This thesis consists in a self-contained study of gauge/gravity dualities in the line of the Klebanov-Witten model. Here we explore first the known Maldacena duality that relates N=4 SYM theory in four dimensions to type IIB supergravity on AdS_5×S^5 in reasonable detail, after some necessary preliminaries on supersymmetric gauge theories, where we display in detail the supersymmetry algebra and representations for N 1 supersymmetry. There we also construct the so-called superfields that will be helpful to write invariant lagrangians for gauge theoriesmreadily, and then useful to construct the gauge theory side of the Klebanov-Witten model. In the original AdS/CFT correspondence and its phenomenologically interesting extensions, Dp-branes as solutions of supergravity and nonperturbative objects in string theory where gauge theory lives are crucial. So, to preserve the self-contained nature of this work, we include a brief review of superstring theory addressed to understand the need to include this higher-dimensional objects by T-duality and, at low-energy limit of the string theory, as solutions of the Einstein equations. The first climax of this work occurs when we use all we learned to establish the Maldacena conjecture, N=4 SU(Nc) SYM theory we study in the supersymmetry chapter, living on the four-dimensional worldvolume of a stack of Nc D3-branes in a flat-space, corresponds exactly to type IIB supergravity on AdS_5×S^5 .In order to prove it, we match symmetries and operators with states in both sides. But actually this corresponds to the weak form of the correspondence, because it is not possible to handle neither string theory or gauge theory at strong coupling. The focus and main motive to have to learn the first hundred of pages here will be to extend the dual gauge theory we studied in AdS/CFT towards more realistic gauge theories as duals of some supergravity theory. The Klebanov-Witten model, consists in replacing the five-sphere in the gravity background of type IIB for a more interesting Einstein manifold X5 , a coset space called T^1,1 .The resulting dual gauge theory is expected to be less supersymmetric, and it is indeed N = 1 superconformal field theory with matter content in the bifundamental representation of the gauge group SU(N)×SU(N), and a quartic superpotential that exhibits SU(2)×SU(2)×U(1) global symmetry, which is precisely the symmetry of the coset space in the gravity side. This is not the end of the story, the Klebanov-Witten model extended the Maldacena correspondence and found as a dual gauge theory a less supersymmetric but still conformal theory. Breaking of the conformal theory, proposed by Klebanov, Nekrasov and Tseytlin, is achieved by introducing fractional M D3-branes in addition to the N regular D3-branes. The resulting theory is an SU(N+M)×SU(N) gauge theory with N = 1 supersymmetry, no longer conformal and then a little more interesting as a part of the crusade to find a QCD-like theory. This is still not the end, the last model suffers from a singularity in the deep IR, rendering the gravitational description invalid in that regime. It was conjectured that the strong dynamics of the gauge theory should somehow resolve this problem. Klebanov, again, and Strassler showed that this conjecture was correct, and argue that the RG flow is in fact an infinite series of Seiberg duality transformations- a cascade - in which the number of colors repeatedly drops from N NM , so the gaugegroup changes from SU(N+M)×SU(N) to SU(NM) ×SU(N). This process can be repeated until the IR limit where the gauge group simply becomes SU(M). So, at the end we get a N=1 SU(M) gauge theory, a QCD-like theory. We say that the standard model itself may lie at the base of a duality cascade. / Essa tese consiste num estudo autocontido das dualidades calibre/gravidade na linha do modelo do Klebanov-Witten. Aqui nos exploramos primeiro de um jeito razoavelmente detalhado,a conhecida dualidade do Maldacena que relaciona a teoria N=4 SYM em quatro dimensões com as supercordas tipo IIB no espaço AdS_5×S^5, depois de alguns preliminares necessários sobre teorias supersimétricas de calibre, onde nós mostramos em detalhe à algebra supersimétrica e as representações para N 1 supersimetria. Nós também construímos os conhecidos supercampos que são úteis para escrever lagrangianas invariantes para teorias de calibre facilmente, e então serão úteis para construir a teoría de calibre do modelo de Klebanov-Witten. Na correspondência AdS/CFT original e as suas extensões fenomenologicamente interessantes, as Dp-branas, como soluções de supergravidade e objetos não perturbativos na teoria de cordas onde as teorias de calibre moram, são essenciais. Assim ,a fim de preservar a natureza autocontida desse trabalho, nós incluímos uma breve revisão sobre teoria de supercordas dirigida a entender a necessidade de incluir esses objetos extra-dimensionais usando dualidade-T e, no limite de baixa-energia da teoria de cordas, como soluções das equações de Einstein. O primeiro clímax desse trabalho ocorre quando nós usamos tudo o que aprendemos para estabelecer a conjectura do Maldacena, a teoria de calibre N=4 SYM que nós estudamos no capítulo de supersimetria, morando no volume de mundo quadridimensional de uma pilha de Nc D3-branas (sim, o subscrito c significa cor!) em espaço plano, corresponde exatamente à teoria de supergravidade tipo IIB no espaço AdS_5×S^5 . A fim de testar ela, nós identificamos simetrias e operadores com estados em ambos lados da dualidade. Mas na verdade isto corresponde à forma fraca da correspondência, porque não é possível lidar nem com a teoria de cordas nem com a teoria de calibre no limite de acoplamento forte. O foco e motivo principal de porque nós temos que aprender as primeiras cem páginas aqui, será estender a teoria de calibre dual que estudamos em AdS/CFT, para teorias de calibre mais realisticas como duais de alguma teoria de supergravidade. O modelo do Klebanov-Witten, consiste em substituir a esfera de cinco dimensões no fundo de supergravidade da teoria de supercordas tipo IIB por um espaço que é mais interessante X5, um espaço coset chamado T^1,1. Nós esperamos que a teoria de calibre dual que resulta é menos supersimetrica, e na verdade é N =1 superconforme com um conteúdo de matéria na representação bifundamental do grupo de calibre SU(N)×SU(N), e um superpotencial quártico que tem simetria global SU(2)×SU(2)×U(1), que é precisamente a simetria do espaço coset no lado da gravidade. Mas isso não é tudo, o modelo do Klebanov-Witten estendeu a correspondência do Maldacena e encontrou como teoria dual uma teoria menos supersimetrica mas ainda conforme. A quebra da simetria conforme, proposta pelo Klebanov, Nekrasov e Tseytlin, é obtida introduzindo M D3-branas fracionais além das N D3-branas regulares. A teoria resultante é uma teoria de calibre SU(N+M)×SU(N) com N = 1 supersimetria, não mais conforme e então um pouco mais interessante como parte da nossa cruzada para encontrar uma teoria tipo-QCD. Isso ainda não é o final, o modelo anterior sofre de uma singularidade no IR profundo, tornando inválido a descrição gravitacional. Foi conjeturado então que a dinâmica do acoplamento forte na teoria de gauge deveria de algum jeito resolver esse problema. Klebanov, de novo, e Strassler mostraram que essa conjetura foi correta, e argumentaram que o fluxo do GR é de fato uma serie infinita de transformações de dualidade de Seiberg - uma cascata - onde o numero de cores cai repetidamente de NNM, e o grupo de calibre muda de SU(N+M)×SU(N) a SU(NM)×SU(N). O processo pode ser repetido até o limite IV onde o grupo de calibre simplesmente torna-se SU(M). Então, no final nós obtemos uma N = 1 teoria de calibre SU (M ), ou seja uma teoria tipo-QCD. Então, nós dissemos que o modelo padrão mesmo pode se situar na base da cascata de dualidade.

L'objectif de cette thèse est de proposer de nouvelles approches plus efficaces pour améliorer la situation du trafic aérien dans l'Atlantique Nord (NAT). NAT est considéré comme l'espace aérien océanique le plus utilisé dans le monde. Le contrôle du trafic aérien dans cet espace confronte plusieurs difficultés dues aux différences de fuseaux horaires, aux demandes des passagers et aux vents forts induits par les jet-streams. De plus, la prédiction et le contrôle des trajectoire de vol sont très limités à cause de l'abscence de couverture radar. Par conséquent, une structure de routes, appelée Organized Track System (OTS), est établie dans le NAT et des normes de séparation très rigide sont imposés. Tous ces facteurs obligent les vols à suivre des trajectoires non optimales, ce qui influence négativement la consommation de carburant et le coût total du vol. Dans le cadre des projet lancé pour moderniser le systéme de gestion du trafic aérien, de nouvelles technologie de communication, de navigation et de surveillance ont été développés, l'un des plus prometteurs étant l'ADS-B. L'utilisation de l'ADS-B permet d'exploiter de nouvelles et différentes méthodes d'organiser le trafic, alternative à l'OTS, ce qui constitue l'axe principal de notre travail. Tout d'abord, nous étudions la possibilité d'introduire le Free Flight Concept (FFC) dans le NAT. En effet, nous proposons une nouvelle approche pour organiser le trafic aérien NAT en se basant sur un comportement d'essaim. En effet, le trafic est considéré comme un système Multi-Agent où tous les vols coopèrent, grâce à l'ADSB, afin de construire leurs trajectoires, tout en détectant et en résolvant les conflits entre eux. Les trajectoires résultantes sont efficaces en terme de temps de croisière. Cependant, ils ne sont pas robustes contre les changements du vents. Ensuite, nous proposons une nouvelle structure de route qui bénéficie du jet stream. Cette structure de route est appelée Wind-Optimal Track Network (WOTN), et est construite en considérant les normes de séparation réduites. WOTN couvre un plus grand espace aérien que l'OTS, afin de gérer un trafic plus dense. En gros, WOTN est construit de telle sorte que des pistes parallèles proches sont mis-en place pour suivre le jet- stream et les transitions entre les pistes n'est autorisé que dans les sections d'entrée et de sortie de la structure. Les résultats révèlent l'importance de mettre en place une structure de route afin de garantir des trajectoires robustes face aux vents forts. Enfin, nous proposons une approche permettant aux aéronefs de sortir en toute sécurité de la structure de la route en cas d'urgence. / The objective of the present thesis is to propose new more efficient trends to improve the air traffic situation over the North Atlantic (NAT) airspace. In fact, the NAT is considered to be the most congested oceanic airspace in the world. For many years, air traffic control in this airspace has experienced many difficulties caused by the time zone differences, passenger demands and strong winds induced by the jet streams. This leads to high congestion in the airspace especially at peak hours. Furthermore, flight trajectory prediction and control are very limited due to the lack of radar coverage in oceanic airspace. To support conflict-free flight progress, a structure of routes, called Organized Track System (OTS), is established in the NAT and very restrictive separation standards are applied. These rigid rules oblige flights to follow non-optimal trajectories, which negatively influences the fuel consumption and the total flight cost. In order to guarantee efficient traffic separation in the context of ever increasing trafic density, alternative means of communication, navigation and surveillance were developed and progressively be implemented, one of the most promising being the Automatic Dependent Surveillance-Broadcast (ADS-B). The widespread use of ADS-B makes it possible to organize traffic in new ways, as an alternative to the OTS, which is the main focus of the current work. First of all, we investigate the possibility of introducing the Free Flight Concept (FFC) in NAT. Indeed, we present an approach to construct and organize NAT traffic based on a swarm behavior. Here, the traffic is considered as a Multi-Agent system where all flights cooperate, thanks to ADS-B equipage, in order to construct their trajectories, while detecting and resolving conflicts between each other. The resulting trajectories are efficient in term of cruise time. However, they are not robust regarding changing winds. Next, we propose a new route structure for eastbound NAT traffic that benefit from the jet stream. This route structure is called Wind-Optimal Track Network (WOTN), and is constructed based on the reduced separation norms. WOTN covers larger airspace than the OTS, in order to handle the growing traffic. Roughly, WOTN is constructed in such a way that nearby parallel tracks are made to follow the jet streams and re-routing between tracks is only allowed in the input and output sections of the structure. Results reveal the importance of implementing a route structure in order to guaranty robust trajectories in the face of strong winds. Finally, we propose an approach to allow aircraft to safely exit the route structure in case of an emergency. The overall methodologies are implemented and tested with eastbound flight data over the NAT. We thereby produce conflict-free and robust trajectory planning for eastbound NAT flights, while benefiting from the reduced separation norms and the jet stream thus proving the efficiency of our approaches.

No description available.

With the rapid advancement of mobile devices, people have become more attached to them than ever. This rapid growth combined with millions of applications (apps) make smartphones a favourite means of communication among users. In general, the available contents on smartphones, apps and the web, come into two versions: (i) free contents that are monetized via advertisements (ads), and (ii) paid ones that are monetized by user subscription fees. However, the resources (energy, bandwidth, processing power) on-board are limited, and the existence of ads in either websites or free apps can adversely impact these resources. These issues brought the need for good understanding of the mobile advertising eco-system and how such limited resources can be efficiently used. This thesis focuses on mobile web browsing. Surfing web-pages on smatphones is one of the most commonly used task among smartphone users. However, web-page complexity is increasing, especially when designed for desktop computers. On one hand, the existence of ads in web-pages is essential for publishers' monetization strategy. On the other hand, their existence in webpages leads to even higher complexity of the webpages. This complexity in the smartphone environment, where the battery and bandwidth resources are limited, is reflected in longer loading time, more energy consumed, and more bytes transferred. With this view, quantifying the energy consumption due to web ads in smartphones is essential for publishers to optimize their webpages, and for system designers to develop an energy-aware applications (browsers) and protocols. Apart from their energy impact, ads consume network bandwidth as well. Therefore, quantifying the bandwidth consumption due to downloading web ads is crucial to creating more energy and bandwidth aware applications. This thesis first classifies web content into: (i) core information, and (ii) forced ``unwanted" information, namely ads. Then, describes an approach that enables the separation of web content in a number of a websites. Having done so, the energy cost due to downloading, rendering, and displaying web ads over Wi-Fi and 3G networks is evaluated. That is, how much energy web ads contribute to the total consumed energy when a user accesses the web. Furthermore, the bandwidth consumed by web ads in a number of well-known websites is also evaluated. Motivated by our findings about ads' impact on the energy and bandwidth, the thesis proposes and implements a novel web-browsing technique that adapts the webpages delivered to smartphones, based on a smartphone's current battery level and the network type. Webpages are adapted by controlling the amount of ads to be displayed. Validation tests confirm that the system, in some cases, can extend smartphone battery life by up to ~ 30\% and save wireless bandwidth up to ~ 44\%.

As an operational approach to the Bekenstein-Hawking formula S_{BH}=A/4l_{Pl}^{2} for the black hole entropy, we consider the reversible contraction of a spinning thin shell to its event horizon and find that its thermodynamic entropy approaches $S_{\mathrm{BH}}$. In this sense the shell, called a "black shell", imitates and is externally indistinguishable from a black hole. Our work is a generalization of the previous result [10] for the spherical case. We assume the exterior space-time of the shell is given by the Kerr metric and match it to two different interior metrics, a vacuum one and a non-vacuum one. We find the vacuum interior embedding breaks down for fast spinning shells. The mechanism is not clear and worth further exploring. We also examine the case of a Kerr-AdS exterior, without trying to find a detailed interior solution. We expect the same behavior of the shell when the horizon limit is approached.

As an operational approach to the Bekenstein-Hawking formula S_{BH}=A/4l_{Pl}^{2} for the black hole entropy, we consider the reversible contraction of a spinning thin shell to its event horizon and find that its thermodynamic entropy approaches $S_{\mathrm{BH}}$. In this sense the shell, called a "black shell", imitates and is externally indistinguishable from a black hole. Our work is a generalization of the previous result [10] for the spherical case. We assume the exterior space-time of the shell is given by the Kerr metric and match it to two different interior metrics, a vacuum one and a non-vacuum one. We find the vacuum interior embedding breaks down for fast spinning shells. The mechanism is not clear and worth further exploring. We also examine the case of a Kerr-AdS exterior, without trying to find a detailed interior solution. We expect the same behavior of the shell when the horizon limit is approached.

Submitted by FERNANDO ENRIQUE SERNA ALGARÍN null (ferse1129@gmail.com) on 2018-01-10T21:52:53Z No. of bitstreams: 1 tese.pdf: 948147 bytes, checksum: 94d535ccc424f5f4201747cae4382d6a (MD5) / Approved for entry into archive by Hellen Sayuri Sato null (hellen@ift.unesp.br) on 2018-01-12T15:54:08Z (GMT) No. of bitstreams: 1 algarin_fcs_dr_ift.pdf: 948147 bytes, checksum: 94d535ccc424f5f4201747cae4382d6a (MD5) / Made available in DSpace on 2018-01-12T15:54:08Z (GMT). No. of bitstreams: 1 algarin_fcs_dr_ift.pdf: 948147 bytes, checksum: 94d535ccc424f5f4201747cae4382d6a (MD5) Previous issue date: 2017-10-02 / Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) / Nesta tese empregamos um modelo de interação de contato que preserva simetrias para estudar estrututura hadrônica e matéria de quarks. A interação de contato é uma representação de kernels não perturbativos usados em equações de Dyson-Schwinger e Bethe-Salpeter da Cromodinâmica Quântica (QCD). A ideia básica do modelo está baseada num esquema de subtração que evita passos tradicionais no cálculo de de integrais divergentes que invariavelmente levam a violações de simetrias. Em temperatura zero, as equações de Dyson-Schwinger equation para os propagadores dos quarks u; d; s and c são resolvidas e amplitudes de estado ligado de Bethe-Salpeter, que respeitam a invariância sob translações espaço-temporais e as identidades de Ward-Takahashi associadas com simetrias globais da QCD, são obtidas para calcular as massas e as constantes de decaimento eletrofracas dos mésons pseudoscalares π; K, D e Ds e dos mésons vetorias ρ, K*, D* e Ds*. As predições do modelo estão em bom acordo com dados experimentais e da QCD na rede. Em adição, estendemos o modelo para temperaturas diferentes de zero; neste caso, o problema de violação de simetrias está restrito apenas às partes puramente divergentes porque os termos que dependem das distribuições térmicas são finitas e não requerem regularização. Finalmente, investigamos a dependência com a temperatura das contribuições das flutuações quânticas quark-π e quark-σ aos coeficientes de transporte de viscosidade de cisalhamento η e volumétrica ζ e as suas razões com a densidade de entropia s. As larguras térmicas originárias dessas fluctuações são calculadas com o formalismo de teoria de campos a temperatura finita de tempo real. Para esse cálculo, empregamos os resultados obtidos com as equações de Dyson-Schwinger e Bethe-Salpeter para a dependência com a temperatura das massas dos mésons e as contantes de acoplamento quark-méson. Os resultados para as razões η/s and ζ/s estão em bom acordo com resultados com a literatura obtidos com modelos e técnicas diferentes. Em particular, nossos resultados para η/s possuem um mínimo muito próximo ao limite inferior da conjectura AdS/CFT, η/s = 1/4π. / In thesis, a symmetry-preserving contact interaction model is used to study hadron structure and quark matter. The contact interaction is a representation of nonperturbative kernels used in Dyson-Schwinger and Bethe-Salpeter equations of Quantum Chromodynamics (QCD). The basic idea of the model is based on a subtraction scheme that avoids standard steps in the evaluation of divergent integrals that invariably lead to symmetry violation. At zero temperature, the Dyson-Schwinger equation is solved for the u; d; s and c quark propagators and the boundstate Bethe-Salpeter amplitudes respecting spacetime-translation invariance and the Ward-Green-Takahashi identities associated with global symmetries of QCD are obtained to calculate masses and electroweak decay constants of the pseudoscalar π; K, D and Ds and vector ρ, K*, D*, and Ds* mesons. The predictions of the model are in good agreement with available experimental and lattice QCD data. In addition, we extend the model to nonzero temperature; here, the problem of symmetry violation is associated only with the purely divergent parts because the effects due to the termal distributions are finite and do not need regularization. We compute the temperature dependence of the masses and decay constants of the pseudoscalar mesons considered here. Finally, we have investigated the temperature dependence of the contributions of quark-π and quark-σ quantum fluctuations to the transport coefficients of shear η and bulk ζ viscosities and their ratios to the entropy density s. The quark thermal widths originating those fluctuations are calculated with the formalism of real-time thermal field theory. For these calculations, we have used the results obtained via Dyson-Schwinger and Bethe-Salpeter equations for the temperature dependence of constituent quark and meson masses and quark-meson couplings. The results for the ratios η/s and ζ/s are in fair agreement with results of the literature obtained from different models and techniques. In particular, our result for η/s has a minimum very close to the conjectured AdS/CFT lower bound, η/s = 1/4π. / CNPq:140041/2014-1

SILVA, José Euclides Gomes da. Brane resolution em conifold com torção. 2010. 120 f. Dissertação (Mestrado em Física) - Programa de Pós-Graduação em Física, Departamento de Física, Centro de Ciências, Universidade Federal do Ceará, Fortaleza, 2010. / Submitted by francisco lima (admir@ufc.br) on 2014-03-20T14:00:30Z No. of bitstreams: 1 2010_dis_jegdasilva.pdf: 606336 bytes, checksum: 7d1080495b039a4501073a2c1711042a (MD5) / Approved for entry into archive by Edvander Pires(edvanderpires@gmail.com) on 2014-05-16T21:06:49Z (GMT) No. of bitstreams: 1 2010_dis_jegdasilva.pdf: 606336 bytes, checksum: 7d1080495b039a4501073a2c1711042a (MD5) / Made available in DSpace on 2014-05-16T21:06:49Z (GMT). No. of bitstreams: 1 2010_dis_jegdasilva.pdf: 606336 bytes, checksum: 7d1080495b039a4501073a2c1711042a (MD5) Previous issue date: 2010 / We will study a technique for smoothing a naked singularity in a conifold called Brane Resolution On the one hand the singularity appears as a brane solution of supergravity containing only terms of sector Neveu-Schwarz On the other hand we can see the singularity of the conifold as coming from a fixed point of the discrete symmetry group responsible for generating the conifold The conifold is of most importance in the process of compactification in string theories in particular in so-called conical transitions In fact there are different kinds Calabi-Yau varieties that can be built Despite such spaces have distint topological characteristics it can become a space on the other transitions through conical transitions This is done through the generation of singularities in Calabi-Yau that surprisingly does not generate quantum problems. The technique consists of adding a topological term sector Ramond-Ramond action to the inclusion of a Chern-Simons term responsible for interaction between the fields of the Ramond-Ramond sector (Cn), generates a flow field and H3 = DB2 F3 = DC2 on the singularity of the conifold. From the equation of motion of the field and an appropriate choice for the configuration of the metric and fields find the warp factors that are responsible for the removal of the singularity method can also be understood topologically as the incision of a sphere in the vicinity of the place node of the cone The behavior of fields on the conifold is done in order to extend the correspondence AdS-CFT correspondence was originally proposed for the space AdS5 × S 5 but soon emerged as extensions using other varieties M4 × C6 Near the natural perity space can be written as AdS5 5 × X 5 where X is the base of the conifold space usually takes up the space base as a homogeneous space of Ricci-flat Einstein where X = 5 SU (3) / SU (2) × SU (2). However, to maintain conformal invariance of the theory of dual fields is necessary to soften the conifold through incisions of the Eguchi-Hanson type that can be of two types: a 3-sphere S 3 is called deformation or by a 2-sphere S 2 is called resolution Recently it has been proposed resolutions conifold in a scenario of heterotic theory endowed with torsion Such an effect is relevant in theories where the black hole type solutions exist in the internal variety as the branes and spinning black branes latter takes into account the black hole's angular momentum - spin - and it is a solution of Kerr From the transgression of the Bianchi identity for the 3-form field strength of the Kalb-Ramond term derived from a Gauss-Bonnet and instanton can introduce a twist and hence a new term not dependent on the connection meter. We will study the effects of such terms on conifold a smoothing compared with the case without torsion Furthermore we study the effect that another term has topological branes on the resolution of the term BF This term originated as an extension of the Chern-Simons term to four dimensions with topologically generate mass function as gauge fields for this work, we modify the action of the heterotic theory in order to obtain the term BF as one of the terms fault and then responsible for the flow that removes the singularity found for an ansatz well known a configuration where the flow generated by the BF term is responsible for resolution / Estudaremos uma técnica de suavização de uma singularidade nua em um conifold chamada Brane Resolution Por um lado a singularidade aparece como uma solução de brana de supergravidade contendo apenas termos do setor de Neveu-Schwarz Por outro lado podemos ver a singularidade do conifold como oriunda de um ponto fixo do grupo de simetria discreto responsável pela geração do conifold O conifold tem bastante importância no processo de compactificação em teorias de cordas em particular nas chamadas transições cônicas De fato existem diferentes tipos de espaços deCalabi-Yau que podem ser variedades internas Apesar de tais espaços terem características to- pológicas distintas pode-se transformar um espaço no outro através das transições cônicas Isso se faz através da geração de singularidades no espaço de Calabi-Yau que surpreendentemente não gera problemas quânticos. A técnica consiste em acrescentar um termo topológico do setor de Ramond-Ramond à ação A inclusão de um termo de Chern-Simons responsável pela interação entre os campos do setor de Ramond-Ramond (Cn ), gera um fluxo dos campos H3 = dB2 e F3 = dC2 sobre a singularidade do conifold. A partir da equação de movimento do campo pode-se, dado uma escolha adequada para a configuração da métrica e dos campos, encontrar os fatores de warp que são responsáveis pela retirada da singularidade O método também pode ser entendido topologicamente como a incisão de uma esfera no lugar da vizinhança do nodo do cone O estudo do comportamento de campos sobre o conifold é feito no intuito de extender a correspondência AdS-CFT originalmente a correspondência foi proposta para o espaço AdS5 ×S 5 mas logo surgiram extensões utilizando outras variedades como M4 × C6 Próximo a singula- ridade o espaço pode ser escrito como AdS5 × X 5 onde X 5 é o espaço base do conifold Geralmente toma-se o espaço base como um espaço homogêneo de Einstein Ricci-plana onde X 5 = SU (3)/SU (2) × SU (2). Contudo, para manter a invariância conforme da teoria de campos dual é necessário suavizar o conifold através de incisões do tipo Eguchi-Hanson que podem ser de dois tipos: por uma 3-esfera S 3 é chamada deformation ou por uma 2-esfera S 2 é chamada resolution Recentemente foram propostas resoluções do conifold em um cenário de teoria heterótica dotada de torção Tal efeito é relevante em teorias onde soluções do tipo buraco negro existem na variedade interna como as black branes e spinning branes esta última leva em conta o momento angular do buraco negro - spin - e é uma solução do tipo Kerr A partir da transgressão da identidade de Bianchi para a 3-forma intensidade de campo de Kalb-Ramond oriundo de um termo de Gauss-Bonnet e de instanton podemos introduzir uma torção e com isso um novo termo na conexão não dependente da métrica. Estudaremos os efeitos de tais termos sobre a suavização de um conifold comparando com o caso sem torção Além disso buscamos estudar o efeito que um outro termo topológico tem sobre a resolução de branas o termo BF Tal termo surgiu como uma extensão do termo de Chern-Simons para quatro dimensões tendo como função gerar massa topologicamente para campos de calibre Nesse trabalho iremos modificar a ação da teoria heterótica de modo a obtermos o termo BF como um dos termos de anomalia e logo responsável pelo fluxo que retira a singularidade Encontramos para um ansatz bastante conhecido uma configuração onde o fluxo gerado pelo termo BF é o responsável pela desingularização do espaço

Les antennes reconfigurables offrent de multiples fonctions en changeant dynamiquement leurs propriétés telles que la fréquence de fonctionnement, la polarisation, le diagramme de rayonnement ou toute combinaison de ces trois paramètres. Leur agilité et leur diversité créent de nouvelles possibilités d'applications pour les systèmes radio tels que les réseaux locaux, les liaisons par satellite et notamment la radio cognitive. Dans cette thèse, deux antennes reconfigurables en fréquence fonctionnant dans les bandes des standards sans fil actuels ont été proposées. Elles sont basées sur la modification de la géométrie du patch rayonnant. Leurs dimensions ont été optimisées par algorithmes génétiques embarqués et combinés à un logiciel de simulation électromagnétique. La commande de la reconfiguration de ces antennes est réalisée à l'aide d'un microcontrôleur qui pilote l'état des commutateurs (des diodes PIN). De ce fait, un système d'antenne reconfigurable intelligent dédié à la radio cognitive a été développé. / Reconfigurable antennas offer multiple functions by dynamically changing their properties such as operating frequency, polarization, radiation pattern, and a combination of all these factors. Their agility and diversity create a wide range of different and new applications for radio systems such as local networks, satellites, and especially in cognitive radio. In this thesis, two new frequency reconfigurable antennas are proposed. The frequency reconfiguration is obtained by changing the geometry of radiating patch. Their dimensions have been optimized by genetic algorithm embedded in the electromagnetic simulation software. These antennas operate at the frequency band for IEEE 802.11b/g standard with satisfactory radiation characteristics. This thesis also presents a method of controlling the operation of the frequency reconfigurable antenna by a micro-controller. The operation of electronic switches (PIN diodes) are carried out through programs which allows an adaptive operating system like smart antennas and work well in cognitive radio environment.

En vue de permettre l'incinération des déchets nucléaires à vie longue, les réacteurs sous-critiques pilotés par accélérateur, plus communément dénommés ADS (Accelerator Driven System), sont l'une des solutions envisagées. Afin de permettre le monitorage de la puissance et donc le pilotage de tels systèmes, de multiples méthodes d'extraction de la réactivité ont été développées pendant les soixante dernières années. La méthode « kprompt », dernière en date, a démontré de multiples avantages et avait donné d'excellents résultats lors de l'expérience MUSE-4 dans le début des années 2000. Cette méthode, reposant sur la détermination de la distribution du temps de vie de fission intergénération, ne nécessite pas l'accès à la configuration critique pour la calibration (comme dans la méthode MSM) mais également l'investigation des taux de comptage sur de longs temps (comme dans la méthode des Aires). Sa robustesse, vis-à-vis de plusieurs facteurs physico-chimico-géométriques, a été éprouvée et confirmée pour le cas de l'expérience GUINEVERE. Par comparaison des résultats obtenus avec les méthodes usuelles de détermination de la réactivité, nous avons réussi à appliquer la méthode « kprompt » de façon satisfaisante aux différentes expériences dynamiques que sont les PNS et les Beam Trips. Finalement, suite à cette transposition de la méthode « kprompt » avec succès à l'expérience GUINEVERE, l'étape suivante consistera en son application au démonstrateur de puissance que sera le projet MYRRHA. / In order to allow the incineration of the long-lived nuclear wastes, the sub-critical reactors, more commonly named ADS (Accelerator Driven System), is one of the proposed solutions. To allow the monitoring of the power and therefore the control of such systems, several methods, developed during the last sixty years, give the reactivity. The last in date method, called « kprompt » method, has demonstrated many advantages and gave excellent results during the MUSE-4 experiment in the early 2000s. This method, based on the determination of the intergeneration fission lifetime distribution, does not require the access to the critical configuration for calibration (as for the MSM method) and the investigation of the counting rate on long times (as for the Area method). Its robustness, regarding several physical-chemical-geometrical factors, was tested and confirmed in the case of the GUINEVERE experience. By comparing the results obtained with the usual methods of reactivity determination, we applied adequately the « kprompt » method to the different dynamical experiments, the so-called PNS and Beam Trips. Finally, following the successfully transposition of the « kprompt » method to the GUINEVERE experience, the next step, in its application, will be to the power demonstrator MYRRHA.