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The influence of structure formation on the evolution of the universe

Includes abstract.

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Bibliographic Details
Main Author: Umeh, Obinna
Other Authors: Clarkson, Chris
Format: Thesis
Language:English
Published: Department of Mathematics and Applied Mathematics 2014
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access_status_str Open Access
author Umeh, Obinna
author2 Clarkson, Chris
author_browse Clarkson, Chris
Umeh, Obinna
author_facet Clarkson, Chris
Umeh, Obinna
author_sort Umeh, Obinna
collection Thesis
description Includes abstract.
format Thesis
id oai:open.uct.ac.za:11427/4938
institution University of Cape Town (South Africa)
language eng
last_indexed 2026-06-10T12:32:31.718Z
license_str Not specified — see source repository
provenance_str_mv Harvested via OAI-PMH from UCTD — University of Cape Town Open Access Repository
publishDate 2014
publishDateRange 2014
publishDateSort 2014
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:11427/4938 The influence of structure formation on the evolution of the universe Umeh, Obinna Clarkson, Chris Ellis, GFR Mathematics and Applied Mathematics Includes abstract. Includes bibliographical references. The next generation of telescopes will usher in a new era of precision cosmology capable of determining key parameters of a cosmological model to percent level and beyond. For this to be effective, the theoretical model must be understood to at least the same level of precision. A range of subtle physical spacetime effcts remain to be explored theoretically, for example, the effect of backreaction on cosmological observables. A good understanding of this effect is paramount given that it is a consequence of any space-time theory of gravity. We provide a comprehensive study of this effect from the perspective of geometric averaging on a hyper-surface and averaging on the celestial sphere. We concentrate on Friedmann-Lemaitre-Robertson-Walker spacetime with small perturbation up to non-linear order . This enables us to quantify by how much this effect could change the standard model interpretation of the universe. We study in great detail key parameters of the standard model, Hubble rate, deceleration parameter and area distance. 2014-07-31T08:11:05Z 2014-07-31T08:11:05Z 2013 Doctoral Thesis Doctoral PhD http://hdl.handle.net/11427/4938 eng application/pdf Department of Mathematics and Applied Mathematics Faculty of Science University of Cape Town
spellingShingle Mathematics and Applied Mathematics
Umeh, Obinna
The influence of structure formation on the evolution of the universe
thesis_degree_str Doctoral
title The influence of structure formation on the evolution of the universe
title_full The influence of structure formation on the evolution of the universe
title_fullStr The influence of structure formation on the evolution of the universe
title_full_unstemmed The influence of structure formation on the evolution of the universe
title_short The influence of structure formation on the evolution of the universe
title_sort influence of structure formation on the evolution of the universe
topic Mathematics and Applied Mathematics
url http://hdl.handle.net/11427/4938
work_keys_str_mv AT umehobinna theinfluenceofstructureformationontheevolutionoftheuniverse
AT umehobinna influenceofstructureformationontheevolutionoftheuniverse