Second post-Newtonian approximation of Einstein-aether theory

被引:18
作者
Xie, Yi [1 ]
Huang, Tian-Yi [1 ,2 ]
机构
[1] Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China
[2] Chinese Acad Sci, Shanghai Astron Observ, Shanghai 20030, Peoples R China
来源
PHYSICAL REVIEW D | 2008年 / 77卷 / 12期
关键词
D O I
10.1103/PhysRevD.77.124049
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, second post-Newtonian approximation of Einstein-aether theory is obtained by Chandrasekhar's approach. Five parametrized post-Newtonian parameters in first post-Newtonian approximation are presented after a time transformation and they are identical with previous works, in which gamma = 1, beta = 1, and two preferred-frame parameters remain. Meanwhile, in second post-Newtonian approximation, a parameter, which represents third order nonlinearity for gravity, is zero-the same as in general relativity. For an application for future deep space laser ranging missions, we reduce the metric coefficients for light propagation in a case of N point masses as a simplified model of the Solar System. The resulting light deflection angle in second post-Newtonian approximation poses another constraint on the Einstein-aether theory.
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页数:15
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