Development of new tools and devices for CMB and foreground data analysis and future experiments

The discovery of the Cosmic Microwave Background (CMB) radiation in 1965 is one of the fundamental milestones supporting the Big Bang theory. The CMB is one of the most important source of information in cosmology. The excellent accuracy of the recent CMB data of WMAP and Planck satellites confirmed the validity of the standard cosmological model and set a new challenge for the data analysis processes and their interpretation. In this thesis we deal with several aspects and useful tools of the data analysis. We focus on their optimization in order to have a complete exploitation of the Planck data and contribute to the final published results. The issues investigated are: the change of coordinates of CMB maps using the HEALPix package, the problem of the aliasing effect in the generation of low resolution maps, the comparison of the Angular Power Spectrum (APS) extraction performances of the optimal QML method, implemented in the code called BolPol, and the pseudo-Cl method, implemented in Cromaster. The QML method has been then applied to the Planck data at large angular scales to extract the CMB APS. The same method has been applied also to analyze the TT parity and the Low Variance anomalies in the Planck maps, showing a consistent deviation from the standard cosmological model, the possible origins for this results have been discussed. The Cromaster code instead has been applied to the 408 MHz and 1.42 GHz surveys focusing on the analysis of the APS of selected regions of the synchrotron emission. The new generation of CMB experiments will be dedicated to polarization measurements, for which are necessary high accuracy devices for separating the polarizations. Here a new technology, called Photonic Crystals, is exploited to develop a new polarization splitter device and its performances are compared to the devices used nowadays.

The Perception of American Adolescent Culture Through the Dubbing and Fansubbing of a Selection of US Teen Series from 1990 to 2013

The present dissertation aims at analyzing the construction of American adolescent culture through teen-targeted television series and the shift in perception that occurs as a consequence of the translation process. In light of the recent changes in television production and consumption modes, largely caused by new technologies, this project explores the evolution of Italian audiences, focusing on fansubbing (freely distributed amateur subtitles made by fans for fan consumption) and social viewing (the re-aggregation of television consumption based on social networks and dedicated platforms, rather than on physical presence). These phenomena are symptoms of a sort of ‘viewership 2.0’ and of a new type of active viewing, which calls for a revision of traditional AVT strategies. Using a framework that combines television studies, new media studies, and fandom studies with an approach to AVT based on Descriptive Translation Studies (Toury 1995), this dissertation analyzes the non-Anglophone audience’s growing need to participation in the global dialogue and appropriation process based on US scheduling and informed by the new paradigm of convergence culture, transmedia storytelling, and affective economics (Jenkins 2006 and 2007), as well as the constraints intrinsic to multimodal translation and the different types of linguistic and cultural adaptation performed through dubbing (which tends to be more domesticating; Venuti 1995) and fansubbing (typically more foreignizing). The study analyzes a selection of episodes from six of the most popular teen television series between 1990 and 2013, which has been divided into three ages based on the different modes of television consumption: top-down, pre-Internet consumption (Beverly Hills, 90210, 1990 – 2000), emergence of audience participation (Buffy the Vampire Slayer, 1997 – 2003; Dawson’s Creek, 1998 – 2003), age of convergence and Viewership 2.0 (Gossip Girl, 2007 – 2012; Glee, 2009 – present; The Big Bang Theory, 2007 - present).

L'atomo di idrogeno: Righe, serie e sua importanza in astrofisica.

L’idrogeno è l’elemento chimico più semplice, leggero e abbondante nell’universo. L’atomo è composto da un nucleo, nella maggior parte dei casi formato da un unico protone o al più da un protone e un neutrone (che formano l’isotopo meno stabile detto deuterio), e da un elettrone che orbita attorno al nucleo. Per tale motivo viene classificato come il primo elemento della tavola periodica, con simbolo H e con numero atomico pari ad 1 (Z = 1) e stesso numero di massa (o numero di massa pari a 2 per il deuterio A = 2). Dal punto di vista isotopico l’idrogeno è composto per il 99.985% da prozio (idrogeno con A=1) e per il 0,015% da deuterio (A=2). Tutti gli altri isotopi sono instabili e meno abbondanti in natura. Data la sua semplicità l’idrogeno è il primo elemento formatosi dopo il Big Bang e da ciò ne deriva la sua abbondanza nell’universo e dunque la sua importanza in astrofisica.

Inflazione cosmica e onde gravitazionali primordiali

La teoria dell'inflazione risolve alcuni problemi fondamentali posti dalla teoria standard dell'origine dell'universo, in particolare chiarisce perché l'universo è piatto e omogeneo quando secondo la cosmologia standard non lo dovrebbe essere (o meglio: lo potrebbe essere solo con probabilità molto bassa). Inoltre la teoria dell'inflazione spiega l'origine delle anisotropie della radiazione cosmica di fondo e in tal modo l'inflazione è responsabile anche dell'origine della struttura a grande scala dell'universo. La teoria inflazionaria presenta la possibilità di una conferma sperimentale. Alcune sue predizioni sono già state verificate e una forte prova era sembrata venire dall'esperimento BICEP2, ma per ora (novembre 2014) non c'è stata una conferma. Nello specifico, l'esperimento BICEP2 aveva dichiarato a marzo 2014 di aver rilevato nella radiazione cosmica di fondo il segnale di onde gravitazionali che potevano essere state provocate soltanto dall'inflazione. La presente tesi descrive gli aspetti classici (non quantistici) della teoria dell'inflazione, riporta i risultati relativi alla trattazione quantistica delle perturbazioni della radiazione cosmica di fondo e illustra la questione delle verifiche sperimentali della teoria dell'inflazione, dedicando particolare rilievo al recente esperimento BICEP2.

Ricostruzione di segnali multipli del rivelatore a tempo di volo (ToF) di ALICE: confronto fra dati e Monte Carlo

La fisica delle collisioni ad alte energie è, ad oggi, uno dei campi di ricerca più interessante per la verifica di modelli teorici che spieghino la nascita e la formazione dell'universo in cui viviamo. In quest'ottica lavorano esperimenti presso i più importanti acceleratori di particelle: tra questi anche l'esperimento ALICE, presso il Large Hadron Collider LHC del CERN di Ginevra. Il suo scopo principale è quello di verificare e ampliare l'insieme delle prove sperimentali alla base sull'esistenza di un nuovo stato della materia: il Quark Gluon Plasma. La presenza della transizione di fase della materia adronica ordinaria a QGP era stata teorizzata da diversi studi termodinamici e da calcoli di QCD su reticolo: in particolare si prevedeva l'esistenza di uno stato della materia in cui i quark sono deconfinati. Il QGP è dunque un plasma colorato e densissimo di quark e gluoni, liberi di interagire tra loro. Queste condizioni sarebbero state quelle dell'universo primordiale, circa 1µs dopo il Big Bang: a seguito di una transizione di fase, si sarebbe poi formata tutta la materia adronica ordinaria. Per riprodurre le condizioni necessarie alla formazione del QGP occorrono collisioni ad energie ultrarelativistiche come quelle prodotte, negli ultimi anni, dall'acceleratore LHC. Uno dei principali rivelatori dedicati all'identificazione di particelle in ALICE è il sistema a tempo di volo TOF. Nonostante un attento processo di ottimizzazione della risoluzione delle sue componenti, persistono residui errori strumentali che limitano la qualità (già ottima) del segnale, tutt'oggi oggetto di studio. L'elaborato presentato in questa tesi è suddiviso in tre capitoli: nel primo ripercorriamo gli aspetti teorici del Modello Standard e del Quark Gluon Plasma. Nel secondo descriviamo la struttura di rivelazione di ALICE, analizzando il funzionamento delle singole componenti. Nel terzo, infine, verifichiamo le principali correzioni al TOF ad oggi note, confrontando i dati a nostra disposizione con delle simulazioni Monte Carlo: questo ci permette da un lato di approfondirne la conoscenza, dall'altro di cercarne di migliorare la descrizione del comportamento del rivelatore.

The Pre-1980 Roots of Neoliberal Financial Deregulation

U.S. financial deregulation is often popularly presented as a fundamental attack on financial regulation that began with neoliberalism's Big Bang in 1980. This paper argues this position is wrong in two ways. First, it is a process that stretches back decades before 1980. Textbook mentions of 1970s precursor "financial innovations" fall far short of presenting the breadth and duration of the pre-1980 attack on the system of regulation. Second, it has not been an across-the-board attack on financial regulation in the name of market efficiency as required by its ideology and claimed by its advocates, but rather a focused attack on only one of the five pillars of the system of regulation. This paper develops both of these assertions through a presentation of the five central pillars of the pre-1980 system of financial regulation, and the four major attacks on the three different aspects of the restrictions on financial competition.

"Évaluer", "accompagner", "contrarier":

Diskutiert werden die Möglichkeiten architektonischen Einfügens anhand der Position, die der französische Architekt Jean Nouvel in Theorie wie Praxis einnimmt. Im Rückblick auf sein Werk zeigt sich dabei, dass er sich von Anbeginn mit der Reflexion über die Möglichkeiten und die Grenzen architektonischen Einfügens in bereits bestehende bauliche Ensembles auseinandergesetzt und eine Reihe von Konzepten entwickelt hat, deren Begrifflichkeit sich an Philosophen wie Félix Guattari, Gilles Deleuze und Michel Foucault orientiert. Die konkrete Anwendung dieser Begriffe wird anhand von zwei Projekten erörtert, die einmal die Einfügung eines kompletten Gebäudeinnern in bereits bestehende Außenwände eines historischen Baus (Oper Lyon), ein anderes Mal die Einfügung eines Neubaus in ein prägnantes, städtebauliches Ensemble (Hotel "Sofitel Vienna Stephansdom“) betreffen.

Los latidos del tiempo : Un viaje imaginario desde el origen del universo hasta nuestros días

El conocimiento científico provisorio y cambiante, nos permite entender la realidad que nos rodea de una determinada manera. Esta no es la única forma de comprender nuestro universo pero sin duda explica los fenómenos de un modo racional y empírico. Esto se realiza mediante la formulación de hipótesis, la corroboración y contrastación de las mismas, comunicando los resultados y abriendo el juego a diversas opiniones que, lejos de criticar destructivamente, afianzan los conocimientos, solidificando las bases en una construcción colectiva del saber (Desantes-Guanter et al 2000). Este es el espíritu que se transmite a quienes participan de Latidos del Tiempo; una propuesta de extensión. Un recorrido guiado por especialistas en astronomía, zoología, ecología, biología de la conservación y antropología, que articula tres importantes centros de formación, divulgación y entretenimiento: el Observatorio Astronómico, el Museo de Ciencias Naturales y el Jardín Zoológico y Botánico de La Plata. La actividad, abarca los hitos más importantes de la evolución cósmica. Comienza con el Big Bang, incursionando por el Origen de la Vida y el Origen del Hombre hasta el presente, reflexionando sobre las problemáticas ambientales actuales y sobre nuestra responsabilidad como especie racional sobre el Planeta. El desafío y principal logro de la actividad, consiste en abordar cada tema de manera amena y multidisciplinar pero desdibujando los límites de cada disciplina, tratando de que los participantes experimenten la continuidad de los diversos hitos, integrando y relacionando los eventos, discutiendo ante distintas interpretaciones y generando nuevos interrogantes, más que de respuestas definitivas.

Los latidos del tiempo : Un viaje imaginario desde el origen del universo hasta nuestros días

El conocimiento científico provisorio y cambiante, nos permite entender la realidad que nos rodea de una determinada manera. Esta no es la única forma de comprender nuestro universo pero sin duda explica los fenómenos de un modo racional y empírico. Esto se realiza mediante la formulación de hipótesis, la corroboración y contrastación de las mismas, comunicando los resultados y abriendo el juego a diversas opiniones que, lejos de criticar destructivamente, afianzan los conocimientos, solidificando las bases en una construcción colectiva del saber (Desantes-Guanter et al 2000). Este es el espíritu que se transmite a quienes participan de Latidos del Tiempo; una propuesta de extensión. Un recorrido guiado por especialistas en astronomía, zoología, ecología, biología de la conservación y antropología, que articula tres importantes centros de formación, divulgación y entretenimiento: el Observatorio Astronómico, el Museo de Ciencias Naturales y el Jardín Zoológico y Botánico de La Plata. La actividad, abarca los hitos más importantes de la evolución cósmica. Comienza con el Big Bang, incursionando por el Origen de la Vida y el Origen del Hombre hasta el presente, reflexionando sobre las problemáticas ambientales actuales y sobre nuestra responsabilidad como especie racional sobre el Planeta. El desafío y principal logro de la actividad, consiste en abordar cada tema de manera amena y multidisciplinar pero desdibujando los límites de cada disciplina, tratando de que los participantes experimenten la continuidad de los diversos hitos, integrando y relacionando los eventos, discutiendo ante distintas interpretaciones y generando nuevos interrogantes, más que de respuestas definitivas.

Is redshift-dependent evolution of galaxies a theoretical artifact?

The physical validity of the hypothesis of (redshift-dependent) luminosity evolution in galaxies is tested by statistical analysis of an intensively studied complete high-redshift sample of normal galaxies. The necessity of the evolution hypothesis in the frame of big-bang cosmology is confirmed at a high level of statistical significance; however, this evolution is quantitatively just as predicted by chronometric cosmology, in which there is no such evolution. Since there is no direct observational means to establish the evolution postulated in big-bang studies of higher-redshift galaxies, and the chronometric predictions involve no adjustable parameters (in contrast to the two in big-bang cosmology), the hypothesized evolution appears from the standpoint of conservative scientific methodology as a possible theoretical artifact.

Supernovae, an accelerating universe and the cosmological constant

Observations of supernova explosions halfway back to the Big Bang give plausible evidence that the expansion of the universe has been accelerating since that epoch, approximately 8 billion years ago and suggest that energy associated with the vacuum itself may be responsible for the acceleration.

The microwave background anisotropies: Observations

Most cosmologists now believe that we live in an evolving universe that has been expanding and cooling since its origin about 15 billion years ago. Strong evidence for this standard cosmological model comes from studies of the cosmic microwave background radiation (CMBR), the remnant heat from the initial fireball. The CMBR spectrum is blackbody, as predicted from the hot Big Bang model before the discovery of the remnant radiation in 1964. In 1992 the cosmic background explorer (COBE) satellite finally detected the anisotropy of the radiation—fingerprints left by tiny temperature fluctuations in the initial bang. Careful design of the COBE satellite, and a bit of luck, allowed the 30 μK fluctuations in the CMBR temperature (2.73 K) to be pulled out of instrument noise and spurious foreground emissions. Further advances in detector technology and experiment design are allowing current CMBR experiments to search for predicted features in the anisotropy power spectrum at angular scales of 1° and smaller. If they exist, these features were formed at an important epoch in the evolution of the universe—the decoupling of matter and radiation at a temperature of about 4,000 K and a time about 300,000 years after the bang. CMBR anisotropy measurements probe directly some detailed physics of the early universe. Also, parameters of the cosmological model can be measured because the anisotropy power spectrum depends on constituent densities and the horizon scale at a known cosmological epoch. As sophisticated experiments on the ground and on balloons pursue these measurements, two CMBR anisotropy satellite missions are being prepared for launch early in the next century.

Galaxy formation

It is argued that within the standard Big Bang cosmological model the bulk of the mass of the luminous parts of the large galaxies likely had been assembled by redshift z ∼ 10. Galaxy assembly this early would be difficult to fit in the widely discussed adiabatic cold dark matter model for structure formation, but it could agree with an isocurvature version in which the cold dark matter is the remnant of a massive scalar field frozen (or squeezed) from quantum fluctuations during inflation. The squeezed field fluctuations would be Gaussian with zero mean, and the distribution of the field mass therefore would be the square of a random Gaussian process. This offers a possibly interesting new direction for the numerical exploration of models for cosmic structure formation.

Primordial emergence of the recombination activating gene 1 (RAG1): sequence of the complete shark gene indicates homology to microbial integrases.

The rearrangement of antibody and T-cell receptor gene segments is indispensable to the vertebrate immune response. All extant jawed vertebrates can rearrange these gene segments. This ability is conferred by the recombination activating genes I and II (RAG I and RAG II). To elucidate their origin and function, the cDNA encoding RAG I from a member of the most ancient class of extant gnathostomes, the Carcharhine sharks, was characterized. Homology domains identified within shark RAG I prompted sequence comparison analyses that suggested similarity of the RAG I and II genes, respectively, to the integrase family genes and integration host factor genes of the bacterial site-specific recombination system. Thus, the apparent explosive evolution (or "big bang") of the ancestral immune system may have been initiated by a transfer of microbial site-specific recombinases.

Constraining the GRB-Magnetar Model by Means of the Galactic Pulsar Population

A large fraction of Gamma-ray bursts (GRBs) displays an X-ray plateau phase within <105 s from the prompt emission, proposed to be powered by the spin-down energy of a rapidly spinning newly born magnetar. In this work we use the properties of the Galactic neutron star population to constrain the GRB-magnetar scenario. We re-analyze the X-ray plateaus of all Swift GRBs with known redshift, between 2005 January and 2014 August. From the derived initial magnetic field distribution for the possible magnetars left behind by the GRBs, we study the evolution and properties of a simulated GRB-magnetar population using numerical simulations of magnetic field evolution, coupled with Monte Carlo simulations of Pulsar Population Synthesis in our Galaxy. We find that if the GRB X-ray plateaus are powered by the rotational energy of a newly formed magnetar, the current observational properties of the Galactic magnetar population are not compatible with being formed within the GRB scenario (regardless of the GRB type or rate at z = 0). Direct consequences would be that we should allow the existence of magnetars and "super-magnetars" having different progenitors, and that Type Ib/c SNe related to Long GRBs form systematically neutron stars with higher initial magnetic fields. We put an upper limit of ≤16 "super-magnetars" formed by a GRB in our Galaxy in the past Myr (at 99% c.l.). This limit is somewhat smaller than what is roughly expected from Long GRB rates, although the very large uncertainties do not allow us to draw strong conclusion in this respect.