Relativistic Roche-Riemann Problems around a Black Hole : Astrophysics and Relativity
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概要
- 論文の詳細を見る
Based on a framework of the hydrodynamics for a fluid star of mass m orbiting a Kerr black hole of mass M ≫ m, relativistic Roche-Riemann ellipsoids for incompressible fluids are considered. It is found that in the relativistic Roche-Riemann limit for the irrotational Roche-Riemann ellipsoid moving at the innermost stable circular orbit around Kerr black holes, the angular velocity, Ω, becomes Ω^2 ⋍0.063637πρ. We also argue implications of present results on the final fate of black hole-neutron star binary systems.
- 理論物理学刊行会の論文
- 1996-11-25
著者
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Sakka Makiko
Graduate School Of Bioresources Mie Univ.
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Shibata M
Univ. Tokyo Tokyo Jpn
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Shibata Masaru
Department Of Agricultural Chemistry Kyoto University:(present)asahi Kasei Chemicals Industry Co. Lt
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SHIBATA Masaru
Department of Earth and Space Science Faculty of Science, Osaka University
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SHIBATA Masaru
Graduate School of Arts and Sciences, University of Tokyo
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