Constraining Newtonian stellar configurations in f (R) theories of gravity

被引:24
作者
Multamaki, T. [1 ]
Vilja, I. [1 ]
机构
[1] Univ Turku, Dept Phys, FIN-20014 Turku, Finland
基金
芬兰科学院;
关键词
D O I
10.1016/j.physletb.2007.12.022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider general metric f (R) theories of gravity by solving the field equations in the presence of a spherical static mass distribution by analytical perturbative means. Expanding the held equations systematically in O(G), we solve the resulting set of equations and show that f (R) theories which attempt to solve the dark energy problem very generally lead to gamma PPN = 1/2 in the solar system. This excludes a large class of theories as possible explanations of dark energy. We also present the first order correction to gamma PPN and show that it cannot have a significant effect. (C) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:843 / 846
页数:4
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