Calculation of the first nonlinear contribution to the general-relativistic spin-spin interaction for binary systems

被引:147
作者
Porto, Rafael A. [1 ]
Rothstein, Ira Z. [1 ]
机构
[1] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA
关键词
D O I
10.1103/PhysRevLett.97.021101
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We use recently developed effective field theory techniques to calculate the third order post-Newtonian correction to the spin-spin potential between two spinning objects. This correction represents the first contribution to the spin-spin interaction due to the nonlinear nature of general relativity and will play an important role in forthcoming gravity wave experiments.
引用
收藏
页数:4
相关论文
共 22 条
[21]   LAWS OF MOTION AND PRECESSION FOR BLACK-HOLES AND OTHER BODIES [J].
THORNE, KS ;
HARTLE, JB .
PHYSICAL REVIEW D, 1985, 31 (08) :1815-1837
[22]   Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. III. Radiation reaction for binary systems with spinning bodies [J].
Will, CM .
PHYSICAL REVIEW D, 2005, 71 (08) :1-15