Iura novit curia

Al principio iura novit curia si assegnano tradizionalmente due significati: il giudice conosce le norme, quindi le parti non hanno onori al riguardo, e il giudice non è vincolato dalle indicazioni delle parti, quanto alle norme di diritto da applicare. La tesi delimita inizialmente la nozione di questione di diritto, quindi affronta partitamente due problemi che si pongono con riferimento alle questioni di diritto e che sono soliti essere risolti con il richiamo al principio iura novit curia: la conoscenza delle norme da una parte e la qualificazione giuridica della domanda e quindi della situazione soggettiva dall’altra. Quanto alla conoscenza delle norme, motivata la scelta per l’obbligatorietà della conoscenza ufficiosa di tutte le fonti di diritto, la tesi verifica la regola in relazione alle diverse fonti descrivendone la disciplina. Quanto alla qualificazione giuridica della domanda, la tesi, verificata la vigenza del principio iura novit curia, descrive sul piano processuale le relazioni del potere-dovere di qualificazione giuridica a) individuandone i limiti oggettivi, ricompresi nei limiti della domanda, e risultanti dal confronto con la regola della corrispondenza del chiesto con il pronunciato, del concorso di diritti, della natura autodeterminata dei diritti, b) tracciandone le modalità legittime di esercizio in conformità al principio del contradditorio; c) verificandone i limiti esterni, ravvisati in quegli istituti che impediscono al giudice di formulare un giudizio sulla questione di diritto: le sentenze non definitive su questioni di diritto, il principio di diritto, il giudicato interno e i limiti alla cognizione del giudice dell’impugnazione tra i gradi di giudizio.

I "governi del Presidente"

Gli avvenimenti politico-istituzionali degli ultimi anni hanno determinato un vivace dibattito sulla questione dei cc.dd. “governi del Presidente”, con cui si suole far riferimento ad Esecutivi il cui procedimento di formazione e le cui crisi registrano un interventismo del Presidente della Repubblica superiore a quello richiesto e/o consentito dal dettato costituzionale. Obiettivo dell’elaborato è duplice: fornire un tentativo definitorio della categoria “governi del Presidente”, nonché valutare la compatibilità di questa con la forma di governo parlamentare, soprattutto in considerazione dei recenti sviluppi delle dinamiche politico-istituzionali italiane. Sulla base di questo presupposto, nel presente lavoro si procede a una ricostruzione dell’evoluzione della prassi e delle consuetudini costituzionali in merito all’esercizio dei poteri presidenziali nella gestione delle crisi di governo, con particolare riferimento al procedimento di formazione dell’Esecutivo. La tesi si presenta articolata in due parti, corrispondenti a due differenti periodi storici (cc.dd. Prima e Seconda Repubblica), organizzate per capitoli, relativi alle principali fasi di evoluzione del sistema politico attraversate nel corso della storia della Repubblica. Questa scelta si giustifica in ragione del fatto che il modus operandi del Presidente della Repubblica risulta fortemente condizionato dai mutamenti del contesto politico-istituzionale. Nei singoli paragrafi, dedicati ai presidenti, vengono trattati l’elezione del Presidente, le modalità di formazione dei governi nominati, nonché ulteriori temi la cui disamina è stata ritenuta opportuna allo scopo di fornire una contestualizzazione più adeguata dell’analisi svolta (utilizzo del potere di esternazione e di scioglimento delle Camere, gestione delle attività di politica interna e politica estera, principali avvenimenti dei periodi storici considerati, e così via).

The special rights other than shares in cross-border mergers of limited liability companies within the European Union. A perspective from the Spanish Law

The present research aims to study the special rights other than shares in Spanish Law and the protection of their holders in cross-border mergers of limited liability companies within the European Union frame. Special rights other than shares are recognised as an independent legal category within legal systems of some EU Member States, such as Germany or Spain, through the implementation of the Third Directive 78/855/CEE concerning mergers of public limited liability companies. The above-cited Directive contains a special regime of protection for the holders of securities, other than shares, to which special rights are attached, consisting of being given rights in the acquiring company, at least equivalent to those they possessed in the company being acquired. This safeguard is to highlight the intimate connection between this type of rights and the company whose extinction determines the existence of those. Pursuant to the Directive 2005/56/CE on cross-border mergers of limited liability companies, each company taking part in these operations shall comply with the safeguards of members and third parties provided in their respective national law to which is subject. In this regard, the protection for holders of special rights other than shares shall be ruled by the domestic M&A regime. As far as Spanish Law are concerned, holders of these special rights are recognized a right of merger information, in the same terms as shareholders, as well as equal rights in the company resulting from the cross-border merger. However, these measures are not enough guarantee for a suitable protection, thus considering those holders of special rights as special creditors, sometimes it will be necessary to go to the general protection regime for creditors. In Spanish Law, it would involve the recognition of right to the merger opposition, whose exercise would prevent the operation was completed until ensuring equal rights.

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.

La filosofia di Hans-Georg Gadamer e il problema del disagio della modernità. Ermeneutica, estetica, etica e politica

L’ermeneutica filosofica di Hans-Georg Gadamer – indubbiamente uno dei capisaldi del pensiero novecentesco – rappresenta una filosofia molto composita, sfaccettata e articolata, per così dire formata da una molteplicità di dimensioni diverse che si intrecciano l’una con l’altra. Ciò risulta evidente già da un semplice sguardo alla composizione interna della sua opera principale, Wahrheit und Methode (1960), nella quale si presenta una teoria del comprendere che prende in esame tre differenti dimensioni dell’esperienza umana – arte, storia e linguaggio – ovviamente concepite come fondamentalmente correlate tra loro. Ma questo quadro d’insieme si complica notevolmente non appena si prendano in esame perlomeno alcuni dei numerosi contributi che Gadamer ha scritto e pubblicato prima e dopo il suo opus magnum: contributi che testimoniano l’importante presenza nel suo pensiero di altre tematiche. Di tale complessità, però, non sempre gli interpreti di Gadamer hanno tenuto pienamente conto, visto che una gran parte dei contributi esegetici sul suo pensiero risultano essenzialmente incentrati sul capolavoro del 1960 (ed in particolare sui problemi della legittimazione delle Geisteswissenschaften), dedicando invece minore attenzione agli altri percorsi che egli ha seguito e, in particolare, alla dimensione propriamente etica e politica della sua filosofia ermeneutica. Inoltre, mi sembra che non sempre si sia prestata la giusta attenzione alla fondamentale unitarietà – da non confondere con una presunta “sistematicità”, da Gadamer esplicitamente respinta – che a dispetto dell’indubbia molteplicità ed eterogeneità del pensiero gadameriano comunque vige al suo interno. La mia tesi, dunque, è che estetica e scienze umane, filosofia del linguaggio e filosofia morale, dialogo con i Greci e confronto critico col pensiero moderno, considerazioni su problematiche antropologiche e riflessioni sulla nostra attualità sociopolitica e tecnoscientifica, rappresentino le diverse dimensioni di un solo pensiero, le quali in qualche modo vengono a convergere verso un unico centro. Un centro “unificante” che, a mio avviso, va individuato in quello che potremmo chiamare il disagio della modernità. In altre parole, mi sembra cioè che tutta la riflessione filosofica di Gadamer, in fondo, scaturisca dalla presa d’atto di una situazione di crisi o disagio nella quale si troverebbero oggi il nostro mondo e la nostra civiltà. Una crisi che, data la sua profondità e complessità, si è per così dire “ramificata” in molteplici direzioni, andando ad investire svariati ambiti dell’esistenza umana. Ambiti che pertanto vengono analizzati e indagati da Gadamer con occhio critico, cercando di far emergere i principali nodi problematici e, alla luce di ciò, di avanzare proposte alternative, rimedi, “correttivi” e possibili soluzioni. A partire da una tale comprensione di fondo, la mia ricerca si articola allora in tre grandi sezioni dedicate rispettivamente alla pars destruens dell’ermeneutica gadameriana (prima e seconda sezione) ed alla sua pars costruens (terza sezione). Nella prima sezione – intitolata Una fenomenologia della modernità: i molteplici sintomi della crisi – dopo aver evidenziato come buona parte della filosofia del Novecento sia stata dominata dall’idea di una crisi in cui verserebbe attualmente la civiltà occidentale, e come anche l’ermeneutica di Gadamer possa essere fatta rientrare in questo discorso filosofico di fondo, cerco di illustrare uno per volta quelli che, agli occhi del filosofo di Verità e metodo, rappresentano i principali sintomi della crisi attuale. Tali sintomi includono: le patologie socioeconomiche del nostro mondo “amministrato” e burocratizzato; l’indiscriminata espansione planetaria dello stile di vita occidentale a danno di altre culture; la crisi dei valori e delle certezze, con la concomitante diffusione di relativismo, scetticismo e nichilismo; la crescente incapacità a relazionarsi in maniera adeguata e significativa all’arte, alla poesia e alla cultura, sempre più degradate a mero entertainment; infine, le problematiche legate alla diffusione di armi di distruzione di massa, alla concreta possibilità di una catastrofe ecologica ed alle inquietanti prospettive dischiuse da alcune recenti scoperte scientifiche (soprattutto nell’ambito della genetica). Una volta delineato il profilo generale che Gadamer fornisce della nostra epoca, nella seconda sezione – intitolata Una diagnosi del disagio della modernità: il dilagare della razionalità strumentale tecnico-scientifica – cerco di mostrare come alla base di tutti questi fenomeni egli scorga fondamentalmente un’unica radice, coincidente peraltro a suo giudizio con l’origine stessa della modernità. Ossia, la nascita della scienza moderna ed il suo intrinseco legame con la tecnica e con una specifica forma di razionalità che Gadamer – facendo evidentemente riferimento a categorie interpretative elaborate da Max Weber, Martin Heidegger e dalla Scuola di Francoforte – definisce anche «razionalità strumentale» o «pensiero calcolante». A partire da una tale visione di fondo, cerco quindi di fornire un’analisi della concezione gadameriana della tecnoscienza, evidenziando al contempo alcuni aspetti, e cioè: primo, come l’ermeneutica filosofica di Gadamer non vada interpretata come una filosofia unilateralmente antiscientifica, bensì piuttosto come una filosofia antiscientista (il che naturalmente è qualcosa di ben diverso); secondo, come la sua ricostruzione della crisi della modernità non sfoci mai in una critica “totalizzante” della ragione, né in una filosofia della storia pessimistico-negativa incentrata sull’idea di un corso ineluttabile degli eventi guidato da una razionalità “irrazionale” e contaminata dalla brama di potere e di dominio; terzo, infine, come la filosofia di Gadamer – a dispetto delle inveterate interpretazioni che sono solite scorgervi un pensiero tradizionalista, autoritario e radicalmente anti-illuminista – non intenda affatto respingere l’illuminismo scientifico moderno tout court, né rinnegarne le più importanti conquiste, ma più semplicemente “correggerne” alcune tendenze e recuperare una nozione più ampia e comprensiva di ragione, in grado di render conto anche di quegli aspetti dell’esperienza umana che, agli occhi di una razionalità “limitata” come quella scientista, non possono che apparire come meri residui di irrazionalità. Dopo aver così esaminato nelle prime due sezioni quella che possiamo definire la pars destruens della filosofia di Gadamer, nella terza ed ultima sezione – intitolata Una terapia per la crisi della modernità: la riscoperta dell’esperienza e del sapere pratico – passo quindi ad esaminare la sua pars costruens, consistente a mio giudizio in un recupero critico di quello che egli chiama «un altro tipo di sapere». Ossia, in un tentativo di riabilitazione di tutte quelle forme pre- ed extra-scientifiche di sapere e di esperienza che Gadamer considera costitutive della «dimensione ermeneutica» dell’esistenza umana. La mia analisi della concezione gadameriana del Verstehen e dell’Erfahrung – in quanto forme di un «sapere pratico (praktisches Wissen)» differente in linea di principio da quello teorico e tecnico – conduce quindi ad un’interpretazione complessiva dell’ermeneutica filosofica come vera e propria filosofia pratica. Cioè, come uno sforzo di chiarificazione filosofica di quel sapere prescientifico, intersoggettivo e “di senso comune” effettivamente vigente nella sfera della nostra Lebenswelt e della nostra esistenza pratica. Ciò, infine, conduce anche inevitabilmente ad un’accentuazione dei risvolti etico-politici dell’ermeneutica di Gadamer. In particolare, cerco di esaminare la concezione gadameriana dell’etica – tenendo conto dei suoi rapporti con le dottrine morali di Platone, Aristotele, Kant e Hegel – e di delineare alla fine un profilo della sua ermeneutica filosofica come filosofia del dialogo, della solidarietà e della libertà.

Securitization and Special Purpose Vehicles in an International Setting: a Systemic View

The present work tries to display a comprehensive and comparative study of the different legal and regulatory problems involved in international securitization transactions. First, an introduction to securitization is provided, with the basic elements of the transaction, followed by the different varieties of it, including dynamic securitization and synthetic securitization structures. Together with this introduction to the intricacies of the structure, a insight into the influence of securitization in the financial and economic crisis of 2007-2009 is provided too; as well as an overview of the process of regulatory competition and cooperation that constitutes the framework for the international aspects of securitization. The next Chapter focuses on the aspects that constitute the foundations of structured finance: the inception of the vehicle, and the transfer of risks associated to the securitized assets, with particular emphasis on the validity of those elements, and how a securitization transaction could be threatened at its root. In this sense, special importance is given to the validity of the trust as an instrument of finance, to the assignment of future receivables or receivables in block, and to the importance of formalities for the validity of corporations, trusts, assignments, etc., and the interaction of such formalities contained in general corporate, trust and assignment law with those contemplated under specific securitization regulations. Then, the next Chapter (III) focuses on creditor protection aspects. As such, we provide some insights on the debate on the capital structure of the firm, and its inadequacy to assess the financial soundness problems inherent to securitization. Then, we proceed to analyze the importance of rules on creditor protection in the context of securitization. The corollary is in the rules in case of insolvency. In this sense, we divide the cases where a party involved in the transaction goes bankrupt, from those where the transaction itself collapses. Finally, we focus on the scenario where a substance over form analysis may compromise some of the elements of the structure (notably the limited liability of the sponsor, and/or the transfer of assets) by means of veil piercing, substantive consolidation, or recharacterization theories. Once these elements have been covered, the next Chapters focus on the regulatory aspects involved in the transaction. Chapter IV is more referred to “market” regulations, i.e. those concerned with information disclosure and other rules (appointment of the indenture trustee, and elaboration of a rating by a rating agency) concerning the offering of asset-backed securities to the public. Chapter V, on the other hand, focuses on “prudential” regulation of the entity entrusted with securitizing assets (the so-called Special Purpose vehicle), and other entities involved in the process. Regarding the SPV, a reference is made to licensing requirements, restriction of activities and governance structures to prevent abuses. Regarding the sponsor of the transaction, a focus is made on provisions on sound originating practices, and the servicing function. Finally, we study accounting and banking regulations, including the Basel I and Basel II Frameworks, which determine the consolidation of the SPV, and the de-recognition of the securitized asset from the originating company’s balance-sheet, as well as the posterior treatment of those assets, in particular by banks. Chapters VI-IX are concerned with liability matters. Chapter VI is an introduction to the different sources of liability. Chapter VII focuses on the liability by the SPV and its management for the information supplied to investors, the management of the asset pool, and the breach of loyalty (or fiduciary) duties. Chapter VIII rather refers to the liability of the originator as a result of such information and statements, but also as a result of inadequate and reckless originating or servicing practices. Chapter IX finally focuses on third parties entrusted with the soundness of the transaction towards the market, the so-called gatekeepers. In this respect, we make special emphasis on the liability of indenture trustees, underwriters and rating agencies. Chapters X and XI focus on the international aspects of securitization. Chapter X contains a conflicts of laws analysis of the different aspects of structured finance. In this respect, a study is made of the laws applicable to the vehicle, to the transfer of risks (either by assignment or by means of derivatives contracts), to liability issues; and a study is also made of the competent jurisdiction (and applicable law) in bankruptcy cases; as well as in cases where a substance-over-form is performed. Then, special attention is also devoted to the role of financial and securities regulations; as well as to their territorial limits, and extraterritoriality problems involved. Chapter XI supplements the prior Chapter, for it analyzes the limits to the States’ exercise of regulatory power by the personal and “market” freedoms included in the US Constitution or the EU Treaties. A reference is also made to the (still insufficient) rules from the WTO Framework, and their significance to the States’ recognition and regulation of securitization transactions.

"All'opera ha fatto seguito il ballo": Danza e stampa nell'Italia fascista

Basata sul reperimento di un’ampia mole di testi giornalistici (come cronache, interviste, elzeviri e articoli di “Terza”) dedicati alle pratiche coreiche e pubblicati in Italia nel corso del ventennio fascista, la tesi ricostruisce i lineamenti di quello che, seppure ancora embrionale e certo non specialistico, si può comunque ritenere una sorta di “pensiero italiano” sulla danza del Primo Novecento. A partire dalla ricognizione sistematica di numerose testate quotidiane e periodiche e, pertanto, dalla costruzione di un nutrito corpus di fonti primarie, si è proceduto all’analisi dei testi reperiti attraverso un approccio metodologico che, fondamentalmente storiografico, accoglie tuttavia alcuni rudimenti interpretativi elaborati in ambito semiotico (con particolare riferimento alle teorizzazioni di Jurij Lotman e Umberto Eco), il tutto al fine di cogliere, pur nell’estrema varietà formale e contenutistica offerta dal materiale documentario, alcune dinamiche culturali di fondo attraverso le quali disegnare, da un lato, il panorama delle tipologie di danza effettivamente praticate sulle scene italiane del Ventennio,e, dall’altro, quello dell’insieme di pensieri, opinioni e gusti orbitanti attorno ad esse Ne è scaturita una trattazione fondamentalmente tripartita in cui, dopo la messa in campo delle questioni metodologiche, si passa dapprima attraverso l’indagine dei tre principali generi di danza che, nella stampa del periodo fascista, si ritenevano caratteristici della scena coreica internazionale – qui definiti nei termini di “ballo teatrale”, “ballo russo” e “danze libere” – e, successivamente, si presenta un approfondimento su tre singolari figure di intellettuali che, ognuno con un’attitudine estremamente personale, hanno dedicato alla danza un’attenzione speciale: Anton Giulio Bragaglia, Paolo Fabbri e Marco Ramperti. Un’ampia antologia critica completa il lavoro ripercorrendone gli snodi principali.

Black Hole and Galaxy Growth over Cosmic Time: the Chandra COSMOS Legacy Survey

The study of supermassive black hole (SMBH) accretion during their phase of activity (hence becoming active galactic nuclei, AGN), and its relation to the host-galaxy growth, requires large datasets of AGN, including a significant fraction of obscured sources. X-ray data are strategic in AGN selection, because at X-ray energies the contamination from non-active galaxies is far less significant than in optical/infrared surveys, and the selection of obscured AGN, including also a fraction of heavily obscured AGN, is much more effective. In this thesis, I present the results of the Chandra COSMOS Legacy survey, a 4.6 Ms X-ray survey covering the equatorial COSMOS area. The COSMOS Legacy depth (flux limit f=2x10^(-16) erg/s/cm^(-2) in the 0.5-2 keV band) is significantly better than that of other X-ray surveys on similar area, and represents the path for surveys with future facilities, like Athena and X-ray Surveyor. The final Chandra COSMOS Legacy catalog contains 4016 point-like sources, 97% of which with redshift. 65% of the sources are optically obscured and potentially caught in the phase of main BH growth. We used the sample of 174 Chandra COSMOS Legacy at z>3 to place constraints on the BH formation scenario. We found a significant disagreement between our space density and the predictions of a physical model of AGN activation through major-merger. This suggests that in our luminosity range the BH triggering through secular accretion is likely preferred to a major-merger triggering scenario. Thanks to its large statistics, the Chandra COSMOS Legacy dataset, combined with the other multiwavelength COSMOS catalogs, will be used to answer questions related to a large number of astrophysical topics, with particular focus on the SMBH accretion in different luminosity and redshift regimes.

Topics in climate change risk

In this Thesis, we analyze how climate risk impacts economic players and its consequences on the financial markets. Essentially, literature unravels two main channels through which climate change poses risks to the status quo, namely physical and transitional risk, that we cover in three works. Firstly, the call for a global shift to a net-zero economy implicitly devalues assets that contribute to global warming that regulators are forcing to dismiss. On the other hand, abnormal changes in the temperatures as well as weather-related events challenge the environmental equilibrium and could directly affect operations as well as profitability. We start the analysis with the physical component, by presenting a statistical measure that generally represents shocks to the distribution of temperature anomalies. We oppose this statistic to classical physical measures and assess that it is the driver of the electricity consumption, in the weather derivatives market, and in the cross-section of equity returns. We find two transmission channels, namely investor attention, and firm operations. We then analyze the transition risk component, by associating a regulatory horizon characterization to fixed income valuation. We disentangle a risk driver for corporate bond overperformance that is tight to change in credit riskiness. After controlling a statistical learning algorithm to forecast excess returns, we include carbon emission metrics without clear evidence. Finally, we analyze the effects of change in carbon emission on a regulated market such as the EU ETS by selecting utility sector corporate bond and, after controlling for the possible risk factor, we document how a firm’s carbon profile differently affects the term structure of credit riskiness.

Obscured AGN in deep fields: tracing accretion and star-formation up to z ∼ 5

The discovery of scaling relations between the mass of the SMBH and some key physical properties of the host galaxy suggests that the growth of the SMBH and that of the galaxy are coupled, with the AGN activity and the star-formation (SF) processes influencing each other. Although the mechanism of this co-evolution are still a matter of debate, all scenarios agree that a key phase of the co-evolution is represented by the obscured accretion phase. This phase is of the co-evolution is the least studied, mostly due to the challenge in detecting and recognizing such obscured AGN. My thesis aims at investigating the AGN-galaxy co-evolution paradigm by identifying and studying AGN in the obscured accretion phase. The study of obscured AGN is key for our understanding of the feedback processes and of the mutual influence of the SF and the AGN activity. Moreover, these obscured and elusive AGN are needed to explain the X-ray background spectrum and to reconcile the measurements and the theoretical prediction of the BH accretion rate density. In this thesis, we firstly investigate the synergies between IR and X-ray missions in detecting and characterizing AGN, with a particular focus on the most obscured ones. We exploited UV/optical emission lines to select high-redshift obscured AGN at the cosmic noon, where the highest SFR density and BH accretion rate density are expected. We provide X-ray spectral analysis and UV-to-far-IR SED-fitting. We show that our samples host a significant fraction of very obscured sources; many of these are highly accreting. Finally, we performe a thoughtful investigation of a galaxy at z~5 with unusual and peculiar features, that lead us to identify a second extremely young population of stars and hidden AGN activity.