Non-Axisymmetric Modes in Relativistic Singular Isothermal Disks(Poster)

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概要

• 論文の詳細を見る

• The relativistic singular isothermal disk equilibrium solutions are self-similar and form a two-parameter family described by the sound speed and the linear rotational velocity. Using the equilibrium model as the base state, we study its stability against self-similar but non-axisymmetric perturbations. We discovered that instability can be manifested through radiation driven neutral modes and bifurcation points to non-axisymmetric equilibria.

• 理論物理学刊行会の論文
• 2004-11-15

著者

• Cai Michael

  Academia Sinica Institute Of Astronomy And Astrophysics

• SHU Frank

  Physics Department, National Tsing Hua University

• CAI Michael

  Academia Sinica, Institute of Astronomy and Astrophysics

関連論文

• Non-Axisymmetric Modes in Relativistic Singular Isothermal Disks(Poster)
• Non-Axisymmetric Modes in Relativistic Singular Isothermal Disks(Poster)

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