We examine the effect of thermal conduction on low-angular momentum hot accretion flow (HAF) around non-rotating black holes accreting mass at very low rate. While doing so, we adopt conductive heat flux in saturated form, and solve set dynamical equations corresponding to a steady, axisymmetric, viscous, advective using numerical methods. study thermodynamical properties matter terms input par...

In 1997, Macal and Hurter [7] have found that adding a constraint to the lower level problem, which is not active at the computed global optimal solution, can destroy global optimality. In this paper this property is reconsidered and it is shown that this solution remains locally optimal under inner semicontinuity of the original solution set mapping. In the second part of the paper we prove th...