Phthalocyanine-based systems: synthesis, properties and applications

A presente dissertação descreve a síntese e o estudo de propriedades fotofísicas e biológicas de sistemas baseados em ftalocianinas. Os sistemas sintetizados consistem em ftalocianinas contendo unidades de D-galactose, ciclodextrinas, [60]fulereno ou porfirinas. Na primeira parte da dissertação aborda-se a síntese de ftalocianinas substituídas com unidades de D-galactose, com o intuito de serem utilizadas como fotossensibilizadores em terapia fotodinâmica. A eficiência de geração de oxigénio singuleto induzida pelas glicoftalocianinas, bem como a sua actividade fotodinâmica in vitro em células HeLa são avaliadas. Adicionalmente são descritos os estudos de MALDI-MS/MS de dois pares de glicoftalocianinas isoméricas. Numa segunda parte, descrevem-se a síntese e a caracterização de sistemas supramoleculares de ftalocianinas ligadas a ciclodextrinas ou [60]fulereno. Foram desenvolvidas metodologias sintéticas para obter complexos ftalocianínicos de ruténio(II) substituídos axialmente com derivados de ciclodextrinas, e complexos ftalocianínicos de zinco(II) ligados covalentemente a ciclodextrinas. Descreve-se também a síntese de uma díade ftalocianina- [60]fulereno. A estratégia sintética envolve um peculiar primeiro passo, uma reacção de aminação redutiva, no qual se obtém uma ftalocianina funcionalizada com glicina, seguida da habitual reacção de cicloadição 1,3- dipolar. Na terceira parte, abordam-se sistemas dador-aceitador de díades porfirinaftalocianina, como modelos promissores para mimetizar sistemas fotossintéticos naturais. Diferentes tipos de díades porfirina-ftalocianina, ligadas através do grupo fenilo da posição meso ou da posição β-pirrólica da porfirina, são sintetizadas e caracterizadas. As abordagens sintéticas envolvem reacções de aminação catalisadas por paládio e reacções de condensação cruzada de dois ftalonitrilos adequadamente substituídos. Também se descrevem processos de transferência de energia e electrónica fotoinduzidos que se formam a partir das díades porfirina-ftalocianina.

Model-based systems engineering: a system for traffic & environment

The contemporary world is crowded of large, interdisciplinary, complex systems made of other systems, personnel, hardware, software, information, processes, and facilities. The Systems Engineering (SE) field proposes an integrated holistic approach to tackle these socio-technical systems that is crucial to take proper account of their multifaceted nature and numerous interrelationships, providing the means to enable their successful realization. Model-Based Systems Engineering (MBSE) is an emerging paradigm in the SE field and can be described as the formalized application of modelling principles, methods, languages, and tools to the entire lifecycle of those systems, enhancing communications and knowledge capture, shared understanding, improved design precision and integrity, better development traceability, and reduced development risks. This thesis is devoted to the application of the novel MBSE paradigm to the Urban Traffic & Environment domain. The proposed system, the GUILTE (Guiding Urban Intelligent Traffic & Environment), deals with a present-day real challenging problem “at the agenda” of world leaders, national governors, local authorities, research agencies, academia, and general public. The main purposes of the system are to provide an integrated development framework for the municipalities, and to support the (short-time and real-time) operations of the urban traffic through Intelligent Transportation Systems, highlighting two fundamental aspects: the evaluation of the related environmental impacts (in particular, the air pollution and the noise), and the dissemination of information to the citizens, endorsing their involvement and participation. These objectives are related with the high-level complex challenge of developing sustainable urban transportation networks. The development process of the GUILTE system is supported by a new methodology, the LITHE (Agile Systems Modelling Engineering), which aims to lightening the complexity and burdensome of the existing methodologies by emphasizing agile principles such as continuous communication, feedback, stakeholders involvement, short iterations and rapid response. These principles are accomplished through a universal and intuitive SE process, the SIMILAR process model (which was redefined at the light of the modern international standards), a lean MBSE method, and a coherent System Model developed through the benchmark graphical modeling languages SysML and OPDs/OPL. The main contributions of the work are, in their essence, models and can be settled as: a revised process model for the SE field, an agile methodology for MBSE development environments, a graphical tool to support the proposed methodology, and a System Model for the GUILTE system. The comprehensive literature reviews provided for the main scientific field of this research (SE/MBSE) and for the application domain (Traffic & Environment) can also be seen as a relevant contribution.

Close-in planets around giant stars: lack of hot-Jupiters and prevalence of multiplanetary systems

Extrasolar planets abound in almost any possible configuration. However, until five years ago, there was a lack of planets orbiting closer than 0.5 au to giant or subgiant stars. Since then, recent detections have started to populated this regime by confirming 13 planetary systems. We discuss the properties of these systems in terms of their formation and evolution off the main sequence. Interestingly, we find that 70.0 ± 6.6% of the planets in this regime are inner components of multiplanetary systems. This value is 4.2σ higher than for main-sequence hosts, which we find to be 42.4 ± 0.1%. The properties of the known planets seem to indicate that the closest-in planets (a< 0.06 au) to main-sequence stars are massive (i.e., hot Jupiters) and isolated and that they are subsequently engulfed by their host as it evolves to the red giant branch, leaving only the predominant population of multiplanetary systems in orbits 0.06 and evolution of hot Jupiters.