Constructing realistic Szekeres models from initial and final data
The Szekeres family of inhomogeneous solutions, which are defined by six arbitrary metric functions, offers a wide range of possibilities for modelling cosmic structure. Within this family, the quasispherical case is the best understood, and is interpreted as being an arrangement on non-concentric m...
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ndltd-netd.ac.za-oai-union.ndltd.org-uct-oai-localhost-11427-143822020-10-06T05:10:54Z Constructing realistic Szekeres models from initial and final data Walters, Anthony Paul Hellaby, Charles Mathematics and Applied Mathematics The Szekeres family of inhomogeneous solutions, which are defined by six arbitrary metric functions, offers a wide range of possibilities for modelling cosmic structure. Within this family, the quasispherical case is the best understood, and is interpreted as being an arrangement on non-concentric mass shells, each a density dipole. Here we present a model construction procedure for the quasispherical case using given data at initial and final times. Of the six arbitrary metric functions, the three which are common to both Szekeres and Lemaitre-Tolman models are determined by the model construction procedure of Krasinski & Hellaby. For the remaining three functions, which are unique to Szekeres models, we derive exact analytic expressions in terms of more physically intuitive quantities - density profiles and dipole orientation angles. Using MATLAB, we implement the model construction procedure and simulate the time evolution. 2015-10-28T05:29:57Z 2015-10-28T05:29:57Z 2012 Master Thesis Masters MSc http://hdl.handle.net/11427/14382 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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Mathematics and Applied Mathematics |
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Mathematics and Applied Mathematics Walters, Anthony Paul Constructing realistic Szekeres models from initial and final data |
description |
The Szekeres family of inhomogeneous solutions, which are defined by six arbitrary metric functions, offers a wide range of possibilities for modelling cosmic structure. Within this family, the quasispherical case is the best understood, and is interpreted as being an arrangement on non-concentric mass shells, each a density dipole. Here we present a model construction procedure for the quasispherical case using given data at initial and final times. Of the six arbitrary metric functions, the three which are common to both Szekeres and Lemaitre-Tolman models are determined by the model construction procedure of Krasinski & Hellaby. For the remaining three functions, which are unique to Szekeres models, we derive exact analytic expressions in terms of more physically intuitive quantities - density profiles and dipole orientation angles. Using MATLAB, we implement the model construction procedure and simulate the time evolution. |
author2 |
Hellaby, Charles |
author_facet |
Hellaby, Charles Walters, Anthony Paul |
author |
Walters, Anthony Paul |
author_sort |
Walters, Anthony Paul |
title |
Constructing realistic Szekeres models from initial and final data |
title_short |
Constructing realistic Szekeres models from initial and final data |
title_full |
Constructing realistic Szekeres models from initial and final data |
title_fullStr |
Constructing realistic Szekeres models from initial and final data |
title_full_unstemmed |
Constructing realistic Szekeres models from initial and final data |
title_sort |
constructing realistic szekeres models from initial and final data |
publisher |
University of Cape Town |
publishDate |
2015 |
url |
http://hdl.handle.net/11427/14382 |
work_keys_str_mv |
AT waltersanthonypaul constructingrealisticszekeresmodelsfrominitialandfinaldata |
_version_ |
1719347678650826752 |