Numerical Simulation of Viscous Shocked Accretion Flows Around Black Holes

  • KinsukĀ Giri

Part of the Springer Theses book series (Springer Theses)

Table of contents

About this book

Introduction

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.

Keywords

Accretion Models Accretion onto Black Hole Active Galactic Nuclei Inviscid Accretion Discs Quasi-period Oscillations Shocked Accretion Flows Two Component Advective Flow X-ray Binaries

Authors and affiliations

  • KinsukĀ Giri
    • 1
  1. 1.National Tsing Hua UniversityTaiwanChina

Bibliographic information

  • DOI https://doi.org/10.1007/978-3-319-09540-0
  • Copyright Information Springer International Publishing Switzerland 2015
  • Publisher Name Springer, Cham
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-3-319-09539-4
  • Online ISBN 978-3-319-09540-0
  • Series Print ISSN 2190-5053
  • Series Online ISSN 2190-5061
  • About this book
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