A method is investigated which enables exact solutions to be found for vacuum and radiation-dominated Friedmann universes of all curvatures in scalar-tensor theories with an arbitrary form for the coupling, omega(phi), of the scalar field which determines the strength of the gravitational field. Particular classes of solution are presented for specific representative choices of omega(phi), including the theories of Brans and Dicke, Barker, and Bekenstein, to illustrate the range of cosmological behaviors that are possible.
机构:
Univ Fed Alfenas, Inst Ciencia & Tecnol, Rodovia Jose Aurelio Vilela 11999, Pocos De Caldas, MG, BrazilUniv Fed Alfenas, Inst Ciencia & Tecnol, Rodovia Jose Aurelio Vilela 11999, Pocos De Caldas, MG, Brazil
Cuzinatto, R. R.
de Morais, E. M.
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Sao Paulo State Univ, Inst Theoret Phys, R Dr Bento Teohaldo Ferraz 271, Sao Paulo, SP, BrazilUniv Fed Alfenas, Inst Ciencia & Tecnol, Rodovia Jose Aurelio Vilela 11999, Pocos De Caldas, MG, Brazil
de Morais, E. M.
Pimentel, B. M.
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Sao Paulo State Univ, Inst Theoret Phys, R Dr Bento Teohaldo Ferraz 271, Sao Paulo, SP, BrazilUniv Fed Alfenas, Inst Ciencia & Tecnol, Rodovia Jose Aurelio Vilela 11999, Pocos De Caldas, MG, Brazil