Radiações evolutivas estão entre os eventos mais fascinantes da evolução. Grande parte da diversidade da vida, tanto de espécies como ecológica, surgiu nos breves intervalos temporais de rápida especiação que configuram as radiações. As causas ecológicas e não-ecológicas do surgimento da diversidade em radiações evolutivas, em especial nas radiações adaptativas, são tema de pesquisa há muito tempo, pelo menos desde que Darwin observou a imensa diversidade de um grupo de pássaros nas ilhas Galápagos. Desde então, as ilhas têm sido os ambientes ideais para o estudo desse fenômeno, e foi a partir das observações e experimentos em ilhas que toda a teoria ecológica das radiações evolutivas surgiu. Contudo, as causas ecológicas das radiações explosivas ocorridas em amplas escalas continentais permanecem tema de constante debate. Nesta tese, foram investigados os determinantes ecológicos e não-ecológicos (e.g., geografia, contingências históricas, efeitos filogenéticos) da evolução morfológica dos roedores sigmodontíneos durante sua radiação na região Neotropical, em especial no continente sul-americano. Para isso, foi quantificada a morfologia do crânio e mandíbula de mais de dois mil exemplares do grupo, e foram investigadas variações ecomorfológicas nos níveis interespecífico (I), intraespecífico (II), e entre assembleias de sigmodontíneos (III). Na Parte I da tese, foram investigadas duas predições da teoria da radiação adaptativa, a correlação-fenótipo ambiente (capítulo 1) e a funcionalidade do fenótipo através da força da mordida (capítulo 2), permitindo determinar o papel da divergência ecológica na evolução morfológica das espécies. Na Parte II (capítulo 3), foram investigadas as contribuições relativas de processos determinísticos e neutros sobre a variação morfológica entre populações de uma espécie de roedor sigmodontíneo amplamente distribuída, Akodon cursor. Na Parte III, a influência da variação ambiental e da distribuição espacial das linhagens filogenéticas de sigmodontíneos sobre o tamanho corporal (capítulo 4) e forma do crânio e mandíbula (capítulo 5), foram investigados no contexto biogeográfico da variação no tamanho e forma média entre assembleias de sigmodontíneos. As contribuições originais desta tese foram: (i) mostrar que a radiação evolutiva dos roedores sigmodontíneos foi guiada principalmente por fatores históricos e geográficos ao invés de fatores ecológicos; (ii) sugerir que radiações evolutivas ocorridas em escalas continentais, especialmente de roedores, têm um componente geográfico e histórico mais determinante do que o componente ecológico; (iii) revelar que a força da mordida varia pouco entre roedores sigmodontíneos herbívoros e granívoros, o que provavelmente é resultado do fenótipo generalista desses roedores; (iv) apontar que sigmodontíneos com dieta insetívora têm uma taxa de evolução mais rápida, e parecem estar evoluindo sua forma do crânio/mandíbula e sua força da mordida em uma direção diferente das demais espécies; (v) demonstrar que, dentro de uma espécie de sigmodontíneo (Akodon cursor), fluxo gênico e deriva genética explicam melhor a forma do crânio entre populações, enquanto a variação ambiental explica melhor o tamanho do crânio, indicando que o tamanho é uma característica mais lábil e mais sujeita a pressões ambientais do que a forma do crânio; (vi) mostrar que a variação biogeográfica, tanto do tamanho quanto da forma média do crânio/mandíbula entre assembleias de sigmodontíneos, está sob influência da distribuição diferencial das linhagens filogenéticas ao longo do espaço geográfico, bem como de variáveis ambientais; o que indica conservação filogenética de nicho à nível de metacomunidades. De modo geral, ao investigar as contribuições relativas dos componentes adaptativo e não-adaptativo da evolução morfológica, foram obtidas informações importantes para conhecer as causas da diversificação morfológica em Sigmodontinae, aumentando nosso conhecimento sobre as origens de toda a diversidade biológica. / Evolutionary radiations are among the most fascinating phenomena of evolution. Most of the biological diversity on the planet, both in terms of species and ecological diversity, appeared during these brief intervals of rapid speciation. The ecological and non-ecological causes of the emergence of diversity in evolutionary radiations, especially in adaptive radiations, have long been the subject of research, beginning with Darwin and his notice of the astonishing diversity of bird forms in the Galapagos Islands. Islands have since been ideal environments in which to study evolutionary and adaptive radiations, and indeed it was from observations and experiments on islands that all ecological theory of evolutionary radiations arose. However, the ecological causes of explosive radiations occurring on large continental scales are still a matter of debate. In this dissertation, I investigated the ecological and non-ecological (e.g., geography, historical contingencies, phylogenetic effects) determinants of morphological evolution in sigmodontine rodents during their radiation in the Neotropical region, particularly on the South-American continent. The skull and mandible morphology of more than two thousand specimens was quantified, and ecomorphological variation was investigated on three levels: interspecific (I), intraspecific (II), and among sigmodontine assemblages (III). In part I, two predictions from the ecological theory of adaptive radiation were investigated: the phenotype-environment correlation (chapter 1), and the trait utility through the bite force (chapter 2). This approach enabled determination of the role of ecological divergence in species morphological evolution. In part II (chapter 3), I investigated the relative contributions of deterministic and neutral processes to morphological variation among populations of one widely distributed sigmodontine species, Akodon cursor. In part III, I investigated the influence of environmental variation and spatial distribution of phylogenetic lineages on body size (chapter 4) and on shape of the skull and mandible (chapter 5), in the context of biogeographical variation of mean size and shape in sigmodontine assemblages. The original contributions of this dissertation are as follows: (i) to demonstrate that the evolutionary radiation of sigmodontines was driven mainly by historical and geographical factors instead of ecological factors; (ii) to suggest that evolutionary radiations on continental scales, especially rodent radiations, have a more determinant historical and geographical component than an ecological one; (iii) to show small variation in bite force between sigmodontine herbivores and granivores, which is likely a consequence of the generalist phenotype of these rodents; (iv) to highlight that insectivorous sigmodontines have a faster rate of morphological evolution than other diet groups, and that skull and mandible morphology and bite force are evolving in different directions than in other species; (v) to demonstrate that within a sigmodontine species (Akodon cursor), gene flow and genetic drift better explain variation in skull shape among populations, while environmental variation better explains variation in skull size, which suggests that size is more labile feature than shape and thus more prone to change with environmental pressures; and (vi) to show that biogeographical variation in mean body size, mean skull shape, and mean mandible shape across sigmodontine assemblages is influenced by the different distributions of phylogenetic lineages over geographical space, as well by environmental variables, which indicates phylogenetic niche conservatism at the metacommunity level. These results shed light on some of the factors driving morphological diversification in Sigmodontinae. Further, the analytical approach(es) utilized may be useful for general investigations of the relative contributions of adaptive and non-adaptive components of morphological evolution, thereby potentially increasing our knowledge of the origins of all biological diversity.

Radiações evolutivas estão entre os eventos mais fascinantes da evolução. Grande parte da diversidade da vida, tanto de espécies como ecológica, surgiu nos breves intervalos temporais de rápida especiação que configuram as radiações. As causas ecológicas e não-ecológicas do surgimento da diversidade em radiações evolutivas, em especial nas radiações adaptativas, são tema de pesquisa há muito tempo, pelo menos desde que Darwin observou a imensa diversidade de um grupo de pássaros nas ilhas Galápagos. Desde então, as ilhas têm sido os ambientes ideais para o estudo desse fenômeno, e foi a partir das observações e experimentos em ilhas que toda a teoria ecológica das radiações evolutivas surgiu. Contudo, as causas ecológicas das radiações explosivas ocorridas em amplas escalas continentais permanecem tema de constante debate. Nesta tese, foram investigados os determinantes ecológicos e não-ecológicos (e.g., geografia, contingências históricas, efeitos filogenéticos) da evolução morfológica dos roedores sigmodontíneos durante sua radiação na região Neotropical, em especial no continente sul-americano. Para isso, foi quantificada a morfologia do crânio e mandíbula de mais de dois mil exemplares do grupo, e foram investigadas variações ecomorfológicas nos níveis interespecífico (I), intraespecífico (II), e entre assembleias de sigmodontíneos (III). Na Parte I da tese, foram investigadas duas predições da teoria da radiação adaptativa, a correlação-fenótipo ambiente (capítulo 1) e a funcionalidade do fenótipo através da força da mordida (capítulo 2), permitindo determinar o papel da divergência ecológica na evolução morfológica das espécies. Na Parte II (capítulo 3), foram investigadas as contribuições relativas de processos determinísticos e neutros sobre a variação morfológica entre populações de uma espécie de roedor sigmodontíneo amplamente distribuída, Akodon cursor. Na Parte III, a influência da variação ambiental e da distribuição espacial das linhagens filogenéticas de sigmodontíneos sobre o tamanho corporal (capítulo 4) e forma do crânio e mandíbula (capítulo 5), foram investigados no contexto biogeográfico da variação no tamanho e forma média entre assembleias de sigmodontíneos. As contribuições originais desta tese foram: (i) mostrar que a radiação evolutiva dos roedores sigmodontíneos foi guiada principalmente por fatores históricos e geográficos ao invés de fatores ecológicos; (ii) sugerir que radiações evolutivas ocorridas em escalas continentais, especialmente de roedores, têm um componente geográfico e histórico mais determinante do que o componente ecológico; (iii) revelar que a força da mordida varia pouco entre roedores sigmodontíneos herbívoros e granívoros, o que provavelmente é resultado do fenótipo generalista desses roedores; (iv) apontar que sigmodontíneos com dieta insetívora têm uma taxa de evolução mais rápida, e parecem estar evoluindo sua forma do crânio/mandíbula e sua força da mordida em uma direção diferente das demais espécies; (v) demonstrar que, dentro de uma espécie de sigmodontíneo (Akodon cursor), fluxo gênico e deriva genética explicam melhor a forma do crânio entre populações, enquanto a variação ambiental explica melhor o tamanho do crânio, indicando que o tamanho é uma característica mais lábil e mais sujeita a pressões ambientais do que a forma do crânio; (vi) mostrar que a variação biogeográfica, tanto do tamanho quanto da forma média do crânio/mandíbula entre assembleias de sigmodontíneos, está sob influência da distribuição diferencial das linhagens filogenéticas ao longo do espaço geográfico, bem como de variáveis ambientais; o que indica conservação filogenética de nicho à nível de metacomunidades. De modo geral, ao investigar as contribuições relativas dos componentes adaptativo e não-adaptativo da evolução morfológica, foram obtidas informações importantes para conhecer as causas da diversificação morfológica em Sigmodontinae, aumentando nosso conhecimento sobre as origens de toda a diversidade biológica. / Evolutionary radiations are among the most fascinating phenomena of evolution. Most of the biological diversity on the planet, both in terms of species and ecological diversity, appeared during these brief intervals of rapid speciation. The ecological and non-ecological causes of the emergence of diversity in evolutionary radiations, especially in adaptive radiations, have long been the subject of research, beginning with Darwin and his notice of the astonishing diversity of bird forms in the Galapagos Islands. Islands have since been ideal environments in which to study evolutionary and adaptive radiations, and indeed it was from observations and experiments on islands that all ecological theory of evolutionary radiations arose. However, the ecological causes of explosive radiations occurring on large continental scales are still a matter of debate. In this dissertation, I investigated the ecological and non-ecological (e.g., geography, historical contingencies, phylogenetic effects) determinants of morphological evolution in sigmodontine rodents during their radiation in the Neotropical region, particularly on the South-American continent. The skull and mandible morphology of more than two thousand specimens was quantified, and ecomorphological variation was investigated on three levels: interspecific (I), intraspecific (II), and among sigmodontine assemblages (III). In part I, two predictions from the ecological theory of adaptive radiation were investigated: the phenotype-environment correlation (chapter 1), and the trait utility through the bite force (chapter 2). This approach enabled determination of the role of ecological divergence in species morphological evolution. In part II (chapter 3), I investigated the relative contributions of deterministic and neutral processes to morphological variation among populations of one widely distributed sigmodontine species, Akodon cursor. In part III, I investigated the influence of environmental variation and spatial distribution of phylogenetic lineages on body size (chapter 4) and on shape of the skull and mandible (chapter 5), in the context of biogeographical variation of mean size and shape in sigmodontine assemblages. The original contributions of this dissertation are as follows: (i) to demonstrate that the evolutionary radiation of sigmodontines was driven mainly by historical and geographical factors instead of ecological factors; (ii) to suggest that evolutionary radiations on continental scales, especially rodent radiations, have a more determinant historical and geographical component than an ecological one; (iii) to show small variation in bite force between sigmodontine herbivores and granivores, which is likely a consequence of the generalist phenotype of these rodents; (iv) to highlight that insectivorous sigmodontines have a faster rate of morphological evolution than other diet groups, and that skull and mandible morphology and bite force are evolving in different directions than in other species; (v) to demonstrate that within a sigmodontine species (Akodon cursor), gene flow and genetic drift better explain variation in skull shape among populations, while environmental variation better explains variation in skull size, which suggests that size is more labile feature than shape and thus more prone to change with environmental pressures; and (vi) to show that biogeographical variation in mean body size, mean skull shape, and mean mandible shape across sigmodontine assemblages is influenced by the different distributions of phylogenetic lineages over geographical space, as well by environmental variables, which indicates phylogenetic niche conservatism at the metacommunity level. These results shed light on some of the factors driving morphological diversification in Sigmodontinae. Further, the analytical approach(es) utilized may be useful for general investigations of the relative contributions of adaptive and non-adaptive components of morphological evolution, thereby potentially increasing our knowledge of the origins of all biological diversity.

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This study focusses on modelling important aspects of the evolution of pulsar wind nebulae using two different approaches. The first uses a hydrodynamic model to simulate the morphological evolution of a spherically-symmetric composite supernova remnant that is expanding into a homogeneous interstellar medium. In order to extend this model, a magnetic field is included in a kinematic fashion, implying that the reaction of the fluid on the magnetic field is taken into account, while neglecting any counter-reaction of the field on the fluid. This approach is valid provided that the ratio of electromagnetic to particle energy in the nebula is small, or equivalently, for a large plasma β environment. This model therefore allows one to not only calculate the evolution of the convection velocity but also, for example, the evolution of the average magnetic field. The second part of this study focusses on calculating the evolution of the energy spectra of the particles in the nebula using a number of particle evolution models. The first of these is a spatially independent temporal evolution model, similar to the models that can be found in the literature. While spatially independent models are useful, a large part of this study is devoted to developing spatially dependent models based on the Fokker-Planck transport equation. Two such models are developed, the first being a spherically-symmetric model that includes the processes of convection, diffusion, adiabatic losses, as well as the non-thermal energy loss processes of synchrotron radiation and inverse Compton scattering. As the magnetic field geometry can lead to the additional transport process of drift, the previous model is extended to an axisymmetric geometry, thereby allowing one to also include this process. / PhD (Space Physics), North-West University, Potchefstroom Campus, 2014

This diploma thesis deals with an analysis of Old Czech poem Tristram and Izalda. The source of the analysed text is the Strahov manuscript dated to 1449, in edition by Zdeňka Tichá. The thesis includes a brief description of the history and origin of the analysed piece in both European and especially Czech literary context. The main focus of this text is the linguistic analysis of selected language phenomena. That comprises of phonological and morphological evolution of most grammar categories of nouns, adjectives and verbs in Czech language. With nouns and adjectives, the thesis focuses on the declination paradigm, specifically on the system of grammatical cases and the animacy of the masculine gender. With verbs, the attention is given to the analysis of the tenses, with emphasis on the simple past tenses. First and foremost, the thesis focuses on the analysis of the aorist and imperfect tense with emphasis on verbal aspect affiliation, from which these tenses are often created. A part of the work is dedicated to the preterite, the compound past tense. Where individual verbal forms are analysed, the main focus is given to the nt- and s- participles, their suffix system and also the connection to the category of verbal aspect. Many distinct examples from the analysed text are provided throughout the thesis, as well as detailed statistic data on the occurrence frequency of selected phenomena

This study focusses on modelling important aspects of the evolution of pulsar wind nebulae using two different approaches. The first uses a hydrodynamic model to simulate the morphological evolution of a spherically-symmetric composite supernova remnant that is expanding into a homogeneous interstellar medium. In order to extend this model, a magnetic field is included in a kinematic fashion, implying that the reaction of the fluid on the magnetic field is taken into account, while neglecting any counter-reaction of the field on the fluid. This approach is valid provided that the ratio of electromagnetic to particle energy in the nebula is small, or equivalently, for a large plasma β environment. This model therefore allows one to not only calculate the evolution of the convection velocity but also, for example, the evolution of the average magnetic field. The second part of this study focusses on calculating the evolution of the energy spectra of the particles in the nebula using a number of particle evolution models. The first of these is a spatially independent temporal evolution model, similar to the models that can be found in the literature. While spatially independent models are useful, a large part of this study is devoted to developing spatially dependent models based on the Fokker-Planck transport equation. Two such models are developed, the first being a spherically-symmetric model that includes the processes of convection, diffusion, adiabatic losses, as well as the non-thermal energy loss processes of synchrotron radiation and inverse Compton scattering. As the magnetic field geometry can lead to the additional transport process of drift, the previous model is extended to an axisymmetric geometry, thereby allowing one to also include this process. / PhD (Space Physics), North-West University, Potchefstroom Campus, 2014