Numerical Simulation of Viscous Shocked Accretion Flows Around Black Holes

Nominated for Springer Theses by S.N. Bose National Research Centre for Basic Sciences, Kolkata, India Instead of assumptions of toy models, this thesis contains step-by-step numerically simulated results to verify the existence of theoretical self-consistent generalized viscous transonic flow shock solutions Demonstrates that the latest 'Avatar' of the accretion/outflow picture, the Generalized Two Component Advective Flow (GTCAF), is capable of explaining almost all the black hole observational results Addresses the challenge of approximating the turbulent viscosity Includes supplementary material: sn.pub/extras

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