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Ricci Time in Lemaître-Tolman Model and Block Universe

Includes bibliographical references.

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Bibliographic Details
Main Author: Elmahalawy,Yasser Reda Ahmed Abdelhamid
Other Authors: Hellaby, Charles
Format: Thesis
Language:English
Published: Department of Mathematics and Applied Mathematics 2015
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access_status_str Open Access
author Elmahalawy,Yasser Reda Ahmed Abdelhamid
author2 Hellaby, Charles
author_browse Elmahalawy,Yasser Reda Ahmed Abdelhamid
Hellaby, Charles
author_facet Hellaby, Charles
Elmahalawy,Yasser Reda Ahmed Abdelhamid
author_sort Elmahalawy,Yasser Reda Ahmed Abdelhamid
collection Thesis
description Includes bibliographical references.
format Thesis
id oai:open.uct.ac.za:11427/13373
institution University of Cape Town (South Africa)
language eng
last_indexed 2026-06-10T12:32:44.899Z
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 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:11427/13373 Ricci Time in Lemaître-Tolman Model and Block Universe Elmahalawy,Yasser Reda Ahmed Abdelhamid Hellaby, Charles Ellis, GFR Mathematics and Applied Mathematics Includes bibliographical references. It is common to think of our universe according to the "block universe" idea, which says that spacetime consists of many "stacked" 3-surfaces varied as a function of some kind of proper time Ƭ. Standard ideas do not distinguish past and future, but Ellis' "evolving block universe" tries to make a fundamental distinction. One proposal for this proper time is the proper time measured along the timelike Ricci eigenlines, starting from the big bang. The main idea of this work is to investigate the shape of the {Ƭ=constant} surfaces relative to the the null surfaces, and determine what makes these surfaces timelike or spacelike. We use the Lemaître-Tolman metric as our inhomogeneous spacetime model, and we find the necessary and sufficient conditions for these {Ƭ=constant} surfaces to be spacelike or timelike. Furthermore, we indicate whether or not timelike surfaces appear inside black holes and other strong gravity domains, by determining the location of the timelike regions relative to the apparent horizon. Based on this idea, we find that the regions where these surfaces become timelike are often close to the apparent horizons, but always outside them, and in particular timelike regions occur outside black holes. They are always spacelike near the big bang, and at late times (near the crunch or the extreme far future), they are only timelike under special circumstances. 2015-07-03T10:33:42Z 2015-07-03T10:33:42Z 2014 Master Thesis Masters MSc http://hdl.handle.net/11427/13373 eng application/pdf Department of Mathematics and Applied Mathematics Faculty of Science University of Cape Town
spellingShingle Mathematics and Applied Mathematics
Elmahalawy,Yasser Reda Ahmed Abdelhamid
Ricci Time in Lemaître-Tolman Model and Block Universe
thesis_degree_str Master's
title Ricci Time in Lemaître-Tolman Model and Block Universe
title_full Ricci Time in Lemaître-Tolman Model and Block Universe
title_fullStr Ricci Time in Lemaître-Tolman Model and Block Universe
title_full_unstemmed Ricci Time in Lemaître-Tolman Model and Block Universe
title_short Ricci Time in Lemaître-Tolman Model and Block Universe
title_sort ricci time in lemaitre tolman model and block universe
topic Mathematics and Applied Mathematics
url http://hdl.handle.net/11427/13373
work_keys_str_mv AT elmahalawyyasserredaahmedabdelhamid riccitimeinlemaitretolmanmodelandblockuniverse