabilire l’efficacia dell’elastometria epatica (Fibroscan®) e dei parametri sierici di fibrosi, attualmente disponibili nella pratica clinica, per predire il grado di fibrosi nei pazienti sottoposti a trapianto epatico. METODI: La correlazione fra fibrosi epatica, determinata mediante biopsia epatica ed esame istologico, e Fibroscan® o indici clinico-sierologici di fibrosi (Benlloch, Apri, Forns, Fibrotest and Doppler resistance index), è stata studiata in pazienti che avevano ricevuto un trapianto ortotopico di fegato con evidenza di recidiva d’epatite da HCV. Un totale di 36 pazienti, con la seguente classificazione istologica: fibrosi secondom METAVIR F1=24, F2=8, F3=3, F4=1, sono stati arruolati nella popolazione oggetto di studio. Un totale di 29 individui volontari sani sono serviti come controllo. Le differenze fra gli stadi di fibrosi sono state calcolate mediante analisi statistica non parametrica. Il miglior cut-off per la differenziazione di fibrosi significativa (F2-F4) è stato identificato mediante l’analisi delle curve ROC. RISULTATI: La rigidità epatica ha presentato valori di 4.4 KPa (2.7-6.9) nei controlli (mediane e ranges), con valori in tutti i soggeti <7.0 KPa; 7.75 KPa (4.2-28.0) negli F1; 16.95 KPa (10.2-31.6) negli F2; 21.10 KPa nell’unico paziente F4 cirrotico. Le differenze sono state statisticamente significative per i soggetti controllo versus F1 e F2 (p<0.0001) e per F1 versus F2 (p<0.0001). Un cut-off elastografico di 11.2 KPagarantisce 88% di Sensibilità, 90% di Specificità, 79% di PPV e 95% di NPV nel differenziare i soggetti F1 dagli F2-F4. Le AUROC, relativamente alla capacità di discriminare fra i differenti gradi di fibrosi, evidenziavano un netto vantaggio per il Fibroscan® rispetto ad ognuno degli indici non invasivi di fibrosi. CONCLUSIONI: L’elastometria epatica presenta una buona accuratezza diagnostica nell’identificare pazienti con fibrosi epatica di grado significativo, superiore a quella di tutti gli altri test non invasivi al momento disponibili nella clinica, nei pazienti portatori di trapianto epatico ortotopico da cadavere con recidiva di HCV.

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.

Sistema per l'estrazione e purificazione di sostanze antiossidanti naturali nelle acque di vegetazione delle olive

The olive oil extraction industry is responsible for the production of high quantities of vegetation waters, represented by the constitutive water of the olive fruit and by the water used during the process. This by-product represent an environmental problem in the olive’s cultivation areas because of its high content of organic matter, with high value of BOD5 and COD. For that reason the disposal of the vegetation water is very difficult and needs a previous depollution. The organic matter of vegetation water mainly consists of polysaccharides, sugars, proteins, organic acids, oil and polyphenols. This last compounds are the principal responsible for the pollution problems, due to their antimicrobial activity, but, at the same time they are well known for their antioxidant properties. The most concentrate phenolic compounds in waters and also in virgin olive oils are secoiridoids like oleuropein, demethyloleuropein and ligstroside derivatives (the dialdehydic form of elenolic acid linked to 3,4-DHPEA, or p-HPEA (3,4-DHPEA-EDA or p-HPEA-EDA) and an isomer of the oleuropein aglycon (3,4-DHPEA-EA). The management of the olive oil vegetation water has been extensively investigated and several different valorisation methods have been proposed, such as the direct use as fertilizer or the transformation by physico-chemical or biological treatments. During the last years researchers focused their interest on the recovery of the phenolic fraction from this waste looking for its exploitation as a natural antioxidant source. At the present only few contributes have been aimed to the utilization for a large scale phenols recovery and further investigations are required for the evaluation of feasibility and costs of the proposed processes. The present PhD thesis reports a preliminary description of a new industrial scale process for the recovery of the phenolic fraction from olive oil vegetation water treated with enzymes, by direct membrane filtration (microfiltration/ultrafiltration with a cut-off of 250 KDa, ultrafiltration with a cut-off of 7 KDa/10 KDa and nanofiltration/reverse osmosis), partial purification by the use of a purification system based on SPE analysis and by a liquid-liquid extraction system (LLE) with contemporary reduction of the pollution related problems. The phenolic fractions of all the samples obtained were qualitatively and quantitatively by HPLC analysis. The work efficiency in terms of flows and in terms of phenolic recovery gave good results. The final phenolic recovery is about 60% respect the initial content in the vegetation waters. The final concentrate has shown a high content of phenols that allow to hypothesize a possible use as zootechnic nutritional supplements. The purification of the final concentrate have garanteed an high purity level of the phenolic extract especially in SPE analysis by the use of XAD-16 (73% of the total phenolic content of the concentrate). This purity level could permit a future food industry employment such as food additive, or, thanks to the strong antioxidant activity, it would be also use in pharmaceutical or cosmetic industry. The vegetation water depollutant activity has brought good results, as a matter of fact the final reverse osmosis permeate has a low pollutant rate in terms of COD and BOD5 values (2% of the initial vegetation water), that could determinate a recycling use in the virgin olive oil mechanical extraction system producing a water saving and reducing thus the oil industry disposal costs .

La valutazione degli effetti delle politiche di coesione dell'Unione europea sulla crescita regionale

This PhD thesis aims at providing an evaluation of EU Cohesion policy impact on regional growth. It employs methodologies and data sources never before applied for this purpose. Main contributions to the literature concerning EU regional policy effectiveness have been extensively analysed. Moreover, having carried out an overview of the current literature on Cohesion Policy, we deduce that this work introduces innovative features in the field. The work enriches the current literature with regards to two aspects. The first aspect concerns the use of the instrument of Regression Discontinuity Design in order to examine the presence of a different outcome in terms of growth between Objectives 1 regions and non-Objective 1 regions at the cut-off point (75 percent of EU-15 GDP per capita in PPS) during the two programming periods, 1994-1999 and 2000-2006. The results confirm a significant difference higher than 0.5 percent per year between the two groups. The other empirical evaluation regards the study of a cross-section regression model based on the convergence theory that analyses the dependence relation between regional per capita growth and EU Cohesion policy expenditure in several fields of interventions. We have built a very fine dataset of spending variables (certified expenditure), using sources of data directly provided from the Regional Policy Directorate of the European Commission.

Studio di marcatori biologici prognostici nel linfoma di Hodgkin

Recent reports showed that early-interim PET-scan is the only tool predicting treatment outcome in advanced-stage classical Hodgkin lymphoma (asCHL). We evaluated the prognostic impact of a series of immunohistochemical markers, mentioned in literature as prognostic factors, on tissue microarrays assembled from biopsies of 220 patients: STAT1, SAP, TOP2A, PCNA and CD20, both in neoplastic (HRSC) and microenvironment cells (MC); RRM2, MAD2, CDC2, BCL2, P53, BCL11A and EBER in HRSC; ALDH1A1, TIA-1, granzyme B, perforin, FOXP3, and PD-1 in MC. All patients had been treated with standard ABVD ± Rx therapy. Interim-PET after 2 ABVD courses was evaluated according to the criteria indicated by Gallamini in his study (Journal of Clinical Oncology, 2007). The survival analysis has been performed in a subset of 138 patients whose complete clinical information were available: the mean age was 33.3 years (14-79), the stage III-IVB in 98 and IIB in 40, and the mean follow-up 38.1 months (7.6-71.9). Histopathology review showed: NS-I 75, NS-II 22, MC 20, DL 3, and CHL/nos 18 cases. Interim-PET was positive in 30 patients, while treatment failure was recorded in 32. In univariate analysis the factors related to treatment outcome were BCL2 on HRSC (cut-off value 50%), STAT1/SAP on MC, and PET (Log-rank 6.9, 7.9 and 93.9 respectively). The combined expression of STAT1 and SAP was scored in three levels depending on the architectural pattern: score 0 for expression of both with a diffuse/rosetting pattern; score 1 for discordant combination of diffuse/rosetting and scattered patterns; score 2 for both markers with a scattered pattern; the 3y-PFS were 87.4%, 69.9% and 61.9% respectively. In multivariate analysis PET, BCL2 and STAT1/SAP remained significant (HR: 24.8, 4.6, 7.5 and 5.6, respectively; p<.01). The proposed model is able to predict treatment response in AsCHL, even if with a lower efficacy than PET. However, unlike PET, it can be applied upfront therapy.

Accuratezza diagnostica dell'ecografia con mezzo di contrasto nel predire l'evoluzione a breve termine in pazienti con morbo di Crohn

Obiettivi. L’ecografia con mezzo di contrasto (CEUS) può fornire informazioni sulla microvascolarizzazione della parete intestinale nella malattia di Crohn. L’infiammazione della parete intestinale non sembra essere correlata alla quantità di parete vascolarizzata (studi di pattern di vascolarizzazione, SVP) ma all’intensità del flusso di parete in un determinato periodo di tempo (studi di intensità-tempo, SIT). Scopo dello studio è valutare se gli studi SVP e/o SIT mediante CEUS siano in grado di mostrare il reale grado d’infiammazione della parete vascolare e se possano predire l’attività di malattia a 3 mesi. Materiali e metodi: 30 pazienti con malattia di Crohn venivano sottoposti a SVP e SIT mediante CEUS e venivano rivisti dopo 3 mesi. L’eCografia era eseguita con uno strumento dedicato con un software particolare per il calcolo delle curve intensità-tempo e con l’ausilio di un mezzo di contrasto (Sonovue). L’analisi quantitativa consisteva nella misura dell’area sotto la curva (AUC) (con cut-off tra malattia attiva e inattiva di 15) e di un intensità media (IM) con un cut-off di 10. Tutti gli esami venivano registrati e analizzati in modo digitale. Risultati: A T0: CDAI era inferiore a 150 in 22 pazienti e superiore a 150 in 8 pazienti; a T3: CDAI era inferiore a 150 in 19 pazienti e superiore a 150 in 11 pazienti. A T0 sia la CEUS SPV che la SIT evidenziavano bassa specificità, accuratezza diagnostica e valore predittivo negativo; a T3 la CEUS SVP mostrava bassa sensibilità e accuratezza diagnostica rispetto alla SIT che era in grado, in tutti i casi tranne uno, di predire l’attività clinica di malattia a tre mesi. Conclusioni: in questo studio, la CEUS-SIT ha mostrato buona accuratezza diagnostica nel predire l’attività clinica di malattia nel follow-up a breve termine di pazienti con malattia di Crohn.

Portal hypertension: a comparison between portal-venous pressure measurement and ARFI measurement of liver and spleen stiffness

PURPOSE. Portal pressure is measured invasively as Hepatic Venous Pressure Gradient (HVPG) in the angiography room. Liver stiffness measured by Fibroscan was shown to correlate with HVPG values below 12 mmHg. This is not surprising, since in cirrhosis the increase of portal pressure is not directly linked with liver fibrosis and consequently to liver stiffness. We hypothesized that, given the spleen’s privileged location upstream to the whole portal system, splenic stiffness could provide relevant information about portal pressure. Aim of the study was to assess the relationship between liver and spleen stiffness measured by Virtual Touch™ (ARFI) and HVPG in cirrhotic patients. METHODS. 40 consecutive patients (30 males, mean age 62y, mean BMI=26, mean Child-Pugh A6, mean platelet count=92.000/mmc, 19 HCV+, 7 with ascites) underwent to ARFI stiffness measurement (10 valid measurements in right liver lobe both surface and centre, left lobe and 20 in the spleen) and HPVG, blindly to each other. Median ARFI values of 10 samplings on every liver area and of 20 samplings on spleen were calculated. RESULTS. Stiffness could be easily measured in all patients with ARFI, resulting a mean of 2,61±0,76, 2,5±0,62 and 2,55±0,66 m/sec in the liver areas and 3.3±0,5 m/s in the spleen. Median HPVG was 14 mmHg (range 5-27); 28 patients showed values ≥10 mmHg. A positive significant correlation was found between spleen stiffness and HPVG values (r=0.744, p<0.001). No significant correlation was found between all liver stiffness and HVPG (p>0,05). AUROC was calculated to test spleen stiffness ability in discriminating patients with HVPG ≥10. AUROC = 0.911 was obtained, with sensitivity of 69% and specificity of 91% at a cut-off of 3.26 m/s. CONCLUSION. Spleen stiffness measurement with ARFI correlates with HVPG in patients with cirrhosis, with a potential of identifying patients with clinically significant portal hypertension.

Proteinuria e sindrome nefrosica nel cane: studio reptrospettivo di 338 casi

La sindrome nefrosica (SN) è definita come la presenza concomitante di una proteinuria maggiore di 3.5g/24 h, ipoalbuminemia, ipercolesterolemia e presenza di edemi. I pazienti con SN sono più a rischio di quelli che presentano una nefropatia glomerulare non nefrosica (NNGD) per lo sviluppo di ipertensione, ipernatremia, complicazioni tromboemboliche e comparsa di insufficienza renale. In Medicina Veterinaria, la Letteratura riguardante l’argomento è molto limitata e non è ben nota la correlazione tra SN e gravità della proteinuria, ipoalbuminemia e sviluppo di tromboembolismo. L’obiettivo del presente studio retrospettivo è stato quello di descrivere e caratterizzare le alterazioni cliniche e clinicopatologiche che si verificano nei pazienti con rapporto proteine urinarie:creatinina urinaria (UPC) >2 con lo scopo di inquadrare con maggiore precisione lo stato clinico di questi pazienti e individuare le maggiori complicazioni a cui possono andare incontro. In un periodo di nove anni sono stati selezionati 338 cani e suddivisi in base ad un valore cut-off di UPC≥3.5. Valori mediani di creatinina, urea, fosforo, albumina urinaria, proteina C reattiva (CRP) e fibrinogeno sono risultati al di sopra del limite superiore dell’intervallo di riferimento, valori mediani di albumina sierica, ematocrito, antitrombina al disotto del limite inferiore di riferimento. Pazienti con UPC≥3.5 hanno mostrato concentrazioni di albumine, ematocrito, calcio, Total Iron Binding Capacity (TIBC), significativamente minori rispetto a quelli con UPC<3.5, concentrazioni di CRP, di urea e di fosforo significativamente maggiori. Nessuna differenza tra i gruppi nelle concentrazioni di creatinina colesterolo, trigliceridi, sodio, potassio, cloro, ferro totale e pressione sistolica. I pazienti con UPC≥3.5 si trovano verosimilmente in uno “stato infiammatorio” maggiore rispetto a quelli con UPC<3.5, questa ipotesi avvalorata dalle concentrazioni minori di albumina, di transferrina e da una concentrazione di CRP maggiore. I pazienti con UPC≥3.5 non presentano concentrazioni di creatinina più elevate ma sono maggiormente a rischio di anemia.

Metodi di misurazione e implicazioni dell'albuminuria e della proteinuria nel cane

La proteinuria è un marker di danno renale nel cane. L’obiettivo dello studio è di valutare la capacità del dipstick urinario e dell’UPC di diagnosticare precocemente l’albuminuria nel cane. Sono stati raccolti 868 campioni di urina, con sedimento spento e assenza di ematuria, nell’Ospedale Didattico Veterinario della Facoltà di Medicina Veterinaria di Bologna. Per 550 campioni è stata effettuata l’analisi delle urine, la misurazione dell’UPC e dell’UAC, mentre UPC e UAC sono stati misurati in tutti gli 868 campioni. I campioni di urina sono stati analizzati con il metodo dipstick mediante lettura automatizzata. Utilizzando come valore di riferimento l’UAC è stata valutata l’accuratezza diagnostica del dipstick urinario e dell’UPC. L’intervallo di riferimento dell’UAC (0-0,024) è stato determinato utilizzando 60 cani sani. I dati raccolti sono stati classificati utilizzando differenti cut-off per il peso specifico urinario (1012 o 1030), per la proteinuria al dipstick (30 o 100 mg/dl), per l’UPC (0,2) e per l’UAC (0,024). Sono stati valutati l’agreement diagnostico e la correlazione di Spearman tra dipstick, UPC e UAC. E’ stata stimata l’accuratezza diagnostica misurando l’area al di sotto della curva di ROC nell’analisi dell’UAC. Il livello di significatività è stato definito per p < 0,05. Indipendentemente dal peso specifico urinario, l’agreement diagnostico tra dipstick, UPC e UAC è risultato forte (k=0,62 e k=0,61, rispettivamente; p<0,001) con valori di dipstick ≥30 mg/dl, debole (k=0,27 e k=0,26, rispettivamente; p<0,001) con valori di dipstick ≥100 mg/dl. L’accuratezza diagnostica del dipstick messa a confronto con UPC e con UAC è molto buona (AUC 0,84 e 0,84, rispettivamente; p<0,001) e i risultati negativi al dipstick presentano il 100% di sensitività. UPC e UAC sono fortemente correlate (r=0,90; p<0,001). Mettendo a confronto UPC e UAC, l’accuratezza diagnostica è risultata eccellente (AUC 0,94; p<0,001), con massima sensitività e specificità per UPC≥0.3.

Carcinoma polmonare non a piccole cellule T1aN0M0: Ruolo prognostico della Microvessel Density

Obiettivi. Valutare l’angiogenesi tumorale mediante la Microvessel density (MVD) come fattore predittivo di mortalità per tumore polmonare non a piccole cellule (NSCLC) pT1aN0M0 trattato chirurgicamente. Metodi. I dati demografici, clinici e istopatologici sono stati registrati per 82 pazienti (60 maschi, 22 femmine) sottoposti a resezione chirurgica in due diverse Chirurgie Toraciche tra gennaio 2002 e dicembre 2007 per tumori polmonari non a piccole cellule pT1AN0M0. La MVD è stata valutata mediante il conteggio visivo dei microvasi positivi alla colorazione immunoistochimica con anticorpo monoclonale anti-CD31 e definita come il numero medio di microvasi per 1 mm2 di campo ottico. Risultati. Sono state eseguite 59 lobectomie (72%) e 23 resezioni sublobari (28%). Reperti istopatologici: 43 adenocarcinomi (52%) e 39 neoplasie non- adenocarcinoma (48%) pT1aN0M0; MVD media: 161 (CD31/mm2); mediana: 148; range 50-365, cut-off=150. Una MVD elevata (> 150 CD31/mm2) è stata osservata in 40 pazienti (49%), una MVD ridotta ( ≤ 150 CD31/mm2 ) in 42 pazienti (51%). Sopravvivenze a 5 anni: 70 % e 95%, rispettivamente per il gruppo ad elevata MVD vs il gruppo a ridotta MVD con una p = 0,0041, statisticamente significativa. Il tipo di resezione chirurgica, il diametro del tumore, le principali comorbidità e l’istotipo nono sono stati fattori predittivi significativi di mortalità correlata alla malattia. La MVD è risultata essere superiore nel gruppo “Adenocarcinoma” (MVD mediana=180) rispetto al gruppo “Non-Adenocarcinoma (MVD mediana=125), con un test di Mann-Whitney statisticamente significativo (p < 0,0001). Nel gruppo “Adenocarcinoma” la sopravvivenza a 5 anni è stata del 66% e 93 %, rispettivamente per i pazienti con MVD elevata e ridotta (p = 0.043. Conclusioni. Il nostro studio ha mostrato che la Microvessel density valutata con la colorazione immunoistochimica per CD31 ha un valore prognostico rilevante nel carcinoma polmonare in stadio precoce pT1aN0M0.

Il monitoraggio della qualità di vita e dei bisogni di pazienti oncologici e caregiver: il caso ANT

La Fondazione ANT rappresenta una delle più ampie esperienze al mondo di assistenza socio-sanitaria gratuita a domicilio ai malati di tumore, tramite équipe di specialisti costituite da medici, psicologi e infermieri. La patologia oncologica ha un enorme impatto sul benessere dei pazienti. Un modo per raggruppare i diversi sintomi di disagio psicologico è utilizzare il concetto di distress, che sarebbe importante monitorare in modo semplice e veloce. Primo studio: 66 pazienti oncologici (40% uomini; età media 54 anni) in cure palliative domiciliari. Il 79% dei pazienti ha mostrato livelli clinicamente significativi di distress. Il 55% dei partecipanti allo studio ha riportato alti livelli di ansia, e l'81% dei pazienti ha riportato alti livelli di depressione. Dall'analisi delle curve ROC il singolo item del Distress Thermometer, con un cut-off maggiore o uguale a 4, è stato in grado di rilevare il 97% dei soggetti con punteggi clinici di ansia e depressione, quindi può essere utilizzato anche come uno strumento di screening precoce rapido ed affidabile per i disturbi dell'umore. I familiari sono la prima risorsa dei malati di tumore, e l'identificazione dei loro bisogni è utile per individuare chi ha maggiore necessità di aiuto ed in quali aree. Secondo studio: 115 caregiver di pazienti oncologici (37% uomini; età media 52 anni). Di seguito i bisogni più frequenti. Salute psicofisica: “preoccupazioni circa il/la paziente” (72%), ansia (53%) e rabbia (52%). Informazioni: “come prendersi cura del paziente” (64%), “terapie alternative e/o complementari” (64%) e “come gestire lo stress” (57%). Servizi e strutture sanitarie: “un operatore di riferimento”, (65%), “cure infermieristiche a domicilio” (62%), “indicazioni su servizi ospedalieri” (57%), ed “assistenza per caregiver, ad esempio consulenza psicologica” (55%). Il monitoraggio dei bisogni consentirebbe un'ottimizzazione dell'assistenza, prevenendo situazioni che potrebbero compromettere il benessere della famiglia e la qualità dell'assistenza fornita al paziente.

Application of Submerged Grouted Anchors in Sheet Pile Quay Walls

Sheet pile walls are one of the oldest earth retention systems utilized in civil engineering projects. They are used for various purposes; such as excavation support system, cofferdams, cut-off walls under dams, slope stabilization, waterfront structures, and flood walls. Sheet pile walls are one of the most common types of quay walls used in port construction. The worldwide increases in utilization of large ships for transportation have created an urgent need of deepening the seabed within port areas and consequently the rehabilitation of its wharfs. Several methods can be used to increase the load-carrying capacity of sheet-piling walls. The use of additional anchored tie rods grouted into the backfill soil and arranged along the exposed wall height is one of the most practical and appropriate solutions adopted for stabilization and rehabilitation of the existing quay wall. The Ravenna Port Authority initiated a project to deepen the harbor bottom at selected wharves. An extensive parametric study through the finite element program, PLAXIS 2D, version 2012 was carried out to investigate the enhancement of using submerged grouted anchors technique on the load response of sheet-piling quay wall. The influence of grout-ties area, length of grouted body, anchor inclination and anchor location were considered and evaluated due to the effect of different system parameters. Also a comparative study was conducted by Plaxis 2D and 3D program to investigate the behavior of these sheet pile quay walls in terms of horizontal displacements induced along the sheet pile wall and ground surface settlements as well as the anchor force and calculated factor of safety. Finally, a comprehensive study was carried out by using different constitutive models to simulate the mechanical behavior of the soil to investigate the effect of these two models (Mohr-Coulomb and Hardening Soil) on the behavior of these sheet pile quay walls.

Il discorso politico culturale del Deutscher Geist in Gefahr di Ernst Robert Curtius

Nel 1932 Ernst Robert Curtius pubblica il pamphlet politico culturale Deutscher Geist in Gefahr nel quale chiarisce il suo pensiero di fronte alla grave crisi in cui versa la Germania. Egli si schiera contro le posizioni di destra del suo tempo, delle quali critica apertamente la boria nazionalista, il rozzo antisemitismo e la creazione di un mito nazionale elaborato come strumento di manipolazione dell’opinione pubblica. Ritiene inoltre inaccettabili le posizioni rivoluzionarie, tanto di destra quanto di sinistra, che vogliono liberarsi della tradizione umanistica europea e disprezzano la Zivilisation francese; allo stesso modo rifiuta l’ideale di un germanesimo eroico avulso dalla storia europea e respinge infine tutte le forme di nichilismo che si risolvono in un atteggiamento di indifferenza nei confronti della realtà, dei valori e della storia. Curtius accetta il sistema democratico come unica soluzione e ritiene che le decisioni politiche debbano mirare al bene di tutti i ceti sociali indipendentemente dagli interessi di partiti e di singoli gruppi. Rifiuta qualunque forma, anche culturale, di supremazia della Germania, aspira a un’Europa cosmopolita, le cui nazioni siano valorizzate nelle loro caratteristiche specifiche, ed è convinto che per la costruzione della pace gli europei debbano vivere, studiare e lavorare insieme imparando gli uni le lingue degli altri. Per Curtius l’Umanesimo della tradizione classica e la letteratura del Medioevo sono parte integrante della vita di ogni europeo e fonte di energie spirituali per affrontare in modo creativo il presente e il futuro.

Outcome a lungo termine dei pazienti pediatrici con rene singolo. Valutazione di marker laboratoristici e strumentali di danno renale

Obiettivi: valutare in pazienti con rene singolo congenito la correlazione tra il filtrato glomerulare misurato con il DTPA (DTPA-VFG) e 1) marker laboratoristici di danno renale (creatinina, cistatinaC, proteinuria) 2) formule per stimare il filtrato glomerulare 3) parametri di valutazione della crescita renale ecografica. Materiali e metodi: Sono stati arruolati 118 pazienti con rene singolo congenito tra 0 e 18 anni. Sono stati valutati a ogni visita altezza, creatinina, cistatinaC, proteinuria e lunghezza ecografica renale. E’ stato calcolato il filtrato stimato con formule basate sulla creatinina (Schwartz), sulla cistatina C (Zappitelli, Filler, Grubb e Bokenkamp) e su entrambe (equazione di Zappitelli). La crescita renale è stata valutata come rapporto lunghezza ecografica/altezza corporea (USL/H), differenza percentuale tra lunghezza renale misurata e attesa per età (delta%) e presenza o meno d’ipertrofia compensatoria. In 74 bambini è stata misurata la DTPA-VFG. Risultati: Il follow-up è di 2.1 ± 0.9 anni. Il 65% sono maschi. Nessun paziente ha sviluppato danno renale cronico. La media del DTPA-VFG era di 135±44ml/min/1.73m², il valore medio della creatinina 0.47±0.17mg/dl e di cistatinaC di 1±0.4mg/L. La lunghezza ecografica renale media era di 100±17 mm, il rapporto USL/H medio di 0.8±0,1 e il delta% di 1,13±11,4, il 66% presentava ipertrofia renale. Le uniche correlazioni significative con DTPA-VFG sono inversa con la creatinina (p=<.001) e lineare con USL/H (p=<.001). Discussione: Lo studio ha mostrato che come per altre nefrouropatie, la creatina e l’ecografia renale siano due strumenti validi per il follow-up dei pazienti con rene singolo congenito. Il limite principale è dovuto al fatto che nessuno dei pazienti ha sviluppato danno renale cronico e pertanto non è stato possibile stabilire dei cutt-off di rischio per parametri quali USL/H.