The Gravitational Reaction Force on a Particle in the Schwarzschild Background
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概要
- 論文の詳細を見る
We formulate a new method to calculate the gravitational reaction force on a particle of mass μ orbiting a massive black hole of mass M. In this formalism, the tail part of the retarded Green function, which is responsible for the reaction force, is calculated at the level of the Teukolsky equation. Our method naturally allows a systematic post-Minkowskian(PM)expansion of the tail part at short distances. As a first step, we consider the case of a Schwarzschild black hole and explicitly calculate the first post-Newtonian(1PN)tail part of the Green function. There are, however, a couple of issues to be resolved before explicitly evaluating the reaction force by applying the present method. We discuss possible resolutions of these issues.
- 理論物理学刊行会の論文
- 2001-02-25
著者
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SASAKI Misao
Yukawa Institute for Theoretical Physics, Kyoto 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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Nakano H
Department Of Physics And Astronomy And Center For Gravitational Wave Astronomy The University Of Te
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NAKANO Hiroyuki
Theoretical Astrophysics, California Institute of Technology Pasadena
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Nakano Hiroyuki
Department Of Public Health Nagasaki University School Of Medicine
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Nakano Hiroyuki
Department Of Earth And Space Science 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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SASAKI Misao
Research Institute for Theoretical Physics, Hiroshima University
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SASAKI Misao
Department of Physics, School of Science, University of Tokyo
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NAKANO Hiroyuki
Department of Physics and Astronomy, and Center for Gravitational Wave Astronomy, The University of Texas at Brownsville
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NAKANO Hiroyuki
Department of Earth and Space Science, Graduate School of Science Osaka University
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