Forecasts on the dark energy anisotropic stress for the esa euclid survey

The cosmological constant Λ seems to be a not satisfactory explanation of the late-time accelerated expansion of the Universe, for which a number of experimental evidences exist; therefore, it has become necessary in the last years to consider alternative models of dark energy, meant as cause of the accelerated expansion. In the study of dark energy models, it is important to understand which quantities can be determined starting from observational data, without assuming any hypothesis on the cosmological model; such quantities have been determined in Amendola, Kunz et al., 2012. In the same paper it has been further shown that it is possible to estabilish a relation between the model-independent parameters and the anisotropic stress η, which can be also expressed as a combination of the functions appearing in the most general Lagrangian for the scalar-tensor theories, the Horndeski Lagrangian. In the present thesis, the Fisher matrix formalism is used to perform a forecast on the constraints that will be possible to make on the anisotropic stress η in the future, starting from the estimated uncertainties for the galaxy clustering and weak lensing measurements which will be performed by the European Space Agency Euclid mission, to be launched in 2020. Further, constraints coming from supernovae-Ia observations are considered. The forecast is performed for two cases in which (a) η is considered as depending from redshift only and (b) η is constant and equal to one, as in the ΛCDM model.

Classificazione a faccette di obiettivi formativi dell’insegnamento universitario, nelle discipline umanistiche in Austria, Germania, Italia e Regno Unito

Il processo di riforma a carattere europeo che ha condotto alla nascita di uno Spazio Europeo dell’Istruzione Superiore ha conosciuto diverse tappe fondamentali, fra cui, per esempio, la ripartizione in cicli e l’adozione dei crediti ECTS. Una di queste tappe, ossia il passaggio da una pianificazione della didattica basata sui contenuti ad una basata sui risultati dell’apprendimento, ricopre un ruolo di primo piano nel presente progetto di dottorato. Lo studio qui descritto ha esaminato, da un punto di vista sintattico e semantico, un campione di obiettivi e risultati dell’apprendimento di insegnamenti di alcuni corsi di laurea di primo e secondo ciclo, delle scienze umanistiche, in Austria, Germania, Italia e Regno Unito. L’obiettivo del progetto è proporre uno schema per una classificazione a faccette di obiettivi dell’apprendimento denominato FLOC. Tale schema è adottato per classificare gli obiettivi dell’apprendimento di quattro contesti linguistico-culturali (nei paesi summenzionati), dando vita a FLOC-AT, FLOC-DE, FLOC-IT e FLOC-EN. Queste quattro classificazioni forniscono inoltre il contesto per un’analisi contrastiva multilingue fra unità di obiettivi di apprendimento.

The AMS-02 Experiment and the Dark Matter Search

AMS-02 is running after great scientific goals since one year and a half: a final setting up for dark matter searches has been achieved, allowing to study the so important antiparticle to particle ratios, which will probably be the first dark matter signals ever corroborated. Even if primary cosmic rays fluxes are subjected to a lot of uncertainties sources, some statements can be done and have been written down about dark matter properties: DM should be a heavy Majorana fermion or Spin 0 or 1 boson, with a mass from about 1 TeV to 10 TeV - unveiling a new TeV-ish search age - which could be able to originate antiparticle fluxes enhancements at high energies, both for positrons and antiprotons. All the observations, direct and indirect, point to these new paradigms or can be traced back to them quite easily. These enhancements perfectly fall into the research window of AMS-02, allowing the experiment to attack each today credible theory. Also an investigation of the Sommerfeld effect-associated dark boson will be possible, in terms of antiparticle to particle ratios substructures. The first great AMS-02 measurement is the positron fraction: an official paper is going to be submitted in few months, where the correct behavior of the apparatus will be reviewed and the full positron fraction rate will be analyzed up to 200 GeV. In this concern, one of the objectives of this work is to test the AMS-02 capability and versatility in doing these dark matter researches, thanks to an orbital temporal (and geomagnetic) stability. The goal has been accomplished: the experiment is very stable in time, so that the temporal error associated to the positron fraction measurement is compatible with zero, offering a beyond belief opportunity to measure CR antiparticle to particle ratios.