A relativistic orbit model for the LISA mission to be used in LISA TDI simulators

被引：0
|
作者：
Pireaux, Sophie [1 ]
Chauvineau, Bertrand [2 ]
机构：
[1] Observ Royal Belgique, Dept 1, 3 Ave Circulaire, B-1180 Brussels, Belgium
[2] Observ Cote Azur, ARTEMIS Dept, Grasse, France
来源：
RELATIVITY IN FUNDAMENTAL ASTRONOMY: DYNAMICS, REFERENCE FRAMES, AND DATA ANALYSIS | 2010年 / 261期
关键词：
gravitation; relativity; methods: analytical; numericical;
D O I：
10.1017/S1743921309990251
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The LISA mission is an interferometer, formed by three spacecraft, that aims at the detection of gravitational waves in the [10(-4),10(-1)] Hz frequency band. Present LISA TDI simulators, aimed at validating the novel Time Delay Interferometry method, use a classical Keplerian orbit model at first order in eccentricity in the gravitational field of a spherical non-rotating Sun, without planets. We propose to use the same model but described in the framework of relativistic gravity, and we focus here on quantifying the differences between classical and relativistic orbits for the LISA spacecraft, under the same assumptions.
引用
收藏
页码：124 / +
页数：3
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