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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.
[1] Kidder L E 1995 Phys. Rev. D 52 821
[2] Will C M, Wiseman A G 1996 Phys. Rev. D 54 4813
[3] Baker J 2001 Phys. Rev. Lett. 87 121103
[4] Suzuki S, Maeda K 1999 Phys. Rev. D 61 024005
[5] Kiuchi K, Maeda K 2004 Phys. Rev. D 70 064036
[6] Faye G, Blanchet L, Buonanno A 2006 Phys. Rev. D 74 104033
[7] Levin J 2000 Phys. Rev. Lett. 84 3515
[8] Damour T 2001 Phys. Rev. D 64 124013
[9] Konigsdorffer C, Gopakumar A 2005 Phys. Rev. D 71 024039
[10] Gopakumar A, Konigsdorffer C 2005 Phys. Rev. D 72 121501
[11] Levin J 2006 Phys. Rev. D 74 124027
[12] Wu X, Xie Y 2010 Phys. Rev. D 81 084045
[13] Wu X, Zhong S Y 2011 Gen. Relativ Gravit 43 2185
[14] Zhong S Y, Wu X 2010 Phys. Rev. D 81 104037
[15] Zhong S Y, Wu X, Liu S Q, Deng X F 2010 Phys. Rev. D 82 124040
[16] Wang Y Z, Wu X 2011 Class. Quantum Grav. 28 025010
[17] Wu X, Xie Y 2007 Phys. Rev. D 76, 124004
[18] Wu X, Xie Y 2008 Phys. Rev. D 77 103012
[19] Wu X, Huang T Y, Zhang H 2006 Phys. Rev. D 74 083001
[20] Xu J, Wu X 2010 Res. Astron. Astrophys. 10 173
[21] Li R, Wu X 2010 Acta. Phys. Sin. 59 7135 (in Chinese) [李荣, 伍歆 2010 59 7135]
[22] Lubich C, Walther B, Braugmann B 2010 Phys. Rev. D 81 104025
[23] Zhong S Y, Wu X 2011 Acta. Phys. Sin. 60 090402 (in Chinese) [钟双英, 伍歆 2011 60 090402]
[24] Hartl M D, Buonanno A 2005 Phys. Rev. D 71 024027
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[1] Kidder L E 1995 Phys. Rev. D 52 821
[2] Will C M, Wiseman A G 1996 Phys. Rev. D 54 4813
[3] Baker J 2001 Phys. Rev. Lett. 87 121103
[4] Suzuki S, Maeda K 1999 Phys. Rev. D 61 024005
[5] Kiuchi K, Maeda K 2004 Phys. Rev. D 70 064036
[6] Faye G, Blanchet L, Buonanno A 2006 Phys. Rev. D 74 104033
[7] Levin J 2000 Phys. Rev. Lett. 84 3515
[8] Damour T 2001 Phys. Rev. D 64 124013
[9] Konigsdorffer C, Gopakumar A 2005 Phys. Rev. D 71 024039
[10] Gopakumar A, Konigsdorffer C 2005 Phys. Rev. D 72 121501
[11] Levin J 2006 Phys. Rev. D 74 124027
[12] Wu X, Xie Y 2010 Phys. Rev. D 81 084045
[13] Wu X, Zhong S Y 2011 Gen. Relativ Gravit 43 2185
[14] Zhong S Y, Wu X 2010 Phys. Rev. D 81 104037
[15] Zhong S Y, Wu X, Liu S Q, Deng X F 2010 Phys. Rev. D 82 124040
[16] Wang Y Z, Wu X 2011 Class. Quantum Grav. 28 025010
[17] Wu X, Xie Y 2007 Phys. Rev. D 76, 124004
[18] Wu X, Xie Y 2008 Phys. Rev. D 77 103012
[19] Wu X, Huang T Y, Zhang H 2006 Phys. Rev. D 74 083001
[20] Xu J, Wu X 2010 Res. Astron. Astrophys. 10 173
[21] Li R, Wu X 2010 Acta. Phys. Sin. 59 7135 (in Chinese) [李荣, 伍歆 2010 59 7135]
[22] Lubich C, Walther B, Braugmann B 2010 Phys. Rev. D 81 104025
[23] Zhong S Y, Wu X 2011 Acta. Phys. Sin. 60 090402 (in Chinese) [钟双英, 伍歆 2011 60 090402]
[24] Hartl M D, Buonanno A 2005 Phys. Rev. D 71 024027
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