Structure and Evolution of an Isothermal Thin Accretion Disk Around a Black Hole

Details Structure and Evolution of an Isothermal Thin Accretion Disk Around a Black Hole Structure and Evolution of an Isothermal Thin Accretion Disk Around a Black Hole

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995chphl..12..505z&link_type=abstract

Chinese Physics Letters, Volume 12, Issue 8, pp. 505-508 (1995).

Physics

Scientific paper

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 = ρoe - s2/2so2. 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.

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