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Gravitational Waves from a Pseudo-Newtonian Kerr Field with Halos
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作者 王颖 伍歆 《Communications in Theoretical Physics》 SCIE CAS CSCD 2011年第12期1045-1051,共7页
A close relation between gravitational waveforms and the types of trajectories in a superposed field between a pseudo-Newtonian Kerr black hole and quadrupolax halos is shown in detail.The gravitational waveforms emit... A close relation between gravitational waveforms and the types of trajectories in a superposed field between a pseudo-Newtonian Kerr black hole and quadrupolax halos is shown in detail.The gravitational waveforms emitted from circular,KAM tori and chaotic orbits must be periodic,quasiperiodic and stochastic,respectively.The chaotic motion can maximally enhance both the amplitudes and the energy emission rates of the waves. 展开更多
关键词 引力波 牛顿 克尔场 KERR黑洞 字段类型 周期性 准周期 排放率
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