Space charge and dielectric response measurements to assess insulation aging of low-voltage cables used in nuclear power plants

The current design life of nuclear power plant (NPP) could potentially be extended to 80 years. During this extended plant life, all safety and operationally relevant Instrumentation & Control (I&C) systems are required to meet their designed performance requirements to ensure safe and reliable operation of the NPP, both during normal operation and subsequent to design base events. This in turn requires an adequate and documented qualification and aging management program. It is known that electrical insulation of I&C cables used in safety related circuits can degrade during their life, due to the aging effect of environmental stresses, such as temperature, radiation, vibration, etc., particularly if located in the containment area of the NPP. Thus several condition monitoring techniques are required to assess the state of the insulation. Such techniques can be used to establish a residual lifetime, based on the relationship between condition indicators and ageing stresses, hence, to support a preventive and effective maintenance program. The object of this thesis is to investigate potential electrical aging indicators (diagnostic markers) testing various I&C cable insulations subjected to an accelerated multi-stress (thermal and radiation) aging.

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.

Charge and spin transport in memristive La0.7Sr0.3Mno3/SrTiO3/Co devices

Il lavoro svolto si concentra sul trasporto di carica e spin in dispositivi trilayer La0.7Sr0.3MnO3/SrTiO3/Co multifunzionali. Questi dispositivi mostrano sia magnetoresistenza che resistive switching, con un'interessante interazione fra i due effetti. Le giunzioni SrTiO3 sono state scelte per questo lavoro sia per via dei precedenti studi su SrTiO3 come barriera in dispositivi spintronici (cioè dispositivi con magnetoresistenza), sia perché sono promettenti come materiale base per costruire memristor (cioè dispositivi con resistive switching). Il lavoro di tesi è stato svolto all'Istituto per lo studio dei materiali nanostrutturati (ISMN-CNR) a Bologna. Nella prima parte di questa tesi illustrerò la fisica dietro al resistive switching e alla magnetoresistenza di dispositivi trilayer, mostrando anche risultati di studi su dispositivi simili a quelli da me studiati. Nella seconda parte mostrerò la complessa fisica degli ossidi utilizzati nei nostri dispositivi e i possibili meccanismi di trasporto attraverso essi. Nell'ultima parte descriverò i risultati ottenuti. I dispositivi La0.7Sr0.3MnO3/SrTiO3/Co sono stati studiati tramite caratterizzazione elettrica, di magnetotrasporto e con spettroscopia di impedenza. Le misure ottenute hanno mostrato una fisica molto ricca dietro al trasporto di spin e carica in questi dispositivi, e la mutua interazione fra fenomeni spintronici e di resistive switching rappresenta una chiave per comprendere la fisica di questi fenomeni. Analisi dati della dipendenza della resistenza della temperature e caratteristiche corrente-tensioni saranno usati per quantificare e descrivere il trasporto in questi dispositivi.