Zusammenfassung: Ausschluss von Minderheiten (Zwangsübergang von Beteiligungswertpapieren) Diese Arbeit befasst sich mit dem Recht auf einen nachträglichen Ausgleich bei dem Zwangsübergang von Beteiligungswertpapieren, das eine der Grundvoraussetzungen der Verfassungsmäßigkeit des Ausschlusses von Minderheiten darstellt. Die gerichtliche Nachprüfung der den verdrängten Inhabern bezahlten Abfindung sowie der Ablauf der Bezahlung des nachträglichen Ausgleichs werden in dem Text der Arbeit ausführlich erörtert. Ziel dieser Arbeit ist es, die umstrittenen und unklaren Bestimmungen der wirksamen Regelung des Rechts auf einen nachträglichen Ausgleich aufzuzeigen, mögliche Auslegungen solcher Bestimmungen darzulegen und aus diesen die geeignetste Auslegung zu wählen. Diese Auslegung wird dann mit den zur Regelung des Ausschlusses im Handelsgesetzbuch verfassten Schlussfolgerungen der Rechtsprechung verglichen um zu beurteilen, ob diese Schlussfolgerungen der Rechtsprechung auch nach dem 01. 01. 2014 weiterhin gelten. In dieser Arbeit wird die Bedeutung des Rechts auf einen nachträglichen Ausgleich sowie die allgemeinen Aspekte der Geltendmachung dieses Rechts erklärt. Das gerichtliche Verfahren und die außengerichtliche Vereinbarung das nachträgliche Ausgleich wird ausführlich erörtert. Der Ablauf der Bezahlung...

Bien que représentant plus d’un quart de la distribution en énergie de notre Univers ainsi que la majorité (84\%) de la masse de celui-ci, la nature de la matière noire n’a pas encore été percée à ce jour. Dans cette thèse, il sera supposé que la matière noire est une nouvelle particule élémentaire, stable et dont la connexion (hors interactions gravitationnelles) avec le secteur visible est réalisée grâce à une autre particule, le médiateur. Au sein de ces lignes, la matière noire sera supposée être un fermion de Dirac et le médiateur un boson (vecteur ou scalaire), ce dernier étant choisi comme étant plus léger que la matière noire. Cette thèse propose d’explorer les aspects infrarouges de la production de la matière noire dans l’Univers primordial, le potentiel de détection d’une importante classe de candidats dits \enquote{freeze-in}, caractérisés par de très faibles interactions avec le Modèle Standard, auprès des expériences de détection directe et l’effet des auto-interactions de la matière noire sur son comportement superfluide dans les régions de haute densité de matière noire (halos, capture par des astres compacts) asymétrique. Sous ces hypothèses, premièrement, une étude exhaustive des différents mécanismes de production de la matière noire est réalisée, illustrée dans un modèle où le médiateur est un photon du secteur caché, issu d’un nouveau groupe de jauge U(1)’, qui mélange de façon cinématique avec le photon du Modèle Standard. En particulier, de nouveaux canaux de production sont mis en avant, nommément \textit{freeze-in from mediator} et \textit{sequential freeze-in}. Ceux-ci correspondent à des scénarios où la matière noire est très faiblement couplée au Modèle Standard, n’atteint jamais l’équilibre avec celui-ci dans l’Univers primordial et est produit petit à petit par des annihilations de médiateurs (en équilibre ou non avec le Modèle Standard). Il est ensuite montré que pour l’important et très attractif cas d’une matière noire milli-chargée (ainsi que pour des scénarios où le médiateur n’est pas plus massif que 40 méga-electronvolt), l’expérience de détection indirect Xenon1T contraint aujourd’hui l’espace des paramètres de la phase de freeze-in de ces modèles, et est, dans cette région de l’espace des paramètres, la contrainte la plus importante. Une réinterprétation des limites sur les interactions indépendantes du spin matière noire – nucléon est par ailleurs nécessaire, détaillée et validée. Dans la seconde partie de la thèse, l’effet des auto-interactions dans les scénarios de matière noire asymétrique est exploré. Sous l’hypothèse qu’un halo (galactique ou non) de matière noire atteint l’équilibre thermodynamique à très basse température (comparée à sa masse) et développe donc un potentiel chimique fini, des interactions matière noire – matière noire au voisinage de la surface de Fermi peut entraîner la formation de condensats, de transitions de phase du milieu et dès lors modifier drastiquement l’équation d’état du halo. Un système d’équations auto-consistant pour les condensats est présenté et résolu numériquement. Ensuite, la thermodynamique du système de gaz interagissant est explorée. Finalement, les interactions gravitationnelles sont considérées et les configurations auto-gravitantes, prenant en compte l’ensemble des auto-interactions, sont déterminées et leurs aspects phénoménologiques sont explorés.Even though dark matter represents more than a quarter of the energy budget of our Universe and the majority (84\%) of its mass, the nature of dark matter has not yet been unravelled. In this thesis, it will be assumed that dark matter is a new elementary particle, stable and whose connection (on top of gravitational interactions) with the visible sector is realized through another particle, the mediator. In this thesis, dark matter will be assumed to be a Dirac fermion and the mediator will be a boson (either vector or scalar). This thesis proposes to explore infrared aspects of the production of dark matter in the primeval Universe, aspects of detection of the important class of feebly coupled \enquote{freeze-in} candidates at direct detection experiments and aspects of condensed matter physics such as superfluidity in region of high dark matter density (halos or inside compact objects such as neutron stars). Under these hypothesis, we will first detail an exhaustive study of the possible thermal mechanism of dark matter production, illustrated in a model where the mediator is a dark photon, arising from a new $U\left(1\right)'$ gauge group, which kinematically mixes with the Standard Model photon. In particular, new production channels are put forward, namely the \textit{freeze-in from mediator} and \textit{sequential freeze-in}. They correspond to scenarios where dark matter is very feebly coupled to the Standard Model, do not reach equilibrium with the visible sector thermal bath in the Early Universe and are slowly produced by mediator annihilations (in-equilibrium or not with the Standard Model). It is then showed that for the popular case of a millicharged dark matter ( and for scenarios in which the mediator mass is not bigger than $40$ mega electronvolt), the direct detection experiment XENON1T constrains today the freeze-in parameter space of such models and is the strongest constraint overall for such candidates. A recast of the bounds on spin-independent dark matter$-$nucleon interactions was needed and we validate our procedure against other recast. In the second part of this thesis, the effects of self-interactions in asymmetric dark mater scenarios are explored. Under the hypothesis that a dark matter halo reaches thermodynamic equilibrium at very low temperature (compared to its mass) and develops a finite chemical potential, dark matter$-$ dark matter interactions at the vicinity of the Fermi surface can lead to the formation of condensates, to phase transitions and therefore modify drastically the equation of state of the halo. A self-consistant set of equations for the condensates is presented and solved numerically. The thermodynamics of the interacting dark matter cloud is also explored. Finally, gravitational interactions are considered and self-gravitating configurations of halos, taking into account self-interactions, are determined and their phenomenological aspects is explored. / Doctorat en Sciences / info:eu-repo/semantics/nonPublished

Numerous glacial advances over the past 2 million years have covered the entire Canadian and Fennoscandian Shield outcrop. During glacial advance and retreat, permafrost is expected to form in front of the glacier. The question of how permafrost and freezing impact the formation and evolution of brines in natural systems may be vital to understanding the chemistry of groundwater in crystalline rocks. Investigations of groundwater conditions beneath thick permafrost can provide valuable information that can be applied to assessing safety of deep, underground nuclear waste repositories and understanding analogues to potential life-bearing zones on Mars. However, very little scientific investigation of cryogenic processes and hydrogeology deep within crystalline systems has been published. The purpose of this research is to evaluate the impacts of thick permafrost (>300m) formation on groundwater chemical and flow system evolution in the crystalline rock environment over geologic timescales. A field investigation was conducted at the Lupin Mine in Nunavut, Canada, to characterize the physical and hydrogeochemical conditions within and beneath a thick permafrost layer. Taliks, or unfrozen channels within the permafrost, are found beneath large lakes in the field area, and provide potential hydraulic connections through the permafrost. Rock matrix waters are dilute and do not appear to affect groundwater salinity. Permafrost waters are Na-Cl and Na-Cl-SO4 type, and have been contaminated with chloride and nitrate by mining activities. Sulfide oxidation in the permafrost may be naturally occurring or is enhanced by mining activities. Basal permafrost waters (550 to 570 mbgs) are variably affected by mining. The less contaminated basal waters have medium sulfate concentrations and are Ca-Na dominated. This is similar to deeper, uncontaminated subpermafrost waters, which are Ca-Na-Cl or Na-Ca-Cl type with a wide range of salinities (2.6 to 40 g•L-1). The lower salinity subpermafrost waters are attributed to dissociation of methane hydrate and drawdown of dilute talik waters by the hydraulic gradient created by mine dewatering. This investigation was unable to determine the influence of talik waters to the subpermafrost zone in undisturbed conditions. Pressures are also highly variable, and do not correlate with salinity. Fracture infillings are scarce and calcite δ18O and δ13C values have a large range. Microthermometry indicates a large range in salinities and homogenization temperatures as well, indicative of a boiling system. In situ freezing of fluids and methane hydrate formation may have concentrated the remaining fluids. Field activities at the Lupin mine also provided an opportunity to study the nature of gases within crystalline rocks in a permafrost environment. Gases were generally methane-dominated (64 to 87), with methane δ13C and δ2H values varying between -56 and -42‰ VPDB and -349 to -181 ‰ VSMOW, respectively. The gases sampled within the Lupin mine have unique ranges of chemical and isotopic compositions compared with other Canadian and Fennoscandian Shield gases. The gases may be of thermogenic origin, mixed with some bacteriogenic gas. The generally low δ2H-CH4 ratios are somewhat problematic to this interpretation, but the geologic history of the site, a metaturbidite sequence, supports a thermogenic gas origin. The presence of gas hydrate in the rock surrounding Lupin was inferred, based on temperature measurements and hydrostatic pressures. Evidence also suggests fractures near the mine have been depressurized, likely due to mine de-watering, resulting in dissipation of methane hydrate near the mine. Modeling results indicate methane hydrates were stable throughout the Quaternary glacial-interglacial cycles, potentially limiting subglacial recharge. The effects of deep permafrost formation and dissipation during the Pleistocene glacial/interglacial cycle to deep groundwaters in the Canadian Shield were also investigated by compiling data from thirty-nine sites at twenty-four locations across the Canadian Shield. Impacts due to glacial meltwater recharge and surficial cryogenic concentration of fluids, which had been previously considered by others, and in situ freeze-out effects due to ice and/or methane hydrate formation were considered. At some Canadian Shield sites, there are indications that fresh, brackish, and saline groundwaters have been affected by one of these processes, but the data were not sufficient to differentiate between mixed, intruded glacial meltwaters, or residual waters resulting from either permafrost or methane hydrate formation. Physical and geochemical data do not support the cryogenic formation of Canadian Shield brines from seawater in glacial marginal troughs. The origin and evolution of Canadian and Fennoscandian Shield brines was explored with a survey of chlorine and bromine stable isotope ratios. The δ37Cl and δ81Br isotopic ratios varied between -0.78 ‰ and 1.52 ‰ (SMOC) and 0.01 ‰ and 1.52 ‰ (SMOB), respectively. Variability of chlorine and bromine isotope ratios decreases with increasing depth. Fennoscandian Shield groundwaters tend to be more enriched than Canadian Shield groundwaters for both 37Cl and 81Br. Other sources and processes which may affect δ37Cl and δ81Br composition are also explored. Primary processes such as magmatic and/or hydrothermal activity are thought to be responsible for the isotopic composition of the most concentrated fluids at each site. Positive correlations between δ81Br, and δ37Cl with δ2H-CH4 and δ13C-CH4 were noted. At this time the cause of the relationship is unclear, and may be a result of changing redox, pH, temperature, and/or pressure conditions during hydrothermal, metamorphic, or volcanogenic processes. The data suggest solute sources and fluid evolution at individual sites would be better constrained utilizing a multi-tracer investigation of δ37Cl, δ81Br, and 87Sr/86Sr ratios comparing fluids, rocks, and fracture filling minerals (including fluid inclusions).

Numerous glacial advances over the past 2 million years have covered the entire Canadian and Fennoscandian Shield outcrop. During glacial advance and retreat, permafrost is expected to form in front of the glacier. The question of how permafrost and freezing impact the formation and evolution of brines in natural systems may be vital to understanding the chemistry of groundwater in crystalline rocks. Investigations of groundwater conditions beneath thick permafrost can provide valuable information that can be applied to assessing safety of deep, underground nuclear waste repositories and understanding analogues to potential life-bearing zones on Mars. However, very little scientific investigation of cryogenic processes and hydrogeology deep within crystalline systems has been published. The purpose of this research is to evaluate the impacts of thick permafrost (>300m) formation on groundwater chemical and flow system evolution in the crystalline rock environment over geologic timescales. A field investigation was conducted at the Lupin Mine in Nunavut, Canada, to characterize the physical and hydrogeochemical conditions within and beneath a thick permafrost layer. Taliks, or unfrozen channels within the permafrost, are found beneath large lakes in the field area, and provide potential hydraulic connections through the permafrost. Rock matrix waters are dilute and do not appear to affect groundwater salinity. Permafrost waters are Na-Cl and Na-Cl-SO4 type, and have been contaminated with chloride and nitrate by mining activities. Sulfide oxidation in the permafrost may be naturally occurring or is enhanced by mining activities. Basal permafrost waters (550 to 570 mbgs) are variably affected by mining. The less contaminated basal waters have medium sulfate concentrations and are Ca-Na dominated. This is similar to deeper, uncontaminated subpermafrost waters, which are Ca-Na-Cl or Na-Ca-Cl type with a wide range of salinities (2.6 to 40 g•L-1). The lower salinity subpermafrost waters are attributed to dissociation of methane hydrate and drawdown of dilute talik waters by the hydraulic gradient created by mine dewatering. This investigation was unable to determine the influence of talik waters to the subpermafrost zone in undisturbed conditions. Pressures are also highly variable, and do not correlate with salinity. Fracture infillings are scarce and calcite δ18O and δ13C values have a large range. Microthermometry indicates a large range in salinities and homogenization temperatures as well, indicative of a boiling system. In situ freezing of fluids and methane hydrate formation may have concentrated the remaining fluids. Field activities at the Lupin mine also provided an opportunity to study the nature of gases within crystalline rocks in a permafrost environment. Gases were generally methane-dominated (64 to 87), with methane δ13C and δ2H values varying between -56 and -42‰ VPDB and -349 to -181 ‰ VSMOW, respectively. The gases sampled within the Lupin mine have unique ranges of chemical and isotopic compositions compared with other Canadian and Fennoscandian Shield gases. The gases may be of thermogenic origin, mixed with some bacteriogenic gas. The generally low δ2H-CH4 ratios are somewhat problematic to this interpretation, but the geologic history of the site, a metaturbidite sequence, supports a thermogenic gas origin. The presence of gas hydrate in the rock surrounding Lupin was inferred, based on temperature measurements and hydrostatic pressures. Evidence also suggests fractures near the mine have been depressurized, likely due to mine de-watering, resulting in dissipation of methane hydrate near the mine. Modeling results indicate methane hydrates were stable throughout the Quaternary glacial-interglacial cycles, potentially limiting subglacial recharge. The effects of deep permafrost formation and dissipation during the Pleistocene glacial/interglacial cycle to deep groundwaters in the Canadian Shield were also investigated by compiling data from thirty-nine sites at twenty-four locations across the Canadian Shield. Impacts due to glacial meltwater recharge and surficial cryogenic concentration of fluids, which had been previously considered by others, and in situ freeze-out effects due to ice and/or methane hydrate formation were considered. At some Canadian Shield sites, there are indications that fresh, brackish, and saline groundwaters have been affected by one of these processes, but the data were not sufficient to differentiate between mixed, intruded glacial meltwaters, or residual waters resulting from either permafrost or methane hydrate formation. Physical and geochemical data do not support the cryogenic formation of Canadian Shield brines from seawater in glacial marginal troughs. The origin and evolution of Canadian and Fennoscandian Shield brines was explored with a survey of chlorine and bromine stable isotope ratios. The δ37Cl and δ81Br isotopic ratios varied between -0.78 ‰ and 1.52 ‰ (SMOC) and 0.01 ‰ and 1.52 ‰ (SMOB), respectively. Variability of chlorine and bromine isotope ratios decreases with increasing depth. Fennoscandian Shield groundwaters tend to be more enriched than Canadian Shield groundwaters for both 37Cl and 81Br. Other sources and processes which may affect δ37Cl and δ81Br composition are also explored. Primary processes such as magmatic and/or hydrothermal activity are thought to be responsible for the isotopic composition of the most concentrated fluids at each site. Positive correlations between δ81Br, and δ37Cl with δ2H-CH4 and δ13C-CH4 were noted. At this time the cause of the relationship is unclear, and may be a result of changing redox, pH, temperature, and/or pressure conditions during hydrothermal, metamorphic, or volcanogenic processes. The data suggest solute sources and fluid evolution at individual sites would be better constrained utilizing a multi-tracer investigation of δ37Cl, δ81Br, and 87Sr/86Sr ratios comparing fluids, rocks, and fracture filling minerals (including fluid inclusions).