Late Time Acceleration in Scalar-Tensor Theory with GB Interaction

被引:2
|
作者
Bose, R. N. [1 ]
Modak, B. [1 ]
机构
[1] Univ Kalyani, Dept Phys, Kalyani 741235, W Bengal, India
关键词
Cosmology; Gauss-Bonnet interaction; Chameleon mechanism and Late time acceleration; DARK ENERGY; COSMOLOGICAL CONSEQUENCES; GENERAL-RELATIVITY; COMPONENT; EQUATION; UNIVERSE;
D O I
10.1007/s10773-011-0912-x
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We present some solutions of late time transition to an accelerating universe showing a quintessence or a de-Sitter era of expansion at late time using Gauss-Bonnet interaction in a Jordan Brans-Dicke theory in FLRW spacetime. The Gauss-Bonnet term yields an effective cosmological constant characterized by a de-Sitter era of late time expansion when the Gauss-Bonnet interaction is equivalent with an ideal fluid. The quintessence era of late time expansion have been obtained assuming the evolution of scalar field is a single valued function. The Chameleon mechanism shows that the correction to the Newton law could be small.
引用
收藏
页码:350 / 361
页数:12
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