Post-Newtonian approximation of gravitational waves from the inspiral phase

被引：5

作者：

Antelis, Javier M. ^{[1
]}

Hernandez, Jaime M. ^{[2
]}

Moreno, Claudia ^{[3
]}

机构：

[1] Tecnol Monterrey Guadalajara, Av Gral Ramon Corona 2514, Zapopan 45201, Jalisco, Mexico

[2] Univ Guadalajara, Ctr Univ Valles, Dept Ciencias Exactas & Nat, Carretera Guadalajara Ameca Km 45-5, Ameca 46600, Jalisco, Mexico

[3] Univ Guadalajara, Ctr Univ Ciencias Exactas & Ingn, Dept Fis, Av Revoluci 1500,Colonia Olmp, Guadalajara 44430, Jalisco, Mexico

来源：

XI MEXICAN SCHOOL ON GRAVITATION AND MATHEMATICAL PHYSICS, QUANTUM GRAVITY: SCHEMES, MODELS AND PHENOMENOLOGY | 2018年 / 1030卷

关键词：

D O I：

10.1088/1742-6596/1030/1/012005

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review the post-Newtonian (PN) expansion for the relativistic correction to the motion of a binary system of black holes. Using the Newtonian formalism, we derive the orbital equations for the 2nd order PN corrections, considering small velocities and weak fields. From a wave equation obtained by the post-Newtonian approximation, we find the h(+) and h(x) polarization of the Gravitational Waves (GW) which could be detected by Laser Interferometer Gravitational Observatory (LIGO).

引用

页数：6

共 50 条

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