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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

On the equivalence of Lambda(t) and gravitationally induced particle production cosmologies

Texto completo
Autor(es):
Graef, L. L. [1] ; Costa, F. E. M. [2, 3] ; Lima, J. A. S. [2]
Número total de Autores: 3
Afiliação do(s) autor(es):
[1] Univ Sao Paulo, Inst Fis, BR-05508900 Sao Paulo - Brazil
[2] Univ Sao Paulo, Dept Astron, BR-05508900 Sao Paulo - Brazil
[3] Univ Fed Rural Semi Arido, BR-59900000 Pau Dos Ferros, RN - Brazil
Número total de Afiliações: 3
Tipo de documento: Artigo Científico
Fonte: Physics Letters B; v. 728, p. 400-406, JAN 20 2014.
Citações Web of Science: 20
Resumo

The correspondence between cosmological models powered by a decaying vacuum energy density and gravitationally induced particle production is investigated. Although being physically different in the physics behind them we show that both classes of cosmologies under certain conditions can exhibit the same dynamic and thermodynamic behavior. Our method is applied to obtain three specific models that may be described either as A(t)CDM or gravitationally induced particle creation. In the point of view of particle production models, such cosmologies can be interpreted as a kind of one-component unification of the dark sector. By using current type la supernovae data, recent estimates of the cosmic microwave background shift parameter and baryon acoustic oscillations measurements we also perform a statistical analysis to test the observational viability within the two equivalent classes of models and we obtain the best-fit of the free parameters. By adopting the Akaike information criterion we also determine the rank of the models considered here. Finally, the particle production cosmologies (and the associated decaying A(t)-models) are modeled in the framework of field theory by a phenomenological scalar field model. (C) 2013 The Authors. Published by Elsevier B.V. All rights reserved. (AU)

Processo FAPESP: 11/13018-0 - Energia escura e teorias F(R): aspectos teóricos e observacionais
Beneficiário:Francisco Ernandes Matos Costa
Modalidade de apoio: Bolsas no Brasil - Pós-Doutorado
Processo FAPESP: 04/13668-0 - Cosmologia na era da precisão: energia escura, matéria escura e radiação cósmica de fundo
Beneficiário:Jose Ademir Sales de Lima
Modalidade de apoio: Auxílio à Pesquisa - Temático
Processo FAPESP: 12/09380-8 - Decaimento do vácuo, inflação morna e conexões com o atual estágio acelerado do universo: aspectos conceituais e testes observacionais
Beneficiário:Leila Lobato Graef
Modalidade de apoio: Bolsas no Brasil - Doutorado