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Fluid and gas models in FLRW and almost FLRW universes

Includes bibliographical references.

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Bibliographic Details
Main Author: Gebbie, Timothy John
Other Authors: Ellis, George F R
Format: Thesis
Language:English
Published: Department of Mathematics and Applied Mathematics 2016
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access_status_str Open Access
author Gebbie, Timothy John
author2 Ellis, George F R
author_browse Ellis, George F R
Gebbie, Timothy John
author_facet Ellis, George F R
Gebbie, Timothy John
author_sort Gebbie, Timothy John
collection Thesis
description Includes bibliographical references.
format Thesis
id oai:open.uct.ac.za:11427/17936
institution University of Cape Town (South Africa)
language eng
last_indexed 2026-06-10T12:34:14.045Z
license_str Not specified — see source repository
provenance_str_mv Harvested via OAI-PMH from UCTD — University of Cape Town Open Access Repository
publishDate 2016
publishDateRange 2016
publishDateSort 2016
publisher Department of Mathematics and Applied Mathematics
publisherStr Department of Mathematics and Applied Mathematics
record_format dspace
source_str UCTD — University of Cape Town Open Access Repository
spelling oai:open.uct.ac.za:11427/17936 Fluid and gas models in FLRW and almost FLRW universes Gebbie, Timothy John Ellis, George F R Maartens, Roy Dunsby, Peter K S Mathematics and Applied Mathematics Cosmology Includes bibliographical references. Recently the universe has been modeled in the covariant sense, in terms of fluid models and perturbations thereof, leading to Gauge Invariant Covariant (GIC) perturbations of these fluid models. It is well known that kinetic theory provides a physically sound and consistent description of the matter and radiation in the universe, so a perturbative theory of gas models using kinetic theory would be most helpful. This has been done to a large degree in the Gauge Invariant (GI) Bardeen approach to perturbation theory by studies of gases based on the relativistic Boltzmann equation. These treatments, however, were not fully covariant. The GI Bardeen approach is dependent on a co-ordinate choice, while in the full GIC perturbation theory full covariance is maintained along with gauge invariance by describing the theory in a particular set of perturbation variables that differ from the Bardeen choice but can be related to the Bardeen variables. The covariant formulation of the relativistic Boltzmann equation in terms of variables that are of use in the GIC theory for gases has been well described. In this thesis, I provide both a good introduction to the full GIC perturbation theory of a photon gas and matter fluid system in the linear theory as well as a solid grounding with respect to the exact FLRW fluid model upon which most of the original ideas and concepts of modern cosmology are based. The introduction to the exact FLRW model is done in the sense of the dynamical systems approach to cosmology which provides the easiest access to understanding the evolution of single and multi-fluid FLRW models. 2016-03-17T12:37:19Z 2016-03-17T12:37:19Z 1996 Master Thesis Masters MSc http://hdl.handle.net/11427/17936 eng application/pdf Department of Mathematics and Applied Mathematics Faculty of Science University of Cape Town
spellingShingle Mathematics and Applied Mathematics
Cosmology
Gebbie, Timothy John
Fluid and gas models in FLRW and almost FLRW universes
thesis_degree_str Master's
title Fluid and gas models in FLRW and almost FLRW universes
title_full Fluid and gas models in FLRW and almost FLRW universes
title_fullStr Fluid and gas models in FLRW and almost FLRW universes
title_full_unstemmed Fluid and gas models in FLRW and almost FLRW universes
title_short Fluid and gas models in FLRW and almost FLRW universes
title_sort fluid and gas models in flrw and almost flrw universes
topic Mathematics and Applied Mathematics
Cosmology
url http://hdl.handle.net/11427/17936
work_keys_str_mv AT gebbietimothyjohn fluidandgasmodelsinflrwandalmostflrwuniverses