Titlebook: Numerical Simulation of Viscous Shocked Accretion Flows Around Black Holes; Kinsuk Giri Book 2015 Springer International Publishing Switze

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Effects of Power-Law Cooling in Viscous Flows,the power-law cooling throughout the flow. We show that in agreement with the theoretical solutions of viscous transonic flows, matter having viscosity parameter above a critical value becomes a Keplerian disc while matter having lesser viscosity remains a low angular momentum, sub-Keplerian flow. T

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2190-5053 this thesis contains step-by-step numerically simulated resThe work developed in this thesis addresses very important and relevant issues of accretion processes around black holes. Beginning by studying the time variation of the evolution of inviscid accretion discs around black holes and their pro

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Governing Equations and Computational Methods, for both non-viscous and viscous flows. We discuss the solution technique for a non-viscous system. Subsequently, we give all the schemes to incorporate turbulent viscosity in the non-viscous system. Finally, we add a power-law cooling in our viscous system and study the properties.

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