959 resultados para teleparallel gravity


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Tungsten carbide used in snowplow blades was studied from three manufacturers. The carbides were measured for common industry properties including specific gravity and hardness. In addition, an abrasion resistance was performed. There was no significant difference found in abrasion resistance between the Kenametal and the Valk carbides. The Bucyrus carbides showed improved abrasion resistance, but were outside industry specifications for specific gravity.

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In this study, the asphalt absorption of six Iowa limestones were investigated. It was found that the most important factors that determined the nature, amount, and rate of asphalt absorption are porosity and pore-size distribution of the aggregate, viscosity of the asphalt, and time. Methods needed to determine the realistic maximum and minimum asphalt absorption by aggregates are recommended. Simple methods of asphalt absorption were developed. Since the most important factor that determines the accuracy of asphalt absorption is the bulk specific gravity of aggregates and since the current ASTM method is not adequate in this respect, several new methods were developed. Preliminary treatment studies for the purpose of upgrading absorptive aggregates were conducted using close to 40 chemicals. The improvements of some of these treatments on the mixture properties were demonstrated.

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Résumé La réalisation d'une seconde ligne de métro (M2) dès 2004, passant dans le centre ville de Lausanne, a été l'opportunité de développer une méthodologie concernant des campagnes microgravimétriques dans un environnement urbain perturbé. Les corrections topographiques prennent une dimension particulière dans un tel milieu, car de nombreux objets non géologiques d'origine anthropogénique comme toutes sortes de sous-sols vides viennent perturber les mesures gravimétriques. Les études de génie civil d'avant projet de ce métro nous ont fournis une quantité importante d'informations cadastrales, notamment sur les contours des bâtiments, sur la position prévue du tube du M2, sur des profondeurs de sous-sol au voisinage du tube, mais aussi sur la géologie rencontré le long du corridor du M2 (issue des données lithologiques de forages géotechniques). La planimétrie des sous-sols a été traitée à l'aide des contours des bâtiments dans un SIG (Système d'Information Géographique), alors qu'une enquête de voisinage fut nécessaire pour mesurer la hauteur des sous-sols. Il a été alors possible, à partir d'un MNT (Modèle Numérique de Terrain) existant sur une grille au mètre, de mettre à jour celui ci avec les vides que représentent ces sous-sols. Les cycles de mesures gravimétriques ont été traités dans des bases de données Ac¬cess, pour permettre un plus grand contrôle des données, une plus grande rapidité de traitement, et une correction de relief rétroactive plus facile, notamment lorsque des mises à jour de la topographie ont lieu durant les travaux. Le quartier Caroline (entre le pont Bessières et la place de l'Ours) a été choisi comme zone d'étude. Le choix s'est porté sur ce quartier du fait que, durant ce travail de thèse, nous avions chronologiquement les phases pré et post creusement du tunnel du M2. Cela nous a permis d'effectuer deux campagnes gravimétriques (avant le creu¬sement durant l'été 2005 et après le creusement durant l'été 2007). Ces réitérations nous ont permis de tester notre modélisation du tunnel. En effet, en comparant les mesures des deux campagnes et la réponse gravifique du modèle du tube discrétisé en prismes rectangulaires, nous avons pu valider notre méthode de modélisation. La modélisation que nous avons développée nous permet de construire avec détail la forme de l'objet considéré avec la possibilité de recouper plusieurs fois des interfaces de terrains géologiques et la surface topographique. Ce type de modélisation peut s'appliquer à toutes constructions anthropogéniques de formes linéaires. Abstract The realization of a second underground (M2) in 2004, in downtown Lausanne, was the opportunity to develop a methodology of microgravity in urban environment. Terrain corrections take on special meaning in such environment. Many non-geologic anthropogenic objects like basements act as perturbation of gravity measurements. Civil engineering provided a large amount of cadastral informations, including out¬lines of buildings, M2 tube position, depths of some basements in the vicinity of the M2 corridor, and also on the geology encountered along the M2 corridor (from the lithological data from boreholes). Geometry of basements was deduced from building outlines in a GIS (Geographic Information System). Field investigation was carried out to measure or estimate heights of basements. A DEM (Digital Elevation Model) of the city of Lausanne is updated from voids of basements. Gravity cycles have been processed in Access database, to enable greater control of data, enhance speed processing, and retroactive terrain correction easier, when update of topographic surface are available. Caroline area (between the bridge Saint-Martin and Place de l'Ours) was chosen as the study area. This area was in particular interest because it was before and after digging in this thesis. This allowed us to conduct two gravity surveys (before excavation during summer 2005 and after excavation during summer 2007). These re-occupations enable us to test our modélisation of the tube. Actually, by comparing the difference of measurements between the both surveys and the gravity response of our model (by rectangular prisms), we were able to validate our modeling. The modeling method we developed allows us to construct detailed shape of an object with possibility to cross land geological interfaces and surface topography. This type of modélisation can be applied to all anthropogenic structures.

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Recently a fingering morphology, resembling the hydrodynamic Saffman-Taylor instability, was identified in the quasi-two-dimensional electrodeposition of copper. We present here measurements of the dispersion relation of the growing front. The instability is accompanied by gravity-driven convection rolls at the electrodes, which are examined using particle image velocimetry. While at the anode the theory presented by Chazalviel et al. [J. Electroanal. Chem. 407, 61 (1996)] describes the convection roll, the flow field at the cathode is more complicated because of the growing deposit. In particular, the analysis of the orientation of the velocity vectors reveals some lag of the development of the convection roll compared to the finger envelope.

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The flow of two immiscible fluids through a porous medium depends on the complex interplay between gravity, capillarity, and viscous forces. The interaction between these forces and the geometry of the medium gives rise to a variety of complex flow regimes that are difficult to describe using continuum models. Although a number of pore-scale models have been employed, a careful investigation of the macroscopic effects of pore-scale processes requires methods based on conservation principles in order to reduce the number of modeling assumptions. In this work we perform direct numerical simulations of drainage by solving Navier-Stokes equations in the pore space and employing the Volume Of Fluid (VOF) method to track the evolution of the fluid-fluid interface. After demonstrating that the method is able to deal with large viscosity contrasts and model the transition from stable flow to viscous fingering, we focus on the macroscopic capillary pressure and we compare different definitions of this quantity under quasi-static and dynamic conditions. We show that the difference between the intrinsic phase-average pressures, which is commonly used as definition of Darcy-scale capillary pressure, is subject to several limitations and it is not accurate in presence of viscous effects or trapping. In contrast, a definition based on the variation of the total surface energy provides an accurate estimate of the macroscopic capillary pressure. This definition, which links the capillary pressure to its physical origin, allows a better separation of viscous effects and does not depend on the presence of trapped fluid clusters.

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OBJECTIVES: To assess the performance of 45F vs. 36F smartcanula in CPB with gravity drainage alone. METHODS: Twenty patients were randomly assigned to two groups receiving for venous drainage a smartcanula which is collapsed over a mandrel for trans-atrial insertion into the inferior vena cava and expanded in situ to either 45F or 36F. RESULTS: Valve replacement/repair was realized in 7/10 and/or CABG in 6/10 for 36F (69+/-13 years) vs. 5/10 and 5/10, respectively, for 45F (63+/-11 years: NS). Body weight and surface area (BSA) were 83+/-9 kg (1.9+/-0.2 m2, max 2.2 m2) for 36F vs. 79+/-6 kg: NS (1.9+/-0.1 m2 (NS), max 2.1 m2) for 45F. Insertion and access orifice diameter (area) was 6 mm and 10 mm (78.5 mm2) for the 36F vs. 6 mm and 13 mm (132 mm2) for the 45F (+69%). Calculated target pump flow (2.4 l/min/m2) was 4.7+/-0.4 l/min for 36F vs. 4.5+/-0.3 l/min for 45F. Achieved pump flow accounted for 5.0+/-0.3 l/min for 36F (8% above target) vs. 4.8+/-0.3 l/min for 45F (8% above target): NS. The water balance during the pump run (clear volume added minus hemofilter and urine output) was 2.2+/-0.3 l for 36F vs. 2.0 l for 45F: NS. CONCLUSION: Due to its 'open' wall (the vena cava provides the seal), its reduced wall thickness (range: 0.0-0.4 mm), and its self-expanding design, the 36F smartcanula requiring a 30F access orifice has sufficient drainage capacity by gravity alone for full CPB in adults with a BSA up to 2.2 mm2.

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Using the blackfold approach, we study new classes of higher-dimensional rotating black holes with electric charges and string dipoles, in theories of gravity coupled to a 2-form or 3-form field strength and to a dilaton with arbitrary coupling. The method allows to describe not only black holes with large angular momenta, but also other regimes that include charged black holes near extremality with slow rotation. We construct explicit examples of electric rotating black holes of dilatonic and non-dilatonic Einstein-Maxwell theory, with horizons of spherical and non-spherical topology. We also find new families of solutions with string dipoles, including a new class of prolate black rings. Whenever there are exact solutions that we can compare to, their properties in the appropriate regime are reproduced precisely by our solutions. The analysis of blackfolds with string charges requires the formulation of the dynamics of anisotropic fluids with conserved string-number currents, which is new, and is carried out in detail for perfect fluids. Finally, our results indicate new instabilities of near-extremal, slowly rotating charged black holes, and motivate conjectures about topological constraints on dipole hair.

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We consider the linearized semiclassical Einstein equations for small deviations around de Sitter spacetime including the vacuum polarization effects of conformal fields. Employing the method of order reduction, we find the exact solutions for general metric perturbations (of scalar, vector and tensor type). Our exact (nonperturbative) solutions show clearly that in this case de Sitter is stable with respect to small metric deviations and a late-time attractor. Furthermore, they also reveal a breakdown of perturbative solutions for a sufficiently long evolution inside the horizon. Our results are valid for any conformal theory, even self-interacting ones with arbitrarily strong coupling.

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Understanding the emplacement and growth of intrusive bodies in terms of mechanism, duration, ther¬mal evolution and rates are fundamental aspects of crustal evolution. Recent studies show that many plutons grow in several Ma by in situ accretion of discrete magma pulses, which constitute small-scale magmatic reservoirs. The residence time of magmas, and hence their capacities to interact and differentiate, are con¬trolled by the local thermal environment. The latter is highly dependant on 1) the emplacement depth, 2) the magmas and country rock composition, 3) the country rock thermal conductivity, 4) the rate of magma injection and 5) the geometry of the intrusion. In shallow level plutons, where magmas solidify quickly, evi¬dence for magma mixing and/or differentiation processes is considered by many authors to be inherited from deeper levels. This work shows however that in-situ differentiation and magma interactions occurred within basaltic and felsic sills at shallow depth (0.3 GPa) in the St-Jean-du-Doigt (SJDD) bimodal intrusion, France. This intrusion emplaced ca. 347 Ma ago (IDTIMS U/Pb on zircon) in the Precambrian crust of the Armori- can massif and preserves remarkable sill-like emplacement processes of bimodal mafic-felsic magmas. Field evidence coupled to high precision zircon U-Pb dating document progressive thermal maturation within the incrementally built ioppolith. Early m-thick mafic sills (eastern part) form the roof of the intrusion and are homogeneous and fine-grained with planar contacts with neighboring felsic sills; within a minimal 0.8 Ma time span, the system gets warmer (western part). Sills are emplaced by under-accretion under the old east¬ern part, interact and mingle. A striking feature of this younger, warmer part is in-situ differentiation of the mafic sills in the top 40 cm of the layer, which suggests liquids survival in the shallow crust. Rheological and thermal models were performed in order to determine the parameters required to allow this observed in- situ differentiation-accumulation processes. Strong constraints such as total emplacement durations (ca. 0.8 Ma, TIMS date) and pluton thickness (1.5 Km, gravity model) allow a quantitative estimation of the various parameters required (injection rates, incubation time,...). The results show that in-situ differentiation may be achieved in less than 10 years at such shallow depth, provided that: (1) The differentiating sills are injected beneath consolidated, yet still warm basalt sills, which act as low conductive insulating screens (eastern part formation in the SJDD intrusion). The latter are emplaced in a very short time (800 years) at high injection rate (0.5 m/y) in order to create a "hot zone" in the shallow crust (incubation time). This implies that nearly 1/3 of the pluton (400m) is emplaced by a subsequent and sustained magmatic activity occurring on a short time scale at the very beginning of the system. (2) Once incubation time is achieved, the calculations show that a small hot zone is created at the base of the sill pile, where new injections stay above their solidus T°C and may interact and differentiate. Extraction of differentiated residual liquids might eventually take place and mix with newly injected magma as documented in active syn-emplacement shear-zones within the "warm" part of the pluton. (3) Finally, the model show that in order to maintain a permanent hot zone at shallow level, injection rate must be of 0.03 m/y with injection of 5m thick basaltic sills eveiy 130yr, imply¬ing formation of a 15 km thick pluton. As this thickness is in contradiction with the one calculated for SJDD (1.5 Km) and exceed much the average thickness observed for many shallow level plutons, I infer that there is no permanent hot zone (or magma chambers) at such shallow level. I rather propose formation of small, ephemeral (10-15yr) reservoirs, which represent only small portions of the final size of the pluton. Thermal calculations show that, in the case of SJDD, 5m thick basaltic sills emplaced every 1500 y, allow formation of such ephemeral reservoirs. The latter are formed by several sills, which are in a mushy state and may interact and differentiate during a short time.The mineralogical, chemical and isotopic data presented in this study suggest a signature intermediate be¬tween E-MORB- and arc-like for the SJDD mafic sills and feeder dykes. The mantle source involved produced hydrated magmas and may be astenosphere modified by "arc-type" components, probably related to a sub¬ducting slab. Combined fluid mobile/immobile trace elements and Sr-Nd isotopes suggest that such subduc¬tion components are mainly fluids derived from altered oceanic crust with minor effect from the subducted sediments. Close match between the SJDD compositions and BABB may point to a continental back-arc setting with little crustal contamination. If so, the SjDD intrusion is a major witness of an extensional tectonic regime during the Early-Carboniferous, linked to the subduction of the Rheno-Hercynian Ocean beneath the Variscan terranes. Also of interest is the unusual association of cogenetic (same isotopic compositions) K-feldspar A- type granite and albite-granite. A-type granites may form by magma mixing between the mafic magma and crustal melts. Alternatively, they might derive from the melting of a biotite-bearing quartz-feldspathic crustal protolith triggered by early mafic injections at low crustal levels. Albite-granite may form by plagioclase cu¬mulate remelting issued from A-type magma differentiation.

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Usefulness of a predictive score in subarachnoid hemorrhage diagnosis Nearly half of the patients with non-traumatic subarachnoid hemorrhage (SAH) present with no neurological signs, inducing clinical underestimation of the gravity of their affection. As the outcome of aneurismal SAH is highly dependant on the initial neurological status and the recurrence of untreated hemorrhagic events, these neurologically intact patients stand to suffer the most from delayed diagnosis. Although there is currently no validated predictive score that reliably identifies SAH-induced headache, a combination of clinical criteria derived from a cohort of sudden-onset headache patients should allow risk stratification and identification of those patients requiring further investigation.

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Abstract:The objective of this work was to evaluate the effect of limestone particle sizes in the diet and of lighting regimes on the egg and bone quality and on the performance of commercial laying hens. Three hundred Hissex White layers, at 18 weeks of age, were distributed in a completely randomized design, in a 5×2 factorial arrangement (coarse limestone in the diet at 0, 25, 50, 75, and 100%; with or without artificial light), with five replicates of six birds. No significant interaction was observed between particle sizes and lighting regime for the evaluated parameters. There was no significant effect of coarse limestone level in the diet on the performance and egg quality of hens; however, bone deformity (3.23 to 4.01 mm), strength (5.19 to 6.70 kgf cm-2), and mineral matter (51.09 to 59.61%) improved as the proportion of coarse limestone increased. For lighting regime, the treatment with artificial light yielded higher Haugh unit values (87.17 vs. 85.54) than that with natural light only. Greater limestone particles improve bone quality of laying hens, and the use of artificial light can benefit the albumen quality of the eggs.

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Background: To evaluate the long-term efficacy of multilayer amniotic membrane transplantation for reconstruction of epithelium and stroma in non-traumatic corneal perforations (less than 2 mm) or deep ulcers with descemetocele.Design: Retrospective, non-comparative, interventional case series.Patients and Methods: Eleven consecutive patients with non-traumatic corneal perforations or deep corneal ulcers with descemetocele refractory to conventional treatments: herpetic or zoster keratitis (n = 4), Sjögren's syndrome (n = 2), rosacea (n = 1), hydrops (n = 1), mucous membrane pemphigoid (n = 1), bacterial keratitis (n = 1) and perforation after protontherapy for melanoma (n = 1). Intervention was: multilayer amniotic membrane transplantation with cryopreserved amniotic membrane. Complication rate and clinical outcome were evaluated in this long-term follow-up.Results: Mean follow-up was 32 months (12 to 60). Integration of the multilayer amniotic membrane was obtained in 10 cases after one year. Corneal epithelium healed above the membrane in 10 cases within 3 weeks and remained stable after 32 months in 9 cases. Thickness of the stroma was increased and remained stable during the follow-up in 9 cases. In one case herpetic keratitis recurred with a corneal perforation. The clearing of the amniotic membrane was gradually obtained over a period of 11 months. Complications occurred in 15 % of the eyes during the long-term follow-up.Conclusion: Multilayer amniotic membrane transplantation is a safe and efficient technique for a long restoration of the corneal integrity after non-traumatic corneal perforations or deep corneal ulcers with descemetocele. Long-term prognosis of these eyes depends of the gravity of the initial disease.

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Résumé : Les corps magmatiques sont des indicateurs essentiels dans toute reconstitution paléogéographique et/ou géodynamique d'un cycle orogénique, en particulier en contexte polycyclique, où la plupart des autres indices ont été oblitérés. Ils sont aisément datables et leurs caractéristiques géochimiques permettent de contraindre leur contexte tectonique de mise en place. Cette approche a été appliquée aux socles pré-mésozoïques des nappes penniques inférieures de Sambuco et de la Maggia, dans les Alpes centrales lepontines. Plusieurs événements magmatiques ont été identifiés dans le socle de Sambuco et datés par la méthode U-Pb sur zircon couplée à la technique LA-ICPMS. La suite calco-alcaline mafique rubanée de Scheggia est datée du Cambrien inférieur à 540-530 Ma ; le métagranite alumineux oeillé de Sasso Nero a un âge de 480-470 Ma, tout comme bien d'autres «older orthogneisses» des socles alpins. Il contient des zircons hérités d'âge panafricain à 630-610 Ma, indicateur d'une affiliation gondwanienne de ces terrains. Le pluton calco-alcalin du Matorello est daté à environ 300-310 Ma, et les filons lamprophyriques qu'il abrite à 300 Ma. La granodiorite de Cocco et le leucogranite de Ruscada, tous deux intrudés dans le socle de la nappe adjacente de la Maggia, ont des âges similaires à celui du Matorello. Ceci ajouté aux similitudes magmatiques observées entre Cocco et Matorello suggère une proximité paléogéographique des deux nappes au Permien-Carbonifère. Or ces dernières sont actuellement considérées appartenir à deux domaines paléogéographiques mésozoïques distincts : helvétique pour Sambuco et briançonnais pour Maggia, séparés par un bassin océanique. Si tel fut le cas, aucun mouvement décrochant ne doit avoir décalé les marges continentales de l'océan, retrouvées en parfaite coïncidence lors de sa fermeture. Le Matorello est un pluton recristallisé en faciès amphibolite et plissé par cinq phases successives de déformation non-coaxiales, qui ont conduit à son renversement complet, attesté par des indicateurs de paléogravité. Il préserve de spectaculaires phénomènes de coexistence liquide de magmas (essaims d'enclaves et Bills composites). Ce pluton était originellement tabulaire, construit par l'accumulation de multiples injections de magma en feuillets d'épaisseur métrique à décamétrique. Suivant le rythme de mise en place, les injections successives ont rapidement cristallisé avec des contours nets et bien définis (Bills composites) ou se sont mélangées avec les précédentes pour former une couche non consolidée de plusieurs dizaines de mètres d'épaisseur (granodiorite principale). Les injections individuelles sont délimitées par de subtils contrastes en granulométrie, proportions modales ou ségrégation de minéraux (schlieren), ou par des phénomènes d'érosion le long des surfaces de contact. Deux couches métriques à contour sinueux consistent en une accumulation compacte d'enclaves mafiques arrondies dans une matrice granodioritique fine. Le granoclassement des enclaves, la présence de figures de charge et de phénomènes érosifs en base de couche, ainsi que des schlieren de biotite entrecroisés évoquent l'injection de coulées de magma chargé d'enclaves et de faible viscosité en régime hydrodynamique turbulent dans un encaissant granodioritique encore largement liquide. La nature hybride des roches implique une chambre magmatique sous-jacente, en cours de différenciation et périodiquement réalimentée. Les magmas sont des liquides mafiques dérivés du manteau et des liquides anatectiques d'origine crustale, comme l'indique la gamme mesurée des rapports isotopiques initiaux du Sr (0.704 à 0.709) et des valeurs epsilon Nd (-2.1 à -4.7). Ces données montrent également que la contribution crustale est dominante, en accord avec les isotopes du plomb. Les phénomènes d'hybridation ont vraisemblablement eu lieu en base de croûte et dans la chambre magmatique sous-jacente au laccolite du Matorello. Les indicateurs de paléogravité du Matorello contribuent accessoirement à la compréhension de l'architecture actuelle de la nappe de Sambuco. Des plis isoclinaux à surface axiale verticale peuvent être mis en évidence par le contact entre les faciès dioritique et granodioritique. L'antiforme dont le Matorello forme le coeur est un synclinal, ce qui le positionne dans le Flanc inverse du grand pli couché que forme la nappe de Sambuco. Par ailleurs, des blocs de gneiss retrouvés dans le wildflysch sommital de la couverture de la nappe d'Antigorio ont été affiliés dans cette étude au pluton du Matorello. Ceci implique que le front de la nappe de Sambuco chevauchait déjà la partie est du bassin d'Antigorio au moment de sa fermeture. Par conséquent, ce n'est qu'en position externe que la nappe du Lebendun chevauche directement la nappe d'Antigorio. Abstract Magmatic bodies are important markers in paleo-geographic or geodynamic reconstructions of orogenic cycles, even more so in the case of polycyclic events where many of the other markers have been overwritten or destroyed. Plutons are relatively easy to date and their geochemical properties help constrain the tectonic context in which they were emplaced. This study focuses on the pre-mesozoic basement in the Sambuco and Maggia lower Penninic nappes located in the central Lepontine domain of the Alps. A number of magmatic events have been identified in the Sambuco basement. These events were dated using LA-ICPMS U/Pb on zircon grains. The mafic calc-alkaline banded Scheggia suite is dated as lower Cambrian, 540-530 Ma. The Al-rich Sasso-Nero lenticular gneiss is 480-470 Ma old (similarly to many older orfhogneisses of the Alpine basement) and contains 630-610 Ma old pan-African inherited zircons that illustrate the Gondwanian origin of these terranes.The calc-alkaline Matorello pluton is dated as 310-300 Ma whereas the lamprophyric bodies it contains are of 300 Ma. The Cocco granodiorite and the Ruscada leucogranite both intrude the basement of the adjacent Maggia nappe and are of similar ages to the Matorello. The ages as well as the geochemical similarities between the Cocco, Rucada and Matorello plutons suggest their paleo-geographic proximity at the Permian-Carboniferous boundary. However, these nappes are currently considered as belonging to two different Mesozoic paleo-geographic domains. Indeed, the Sambuco is considered as Helvetic whereas the Maggia is said to be Briançonnais, both separated by an oceanic basin. If this is the case, then it is essential that nostrike-slip movement has misaligned both continental margins since these coincide perfectly now that the oceanic domain closed. The Matorello pluton was originally a tabular intrusion, built up by the accumulation of multiple, several meter-thick, subhorizontal sheet-like injections of magma. Depending on their emplacement rate, the successive magma injections either solidified rapidly with sharp and rather well-defined boundaries (like the composite sills) or mingled with previous injections generating a thick molten layer up to several tens to hundred meters thick, like in the main granodioritic facies. These coalesced injections are hardly distinguishable, however subtle contrasts in granulometry, mineral modal proportions or mineral sorting (cross-bedded biotite-rich schlieren), as well as erosional features and/or crystal entrapment along contact surfaces allow to distinguish between the different injections. Two exceptional meter-thick layers display sinuous boundaries with the host granodiorite and consist of a densely packed accumulation of mafic enclaves in a granodioritic matrix. Gravitational sorting of the enclaves with load cast features at the base of the layers and sinuous biotite schlieren point to injection of low viscosity turbulent composite magma flows in the still largely molten granodiorite host. The hybrid nature of these rocks implies the existence of á periodically replenished and differentiated underlying magma chamber. Magmas are mafic liquids derived from the mantle and anatectic liquids of crustal origin, as shown by the (87Sr/86Sr), and epsilon Nd values (0.704-0.709 and -2.1 to -4.7 respectively. These data show that the crustal contribution is important, as confirmed by the Pb isotopes. The hybridisation processes seem to have occurred in the lower crust in magma chambers underlying the Matorello laccolith. The paleo-gravity markers in the Matorello help understand the architecture of the Sambuco nappe. Isoclinal folds with a vertical axial plane can be seen at the contact between dioritic and granodioritic facies. The antiform structure of which the Matorello is the heart is in fact a syncline. This places it in the inverse flanc of the large recumbent fold that constitutes the Sambuco nappe. The gneiss blocs found in the summital wildflysh cover of the Antigorio nappe have been linked to the Matorello pluton. This means that the front of the Sambuco nappe already overlapped the Antigorio basin when it closed. This implies that the Lebendun nappe can only overlap the Antigorio nappe in it's external position. Résumé grand public La chaîne alpine est la conséquence de la collision tertiaire entre deux masses continentales, l'Europe au nord et la péninsule apulienne africaine au sud, originellement séparées par l'océan mésozoïque téthysien. Cette collision a fermé un espace large de plusieurs centaines de km avec pour résultat l'écaillage de la croûte terrestre en unités tectoniques de dimensions variables, qui se sont empilées, imbriquées, éventuellement replissées en nappes de géométrie complexe. Cet amoncellement de 40 km d'épaisseur a vu sa température et sa pression lithostatique internes augmenter jusqu'à des valeurs de l'ordre de 680 °C et 6000 bars, induisant une recristallisation métamorphique des roches. L'un des objectifs de la géologie alpine est de reconstituer la géographie de la région aux temps mésozoïques de l'océan téthysien, en d'autres termes, de replacer chacune des unités tectoniques identifiées au sein de l'empilement alpin dans sa position originelle. Le défi est de taille et peut être comparé à celui de la reconstitution d'un vaste puzzle, dont certaines pièces seraient endommagées au niveau de leur contour ou leurs couleurs (métamorphisme), dissimulées par d'autres (enfouissement), voire tombées de la table de jeu (subduction, échappement latéral). Plusieurs approches ont été mises en oeuvre au cours du siècle écoulé. On citera en particulier la stratigraphie, la tectonique et le paléomagnétisme. Dans ce travail, nous avons essentiellement utilisé des techniques de datation isotopique absolue des roches (U/Pb sur zircon) qui, sur la base des connaissances acquises par l'ensemble des autres disciplines géologiques, nous ont permis de mieux contraindre ta paléogéographie mésozoïque du domaine «pennique inférieur » des Alpes centrales lépontines. Et au-delà? Nous savons tous que la disposition des continents à la surface de la Terre évolue constamment. Il est donc tentant d'essayer de remonter plus loin encore dans le temps et de reconstituer la physionomie de la marge sud européenne, tout au moins certains éléments de son histoire, au cours de l'ère paléozoïque. Les traces de ces événements très anciens sont naturellement ténues et dans ce contexte, les techniques de datation mentionnées ci-dessus deviennent les outils les plus performants. Ainsi, des datations u/Pb sur zircon nous ont permis de recenser plusieurs intrusions magmatiques, attribuées à quatre événements orogéniques anté-alpins. Des âges néoprotérozoïques (630-610 millions d'années ou Ma), cambrien inférieur (540-530 Ma), ordovicien inférieur (480-470 Ma) et carbonifère supérieur-permien inférieur (310-285 Ma) ont été obtenus dans le socle de la nappe de Sambuco. Des âges similaires à 300 Ma ont été obtenus dans la nappe voisine de la Maggia, qui permettent de relier ces deux unités. Aujourd'hui côte à côte, ces deux nappes devaient également se trouver proches l'une de l'autre il y a 300 Ma, lors de l'extension post-varisque. Les structures magmatiques spectaculaires préservées dans le pluton du Matorello (300 Ma) contraignent la géométrie actuelle de la nappe de Sambuco dans laquelle l'intrusion s'est mise en place. La forme originelle du pluton, aujourd'hui retourné et replissé plusieurs fois, s'avère être tabulaire, faite d'intrusions de faible épaisseur (1-300 m) s'étalant en forme de disque (30m à 2 km de diamètre). Les injections successives de magma se sont accumulées sous un toit dioritique précoce; elles sont issues, par le refais de fractures, d'une chambre magmatique plus profonde, périodiquement réalimentée par des magmas calco-alcalins d'origine mantellique contaminés parla croûte continentale profonde (εNd = -2.1 à -4.7). Des accumulations d'enclaves magmatiques arrondies et granoclassées dans des paléo-chenaux à fond érosif témoignent de conditions de mise en place hydrodynamiques à haute énergie. Ces enclaves sont emmenées de la chambre magmatique sous-jacente à la faveur d'épisodes de fracturation hydraulique liés à l'injection de magmas matelliques chauds dans des liquides différenciés riches en eau. Cette hypothèse est étayée par l'existence de filons composites. Une paléohorizontale a pu être déduite au sein du pluton, indiquant que cette partie de la nappe de Sambuco est verticalisée et isoclinalement replissée par la déformation alpine. Finalement, des blocs érodés du socle Sambuco ont été retrouvés dans le wildflysch sommital de la couverture sédimentaire mésozoïque de la nappe d'Antigorio sous-jacente. Ceci suggère que les blocs ont été fournis parle front de la nappe de Sambuco en train de chevaucher sur la nappe d'Antigorio au moment de la fermeture du bassin sédimentaire de cette dernière.

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The purpose of this study was to investigate some important features of granular flows and suspension flows by computational simulation methods. Granular materials have been considered as an independent state ofmatter because of their complex behaviors. They sometimes behave like a solid, sometimes like a fluid, and sometimes can contain both phases in equilibrium. The computer simulation of dense shear granular flows of monodisperse, spherical particles shows that the collisional model of contacts yields the coexistence of solid and fluid phases while the frictional model represents a uniform flow of fluid phase. However, a comparison between the stress signals from the simulations and experiments revealed that the collisional model would result a proper match with the experimental evidences. Although the effect of gravity is found to beimportant in sedimentation of solid part, the stick-slip behavior associated with the collisional model looks more similar to that of experiments. The mathematical formulations based on the kinetic theory have been derived for the moderatesolid volume fractions with the assumption of the homogeneity of flow. In orderto make some simulations which can provide such an ideal flow, the simulation of unbounded granular shear flows was performed. Therefore, the homogeneous flow properties could be achieved in the moderate solid volume fractions. A new algorithm, namely the nonequilibrium approach was introduced to show the features of self-diffusion in the granular flows. Using this algorithm a one way flow can beextracted from the entire flow, which not only provides a straightforward calculation of self-diffusion coefficient but also can qualitatively determine the deviation of self-diffusion from the linear law at some regions nearby the wall inbounded flows. Anyhow, the average lateral self-diffusion coefficient, which was calculated by the aforementioned method, showed a desirable agreement with thepredictions of kinetic theory formulation. In the continuation of computer simulation of shear granular flows, some numerical and theoretical investigations were carried out on mass transfer and particle interactions in particulate flows. In this context, the boundary element method and its combination with the spectral method using the special capabilities of wavelets have been introduced as theefficient numerical methods to solve the governing equations of mass transfer in particulate flows. A theoretical formulation of fluid dispersivity in suspension flows revealed that the fluid dispersivity depends upon the fluid properties and particle parameters as well as the fluid-particle and particle-particle interactions.

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Este texto ahonda en las geografías políticas, sociales y familiares de Aurèlia Pijoan, la primera mujer que, médico de profesión, ha accedido a un cargo de representación municipal en Lleida. Casada con Luis Pérez García-Lago –secretario general del PSUC y la UGT en la Lleida de los años trenta y posteriormente máximo responsable del partido en el exilio mejicano-, continuó su compromiso a través de la Unión de Mujeres Españolas de México de la que llegó a convertirse en secretaria general. El artículo pretende, a la vez que reflexionar sobre el diálogo que se establece entre recuerdo y olvido, hacer visible la historia de los sin historia a partir de un centro de gravedad concreto, puesto que los itinerarios personales y familiares de Aurèlia Pijoan permiten recorrer las diversas caras del universo represivo franquista: exilio,clandestinidad y prisión.