Post-Newtonian Expansion of Gravitational Waves from a Compact Star Orbiting a Rotating Black Hole in Brans-Dicke Theory : Circular Orbit Case : Astrophysics and Relativity
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概要
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In the context of Brans-Dicke theory, we calculate the post-Newtonian expansion of the scalar part of gravitational radiation from a compact star in a circular orbit around a rotating black hole up to O(υ^5) beyond the leading, Newtonian-dipole formula. The calculation is based on a method developed recently by Sasaki in the Schwarzschild case in the context of general relativity. The orbit of a compact star is restricted on the equatorial plane. Then we estimate the post-Newtonian effect of scalar radiation to the orbital evolution of coalescing compact binaries. We find that the post-Newtonian effect of scalar radiation is small in the LIGO band if we take into account the experimental bound of the Brans-Dicke parameter ω_<BD>500. On the other hand, we find that the post-Newtonian effect of the scalar radiation is not negligible for the LISA experiment.
- 理論物理学刊行会の論文
- 1996-10-25
著者
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大橋 朗
Department Of Environmental Sciences Faculty Of Science Ibaraki University
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Sasaki M
Department Of Earth And Space Science Osaka University
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Sasaki Misao
Department Of Earth And Space Science Graduate School Of Science Osaka University
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Ohashi A
Ochanomizu Univ. Tokyo Jpn
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TAGOSHI Hideyuku
National Astronomical Observatory
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TAGOSHI Hideyuki
National Astronomical Observator
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TAGOSHI Hideyuki
Department of Physics, Kyoto University
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Ohashi Akira
Department Of Environmental Sciences Faculty Of Science Ibaraki University
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Ohashi Akira
Department Of Chemistry Graduate School Of Science Osaka University
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SASAKI Misao
Department of Earth and Space Science, Osaka University
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SASAKI Misao
Department of Earth and Space Science, Graduate School of Science Osaka University
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SASAKI Misao
Research Institute for Fundamental Physics, Kyoto University
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OHASHI Akira
Department of Physics, Ochanomizu University
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OHASHI Akira
Department of Physics, Kyoto University
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