Relativistic Accreting Flow onto Kerr Black Holes
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概要
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We have proven that the radial drift velocity of the adiabatic accretion torus orbiting around a Kerr black hole must be subsonic at the inner edge of any torus. This result is irrespective of distributions of angular momentum of any torus.
- 理論物理学刊行会の論文
- 1989-03-25
著者
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Kuwahara Fumiko
Department Of Physics Rikkyo University
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KAWAHARA Fumiko
Department of Physics, Rikkyo University
関連論文
- Effects of Rotation and Deformation of Central Black Holes on the Structure of Rotating Disks : Astrophysics and Relativity
- Relativistic Accreting Flow onto Kerr Black Holes
- Relativistic Accretion Tori around Schwarzschild Black Holes : Astrophysics and Relativity