Afin de mieux comprendre la stabilité des mousses de verre, des expériences à l'échelle d'une bulle et d'un film vertical sont réalisées pour différentes composition de verre, viscosité, taille de bulle, et gaz à l'intérieur de la bulle. L'épaisseur du film au-dessus de la bulle est mesurée par interférence optique et décroît exponentiellement avec le temps sous l'effet des forces de pesanteur et capillaires. Le temps de vie de la bulle doit être divisé en deux étapes. En premier, le taux d'amincissement dépend du nombre de Bond. Ensuite, un écoulement contraire est observé aux fortes températures pour les verres sodo-sili-calcite. Ce phénomène également observé pour des films verticaux et s'explique par des écoulements Marangoni dus à l'évaporation de substances telles que le sodium qui engendre des variations de composition et de tension de surface. Des petites bulles sont crées à la surface libre lors de l'éclatement de grosses bulles à la surface d'un verre fondu faiblement visqueux / For investigating glass foams stability, experiments with a single bubble rising towards the free surface of molten glass and with vertical films are performed for several values of glass chemical composition, viscosity, bubble size and gas nature. The glass lamella on top of the bubble is observed by video-recording and its thickness evolution is measured by optical interferometry. The lamella thins as a result of buoyancy and capillary forces and then it ruptures. Actually the lamella thinning occurs in two steps. In the first step, the drainage is regular and the thinning rate depends on Bond number. In the second step a backward flow is observed above 1200°C for ordinary soda-lime-silica glass, which is explained as Marangoni counter flow due to evaporation of volatile species such as sodium. As the lamella ruptures tiny bubbles are created by the rupture of bubble lamella on the free surface for large bubbles and low viscosity of the melt

This is a dissertation about urban systems; within this broad subject I tackle three issues, one that focuses on an observed inter-city relationship and two that focus on an intra-city phenomenon. In Chapter II I adapt a model of random emergence of economic opportunities from the firm growth literature to the urban dynamics situation and present several predictions for urban system dynamics. One of these predictions is that the older the city the larger and more diversified it is going to be on average, which I proceed to verify empirically using two distinct datasets. In Chapter III I analyze the Residential Real Estate Bubble that took place in Miami-Dade County from 1999 to 2006. I adopt a Spatial-Economic model developed for the Paris Bubble episode of 1984-1993 and formulate an innovative test of the results in terms of speculative intensity on the basis of proxies of investor activity available in my dataset. My results support the idea that the best or more expensive areas are also where the greatest speculative activity takes place and where the rapid increase in prices begins. The most significant departure from previous studies that emerges in my results is the absence of a wider gap between high priced areas and low priced areas in the peak year. I develop a measure of dispersion in value among areas and contrast the Miami-Dade and Paris episodes. In Chapter IV I analyze the impact on tax equity of a Florida tax-limiting legislation known as Save Our Homes. I first compare homesteaded and non-homesteaded properties, and second, look within the subset of homesteaded properties. I find that non- homesteaded properties increase their share of taxes paid relative to homesteaded properties during an up market, but that this is reversed during a down market. For the subset of homesteaded properties I find that the impact on tax equity of SOH will depend on differential growth rates among higher and lower valued homes, but during times of rapid home price appreciation, in a scenario of no differential growth rates in property values, SOH increases progressivity relative to the prior system.

abstract: The “filter bubble” has been a heated discussion topic since several years ago. In addition to possible algorithmic contribution to this phenomenon, people’s selective exposure tendency may be another primary cause of the “filter bubble” on social media. Prior research indicates that, under the influence of selective exposure tendency, people tend to perceive pro-attitudinal news as more credible than counter-attitudinal news, with strong partisans more likely to be affected. The proposed thesis seeks to examine whether the perceived credibility of a news source and story on social media is influenced by selective exposure and strength of partisanship. Through an experimental study via Amazon’s Mechanical Turk, 468 participants chose or were assigned to read an ostensible news story from a social media feed with the news source and ideological slant varied between participants. The results showed that people reported higher perceived source and story credibility when the source and stories were pro-attitudinal (consistent with their political ideology) as opposed to counter-attitudinal, regardless of participants’ age, race, perceived credibility of news from social media, in general, and strength of partisanship. However, contrary to the hypotheses, selective exposure behavior (i.e., choosing a preferred news source before reading a news story) did not affect credibility perceptions when participants read counter-attitudinal news from a pro-attitudinal source. Last, strength of partisanship did not moderate the influence of selective exposure on credibility perceptions. In sum, this study suggests that although selective exposure tendency may affect people’s credibility perceptions and contribute to “filter bubbles,” the impact of selective exposure behavior may be overestimated in terms of perceived source and story credibility of news on social media. / Dissertation/Thesis / Masters Thesis Public Administration 2020

L’interaction spin-orbite a permis de reproduire dans les modèles nucléaires théoriques, les nombres magiques N=28 et 50 observés dans les noyaux atomiques. Ces dernières décennies, l’étude expérimentale de noyaux exotiques a mis en évidence une évolution des nombres magiques loin de la vallée de stabilité. On peut alors se poser la question de l’évolution des potentiels d’interaction eux-mêmes, et en particulier de l’interaction spin-orbite. Si cette interaction a été historiquement incluse « à la main » dans les modèles de champ moyen « classiques », elle émerge cependant naturellement dans les modèles relativistes. La description de l’interaction spin-orbite est très similaire dans ces deux types de modèles, mais il subsiste a priori un désaccord du point de vue de sa dépendance en isospin : les modèles non-relativistes de type Hartree-Fock présentent en effet un potentiel spin-orbite dépendant fortement de l’isospin, contrairement aux modèles de type Relativistic Mean Field.En 2009, des calculs mettant en œuvre différents modèles théoriques ont prédit l’existence d’une « bulle », caractérisée par une déplétion en densité protonique centrale, dans le ³⁴Si. Ce dernier aurait une densité protonique très exotique, et bien différente de sa densité neutronique. Le ³⁴Si constituerait alors une sonde idéale de l’évolution du potentiel spin-orbite dans les systèmes présentant une forte asymétrie protons-neutrons. L’émergence d’un tel effet trouverait son origine dans la déplétion de l’orbitale protonique2s½, les orbitales s étant les seules à contribuer à la densité nucléaire centrale.Une expérience réalisée en Septembre 2012 à NSCL (MSU, Etats-Unis), a permis de mettre en évidence pour la première fois un effet de bulle nucléaire dans le ³⁴Si. L’étude des facteurs spectroscopiques des états peuplés lors des réactions d’arrachage de proton ou de neutron ³⁴Si(-1p) ³³Al et ³⁴Si(-1n) ³³Si indique que sa structure neutronique est très proche d’un système sans corrélations au-delà du champ moyen, tandis que son orbitale protonique est très faiblement occupée : n(2s½) = 0,16(4).Les réactions ³⁶S(-1p) ³⁵P et ³⁶S(-1n) ³⁵S ont été étudiées dans les mêmes conditions expérimentales. L’évolution de l’occupation n(2s½) mesurée entre le ³⁶S et le ³⁴Si, ainsi que la variation de l’écart en énergie des partenaires spin-orbite neutroniques 2p½-2p^3/2, mesurée entre ces deux noyaux dans une expérience antérieure, sont en faveur des modèles de champ moyen non-relativistes. La partie théorique de cette thèse a cependant montré que la différence de comportement de l’interaction spin-orbite entre modèles relativistes et non-relativistes est en fait un artefact causé par l’omission du terme d’échange dans les calculs de type Relativistic Mean Field. En effet, l’inclusion du terme de Fock dans les modèles relativistes permet de rétablir la dépendance en isospin du potentiel spin-orbite observée dans le cas non-relativiste. / The spin-orbit interaction is essential for the reproduction of magic numbers N=28 and 50 in theoretical nuclear models. Over the past few decades, the experimental study of exotic nuclei has highlighted an evolution of magic numbers far from stability. One can then wonder about the evolution of nuclear potentials themselves, and in particular the one of spin-orbit interaction. Historically, this interaction was included « by hand » in mean field models, whereas it naturally arises in relativistic mean field models. The description of the spin-orbit interaction happens to be very similar in those two kinds of models, but there remains a disagreement regarding its isospin dependance. Indeed, Hartree-Fock models exhibit a spin-orbit potential which strongly depends on isospin, contrary to relativistic mean field models.In 2009, a proton bubble was predicted in ³⁴Si by means of several different nuclear models. This effect consists in a central proton central density depletion. ³⁴Si would exhibit a quite exotic proton density, and very different from its neutron density. This nucleus would then constitute an ideal probe to test the behaviour of the spin-orbit potential in systems with strong proton-neutron asymmetry. The appearance of such an effect would originate from the depletion of proton 2s½ orbitals, as s orbitals are the only ones contributing to the central density.An experiment which was performed in September 2012 at NSCL (MSU, United States) highlighted for the first time a proton bubble in ³⁴Si. The spectroscopic strengths of states populated in the knockout reactions ³⁴Si(-1p)³³Al and ³⁴Si(-1n)³³Si reveal that the neutron structure of ³⁴Si is close to the one of a system without beyond-mean-field correlations, whereas its proton orbital is only weakly occupied : n(2s½) = 0,16(4).The reactions ³⁶S(-1p)³⁵P and ³⁶S(-1n)³⁵S were studied in similar experimental conditions. The change in occupancy n(2s½) measured between ³⁶S and ³⁴Si, as well as the variation in the neutron spin-orbit splitting 2p½-2p^3/2 measured in an earlier experiment, suggest that non-relativistic models exhibit the right isospin dependance. The theoretical part of this thesis showed however that the difference in behaviour of the spin-orbit interaction between relativistic and non-relativistic model is actually an artefact caused by the omission of the exchange term in relativistic mean field calculations. Indeed, including the Fock term in relativistic models enables to restore the isospin dependance observed in the non-relativistic case.

This thesis deals with the numerical solution of cavitation bubble dynamics and with cyanobacteria gas vesicle behaviour. A program for the numerical calculation of bubble dynamics is created using the Rayleigh-Plesset equation and its modifications. Subsequently, bubbles of different sizes are investigated during acoustic cavitation with various driving frequencies. Furthermore, a model for hydrodynamic cavitation is created. The model combines CFD computation of flow in the Venturi nozzle with the cavitation bubble dynamics calculation. The last part of the work is dedicated to cyanobacteria gas vesicle behaviour in a variable pressure field and during passage through the Venturi nozzle.

In this thesis, the dynamics of an isolated cavitation bubble submerged in a steady flow is studied numerically. A Lagrangian-Eulerian approach is considered, in which properties of the fluid are computed first by means of Eulerian methods (in this study the commercial CFD software Ansys Fluent 19 was used) and the trajectory of the bubble is then computed in a Lagrangian fashion, i.e. the bubble is considered as a small particle moving relative to the fluid, due to the effect of several forces depending on fluid's pressure field, fluid's velocity field and bubble's radius. Bubble's radius dynamics, modeled by Rayleigh-Plesset equation, has a big influence on its kinetics, so a special attention is given to it. Two study cases are considered. The first one, motivated by acoustic cavitation is concerned with the response of the bubble's radius in a static flow under the influence of an oscillatory pressure field, the second one studies the trajectory of the bubble submerged in a fluid passing by a Venturi tube and a sharp-edged orifice plate.

L'objectif de ces travaux est de déterminer l'atténuation des effets d'une explosion sous-marine par un rideau de bulles. Dans ce cadre, une modélisation de la propagation d'un chocdans les liquides à bulles a été développée, basée sur une technique de transition d'échelles.Cette méthode permet la formulation de modèles continus de liquides aérés, dont la mise enoeuvre est aisée et rapide. Nous avons d'abord développé une modélisation pour des liquidesdiphasiques au sein desquels les bulles sont régulièrement réparties dans l'espace, avant deproposer une extension de ce modèle au cas des liquides à bulles présentant des hétérogénéitésde porosité sous la forme d'amas sphériques de bulles. Un modèle de fragmentation des bulleslors du passage du choc a également été développé, basé sur une analyse linéaire de stabilitédes bulles. L'étude a permis d'établir un critère prédictif de fission et de déterminer le nombrede fragments associés. L'ensemble des modélisations proposées a fait l'objet de comparaisonsavec des résultats expérimentaux issus de la littérature. La concordance entre résultats d'essaiset résultats issus de la modélisation démontre les capacités prédictives de l'approche proposée.Cette modélisation a enfin été appliquée au cas de rideaux de bulles soumis à une explosionsous-marine. Une étude de sensibilité sur les paramètres physiques du rideau a été menée, eta permis de confirmer les tendances expérimentales : sous certaines conditions, la dispositiond'un rideau de bulles sous l'eau permet de diminuer de façon très conséquente l'énergie duchoc transmis en aval du rideau. / The present work deals with the modelling of shock wave propagation in bubbly liquids, inorder to assess the damping of underwater explosion by bubble curtains. The modelling is basedon a scale transition technique, which allows to formulate efficient continuum models of bubblyliquids. A modelling of homogeneous bubbly liquids has first been proposed, then extended tothe case of liquids with spherical bubble clusters. A modelling of bubble fragmentation duringshock propagation has also been developed, based on a stability analysis of the bubbles. Thisstudy enables us to establish a criterion for bubble fission and to determine the numberof fragments. The accuracy of the proposed models has been assessed through comparisonwith experimental data of the literature. The agreement between numerical and experimentalresults proves the predictive capabilities of the whole approach. The modelling has then beenapplied to the mitigation of UNDEX-induced shock wave by bubble curtain. A sensitive studyabout physical parameters of the curtain has been performed, and confirms the experimentaltendencies : the use of a bubble curtain can dissipate a significant part of the shock energy.

The development of hydroelectric power production and the damming of water courses that ensues causes a threat to the migration patterns of Atlantic salmon (Salmo salar), by altering their habitat and compromising river connectivity. Because the species’ survival heavily depends on the completion of their migration between rivers and oceans, the design of guidance structures that promote successful passages around dams is a critical goal. Physical structures have been used to steer downwards-migrating smolts through safe fishways but they have not always proven effective, both from an ecological and economical perspective. In this study, the potential of bubbles in guiding salmon trajectories around a hydropower dam was tested as an alternative to existing guiding systems. Here the hypotheses were: i) bubbles guide downstream-migrating smolts around dams; ii) the reaction of smolts to a bubble barrier is linked to their individual boldness; iii) bubbles have varying effects on different school sizes. The first and third hypotheses were tested in the field, by recording sonar footage at the entrance of a fishway, downstream of a bubble barrier. The second hypothesis was evaluated by conducting a scototaxis experiment and an assessment of the reaction of young salmon to bubbles in the laboratory. My analysis of the fish abundance data collected in the river confirmed the first and third hypotheses. In the field, the presence of a predator (Esox lucius) was revealed to be a more influential factor than bubbles in regulating the number of smolts steered towards the fishway, indicating that predators generated a larger anxiety-like response in smolts than bubbles. In the controlled laboratory setting, there was no significant correlation between anxiety-like behaviour and reaction to bubbles and the second hypothesis did not appear to be valid. Therefore, the cause of avoidance of the barrier remains unclear, but bubble barriers seem to be an efficient and cost-effective structure for guiding downstream-migrating salmon smolts.

Purpose – At the beginning of this year the number of social media user worldwide was recorded to be at 3.80 billion and is estimated to keep rising (Kemp, 2020). Along with this connectivity, new concepts have been acknowledged that have caused some controversy. These concepts have been named echo chambers and filter bubbles. This study investigates how social media users experience personalisation algorithms and the perceived existence of filter bubbles and echo chambers on various social media platforms and channels. Furthermore, it explores to what extent these users make use of strategies when navigating their social media feeds and if they believe that said strategies have any effect on personalisation algorithms, filter bubbles, and echo chambers. Method – Semi-structured interviews were conducted with 10 participants currently studying at Jönköping University. The interviews were then transcribed and analysed using a thematic approach.  Findings – The perception of students at Jönköping University is that filter bubbles and echo chambers exist in a varying degree of visibility and commonality depending on the situation and medium. These are also experienced to be interconnected with personalisation algorithms. The experience of personalisation algorithms is mainly positive, as it allows the users to easily navigate the feed but negative implications are also mentioned.  These are isolation, the negative strengthening and creation of filter bubbles or echo chambers. However, the algorithm is not believed to be the only thing responsible for the creation. The users believe that their own navigation and strategies can have such an effect. The strategies that users use are (1) Passive navigation, (2) Source evaluation, (3) Multiple source searching, (4) Responsibility taking, and the (5) Creation of filter bubbles. The effect these have on filter bubbles, personalisation algorithms and echo chambers is helping, to an extent, alleviate some of the negative effects that these are experienced to have. However, the passive navigation and creation of filter bubbles have a somewhat opposite effect as they help the creation or maintaining of filter bubbles and personalisation algorithms. Implications – The findings in this study build on existing evidence of echo chambers being more easily formed when the topic of discussion is of a political nature, as it is described by Barberá, Jost, Nagler, Tucker, and Bonneau (2015) in their research on how echo chambers form on Twitter. Furthermore, these findings could be considered to disagree with the research of Dubois and Blank (2018) who found that people who had a high political interest were less likely of ending up in an echo chamber. Although, due to their research taking all media into account, such as television, radio, newspaper, and so forth, while the current study is focused on social media alone the comparison is a bit more difficult to make. Finally, in the study made by Seargeant and Tagg (2019), it was concluded that the personalisation algorithms are not the sole contributor to filter bubbles forming on Facebook and that the users play a key role in how their online environment is shaped. The results of this study build on their research that the users do use strategies when navigating that affect what is being shown to them on their social media feeds. However, the participants of the current study claimed that the algorithms played a pretty large role too, which is not quite in line with the research conducted by Seargeant and Tagg (2019). Limitations – The generalisability of this study is limited due to the small sample size chosen to conduct this study, although instead, it provides deeper insight into the relationship between humans and their social media platforms and channels. Moreover, a bias that should be acknowledged is that when conducting interviews there is a risk of encountering response bias, which is when the participants assume the purpose of the study and adapt their answers to fit what they believe the researcher(s) want to hear. To avoid this precautions were taken when designing the questions to make sure that they would not lead the participants in any directions.

Die in dieser Arbeit vorgestellten Simulationen aufsteigender fluider Partikel wurden mit dem CFD-Programm FS3D durchgeführt, welches auf der Volume-of-Fluid (VoF) Methode basiert. Die Validierung des Codes erfolgt durch Vergleich der numerischen Lösungen für schleichende Strömungen mit analytischen Lösungen, wobei eine gute Übereinstimmung festgestellt wird. Im ersten Teil der Dissertation werden Simulationen für den freien Aufstieg von Öltropfen in Wasser mit experimentellen Beobachtungen hinsichtlich der Aufstiegsgeschwindigkeit, der Tropfenform und der Bewegungsbahn verglichen. Die Aufstiegsgeschwindigkeiten und Widerstandsbeiwerte sind vergleichbar, die simulierten Tropfen sind jedoch deutlich flacher. Dieser Unterschied kann durch Verunreinigungen der Grenzfläche im Experiment verursacht sein. Der Übergang von einem gradlinigen Aufstieg zu zickzack-förmigen Aufstiegsbahnen kann mit Hilfe der Simulationen auf Instabilitäten im Nachlauf der Blasen zurückgeführt werden, die zu einer periodischen Wirbelablösung führen. Im zweiten Teil der Dissertation wird der Aufstieg von Blasen in linearen Scherströmungen untersucht. Steigen die Blasen in einer vertikalen Scherströmung auf, so beobachtet man eine seitliche Migration. Diese seitliche Migration der Blasen wird durch die sogenannte Liftkraft verursacht, deren Vorzeichen und Betrag von der Blasengröße und den Stoffeigenschaften der Flüssigkeit abhängt. Die Simulationen zeigen, daß das Vorzeichen der Liftkraft für eher sphärische Blasen durch den Bernoulli-Effekt erklärt werden kann. An stark deformierten Blasen hingegen wirkt die Liftkraft in umgekehrter Richtung. Dieses Phänomen tritt auch in den Simulationen auf. Verschiedene Hypothesen für die Ursache dieses Phänomens werden überprüft. Die bekannteste experimentelle Korrelation für die Liftkraft von Tomiyama u.a. (2002) wird durch Simulation von realen Flüssigkeiten mit bekannten Stoffeigenschaften wie auch von Modellfluiden mit willkürlichen Stoffeigenschaften validiert und weitgehend bestätigt. Die Lift-Korrelation hat demnach hinsichtlich der Stoffeigenschaften der Flüssigkeit einen größeren Geltungsbereich, als bisher experimentell überprüft wurde. The simulations presented in this thesis were performed with the CFD code FS3D which is based on the Volume of Fluid method. The code is validated using analytical solutions for creeping flows and a good agreement is observed between simulation and analytical solution. In the first part of the thesis, the free rise of oil drops in water is simulated and compared with experimental observations. The results show that the rising velocities and the drag coefficients are similar in both cases, but the simulated drops are flatter (more oblate). This difference may be caused by impurities of the particle surface (surfactants) in the experiments. The simulations show that the transition from rectilinear to periodic trajectories is caused by instabilities in the wake, which lead to a periodic vortex shedding. In the second part of the thesis, the rise of bubbles in linear shear flows is investigated. If bubbles rise in a vertical shear flow, a lateral migration can be observed. This migration is caused by the so called lift force. Sign and magnitude of the lift force depend on the size of the bubble and the material properties of the liquid. The simulation results show that the sign of the lift force on spherical bubbles can be explained by the Bernoulli effect. However, the lift force on more distorted bubbles acts in the opposite direction. This phenomenon can also be observed in the simulation. In this work several hypotheses for the reason of this phenomenon are checked. Furthermore, most common correlation for the lift force (developed by Tomiyama et al. in 2002) is validated for fluids of known material and model fluids with arbitrary material data. The correlation is valid in a wider range of fluid material properties than proved experimentally up to now.