The field of real numbers does not permit a direct representation of the (improper) delta functions used for the description of impulsive (instantaneous) or concentrated (localized) sources. Of course, within the framework of distributions, these concepts can be accounted for in a rigorous fashion, but at the expense of the intuitive interpretation. The existence of infinitely small numbers and infinitely large numbers in the Levi-Civita field allows us to have well-behaved delta functions which, when restricted to the real numbers, reduce to the Dirac delta function. Here we develop the foundations for a mathematically rigorous theory of localized and instantaneous sources that has a clear and unambiguous way of specifying a mathematically concentrated source. We use the already existent one variable measure and integration theory on Levi-Civita field to construct the foundations of a measure and integration theory in two and three dimensions. First we construct measurable sets using sets with boundaries that can be expressed as analytic functions and we show the the resulting measure is Lebesgue-like. In particular we prove the measurability of countable sets, the countable union of measurable sets, and the finite intersection of measurable sets. Following that we use analytic functions to construct a larger class of measurable functions, we then define the integral of a measurable function over a measurable set. We prove several propositions regarding measurable functions and the associated integration theory including that the set of measurable functions is closed under multiplication and addition, and that integration is linear. This allows for a wide range of applications for the delta function in one, two, and three dimensions and sets the course for a more extensive study of this topic in the future.

Submitted by Johnny Rodrigues (johnnyrodrigues@ufcg.edu.br) on 2018-08-09T17:38:25Z No. of bitstreams: 1 JAMILLY LOURÊDO ROCHA - DISSERTAÇÃO PPGMAT 2014..pdf: 5707925 bytes, checksum: 8010cd451ac64c8a7fccc36a2f8313f6 (MD5) / Made available in DSpace on 2018-08-09T17:38:25Z (GMT). No. of bitstreams: 1 JAMILLY LOURÊDO ROCHA - DISSERTAÇÃO PPGMAT 2014..pdf: 5707925 bytes, checksum: 8010cd451ac64c8a7fccc36a2f8313f6 (MD5) Previous issue date: 2014-08 / Capes / Com uma aplicação adequada do conhecido princípio do máximo generalizado de Omori-Yau, obtemos resultados de rigidez com relação a hipersuperfícies imersas completascomcurvaturamédiadelimitadanoespaçohiperbólicoHn+1 (n+1)-dimensional. Em nossa abordagem exploramos a existência de uma dualidade natural entreHn+1 e a metade Hn+1 do espaço de SitterSn+11 , cujo modelo é chamado de steady state space. / As a suitable application of the well known generalized maximum principle of Omori-Yau, we obtain rigidity results concerning to a complete hypersurface immersed with bounded mean curvature in the (n+1)-dimensional hyperbolic spaceHn+1. In our approach, we explore the existence of a natural duality betweenHn+1 and the half Hn+1 of the de Sitter spaceSn+11 , which models the so-called steady state space.

Submitted by Johnny Rodrigues (johnnyrodrigues@ufcg.edu.br) on 2018-08-09T17:52:47Z No. of bitstreams: 1 CARLOS ANTONIO PEREIRA DA SILVA - DISSERTAÇÃO PPGMAT 2014..pdf: 597533 bytes, checksum: 741e2e32988fe89dd00df90b6aa0c5c9 (MD5) / Made available in DSpace on 2018-08-09T17:52:47Z (GMT). No. of bitstreams: 1 CARLOS ANTONIO PEREIRA DA SILVA - DISSERTAÇÃO PPGMAT 2014..pdf: 597533 bytes, checksum: 741e2e32988fe89dd00df90b6aa0c5c9 (MD5) Previous issue date: 2014-08 / Capes / Neste trabalho, como uma aplicação adequada do bem conhecido Princípio do Máximo Generalizado de Omori-Yau, obtemos resultados relativos a rigidez para hipersuperfícies tipo-espaço completas imersas na metade Hn+1 do espaço de De Sitter Sn+11 , que é chamado de steady state space. Por outro lado, usando uma isometria equivalente para o modeloHn+1, estenderemos nossos resultados a uma família maior de espaços-tempos. Por fim, estudaremos também a singularidade de gráficos verticais inteiros nesses espaços-tempos ambiente. / In this work, as a suitable application of the well known generalized Maximum Principle of Omori-Yau, we obtain rigidity results concerning to complete spacelike hypersurfaces immersed in the half Hn+1 of the de Sitter spaceSn+11 , which models the so-called steady state space. Moreover, by using an isometrically equivalent model for Hn+1, we extend our results to a wider family of spacetimes. Finally, we also study the uniqueness of entire vertical graphs in such ambient spacetimes.

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.