Scalar-tensor nonlocal gravity

被引:9
|
作者
Tian, Shuxun [1 ]
机构
[1] Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Hubei, Peoples R China
基金
中国国家自然科学基金;
关键词
ENERGY COMPONENT; EQUATION;
D O I
10.1103/PhysRevD.98.084040
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In order to explain the late-time cosmological acceleration, we propose a new pure geometric gravity based on Deser-Woodard theory [Phys. Rev. Lett. 99, 111301 (2007)], in which the expansion of a matter-dominated universe can be accelerating. This new theory behaves as well as general relativity in solar system and gravitational waves, which is an important improvement over Deser-Woodard nonlocal gravity. Especially, for the simplest case, theoretical considerations determine all the parameters that appear in the Lagrangian.
引用
收藏
页数:5
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