MG12 - Talk detail
 

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Abstract

Accretion disks around black holes

Accretion disks around nonrotating black holes have been considered. It was taking into account advection and transition between the effectively optically thick outer and optically thin inner disk regions. It was shown relevance of including of advection into the model at large accretion rate. We have used expressions for radiative losses and radiation pressure at high and low effective optical depths. Effective optical depth was defined by general formula that is right at any magnitudes of optical depth. In this report it was described numeric method of solution resulting differential equation.

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