Quebra de Simetria no Universo Primordial

• Ano de defesa: 2007
• Autor(a) principal: Cuzinatto, R. R [UNESP]
• Tipo de documento: Tese
• Tipo de acesso: Acesso aberto
• Idioma: por
• Instituição de defesa: Universidade Estadual Paulista (Unesp)
• Palavras-chave em Português: Simetria quebrada (Fisica); Broken symmetry (Physics)
• Link de acesso: http://hdl.handle.net/11449/138365; http://www.athena.biblioteca.unesp.br/exlibris/bd/cathedra/11-04-2016/000855676.pdf

Analytic expressions for solutions in the Standard Model are presented here for all combinations of 'lâmbda' = 0, 'lâmbda'diferente 0, 'capa' = 0 and 'capa'diferente'0 in the presence and absence of radiation and nonrelativistic matter. The most complete case (here called the 'lâmbda' IND. 'gama'CDM Model) has 'lâmbda'diferente 0, 'capa'diferente'0, and supposes the presence of radiation and dust. It exhibits clearly the recent onset of acceleration and reduces to the particular models such as the 'lâmbda'CDM Model. A detailed examination of the Killing equations in Robertson-Walker coordinates shows how the addition of matter and/or radiation to a de Sitter Universe breaks the symmetry generated by four of its Killing fields. The product U = 'a POT. 2'H of the squared scale parameter by the time-derivative of the Hubble function encapsulates the relationship between the two cases: the symmetry is maximal when U is a constant, and reduces to the 6-parameter symmetry of a generic Friedmann-Robertson-Walker model when it is not. As the fields physical interpretation is not clear in these coordinates, comparison is made with the Killing fields in static coordinates, whose interpretation is made clearer by their direct relationship to the Poincaré group generators via Wigner-Inönü contractions