Orientador: Marco Antonio Teixeira / Tese (doutorado) - Universidade Estadual de Campinas, Instituto de Matemática, Estatística e Computação Científica / Made available in DSpace on 2018-08-17T14:36:33Z (GMT). No. of bitstreams: 1 Martins_RicardoMiranda_D.pdf: 1398633 bytes, checksum: 5ac0dfa4d175b6407f0b574a1aefd3e5 (MD5) Previous issue date: 2011 / Resumo: Na primeira parte desta tese, estudamos a semelhança entre sistemas dinâmicos reversíveis e Hamiltonianos, sob um ponto de vista formal. Nos restringimos a sistemas definidos ao redor de pontos de equilíbrio simples e simétricos. Mostramos que, sob algumas hipóteses, tais sistemas são formalmente orbitalmente equivalentes. Na segunda parte, estudamos a existência de conjuntos minimais em certas famílias de equações diferenciais. Especificamente, exibimos condições sob as quais existem cilindros e toros invariantes para sistemas de equações que são perturbações de sistemas reversíveis. / Abstract: In the first part of this thesis, we study the similarity between reversible and Hamiltonian dynamical systems, from a formal viewpoint. We restrict ourselves to systems defined around an isolated and symmetric equilibria. We show that, under some conditions, such systems are formally orbitally equivalent to Hamiltonian vector fields. In the second part, we study the existence of minimal sets for some families of diferential equations. We obtain conditions for the existence of the invariant cylinders and tori for perturbed reversible systems. / Doutorado / Sistemas Dinamicos / Doutor em Matemática

Orientadores: Rodney Carlos Bassanezi, Adilson Jose Vieira Brandão / Tese (doutorado) - Universidade Estadual de Campinas, Instituto de Matematica, Estatistica e Computação Cientifica / Made available in DSpace on 2018-08-15T01:52:00Z (GMT). No. of bitstreams: 1 Cecconello_MoiseisdosSantos_D.pdf: 62393038 bytes, checksum: b7f0d1f9138d8e787749532bf661d026 (MD5) Previous issue date: 2010 / Resumo: Neste trabalho desenvolvemos ferramentas de análise qualitativa para sistemas dinâmicos definidos sobre o espaço formado pelos conjuntos fuzzy com a níveis compactos e não vazios. São propostas condições para existência de pontos de equilíbrio para o fluxo fuzzy cuja função de pertinência é sobrejetiva, generalizando alguns resultados já conhecidos. Os fluxos fuzzy considerados aqui são determinados pela extensão de Zadeh aplicada em soluções de equações diferenciais autônomas. São obtidos também condições para a existência de pontos e órbitas periódicas para o fluxo fuzzy. Em particular, demonstramos um teorema tipo Poincaré-Bendixson para tais fluxos gerados por equações autônomas bidimensionais. A análise qualitativa desenvolvida é aplicada em sistemas dinâmicos fuzzy provenientes de modelos significativos da Biomatemática. / Abstract: In this work we develop some tools for qualitative analysis of dynamical systems defined on the metric space of fuzzy sets with compact and nonempty a cuts. Conditions are offered for the existence of equilibrium points for the flow whose fuzzy membership function is surjective, generalizing some results already known. Fuzzy flows considered here are determined by Zadeh's extension applied in solutions of autonomous differential equations. We also obtained conditions for the existence of periodic points and periodic orbits for the fuzzy flow. In particular, we demonstrate a theorem like Poincaré-Bendixson for such flows generated by two-dimensional autonomous equations. The qualitative analysis results are applied to fuzzy dynamic systems from meaningful models of Biomathematics. / Doutorado / Biomatematica / Doutor em Matemática Aplicada

Submitted by Luciana Ferreira (lucgeral@gmail.com) on 2016-09-09T12:27:04Z No. of bitstreams: 2 Tese - Tharsis Souza Silva - 2016.pdf: 3242823 bytes, checksum: 4cdf7de6c7ba7cfe6f4fc07cc9501592 (MD5) license_rdf: 0 bytes, checksum: d41d8cd98f00b204e9800998ecf8427e (MD5) / Approved for entry into archive by Luciana Ferreira (lucgeral@gmail.com) on 2016-09-09T12:27:26Z (GMT) No. of bitstreams: 2 Tese - Tharsis Souza Silva - 2016.pdf: 3242823 bytes, checksum: 4cdf7de6c7ba7cfe6f4fc07cc9501592 (MD5) license_rdf: 0 bytes, checksum: d41d8cd98f00b204e9800998ecf8427e (MD5) / Made available in DSpace on 2016-09-09T12:27:26Z (GMT). No. of bitstreams: 2 Tese - Tharsis Souza Silva - 2016.pdf: 3242823 bytes, checksum: 4cdf7de6c7ba7cfe6f4fc07cc9501592 (MD5) license_rdf: 0 bytes, checksum: d41d8cd98f00b204e9800998ecf8427e (MD5) Previous issue date: 2016-05-13 / Fundação de Amparo à Pesquisa do Estado de Goiás - FAPEG / In this work we _rstly study a relay system X on the Rn that, under certain conditions, it has a one parameter family of 1-periodic orbits that arises in the origin and increase inde_nitely. We study yet another relay system class X_, that it is formed from the initial relay system by aditions of nilpotent parameters that, under certain conditions, it has the same result of the previous, and yet family of periodic orbits that arises in the origin and ends in a loop, or family that bifurcate of a loop and arise inde_nitelly. Furthermore the periodic solutions are explicitely given by Euler polynomials. Finally we study a third order di_erential equation with relay looking for periodic orbits of di_erent degrre of di_erentiability and this is done by the associated vector _eld with jump. / Neste trabalho estudamos primeiramente um campo vetorial descontínuo com chaveamento X atuando no Rn que, sob certas condições, possui uma família a um parâmetro de órbitas 1-periódicas que surge na origem e cresce indenidamente. Estudamos também uma classe de campos vetoriais descontínuos com chaveamento (relay systems) X, que se diferencía do campo inicial pela adição de parâmetros i;j de forma linear Nilpotente que, sob certas condições, possui o mesmo resultado que o caso anterior, e ainda famílias que surgem na origem e termina em um Laço ou mesmo que bifurcam de um laço e crescem indenidamente. Além disso as soluções periódicas são dadas explicitamente através dos polinômios de Euler. Ainda estudamos uma equação diferencial de terceira ordem com chaveamento a m de buscar órbitas periódicas de diferentes graus de diferenciabilidade e esse estudo é feito através do campo vetorial associado com impulso.

Neste trabalho, apresentamos um método computacional rigoroso para a demonstração de existência de órbitas periódicas de alguns sistemas de equações diferenciais ordinárias com campo autônomo do tipo polinomial. Mostraremos que o problema de encontrar órbitas periódicas para esses sistemas de equações é equivalente a buscar por raízes de certas funções definidas no espaço de Banach das sequências com decaimento algébrico. O método pode ser dividido em duas etapas. Na primeira, buscamos numericamente por soluções periódicas aproximadas. Na segunda, mostraremos a existência de uma órbita periódica numa vizinhança da curva encontrada numericamente. O rigor das verificações computacionais é garantido pelo uso de aritimética intervalar. / In this work, we present a rigorous computational method for proving the existence of periodic orbits of some systems of ordinary differential equations with autonomous vector field of polynomial type. We show that the problem of finding periodic orbits for these systems is equivalent to check for roots of certain functions defined in the Banach space of sequences with algebraic decay. The method can be divided into two steps. First, we seek, numerically, to approximated periodic solutions. Then, we show the existence of a periodic orbit in a neighborhood of the curve numerically found in the previous stage. The accuracy of the computational verifications is guaranteed by the use of interval arithmetic.

Le sujet de cette thèse est la question du nombre minimal d'orbites de Reeb distinctes sur une variété de contact qui est le bord d'une variété symplectique compacte.<p>L'homologie symplectique $S^1$-équivariante positive est un des outils principaux de cette thèse; elle est construite à partir d'orbites périodiques de champs de vecteurs hamiltoniens sur une variété symplectique<p>dont le bord est la variété de contact considérée.<p>Nous analysons la relation entre les différentes variantes d'homologie symplectique d'une variété symplectique exacte compacte (domaine de Liouville) et les orbites de Reeb de son bord.<p>Nous démontrons certaines propriétés de ces homologies.<p>Pour un domaine de Liouville plongé dans un autre, nous construisons un morphisme entre leurs homologies.<p>Nous étudions ensuite l'invariance de ces homologies par rapport au choix de la forme de contact sur le bord.<p>Nous utilisons l'homologie symplectique $S^1$-équivariante positive pour donner une nouvelle preuve d'un théorème de Ekeland et Lasry<p>sur le nombre minimal d'orbites de Reeb distinctes sur certaines hypersurfaces dans $R^{2n}$.<p>Nous indiquons comment étendre au cas de certaines hypersurfaces dans certains fibrés en droites complexes négatifs.<p>Nous donnons une caractérisation et une nouvelle façon de calculer l'indice de Conley-Zehnder généralisé, défini par Robbin et Salamon pour tout chemin de matrices symplectiques.<p>Ceci nous a mené à développer de nouvelles formes normales de matrices symplectiques.<p>/<p>This thesis deals with the question of the minimal number of distinct periodic Reeb orbits on a contact manifold which is the boundary of a compact symplectic manifold.<p>The positive $S^1$-equivariant symplectic homology is one of the main tools considered in this thesis.<p>It is built from periodic orbits of Hamiltonian vector fields in a symplectic manifold whose boundary is the given contact manifold.<p>Our first result describes the relation between the symplectic homologies of an exact compact symplectic manifold with contact type boundary (also called Liouville domain), and the periodic Reeb orbits on the boundary.<p>We then prove some properties of these homologies.<p>For a Liouville domain embedded into another one, we construct a morphism between their homologies.<p>We study the invariance of the homologies with respect to the choice of the contact form on the boundary.<p>We use the positive $S^1$-equivariant symplectic homology to give a new proof of a Theorem by Ekeland and Lasry about the minimal number of distinct periodic Reeb orbits on some hypersurfaces in $R^{2n}$.<p>We indicate how it extends to some hypersurfaces in some negative line bundles.<p>We also give a characterisation and a new way to compute the generalized Conley-Zehnder index defined by Robbin and Salamon for any path of symplectic matrices.<p>A tool for this is a new analysis of normal forms for symplectic matrices. / Doctorat en Sciences / info:eu-repo/semantics/nonPublished

Soit M une variété lisse fermée et considérons sont fibré cotangent T*M muni de la structure symplectique usuelle induite par la forme de Liouville. Une hypersurface S de T*M$ est dite étoilée fibre par fibre si pour tout point q de M, l'intersection Sq de S avec la fibre au dessus de q est le bord d'un domaine étoilé par rapport à l'origine 0q de la fibre T*qM. Un flot est naturellement associé à S, il s'agit de l'unique flot généré par le champ de Reeb le long de S, le flot de Reeb. <p><p>L'existence d'une orbite orbite fermée du flot de Reeb sur S fut annoncée par Weinstein dans sa conjecture en 1978. Indépendamment, Weinstein et Rabinowitz ont montré l'existence d'une orbite fermée sur les hypersurfaces de type étoilées dans l'espace réel de dimension 2n. Sous les hypothèses précédentes, l'existence d'une orbite fermée fut démontrée par Hofer et Viterbo. Dans le cas particulier du flot géodésique, l'existence de plusieurs orbites fermées fut notamment étudiée par Gromov, Paternain et Paternain-Petean. Dans cette thèse, ces résultats sont généralisés. <p><p>Les résultats principaux de cette thèse montrent que la structure topologique de la variété M implique, pour toute hypersurface étoilée fibre par fibre, l'existence de beaucoup d'orbites fermées du flot de Reeb. Plus précisément, une borne inférieure de la croissance du nombre d'orbites fermées du flot de Reeb en fonction de leur période est mise en évidence. /<p><p>Let M be a smooth closed manifold and denote by T*M the cotangent bundle over M endowed with its usual symplectic structure induced by the Liouville form. A hypersurface S of T*M is said to be fiberwise starshaped if for each point q in M the intersection Sq of S with the fiber at q bounds a domain starshaped with respect to the origin 0q in T*qM. There is a flow naturally associated to S, generated by the unique Reeb vector field R along S ,the Reeb flow. <p><p>The existence of one closed orbit was conjectured by Weinstein in 1978 in a more general setting. Independently, Weinstein and Rabinowitz established the existence of a closed orbit on star-like hypersurfaces in the 2n-dimensional real space. In our setting the Weinstein conjecture without the assumption was proved in 1988 by Hofer and Viterbo. The existence of many closed orbits has already been well studied in the special case of the geodesic flow, for example by Gromov, Paternain and Paternain-Petean. In this thesis we will generalize their results.<p><p>The main result of this thesis is to prove that the topological structure of $M$ forces, for all fiberwise starshaped hypersurfaces S, the existence of many closed orbits of the Reeb flow on S. More precisely, we shall give a lower bound of the growth rate of the number of closed Reeb-orbits in terms of their periods. / Doctorat en Sciences / info:eu-repo/semantics/nonPublished

Ce mémoire de maîtrise porte sur les billards mathématiques et la distribution des points de réflexion des trajectoires périodiques d’une table de billard strictement convexe. Un billard mathématique est un système dynamique généré par le mouvement libre d’une particule à l’intérieur d’un domaine dont la frontière est parfaitement réfléchissante. Une question d’intérêt particulier dans l’étude des billards mathématiques est celle de ses trajectoires périodiques. Nous considérons le cas des billards planaires strictement convexes. Il est connu que les points de réflexion des trajectoires périodiques de période n faisant un tour de table sont équidistribués par rapport à une mesure naturelle sur la frontière. Nous montrons ce résultat par une méthode nouvelle et relativement élémentaire utilisant la théorie de Lazuktin [12]. Dans le premier chapitre, nous donnons une description précise de la dynamique des billards et une brève introduction à la théorie de Lazuktin, aux applications de torsion et aux caustiques. Dans les chapitres 2 à 4, nous développons chacun des concepts précédents et expliquons comment ceux-ci sont liés aux billards. Le chapitre 5 est consacré à la preuve de notre résultat principal, divisée en deux parties. Nous concluons en donnant une annexe sur la théorie de la mesure. / This master’s thesis is concerned with mathematical billiards and distribution of reflection points of periodic trajectories of a strictly convex billiard table. A mathematical billiard is a dynamical system generated by the free motion of a particle inside of a domain with a perfectly reflecting boundary. A question of particular interest in the study of mathematical billiards is that of its periodic trajectories. We consider the case of planar strictly convex billiards. It is known that the reflection points of periodic trajectories of period n making one turn around the table are equidistributed with respect to a natural measure on the boundary. We show this result by a new and relatively elementary method using Lazuktin’s theory [12]. In the first chapter, we give a precise description of billiard dynamics and a brief introduction of Lazuktin’s theory, twist mappings and caustics. In Chapter 2 to 4, we elaborate each of the previous concepts and explain how they are related to billiards. Chapter 5 is dedicated to the proof of our main result, divided into two parts. We conclude by giving an appendix about measure theory.

<p dir="ltr">In the pursuit of establishing a sustainable space economy within the cislunar region, it is vital to formulate transfer design strategies that uncover economically viable highways between different regions of the space domain. The inherent complexity of spacecraft dynamics in the cislunar space poses challenges in determining feasible transfer options. However, the motion characterized by known dynamical structures modeled through the circular restricted three-body problem (CR3BP) aids in the identification of pathways with reasonable maneuver costs and flight times. A framework is proposed that incorporates a quasi-periodic orbit (QPOs) as an option to design transfer scenarios. This investigation focuses on the construction of transfers between periodic orbits. The framework is exemplified by the construction of pathways between an L2 9:2 synodic resonant Near-Rectilinear Halo Orbit (NRHO) and a planar Moon-centered Distant Retrograde Orbit (DRO). The innate difference in the geometries of the departure and arrival orbits of the sample case, along with the lack of natural flows towards and away from them, imply that links between these orbits may necessitate costly maneuvers. A strategy is formulated that leverages the stable and unstable manifolds associated with intermediate periodic orbits and quasi-periodic orbits to construct end-toend trajectories. As part of this strategy, a systematic methodology is outlined to streamline the determination of transfer options provided by the 5-dimensional manifolds associated with a QPO family. This approach reveals multiple local basins of solutions, both interior and exterior-types, characterized by selected intermediate orbits. The construction of transfers informed by the manifolds associated with QPOs is more intricate than those based on periodic orbits. However, QPO-derived solutions allow for the recognition of alternative local basins of solutions and often offer more cost-effective transfer options when compared to trajectories designed using periodic orbits that underlie the QPOs.</p>

Στην παρούσα διατριβή ασχολούμαστε με την μελέτη περιοδικών και ασυμπτωτικών λύσεων στο περιορισμένο πρόβλημα των τεσσάρων σωμάτων. Πιο συγκεκριμένα: Στο κεφάλαιο 1 περιγράφουμε το πρόβλημα των τριών και των τεσσάρων σωμάτων, κάνοντας μια ιστορική αναδρομή και παραθέτουμε τις αρχικές εξισώσεις της κίνησης. Στο κεφάλαιο 2 μελετάμε αριθμητικά το περιορισμένο πρόβλημα των τεσσάρων σωμάτων, στην Lagrangian διαμόρφωση. Υπολογίζουμε τα σημεία ισορροπίας, καθώς και τις επιτρεπτές περιοχές κίνησης του τέταρτου σώματος. Στο κεφάλαιο 3 μελετάμε την ευστάθεια των σημείων ισορροπίας. Επίσης υπολογίζουμε και παρουσιάζουμε τις περιοχές έλξης, για το δυναμικό σύστημα των τεσσάρων σωμάτων. Στο κεφάλαιο 4 μελετάμε οικογένειες απλών συμμετρικών και μη συμμετρικών περιοδικών τροχιών του περιορισμένου προβλήματος των τεσσάρων σωμάτων. Υπολογίζουμε για κάθε περίπτωση τιμών των μαζών, σειρές κρίσιμων περιοδικών τροχιών κάθε οικογένειας ξεχωριστά. Τέλος στο κεφάλαιο 5 μελετάμε αριθμητικά οικογένειες απλών ασύμμετρων περιοδικών τροχιών στο περιορισμένο πρόβλημα των τεσσάρων σωμάτων, έχοντας θέσει ως πρωτεύοντα σώματα τους ΄Ηλιο - Δία και έναν Τρωικό Αστεροειδή και θεωρώντας ως τέταρτο αμελητέας μάζας σώμα ένα διαστημόπλοιο. Τα πρωτεύοντα σώματα υπακούουν στην ευσταθή Lagrangian τριγωνική διαμόρφωση. Μελετήσαμε επίσης αναλυτικά και αριθμητικά τις λύσεις στην περιοχή των ευσταθών σημείων ισορροπίας του συστήματος, βρήκαmε οικογένειες περιοδικών λύσεων και μελετήσαμε την γραμμική ευστάθεια τους. Τα αποτελέσματα των κεφαλαίων 2,3,4 και 5 έχουν δημοσιευτεί σε τρία διεθνή περιοδικά και ένα κομμάτι του κεφαλαίου 5 παρουσιάστηκε σε διεθνές συνέδριο (με συγγραφείς τους Μπαλταγιάννη Α. και Παπαδάκη Κ.). Πιο συγκεκριμένα η μελέτη των κεφαλαίων 2 και 3 έχει δημοσιευτεί στο περιοδικό “International Journal of Bifurcation and Chaos, 21, 2011, pp. 2179-2193” με τον τίτλο: “Equilibrium Points and their stability in the restricted four-body problem”. Τα αποτελέσματα του κεφαλαίου 4 δημοσιεύτηκαν mε τον τίτλο: “Families of periodic orbits in the restricted four-body problem” στο περιοδικό “Astrophysics and Space Science, 336, 2011, pp. 357-367”. Επίσης το κεφάλαιο 5 υπό τον τίτλο “Periodic solutions in the Sun - Jupiter - Trojan Asteroid - Spacecraft system”, δημοσιεύτηκε στο περιοδικό ”Planetary and Space Science, 75, 2013, pp. 148-157”. Το διεθνές συνέδριο στο οποίο παρουσιάστηκε τμήμα του κεφαλαίου 5 ήταν το : “10th Hellenic Astronomical Conference, Proceedings of the conference held at Ioannina, Greece, 5-8 September 2011, pp. 23-24” και η εργασία είχε τίτλο: “Families of periodic orbits in the Sun - Jupiter - Trojan Asteroid system”. Η παρούσα διατριβή εκπονήθηκε με την οικονομική υποστήριξη του ερευνητικού προγράμματος του Πανεπιστημίου Πατρών: Κ. Καραθεοδωρή. / In this thesis we are concerned with the periodic and asymptotic solutions of the restricted four - body problem. In chapter 1 we describe the three - body and four - body problem, starting with historical information. We also present the needed equations of motion and integrals of the problem. In chapter 2 we study numerically the problem of four - bodies, according to the Lagrangian equilateral triangle configuration. We find the equilibrium points and the allowed regions of motion. In chapter 3 we study the stability of the relative equibrium solutions. We also illustrate the regions of the basins of attraction for the equilibrium points of the present dynamical model. In chapter 4 we present families of simple symmetric and non-symmetric periodic orbits in the restricted four-body problem. Series of critical periodic orbits of each family and in any case of the mass parameters are also calculated. In chapter 5 we study, numerically, families of simple non-symmetric periodic orbits of the restricted four-body problem, where we consider the three primary bodies as Sun, Jupiter and a Trojan Asteroid and as a massless fourth body, a spacecraft. The primary bodies are set in the stable Lagrangian equilateral triangle configuration. We also study analytically the solutions in the neighborhood of the stable equilibrium points and the linear stability of each periodic solution. The results of the chapters 2,3,4 and 5 have been published in three journals and a part of chapter 5 has been presented in an international conference. Chapters 2 and 3 have been published in “International Journal of Bifurcation and Chaos, 21, 2011, pp. 2179-2193” under the title of “Equilibrium Points and their stability in the restricted four-body problem”. Chapter 4 has been titled “Families of periodic orbits in the restricted four- body problem” and published in “Astrophysics and Space Science, 336, 2011, pp. 357-367”. Chapter 5 has been titled “Periodic solutions in the Sun - Jupiter - Trojan Asteroid - Spacecraft system,” and published in “Planetary and Space Science, 75, 2013, pp. 148-157”. The conference was the “10th Hellenic Astronomical Conference, Proceedings of the conference held at Ioannina, Greece, 5-8 September 2011, pp. 23-24” and part of the chapter 5 was presented under the title of “Families of periodic orbits in the Sun - Jupiter - Trojan Asteroid system”. This thesis was compiled while the author was in receipt of “K.Karatheodory” research grant.

Traditionally, differential-equation models for population dynamics have considered organisms as "fixed" entities in terms of their behaviour and characteristics. However, there have been many observations of adaptivity in organisms, both at the level of behaviour and as an evolutionary change of traits, in response to the environmental conditions. Taking such adaptiveness into account alters the qualitative dynamics of traditional models and is an important factor to be included, for example, when developing reliable model predictions under changing environmental conditions. In this thesis, we consider piecewise-smooth and smooth dynamical systems to represent adaptive change in a 1 predator-2 prey system. First, we derive a novel piecewise-smooth dynamical system for a predator switching between its preferred and alternative prey type in response to prey abundance. We consider a linear ecological trade-off and discover a novel bifurcation as we change the slope of the trade-off. Second, we reformulate the piecewise-smooth system as two novel 1 predator-2 prey smooth dynamical systems. As opposed to the piecewise-smooth system that includes a discontinuity in the vector fields and assumes that a predator switches its feeding strategy instantaneously, we relax this assumption in these systems and consider continuous change in a predator trait. We use plankton as our reference organism because they serve as an important model system. We compare the model simulations with data from Lake Constance on the German-Swiss-Austrian border and suggest possible mechanistic explanations for cycles in plankton concentrations in spring.