Les travaux de cette thèse portent sur une nouvelle structure de machine à double excitation (MSDE) pour l'application des véhicules hybrides et électriques. Ce type de machine, ayant deux sources d'excitation, bénéficie un degré de liberté supplémentaire et un contrôle facile sur le flux. Grâce à ce degré de liberté, la machine peut être dimensionnée de manière que son meilleur rendement coïncide avec la zone de fonctionnement la plus sollicitée de la machine. Cette nouvelle structure a fait l'objet principal de ce mémoire. Le fonctionnement de la MSDE est présenté dans les deux premiers chapitres. La machine est dimensionnée suivant un cahier des charges pour véhicule hybride. La validation expérimentale a confirmé le bon fonctionnement de la structure et montré son intérêt. Une autre problématique dans le dimensionnement de la machine est l'aspect thermique car les machines sont devenues de plus en plus compactes et puissantes. Une estimation correcte des pertes est indispensable pour évaluer correctement les performances de la machine. C'est la raison pour laquelle on a décidé de consacrer une partie de cette thèse à la modélisation des pertes fer, dont l'estimation n'est pas évidente. / The PhD work deals with a new structure of hybrid excited synchronous machine (MSDE) for the application of hybrid and electric vehicles. This kind of machine, with two excitation sources, benefits an additional degree of freedom and an easy control of flux. Due to this degree of freedom, the machine can be designed in the way that its best efficiency coincide with the most solicited operating zone. This new machine structure is the main subject of this study. The principle of this MSDE is presented in the first two chapters. The machine is then designed according to the specifications for an hybrid vehicle. The experimental validation has confirmed the proper functioning of the structure and shown its interest. Another important subject in the machine sizing is the thermal aspect because our machines are becoming more and more compact and powerful. A correct estimation of the iron loss is essential for evaluating correctly the machine performances. That's why we have decided to dedicate a part of this study to the modeling of iron loss, of which the estimation is not evident.

La modélisation numérique est devenue incontournable dans le monde de la conception industrielle et de la recherche scientifique. Les problèmes à résoudre étant de plus en plus complexes, il est nécessaire d'adopter une approche adaptée au problème traité. Dans les domaines d'application de l'électromagnétisme basses fréquences, la méthode des éléments finis (MEF) est la méthode de référence. Actuellement, de plus en plus de dispositifs ouverts comportant de grands entrefers sont développés. Dans ce genre de problèmes, la MEF n'est pas optimale car elle nécessite de mailler un grand volume d'air pour obtenir une bonne précision. Dans cette thèse nous étudions, au travers de deux applications (représentant respectivement un système ouvert et un système à grands entrefers) une méthode alternative qui ne souffre pas des limitations évoquées : la méthode des moments (MoM) de type intégrale volumique. En effet, cette méthode nécessite de mailler uniquement les milieux magnétiques. Le principe de cette méthode est d'abord de calculer l'aimantation induite dans le milieu linéaire ou non linéaire placé sous l'effet d'un champ extérieur. Pour cela, le milieu magnétique est discrétisé en éléments hexaédriques. Dans chaque élément est localisée une aimantation considérée comme uniforme. Ensuite, la connaissance de cette aimantation induite permet de déterminer le champ magnétique en tout point de l'espace: interne, proche ou lointain. Dans un premier temps, un code basé sur la MoM a été développé pour la première application. Il permet de calculer le champ magnétostatique proche ou lointain d'une antenne basse fréquence. Une méthode permettant de calculer l'énergie magnétostatique contenue dans tout l'espace a été également mise au point. Dans deuxième temps, afin de pouvoir traiter une géométrie complexe, des modifications ont été intégrées au code afin de modéliser la deuxième application : le dispositif de test des propulseurs à effet Hall (PPS-Flex). Il s'agit de prendre en compte des symétries géométriques et physiques caractéristiques de ce dispositif. Les résultats montrent que la MoM permet de calculer le champ magnétique à l'intérieur de son canal et éventuellement au-delà. Dans les deux exemples étudiés, la méthode des moments a donné des résultats satisfaisants lors de la comparaison avec la méthode des éléments finis 3D et avec les résultats de mesures. Ces résultats montrent des gains potentiellement significatifs sur le plan des temps de calculs. A l'issu de cette thèse, nous disposons d'un outil de laboratoire permettant de modéliser le comportement du champ magnétostatique dans des systèmes ouverts et/ou à grands entrefers. / The numerical modeling has become essential in the world of industrial design and scientific research. The problems to be solved are increasingly complex making it necessary to adopt an appropriate approach for the problem addressed. In the domains of application of low frequency electromagnetic, the finite element method (FEM) is the reference method. Currently, more and more devices having large open gaps are developed. In this kind of problems, the MEF is not optimal as it requires to mesh a large volume of air to get a good accuracy. In this thesis we study, through two applications (an open system and a large gap system), an alternative method that does not suffer from the limitations discussed: the method of moments (MoM) of volume integral type. Indeed, this method requires to mesh only the magnetic media. The principle of this method is first to calculate the induced magnetization in the linear or nonlinear medium under the effect of an external field. To accomplish this, the magnetic medium is discretized into hexahedral elements. In each element, a uniform magnetization is localized. Then, the determination of this induced magnetization allows to compute the magnetic field at any point in the space: internal, near or far. In the first step, a code based on the MoM has been developed for the first application. It allows to calculate the magnetostatic field near or far from a low-frequency antenna. A method to calculate the magnetostatic energy in the whole space was also developed. Meanwhile, in the second step, in order to treat complex geometry, some modifications have been integrated into the code to model the second application: the test device of Hall effect thrusters (PPS-Flex). It consists in taking into account the physical characteristics and geometric symmetry of the device. The results show that MoM allows to calculate the magnetic field inside the channel and possibly beyond. In both examples studied, the MoM has given satisfactory results when compared with the 3D finite element method and with the results of measurements. These results show potentially significant gains in the computation time. At the end of this thesis, we have developed a laboratory tool allowing to model the behavior of the static magnetic field in open and/or wide-gap systems.

La dissolution du dioxyde d’uranium en milieu nitrique est une étape clef du traitement des combustibles nucléaires usés. Elle précède en effet le procédé PUREX, qui permet l’extraction liquide - liquide des radionucléides valorisables. Cette dissolution est triphasique et autocatalytique, ce qui fait que de nombreux phénomènes impactent la réaction. Une bonne compréhension de ces phénomènes, autant à l’échelle microscopique que macroscopique, est nécessaire pour pouvoir proposer un modèle de la vitesse de disparition du solide au sein des dissolveurs. Les paramètres cinétiques de la réaction de dissolution ont été déterminés, en intégrant son aspect autocatalytique. L’étude cinétique a été réalisée en suivant la dissolution par microscopie optique. Cette technique d’analyse permet une approche uni-particulaire, qui est nécessaire car elle permet de limiter l’accumulation de l’espèce autocatalytique à l’interface solide – liquide. De plus, la dissolution du dioxyde d’uranium produit des oxydes d’azote. Une réaction volumique entre ces gaz et le catalyseur a été mise en évidence. Les cinétiques de cette réaction ont été estimées à partir des résultats expérimentaux. L’importance de la prise en compte des échanges à l’interface gaz – liquide pour définir la concentration de catalyseur en solution a été démontrée. Un modèle a été réalisé sur Matlab pour permettre de discriminer l’influence de ces différents éléments. Ce modèle donne des résultats cohérents avec l’expérimental, aussi bien à l’échelle microscopique que macroscopique. Plusieurs nombres adimensionnels ont également été mis en évidence pour cerner les phénomènes dont l’impact est prépondérant, en fonction de la géométrie et de l’hydrodynamique du dissolveur. Ce modèle a permis de cerner quelques pistes d’optimisation de procédés mettant en jeux des réactions autocatalytiques. Notamment, le fait que pour ces réactions particulières, les échanges aux interfaces solide - liquide et liquide - gaz peuvent être utilisés comme leviers pour maitriser la vitesse de disparition du solide / Recycling of nuclear fuel is based on liquid – liquid extraction. The dissolution of uranium dioxide in nitric medium is hence a key step at the head - end of the entire process. This particular dissolution is triphasic and autocatalytic, which means that numerous phenomena must be taken into account. A complete understanding of these phenomena, at macroscopic and microscopic scale, is necessary in order to model the solid disappearance rate in dissolvers. The kinetical parameters of the reaction were determined for both the catalyzed and non-catalyzed reactions. The kinetic study was realized thanks to a single particle approach. The reaction rates were measured by optical microscopy. This analytical technic enables to limit the catalyst accumulation at the solid - liquid interface. Moreover, nitrous oxides are products of the uranium dioxide dissolution. Evidence of a volumic reaction between these gases and the catalyst were found, and the kinetics of this reaction was estimated from the experimental results. Gas – liquid exchanges were shown to have an important impact on the catalyst concentration in the reactor. A model was realized thanks to the software Matlab to simulate these different phenomena. It was shown to be in good agreement with experimental results, at the microscopic and macroscopic scale. Dimensionless numbers were highlighted to describe the impact of each phenomenon on the solid disappearance, including the influence of the geometry and hydrodynamics of the reactor. Finally, ways of process optimization for autocatalytic reactions were determined thanks to the model. For instance, gas – liquid and solid – liquid exchanges were shown to be an interesting lever to fix the catalyst concentration in the reactor and at the solid surface

Submitted by Vasti Diniz (vastijpa@hotmail.com) on 2017-09-13T14:39:21Z No. of bitstreams: 1 arquivototal.pdf: 851323 bytes, checksum: 599a5da8bbbe70ff2f4ba121890878e2 (MD5) / Made available in DSpace on 2017-09-13T14:39:21Z (GMT). No. of bitstreams: 1 arquivototal.pdf: 851323 bytes, checksum: 599a5da8bbbe70ff2f4ba121890878e2 (MD5) Previous issue date: 2014-07-29 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES / In this cool thesis, we consider an approach to Brans-Dicke theory of gravity in which the scalar eld has a geometrical nature. By postulating the Palatini variation, we nd out that the role played by the scalar eld consists in turning the space-time geometry into a Weyl integrable manifold. This procedure leads to a scalar-tensor theory that di ers from the original Brans-Dicke theory in many aspects and presents some new features. We also consider the Weyl integrable geometry to investigate gravity in (2+1)-dimensions. We show that, in addition to leading to a Newtonian limit, WIST in (2+1) dimensions presents some interesting properties that are not shared by Einstein theory, such as geodesic deviation between particles in a dust distribution. Finally, taking advantage of the duality between the geometrical scalar-tensor theory and general relativity coupled with a massless scalar eld we study naked singularities and wormholes. / Esta tese trata de tópicos relacionados às teorias escalares-tensoriais e a geometria de Weyl integrável. Nossa abordagem será no sentido de indicar a geometria de Weyl integr ável como sendo um ambiente natural para a introdução de teorias escalares-tensorias. Nossa discussão será em torno da teoria de Brans-Dicke, considerada o protótipo das teorias escalares tensoriais, no entanto a discussão é facilmente estendida para essas versões mais gerais. Fazemos isso em dois momentos. Primeiro, indicando, no âmbito da teoria de Brans-Dicke, que na estrutura geométrica e de campos adotadas pela teoria existe uma relação estreita com a geometria de Weyl, inclusive associando o efeito descrito na literatura como "quinta força"(que violaria o princípio de equivalência) com o movimento geodésico da geometria de Weyl integrável, reformulando o postulado geodésico. E, num segundo momento, usando o método variacional de Palatini, acabamos por formular uma nova teoria escalar-tensorial, agora com ingredientes completamente geométricos, ambientada numa geometria de Weyl integrável. Estudamos ainda soluções no vazio do problema estático de uma distribuição de massa esfericamente simétrica, onde surgem objetos de interesse astrofísico como singularidades nuas e buracos de minhoca. Também formulamos a teoria conhecida por WIST (Weyl Integrable Spacetimes) em (2 + 1)D, o que resulta numa teoria consistente, não sofrendo das falhas associadas à teoria da relatividade geral nessa dimensionalidade

Submitted by Vasti Diniz (vastijpa@hotmail.com) on 2017-09-18T11:29:37Z No. of bitstreams: 1 arquivototal.pdf: 1956067 bytes, checksum: 845c3d0cd5113c8498d955af9cdcd907 (MD5) / Made available in DSpace on 2017-09-18T11:29:37Z (GMT). No. of bitstreams: 1 arquivototal.pdf: 1956067 bytes, checksum: 845c3d0cd5113c8498d955af9cdcd907 (MD5) Previous issue date: 2016-09-27 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES / In this thesis, we deal with a particular geometric scalar tensor theory, which is a version of the Brans-Dicke gravitation, formulated in aWeyl integrable space-time. This formulation is done using the Palatini's variation procedure. The main point of our work is to perform two particular applications of the geometrical Brans-Dicke theory. The rst one is the study of geometric fase transition phenomena, that's related to a continuous change in the space-time structure of the universe from a Riemann's geometry to a Weyl's geometry, or in the inverse sense, from Weyl's geometry to Riemann's geometry. This phenomena seems to take place when the universe starts to expand in a accelerated rate. The second one is the investigation of classical and quantum behaviour of a anisotropic n-dimensional universe . To nd solutions that display the dynamical compacti cation of non observed extra dimensions is the main motivation to study such universe. / Nesta tese, reapresentamos uma teoria escalar tensorial geométrica, que é uma versão da gravitação de Brans-Dicke formulada em um espaço-tempo de Weyl integrável. Com esta teoria fazemos duas aplicações especí cas. Uma delas para o estudo de um fenômeno, que chamamos de transição de fase geométrica, uma mudança contínua na estrutura geom étrica do espaço-tempo. Este fenômeno parece ocorrer quando o universo se expande aceleradamente. A segunda aplicação reside no estudo clássico e quântico do comportamento de um modelo de universo n-dimensional anisotrópico. A motivação para esta investigação é a busca de soluções que exibem o compactação dinâmica das dimensões extras, que não são observadas.

Submitted by Vasti Diniz (vastijpa@hotmail.com) on 2017-09-18T13:45:16Z No. of bitstreams: 1 arquivototal.pdf: 1340608 bytes, checksum: 8cceaa9c73ae05a5a903b4b78e3fa6ba (MD5) / Made available in DSpace on 2017-09-18T13:45:16Z (GMT). No. of bitstreams: 1 arquivototal.pdf: 1340608 bytes, checksum: 8cceaa9c73ae05a5a903b4b78e3fa6ba (MD5) Previous issue date: 2010-04-15 / Conselho Nacional de Pesquisa e Desenvolvimento Científico e Tecnológico - CNPq / It is presented a review on three subjects: the origin and nature of topological defects, the non-relativistic and relativistic quantum mechanics, and the gravitational and eletrostatic selfforces that emerge from a conical spacetime surrounding a cosmic string. After setting up this theoretical framework, it is studied the behavior of a charged particle in the presence of a cosmic string, parallel to an uniform, constant magnetic field, which may be used as a model to a primordial large-scale magnetic field that permeates the universe. The geometry of a negative disclination is taken into account, this being a typically condensed matter physics topological defect equivalent to a cosmic string, where a wedge of material is inserted into the lattice. We computed exactly, the topological and electrostatic influences on the particles energy spectrum, and the phase shift for the charged scalar particle scattered states. Switching to a flat-spacetime context, spherically symmetric systems were studied, solving exactly, Klein-Gordon and Dirac equations which describe a scalar particle subject to a Coulomb vector potential and scalar central potentials. / Apresentamos uma revisão sobre a origem e a natureza dos defeitos topológicos, que surgem a partir de transições de fase que podem ter ocorrido no início do processo de formação do universo; sobre a mecânica quântica não-relativística e relativística; e sobre as auto-forças gravitacional e eletrostática que emergem da topologia cônica do espaço-tempo gerado pela corda cósmica. Utilizando estas ferramentas, estudamos o movimento de uma partícula carregada na presença de uma corda cósmica, paralela a um campo magnético uniforme, de magnitude constante, que poderia servir de modelo para um campo magnético primordial. Também consideramos a geometria anti-cônica de uma desclinação negativa, defeito topológico análogo à corda cósmica estudado em matéria condensada. Calculamos, exatamente, a influência da topologia e do campo magnético no espectro de energia da partícula e encontramos o ângulo de mudança de fase para seus estados espalhados. No espaço-tempo plano, estudamos sistemas com simetria esférica e investigamos a dinâmica de uma partícula escalar, resolvendo, exatamente, as equações de Klein-Gordon e Dirac, considerando potenciais centrais.

The description of the effects of the wind meandering in the scalar dispersion is a challenging task, since this type of flow represents a physical state characterized by multiple scales. In this study, a Lagrangian stochastic diffusion model is derived to describe the scalar transport during the horizontal wind meandering phenomenon, occurring in a PBL. The model is derived from the linearization of the Langevin equation and employs a heuristic functional form, which represents the autocorrelation functions of the meandering. The new solutions, which describe the longitudinal and lateral wind components, were used to simulate two experiments of contaminants dispersion in low-wind conditions, INEL (USA) and GRAZ (Austria). The results of the comparison indicate that the new model reproduces fairly well the observed concentrations of contaminants and, therefore, satisfactorily describes the enhanced dispersion due to the presence of meandering. / Descrever os efeitos provocados pelo meandro do vento na dispersão de escalares é uma tarefa desafiadora, uma vez que este tipo de escoamento representa um estado físico caracterizado por múltiplas escalas. Neste trabalho, deriva-se um modelo estocátisco Lagrangiano para descrever a dispersão de escalares, na camada limite planetária, durante o fenômeno de meandro do vento horizontal. O modelo é derivado a partir da linearização da equação de Langevin e emprega uma forma funcional heurística, que representa as funções de autocorrelação do meandro. As novas soluções, que descrevem as componentes longitudinais e laterais do vento, foram empregadas para simular dois experimentos de dispersão de contaminantes em condições de vento fraco, INEL (USA) e GRAZ (Áustria). Os resultados das comparações indicam que o novo modelo pode ser usado para reproduzir as concentrações observadas de contaminantes e, portanto descreve de forma satisfatória a difusão reforçada provocada pelo meandro do vento.

Made available in DSpace on 2015-05-14T12:14:04Z (GMT). No. of bitstreams: 1 arquivototal.pdf: 639748 bytes, checksum: 09ac6e93733c265a01578d25967f780c (MD5) Previous issue date: 2009-10-02 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES / In this thesis, we develop some phenomenological aspects of a model based on the gauge symmetry SU(3)CNSU(3)LNU(1)N (311νR), that include righthanded neurinos in its matter content. We establish all the necessary structure for the study of the phenomenological aspects of the model. First, we obtain bounds on the angle that mix the gauge bosons Z and Z′, taking into account a requirement of the model, namely, that the number of fermionic families is exactly three. Also we implement the mass for both species of neutrinos (left-hand and right-handed) via type II seesaw mechanism, obtained adding to the model a sextet of scalars which will be responsible by the violation of the lepton number. The main consequence is the rising of a sterile neutrino with mass in the KeV range, satisfying all the cosmological and astrophysical constraints. This neutrino will a viable candidate for warm dark matter in the universe. / Nesta tese, desenvolvemos alguns aspectos relacionados `a fenomenologia de um modelo com simetria de gauge SU(3)CNSU(3)LNU(1)N (331νR), que possui neutrinos de m ao direita no seu conte´udo de mat´eria. Estabelecemos toda a estrutura necess´aria para o estudo dos aspectos fenomenol´ogicos do modelo. Primeiro, vamos obter v´ınculos no angulo que mistura os b´osons de gauge Z e Z′, levando em conta uma exig encia imposta pelo modelo, ou seja, que o n´umero de fam´ılias fermi onicas ´e exatamente tr es. Tamb´em implementamos termos de massa para ambas as esp´ecies de neutrinos (m ao esquerda e m ao dieita) via mecanismo seesaw tipo II, obtido adicionado ao modelo um sexteto de escalares, que ser´a respons ´avel pela viola¸c ao do n´umero lept onico. A principal consequ encia ´e o surgimento de um neutrino est´eril com massa na escala de KeV , satisfazendo todas as restri¸c oes cosmol´ogicas e astrof´ısicas. Esse neutrino ser´a um vi´avel candidato `a mat´eria escura morna do universo.

Made available in DSpace on 2015-05-14T12:14:11Z (GMT). No. of bitstreams: 1 arquivototal.pdf: 2344020 bytes, checksum: 1d77972a45b8beef7c3fe6631dfddaa2 (MD5) Previous issue date: 2014-02-28 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES / In this dissertation we consider the influence of gravitational fields due to the black holes of Kerr-Newman and Kerr-Newman-de Sitter, on a massive scalar field, with and without charge. We obtain the exact solutions of the radial Klein-Gordon equation in the spacetime of Kerr-Newman which are given in terms of the confluent Heun functions. In the particular case of a extreme Kerr-Newman black hole, the solution is given in terms of double confluent Heun functions. We also investigate the solutions close to the exterior event horizon and very far from the black hole. For a charged scalar field, we obtain exact solutions corresponding to the angular Klein-Gordon equation in the Kerr-Newman-de Sitter spacetime which are given in terms of the Heun functions. Using a method due to Damour and Ruffini, we study the Hawking radiation of massive scalar particles. In the Kerr-Newman black hole, we obtain the exact solutions for both the angular and radial Klein-Gordon equations, which are given in terms of the confluent Heun functions. From the radial solution, we obtain the exact wave solutions near to the exterior horizon of the black hole, and discuss the Hawking radiation of charged massive scalar particles. / Nesta dissertação tratamos da influência do campo gravitacional produzido pelos buracos negros de Kerr-Newman e Kerr-Newman-de Sitter sobre um campo escalar massivo com e sem carga. Obtemos as soluções exatas da parte radial da equação de Klein-Gordon em um espaço-tempo de Kerr-Newman, que são dadas em termos das funções confluentes de Heun. No caso particular correspondente ao buraco negro de Kerr-Newman extremo, a solução é dada em termos das funções duplamente confluentes de Heun. Investigamos, também, as soluções nas proximidades do horizonte de evento exterior e longe do buraco negro. Para um campo escalar massivo carregado, obtemos as soluções exatas para a parte angular da equação de Klein-Gordon em um espaço-tempo de Kerr-Newman-de Sitter, que são dadas em temos das funções de Heun. Utilizando o método de Damour & Ruffini, estudamos a radiação Hawking para partículas escalares massivas. No buraco negro de Kerr-Newman, obtemos as soluções exatas de ambas as partes radial e angular da equação de Klein-Gordon, que são dadas em termos das funções confluentes de Heun. A partir da solução radial, obtemos as soluções de ondas exatas próximas ao horizonte exterior do buraco negro e discutimos a radiação Hawking para partículas escalares massivas carregadas.

Made available in DSpace on 2015-05-14T12:14:12Z (GMT). No. of bitstreams: 1 arquivototal.pdf: 3660633 bytes, checksum: 7309d28729d29dd071bc87f7c5609ebc (MD5) Previous issue date: 2013-11-20 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES / The non-linear science is a central topic covering several investigation areas, such as biology, chemistry, mathematics and physics. In the first part of this thesis, we studied the non-linearity in the scope of classical field theory. The discussions are based on static solutions in (1, 1) space-time dimensions, and they are focused on kinks and lumps defects. In the related procedures, we show several techniques which allowed us to determine new models with their respective analytical solutions. The main mathematical tool to obtain these results is the so called deformation method, which was also an essential piece in the construction of a new extension method. This method presents the determination of new two scalar fields models from the coupling between two one scalar field systems. The method was analyzed carefully, as well as the linear stability, the zero modes, the total energy and the superpotentials, related with the new families of potentials. Furthermore, in the second part we presented the basics concepts about the Brownian Motion, where we analised the features of the solution of the Langevin Equation, and we also introduced a path integral approach to this problem in a quantum field theory way. / A ciência não-linear é tema central de diversas linhas de investigação, cobrindo áreas como a biologia, a física, a matemática e a química. Nossa primeira vertente de trabalho nesta tese, consiste no estudo de não-linearidades via abordagem de teoria clássica de campos. As discussões estão baseadas em soluções estáticas em (1, 1) dimensões, com destaque para o chamados defeitos tipo kink e lump. Nos procedimentos relatados, discorremos a respeito de diversas técnicas para a determinação de novos modelos com suas respectivas soluções analíticas. Um ferramental fundamental para a obtenção desses resultados é o chamado método de deformação, o qual também foi parte essencial para a criação de um método de extensão de modelos, onde visamos a construção de modelos de dois campos reais a partir do acoplamento entre dois modelos de um campo. Tal método também foi exposto em detalhes, bem como as análises sobre estabilidade linear, cálculo de modos zeros, determinação da energia total e dos superpotenciais, relativos às novas famílias de potenciais. Já a segunda linha de pesquisa, refere-se aos conceitos básicos do movimento browniano, onde analisamos as propriedades da solução da equação de Langevin, e na introdução de uma abordagem via integrais de trajetória para descrevê-lo nos moldes de teoria de quântica de campos.