A note on the radiation reaction in the 2.5PN waveform from inspiralling binaries in quasi-circular orbits

被引：24

作者：

Kidder, Lawrence E. ^{[1
]}

Blanchet, Luc

Iyer, Bala R.

机构：

[1] Cornell Univ, Ctr Radiophys & Space Res, Ithaca, NY 14853 USA

[2] CNRS, GRECO Inst Astrophys, F-75014 Paris, France

[3] Raman Res Inst, Bangalore 560080, Karnataka, India

来源：

CLASSICAL AND QUANTUM GRAVITY | 2007年 / 24卷 / 20期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1088/0264-9381/24/20/N01

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this note we compute the contributions of the radiation reaction force in the 2.5 post-Newtonian (PN) gravitational wave polarizations for compact binaries in quasi-circular orbits. (i) We point out and correct an inconsistency in the derivation of [ 1]. (ii) We prove that all contributions from the radiation reaction in the 2.5PN waveform are actually negligible since they can be absorbed into a modification of the orbital phase at the 5PN order.

引用

页码：5307 / 5312

页数：6

共 4 条

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[4] POST-NEWTONIAN EXPANSION OF GRAVITATIONAL-WAVES FROM A PARTICLE IN CIRCULAR ORBIT AROUND A SCHWARZSCHILD BLACK-HOLE [J].

TAGOSHI, H ;

SASAKI, M .

PROGRESS OF THEORETICAL PHYSICS, 1994, 92 (04) :745-771

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