Precessing supermassive black hole binaries and dark energy measurements with LISA

被引:13
|
作者
Stavridis, Adamantios [1 ]
Arun, K. G. [1 ]
Will, Clifford M. [1 ,2 ]
机构
[1] Washington Univ, McDonnell Ctr Space Sci, Dept Phys, St Louis, MO 63130 USA
[2] Univ Paris 06, GReCO, Inst Astrophys Paris, CNRS, F-75014 Paris, France
来源
PHYSICAL REVIEW D | 2009年 / 80卷 / 06期
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
D O I
10.1103/PhysRevD.80.067501
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Spin induced precessional modulations of gravitational wave signals from supermassive black hole binaries can improve the estimation of luminosity distance to the source by space based gravitational wave missions like the Laser Interferometer Space Antenna (LISA). We study how this impacts the ability of LISA to do cosmology, specifically, to measure the dark energy equation of state (EOS) parameter w. Using the Lambda CDM model of cosmology, we show that observations of precessing binaries with mass ratio 10.1 by LISA, combined with a redshift measurement, can improve the determination of w up to an order of magnitude with respect to the nonprecessing case depending on the total mass and the redshift.
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页数:4
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