Main Numerical Simulation of Viscous Shocked Accretion Flows Around Black Holes
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Numerical Simulation of Viscous Shocked Accretion Flows Around Black Holes

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The 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 properties, the author investigates the change of the pattern of the flows when the strength of the shear viscosity is varied and cooling is introduced. He succeeds to verify theoretical predictions of the so called Two Component Advective Flow (TCAF) solution of the accretion problem onto black holes through numerical simulations under different input parameters. TCAF solutions are found to be stable. And thus explanations of spectral and timing properties (including Quasi-Period Oscillations, QPOs) of galactic and extra-galactic black holes based on shocked TCAF models appear to have a firm foundation.
Request Code : ZLIBIO1207252
Categories:
Year:
2014
Edition:
2015
Publisher:
Springer
Language:
English
Pages:
129
ISBN 10:
3319095390
ISBN 13:
9783319095394
ISBN:
3319095390,9783319095394
Series:
Springer Theses
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