Structure and Evolution of an Isothermal Thin Accretion Disk
Around a Black Hole
ZHOU Hongnan1 , HUANG Keliang2
1 Department of Astronomy, Nanjing University, Nanjing 210008
2 Department of Physics, Nanjing Normal University, Nanjing 210024
Structure and Evolution of an Isothermal Thin Accretion Disk
Around a Black Hole
ZHOU Hongnan1 ;HUANG Keliang2
1 Department of Astronomy, Nanjing University, Nanjing 210008
2 Department of Physics, Nanjing Normal University, Nanjing 210024
关键词 :
97.10.Gz ,
97.60.Lf
Abstract : In this paper, we construct an isothermal thin accretion disk model around a black hole for which the vertical mass density is expressed as ρ = ρ0 e-z2 /2z0 2 . The hydrostatic equilibrium equations of the model disk and their difference forms are derived. We solve the basic balance equations by numerical method. According to the calculation results, the structure and evolution of model disk are discussed.
Key words :
97.10.Gz
97.60.Lf
出版日期: 1995-08-01
引用本文:
ZHOU Hongnan;HUANG Keliang. Structure and Evolution of an Isothermal Thin Accretion Disk
Around a Black Hole[J]. 中国物理快报, 1995, 12(8): 505-508.
ZHOU Hongnan, HUANG Keliang. Structure and Evolution of an Isothermal Thin Accretion Disk
Around a Black Hole. Chin. Phys. Lett., 1995, 12(8): 505-508.
链接本文:
https://cpl.iphy.ac.cn/CN/
或
https://cpl.iphy.ac.cn/CN/Y1995/V12/I8/505
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