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Numerical Simulation of Viscous Shocked Accretion Flows Around Black Holes

Kinsuk Giri

978-3-319-09540-0

2015
Edition 1
- 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
€100

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