Constraining f(R) gravity models with disappearing cosmological constant

被引:56
|
作者
Thongkool, I. [1 ]
Sami, M. [1 ]
Gannouji, R. [2 ]
Jhingan, S. [1 ]
机构
[1] Jamia Millia Islamia, Ctr Theoret Phys, New Delhi 110025, India
[2] IUCAA, Pune 411007, Maharashtra, India
来源
PHYSICAL REVIEW D | 2009年 / 80卷 / 04期
关键词
DARK ENERGY; ACCELERATING UNIVERSE; COSMIC ACCELERATION; LAMBDA;
D O I
10.1103/PhysRevD.80.043523
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The f(R) gravity models proposed by Hu-Sawicki and Starobinsky are generic for local gravity constraints to be evaded. The large deviations from these models result in either violation of local gravity constraints or the modifications indistinguishable from cosmological constant. The curvature singularity in these models is generic but can be avoided, provided that proper fine-tuning is imposed on the evolution of scalaron in the high curvature regime. In principle, the problem can be circumvented by incorporating quadratic curvature correction in the Lagrangian, though it might be quite challenging to probe the relevant region numerically.
引用
收藏
页数:7
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