Dissipação no modelo Fermi-Ulam
| Ano de defesa: | 2012 |
|---|---|
| Autor(a) principal: | |
| Orientador(a): | |
| Banca de defesa: | |
| Tipo de documento: | Tese |
| Tipo de acesso: | Acesso aberto |
| Idioma: | por |
| Instituição de defesa: |
Não Informado pela instituição
|
| Programa de Pós-Graduação: |
Não Informado pela instituição
|
| Departamento: |
Não Informado pela instituição
|
| País: |
Não Informado pela instituição
|
| Palavras-chave em Português: | |
| Link de acesso: | http://www.repositorio.ufc.br/handle/riufc/13628 |
Resumo: | In this work, we revisit the Fermi accelerator model, also known as Fermi-Ulam model. This model consists of a classical particle of unitary mass wich is confined to bounce between two rigid walls. One of them is fixed and the other one is assumed to move periodically in time. The particle collisions with the walls are assumed to be elastic. The description of the dynamic is made everytime the particle collides with the moving wall, so that we know the particle’s time and velocity at each collision needed to describe the dynamic of the system. Two versions for this model are studied: the complete and the simplified versions. In the simplified version, two walls of the model are assumed to be fixed. The Fermi-Ulam model is a conservative model because it preserves area of the phase space. Our analytical and numerical results for this conservative model are presented and discussed. Some dynamical properties for a particle suffering the action of a drag force are obtained for a dissipative Fermi-Ulam model. The dissipation is introduced via a viscous drag force, like a gas, wich is assumed to be proportional to any power of the velocity, F = −ηV γ . The dynamics of the models are described by two dimensional nonlinear mappings obtained via the solution of the second Newtons’ law of motion. We prove analytically that the decay of high energy is given by a continued fraction wich recovers the following expressions: (i) linear for γ = 1, (ii) exponential for γ = 2 and (iii) second degree polynomial type for γ = 1.5. For any value of γ, the numerical results shows a polynomial behavior for the velocity decay. Our results are discussed for both the complete and simplified versions. The phase spaces and the basin of attraction for some values of γ are obtained. Complementing our studies on this dissipative version of the Fermi-Ulam model, a mixed model was proposed. In this model, one particle travels through two different media. It started in a medium with no dissipation lets say vacuum and at some point it enters a region with a dissipative medium. The dissipation is also introduced by a viscous drag force, such that F = −ηV γ . In particular, for the study of the mixed model we use γ = 1 and γ = 2. The system is characterized by the ratio of the two medium length ξ. We show that there is a smooth transition of the velocity regime with ξ. We construct the phase spaces for the complete and simplified versions of the models. For the limiting cases, ξ = 0 or ξ = 1, the system behaves like one medium only. |
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Sousa, Danila Fernandes Tavares deLeonel, Edson DenisCosta Filho, Raimundo Nogueira da2015-10-20T20:56:08Z2015-10-20T20:56:08Z2012SOUSA, D. F. T. Dissipação no modelo Fermi-Ulam. 2012. 131 f. Tese (Doutorado em Física) - Centro de Ciências, Universidade Federal do Ceará, Fortaleza, 2012.http://www.repositorio.ufc.br/handle/riufc/13628In this work, we revisit the Fermi accelerator model, also known as Fermi-Ulam model. This model consists of a classical particle of unitary mass wich is confined to bounce between two rigid walls. One of them is fixed and the other one is assumed to move periodically in time. The particle collisions with the walls are assumed to be elastic. The description of the dynamic is made everytime the particle collides with the moving wall, so that we know the particle’s time and velocity at each collision needed to describe the dynamic of the system. Two versions for this model are studied: the complete and the simplified versions. In the simplified version, two walls of the model are assumed to be fixed. The Fermi-Ulam model is a conservative model because it preserves area of the phase space. Our analytical and numerical results for this conservative model are presented and discussed. Some dynamical properties for a particle suffering the action of a drag force are obtained for a dissipative Fermi-Ulam model. The dissipation is introduced via a viscous drag force, like a gas, wich is assumed to be proportional to any power of the velocity, F = −ηV γ . The dynamics of the models are described by two dimensional nonlinear mappings obtained via the solution of the second Newtons’ law of motion. We prove analytically that the decay of high energy is given by a continued fraction wich recovers the following expressions: (i) linear for γ = 1, (ii) exponential for γ = 2 and (iii) second degree polynomial type for γ = 1.5. For any value of γ, the numerical results shows a polynomial behavior for the velocity decay. Our results are discussed for both the complete and simplified versions. The phase spaces and the basin of attraction for some values of γ are obtained. Complementing our studies on this dissipative version of the Fermi-Ulam model, a mixed model was proposed. In this model, one particle travels through two different media. It started in a medium with no dissipation lets say vacuum and at some point it enters a region with a dissipative medium. The dissipation is also introduced by a viscous drag force, such that F = −ηV γ . In particular, for the study of the mixed model we use γ = 1 and γ = 2. The system is characterized by the ratio of the two medium length ξ. We show that there is a smooth transition of the velocity regime with ξ. We construct the phase spaces for the complete and simplified versions of the models. For the limiting cases, ξ = 0 or ξ = 1, the system behaves like one medium only.Neste trabalho, revisitamos o modelo do acelerador de Fermi, também conhecido como modelo Fermi-Ulam. Este modelo consiste de uma partícula clássica de massa unitária que está confinada e colidindo elasticamente entre duas paredes rígidas, uma delas sendo fixa e a outra dependente do tempo. A descrição da dinâmica é feita todas as vezes que a partícula colide com a parede móvel, de modo que o conhecimento dos valores da velocidade da partícula e do tempo no instante da colisão descrevem toda a dinâmica. Duas versões para este modelo são estudadas: a versão completa e a versão simplificada. Na versão simplificada, as duas paredes do modelo são assumidas como sendo fixas. O modelo Fermi-Ulam é um modelo conservativo, pois preserva medida do espaço de fases. Nossos resultados analíticos e numéricos para este modelo conservativo são apresentados e discutidos. Algumas propriedades dinâmicas para uma partícula sofrendo a ação de uma força de arrasto são obtidas para um modelo Fermi-Ulam dissipativo. A dissipação é introduzida via uma força de arrasto viscoso, como um gás, que é assumida como sendo proporcional `a velocidade elevada a um expoente γ, F = −ηV^{ γ}. As dinâmicas dos modelos são descritas por mapeamentos bidimensionais não-lineares obtidos via solucões da segunda lei de Newton. Nós provamos, analiticamente, que o decaimento para altas energias é dado por uma fração continuada que recupera as seguintes expressões: (i) linear para γ = 1; (ii) exponencial para γ = 2 e (iii) um polinômio de segundo grau para γ = 1.5. Os resultados numéricos mostram um comportamento polinomial para o decaimento da velocidade. Nossos resultados são discutidos para as versões completa e simplificada dos modelos. Os espaços de fases e as bacias de atração para alguns valores de γ são obtidos. Complementando nossos estudos sobre esta versão dissipativa do modelo Fermi-Ulam, um modelo misto também é proposto. Neste modelo, a partícula viaja através de dois meios distintos. Sua dinâmica é iniciada em um meio sem dissipação, digamos, um vácuo e em algum ponto ela entra em uma região dissipativa. A dissipação também é introduzida por uma força de arrasto viscoso, tal que F = −ηV^{γ}. Em particular, para o estudo do modelo misto utilizamos γ = 1 e γ = 2. O sistema é caracterizado pela relação de dois meios de comprimento λ. Nós mostramos que existe uma transição suave do regime de velocidade conforme λ é variado. Construímos os espaços de fases para as versões completa e simplificada dos modelos. Para os casos limites, λ=0 ou λ=1, o sistema comporta-se como um único meio.FísicaSistemas dinâmicosModelo Fermi-UlamCaos quânticoDissipação no modelo Fermi-Ulaminfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/doctoralThesisporreponame:Repositório Institucional da Universidade Federal do Ceará (UFC)instname:Universidade Federal do Ceará (UFC)instacron:UFCinfo:eu-repo/semantics/openAccessLICENSElicense.txtlicense.txttext/plain; charset=utf-81786http://repositorio.ufc.br/bitstream/riufc/13628/2/license.txt8c4401d3d14722a7ca2d07c782a1aab3MD52ORIGINAL2012_tese_dftsousa.pdf2012_tese_dftsousa.pdfapplication/pdf14704159http://repositorio.ufc.br/bitstream/riufc/13628/1/2012_tese_dftsousa.pdfbf2d7f19ae743de453cdf3921e42e4fbMD51riufc/136282019-07-31 10:36:52.564oai:repositorio.ufc.br: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Repositório InstitucionalPUBhttp://www.repositorio.ufc.br/ri-oai/requestbu@ufc.br || repositorio@ufc.bropendoar:2019-07-31T13:36:52Repositório Institucional da Universidade Federal do Ceará (UFC) - Universidade Federal do Ceará (UFC)false |
| dc.title.pt_BR.fl_str_mv |
Dissipação no modelo Fermi-Ulam |
| title |
Dissipação no modelo Fermi-Ulam |
| spellingShingle |
Dissipação no modelo Fermi-Ulam Sousa, Danila Fernandes Tavares de Física Sistemas dinâmicos Modelo Fermi-Ulam Caos quântico |
| title_short |
Dissipação no modelo Fermi-Ulam |
| title_full |
Dissipação no modelo Fermi-Ulam |
| title_fullStr |
Dissipação no modelo Fermi-Ulam |
| title_full_unstemmed |
Dissipação no modelo Fermi-Ulam |
| title_sort |
Dissipação no modelo Fermi-Ulam |
| author |
Sousa, Danila Fernandes Tavares de |
| author_facet |
Sousa, Danila Fernandes Tavares de |
| author_role |
author |
| dc.contributor.co-advisor.none.fl_str_mv |
Leonel, Edson Denis |
| dc.contributor.author.fl_str_mv |
Sousa, Danila Fernandes Tavares de |
| dc.contributor.advisor1.fl_str_mv |
Costa Filho, Raimundo Nogueira da |
| contributor_str_mv |
Costa Filho, Raimundo Nogueira da |
| dc.subject.por.fl_str_mv |
Física Sistemas dinâmicos Modelo Fermi-Ulam Caos quântico |
| topic |
Física Sistemas dinâmicos Modelo Fermi-Ulam Caos quântico |
| description |
In this work, we revisit the Fermi accelerator model, also known as Fermi-Ulam model. This model consists of a classical particle of unitary mass wich is confined to bounce between two rigid walls. One of them is fixed and the other one is assumed to move periodically in time. The particle collisions with the walls are assumed to be elastic. The description of the dynamic is made everytime the particle collides with the moving wall, so that we know the particle’s time and velocity at each collision needed to describe the dynamic of the system. Two versions for this model are studied: the complete and the simplified versions. In the simplified version, two walls of the model are assumed to be fixed. The Fermi-Ulam model is a conservative model because it preserves area of the phase space. Our analytical and numerical results for this conservative model are presented and discussed. Some dynamical properties for a particle suffering the action of a drag force are obtained for a dissipative Fermi-Ulam model. The dissipation is introduced via a viscous drag force, like a gas, wich is assumed to be proportional to any power of the velocity, F = −ηV γ . The dynamics of the models are described by two dimensional nonlinear mappings obtained via the solution of the second Newtons’ law of motion. We prove analytically that the decay of high energy is given by a continued fraction wich recovers the following expressions: (i) linear for γ = 1, (ii) exponential for γ = 2 and (iii) second degree polynomial type for γ = 1.5. For any value of γ, the numerical results shows a polynomial behavior for the velocity decay. Our results are discussed for both the complete and simplified versions. The phase spaces and the basin of attraction for some values of γ are obtained. Complementing our studies on this dissipative version of the Fermi-Ulam model, a mixed model was proposed. In this model, one particle travels through two different media. It started in a medium with no dissipation lets say vacuum and at some point it enters a region with a dissipative medium. The dissipation is also introduced by a viscous drag force, such that F = −ηV γ . In particular, for the study of the mixed model we use γ = 1 and γ = 2. The system is characterized by the ratio of the two medium length ξ. We show that there is a smooth transition of the velocity regime with ξ. We construct the phase spaces for the complete and simplified versions of the models. For the limiting cases, ξ = 0 or ξ = 1, the system behaves like one medium only. |
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2012 |
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2012 |
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2015-10-20T20:56:08Z |
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2015-10-20T20:56:08Z |
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info:eu-repo/semantics/doctoralThesis |
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SOUSA, D. F. T. Dissipação no modelo Fermi-Ulam. 2012. 131 f. Tese (Doutorado em Física) - Centro de Ciências, Universidade Federal do Ceará, Fortaleza, 2012. |
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http://www.repositorio.ufc.br/handle/riufc/13628 |
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SOUSA, D. F. T. Dissipação no modelo Fermi-Ulam. 2012. 131 f. Tese (Doutorado em Física) - Centro de Ciências, Universidade Federal do Ceará, Fortaleza, 2012. |
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