Dans le champ de l'obésité massive, le corps est otage, l'individu est victime et agresseur. Le regard stigmatisant de l'Autre induit une souffrance psychique indicible par ceux dont le corps est différent de celui attendu dans une conformité imposée par des normes. L'individu, dans une présentification corporelle singulière, est déchiré entre le principe de plaisir offrant la satisfaction pulsionnelle, et le principe de réalité organisant l'indépassable culpabilité. Elle est renforcée par l’atteinte narcissique, majorée par le regard de l’autre, induit la haine de l'image, favorise le silence des affects. Que signifie : fabriquer plus de corps qui se traduit par plus de poids ? Quelle disjonction traverse Ie sujet entre son vouloir et son pouvoir, son savoir conscient et son désir inconscient ? L'étude des rapports ambivalents médecine/culture/norme/oralité aide à entrevoir des hypothèses différentes de celles des TCA classiques. A partir de la clinique, on peut envisager celle d'un état psychique entre deuil et mélancolie. A partir de la pratique en entretien apparait l'opportunité pour le sujet obèse d'engager un mouvement du regard à la parole afin de le dégager de l'entremêlement honte/rejet, et lui rendre une dignité. / In the field of massive obesity the body is the hostage and the dictator, the subject beingsimultaneously the victim and the assailant. The stigmatizing look of the other implies anunspeakable psychic pain for those whose body is different from the one expected to be conform to the present norms. The obese subject in a singular corporal presentification is torn between the principle of pleasure which gives him an urge-driven satisfaction and the principle of reality which organizes the impassable guilt. This culpability is strengthened by a narcissistic infringement and increased the other's look. This guilt also implies the hate of the image and furthers the silence of affects. What does it mean to produce more of body which manifests as more weight? Which disjunction goes through the subjects, between their will and their capacities, between what they consciously know and what they unconsciously desire? The study of the ambivalent relationships between medicine/culture/norm/orality helps us to foresee hypotheses which are different from those of the eating disorders 'classic theories. Through a clinical work, one can consider the hypothesis of a psychic state between loss and melancholy. Starting from the practice of interviews the obese subjects has an to start a motion from the look to the speech in order to free him from his mixed up state between shame and rejection, and to give him back dignity.

Paderborn, Universiẗat, Diss., 2002.

No description available.

Secondary ion mass spectrometry, SIMS, is one of the most versatile surface analytical techniques. The significant parameter determining the performance of SIMS is the secondary ion yield. Atomic projectiles, traditionally used in SIMS, are an inefficient method to desorb and generate secondary ions. The use of poly-atomic projectiles, such as (CsI)nCs, Au3, SF5 and C60, has been demonstrated to be an effective means to enhance secondary ion yields. Still larger secondary ion yields can be obtained with massive gold clusters, specifically Au4004+. Secondary ion yields from organic targets approach unity and are in excess of unity for selected inorganic targets. This dissertation is a first study of the secondary ion emission characteristics resulting from surface bombardment of keV Au400. The enhanced secondary ion yields from these massive clusters resulted in a need to detect isobaric secondary ions. An eight-anode detector was designed, built and implemented to study secondary ion emission resulting from massive projectile impacts. Secondary ion yield enhancements, resulting from use of the multi-anode detector, are reported along with secondary ion distributions for organic and inorganic targets. Au-adduct ions have been observed in mass spectra resulting form organic and inorganic targets bombarded by Au400. Data indicate that these adducts are a result of projectile/surface molecule interactions and not a product of Au implantation. Secondary ion yields of these adducts are reported. Although these adduct ion yields are an order of magnitude lower than the non-adduct ions, we have demonstrated their potential usefulness in analytical applications, such as examining surface homogeneity. Finally, these novel projectiles have been used to examine secondary ion emission from targets with different structural properties which have the same stoichiometry. In a comparative study, we have measured a significant difference in secondary ion emission and yields from the two systems, graphite and α-ZrP. Au400, at 136 keV, is effective in terms of secondary ion yield and secondary ion multiplicity enhancement. When used in the event-by-event bombardment/detection mode, the desorption volume has a diameter between 10-20 nm with and emission depth of approximately 5 nm, perturbing less than an attomole of analyte.

Depuis sa formulation au début du 20ème siècle, la théorie de la Relativité Générale a été vérifiée avec une précision sans cesse croissante. Cette théorie prédit, entre autre, l'existence d'ondes gravitationnelles qui restent à ce jour inobservées, et ce malgré de nombreuses tentatives de détections. Ces ondes sont caractérisées par leur absence de masse. Une des questions qui se pose alors est de savoir si cette absence de masse est une condition nécessaire pour que théorie et observations concordent. Pour répondre à cette question, il est indispensable d'étudier les différents aspects des théories décrivant des ondes gravitationnelles massives. Au-delà de cet intérêt purement théorique, l'étude de ces théories est, entre autre, motivée par de récentes observations cosmologiques. Celles-ci indiquent que l'accord entre la Relativité Générale et les observations n'est possible que si on suppose l'existence de matière et d'énergie noires. Cette thèse est dédiée à une classe de théories décrivant des ondes gravitationnelles massives. Dans un premier temps, nous résumons les différents problèmes qui surgissent lorsqu'on tente de donner une masse aux ondes gravitationnelles. Ensuite, nous introduisons une classe de modèles et étudions certaines de leurs caractéristiques. Le premier aspect étudié concerne l'existence d'une interaction de type instantanée. De telles interactions sont possibles étant donné que l'invariance de Lorentz est spontanément brisée dans les modèles considérés. Celles-ci sont dès lors discutées et un exemple concret est fourni. La présence d'une interaction instantanée dans ces modèles a une conséquence directe sur les solutions "trous noirs" des équations du champ. En effet, on s'attend à ce que l'interaction instantanée puisse propager de l'information à l'extérieur d'un trou noir, ce qui entraînerait une modification de ces solutions par rapport à celles de la Relativité Générale. Cette supposition est confirmée par les solutions "trous noirs" obtenues dans cette thèse. Celles-ci peuvent soit imiter une certaine quantité de matière noire, soit conduire à un champ gravitationnel répulsif. Finalement, les mécanismes de formation des grandes structures de l'Univers (galaxies, amas de galaxies, ... ) sont étudiés pour les théories considérées. Cette dernière discussion démontre que ces modèles reproduisent le comportement prévu par la Relativité Générale et sont, par conséquent, en accord avec les observations.

Secondary ion mass spectrometry, SIMS, is one of the most versatile surface analytical techniques. The significant parameter determining the performance of SIMS is the secondary ion yield. Atomic projectiles, traditionally used in SIMS, are an inefficient method to desorb and generate secondary ions. The use of poly-atomic projectiles, such as (CsI)nCs, Au3, SF5 and C60, has been demonstrated to be an effective means to enhance secondary ion yields. Still larger secondary ion yields can be obtained with massive gold clusters, specifically Au4004+. Secondary ion yields from organic targets approach unity and are in excess of unity for selected inorganic targets. This dissertation is a first study of the secondary ion emission characteristics resulting from surface bombardment of keV Au400. The enhanced secondary ion yields from these massive clusters resulted in a need to detect isobaric secondary ions. An eight-anode detector was designed, built and implemented to study secondary ion emission resulting from massive projectile impacts. Secondary ion yield enhancements, resulting from use of the multi-anode detector, are reported along with secondary ion distributions for organic and inorganic targets. Au-adduct ions have been observed in mass spectra resulting form organic and inorganic targets bombarded by Au400. Data indicate that these adducts are a result of projectile/surface molecule interactions and not a product of Au implantation. Secondary ion yields of these adducts are reported. Although these adduct ion yields are an order of magnitude lower than the non-adduct ions, we have demonstrated their potential usefulness in analytical applications, such as examining surface homogeneity. Finally, these novel projectiles have been used to examine secondary ion emission from targets with different structural properties which have the same stoichiometry. In a comparative study, we have measured a significant difference in secondary ion emission and yields from the two systems, graphite and α-ZrP. Au400, at 136 keV, is effective in terms of secondary ion yield and secondary ion multiplicity enhancement. When used in the event-by-event bombardment/detection mode, the desorption volume has a diameter between 10-20 nm with and emission depth of approximately 5 nm, perturbing less than an attomole of analyte.

Seismic imaging of shallow sediment hosted massive sulphides has not been studied in detail. In this research two shallow sediment hosted massive sulphide deposits (one deeper and larger than the other) were modeled and synthetic seismic data generated using a 2D elastic wavefield finite difference code. F-k filtering can be used to attenuating surface waves (conventional processing). This requires small trace spacing so that spatially aliasing of energy is avoided. An alternative to this involves avoiding the surface wave using an optimum offset window technique. Both of these approaches, attenuation and avoidance, produce a high amplitude image of the deeper larger orebody. For the smaller, shallower orebody, conventional processing produced only a weak image of the orebody. However, there is a significant amount of shear wave energy from this target, and therefore multicomponent geophones should be used to capture this energy.

Seismic imaging of shallow sediment hosted massive sulphides has not been studied in detail. In this research two shallow sediment hosted massive sulphide deposits (one deeper and larger than the other) were modeled and synthetic seismic data generated using a 2D elastic wavefield finite difference code. F-k filtering can be used to attenuating surface waves (conventional processing). This requires small trace spacing so that spatially aliasing of energy is avoided. An alternative to this involves avoiding the surface wave using an optimum offset window technique. Both of these approaches, attenuation and avoidance, produce a high amplitude image of the deeper larger orebody. For the smaller, shallower orebody, conventional processing produced only a weak image of the orebody. However, there is a significant amount of shear wave energy from this target, and therefore multicomponent geophones should be used to capture this energy.

Stuttgart, Univ., Diss., 2000.

Core-collapse supernovae (CCSNe) have very distinct observational properties that depend on the composition of the progenitor star, the dynamics of the explosion mechanism, and the surrounding stellar wind environment. In recent years, due to the uncertainty behind the type of massive star that evolves into different types of core-collapse events, there has been an increase in core-collapse supernova surveys aiding the advancement of numerical supernova simulations that explore the properties of the star before the explosion. Observationally, the unpredictable nature of these events makes it difficult to identify the type of star from which the CCSNe subtype evolves, but the issue from a theoretical standpoint relies on a gap in our current understanding of the explosion mechanism. The general light curve properties of CCSNe (rise, peak, and decay) by subtype are diverse, but appear to be homogeneous within each subtype, with the exception of Type IIn.. Simplified SN models can be processed quickly in order to explore the properties of the progenitor star along with the explosion mechanism and circumstellar medium. Here, we present a suite of SN light curve models presented using a 1-temperature, homologous outflow light curve code. The SN explosion is modeled from shock breakout through the ultimate uncovering of the nickel core. We are able to rapidly explore the diversity of the SN light curves by studying the effects of various explosion and progenitor star parameters, including ejecta mass, explosion energy, shock temperature, and stellar radii using this "simple" calculation technique. Furthermore, we compare UV and optical modeled light curves to Swift UVOT IIn observations to identify the general initial conditions that enable the difference between SN 2009ip and SN 2011ht light curve properties. Our results indicate that the peak light curve is dominated by the shock temperature and explosion energy, whereas the shape depends on the mass of the ejecta and the explosion energy. Based on this modeling approach, the comparison SN light curves are a product of processes occurring after shock breakout, but before Ni-56 decay. Therefore, the energy from nickel decay does not play a major role in the light curves of these explosions. In general, the diversity between SN 2009ip and SN 2011ht can be explained by the differences in the outer ejecta mass and the explosion energy.