Origin of cold gas and dust in massive elliptical galaxies

The recent availability of multi-wavelength data revealed the presence of large reservoirs of warm and cold gas and dust in the innermost regions of the majority of massive elliptical galaxies. To prove an internal origin of cold and warm gas, the investigation of the spatially distributed cooling process which occurs because of non-linear density perturbations and subsequent thermal instabilities is of crucial importance. The first goal of this work of thesis is to investigate the internal origin of warm and cold phases. Numerical simulations are the powerful tool of analysis. The way in which a spatially distributed cooling process originates has been examined and the off-centre amount of gas mass which cools when different and differently characterized AGN feedback mechanisms operate has been quantified. This thesis demonstrates that the aforementioned non-linear density perturbations originate and develop from AGN feedback mechanisms in a natural fashion. An internal origin of the warm phase from the once hot gas is shown to be possible. Computed velocity dispersions of ionized and hot gas are similar. The cold gas as well can originate from the cooling process: indeed, it has been estimated that the surrounding stellar radiation, which is one of the most feasible sources of ionization of the warm gas, does not manage to keep ionized all the gas at 10^4 K. Therefore, cooled gas does undergo a further cooling which can lead the warm phase to lower temperatures. However, the gas which has cooled from the hot phase is expected to be dustless; nonetheless, a large fraction of early type galaxies has detectable dust in their cores, both concentrated in filamentary and disky structures and spread over larger regions. Therefore a regularly rotating disk of cold and dusty gas has been included in the simulations. A new quantitative investigation of the spatially distributed cooling process has therefore been essential: the contribution of the included amount of dust which is embedded in the cold gas does have a role in promoting and enhancing the cooling. The fate of dust which was at first embedded in cold gas has been investigated. The role of AGN feedback mechanisms in dragging (if able) cold and dusty gas from the core of massive ellipticals up to large radii has been studied.

Natural Wax-Based Water Vapour Barrier Coatings on PLA for MAP Food Packaging

PLA is a bio-based polymer that is obtained from renewable resources and it is very promising for a sustainable packaging manufacturing. However, its gas and vapour barrier properties are not enough to comply with the requirements of MAP packaging of fresh foods, which need specific concentration of water and oxygen to avoid spoilage and to keep the organoleptic properties unaltered throughout their shelf-life. The use of waxes from natural renewable sources such as plants (e.g., candelilla wax, carnauba wax, rice bran wax, sunflower wax) or animals (e.g., beeswax) could tackle down the permeation of water vapour through the packaging without affecting its bio-based content. The core of this work is developing wax-based coatings with enhanced thermo-mechanical properties so that they can undergo thermoforming and a proper adhesion to the PLA substrate can be ensured. Chemical modifications and crosslinking of waxes are performed to produce wax-based alkyd resins. The synthesised materials are characterised both by DSC and FTIR. Films of the wax-based alkyds are produced in order to assess their water vapour permeability.