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

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

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004acasn..45..266l&link_type=abstract

Acta Astronomica Sinica, vol. 45, no. 3, p. 266-271

Physics

Black Hole Physics, Accretion, Accretion Disks, Hydrodynamics

Scientific paper

This paper solves a set of basic equations describing black hole accretion flows using the standard Runge-Kutta method, and shows that a transition from a standard thin disk to an advection-dominated accretion flow is realizable for the high-viscosity case, without the need of involving any extra mechanism of energy transport or specifying any ad hoc outer boundary condition.

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