Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral

Detalhes bibliográficos
Autor(a) principal: Gonçalves, Victor Rodrigues
Data de Publicação: 2022
Tipo de documento: Tese
Idioma: por
Título da fonte: Biblioteca Digital de Teses e Dissertações da UFPB
Texto Completo: https://repositorio.ufpb.br/jspui/handle/123456789/26395
Resumo: The objective of this thesis is to evaluate the consistency of the gravitational energy obtained when the Teleparallel Equivalent of General Relativity is applied, as well as which teleparallel frame is more suitable for this purpose. In order to do that, we have used this approach to calculate the energy of the gravitational field of the Schwarzschild spacetime and to obtain the gravitational energy-momentum tensor of the Friedmann- Lemaître-Robertson-Walker spacetimes. In the first case, we have used tetrads adapted to Kruskal and Novikov coordinates. We have obtained that the energy of the black/white hole is the famous 2 when the wormhole throat is closed. In this result, we have verified that the singularity does not contribute to the energy, which indicates that the energy obtained is purely gravitational. For the second case, we have found the gravitational energy-momentum density tensor of the universe from the tetrad adapted to the Friedmann-Lemaître-Robertson-Walker coordinates.We have decomposed this tensor into its symmetrical and antisymmetrical parts, and we have analysed each one of them. The symmetrical part obeys a radiation-like equation of state, then we have pointed out that, actually, this is a general characteristic of the gravitational energy-momentum density tensor, since it is traceless. The antisymmetric part does not contribute to the energy of the universe. We have observed that the field equations have a well-defined vacuum and that, for spatially flat universes, the total energy density of the universe is zero. In the penultimate chapter, we have also verified the 4-momentum of the Teleparallel Equivalent of General Relativity can be made to coincide with that of the ADM formalism. In this chapter, we discuss the idea that the best frame to analyze the gravitational energy is a frame adapted to free particles and that is free from artificial properties. Based on the results obtained in this thesis, we have concluded the Teleparallel Equivalent of General Relativity is quite suitable for calculating gravitational energy as long as a suitable teleparallel frame is used.
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spelling Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geralFísicaTeleparalelismoEnergia gravitacional - LocalizaçãoReferencial teleparaleloPhysicalTeleparallelismGravitational energy - LocalizationTeleparallel frameCNPQ::CIENCIAS EXATAS E DA TERRA::FISICAThe objective of this thesis is to evaluate the consistency of the gravitational energy obtained when the Teleparallel Equivalent of General Relativity is applied, as well as which teleparallel frame is more suitable for this purpose. In order to do that, we have used this approach to calculate the energy of the gravitational field of the Schwarzschild spacetime and to obtain the gravitational energy-momentum tensor of the Friedmann- Lemaître-Robertson-Walker spacetimes. In the first case, we have used tetrads adapted to Kruskal and Novikov coordinates. We have obtained that the energy of the black/white hole is the famous 2 when the wormhole throat is closed. In this result, we have verified that the singularity does not contribute to the energy, which indicates that the energy obtained is purely gravitational. For the second case, we have found the gravitational energy-momentum density tensor of the universe from the tetrad adapted to the Friedmann-Lemaître-Robertson-Walker coordinates.We have decomposed this tensor into its symmetrical and antisymmetrical parts, and we have analysed each one of them. The symmetrical part obeys a radiation-like equation of state, then we have pointed out that, actually, this is a general characteristic of the gravitational energy-momentum density tensor, since it is traceless. The antisymmetric part does not contribute to the energy of the universe. We have observed that the field equations have a well-defined vacuum and that, for spatially flat universes, the total energy density of the universe is zero. In the penultimate chapter, we have also verified the 4-momentum of the Teleparallel Equivalent of General Relativity can be made to coincide with that of the ADM formalism. In this chapter, we discuss the idea that the best frame to analyze the gravitational energy is a frame adapted to free particles and that is free from artificial properties. Based on the results obtained in this thesis, we have concluded the Teleparallel Equivalent of General Relativity is quite suitable for calculating gravitational energy as long as a suitable teleparallel frame is used.Conselho Nacional de Pesquisa e Desenvolvimento Científico e Tecnológico - CNPqO objetivo desta tese é avaliar a consistência da energia do campo gravitacional obtida quando o formalismo do Teleparalelismo Equivalente à Relatividade Geral é empregado, bem como qual referencial teleparalelo é mais adequado para esse fim. Com esse intuito, usamos essa abordagem para calcular a energia do campo gravitacional do espaço-tempo de Schwarzschild e obter o tensor densidade de energia-momento gravitacional para os espaços-tempos de Friedmann-Lemaître-Robertson-Walker. No primeiro caso, utilizamos tetradas adaptadas às coordenadas de Kruskal e às de Novikov. Obtivemos que a energia do buraco negro/branco é o famoso 2 quando a garganta do buraco de minhoca está fechada. Nesse resultado, verificamos que a singularidade não contribui para a energia, o que indica que a energia obtida é puramente gravitacional. Já para o segundo caso, encontramos o tensor densidade de energia-momento gravitacional do universo a partir da tetrada adapta às coordenadas de Friedmann-Lemaître-Robertson-Walker. Decompomos esse tensor em sua parte simétrica e antissimétrica, analisando cada uma delas. A parte simétrica obedece uma equação de estado tipo-radiação, depois pontuamos que, na verdade, essa é uma característica geral do tensor densidade energia-momento gravitacional, já que o mesmo tem traço nulo. Já a parte antissimétrica não contribui para a energia do universo. Observamos que as equações de campo tem um vácuo bem definido e que, para universos com seção espacial plana, a densidade de energia total do universo é nula. No penúltimo capítulo, verificamos que o 4-momento do Teleparalelismo Equivalente à Relatividade Geral pode ser visto como uma generalização do 4-momento do formalismo ADM. Ao final desse capítulo, discutimos a ideia de que o referencial mais adequado para analisar o problema da energia gravitacional seja o referencial adaptado à partículas livres e que esteja livre de propriedades artificiais. Concluímos, a partir dos resultados obtidos nesta tese, que o Teleparalelismo Equivalente à Relatividade Geral é bastante propício no cálculo da energia gravitacional desde que se use um referencial teleparalelo adequado.Universidade Federal da ParaíbaBrasilFísicaPrograma de Pós-Graduação em FísicaUFPBFormiga, Jansen Brasileirohttp://lattes.cnpq.br/1666058727081809Gonçalves, Victor Rodrigues2023-03-07T13:21:46Z2022-09-062023-03-07T13:21:46Z2022-07-27info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/doctoralThesishttps://repositorio.ufpb.br/jspui/handle/123456789/26395porAttribution-NoDerivs 3.0 Brazilhttp://creativecommons.org/licenses/by-nd/3.0/br/info:eu-repo/semantics/openAccessreponame:Biblioteca Digital de Teses e Dissertações da UFPBinstname:Universidade Federal da Paraíba (UFPB)instacron:UFPB2023-05-22T12:30:33Zoai:repositorio.ufpb.br:123456789/26395Biblioteca Digital de Teses e Dissertaçõeshttps://repositorio.ufpb.br/PUBhttp://tede.biblioteca.ufpb.br:8080/oai/requestdiretoria@ufpb.br|| diretoria@ufpb.bropendoar:2023-05-22T12:30:33Biblioteca Digital de Teses e Dissertações da UFPB - Universidade Federal da Paraíba (UFPB)false
dc.title.none.fl_str_mv Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral
title Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral
spellingShingle Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral
Gonçalves, Victor Rodrigues
Física
Teleparalelismo
Energia gravitacional - Localização
Referencial teleparalelo
Physical
Teleparallelism
Gravitational energy - Localization
Teleparallel frame
CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA
title_short Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral
title_full Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral
title_fullStr Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral
title_full_unstemmed Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral
title_sort Um estudo sobre a energia gravitacional na abordagem do teleparalelismo equivalente à relatividade geral
author Gonçalves, Victor Rodrigues
author_facet Gonçalves, Victor Rodrigues
author_role author
dc.contributor.none.fl_str_mv Formiga, Jansen Brasileiro
http://lattes.cnpq.br/1666058727081809
dc.contributor.author.fl_str_mv Gonçalves, Victor Rodrigues
dc.subject.por.fl_str_mv Física
Teleparalelismo
Energia gravitacional - Localização
Referencial teleparalelo
Physical
Teleparallelism
Gravitational energy - Localization
Teleparallel frame
CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA
topic Física
Teleparalelismo
Energia gravitacional - Localização
Referencial teleparalelo
Physical
Teleparallelism
Gravitational energy - Localization
Teleparallel frame
CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA
description The objective of this thesis is to evaluate the consistency of the gravitational energy obtained when the Teleparallel Equivalent of General Relativity is applied, as well as which teleparallel frame is more suitable for this purpose. In order to do that, we have used this approach to calculate the energy of the gravitational field of the Schwarzschild spacetime and to obtain the gravitational energy-momentum tensor of the Friedmann- Lemaître-Robertson-Walker spacetimes. In the first case, we have used tetrads adapted to Kruskal and Novikov coordinates. We have obtained that the energy of the black/white hole is the famous 2 when the wormhole throat is closed. In this result, we have verified that the singularity does not contribute to the energy, which indicates that the energy obtained is purely gravitational. For the second case, we have found the gravitational energy-momentum density tensor of the universe from the tetrad adapted to the Friedmann-Lemaître-Robertson-Walker coordinates.We have decomposed this tensor into its symmetrical and antisymmetrical parts, and we have analysed each one of them. The symmetrical part obeys a radiation-like equation of state, then we have pointed out that, actually, this is a general characteristic of the gravitational energy-momentum density tensor, since it is traceless. The antisymmetric part does not contribute to the energy of the universe. We have observed that the field equations have a well-defined vacuum and that, for spatially flat universes, the total energy density of the universe is zero. In the penultimate chapter, we have also verified the 4-momentum of the Teleparallel Equivalent of General Relativity can be made to coincide with that of the ADM formalism. In this chapter, we discuss the idea that the best frame to analyze the gravitational energy is a frame adapted to free particles and that is free from artificial properties. Based on the results obtained in this thesis, we have concluded the Teleparallel Equivalent of General Relativity is quite suitable for calculating gravitational energy as long as a suitable teleparallel frame is used.
publishDate 2022
dc.date.none.fl_str_mv 2022-09-06
2022-07-27
2023-03-07T13:21:46Z
2023-03-07T13:21:46Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/doctoralThesis
format doctoralThesis
status_str publishedVersion
dc.identifier.uri.fl_str_mv https://repositorio.ufpb.br/jspui/handle/123456789/26395
url https://repositorio.ufpb.br/jspui/handle/123456789/26395
dc.language.iso.fl_str_mv por
language por
dc.rights.driver.fl_str_mv Attribution-NoDerivs 3.0 Brazil
http://creativecommons.org/licenses/by-nd/3.0/br/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution-NoDerivs 3.0 Brazil
http://creativecommons.org/licenses/by-nd/3.0/br/
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Universidade Federal da Paraíba
Brasil
Física
Programa de Pós-Graduação em Física
UFPB
publisher.none.fl_str_mv Universidade Federal da Paraíba
Brasil
Física
Programa de Pós-Graduação em Física
UFPB
dc.source.none.fl_str_mv reponame:Biblioteca Digital de Teses e Dissertações da UFPB
instname:Universidade Federal da Paraíba (UFPB)
instacron:UFPB
instname_str Universidade Federal da Paraíba (UFPB)
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institution UFPB
reponame_str Biblioteca Digital de Teses e Dissertações da UFPB
collection Biblioteca Digital de Teses e Dissertações da UFPB
repository.name.fl_str_mv Biblioteca Digital de Teses e Dissertações da UFPB - Universidade Federal da Paraíba (UFPB)
repository.mail.fl_str_mv diretoria@ufpb.br|| diretoria@ufpb.br
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