Aspects of a spherically symmetric model of the post-decoupling universe
Bibliography: pages 84-88. === The central aim of this thesis is to consider aspects of the spherically symmetric Lemaitre-Tolman-Bondi (LTB) solution as a model of the post-decoupling universe. To do this comprehensively is a massive task and is not our aim here. Indeed, far from it, we will concen...
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ndltd-netd.ac.za-oai-union.ndltd.org-uct-oai-localhost-11427-175242020-10-06T05:10:58Z Aspects of a spherically symmetric model of the post-decoupling universe Mustapha, Nazeem Applied Mathematics Cosmology Bibliography: pages 84-88. The central aim of this thesis is to consider aspects of the spherically symmetric Lemaitre-Tolman-Bondi (LTB) solution as a model of the post-decoupling universe. To do this comprehensively is a massive task and is not our aim here. Indeed, far from it, we will concentrate on select instances of this programme and attempt in some places to indicate possibilities for further study. There are many solutions of the EFE which satisfy what we consider to be 'reasonable criteria' for a cosmology and others that do not. The LTB solution may be accepted as a reasonable cosmological model because ■ It allows non-empty solutions. ■ It allows expanding solutions. ■ It has a homogeneous and isotropic limit. ■ It allows for inhomogeneity. 2016-03-07T04:09:33Z 2016-03-07T04:09:33Z 1997 Master Thesis Masters MSc http://hdl.handle.net/11427/17524 eng application/pdf University of Cape Town Faculty of Science Department of Mathematics and Applied Mathematics |
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English |
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Dissertation |
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Applied Mathematics Cosmology |
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Applied Mathematics Cosmology Mustapha, Nazeem Aspects of a spherically symmetric model of the post-decoupling universe |
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Bibliography: pages 84-88. === The central aim of this thesis is to consider aspects of the spherically symmetric Lemaitre-Tolman-Bondi (LTB) solution as a model of the post-decoupling universe. To do this comprehensively is a massive task and is not our aim here. Indeed, far from it, we will concentrate on select instances of this programme and attempt in some places to indicate possibilities for further study. There are many solutions of the EFE which satisfy what we consider to be 'reasonable criteria' for a cosmology and others that do not. The LTB solution may be accepted as a reasonable cosmological model because ■ It allows non-empty solutions. ■ It allows expanding solutions. ■ It has a homogeneous and isotropic limit. ■ It allows for inhomogeneity. |
author |
Mustapha, Nazeem |
author_facet |
Mustapha, Nazeem |
author_sort |
Mustapha, Nazeem |
title |
Aspects of a spherically symmetric model of the post-decoupling universe |
title_short |
Aspects of a spherically symmetric model of the post-decoupling universe |
title_full |
Aspects of a spherically symmetric model of the post-decoupling universe |
title_fullStr |
Aspects of a spherically symmetric model of the post-decoupling universe |
title_full_unstemmed |
Aspects of a spherically symmetric model of the post-decoupling universe |
title_sort |
aspects of a spherically symmetric model of the post-decoupling universe |
publisher |
University of Cape Town |
publishDate |
2016 |
url |
http://hdl.handle.net/11427/17524 |
work_keys_str_mv |
AT mustaphanazeem aspectsofasphericallysymmetricmodelofthepostdecouplinguniverse |
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