Dey, Pranayjit (2023) Numerical simulation of the accretion of mass onto a black hole. Masters thesis, Indian Institute of Science Education and Research Kolkata.
Text (MS dissertation of Pranayjit Dey (18MS171))
Thesis_18MS171.pdf - Submitted Version Restricted to Repository staff only Download (3MB) |
Abstract
The study of fluid dynamics in the vicinity of a black hole has been conducted through the utilization of the equations of general relativistic hydrodynamics (GRHD). A numerical solution has been devised for the general relativistic hydrodynamic system of equations in three dimensions, utilizing the 3+1 formalism. The present study concerns the derivation of the requisite theoretical components for constructing a numerical algorithm predicated on the resolution of local Riemann problems. Subsequently, we investigate the temporal progression of Bondi accretion flows and sub-Keplerian transonic accretion flows onto black holes through the utilization of a numerical simulation code that incorporates general relativity. Simulations are conducted within the Schwarzschild space-time framework. Initially, we compare the outcomes of our one-dimensional simulation with the theoretical results to authenticate the efficacy of our code. Subsequently, the outcomes of the axisymmetric and two-dimensional simulation of advective currents are exhibited. Shortcomings of the code and future improvements have been discussed.
Item Type: | Thesis (Masters) |
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Additional Information: | Supervisor: Dr. Sudip K Garain |
Uncontrolled Keywords: | Accretion; Black-Hole Physics; General Relativistic Hydrodynamics; Shock |
Subjects: | Q Science > QC Physics |
Divisions: | Department of Physical Sciences |
Depositing User: | IISER Kolkata Librarian |
Date Deposited: | 13 Jun 2024 10:31 |
Last Modified: | 13 Jun 2024 10:31 |
URI: | http://eprints.iiserkol.ac.in/id/eprint/1634 |
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