The idea that we live in a higher-dimensional space was first introduced almost 100 years ago. In the past two decades many extra-dimensional models have been proposed in order to solve fundamental problems of nature such as the hierarchy problem. Most of them need exploration via non-perturbative approaches and Lattice Gauge Theory provides a tool for doing this. In this thesis, we make attempts to find a non-perturbative way to localize gauge fields that arise from five-dimensional SU(2) gauge theories on 3-branes. In 1984, it was proposed that the phase diagram of anisotropic extra-dimensional lattice gauge theories inherits a new phase, called the "layered" phase, where the gauge fields behave as four-dimensional ones. This was shown for the abelian case, but the existence of this new phase for the simplest non-abelian group, SU(2), was still in doubt. We investigated this system in large volumes using Monte Carlo simulations and we could not find a second order phase transition from a five-dimensional to a continuous four-dimensional theory when all directions were kept large. This made the model unattractive for further exploration as nothing suggests that a non-trivial fixed point could exist. The above investigation was done in a flat background metric. We extended the previous work by putting our theory into a slice of AdS5 space, usually called the warped background. The motivation for this is that our SU(2) theory looks like the gauge-sector of the Randall-Sundrum model, which does not have a concrete solution to the problem of localization of the gauge fields on a 3-brane. We carried out our investigation using the Mean-Field Approach and we present novel results for the phase diagram and measurements of important observables. In our implementation we have a finite extent of the extra dimension and one layer (or 3-brane) on each extra-dimensional coordinate. At weak coupling, we observed that each layer decouples one at a time in the transition to the fully layered phase of the system, forming a mixed phase, whereas there is a strong and sharp transition between the fully layered and the strong-coupling phase. Within the mixed phase, close to the transition into the layered phase, we found evidence that the system is four-dimensional acquiring a Yukawa mass and resembling a Higgs-like phase. The mixed phase grows as the curvature increases suggesting that for an infinite extra dimension the entire weak-coupling phase is mixed.

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Frequency domain photon migration (FDPM) measurements are used to study the properties of dense colloidal dispersions with hard sphere and electrostatic interactions, which are otherwise difficult to analyze due to multiple scattering effects. Hard sphere interactions were studied using a theoretical model based upon a polydisperse mixture of particles using the hard sphere Percus Yevick theory. The particle size distribution and volume fraction were recovered by solving a non linear inverse problem using genetic algorithms. The mean sizes of the particles of 144 and 223 nm diameter were recovered within an error range of 0-15.53% of the mean diameters determined from dynamic light scattering measurements. The volume fraction was recovered within an error range of 0-24% of the experimentally determined volume fractions. At ionic strengths varying between 0.5 and 4 mM, multiple wavelength (660, 685, 785 and 828 nm) FDPM measurements of isotropic scattering coefficients were made of 144 and 223 nm diameter, monodisperse dispersions varying between 15% - 22% volume fraction, as well as of bidisperse mixtures of 144 and 223 nm diameter latex particles in 1:3, 1:1 and 3:1 mixtures varying between volume fractions of 15% - 24%. Structure factor models with Yukawa potential were computed by Monte Carlo (MC) simulations and numerical solution of the coupled Ornstein Zernike equations. In monodisperse dispersions of particle diameter 144 nm the isotropic scattering coefficient versus ionic strength show an increase with increasing ionic strength consistent with model predictions, whereas there was a reversal of trends and fluctuations for the particle diameter of 223 nm. In bidisperse mixtures for the case of maximum number of smaller particles, the isotropic scattering coefficient increased with increasing ionic strength and the trends were in conformity with MC simulations of binary Yukawa potential models. As the number of larger diameter particles increased in the dispersions, the isotropic scattering coefficients depicted fluctuations, and no match was found between the models and measurements for a number ratio of 1:3. The research lays the foundation for the determination of particle size distribution, volume fractions and an estimate of effective charge for high density of particles.

<p>As successful as the Standard Model has been in describing particle interactions, there are still many open questions it does not answer; the strong CP violation and the existence of dark matter among them. To address these issues many extensions to the Standard Model have been devised. Some of these extensions propose a new force mediating particle; a massive particle results in a potential described by a Yukawa-like interaction, while a massless exchange particle leads to power law type potentials. Limits on the strength of these interactions at the sub-micron range of separation between two particles are poorly characterized, but previous experiments conducted at IUPUI placed the best limits to date on the strength of a Yukawa-like interaction. Those experiments used a spherical test mass and a planar source mass. However, if a cylindrical test mass was used, the increased interaction volume of the cylinder would result in an increased sensitivity of about an order of magnitude over the spherical test mass experiment. Building such a system presents many challenges, namely the alignment of the cylinder with respect to the planar source mass. A capacitance based scheme to determine the alignment of a cylinder with respect to a plane will be discussed. The thesis concludes with an outline for a new type of measurement system. The new experiment attempts to induce a gravitational Π-pulse in a nanoshphere to probe extensions to the Standard Model.</p> <p> </p>

In dieser Arbeit berechnen wir die gravitativen Ein-Schleifen-Korrekturen zu den Propagatoren und Wechselwirkungen der Felder des Standardmodells der Elementarteilchenphysik. Wir betrachten hierzu ein höherdimensionales brane-world-Modell: Wärend die Gravitonen, die Austauchteilchen der Gravitationswechselwirkung, in der gesamten D-dimensionalen Raumzeit propagieren können, sind die Materiefelder an eine d-dimensionale Untermanigfaltigkeit (brane) gebunden. Um die divergenten Anteile der Ein-Schleifen-Diagramme zu bestimmen, entwickeln wir ein neues Regularisierungschema welches einerseits die Wardidentitäten der Yang-Mills-Theorie respektiert anderseits sensitiv für potenzartige Divergenzen ist. Wir berechnen die gravitativen Beiträge zu den beta-Funktionen der Yang-Mills-Eichtheorie, der quartischen Selbst-Wechselwirkung skalarer Felder und der Yukawa-Wechselwirkung zwischen Skalaren und Fermionen. Im physikalisch besonders interessanten Fall einer vier-dimensionalen Materie-brane verschwinden die gravitativen Beiträge zum Laufen der Yang-Mills-Kopplungskonstante. Die führenden Beiträge zum Laufen der anderen beiden Kopplungskonstanten sind positiv. Diese Ergebnisse sind unabhängig von der Anzahl der Extradimensionen in denen die Gravitonen propagieren können. Des Weiteren bestimmen wir alle gravitationsinduzierten Ein-Schleifen-Konterterme mit höheren kovarianten Ableitungen für skalare Felder, Dirac-Fermionen und Eichbosonen. Ein Vergleich dieser Konterterme mit den höheren Ableitungsoperatoren des Lee-Wick-Standardmodells zeigt, dass die Gravitationskorrekturen nicht auf letzte beschränkt sind. Eine Beziehung zwischen Quantengravitation und dem Lee-Wick-Standardmodell besteht somit nicht. / In this thesis, we derive the gravitational one-loop corrections to the propagators and interactions of the Standard Model field. We consider a higher dimensional brane world scenario: Here, gravitons can propagate in the whole D dimensional space-time whereas the matter fields are confined to a d dimensional sub-manifold (brane). In order to determine the divergent part of the one-loop diagrams, we develop a new regularisation scheme which is both sensitive for polynomial divergences and respects the Ward identities of the Yang-Mills theory. We calculate the gravitational contributions to the beta functions of non-Abelian gauge theories, the quartic scalar self-interaction and the Yukawa coupling between scalars and fermions. In the physically interesting case of a four dimensional matter brane, the gravitational contributions to the running of the Yang-Mills coupling constant vanish. The leading contributions to the other two couplings are positive. These results do not depend on the number of extra dimensions. We further compute the gravitationally induced one-loop counterterms with higher covariant derivatives for scalars, Dirac fermions and gauge bosons. In is shown that these counterterms do not coincide with the higher derivative terms in the Lee-Wick standard model. A possible connection between quantum gravity and the latter cannot be inferred.

Le but est d’explorer l’interaction entre les particules quantiques et la gravitation. On utilisera la quantification de Landau, l’effet Hall quantique et on examinera la relation entre la gravitation et l’effet Josephson. On propose une version de l’expérience "COW" (Colella-Overhauser-Werner) pour examiner les déviations de la loi du carré inverse de type Yukawa et de puissance inverse. Il est question de montages permettant d’investiguer la possibilité de mesurer le gravitomagnétisme et la constante de la gravitation G. On a examiné les transitions quantiques pour des neutrons ultra-froids (Ultra-Cold Neutron : UCN). Les résultats étaient satisfaisants pour 105 UCN. On a imaginé un effet laser avec ces neutrons émetteurs de gravitons : le phénomène est cependant très faible. Pour les corrections des niveaux de Landau : on a utilisé trois types d’espace-temps. Pour Schwarzschild, en utilisant une masse perturbatrice, les corrections d’ordres 1 et 2 dépendent du niveau n et du nombre quantique `. Cela enlève la dégénérescence des niveaux conventionnels. On obtient des résultats similaires pour les espaces-temps de Kerr et de Levi-Civita. On a proposé une expérience analogue à l’expérience COW. On a des déphasages malgré de faibles valeurs anticipées : de 10^−18 rad à 10^−4 rad pour le type Yukawa et de 10^−3 rad à 10^−9 rad pour puissance inverse. On a proposé des mesures possibles pour le gravitomagnétisme. On a aussi repris l’étude de l’influence de la gravitation sur l’effet Hall quantique. On obtient de faibles corrections pour un champ gravitationnel. On ne peut toutefois pas conclure à des quantités mesurables pour les déviations de type Yukawa et de puissance inverse. Par contre, on peut utiliser l’effet pour mesurer G avec grande précision. On a examiné l’effet Josephson sous l’effet de la gravitation en imaginant un montage simple. On a d’excellents résultats : des corrections de 10^−7 à 10^−9 Hz pour des déviations de type Yukawa et 10^−6 Hz pour des déviations en puissance inverse. Surtout, le lien entre la gravitation et la fréquence du courant de Josephson est clairement établit et mesurable. / The goal is to explore the interaction between quantum particles and gravitation. We will use Landau quantization, the quantum Hall effect and we will examine the relationship between gravity and Josephson’s effect. We propose a version of "COW" experience (Colella-Overhauser-Werner) to examine the Yukawa and inverse power deviations. We propose setups to investigate the possibility to measure gravitomagnetism and the gravitational constant G. Quantum transitions for ultra-cold neutrons (UCN) have been examined. The results were satisfactory for 105 UCN. We imagined a laser effect with these graviton emitting neutrons: the phenomenon is however very weak. For Landau level corrections: we proceeded with three types of space-times. For Schwarzschild, using a disturbing mass, the corrections of orders 1 and 2 depend on the level n and the quantum number "`". This removes the degeneracy of conventional levels. Similar results are obtained for the Kerr and the Levi-Civita spacetimes. We took over an analog of the COW experiment. We have phase shifts despite low expected values: from 10^−18 rad to 10^−4 rad for Yukawa and from 10^−3 rad to 10^−9 rad for inverse power laws. The same setup has been proposed for testing gravitomagnetism. We have also resumed the study of the influence of gravity on the quantum Hall effect. Small corrections are obtained for a gravitational field. We cannot however conclude with measurable quantities for Yukawa and inverse power laws. On the other hand, one can use the effect to measure G with great precision. We examined the Josephson effect under the effect of gravity by imagining a simple setup. We have excellent results: corrections from 10^−7 to 10^−9 Hz for Yukawa and 10^−6 Hz for inverse power law. Above all, the link between gravity and the frequency of Josephson’s current is clearly established and measurable.

Title: Electroweak symmetry breaking by dynamically generated masses of quarks and leptons Author: Adam Smetana Department: Institute of Particle and Nuclear Physics, Faculty of Mathematics and Physics, Charles University Supervisor: Ing. Jiří Hošek, DrSc., Department of Theoretical Physics, Nuclear Physics Institute, Academy of Sciences of the Czech Republic Abstract: The aim of the thesis is to study models of the electroweak symmetry breaking caused by dynamically generated masses of quarks and lep- tons. (1) We perform the basic analysis whether the main underlying idea, that the masses of only known fermions can provide the elec- troweak symmetry breaking, is actually feasible. For that we elaborate a two-composite-Higgs-doublet model of the top-quark and neutrino condensation. The model suggests rather large number, O(100), of right-handed neutrinos. (2) We analyze the model of strong Yukawa dynamics where the dynamical fermion mass generation is provided by exchanges of new elementary massive complex doublet scalar fields. We focus on solving the coupled Schwinger-Dyson equations for fermion and scalar self-energies by means of approximative methods. We doc- ument that strongly hierarchical mass spectra can be reproduced. (3) We elaborate the flavor gauge model where the dynamical fermion mass...