Emissão de ondas gravitacionais em teorias de gravitação quadrática

Despite the unquestionable success of General Relativity (GR) in being able to describe and predict several gravitational phenomena, this theory still has some internal issues of interest for cosmology and high energy physics, e.g. singularities, dark energy, cosmology of the early universe, quantum...

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Detalhes bibliográficos
Autor: Reis, Luís Felipe Martins de Almeida Morena
Formato: tesis de maestría
Estado:Versión publicada
Fecha de publicación:2021
País:Brasil
Recursos:Universidade Federal do Rio Grande do Norte (UFRN)
Repositorio:Repositório Institucional da UFRN
Idioma:portugués
OAI Identifier:oai:repositorio.ufrn.br:123456789/45617
Acesso em linha:https://repositorio.ufrn.br/handle/123456789/45617
Access Level:acceso abierto
Palavra-chave:Ondas gravitacionais
Gravitação modificada
Gravitação quadrática
Órbitas circulares
Descrição
Resumo:Despite the unquestionable success of General Relativity (GR) in being able to describe and predict several gravitational phenomena, this theory still has some internal issues of interest for cosmology and high energy physics, e.g. singularities, dark energy, cosmology of the early universe, quantum gravity, etc. Extended theories of gravity, which consist of modifications in GR, have been shown to be a possible solution to these problems. Therefore, in this work we will study a quadratic theory of gravity, where the terms αR2 and γRµνRµν are added to the Einstein-Hilbert action with α and γ being coupling constants. This theory is usually present in several works being linked to the renormalization issues of gravity. In this work we will study the main aspects of this quadratic theory, focusing mainly on the properties of new fields that manifest themselves in the theory through the solution of linearized field equations. Thus, we will analyze the role that these fields play in the orbital evolution of a point mass system in a circular orbit due to the emission of gravitational waves.