Eccentricity content of binary black hole initial data

被引:17
作者
Berti, Emanuele [1 ]
Iyer, Sai [1 ]
Will, Clifford M. [1 ]
机构
[1] Washington Univ, Dept Phys, McDonnell Ctr Space Sci, St Louis, MO 63130 USA
来源
PHYSICAL REVIEW D | 2006年 / 74卷 / 06期
关键词
D O I
10.1103/PhysRevD.74.061503
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using a post-Newtonian diagnostic tool developed by Mora and Will, we examine numerically generated quasiequilibrium initial data sets that have been used in recently successful numerical evolutions of binary black holes through plunge, merger and ringdown. We show that a small but significant orbital eccentricity is required to match post-Newtonian and quasiequilibrium calculations. If this proves to be a real eccentricity, it could affect the fine details of the subsequent numerical evolutions and the predicted gravitational waveforms.
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页数:4
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