scalar tensor theories;
bianchi VII cosmological model;
D O I:
10.1016/S0375-9601(99)00357-6
中图分类号:
O4 [物理学];
学科分类号:
0702 ;
摘要:
The dynamical effects on the scale factors due to the scalar phi-field at the early stages of a supposedly anisotropic Universe expansion in the scalar-tensor cosmology of Jordan, Brans and Dicke is studied. This universe shows an isotropic evolution and, depending on the value of the theorie's coupling parameter omega, it can begin from a singularity if omega > 0 and after expanding shrink to another one; or, if omega < 0 and -3/2 < omega less than or equal to - 4/3, it can evolve from a flat spatially-infinite state to a non extended singularity; or, if -4/3 < omega < 0, evolve from an extended singularity to a non singular state and, at last, proceed towards a singularity. (C) 1999 Published by Elsevier Science B.V. All rights reserved.
机构:
ICREA, Passeig Lluis Companys 23, Barcelona 08010, Spain
CSIC, Inst Space Sci ICE, C Can Magrans S-N, Barcelona 08193, SpainCent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China