Nesta tese, obtemos estados quânticos que satisfazem a equação de Schrödinger, para Hamiltonianos quadráticos de forma geral e, ao mesmo tempo, permitem de maneira natural obter a correspondência com a descrição clássica. Usamos o método de integrais de movimento para construir operadores de criação e aniquilação, que satisfazem a álgebra de Weyl-Heisenberg. Dessa forma, construímos os estados de número generalizados (ENG) de maneira análoga ao que é feito para os estados de Fock. Obtemos diferentes famílias de estados coerentes (EC), através de uma superposição dos ENG, que chamamos de estados coerentes generalizados (ECG). Esses estados são rotulados pela constante complexa z escrita em termos do valor esperado inicial da coordenada e do momento. Escrevemos os ECG em função do desvio padrão inicial na coordenada, $\\sigma_q$, de modo a minimizar a relação de incerteza de Heisenberg no instante de tempo inicial. Obtemos, de forma pioneira, os ECG para partícula livre e discutimos em detalhes suas propriedades, tal como a relação de completeza, a minimização das relações de incerteza e a evolução da correspondente densidade de probabilidade. Mostramos que o valor esperado da coordenada e do momento segue ao longo da trajetória clássica no espaço de fase. Mostramos que, quando o comprimento de onda da partícula livre é muito menor que $\\sigma_q$, os EC se comportam como estados semiclássicos. Além da partícula livre, construímos pela primeira vez, os ECG para o oscilador invertido e discutimos em detalhes suas propriedades. Mostramos que os ECG de sistemas diferentes podem ser relacionados, impondo condições sobre os parâmetros do Hamiltoniano. Por fim, consideramos Hamiltonianos dependentes do tempo, em particular, construímos os ECG, de forma exata, para um oscilador harmônico cuja frequência varia explicitamente no tempo. Mostramos ainda modelos úteis para obter solução exata de sistemas dependentes do tempo, fazendo analogia com a equação de spin ou equação de Schrödinger unidimensional independente do tempo. Além disso, desenvolvemos um método próprio, que fixa a solução e em seguida determinamos a forma da frequência. / In this thesis we obtain quantum states that satisfy the Schrödinger equation for quadratic Hamiltonians in the general form and at the same time allow, naturally, to obtain the correspondence with the classical description. For this, we use the method of integrals of motion to construct creation and annihilation operators, which satisfy the algebra of Weyl-Heisenberg. Thus, we obtain the generalized number states (GNS) in the same way that is done for the Fock states. We obtain diferent families of coherent states (CS) that we call generalized CS (GCS), by a superposition of GNS. These states are labeled by a complex constant z which is written in terms of the initial expected values of the coordinate and momentum. We write the GCS in terms of the initial standard deviation of the coordinate, $\\sigma_q$, which provides the minimization of Heisenberg uncertainty relation at the initial instant time. In particular, we obtain for the first time the GCS for the free particle and discuss in detail their properties, such as the completeness relation, the minimization of uncertainty relations, and the evolution of the corresponding probability density. We show that the expected values of coordinated and momentum propagate along the classical trajectory in phas espace. When the Compton wavelength is much smaller than $\\sigma_q$, the CS can be considered a semiclassical state. In addition to the free particle, we obtain for the first time the GCS for the inverted oscillator and discuss in detail their properties. We show that the GCS of diferent systems can be related by imposing conditions on the parameters of the Hamiltonian. Finally, we consider the time-dependent Hamiltonian, especially to obtain the GCS for a harmonic oscillator whose frequency varies explicitly in time. We also show useful models to obtain exact solution for time-dependent systems, by analogy with the spin equation or one-dimensionaltime-independent Schrödinger equation, as well as a method which consists first to find the solution and then determine the shape of the frequency.

Motiviert durch neuere Vorschläge zur experimentellen Untersuchung von Quantengravitationseffekten werden in der vorliegenden Arbeit Annahmen und Methoden untersucht, die für die Vorhersagen solcher Effekte im Rahmen der Loop-Quantengravitation verwendet werden können. Dazu wird als Modellsystem ein skalares Feld, gekoppelt an das Gravitationsfeld, betrachtet. <br /> Zunächst wird unter bestimmten Annahmen über die Dynamik des gekoppelten Systems eine Quantentheorie für das Skalarfeld vorgeschlagen. Unter der Annahme, dass sich das Gravitationsfeld in einem semiklassischen Zustand befindet, wird dann ein &quot;QFT auf gekrümmter Raumzeit-Limes&quot; dieser Theorie definiert. Im Gegensatz zur gewöhnlichen Quantenfeldtheorie auf gekrümmter Raumzeit beschreibt die Theorie in diesem Grenzfall jedoch ein quantisiertes Skalarfeld, das auf einem (klassisch beschriebenen) Zufallsgitter propagiert. <br /> Sodann werden Methoden vorgeschlagen, den Niederenergieliemes einer solchen Gittertheorie, vor allem hinsichtlich der resultierenden modifizierten Dispersonsrelation, zu berechnen. Diese Methoden werden anhand von einfachen Modellsystemen untersucht. <br /> Schließlich werden die entwickelten Methoden unter vereinfachenden Annahmen und der Benutzung einer speziellen Klasse von semiklassischen Zuständen angewandt, um Korrekturen zur Dispersionsrelation des skalaren und des elektromagnetischen Feldes im Rahmen der Loop-Quantengravitation zu berechnen. Diese Rechnungen haben vorläufigen Charakter, da viele Annahmen eingehen, deren Gültigkeit genauer untersucht werden muss. Zumindest zeigen sie aber Probleme und Möglichkeiten auf, im Rahmen der Loop-Quantengravitation Vorhersagen zu machen, die sich im Prinzip experimentell verifizieren lassen. / Motivated by recent proposals on the experimental detectability of quantum gravity effects, the present thesis investigates assumptions and methods which might be used for the prediction of such effects within the framework of loop quantum gravity. To this end, a scalar field coupled to gravity is considered as a model system. <br /> Starting from certain assumptions about the dynamics of the coupled gravity-matter system, a quantum theory for the scalar field is proposed. Then, assuming that the gravitational field is in a semiclassical state, a &quot;QFT on curved space-time limit&quot; of this theory is defined. In contrast to ordinary quantum field theory on curved space-time however, in this limit the theory describes a quantum scalar field propagating on a (classical) random lattice. <br /> Then, methods to obtain the low energy limit of such a lattice theory, especially regarding the resulting modified dispersion relations, are discussed and applied to simple model systems. <br /> Finally, under certain simplifying assumptions, using the methods developed before as well as a specific class of semiclassical states, corrections to the dispersion relations for the scalar and the electromagnetic field are computed within the framework of loop quantum gravity. These calculations are of preliminary character, as many assumptions enter whose validity remains to be studied more thoroughly. However they exemplify the problems and possibilities of making predictions based on loop quantum gravity that are in principle testable by experiment.

Nesta tese, obtemos estados quânticos que satisfazem a equação de Schrödinger, para Hamiltonianos quadráticos de forma geral e, ao mesmo tempo, permitem de maneira natural obter a correspondência com a descrição clássica. Usamos o método de integrais de movimento para construir operadores de criação e aniquilação, que satisfazem a álgebra de Weyl-Heisenberg. Dessa forma, construímos os estados de número generalizados (ENG) de maneira análoga ao que é feito para os estados de Fock. Obtemos diferentes famílias de estados coerentes (EC), através de uma superposição dos ENG, que chamamos de estados coerentes generalizados (ECG). Esses estados são rotulados pela constante complexa z escrita em termos do valor esperado inicial da coordenada e do momento. Escrevemos os ECG em função do desvio padrão inicial na coordenada, $\\sigma_q$, de modo a minimizar a relação de incerteza de Heisenberg no instante de tempo inicial. Obtemos, de forma pioneira, os ECG para partícula livre e discutimos em detalhes suas propriedades, tal como a relação de completeza, a minimização das relações de incerteza e a evolução da correspondente densidade de probabilidade. Mostramos que o valor esperado da coordenada e do momento segue ao longo da trajetória clássica no espaço de fase. Mostramos que, quando o comprimento de onda da partícula livre é muito menor que $\\sigma_q$, os EC se comportam como estados semiclássicos. Além da partícula livre, construímos pela primeira vez, os ECG para o oscilador invertido e discutimos em detalhes suas propriedades. Mostramos que os ECG de sistemas diferentes podem ser relacionados, impondo condições sobre os parâmetros do Hamiltoniano. Por fim, consideramos Hamiltonianos dependentes do tempo, em particular, construímos os ECG, de forma exata, para um oscilador harmônico cuja frequência varia explicitamente no tempo. Mostramos ainda modelos úteis para obter solução exata de sistemas dependentes do tempo, fazendo analogia com a equação de spin ou equação de Schrödinger unidimensional independente do tempo. Além disso, desenvolvemos um método próprio, que fixa a solução e em seguida determinamos a forma da frequência. / In this thesis we obtain quantum states that satisfy the Schrödinger equation for quadratic Hamiltonians in the general form and at the same time allow, naturally, to obtain the correspondence with the classical description. For this, we use the method of integrals of motion to construct creation and annihilation operators, which satisfy the algebra of Weyl-Heisenberg. Thus, we obtain the generalized number states (GNS) in the same way that is done for the Fock states. We obtain diferent families of coherent states (CS) that we call generalized CS (GCS), by a superposition of GNS. These states are labeled by a complex constant z which is written in terms of the initial expected values of the coordinate and momentum. We write the GCS in terms of the initial standard deviation of the coordinate, $\\sigma_q$, which provides the minimization of Heisenberg uncertainty relation at the initial instant time. In particular, we obtain for the first time the GCS for the free particle and discuss in detail their properties, such as the completeness relation, the minimization of uncertainty relations, and the evolution of the corresponding probability density. We show that the expected values of coordinated and momentum propagate along the classical trajectory in phas espace. When the Compton wavelength is much smaller than $\\sigma_q$, the CS can be considered a semiclassical state. In addition to the free particle, we obtain for the first time the GCS for the inverted oscillator and discuss in detail their properties. We show that the GCS of diferent systems can be related by imposing conditions on the parameters of the Hamiltonian. Finally, we consider the time-dependent Hamiltonian, especially to obtain the GCS for a harmonic oscillator whose frequency varies explicitly in time. We also show useful models to obtain exact solution for time-dependent systems, by analogy with the spin equation or one-dimensionaltime-independent Schrödinger equation, as well as a method which consists first to find the solution and then determine the shape of the frequency.

In this thesis, we study Schrödinger equations with an external magnetic field. In the first part, we are interested in an eigenvalue problem. We work in an open, bounded and simply connected domain in dimension two. We consider a magnetic potential singular at one point in the domain, and related to the magnetic field being a multiple of a Dirac delta. Those two objects are related to the Bohm-Aharonov effect, in which a charged particle is influenced by the presence of the magnetic potential although it remains in a region where the magnetic field is zero. We consider the Schrödinger magnetic operator appearing in the Schrödinger equation in presence of an external magnetic field. We want to study the spectrum of this operator, and more particularly how it varies when the singular point moves in the domain. We prove some results of continuity and differentiability of the eigenvalues when the singular point moves in the domain or approaches its boundary. Finally, in case of half-integer circulation of the magnetic potential, we study some asymptotic behaviour of the eigenvalues close to their critical points. In the second part, we study nonlinear Schrödinger equations in a cylindrically setting. We are interested in the semiclassical limit of the equation. We prove the existence of a semiclassical solution concentrating on a circle. Moreover, the radius of that circle is determined by the electric potential, but also by the magnetic potential. This result is totally new with respect to the ones before, in which the concentration is driven only by the electric potential. / Doctorat en Sciences / info:eu-repo/semantics/nonPublished