This thesis is devoted to various questions connected with duality. It is composed of two parts.The first part discusses some aspects of timelike T-duality. We explore the possibility of compactification of supergravity theories with various signatures(low energy limit of M-theories which are dual under timelike T-dualities) on parallelizable internal seven dimensional (pseudo-)spheres. We show that, beside the standard theory, only one of the dual theories known as M'-theory can admit such a solution. The effective four dimensional theory is non-supersymmetric and due to the presence of torsion the symmetry of seven dimensional (pseudo-)sphere breaks down to Spin(3, 4). In the second part, in an attempt to have a systematic discussion of gaugings in supergravity, we show the isomorphism between the space of local deformations of the appropriate zero coupling limit of the embedding tensor Lagrangian and that of the second-order scalar-vector Lagrangian, describing the bosonic sector of supergravity ignoring gravity, in a chosen duality frame determined by embedding tensors. We analyze the BV-BRST deformation of a class of scalar-vector coupled Lagrangians, which contains supergravity Lagrangians as examples, and find a set of constraints that guarantee the consistency of the deformations of the Lagrangians. We show in principle that for a large class of theories considered in this thesis, the only deformations are those of the Yang-Mills type associated with a subgroup of the rigid symmetries. / Doctorat en Sciences / info:eu-repo/semantics/nonPublished

Orientador: Patricio Anibal Letelier Sotomayor / Tese (doutorado) - Universidade Estadual de Campinas, Instituto de Matematica, Estatistica e Computação Cientifica / Made available in DSpace on 2018-08-08T22:19:55Z (GMT). No. of bitstreams: 1 Rosa_ValeriaMattosda_D.pdf: 1232759 bytes, checksum: e4b5f9dd20a1bb1f521f2972b43bbfaf (MD5) Previous issue date: 2007 / Resumo: Várias soluções das equações de Einstein admitem curvas tipo-tempo fechadas (CTCs). Estudamos o comportamento deste tipo de curva quanto à estabilidade linear. Analisando as CTCs no universo de Gödel, encontramos que elas são linearmente estáveis, assim como as curvas desse tipo encontradas em um exemplo particular de métrica tipo-Gödel com fundo plano. As CTCs que aparecem no modelo contendo uma única corda cósmica girante também apresentam estabilidade linear. Estudamos todos os exemplos conhecidos de soluções das equações de Einstein que possuem geodésicas tipo-tempo fechadas (CTGs). Encontramos que a CTG apresentada pelos autores da solução dos dois perjeons não é linearmente estável, mas obtivemos condições, para os parâmetros desse modelo, sob as quais ela admite outras CTGs e, sob condições mais restritivas, obtivemos CTGs linearmente estáveis. As CTGs apresentadas por Soares em seu modelo topológico e por Grøn e Johannesen em seu modelo da núvem de cordas não possuem estabilidade linear. Já as CTGs de uma das soluções dada por van Stockum foram analisadas e verificamos que são linearmente estáveis. Encontramos CTGs em um exemplo particular de métrica tipo-Gödel com fundo conformemente plano, e estas também são estáveis. Analisamos, também, a deformação provocada pelo buraco negro de Schwarzschild ao ser colocado em um espaço-tempo com uma corda cósmica girante. Encontramos as CTGs desse espaço-tempo e determinamos as condições para que estas sejam estáveis / Abstract: Several solutions of Einstein¿s field equations admit closed timelike curves (CTCs). We study the linear stability of this kind of curve. We analyze the CTCs in Gödel universe and we find that these curves are stable. The same occurs with the CTCs of a particular case of Gödel-type metric with flat background and with CTCs of a model that contains a single spinning cosmic string. We study all known solutions of Einstein¿s equations that contain closed timelike geodesics (CTGs). We find that the CTG presented by Bonnor and Steadman in their model of two Perjeons is not stable under linear perturbations, but we present conditions to have stable CTGs in this model. The CTGs presented by Soares in his topological model and those presented by Grøn and Johannensen in their model of the cloud of strings are not stable. But, analizing the CTGs presented by Steadman in a solution gave by van Stockum, we conclude that these curves are stable. Besides these known CTGs, we find this kind of curve in a particular case of G¨odel-type metric with conformally flat background and we also find that they are stable. We also study the deformation that a Schwarzschild black hole causes in the spacetime of a single spinning cosmic string. We find the CTGs of this new spacetime and we determine conditions to have linear stability / Doutorado / Fisica-Matematica / Doutor em Matemática Aplicada

This project aims to study general relativity to the extent to understand the occurrence and behaviors of closed timelike curves (CTCs) in several exact solutions of Einstein’s field equations. The rotating black hole solution, the Gödel universe and the cosmic string solutions are studied in detail to show how CTCs arise in these spacetimes. The chronology-violationing paradoxes and other unphysical aspects of CTCs are discussed. The spacetimes where CTCs arise possess properties which are argumented to be unphysical, such as lack of asymptotic flatness and being innite models. With quantum computational networks it is possible to resolve the paradoxes which CTCs evoke. With all these attempts of resolving CTCs, our conclusion is that CTCs exist quantum mechanically, but there is a mechanism which inhibits them to be detected classically. / Detta projekt åsyftar att studera allmän relativitet i den grad att kunna förstå uppkomsten och företeelsen av tidsliknande slutna kurvor (CTC) i några exakta lösningar till Einsteins ekvationer. Dessa lösningar inkluderar Gödel universen, kosmiska strängar och det roterande svarta hålet, där CTC studeras i mer detalj. CTC är kronologi-kränkande företeelser och paradoxen som uppstår presenteras, samt de argument som ligger till grund till att CTC inte är fysikaliskt verkliga objekt. De tidrum där CTC uppkommer delar gemensamma egenskaper som anses ofysikaliska, som att vara icke asymptotiskt platta tidrum, samt att vara oändliga modeller. Med kvantinformatiska nätverk kan CTC illustreras och de klassiska kronologi-paradoxen kan rättas ut. Slutsatsen är att CTC existerar kvantmekaniskt, men det fnns en mekanism i verkligheten som förhindrar dessa att bli detekterade klassiskt.

In this paper, we study Bézier surfaces in View the MathML source three-dimensional Minkowski space. In particular, we focus on timelike and spacelike cases for Bézier surfaces. We also deal with the Plateau¿Bézier problem in View the MathML source, obtaining conditions over the control net to be extremal of the Dirichlet function for both timelike and spacelike Bézier surfaces. Moreover, we provide interesting examples showing the behavior of the Plateau¿Bézier problem in View the MathML source and illustrating the relationship between it and the corresponding Plateau¿Bézier problem in the Euclidean space R3.

No description available.

In this thesis properties of the G&ouml / del spacetime are analyzed and it is explicitly shown that there exist closed timelike curves in this spacetime. Geodesic motions for massive particles and light rays are investigated. One observes the focusing effect as a result of the solution of the geodesic equations. The time it takes for a free particle released from a point to come back to its starting point is calculated. A geometrical interpretation of the G&ouml / del spacetime is given and the question of what the G&ouml / del spacetime looks like is answered.

The existence and -if exists- the nature of the solutions of the scalar wave equation in spacetimes with closed timelike curves are investigated. The general properties of the solutions on some class of spacetimes are obtained. Global monochromatic solutions of the scalar wave equation are obtained in flat wormholes of dimensions 2+1 and 3+1. The solutions are in the form of infinite series involving cylindirical and spherical wave functions and they are elucidated by the multiple scattering method. Explicit solutions for some limiting cases are illustrated as well. The results of 2+1 dimensions are verified by using numerical methods.

Les travaux récents en fondements de la théorie quantique (des champs) et en information quantique relativiste tentent de mieux comprendre les effets des contraintes de causalité imposées aux opérations physiques sur la structure des corrélations quantiques. Le premier chapitre de cette thèse est consacré à l'étude des implications conceptuelles de la non-localité quantique, notion qui englobe celle d'intrication dans un sens précis. Nous détaillons comment les récentes approches informationnelles tentent de saisir la structure des corrélations non-locales, ainsi que les questions que ces dernières soulèvent concernant la capacité d'un observateur localisé à isoler un système de son environnement. Le second chapitre détaille les effets de l'invariance de Poincaré sur la détection et la quantification de l'intrication. Cette invariance impose que tous les systèmes soient modélisés en dernière instance dans le cadre de la théorie des champs, ce qui implique qu'aucun système à énergie finie ne puisse être localisé, ainsi que la divergence de toute mesure d'intrication pour des observateurs localisés. Nous fournissons une solution à ces deux problèmes en démontrant l'équivalence générique qui existe entre une résolution spatiale finie des appareils de mesure et l'exclusion des degrés de liberté de haute énergie de la définition du système observé. Cette équivalence permet une interprétation épistémique du formalisme quantique standard décrivant les systèmes localisés non-relativistes et leurs corrélations, clarifiant ainsi l'origine des mesures finies d'intrication pour de tels systèmes. Le dernier chapitre explore un cadre théorique récemment introduit qui prédit l'existence de corrélations quantiques sans ordre causal défini. Procédant par analogie avec le cas des corrélations non-locales, nous présentons quelques principes informationnels contraignant la structure de ces corrélations dans le but de mieux en comprendre l'origine physique. / Recent works in foundations of quantum (field) theory and relativistic quantum information try to better grasp the interplay between the structure of quantum correlations and the constraints imposed by causality on physical operations. Chapter 1 is dedicated to the study of the conceptual implications of quantum nonlocality, a concept that subsumes that of entanglement in a certain way. We detail the recent information-theoretic approaches to understanding the structure of nonlocal correlations, and the issues the latter raise concerning the ability of local observers to isolate a system from its environment. Chapter 2 reviews in what sense imposing Poincaré invariance affects entanglement detection and quantification procedures. This invariance ultimately forces a description of all quantum systems within the framework of quantum field theory, which leads to the impossibility of localized finite-energy states and to the divergence of all entanglement measures for local observers. We provide a solution to these two problems by showing that there exists a generic equivalence between a finite spatial resolution of the measurement apparatus and the exclusion of high-energy degrees of freedom from the definition of the observed system. This equivalence allows for an epistemic interpretation of the standard quantum formalism describing nonrelativistic localized systems and their correlations, hence a clarification of the origin of the finite measures of entanglement between such systems. Chapter 3 presents a recent theoretical framework that predicts the existence of correlations with indefinite causal order. In analogy to the information-theoretic approaches to nonlocal correlations, we introduce some principles that constrain the structure of such correlations, which is a first step toward a clear understanding of their physical origin.

Plus de quarante ans après la découverte de constituants ponctuels dans le nucléon, sa structure en quarks et gluons (partons) fait toujours l'objet d'études intenses. Certains processus exclusifs (où tous les produits de l'état final sont connus) de leptoproduction ou de photoproduction exclusive de photon ou de méson sur le nucléon permettent d'accéder aux Distributions de Parton Généralisées (GPDs). Ces fonctions paramétrisent la structure complexe du nucléon et contiennent des informations sur l'impulsion longitudinale et la position transverse des partons dans le nucléon. De tels processus exclusifs sont la Diffusion Compton Profondément Virtuelle "genre espace" et "genre temps" (DVCS et TCS respectivement) qui correspondent à la diffusion d'un photon de haute énergie sur un quark du nucléon et sont mesurés respectivement à partir des réactions lN⇾l'N'γ (N = proton ou neutron, l = lepton) et γN⇾N'l+l-. La première partie de cette thèse est une étude expérimentale du DVCS avec les données 2009 de l'expérience COMPASS au CERN. Dans un premier temps, la section efficace de diffusion profondément inélastique est mesurée, de façon à valider la mesure du flux de muons et à déterminer certains effets systématiques dans la recontruction des traces. Ensuite, la section efficace de production exclusive d'un photon est mesurée. Elle contient le processus DVCS (photon émis par un quark du nucléon) et le processus Bethe-Heitler (photon émis par le lepton diffusé) qui ont le même état final. L'étude des bruits de fond a aussi conduit à estimer une limite à la section efficace de production exclusive d'un pion neutre. La seconde partie de la thèse est dédiée à une étude phénoménologique du TCS aux énergies typiques de JLab 12 GeV. Les amplitudes du TCS et du Bethe-Heitler associé sont d'abord calculées. Puis, toutes les asymétries de simple et de double polarisation de la cible et/ou du faisceau linéairement ou circulairement polarisé sont calculées en fonction de diverses contributions de GPDs. Enfin, une méthode d'ajustement est présentée pour extraire les Facteurs de Forme Compton (qui sont des fonctions des GPDs) avec des données et/ou des simulations de DVCS et/ou de TCS. / More than forty years after the discovery of pointlike constituents inside the nucleon, its quarks and gluons structure is still intensively studied. Some exclusive processes (where all the final state products are known) of leptoproduction or of photoproduction of photon or meson off the nucleon provide access to the Generalized Parton Distributions (GPDs). These functions parameterize the complex structure of the nucleon and contain informations about the longitudinal momentum and the spatial transverse distribution of partons inside the nucleon. Such exclusive processes are the "Spacelike" and the "Timelike" Deeply Virtual Compton Scattering processes (DVCS and TCS respectively) which correspond to the scattering of a high-energy photon off a quark in the nucleon and are respectively measured in the reactions lN⇾l'N'γ (N = proton or neutron, l' = lepton) and γN⇾N'l+l- The first part of this thesis is devoted to the experimental study of DVCS, using the 2009 data from the COMPASS experiment at CERN. In a first step, the Deep Inelastic Scattering cross section is measured in order to check the muon flux measurement and to evaluate some systematic effects. Then, the cross section for the exclusive production of a photon is measured. It is made up of the DVCS process (the photon is emitted by a quark) and of the Bethe-Heitler process (the photon is emitted by the scattered lepton) which has the same final state. The study of the background has allowed to estimate in parallel an upper limit for the cross section of the exclusive production of a π° meson. The second part of the thesis is devoted to a phenomenological study of TCS at typical energies for the JLab 12 GeV upgrade. Firstly, the amplitudes for the TCS and for the associated Bethe-Heitler process are derived. Then, all single and double polarization (beam and/or target) observables are calculated as a function of different GPD contributions. Finally, a method is presented to extract the Compton Form Factors (functions of GPDs) from fits on DVCS and/or TCS data and/or simulations.