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旋转致密双星后牛顿轨道的引力波研究

钟双英 刘崧

物理学报2012,Vol.61Issue(12):42-52,11.
物理学报2012,Vol.61Issue(12):42-52,11.

旋转致密双星后牛顿轨道的引力波研究

Study on gravitational waveform from post-Newtonian orbits of spinning compact binar

钟双英 1刘崧1

作者信息

  • 1. 南昌大学理学院,南昌330031
  • 折叠

摘要

Abstract

The purpose of this paper is to investigate the effects of the dynamical parameters, the spin-orbit coupling, the spin-spin coupling and the classification of orbits on the gravitational waveforms emitted by the conservative post-Newtonian Hamiltonian system for the spinning compact binaries by means of symplectic integrator and power spectrum. The numerical results show that the gravitational waveforms of ordered orbits vary periodically with time, while those of chaotic orbits are stochastic under the radiation-reaction force turning off. In particular, the chaotic dynamic behavior can enhance the strength of emission power. In addition, the magnitude of the spin parameter does exert a significant influence on the gravitational waveforms.

关键词

保守的/旋转致密双星/引力波/辛算法

Key words

conservative/spinning compact binaries/gravitational waves/symplectic integrator

分类

数理科学

引用本文复制引用

钟双英,刘崧..旋转致密双星后牛顿轨道的引力波研究[J].物理学报,2012,61(12):42-52,11.

基金项目

国家自然科学基金(批准号:11165011)资助的课题. ()

物理学报

OA北大核心CSCDCSTPCDSCI

1000-3290

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