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Structure analysis of solution to equations of quasi 3-D accretion disk model
Authors:Wu Mei  ZHANG Peng  WANG Jianmin  MA Yuqian  CHEN Li
Affiliation:1. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039, China
2. Laboratory of Cosmic Ray and High Energy Astrophysics, Chinese Academy of Sciences, Beijing 100039, China;Beijing Information Technology Institute, Beijing 100101, China
3. Department of Astronomy, Beijing Normal University, Beijing 100875, China
Abstract:In this paper we discuss the problems contained in the solution to the equations of quasi 3-D accretion disk model, and point out that the angular momentum equation should not be integrated directly. Finally, we develop a criterion of the existence of a disconnected solution to this model.
Keywords:acrretion disk  shock
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