A search for diphoton events with large missing transverse energy is conducted using 3.1 pb^{-1} of integrated luminosity of proton-proton collisions at center of mass energy \sqrt{s}=7 TeV. The data were collected with the ATLAS detector at the CERN Large Hadron Collider during the period from March 30, 2010 until August 30, 2010. No excess of such events is observed above the Standard Model background prediction. This result is interpreted in the context of a gravity mediated One Universal Extra Dimension model with \Lambda R=20, N=6 and M_{D}=5 TeV, where \Lambda is the cutoff scale, N is the number of large extra dimensions and M_{D} is the Planck scale in the higher dimensional theory. The compactification radius of the Universal Extra Dimension, R, is excluded for values of 1/R < 728 GeV at 95\% CL, providing the most stringent limit on this model at the time of publication.

A search for diphoton events with large missing transverse energy is conducted using 3.1 pb^{-1} of integrated luminosity of proton-proton collisions at center of mass energy \sqrt{s}=7 TeV. The data were collected with the ATLAS detector at the CERN Large Hadron Collider during the period from March 30, 2010 until August 30, 2010. No excess of such events is observed above the Standard Model background prediction. This result is interpreted in the context of a gravity mediated One Universal Extra Dimension model with \Lambda R=20, N=6 and M_{D}=5 TeV, where \Lambda is the cutoff scale, N is the number of large extra dimensions and M_{D} is the Planck scale in the higher dimensional theory. The compactification radius of the Universal Extra Dimension, R, is excluded for values of 1/R < 728 GeV at 95\% CL, providing the most stringent limit on this model at the time of publication.

This thesis examines the possible creation of (4+n)-dimensional black holes at Large Hadron Collider (LHC) at CERN, consequent decays of such black holes via Hawking radiation and probable formation of Higgs boson among black hole decay products. Firstly, a theoretical background was presented including black hole physics, Hawking radiation, large extra dimensions, brane-bulk models, 4+n black holes and Higgs mechanism. Then, a simulation modeling black hole formation and decay including 130 GeV Higgs as a decay product at LHC interfaced with a detector simulation of Compact Muon Selenoid (CMS) was analysed focusing especially on the Higgs decay channels and properties of Hawking radiation. Both theoretical assumptions and simulation analysis point out that black hole production and the signatures of black hole decay products could carry crucial information on dimensionality and structure of spacetime Furthermore there is a significant possibility to observe 130 GeV Higgs boson especially in the Black Hole -&gt / H -&gt / jj and Black Hole -&gt / H &amp / #8211 / &gt / WW/ZZ -&gt / lnln decay channels.

Consideramos quatro modelos de branas, a saber, o modelo de Binétruy, Deffayet e Langlois com uma brana estática em um bulk dinâmico, o modelo de Chamblin e Reall para paredes de domínio dinâmicas, o modelo de brana estática em um espaço-tempo AdS contendo uma singularidade, e a generalização do último caso, isto é, o modelo de brana dinâmica em um bulk AdS ou dS contendo uma singularidade nua ou protegida. Das equações de Einstein e das condições de Darmois-Israel, estudamos a dinâmica da 4-brana nos casos pertinentes. Usando o formalismo de Euler-Lagrange, derivamos uma equação para o caminho mais curto em 5 e 6 dimensões. Aplicando esta equação, investigamos a possibilidade de se ter atalhos, verificando sua existência nos três últimos modelos. Calculamos os atrasos relevantes entre os sinais de gráviton e do fóton e a razão dos horizontes subentendidos correspondentes. As consequências são discutidas. / We consider four brane world models, namely, the modelo f Binétruy, Deffayet and Langlois with a static brane in a dynamical bulk, the modelo f Chamblin and Reall for dynamic domain dilatonic domain walls, the static brane model in na AdS spacetime containing a shielded singularity, and the generalization of the latter case, i.e., the dynamic brane model in na AdS or dS bulk containing a naked or shielded singularity. From the Einstein equations and the Darmois-Israel conditions we study the 4-brane dynamics in the pertinent cases. Using the Euler-Lagrange formalism we derive na equation for the shortest path in 5 and 6 dimensions. Applying this equation we investigate the possibility of having shortcuts verifying its existence in the three last models. We calculate the relevant delay between gráviton and photon sinals and the ratio of the corresponding subtended horizons. Consequences are discussed.

Light scalar fields such as axions and string moduli can play an important role in early-universe cosmology. However, many factors can significantly impact their late-time cosmological abundances. For example, in cases where the potentials for these fields are generated dynamically --- such as during cosmological mass-generating phase transitions --- the duration of the time interval required for these potentials to fully develop can have significant repercussions. Likewise, in scenarios with multiple scalars, mixing amongst the fields can also give rise to an effective timescale that modifies the resulting late-time abundances. Previous studies have focused on the effects of either the first or the second timescale in isolation. In this thesis, by contrast, we examine the new features that arise from the interplay between these two timescales when both mixing and time-dependent phase transitions are introduced together. First, we find that the effects of these timescales can conspire to alter not only the total late-time abundance of the system --- often by many orders of magnitude --- but also its distribution across the different fields. Second, we find that these effects can produce large parametric resonances which render the energy densities of the fields highly sensitive to the degree of mixing as well as the duration of the time interval over which the phase transition unfolds. Finally, we find that these effects can even give rise to a "re-overdamping" phenomenon which causes the total energy density of the system to behave in novel ways that differ from those exhibited by pure dark matter or vacuum energy. All of these features therefore give rise to new possibilities for early-universe phenomenology and cosmological evolution. They also highlight the importance of taking into account the time dependence associated with phase transitions in cosmological settings. In the second part of this thesis, we proceed to study the early-universe cosmology of a Kaluza-Klein (KK) tower of scalar fields in the presence of a mass-generating phase transition, focusing on the time-development of the total tower energy density (or relic abundance) as well as its distribution across the different KK modes. We find that both of these features are extremely sensitive to the details of the phase transition and can behave in a variety of ways significant for late-time cosmology. In particular, we find that the interplay between the temporal properties of the phase transition and the mixing it generates are responsible for both enhancements and suppressions in the late-time abundances, sometimes by many orders of magnitude. We map out the complete model parameter space and determine where traditional analytical approximations are valid and where they fail. In the latter cases we also provide new analytical approximations which successfully model our results. Finally, we apply this machinery to the example of an axion-like field in the bulk, mapping these phenomena over an enlarged axion parameter space that extends beyond those accessible to standard treatments. An important by-product of our analysis is the development of an alternate "UV-based" effective truncation of KK theories which has a number of interesting theoretical properties that distinguish it from the more traditional "IR-based" truncation typically used in the literature.

The vast majority of experiments in particle physics can be described by the Standard Model of particle physics (SM). However, there are indications for physics beyond it. The only experimentally demonstrated problem of the model is the difficulty to describe neutrino masses and leptonic mixing. There is a plethora of models that try to describe these phenomena and this thesis investigates several possibilities for new models, both full theories and effective frameworks.   The values of the parameters in a model are dependent on the energy scale and we say that the parameters run. The exact behavior of the running depends on the model and it provides a signature of the model. For a model defined at high energies it is necessary to run the parameters down to the electroweak scale in order to perform a comparison to the known values of observed quantities. In this thesis, we discuss renormalization group running in the context of extra dimensions and we provide an upper limit on the cutoff scale. We perform renormalization group running in two versions of a non-supersymmetric SO(10) model and we show that the SM parameters can be accommodated in both versions. In addition, we perform the running for the gauge couplings in a large set of radiative neutrino mass models and conclude that unification is possible in some of them.   The Higgs boson provides new possibilities to study physics beyond the SM. Its properties have to be tested with extremely high precision before it could be established whether the particle is truly the SM Higgs boson or not. In this thesis, we perform Bayesian parameter inference and model comparison. For models where the magnitude of the Higgs couplings is varied, we show that the SM is favored in comparison to all other models. Furthermore, we discuss lepton flavor violating processes in the context of the Zee model. We find that these can be sizeable and close to the experimental limits. / <p>QC 20170221</p>

Les extensions du Modèle Standard (MS) des particules sont maintenant dans une époque de développement très actif. Les motivations de l'introduction des dimensions supplémentaires sont basées d'une part sur la théorie des cordes qui nécessitent l'existence de nouvelles dimensions pour être cohérent. D'un autre côté ces théories peuvent potentiellement expliquer le problème de hiérarchie, le nombre de générations de fermions ou la stabilité du proton. La caractéristique commune de ces modèles est qu'ils fournissent une nouvelle particule neutre interagissant faiblement –un candidat idéal de la matière noire. Sa stabilité est préservée par la parité KK qui interdit les désintégrations du LKP en particules du MS. La géométrie de l'espace sous-jacent détermine le spectre de particules du modèle donc la masse et le spin du candidat DM, qui à leur tour jouent un rôle clé dans les études phénoménologiques. Nous présentons un modèle à deux dimensions supplémentaires universelles compactifiées sur le plan projectif réel. Cette géométrie particulière permet la définition des fermions chiraux et la stabilité de la matière noire neutre candidat dérive naturellement des propriétés intrinsèques de l'espace sans ajouter de nouvelles symétries ad hoc. Nous présentons le spectre de deux premiers niveaux KK à une boucle. Le spectre au sein de chaque niveau KK est fortement dégénéré ce qui fournit des signatures très intéressantes du modèle. Nous étudions la phénoménologie de la matière noire dans notre modèle pour limiter l'espace des paramètres en comparant nos résultats avec les données de WMAP et les expériences de détection directe. En utilisant les bornes obtenues, nous nous concentrons sur la phénoménologie LHC de notre modèle / The extra-dimensional extensions of the Standard Model of particles are now in a very active epoch of development. The motivations of introducing extra dimensions are based on one hand on string theories that require the existence of new dimensions to be consistent. On the other hand such theories can potentially explain the hierarchy problem, number of fermion generations, proton stability and other enigmas of the Standard Model. The common feature of these models is that they provide a new neutral weakly interacting particle - perfect candidate to the Dark Matter. Its stability is preserved by the so-called KK parity which prohibits the decays of the LKP into SM particles. The geometry of the underlying space determines the particle spectrum of the model, thus the mass and the spin of the DM candidate, which in turn plays the key role in the phenomenological studies We present a model with two universal extra dimensions compactified on a real projective plane. This particular geometry is chosen because chiral fermions can be defined on such orbifold and the stability of the neutral dark matter candidate arise naturally from the intrinsic geometrical properties of the space without adding any new symmetries ad hoc. We present the particle spectrum at loop order up to the second level in Kaluza-Klein expansion. The particularity of the spectrum is that the mass splittings within each KK level are highly degenerated providing a very interesting potential signatures in the LHC. We study the dark matter phenomenology in our model and constrain the parameter space by comparing our results with WMAP data and direct detection experiments. Using the obtained bounds we focus on the collider phenomenology of our model

The vast majority of all experimental results in particle physics can be described by the Standard Model (SM) of particle physics. However, neither the existence of neutrino masses nor the mixing in the leptonic sector, which have been observed, can be described within this model. In fact, the model only describes a fraction of the known energy in the Universe. Thus, we know there must exist a theory beyond the SM. There is a plethora of possible candidates for such a model, such as supersymmetry, extra dimensional theories, and string theory. So far, there are no evidence in favor of these models. These theories often reside at high energies, and will therefore be manifest as effective theories at the low energies experienced here on Earth. A first example in extra-dimensional theories. From our four-dimensional point of view, particles which propagate through the extra dimensions will effectivel be perceived as towers of heavy particles. In this thesis we consider an extra-dimensional model with universal extra dimensions, where all SM particles are allowed to propagate through the extra dimensions. Especially, we place a bound on the range of validity for this model. We study the renormalization group running of the leptonic parameters as well as the Higgs self-coupling in this model with the neutrino masses generated by a Weinberg operator. Grand unified theories, where the gauge couplings of the SM are unified into a single oe at some high energy scale, are motivated by the electroweak unification. The unification must necessarily take place at energies many orders of magnitude greater than those that ever can be achieved on Earth. In order to make sense of the theoru, ehich is given at the grand unified scale, at the electroweak scale, the symmetry at the grand unified scale is broken down to the SM symmetry. Within these models the SM is considered as an effective field theory. We study renormalization group running of the leptonic parameters in a non-supersymmetric SO(10) model which is broken in two steps via the Pati-Salam group. Finally, the discovery of the new boson at the LHC provides a new opportunity to search for physics beyond the SM. We consider an effective model where the magnitudes of the couplings in the Higgs sector are scaled by so-called coupling scale factors. We perform Bayesian parameter inference based on the LHC data. Furthermore, we perform Bayesian model comparison, comparing models where one or several of the Higgs couplings are allowed, to the SM, where the couplings are fixed. / <p>QC 20141020</p>

Aim: The overall aim was to create knowledge about what it means to live with bipolar disorder from an existential perspective, both for individuals with the diagnosis and for their close relatives.Method: An existential perspective in this context entails that it is explored and described from a lifeworld perspective of individuals who in various ways experience that which is termed as bipolar disorder. The lifeworld phenomenological approach Reflective Lifeworld Research (RLR) was used in the four empirical studies. Meaning-oriented interviews and analysis were conducted following the leading methodological principles of the chosen scientific approach. A synthesis, based on lifeworld hermeneutic existential philosophy, then presents how it is possible to understand the perspective of individuals with bipolar disorder and their close relatives as a coherent whole.Findings and conclusions: A magnitude and complexity of experiencing, which means that life with bipolar disorder is characterized by extra dimensions, specific tension and contradictions, has been elucidated. Knowledge of the meaning of these aspects enables for the persons with the illness and for their close relatives to understand, to put words to, and to communicate how their life is and what they need, which in turn enhances their ability to influence their lives. It also increases the opportunities for professional caregivers to develop care, both in content and organization, so that it can meet the actual needs of those concerned in an adequate way.Living with bipolar disorder means so much more than the usual description with changes between episodes of depression and mania. The diagnosis “bipolar disorder” thus appears to be an inadequate label that only reflects the more obvious and visible dimensions of the illness, while those that characterize life in its entirety remain hidden.The thesis also shows that the importance of the common everyday life of persons with bipolar disorder and their close relatives should be highlighted as the most important factor in a liveable existence. A change in the view of mental health care is thus needed; a change that is characterized by consensus, collaboration and transparent communication between the person with the illness, their close relatives and mental health care. The common goal should be about meeting actual needs, and to strengthen a profound connectedness in order to make everyday life more liveable. / Disputationen sker den 2012-11-16, Sal Myrdal, Hus K, Växjö, kl. 10:30.

Angular distributions of jet pairs (dijets) produced in proton-proton collisions at a centre-of- mass energy √s = 7 TeV have been studied with the ATLAS detector at the Large Hadron Collider using the full 2011 data set with an integrated luminosity of 4.8 fb−1, and reaching dijet masses up to 4.5 TeV. All angular distributions are consistent with QCD predictions. Analysis of the dijet angular distribution, using a novel technique simultaneously employing the dijet mass, is employed. This analysis is sensitive to both resonant new physics and phenomena with a slow-onset in mass. Using this technique, new exclusion limits have been set at 95% credibility level for several hypotheses of physics beyond the standard model including: quantum gravity scales, with 6 extra dimensions, below 4.11 TeV, quark contact interactions below a compositeness scale of 7.6 TeV, and excited quarks with a mass below 2.75 TeV. In a large and complex scientific experiment, such as ATLAS, the collection, management and usability of coherent data and metadata is a challenging operation. The availability of these data to physicists within the experiment is essential to all analysis efforts. A new web-based interface called “RunBrowser”, which makes ATLAS and LHC operations data available to the ATLAS Collaboration, is introduced.