When the Iron spirals investigated in this paper saw the light again no one looked at them as nothing more than decoration. It was first during the 2011 excavation in Old Uppsala that the symbolism of the items no longer could be ignored. The spirals of Old Uppsala lay along the walls of the great hall, which stood upon one of the human constructed plateaus in the area. The hall had been burned down and then cleared of all lumber. Then the iron spirals had been placed in the positions and then everything was sealed with a layer of clay. A study of the artifact began with the purpose to contextualize and interpret the iron spiral. Several others iron spirals were investigated and compared. The others comparing context were found in boat graves or boat contexts. With a new perspective on the spirals as active agents I soon realized the symbolic value of the artifact. The spiral contexts were clearly sym-bolic and connected with the belief about the Hall and Ship symbolism. Several evidences indicated that the hall in Old Uppsala was meant to look as a boat and the iron spirals helped the hall doing so as well as reinforce the symbolism of the ship. The hall and the ship stood for power and structure on land respectively on water. The spiral symbol itself may well be a symbol connected with law, power and structure. / Gamla Uppsala - framväxten av ett mytiskt centrum

This thesis is a reflection on both the conceptual frameworks and the personal narratives that have shaped the development of the Spirals Programme. The Programme is a participatory drama and creative arts based initiative established in 2000 in Grahamstown, South Africa, to explore issues of identity in the emerging democratic context of South African society - and support both personal and contextual processes of transformation. Working within a poststructuralist and social constructionist paradigm, Spirals works with groups and communities to facilitate and enable experiential links between the drama based and performative nature of identity construction - and the possibilities for transformation and healing provided by participative drama methodologies. The structure of the thesis follows the principles of the Freirian based Action Learning praxis within which Spirals works. It begins with an account of the contextual dynamics and events that gave rise to the development of the Programme, followed by a reflection on the conceptual frameworks regarding both identity construction and participative drama methodologies that informed Spirals' development. These paradigms are then analysed in relation to the articulated experiences of three workshop participants using critical discourse analysis. The thesis concludes with an assessment of the issues emerging from this analysis - the aspects of the Programme that need to be strengthened and sustained, those that need to be changed and possible new strategies that could be developed. / Also known as: Edlmann, Theresa

Dans cette thèse, nous étudions différentes structures de végétation issues de l’auto-organisation spatiale. Ce phénomène est visible dans des zones (semi-)arides où le potentiel d’évaporotranspiration dépasse sensiblement la moyenne des précipitations annuelles. Ce déficit hydrique freine le développement des plantes individuelles et, au niveau communautaire, stimule des comportements de « clustering » même si la topographie est isotrope. Dans ce contexte, nous adoptons une approche basée sur l’équation F-KPP non-locale permettant de formuler ces hypothèses en termes de propriétés des plantes individuelles.Une partie importante de cette thèse concerne l’étude d’un exemple de structure de végétation localisée bien connu dans la littérature, les cercles de fées. Les cercles de fées ont été découverts dans le désert de Namibie. Cependant, ces dernières années, ils ont aussi été observés en Australie. Plusieurs hypothèses ont été proposées dans la littérature. Nous proposons la compétition non-locale forte entre plantes individuelles (en utilisant un noyau de type Lorentzien) comme ingrédient principal pour expliquer la formation des cercles de fées. Le couplage non-local fort influence l’interaction entre fronts dans le régime bistable (loin de toute forme d’instabilité briseuse de symétrie). Dans le cas d’un couplage non-local faible, par exemple dans un noyau Gaussien, l’interaction entre fronts est toujours attractive. Par conséquent, les structures localisées qui résultent de l’interaction des fronts sont instables. Le couplage non-local fort peut induire la stabilisation de structures localisées que nous interprétons comme étant des cercles de fées. Notre mécanisme permet d’expliquer les principales caractéristiques des cercles de fées, comme la relation entre leur diamètre et la disponibilité des ressources. De plus, nous avons appliqué ces résultats à d’autres modèles de végétation. Nos résultats concordent avec les observations sur le terrain.Nous avons analysé la formation de « spots » de végétation dans la région Andine en Bolivie. Nous avons étudié comment un modèle standard d’interaction-redistribution génère des « spots », de longueur d’onde d'approximativement 1.36m, via une instabilité qui brise la symétrie. En considérant des paramètres réalistes, nos résultats concordent avec les observations sur le terrain.Enfin, nous avons étudié la formation de structure en forme de spirale dans un système qui couple la végétation et les herbivores dans un modèle proie-prédateur. Nous avons trouvé que le mécanisme qui induit la formation de spirales est l’excitabilité. Nos observations sur le terrain et nos résultats numériques du modèle montrent que les spirales de végétation ont une profondeur de quelques centimètres et une longueur de quelques mètres. En ce qui concerne l'échelle de temps, nos estimations donnent une période de rotation de l’ordre de 10 ans. / Option Physique du Doctorat en Sciences / info:eu-repo/semantics/nonPublished

A better understanding of several mineral processing devices and applications was gained through studies conducted with mathematical analysis tools. Linear circuit analysis and population balance modeling were utilized to remedy inefficiencies found in a number of popular mineral processing water-based unit operations. Improvements were made in areas, including unit capacity and separation efficiency. One process-engineering tool, known as linear circuit analysis, identified an alternative coal spiral circuit configuration that offered improved performance while maintaining a reasonable circulating load. In light of this finding, a full-scale test circuit was installed and evaluated at an existing coal preparation facility. Data obtained from the plant tests indicate that the new spiral circuit can simultaneously reduce cut-point and improve separation efficiency. A mathematical population balance model has also been developed which accurately simulates a novel hindered-bed separator. This device utilizes a tangential feed presentation system to improve the performance of conventional teeter-bed separators. Investigations utilizing the mathematical model were carried out and have predicted solid feed rates of up to 71 tph/m² (6 tph/ft²) can be achieved at acceptable efficiencies. The model also predicts that the unfavorable impact of operating at low feed percent solids is severely reduced by the innovative feed presentation design. Tracer studies have verified that this system allows excess feed water to cross over the top of the separator without entering the separation chamber, thereby reducing turbulence. A hindered-bed separator population balance model was also developed whose results were utilized to improve the efficiencies encountered when using a teeter-bed separator as a mineral concentrator. It was found that by altering the apparent density of one of the feed components, the efficiency of the gravity separation could be greatly improved. These results led to the development of a new separator which segregates particles based on differences in mass after the selective attachment of air bubbles to the hydrophobic component of the feed stream. Proof-of-concept and in-plant testing indicate that significant improvements in separation efficiency can be achieved using this air-assisted teeter-bed system. The in-plant test data suggest that in some cases, recoveries of the plus 35 mesh plant feed material can be increased by more than 40% through the application of this new technology. / Ph. D.

Dans la première partie de la thèse, nous présentons un nouveau système permettant de produire des mouvements de caméra réalistes pour l’animation stopmotion. Le système permettra d’enrichir les logiciels d’animation 3D classiques (comme par exemple Maya et 3D Studio Max) afin de leur faire contrôler des mouvements de caméra pour la stop motion, grâce à l’utilisation d’une interface haptique. Nous décrivons le fonctionnement global du système. La première étapeconsiste à récupérer et enregistrer les données envoyées par le périphérique haptique de motion capture. Dans la seconde étape, nous réélaborons ces données par un procédé mathématique, puis les exportons vers un logiciel de 3D pour prévisualiser les mouvements de la caméra. Finalement la séquence est exécutée avec un robot de contrôle de mouvement et un appareil photo. Le système est évalué par un groupe d’étudiants du Master "Art plastiques et Création numérique" de l’Université de Valenciennes. Dans la deuxième partie, nous définissons une nouvelle classe de courbes à partir des courbes polynomiales paramétriques à hodographe pythagorien (PH) construite sur un espace algébrique-trigonométrique. Nous montrons leurs propriétés fondamentaleset leurs avantages importants par rapport à leur équivalent polynomial, grâce à l’utilisation d’un paramètre de forme. Nous introduisons une formulation complexe et nous résolvons le problème d’interpolation de Hermite. / In the first part, we present a new system that allows to create realistic cameramovements for a stop motion animation. The system improves traditional 3D software animation programs (for example Maya and 3D Studio Max) for creatingstop motion camera movements by using an haptic interface. After describing thewhole system, we explain in detail the mathematical processing to obtain differentcamera movements by using an haptic interface for motion capture. The recordedhaptic positions, once elaborated, are exported, frame by frame, to the motioncontrol software, which allows to calibrate the motion control robot, to control thecamera settings and, finally, to execute the sequences. A class of students of the"Art plastiques et Création numérique" Master of the University of Valenciennesevaluated the system. In the second part, we define a new class of Pythagorean Hodograph curves built upon a five dimensional mixed algebraic trigonometric space, and show their fundamental properties and important advantages over their well known polynomial counterpart. A complex representation for these curves is introduced and constructive approaches are provided to solve the first order Hermite interpolation problem.

In this thesis, non-collinear magnetism has been studied by using density functional theory and the augmented plane wave method with local orbitals (APW+lo). Two conditions for non-collinear instabilities have been identified in this thesis. First, the Fermi energy should cut through both spin up and down states. Secondly, strong nesting between the spin up and spin down Fermi surfaces is needed. The two criteria described here can be fulfilled by tuning the exchange-splitting and/or by modifying the volume. Calculations on several elements; bcc V, bcc and fcc Mn, bcc Fe, bcc and fcc Co, and bcc and fcc Ni show that a non-collinear state can be stabilized provided that the criteria discussed above are met. More complex materials have also been analyzed in terms of these two criteria. The substitutional alloys TlCo2Se2-xSx are found in experiments to possess spin spiral structures for x = {0-1.5} and at a concentration x = 1.75 the alloys become ferromagnetic. As S takes the place of Se in the crystal structure the distance between the Co layers is reduced and the turn angle of the spin spiral becomes smaller until it totally vanishes at x = 1.75. This thesis show that the evolution of the magnetic structure in these alloys is the consequence of a modification of the distance between Co layers, which induces a change in the interlayer exchange coupling. Fermi surfaces have been analyzed in TbNi5 in order to determine nesting features which would be responsible for the magnetic spin spiral observed in this material. The electronic structure of CeRhIn5 is also reported in this thesis. Furthermore, the 3-k magnetic structure of UO2 was investigated and the crystal field levels were calculated. Transition metal systems such as Fe in the superconducting high-pressure hcp phase and in the fcc crystal structure were also studied. The results obtained for fcc Fe are in accordance with previous reports. However the paramagnetic state in hcp Fe is found to be more stable than the antiferromagnetic configurations discussed earlier in the literature as being favored in the volume range where the hcp phase is stable and superconductivity appears (~ 15 GPa). The complex non-collinear magnetic structure in Mn3IrSi was calculated and the results are found to be in good agreement with experiments.

The aim of this study is to gather insights into market efficiency and mechanisms that work in the financial markets. It provides a framework with an emphasis on liquidity and the failure of arbitrage that deepens our understanding of various financial crises. Described mechanisms are particularly relevant for the last financial crises - including 2007-2009, LTCM, and dot-com bubble. In the first chapter the concept of efficient markets is introduced. In the second chapter it is challenged from the point of view of noise trader theory and limits of arbitrage. The third chapter deals with market microstructure and liquidity. Last chapter shows importance and adverse effects of externalities, particularly of those causing liquidity spirals.

We present a detailed study of mid-infrared spectroscopy and optical imaging of Seyfert galaxies with the goal of understanding the properties of astronomical dust around the central supermassive black hole and the accretion disk. Specifically, we have studied Spitzer Space Telescope mid-infrared spectra of 12 Seyfert 1.8-1.9s and 58 Seyfert 1s and 2s available in the Spitzer public archive, and the nuclear dust morphology in the central 500 pc of 91 narrow and broad-line Seyfert 1s using optical images from the Hubble Space Telescope. We have also developed visualization software to aid the understanding of the geometry of the central engine. Based on these studies, we conclude that the nuclear regions of Seyfert galaxies are fueled by dusty spirals driven by the large-scale stellar bars in the host galaxy. The accumulation of dusty gas in the central kiloparsec leads to enhanced star formation. In this case, the circumnuclear starburst and the central engine compete for dominance in the heating of the circumnuclear dust. Emission from the heated dust is most clearly seen in the mid-infrared. We find that the spectra of Seyfert 2s show the most variety in the continuum shapes due to different starburst contributions. We find that the spectra of Seyfert 2s that are devoid of starburst contribution are dominated by a single thermal component at a temperature of T ~ 170 K. We also find that the mid-IR continua of Seyfert 1.8/1.9 galaxies are more like those of starburst-dominated Seyfert 2s than Seyfert 1s, contrary to expectations. We discuss the implications of these findings in the context of the Unified Model of AGN and the secular evolution of Seyfert nuclei.

This thesis examines the stone-carved architectural spiral fluted column from second-millennium B.C. Mesopotamia to the fourth-century A.D. Roman Empire, and establishes its relationship to technological devices such as water screws, screw presses, and other machines. Evidence from literary sources and archaeological records shows the increasing architectural use of the helical spiral during that time, particularly in structures such as theatres, nymphaea, colonnades and decorative gateways. The use of spiral designs on coins, sarcophagi, pottery and wall paintings is also discussed. The thesis presents: the mathematics of the spiral as applied in Mesopotamian architecture; spiral use in the Aegean Bronze and Iron Ages and the Greek and Roman worlds; and its use in technology and mechanical devices, specifically those of Archimedes and Hero. The conclusion summarises the evidence, demonstrating that the construction of the spiral fluted column evolved from that of the Archimedean water screw. / Graduate / 2015-08-20 / 0324 / 0346 / 0579 / ghenders@uvic.ca

In this thesis, I study numerical and semi-analytical models of self-gravitating protostellar discs, with the aim of furthering our understanding of the role of disc-self gravity in planet formation. At the time of writing, the ALMA era of observational astronomy is upon us. Therefore, I place my research into this context with synthetic images of both numerical and semi-analytical models. I begin with an examination into the apparent lack of convergence, with increasing resolution, of the fragmentation boundary in Smoothed Particle Hydrodynamics (SPH) simulations of a protostellar disc. I run a suite of SPH with different numerical implementations, and find that even very similar implementations can fundamentally change the final answer. I analyse a suite of SPH simulations that fragment to form gravitationally bound objects, with the motivation of informing future population synthesis model development. I find that fragment-fragment and fragment-disc interaction dominates the orbital evolution of the system even at very early times, and any attempt to produce a population of objects from the gravitational instability process must include these interactions. Before a disc fragments, it will go through a self-gravitating phase. If the disc cools globally on a timescale such that it is balanced by heating due to gravitational stresses, the disc will be in a state of quasi-equilibrium. So long as the disc mass is sufficiently low, and spirals are sufficiently tightly wound, then angular momentum transport can be described by the local approximation, for which there is an analytical description. Using this analytical description, I develop an existing 1D model into 3D, and examine a wide range of parameter space for which disc self-gravity produces significant non-axisymmetry. Using radiative transfer calculations coupled with synthetic observations, I determine that there is a very narrow range of parameter space in which a disc will have sufficiently large gravitational stresses so as to produce detectable spirals, but the stresses not be so large as to cause the disc to fragment. By developing a simple analytical prescription for dust, I show that this region of parameter space can be broadened considerably. However, it requires grains that are large enough to become trapped by pressure maxima in the disc, so I conclude that if self-gravitating spiral arms are detected in the continuum, it is likely that at least some grain growth has taken place.