The connection of standard thin disk with advection-dominated accretion flow

Details The connection of standard thin disk with advection-dominated accretion flow The connection of standard thin disk with advection-dominated accretion flow

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cha%26a..29..113l&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 29, Issue 2, p. 113-119.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using the standard Runge-Kutta method, a global solution of the basic equations describing black hole accretion flows is derived. It is proved that transition from a standard thin disk to an advection-dominated accretion flow is realizable in case of high viscosity, without introducing any additional mechanism of energy transfer or specifying any ad hoc outer boundary condition.

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