Full Text Available

Note: Clicking the button above will open the full text document at the original institutional repository in a new window.

A study in spherical accretion of self-gravitating fluids in a general relativistic framework

Includes abstract.

Saved in:
Bibliographic Details
Main Author: Richter, M C
Other Authors: Viollier, Raoul D
Format: Thesis
Language:English
Published: Department of Physics 2015
Subjects:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1867613174376693760
access_status_str Open Access
author Richter, M C
author2 Viollier, Raoul D
author_browse Richter, M C
Viollier, Raoul D
author_facet Viollier, Raoul D
Richter, M C
author_sort Richter, M C
collection Thesis
description Includes abstract.
format Thesis
id oai:open.uct.ac.za:11427/11576
institution University of Cape Town (South Africa)
language eng
last_indexed 2026-06-10T12:31:56.645Z
license_str Not specified — see source repository
provenance_str_mv Harvested via OAI-PMH from UCTD — University of Cape Town Open Access Repository
publishDate 2015
publishDateRange 2015
publishDateSort 2015
publisher Department of Physics
publisherStr Department of Physics
record_format dspace
source_str UCTD — University of Cape Town Open Access Repository
spelling oai:open.uct.ac.za:11427/11576 A study in spherical accretion of self-gravitating fluids in a general relativistic framework Richter, M C Viollier, Raoul D Tupper, Gary B Physics Includes abstract. Includes bibliographical references (leaves 46-49). A new general framework for studying relativistic spherical accretion of a self-gravitating fluid onto a central black hole is introduced in stationary coordinates for an observer at infinity. The important feature of gravitational backreaction due to a self-gravitating fluid on the metric is included in the model. The model is solved numerically for the most simple case of a polytropic fluid and compared to analytical solutions, which the model approximates in the "test-fluid" limit. The model is then focused on the accretion of a relativistic Fermi gas and the implications this might have on the rapid growth of supermassive black holes from clouds of sterile neutrino dark matter in the early universe. The results give good agreement with a Newtonian model of supermassive black hole growth called the symbiotic scenario. 2015-01-06T12:12:40Z 2015-01-06T12:12:40Z 2010 Doctoral Thesis Doctoral PhD http://hdl.handle.net/11427/11576 eng application/pdf Department of Physics Faculty of Science University of Cape Town
spellingShingle Physics
Richter, M C
A study in spherical accretion of self-gravitating fluids in a general relativistic framework
thesis_degree_str Doctoral
title A study in spherical accretion of self-gravitating fluids in a general relativistic framework
title_full A study in spherical accretion of self-gravitating fluids in a general relativistic framework
title_fullStr A study in spherical accretion of self-gravitating fluids in a general relativistic framework
title_full_unstemmed A study in spherical accretion of self-gravitating fluids in a general relativistic framework
title_short A study in spherical accretion of self-gravitating fluids in a general relativistic framework
title_sort study in spherical accretion of self gravitating fluids in a general relativistic framework
topic Physics
url http://hdl.handle.net/11427/11576
work_keys_str_mv AT richtermc astudyinsphericalaccretionofselfgravitatingfluidsinageneralrelativisticframework
AT richtermc studyinsphericalaccretionofselfgravitatingfluidsinageneralrelativisticframework