Gravitational Radiation of Binaries Coalescence into Intermediate Mass Black Holes |
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Authors: | LI Jin ZHONG Yuan-Hong PAN Yu |
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Affiliation: | 1.College of Physics, Chongqing University, Chongqing 401331, China;2.College of Engineering and Communication, Chongqing University, Chongqing 400030, China;3.College of Mathmatic and Physics, Chongqing University of Posts and Telecommunications, Chongqing 400065, China |
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Abstract: | This paper discusses the gravitation waveforms of binaries coalescence into intermediate mass black holes(about 30 times of the solar mass).We focus on the non-spinning intermediate mass black hole located less than 100 Mpc from earth.By comparing two simulation waveforms(effective one body numerical relativity waveform(EOBNR),phenomenological waveform),we discuss the relationship between the effective distance and frequency;and through analyzing large amounts of data in event,we find that the phenomenological waveform is much smoother than EOBNR waveform,and has higher accuracy at the same effective distance. |
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Keywords: | binary coalescence intermediate mass black hole effective one body numerical relativity waveform(EOBNR) phenomenological waveform |
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