Correções radiativas no modelo Bumblebee-Stueckelberg

Detalhes bibliográficos
Ano de defesa: 2021
Autor(a) principal: Belchior, Fernando de Menezes
Orientador(a): Cavalcante, Roberto Vinhaes Maluf
Banca de defesa: Não Informado pela instituição
Tipo de documento: Dissertação
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/61248
Resumo: The Lorentz Symmetry plays a fundamental role in the building of General Relativity and Quantum Field Theory. However, in order to understand the Physics beyond the Standard Model, the physicists have considered that the Lorentz symmetry could be violated in a fundamental theory. In this work, we start by introducing the Path integral formalism and then talk about the possibility of Lorentz symmetry violation and study radiative corrections in a vector model with Spontaneous Lorentz violation, known in the literature as the Bumblebee model. First, we consider the Bumblebee model with self interaction smooth potential, which is responsible for Spontaneous Lorentz violation. The spectrum of this model displays a transversal non massive mode, which is identified as Nambu-Goldstone, and a longitudinal massive mode. Besides the Lorentz symmetry, this model also exhibits gauge symmetry violation. We calculate the two point function by employing the PV prescription and the result is non-transversal, leading to an excited massive mode. In order to restore the gauge symmetry, we introduce the Stueckelberg field and calculate the two point function. Our result is also non-transversal.
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spelling Belchior, Fernando de MenezesCavalcante, Roberto Vinhaes Maluf2021-10-15T17:16:08Z2021-10-15T17:16:08Z2021BELCHIOR, F. M. Correções radiativas no modelo Bumblebee-Stueckelberg. 73 f. Dissertação (Mestrado em Física) - Centro de Ciências, Universidade Federal do Ceará, Fortaleza, 2021.http://www.repositorio.ufc.br/handle/riufc/61248The Lorentz Symmetry plays a fundamental role in the building of General Relativity and Quantum Field Theory. However, in order to understand the Physics beyond the Standard Model, the physicists have considered that the Lorentz symmetry could be violated in a fundamental theory. In this work, we start by introducing the Path integral formalism and then talk about the possibility of Lorentz symmetry violation and study radiative corrections in a vector model with Spontaneous Lorentz violation, known in the literature as the Bumblebee model. First, we consider the Bumblebee model with self interaction smooth potential, which is responsible for Spontaneous Lorentz violation. The spectrum of this model displays a transversal non massive mode, which is identified as Nambu-Goldstone, and a longitudinal massive mode. Besides the Lorentz symmetry, this model also exhibits gauge symmetry violation. We calculate the two point function by employing the PV prescription and the result is non-transversal, leading to an excited massive mode. In order to restore the gauge symmetry, we introduce the Stueckelberg field and calculate the two point function. Our result is also non-transversal.A simetria de Lorentz tem um papel fundamental na construção da Relatividade Geral e Teoria Quântica de Campos. Todavia, a fim de compreender a física além do modelo padrão, os físicos têm considerado que a simetria de Lorentz pode ser violada em uma teoria mais fundamental. Nesse trabalho, iniciamos introduzindo o formalismo de integrais de trajetória e então falamos sobre a possibilidade de Violação de simetria de Lorentz e destacamos o mecanismo de violação espontânea proposto por Kostelecky e Samuel. Feito isso, estudamos as correções radiativas a um loop em um modelo vetorial com violação espontânea da simetria de Lorentz, conhecido na literatura como modelo Bumblebee. Primeiro, consideramos o modelo Bumblebee com um potencial suave de auto interação, que é responsável pela violação espontânea de Lorentz. O espectro desse modelo exibe um modo não-massivo transversal, que é identificado como modo de Nambu-Goldstone, e um modo massivo longitudinal. Além da quebra da simetria de Lorentz, esse modelo também exibe violação da simetria de calibre. Calculamos a função de dois pontos empregando a prescrição PV e o resultado é não transversal, levando a um modo massivo excitado. A fim de restaurar a simetria de calibre, introduzimos o campo de Stueckelberg e calculamos a função de dois pontos. Nosso resultado também é não transversal.Modelo BumblebeeCampo de StueckelbergFunção de dois pontosViolação de LorentzCorreções radiativas no modelo Bumblebee-Stueckelberginfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/masterThesisporreponame: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-81748http://repositorio.ufc.br/bitstream/riufc/61248/4/license.txt8a4605be74aa9ea9d79846c1fba20a33MD54ORIGINAL2021_dis_fmbelchior.pdf2021_dis_fmbelchior.pdfapplication/pdf2239861http://repositorio.ufc.br/bitstream/riufc/61248/3/2021_dis_fmbelchior.pdfb1ffb3c31a9efbe782a23f01fbe38ec4MD53riufc/612482021-10-15 14:16:08.59oai:repositorio.ufc.br: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Repositório InstitucionalPUBhttp://www.repositorio.ufc.br/ri-oai/requestbu@ufc.br || repositorio@ufc.bropendoar:2021-10-15T17:16:08Repositório Institucional da Universidade Federal do Ceará (UFC) - Universidade Federal do Ceará (UFC)false
dc.title.pt_BR.fl_str_mv Correções radiativas no modelo Bumblebee-Stueckelberg
title Correções radiativas no modelo Bumblebee-Stueckelberg
spellingShingle Correções radiativas no modelo Bumblebee-Stueckelberg
Belchior, Fernando de Menezes
Modelo Bumblebee
Campo de Stueckelberg
Função de dois pontos
Violação de Lorentz
title_short Correções radiativas no modelo Bumblebee-Stueckelberg
title_full Correções radiativas no modelo Bumblebee-Stueckelberg
title_fullStr Correções radiativas no modelo Bumblebee-Stueckelberg
title_full_unstemmed Correções radiativas no modelo Bumblebee-Stueckelberg
title_sort Correções radiativas no modelo Bumblebee-Stueckelberg
author Belchior, Fernando de Menezes
author_facet Belchior, Fernando de Menezes
author_role author
dc.contributor.author.fl_str_mv Belchior, Fernando de Menezes
dc.contributor.advisor1.fl_str_mv Cavalcante, Roberto Vinhaes Maluf
contributor_str_mv Cavalcante, Roberto Vinhaes Maluf
dc.subject.por.fl_str_mv Modelo Bumblebee
Campo de Stueckelberg
Função de dois pontos
Violação de Lorentz
topic Modelo Bumblebee
Campo de Stueckelberg
Função de dois pontos
Violação de Lorentz
description The Lorentz Symmetry plays a fundamental role in the building of General Relativity and Quantum Field Theory. However, in order to understand the Physics beyond the Standard Model, the physicists have considered that the Lorentz symmetry could be violated in a fundamental theory. In this work, we start by introducing the Path integral formalism and then talk about the possibility of Lorentz symmetry violation and study radiative corrections in a vector model with Spontaneous Lorentz violation, known in the literature as the Bumblebee model. First, we consider the Bumblebee model with self interaction smooth potential, which is responsible for Spontaneous Lorentz violation. The spectrum of this model displays a transversal non massive mode, which is identified as Nambu-Goldstone, and a longitudinal massive mode. Besides the Lorentz symmetry, this model also exhibits gauge symmetry violation. We calculate the two point function by employing the PV prescription and the result is non-transversal, leading to an excited massive mode. In order to restore the gauge symmetry, we introduce the Stueckelberg field and calculate the two point function. Our result is also non-transversal.
publishDate 2021
dc.date.accessioned.fl_str_mv 2021-10-15T17:16:08Z
dc.date.available.fl_str_mv 2021-10-15T17:16:08Z
dc.date.issued.fl_str_mv 2021
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/masterThesis
format masterThesis
status_str publishedVersion
dc.identifier.citation.fl_str_mv BELCHIOR, F. M. Correções radiativas no modelo Bumblebee-Stueckelberg. 73 f. Dissertação (Mestrado em Física) - Centro de Ciências, Universidade Federal do Ceará, Fortaleza, 2021.
dc.identifier.uri.fl_str_mv http://www.repositorio.ufc.br/handle/riufc/61248
identifier_str_mv BELCHIOR, F. M. Correções radiativas no modelo Bumblebee-Stueckelberg. 73 f. Dissertação (Mestrado em Física) - Centro de Ciências, Universidade Federal do Ceará, Fortaleza, 2021.
url http://www.repositorio.ufc.br/handle/riufc/61248
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